{"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"B_iram"}} {"id": "B/iram", "title_cds": "IRAM Observation Logs", "title_create": "IRAM 1991-2020", "year": "2020", "author": "Dan M., Neri R., Sievers A.", "title_pub": "IRAM Observation Logs (Plateau de Bure Interferometer and 30-m telescope)", "first_author": "Dan M.", "ref_biblio": [""], "see_also": ["http://www.iram-institute.org/ : the IRAM Home Page"], "keyword_cds": "Observatory log ; Interferometry ; Radio sources", "description": ["The Institut de Radio Astronomie Millimetrique (IRAM) was founded in", "1979 and is operated as a French-German-Spanish collaboration. Its", "partner institutes are the CNRS (Centre National de la Recherche", "Scientifique, France), the MPG (Max Planck Gesellschaft, Germany), and", "the IGN (Instituto Geografico Nacional, Spain). The principal activity", "of IRAM is the study of cold matter (molecular gas and dust) in the", "solar system, in our Galaxy, and out to cosmological distances in", "order to determine its composition, density, mass, temperature, and", "kinematics.", "IRAM operates two observatories at millimeter wavelengths which are", "open to the international astronomical community: The 30-m single-dish", "telescope on Pico Veleta (2850m), Spain, and the six-antenna", "interferometer on the Plateau de Bure (2550m) in France. Both sites", "are at high altitude to reduce the absorption by water vapor. The", "observatories are supported by the IRAM offices and laboratories in", "Granada and Grenoble.", "The observation log included here concerns the Plateau de Bure site,", "and summarizes the observations made there from December 1990.", "The observations log of the 30-m single-dish telescope covers a", "period starting in January 2009. This log was produced using a header", "archive, a collaborative effort between IRAM and IAA/CSIC.", "NOEMA (NOrthern Extended Millimeter Array) is the successor to the", "Plateau du Bure observatory. During its history, the observatory at", "the Plateau de Bure underwent several track extensions, received", "additional antennas (all of 15m diameter and similar construction as", "the first ones) and technical upgrades. From a three antenna", "interferometer with a maximum baseline of 288 meters in 1988, it has", "evolved to a eight-antenna array with baselines up to 760 meters in", "2016. With the inauguration of the seventh antenna in September 2014,", "the observatory has started its transformation into NOEMA."], "alias": ["logIRAM", "IRAM", "PdBI"], "type": ["OC"], "records": ["653695 obs."], "data": "f-v", "date_creation": "29-Jun-2004", "xmatch": "B/iram/pdbi", "last_update": "07-Oct-2022", "catid": "102016", "date_update": "08-Aug-2022", "tables": [{"name": "pdbi.dat", "desc": "The Plateau de Bure Interferometer Observation Log since 1991-12-01", "columns": [{"name": "Nw", "desc": "[11,18] Internal indicator "}, {"name": "Prog", "desc": "Identification code of the program "}, {"name": "Name", "desc": "Source name, as mentioned in the observing program"}, {"name": "Obs.Y", "desc": "Starting date of the Observation (year) (5) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.M", "desc": "Starting date of the Observation (month) (5) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.D", "desc": "Starting date of the Observation (day) (5) "}, {"name": "t1.h", "desc": "LST Time of the first scan on source "}, {"name": "---", "desc": "[:] "}, {"name": "t1.m", "desc": "LST Time of the first scan on source "}, {"name": "t2.h", "desc": "LST Time of the last scan on source "}, {"name": "---", "desc": "[:] "}, {"name": "t2.m", "desc": "LST Time of the last scan on source "}, {"name": "tos", "desc": "Total on-source correlation time "}, {"name": "Type", "desc": "Program type (1) "}, {"name": "oEq", "desc": "? Original equinox of position (2) "}, {"name": "RAh", "desc": "? Right Ascension J2000 (hours) "}, {"name": "---", "desc": "[:] "}, {"name": "RAm", "desc": "? Right Ascension J2000 (minutes) "}, {"name": "---", "desc": "[:] "}, {"name": "RAs", "desc": "? Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? Declination J2000 (degrees) "}, {"name": "---", "desc": "[:] "}, {"name": "DEm", "desc": "? Declination J2000 (minutes) "}, {"name": "---", "desc": "[:] "}, {"name": "DEs", "desc": "? Declination J2000 (seconds) "}, {"name": "Vel", "desc": "Velocity of the source (3) "}, {"name": "n_Vel", "desc": "[LH] LSR or Heliocentric velocity "}, {"name": "Flow", "desc": "?=0 Sky Frequency of the 3mm receiver (6) "}, {"name": "n_Flow", "desc": "[UL] Signal Upper/Lower band of the 3mm receiver "}, {"name": "Fhigh", "desc": "?=0 Sky Frequency of the 1mm receiver (6) "}, {"name": "n_Fhigh", "desc": "[UL] Signal Upper/Lower band of the 1mm receiver "}, {"name": "pol", "desc": "[HV ] Horizontal/Vertical polarisations (6) "}, {"name": "p4", "desc": "[HV ] Polarisation of 4GHz continuum (6) "}, {"name": "Conf", "desc": "Configuration code of the interferometer "}, {"name": "Config", "desc": "Detailed configuration (4) "}]}, {"name": "pdbi_pi.dat", "desc": "List of PI investigators of PdBI instrument ", "columns": [{"name": "Prog", "desc": "Identification code of the program "}, {"name": "PI", "desc": "Principal Investigator's name "}]}, {"name": "noema.dat", "desc": "The Plateau de Bure Interferometer (Noema) Observation Log since 2016", "columns": [{"name": "Nw", "desc": "[11,19] Internal indicator "}, {"name": "Prog", "desc": "Identification code of the program "}, {"name": "Name", "desc": "Source name, as mentioned in the observing program"}, {"name": "Obs.Y", "desc": "Starting date of the Observation (year) (5) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.M", "desc": "Starting date of the Observation (month) (5) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.D", "desc": "Starting date of the Observation (day) (5) "}, {"name": "t1.h", "desc": "LST Time of the first scan on source "}, {"name": "---", "desc": "[:] "}, {"name": "t1.m", "desc": "LST Time of the first scan on source "}, {"name": "t2.h", "desc": "LST Time of the last scan on source "}, {"name": "---", "desc": "[:] "}, {"name": "t2.m", "desc": "LST Time of the last scan on source "}, {"name": "tos", "desc": "Total on-source correlation time "}, {"name": "Type", "desc": "Program type (1) "}, {"name": "oEq", "desc": "? Original equinox of position (2) "}, {"name": "RAh", "desc": "? Right Ascension J2000 (hours) "}, {"name": "---", "desc": "[:] "}, {"name": "RAm", "desc": "? Right Ascension J2000 (minutes) "}, {"name": "---", "desc": "[:] "}, {"name": "RAs", "desc": "? Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? Declination J2000 (degrees) "}, {"name": "---", "desc": "[:] "}, {"name": "DEm", "desc": "? Declination J2000 (minutes) "}, {"name": "---", "desc": "[:] "}, {"name": "DEs", "desc": "? Declination J2000 (seconds) "}, {"name": "Vel", "desc": "Velocity of the source (3) "}, {"name": "n_Vel", "desc": "[LH] LSR or Heliocentric velocity "}, {"name": "Flow", "desc": "?=0 Sky Frequency of the 3mm receiver (6) "}, {"name": "n_Flow", "desc": "[UL] Signal Upper/Lower band of the 3mm receiver "}, {"name": "Fhigh", "desc": "?=0 Sky Frequency of the 1mm receiver (6) "}, {"name": "n_Fhigh", "desc": "[UL] Signal Upper/Lower band of the 1mm receiver "}, {"name": "pol", "desc": "[HV ] Horizontal/Vertical polarisations (6) "}, {"name": "p4", "desc": "[HV ] Polarisation of 4GHz continuum (6) "}, {"name": "Conf", "desc": "Configuration code of the interferometer "}, {"name": "Config", "desc": "Detailed configuration (4) "}]}, {"name": "noema_pi.dat", "desc": "List of PI investigators of Noema instrument ", "columns": [{"name": "Prog", "desc": "Identification code of the program "}, {"name": "PI", "desc": "Principal Investigator's name "}]}, {"name": "30m.dat", "desc": "List of observations at 30m instrument since 2009-09-30", "columns": [{"name": "Name", "desc": "Target source name "}, {"name": "sys", "desc": "[BJG] equinox system "}, {"name": "Eq", "desc": "? equinox year "}, {"name": "RAh", "desc": "[]? Right ascension (hours) J2000 "}, {"name": "---", "desc": "[:] "}, {"name": "RAm", "desc": "? Right ascension (minutes) J2000 "}, {"name": "---", "desc": "[:] "}, {"name": "RAs", "desc": "? Right ascension (seconds) J2000 "}, {"name": "DE-", "desc": "Declination (sign) J2000 "}, {"name": "DEd", "desc": "? Declination (degrees) J2000 "}, {"name": "---", "desc": "[:] "}, {"name": "DEm", "desc": "? Declination (minutes) J2000 "}, {"name": "---", "desc": "[:] "}, {"name": "DEs", "desc": "? Declination (seconds) J2000 "}, {"name": "Obs.Y", "desc": "Starting date of the Observation (year) (from ncsID)"}, {"name": "---", "desc": "[-] "}, {"name": "Obs.M", "desc": "Starting date of the Observation (month) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.D", "desc": "Starting date of the Observation (day) "}, {"name": "---", "desc": "[.] "}, {"name": "scan", "desc": "Scan No. (Date.scan = ncsID) "}, {"name": "t1.h", "desc": "? Starting time in UTC (hour) "}, {"name": "---", "desc": "? [:] "}, {"name": "t1.m", "desc": "? Starting time (min) "}, {"name": "---", "desc": "? [:] "}, {"name": "t1.s", "desc": "? Starting time (sec) "}, {"name": "t2.h", "desc": "? End time (hour) "}, {"name": "---", "desc": "? [:] "}, {"name": "t2.m", "desc": "? End time (min) "}, {"name": "---", "desc": "? [:] "}, {"name": "t2.s", "desc": "? End time (sec) "}, {"name": "obsMode", "desc": "Observation mode (1) "}, {"name": "Prog", "desc": "Identification code of the program "}, {"name": "tau", "desc": "? Zenith {tau} at 225 GHz from tipping taumeter "}, {"name": "receiv", "desc": "Short name of the receiver(band) used "}, {"name": "line", "desc": "Name of line observed "}, {"name": "Freq", "desc": "Frequency used for the observation "}]}, {"name": "30m_pi.dat", "desc": "List of PI investigators of 30m instrument ", "columns": [{"name": "Prog", "desc": "Identification code of the program "}, {"name": "PI", "desc": "Principal Investigator's name "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"B_afoev"}} {"id": "B/afoev", "title_cds": "Afoev catalogue", "title_create": "Schweitzer, 2008-", "year": "2008", "author": "E. Schweitzer, L. Vadrot, J. Minois, D. Naillon", "title_pub": "AFOEV catalogue", "first_author": "E. Schweitzer", "bibcode": ["References"], "keyword_cds": "Stars, variable", "abstract": ["Observations of Variable Stars collected by", "E. Schweitzer up to 2008 and then by L. Vadrot, J. Minois and D. Naillon", "Association Francaise des Observateurs d'Etoiles Variables", "STRASBOURG, France"], "alias": ["AFOEV"], "records": ["4780875 records"], "data": "", "date_update": "11-Aug-2022", "tables": [{"name": "afoev.dat", "desc": "AFOEV table ", "columns": [{"name": "Obs", "desc": "Observer's Acronym (see file observer) "}, {"name": "JD-2400000", "desc": "[12397.5/2449911.46] Observation date, offset 2400000"}, {"name": "n_mag", "desc": "? System in which mag is measured "}, {"name": "u_mag", "desc": "[<:?-/>Q0-9RN;]? Uncertainty mag "}, {"name": "mag", "desc": "Magnitude (in system defined by n_mag) "}, {"name": "Assoc", "desc": "? Association designation "}, {"name": "Name", "desc": "Star Name "}, {"name": "FileName", "desc": "Original filename "}]}, {"name": "afoev_list.dat", "desc": "AFOEV table list ", "columns": [{"name": "FileName", "desc": "Description of FileName "}, {"name": "Name", "desc": "Star Name "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"B_pn"}} {"id": "B/pn", "title_cds": "Atlas of Galactic Planetary Nebulae", "title_create": "Miszalski+ 2011", "year": "2011", "author": "Miszalski B., Acker A., Ochsenbein F., Parker Q.", "title_pub": "A digital Atlas of Galactic Planetary Nebulae", "first_author": "Miszalski B.", "ref_biblio": ["< (in preparation) >"], "bibcode": ["2010yCat.0....0M"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "records": ["records"], "data": "", "date_update": "16-Nov-2010"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"B_simbad"}} {"id": "B/simbad", "title_cds": "Simbad objects catalogue", "title_create": "M.Wenger 2000", "year": "2000", "author": "M.Wenger; Ochsenbein, F.; Egret, D.; Dubois, P.; Bonnarel, F.; Borde, S.; Genova, F.; Jasniewicz, G.; Laloe, S.; Lesteven, S.; Monier, R", "title_pub": "Simbad objects catalogue", "first_author": "M.Wenger; Ochsenbein", "ref_biblio": ["<2000A&AS..143....9W>"], "bibcode": ["2000A&AS..143....9W"], "keyword_cds": "Bibliography; Photometry; Positional data; Proper motions", "description": ["Simbad is the reference database for identification and bibliography of", "astronomical objects. It contains identifications, ``basic data'',", "bibliography, and selected observational measurements for several million", "astronomical objects. Simbad is developed and maintained by CDS, Strasbourg.", "Building the database contents is achieved with the help of several", "contributing institutes. Scanning the bibliography is the result of the", "collaboration of CDS with bibliographers in Observatoire de Paris (DASGAL),", "Institut d'Astrophysique de Paris, and Observatoire de Bordeaux. When", "selecting catalogues and tables for inclusion, priority is given to optimal", "multi-wavelength coverage of the database, and to support of research", "developments linked to large projects. In parallel, the systematic scanning", "of the bibliography reflects the diversity and general trends of", "astronomical research. A WWW interface to Simbad is available at:", "{http://simbad.u-strasbg.fr/Simbad}."], "alias": ["simbad"], "type": ["GCC"], "records": ["7000000 sources"], "doi_pub": ["10.1051/aas:2000332"], "data": "f", "islargetable": true, "date_creation": "12-Feb-2013", "date_update": "08-Aug-2018", "tables": [{"name": "simbad.out", "desc": "Simbad sample ", "columns": [{"name": "Id", "desc": "Main Simbad Identifier "}, {"name": "RAdeg", "desc": "Right ascention (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "errMaj", "desc": "?Half Major axis of the positional error "}, {"name": "errMin", "desc": "?Half Minor axis of the positional error "}, {"name": "errPA", "desc": "?Position angle of the positional error "}, {"name": "Bmag", "desc": "?Magnitude in B "}, {"name": "Vmag", "desc": "?Magnitude in V "}, {"name": "Rmag", "desc": "?Magnitude in R "}, {"name": "Jmag", "desc": "?Magnitude in J "}, {"name": "Hmag", "desc": "?Magnitude in H "}, {"name": "Kmag", "desc": "?Magnitude in K "}, {"name": "oType", "desc": "Object type "}, {"name": "pmRa", "desc": "?Proper motion in rigth ascention "}, {"name": "pmDe", "desc": "?Proper motion in declination "}, {"name": "sp", "desc": "Spectral type "}, {"name": "nBibCode", "desc": "Number of bibcode associated "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"I_253"}} {"id": "I/253", "title_cds": "STARNET", "title_create": "Roeser 1996", "year": "1996", "author": "Roeser S.", "title_pub": "STARNET, an updated GSC for minor planet observations", "first_author": "Roeser S.", "ref_biblio": [""], "see_also": ["http://ad.usno.navy.mil/wds/ : the WDS Home page", "V/111 : Fifth Catalog of Orbits of Visual Double Stars"], "keyword_cds": "Stars, double and multiple ; Positional data", "description": ["The Washington Double Star Catalog (WDS), maintained by the United", "States Naval Observatory, is the world's principal database of", "astrometric double and multiple star information. The WDS Catalog", "contains positions (J2000), discoverer designations, epochs, position", "angles, separations, magnitudes, spectral types, proper motions and", "when available, Durchmusterung numbers and notes for the components of", "84,486 systems based on 563,326 means. The current version (updated", "nightly) is available online. A brief summary and statistical analysis", "of the contents of the catalog are presented."], "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["WDS", "WDS\\_20001"], "type": ["GCC"], "records": ["84486 binaries"], "data": "", "date_update": "12-Aug-2012"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"I_286"}} {"id": "I/286", "title_cds": "The Astrometric Catalogue ARIHIP", "title_create": "Wielen+ 2001", "year": "2001", "author": "Wielen R., Schwan H., Dettbarn C., Lenhardt H., Jahreiss H., Jaehrling R., Khalisi E.", "title_pub": "Astrometric Catalogue ARIHIP containing stellar data selected from the Combination Catalogues FK6, GC+HIP, TYC2+HIP and from the HIPPARCOS Catalogue.", "first_author": "Wielen R.", "ref_biblio": [""], "bibcode": ["2001VeARI..40....1W"], "see_also": ["http://www.ari.uni-heidelberg.de/arihip/ : ARIHIP home page", "I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)", "I/264 : Sixth Catalogue of Fundamental Stars (FK6) (Wielen+ 2000)", "I/113 : General Catalogue of 33342 stars (GC) (Boss 1937)"], "keyword_cds": "Fundamental catalog ; Positional data ; Proper motions", "alias": ["ARIHIP"], "records": ["90842 stars"], "data": "", "date_update": "29-Oct-2014", "tables": [{"name": "arihcx01.dat", "desc": "The big astrometric Catalogue ARIHIP (lastr update: 2003-04-11)", "columns": [{"name": "HIP", "desc": "[1/120404] Hipparcos Catalog Number (I/239) (#1) "}, {"name": "FK6", "desc": "[4/6125]? FK6 number of the star (Wielen et al. I/264) (#2) "}, {"name": "n_FK6", "desc": "FK6 subsample (#3) (1) "}, {"name": "GC", "desc": "[1/33343]? General Catalogue number (I/113) (#4) "}, {"name": "TYC1", "desc": "[1/9537] Explain column (#5) "}, {"name": "TYC2", "desc": "[1/12111] Explain column (#5) "}, {"name": "TYC3", "desc": "[1] Tycho "}, {"name": "Sel", "desc": "Selected catalogue (#6) (2) "}, {"name": "---", "desc": "Reference flag for double systems (empty) (#7) "}, {"name": "RAh", "desc": "Right Ascension ICRS, Sp=J2000 (hours) (#8) "}, {"name": "RAm", "desc": "Right Ascension ICRS, Sp=J2000 (minutes) (#8) "}, {"name": "RAs", "desc": "Right Ascension ICRS, Sp=J2000 (seconds) (#8) "}, {"name": "DE-", "desc": "Declination ICRS, Sp=J2000 (sign) (#9) "}, {"name": "DEd", "desc": "Declination ICRS, Sp=J2000 (degrees) (#9) "}, {"name": "DEm", "desc": "Declination ICRS, Sp=J2000 (minutes) (#9) "}, {"name": "DEs", "desc": "Declination ICRS, Sp=J2000 (seconds) (#9) "}, {"name": "pmRA", "desc": "[-3257.91/6766.91] proper-motion component {mu}_{alpha}*_ (#10) "}, {"name": "pmDE", "desc": "[-5815.07/10328] proper motionn component {mu}_{delta}_ (#11) "}, {"name": "EpRA", "desc": "[89.87/92.33] Central RA epoch -1900 (#12) "}, {"name": "e_RA", "desc": "[0.28/17.44] Mean error on {alpha}* at EpRA (#13) "}, {"name": "e_pmRA", "desc": "[0.2/33.74] Mean error on pmRA (#14) "}, {"name": "EpDE", "desc": "[90.35/92.41] Central Declination epoch -1900 (#15) "}, {"name": "e_DE", "desc": "[0.3/10.88] Mean error on Declination (#16) "}, {"name": "e_pmDE", "desc": "[0.18/26.46] Mean error on pmDE (#17) "}, {"name": "plx", "desc": "[-29.58/549.01] Parallax of the star (#18) "}, {"name": "e_plx", "desc": "[0.04/20.8] Mean error on plx (#19) "}, {"name": "r_plx", "desc": "[HP] Origin of plx: H=Hippacros, P=photometric (#20) "}, {"name": "RV", "desc": "[-409/471]? Radial velocity of star (#21) "}, {"name": "Vmag", "desc": "[-0.62/14.08] Apparent visual magnitude of star (#22) "}, {"name": "f_Vmag", "desc": "[1/3]? variability of star (#23) (3) "}, {"name": "bin", "desc": "[11/99] Flag for the object binarity (#24) (4) "}, {"name": "Kp", "desc": "[1/2]? double-star nature of the object (#25) (5) "}, {"name": "Q", "desc": "[1/3]? astrometrically excellent star (#26) (6) "}, {"name": "dRA1", "desc": "[-206.34/334.92] LTP {Delta}{alpha}* (#27) (7) "}, {"name": "dRA2", "desc": "[-99.55/127.47] STP {Delta}{alpha}* (#28) (7) "}, {"name": "dRA3", "desc": "[-153.77/190.35] HIP {Delta}{alpha}* (#29) (7) "}, {"name": "dRA4", "desc": "[-15861/12259.9]? CAT1 {Delta}{alpha}* (#30) (7) "}, {"name": "dDE1", "desc": "[-251.7/232.99] LTP {Delta}{delta} (#31) (7) "}, {"name": "dDE2", "desc": "[-154.41/96.01] STP {Delta}{delta} (#32) (7) "}, {"name": "dDE3", "desc": "[-350.04/140.66] HIP {Delta}{delta} (#33) (7) "}, {"name": "dDE4", "desc": "[-7277.05/5483.3]? CAT1 {Delta}{delta}(#34) (7) "}, {"name": "dpmRA1", "desc": "[-24.87/40.64] LTP {Delta}{mu}_{alpha}*_ (#35) (7) "}, {"name": "dpmRA2", "desc": "[-11.03/14.59] STP {Delta}{mu}_{alpha}*_ (#36) (7) "}, {"name": "dpmRA3", "desc": "[-17.24/20.76] HIP {Delta}{mu}_{alpha}*_ (#37) (7) "}, {"name": "dpmRA4", "desc": "[-129.35/146.72]? CAT1 {Delta}{mu}_{alpha}*_ (#38) (7) "}, {"name": "dpmRA5", "desc": "[-28.93/62.39]? mu0 {Delta}{mu}_{alpha}*_ (#39) (7) "}, {"name": "dpmDE1", "desc": "[-29.99/25.87] LTP {Delta}{mu}_{delta}_ (#40) (7) "}, {"name": "dpmDE2", "desc": "[-17.69/11.04] STP {Delta}{mu}_{delta}_ (#41) (7) "}, {"name": "dpmDE3", "desc": "[-42.38/16.27] HIP {Delta}{mu}_{delta}_ (#42) (7) "}, {"name": "dpmDE4", "desc": "[-79.24/80.87]? CAT1 {Delta}{mu}_{delta}_ (#43) (7) "}, {"name": "dpmDE5", "desc": "[-39.43/28.18]? mu0 {Delta}{mu}_{delta}_ (#44) (7) "}, {"name": "EpRA1", "desc": "[1957.05/1992.27] LTP RA epoch (#45) "}, {"name": "EpRA2", "desc": "[1989.87/1992.33] STP RA epoch (#46) "}, {"name": "EpRA3", "desc": "[1989.87/1992.38] HIP RA epoch (#47) "}, {"name": "EpRA4", "desc": "[1877.5/1992.47]? CAT1 RA epoch (#48) "}, {"name": "eRA1", "desc": "[0.33/18.57] LTP {epsilon}_{alpha}*_ (#49) "}, {"name": "eRA2", "desc": "[0.28/17.44] STP {epsilon}_{alpha}*_ (#50) "}, {"name": "eRA3", "desc": "[0.28/17.44] HIP {epsilon}_{alpha}*_ (#51) "}, {"name": "eRA4", "desc": "[3/326.77]? CAT1 {epsilon}_{alpha}*_ (#52) "}, {"name": "pmRA1", "desc": "[0.24/33.74] LTP {epsilon}_{mu}{alpha}*_ (#53) "}, {"name": "pmRA2", "desc": "[0.3/33.74] STP {epsilon}_{mu}{alpha}*_ (#54) "}, {"name": "pmRA3", "desc": "[0.31/33.74] HIP {epsilon}_{mu}{alpha}*_ (#55) "}, {"name": "pmRA4", "desc": "[0.3/40.03]? CAT1 {epsilon}_{mu}{alpha}*_ (#56) "}, {"name": "pmRA5", "desc": "[0.24/8.58]? mu0 {epsilon}_{mu}{alpha}*_ (#57) "}, {"name": "EpDE1", "desc": "[1954.47/1992.41] LTP {delta} epoch (#58) "}, {"name": "EpDE2", "desc": "[1990.35/1992.41] STP {delta} epoch (#59) "}, {"name": "EpDE3", "desc": "[1990.32/1992.5] HIP {delta} epoch (#60) "}, {"name": "EpDE4", "desc": "[1876.8/1991.96]? CAT1 {delta} epoch (#61) "}, {"name": "eDE1", "desc": "[0.36/18.44] LTP {epsilon}_{delta} (#62) "}, {"name": "eDE2", "desc": "[0.3/10.88] STP {epsilon}_{delta} (#63) "}, {"name": "eDE3", "desc": "[0.3/10.88] HIP {epsilon}_{delta} (#64) "}, {"name": "eDE4", "desc": "[3/282.26]? CAT1 {epsilon}_{delta} (#65) "}, {"name": "pmDE1", "desc": "[0.21/26.52] LTP {epsilon}_{mu}{delta}_ (#66) "}, {"name": "pmDE2", "desc": "[0.31/26.46] STP {epsilon}_{mu}{delta}_ (#67) "}, {"name": "pmDE3", "desc": "[0.32/26.46] HIP {epsilon}_{mu}{delta}_ (#68) "}, {"name": "pmDE4", "desc": "[0.3/43]? CAT1 {epsilon}_{mu}{delta}_ (#69) "}, {"name": "pmDE5", "desc": "[0.23/14.65]? mu0 {epsilon}_{mu}{delta}_ (#70) "}, {"name": "plx0", "desc": "[-29.58/548.37] SI parallax (#71) "}, {"name": "plx1", "desc": "[-29.58/548.82] LTP parallax (#72) "}, {"name": "plx3", "desc": "[-29.58/549.01] HIP parallax (#73) "}, {"name": "eplx0", "desc": "[0.42/20.8] SI error on parallax (#74) "}, {"name": "eplx1", "desc": "[0.42/20.8] LTP error on parallax (#75) "}, {"name": "eplx3", "desc": "[0.42/20.8] HIP error on parallax (#76) "}, {"name": "da", "desc": "[-325.11/401.93]? {Delta}{alpha}*_sys_ (#77) "}, {"name": "dd", "desc": "[-283.52/228.76]? {Delta}{delta}_sys_ (#78) "}, {"name": "dpa", "desc": "[-11.9/12.21]? {Delta}{mu}_{alpha}*sys_ (#79) "}, {"name": "dpd", "desc": "[-13.57/14.33]? {Delta}{mu}_{delta}sys_ (#80) "}, {"name": "ea", "desc": "[5.63/41.88]? {epsilon}{alpha}*_sys_ (#81) "}, {"name": "ed", "desc": "[5.38/38.07]? {epsilon}{delta}_sys_ (#82) "}, {"name": "epa", "desc": "[0.21/1.82]? {epsilon}{mu}{alpha}*_sys_ (#83) "}, {"name": "epd", "desc": "[0.13/1.9]? {epsilon}{mu}{delta}_sys_ (#84) "}, {"name": "Kpos", "desc": "[1/1]? Flag indicating that the star was used in the comparison of positions in CAT1 and HIP (#85) "}, {"name": "Kpm", "desc": "[1/1]? Flag indicating that the star was used in the comparison of proper motions in CAT1 and HIP (#86) "}, {"name": "F(FH)", "desc": "[0.03/28.32]? F parameter based on the difference Delta_mu_{FH} = mu_F - mu_H between "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"I_288"}} {"id": "I/288", "title_cds": "Low-luminosity members of the Hyades cluster", "title_create": "van Altena, 1966", "year": "1966", "author": "Van Altena W.F.", "title_pub": "Low-luminosity members of the Hyades cluster", "first_author": "Van Altena W.F.", "ref_biblio": [""], "bibcode": ["1966AJ.....71..482V", "1966AJ.....71..482V", "2013yCat.1288....0V"], "keyword_cds": "Clusters, open ; Positional data ;", "keyword_pub": "", "curator": "Francois Ochsenbein [CDS]", "alias": ["VA"], "type": ["OC"], "records": ["778 stars"], "doi_pub": ["10.1086/109952"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"I_301"}} {"id": "I/301", "title_cds": "WDS 2005", "title_create": "Mason+ 2005", "year": "2005", "author": "Brian D. Mason, Gary L. Wycoff, William I. Hartkopf, Geoffrey G. Douglass, Charles E. Worley", "title_pub": "The Washington Visual Double Star Catalog, Version 2005-05-09", "first_author": "Brian D. Mason", "ref_biblio": ["< Astrometry Department, U.S. Naval Observatory >"], "see_also": ["http://ad.usno.navy.mil/wds/ : the WDS home page"], "keyword_cds": "Stars, double and multiple ; Positional data", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["WDS", "WDS\\_2005"], "type": ["GCC"], "records": ["102234 binaries"], "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"I_314"}} {"id": "I/314", "title_cds": "Second Hispano-Argentinian Meridian Catalogue (HAMC2)", "title_create": "HAMC, 2008", "year": "2008", "author": "HAMC", "title_pub": "Second Hispano-Argentinian Meridian Catalogue. Observations from December 1999 to May 2007.", "first_author": "HAMC", "ref_biblio": [""], "keyword_cds": "Meridian observations ; Surveys ; Positional data ; Photometry, CCD", "keyword_pub": "astrometry -- catalogs -- methods: data analysis", "abstract": ["The Brorfelde Schmidt CCD Catalog (BSCC) contains about 13.7 million", "stars, north of +49{deg} Declination with precise positions and V, R", "photometry. The catalog has been constructed from the reductions of", "18,667 CCD frames observed with the Brorfelde Schmidt Telescope", "between 2000 and 2007. The Tycho-2 catalog was used for astrometric", "and photometric reference stars. Errors of individual positions are", "about 20 to 200 mas for stars in the R = 10 to 18 mag range. External", "comparisons with 2MASS and SDSS reveal possible small systematic", "errors in the BSCC of up to about 30 mas. The catalog is supplemented", "with J, H, and Ks magnitudes from the 2MASS catalog."], "description": ["All data are on a single file, formatted (ASCII), sorted by", "declination. Positions are mean, observed positions on the", "International Celestial Reference System (ICRS, as represented by the", "Tycho-2 catalog) at mean epoch of observation. There are no proper", "motions provided in the BSCC. There are 13,771,775 data rows (stars).", "Stars are identified by the IAU registered acronym \"BSCC\", followed by", "a fixed-length, 8-digit running record number without a space, thus", "star names are BSCC00000001 to BSCC13771775."], "curator": "Francois Ochsenbein [CDS]", "alias": ["BSCC"], "type": ["OC"], "records": ["13771775 stars"], "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"I_336"}} {"id": "I/336", "title_cds": "Gaia rehearsal test data", "title_create": "Gaia consortium, 2016", "year": "2016", "author": "Gaia consortium", "title_pub": "Gaia rehearsal test data", "first_author": "Gaia consortium", "ref_biblio": [""], "bibcode": ["2016yCat.1336....0G"], "keyword_cds": "Positional data", "keyword_pub": "catalogs - surveys - astrometry", "mission": "Gaia", "abstract": ["Gaia CU9 rehearsal data. This catalogue provides simulated Gaia data and is", "for testing purposes only."], "alias": ["Gaia test data"], "type": ["OC"], "records": ["1079921303 records"], "data": "", "islargetable": true, "date_update": "01-Sep-2016", "tables": [{"name": "gaia.sam", "desc": "Sample of GaiaSource test data ", "columns": [{"name": "srcId", "desc": "(source_id) "}, {"name": "RAJ2000", "desc": "Right ascension in ICRS at epoch \"ref_epoch\" (ra)"}, {"name": "DEJ2000", "desc": "Declination in ICRS at epoch \"ref_epoch\" (dec)"}, {"name": "solution_id", "desc": "(solution_id) "}, {"name": "random_index", "desc": "? (random_index) "}, {"name": "ref_epoch", "desc": "(ref_epoch) "}, {"name": "e_RAJ2000", "desc": "(ra_error) "}, {"name": "e_DEJ2000", "desc": "(dec_error) "}, {"name": "Plx", "desc": "? (parallax) "}, {"name": "e_Plx", "desc": "? (parallax_error) "}, {"name": "pmRA", "desc": "? Proper motion in right ascension (pmra)"}, {"name": "e_pmRA", "desc": "? Standard error of proper motion in right ascension (pmra_error)"}, {"name": "pmDE", "desc": "? Proper motion in declination (pmdec)"}, {"name": "e_pmDE", "desc": "? Standard error of proper motion in declination (pmdec_error)"}, {"name": "ra_dec_corr", "desc": "? (ra_dec_corr) "}, {"name": "ra_parallax_corr", "desc": "? (ra_parallax_corr) "}, {"name": "ra_pmra_corr", "desc": "? (ra_pmra_corr) "}, {"name": "ra_pmdec_corr", "desc": "? (ra_pmdec_corr) "}, {"name": "dec_parallax_corr", "desc": "? (dec_parallax_corr) "}, {"name": "dec_pmra_corr", "desc": "? (dec_pmra_corr) "}, {"name": "dec_pmdec_corr", "desc": "? (dec_pmdec_corr) "}, {"name": "parallax_pmra_corr", "desc": "? (parallax_pmra_corr) "}, {"name": "parallax_pmdec_corr", "desc": "? (parallax_pmdec_corr) "}, {"name": "pmra_pmdec_corr", "desc": "? (pmra_pmdec_corr) "}, {"name": "astro_n_obs_al", "desc": "? (astrometric_n_obs_ac) "}, {"name": "astro_n_obs_ac", "desc": "? (astrometric_n_obs_al) "}, {"name": "astro_n_outliers_al", "desc": "? (astrometric_n_outliers_al) "}, {"name": "astro_n_outliers_ac", "desc": "? (astrometric_n_outliers_ac) "}, {"name": "astro_chi2_al", "desc": "? (astrometric_chi2_al) "}, {"name": "astro_chi2_ac", "desc": "? (astrometric_chi2_ac) "}, {"name": "astro_xs_noise", "desc": "? (astrometric_excess_noise) "}, {"name": "astro_xs_noise_sig", "desc": "(astrometric_excess_noise_sig) "}, {"name": "astro_params_solved", "desc": "(astrometric_params_solved) "}, {"name": "astro_primary_flag", "desc": "(astrometric_primary_flag) "}, {"name": "astro_rel_factor", "desc": "(astrometric_relegation_factor) "}, {"name": "astro_weight_al", "desc": "? (astrometric_weight_al) "}, {"name": "astro_weight_ac", "desc": "? (astrometric_weight_ac) "}, {"name": "astro_priors_used", "desc": "(astrometric_priors_used) "}, {"name": "matched_obs", "desc": "(matched_observations) "}, {"name": "scan_dir_strength_k1", "desc": "? Mean position angle of scan directions across the source"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"I_41"}} {"id": "I/41", "title_cds": "Catalogue of 964 Stars, Zones +5 to +15", "title_create": "Fayet, 1963", "year": "1963", "author": "Fayet G.", "title_pub": "Etoiles intermediaires (zone +5 a +15deg): catalogue deduit des positions observees a l'aide du cercle meridien de l' Observatoire de Nice de 1912 a 1914", "first_author": "Fayet G.", "ref_biblio": [""], "keyword_cds": "Positional data", "description": ["This catalog contains meridian circle positions for 4 to 6 stars in", "each hour of right ascension, between the eighth and ninth magnitude,", "and in the declination range +5 deg. to +15 deg. The equinox of the", "positions is 1910.0. Mean errors in right ascension range from 0.025s", "to 0.30s. Those in declination range from 0.47\" to 0.58\". The catalog", "also contains a running number, the magnitude, from the \"Henry Draper", "Catalog\" when available, annual precession and secular variation, and", "the number of observations and their mean date. Proper motions have", "not been included in the reduction of the positions."], "records": ["964 stars"], "data": "", "date_update": "21-Jan-2019", "tables": [{"name": "data_01.dat", "desc": "Data ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"I_999"}} {"id": "I/999", "title_cds": "Test Gaia", "title_create": "Gaia collaboration, 2022", "year": "2022", "author": "Gaia collaboration", "title_pub": "Gaia Data Release 3 (Gaia DR3) Part 1: Main source.", "first_author": "Gaia collaboration", "ref_biblio": [""], "bibcode": ["2022yCat.1355....0G"], "see_also": ["I/355 : Gaia DR3 Part 1: Main sources", "I/356 : Gaia DR3 Part 2: Extra-galactic", "I/357 : Gaia DR3 Part 3: Non-single stars", "I/358 : Gaia DR3 Part 4: Variability", "I/359 : Gaia DR3 Part 5: Solar System", "I/360 : Gaia DR3 Part 6: Performance verification"], "keyword_cds": "Surveys ; Stars, standard ; Positional data ; Proper motions ; Photometry, photographic ; Cross identifications ; Radial velocities ; Stars, variable ; Minor planets; Parallaxes, trigonometric", "keyword_pub": "catalogs - astrometry - parallaxes - proper motions - techniques: photometric - techniques: radial velocities", "mission": "Gaia", "abstract": ["Gaia Data Release 3 (Gaia DR3) will be released on 13 June 2022.", "The Gaia DR3 catalogue builds upon the Early Data Release 3 (released", "on 3 December 2020) and combines, for the same stretch of time and the", "same set of observations, these already-published data products with", "numerous new data products such as extended objects and non-single", "stars."], "description": ["The set of data released as Gaia Early Data Release 3 (Gaia EDR3) on 3", "December 2020 comprises:", "The full astrometric solution --- positions on the sky ({alpha},", "{delta}), parallaxes, and proper motions --- for around 1.46 billion", "(1.46*10^9^) sources, with a limiting magnitude of about G=~21 and a", "bright limit of about G=~3. The astrometric solution is accompanied", "with some new quality indicators, like RUWE, and source image", "descriptors. The full astrometric solution has been done as", "5-parameter solution for 585 million sources and as 6-parameter", "solution for 882 million sources. In the 6-parameter solution, the", "additional fitted quantity is the so-called pseudo-colour that had to", "be included for sources without high-quality colour information. In", "addition, two-parameters solutions --- positions on the sky ({alpha},", "{delta}) --- for around 344 million additional sources. G magnitudes", "for around 1.806 billion sources (with the known issue present in EDR3", "corrected in Gaia DR3). GBP and GRP magnitudes for around 1.54 billion", "and 1.55 billion sources, respectively.", "In Gaia Data Release 3 (Gaia DR3), the above set of data is", "complemented with new products released on 13 June 2022 (EAS", "presentation A. Vallenari):", "Object classifications for 1.59 billion sources and astrophysical", "parameters (Teff, logg, [M/H], AG, distance, etc.) from BP/RP spectra", "for 470 million objects, including MCMC samples for most sources with", "astrophysical parameters (EAS presentation O.Creevey). Other", "astrophysical parameters from the BP/RP spectra include:", "Spectral types (217 million stars) and emission-line star", "classifications (57,000 stars);", "Spectroscopic parameters for 2.3 million hot stars, 94,000 ultra-cool", "stars, activity index for 1.3 million cool stars, and H-alpha emission", "for 235 million stars;", "Evolutionary parameters (mass and age) for 128 million stars;", "Astrophysical parameters for 348 million objects based on the", "assumption of an unresolved binary in the BP/RP spectra;", "Self-organised map (outlier) analysis based on 56 million sources with", "the weakest object classifications. Astrophysical parameters (Teff,", "logg, [M/H], [X/M] for 12 elements, etc.) from RVS spectra for 5.5", "million objects, including diffuse interstellar bands for 472,000", "objects.", "All-sky total galactic extinction maps at 4 different spatial", "resolutions (HEALPix levels 6, 7, 8, and 9).", "Mean BP/RP spectra for 219 million sources, most of them with G < 17.6", "mag (EAS Presentation F. De Angeli).", "Mean RVS spectra for 1 million well-behaved objects (EAS presentation", "P. Sartoretti).", "Mean radial velocities for 33 million stars and mean GRVS magnitudes", "for 32 million objects with G_RVS_<~14mag with effective temperatures", "(Teff) in the range of ~3100 to 14500K (EAS presentation P.", "Sartoretti).", "Rotational velocities for 3.5 million sources with G_RVS_<~12mag.", "Variability analysis, together with the underlying epoch photometry,", "for 10.5 million sources. Apart from classification into 24", "variability classes, detailed variability results are provided in", "separate tables for the following candidates (EAS presentation L.", "Eyer):", "Cepheids (15,021 objects);", "Compact companions (6306 objects);", "Eclipsing binaries (2,184,477 objects);", "Long-period variables (1,720,588 objects);", "Microlensing events (363 objects);", "Planetary transits (214 objects);", "RR Lyrae stars (271,779 objects);", "Short-timescale variables (471,679 objects);", "Solar-like rotational modulation variables (474,026 objects);", "Upper-main-sequence oscillators (54,476 objects);", "Active galactic nuclei (872,228 objects).", "Solar-system results for 158,000 sources (including 31 planetary", "satellites), with orbital solutions and individual epoch observations", "for 154,000 objects and with mean BP/RP reflectance spectra for more", "than 60,000 objects (EAS presentation P. Tanga). Some 813,000", "non-single stars, including amongst others non-single-star models for", "sources compatible with an astrometric acceleration solution,", "non-single-star orbital models for spectroscopic binaries compatible", "with a trend, and non-single-star orbital models for sources", "compatible with a two-body solution (EAS presentation F. Arenou).", "Some 6.6 million quasar candidates with redshift estimates for most of", "them (EAS presentation L. Galluccio).", "Some 1.1 million quasars analysed with 60,000 host galaxies detected", "and 15,000 surface brightness profiles of the host galaxy.", "Some 4.8 million galaxy candidates with redshift estimates for more", "than 1 million objects (EAS presentation L. Galluccio).", "Some 900,000 galaxies analysed with two surface brightness profiles.", "The Gaia Andromeda Photometric Survey (GAPS), consisting of the", "photometric time series for all 1.2 million sources located in a", "5.5-degree radius field centred on the Andromeda galaxy.", "Selected tables from Gaia Collaboration performance verification", "papers published with Gaia DR3.", "All 2612 science alerts triggered in the period underlying Gaia DR3.", "The new data set neither contains new astrometry nor new photometric", "calibrations such that the following elements are in common for and", "apply to both Gaia EDR3 and Gaia DR3:", "About 1.61 million celestial reference frame (Gaia-CRF3) sources.", "Cross-matches between Gaia (E)DR3 sources on the one hand and", "Hipparcos-2, Tycho-2 + TDSC merged, 2MASS PSC (merged with 2MASS XSC),", "SDSS DR13, Pan-STARRS1 DR1, SkyMapper DR2, GSC 2.3, APASS DR9, RAVE", "DR5, allWISE, URAT-1, and RAVE DR6 data on the other hand.", "Additionally, a Gaia DR2 to Gaia (E)DR3 match table.", "Full photometric passband definitions for G, GBP, GRP, and GRVS. More", "information is available here. Please be aware that the photometric", "system for the G, GBP, and GRP bands in Gaia (E)DR3 is different from", "the photometric systems as used in Gaia DR2 and in Gaia DR1.", "Simulated data from the Gaia Object Generator (GOG) and the Gaia", "Universe Model Snapshot (GUMS).", "The commanded scan law covering the Gaia (E)DR3 data collection", "period. Also the major periods where data was not sent to the ground", "or could not be processed are identified.", "All of the above combined makes up the full Gaia Data Release 3."], "alias": ["Gaia Gaia-DR3"], "type": ["OC"], "records": ["219197643 sources"], "data": "f", "islargetable": true, "date_creation": "13-Jun-2022", "date_update": "20-Jun-2022", "tables": [{"name": "gaiadr3.sam", "desc": "Gaia DR3 source catalog (1811709771 sources) ", "columns": [{"name": "DR3Name", "desc": "Unique source designation (unique across all Data Releases) (designation)"}, {"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2016.0 (ra)"}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2016.0 (dec) "}, {"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "Source", "desc": "Unique source identifier (unique within a particular Data Release) (source_id)"}, {"name": "RandomI", "desc": "Random index for use when selecting subsets (random_index)"}, {"name": "e_RAdeg", "desc": "Standard error of right ascension (ra_error)"}, {"name": "e_DEdeg", "desc": "Standard error of declination (dec_error)"}, {"name": "Plx", "desc": "? Parallax (parallax) "}, {"name": "e_Plx", "desc": "? Standard error of parallax (parallax_error)"}, {"name": "RPlx", "desc": "? Parallax divided by its standard error (parallax_over_error)"}, {"name": "PM", "desc": "? Total proper motion (pm) "}, {"name": "pmRA", "desc": "? Proper motion in right ascension direction, pmRA*cosDE (pmra)"}, {"name": "e_pmRA", "desc": "? Standard error of proper motion in right ascension direction (pmra_error)"}, {"name": "pmDE", "desc": "? Proper motion in declination direction (pmdec)"}, {"name": "e_pmDE", "desc": "? Standard error of proper motion in declination direction (pmdec_error)"}, {"name": "RADEcor", "desc": "[-1/1] Correlation between right ascension and declination (ra_dec_corr)"}, {"name": "RAPlxcor", "desc": "[-1/1]? Correlation between right ascension and parallax (ra_parallax_corr)"}, {"name": "RApmRAcor", "desc": "[-1/1]? Correlation between right ascension and proper motion in right ascension (ra_pmra_corr)"}, {"name": "RApmDEcor", "desc": "[-1/1]? Correlation between right ascension and proper motion in declination (ra_pmdec_corr)"}, {"name": "DEPlxcor", "desc": "[-1/1]? Correlation between declination and parallax (dec_parallax_corr)"}, {"name": "DEpmRAcor", "desc": "[-1/1]? Correlation between declination and proper motion in right ascension (dec_pmra_corr)"}, {"name": "DEpmDEcor", "desc": "[-1/1]? Correlation between declination and proper motion in declination (dec_pmdec_corr)"}, {"name": "PlxpmRAcor", "desc": "[-1/1]? Correlation between parallax and proper motion in right ascension (parallax_pmra_corr)"}, {"name": "PlxpmDEcor", "desc": "[-1/1]? Correlation between parallax and proper motion in declination (parallax_pmdec_corr)"}, {"name": "pmRApmDEcor", "desc": "[-1/1]? Correlation between proper motion in right ascension and proper motion in declination (pmra_pmdec_corr)"}, {"name": "NAL", "desc": "Total number of observations in the along-scan (AL) direction (astrometric_n_obs_al)"}, {"name": "NAC", "desc": "Total number of observations in the across-scan (AC) direction (astrometric_n_obs_ac)"}, {"name": "NgAL", "desc": "Number of good observations in the along-scan (AL) direction (astrometric_n_good_obs_al)"}, {"name": "NbAL", "desc": "Number of bad observations in the along-scan (AL) direction (astrometric_n_bad_obs_al)"}, {"name": "gofAL", "desc": "Goodness of fit statistic of model wrt along-scan observations (astrometric_gof_al)"}, {"name": "chi2AL", "desc": "AL chi-square value (astrometric_chi2_al)"}, {"name": "epsi", "desc": "Excess noise of the source (astrometric_excess_noise)"}, {"name": "sepsi", "desc": "Significance of excess noise (astrometric_excess_noise_sig)"}, {"name": "Solved", "desc": "[3/95] Which parameters have been solved for? (astrometric_params_solved) (1)"}, {"name": "APF", "desc": "[0/1] Primary or secondary (astrometric_primary_flag)"}, {"name": "nueff", "desc": "? Effective wavenumber of the source used in the astrometric solution (nu_eff_used_in_astrometry)"}, {"name": "pscol", "desc": "? Astrometrically estimated pseudocolour of the source (pseudocolour)"}, {"name": "e_pscol", "desc": "? Standard error of the pseudocolour of the source (pseudocolour_error)"}, {"name": "RApscolCorr", "desc": "[-1/1]? Correlation between right ascension and pseudocolour (ra_pseudocolour_corr)"}, {"name": "DEpscolCorr", "desc": "[-1/1]? Correlation between declination and pseudocolour (dec_pseudocolour_corr)"}, {"name": "PlxpscolCorr", "desc": "[-1/1]? Correlation between parallax and pseudocolour (parallax_pseudocolour_corr)"}, {"name": "pmRApscolCorr", "desc": "[-1/1]? Correlation between proper motion in right ascension and pseudocolour (pmra_pseudocolour_corr)"}, {"name": "pmDEpscolCorr", "desc": "[-1/1]? Correlation between proper motion in declination and pseudocolour (pmdec_pseudocolour_corr)"}, {"name": "MatchObsA", "desc": "Matched FOV transits used in the AGIS solution (astrometric_matched_transits)"}, {"name": "Nper", "desc": "[1/33] Number of visibility periods used in Astrometric solution (visibility_periods_used)"}, {"name": "amax", "desc": "The longest semi-major axis of the 5-d error ellipsoid (astrometric_sigma5d_max)"}, {"name": "MatchObs", "desc": "The number of transits matched to this source (matched_transits)"}, {"name": "NewMatchObs", "desc": "The number of transits newly incorporated into an existing source in the current cycle (new_matched_transits)"}, {"name": "MatchObsrm", "desc": "The number of transits removed from an existing source in the current cycle (matched_transits_removed)"}, {"name": "IPDgofha", "desc": "Amplitude of the IPD GoF versus position angle of scan (ipd_gof_harmonic_amplitude)"}, {"name": "IPDgofhp", "desc": "Phase of the IPD GoF versus position angle of scan (ipd_gof_harmonic_phase)"}, {"name": "IPDfmp", "desc": "[0/100] Percent of successful-IPD windows with more than one peak (ipd_frac_multi_peak)"}, {"name": "IPDfow", "desc": "[0/100] Percent of transits with truncated windows or multiple gate (ipd_frac_odd_win)"}, {"name": "RUWE", "desc": "? Renormalised unit weight error (ruwe)"}, {"name": "SDSk1", "desc": "? Degree of concentration of scan directions across the source (scan_direction_strength_k1)"}, {"name": "SDSk2", "desc": "? Degree of concentration of scan directions across the source (scan_direction_strength_k2)"}, {"name": "SDSk3", "desc": "? Degree of concentration of scan directions across the source (scan_direction_strength_k3)"}, {"name": "SDSk4", "desc": "? Degree of concentration of scan directions across the source (scan_direction_strength_k4)"}, {"name": "SDMk1", "desc": "? Mean position angle of scan directions across the source (scan_direction_mean_k1)"}, {"name": "SDMk2", "desc": "? Mean position angle of scan directions across the source (scan_direction_mean_k2)"}, {"name": "SDMk3", "desc": "? Mean position angle of scan directions across the source (scan_direction_mean_k3)"}, {"name": "SDMk4", "desc": "? Mean position angle of scan directions across the source (scan_direction_mean_k4)"}, {"name": "Dup", "desc": "[0/1] Source with multiple source identifiers (duplicated_source)"}, {"name": "o_Gmag", "desc": "Number of observations contributing to G photometry (phot_g_n_obs)"}, {"name": "FG", "desc": "? G-band mean flux (phot_g_mean_flux) "}, {"name": "e_FG", "desc": "? Error on G-band mean flux (phot_g_mean_flux_error)"}, {"name": "RFG", "desc": "? G-band mean flux divided by its error (phot_g_mean_flux_over_error)"}, {"name": "Gmag", "desc": "? G-band mean magnitude (phot_g_mean_mag)"}, {"name": "e_Gmag", "desc": "? Error on G-band mean magnitude (added by CDS) (phot_g_mean_mag_error)"}, {"name": "o_BPmag", "desc": "Number of observations contributing to BP photometry (phot_bp_n_obs)"}, {"name": "FBP", "desc": "? Integrated BP mean flux (phot_bp_mean_flux)"}, {"name": "e_FBP", "desc": "? Error on the integrated BP mean flux (phot_bp_mean_flux_error)"}, {"name": "RFBP", "desc": "? Integrated BP mean flux divided by its error (phot_bp_mean_flux_over_error)"}, {"name": "BPmag", "desc": "? Integrated BP mean magnitude (phot_bp_mean_mag)"}, {"name": "e_BPmag", "desc": "? Error on integrated BP mean magnitude (added by CDS) (phot_bp_mean_mag_error)"}, {"name": "o_RPmag", "desc": "Number of observations contributing to RP photometry (phot_rp_n_obs)"}, {"name": "FRP", "desc": "? Integrated RP mean flux (phot_rp_mean_flux)"}, {"name": "e_FRP", "desc": "? Error on the integrated RP mean flux (phot_rp_mean_flux_error)"}, {"name": "RFRP", "desc": "? Integrated RP mean flux divided by its error (phot_rp_mean_flux_over_error)"}, {"name": "RPmag", "desc": "? Integrated RP mean magnitude (phot_rp_mean_mag)"}, {"name": "e_RPmag", "desc": "? Error on integrated RP mean magnitude (added by CDS) (phot_rp_mean_mag_error)"}, {"name": "E(BP/RP)", "desc": "? Photometry processing mode (phot_proc_mode)"}, {"name": "NBPcont", "desc": "? BP/RP excess factor (phot_bp_rp_excess_factor)"}, {"name": "NBPblend", "desc": "? Number of BP contaminated transits (phot_bp_n_contaminated_transits)"}, {"name": "NRPcont", "desc": "? Number of BP blended transits (phot_bp_n_blended_transits)"}, {"name": "NRPblend", "desc": "? Number of RP contaminated transits (phot_rp_n_contaminated_transits)"}, {"name": "Mode", "desc": "[0/2]? Number of RP blended transits (phot_rp_n_blended_transits)"}, {"name": "BP-RP", "desc": "? BP-RP colour (bp_rp) "}, {"name": "BP-G", "desc": "? BP-G colour (bp_g) "}, {"name": "G-RP", "desc": "? G-RP colour (g_rp) "}, {"name": "RV", "desc": "? Radial velocity (radial_velocity) "}, {"name": "e_RV", "desc": "? Radial velocity error (radial_velocity_error)"}, {"name": "n_RV", "desc": "[0/2]? Method used to obtain the radial velocity (rv_method_used)"}, {"name": "o_RV", "desc": "? Number of transits used to compute the radial velocity (rv_nb_transits)"}, {"name": "o_RVd", "desc": "? Number of valid transits that have undergone deblending (rv_nb_deblended_transits)"}, {"name": "RVNper", "desc": "[0/33]? Number of visibility periods used to estimate the radial velocity (rv_visibility_periods_used)"}, {"name": "RVS/N", "desc": "? Expected signal to noise ratio in the combination of the spectra used to obtain the radial velocity (rv_expected_sig_to_noise)"}, {"name": "RVgof", "desc": "? Radial velocity renormalised goodness of fit (rv_renormalised_gof)"}, {"name": "RVchi2", "desc": "? P-value for constancy based on a chi-squared criterion (rv_chisq_pvalue)"}, {"name": "RVTdur", "desc": "? Time coverage of the radial velocity time series (rv_time_duration)"}, {"name": "RVamp", "desc": "? Total amplitude in the radial velocity time series after outlier removal (rv_amplitude_robust)"}, {"name": "RVtempTeff", "desc": "? Teff of the template used to compute the radial velocity (rv_template_teff)"}, {"name": "RVtemplogg", "desc": "? Logg of the template used to compute the radial velocity (rv_template_logg)"}, {"name": "RVtemp[Fe/H]", "desc": "? [Fe/H] of the template used to compute the radial velocity (rv_template_fe_h)"}, {"name": "Vatmparam", "desc": "? Origin of the atmospheric parameters associated to the template (rv_atm_param_origin)"}, {"name": "Vbroad", "desc": "? Spectral line broadening parameter "}, {"name": "e_Vbroad", "desc": "? Uncertainty on the spectral line broadening (vbroad_error)"}, {"name": "o_Vbroad", "desc": "? Number of transits used to compute vbroad (vbroad_nb_transits)"}, {"name": "GRVSmag", "desc": "? Integrated Grvs magnitude (grvs_mag) "}, {"name": "e_GRVSmag", "desc": "? Grvs magnitude uncertainty (grvs_mag_error)"}, {"name": "o_GRVSmag", "desc": "? Number of transits used to compute Grvs (grvs_mag_nb_transits)"}, {"name": "RVSS/N", "desc": "? Signal to noise ratio in the mean RVS spectrum (rvs_spec_sig_to_noise)"}, {"name": "VarFlag", "desc": "Photometric variability flag (phot_variable_flag)"}, {"name": "GLON", "desc": "Galactic longitude (l) "}, {"name": "GLAT", "desc": "Galactic latitude (b) "}, {"name": "ELON", "desc": "Ecliptic longitude (ecl_lon) "}, {"name": "ELAT", "desc": "Ecliptic latitude (ecl_lat) "}, {"name": "QSO", "desc": "[0/1] Flag indicating the availability of additional information in the QSO candidates table (in_qso_candidates)"}, {"name": "Gal", "desc": "[0/1] Flag indicating the availability of additional information in the galaxy candidates table (in_galaxy_candidates)"}, {"name": "NSS", "desc": "[0/7] Flag indicating the availability of additional information in the various Non-Single Star tables (non_single_star)"}, {"name": "XPcont", "desc": "[0/1] Flag indicating the availability of mean BP/RP spectrum in continuous representation for this source (has_xp_continuous)"}, {"name": "XPsamp", "desc": "[0/1] Flag indicating the availability of mean BP/RP spectrum in sampled form for this source (has_xp_sampled)"}, {"name": "RVS", "desc": "[0/1] Flag indicating the availability of mean RVS spectrum for this source (has_rvs)"}, {"name": "EpochPh", "desc": "[0/1] Flag indicating the availability of epoch photometry for this source (has_epoch_photometry)"}, {"name": "EpochRV", "desc": "[0/1] Flag indicating the availability of epoch radial velocity for this source (has_epoch_rv)"}, {"name": "MCMCGSP", "desc": "[0/1] Flag indicating the availability of GSP-Phot MCMC samples for this source (has_mcmc_gspphot)"}, {"name": "MCMCMSC", "desc": "[0/1] Flag indicating the availability of MSC MCMC samples for this source (has_mcmc_msc)"}, {"name": "And", "desc": "[0/1] Flag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS) (in_andromeda_survey)"}, {"name": "PQSO", "desc": "? Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum) (classprob_dsc_combmod_quasar)"}, {"name": "PGal", "desc": "? Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_combmod_galaxy)"}, {"name": "PSS", "desc": "? Probability from DSC-Combmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum) (classprob_dsc_combmod_star)"}, {"name": "Teff", "desc": "? Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot)"}, {"name": "b_Teff", "desc": "? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_lower)"}, {"name": "B_Teff", "desc": "? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_upper)"}, {"name": "logg", "desc": "? Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot)"}, {"name": "b_logg", "desc": "? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_lower)"}, {"name": "B_logg", "desc": "? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_upper)"}, {"name": "[Fe/H]", "desc": "? Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot)"}, {"name": "b_[Fe/H]", "desc": "? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_lower)"}, {"name": "B_[Fe/H]", "desc": "? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_upper)"}, {"name": "Dist", "desc": "? Distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot)"}, {"name": "b_Dist", "desc": "? Lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_lower)"}, {"name": "B_Dist", "desc": "? Upper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_upper)"}, {"name": "A0", "desc": "? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot)"}, {"name": "b_A0", "desc": "? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_lower)"}, {"name": "B_A0", "desc": "? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_upper)"}, {"name": "AG", "desc": "? Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot)"}, {"name": "b_AG", "desc": "? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_lower)"}, {"name": "B_AG", "desc": "? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_upper)"}, {"name": "E(BP-RP)", "desc": "? Reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot)"}, {"name": "b_E(BP-RP)", "desc": "? Lower confidence level (16%) of reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_lower)"}, {"name": "B_E(BP-RP)", "desc": "? Upper confidence level (84%) of reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_upper)"}, {"name": "Lib", "desc": "Name of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this table (libname_gspphot)"}, {"name": "HIP", "desc": "? HIP cross-id number, van Leeuwen, Cat. I/311"}]}, {"name": "paramp.sam", "desc": "1D astrophysical parameters produced by the Apsis processing chain developed in Gaia DPAC CU8 (1590932717 sources) (astrophysical_parameters)", "columns": [{"name": "Source", "desc": "Source Identifier (source_id) "}, {"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2016.0 (ra)"}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2016.0 (dec) "}, {"name": "PQSO", "desc": "? Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum) (classprob_dsc_combmod_quasar)"}, {"name": "PGal", "desc": "? Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_combmod_galaxy)"}, {"name": "Pstar", "desc": "? Probability from DSC-Combmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum) (classprob_dsc_combmod_star)"}, {"name": "PWD", "desc": "? Probability from DSC-Combmod of being a white dwarf (data used: BP/RP spectrum) (classprob_dsc_combmod_whitedwarf)"}, {"name": "Pbin", "desc": "? Probability from DSC-Combmod of being a binary star (data used: BP/RP spectrum) (classprob_dsc_combmod_binarystar)"}, {"name": "PQSO-S", "desc": "? Probability from DSC-Specmod of being a quasar (data used: BP/RP spectrum) (classprob_dsc_specmod_quasar)"}, {"name": "Pgal-S", "desc": "? Probability from DSC-Specmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_specmod_galaxy)"}, {"name": "Pstar-S", "desc": "? Probability from DSC-Specmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum) (classprob_dsc_specmod_star)"}, {"name": "PWD-S", "desc": "? Probability from DSC-Specmod of being a white dwarf (data used: BP/RP spectrum) (classprob_dsc_specmod_whitedwarf)"}, {"name": "Pbin-S", "desc": "? Probability from DSC-Specmod of being a binary star (data used: BP/RP spectrum) (classprob_dsc_specmod_binarystar)"}, {"name": "PQSO-A", "desc": "? Probability from DSC-Allosmod of being a quasar (data used: photometry) (classprob_dsc_allosmod_quasar)"}, {"name": "PGal-A", "desc": "? Probability from DSC-Allosmod of being a galaxy (data used: photometry) (classprob_dsc_allosmod_galaxy)"}, {"name": "Pstar-A", "desc": "? Probability from DSC-Allosmod of being a star (data used: photometry) (classprob_dsc_allosmod_star)"}, {"name": "Teff", "desc": "? Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot)"}, {"name": "b_Teff", "desc": "? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_lower)"}, {"name": "B_Teff", "desc": "? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_upper)"}, {"name": "logg", "desc": "? Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot)"}, {"name": "b_logg", "desc": "? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_lower)"}, {"name": "B_logg", "desc": "? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_upper)"}, {"name": "[Fe/H]", "desc": "? Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot)"}, {"name": "b_[Fe/H]", "desc": "? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_lower)"}, {"name": "B_[Fe/H]", "desc": "? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_upper)"}, {"name": "Dist", "desc": "? Distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot)"}, {"name": "b_Dist", "desc": "? Lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_lower)"}, {"name": "B_Dist", "desc": "? Upper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_upper)"}, {"name": "A0", "desc": "? Monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot)"}, {"name": "b_A0", "desc": "? Lower confidence level (16%) of monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_lower)"}, {"name": "B_A0", "desc": "? Upper confidence level (84%) of monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_upper)"}, {"name": "AG", "desc": "? Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot)"}, {"name": "b_AG", "desc": "? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_lower)"}, {"name": "B_AG", "desc": "? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_upper)"}, {"name": "ABP", "desc": "? Extinction in G_BP_ band from GSP-Phot Aeneas best library using BP/RP spectra (abp_gspphot)"}, {"name": "b_ABP", "desc": "? Lower confidence level (16%) of extinction in G_BP_ band from GSP-Phot Aeneas best library using BP/RP spectra (abp_gspphot_lower)"}, {"name": "B_ABP", "desc": "? Upper confidence level (84%) of extinction in G_BP_ band from GSP-Phot Aeneas best library using BP/RP spectra (abp_gspphot_upper)"}, {"name": "ARP", "desc": "? Extinction in G_RP_ band from GSP-Phot Aeneas best library using BP/RP spectra (arp_gspphot)"}, {"name": "b_ARP", "desc": "? Lower confidence level (16%) of extinction in G_RP_ band from GSP-Phot Aeneas best library using BP/RP spectra (arp_gspphot_lower)"}, {"name": "B_ARP", "desc": "? Upper confidence level (84%) of extinction in G_RP_ band from GSP-Phot Aeneas best library using BP/RP spectra (arp_gspphot_upper)"}, {"name": "E(B-V)", "desc": "? Upper confidence level (84%) of reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot)"}, {"name": "b_E(B-V)", "desc": "? Lower confidence level (16%) of reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_lower)"}, {"name": "B_E(B-V)", "desc": "? Upper confidence level (84%) of reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_upper)"}, {"name": "GMAG", "desc": "? Absolute magnitude M_G_ from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot)"}, {"name": "b_GMAG", "desc": "? Lower confidence level (16%) of absolute magnitude M_G_ from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot_lower)"}, {"name": "B_GMAG", "desc": "? Upper confidence level (84%) of absolute magnitude M_G_ from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot_upper)"}, {"name": "Rad", "desc": "? Radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot)"}, {"name": "b_Rad", "desc": "? Lower confidence level (16%) of radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot_lower)"}, {"name": "B_Rad", "desc": "? Upper confidence level (84%) of radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot_upper)"}, {"name": "logpost", "desc": "? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC best library (logposterior_gspphot)"}, {"name": "Accp", "desc": "? MCMC acceptance rate of GSP-Phot Aeneas MCMC best library (mcmcaccept_gspphot)"}, {"name": "Lib", "desc": "Name of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this table (libname_gspphot)"}, {"name": "Teff-S", "desc": "? Effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec)"}, {"name": "b_Teff-S", "desc": "? 16th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec_lower)"}, {"name": "B_Teff-S", "desc": "? 84th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec_upper)"}, {"name": "logg-S", "desc": "? Logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (logg_gspspec)"}, {"name": "b_logg-S", "desc": "? 16th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (logg_gspspec_lower)"}, {"name": "B_logg-S", "desc": "? 84th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (logg_gspspec_upper)"}, {"name": "[M/H]-S", "desc": "? Global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mh_gspspec)"}, {"name": "b_[M/H]-S", "desc": "? 16th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mh_gspspec_lower)"}, {"name": "B_[M/H]-S", "desc": "? 84th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mh_gspspec_upper)"}, {"name": "[alpha/Fe]-S", "desc": "? Abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (alphafe_gspspec)"}, {"name": "b_[alpha/Fe]-S", "desc": "? 16th percentile of the abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (alphafe_gspspec_lower)"}, {"name": "B_[alpha/Fe]-S", "desc": "? 84th percentile of the abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (alphafe_gspspec_upper)"}, {"name": "[Fe/H]-S", "desc": "? Abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (fem_gspspec)"}, {"name": "b_[Fe/H]-S", "desc": "? 16th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (fem_gspspec_lower)"}, {"name": "B_[Fe/H]-S", "desc": "? 84th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (fem_gspspec_upper)"}, {"name": "o_[Fe/H]-S", "desc": "[0/8]? Number of lines used for [Fe/M] abundance estimation (fem_gspspec_nlines)"}, {"name": "s_[Fe/H]-S", "desc": "? Uncertainty estimation of [Fe/M] abundance using N lines of the element (fem_gspspec_linescatter)"}, {"name": "[Si/Fe]-S", "desc": "? Abundance of Silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sife_gspspec)"}, {"name": "b_[Si/Fe]-S", "desc": "? 16th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sife_gspspec_lower)"}, {"name": "B_[Si/Fe]-S", "desc": "? 84th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sife_gspspec_upper)"}, {"name": "o_[Si/Fe]-S", "desc": "[0/3]? Number of lines used for [Si/Fe] abundance estimation (sife_gspspec_nlines)"}, {"name": "s_[Si/Fe]-S", "desc": "? Uncertainty estimation of [Si/Fe] abundance using N lines of the element (sife_gspspec_linescatter)"}, {"name": "[Ca/Fe]-S", "desc": "? Abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cafe_gspspec)"}, {"name": "b_[Ca/Fe]-S", "desc": "? 16th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cafe_gspspec_lower)"}, {"name": "B_[Ca/Fe]-S", "desc": "? 84th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cafe_gspspec_upper)"}, {"name": "o_[Ca/Fe]-S", "desc": "[0/7]? Number of lines used for [Ca/Fe] abundance estimation (cafe_gspspec_nlines)"}, {"name": "s_[Ca/Fe]-S", "desc": "? Uncertainty estimation of [Ca/Fe] abundance using N lines of the element (cafe_gspspec_linescatter)"}, {"name": "[Ti/Fe]-S", "desc": "? Abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (tife_gspspec)"}, {"name": "b_[Ti/Fe]-S", "desc": "? 16th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (tife_gspspec_lower)"}, {"name": "B_[Ti/Fe]-S", "desc": "? 84th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (tife_gspspec_upper)"}, {"name": "o_[Ti/Fe]-S", "desc": "[0/3]? Number of lines used for [Ti/Fe] abundance estimation (tife_gspspec_nlines)"}, {"name": "s_[Ti/Fe]-S", "desc": "? Uncertainty estimation of [Ti/Fe] abundance using N lines of the element (tife_gspspec_linescatter)"}, {"name": "[Mg/Fe]-S", "desc": "? Abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mgfe_gspspec)"}, {"name": "b_[Mg/Fe]-S", "desc": "? 16th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mgfe_gspspec_lower)"}, {"name": "B_[Mg/Fe]-S", "desc": "? 84th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mgfe_gspspec_upper)"}, {"name": "[Nd/Fe]-S", "desc": "? Abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (ndfe_gspspec)"}, {"name": "b_[Nd/Fe]-S", "desc": "? 16th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (ndfe_gspspec_lower)"}, {"name": "B_[Nd/Fe]-S", "desc": "? 84th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (ndfe_gspspec_upper)"}, {"name": "[FeII/M]-S", "desc": "? Abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (feiim_gspspec)"}, {"name": "b_[FeII/M]-S", "desc": "? 16th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (feiim_gspspec_lower)"}, {"name": "B_[FeII/M]-S", "desc": "? 84th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (feiim_gspspec_upper)"}, {"name": "[S/Fe]-S", "desc": "? Abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sfe_gspspec)"}, {"name": "b_[S/Fe]-S", "desc": "? 16th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sfe_gspspec_lower)"}, {"name": "B_[S/Fe]-S", "desc": "? 84th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sfe_gspspec_upper)"}, {"name": "o_[S/Fe]-S", "desc": "[0/2]? Number of lines used for [S/Fe] abundance estimation (sfe_gspspec_nlines)"}, {"name": "s_[S/Fe]-S", "desc": "? Uncertainty estimation of [S/Fe] abundance using N lines of the element (sfe_gspspec_linescatter)"}, {"name": "[Zr/Fe]-S", "desc": "? Abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (zrfe_gspspec)"}, {"name": "b_[Zr/Fe]-S", "desc": "? 16th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (zrfe_gspspec_lower)"}, {"name": "B_[Zr/Fe]-S", "desc": "? 84th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (zrfe_gspspec_upper)"}, {"name": "[N/Fe]-S", "desc": "? Abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nfe_gspspec)"}, {"name": "b_[N/Fe]-S", "desc": "? 16th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nfe_gspspec_lower)"}, {"name": "B_[N/Fe]-S", "desc": "? 84th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nfe_gspspec_upper)"}, {"name": "o_[N/Fe]-S", "desc": "[0/2]? Number of lines used for [N/Fe] abundance estimation (nfe_gspspec_nlines)"}, {"name": "s_[N/Fe]-S", "desc": "? Uncertainty estimation of [N/Fe] abundance using N lines of the element (nfe_gspspec_linescatter)"}, {"name": "[Cr/Fe]-S", "desc": "? Abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (crfe_gspspec)"}, {"name": "b_[Cr/Fe]-S", "desc": "? 16th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (crfe_gspspec_lower)"}, {"name": "B_[Cr/Fe]-S", "desc": "? 84th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (crfe_gspspec_upper)"}, {"name": "o_[Cr/Fe]-S", "desc": "[0/2]? Number of lines used for [Cr/Fe] abundance estimation (crfe_gspspec_nlines)"}, {"name": "s_[Cr/Fe]-S", "desc": "? Uncertainty estimation of [Cr/Fe] abundance using N lines of the element (crfe_gspspec_linescatter)"}, {"name": "[Ce/Fe]-S", "desc": "? Abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cefe_gspspec)"}, {"name": "b_[Ce/Fe]-S", "desc": "? 16th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cefe_gspspec_lower)"}, {"name": "B_[Ce/Fe]-S", "desc": "? 84th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cefe_gspspec_upper)"}, {"name": "[Ni/Fe]-S", "desc": "? Abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nife_gspspec)"}, {"name": "b_[Ni/Fe]-S", "desc": "? 16th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nife_gspspec_lower)"}, {"name": "B_[Ni/Fe]-S", "desc": "? 84th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nife_gspspec_upper)"}, {"name": "EWCN0", "desc": "? Equivalent width of cyoanogen line (cn0ew_gspspec)"}, {"name": "e_EWCN0", "desc": "? Uncertainty of equivalent width of cyanogen absorption line (cn0ew_gspspec_uncertainty)"}, {"name": "CN0", "desc": "? Central wavelength of cyanogen line (cn0_gspspec_centralline)"}, {"name": "CN0W", "desc": "? Width of cyoanogen line (cn0_gspspec_width)"}, {"name": "DIB", "desc": "? DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra (dib_gspspec_lambda)"}, {"name": "e_DIB", "desc": "? Uncertainty on DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra (dib_gspspec_lambda_uncertainty)"}, {"name": "EWDIB", "desc": "? Equivalent width of the DIB from GSP-Spec MatisseGauguin using RVS spectra (dibew_gspspec)"}, {"name": "e_EWDIB", "desc": "? Global uncertainty on DIB equivalent width value using DIB algorithm (dibew_gspspec_uncertainty)"}, {"name": "s_EWDIB", "desc": "? Uncertainty on DIB equivalent width value occuring from noise part (dibewnoise_gspspec_uncertainty)"}, {"name": "DIBp0", "desc": "? Depth (p_0 parameter) of the DIB derived from a Gaussian model fit (dibp0_gspspec)"}, {"name": "DIBp2", "desc": "? Width (p_2 parameter) of the DIB derived from a Gaussian model fit (dibp2_gspspec)"}, {"name": "e_DIBp2", "desc": "? Uncertainty on the dibp2Gspspec parameter (dibp2_gspspec_uncertainty)"}, {"name": "q_DIB", "desc": "[-2/5]? Quality flag of the DIB computation (dibqf_gspspec)"}, {"name": "Flags", "desc": "? Catalogue flags for GSP-Spec MatisseGauguin (flags_gspspec) (1)"}, {"name": "chi2", "desc": "? Logarithm of the goodness-of-fit for the GSP-Spec MatisseGauguin parameters (logchisq_gspspec)"}, {"name": "EWHa", "desc": "? Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha)"}, {"name": "e_EWHa", "desc": "? Uncertainty of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_uncertainty)"}, {"name": "f_EWHa", "desc": "[0/9]? Quality flag of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_flag)"}, {"name": "EWHamod", "desc": "? Halpha pseudo-equivalent width from ESP-ELS measured on the synthetic spectrum (ew_espels_halpha_model)"}, {"name": "ClassELS", "desc": "Adopted ELS class label from ESP-ELS (classlabel_espels)"}, {"name": "f_ClassELS", "desc": "? Quality flag of the adopted ELS class label from ESP-ELS (classlabel_espels_flag)"}, {"name": "PWC", "desc": "? Probability from ESP-ELS of being a Wolf-Rayet star of type WC (classprob_espels_wcstar)"}, {"name": "PWN", "desc": "? Probability from ESP-ELS of being a Wolf-Rayet star of type WN (classprob_espels_wnstar)"}, {"name": "PBe", "desc": "? Probability from ESP-ELS of being a Be Star (classprob_espels_bestar)"}, {"name": "PTTau", "desc": "? Probability from ESP-ELS of being a T Tauri Star (classprob_espels_ttauristar)"}, {"name": "PHAe/Be", "desc": "? Probability from ESP-ELS of being a Herbig Ae/Be Star (classprob_espels_herbigstar)"}, {"name": "PdMactive", "desc": "? Probability from ESP-ELS of being an active M dwarf Star (classprob_espels_dmestar)"}, {"name": "PPN", "desc": "? Probability from ESP-ELS of being a planetary nebula (classprob_espels_pne)"}, {"name": "A0-HS", "desc": "? Monochromatic interstellar extinction (azero_esphs)"}, {"name": "e_A0-HS", "desc": "? Uncertainty at a 68% confidence level on A_0_ from ESP-HS (azero_esphs_uncertainty)"}, {"name": "AG-HS", "desc": "? Intersterstellar extinction in G band from ESP-HS (ag_esphs)"}, {"name": "e_AG-HS", "desc": "? Uncertainty on A_G_ from ESP-HS (ag_esphs_uncertainty)"}, {"name": "E(BP-RP)-HS", "desc": "? Reddening E(G_BP_-G_RP_) from ESP-HS (ebpminrp_esphs)"}, {"name": "e_E(BP-RP)-HS", "desc": "? Uncertainty on E(G_BP_-G_RP_) from ESP-HS (ebpminrp_esphs_uncertainty)"}, {"name": "Teff-HS", "desc": "? Effective temperature from ESP-HS (teff_esphs)"}, {"name": "e_Teff-HS", "desc": "? Uncertainty at a 68% confidence level on the effective temperature from ESP-HS (teff_esphs_uncertainty)"}, {"name": "logg-HS", "desc": "? Surface gravity from ESP-HS (logg_esphs)"}, {"name": "e_logg-HS", "desc": "? Uncertainty at a 68% confidence level on the surface gravity from ESP-HS (logg_esphs_uncertainty)"}, {"name": "vsini-HS", "desc": "? Projected rotational velocity from ESP-HS (vsini_esphs)"}, {"name": "e_vsini-HS", "desc": "? Uncertainty on the projected rotational velocity from ESP-HS (vsini_esphs_uncertainty)"}, {"name": "Flags-HS", "desc": "? Quality flag of the ESP-HS parametrisation (flags_esphs) (2)"}, {"name": "SpType-ELS", "desc": "Spectral type from ESP-ELS (spectraltype_esphs)"}, {"name": "CA-CS", "desc": "? Chromospheric activity index from ESP-CS (activityindex_espcs)"}, {"name": "e_CA-CS", "desc": "? Uncertainty in the chromospheric activity index from ESP-CS (activityindex_espcs_uncertainty)"}, {"name": "n_CA-CS", "desc": "[12M] Source of input stellar parameters for the computation of the activity index by ESP-CS (activityindex_espcs_input)"}, {"name": "Teff-UCD", "desc": "? Effective temperature estimate from ESP-UCD based on the RP spectrum (teff_espucd)"}, {"name": "e_Teff-UCD", "desc": "? Uncertainty of the effective temperature estimate produced by ESP-UCD (teff_espucd_uncertainty)"}, {"name": "Flags-UCD", "desc": "[0/21]? Quality flags of the ESP-UCD parameter estimates (flags_espucd) (3)"}, {"name": "Rad-Flame", "desc": "? Radius of the star from FLAME using teff_gspphot and lum_flame (radius_flame)"}, {"name": "b_Rad-Flame", "desc": "? Lower confidence level (16%) of radiusFlame (radius_flame_lower)"}, {"name": "B_Rad-Flame", "desc": "? Upper confidence level (84%) of radiusFlame (radius_flame_upper)"}, {"name": "Lum-Flame", "desc": "? Luminosity of the star from FLAME using G band magnitude, extinction (ag_gspphot), parallax or distance, and a bolometric correction bc_flame (lum_flame)"}, {"name": "b_Lum-Flame", "desc": "? Lower confidence level (16%) of lumFlame (lum_flame_lower)"}, {"name": "B_Lum-Flame", "desc": "? Upper confidence level (84%) of lumFlame (lum_flame_upper)"}, {"name": "Mass-Flame", "desc": "? Mass of the star from FLAME using stellar models, lum_flame, and teff_gspphot (mass_flame)"}, {"name": "b_Mass-Flame", "desc": "? Lower confidence level (16%) of mass of the star from FLAME (mass_flame_lower)"}, {"name": "B_Mass-Flame", "desc": "? Upper confidence level (84%) of mass of the star from FLAME (mass_flame_upper)"}, {"name": "Age-Flame", "desc": "? Age of the star from FLAME using stellar models (age_flame)"}, {"name": "b_Age-Flame", "desc": "? Lower confidence level (84%) of age of the star from FLAME (age_flame_lower)"}, {"name": "B_Age-Flame", "desc": "? Upper confidence level (84%) of age of the star from FLAME (age_flame_upper)"}, {"name": "Flags-Flame", "desc": "[0/22]? Flags indicating quality and processing information from FLAME (flags_flame) (4)"}, {"name": "Evol", "desc": "? Evolutionary stage of the star from FLAME using stellar models (evolstage_flame)"}, {"name": "z-Flame", "desc": "? Gravitational redshift from FLAME using radiusFlame and loggGspphot (gravredshift_flame)"}, {"name": "b_z-Flame", "desc": "? Lower confidence level (16%) of gravitational redshift from FLAME (gravredshift_flame_lower)"}, {"name": "B_z-Flame", "desc": "? Upper confidence level (84%) of gravitational redshift from FLAME (gravredshift_flame_upper)"}, {"name": "BolCorr", "desc": "? Bolometric correction used to derive lumFlame (bc_flame)"}, {"name": "[M/H]-MSC", "desc": "? Metallicity of the source treated as a binary system from MSC using BP/RP spectra and parallax (mh_msc)"}, {"name": "B_[M/H]-MSC", "desc": "? Upper confidence level (84%) of the metallicity from MSC using BP/RP spectra and parallax (mh_msc_upper)"}, {"name": "b_[M/H]-MSC", "desc": "? Lower confidence level (16%) of the metallicity from MSC using BP/RP spectra and parallax (mh_msc_lower)"}, {"name": "A0-MSC", "desc": "? Monochromatic extinction A0 at 541.4nm of the source treated as a binary system from MSC using BP/RP spectra and parallax (azero_msc)"}, {"name": "B_A0-MSC", "desc": "? Upper confidence level (84%) of monochromatic extinction A0 at 547.7nm from MSC using BP/RP spectra and parallax (azero_msc_upper)"}, {"name": "b_A0-MSC", "desc": "? Lower confidence level (16%) of monochromatic extinction A0 at 547.7nm from MSC using BP/RP spectra and parallax (azero_msc_lower)"}, {"name": "Dist-MSC", "desc": "? Distance from MSC using BP/RP spectra and parallax (distance_msc)"}, {"name": "B_Dist-MSC", "desc": "? Upper confidence level (84%) of distance from MSC using BP/RP spectra and parallax (distance_msc_upper)"}, {"name": "b_Dist-MSC", "desc": "? Lower confidence level (16%) of distance from MSC using BP/RP spectra and parallax (distance_msc_lower)"}, {"name": "Teff1-MSC", "desc": "? Effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1)"}, {"name": "B_Teff1-MSC", "desc": "? Upper confidence level (84%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_upper)"}, {"name": "b_Teff1-MSC", "desc": "? Lower confidence level (16%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_lower)"}, {"name": "Teff2-MSC", "desc": "? Effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2)"}, {"name": "B_Teff2-MSC", "desc": "? Upper confidence level (84%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_upper)"}, {"name": "b_Teff2-MSC", "desc": "? Lower confidence level (16%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_lower)"}, {"name": "logg1-MSC", "desc": "? Surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1)"}, {"name": "B_logg1-MSC", "desc": "? Upper confidence level (84%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1_upper)"}, {"name": "b_logg1-MSC", "desc": "? Lower confidence level (16%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1_lower)"}, {"name": "logg2-MSC", "desc": "? Surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2)"}, {"name": "B_logg2-MSC", "desc": "? Upper confidence level (84%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2_upper)"}, {"name": "b_logg2-MSC", "desc": "? Lower confidence level (16%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2_lower)"}, {"name": "AG-MSC", "desc": "? Extinction in G band from MSC using BP/RP spectra and parallax (ag_msc)"}, {"name": "B_AG-MSC", "desc": "? Upper confidence level (84%) of extinction in G band from MSC using BP/RP spectra and parallax (ag_msc_upper)"}, {"name": "b_AG-MSC", "desc": "? Lower confidence level (16%) of extinction in G band from MSC using BP/RP spectra and parallax (ag_msc_lower)"}, {"name": "logpost-MSC", "desc": "? Goodness-of-fit score (normalised log-posterior) of MSC MCMC (logposterior_msc)"}, {"name": "Accp-MSC", "desc": "? Mean MCMC acceptance rate of MSC MCMC (mcmcaccept_msc)"}, {"name": "drift-MSC", "desc": "? Mean drift of the MSC MCMC chain in units of parameter standard deviation (mcmcdrift_msc)"}, {"name": "Flag-MSC", "desc": "[0/1]? Flag indicating quality information from MSC (flags_msc) (5)"}, {"name": "NOAId", "desc": "? Identifier of the OA SOM map neuron that represents the source (neuron_oa_id)"}, {"name": "NOADist", "desc": "? Distance between the source XP spectra and the OA neuron XP prototype that represents the source (neuron_oa_dist)"}, {"name": "NOADistRank", "desc": "[0/95]? Percentile rank according to the distance distribution of the OA neuron that represents the source (neuron_oa_dist_percentile_rank)"}, {"name": "Flags-NOA", "desc": "? Flags indicating quality and processing information from OA (flags_oa) (6)"}]}, {"name": "paramsup.sam", "desc": "Additional parameters from the Apsis processing chain, compared to the main table astrophysical parameters, from modules that produce more than one result for a parameter (473020612 sources) (astrophysical_parameters_supp)", "columns": [{"name": "Source", "desc": "Source Identifier (source_id) "}, {"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2016.0 (ra)"}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2016.0 (dec) "}, {"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "Lib", "desc": "Name of library that achieves the highest mean log-posterior in MCMC samples from GSP-Phot Aeneas (libname_best_gspphot)"}, {"name": "Teff", "desc": "? Effective temperature from GSP-Phot Aeneas for MARCS library using BP/RP spectra (teff_gspphot_marcs)"}, {"name": "b_Teff", "desc": "? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas for MARCS library using BP/RP spectra (teff_gspphot_marcs_lower)"}, {"name": "B_Teff", "desc": "? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas for MARCS library using BP/RP spectra (teff_gspphot_marcs_upper)"}, {"name": "logg", "desc": "? Surface gravity from GSP-Phot Aeneas for MARCS library using BP/RP spectra (logg_gspphot_marcs)"}, {"name": "b_logg", "desc": "? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas for MARCS library using BP/RP spectra (logg_gspphot_marcs_lower)"}, {"name": "B_logg", "desc": "? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas for MARCS library using BP/RP spectra (logg_gspphot_marcs_upper)"}, {"name": "[M/H]", "desc": "? Iron abundance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mh_gspphot_marcs)"}, {"name": "b_[M/H]", "desc": "? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mh_gspphot_marcs_lower)"}, {"name": "B_[M/H]", "desc": "? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mh_gspphot_marcs_upper)"}, {"name": "Dist", "desc": "? Distance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (distance_gspphot_marcs)"}, {"name": "b_Dist", "desc": "? Lower confidence level (16%) of distance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (distance_gspphot_marcs_lower)"}, {"name": "B_Dist", "desc": "? Upper confidence level (84%) of distance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (distance_gspphot_marcs_upper)"}, {"name": "A0", "desc": "? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for MARCS library using BP/RP spectra (azero_gspphot_marcs)"}, {"name": "b_A0", "desc": "? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for MARCS library using BP/RP spectra (azero_gspphot_marcs_lower)"}, {"name": "B_A0", "desc": "? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for MARCS library using BP/RP spectra (azero_gspphot_marcs_upper)"}, {"name": "AG", "desc": "? Extinction in G band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ag_gspphot_marcs)"}, {"name": "b_AG", "desc": "? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ag_gspphot_marcs_lower)"}, {"name": "B_AG", "desc": "? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ag_gspphot_marcs_upper)"}, {"name": "ABP", "desc": "? Extinction in G_BP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (abp_gspphot_marcs)"}, {"name": "b_ABP", "desc": "? Lower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (abp_gspphot_marcs_lower)"}, {"name": "B_ABP", "desc": "? Upper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (abp_gspphot_marcs_upper)"}, {"name": "ARP", "desc": "? Extinction in G_RP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (arp_gspphot_marcs)"}, {"name": "b_ARP", "desc": "? Lower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (arp_gspphot_marcs_lower)"}, {"name": "B_ARP", "desc": "? Upper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (arp_gspphot_marcs_upper)"}, {"name": "E(BP-RP)", "desc": "? Reddening E(BP-RP) from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ebpminrp_gspphot_marcs)"}, {"name": "b_E(BP-RP)", "desc": "? Lower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ebpminrp_gspphot_marcs_lower)"}, {"name": "B_E(BP-RP)", "desc": "? Upper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ebpminrp_gspphot_marcs_upper)"}, {"name": "GMAG", "desc": "? Absolute magnitude M_G from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mg_gspphot_marcs)"}, {"name": "b_GMAG", "desc": "? Lower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mg_gspphot_marcs_lower)"}, {"name": "B_GMAG", "desc": "? Upper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mg_gspphot_marcs_upper)"}, {"name": "Rad", "desc": "? Radius from GSP-Phot Aeneas for MARCS library using BP/RP spectra (radius_gspphot_marcs)"}, {"name": "b_Rad", "desc": "? Lower confidence level (16%) of radius from GSP-Phot Aeneas for MARCS library using BP/RP spectra (radius_gspphot_marcs_lower)"}, {"name": "B_Rad", "desc": "? Upper confidence level (84%) of radius from GSP-Phot Aeneas for MARCS library using BP/RP spectra (radius_gspphot_marcs_upper)"}, {"name": "logpost", "desc": "? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for MARCS library (logposterior_gspphot_marcs)"}, {"name": "Accp", "desc": "? MCMC acceptance rate of GSP-Phot Aeneas MCMC for MARCS library (mcmcaccept_gspphot_marcs)"}, {"name": "Teff-Phx", "desc": "? Effective temperature from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (teff_gspphot_phoenix)"}, {"name": "b_Teff-Phx", "desc": "? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (teff_gspphot_phoenix_lower)"}, {"name": "B_Teff-Phx", "desc": "? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (teff_gspphot_phoenix_upper)"}, {"name": "logg-Phx", "desc": "? Surface gravity from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (logg_gspphot_phoenix)"}, {"name": "b_logg-Phx", "desc": "? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (logg_gspphot_phoenix_lower)"}, {"name": "B_logg-Phx", "desc": "? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (logg_gspphot_phoenix_upper)"}, {"name": "[M/H]-Phx", "desc": "? Iron abundance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mh_gspphot_phoenix)"}, {"name": "b_[M/H]-Phx", "desc": "? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mh_gspphot_phoenix_lower)"}, {"name": "B_[M/H]-Phx", "desc": "? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mh_gspphot_phoenix_upper)"}, {"name": "Dist-Phx", "desc": "? Distance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (distance_gspphot_phoenix)"}, {"name": "b_Dist-Phx", "desc": "? Lower confidence level (16%) of distance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (distance_gspphot_phoenix_lower)"}, {"name": "B_Dist-Phx", "desc": "? Upper confidence level (84%) of distance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (distance_gspphot_phoenix_upper)"}, {"name": "A0Phoenix", "desc": "? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (azero_gspphot_phoenix)"}, {"name": "b_A0Phoenix", "desc": "? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (azero_gspphot_phoenix_lower)"}, {"name": "B_A0Phoenix", "desc": "? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (azero_gspphot_phoenix_upper)"}, {"name": "AG-Phx", "desc": "? Extinction in G band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ag_gspphot_phoenix)"}, {"name": "b_AG-Phx", "desc": "? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ag_gspphot_phoenix_lower)"}, {"name": "B_AG-Phx", "desc": "? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ag_gspphot_phoenix_upper)"}, {"name": "ABP-Phx", "desc": "? Extinction in G_BP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (abp_gspphot_phoenix)"}, {"name": "b_ABP-Phx", "desc": "? Lower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (abp_gspphot_phoenix_lower)"}, {"name": "B_ABP-Phx", "desc": "? Upper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (abp_gspphot_phoenix_upper)"}, {"name": "ARP-Phx", "desc": "? Extinction in G_RP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (arp_gspphot_phoenix)"}, {"name": "b_ARP-Phx", "desc": "? Lower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (arp_gspphot_phoenix_lower)"}, {"name": "B_ARP-Phx", "desc": "? Upper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (arp_gspphot_phoenix_upper)"}, {"name": "E(BP-RP)-Phx", "desc": "? Reddening E(BP-RP) from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ebpminrp_gspphot_phoenix)"}, {"name": "b_E(BP-RP)-Phx", "desc": "? Lower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ebpminrp_gspphot_phoenix_lower)"}, {"name": "B_E(BP-RP)-Phx", "desc": "? Upper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ebpminrp_gspphot_phoenix_upper)"}, {"name": "GMAG-Phx", "desc": "? Absolute magnitude M_G from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mg_gspphot_phoenix)"}, {"name": "b_GMAG-Phx", "desc": "? Lower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mg_gspphot_phoenix_lower)"}, {"name": "B_GMAG-Phx", "desc": "? Upper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mg_gspphot_phoenix_upper)"}, {"name": "Rad-Phx", "desc": "? Radius from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (radius_gspphot_phoenix)"}, {"name": "b_Rad-Phx", "desc": "? Lower confidence level (16%) of radius from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (radius_gspphot_phoenix_lower)"}, {"name": "B_Rad-Phx", "desc": "? Upper confidence level (84%) of radius from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (radius_gspphot_phoenix_upper)"}, {"name": "logpost-Phx", "desc": "? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for PHOENIX library (logposterior_gspphot_phoenix)"}, {"name": "Accp-Phx", "desc": "? MCMC acceptance rate of GSP-Phot Aeneas MCMC for PHOENIX library (mcmcaccept_gspphot_phoenix)"}, {"name": "Teff-OB", "desc": "? Effective temperature from GSP-Phot Aeneas for OB library using BP/RP spectra (teff_gspphot_ob)"}, {"name": "b_Teff-OB", "desc": "? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas for OB library using BP/RP spectra (teff_gspphot_ob_lower)"}, {"name": "B_Teff-OB", "desc": "? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas for OB library using BP/RP spectra (teff_gspphot_ob_upper)"}, {"name": "logg-OB", "desc": "? Surface gravity from GSP-Phot Aeneas for OB library using BP/RP spectra (logg_gspphot_ob)"}, {"name": "b_logg-OB", "desc": "? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas for OB library using BP/RP spectra (logg_gspphot_ob_lower)"}, {"name": "B_logg-OB", "desc": "? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas for OB library using BP/RP spectra (logg_gspphot_ob_upper)"}, {"name": "[M/H]-OB", "desc": "? Iron abundance from GSP-Phot Aeneas for OB library using BP/RP spectra (mh_gspphot_ob)"}, {"name": "b_[M/H]-OB", "desc": "? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas for OB library using BP/RP spectra (mh_gspphot_ob_lower)"}, {"name": "B_[M/H]-OB", "desc": "? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas for OB library using BP/RP spectra (mh_gspphot_ob_upper)"}, {"name": "Dist-OB", "desc": "? Distance from GSP-Phot Aeneas for OB library using BP/RP spectra (distance_gspphot_ob)"}, {"name": "b_Dist-OB", "desc": "? Lower confidence level (16%) of distance from GSP-Phot Aeneas for OB library using BP/RP spectra (distance_gspphot_ob_lower)"}, {"name": "B_Dist-OB", "desc": "? Upper confidence level (84%) of distance from GSP-Phot Aeneas for OB library using BP/RP spectra (distance_gspphot_ob_upper)"}, {"name": "A0-OB", "desc": "? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for OB library using BP/RP spectra (azero_gspphot_ob)"}, {"name": "b_A0-OB", "desc": "? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for OB library using BP/RP spectra (azero_gspphot_ob_lower)"}, {"name": "B_A0-OB", "desc": "? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for OB library using BP/RP spectra (azero_gspphot_ob_upper)"}, {"name": "AG-OB", "desc": "? Extinction in G band from GSP-Phot Aeneas for OB library using BP/RP spectra (ag_gspphot_ob)"}, {"name": "b_AG-OB", "desc": "? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for OB library using BP/RP spectra (ag_gspphot_ob_lower)"}, {"name": "B_AG-OB", "desc": "? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for OB library using BP/RP spectra (ag_gspphot_ob_upper)"}, {"name": "ABP-OB", "desc": "? Extinction in G_BP band from GSP-Phot Aeneas for OB library using BP/RP spectra (abp_gspphot_ob)"}, {"name": "b_ABP-OB", "desc": "? Lower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for OB library using BP/RP spectra (abp_gspphot_ob_lower)"}, {"name": "B_ABP-OB", "desc": "? Upper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for OB library using BP/RP spectra (abp_gspphot_ob_upper)"}, {"name": "ARP-OB", "desc": "? Extinction in G_RP band from GSP-Phot Aeneas for OB library using BP/RP spectra (arp_gspphot_ob)"}, {"name": "b_ARP-OB", "desc": "? Lower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for OB library using BP/RP spectra (arp_gspphot_ob_lower)"}, {"name": "B_ARP-OB", "desc": "? Upper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for OB library using BP/RP spectra (arp_gspphot_ob_upper)"}, {"name": "E(BP-RP)-OB", "desc": "? Reddening E(BP-RP) from GSP-Phot Aeneas for OB library using BP/RP spectra (ebpminrp_gspphot_ob)"}, {"name": "b_E(BP-RP)-OB", "desc": "? Lower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for OB library using BP/RP spectra (ebpminrp_gspphot_ob_lower)"}, {"name": "B_E(BP-RP)-OB", "desc": "? Upper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for OB library using BP/RP spectra (ebpminrp_gspphot_ob_upper)"}, {"name": "GMAG-OB", "desc": "? Absolute magnitude M_G from GSP-Phot Aeneas for OB library using BP/RP spectra (mg_gspphot_ob)"}, {"name": "b_GMAG-OB", "desc": "? Lower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for OB library using BP/RP spectra (mg_gspphot_ob_lower)"}, {"name": "B_GMAG-OB", "desc": "? Upper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for OB library using BP/RP spectra (mg_gspphot_ob_upper)"}, {"name": "Rad-OB", "desc": "? Radius from GSP-Phot Aeneas for OB library using BP/RP spectra (radius_gspphot_ob)"}, {"name": "b_Rad-OB", "desc": "? Lower confidence level (16%) of radius from GSP-Phot Aeneas for OB library using BP/RP spectra (radius_gspphot_ob_lower)"}, {"name": "B_Rad-OB", "desc": "? Upper confidence level (84%) of radius from GSP-Phot Aeneas for OB library using BP/RP spectra (radius_gspphot_ob_upper)"}, {"name": "logpost-OB", "desc": "? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for OB library (logposterior_gspphot_ob)"}, {"name": "Accp-OB", "desc": "? MCMC acceptance rate of GSP-Phot Aeneas MCMC for OB library (mcmcaccept_gspphot_ob)"}, {"name": "Teff-A", "desc": "? Effective temperature from GSP-Phot Aeneas for A library using BP/RP spectra (teff_gspphot_a)"}, {"name": "b_Teff-A", "desc": "? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas for A library using BP/RP spectra (teff_gspphot_a_lower)"}, {"name": "B_Teff-A", "desc": "? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas for A library using BP/RP spectra (teff_gspphot_a_upper)"}, {"name": "logg-A", "desc": "? Surface gravity from GSP-Phot Aeneas for A library using BP/RP spectra (logg_gspphot_a)"}, {"name": "b_logg-A", "desc": "? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas for A library using BP/RP spectra (logg_gspphot_a_lower)"}, {"name": "B_logg-A", "desc": "? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas for A library using BP/RP spectra (logg_gspphot_a_upper)"}, {"name": "[M/H]-A", "desc": "? Iron abundance from GSP-Phot Aeneas for A library using BP/RP spectra (mh_gspphot_a)"}, {"name": "b_[M/H]-A", "desc": "? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas for A library using BP/RP spectra (mh_gspphot_a_lower)"}, {"name": "B_[M/H]-A", "desc": "? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas for A library using BP/RP spectra (mh_gspphot_a_upper)"}, {"name": "Dist-A", "desc": "? Distance from GSP-Phot Aeneas for A library using BP/RP spectra (distance_gspphot_a)"}, {"name": "b_Dist-A", "desc": "? Lower confidence level (16%) of distance from GSP-Phot Aeneas for A library using BP/RP spectra (distance_gspphot_a_lower)"}, {"name": "B_Dist-A", "desc": "? Upper confidence level (84%) of distance from GSP-Phot Aeneas for A library using BP/RP spectra (distance_gspphot_a_upper)"}, {"name": "A0-A", "desc": "? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for A library using BP/RP spectra (azero_gspphot_a)"}, {"name": "b_A0-A", "desc": "? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for A library using BP/RP spectra (azero_gspphot_a_lower)"}, {"name": "B_A0-A", "desc": "? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for A library using BP/RP spectra (azero_gspphot_a_upper)"}, {"name": "AG-A", "desc": "? Extinction in G band from GSP-Phot Aeneas for A library using BP/RP spectra (ag_gspphot_a)"}, {"name": "b_AG-A", "desc": "? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for A library using BP/RP spectra (ag_gspphot_a_lower)"}, {"name": "B_AG-A", "desc": "? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for A library using BP/RP spectra (ag_gspphot_a_upper)"}, {"name": "ABP-A", "desc": "? Extinction in G_BP band from GSP-Phot Aeneas for A library using BP/RP spectra (abp_gspphot_a)"}, {"name": "b_ABP-A", "desc": "? Lower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for A library using BP/RP spectra (abp_gspphot_a_lower)"}, {"name": "B_ABP-A", "desc": "? Upper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for A library using BP/RP spectra (abp_gspphot_a_upper)"}, {"name": "ARP-A", "desc": "? Extinction in G_RP band from GSP-Phot Aeneas for A library using BP/RP spectra (arp_gspphot_a)"}, {"name": "b_ARP-A", "desc": "? Lower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for A library using BP/RP spectra (arp_gspphot_a_lower)"}, {"name": "B_ARP-A", "desc": "? Upper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for A library using BP/RP spectra (arp_gspphot_a_upper)"}, {"name": "E(BP-RP)-A", "desc": "? Reddening E(BP-RP) from GSP-Phot Aeneas for A library using BP/RP spectra (ebpminrp_gspphot_a)"}, {"name": "b_E(BP-RP)-A", "desc": "? Lower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for A library using BP/RP spectra (ebpminrp_gspphot_a_lower)"}, {"name": "B_E(BP-RP)-A", "desc": "? Upper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for A library using BP/RP spectra (ebpminrp_gspphot_a_upper)"}, {"name": "GMAG-A", "desc": "? Absolute magnitude M_G from GSP-Phot Aeneas for A library using BP/RP spectra (mg_gspphot_a)"}, {"name": "b_GMAG-A", "desc": "? Lower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for A library using BP/RP spectra (mg_gspphot_a_lower)"}, {"name": "B_GMAG-A", "desc": "? Upper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for A library using BP/RP spectra (mg_gspphot_a_upper)"}, {"name": "Rad-A", "desc": "? Radius from GSP-Phot Aeneas for A library using BP/RP spectra (radius_gspphot_a)"}, {"name": "b_Rad-A", "desc": "? Lower confidence level (16%) of radius from GSP-Phot Aeneas for A library using BP/RP spectra (radius_gspphot_a_lower)"}, {"name": "B_Rad-A", "desc": "? Upper confidence level (84%) of radius from GSP-Phot Aeneas for A library using BP/RP spectra (radius_gspphot_a_upper)"}, {"name": "logpost-A", "desc": "? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for A library (logposterior_gspphot_a)"}, {"name": "Accp-A", "desc": "? MCMC acceptance rate of GSP-Phot Aeneas MCMC for A library (mcmcaccept_gspphot_a)"}, {"name": "Teff-ANN", "desc": "? Effective temperature from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (teff_gspspec_ann)"}, {"name": "b_Teff-ANN", "desc": "? Lower confidence level (16%) of effective temperature from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (teff_gspspec_ann_lower)"}, {"name": "B_Teff-ANN", "desc": "? Upper confidence level (84%) of effective temperature from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (teff_gspspec_ann_upper)"}, {"name": "logg-ANN", "desc": "? Surface gravity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (logg_gspspec_ann)"}, {"name": "b_logg-ANN", "desc": "? Lower confidence level (16%) of surface gravity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (logg_gspspec_ann_lower)"}, {"name": "B_logg-ANN", "desc": "? Upper confidence level (84%) of surface gravity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (logg_gspspec_ann_upper)"}, {"name": "[M/H]-ANN", "desc": "? Global metallicity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (mh_gspspec_ann)"}, {"name": "b_[M/H]-ANN", "desc": "? Lower confidence level (16%) of global metallicity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (mh_gspspec_ann_lower)"}, {"name": "B_[M/H]-ANN", "desc": "? Upper confidence level (84%) of global metallicity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (mh_gspspec_ann_upper)"}, {"name": "[alpha/Fe]-ANN", "desc": "? Abundance of alpha-elements with respect to iron from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (alphafe_gspspec_ann)"}, {"name": "b_[alpha/Fe]-ANN", "desc": "? Lower confidence level (16%) of alpha-elements with respect to iron from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (alphafe_gspspec_ann_lower)"}, {"name": "B_[alpha/Fe]-ANN", "desc": "? Upper confidence level (84%) of alpha-elements with respect to iron from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (alphafe_gspspec_ann_upper)"}, {"name": "logpost-ANN", "desc": "? Logarithm of the goodness-of-fit for the GSP-Spec ANN parameters (logchisq_gspspec_ann)"}, {"name": "Flags-ANN", "desc": "? Catalogue flags for GSP-Spec ANN (flags_gspspec_ann) (1)"}, {"name": "Rad-Flame", "desc": "? Radius of the star from FLAME using teffGspspec and lumFlameSpec (radius_flame_spec)"}, {"name": "b_Rad-Flame", "desc": "? Lower confidence level (16%) of radiusFlameSpec (radius_flame_spec_lower)"}, {"name": "B_Rad-Flame", "desc": "? Upper confidence level (84%) of radiusFlameSpec (radius_flame_spec_upper)"}, {"name": "Lum-Flame", "desc": "? Luminosity of the star from FLAME using G band magnitude (lum_flame_spec)"}, {"name": "b_Lum-Flame", "desc": "? Lower confidence level (16%) of lumFlameSpec (lum_flame_spec_lower)"}, {"name": "B_Lum-Flame", "desc": "? Upper confidence level (84%) of lumFlameSpec (lum_flame_spec_upper)"}, {"name": "Mass-Flame", "desc": "? Mass of the star from FLAME using stellar models (mass_flame_spec)"}, {"name": "b_Mass-Flame", "desc": "? Lower confidence level (16%) of massFlameSpec (mass_flame_spec_lower)"}, {"name": "B_Mass-Flame", "desc": "? Upper confidence level (84%) of massFlameSpec (mass_flame_spec_upper)"}, {"name": "Age-Flame", "desc": "? Age of the star from FLAME using stellar models (age_flame_spec)"}, {"name": "b_Age-Flame", "desc": "? Lower confidence level (16%) of ageFlameSpec (age_flame_spec_lower)"}, {"name": "B_Age-Flame", "desc": "? Upper confidence level (84%) of ageFlameSpec (age_flame_spec_upper)"}, {"name": "Flag-Flame", "desc": "[0/2]? Flag indicating quality of parameters from FLAME using GSP-Spec parameters (flags_flame_spec) (2)"}, {"name": "Evol", "desc": "? Evolutionary stage of the star from FLAME using stellar models (evolstage_flame_spec)"}, {"name": "z-Flame", "desc": "? Gravitational redshift from FLAME using GSP-Spec parameters (gravredshift_flame_spec)"}, {"name": "b_z-Flame", "desc": "? Lower confidence interval of gravredshiftFlameSpec (gravredshift_flame_spec_lower)"}, {"name": "B_z-Flame", "desc": "? Upper confidence interval of gravredshiftFlameSpec (gravredshift_flame_spec_upper)"}, {"name": "BolCorr", "desc": "? Bolometric correction applied to derive lumFlameSpec using GSP-Spec parameters (bc_flame_spec)"}]}, {"name": "tgextmap.dat", "desc": "Total Galactic Extinction (TGE) map for extinction parameters A0", "columns": [{"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "HPId", "desc": "Unique HEALPix index number for which the total Galactic extinction parameters are estimated (healpix_id)"}, {"name": "HPlevel", "desc": "[6/9] HEALPix level used (healpix_level) n "}, {"name": "A0", "desc": "? Mean A_0_ extinction parameter (a0) (1) "}, {"name": "e_A0", "desc": "? Uncertainty for the mean A_0_ (a0_uncertainty)"}, {"name": "b_A0", "desc": "? Minimum A_0_ value used for the HEALPix of interest (a0_min)"}, {"name": "B_A0", "desc": "? Maximum A_0_ value used for the HEALPix of interest (a0_max)"}, {"name": "Ntracers", "desc": "Number of tracers used (num_tracers_used) "}, {"name": "foptHP", "desc": "[0/1] Flag to indicate whether a given HEALPix level is the optimum (1) or not (0) (optimum_hpx_flag) (2)"}, {"name": "Status", "desc": "[0/3] Exit status for TGE (status) (3) "}]}, {"name": "tgextopt.dat", "desc": "Optimum version of the Total Galactic Extinction Map, derived from the table tgextmap.dat (total_galactic_extinction_map) at a single HELPix level 9", "columns": [{"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "HPId", "desc": "Unique HEALPix index number for which the total Galactic extinction parameters are estimated (healpix_id)"}, {"name": "A0", "desc": "?=- Median A_0_ extinction parameter (a0) (1) "}, {"name": "e_A0", "desc": "?=- Uncertainty for the mean A_0_ (a0_uncertainty)"}, {"name": "Ntracers", "desc": "Number of tracers used (num_tracers_used) "}, {"name": "Status", "desc": "[0/3] Exit status for TGE (status) (2) "}, {"name": "HPlevel", "desc": "[6/9] Number indicating which HEALPix level was chosen to populate this HEALPix (optimum_hpx_level)"}]}, {"name": "oaninfo.dat", "desc": "Content of a Self-Organized Map calculated from a dataset composed by outliers by the Apsis module OA (oa_neuron_information)", "columns": [{"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "SOMID", "desc": "Self-Organized Map identifier (som_id) "}, {"name": "NeuId", "desc": "Neuron identifier (neuron_id) "}, {"name": "NeuRowIdx", "desc": "[0/29] Row index of the neuron in the Self-Organised Map lattice (neuron_row_index)"}, {"name": "NeuColIdx", "desc": "[0/29] Column index of the neuron in the Self-Organised Map lattice (neuron_column_index)"}, {"name": "hits", "desc": "Number of sources populating the neuron (hits)"}, {"name": "Class", "desc": "? Astronomical class estimated for the neuron (class_label)"}, {"name": "CentId", "desc": "Identifier of the Gaia source that minimizes the classification distance to the neuron (centroid_id)"}, {"name": "CentDist", "desc": "Squared Euclidean distance between the centroid XP spectrum and the neuron XP prototype (centroid_distance)"}, {"name": "TempDist", "desc": "? Squared Euclidean distance between the reference XP template and the neuron XP prototype (template_distance)"}, {"name": "Gmag", "desc": "Mean G value for the sources that belong to the neuron (g_mag_mean)"}, {"name": "s_Gmag", "desc": "Standard deviation of G values for the sources that belong to the neuron (g_mag_std_dev)"}, {"name": "b_Gmag", "desc": "Minimum G value for the sources that belong to the neuron (g_mag_min)"}, {"name": "B_Gmag", "desc": "Maximum G value for the sources that belong to the neuron (g_mag_max)"}, {"name": "BPmag", "desc": "Mean G_BP_ value for the sources that belong to the neuron (bp_mag_mean)"}, {"name": "s_BPmag", "desc": "Standard deviation of G_BP_ values for the sources that belong to the neuron (bp_mag_std_dev)"}, {"name": "b_BPmag", "desc": "Minimum value of G_BP_ for the sources that belong to the neuron (bp_mag_min)"}, {"name": "B_BPmag", "desc": "Maximum value of G_BP_ for the sources that belong to the neuron (bp_mag_max)"}, {"name": "RPmag", "desc": "Mean G_RP_ value for the sources that belong to the neuron neuron (rp_mag_mean)"}, {"name": "s_RPmag", "desc": "Standard deviation of G_RP_ values for the sources that belong to the neuron (rp_mag_std_dev)"}, {"name": "b_RPmag", "desc": "Minimum value of G_RP_ for the sources that belong to the neuron (rp_mag_min)"}, {"name": "B_RPmag", "desc": "Maximum value of G_RP_ for the sources that belong to the neuron (rp_mag_max)"}, {"name": "pmRA", "desc": "Mean value of the proper motion in right ascension for the sources that belong to the neuron (pm_ra_mean)"}, {"name": "s_pmRA", "desc": "Standard deviation of the proper motion in right ascension for the sources that belong to the neuron (pm_ra_std_dev)"}, {"name": "b_pmRA", "desc": "Minimum value of the proper motion in right ascension for the sources that belong to the neuron (pm_ra_min)"}, {"name": "B_pmRA", "desc": "Maximum value of the proper motion in right ascension for the sources that belong to the neuron (pm_ra_max)"}, {"name": "pmDE", "desc": "Mean value of the proper motion in declination for the sources that belong to the neuron (pm_dec_mean)"}, {"name": "s_pmDE", "desc": "Standard deviation of the proper motion in declination for the sources that belong to the neuron (pm_dec_std_dev)"}, {"name": "b_pmDE", "desc": "Minimum value of the proper motion in declination for the sources that belong to the neuron (pm_dec_min)"}, {"name": "B_pmDE", "desc": "Maximum value of the proper motion in declination for the sources that belong to the neuron (pm_dec_max)"}, {"name": "Plx", "desc": "Mean parallax value for the sources that belong to the neuron (parallax_mean)"}, {"name": "s_Plx", "desc": "Standard deviation of the parallax values for the sources that belong to the neuron (parallax_std_dev)"}, {"name": "b_Plx", "desc": "Minimum parallax value for the sources that belong to the neuron (parallax_min)"}, {"name": "B_Plx", "desc": "Maximum parallax value for the sources that belong to the neuron (parallax_max)"}, {"name": "GLON", "desc": "[] Mean galactic latitude for the sources that belong to the neuron (gal_latitude_mean)"}, {"name": "s_GLON", "desc": "Standard deviation of the galactic latitude values for the sources that belong to the neuron (gal_latitude_std_dev)"}, {"name": "b_GLON", "desc": "Minimum galactic latitude for the sources that belong to the neuron (gal_latitude_min)"}, {"name": "B_GLON", "desc": "Maximum galactic latitude for the sources that belong to the neuron (gal_latitude_max)"}, {"name": "intraDist", "desc": "Mean value of the squared Euclidean distance between each of the XP sources in the neuron and the neuron prototype (intra_neuron_distance_mean)"}, {"name": "s_intraDist", "desc": "Standard deviation of the squared Euclidean distance between each of the XP sources in the neuron and the neuron prototype (intra_neuron_distance_std_dev)"}, {"name": "b_intraDist", "desc": "Minimum squared Euclidean distance between each of the XP sources in the neuron and the neuron prototype (intra_neuron_distance_min)"}, {"name": "B_intraDist", "desc": "Maximum squared Euclidean distance between each of the XP sources in the neuron and the neuron prototype (intra_neuron_distance_max)"}, {"name": "interDist", "desc": "Mean value of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighbours (inter_neuron_distance_mean)"}, {"name": "s_interDist", "desc": "Standard deviation of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighbours (inter_neuron_distance_std_dev)"}, {"name": "b_interDist", "desc": "Minimum value of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighbours (inter_neuron_distance_min)"}, {"name": "B_interDist", "desc": "Maximum value of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighbours (inter_neuron_distance_max)"}, {"name": "Template", "desc": "Name of the template used to describe the neuron (template_name)"}, {"name": "dist25", "desc": "25th percentile value for the intra-neuron distance distribution (distance_percentile25)"}, {"name": "dist50", "desc": "50th percentile value for the intra-neuron distance distribution (distance_percentile50)"}, {"name": "dist68", "desc": "68th percentile value for the intra-neuron distance distribution (distance_percentile68)"}, {"name": "dist75", "desc": "75th percentile value for the intra-neuron distance distribution (distance_percentile75)"}, {"name": "dist99", "desc": "95th percentile value for the intra-neuron distance distribution (distance_percentile95)"}, {"name": "distFWHM", "desc": "Full Width at Half Maximum value for the intra-neuron distance distribution (distance_fwhm)"}, {"name": "distSkew", "desc": "Skewness value for the intra-neuron distance distribution (distance_skew)"}, {"name": "distKur", "desc": "Kurtosis value for the intra-neuron distance distribution (distance_kurtosis)"}, {"name": "distiqr", "desc": "Inter-Quartile Range value for the intra-neuron distance distribution (distance_i_q_r)"}, {"name": "distFWHMn", "desc": "Normalized FWHM value for the intra-neuron distance distribution (distance_fwhm_norm)"}, {"name": "Quality", "desc": "[0/6] Quality category assigned to the neuron (quality_category)"}, {"name": "NBP", "desc": "Mean value of the number of BP transits for the sources that belong to the neuron (bp_transits_mean)"}, {"name": "s_NBP", "desc": "Standard deviation of the number of BP transits for the sources that belong to the neuron (bp_transits_std_dev)"}, {"name": "b_NBP", "desc": "Minimum value of the number of BP transits for the sources that belong to the neuron (bp_transits_min)"}, {"name": "B_NBP", "desc": "Maximum value of the number of BP transits for the sources that belong to the neuron (bp_transits_max)"}, {"name": "NRP", "desc": "Mean value of the number of RP transits for the sources that belong to the neuron (rp_transits_mean)"}, {"name": "s_NRP", "desc": "Standard deviation of the number of RP transits for the sources that belong to the neuron (rp_transits_std_dev)"}, {"name": "b_NRP", "desc": "Minimum value of the number of RP transits for the sources that belong to the neuron (rp_transits_min)"}, {"name": "B_NRP", "desc": "Maximum value of the number of RP transits for the sources that belong to the neuron (rp_transits_max)"}, {"name": "RUWE", "desc": "Mean value of the renormalised unit weight error for the sources that belong to the neuron (ruwe_mean)"}, {"name": "s_RUWE", "desc": "Standard deviation of the renormalised unit weight error for the sources that belong to the neuron (ruwe_std_dev)"}, {"name": "b_RUWE", "desc": "Minimum value of the renormalised unit weight error for the sources that belong to the neuron (ruwe_min)"}, {"name": "B_RUWE", "desc": "Maximum value of the renormalised unit weight error for the sources that belong to the neuron (ruwe_max)"}, {"name": "E(BP/RP)", "desc": "Mean value of the BP/RP flux excess for the sources that belong to the neuron (bprp_mean_flux_excess_mean)"}, {"name": "s_E(BP/RP)", "desc": "Standard deviation of the BP/RP flux excess for the sources that belong to the neuron (bprp_mean_flux_excess_std_dev)"}, {"name": "b_E(BP/RP)", "desc": "Minimum value of the BP/RP flux excess for the sources that belong to the neuron (bprp_mean_flux_excess_min)"}, {"name": "B_E(BP/RP)", "desc": "Maximum value of the BP/RP flux excess for the sources that belong to the neuron (bprp_mean_flux_excess_max)"}, {"name": "BP-RP", "desc": "Mean value of the G_BP_-G_RP_ colour for the sources that belong to the neuron (bprp_colour_mean)"}, {"name": "s_BP-RP", "desc": "Standard deviation of the G_BP_-G_RP_ colour for the sources that belong to the neuron (bprp_colour_std_dev)"}, {"name": "b_BP-RP", "desc": "Minimum value of the G_BP_-G_RP_ colour for the sources that belong to the neuron (bprp_colour_min)"}, {"name": "B_BP-RP", "desc": "Maximum value of the G_BP_-G_RP_ colour for the sources that belong to the neuron (bprp_colour_max)"}]}, {"name": "oaxpsp.dat", "desc": "Prototype BP/RP spectrum corresponding to each of the neurons of the Self-Organised-Map produced by the Apsis module OA (oa_neuron_xp_spectra)", "columns": [{"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "NeuId", "desc": "Neuron identifier (neuron_id) "}, {"name": "NeuRowIdx", "desc": "[0/29] Row index of the neuron in the Self-Organised Map lattice (neuron_row_index)"}, {"name": "NeuColIdx", "desc": "[0/29] Column index of the neuron in the Self-Organised Map lattice (neuron_column_index)"}, {"name": "XPFlux", "desc": "Normalised flux at wavelength XPlambda for the preprocessed XP spectrum that best represents the neuron (prototype) (xp_spectrum_prototype_flux)"}, {"name": "XPlambda", "desc": "Wavelength associated with the XP spectrum flux values (xp_spectrum_prototype_wavelength)"}, {"name": "XPFluxTemp", "desc": "? Normalised flux at wavelength XPlambda for the preprocessed XP spectrum corresponding to the neuron template (xp_spectrum_template_flux)"}]}, {"name": "epphot.sam", "desc": "Light curves for a given object in bands G, BP and RP (11754237 rows) (epoch_photometry)", "columns": [{"name": "Source", "desc": "Unique source identifier (unique within a particular Data Release) (source_id)"}, {"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2016.0 (ra) "}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2016.0 (dec) "}, {"name": "TransitID", "desc": "Transit unique identifier (transit_id) "}, {"name": "TimeG", "desc": "? Transit averaged G band observing time JD-2455197.5 (g_transit_time)"}, {"name": "FG", "desc": "? Transit averaged G band flux (g_transit_flux)"}, {"name": "e_FG", "desc": "? Transit averaged G band flux error (g_transit_flux_error)"}, {"name": "RFG", "desc": "? Transit averaged G band flux divided by its error (g_transit_flux_over_error)"}, {"name": "Gmag", "desc": "? Transit averaged G band Vega magnitude (g_transit_mag)"}, {"name": "NG", "desc": "[0-9] Number of CCD observations contributing to transit averaged G band flux (g_transit_n_obs)"}, {"name": "TimeBP", "desc": "? BP CCD transit observing time JD-2455197.5 (bp_obs_time)"}, {"name": "FBP", "desc": "? BP band flux (bp_flux) "}, {"name": "e_FBP", "desc": "? BP band flux error (bp_flux_error) "}, {"name": "RFBP", "desc": "? BP band flux divided by its error (bp_flux_over_error)"}, {"name": "BPmag", "desc": "? BP band Vega magnitude (bp_mag) "}, {"name": "TimeRP", "desc": "? RP CCD transit observing time JD-2455197.5 (rp_obs_time)"}, {"name": "FRP", "desc": "? BP band flux (rp_flux) "}, {"name": "e_FRP", "desc": "? BP band flux error (rp_flux_error) "}, {"name": "RFRP", "desc": "? BP band flux divided by its error (rp_flux_over_error)"}, {"name": "RPmag", "desc": "? BP band Vega magnitude (rp_mag) "}, {"name": "noisyFlag", "desc": "[0/1] G band flux scatter larger than expected by photometry processing (all CCDs considered) (photometry_flag_noisy_data)"}, {"name": "SMuFlag", "desc": "[0/1] SM transit unavailable by photometry processing (photometry_flag_sm_unavailable)"}, {"name": "AF1uFlag", "desc": "[0/1] AF1 transit unavailable by photometry processing (photometry_flag_af1_unavailable)"}, {"name": "AF2uFlag", "desc": "[0/1] AF2 transit unavailable by photometry processing (photometry_flag_af2_unavailable)"}, {"name": "AF3uFlag", "desc": "[0/1] AF3 transit unavailable by photometry processing (photometry_flag_af3_unavailable)"}, {"name": "AF4uFlag", "desc": "[0/1] AF4 transit unavailable by photometry processing (photometry_flag_af4_unavailable)"}, {"name": "AF5uFlag", "desc": "[0/1] AF5 transit unavailable by photometry processing (photometry_flag_af5_unavailable)"}, {"name": "AF6uFlag", "desc": "[0/1] AF6 transit unavailable by photometry processing (photometry_flag_af6_unavailable)"}, {"name": "AF7uFlag", "desc": "[0/1] AF7 transit unavailable by photometry processing (photometry_flag_af7_unavailable)"}, {"name": "AF8uFlag", "desc": "[0/1] AF8 transit unavailable by photometry processing (photometry_flag_af8_unavailable)"}, {"name": "AF9uFlag", "desc": "[0/1] AF9 transit unavailable by photometry processing (photometry_flag_af9_unavailable)"}, {"name": "BPuFlag", "desc": "[0/1] BP transit unavailable by photometry processing (photometry_flag_bp_unavailable)"}, {"name": "RPuFlag", "desc": "[0/1] RP transit unavailable by photometry processing (photometry_flag_rp_unavailable)"}, {"name": "SMrFlag", "desc": "[1] SM transit rejected by photometry processing (photometry_flag_sm_reject)"}, {"name": "AF1rFlag", "desc": "[0/1] AF1 transit rejected by photometry processing (photometry_flag_af1_reject)"}, {"name": "AF2rFlag", "desc": "[0/1] AF2 transit rejected by photometry processing (photometry_flag_af2_reject)"}, {"name": "AF3rFlag", "desc": "[0/1] AF3 transit rejected by photometry processing (photometry_flag_af3_reject)"}, {"name": "AF4rFlag", "desc": "[0/1] AF4 transit rejected by photometry processing (photometry_flag_af4_reject)"}, {"name": "AF5rFlag", "desc": "[0/1] AF5 transit rejected by photometry processing (photometry_flag_af5_reject)"}, {"name": "AF6rFlag", "desc": "[0/1] AF6 transit rejected by photometry processing (photometry_flag_af6_reject)"}, {"name": "AF7rFlag", "desc": "[0/1] AF7 transit rejected by photometry processing (photometry_flag_af7_reject)"}, {"name": "AF8rFlag", "desc": "[0/1] AF8 transit rejected by photometry processing (photometry_flag_af8_reject)"}, {"name": "AF9rFlag", "desc": "[0/1] AF9 transit rejected by photometry processing (photometry_flag_af9_reject)"}, {"name": "BPrFlag", "desc": "[0/1] BP transit rejected by photometry processing (photometry_flag_bp_reject)"}, {"name": "RPrFlag", "desc": "[0/1] RP transit rejected by photometry processing (photometry_flag_rp_reject)"}, {"name": "GrVFlag", "desc": "[0/1] Average G transit photometry rejected by variability processing (variability_flag_g_reject)"}, {"name": "BPrVFlag", "desc": "[0/1] BP transit photometry rejected by variability processing (variability_flag_bp_reject)"}, {"name": "RPrVFlag", "desc": "[0/1] RP transit photometry rejected by variability processing (variability_flag_rp_reject)"}]}, {"name": "gcrf3xm.dat", "desc": "Full cross-match information for the Gaia-CRF3 sources (Gaia_Crf3_Xm)", "columns": [{"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "Source", "desc": "Gaia source identifier (source_id) "}, {"name": "ICRF3sx", "desc": "[0/1] The flag describing if the Gaia-CRF3 source was found in ICRF3 S/X (icrf3sx)"}, {"name": "ICRF3k", "desc": "[0/1] The flag describing if the Gaia-CRF3 source was found in ICRF3 K (icrf3k)"}, {"name": "ICRF3xka", "desc": "[0/1] The flag describing if the Gaia-CRF3 source was found in ICRF3 X/Ka (icrf3xka)"}, {"name": "ICRFname", "desc": "The ICRF name of the source (icrf_name) "}, {"name": "IERSname", "desc": "The IERS name of the source (iers_name) "}, {"name": "OCARS", "desc": "[0/1] The flag describing if the Gaia-CRF3 source was found in OCARS,"}]}, {"name": "rvsmean.sam", "desc": "RVS mean sampled spectrum table (2400147645 lines) (rvs_mean_spectrum)", "columns": [{"name": "Source", "desc": "Unique source identifier (unique within a particular Data Release) (source_id)"}, {"name": "RAdeg", "desc": "Right Ascension ICRS ar Ep=2016.0 (ra) "}, {"name": "DEdeg", "desc": "Declination ICRS ar Ep=2016.0 (dec) "}, {"name": "NTransit", "desc": "Number of combined transits (combined_transits)"}, {"name": "NcCCD", "desc": "Number of combined CCD spectra (combined_ccds) "}, {"name": "NdCDD", "desc": "Number of deblended CCD spectra (deblended_ccds)"}, {"name": "lambda", "desc": "[846/870] Wavelength (wavelength) (1) "}, {"name": "Flux", "desc": "? Normalized flux (flux) (1) "}, {"name": "e_Flux", "desc": "? Uncertainties in Flux (flux_error) (1) "}]}, {"name": "xpsummary.sam", "desc": "Auxiliary information about the mean BP/RP spectrum (219197643 sources) (xp_summary)", "columns": [{"name": "Source", "desc": "Unique source identifier (unique within a particular Data Release) (source_id)"}, {"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2016.0 (ra) "}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2016.0 (dec) "}, {"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "NBPbases", "desc": "? Number of bases that are relevant for the representation of this mean BP spectrum (bp_n_relevant_bases)"}, {"name": "BPrelsh", "desc": "? Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean BP spectrum (bp_relative_shrinking)"}, {"name": "NBP", "desc": "? Number of measurements used for the BP spectrum generation (bp_n_measurements)"}, {"name": "NBPrej", "desc": "? Number of rejected measurements in the BP spectrum generation (bp_n_rejected_measurements)"}, {"name": "BPstddev", "desc": "? Standard deviation for the BP spectrum representation (bp_standard_deviation)"}, {"name": "BPchi2r", "desc": "? Chi squared for the BP spectrum representation (bp_chi_squared)"}, {"name": "NTransBP", "desc": "? Number of transits contributing to the mean in BP (bp_n_transits)"}, {"name": "NcTransBP", "desc": "? Number of contaminated transits in BP (bp_n_contaminated_transits)"}, {"name": "NbTransBP", "desc": "? Number of blended transits in BP (bp_n_blended_transits)"}, {"name": "NRPbases", "desc": "Number of bases that are relevant for the representation of this mean RP spectrum (rp_n_relevant_bases)"}, {"name": "NRPrelsh", "desc": "Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean RP spectrum (rp_relative_shrinking)"}, {"name": "NRP", "desc": "Number of measurements used for the RP spectrum generation (rp_n_measurements)"}, {"name": "NRPrej", "desc": "Number of rejected measurements in the RP spectrum generation (rp_n_rejected_measurements)"}, {"name": "RPstdev", "desc": "Standard deviation for the RP spectrum representation (rp_standard_deviation)"}, {"name": "RPchi2r", "desc": "Chi squared for the RP spectrum representation (rp_chi_squared)"}, {"name": "NTransRP", "desc": "Number of transits contributing to the mean in RP (rp_n_transits)"}, {"name": "NcTransRP", "desc": "Number of contaminated transits in RP (rp_n_contaminated_transits)"}, {"name": "NbTransRP", "desc": "Number of blended transits in RP (rp_n_blended_transits)"}]}, {"name": "xpsample.sam", "desc": "BP/RP externally calibrated sampled mean spectrum (11822651939 rows) (xp_sampled_mean_spectrum)", "columns": [{"name": "Source", "desc": "Unique source identifier (unique within a particular Data Release) (source_id)"}, {"name": "RAdeg", "desc": "Right Ascension (ICRS) at Ep=2016.0 (ra) "}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2016.0 (dec) "}, {"name": "lambda", "desc": "Wavelength (wavelength) (1) "}, {"name": "Flux", "desc": "Mean BP + RP combined spectrum flux (flux) "}, {"name": "e_Flux", "desc": "Mean BP + RP combined spectrum flux error (flux_error)"}]}, {"name": "xpsamp.dat", "desc": "Definition of XP spectra standard sampling schemes (xp_sampling)", "columns": [{"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "Band", "desc": "[BP RP] BP or RP photometric band (band) "}, {"name": "lambda", "desc": "Wavelength (wavelength) (1) "}, {"name": "Func", "desc": "[0/54] Basis function index (basis_function)"}, {"name": "SampCoeff", "desc": "Sampling matrix coefficient (sampling_coefficient)"}]}, {"name": "xpmerge.dat", "desc": "Coefficients used to merge the BP and RP externally calibrated sampled spectra into the final merged product (xp_merge)", "columns": [{"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "lambda", "desc": "Wavelength (wavelength) (1) "}, {"name": "weightBP", "desc": "BP flux weight (bp_weight) "}, {"name": "weightRP", "desc": "RP flux weight (rp_weight) "}]}, {"name": "xpcont.sam", "desc": "Mean BP and RP spectra based on the continuous representation in basis functions (219197643 rows) (gaia_dr3_xpcont)", "columns": [{"name": "Source", "desc": "Unique source identifier (unique within a particular Data Release) (source_id)"}, {"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2016.0 (ra) "}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2016.0 (dec) "}, {"name": "SolID", "desc": "Solution Identifier (solution_id) "}, {"name": "BPDOF", "desc": "? Degrees of freedom for the BP spectrum representation (bp_degrees_of_freedom)"}, {"name": "NBP", "desc": "? Number of measurements used for the BP spectrum generation (bp_n_measurements) "}, {"name": "BPNrej", "desc": "? Number of rejected measurements in the BP spectrum generation (bp_n_rejected_measurements)"}, {"name": "BPstddev", "desc": "? Standard deviation for the BP spectrum representation (bp_standard_deviation)"}, {"name": "BPchi2r", "desc": "? Chi squared for the BP spectrum representation (bp_chi_squared)"}, {"name": "NBPbases", "desc": "? Number of bases that are relevant for the representation of this mean BP"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"II_254"}} {"id": "II/254", "title_cds": "Minnesota Automated Plate Scanner catalog", "title_create": "Cabanela+ 2003", "year": "2003", "author": "Cabanela J.E., Humphreys R.M., Aldering G., Larsen J.A., Odewahn S.C., Thurmes P.M., Cornuelle C.S.", "title_pub": "The Minnesota Automated Plate Scanner catalog of the POSS I (MAPS)", "first_author": "Cabanela J.E.", "ref_biblio": [""], "bibcode": ["2003PASP..115..837C"], "see_also": ["http://iparrizar.stcloudstate.edu/~juan/MAPS_Database/catalog/"], "keyword_cds": "Surveys ; Photometry, photographic ; Photometry, surface", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["MAPS"], "records": ["records"], "doi_pub": ["10.1086/375625"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"II_268"}} {"id": "II/268", "title_cds": "The 2dF QSO Redshift Survey Input Catalogue", "title_create": "Smith+ 2005", "year": "2005", "author": "Smith R.J., Croom S.M., Boyle B.J., Shanks T., Miller L., Loaring N.S.", "title_pub": "The 2dF QSO Redshift Survey - III. The Input Catalogue", "first_author": "Smith R.J.", "ref_biblio": [""], "see_also": ["http://www.2dfquasar.org/Phot_Cat/ubrcatalogue.html"], "keyword_cds": "Photometry, photographic ; Survey", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["2dF"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "04-Jun-2006"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"II_279"}} {"id": "II/279", "title_cds": "EROS-II in the Magellanic Clouds", "title_create": "Marquette+ 2007", "year": "2007", "author": "Marquette J.B., Lesquoy E., (EROS collaboration)", "title_pub": "Final photometric catalog of EROS-II in the Magellanic Clouds", "first_author": "Marquette J.B.", "ref_biblio": ["< Astron. Astrophys. (in press) >"], "keyword_cds": "Magellanic Clouds ; Surveys ; Photometry, CCD ; Stars, variable", "keyword_pub": "(A&A )", "alias": ["EROS2"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "08-Jun-2007", "tables": [{"name": "fields.dat", "desc": "Limits in the EROS-II fields ", "columns": [{"name": "Field", "desc": "Name of field, starting by \"lm\" or \"sm\" for Large and Small Magellanic cloud respectively."}, {"name": "RAmin", "desc": "Lower limit of RA (J2000) in Field "}, {"name": "RAmax", "desc": "Upper limit of RA (J2000) in Field "}, {"name": "DEmin", "desc": "Lower limit of Dec (J2000) in Field "}, {"name": "DEmax", "desc": "Upper limit of Dec (J2000) in Field "}]}, {"name": "CAT/*/*.dat", "desc": "Field files with a total of 32,687,748 stars ", "columns": [{"name": "EROSid", "desc": "EROS identification (1) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Rmag", "desc": "Red magnitude (filter?) "}, {"name": "e_Rmag", "desc": "Mean error on Rmag "}, {"name": "Rx", "desc": "X position in red observation "}, {"name": "Ry", "desc": "Y position in red observation "}, {"name": "Bmag", "desc": "Blue magnitude (filter?) "}, {"name": "e_Bmag", "desc": "Mean error on Bmag "}, {"name": "Bx", "desc": "X position in blue observation "}, {"name": "By", "desc": "Y position in blue observation "}, {"name": "Var", "desc": "[0,511] Variability flags (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"II_291"}} {"id": "II/291", "title_cds": "Third Photometric Magnitude Difference Catalog", "title_create": "Mason, 2008", "year": "2008", "author": "Worley C.E., Mason B.D., Wycoff G.L.", "title_pub": "Third Photometric Magnitude Difference Catalog", "first_author": "Worley C.E.", "ref_biblio": [""], "see_also": ["http://ad.usno.navy.mil/wds/dm3.html : the Magnitude Difference Catalog", "B/wds : Washington Double Star Catalog (WDS)"], "keyword_cds": "Stars, double and multiple ; Photometry", "keyword_pub": "Binaries: General, Stars: Binaries: Visual, Catalogs", "description": ["The Photometric Magnitude Difference Catalog is a collection of all", "double star photometric data which does not contain astrometric", "information and is therefore inappropriate for the Washington Double", "Star Catalog. Magnitude difference information can be useful in", "estimating mass ratios, determining photocentric positions which are", "color dependent, or into investigations of variability in close binary", "systems. Due to uncertainties in bandpass characteristics or", "variability, no summary line is presented, rather a complete listing", "of all data.", "This version supersedes the"], "type": ["BCC"], "records": ["45445 binaries"], "data": "", "date_update": "12-Aug-2012", "tables": [{"name": "deltam.dat", "desc": "Delta-M Catalog ", "columns": [{"name": "RAh", "desc": "*Right Ascension 2000 (hours) "}, {"name": "RAdm", "desc": "*Right Ascension 2000 (minutes) "}, {"name": "DE-", "desc": "*Declination 2000 (sign) "}, {"name": "DEd", "desc": "*Declination 2000 (degrees) "}, {"name": "DEm", "desc": "*Declination 2000 (minutes) "}, {"name": "DiscName", "desc": "*Discoverer Code & Number "}, {"name": "Comp", "desc": "*Component Identification "}, {"name": "dm", "desc": "Magnitude Difference "}, {"name": "o_dm", "desc": "?Number of observations used to compute dm"}, {"name": "r_dm", "desc": "*Reference Code "}, {"name": "Meth", "desc": "*Observational Method "}, {"name": "Notes", "desc": "*?Notes "}]}, {"name": "dm.txt", "desc": "Delta-M Catalog Documentation ", "columns": []}, {"name": "table1.txt", "desc": "ascii version of Table 1 ", "columns": []}, {"name": "method.txt", "desc": "method key for deltam.dat ", "columns": []}, {"name": "refs.dat", "desc": "Reference file ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"II_302"}} {"id": "II/302", "title_cds": "The SWIRE Data Release 2", "title_create": "Surace+ 2005", "year": "2005", "author": "Surace et al.", "title_pub": "The Spitzer Wide-area InfraRed Extragalactic survey (SWIRE) Data Release 2", "first_author": "Surace et al.", "ref_biblio": ["< Caltech, 2005 >"], "bibcode": ["2012yCat.2302....0S"], "see_also": ["http://irsa.ipac.caltech.edu/data/SPITZER/SWIRE/ : SWIRE Home page", "II/290 : SWIRE Photometric Redshift Catalogue (Rowan-Robinson+, 2008)"], "keyword_cds": "Surveys ; Galaxies, IR ; Galaxies, photometry", "mission": "Spitzer", "description": ["The Spitzer Wide-area InfraRed Extragalactic Survey (SWIRE) is a", "wide-area, high galactic latitude, imaging survey to trace the", "evolution of dusty, star-forming galaxies, evolved stellar", "populations, and active galactic nuclei. SWIRE has surveyed roughly 50", "square degrees with the MIPS far-infrared camera and the with the IRAC", "mid-infrared camera. The regions included are ELAIS-N1, ELAIS-N2,", "XMM-LSS, the Lockman Hole (LH), ELAIS-S1 and Chandra Deep Field South", "(CDFS)."], "curator": "Francois Ochsenbein [CDS]", "alias": ["SWIRE-2", "SWIRE"], "records": ["records"], "data": "", "date_update": "12-Dec-2012"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"II_304"}} {"id": "II/304", "title_cds": "UKIDSS-DR5", "title_create": "Lawrence+ 2011", "year": "2011", "author": "UKIDSS Consortium", "title_pub": "UKIRT Infrred Deep Sky Survey (UKIDSS) Release 5", "first_author": "UKIDSS Consortium", "ref_biblio": [""], "bibcode": ["2007MNRAS.379.1599L", "2011yCat.2304....0U"], "see_also": ["http://www.ukidss.org/ : UKIDSS Home page"], "keyword_cds": "Surveys ; Infrared sources ; Photometry, infrared", "keyword_pub": "surveys - infrared: general", "description": ["The UKIRT Infrared Deep Sky Survey (UKIDSS) can be considered the", "near-infrared (near-IR) counterpart of the Sloan Digital Sky Survey", "(SDSS; see Cat. II/294). It does not cover the whole sky, but is many", "times deeper than the Two-Micron All-Sky Survey (2MASS, see Cat.", "II/246; Skrutskie et al. 2006AJ....131.1163S). It is in fact not a", "single survey but a survey programme combining a set of five survey", "components of complementary combinations of depth and area, covering", "several thousand square degrees to K~18, 35deg^2^ to K~21, and", "0.77deg^2^ to K~23. The survey uses the Wide Field Camera (WFCAM) on", "the 3.8m United Kingdom Infra-Red Telescope (UKIRT). WFCAM has an", "instantaneous field of view of 0.21 deg^2^, considerably larger than", "any previous IR camera on a 4-m class telescope, along with a pixel", "size of 0.4arcsec. The tip-tilt system on UKIRT delivers close to", "natural seeing (median size 0.6 arcsec) across the whole field of", "view. The combination of large telescope, large field of view, and", "good image quality, makes possible a survey of considerably greater", "scope than that of 2MASS. The various surveys employ up to five", "filters ZYJHK covering the wavelength range 0.83\u00ad2.37{mu}m and extend", "over both high and low Galactic latitudes. The survey began on 2005", "May 13, and is expected to take 7yr to complete. The survey is being", "carried out by a private consortium but is fully public with no", "proprietary rights for the consortium. Data products are being being", "released in stages, with the intention of having these roughly twice", "a year."], "curator": "Francois Ochsenbein [CDS]", "alias": ["UKIDSS-DR5", "UKIDSS"], "type": ["OC"], "records": ["47230108 sources"], "doi_pub": ["10.1111/j.1365-2966.2007.12040.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"II_352"}} {"id": "II/352", "title_cds": "The VISTA Hemisphere Survey (VHS) catalog", "title_create": "McMahon+, 2013", "year": "2013", "author": "McMahon, R. G., Banerji, M., Gonzalez, E., Koposov, S. E., Bejar, V. J., Lodieu, N., Rebolo, R., The VHS Collaboration", "title_pub": "VISTA Hemisphere Survey band-merged multi-waveband catalogues (VHS)", "first_author": "McMahon", "ref_biblio": [""], "bibcode": ["2013Msngr.154...35M", "2017yCat.2352....0M"], "see_also": ["http://www.vista-vhs.org/ : VHS home page", "http://horus.roe.ac.uk/vsa/ : VISTA Science Archive home page"], "keyword_cds": "Photometry, infrared ; Surveys", "mission": "ESO", "abstract": ["The first Galactic and extragalactic results from the VISTA Hemisphere", "Survey (VHS) are presented. The aim of the VHS is to carry out a", "near-infrared survey which, when combined with other VISTA public", "surveys, will result in coverage of the whole southern celestial", "hemisphere (~20000deg^2^) to a depth 30 times fainter than the Two", "Micron All Sky Survey in at least two wavebands (J and Ks). The VHS", "vision includes a deep optical survey over the same area and this is", "now being realised with the VST surveys and the Dark Energy Survey,", "which has recently started. A summary of the survey progress is", "presented, with some follow-up results on low-mass stars and", "high-redshift quasars."], "description": ["Observations were made with the VIRCAM instrument on the ESO-VISTA", "telescope between 2009 November and 2013 October in Y, J, H and Ks", "filters."], "ack": ["Please include the following acknowledgment in any published material", "that makes use of the VHS products: Based on observations made with", "ESO Telescopes at the La Silla or Paranal Observatories under", "programme ID 179.A-2010"], "alias": ["VHS"], "type": ["OC"], "records": ["590835393 records"], "orcid_pub": ["0000-0001-8447-8869", "0000-0001-8447-8869"], "data": "", "islargetable": true, "date_creation": "21-Nov-2017", "date_update": "25-Feb-2021", "tables": [{"name": "vhs_dr3.sam", "desc": "VISTA Hemisphere Survey band-merged multi-waveband catalogues (VHS) DR3; sample output (on a total of 590,835,393 sources)", "columns": [{"name": "SrcID", "desc": "[472446402561/473037940311] Unique ID of this merged detection as assigned by merge algorithm (SOURCEID)"}, {"name": "RAdeg", "desc": "Celestial Right Ascension; J2000 (RA2000) "}, {"name": "DEdeg", "desc": "Celestial Declination; J2000 (DEC2000) "}, {"name": "Name", "desc": "Source name in IAU convention (SOURCENAME) "}, {"name": "CuID", "desc": "[451771] Unique ID of curation event giving rise to this record (always \"451771\") (CUEVENTID)"}, {"name": "FrID", "desc": "Unique ID of the set of frames that this merged source comes from (FRAMESETID)"}, {"name": "GLON", "desc": "Galactic longitude (L) "}, {"name": "GLAT", "desc": "Galactic latitude (B) "}, {"name": "priOrSec", "desc": "Seam code for a unique (=0) or duplicated (!=0) source (PRIORSEC)"}, {"name": "Y-Jpnt", "desc": "[-13/9]? Point source colour Y-J (using aperMag3) (YMJPNT)"}, {"name": "e_Y-Jpnt", "desc": "[/5999]? Error on Y-Jpnt (YMJPNTERR) "}, {"name": "J-Hpnt", "desc": "[-12/10]? Point source colour J-H (using aperMag3) (JMHPNT)"}, {"name": "e_J-Hpnt", "desc": "[/744]? Error on J-Hpnt (JMHPNTERR) "}, {"name": "H-Kspnt", "desc": "[-11/12]? Point source colour H-Ks (using aperMag3) (HMKSPNT)"}, {"name": "e_H-Kspnt", "desc": "[/627]? Error on H-Kspnt (HMKSPNTERR) "}, {"name": "J-Kspnt", "desc": "[-12/22]? Point source colour J-Ks (using aperMag3) (JMKSPNT)"}, {"name": "e_J-Kspnt", "desc": "[/13621]? Error on J-Kspnt (JMKSPNTERR) "}, {"name": "Y-Jext", "desc": "[-12/9]? Extended source colour Y-J (using aperMagNoAperCorr3) (YMJEXT)"}, {"name": "e_Y-Jext", "desc": "[/5999]? Error on Y-Jext (YMJEXTERR) "}, {"name": "J-Hext", "desc": "[-12/10]? Extended source colour J-H (using aperMagNoAperCorr3) (JMHEXT)"}, {"name": "e_J-Hext", "desc": "[/744]? Error on J-Hext (JMHEXTERR) "}, {"name": "H-Ksext", "desc": "[-11/12]? Extended source colour H-Ks (using aperMagNoAperCorr3) (HMKSEXT)"}, {"name": "e_H-Ksext", "desc": "[/627]? Error on H-Ksext (HMKSEXTERR) "}, {"name": "J-Ksext", "desc": "[-12/23]? Extended source colour J-Ks (using aperMagNoAperCorr3) (JMKSEXT)"}, {"name": "e_J-Ksext", "desc": "[/13621]? Error on J-Ksext (JMKSEXTERR) "}, {"name": "Clst", "desc": "Merged N(0,1) stellarness-of-profile statistic (MERGEDCLASSSTAT)"}, {"name": "Cl", "desc": "[-3/1] Class flag (MERGEDCLASS) (1) "}, {"name": "pStar", "desc": "Probability that the source is a star (PSTAR) "}, {"name": "pGal", "desc": "Probability that the source is a galaxy (PGALAXY) "}, {"name": "pNoise", "desc": "Probability that the source is noise (PNOISE) "}, {"name": "E(B-V)", "desc": "[0.001/8] The galactic dust extinction value measured from the Schlegel maps (EBV)"}, {"name": "AY", "desc": "[0.001/11] The galactic extinction correction in the Y band (AY)"}, {"name": "AJ", "desc": "[0.001/8] The galactic extinction correction in the J band (AJ)"}, {"name": "AH", "desc": "[/5] The galactic extinction correction in the H band (AH)"}, {"name": "AKs", "desc": "[/4] The galactic extinction correction in the Ks band (AKS)"}, {"name": "Ypmag", "desc": "[4/35]? Extended source VISTA Y mag (Petrosian) (YPETROMAG)"}, {"name": "e_Ypmag", "desc": "[0/255661]? Error in Ypmag (YPETROMAGERR) "}, {"name": "Yap3", "desc": "[4/34]? Default point source Y aperture corrected mag (2.0 arcsec diam) (YAPERMAG3)"}, {"name": "e_Yap3", "desc": "[/63914]? Error in default point/extended source Y mag (YAPERMAG3ERR)"}, {"name": "Yap4", "desc": "[4/34]? Point source Y aperture corrected mag (2.8 arcsec aperture diam) (YAPERMAG4)"}, {"name": "e_Yap4", "desc": "[/63442]? Error in point/extended source Y mag (2.8 arcsec aperture diam) (YAPERMAG4ERR)"}, {"name": "Yap6", "desc": "[3/38]? Point source Y aperture corrected mag (5.7 arcsec aperture diam) (YAPERMAG6)"}, {"name": "e_Yap6", "desc": "[/2719583]? Error in point/extended source Y mag (5.7 arcsec aperture diam) (YAPERMAG6ERR)"}, {"name": "Yapc3", "desc": "[4/35]? Default extended source Y aperture mag (2.0 arcsec diam) (YAPERMAGNOAPERCORR3)"}, {"name": "Yapc4", "desc": "[4/35]? Extended source Y aperture mag (2.8\" aperture diameter) (YAPERMAGNOAPERCORR4)"}, {"name": "Yapc6", "desc": "[3/38]? Extended source Y aperture mag (5.7\" aperture diameter) (YAPERMAGNOAPERCORR6)"}, {"name": "Yamaj", "desc": "[0/19]? Seeing corrected half-light, semi-major axis in Y band (YHLCORSMJRADAS)"}, {"name": "Yrms", "desc": "[0.7/303]? RMS of axes of ellipse fit in Y (YGAUSIG)"}, {"name": "Yell", "desc": "? 1-b/a, where a/b=semi-major/minor axes in Y (YELL)"}, {"name": "YPA", "desc": "? Ellipse fit celestial orientation in Y (YPA) "}, {"name": "Yerrb", "desc": "[/28] Processing warning/error bitwise flags in Y (YERRBITS)"}, {"name": "Yavg", "desc": "[0/112]? Average confidence in 2 arcsec diam default aperture 3 Y-band (YAVERAGECONF)"}, {"name": "YCl", "desc": "[/1] Discrete image classification flag in Y (YCLASS) (1)"}, {"name": "YClst", "desc": "[-109/444]? N(0,1) stellarness-of-profile statistic in Y (YCLASSSTAT)"}, {"name": "Yperrb", "desc": "[0/12587216] Additional Wide Field Astronomy Unit (WFAU) post-processing error bits in Y (<256: minor issues) (YPPERRBITS) (2)"}, {"name": "Yseq", "desc": "[/110314] The running number of the Y detection (YSEQNUM)"}, {"name": "Jpmag", "desc": "[-24/]? Extended source VISTA J mag (Petrosian) (JPETROMAG)"}, {"name": "e_Jpmag", "desc": "[0/]? Error in Jpmag (JPETROMAGERR) "}, {"name": "Jap3", "desc": "[-22/35]? Default point source J aperture corrected mag (2.0 arcsec diam) (JAPERMAG3)"}, {"name": "e_Jap3", "desc": "[0/76220]? Error in Jap3 (JAPERMAG3ERR) "}, {"name": "Jap4", "desc": "[-22/36]? Point source J aperture corrected mag (2.8 arcsec aperture diam) (JAPERMAG4)"}, {"name": "e_Jap4", "desc": "[0/1565601]? Error in Jap4 (JAPERMAG4ERR) "}, {"name": "Jap6", "desc": "[-22/38]? Point source J aperture corrected mag (5.7 arcsec aperture diam) (JAPERMAG6)"}, {"name": "e_Jap6", "desc": "[0/8556921]? Error in Jap6 (JAPERMAG6ERR) "}, {"name": "Japc3", "desc": "[-21/35]? Default extended source J aperture mag (2.0 arcsec diam) (JAPERMAGNOAPERCORR3)"}, {"name": "Japc4", "desc": "[-22/37]? Extended source J aperture mag (2.8\" aperture diameter) (JAPERMAGNOAPERCORR4)"}, {"name": "Japc6", "desc": "[-22/38]? Extended source J aperture mag (5.7\" aperture diameter) (JAPERMAGNOAPERCORR6)"}, {"name": "Jamaj", "desc": "[0/19]? Seeing corrected half-light, semi-major axis in J band (JHLCORSMJRADAS)"}, {"name": "Jrms", "desc": "[0.7/584]? RMS of axes of ellipse fit in J (JGAUSIG)"}, {"name": "Jell", "desc": "? 1-b/a, where a/b=semi-major/minor axes in J (JELL)"}, {"name": "JPA", "desc": "? Ellipse fit celestial orientation in J "}, {"name": "Jerrb", "desc": "[/28] Processing warning/error bitwise flags in J (JERRBITS)"}, {"name": "Javg", "desc": "[0/112]? Average confidence in 2 arcsec diam default aperture 3 J-band (JAVERAGECONF)"}, {"name": "JCl", "desc": "[/1] Discrete image classification flag in J (JCLASS) (1)"}, {"name": "JClst", "desc": "[-310/445]? N(0,1) stellarness-of-profile statistic in J (JCLASSSTAT)"}, {"name": "Jperrb", "desc": "[0/12587216] Additional WFAU post-processing error bits in J (<256: minor issues) (JPPERRBITS) (2)"}, {"name": "Jseq", "desc": "[/1661208] The running number of the J detection (JSEQNUM)"}, {"name": "Jxi", "desc": "? Offset of J detection from Y master position (+east/-west) (JXI)"}, {"name": "Jeta", "desc": "? Offset of J detection from Y master position (+north/-south) (JETA)"}, {"name": "Hpmag", "desc": "[-24/36]? Extended source VISTA H mag (Petrosian) (HPETROMAG)"}, {"name": "e_Hpmag", "desc": "[0/2056313]? Error in Hpmag (HPETROMAGERR) "}, {"name": "Hap3", "desc": "[-22/29]? Default point source H aperture corrected mag (2.0 arcsec diam) (HAPERMAG3)"}, {"name": "e_Hap3", "desc": "[0/2609]? Error in Hap3 (HAPERMAG3ERR) "}, {"name": "Hap4", "desc": "[-22/31]? Point source H aperture corrected mag (2.8 arcsec aperture diam) (HAPERMAG4)"}, {"name": "e_Hap4", "desc": "[0/15921]? Error in Hap4 (HAPERMAG4ERR) "}, {"name": "Hap6", "desc": "[-23/35]? Point source H aperture corrected mag (5.7 arcsec aperture diam) (HAPERMAG6)"}, {"name": "e_Hap6", "desc": "[0/737931]? Error in Hap6 (HAPERMAG6ERR) "}, {"name": "Hapc3", "desc": "[-21/30]? Default extended source H aperture mag (2.0 arcsec diam) (HAPERMAGNOAPERCORR3)"}, {"name": "Hapc4", "desc": "[-22/31]? Extended source H aperture mag (2.8\" aperture diameter) (HAPERMAGNOAPERCORR4)"}, {"name": "Hapc6", "desc": "[-23/35]? Extended source H aperture mag (5.7\" aperture diameter) (HAPERMAGNOAPERCORR6)"}, {"name": "Hamaj", "desc": "[0/19]? Seeing corrected half-light, semi-major axis in H band (HHLCORSMJRADAS)"}, {"name": "Hrms", "desc": "[0.7/584]? RMS of axes of ellipse fit in H (HGAUSIG)"}, {"name": "Hell", "desc": "? 1-b/a, where a/b=semi-major/minor axes in H (HELL)"}, {"name": "HPA", "desc": "? Ellipse fit celestial orientation in H (HPA) "}, {"name": "Herrb", "desc": "[/28] Processing warning/error bitwise flags in H (HERRBITS)"}, {"name": "Havg", "desc": "[0/112]? Average confidence in 2 arcsec diam default aperture 3 H (HAVERAGECONF)"}, {"name": "HCl", "desc": "[/1] Discrete image classification flag in H (HCLASS) (1)"}, {"name": "HClst", "desc": "[-96/383]? N(0,1) stellarness-of-profile statistic in H (HCLASSSTAT)"}, {"name": "Hperrb", "desc": "[0/12587216] Additional WFAU post-processing error bits in H (<256: minor issues) (HPPERRBITS) (2)"}, {"name": "Hseq", "desc": "[/125514] The running number of the H detection (HSEQNUM)"}, {"name": "Hxi", "desc": "? Offset of H detection from Y master position (+east/-west) (HXI)"}, {"name": "Heta", "desc": "? Offset of H detection from Y master position (+north/-south) (HETA)"}, {"name": "Kspmag", "desc": "[-20/]? Extended source VISTA Ks mag (Petrosian) (KSPETROMAG)"}, {"name": "e_Kspmag", "desc": "[0/]? Error in Kspmag (KSPETROMAGERR) "}, {"name": "Ksap3", "desc": "[-34/28]? Default point source Ks aperture corrected mag (2.0 arcsec diam) (KSAPERMAG3)"}, {"name": "e_Ksap3", "desc": "[0/2186]? Error Ksap3 (KSAPERMAG3ERR) "}, {"name": "Ksap4", "desc": "[-34/36]? Point source Ks aperture corrected mag (2.8 arcsec aperture diam) (KSAPERMAG4)"}, {"name": "e_Ksap4", "desc": "[0/3715233]? Error in Ksap4 (KSAPERMAG4ERR) "}, {"name": "Ksap6", "desc": "[-34/37]? Point source Ks aperture corrected mag (5.7 arcsec aperture diam) (KSAPERMAG6)"}, {"name": "e_Ksap6", "desc": "[0/]? Error in Ksap6 (KSAPERMAG6ERR) "}, {"name": "Ksapc3", "desc": "[-34/28]? Default extended source Ks aperture mag (2.0 arcsec diam) (KSAPERMAGNOAPERCORR3)"}, {"name": "Ksapc4", "desc": "[-34/36]? Extended source Ks aperture mag (2.8\" aperture diameter) (KSAPERMAGNOAPERCORR4)"}, {"name": "Ksapc6", "desc": "[-34/37]? Extended source Ks aperture mag (5.7\" aperture diameter) (KSAPERMAGNOAPERCORR6)"}, {"name": "Kamaj", "desc": "[0/19]? Seeing corrected half-light, semi-major axis in Ks band (KSHLCORSMJRADAS)"}, {"name": "Ksrms", "desc": "[0.7/549]? RMS of axes of ellipse fit in Ks (KSGAUSIG)"}, {"name": "Ksell", "desc": "? 1-b/a, where a/b=semi-major/minor axes in Ks (KSELL)"}, {"name": "KsPA", "desc": "? Ellipse fit celestial orientation in Ks (KSPA) "}, {"name": "Kserrb", "desc": "[/24] Processing warning/error bitwise flags in Ks (KSERRBITS)"}, {"name": "Ksavg", "desc": "[0/112]? Average confidence in 2 arcsec diam default aperture 3 Ks-band (KSAVERAGECONF)"}, {"name": "KsCl", "desc": "[/1] Discrete image classification flag in Ks (KSCLASS) (1)"}, {"name": "KsClst", "desc": "[-108/385]? N(0,1) stellarness-of-profile statistic in Ks (KSCLASSSTAT)"}, {"name": "Ksperrb", "desc": "[0/12587216] Additional WFAU post-processing error bits in Ks (<256: minor issues) (KSPPERRBITS) (2)"}, {"name": "Ksseq", "desc": "[/1455550] The running number of the Ks detection (KSSEQNUM)"}, {"name": "Ksxi", "desc": "? Offset of Ks detection from Y master position (+east/-west) (KSXI)"}, {"name": "Kseta", "desc": "? Offset of Ks detection from Y master position (+north/-south) (KSETA)"}, {"name": "Prim", "desc": "[0/1] Flag indicates primary sources (=1), otherwise (=0) (PRIMARY_SOURCE)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"II_71"}} {"id": "II/71", "title_cds": "Merged Infrared Catalog, first Edition", "title_create": "Schmitz+ 1978", "year": "1978", "author": "Schmitz M., Brown L.W., Mead J.M., Nagy T.A.", "title_pub": "Merged Infrared Catalog, First Edition", "first_author": "Schmitz M.", "ref_biblio": [""], "see_also": ["II/184 : Catalog of Infrared observations, 3rd Edition (Gezari+ 1993)"], "description": ["A compilation of equatorlal coordinates, spectral types, magnitudes,", "and fluxes from five catalogues of infrared [IR] observations is", "presented. This first edition of the Merged InFrared Catalogue [MIRC]", "contains 11,201 observations from a) the Two-Micron Sky Survey (TMSS)", "b) Observations of Infrared Radiation from Cool Stars (GMS), c) the", "Air Force Geophysics Laboratory Four Color Infrared Sky Survey (AFGL),", "and d) Supplemental Catalog (AFGL S), and e) A Catalog of 10um", "Celestial Objects (HALL). This compilation is a by-product of a", "computerized infrared data base under development at Goddard Space", "Flight Center; the objective is to maintain a complete and current", "record of all infrared observations from 1um to 10um of non-solar", "system objects. These observations are being placed into a", "standardized system. Periodically, updated editions of MIRC will be", "produced as additional catalogues are m erged into the IR data base."], "curator": "Francois Ochsenbein [CDS]", "records": ["11201 records"], "data": "", "date_update": "06-May-2004"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"II_76A"}} {"id": "II/76A", "title_cds": "O star catalogue, 4th Ed.", "title_create": "Goy 1980", "year": "1980", "author": "GOY G.", "title_pub": "Catalogue general d'etoiles de type O (O Star Catalogue, 4th Edition)", "first_author": "GOY G.", "ref_biblio": [""], "bibcode": ["1980A&AS...42...91G"], "curator": "Francois Ochsenbein [CDS]", "records": ["971 stars"], "data": "", "date_update": "04-Jul-1995"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_220"}} {"id": "III/220", "title_cds": "30 Dor spectral types and UBV magnitudes", "title_create": "Schild+, 1998", "year": "1998", "author": "Schild H., Testor G.", "title_pub": "Spectral types and UBV magnitudes of stars in the 30 Doradus complex", "first_author": "Schild H.", "ref_biblio": ["< 92, 729 (1992); 130, 527 (1998) >"], "keyword_cds": "Magellanic Clouds ; MK spectral classification; Photometry, UBV", "keyword_pub": "", "abstract": ["Photometric and spectroscopic observations are described for stars in", "four selected areas in the periphery of the 30 Doradus region. The", "areas are located at distances ranging from 7 to 20 arcmin from the", "central cluster. UBV magnitudes and spectral types for more than 250", "stars are presented. A total of 70 new O stars is reported, most of", "which are located in the two inner regions. Photometric and", "spectroscopic data are given of the Wolf-Rayet stars in the surveyed", "fields. For WR stars in tight clusters, spatially resolved photometry", "is given. A carbon star is also identified."], "curator": "Francois Ochsenbein [CDS]", "alias": ["[ST92]"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "04-Jul-2017"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_241"}} {"id": "III/241", "title_cds": "Spectroscopy of SDSS Data Release 3 (SDSS-DR3)", "title_create": "ARC, 2005", "year": "2005", "author": "Astrophysical Research Consortium (ARC)", "title_pub": "The Sloan Digital Sky Survey Data Release 3 (SDSS-DR3): Spectroscopy", "first_author": "Astrophysical Research Consortium (ARC)", "ref_biblio": [""], "keyword_cds": "Spectroscopy ; Redshifts; Surveys ; Velocity dispersion", "keyword_pub": "", "description": ["The Sloan Digital Sky Survey", "The descrition of the Second Data Release has been published by Abazajian", "et al. (2004AJ....128..502A)", "The Data Release 3 (DR3) spectroscopic data result from 826 plates", "of 640 spectra each, and cover 4188 square degrees", "The technical aspects are described by York D.G., Adelman J.,", "Anderson J.E., et al. (2000AJ....120.1579Y)", "Details at http://www.astro.psu.edu/users/dps/sdsstechrefs.html"], "ack": ["Refer to the SDSS pages at", "http://www.sdss.org/collaboration/credits.html", "Data from the SDSS public archive may not be used for any commercial", "publication or other commercial purpose except with explicit approval", "by the Astrophysical Research Consortium (ARC).", "Non-commercial scientific and technical publications using SDSS data", "should include the acknowledgment detailed at", "http://www.sdss.org/collaboration/credits.html"], "curator": "Francois Ochsenbein [CDS]", "alias": ["SDSS-DR3", "SDSS"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "26-May-2005"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_234"}} {"id": "III/234", "title_cds": "Distribution of stars in Carrington zone", "title_create": "Petersson, 1927", "year": "1927", "author": "Petersson J.H.", "title_pub": "Coordinates and identifications for north polar stars observed spectrophotometrically by Petersson", "first_author": "Petersson J.H.", "ref_biblio": [""], "bibcode": ["1927MeUpp..29....1P"], "see_also": ["III/233 : Catalogue of Stellar Spectral Classifications (Skiff, 2005)"], "keyword_cds": "Spectral types", "keyword_pub": "", "records": ["2007 stars"], "data": "", "date_update": "16-Mar-2006", "tables": [{"name": "catalog.dat", "desc": "Spectral Types by Petersson ", "columns": [{"name": "n_Name", "desc": "[*] Individual notes (1) "}, {"name": "Name", "desc": "Star name (BD or AC) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "rPos", "desc": "[TM] Source of prosition "}, {"name": "Vmag", "desc": "Visual magnitude "}, {"name": "SpType", "desc": "MK spectral type "}, {"name": "Note", "desc": "Remark (by Brian Skiff) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_247"}} {"id": "III/247", "title_cds": "Proven and probable members in the SMC", "title_create": "Sanduleak, 1968-1975", "year": "1975", "author": "Sanduleak N.", "title_pub": "Proven and probable members in the Small Magellanic Cloud", "first_author": "Sanduleak N.", "ref_biblio": ["< Astron. J. 73, 246 (1968); 74, 877 (1969); Astron. Astrophys. 39, 461 (1975) >"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["Sk"], "records": ["records"], "data": "", "date_update": "12-Jan-2007"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_236"}} {"id": "III/236", "title_cds": "Faint stars in two regions of the Milky Way", "title_create": "Apriamashivili, 1964", "year": "1964", "author": "Apriamashivili S.P.", "title_pub": "The catalogue of photographic magnitudes, color-indices, spectra, and", "first_author": "Apriamashivili S.P.", "ref_biblio": [""], "bibcode": ["1964AbaOB..31...27A"], "keyword_cds": "Magnitudes, photographic ; Colors ; Spectral types ; Milky Way", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "type": ["OC"], "records": ["records"], "data": "", "date_update": "12-Aug-2003"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_11"}} {"id": "III/11A", "title_cds": "F2 and earlier stars in SA28, 54, 106, 107", "title_create": "Upgren, Staron 1969", "year": "1969", "author": "Upgren Jr. A.R., Staron R.T.", "title_pub": "F2 and Earlier Stars in S.A. 28, 54, 106, 107", "first_author": "Upgren Jr. A.R.", "ref_biblio": [""], "bibcode": ["1969ApJ...157..327U"], "keyword_cds": "Selected areas", "description": ["The catalog contains the results of an objective-prism survey for", "498 stars of spectral classes F2 and earlier, brighter than", "magnitude 11.5, in four regions of intermediate galactic latitude.", "This objective-prism survey is part of a study of stellar densities", "aiming at the determination of the inclination to the galactic plane", "of surfaces of equal stellar density. Each region is centered on one", "of the Selected Areas 28, 54, 106, and 107. The fields, 4 x 4", "degrees in size, were each photographed on two IIa-O emulsion", "plates, one with an exposure time of three minutes on which bright", "stars could be classified and one with an exposure time of 40", "minutes extending to faint stars. The plates were taken with the", "24-inch Baker-Schmidt telescope of the Dyer Observatory. The", "dispersion of the objective prism is about 330 A/mm at H-gamma. The", "stars were classified according to the criteria established by", "Nassau and Seyfert (1946) and Nassau and van Albada (1947).", "Photographic magnitudes were found from direct IIa-O plates taken", "with the eight-inch Ross camera of the Yale Observatory. The", "catalog includes BD numbers, magnitudes, and spectral classes for BD", "stars. For non BD stars, the BD number listed in column (1)", "indicates a nearby BD star from which the star listed is offset, as", "indicated by the data of columns (2) and (3)."], "date_update": "26-Feb-2016", "tables": [{"name": "bdstars.dat", "desc": "BD stars catalog data ", "columns": [{"name": "Sarea", "desc": "Selected Area number "}, {"name": "BD", "desc": "BD number "}, {"name": "Photomag", "desc": "Photographic magnitude "}, {"name": "Sp", "desc": "Spectral type "}, {"name": "u_Sp", "desc": "uncertainty in Sp "}]}, {"name": "nonbd.dat", "desc": "Non-BD stars ", "columns": [{"name": "Sarea", "desc": "Selected Area number "}, {"name": "BD", "desc": "BD number of nearby star "}, {"name": "RAoffset", "desc": "Right ascension offset from BD star given in bytes 5-12, minutes of arc"}, {"name": "DEoffset", "desc": "Declination offset from BD star given in bytes 5-12, minutes of arc"}, {"name": "Photomag", "desc": "Photographic magnitude "}, {"name": "Sp", "desc": "Spectral type "}, {"name": "u_Sp", "desc": "uncertainty in Sp "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_12"}} {"id": "III/12A", "title_cds": "F5 and Later Stars in SA28, 54, 106, 107", "title_create": "Upgren, Staron 1970", "year": "1970", "author": "Upgren Jr. A.R., Staron R.T.", "title_pub": "F5 and Later Stars in Selected Areas 28, 54, 106, 107", "first_author": "Upgren Jr. A.R.", "ref_biblio": [""], "bibcode": ["1970ApJS...19..367U"], "keyword_cds": "Selected areas", "description": ["The catalog is an objective-prism survey of 2181 stars later than", "spectral class F2; the earlier stars are in catalog ADC# 3011A. The", "limiting magnitude is about 11.5. Four regions of intermediate", "galactic latitude are included in this survey. Each region is", "centered on one of the Selected Areas 28, 54, 106, and 107 and", "consists of a square 7 degrees on a side or about 50 square degrees", "in area. The fields, 4 x 4 degrees in size, were each photographed", "on two IIa-O emulsion plates, one with an exposure time of three", "minutes on which bright stars could be classified and one with an", "exposure time of 40 minutes extending to faint stars. The plates", "were taken with the 24-inch Baker-Schmidt telescope of the Dyer", "Observatory. The dispersion of the objective prism is about 330", "A/mm at H-gamma. The stars were classified according to the", "criteria established by Nassau and Seyfert (1946) and Nassau and van", "Albada (1947). Photographic magnitudes were found from direct IIa-O", "plates taken with the 8-inch Ross camera of the Yale University", "Observatory. The catalog includes BD numbers, magnitudes, and", "spectral classes for BD stars. For non BD stars, the BD number", "listed in bytes 1-3 indicates a nearby BD star from which the star", "listed is offset by the values in bytes 5-12 and 15-17 given in", "minutes of arc."], "date_update": "15-Dec-2015", "tables": [{"name": "bdstars.dat", "desc": "catalog data for BD stars ", "columns": [{"name": "AreaNum", "desc": "Selected Area number "}, {"name": "BD", "desc": "BD number "}, {"name": "PhotoMag", "desc": "Photographic magnitude "}, {"name": "u_PhotoMag", "desc": "Colon for uncertainty in photographic magnitude"}, {"name": "SpTemp", "desc": "Spectral type, temperature class and subclass "}, {"name": "u_SpTemp", "desc": "Colon for uncertainty in temperature class/subclass"}, {"name": "LumCl", "desc": "luminosity class "}, {"name": "u_LumCl", "desc": "Colon for uncertainty in luminosity class "}]}, {"name": "nonbd.dat", "desc": "data for non-BD stars ", "columns": [{"name": "AreaNum", "desc": "Selected Area number "}, {"name": "BD", "desc": "BD number of nearby star "}, {"name": "RAoffset", "desc": "Right ascension offset from BD star given in bytes 5-12, minutes of arc"}, {"name": "DEoffset", "desc": "Declination offset from BD star given in bytes 5-12, minutes of arc"}, {"name": "PhotoMag", "desc": "Photographic magnitude "}, {"name": "u_PhotoMag", "desc": "Colon for uncertainty in photographic magnitude"}, {"name": "SpTemp", "desc": "Spectral type, temperature class and subclass "}, {"name": "u_SpTemp", "desc": "Colon for uncertainty in temperature class/subclass"}, {"name": "LumCl", "desc": "luminosity class "}, {"name": "u_LumCl", "desc": "Colon for uncertainty in luminosity class "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_160A"}} {"id": "III/160A", "title_cds": "Bibliographic Catalogue of Radial Velocities", "title_create": "Barbier+ 1990", "year": "1990", "author": "Barbier-Brossat M., Petit M.", "title_pub": "Catalogue Bibliographique de Vitesses Radiales Stellaires", "first_author": "Barbier-Brossat M.", "ref_biblio": [""], "bibcode": ["1990A&AS...85..885B"], "keyword_cds": "Radial velocities", "description": ["This compilation of stellar radial velocities is a continuation of Abt", "& Biggs (III/4), and supersedes the previous catalog (III/118). It", "includes about 24200 references for Galactic, Large and Small", "Magellanic stars published between 1970 and 1985."], "type": ["BCC"], "data": "", "status": "obsolete", "date_creation": "01-Dec-1994", "date_update": "22-Sep-2015", "tables": [{"name": "main.dat", "desc": "The Bibliography of Stellar Radial Velocities ", "columns": [{"name": "HD", "desc": "Identification in HD (III/135) "}, {"name": "RAh", "desc": "? Right Ascension 1950 (hours) "}, {"name": "RAm", "desc": "? Right Ascension 1950 (minutes) "}, {"name": "u_pos", "desc": "[*] '*' indicates an approximative position "}, {"name": "DE-", "desc": "Declination 1950 (sign) "}, {"name": "DEd", "desc": "[-90/90]? Declination 1950 (degrees) "}, {"name": "DEm", "desc": "[0/60[? Declination 1950 (minutes) "}, {"name": "n_mag", "desc": "[*V] '*' for Photographic magnitude, 'V' for variable"}, {"name": "mag", "desc": "? Visual magnitude, or photographic when byte 22 contains a * . Values as found in"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_187"}} {"id": "III/187", "title_cds": "Classification of stars in BCD", "title_create": "Barbier/Chalonge/Divan", "title_pub": "CLASSIFICATION OF STARS IN THE BCD SYSTEM", "first_author": "BARBIER D.", "author": "BARBIER D., CHALONGE D., DIVAN L.: 1941--1969", "ref_biblio": ["< >"], "bibcode": ["1941AnAp....4...30B", "1951CR....232.2079B", "1952CoIAB..83.....C", "1952CoIAP.124.....F", "1956AnAp....6..287D", "1956AZh....33.....C", "1955JO.....38..345D", "1955CoIAB.129.....B", "1955JO.....38...93D", "1965POHP....7..(39B", "1966CoIAB.286..311D", "1963AnAp....4..289V", "1957CoIAP.227.....D", "1958CoIAB.181.....B", "1958JO.....41...(6A", "1964CoIAP.308.....C", "1969CoIAP.383.....D", "1956AnAp....6..294B"], "curator": "Francois Ochsenbein [CDS]", "alias": ["BCD"], "data": "", "date_update": "12-Oct-2000"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_212"}} {"id": "III/212", "title_cds": "Spectra of V568 Cyg in Period 1982-1988", "title_create": "Coluzzi, 1990", "year": "1990", "author": "Coluzzi R.", "title_pub": "Digitized Photographic Prism Spectrogram Archive of the long-monitored peculiar star V568 Cyg", "first_author": "Coluzzi R.", "ref_biblio": [""], "bibcode": ["1990A&A...230..307B"], "keyword_cds": "Spectroscopy; Stars, variable", "object": [], "curator": "Francois Ochsenbein [CDS]", "records": ["74 spectra"], "data": "", "date_update": "05-Oct-2012"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_240"}} {"id": "III/240", "title_cds": "Near-infrared spectra of MK standards", "title_create": "Wallace+ 1997-2002", "year": "2002", "author": "Wallace L., Meyer M.R., Hinkle K., Edwards S., Strom S.E.", "title_pub": "Near-infrared classification spectroscopy", "first_author": "Wallace L.", "ref_biblio": [""], "keyword_cds": "Spectroscopy ; Redshifts; Surveys ; Velocity dispersion", "keyword_pub": "", "object": [], "ack": ["Refer to the SDSS pages at", "http://www.sdss.org/collaboration/credits.html", "Data from the SDSS public archive may not be used for any commercial", "publication or other commercial purpose except with explicit approval", "by the Astrophysical Research Consortium (ARC).", "Non-commercial scientific and technical publications using SDSS data", "should include the acknowledgment detailed at", "http://www.sdss.org/collaboration/credits.html"], "curator": "Francois Ochsenbein [CDS]", "alias": ["SDSS-DR6", "SDSS"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "30-May-2009"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_259"}} {"id": "III/259", "title_cds": "Stephenson's dwarf K and M stars (StKM)", "title_create": "Stephenson, 1986", "year": "1986", "author": "Stephenson C.B.", "title_pub": "Dwarf K And M stars of small proper motion found in a Large Spectroscopic Survey", "first_author": "Stephenson C.B.", "ref_biblio": ["", ""], "bibcode": ["1986AJ.....91..144S", "1986AJ.....92..139S"], "keyword_cds": "Stars, dwarfs ; Stars, late-type ; Spectral types", "abstract": ["More than 2000 candidates for K and M dwarf status, generally having", "proper motions that are either unknown or less than 0.2\" per annum,", "have been identified in an objective-prism survey covering the entire", "sky north of declination -25deg and more than 10deg from the galactic", "plane. More than 95% have no previous indication that they are dwarfs.", "Several dozen appear to be visual double stars."], "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["StKM"], "type": ["OC"], "records": ["4102 stars"], "doi_pub": ["10.1086/113994"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_269"}} {"id": "III/269", "title_cds": "VIMOS VLT Deep Survey (VVDS)", "title_create": "Le Fevre+, 2013", "year": "2013", "author": "Le Fevre O., Cassata P., O. Cucciati O., Garilli B., Ilbert O., Le Brun V., Maccagni D., Moreau C., Scodeggio M., Tresse L., Zamorani G., Adami C., Arnouts S., Bardelli S., Bolzonella M., Bondi M., Bongiorno A., Bottini D., Cappi A., Charlot S., Ciliegi P., Contini T., de la Torre S., Foucaud S., Franzetti P., Gavignaud I., Guzzo L., Iovino A., Lemaux B., McCracken H.J., Marano B., Marinoni C., Mazure A., Mellier Y., Merighi R., Merluzzi P., Paltani S., Pello R., Pollo A., Pozzetti L., Scaramella R., Vergani D., Vettolani G., Zanichelli A., Zucca} E.", "title_pub": "The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z~6.7 selected with 17.5<=i_AB_<=24.75", "first_author": "Le Fevre O.", "ref_biblio": [""], "bibcode": ["2013A&A...559A..14L"], "keyword_cds": "Photometry, UBVRI ; Photometry, infrared; Galaxies, spectra ; Atlases", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: high redshift - cosmology: observations - cosmology: large-scale structure of Universe - astronomical databases: surveys", "abstract": ["Context. Deep representative surveys of galaxies at different epochs", "are needed to make progress in understanding galaxy evolution.", "Aims. We describe the completed VIMOS VLT Deep Survey, and the final", "data release of 35016 galaxies and type-I AGN with measured", "spectroscopic redshifts covering all epochs up to redshift z~6.7, in", "areas from 0.142 to 8.7 square degrees, and volumes from 0.5x10^6^ to", "2x10^7^h^-3^Mpc^3^.", "Methods. We have selected samples of galaxies based solely on their", "i-band magnitude reaching i_AB_=24.75. Spectra have been obtained with", "VIMOS on the ESO-VLT integrating 0.75h, 4.5h and 18h for the Wide,", "Deep, and Ultra-Deep nested surveys, respectively. We demonstrate that", "any 'redshift desert' can be crossed successfully using spectra", "covering 3650<={lambda}<=9350{AA}. A total of 1263 galaxies have been", "re-observed independently within the VVDS, and from the VIPERS and", "MASSIV surveys. They are used to establish the redshift measurements", "reliability, to assess completeness in the VVDS samples, and to", "provide a weighting scheme taking into account the survey selection", "function"], "curator": "Francois Ochsenbein [CDS]", "alias": ["VVDS"], "type": ["OC"], "records": ["records"], "doi_pub": ["10.1051/0004-6361/201322179"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_o26"}} {"id": "III/26", "title_cds": "Abundances of Na, Mg, and Ca in K giants, Table II", "title_create": "Peat+ 1968", "year": "1968", "author": "Peat D.W., Pemberton A.C.", "title_pub": "Abundances of Sodium, Magnesium and Calcium in K-Type Giant Stars. Table II", "first_author": "Peat D.W.", "ref_biblio": [""], "bibcode": ["1968MNRAS.140...21P"], "keyword_cds": "Abundances; Stars, K-type; Stars, giant", "abstract": ["Narrow band photometric measures of the strengths of the Mg b, Ca triplet,", "and Na D lines in 312 G and K type giant stars have been analyzed with a", "model atmosphere technique to determine abundances of magnesium, calcium", "and sodium."], "date_update": "06-May-2020", "tables": [{"name": "table2.dat", "desc": "Abundance ratios, surface gravity = 500 and 200 ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"III_285"}} {"id": "III/285", "title_cds": "Spectroscopic study of WDs in Southern hemisphere", "title_create": "Subasavage+, 2022", "year": "2022", "author": "Subasavage J., Bergeron P., Lepine S., Blouin S.", "title_pub": "Spectroscopic study of white dwarfs in the Southern hemisphere.", "first_author": "Subasavage J.", "ref_biblio": [""], "bibcode": ["2022yCat.3285....0S"], "see_also": ["B/wd : Spectroscopically identified white dwarfs (McCook+, 2014)", "J/A+A/505/441 : UVES/VLT spectra of white dwarfs (Koester+, 2009)", "J/AJ/145/136 : Astrometry & photometry of nearby white dwarfs (Limoges+, 2013)", "J/ApJS/219/19 : Census of nearby white dwarfs from SUPERBLINK (Limoges+, 2015)", "J/AJ/154/32 : Solar neighborhood. XXXIX. Nearby WDs (Subasavage+, 2017)", "J/AJ/154/118 : WD+dMs from the SUPERBLINK PM survey (Skinner+, 2017)", "J/ApJ/898/84 : Sp. follow-up of 100pc WDs in SDSS & Gaia (Kilic+, 2020)", "J/ApJ/901/93 : Model atmosphere analysis of hot WDs from SDSS (Bedard+, 2020)", "http://www.montrealwhitedwarfdatabase.org/ : The MWDD home page"], "keyword_cds": "Stars, white dwarf; Spectra, optical; Spectral types; Photometry, UBVRI; Parallaxes, trigonometric; Effective temperatures", "abstract": ["We present a brief report on a spectroscopic survey aimed at", "identifying white dwarfs in the Southern hemisphere from the", "SUPERBLINK proper motion database, similar to the survey in the", "Northern hemisphere discussed in Limoges+ (2013, J/AJ/145/136 and", "2015, J/ApJS/219/19). Our main goal here is simply to provide", "spectroscopic classification and data for the Montreal White Dwarf", "Database (MWDD), and to contribute to the ongoing effort of confirming", "spectroscopically all white dwarf candidates in the Gaia survey."], "description": ["The observational data are presented in Table 1 where we provide for", "each object the name, Gaia source ID, trigonometric parallax (and", "uncertainty), optical BVRI and near-infrared JHKs photometry. Each", "white dwarf in this table has been confirmed spectroscopically using", "the Southern Astrophysical Research Telescope (SOAR) 4m telescope with", "the Goodman spectrograph.", "We measured the physical parameters for each white dwarf in our sample", "using the photometric technique and model atmospheres decribed at", "length in Kilic+ (2020, J/ApJ/898/84). The physical parameters are", "reported in Table 2."], "alias": ["MWDD"], "type": ["OC"], "records": ["101 records"], "data": "", "date_update": "16-Aug-2022", "tables": [{"name": "table1.dat", "desc": "Observational results ", "columns": [{"name": "Name", "desc": "Main name of the source "}, {"name": "Gaia", "desc": "Gaia DR2 identifier "}, {"name": "plx", "desc": "[8.3/75] Gaia DR2 parallax "}, {"name": "e_plx", "desc": "[0.02/0.3] plx uncertainty "}, {"name": "Bmag", "desc": "[13.47/20.3]? B magnitude "}, {"name": "Vmag", "desc": "[13.52/19.16] V magnitude "}, {"name": "Rmag", "desc": "[13.54/18.7] R magnitude "}, {"name": "Imag", "desc": "[13.49/18.16] I band magnitude "}, {"name": "Jmag", "desc": "[13.59/16.6]? 2MASS J band magnitude "}, {"name": "Hmag", "desc": "[13.63/16.37]? 2MASS H band magnitude "}, {"name": "Ksmag", "desc": "[13.66/17.12]? 2MASS Ks band magnitude "}]}, {"name": "table2.dat", "desc": "Physical parameters ", "columns": [{"name": "Name", "desc": "Main name of the source "}, {"name": "SpT", "desc": "Spectral type "}, {"name": "Comp", "desc": "Composition "}, {"name": "Teff", "desc": "[4087/26405] Effective temperature "}, {"name": "e_Teff", "desc": "[60/2916] Teff uncertainty "}, {"name": "logg", "desc": "[6.9/8.7] Log of surface gravity "}, {"name": "e_logg", "desc": "[0.026/0.2] logg uncertainty "}, {"name": "Mass", "desc": "[0.2/1.1] Mass "}, {"name": "e_Mass", "desc": "[0.01/0.1] Mass uncertainty "}, {"name": "Dist", "desc": "[13/121] Distance "}, {"name": "e_Dist", "desc": "[0/1.1] Dist uncertainty "}, {"name": "n_SpT", "desc": "[1]? 1=new spectral classification "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"IV_31"}} {"id": "IV/31", "title_cds": "Stars in the open cluster NGC 2567", "title_create": "Lindoff+ 1968", "year": "1968", "author": "Lindoff U.", "title_pub": "The open clusters NGC 2533, NGC 2567, NGC 2571, and Ru 58.", "first_author": "Lindoff U.", "ref_biblio": ["", "", ""], "bibcode": ["1968ArA.....4..587L", "1986AJ.....91..326C"], "keyword_cds": "Clusters, open ; Photometry, UBV ; Cross identifications", "keyword_pub": "", "curator": "Francois Ochsenbein [CDS]", "alias": ["NGC2567"], "type": ["OC"], "records": ["181 stars"], "data": "", "date_update": "15-Aug-2008"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"IV_37"}} {"id": "IV/37", "title_cds": "The ATLAS all-sky stellar reference catalog", "title_create": "Tonry+, 2018", "year": "2018", "author": "Tonry J.L., Denneau L., Flewelling H., Heinze A.N., Onken C.A., Smartt S.J., Stalder B., Weiland H.J., Wolf C.", "title_pub": "The ATLAS all-sky stellar reference catalog.", "first_author": "Tonry J.L.", "ref_biblio": [""], "bibcode": ["2018ApJ...867..105T", "2019yCat.4037....0"], "keyword_cds": "; Parallaxes, trigonometric ; Proper motions ; Effective temperatures ; Extinction ; Photometry, ugriz ; Photometry, infrared", "keyword_pub": "atmospheric effects - instrumentation: photometers - surveys - techniques: photometric", "abstract": ["The Asteroid Terrestrial-impact Last Alert System (ATLAS) observes", "most of the sky every night in search of dangerous asteroids. Its data", "are also used to search for photometric variability, where sensitivity", "to variability is limited by photometric accuracy. Since each exposure", "spans 7.6{deg} corner to corner, variations in atmospheric transparency", "in excess of 0.01 mag are common, and 0.01 mag photometry cannot be", "achieved by using a constant flat-field calibration image. We therefore", "have assembled an all-sky reference catalog of approximately one billion", "stars to m~19 from a variety of sources to calibrate each exposure's", "astrometry and photometry. Gaia DR2 (Cat. I/345) is the source of", "astrometry for this ATLAS Refcat2. The sources of g, r, i, and z photometry", "include Pan-STARRS DR1 (Cat. II/349), the ATLAS Pathfinder photometry", "project, ATLAS reflattened APASS data, SkyMapper DR1 (Cat. II/358),", "APASS DR9 (Cat. II/336), the Tycho-2 catalog (Cat. I/259), and the Yale", "Bright Star Catalog (BSC; Hoffleit 1964cbs..book.....H). We have attempted", "to make this catalog at least 99% complete to m<19, including the brightest", "stars in the sky. We believe that the systematic errors are no larger", "than 5 mmag rms, although errors are as large as 20 mmag in small patches", "near the Galactic plane."], "curator": "Thomas Boch, Tiphaine Pouvreau [CDS]", "alias": [""], "records": ["records"], "doi_pub": ["10.3847/1538-4357/aae386"], "orcid_pub": ["0000-0003-2858-9657"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"IX_26"}} {"id": "IX/26", "title_cds": "Einstein Observatory, Revision 1B. Processings", "title_create": "Giacconi+, 1979", "year": "1979", "author": "Giacconi et al.", "title_pub": "Einstein Observatory, the 1B data revision tables and results.", "first_author": "Giacconi et al.", "ref_biblio": ["< >"], "bibcode": [""], "keyword_cds": "X-ray sources ; Surveys", "mission": "Einstein", "description": ["Various parameters for the IPC observations of the Einstein Observatory", "in the Rev1B Processing."], "records": ["18780 sources"], "data": "", "date_update": "29-Apr-1999", "tables": [{"name": "r1b_det.dat", "desc": "Source Detection Parameters for Rev1B Processing ", "columns": [{"name": "Seqno", "desc": "IPC Sequence Number (G1) "}, {"name": "rev1b", "desc": "IPC Rev1b source number (G2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "LHypos", "desc": "Y position: Ldetect in hard band (1) "}, {"name": "LHzpos", "desc": "Z position: Ldetect in hard band (1) "}, {"name": "e_LHypos", "desc": "Radius of error circle (1) "}, {"name": "LHccnts", "desc": "Cell counts: Ldetect in hard band (2) "}, {"name": "e_LHccnts", "desc": "Error on LH cell counts (2) "}, {"name": "LHbcnts", "desc": "Background cell counts: Ldetect hard band (3) "}, {"name": "e_LHbcnts", "desc": "Error on LH background cell counts (3) "}, {"name": "LHncnts", "desc": "Net cell counts: Ldetect in hard band (4) "}, {"name": "e_LHncnts", "desc": "Error on LH net cell counts (4) "}, {"name": "LHthrc", "desc": "Threshold cell counts: Ldetect hard band (5) "}, {"name": "LH_SNR", "desc": "Signal-to-noise ratio: Ldetect hard band (5) "}, {"name": "LBypos", "desc": "Y position: Ldetect in broad band (1) "}, {"name": "LBzpos", "desc": "Z position: Ldetect in broad band (1) "}, {"name": "e_LBypos", "desc": "Radius of error circle (1) "}, {"name": "LBccnts", "desc": "Cell counts: Ldetect in broad band (2) "}, {"name": "e_LBccnts", "desc": "Error on LB cell counts (2) "}, {"name": "LBbcnts", "desc": "Backgrnd cell counts: Ldetect broad band (3) "}, {"name": "e_LBbcnts", "desc": "Error on LB background cell counts (3) "}, {"name": "LBncnts", "desc": "Net cell counts: Ldetect in broad band (4) "}, {"name": "e_LBncnts", "desc": "Error on LB net cell counts (4) "}, {"name": "LBthrc", "desc": "Threshold cell counts: Ldetect broad band (5) "}, {"name": "LB_SNR", "desc": "Signal-to-noise ratio: Ldetect broad band (5) "}, {"name": "LSypos", "desc": "Y position: Ldetect in soft band (1) "}, {"name": "LSzpos", "desc": "Z position: Ldetect in soft band (1) "}, {"name": "e_LSypos", "desc": "Radius of error circle (1) "}, {"name": "LSccnts", "desc": "Cell counts: Ldetect in soft band (2) "}, {"name": "e_LSccnts", "desc": "Error on LS cell counts (2) "}, {"name": "LSbcnts", "desc": "Background cell counts: Ldetect soft band (3) "}, {"name": "e_LSbcnts", "desc": "Error on LS background cell counts (3) "}, {"name": "LSncnts", "desc": "Net cell counts: Ldetect in soft band (4) "}, {"name": "e_LSncnts", "desc": "Error on LS net cell counts (4) "}, {"name": "LSthrc", "desc": "Threshold cell counts: Ldetect soft band (5) "}, {"name": "LS_SNR", "desc": "Signal-to-noise ratio: Ldetect soft band (5) "}, {"name": "MHypos", "desc": "Y position: Mdetect in hard band (1) "}, {"name": "MHzpos", "desc": "Z position: Mdetect in hard band (1) "}, {"name": "e_MHypos", "desc": "Radius of error circle (1) "}, {"name": "MHccnts", "desc": "Cell counts: Mdetect in hard band (2) "}, {"name": "e_MHccnts", "desc": "Error on MH cell counts (2) "}, {"name": "MHbcnts", "desc": "Background cell counts: Mdetect hard band (3) "}, {"name": "e_MHbcnts", "desc": "Error on MH background cell counts (3) "}, {"name": "MHncnts", "desc": "Net cell counts: Mdetect in hard band (4) "}, {"name": "e_MHncnts", "desc": "Error on MH net cell counts (4) "}, {"name": "MHthrc", "desc": "Threshold cell counts: Mdetect hard band (5) "}, {"name": "MH_SNR", "desc": "Signal-to-noise ratio: Mdetect hard band (5) "}, {"name": "MBypos", "desc": "Y position: Mdetect in broad band (1) "}, {"name": "MBzpos", "desc": "Z position: Mdetect in broad band (1) "}, {"name": "e_MBypos", "desc": "Radius of error circle (1) "}, {"name": "MBccnts", "desc": "Cell counts: Mdetect in broad band (2) "}, {"name": "e_MBccnts", "desc": "Error on MB cell counts (2) "}, {"name": "MBbcnts", "desc": "Backgrnd cell counts: Mdetect broad band (3) "}, {"name": "e_MBbcnts", "desc": "Error on MB background cell counts (3) "}, {"name": "MBncnts", "desc": "Net cell counts: Mdetect in broad band (4) "}, {"name": "e_MBncnts", "desc": "Error on MB net cell counts (4) "}, {"name": "MBthrc", "desc": "Threshold cell counts: Mdetect broad band (5) "}, {"name": "MB_SNR", "desc": "Signal-to-noise ratio: Mdetect broad band (5) "}, {"name": "MSypos", "desc": "Y position: Mdetect in soft band (1) "}, {"name": "MSzpos", "desc": "Z position: Mdetect in soft band (1) "}, {"name": "e_MSypos", "desc": "Radius of error circle (1) "}, {"name": "MSccnts", "desc": "Cell counts: Mdetect in soft band (2) "}, {"name": "e_MSccnts", "desc": "Error on MS cell counts (2) "}, {"name": "MSbcnts", "desc": "Background cell counts: Mdetect soft band (3) "}, {"name": "e_MSbcnts", "desc": "Error on MS background cell counts (3) "}, {"name": "MSncnts", "desc": "Net cell counts: Mdetect in soft band (4) "}, {"name": "e_MSncnts", "desc": "Error on MS net cell counts (4) "}, {"name": "MSthrc", "desc": "Threshold cell counts: Mdetect soft band (5) "}, {"name": "MS_SNR", "desc": "Signal-to-noise ratio: Mdetect soft band (5) "}, {"name": "MS_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "MH_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "MB_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "LS_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "LH_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "LB_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}]}, {"name": "r1b_rad.dat", "desc": "Count distributions for Rev 1B IPC sources ", "columns": [{"name": "Seqno", "desc": "Sequence Number (G1) "}, {"name": "rev1b", "desc": "Rev1b Source Number (G2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "hpe", "desc": "High ph band extent (2) "}, {"name": "e_hpe", "desc": "High ph band extent error (2) "}, {"name": "sabkg", "desc": "Source annulus area background (3) "}, {"name": "sarea", "desc": "Source circle area (3) "}]}, {"name": "r1b_spc.dat", "desc": "IPC Spectral Information from Rev1B Processing ", "columns": [{"name": "Seqno", "desc": "IPC Sequence Number (G1) "}, {"name": "rev1b", "desc": "IPC Rev1b source number (G2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}]}, {"name": "r1b_sum.dat", "desc": "Summary of Observation Parameters for Rev1B Sources ", "columns": [{"name": "Seqno", "desc": "IPC Sequence Number (G1) "}, {"name": "rev1b", "desc": "IPC Rev1b source number (G2) "}, {"name": "pcod", "desc": "[LMSHB] Pcod flag - origin of position (1) "}, {"name": "ypos", "desc": "Pcod Y pixel position (2) "}, {"name": "zpos", "desc": "Pcod Z pixel position (2) "}, {"name": "yzp_err", "desc": "Pixel radius of error circle (2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "ra_err", "desc": "Right ascension error (3) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "dec_err", "desc": "Declination error (3) "}, {"name": "GLONr", "desc": "Pcod galactic longitude (4) "}, {"name": "e_GLONr", "desc": "Galactic longitude error (4) "}, {"name": "GLATr", "desc": "Pcod galactic latitude (4) "}, {"name": "e_GLATr", "desc": "Galactic latitude error (4) "}, {"name": "vigncorr", "desc": "Vignetting correction (5) "}, {"name": "SBcts", "desc": "Pcod position cell counts in soft band (6) "}, {"name": "e_SBcts", "desc": "Error on cell counts in soft band (6) "}, {"name": "HBcts", "desc": "Pcod position cell counts in hard band (6) "}, {"name": "e_HBcts", "desc": "Error on cell counts in hard band (6) "}, {"name": "BBcts", "desc": "Pcod position cell counts in broad band (6) "}, {"name": "e_BBcts", "desc": "Error on cell counts in broad band (6) "}, {"name": "SBbgcts", "desc": "Pcod cell background counts in soft band (7) "}, {"name": "e_SBbgcts", "desc": "Error on cell background counts in soft band (7) "}, {"name": "HBbgcts", "desc": "Pcod cell background counts in hard band (7) "}, {"name": "e_HBbgcts", "desc": "Error on cell background counts in hard band (7) "}, {"name": "BBbgcts", "desc": "Pcod cell background counts in broad band (7) "}, {"name": "e_BBbgcts", "desc": "Error on cell background counts, broad band (7) "}, {"name": "SBccrate", "desc": "Pcod corrected count rate in soft band (8) "}, {"name": "e_SBccrate", "desc": "Error on corrected count rate in soft band (8) "}, {"name": "HBccrate", "desc": "Pcod corrected count rate in hard band (8) "}, {"name": "e_HBccrate", "desc": "Error on corrected count rate in hard band (8) "}, {"name": "BBccrate", "desc": "Pcod corrected count rate in broad band (8) "}, {"name": "e_BBccrate", "desc": "Error on corrected count rate in broad band (8) "}, {"name": "SBflux", "desc": "Pcod source flux in soft band (9) "}, {"name": "e_SBflux", "desc": "Error on source flux in soft band (9) "}, {"name": "HBflux", "desc": "Pcod source flux in hard band (9) "}, {"name": "e_HBflux", "desc": "Error on source flux in hard band (9) "}, {"name": "BBflux", "desc": "Pcod source flux in broad band (9) "}, {"name": "e_BBflux", "desc": "Error on source flux in broad band (9) "}, {"name": "EBflux", "desc": "Pcod source flux in Einstein band (9) "}, {"name": "e_EBflux", "desc": "Error on source flux in Einstein band (9) "}, {"name": "prffit", "desc": "PRF fit\t(10) "}, {"name": "reco", "desc": "Combined ribs and edges code (11) "}, {"name": "sel_flag", "desc": "Flagged 0.0 if source included in EOSCAT (12) "}]}, {"name": "r1b_var.dat", "desc": "Variability Parameters for Rev1B Processing ", "columns": [{"name": "Seqno", "desc": "IPC Sequence Number (G1) "}, {"name": "rev1b", "desc": "IPC Rev1b source number (G2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) (1) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) (1) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "chicode", "desc": "Variability code chisq analysis (2) "}, {"name": "Chi2", "desc": "Reduced chisq (2) "}, {"name": "nChi2", "desc": "Degrees of freedom (2) "}, {"name": "Cprob", "desc": "Probability that source is constant (3) "}, {"name": "eqsigma", "desc": "Equivalent number of sigma (3) "}, {"name": "nbins", "desc": "Number of bins (4) "}, {"name": "bintime", "desc": "Bintime (4) "}, {"name": "counts", "desc": "Source circle counts (5) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"IX_27"}} {"id": "IX/27", "title_cds": "Einstein Observatory Catalog (OCAT) (Yellow Book)", "title_create": "Seward+, 1986", "year": "1986", "author": "Seward F.D., Martenis P.", "title_pub": "Einstein Observations: OCAT alias ``Yellow Book\"", "first_author": "Seward F.D.", "ref_biblio": ["< Einstein Observatory Catalog of Observations (5th ed.; Cambridge: Harvard-Smithsonian Center for Astrophysics). >"], "see_also": ["IX/22 : The CfA Einstein observatory extended deep X-ray survey", "IX/23 : Einstein Observatory Source Catalog", "IX/24 : The Einstein Observatory High Resolution Imager Source List", "IX/25 : Einstein Observatory Imaging Proportional Counter (IPC) Parameters", "IX/26 : Einstein Observatory, Revision 1B. Processings"], "keyword_cds": "X-ray sources ; Surveys", "mission": "Einstein", "description": ["This catalog contains details on the Einstein Observatory Catalog of", "Observations (OCA), observations, databank requests, observers and the", "observations themselves are provided. This is also known as the", "Einstein Observatory's \"Yellow Book\"."], "alias": ["OCAT"], "records": ["5656 sources"], "data": "", "date_update": "29-Apr-1999", "tables": [{"name": "categs.dat", "desc": "Categories of Einstein Observations ", "columns": [{"name": "categ", "desc": "Eight letter category code (1) "}, {"name": "descr", "desc": "Category title as used in the original Yellow Book "}]}, {"name": "db_reqs.dat", "desc": "Einstein Observatory Databank Requests ", "columns": [{"name": "req_num", "desc": "Request's identifying number (1) "}, {"name": "req_date", "desc": "Date of the request (1) "}, {"name": "name", "desc": "Name and institution of the person requesting the data"}, {"name": "title", "desc": "Title describing the topic of the request "}]}, {"name": "obsnames.dat", "desc": "Einstein Observers ", "columns": [{"name": "obs_num", "desc": "The observer's identifying number (1) "}, {"name": "obs_name", "desc": "The observer's name and institution "}]}, {"name": "pointing.dat", "desc": "Einstein Observations (OCAT alias \"Yellow Book\") ", "columns": [{"name": "Seqno", "desc": "The sequence number of the observation (1) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "instr", "desc": "The instrument at the focus (2) "}, {"name": "obs_num", "desc": "The observer identification number (3) "}, {"name": "TIPI", "desc": "Time In Processed Image (3) "}, {"name": "obs_date", "desc": "The date the observation was started (3) "}, {"name": "categ", "desc": "Category code based upon the observation's target (4)"}, {"name": "title", "desc": "The name of target and/or name of observing program (4)"}, {"name": "req_num", "desc": "Identifying numbers of databank requests (5) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"IX_38"}} {"id": "IX/38", "title_cds": "ROSAT Sources for the PSPC with filter (2RXF)", "title_create": "ROSAT Team, 2001", "year": "2001", "author": "ROSAT Scientific Team", "title_pub": "ROSAT Results Archive Sources for the PSPC with filter", "first_author": "ROSAT Scientific Team", "ref_biblio": [""], "keyword_cds": "X-ray sources ; Surveys", "mission": "ROSAT", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["2RXF"], "records": ["records"], "data": "", "date_update": "04-Mar-2004"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_17_326"}} {"id": "J/A+A/17/326", "title_cds": "Positions of GV stars", "title_create": "Sanduleak+, 1972", "year": "1972", "author": "Sanduleak N.", "title_pub": "Comparison of the Large Magellanic Cloud catalogue of Sanduleak and Fehrenbach-Duflot.", "first_author": "Sanduleak N.", "ref_biblio": [""], "bibcode": ["1972A&A....17..326S"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_177_217"}} {"id": "J/A+A/177/217", "title_cds": "Teff and Luminosity from MK spectral class", "title_create": "De Jager+ 1987", "year": "1987", "author": "De Jager C., Nieuwenhuijzen H.", "title_pub": "A new determination of the statistical relations between stellar spectral and luminosity classes and stellar effective temperature and lumonosity.", "first_author": "De Jager C.", "ref_biblio": [""], "bibcode": ["1987A&A...177..217D"], "keyword_cds": "", "keyword_pub": "stars: classificaition ; stars: Hertzsprung-Russel diagrapn ; stars: luminosity ; stars: temperatures", "abstract": ["From a set of 199 determinations of bolometric stellar luminosity L", "and 268 of stellar effective temperature T_eff_ we derived the", "statical dependences of log(T_eff_) and log(L/L{sun}) respectively on", "spectral type and luminosity class. For computer use we introduced", "continuous variables s (for spectral type) and b (for luminosity", "class). The relations T_eff_(s,b) and logL(s,b) are given in terms of", "Chebychev polynomials and their cross-products. A comparison is made", "with existing systems; there are small differences that we ascribe to", "the addition of new data to temperature and luminosity, not used in", "previous determinations. The 1-{sigma} values for determinations of", "unit weight of logT_eff_ and logL respectively appear to be 0.021 and", "0.164, which shows that there is a factor 8 in their relative", "accuracies."], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_18_271"}} {"id": "J/A+A/18/271", "title_cds": "Photometry of bright stars in LMC", "title_create": "Dachs+, 1972", "year": "1972", "author": "Dachs J.", "title_pub": "Photometry of bright stars in the Large Magellanic Cloud.", "first_author": "Dachs J.", "ref_biblio": [""], "bibcode": ["1972A&A....18..271D"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_379_436"}} {"id": "J/A+A/379/436", "title_cds": "EIS survey: selected stellar fields", "title_create": "Momany+, 2001", "year": "2001", "author": "Momany Y., Vandame B., Zaggia S., Mignani R.P., Da Costa L., Arnouts S., Groenewegen M.A.T., Hatziminaoglou E., Madejsky R., Rite C., Schirmer M., Slijkhuis R.", "title_pub": "ESO imaging survey. Pre-FLAMES survey: Observations of selected stellar fields.", "first_author": "Momany Y.", "ref_biblio": [""], "bibcode": ["2001A&A...379..436M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1051/0004-6361:20011325"], "orcid_pub": ["0000-0001-8946-8723"], "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_398_89"}} {"id": "J/A+A/398/89", "title_cds": "Evolutionary synthesis models. II.", "title_create": "Schulz+, 2003", "year": "2003", "author": "Schulz J., Fritze-v. Alvensleben U., Fricke K.J.", "title_pub": "Wavelength and redshift dependence of bulge/total light ratios in galaxies.", "first_author": "Schulz J.", "ref_biblio": [""], "bibcode": ["2003A&A...398...89S"], "see_also": ["http://www.uni-sw.gwdg.de/~galev : The Goettingen Galaxy Evolution Group", "J/A+A/392/1 : Spectrophotometry of simulated SSPs (Schulz+, 2002)", "J/A+A/401/1063 : Evolutionary synthesis models. III. (Anders+, 2003)"], "keyword_cds": "Models, evolutionary ; Galaxies, photometry", "keyword_pub": "galaxies: general - galaxies, evolution - galaxies, formation - galaxies: fundamental parameters - galaxies: stellar content", "abstract": ["HST has opened the possibility to decompose the surface brightness", "profiles of galaxies up to significant redshifts and look-back times", "into r^1/4^-bulge and exponential disk components. This should allow", "to study the redshift evolution of bulge and disk luminosity", "contributions and discriminate between the different formation", "scenarios for these galaxy components currently discussed, i.e. decide", "if star formation in bulges and disks started at the same time or was", "delayed in either of the two components. An indispensable prerequisite", "for the comparison of bulge-to-disk ratios of galaxies at different", "redshifts is to properly account for cosmological band shift and", "evolutionary effects.", "We present evolutionary synthesis models for both components and add", "their spectra in various proportions to obtain the full range of local", "galaxies' B-band bulge-to-total light ratios. Bulge star formation is", "assumed to occur on a short timescale of 10^9^yr, disk star", "formation proceeds at a constant rate. We study the evolution of the", "relative light contributions of both components backward in time and,", "for a given cosmological model, as a function of redshift. This allows", "us to see how far back into the past the locally well-established", "correlation between galaxy morphologies and spectral properties can", "hold. To cope with the present uncertainty about the formation epochs", "of bulge and disk components we present models for three scenarios:", "bulges and disks of equal age, old bulges and delayed disk star", "formation, and old disks with subsequent bulge star formation.", "We quantitatively show the wavelength dependence of bulge-to-total", "(=B/T) light ratios for local galaxies. The different star formation", "timescales for bulge and disk components lead to B/T ratios that", "significantly increase from U through I-bands (by factors 4-6 for", "weak bulge systems ~Sc) with the rate of increase slightly depending", "on the relative ages of the two components.", "The redshift evolution of B/T-ratios in various bands U,B,V,I,H is", "calculated accounting both for cosmological and evolutionary", "corrections assuming a standard cosmology (H_0_=65, Omega_0_)=0.1,", "Lambda_0_=0). In particular, for the two scenarios with old bulges and", "old or younger disks, the redshift evolution of B/T-ratios is dramatic", "in every band and both for galaxies ending up at z~0 with low and high", "B-band B/T light ratios. Our results clearly show that it does not", "make any sense to compare B/T ratios measured in one and the same band", "for galaxies at different redshifts without fully accounting for", "evolutionary and cosmological effects. These, unfortunately,", "significantly depend on the relative ages of the two components and,", "hence, on the galaxy formation scenario adopted.", "We also show that simultaneous decomposition of galaxy profiles in", "several bands can give direct information about these relative ages", "and constrain formation scenarios for the different galaxy components."], "description": ["Spectra, colors, luminosities and B/T ratios in various filter-systems", "as well as cosmological and evolutionary corrections in the cosmology", "(H_0_=65, Omega_0_=0.1, Lambda_0_=0.0) for the 4 components and their", "related B/T scenarios. The timestep is 4*10^6^years. the UBV filters", "are from Buser & Kurucz (1978A&A....70..555B), the RI filter from", "Bessell (1990PASP..102.1181B) and JHK from Bessel & Brett", "(1988PASP..100.1134B). Files are sorted in directorys with following", "naming-convention:", "84-84 = scenario with equally old bulge and disk", "84-50 = scenario with old bulge and young disk", "50-84 = scenario with old disk and young bulge", "the e- & k-corrections can be found in ec*.dat, kc*.dat and ka*.dat", "corresponding to the cosmology with H_0_=65 as seen above. Both", "k-corrections with and without attenuation are included."], "doi_pub": ["10.1051/0004-6361:20021631"], "data": "", "date_update": "10-Oct-2022", "tables": [{"name": "johesd.dat", "desc": "Luminosities and colors from the spectra in Johnson filter-system, Scalo IMF, Only Elliptical or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "Umag", "desc": "Johnson U magnitude "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "Rmag", "desc": "Johnson R magnitude "}, {"name": "Imag", "desc": "Johnson I magnitude "}, {"name": "Jmag", "desc": "Johnson J magnitude "}, {"name": "Hmag", "desc": "Johnson H magnitude "}, {"name": "Kmag", "desc": "Johnson K magnitude "}, {"name": "Lmag", "desc": "Johnson L magnitude "}, {"name": "U-B", "desc": "Johnson U-B colour index "}, {"name": "B-V", "desc": "Johnson B-V colour index "}, {"name": "U-V", "desc": "Johnson U-V colour index "}, {"name": "V-R", "desc": "Johnson V-R colour index "}, {"name": "R-I", "desc": "Johnson R-I colour index "}, {"name": "V-K", "desc": "Johnson V-K colour index "}, {"name": "I-K", "desc": "Johnson I-K colour index "}, {"name": "B-R", "desc": "Johnson B-R colour index "}, {"name": "B-H", "desc": "Johnson B-H colour index "}, {"name": "J-H", "desc": "Johnson J-H colour index "}, {"name": "H-K", "desc": "Johnson H-K colour index "}]}, {"name": "magesd.dat", "desc": "Luminosities from the spectra in Koo, Thuan & Gunn, Washinton and Stroemgren filter-systems, Scalo IMF, Only Elliptical or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "age", "desc": "Age of system "}, {"name": "kumag", "desc": "Koo u magnitude "}, {"name": "kjmag", "desc": "Koo j magnitude "}, {"name": "kfmag", "desc": "Koo f magnitude "}, {"name": "knmag", "desc": "Koo n magnitude "}, {"name": "gmag", "desc": "Thuan & Gunn g magnitude "}, {"name": "rmag", "desc": "Thuan & Gunn r magnitude "}, {"name": "Cmag", "desc": "Washington C magnitude "}, {"name": "Mmag", "desc": "Washington M magnitude "}, {"name": "T1mag", "desc": "Washington T1 magnitude "}, {"name": "T2mag", "desc": "Washington T2 magnitude "}, {"name": "sumag", "desc": "Stroemgren u magnitude "}, {"name": "svmag", "desc": "Stroemgren v magnitude "}, {"name": "sbmag", "desc": "Stroemgren b magnitude "}, {"name": "symag", "desc": "Stroemgren y magnitude "}]}, {"name": "hstesd.dat", "desc": "Luminosities from the spectra in HST filter-system, Scalo IMF, Only E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "F160BW", "desc": "HST F160BW magnitude "}, {"name": "F170W", "desc": "HST F170W magnitude "}, {"name": "F185W", "desc": "HST F185W magnitude "}, {"name": "F218W", "desc": "HST F218W magnitude "}, {"name": "F255W", "desc": "HST F255W magnitude "}, {"name": "F300W", "desc": "HST F300W = U(HDF) magnitude "}, {"name": "F336W", "desc": "HST F336W magnitude "}, {"name": "F380W", "desc": "HST F380W magnitude "}, {"name": "F439W", "desc": "HST F439W magnitude "}, {"name": "F450W", "desc": "HST F450W = B(HDF) magnitude "}, {"name": "F555W", "desc": "HST F555W = V(YSC) magnitude "}, {"name": "F569W", "desc": "HST F569W magnitude "}, {"name": "F606W", "desc": "HST F606W = V(HDF) magnitude "}, {"name": "F622W", "desc": "HST F622W magnitude "}, {"name": "F675W", "desc": "HST F675W magnitude "}, {"name": "F702W", "desc": "HST F702W magnitude "}, {"name": "F791W", "desc": "HST F791W magnitude "}, {"name": "F814W", "desc": "HST F814W = I(HDF) magnitude "}]}, {"name": "ecesd.dat", "desc": "Coefficients of e-correction in luminosity, H0=65 Scalo IMF, E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Model redshift "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies "}, {"name": "z", "desc": "? Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "kcesd.dat", "desc": "Coefficients of k-correction in luminosity, H0=65 Scalo IMF, E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Model redshift "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies "}, {"name": "z", "desc": "? Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "kaesd.dat", "desc": "Coefficients of k-correction with attenuation in Scalo IMF, E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Model redshift "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies "}, {"name": "z", "desc": "? Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "gspesd.dat", "desc": "Spectra, with Scalo IMF, E or SD galaxies ", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial metallicity (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "lambda", "desc": "Wavelength "}, {"name": "Flux1", "desc": "? Flux at a system age of 1.4000E+08yrs "}, {"name": "Flux2", "desc": "? Flux at a system age of 2.8000E+08yrs "}, {"name": "Flux3", "desc": "? Flux at a system age of 4.2000E+08yrs "}, {"name": "Flux4", "desc": "? Flux at a system age of 5.6000E+08yrs "}, {"name": "Flux5", "desc": "? Flux at a system age of 7.0000E+08yrs "}, {"name": "Flux6", "desc": "? Flux at a system age of 8.4000E+08yrs "}, {"name": "Flux7", "desc": "? Flux at a system age of 9.8000E+08yrs "}, {"name": "Flux8", "desc": "? Flux at a system age of 1.1200E+09yrs "}, {"name": "Flux9", "desc": "? Flux at a system age of 1.2600E+09yrs "}, {"name": "Flux10", "desc": "? Flux at a system age of 1.4000E+09yrs "}, {"name": "Flux11", "desc": "? Flux at a system age of 1.5400E+09yrs "}, {"name": "Flux12", "desc": "? Flux at a system age of 1.6800E+09yrs "}, {"name": "Flux13", "desc": "? Flux at a system age of 1.8200E+09yrs "}, {"name": "Flux14", "desc": "? Flux at a system age of 1.9600E+09yrs "}, {"name": "Flux15", "desc": "? Flux at a system age of 2.1000E+09yrs "}, {"name": "Flux16", "desc": "? Flux at a system age of 2.2400E+09yrs "}, {"name": "Flux17", "desc": "? Flux at a system age of 2.3800E+09yrs "}, {"name": "Flux18", "desc": "? Flux at a system age of 2.5200E+09yrs "}, {"name": "Flux19", "desc": "? Flux at a system age of 2.6600E+09yrs "}, {"name": "Flux20", "desc": "? Flux at a system age of 2.8000E+09yrs "}, {"name": "Flux21", "desc": "? Flux at a system age of 2.9400E+09yrs "}, {"name": "Flux22", "desc": "? Flux at a system age of 3.0800E+09yrs "}, {"name": "Flux23", "desc": "? Flux at a system age of 3.2200E+09yrs "}, {"name": "Flux24", "desc": "? Flux at a system age of 3.3600E+09yrs "}, {"name": "Flux25", "desc": "? Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? Flux at a system age of 4.7600E+09yrs "}, {"name": "Flux35", "desc": "Flux at a system age of 4.9000E+09yrs "}, {"name": "Flux36", "desc": "Flux at a system age of 5.0400E+09yrs "}, {"name": "Flux37", "desc": "Flux at a system age of 5.1800E+09yrs "}, {"name": "Flux38", "desc": "Flux at a system age of 5.3200E+09yrs "}, {"name": "Flux39", "desc": "Flux at a system age of 5.4600E+09yrs "}, {"name": "Flux40", "desc": "Flux at a system age of 5.6000E+09yrs "}, {"name": "Flux41", "desc": "Flux at a system age of 5.7400E+09yrs "}, {"name": "Flux42", "desc": "Flux at a system age of 5.8800E+09yrs "}, {"name": "Flux43", "desc": "Flux at a system age of 6.0200E+09yrs "}, {"name": "Flux44", "desc": "Flux at a system age of 6.1600E+09yrs "}, {"name": "Flux45", "desc": "Flux at a system age of 6.3000E+09yrs "}, {"name": "Flux46", "desc": "Flux at a system age of 6.4400E+09yrs "}, {"name": "Flux47", "desc": "Flux at a system age of 6.5800E+09yrs "}, {"name": "Flux48", "desc": "Flux at a system age of 6.7200E+09yrs "}, {"name": "Flux49", "desc": "Flux at a system age of 6.8600E+09yrs "}, {"name": "Flux51", "desc": "Flux at a system age of 7.0000E+09yrs "}, {"name": "Flux52", "desc": "Flux at a system age of 7.1400E+09yrs "}, {"name": "Flux53", "desc": "Flux at a system age of 7.2800E+09yrs "}, {"name": "Flux54", "desc": "Flux at a system age of 7.4200E+09yrs "}, {"name": "Flux55", "desc": "Flux at a system age of 7.5600E+09yrs "}, {"name": "Flux56", "desc": "Flux at a system age of 7.7000E+09yrs "}, {"name": "Flux57", "desc": "Flux at a system age of 7.8400E+09yrs "}, {"name": "Flux58", "desc": "Flux at a system age of 7.9800E+09yrs "}, {"name": "Flux59", "desc": "Flux at a system age of 8.1200E+09yrs "}, {"name": "Flux60", "desc": "Flux at a system age of 8.2600E+09yrs "}, {"name": "Flux61", "desc": "Flux at a system age of 8.4000E+09yrs "}, {"name": "Flux62", "desc": "Flux at a system age of 8.5400E+09yrs "}, {"name": "Flux63", "desc": "Flux at a system age of 8.6800E+09yrs "}, {"name": "Flux64", "desc": "Flux at a system age of 8.8200E+09yrs "}, {"name": "Flux65", "desc": "Flux at a system age of 8.9600E+09yrs "}, {"name": "Flux66", "desc": "Flux at a system age of 9.1000E+09yrs "}, {"name": "Flux67", "desc": "Flux at a system age of 9.2400E+09yrs "}, {"name": "Flux68", "desc": "Flux at a system age of 9.3800E+09yrs "}, {"name": "Flux69", "desc": "Flux at a system age of 9.5200E+09yrs "}, {"name": "Flux70", "desc": "Flux at a system age of 9.6600E+09yrs "}, {"name": "Flux71", "desc": "Flux at a system age of 9.8000E+09yrs "}, {"name": "Flux72", "desc": "Flux at a system age of 9.9400E+09yrs "}, {"name": "Flux73", "desc": "Flux at a system age of 1.0080E+10yrs "}, {"name": "Flux74", "desc": "Flux at a system age of 1.0220E+10yrs "}, {"name": "Flux75", "desc": "Flux at a system age of 1.0360E+10yrs "}, {"name": "Flux76", "desc": "Flux at a system age of 1.0500E+10yrs "}, {"name": "Flux77", "desc": "Flux at a system age of 1.0640E+10yrs "}, {"name": "Flux78", "desc": "Flux at a system age of 1.0780E+10yrs "}, {"name": "Flux79", "desc": "Flux at a system age of 1.0920E+10yrs "}, {"name": "Flux80", "desc": "Flux at a system age of 1.1060E+10yrs "}, {"name": "Flux81", "desc": "Flux at a system age of 1.1200E+10yrs "}, {"name": "Flux82", "desc": "Flux at a system age of 1.1340E+10yrs "}, {"name": "Flux83", "desc": "Flux at a system age of 1.1480E+10yrs "}, {"name": "Flux84", "desc": "Flux at a system age of 1.1620E+10yrs "}, {"name": "Flux85", "desc": "Flux at a system age of 1.1760E+10yrs "}, {"name": "Flux86", "desc": "Flux at a system age of 1.1900E+10yrs "}, {"name": "Flux87", "desc": "Flux at a system age of 1.2040E+10yrs "}, {"name": "Flux88", "desc": "Flux at a system age of 1.2180E+10yrs "}, {"name": "Flux89", "desc": "Flux at a system age of 1.2320E+10yrs "}, {"name": "Flux90", "desc": "Flux at a system age of 1.2460E+10yrs "}, {"name": "Flux91", "desc": "Flux at a system age of 1.2600E+10yrs "}, {"name": "Flux92", "desc": "Flux at a system age of 1.2740E+10yrs "}, {"name": "Flux93", "desc": "Flux at a system age of 1.2880E+10yrs "}, {"name": "Flux94", "desc": "Flux at a system age of 1.3020E+10yrs "}, {"name": "Flux95", "desc": "Flux at a system age of 1.3160E+10yrs "}, {"name": "Flux96", "desc": "Flux at a system age of 1.3300E+10yrs "}, {"name": "Flux97", "desc": "Flux at a system age of 1.3440E+10yrs "}, {"name": "Flux98", "desc": "Flux at a system age of 1.3580E+10yrs "}, {"name": "Flux99", "desc": "Flux at a system age of 1.3720E+10yrs "}, {"name": "Flux100", "desc": "Flux at a system age of 1.3860E+10yrs "}, {"name": "Flux101", "desc": "Flux at a system age of 1.4000E+10yrs "}]}, {"name": "pl1esd.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 1 E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) (1) "}, {"name": "z0", "desc": "? Initial redshift (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "Age", "desc": "Actual age "}, {"name": "MassSys", "desc": "Total mass of system "}, {"name": "MassStar", "desc": "Total mass of stars in system "}, {"name": "MassGas", "desc": "Total mass of gas in system "}, {"name": "Y", "desc": "Helium abundance, Y "}, {"name": "Z0", "desc": "[0.00000] Metallicity Z (0 for SSPs) "}, {"name": "SFR", "desc": "Star formation rate "}, {"name": "---", "desc": "[0.00000] ? "}, {"name": "ezj", "desc": "[0.00000] Ejection rate (0 for SSPs) "}]}, {"name": "pl2esd.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 2 E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "Age", "desc": "Actual age "}, {"name": "mbol", "desc": "Bolometric magnitude "}, {"name": "Umag", "desc": "Johnson U magnitude "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "Rmag", "desc": "Johnson R magnitude "}, {"name": "Imag", "desc": "Johnson I magnitude "}, {"name": "Jmag", "desc": "Johnson J magnitude "}, {"name": "Hmag", "desc": "Johnson H magnitude "}, {"name": "Kmag", "desc": "Johnson K magnitude "}, {"name": "Lmag", "desc": "[0.0000] Johnson L magnitude (not included in the isochrones)"}]}, {"name": "pl3esd.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 3 E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "Age", "desc": "Actual age "}, {"name": "U-B", "desc": "Color U-B "}, {"name": "B-V", "desc": "Color B-V "}, {"name": "V-R", "desc": "Color V-R "}, {"name": "R-I", "desc": "Color R-I "}, {"name": "I-J", "desc": "Color I-J "}, {"name": "J-H", "desc": "Color J-H "}, {"name": "H-K", "desc": "Color H-K "}, {"name": "L-J", "desc": "[0.0000] Color L-J (not included) "}, {"name": "U-V", "desc": "Color U-V "}, {"name": "V-K", "desc": "Color V-K "}]}, {"name": "pl4esd.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 4 E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "Age", "desc": "Actual age "}, {"name": "lbol", "desc": "Bolometric luminosity "}, {"name": "lUmag", "desc": "Luminosity in U band "}, {"name": "lBmag", "desc": "Luminosity in B band "}, {"name": "lVmag", "desc": "Luminosity in V band "}, {"name": "lRmag", "desc": "Luminosity in R band "}, {"name": "lImag", "desc": "Luminosity in I band "}, {"name": "lJmag", "desc": "Luminosity in J band "}, {"name": "lHmag", "desc": "Luminosity in H band "}, {"name": "lKmag", "desc": "Luminosity in k band "}, {"name": "lLmag", "desc": "[0.0000] Luminosity in L band (not included) "}, {"name": "lLya", "desc": "[0.0000] Lyman-continuum-photons (not calculated)"}]}, {"name": "johshift.dat", "desc": "Luminosities and colors from the spectra in Johnson filter-system, Scalo IMF, Shift Only Elliptical or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "Umag", "desc": "Johnson U magnitude "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "Rmag", "desc": "Johnson R magnitude "}, {"name": "Imag", "desc": "Johnson I magnitude "}, {"name": "Jmag", "desc": "Johnson J magnitude "}, {"name": "Hmag", "desc": "Johnson H magnitude "}, {"name": "Kmag", "desc": "Johnson K magnitude "}, {"name": "Lmag", "desc": "Johnson L magnitude "}, {"name": "U-B", "desc": "Johnson U-B colour index "}, {"name": "B-V", "desc": "Johnson B-V colour index "}, {"name": "U-V", "desc": "Johnson U-V colour index "}, {"name": "V-R", "desc": "Johnson V-R colour index "}, {"name": "R-I", "desc": "Johnson R-I colour index "}, {"name": "V-K", "desc": "Johnson V-K colour index "}, {"name": "I-K", "desc": "Johnson I-K colour index "}, {"name": "B-R", "desc": "Johnson B-R colour index "}, {"name": "B-H", "desc": "Johnson B-H colour index "}, {"name": "J-H", "desc": "Johnson J-H colour index "}, {"name": "H-K", "desc": "Johnson H-K colour index "}]}, {"name": "magshift.dat", "desc": "Luminosities from the spectra in Koo, Thuan & Gunn, Washinton and Stroemgren filter-systems, Scalo IMF, Shift, Only E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? 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Model redshift "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies "}, {"name": "z", "desc": "? Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "kcshift.dat", "desc": "Coefficients of k-correction in luminosity, H0=65 Scalo IMF, Shift, E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? 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Model redshift "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies "}, {"name": "z", "desc": "? Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "gspshift.dat", "desc": "Spectra, with Scalo IMF, Shift, E or SD galaxies ", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial metallicity (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "lambda", "desc": "Wavelength "}, {"name": "Flux1", "desc": "? Flux at a system age of 1.4000E+08yrs "}, {"name": "Flux2", "desc": "? Flux at a system age of 2.8000E+08yrs "}, {"name": "Flux3", "desc": "? Flux at a system age of 4.2000E+08yrs "}, {"name": "Flux4", "desc": "? Flux at a system age of 5.6000E+08yrs "}, {"name": "Flux5", "desc": "? Flux at a system age of 7.0000E+08yrs "}, {"name": "Flux6", "desc": "? Flux at a system age of 8.4000E+08yrs "}, {"name": "Flux7", "desc": "? Flux at a system age of 9.8000E+08yrs "}, {"name": "Flux8", "desc": "? Flux at a system age of 1.1200E+09yrs "}, {"name": "Flux9", "desc": "? Flux at a system age of 1.2600E+09yrs "}, {"name": "Flux10", "desc": "? Flux at a system age of 1.4000E+09yrs "}, {"name": "Flux11", "desc": "? Flux at a system age of 1.5400E+09yrs "}, {"name": "Flux12", "desc": "? Flux at a system age of 1.6800E+09yrs "}, {"name": "Flux13", "desc": "? Flux at a system age of 1.8200E+09yrs "}, {"name": "Flux14", "desc": "? Flux at a system age of 1.9600E+09yrs "}, {"name": "Flux15", "desc": "? Flux at a system age of 2.1000E+09yrs "}, {"name": "Flux16", "desc": "? Flux at a system age of 2.2400E+09yrs "}, {"name": "Flux17", "desc": "? Flux at a system age of 2.3800E+09yrs "}, {"name": "Flux18", "desc": "? Flux at a system age of 2.5200E+09yrs "}, {"name": "Flux19", "desc": "? Flux at a system age of 2.6600E+09yrs "}, {"name": "Flux20", "desc": "? Flux at a system age of 2.8000E+09yrs "}, {"name": "Flux21", "desc": "? Flux at a system age of 2.9400E+09yrs "}, {"name": "Flux22", "desc": "? Flux at a system age of 3.0800E+09yrs "}, {"name": "Flux23", "desc": "? Flux at a system age of 3.2200E+09yrs "}, {"name": "Flux24", "desc": "? Flux at a system age of 3.3600E+09yrs "}, {"name": "Flux25", "desc": "? Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? Flux at a system age of 4.7600E+09yrs "}, {"name": "Flux35", "desc": "Flux at a system age of 4.9000E+09yrs "}, {"name": "Flux36", "desc": "Flux at a system age of 5.0400E+09yrs "}, {"name": "Flux37", "desc": "Flux at a system age of 5.1800E+09yrs "}, {"name": "Flux38", "desc": "Flux at a system age of 5.3200E+09yrs "}, {"name": "Flux39", "desc": "Flux at a system age of 5.4600E+09yrs "}, {"name": "Flux40", "desc": "Flux at a system age of 5.6000E+09yrs "}, {"name": "Flux41", "desc": "Flux at a system age of 5.7400E+09yrs "}, {"name": "Flux42", "desc": "Flux at a system age of 5.8800E+09yrs "}, {"name": "Flux43", "desc": "Flux at a system age of 6.0200E+09yrs "}, {"name": "Flux44", "desc": "Flux at a system age of 6.1600E+09yrs "}, {"name": "Flux45", "desc": "Flux at a system age of 6.3000E+09yrs "}, {"name": "Flux46", "desc": "Flux at a system age of 6.4400E+09yrs "}, {"name": "Flux47", "desc": "Flux at a system age of 6.5800E+09yrs "}, {"name": "Flux48", "desc": "Flux at a system age of 6.7200E+09yrs "}, {"name": "Flux49", "desc": "Flux at a system age of 6.8600E+09yrs "}, {"name": "Flux51", "desc": "Flux at a system age of 7.0000E+09yrs "}, {"name": "Flux52", "desc": "Flux at a system age of 7.1400E+09yrs "}, {"name": "Flux53", "desc": "Flux at a system age of 7.2800E+09yrs "}, {"name": "Flux54", "desc": "Flux at a system age of 7.4200E+09yrs "}, {"name": "Flux55", "desc": "Flux at a system age of 7.5600E+09yrs "}, {"name": "Flux56", "desc": "Flux at a system age of 7.7000E+09yrs "}, {"name": "Flux57", "desc": "Flux at a system age of 7.8400E+09yrs "}, {"name": "Flux58", "desc": "Flux at a system age of 7.9800E+09yrs "}, {"name": "Flux59", "desc": "Flux at a system age of 8.1200E+09yrs "}, {"name": "Flux60", "desc": "Flux at a system age of 8.2600E+09yrs "}, {"name": "Flux61", "desc": "Flux at a system age of 8.4000E+09yrs "}, {"name": "Flux62", "desc": "Flux at a system age of 8.5400E+09yrs "}, {"name": "Flux63", "desc": "Flux at a system age of 8.6800E+09yrs "}, {"name": "Flux64", "desc": "Flux at a system age of 8.8200E+09yrs "}, {"name": "Flux65", "desc": "Flux at a system age of 8.9600E+09yrs "}, {"name": "Flux66", "desc": "Flux at a system age of 9.1000E+09yrs "}, {"name": "Flux67", "desc": "Flux at a system age of 9.2400E+09yrs "}, {"name": "Flux68", "desc": "Flux at a system age of 9.3800E+09yrs "}, {"name": "Flux69", "desc": "Flux at a system age of 9.5200E+09yrs "}, {"name": "Flux70", "desc": "Flux at a system age of 9.6600E+09yrs "}, {"name": "Flux71", "desc": "Flux at a system age of 9.8000E+09yrs "}, {"name": "Flux72", "desc": "Flux at a system age of 9.9400E+09yrs "}, {"name": "Flux73", "desc": "Flux at a system age of 1.0080E+10yrs "}, {"name": "Flux74", "desc": "Flux at a system age of 1.0220E+10yrs "}, {"name": "Flux75", "desc": "Flux at a system age of 1.0360E+10yrs "}, {"name": "Flux76", "desc": "Flux at a system age of 1.0500E+10yrs "}, {"name": "Flux77", "desc": "Flux at a system age of 1.0640E+10yrs "}, {"name": "Flux78", "desc": "Flux at a system age of 1.0780E+10yrs "}, {"name": "Flux79", "desc": "Flux at a system age of 1.0920E+10yrs "}, {"name": "Flux80", "desc": "Flux at a system age of 1.1060E+10yrs "}, {"name": "Flux81", "desc": "Flux at a system age of 1.1200E+10yrs "}, {"name": "Flux82", "desc": "Flux at a system age of 1.1340E+10yrs "}, {"name": "Flux83", "desc": "Flux at a system age of 1.1480E+10yrs "}, {"name": "Flux84", "desc": "Flux at a system age of 1.1620E+10yrs "}, {"name": "Flux85", "desc": "Flux at a system age of 1.1760E+10yrs "}, {"name": "Flux86", "desc": "Flux at a system age of 1.1900E+10yrs "}, {"name": "Flux87", "desc": "Flux at a system age of 1.2040E+10yrs "}, {"name": "Flux88", "desc": "Flux at a system age of 1.2180E+10yrs "}, {"name": "Flux89", "desc": "Flux at a system age of 1.2320E+10yrs "}, {"name": "Flux90", "desc": "Flux at a system age of 1.2460E+10yrs "}, {"name": "Flux91", "desc": "Flux at a system age of 1.2600E+10yrs "}, {"name": "Flux92", "desc": "Flux at a system age of 1.2740E+10yrs "}, {"name": "Flux93", "desc": "Flux at a system age of 1.2880E+10yrs "}, {"name": "Flux94", "desc": "Flux at a system age of 1.3020E+10yrs "}, {"name": "Flux95", "desc": "Flux at a system age of 1.3160E+10yrs "}, {"name": "Flux96", "desc": "Flux at a system age of 1.3300E+10yrs "}, {"name": "Flux97", "desc": "Flux at a system age of 1.3440E+10yrs "}, {"name": "Flux98", "desc": "Flux at a system age of 1.3580E+10yrs "}, {"name": "Flux99", "desc": "Flux at a system age of 1.3720E+10yrs "}, {"name": "Flux100", "desc": "Flux at a system age of 1.3860E+10yrs "}, {"name": "Flux101", "desc": "Flux at a system age of 1.4000E+10yrs "}]}, {"name": "joh50-84.dat", "desc": "Luminosities and colors from the spectra in Johnson filter-system, Scalo IMF, scenario with old disk and young bulge", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "Umag", "desc": "Johnson U magnitude "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "Rmag", "desc": "Johnson R magnitude "}, {"name": "Imag", "desc": "Johnson I magnitude "}, {"name": "Jmag", "desc": "Johnson J magnitude "}, {"name": "Hmag", "desc": "Johnson H magnitude "}, {"name": "Kmag", "desc": "Johnson K magnitude "}, {"name": "Lmag", "desc": "Johnson L magnitude "}, {"name": "U-B", "desc": "Johnson U-B colour index "}, {"name": "B-V", "desc": "Johnson B-V colour index "}, {"name": "U-V", "desc": "Johnson U-V colour index "}, {"name": "V-R", "desc": "Johnson V-R colour index "}, {"name": "R-I", "desc": "Johnson R-I colour index "}, {"name": "V-K", "desc": "Johnson V-K colour index "}, {"name": "I-K", "desc": "Johnson I-K colour index "}, {"name": "B-R", "desc": "Johnson B-R colour index "}, {"name": "B-H", "desc": "Johnson B-H colour index "}, {"name": "J-H", "desc": "Johnson J-H colour index "}, {"name": "H-K", "desc": "Johnson H-K colour index "}]}, {"name": "mag50-84.dat", "desc": "Luminosities from the spectra in Koo, Thuan & Gunn, Washinton and Stroemgren filter-systems, Scalo IMF, old disk and young bulge", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "age", "desc": "Age of system "}, {"name": "kumag", "desc": "Koo u magnitude "}, {"name": "kjmag", "desc": "Koo j magnitude "}, {"name": "kfmag", "desc": "Koo f magnitude "}, {"name": "knmag", "desc": "Koo n magnitude "}, {"name": "gmag", "desc": "Thuan & Gunn g magnitude "}, {"name": "rmag", "desc": "Thuan & Gunn r magnitude "}, {"name": "Cmag", "desc": "Washington C magnitude "}, {"name": "Mmag", "desc": "Washington M magnitude "}, {"name": "T1mag", "desc": "Washington T1 magnitude "}, {"name": "T2mag", "desc": "Washington T2 magnitude "}, {"name": "sumag", "desc": "Stroemgren u magnitude "}, {"name": "svmag", "desc": "Stroemgren v magnitude "}, {"name": "sbmag", "desc": "Stroemgren b magnitude "}, {"name": "symag", "desc": "Stroemgren y magnitude "}]}, {"name": "hst50-84.dat", "desc": "Luminosities from the spectra in HST filter-system, Scalo IMF, old disk and young bulge", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "F160BW", "desc": "HST F160BW magnitude "}, {"name": "F170W", "desc": "HST F170W magnitude "}, {"name": "F185W", "desc": "HST F185W magnitude "}, {"name": "F218W", "desc": "HST F218W magnitude "}, {"name": "F255W", "desc": "HST F255W magnitude "}, {"name": "F300W", "desc": "HST F300W = U(HDF) magnitude "}, {"name": "F336W", "desc": "HST F336W magnitude "}, {"name": "F380W", "desc": "HST F380W magnitude "}, {"name": "F439W", "desc": "HST F439W magnitude "}, {"name": "F450W", "desc": "HST F450W = B(HDF) magnitude "}, {"name": "F555W", "desc": "HST F555W = V(YSC) magnitude "}, {"name": "F569W", "desc": "HST F569W magnitude "}, {"name": "F606W", "desc": "HST F606W = V(HDF) magnitude "}, {"name": "F622W", "desc": "HST F622W magnitude "}, {"name": "F675W", "desc": "HST F675W magnitude "}, {"name": "F702W", "desc": "HST F702W magnitude "}, {"name": "F791W", "desc": "HST F791W magnitude "}, {"name": "F814W", "desc": "HST F814W = I(HDF) magnitude "}]}, {"name": "gsp50-84.dat", "desc": "Spectra, with Scalo IMF, old disk and young bulge ", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial metallicity (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "lambda", "desc": "Wavelength "}, {"name": "Flux1", "desc": "? Flux at a system age of 1.4000E+08yrs "}, {"name": "Flux2", "desc": "? Flux at a system age of 2.8000E+08yrs "}, {"name": "Flux3", "desc": "? Flux at a system age of 4.2000E+08yrs "}, {"name": "Flux4", "desc": "? Flux at a system age of 5.6000E+08yrs "}, {"name": "Flux5", "desc": "? Flux at a system age of 7.0000E+08yrs "}, {"name": "Flux6", "desc": "? Flux at a system age of 8.4000E+08yrs "}, {"name": "Flux7", "desc": "? Flux at a system age of 9.8000E+08yrs "}, {"name": "Flux8", "desc": "? Flux at a system age of 1.1200E+09yrs "}, {"name": "Flux9", "desc": "? Flux at a system age of 1.2600E+09yrs "}, {"name": "Flux10", "desc": "? Flux at a system age of 1.4000E+09yrs "}, {"name": "Flux11", "desc": "? Flux at a system age of 1.5400E+09yrs "}, {"name": "Flux12", "desc": "? Flux at a system age of 1.6800E+09yrs "}, {"name": "Flux13", "desc": "? Flux at a system age of 1.8200E+09yrs "}, {"name": "Flux14", "desc": "? Flux at a system age of 1.9600E+09yrs "}, {"name": "Flux15", "desc": "? Flux at a system age of 2.1000E+09yrs "}, {"name": "Flux16", "desc": "? Flux at a system age of 2.2400E+09yrs "}, {"name": "Flux17", "desc": "? Flux at a system age of 2.3800E+09yrs "}, {"name": "Flux18", "desc": "? Flux at a system age of 2.5200E+09yrs "}, {"name": "Flux19", "desc": "? Flux at a system age of 2.6600E+09yrs "}, {"name": "Flux20", "desc": "? Flux at a system age of 2.8000E+09yrs "}, {"name": "Flux21", "desc": "? Flux at a system age of 2.9400E+09yrs "}, {"name": "Flux22", "desc": "? Flux at a system age of 3.0800E+09yrs "}, {"name": "Flux23", "desc": "? Flux at a system age of 3.2200E+09yrs "}, {"name": "Flux24", "desc": "? Flux at a system age of 3.3600E+09yrs "}, {"name": "Flux25", "desc": "? Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? Flux at a system age of 4.7600E+09yrs "}, {"name": "Flux35", "desc": "Flux at a system age of 4.9000E+09yrs "}, {"name": "Flux36", "desc": "Flux at a system age of 5.0400E+09yrs "}, {"name": "Flux37", "desc": "Flux at a system age of 5.1800E+09yrs "}, {"name": "Flux38", "desc": "Flux at a system age of 5.3200E+09yrs "}, {"name": "Flux39", "desc": "Flux at a system age of 5.4600E+09yrs "}, {"name": "Flux40", "desc": "Flux at a system age of 5.6000E+09yrs "}, {"name": "Flux41", "desc": "Flux at a system age of 5.7400E+09yrs "}, {"name": "Flux42", "desc": "Flux at a system age of 5.8800E+09yrs "}, {"name": "Flux43", "desc": "Flux at a system age of 6.0200E+09yrs "}, {"name": "Flux44", "desc": "Flux at a system age of 6.1600E+09yrs "}, {"name": "Flux45", "desc": "Flux at a system age of 6.3000E+09yrs "}, {"name": "Flux46", "desc": "Flux at a system age of 6.4400E+09yrs "}, {"name": "Flux47", "desc": "Flux at a system age of 6.5800E+09yrs "}, {"name": "Flux48", "desc": "Flux at a system age of 6.7200E+09yrs "}, {"name": "Flux49", "desc": "Flux at a system age of 6.8600E+09yrs "}, {"name": "Flux51", "desc": "Flux at a system age of 7.0000E+09yrs "}, {"name": "Flux52", "desc": "Flux at a system age of 7.1400E+09yrs "}, {"name": "Flux53", "desc": "Flux at a system age of 7.2800E+09yrs "}, {"name": "Flux54", "desc": "Flux at a system age of 7.4200E+09yrs "}, {"name": "Flux55", "desc": "Flux at a system age of 7.5600E+09yrs "}, {"name": "Flux56", "desc": "Flux at a system age of 7.7000E+09yrs "}, {"name": "Flux57", "desc": "Flux at a system age of 7.8400E+09yrs "}, {"name": "Flux58", "desc": "Flux at a system age of 7.9800E+09yrs "}, {"name": "Flux59", "desc": "Flux at a system age of 8.1200E+09yrs "}, {"name": "Flux60", "desc": "Flux at a system age of 8.2600E+09yrs "}, {"name": "Flux61", "desc": "Flux at a system age of 8.4000E+09yrs "}, {"name": "Flux62", "desc": "Flux at a system age of 8.5400E+09yrs "}, {"name": "Flux63", "desc": "Flux at a system age of 8.6800E+09yrs "}, {"name": "Flux64", "desc": "Flux at a system age of 8.8200E+09yrs "}, {"name": "Flux65", "desc": "Flux at a system age of 8.9600E+09yrs "}, {"name": "Flux66", "desc": "Flux at a system age of 9.1000E+09yrs "}, {"name": "Flux67", "desc": "Flux at a system age of 9.2400E+09yrs "}, {"name": "Flux68", "desc": "Flux at a system age of 9.3800E+09yrs "}, {"name": "Flux69", "desc": "Flux at a system age of 9.5200E+09yrs "}, {"name": "Flux70", "desc": "Flux at a system age of 9.6600E+09yrs "}, {"name": "Flux71", "desc": "Flux at a system age of 9.8000E+09yrs "}, {"name": "Flux72", "desc": "Flux at a system age of 9.9400E+09yrs "}, {"name": "Flux73", "desc": "Flux at a system age of 1.0080E+10yrs "}, {"name": "Flux74", "desc": "Flux at a system age of 1.0220E+10yrs "}, {"name": "Flux75", "desc": "Flux at a system age of 1.0360E+10yrs "}, {"name": "Flux76", "desc": "Flux at a system age of 1.0500E+10yrs "}, {"name": "Flux77", "desc": "Flux at a system age of 1.0640E+10yrs "}, {"name": "Flux78", "desc": "Flux at a system age of 1.0780E+10yrs "}, {"name": "Flux79", "desc": "Flux at a system age of 1.0920E+10yrs "}, {"name": "Flux80", "desc": "Flux at a system age of 1.1060E+10yrs "}, {"name": "Flux81", "desc": "Flux at a system age of 1.1200E+10yrs "}, {"name": "Flux82", "desc": "Flux at a system age of 1.1340E+10yrs "}, {"name": "Flux83", "desc": "Flux at a system age of 1.1480E+10yrs "}, {"name": "Flux84", "desc": "Flux at a system age of 1.1620E+10yrs "}, {"name": "Flux85", "desc": "Flux at a system age of 1.1760E+10yrs "}, {"name": "Flux86", "desc": "Flux at a system age of 1.1900E+10yrs "}, {"name": "Flux87", "desc": "Flux at a system age of 1.2040E+10yrs "}, {"name": "Flux88", "desc": "Flux at a system age of 1.2180E+10yrs "}, {"name": "Flux89", "desc": "Flux at a system age of 1.2320E+10yrs "}, {"name": "Flux90", "desc": "Flux at a system age of 1.2460E+10yrs "}, {"name": "Flux91", "desc": "Flux at a system age of 1.2600E+10yrs "}, {"name": "Flux92", "desc": "Flux at a system age of 1.2740E+10yrs "}, {"name": "Flux93", "desc": "Flux at a system age of 1.2880E+10yrs "}, {"name": "Flux94", "desc": "Flux at a system age of 1.3020E+10yrs "}, {"name": "Flux95", "desc": "Flux at a system age of 1.3160E+10yrs "}, {"name": "Flux96", "desc": "Flux at a system age of 1.3300E+10yrs "}, {"name": "Flux97", "desc": "Flux at a system age of 1.3440E+10yrs "}, {"name": "Flux98", "desc": "Flux at a system age of 1.3580E+10yrs "}, {"name": "Flux99", "desc": "Flux at a system age of 1.3720E+10yrs "}, {"name": "Flux100", "desc": "Flux at a system age of 1.3860E+10yrs "}, {"name": "Flux101", "desc": "Flux at a system age of 1.4000E+10yrs "}]}, {"name": "pl150-84.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 1 old disk and young bulge", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) (1) "}, {"name": "z0", "desc": "? 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Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? 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Flux at a system age of 1.6800E+09yrs "}, {"name": "Flux13", "desc": "? Flux at a system age of 1.8200E+09yrs "}, {"name": "Flux14", "desc": "? Flux at a system age of 1.9600E+09yrs "}, {"name": "Flux15", "desc": "? Flux at a system age of 2.1000E+09yrs "}, {"name": "Flux16", "desc": "? Flux at a system age of 2.2400E+09yrs "}, {"name": "Flux17", "desc": "? Flux at a system age of 2.3800E+09yrs "}, {"name": "Flux18", "desc": "? Flux at a system age of 2.5200E+09yrs "}, {"name": "Flux19", "desc": "? Flux at a system age of 2.6600E+09yrs "}, {"name": "Flux20", "desc": "? Flux at a system age of 2.8000E+09yrs "}, {"name": "Flux21", "desc": "? Flux at a system age of 2.9400E+09yrs "}, {"name": "Flux22", "desc": "? Flux at a system age of 3.0800E+09yrs "}, {"name": "Flux23", "desc": "? Flux at a system age of 3.2200E+09yrs "}, {"name": "Flux24", "desc": "? Flux at a system age of 3.3600E+09yrs "}, {"name": "Flux25", "desc": "? Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? Flux at a system age of 4.7600E+09yrs "}, {"name": "Flux35", "desc": "Flux at a system age of 4.9000E+09yrs "}, {"name": "Flux36", "desc": "Flux at a system age of 5.0400E+09yrs "}, {"name": "Flux37", "desc": "Flux at a system age of 5.1800E+09yrs "}, {"name": "Flux38", "desc": "Flux at a system age of 5.3200E+09yrs "}, {"name": "Flux39", "desc": "Flux at a system age of 5.4600E+09yrs "}, {"name": "Flux40", "desc": "Flux at a system age of 5.6000E+09yrs "}, {"name": "Flux41", "desc": "Flux at a system age of 5.7400E+09yrs "}, {"name": "Flux42", "desc": "Flux at a system age of 5.8800E+09yrs "}, {"name": "Flux43", "desc": "Flux at a system age of 6.0200E+09yrs "}, {"name": "Flux44", "desc": "Flux at a system age of 6.1600E+09yrs "}, {"name": "Flux45", "desc": "Flux at a system age of 6.3000E+09yrs "}, {"name": "Flux46", "desc": "Flux at a system age of 6.4400E+09yrs "}, {"name": "Flux47", "desc": "Flux at a system age of 6.5800E+09yrs "}, {"name": "Flux48", "desc": "Flux at a system age of 6.7200E+09yrs "}, {"name": "Flux49", "desc": "Flux at a system age of 6.8600E+09yrs "}, {"name": "Flux51", "desc": "Flux at a system age of 7.0000E+09yrs "}, {"name": "Flux52", "desc": "Flux at a system age of 7.1400E+09yrs "}, {"name": "Flux53", "desc": "Flux at a system age of 7.2800E+09yrs "}, {"name": "Flux54", "desc": "Flux at a system age of 7.4200E+09yrs "}, {"name": "Flux55", "desc": "Flux at a system age of 7.5600E+09yrs "}, {"name": "Flux56", "desc": "Flux at a system age of 7.7000E+09yrs "}, {"name": "Flux57", "desc": "Flux at a system age of 7.8400E+09yrs "}, {"name": "Flux58", "desc": "Flux at a system age of 7.9800E+09yrs "}, {"name": "Flux59", "desc": "Flux at a system age of 8.1200E+09yrs "}, {"name": "Flux60", "desc": "Flux at a system age of 8.2600E+09yrs "}, {"name": "Flux61", "desc": "Flux at a system age of 8.4000E+09yrs "}, {"name": "Flux62", "desc": "Flux at a system age of 8.5400E+09yrs "}, {"name": "Flux63", "desc": "Flux at a system age of 8.6800E+09yrs "}, 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III.", "title_create": "Anders+, 2003", "year": "2003", "author": "Anders P., Fritze-v.Alvensleben U.", "title_pub": "Spectral and photometric evolution of young stellar populations: The impact of gaseous emission at various metallicities.", "first_author": "Anders P.", "ref_biblio": [""], "bibcode": ["2003A&A...401.1063A"], "see_also": ["http://www.uni-sw.gwdg.de/~galev : The Goettingen Galaxy Evolution Group", "J/A+A/392/1 : Spectrophotometry of simulated SSPs (Schulz+, 2002)", "J/A+A/398/89 : Evolutionary synthesis models. II. (Schulz+, 2003)"], "keyword_cds": "Clusters, globular ; Clusters, open ; Spectrophotometry ; Colors", "keyword_pub": "globular clusters: general - open clusters and associations: general - galaxies: star clusters - galaxies: evolution", "abstract": ["We include gaseous continuum and line emission into our GALEV models", "for the spectral and photometric evolution of Simple Stellar", "Populations (SSPs) for various metallicities in the range", "0.02<=Z/Z_{Sun}_<=2.5. This allows to extend them to significantly", "younger ages than before. They now cover the age range from 4 Myr all", "through 14 Gyr. We point out the very important contributions of", "gaseous emission to broad band fluxes and their strong metallicity", "dependence during very early evolutionary stages of star clusters,", "galaxies or subgalactic fragments with vigorous ongoing star", "formation. Emission-line contributions are commonly seen in these", "actively star-forming regions. Models without gaseous emission cannot", "explain their observed colors at all, or lead to wrong age estimates.", "We use up-to-date Lyman continuum (=Lyc) emission rates and decided to", "use recent empirical determinations of emission line ratios relative", "to H{beta} for subsolar metallicities. We justify this approach for", "all situations where no or not enough spectral information is", "available to determine all the parameters required by photoionization", "models. The effects of gaseous line and continuum emission on broad", "band fluxes are shown for different metallicities and as a function of", "age. In addition to the many filter systems already included in our", "earlier models, we here also include the HST NICMOS and Advanced", "Camera for Surveys (=ACS) filter systems."], "description": ["The models are calculated for 5 metallicities, Z=0.0004, Z=0.004,", "Z=0.008, Z=0.02, and Z=0.05, with an assumed IMF Phi(m) = m^{alpha}^,", "salpeter <-> {alpha}=-2.35 for all masses;", "scalo <-> {alpha}=-1.25 for m<=1M_{sun}_,", "{alpha}=-2.35 for 1M_{sun}_"], "bibcode": ["1975A&A....41..413M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_413_37"}} {"id": "J/A+A/413/37", "title_cds": "Synthetic spectra of galaxies", "title_create": "Bicker+, 2004", "year": "2004", "author": "Bicker J., Fritze-V.Alvensleben U., Moeller C.S., Fricke K.J.", "title_pub": "Chemically consistent evolution of galaxies. II. Spectrophotometric evolution from zero to high redshift.", "first_author": "Bicker J.", "ref_biblio": [""], "bibcode": ["2004A&A...413...37B"], "keyword_cds": "", "keyword_pub": "", "mission": "", "description": ["All data are available for following galaxy types: E, Sa, Sb,", "Sc, and Sd.", "The e and k- corrections and the apparent magnitudes (VEGAMAG system)", "are given for the Johnson-Cousins-Bessell&Brett U, B, V, Rc, Ic, J, H,", "K passbands and for the HST/WFPC2 wide-band passbands up to a redshift", "of z=5.", "The spectra are given as a function of redshift and as a", "function of evolution time in the restframe.", "In case of the redshift evolution the k-correction and the", "spectra are given with and without the effect of attenuation.", "For the cosmology we assume H0=65, Omega0=0.1 and a formation", "of galaxies at z=5.", "The fluxes of the spectra are given in [erg/cm^2^/s/{AA}"], "object": [], "curator": "James Marcout, Patricia Bauer [CDS]", "doi_pub": ["10.1051/0004-6361:20031483"], "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_445_93"}} {"id": "J/A+A/445/93", "title_cds": "Abundances of DLAs", "title_create": "Dessauges-Zavadsky+, 2006", "year": "2006", "author": "Dessauges-Zavadsky M., Prochaska J.X., D'odorico S., Calura F., Matteucci F.", "title_pub": "A new comprehensive set of elemental abundances in DLAs. II. Data analysis and chemical variation studies.", "first_author": "Dessauges-Zavadsky M.", "ref_biblio": [""], "bibcode": ["2006A&A...445...93D"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1051/0004-6361:20053200"], "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_465_339"}} {"id": "J/A+A/465/339", "title_cds": "Synthetic stellar polarization 400-1000nm", "title_create": "Socas-Navarro+ 2007", "year": "2007", "author": "Socas-Navarro H., Asensio Ramos A., Manso Sainz R.", "title_pub": "A synthetic stellar polarization atlas from 400 to 1000 nm.", "first_author": "Socas-Navarro H.", "ref_biblio": [""], "bibcode": ["2007A&A...465..339S"], "see_also": ["http://download.hao.ucar.edu/pub/PSA : Home Page"], "keyword_cds": "", "keyword_pub": "atlases - stars: atmospheres - stars: magnetic fields - line: formation - polarization - radiative transfer", "abstract": ["With the development of new polarimeters for large telescopes, the", "spectro-polarimetric study of astrophysical bodies is becoming", "feasible and, indeed, more frequent. In particular, this is permitting", "the observational study of stellar magnetic fields.", "With the aim to optimize and interpret this kind of observations, we", "have produced a spectral atlas of circular polarization in a grid of", "stellar atmospheric models with effective temperatures between 3500", "and 10000K, surface gravities log(g)=3.5-5, metallicities between", "10^-2^ and 1, and magnetic field strengths of 100, 1000 and 5000G."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1051/0004-6361:20066388"], "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_468_o.205"}} {"id": "J/A+A/468/205", "title_cds": "Spectra of red giants and supergiants", "title_create": "Lancon+, 2007", "year": "2007", "author": "Lancon A., Hauschildt P.H., Ladjal D., Mouhcine M.", "title_pub": "Near-IR spectra of red supergiants and giants. I- Models with solar and with mixing-induced surface abundance ratios.", "first_author": "Lancon A.", "ref_biblio": [""], "bibcode": ["2007A&A...468..205L"], "keyword_cds": "Stars, giant ; Stars, supergiant ; Spectra, infrared ; Models", "keyword_pub": "stars: fundamental parameters - stars: abundances - infrared: stars - stars: atmospheres", "abstract": ["It remains difficult to interpret the near-IR emission of young", "stellar populations. One main reason is our incomplete understanding", "of the spectra of luminous red stars. This work provides a grid of", "theoretical spectra of red giant (RG) and red supergiant (RSG) stars,", "that extends through optical and near-IR wavelengths. For the first", "time, models are also provided with modified surface abundances of C,", "N and O, as a step towards accounting for the changes that occur due", "to convective dredge-up in red supergiants or may occur at earlier", "evolutionary stages in the case of rotation. The aims are (i) to", "assess how well current models reproduce observed spectra, in", "particular in the near-IR; (ii) to quantify the effects of the", "abundance changes on the spectra; and (iii) to determine how these", "changes affect estimates of fundamental stellar parameters."], "description": ["Each FITS file in this directory contains a theoretical stellar", "spectrum. The spherical model atmospheres and the synthetic spectra", "were computed with PHOENIX version 13.11.00B as described in the", "article, with an initial wavelength sampling step of 0.01nm in the", "wavelength range of interest [510nm-2490nm]. The spectra made", "available here have been smoothed with a Gaussian with a full width", "at half maximum of 0.2nm. They are resampled with a wavelength step", "of 0.025nm."], "date_update": "10-Oct-2022", "tables": [{"name": "table1.dat", "desc": "List of the spectra ", "columns": [{"name": "Model", "desc": "Model (m15rsg, m15solar or m1solar) "}, {"name": "Mass", "desc": "Mass "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "FileName", "desc": "Name of the fits file "}]}, {"name": "m15rsg/*", "desc": "RSG-specific abundances, M=15M_{sun}_ model spectra ", "columns": []}, {"name": "m15solar/*", "desc": "Solar abundances, M=15M_{sun}_ model spectra ", "columns": []}, {"name": "m1solar/*", "desc": "Solar abundances, M=1M_{sun}_ model spectra ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_583_A122"}} {"id": "J/A+A/583/A122", "title_cds": "Variability behaviour of CoRoT M-giant stars", "title_create": "Ferreira+, 2015", "year": "2015", "author": "Ferreira Lopes C.E., Neves V., Leao I.C., De Freitas D.B., Canto Martins B.L., Da Costa A.D., Paz-Chinchon F., Das Chagas M.L., Baglin A., Janot-Pacheco E., De Medeiros J.R.", "title_pub": "The variability behaviour of CoRoT M-giant stars.", "first_author": "Ferreira Lopes C.E.", "ref_biblio": [""], "bibcode": ["2015A&A...583A.122F"], "see_also": ["B/corot : CoRoT observation log (N2-4.4) (CoRoT 2016)", "III/282 : CoRoT Bright Stars Catalogue with variability classes (Baglin+, 2015)"], "keyword_cds": "Stars, giant ; Stars, M-type ; Stars, variable ; Surveys ; Optical", "keyword_pub": "catalogs - stars: oscillations - stars: evolution", "abstract": ["For six years the Convection, Rotation, and planetary Transits (CoRoT)", "space mission has been acquiring photometric data from more than 100", "000 point sources towards and directly opposite the inner and outer", "regions of the Galaxy. The high temporal resolution of the CoRoT data,", "combined with the wide time span of the observations, enabled the", "study of short- and long-time variations in unprecedented detail.", "The aim of this work is to study the variability and evolutionary", "behaviour of M-giant stars using CoRot data.", "From the initial sample of 2534 stars classified as M giants in the", "CoRoT databases, we selected 1428 targets that exhibit well defined", "variability, by visual inspection. Then, we defined three catalogues:", "C1 - stars with T_eff_<4200K and LCs displaying semi-sinusoidal", "signatures; C2 - rotating variable candidates with T_eff_>4200K; C3 -", "long-period variable candidates (with LCs showing a variability period", "up to the total time span of the observations). The variability period", "and amplitude of C1 stars were computed using Lomb-Scargle and", "harmonic fit methods. Finally, we used C1 and C3 stars to study the", "variability behaviour of M-giant stars.", "The trends found in the V-I vs. J-K colour-colour diagram are in", "agreement with standard empirical calibrations for M giants. The", "sources located towards the inner regions of the Galaxy are", "distributed throughout the diagram, while the majority of the stars", "towards the outer regions of the Galaxy are spread between the", "calibrations of M giants and the predicted position for carbon stars.", "The stars classified as supergiants follow a different sequence from", "the one found for giant stars. We also performed a Kolmogorov-Smirnov", "(KS) test of the period and amplitude of stars towards the inner and", "outer regions of the Galaxy. We obtained a low probability that the", "two samples came from the same parent distribution. The observed", "behaviour of the period-amplitude and period-effective temperature", "(T_eff_) diagrams are, in general, in agreement with those found for", "Kepler sources and ground based photometry, with pulsation being the", "dominant cause responsible for the observed modulation. We also", "conclude that short-time variations on M-giant stars do not exist or", "are very rare, and the few cases we found are possibly related to", "biases or background stars."], "description": ["Photometric parameters for 1435 M CoRot stars. For each star, CoRoT", "IDs, coordinates, V, I, J, and Ks magnitudes, temperature, amplitude,", "and period are provided. This table was performed seven years after", "publication and hence minor errors can be found."], "type": ["CCC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "tables.dat", "desc": "Stellar parameters of C1, C2 and C3 samples (tables 2-4)", "columns": [{"name": "CoRoT", "desc": "CoRoT ID "}, {"name": "RAdeg", "desc": "Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "SpType", "desc": "CoRoT-Spectral type "}, {"name": "LC", "desc": "CoRoT-luminosity class "}, {"name": "Type", "desc": "Variable type "}, {"name": "Vmag", "desc": "?=- V magnitude "}, {"name": "V0mag", "desc": "?=- Deredenned V magnitude "}, {"name": "Imag", "desc": "?=- I magnitude "}, {"name": "I0mag", "desc": "?=- Deredenned I magnitude "}, {"name": "Jmag", "desc": "J magnitude "}, {"name": "J0mag", "desc": "Deredenned J magnitude "}, {"name": "Kmag", "desc": "K magnitude "}, {"name": "K0mag", "desc": "?=- Deredenned K magnitude "}, {"name": "Teff", "desc": "?=- Effective temperature "}, {"name": "Per", "desc": "Period "}, {"name": "Amp", "desc": "Amplitude "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_649_A81"}} {"id": "J/A+A/649/A81", "title_cds": "KiDSDR4 QSOs photometric redshifts catalog", "title_create": "Nakoneczny+, 2021", "year": "2021", "author": "Nakoneczny S.J., Bilicki M., Pollo A., Asgari M., Dvornik A., Erben T., Giblin B., Heymans C., Hildebrandt H., Kannawadi A., Kuijken K., Napolitano N.R., Valentijn E.", "title_pub": "Photometric selection and redshifts for quasars in the Kilo-Degree Survey Data Release 4.", "first_author": "Nakoneczny S.J.", "ref_biblio": [""], "bibcode": ["2021A&A...649A..81N\t(SIMBAD/NED"], "see_also": ["J/A+A/624/A13 : KiDS DR3 QSO catalog (Nakoneczny+, 2019)"], "keyword_cds": "Surveys ; Active gal. nuclei ; QSOs ; Galaxy catalogs; Galaxies, photometry ; Redshifts ; Colors", "keyword_pub": "methods: data analysis - methods: observational - catalog - surveys - quasars: general - large-scale structure of Universe", "abstract": ["We present a catalog of quasars with their corresponding redshifts", "derived from the photometric Kilo-Degree Survey (KiDS) Data Release 4.", "We achieved it by training machine learning (ML) models using optical", "ugri and near-infrared ZYJHKs bands, on objects known from SDSS", "spectroscopy. We define inference subsets from the 45 million objects", "of the KiDS photometric data limited to 9-band detections, based on a", "feature space built from magnitudes and their combinations. We show", "that projections of the high-dimensional feature space on two", "dimensions can be successfully used instead of the standard", "color-color plots, to investigate the photometric estimations, compare", "them with spectroscopic data, and efficiently support the process of", "building a catalog. The model selection and fine-tuning employs two", "subsets of objects: those randomly selected and the faintest ones,", "which allows us to properly fit the bias vs. variance trade-off. We", "test three ML models: Random Forest (RF), XGBoost (XGB) and Artificial", "Neural Network (ANN). We find that XGB is the most robust and", "straightforward model for classification, while ANN performs the best", "for combined classification and redshift. The ANN inference results", "are tested using number counts, Gaia parallaxes and other quasar", "catalogs external to the training set. Based on these tests, we derive", "the minimum classification probability for quasar candidates which", "provides the best purity vs. completeness trade-off: p(QSO_cand)>0.9", "for r<22, and p(QSO_cand)>0.98 for 22"], "bibcode": ["2021A&A...654A..79G"], "keyword_cds": "", "keyword_pub": "early Universe - galaxies: active - quasars: general - stars: low-mass - brown dwarfs", "abstract": ["Context. Large-scale surveys over the last years have revealed about", "300 quasi-stellar objects (QSOs) at redshifts above 6. Follow-up", "observations have identified surprising properties, such as the very", "high black hole (BH) masses, spatial correlations with surrounding", "cold gas of the host galaxy, and high CIV-MgIIVelocity shifts. In", "particular, the discovery of luminous high-redshift quasars suggests", "that at least some BHs likely have high masses at birth and grow", "efficiently. Aims. Our aim is to quantify quasar pairs at high", "redshift for a large sample of objects. This provides a new key", "constraint on a combination of parameters related to the origin and", "assembly for the most massive BHs: formation efficiency and", "clustering, growth efficiency, and the relative contribution of BH", "mergers. Methods. We observed 116 spectroscopically confirmed QSOs", "around redshift 6 with the simultaneous seven-channel imager Gamma-ray", "Burst Optical/Near-infrared Detector in order to search for", "companions. Applying colour-colour cuts identical to those which led", "to the spectroscopically confirmed QSOs, we performed Le PHARE fits to", "the 26 best QSO pair candidates, and obtained spectroscopic", "observations for 11 of them. Results. We do not find any QSO pair with", "a companion brighter than M_1450_(AB)<-26mag within our", "0.1-3.3h^-1^cMpc search radius, in contrast to the serendipitous", "findings in the redshift range 4-5. However, a small fraction of such", "pairs at this luminosity and redshift is consistent with indications", "from present-day cosmological-scale galaxy evolution models. In turn,", "the incidence of L- and T-type brown dwarfs, which occupy a similar", "colour space to z~6 QSOs, is higher than expected, by a factor of 5", "and 20, respectively."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_662_A84"}} {"id": "J/A+A/662/A84", "title_cds": "MS 0451.6-0305 ram pressure stripping galaxies", "title_create": "Durret+, 2022", "year": "2022", "author": "Durret F., Degott L., Lobo C., Ebeling H., Jauzac M., Tam S.-I.", "title_pub": "Ram pressure stripping in the z~0.5 galaxy cluster MS 0451.6-0305.", "first_author": "Durret F.", "ref_biblio": [""], "bibcode": ["2022A&A...662A..84D\t(SIMBAD/NED"], "see_also": ["J/A+A/631/A114 : Ram pressure in cluster galaxies a z=0.7 (Boselli+, 2019)"], "keyword_cds": "Clusters, galaxy ; Redshifts ; Photometry, infrared", "keyword_pub": "galaxies: clusters: individual: MS 0451.6-0305 - galaxies: photometry - galaxies: peculiar", "abstract": ["The pressure exerted by the ambient hot X-ray gas on cluster galaxies", "can lead to the presence of ram pressure stripped (RPS) galaxies,", "characterized by asymmetric shapes, and, in some cases, tails of blue", "stars and/or X-ray gas, with increased star formation.", "With the aim of increasing the known sample of RPS galaxies at", "redshift z~0.5, notably higher than most RPS samples presently known,", "we extended our searches for such galaxies to the cluster MS", "0451.6-0305.", "Our study is based on Hubble Space Telescope (HST) imaging in the", "F814W band (corresponding to a restframe wavelength of 529nm),", "covering a region of about 6\u00d76Mpc^2^, an eight magnitude ground-based", "catalogue with photometric redshifts, and a spectroscopic redshift", "catalogue. We defined as cluster members a spectroscopic redshift", "sample of 359 galaxies within +/-4{sigma}v of the mean cluster", "velocity, and a photometric redshift sample covering the [0.48,0.61]", "range. We searched for RPS galaxies in the HST images and tested the", "error on their classification with a Zooniverse collaboration. We also", "computed the phase space diagram of RPS candidates in the", "spectroscopic sample. Finally, we ran the LePhare stellar population", "synthesis code through the GAZPAR interface to analyze and compare the", "properties of RPS and non-RPS galaxies.", "We find 56 and 273 RPS candidates in the spectroscopic and photometric", "redshift samples, respectively. They are distributed throughout the", "cluster and tend to avoid high density regions. The phase space", "diagram gives the percentages of virialized, backsplash, and infall", "galaxies. RPS galaxy candidates typically show rather high star", "formation rates, young ages, and relatively low masses. We compare all", "our results to those previously obtained for the massive merging", "cluster MACS J0717+3745, at a similar redshift.", "This study increases by at least 56 objects if we only consider", "galaxies with spectroscopic redshifts, and probably much more if", "galaxies with photometric redshifts are taken into account. This study", "increases the number of RPS candidates at redshift z>0.5, and", "confirms that they host, on average, younger stellar populations and", "strongly form stars when compared with non-RPS counterparts. The fact", "that RPS candidates with spectroscopic and with photometric redshifts", "have comparable properties shows that large samples of such objects", "could be gathered based on multi-band photometry only, a promising", "result in view of the very large imaging surveys planned in the coming", "years (DES, Euclid, LSST, etc.)."], "description": ["Our study is based on a large HST/ACS mosaic in the F814W filter", "covering a region of about 6\u00d76Mpc^2^ at the cluster redshift,", "collected for the programmes GO-09836, -10493, and -11591. We", "also examined F555W imaging from a single ACS pointing obtained for", "GO-09722 but found the covered area too small to be significant for", "the purpose of this work."], "object": ["04 54 10.9 -03 01 07 MS 0451.6-0305 = ClG 0451-03"], "type": ["OC"], "data": "", "date_update": "10-Oct-2022", "tables": [{"name": "catalog.dat", "desc": "Ram pressure stripping (RPS) galaxy candidates ", "columns": [{"name": "Seq", "desc": "Running number "}, {"name": "RAdeg", "desc": "Right ascension (J2000.0) "}, {"name": "DEdeg", "desc": "Declination (J2000.0) "}, {"name": "z", "desc": "Photometric redshift "}, {"name": "Class", "desc": "[1/5] J classification (according to Poggianti et al., 2016AJ....151...78P,"}, {"name": "(1)", "desc": " "}, {"name": "F814W", "desc": "F814W magnitude "}, {"name": "e_F814W", "desc": "Error on F814W magnitude "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+A_663_A45"}} {"id": "J/A+A/663/A45", "title_cds": "Short Title", "title_create": "Krzesinski+, 2022", "year": "2022", "author": "Krzesinski J., Balona L.A.", "title_pub": "Discovery of new TESS pulsating hot subdwarfs.", "first_author": "Krzesinski J.", "ref_biblio": [""], "bibcode": ["2022A&A...663A..45K"], "keyword_cds": "", "keyword_pub": "subdwarfs - stars: oscillations", "abstract": ["This work is dedicated to a search for new pulsating hot subdwarfs in", "TESS photometric data which could have been missed in previous", "searches.", "By matching catalogues of hot subdwarfs with TESS targets and using", "luminosities from Gaia parallaxes, a list of 1389 candidate hot", "subdwarfs observed by TESS was created. The periodograms of these", "stars were inspected, and the stars were classified according to", "variability type.", "An updated catalogue of all known pulsating hot subdwarfs is", "presented. A number of probable pulsating binaries have been", "identified, which might prove useful for verifying the asteroseismic", "masses. The mean masses of p- and g-mode pulsators are estimated from", "the stellar parameters.", "A list of 63 previously unknown pulsating hot subdwarfs observed by", "TESS is presented. More than half of the stars previously identified", "as pure p-mode pulsators are found to have frequencies in the g-mode", "region as well. As a result, hybrid p- and g-mode pulsators occur over", "the whole instability strip."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_101_447"}} {"id": "J/A+AS/101/447", "title_cds": "Spectral Characteristics of RATAN-600 sources", "title_create": "Bursov+ 1993", "year": "1993", "author": "Bursov N.N., Chepurnov A.V., Lipovka N.M., Soboleva N.S., Temirova A.V.", "title_pub": "The spectral characteristics of the Ratan-600 RC-catalog sources.", "first_author": "Bursov N.N.", "ref_biblio": [""], "bibcode": ["1993A&AS..101..447B"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "21-Mar-2000"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_13_133"}} {"id": "J/A+AS/13/133", "title_cds": "UBV observations of Mira variables", "title_create": "Koester+, 1974", "year": "1974", "author": "Koester D.", "title_pub": "UBV observations of Mira variables near maximum light.", "first_author": "Koester D.", "ref_biblio": [""], "bibcode": ["1974A&AS...13..133K"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["UBV observations are presented for 14 Mira variables near maximum", "light and further observations of about 15 variables made at ESO"], "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_21_109"}} {"id": "J/A+AS/21/109", "title_cds": "O-B2 stars in the Large Magellanic Cloud", "title_create": "Brunet+, 1975", "year": "1975", "author": "Brunet J.P., Imbert M., Martin N., Mianes P., Prevot L., Rebeirot E., Rousseau J.", "title_pub": "Recherches dans le Grand Nuage de Magellan. I. Un catalogue de 272 etoiles O-B2 nouvelles.", "first_author": "Brunet J.P.", "ref_biblio": [""], "bibcode": ["1975A&AS...21..109B"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_29_31"}} {"id": "J/A+AS/29/31", "title_cds": "UBV and spectral classes in Loden associations", "title_create": "Loden+, 1977", "year": "1977", "author": "Loden L.O.", "title_pub": "A study of some loose clusterings in the Southern Milky Way.", "first_author": "Loden L.O.", "ref_biblio": [""], "bibcode": ["1977A&AS...29...31L"], "see_also": ["III/40A : Spectral Survey of Southern Milky Way (Loden+ 1976)"], "keyword_cds": "Photometry, UBV ; Associations, stellar ; Spectral types", "keyword_pub": "clusters ; photometry", "description": ["The catalog contains precise coordinates and identifications for 620", "stars observed in 19 loose open clusters observed by Loden as part of", "a larger survey of similar fields. The UBV data come from the original", "publication (observations made at ESO telescopes between 1969 and", "1976), as well as the spectral types (from objective-prism spectra at", "Boyden Observatory, South Africa in 1956 and 1966). The positions and", "identifications were computed by B. Skiff (Lowell Observatory) from", "Loden's charts in November 2009.", "Although reported as sparse open clusters or cluster remnants,", "probably only NGC 4633 = Loden 623 is likely to contain more", "than a few stars that are physically related."], "type": ["OC"], "data": "", "date_update": "17-Nov-2009", "tables": [{"name": "catalog.dat", "desc": "Positions, identifications, UBV and spectral types of stars in 19 loose groupings.", "columns": [{"name": "---", "desc": "[Cl Loden] "}, {"name": "Fld", "desc": "Field number "}, {"name": "Seq", "desc": "Running number of star in field "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[MTU] Source of position (1) "}, {"name": "UCAC2", "desc": "? Designation in UAC2 catalog (I/289) "}, {"name": "CD", "desc": "Cordoba Ducrnmusterung "}, {"name": "m_CD", "desc": "[ab] Multiplicity index on CD "}, {"name": "CPD", "desc": "Cape Photographic Durchmusterung "}, {"name": "m_CPD", "desc": "[ab] Multiplicity index on CPD "}, {"name": "HD", "desc": "? HD identification (Cat. III/1345) "}, {"name": "m_HD", "desc": "[ab] Multiplicity index on CPD "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "B-V", "desc": "? Johnson (B-V) color "}, {"name": "U-B", "desc": "? Johnson (U-B) color "}, {"name": "Sp", "desc": "Spectal type "}, {"name": "Notes", "desc": "Other identifications and notes from B. Skiff "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_32_25"}} {"id": "J/A+AS/32/25", "title_cds": "Spectral types of stars along the Milky Way", "title_create": "Rydstrom+, 1978", "year": "1978", "author": "Rydstrom B.A.", "title_pub": "A spectrophotometric survey of stars along the Milky Way. IV.", "first_author": "Rydstrom B.A.", "ref_biblio": [""], "bibcode": ["1978A&AS...32...25R"], "see_also": ["B/mk: Catalogue of Stellar Spectral Classifications (Skiff, 2009-2014)"], "keyword_cds": "MK spectral classification", "keyword_pub": "narrow-band photometry ; interstellar matther ; Perseus arm", "abstract": ["In the present paper a catalogue of spectrophotometric quantities,", "spectral types, monochromatic magnitudes and colour equivalents is", "given for all stars brighter than the magnitude m_4400_=10.5 in a", "region of the Milky Way in Perseus. No absorption is found for stars", "closer than about r=100pc. The absorbing clouds are situated at", "distances closer than1 kpc and at about 2.5 kpc in the local arm and", "the Perseus arm, respectively. The space between the two arms is free", "from absorption. It is also concluded that the Perseus arm continues", "beyond l=140{deg}, containing not only hydrogen gas but also dust to", "at least l=150{deg}), while the content of OB stars decreases abruptly", "at l=140{deg}."], "data": "", "date_update": "02-Mar-2014", "tables": [{"name": "stars.dat", "desc": " ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "[0/60] Declination J2000 (seconds) "}, {"name": "r", "desc": "[TU] Origin of position (2MASS or UCAC?) "}, {"name": "Vmag", "desc": " "}, {"name": "---", "desc": "[V] "}, {"name": "SpT", "desc": "MK spectral type "}, {"name": "Comments", "desc": "B. Skiff's comments "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_36_83"}} {"id": "J/A+AS/36/83", "title_cds": "UBV photometry in Southern Milky Way", "title_create": "Loden+, 1979", "year": "1979", "author": "Loden L.O.", "title_pub": "Photometry of loose clusterings in the Southern Milky Way.", "first_author": "Loden L.O.", "ref_biblio": [""], "bibcode": ["1979A&AS...36...83L"], "keyword_cds": "Photometry, UBV ; Photometry, uvby ; MK spectral classification", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_4_51"}} {"id": "J/A+AS/4/51", "title_cds": "Catalogue of galactic southern carbon stars", "title_create": "Westerlund, 1971", "year": "1971", "author": "Westerlund B.E.", "title_pub": "A catalogue of carbon stars in the southern Milky Way.", "first_author": "Westerlund B.E.", "ref_biblio": [""], "bibcode": ["1971A&AS....4...51W"], "see_also": ["III/40 : Spectral Survey of Southern Milky Way (Loden+ 1976)", "III/43 : Luminous Stars in the Southern Milky Way (Stephenson+ 1971)", "VII/216 : H-alpha emission regions in Southern Milky Way (Rodgers+ 1960)", "J/other/SAAOC/15.53 : Southern reddened luminous stars II (Kilkenny 1993)", "J/other/SAAOC/15.65 : Southern reddened luminous stars III (Kilkenny+ 1993)", "J/other/SAAOC/15.73 : Southern reddened luminous stars IV (Spencer Jones+ 1993)"], "keyword_cds": "Stars, carbon ; Photometry, infrared", "keyword_pub": "Southern Milky Way - carbon stars - infrared survey", "abstract": ["An objective-prism survey in infrared light has been carried out of", "the Southern Milky Way from l^II^=235{deg} to l^II^=7{deg} and between", "b^II^=+/-5{deg}. The present catalogue gives positions and estimated", "visual and infrared magnitudes for 1124 carbon stars identified in the", "survey. The positions of the stars will be given on overlays to an", "Atlas of the Southern Milky Way, which is under preparation."], "data": "", "date_update": "20-Jun-2002", "tables": [{"name": "table1.dat", "desc": "Carbon stars in the Southern Milky Way ", "columns": [{"name": "[W71b]", "desc": "Sequential number "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "RAs", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "Vmag", "desc": "? V magnitude "}, {"name": "Imag", "desc": "I magnitude "}]}, {"name": "table2.dat", "desc": "Carbon stars identified by Blanco and Munch ", "columns": [{"name": "BM", "desc": "Blanco-Munch (1955BOTT....2l..17B) number (BM IV NNN)"}, {"name": "[W71b]", "desc": "Westerlund number "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_41_173"}} {"id": "J/A+AS/41/173", "title_cds": "UBV and spectral classification in the Galaxy", "title_create": "Loden+, 1980", "year": "1980", "author": "Loden L.O.", "title_pub": "Concluding observations of loose stellar clusterings in the Southern Milky Way.", "first_author": "Loden L.O.", "ref_biblio": [""], "bibcode": ["1980A&AS...41..173L"], "see_also": ["J/A+AS/44/155 :"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["UBV photometry and spectral classification have been performed on 280", "stars in the Carina-Crux-Centaurus-Norma region, suspected of", "belonging to poor open clusters or associations. The work is a", "concluding part of a large project for detecting and listing of such", "objects in order to obtain an improved concept about the true", "frequency of clusterings in the Milky Way. The result indicates that a", "majority of the suspected objects are members of various types of", "physical stellar clusterings, occasionally cluster remnants."], "object": [], "data": "", "date_update": "08-Dec-2013", "tables": [{"name": "loden4.dat", "desc": " ", "columns": [{"name": "---", "desc": "[Cl Loden] "}, {"name": "Cl", "desc": "Cluster number "}, {"name": "Seq", "desc": "Number of star in cluster in Simbad "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[MTU] Source of postiion "}, {"name": "UCAC2", "desc": "? Number in UCAC2 (Cat. I/289) "}, {"name": "CD", "desc": "Cordoba Durchmusterung identification "}, {"name": "m_CD", "desc": "[ab] "}, {"name": "CPD", "desc": "Cape Photographic Durchmusterung identification "}, {"name": "HD", "desc": "? Henry Draper Catalog identification "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "B-V", "desc": "Johnson (B-V) color index "}, {"name": "U-B", "desc": "? Johnson (U-B) color index "}, {"name": "Sp", "desc": "Spectral class (no luminosity class) "}, {"name": "Rem", "desc": "Remarks by B. Skiff "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_41_43"}} {"id": "J/A+AS/41/43", "title_cds": "Color excesses in 5 regions of Milky Way", "title_create": "Johansson, 1980", "year": "1980", "author": "Johansson K.L.V.", "title_pub": "Colour excess and stellar distribution in five selected directions of the Milky Way in Carina, Crux, Centaurus and Norma.", "first_author": "Johansson K.L.V.", "ref_biblio": [""], "bibcode": ["1980A&AS...41...43J"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_43_103"}} {"id": "J/A+AS/43/103", "title_cds": "OB stars found in a Perseus arm field", "title_create": "Wramdemark+, 1981", "year": "1981", "author": "Wramdemark S.", "title_pub": "A study of early-type stars in a Perseus arm area", "first_author": "Wramdemark S.", "ref_biblio": [""], "bibcode": ["1981A&AS...43..103W"], "keyword_cds": "Stars, early-type ; Photometry, UBV", "keyword_pub": "OB stars ; UBV{beta} photometry ; HII retgions ; galactic structure", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "22-Mar-2016"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_44_155"}} {"id": "J/A+AS/44/155", "title_cds": "Loden 28 and 915 photometry", "title_create": "Loden+, 1981", "year": "1981", "author": "Loden L.O.", "title_pub": "A photometric study of two stellar clusterings in the southern Milky Way (and a general consideration on previous and present data concerning galactic clusterings).", "first_author": "Loden L.O.", "ref_biblio": [""], "bibcode": ["1981A&AS...44..155L"], "see_also": ["J/A+AS/41/173 :"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["The paper analyzes photometrically obtained data on approximately 100", "stars and two suspected stellar clusterings in the Southern Milky Way,", "using objective-prism spectral classification methods. The", "observations, carried out with the 50cm ESO telescope, achieved", "estimated accuracy in the photometric parameters of: V:0.023,", "B-V:0.011, U-B:0.022. Strong evidence for the presence of a pronounced", "concentration of A-F (partly evolved) stars was found. One of the", "stellar clusterings found (in Carina) reveals an ordinary B", "association with an estimated 3 million years, while the second (in", "Centaurus), a very loose open cluster, is of intermediate age,", "approximately 100 million years. Conclusively it is stated that,", "wherever in the Milky Way an apparent densification of stars of a", "certain spectral type is found, there is also an enhanced probability", "of detecting a physical clustering of some kind. Moreover, it may be", "difficult to find any line of sight through the Milky Way that does", "not pass through one or more star clusterings within the nearest", "1-2kpc."], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_46_347"}} {"id": "J/A+AS/46/347", "title_cds": "BV photometry of M15 central part", "title_create": "Auriere+, 1981", "year": "1981", "author": "Auriere M., Cordoni J.-P.", "title_pub": "Position, magnitudes and color for stars of the central part of the X-ray globular cluster M 15.", "first_author": "Auriere M.", "ref_biblio": [""], "bibcode": ["1981A&AS...46..347A"], "see_also": ["J/A+AS/119/307 : Position in M15 (Le Campion+, 1996)", "J/AJ/113/1026 : Fabry-Perot Observations of M15 (Gebhardt+ 1997)", "J/AJ/124/3255 : UBV photometry in M15 (van der Marel+, 2002)"], "keyword_cds": "Clusters, globular ; X-ray sources ; Photometry, photographic", "keyword_pub": "globular cluster - X-ray source - stellar photometry", "abstract": ["Position, magnitudes and color for 734 stars in a 1'x1' square field", "centered on the X-ray globular cluster M 15 are given. The", "observations consist of long focus (about 35m) high spatial resolution", "(FWHM down to 0.55arcsec) unfiltered image tube B and V classical", "photographs of the central part of the cluster obtained with two", "specially designed cameras at the 1 meter telescope of Pic du Midi", "Observatory. The reduction procedure is a compromise between automatic", "and interactive techniques. Errors in the data relative to photometry", "as well as astrometry are discussed."], "type": ["OC"], "data": "", "date_update": "06-Jun-2006", "tables": [{"name": "position.dat", "desc": "Star positions (from Simbad) ", "columns": [{"name": "Seq", "desc": "Sequential number "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "SName", "desc": "Simbad name "}]}, {"name": "table2.dat", "desc": "Position, magnitudes and color ", "columns": [{"name": "Seq", "desc": "Sequential number, Cl* NGC 7078 AC NNN in Simbad "}, {"name": "Xpos", "desc": "X position (1) "}, {"name": "Ypos", "desc": "Y position (1) "}, {"name": "R", "desc": "Distance from star No 216 (1) "}, {"name": "Bmag", "desc": "B magnitude "}, {"name": "n_Bmag", "desc": "[)] uncertainty flag on Bmag "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "n_Vmag", "desc": "[)] uncertainty flag on Vmag "}, {"name": "B-V", "desc": "? B-V colour index "}, {"name": "ONames", "desc": "Other names (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_53_255"}} {"id": "J/A+AS/53/255", "title_cds": "Catalog of late-type supergiants in SMC", "title_create": "Prevot+, 1983", "year": "1983", "author": "Prevot L., Martin N., Maurice E., Rebeirot E., Rousseau J.", "title_pub": "A catalogue of late-type supergiant stars in the Small Magellanic Cloud.", "first_author": "Prevot L.", "ref_biblio": [""], "bibcode": ["1983A&AS...53..255P"], "keyword_cds": "", "keyword_pub": "", "abstract": ["An objective-prism survey of the Small Magellanic Cloud has been made", "on IIIaJ plates taken with the 1 m ESO Schmidt telescope and has", "resulted in the detection of nearly 200 late K and M supergiant stars.", "Most of these are new probable members of the SMC which do not appear", "in previous catalogues. The mean visual absolute magnitude of -6.0", "agrees with the visual absolute magnitude of lab-lb galactic", "supergiants of spectral types M0 to M4. The fraction of known variable", "stars found in this catalogue is barely 10 percent; this is 2.5 times", "less than the value found for the corresponding stars in the LMC. The", "catalogue provides accurate 1975 coordinates, finding charts, spectral", "types, V magnitudes, indications concerning radial velocities when", "available and designations of the stars in other catalogues."], "description": ["accurate coordinates for the PMMR red stars in and around the SMC. I", "used the published finder charts to identify the stars. The format of", "the file is the same as for 'mktypes.dat' ---> B/mk. The improved", "coordinates allow the stars to be linked with the similar list by", "Sanduleak (acronym SkKM)."], "curator": "Francois Ochsenbein [CDS]", "alias": ["PMMR"], "type": ["OC"], "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_9_163"}} {"id": "J/A+AS/9/163", "title_cds": "UBV photometry in four areas", "title_create": "Ardeberg+, 1973", "year": "1973", "author": "Ardeberg A., Sarg K., Wramdemark S.", "title_pub": "Photoelectric UBV photometry in four areas of intermediate-high galactic latitude.", "first_author": "Ardeberg A.", "ref_biblio": [""], "bibcode": ["1973A&AS....9..163A"], "keyword_cds": "", "keyword_pub": "UBV photometry ; high latitudes ; galactic structure ; interstellar absorption", "description": ["The table contains photoelectric UBV photometry for a total of 127 stars", "situated in 4 fields with 55"], "bibcode": ["1973A&AS....9..183W"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["UHA"], "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_94_245"}} {"id": "J/A+AS/94/245", "title_cds": "Morphologies of ring-shaped galaxies", "title_create": "Faundez-abans+, 1992", "year": "1992", "author": "Faundez-abans M., Hertling G., Ramirez A.C.", "title_pub": "The visual appearance of the nuclei of ring-shaped galaxies as an alternative classification criterion.", "first_author": "Faundez-abans M.", "ref_biblio": [""], "bibcode": ["1992A&AS...94..245F"], "see_also": ["J/A+AS/104/1 : Faint ring-shaped galaxies near South Pole (Faundez-Abans+ 1994", "J/ApJS/96/39 : Catalog of Southern Ringed Galaxies (Buta+, 1995)", "J/A+AS/129/357 : Morphology of peculiar ring galaxies (Faundez-Abans+ 1998)", "J/ApJS/181/572 : Collisional ring galaxies atlas (Madore+, 2009)"], "keyword_cds": "Galaxy catalogues ; Morphology", "keyword_pub": "galaxies: general ; galaxies, nuclei of ; galaxies: structure of", "abstract": ["An alternative classification of apparent ring galaxies is introduced", "concerning the morphology of the main body (nucleus). For this", "purpose, a list of probable ring galaxies has been prepared based on", "visual inspection of 58 film copies of the J-band SRC/ESO survey. The", "candidate objects have also been classified following Few and Madore's", "(1986MNRAS.222..673F) criteria."], "data": "", "date_update": "07-Dec-2013", "tables": [{"name": "table1.dat", "desc": "List of ring-shpoaed galaxies ", "columns": [{"name": "---", "desc": "[HRG] "}, {"name": "HRG", "desc": "our own designation "}, {"name": "Name", "desc": "Other identifier (ESO or other) "}, {"name": "RAh", "desc": "Right Ascension B1950 (hours) "}, {"name": "RAm", "desc": "Right Ascension B1950 (minutes) "}, {"name": "RAs", "desc": "Right Ascension B1950 (seconds) "}, {"name": "DE-", "desc": "Declination B1950 (sign) "}, {"name": "DEd", "desc": "Declination B1950 (degrees) "}, {"name": "DEm", "desc": "Declination B1950 (minutes) "}, {"name": "DEs", "desc": "Declination B1950 (seconds) "}, {"name": "RAJ.h", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAJ.m", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAJ.s", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DEJ.-", "desc": "Declination J2000 (sign) "}, {"name": "DEJ.d", "desc": "Declination J2000 (degrees) "}, {"name": "DEJ.m", "desc": "Declination J2000 (minutes) "}, {"name": "DEJ.s", "desc": "Declination J2000 (seconds) "}, {"name": "HuCl", "desc": "the estimated Hubble class from the ESO/Uppsala survey, "}, {"name": "Rt", "desc": "[OP? ] the FM ring galaxies classification, "}, {"name": "NuCl", "desc": "the estimated diffuse stellar component classification, "}, {"name": "Comments", "desc": "Comments and remarks "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_A+AS_99_1"}} {"id": "J/A+AS/99/1", "title_cds": "UBV study of open cluster NGC 5460", "title_create": "Claria+, 1993", "year": "1993", "author": "Claria J.J., Lapasset E., Bosio M.A.", "title_pub": "Further observations of stars in the open cluster NGC 5460.", "first_author": "Claria J.J.", "ref_biblio": [""], "bibcode": ["1993A&AS...99....1C"], "keyword_cds": "Photometry, UBV ; Clusters, open", "keyword_pub": "Clusters, open - Photometry, UBV, DDO, CMT1T2", "abstract": ["New photoelectric UBV photometry in the open cluster NGC 5460 is", "presented for 155 stars brighter than 14.0 mag. In addition, six", "comparatively bright red stars in the cluster field were observed in", "the DDO and Washington systems. Nearly 40 percent of the observed", "stars are found to be members or probable members. The analysis of the", "new data yields E(B-V)=0.12+/-0.03 and V(0)-M(v)=9.34+/-0.20", "(740+/-68 pc) for the cluster reddening and true distance modulus,", "respectively. An age of 1.1 x 10 exp 8 yr was derived, which places", "this cluster within the NGC 2516 age group. NGC 5460 does not probably", "contain any red giant."], "data": "", "date_update": "08-Dec-2013", "tables": [{"name": "n5460.dat", "desc": "Photometric magnitudes in the region of NGC 1904 ", "columns": [{"name": "---", "desc": "[Cl* NGC 5460 CLB] "}, {"name": "Seq", "desc": "[1/155] Star sequence number "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[UTM] Source of position "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "B-V", "desc": "Johnson B-V magnitude "}, {"name": "U-B", "desc": "? Johnson U-B magnitude "}, {"name": "Comments", "desc": "Additional comments, from B. Skiff. "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_100_569"}} {"id": "J/AJ/100/569", "title_cds": "S stars in the Northern Milky Way", "title_create": "Stephenson+, 1990", "year": "1990", "author": "Stephenson C.B.", "title_pub": "New and relatively faint S stars found in the Northern Milky Way.", "first_author": "Stephenson C.B.", "ref_biblio": [""], "bibcode": ["1990AJ....100..569S"], "keyword_cds": "Stars, S", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["CSS2"], "type": ["OC"], "doi_pub": ["10.1086/115540"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_103_263"}} {"id": "J/AJ/103/263", "title_cds": "Stephenson's highly reddened stars", "title_create": "Stephenson+, 1992", "year": "1992", "author": "Stephenson C.B.", "title_pub": "A list of highly reddened stars likely to be distant luminous stars.", "first_author": "Stephenson C.B.", "ref_biblio": [""], "bibcode": ["1992AJ....103..263S"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/116059"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_104_495"}} {"id": "J/AJ/104/495", "title_cds": "Galaxy redshifts", "title_create": "Malumuth+, 1992", "year": "1992", "author": "Malumuth E.M., Kriss G.A., Dixon W.V., Ferguson H.C., Ritchie C.", "title_pub": "Dynamics of clusters of galaxies with central dominant galaxies. I. Galaxy redshifts.", "first_author": "Malumuth E.M.", "ref_biblio": [""], "bibcode": ["1992AJ....104..495M"], "keyword_cds": "Galaxies, optical ; Redshifts", "abstract": ["Optical redshifts are presented for a sample of 638 galaxies in the", "fields of the clusters Abell 85, DC 0107-46, Abell 496, Abell 2052,", "and DC 1842-63. The velocity histograms and wedge diagrams show", "evidence for a foreground sheet of galaxies in Abell 85 and background", "sheets of galaxies in DC 0107-46 and Abell 2052. The foreground group", "projected against the center of Abell 85 found by Beers et al.", "(1991AJ....102.1581B) is confirmed. No evidence of substructure was", "found in Abell 496, Abell 2052, and DC 1842-63. The clusters have", "global velocity dispersions ranging from 551 km/s for DC 1842-63 to", "714km/s for A496, and flat dispersion profiles. Mass estimates using", "the virial theorem and the projected mass method range from 2.3x10^14^", "solar masses for DC 0107-46 to 1.1x10^15^ solar masses for A85."], "doi_pub": ["10.1086/116250"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table7.dat", "desc": "Galaxy redshifts in DC 1842-63 ", "columns": [{"name": "[MKD92]", "desc": "[1/154]+ Sequential number, [MKD92] DRCG 1842-63 NNN in Simbad"}, {"name": "n_[MKD92]", "desc": "[*] * for D or cD galaxy "}, {"name": "[D80]", "desc": "? Dressler (1980, Cat. ) number ([D80] DRCG 1842-63 NNN)"}, {"name": "[BW89]", "desc": "Bell & Whitemore (1989ApJS...70..139B) number "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "RAs", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "DEs", "desc": "Declination (1950) "}, {"name": "cz", "desc": "Heliocentric velocity "}, {"name": "e_cz", "desc": "rms uncertainty on cz "}, {"name": "r_cz", "desc": "Sources of the redshift (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_105_1206"}} {"id": "J/AJ/105/1206", "title_cds": "Exposure guide for large format CCDs", "title_create": "Tyson+, 1993", "year": "1993", "author": "TYSON N.D., GAL R.R.", "title_pub": "An exposure guide for taking twilight flatfields with large format CCDs", "first_author": "TYSON N.D.", "ref_biblio": [""], "bibcode": ["1993AJ....105.1206T"], "abstract": ["Driven by the long readout times of today's large format CCDs, we", "present an efficient method to compute an ideal sequence of exposure", "times for twilight skyflats. The procedure will allow the observer to", "maximize the number of flats that can be obtained in the rapidly", "changing surface brightness of the dusk or dawn sky."], "curator": "Patricia Bauer [CDS]", "doi_pub": ["10.1086/116505"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_106_964"}} {"id": "J/AJ/106/964", "title_cds": "BVRI photometry of NGC 185 stellar population", "title_create": "Lee+, 1993", "year": "1993", "author": "Lee M.G., Freedman W.L., Madore B.F.", "title_pub": "Stellar populations in the dwarf elliptical galaxy NGC 185.", "first_author": "Lee M.G.", "ref_biblio": [""], "bibcode": ["1993AJ....106..964L"], "keyword_cds": "Galaxies, photometry ; Photometry, UBVRI ; Photometry, CCD", "abstract": ["BVRI CCD photometry of ~5300 stars in the central (2'2x3'5) area of", "the dwarf elliptical galaxy NGC 185 in the Local Group is presented.", "The color-magnitude diagrams of NGC 185 show three distinct stellar", "populations: (1) a strong red giant branch (RGB) population, the tip", "of which is found to be at I_TRGB_=20.3+/-0.2mag, and", "(V-I)_TRGB_=1.95+/-0.05, (2) an asymptotic giant branch (AGB) located", "above the tip of the RGB, and (3) a small number of young stars having", "blue to yellow colors. The reddening of the bright foreground stars", "has been determined using the (B-V)-(V-I) diagram to be", "E(B-V)=0.19+/-0.03 mag. The distance has been estimated from the I", "magnitude of the tip of the RGB, giving (m-M)_0_=23.96+/-0.21mag for", "A_I_=0.38mag, corresponding to 620+/-60kpc. The mean metallicity of", "the RGB stars has been determined using the median color of the RGB", "stars at M_I_=-3.5mag, (V-I)_-3.5,0_=1.727mag: giving a mean", "metallicity of [Fe/H]=-1.23+/-0.16dex. The dispersion in color at", "M_I_=-3.5mag is {delta}(V-I)_-3.5_=0.12mag, implying a metallicity", "dispersion of -1.6<[Fe/H]<-0.9dex. Surface photometry of the area", "within R=50\" is also presented, showing that colors get rapidly bluer", "inside R~10\". A V luminosity function for the blue stars has been", "derived, the slope of which is very similar to that for other nearby", "galaxies. The AGB stars extend to M_bol_~-5.0mag, and Most of the AGB", "stars above the tip of the RGB are likely to belong to an", "intermediate-age population. The bolometric luminosity function of the", "red giant stars in NGC 185 is found to be very similar to that of M32."], "object": ["00 39 01.5 +48 20 27 NGC 185"], "doi_pub": ["10.1086/116697"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table3a.dat", "desc": "BVRI CCD photometry of stars in NGC 185. ", "columns": [{"name": "[LFM93a]", "desc": "Star number ([LFM93a] NNNN in Simbad) "}, {"name": "Xpos", "desc": "X position (1) "}, {"name": "Ypos", "desc": "Y position (1) "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "V-R", "desc": "? V-R colour index "}, {"name": "V-I", "desc": "? V-I colour index "}, {"name": "Imag", "desc": "? I magnitude "}]}, {"name": "table3b.dat", "desc": "Blue stars [(B-V)<0.6] in NGC 185. ", "columns": [{"name": "[LFM93a]", "desc": "Star number ([LFM93a] NNNN in Simbad) "}, {"name": "Xpos", "desc": "X position (1) "}, {"name": "Ypos", "desc": "Y position (1) "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "V-R", "desc": "? V-R colour index "}, {"name": "V-I", "desc": "? V-I colour index "}, {"name": "Imag", "desc": "? I magnitude "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_107_2184"}} {"id": "J/AJ/107/2184", "title_cds": "FK giants and supergiants photometry", "title_create": "Eggen 1994", "year": "1994", "author": "Eggen O.J.", "title_pub": "Photometry of F-K type bright giants and supergiants. III. The luminosity, reddening, and heavy element abundance of GK stars.", "first_author": "Eggen O.J.", "ref_biblio": [""], "bibcode": ["1994AJ....107.2184E"], "see_also": ["VIII/4 : Fourth Cambridge Survey (4C) (Pilkington+ 1965; Gower+1967)"], "keyword_cds": "Stars, giant ; Stars, supergiant ; Photometry ; Abundances, [Fe/H] ; Reddening ; Radial velocities", "abstract": ["The reddening, luminosity, and heavy element abundance of 250 bright", "giants and supergiants of type GK are discussed on the basis of", "4 color, DDO, RI, and Geneva photometry. Bright giants of type GK with", "age greater than 5x10^8^yr, and of type G0/3 with age greater than", "2x10^8^yr, are very scarce in the solar neighborhood. The median space", "motion vectors of the bright giants and supergiants with well", "determined space motions are", "(U, V, W)=(+10.6, -13.2, -7.7)+/-(12.3, 8.8, 8.8)km/s. The M_1 index", "for 4 color photometry, when corrected for luminosity (gravity)", "effects, is sensitive to heavy element abundance in the F type stars", "but not in those of GK type. The CN index reflects the heavy element", "abundance of the GK stars but may not be reliable for those of type", "G0/3. The available spectroscopic determinations of [Fe/H] give mixed", "results with the two largest samples (McWilliam, 1990ApJS...74.1075M;", "Brown et al, 1989ApJS...71..293B) being internally consistent but with", "a large zero-point difference. There is a similar zero-point shift in", "the peak frequency of the photometrically determined values of P[Fe/H]", "for the F type and for the GK type stars. There is little evidence for", "an appreciable galactic, radial gradient in the P[Fe/H] values. A", "previously noted correlation of the heavy element abundance index,", "{DELTA}M_1_, with the amplitude defect in the B light curves of", "Cepheids, F_B_, and interpretation of the (PLF_B_) relation as a", "(PL[Fe/H]) relation needs further investigation in light of the", "apparent sensitivity of M_1_ to Fe/H for the F stars (the domain of", "the Cepheids with P<10d) and lack of this sensitivity for the G0/3", "star (domain of the Cepheids with P>10d)."], "doi_pub": ["10.1086/117030"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table1.dat", "desc": "(R-I) photometry ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "m_HD", "desc": "Multiplicity index on HD "}, {"name": "Name", "desc": "Other name "}, {"name": "Rmag", "desc": "? R magnitude "}, {"name": "n_Rmag", "desc": "[V] "}, {"name": "R-I", "desc": "R-I colour index "}, {"name": "u_R-I", "desc": "Uncertainty flag on R-I "}, {"name": "DR-I", "desc": "? Mean deviation of a single observation from the mean value"}, {"name": "Nobs", "desc": "Number of observations "}]}, {"name": "table2.dat", "desc": "Previously unpublished DDO photometry (McClure, 1976AJ.....81..182M)", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "m_HD", "desc": "Multiplicity index on HD "}, {"name": "Name", "desc": "Other name "}, {"name": "m48", "desc": "m49 magnitude "}, {"name": "u_m48", "desc": "Uncertainty flag on m48 "}, {"name": "(45-48)", "desc": "45-48 colour index "}, {"name": "u_(45-48)", "desc": "Uncertainty flag on (45-48) "}, {"name": "(42-45)", "desc": "42-45 colour index "}, {"name": "u_(42-45)", "desc": "Uncertainty flag on (42-45) "}, {"name": "(41-42)", "desc": "? 41-42 colour index (1) "}, {"name": "u_(41-42)", "desc": "Uncertainty flag on (41-42) "}, {"name": "D(45-48)", "desc": "? Mean deviation of a single observation from the mean (45-48) value"}, {"name": "D(42-45)", "desc": "? Mean deviation of a single observation from the mean (42-45) value"}, {"name": "D(41-42)", "desc": "? Mean deviation of a single observation from the mean (41-42) value"}, {"name": "Nobs", "desc": "Number of observations "}]}, {"name": "table5.dat", "desc": "Photometry of early type stars in NGC 3114 (Schmidt, 1982PASP...94..232S)", "columns": [{"name": "NGC3114", "desc": "NGC 3114 NNN star number "}, {"name": "E(b-y)", "desc": "? (b-y) colour excess (1) "}, {"name": "[u-b]", "desc": "Colour index [u-b] "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "n_VMAG", "desc": "[)] Uncertainty flag on VMAG "}, {"name": "MOD", "desc": "? MOD magnitude (1) "}, {"name": "SpType", "desc": "Spectral type "}]}, {"name": "table6.dat", "desc": "Reddening, luminosity, and space motion of bright giants and supergiants near the Sun", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "n_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Cm0", "desc": "? Dereddened Cm colour index "}, {"name": "d(45-48)0", "desc": "? Dereddened (45-48) colour index "}, {"name": "d[u-b]", "desc": "? d[u-b] colour index (=[u-b]-3.80(R-I)_0_-0.240)"}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "? DDO absolute V magnitude "}, {"name": "VMAG4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "pmRA", "desc": "Proper motion in right ascension "}, {"name": "pmDE", "desc": "Proper motion in declination "}, {"name": "n_pmRA", "desc": "[)] Uncertainty flag on proper motions "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "n_RV", "desc": "[:V] "}, {"name": "Uvel", "desc": "U velocity "}, {"name": "u_Uvel", "desc": "Uncertainty flag on Uvel "}, {"name": "Vvel", "desc": "V velocity "}, {"name": "u_Vvel", "desc": "Uncertainty flag on Vvel "}, {"name": "Wvel", "desc": "W velocity "}, {"name": "u_Wvel", "desc": "Uncertainty flag on Wvel "}, {"name": "n_Uvel", "desc": "[)] Uncertainty flag on U, V, W velocities "}, {"name": "HR", "desc": "? HR (Cat. ) number "}, {"name": "SpTypeC", "desc": "Combined spectral type "}, {"name": "SpTypeO", "desc": "Observed spectral type "}, {"name": "Note", "desc": "[X] X: note in note6.dat file "}]}, {"name": "note6.dat", "desc": "Individual notes to table6.dat ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "Note", "desc": "Note "}]}, {"name": "table7.dat", "desc": "Metallicity parameters for the stars in table 5 ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "M10O", "desc": "? Observed (M_1_)_0_ metallicity index "}, {"name": "M10C", "desc": "? Computed (M_1)_0_ metallicity index (1) "}, {"name": "M10O-C", "desc": "? Observed minus computed (M_1)_0_ values (2) "}, {"name": "n_M10O-C", "desc": "[)] Uncertainty flag on M10O-C "}, {"name": "m2O", "desc": "? Observed m_2_ metallicity index "}, {"name": "m2C", "desc": "? Computed m_2_ metallicity index "}, {"name": "m2O-C", "desc": "? Observed minus computed m_2_ values (2) "}, {"name": "n_m2O-C", "desc": "[)] Uncertainty flag on m2O-C "}, {"name": "DCN", "desc": "? {DELTA}CN metallicity index (3) "}, {"name": "P[Fe/H]", "desc": "? P[Fe/H] from DCN (P[Fe/H]=5DCN-0.12) "}, {"name": "n_P[Fe/H]", "desc": "[)] Uncertainty flag on P[Fe/H] "}, {"name": "X", "desc": "Radial distance from the Sun, positive in the direction away from the galactic center"}]}, {"name": "table8.dat", "desc": "Bright giants and supergiants observed spectroscopically by McWilliams (1990ApJS...74.1075M) and Luck and Bond (1989ApJS...71..559L)", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "DCN", "desc": "{DELTA}CN metallicity index "}, {"name": "P[Fe/H]", "desc": "P[Fe/H] index "}, {"name": "D[Fe/H]", "desc": "P[Fe/H] minus [Fe/H] difference (1) "}, {"name": "n_D[Fe/H]", "desc": "[)] Uncertainty flag on D[Fe/H] "}, {"name": "TeffO", "desc": "Observed effective temperature "}, {"name": "TeffC", "desc": "Combined effective temperature "}, {"name": "TeffO-C", "desc": "TeffO minus TeffC difference "}, {"name": "r_TeffO", "desc": "[ML] Origin of TeffO value (2) "}]}, {"name": "table9.dat", "desc": "F type supergiants common to Luck & Bond (1989ApJS...71..559L) and the Geneva Photometry Catalogue (Rufener 1988, Cat. )", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "m2", "desc": "m_2_ index "}, {"name": "Del", "desc": "Del index "}, {"name": "beta", "desc": "{beta} index "}, {"name": "dDel", "desc": "{delta}Del index (=Del-3.20{beta}+8.130) "}, {"name": "dm2", "desc": "{delta}m_2_ index "}, {"name": "dm2Corr", "desc": "{delta}m_2_ index corrected for gravity effects (={delta}m_2_+0.150{delta}Del+0.125)"}, {"name": "Fe/H", "desc": "Fe/H value "}]}, {"name": "table10.dat", "desc": "Stars common to Paper II (1991AJ....102.1826E) and the Geneva Photometry Catalogue ()", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "m2", "desc": "m_2_ index "}, {"name": "Del", "desc": "Del index (=3.20{beta}-8.130) "}, {"name": "beta", "desc": "{beta} index "}, {"name": "dDel", "desc": "{delta}Del (=Del-3.20{beta}+8.130) index "}, {"name": "dm2", "desc": "{delta}m_2_ index "}, {"name": "dm2Corr", "desc": "{delta}m_2_ index corrected for gravity effects (={delta}_m_2_+0.150{delta}Del+0.125)"}, {"name": "P[Fe/H]m2", "desc": "P[Fe/H] index derived from m_2_ index "}, {"name": "P[Fe/H]M1", "desc": "P[Fe/H] index derived from M_1_ index (1) "}, {"name": "DP[Fe/H]", "desc": "P[Fe/H]m2 - P[Fe/H]M1 value (2) "}, {"name": "n_DP[Fe/H]", "desc": "[)] Uncertainty flag on DP[Fe/H] "}]}, {"name": "table11.dat", "desc": "Metallicities of bright giants and supergiants stars by Brown et al. (1989ApJS...71..293B)", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "DCN", "desc": "{DELTA}CN index "}, {"name": "TeffO", "desc": "Observed effective temperature "}, {"name": "u_TeffO", "desc": "Uncertainty flag on TeffO "}, {"name": "TeffC", "desc": "Computed effective temperature (1) "}, {"name": "TeffC_O", "desc": "Computed minus observed effective temperature "}]}, {"name": "table12.dat", "desc": "Faint SG and BG of GK type ", "columns": [{"name": "Hd", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "n_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "(R-I)0", "desc": "Dereddened (R-I) colour index "}, {"name": "Cm0", "desc": "? Dereddened C_m index "}, {"name": "d(45-48)0", "desc": "? Dereddened {delta}(54-48) index "}, {"name": "D[u-b]", "desc": "{DELTA}[u-b] index "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "? DDO absolute V magnitude "}, {"name": "VMAG4C", "desc": "4C (Cat. ) absolute V magnitude "}, {"name": "M10O", "desc": "Observed dereddened M_1_ index "}, {"name": "M10C", "desc": "Computed dereddened M_1_ index "}, {"name": "n_M10C", "desc": "[)] Uncertainty flag on M10C "}, {"name": "DCN", "desc": "? {DELTA}CN index "}, {"name": "n_DCN", "desc": "[)] Uncertainty flag on DCN "}, {"name": "P[Fe/H]", "desc": "? P[Fe/H] index from DCN (1) "}, {"name": "n_P[Fe/H]", "desc": "[)] Uncertainty flag on [Fe/H] "}, {"name": "SpTypeC", "desc": "Computed spectral type "}, {"name": "SpTypeO", "desc": "Observed spectral type "}, {"name": "r_SpTypeO", "desc": "? Reference for SpTypeO (2) "}, {"name": "X", "desc": "Radial distance from the Sun, positive in the direction away from the galactic center"}, {"name": "Note", "desc": "[X] X: individual note (3) "}]}, {"name": "table13.dat", "desc": "R type SG near NGC 2414 and NGC 2437 ", "columns": [{"name": "Star", "desc": "Star name "}, {"name": "Vmag", "desc": "V magnitude (1) "}, {"name": "b-y", "desc": "b-y colour index "}, {"name": "M1", "desc": "M_1_ colour index "}, {"name": "C1", "desc": "C_1_ colour index "}, {"name": "Rmag", "desc": "? R magnitude "}, {"name": "R-I", "desc": "R-I colour index (2) "}, {"name": "DM1", "desc": "Mean deviation of a single observation from the mean M_1_ value"}, {"name": "DC1", "desc": "Mean deviation of a single observation from the mean C_1_ value"}, {"name": "DRmag", "desc": "Mean deviation of a single observation from the mean Rmag value"}, {"name": "DR-I", "desc": "Mean deviation of a single observation from the mean R-I value"}, {"name": "Nobs", "desc": "Number of observations "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "D[u-b]", "desc": "? {delta}[u-b] colour index "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "beta", "desc": "{beta} index "}, {"name": "SpTypeC", "desc": "Computed spectral type "}, {"name": "Note", "desc": "[X] X: individual note (3) "}]}, {"name": "table14.dat", "desc": "*Stars classified as supergiants or bright giants but with photometric indices of normal galaxies", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "n_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "(R-I)0", "desc": "? Dereddened R-I colour index "}, {"name": "Cm0", "desc": "? Dereddened C_m_ index (1) "}, {"name": "D(45-48)0", "desc": "? Dereddened {Delta}(45-48) index (2) "}, {"name": "[C1]", "desc": "? [C_1_] index "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "MVDDO", "desc": "DDO absolute V magnitude "}, {"name": "MV4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "n_MV4C", "desc": "[)o] ): uncertainty flag; o: optical "}, {"name": "D(M1)0", "desc": "? Dereddened {Delta}M_1_ index "}, {"name": "n_D(M1)0", "desc": "[)] Uncertainty flag on D(M1)0 "}, {"name": "DCN", "desc": "? {Delta}CN index "}, {"name": "P[Fe/H]4C", "desc": "? P[Fe/H] index from 4C (Cat. ) "}, {"name": "n_P[Fe/H]4C", "desc": "[)] Uncertainty flag on P[Fe/H]4C "}, {"name": "P[Fe/H]DDO", "desc": "? P[Fe/H] index from DDO (=3.12DCN+0.031) "}, {"name": "SpTypeC", "desc": "Computed spectral type "}, {"name": "SpTypeO", "desc": "Observed spectral type "}, {"name": "r_SpTypeO", "desc": "? Source of spectral type (3) "}, {"name": "Note", "desc": "[XA] Individual notes (4) "}]}, {"name": "table15.dat", "desc": "Problem stars ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "n_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Cm0", "desc": "Dereddened C_m_ colour index "}, {"name": "d(45-48)0", "desc": "Dereddened {delta}(45-48) colour index "}, {"name": "n_d(45-48)0", "desc": "[)] Uncertainty flag on d(45-48)0 "}, {"name": "D[u-b]", "desc": "? {Delta}[u-y] index "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "? DDO absolute V magnitude "}, {"name": "n_VMAGDDO", "desc": "[)] Uncertainty flag on VMAGDDO "}, {"name": "VMAG4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "n_VMAG4C", "desc": "[)] Uncertainty flag on VMAG4C "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "SpTypeC", "desc": "Computed spectral type "}, {"name": "SpTypeO", "desc": "Observed spectral type "}, {"name": "Note", "desc": "[XA] Individual notes (1) "}]}, {"name": "note15.dat", "desc": "Individual notes to table15.dat ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "table16.dat", "desc": "G0/3 I stars ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E[b-y]", "desc": "! [b-y] colour excess "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Cm0", "desc": "Dereddened C_m_ index "}, {"name": "d(45-48)0", "desc": "Dereddened {delta}(45-48) index "}, {"name": "D[u-b]", "desc": "? {Delta}[u-b] index "}, {"name": "n_D[u-b]", "desc": "[)] Uncertainty flag on D[u-b] "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "DDO absolute V magnitude "}, {"name": "VMAG4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "n_VMAG4C", "desc": "[)] Uncertainty flag on VMAG4C "}, {"name": "DCN", "desc": "{Delta}CN index "}, {"name": "n_DCN", "desc": "[)] Uncertainty flag on DCN "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "References for SpType (1) "}, {"name": "Note", "desc": "[X] Individual notes (2) "}]}, {"name": "table17.dat", "desc": "Stars in table 16 with Geneva photometry ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "m2O", "desc": "Observed m_2_ index (=[B1-B2]-0.457[B2-VI]) "}, {"name": "DelO", "desc": "Observed Del index (=[U-B2]-0.832[B2-G]) "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Dm2", "desc": "{Delta}m_2_ index (=m_2_-1.95(R-I)_0_+0.695) "}, {"name": "DDel", "desc": "{Delta}Del index (=Del-1.60(R-I)_0_+0.695) "}, {"name": "m2C", "desc": "Computed m_2_ index "}, {"name": "m2O-C", "desc": "Observed minus computed m_2_ index (1) "}, {"name": "n_m2O-C", "desc": "[)] Uncertainty flag on m2O-C "}]}, {"name": "table18.dat", "desc": "G0/3 II stars ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Cm0", "desc": "Dereddened C_m_ colour index "}, {"name": "d(45-48)0", "desc": "Dereddened {delta}(45-48) colour index "}, {"name": "d[u-b]", "desc": "? {delta}[u-y] index (=[u-b]-3.80(R-I)_0_-0.240) "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "? DDO absolute V magnitude "}, {"name": "VMAG4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "DCN", "desc": "{Delta}CN index "}, {"name": "n_DCN", "desc": "[)] Uncertainty flag on DCN "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "References to spectral type (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_108_1843"}} {"id": "J/AJ/108/1843", "title_cds": "Serendipitous EUV sources", "title_create": "McDonald+, 1994", "year": "1994", "author": "McDonald K., Craig N., Sirk M.M., Drake J.J., Fruscione A., Vallerga J.V., Malina R.F.", "title_pub": "Serendipitous EUV sources detected during the first year of the Extreme Ultraviolet Explorer right angle program.", "first_author": "McDonald K.", "ref_biblio": [""], "bibcode": ["1994AJ....108.1843M"], "keyword_cds": "Ultraviolet ; Cross identifications", "abstract": ["We report the detection of 114 extreme ultraviolet (EUV; 58-740{AA})", "sources, of which 99 are new serendipitous sources, based on", "observations made with the imaging telescopes on board the Extreme", "Ultraviolet Explorer (EUVE) during the Right Angle Program (RAP).", "These data were obtained using the survey scanners and the Deep Survey", "instrument during the first year of the spectroscopic guest observer", "phase of the mission, from January 1993 to January 1994. The data set", "consists of 162 discrete pointings whose exposure times are typically", "two orders of magnitude longer than the average exposure times during", "the EUVE all-sky survey. Based on these results, we can expect that", "EUVE will serendipitously detect approximately 100 new EUV sources per", "year, or about one new EUV source per 10 sq deg, during the guest", "observer phase of the EUVE mission. New EUV sources of note include", "one B star and three extragalactic objects. The B star (HR 2875, EUVE", "J0729-38.7) is detected in both the Lexan/B (~100{AA}) and Al/Ti/C", "(~200{AA}) bandpasses, and the detection is shown not to be a result", "of UV leaks. We suggest that we are detecting EUV and/or soft x rays", "from a companion to the B star. Three sources, EUVE J2132+10.1, EUVE", "J2343-14.9, and EUVE J2359-30.6 are identified as the active galactic", "nuclei MKN 1513, MS2340.9-1511, and 1H2354-315, respectively."], "doi_pub": ["10.1086/117197"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table2.dat", "desc": "EUVE right angle program source list ", "columns": [{"name": "EUVE", "desc": "EUVE name "}, {"name": "n_EUVE", "desc": "[+ b] Note on Name (1) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "Lex", "desc": "? Lexan/B count rates "}, {"name": "AlC", "desc": "? Al/Ti/C count rates "}, {"name": "Dag", "desc": "? Ti/Sb/Al count rates "}, {"name": "Tin", "desc": "? Sn/SiO count rates "}, {"name": "DSL", "desc": "? DS Lexan count rates "}, {"name": "DSA", "desc": "? DS Al/C count rates "}, {"name": "Q", "desc": "[12U] Identification quality (2) "}, {"name": "ID", "desc": "Possible optical identification "}, {"name": "Name", "desc": "Other name of ID "}, {"name": "SpType", "desc": "Spectral type of ID "}, {"name": "Type", "desc": "Type of ID (SB, Em, WD ...) "}, {"name": "Vmag", "desc": "? V or B magnitude "}, {"name": "n_Vmag", "desc": "Note on Vmag (variability or uncertainty flag) "}, {"name": "Band", "desc": "[B] B if B magnitude in Vmag column "}, {"name": "Sep", "desc": "? Separation between the EUVE RAP source and the candidate counterpart"}, {"name": "Notes", "desc": "Notes (3) "}]}, {"name": "notes.dat", "desc": "Notes to table2.dat ", "columns": [{"name": "Note", "desc": "Note abbreviation "}, {"name": "Text", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_109_2229"}} {"id": "J/AJ/109/2229", "title_cds": "South Galactic Pole stars photometry", "title_create": "Eggen 1995", "year": "1995", "author": "Eggen O.J.", "title_pub": "Stellar populations at the South Galactic Pole.", "first_author": "Eggen O.J.", "ref_biblio": [""], "bibcode": ["1995AJ....109.2229E"], "see_also": ["J/AJ/112/772 : VI photometry in South Galactic Pole (Caldwell+ 1996)", "J/A+AS/97/835 : K giants at the South Galactic Pole (Flynn+ 1993)", "V/33 : Radial velocities of stars at the North & South Galactic Poles", "II/120 : Phot and Spectrophot Investigation, SGP (Eriksson 1978)", "I/129 : Parallaxes and Proper Motions near SGP (Murray+ 1986)"], "keyword_cds": "Galactic pole, south ; Populations, stellar ; Photometry ; Proper motions ; Radial velocities", "abstract": ["Four-color, (R, I), H{beta}, and DDO photometry for some 500 stars", "with known proper motion and within 10{deg} of the South Galactic Pole", "is analyzed for reddening, luminosity, metal abundance, and space", "motion. The sample contains 275, mostly evolved, GK stars and 225 near", "main sequence, AF stars. The stars are divided into young disk and old", "disk population objects on the basis of their motion vectors and this", "also separates them into stars younger and older than 2x10^9^yr, on", "the basis of models with convective overshoot at the cores. The", "critical mass separating the two populations is 1.7M_{sun}_, which is", "also the critical mass separating the stars that develop degenerate", "helium cores and evolve to a giant luminosity that is an order of", "magnitude greater than the main sequence turnoff, and the more massive", "stars that do not form degenerate cores and maintain, as giants, their", "mean sequence luminosity. The dispersions in the W velocity, for the", "OD samples of AF and GK stars, with the addition of small samples of", "AGB stars and high latitude A stars (presumable OD, BS) at the SGP,", "define the relation ({omega}_w_=9.5+0.025|Z|(pc). The stars discussed", "here do not, generally, follow the pattern of decreasing metallicity", "with increasing Z. found by others for unevolved GK stars. The BS", "population at the NGP consists of 20% of the OD, AF stars, whereas it", "is only 4% at the SGP and this result may be associated with the fact", "that the OD/YD ratio is near 1.5 for most reliable samples, whereas it", "is only about 0.5 for the AF stars at the NGP."], "doi_pub": ["10.1086/117448"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "position.dat", "desc": "Object positions ", "columns": [{"name": "RAh", "desc": "Right ascension (2000.0) "}, {"name": "RAm", "desc": "Right ascension (2000.0) "}, {"name": "RAs", "desc": "Right ascension (2000.0) "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (2000.0) "}, {"name": "DEm", "desc": "Declination (2000.0) "}, {"name": "DEs", "desc": "? Declination (2000.0) "}, {"name": "CPC", "desc": "? CPC number "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "CD", "desc": "CD number "}, {"name": "HD", "desc": "HD number "}, {"name": "Names", "desc": "Other names "}]}, {"name": "table1.dat", "desc": "Cape Zone Catalogue stars within 10{deg} of the South Calactic Pole.", "columns": [{"name": "CPC", "desc": "Cape (Cat. ) number "}, {"name": "m_CPC", "desc": "[ABEW] Multiplicity index on CPC "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "CD", "desc": "? CD (Cat. ) number "}, {"name": "m_CD", "desc": "[AB] Multiplicity index on CPD "}, {"name": "n_CD", "desc": "Distance from the companion when no CPD number "}, {"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "m_HD", "desc": "[AB] Multiplicity index on HD "}, {"name": "Vmag", "desc": "? V magnitude "}, {"name": "n_Vmag", "desc": "[V] V for variable "}, {"name": "b-y", "desc": "? b-y colour index "}, {"name": "M1", "desc": "? M1 colour index "}, {"name": "C1", "desc": "? C1 colour index "}, {"name": "Rmag", "desc": "? R magnitude "}, {"name": "beta", "desc": "? beta colour index "}, {"name": "R-I", "desc": "? R-I colour index "}, {"name": "e_b-y", "desc": "? rms uncertainty on b-y "}, {"name": "e_M1", "desc": "? rms uncertainty on M1 "}, {"name": "e_C1", "desc": "? rms uncertainty on C1 "}, {"name": "e_R-I", "desc": "? rms uncertainty on R-I "}, {"name": "Nobs", "desc": "? Number of observations "}]}, {"name": "table2.dat", "desc": "Previously unpublished DDO photometry. ", "columns": [{"name": "Star", "desc": "Star name (HD or CD) "}, {"name": "M48", "desc": "? M48 magnitude "}, {"name": "(45-48)", "desc": "(45-48) DDO colour index "}, {"name": "u_(45-48)", "desc": "Uncertainty flag on (45-48) "}, {"name": "(42-45)", "desc": "(42-45) DDO colour index "}, {"name": "u_(42-45)", "desc": "Uncertainty flag on (42-45) "}, {"name": "(41-42)", "desc": "(41-42) DDo colour index "}, {"name": "u_(41-42)", "desc": "Uncertainty flag on (41-42) "}]}, {"name": "table3.dat", "desc": "The GK stars of the SGP ", "columns": [{"name": "CPC", "desc": "Cape number "}, {"name": "m_CPC", "desc": "[AB] Multiplicity index on CPC "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "Name", "desc": "Object name "}, {"name": "E(b-y)", "desc": "Interstellar reddening "}, {"name": "u_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "D(45-48)", "desc": "? Luminosity-dependent index from the DDO system"}, {"name": "n_D(45-48)", "desc": "[)n] ): Uncertainty flag on D(45-48) n: See text"}, {"name": "Cm0", "desc": "? Measure of the CN strength "}, {"name": "n_Cm0", "desc": "[)n] ): Uncertainty flag on Cm0 n: See text"}, {"name": "MV4C", "desc": "? Four-colour photometry V magnitude (2) "}, {"name": "u_MV4C", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "MVDDO", "desc": "? DDO photometry V magnitude (3) "}, {"name": "u_MVDDO", "desc": "[)] Uncertainty flag on MVDDO "}, {"name": "P[Fe/H]4C", "desc": "? Four-colour photometry metallicity (4) "}, {"name": "u_P[Fe/H]4C", "desc": "[)] Uncertainty flag on P[Fe/H]4C "}, {"name": "P[Fe/H]DDO", "desc": "? DDO metallicity (4) "}, {"name": "u_P[Fe/H]DDO", "desc": "[)] Uncertainty flag on P[Fe/H]DDO "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] Dash "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "u_pmRA", "desc": "[)] Uncertainty flag on pmRA and pmDE "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "n_Uvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "n_Vvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "n_Wvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Z", "desc": "? Distance from the galactic plane "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "n_SpType", "desc": "[a] Note on SpType (5) "}, {"name": "Pop", "desc": "Population (OD, YD) "}]}, {"name": "table4.dat", "desc": "Anomalous CN ", "columns": [{"name": "CPC", "desc": "Cape (Cat. ) number "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "P[Fe/H]4C", "desc": "Four-colour photometry metallicity "}, {"name": "P[Fe/H]DDO", "desc": "DDO photometry metallicity "}, {"name": "CN", "desc": "wk: CN weak star; str: CN strong star "}, {"name": "Pop", "desc": "OD: old disk, YD: young disk "}]}, {"name": "table5.dat", "desc": "YD evolved GK stars near the NGP (SA 79, 80, 81, and 82)", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "BD", "desc": "BD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "D(45-48)0", "desc": "Dereddened {DELTA}(45-48) colour index "}, {"name": "Cm0", "desc": "Dereddened C_m_ colour index "}, {"name": "MV4C", "desc": "Four-colour photometry absolute V magnitude "}, {"name": "MVDDo", "desc": "DDO photometry absolute V magnitude "}, {"name": "P[Fe/H]4C", "desc": "Four-colour photometry metallicity "}, {"name": "P[Fe/H]DDO", "desc": "DDO photometry metallicity "}, {"name": "pmRA", "desc": "Proper motion in RA "}, {"name": "---", "desc": "[/] Dash "}, {"name": "pmDE", "desc": "Proper motion in DE "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "Uvel", "desc": "U velocity "}, {"name": "Vvel", "desc": "V velocity "}, {"name": "Wvel", "desc": "W velocity "}, {"name": "Z", "desc": "Distance from the galactic plane "}]}, {"name": "table6.dat", "desc": "Problem stars ", "columns": [{"name": "CPC", "desc": "Cape number "}, {"name": "m_CPC", "desc": "[AB] Multiplicity index on CPC "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "Name", "desc": "Object name "}, {"name": "E(b-y)", "desc": "Interstellar reddening "}, {"name": "u_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "D(45-48)", "desc": "? Luminosity-dependent index from the DDO system"}, {"name": "n_D(45-48)", "desc": "[)n] ): Uncertainty flag on D(45-48) n: See text"}, {"name": "Cm0", "desc": "? Measure of the CN strength "}, {"name": "n_Cm0", "desc": "[)n] ): Uncertainty flag on Cm0 n: See text"}, {"name": "MV4C", "desc": "? Four-colour photometry V magnitude (2) "}, {"name": "u_MV4C", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "MVDDO", "desc": "? DDO photometry V magnitude (3) "}, {"name": "u_MVDDO", "desc": "[)] Uncertainty flag on MVDDO "}, {"name": "P[Fe/H]4C", "desc": "? Four-colour photometry metallicity (4) "}, {"name": "u_P[Fe/H]4C", "desc": "[)] Uncertainty flag on P[Fe/H]4C "}, {"name": "P[Fe/H]DDO", "desc": "? DDO metallicity (4) "}, {"name": "u_P[Fe/H]DDO", "desc": "[)] Uncertainty flag on P[Fe/H]DDO "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] Dash "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "u_pmRA", "desc": "[)] Uncertainty flag on pmRA and pmDE "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "n_Uvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "n_Vvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "n_Wvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Z", "desc": "? Distance from the galactic plane "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "n_SpType", "desc": "[a] Note on SpType (5) "}, {"name": "Pop", "desc": "Population (OD, YD) "}]}, {"name": "table7.dat", "desc": "Stars at the SGP ", "columns": [{"name": "Cape", "desc": "Cape number "}, {"name": "m_Cape", "desc": "[A] Multilicity index on CPC "}, {"name": "n_Cape", "desc": "[X] Note on CPC (1) "}, {"name": "Note", "desc": "[a] Individual note (2) "}, {"name": "Name", "desc": "Other name "}, {"name": "beta", "desc": "? beta magnitude "}, {"name": "u_beta", "desc": "[)] Uncertainty flag on beta "}, {"name": "VMag", "desc": "? Absolute V magnitude "}, {"name": "u_VMag", "desc": "[)] Uncertainty flag on VMag "}, {"name": "Z", "desc": "? Distance from the galactic plane "}, {"name": "P[Fe/H]", "desc": "? Metallicity "}, {"name": "u_P[Fe/H]", "desc": "[)] Uncertainty flag on P[Fe/H] "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "n_Uvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "n_Vvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "SpType", "desc": "Spectral type "}, {"name": "pmRA", "desc": "Proper motion in RA "}, {"name": "---", "desc": "[/] Dash "}, {"name": "pmDE", "desc": "Proper motion in DE "}, {"name": "u_pmDE", "desc": "[)] Uncertainty flag on proper motions "}, {"name": "Pop", "desc": "Population (OD: old disk, YD: Young Disk) "}]}, {"name": "table8.dat", "desc": "SGP A stars with Z>700 pc ", "columns": [{"name": "Name", "desc": "Object name (1) "}, {"name": "(b-y)0", "desc": "Dereddened (b-y) colour index "}, {"name": "u_(b-y)0", "desc": "[)] Uncertainty flag on (b-y)0 "}, {"name": "VMag", "desc": "Absolute V magnitude "}, {"name": "|Z|", "desc": "Absolute distance above the plane (2) "}, {"name": "W", "desc": "Radial velocity times sin(b) (2) "}, {"name": "[Ca/H]", "desc": "? Calcium relative abundance (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_110_823"}} {"id": "J/AJ/110/823", "title_cds": "Blue stragglers in solar vicinity", "title_create": "Eggen+, 1995", "year": "1995", "author": "Eggen O.J.", "title_pub": "Blue stragglers in the solar vicinity: newborn or reborn.", "first_author": "Eggen O.J.", "ref_biblio": [""], "bibcode": ["1995AJ....110..823E"], "see_also": ["J/AJ/115/2397 : Stars in the solar region (Eggen 1998)", "J/A+AS/109/375 : Blue stragglers in open clusters (Ahumada+, 1995)"], "keyword_cds": "Stars, blue ; Photometry, Geneva ; Photometry, uvby, beta ; Rotational velocities ; Space velocities ; Effective temperatures", "abstract": ["A selected sample of 1400 A0/1 to F2/ (logTeff=3.96 to 3.82) stars", "with accurate photometric and astrometric data are discussed on the", "basis of luminosities obtained from both Stroemgren+H{beta} and Geneva", "photometry. The sample contains members of the Hyades, Sirius, and HR", "1614 superclusters, all of which show an appreciable age spread. The", "spread of 6 to 20x10^8^yr in the Hyades supercluster is reflected in a", "spread of about 6 to 10x10^8^yr in the Praesepe and Hyades clusters", "within the supercluster. Strong arguments are presented for the", "presence of a larger age spread in the noncluster supercluster members", "than in the contained clusters. The age range for members of the", "Sirius supercluster is 2 to 6x10^8^yr and nearly all of this range is", "seen in the UMa nucleus of the Sirius supercluster, contained within", "the supercluster. The HR 1614 supercluster is near 4x10^9^yr old and", "may include the old disk cluster NGC 6791. About three-quarters of", "bright A-star sample consists of young disk stars, on the basis of", "their (U, V) velocities. The Am, USPC ({delta} Sct), and A Boo stars", "represent about 10%, 6%, and 1%, respectively, of the total sample as", "well as of the young disk and old disk constituents of the sample."], "doi_pub": ["10.1086/117567"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Stars of type A2 or later ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number (1) "}, {"name": "---", "desc": "[/] "}, {"name": "n_HR", "desc": "? When multiple HR name "}, {"name": "Q", "desc": "[AB] Note (2) "}]}, {"name": "table3.dat", "desc": "Conflict of spectroscopic and photometric luminosities", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "u_E(b-y)", "desc": "Uncertainty flag on E(b-y) "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "Uncertainty flag on V0 "}, {"name": "l_V0", "desc": "Limit flag on V0 "}, {"name": "VMAG4c", "desc": "? 4C absolute V magnitude "}, {"name": "l_VMAGg", "desc": "Limit flag on VMAGg "}, {"name": "VMAGg", "desc": "? Geneva absolute V magnitude "}, {"name": "SpType", "desc": "Spectral type (1) "}]}, {"name": "table4.dat", "desc": "Sample stars in the Hyades supercluster ", "columns": [{"name": "Group", "desc": "[CS] C: cluster, S: supercluster "}, {"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[ABC ] Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "nu", "desc": "? Proper motion in the direction of (A, D) "}, {"name": "---", "desc": "[/] "}, {"name": "tau", "desc": "? Motion perpendicular to the direction of (A, D)"}, {"name": "n_tau", "desc": "[*] Note (1) "}, {"name": "DT", "desc": "? Pecular motion, tau, in km/s "}, {"name": "X", "desc": "? Distance of the member to the Sun "}, {"name": "Vtot", "desc": "? Total velocity "}, {"name": "MOD", "desc": "? Distance modulus "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGc", "desc": "Cluster absolute V magnitude "}, {"name": "u_VMAGc", "desc": "[)] Uncertainty flag on VMAGc "}, {"name": "VMAGp", "desc": "? Photometric absolute V magnitude "}, {"name": "u_VMAGp", "desc": "Uncertainty flag on VMAGp "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "(B-V)0", "desc": "Dereddened B-V colour index "}, {"name": "RVC", "desc": "? Comparison radial velocity "}, {"name": "n_RVC", "desc": "[V] Note on RVC (2) "}, {"name": "RVO", "desc": "? Observed radial velocity "}, {"name": "n_RVO", "desc": "[V:ns] Note on RVO (2) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Note", "desc": "[X] Note in notes.dat file "}]}, {"name": "table5.dat", "desc": "USPC ({delta} Sct) variables in the Hyades supercluster", "columns": [{"name": "HR", "desc": "? HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AB ] Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "Name", "desc": "Name "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "l_vsini", "desc": "Limit flag on vsini "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "SpType", "desc": "Spectral type (only in table5.dat) "}, {"name": "beta", "desc": "{beta} index "}, {"name": "logTeff", "desc": "Effective temperature "}, {"name": "Note", "desc": "Notes "}]}, {"name": "table6.dat", "desc": "Am Stars in the Hyades supercluster ", "columns": [{"name": "HR", "desc": "? HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AB ] Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "Name", "desc": "Name "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "l_vsini", "desc": "Limit flag on vsini "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "SpType", "desc": "Spectral type (only in table5.dat) "}, {"name": "beta", "desc": "{beta} index "}, {"name": "logTeff", "desc": "Effective temperature "}, {"name": "Note", "desc": "Notes "}]}, {"name": "table7.dat", "desc": "Effective temperature of USPC, Am, and normal stars.", "columns": [{"name": "HR", "desc": "? HR (Cat. ) number "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logTeffs", "desc": "Spectrophotometric logarithmic effective temperature"}, {"name": "logTeffc", "desc": "Comparison logarithmic effective temperature "}, {"name": "DlogTeff", "desc": "logTeffs minus logTeffc (1) "}, {"name": "Type", "desc": "Stellar type "}, {"name": "Note", "desc": "Note "}]}, {"name": "table8.dat", "desc": "Am Stars in the sample but not in the Hyades or Sirius supercluster.", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AB ab] Multiplicity index on HR "}, {"name": "Name", "desc": "Name (only in table9.dat) "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "? (b-y) colour excess "}, {"name": "V0", "desc": "? Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGs", "desc": "? Stroemgren absolute V magnitude "}, {"name": "u_VMAGs", "desc": "[)] Uncertainty flag on VMAGs "}, {"name": "VMAGg", "desc": "? Geneva absolute V magnitude "}, {"name": "u_VMAGg", "desc": "[)] Uncertainty flag on VMAGg "}, {"name": "MOD", "desc": "? Distance modulus "}, {"name": "u_MOD", "desc": "[)] Uncertainty flag on MOD "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "(B-V)0", "desc": "? Dereddened B-V colour index "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Note", "desc": "[X] X: note in notes.dat file "}]}, {"name": "table9.dat", "desc": "USPC ({delta} Sct) variables in the bright A-star sample but not in the Hyades supercluster", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AB ab] Multiplicity index on HR "}, {"name": "Name", "desc": "Name (only in table9.dat) "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "? (b-y) colour excess "}, {"name": "V0", "desc": "? Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGs", "desc": "? Stroemgren absolute V magnitude "}, {"name": "u_VMAGs", "desc": "[)] Uncertainty flag on VMAGs "}, {"name": "VMAGg", "desc": "? Geneva absolute V magnitude "}, {"name": "u_VMAGg", "desc": "[)] Uncertainty flag on VMAGg "}, {"name": "MOD", "desc": "? Distance modulus "}, {"name": "u_MOD", "desc": "[)] Uncertainty flag on MOD "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "(B-V)0", "desc": "? Dereddened B-V colour index "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Note", "desc": "[X] X: note in notes.dat file "}]}, {"name": "table10.dat", "desc": "Possible Am stars in the Orion association ", "columns": [{"name": "WH", "desc": "Warren and Hesser (1978ApJS...36..497W) number "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "beta", "desc": "{beta} index "}, {"name": "VMAGs", "desc": "Stroemgren absolute V magnitude "}, {"name": "VMAGg", "desc": "? Geneva absolute V magnitude "}, {"name": "MODp", "desc": "Photometry distance modulus "}, {"name": "MODwh", "desc": "Warren and Hesser distance modulus "}, {"name": "e_MODwh", "desc": "rms uncertainty on MODwh "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Name", "desc": "Name "}]}, {"name": "table11.dat", "desc": "{lambda} Boo stars ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AC] Multiplicity index on HR "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGs", "desc": "? Stroemgren absolute V magnitude "}, {"name": "VMAGgnv", "desc": "? Geneva absolute V magnitude "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "n_RV", "desc": "[V] Note on RV "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "u_Uvel", "desc": "[)] Uncertainty flag on Uvel "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "u_Vvel", "desc": "[)] Uncertainty flag on Vvel "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "u_Wvel", "desc": "[)] Uncertainty flag on Wvel "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "SpType", "desc": "Spectral type (1) "}, {"name": "Note", "desc": "[ab] ???????? "}]}, {"name": "table12.dat", "desc": "A2 IV stars ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[ABC] Multiplicity index on HR "}, {"name": "n_HR", "desc": "[*] Note on HR (1) "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGp", "desc": "? Photometric absolute V magnitude "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "VVel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "Note", "desc": "[hs] Note on space velocities (2) "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "logTeff", "desc": "? Effective temperature "}]}, {"name": "table13.dat", "desc": "Members of the Sirius supercluster ", "columns": [{"name": "Group", "desc": "[CS] C: cluster, S: supercluster "}, {"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[ABC ] Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "nu", "desc": "? Proper motion in the direction of (A, D) "}, {"name": "---", "desc": "[/] "}, {"name": "tau", "desc": "? Motion perpendicular to the direction of (A, D)"}, {"name": "n_tau", "desc": "[*] Note (1) "}, {"name": "DT", "desc": "? Pecular motion, tau, in km/s "}, {"name": "X", "desc": "? Distance of the member to the Sun "}, {"name": "Vtot", "desc": "? Total velocity "}, {"name": "MOD", "desc": "? Distance modulus "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGc", "desc": "Cluster absolute V magnitude "}, {"name": "u_VMAGc", "desc": "[)] Uncertainty flag on VMAGc "}, {"name": "VMAGp", "desc": "? Photometric absolute V magnitude "}, {"name": "u_VMAGp", "desc": "Uncertainty flag on VMAGp "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "(B-V)0", "desc": "Dereddened B-V colour index "}, {"name": "RVC", "desc": "? Comparison radial velocity "}, {"name": "n_RVC", "desc": "[V] Note on RVC (2) "}, {"name": "RVO", "desc": "? Observed radial velocity "}, {"name": "n_RVO", "desc": "[V:ns] Note on RVO (2) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Note", "desc": "[X] Note in notes.dat file "}]}, {"name": "table14.dat", "desc": "Normal old disk stars in the bright A-star sample ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "m_HD", "desc": "Multiplicity index on HD "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAG", "desc": "? Absolute V magnitude "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "l_vsini", "desc": "Limit flag on vsini "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "Note", "desc": "[X] Note in notes.dat file "}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_110_o.2288"}} {"id": "J/AJ/110/2288", "title_cds": "Kinematics of local RR Lyrae stars. II.", "title_create": "Layden 1995", "year": "1995", "author": "Layden A.C.", "title_pub": "The metallicities and kinematics of RR Lyrae variables. II. Galactic structure and formation from local stars", "first_author": "Layden A.C.", "ref_biblio": [""], "bibcode": ["1995AJ....110.2288L"], "see_also": ["J/AJ/108/1016 : Kinematics of local RR lyrae stars I. (Layden, 1994)"], "keyword_cds": "Stars, variable ; Proper motions ; Space velocities", "abstract": ["We investigate the kinematics and spatial distribution of a sample of", "302 nearby RR Lyrae variable stars with the goal of learning more", "about the formation history and present-day structure of the galaxy.", "We find that the kinematics change abruptly at [Fe/H]~-1.0. Above", "this value, the stars exhibit kinematic properties like those of other", "tracers of the galaxy's thick disk, while below [Fe/H]=-1.3, halo", "kinematics are observed. The stars with -1.3<=[Fe/H]<=-1.0 are a", "mixture of these populations, though the fraction of thick disk RR", "Lyrae stars with [Fe/H]<=-1.0 is significantly smaller than found", "among red giant stars by other authors; we discuss several", "possibilities for this discrepancy. The RR Lyraes with [Fe/H]>-0.5", "exhibit somewhat cooler kinematics and a flatter spatial distribution", "than those of the thick disk, and may include some members of the old", "thin disk population. We find the kinematics of the halo RR Lyraes to", "be uncorrelated with abundance over the range -2.2<=[Fe/H]<=-1.0,", "and interpret this as evidence that the motions and chemical", "enrichment of gas in the early galaxy was characterized by a high", "degree of randomization, consistent with fragment accretion pictures", "of galaxy formation. We argue that the small number of thick disk", "stars with [Fe/H]<=-1.0 cannot be called upon to balance the net", "kinematics of a retrograde-rotating halo to produce the slow prograde", "rotations seen in this and other local samples; however, a hotter,", "slowly rotating, somewhat flattened second halo component may be", "consistent with kinematics both of local samples and of samples far", "from the galactic plane. We find the local density of halo RR Lyraes", "to be 11-15kpc^-3^, with a firm lower limit of 8+/-3kpc^-3^. This is", "larger than that predicted from counts of faint RR Lyraes far from the", "plane; either the flattening of the local halo is larger than c/a~0.7,", "or a two- component halo exists in which one component is quite", "flattened. We derive an exponential scale height of 0.7(+0.5)(-0.3)kpc", "and a midplane density of 10+/-4kpc^-3^ for the disk RR Lyraes with", "[Fe/H]>-1.0."], "date_update": "18-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Proper motions and space velocities of 154 RR Lyrae variables", "columns": [{"name": "Star", "desc": "Star name "}, {"name": "pmRA", "desc": "Proper motion in right ascension (1) "}, {"name": "e_pmRA", "desc": "Error in pmRA "}, {"name": "pmDE", "desc": "Proper motion in declination "}, {"name": "e_pmDE", "desc": "Error in pmDE "}, {"name": "Note", "desc": "[a-d] Note flag (2) "}, {"name": "Vrho", "desc": "Rho component of space velocity (3) "}, {"name": "e_Vrho", "desc": "Error in Vrho "}, {"name": "Vphi", "desc": "Phi component of space velocity (3) "}, {"name": "e_Vphi", "desc": "Error in Vphi "}, {"name": "Vz", "desc": "z component of space velocity (3) "}, {"name": "e_Vz", "desc": "Error in Vz "}, {"name": "[Fe/H]", "desc": "Metal abundance "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_114_1365"}} {"id": "J/AJ/114/1365", "title_cds": "Physical properties of stellar systems", "title_create": "Burstein+, 1997", "year": "1997", "author": "Burstein D., Bender R., Faber S.M., Nolthenious R.", "title_pub": "Global relationships among the physical properties of stellar systems.", "first_author": "Burstein D.", "ref_biblio": [""], "bibcode": ["1997AJ....114.1365B"], "keyword_cds": "Associations, stellar", "abstract": ["The {kappa}-space three-dimensional parameter system was originally", "defined to examine the physical properties of dynamically hot", "elliptical galaxies and bulges (DHGs). The axis of {kappa}-space are", "proportional to the logarithm of galaxy mass, mass-to-light ratio, and", "a third quantity that is mainly surface brightness. In this paper, we", "define self-consistent {kappa} parameters for disk galaxies, galaxy", "groups and clusters, and globular stellar systems in the Universe."], "doi_pub": ["10.1086/118570"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Stellar system physical properties ", "columns": [{"name": "Name", "desc": "Common name for object (1) "}, {"name": "Intnum", "desc": "Internal number for object "}, {"name": "IDnum", "desc": "ID number, stellar system type (2) "}, {"name": "Dist", "desc": "Distance for object (3) "}, {"name": "logVcharO", "desc": "log of observed characteristic dynamic velocity (4)"}, {"name": "logVchaU", "desc": "log of used characteristic dynamic velocity (4)"}, {"name": "logreff", "desc": "log of effective radius used (5) "}, {"name": "logIeff", "desc": "log of effective surface brightness used (5)"}, {"name": "Stellpop", "desc": "?=-1.00 Stellar population index (6) "}, {"name": "kappa1", "desc": "Kappa_1 (7) "}, {"name": "kappa2", "desc": "Kappa_2 (7) "}, {"name": "kappa3", "desc": "Kappa_3 (7) "}, {"name": "delta2:1", "desc": "Delta_2:1 (8) "}, {"name": "delta3:1", "desc": "Delta_3:1 (8) "}, {"name": "logMasseff", "desc": "log of effective mass of object (9) "}, {"name": "logLeff", "desc": "log of effective luminosity of object (9)"}, {"name": "log(Me/Le)", "desc": "log of mass-to-light ratio within reff (9)"}, {"name": "logTeff", "desc": "log of effective temperature (9) "}, {"name": "lognb", "desc": "log of baryon number (9) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_117_1668"}} {"id": "J/AJ/117/1668", "title_cds": "Sc galaxies I photometry, optical data", "title_create": "Haynes+, 1999", "year": "1999", "author": "Haynes M.P., Giovanelli R., Salzer J.J., Wegner G., Freudling W., Da Costa L.N., Herter T., Vogt N.P.", "title_pub": "The I-band Tully-Fisher relation for Sc galaxies: optical imaging data.", "first_author": "Haynes M.P.", "ref_biblio": [""], "bibcode": ["1999AJ....117.1668H"], "see_also": ["VII/26 : Uppsala General Catalogue of Galaxies (UGC) (Nilson 1973)", "J/AJ/113/22 : Tully-Fisher Relation. I. (Giovanelli+ 1997)", "J/AJ/116/2728 : I photometry of early-type galaxies (Scodeggio+, 1998)", "J/AJ/116/2738 : Spectroscopy of early-type galaxies (Scodeggio+ 1998)", "J/A+AS/130/333 : 2112 new 21-cm line measurements (Theureau+ 1998)", "J/AJ/117/2039 : Sc galaxies I photometry, 21cm data (Haynes+, 1999)"], "keyword_cds": "Galaxy catalogs ; Galaxies, photometry", "keyword_pub": "galaxies: photometry - galaxies: spiral - techniques: spectroscopic", "abstract": ["Properties derived from the analysis of photometric I-band imaging", "observations are presented for 1727 inclined spiral galaxies, mostly", "of types Sbc and Sc. The reduction, parameter extraction, and error", "estimation procedures are discussed in detail. The asymptotic behavior", "of the magnitude curve of growth and the radial variation in", "ellipticity and position angle are used in combination with the", "linearity of the surface brightness falloff to fit the disk portion of", "the profile. Total I-band magnitudes are calculated by extrapolating", "the detected surface brightness profile to a radius of eight disk", "scale lengths. Errors in the magnitudes, typically ~0.04 mag, are", "dominated by uncertainties in the sky subtraction and disk-fitting", "procedures. Comparison is made with the similar imaging database of", "Mathewson, Ford, & Buchhorn, both as presented originally by those", "authors and after reanalyzing their digital reduction files using", "identical disk-fitting procedures. Direct comparison is made of", "profile details for 292 galaxies observed in common. Although some", "differences occur, good agreement is found, proving that the two data", "sets can be used in combination with only minor accommodation of those", "differences. The compilation of optical properties presented here is", "optimized for use in applications of the Tully-Fisher relation as a", "secondary distance indicator in studies of the local peculiar velocity", "field."], "doi_pub": ["10.1086/300817"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "stars.dat", "desc": "J2000.0 coordinates from Simbad Database ", "columns": [{"name": "RAh", "desc": "? Right ascension (J2000.0) "}, {"name": "RAm", "desc": "? Right ascension (J2000.0) "}, {"name": "RAs", "desc": "? Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "? Declination (J2000.0) "}, {"name": "DEm", "desc": "? Declination (J2000.0) "}, {"name": "DEs", "desc": "? Declination (J2000.0) "}, {"name": "Name", "desc": "Galaxy name (UGC NNNNNN or AGC NNNNNN) "}, {"name": "Simbad", "desc": "Other name taken form Simbad database "}, {"name": "table2", "desc": "Other name from table2.dat when it differs from Simbad"}, {"name": "Com", "desc": "Comments "}]}, {"name": "table2.dat", "desc": "Optical properties ", "columns": [{"name": "UGC/AGC", "desc": "UGC (Cat. ) number where applicable or else in our private database, referred to as the Arecibo General Catalog (AGC) (1)"}, {"name": "Name", "desc": "Other galaxy designation (2) "}, {"name": "RAh", "desc": "Right ascension (1950.0) "}, {"name": "RAm", "desc": "Right ascension (1950.0) "}, {"name": "RAs", "desc": "Right ascension (1950.0) "}, {"name": "DE-", "desc": "Declination sign (1950.0) "}, {"name": "DEd", "desc": "Declination (1950.0) "}, {"name": "DEm", "desc": "Declination (1950.0) "}, {"name": "DEs", "desc": "Declination (1950.0) "}, {"name": "TType", "desc": "Hubble morphological type code "}, {"name": "r23.5", "desc": "Isophotal radius measured at an I-band surface magnitude of 23.5mag/arcsec^2^"}, {"name": "r83L", "desc": "Characteristic optical radius (3) "}, {"name": "mu", "desc": "Surface magnitude at the other most detected isophote in the I-band image"}, {"name": "E0", "desc": "disk ellipticity, corrected for seeing "}, {"name": "e_E0", "desc": "rms uncertainty on E0 "}, {"name": "PA", "desc": "Mean disk position angle "}, {"name": "e_PA", "desc": "rms uncertainty on PA "}, {"name": "Imag", "desc": "Total I-band magnitude "}, {"name": "e_Imag", "desc": "rms uncertainty on Imag "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_118_1073"}} {"id": "J/AJ/118/1073", "title_cds": "Orbiting astronomical observatory catalog", "title_create": "Meade+, 1999", "year": "1999", "author": "Meade M.R.", "title_pub": "A second catalog of orbiting astronomical observatory 2 filter photometry: ultraviolet photometry of 614 stars.", "first_author": "Meade M.R.", "ref_biblio": [""], "bibcode": ["1999AJ....118.1073M"], "keyword_cds": "Photometry, ultraviolet", "keyword_pub": "catalogs - stars: general", "abstract": ["Ultraviolet photometry from the Wisconsin Experiment Package on the", "Orbiting Astronomical Observatory 2 (OAO 2) is presented for 614", "stars. Previously unpublished magnitudes from 12 filter bandpasses", "with wavelengths ranging from 1330 to 4250{AA} have been placed on the", "white dwarf model atmosphere absolute flux scale. The fluxes were", "converted to magnitudes using V=0 for F(V)=3.46x10-9ergs/cm2/s1/{AA},", "or m_{lambda}_=-2.5logF_{lambda}_-21.15. This second catalog", "effectively doubles the amount of OAO 2 photometry available in the", "literature and includes many objects too bright to be observed with", "modern space observatories."], "doi_pub": ["10.1086/300955"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Second OAO-2 Filter Photometry Catalogue ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "n_HD", "desc": "Last digit when two number for the same object "}, {"name": "Name", "desc": "Name "}, {"name": "SpType", "desc": "Spectral classification "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "B-V", "desc": "? B-V colour index "}, {"name": "U-B", "desc": "? U-B colour index "}, {"name": "Ref", "desc": "Reference (1) "}, {"name": "Var", "desc": "[V] V: variable "}, {"name": "UV", "desc": "Other UV observations (2) "}, {"name": "4250{AA}", "desc": "? 4250{AA} filter magnitude "}, {"name": "3320{AA}", "desc": "? 3320{AA} filter magnitude "}, {"name": "2980{AA}", "desc": "? 2980{AA} filter magnitude "}, {"name": "2940{AA}", "desc": "? 2940{AA} filter magnitude "}, {"name": "2460{AA}", "desc": "? 2460{AA} filter magnitude "}, {"name": "2380{AA}", "desc": "? 2380{AA} filter magnitude "}, {"name": "2035{AA}", "desc": "? 2035{AA} filter magnitude "}, {"name": "1910{AA}", "desc": "? 1910{AA} filter magnitude "}, {"name": "1680{AA}", "desc": "? 1680{AA} filter magnitude "}, {"name": "1550{AA}", "desc": "? 1550{AA} filter magnitude "}, {"name": "1430{AA}", "desc": "? 1430{AA} filter magnitude "}, {"name": "1330{AA}", "desc": "? 1330{AA} filter magnitude "}]}, {"name": "table3.dat", "desc": "Variable-star information for OAO-2 objects ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "m_HD", "desc": "Last digit when two number for the same object "}, {"name": "Name", "desc": "Name "}, {"name": "Var", "desc": "Variable type "}, {"name": "Amp", "desc": "? Amplitude "}, {"name": "JD", "desc": "Julian Date (-2440000) for OAO2 observations "}, {"name": "JD2", "desc": "? Julian Date (-2440000) for OAO2 observations "}, {"name": "n_JD2", "desc": "[*] Note (1) "}, {"name": "JD3", "desc": "? Julian Date (-2440000) for OAO2 observations "}, {"name": "JD4", "desc": "? Julian Date (-2440000) for OAO2 observations "}, {"name": "JD5", "desc": "? Julian Date (-2440000) for OAO2 observations "}, {"name": "JD6", "desc": "? Julian Date (-2440000) for OAO2 observations "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_118_752"}} {"id": "J/AJ/118/752", "title_cds": "BI photometry of NGC 3256 young globular clusters", "title_create": "Zepf+, 1999", "year": "1999", "author": "Zepf S.E., Ashman K.M., English J., Freeman K.C., Sharples R.M.", "title_pub": "The formation and evolution of candidate young globular clusters in NGC 3256.", "first_author": "Zepf S.E.", "ref_biblio": [""], "bibcode": ["1999AJ....118..752Z"], "keyword_cds": "Clusters, globular ; Photometry", "keyword_pub": "galaxies: formation - galaxies: individual (NGC 3256) - galaxies: interactions - galaxies: starburst - galaxies: star clusters", "mission": "HST", "abstract": ["We present images of the recent galaxy merger NGC 3256 obtained with", "the Wide Field Planetary Camera 2 of the Hubble Space Telescope in B", "and I filters. We show that there is a large population of more than", "1000 compact, bright, blue objects in this galaxy within the 7kpcx7kpc", "region studied. These objects have sizes, colors, and luminosities", "like those expected for young Galactic globular clusters, with ages", "ranging from a few to several hundred megayears. On this basis, we", "identify at least some fraction of the compact, bright, blue objects", "in NGC 3256 as young globular clusters."], "object": ["10 27 51.3 -43 54 17 NGC 3256"], "doi_pub": ["10.1086/300961"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Candidate young globular clusters in NGC 3256 ", "columns": [{"name": "RAh", "desc": "Right ascension (J2000) (1) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Bmag", "desc": "B magnitude "}, {"name": "B-I", "desc": "B-I colour index "}, {"name": "R1/2", "desc": "Size (1 pix = 8 pc) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_120_1794"}} {"id": "J/AJ/120/1794", "title_cds": "Far-UV observations of the shell in IC 2574", "title_create": "Stewart+, 2000", "year": "2000", "author": "Stewart S.G., Walter F.", "title_pub": "Ultraviolet observations of the powering source of the supergiant shell in IC 2574.", "first_author": "Stewart S.G.", "ref_biblio": [""], "bibcode": ["2000AJ....120.1794S"], "keyword_cds": "Photometry, ultraviolet ; Photometry, H-alpha ; Stars, ages ; Stars, masses", "keyword_pub": "Galaxies: Individual: IC 2574 - Galaxies: ISM - ISM: Bubbles - ISM: Structure - Ultraviolet Emission", "abstract": ["A multiband analysis of the region containing the supergiant H I shell", "in the nearby dwarf irregular galaxy IC 2574 presents evidence of a", "causal relationship between a central star cluster, the surrounding", "expanding H I shell, and secondary star formation sites on the rim of", "the H I shell. Comparisons of the far-UV (FUV, 1521 {AA}), optical", "broad band, H-alpha, X-ray, and H I morphologies suggest that the", "region is in an auspicious moment of star formation triggered by the", "central stellar cluster. The derived properties of the H I shell, the", "central stellar cluster, and the star-forming regions on the rim", "support this scenario: The kinematic age of the H I shell is <14 Myr", "and in agreement with the age of the central stellar cluster derived", "from the FUV observations (~11 Myr). An estimate for the mechanical", "energy input from supernovae and stellar winds of the central stellar", "cluster, made from FUV photometry and the derived cluster age, is", "4.1x10^52^ ergs, roughly a few times higher than the kinetic energy of", "the H I shell. The requisite energy input needed to create the H I", "shell, derived in the ``standard'' fashion from the H I observations", "(using the numerical models of Chevalier), is 2.6x10^53^ ergs, which is", "almost 1 order of magnitude higher than the estimated energy input as", "derived from the FUV data. Given the overwhelming observational", "evidence that the central cluster is responsible for the expanding H I", "shell, this discrepancy suggests that the required energy input is", "overestimated using the ``standard'' method. This may explain why some", "other searches for remnant stellar clusters in giant H I holes have", "been unsuccessful so far. Our observations also show that stellar", "clusters are indeed able to create supergiant H I shells, even at", "large galactocentric radii; a scenario that has recently been", "questioned by a number of authors."], "object": ["10 28 47 +68 28 18 NAME IC2574 SGS"], "doi_pub": ["10.1086/301584"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Observations for star-forming regions ", "columns": [{"name": "Region", "desc": "The supergiant shell region in IC 2574 (1) "}, {"name": "Bmag", "desc": "The B band magnitude (2) "}, {"name": "Halpha", "desc": "The H{alpha} flux in units of 10^-15^ ergs/cm^2^/s/{AA} (2)"}, {"name": "FUV", "desc": "The Far-UV flux in units of 10^-15^ ergs/cm^2^/s/{AA} (2)"}, {"name": "FUVmag", "desc": "The Far-UV magnitude "}, {"name": "(FUV-B)", "desc": "The (Far-UV - B) color (3) "}, {"name": "Ratio", "desc": "Logarithmic ratio of Lyman continuum photons to FUV flux (4)"}]}, {"name": "table2.dat", "desc": "Derived parameters for star-forming regions ", "columns": [{"name": "Region", "desc": "The supergiant shell region in IC 2574 (1) "}, {"name": "Age", "desc": "The mean age of the stars in the aperture "}, {"name": "LFUV", "desc": "Far-UV luminosity corrected for internal extinction and assuming a distance of 3.2 Mpc"}, {"name": "Mass", "desc": "Mass estimate based on Age "}, {"name": "EMech", "desc": "Estimate of the net mechanical energy deposited into the ISM by SN and stellar winds (2)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_122_2190"}} {"id": "J/AJ/122/2190", "title_cds": "HDF-South multicolor observations", "title_create": "Vanzella+, 2001", "year": "2001", "author": "Vanzella E., Cristiani S., Saracco P., Arnouts S., Bianchi S., D'Odorico S., Fontana A., Giallongo E., Grazian A.", "title_pub": "Multicolor observations of the Hubble Deep Field South.", "first_author": "Vanzella E.", "ref_biblio": [""], "bibcode": ["2001AJ....122.2190V"], "see_also": ["J/AJ/112/1335 : Hubble Deep Field observations (Williams+ 1996)", "J/ApJ/513/34 : HDF photometric redshifts catalog (Fernandez-Soto+, 1999)", "J/AJ/120/2206 : NTT, HDF-S and HDF-N photometric redshifts (Fontana+, 2000)", "J/A+A/375/1 : IR obs. of Chandra Deep Field + HDF-South (Saracco+, 2001)", "J/A+A/364/517 : HDF-N spiral and irregular galaxies (Rodighiero+, 2000)", "J/AJ/120/2747 : HDF-South WFPC2 observations (Casertano+, 2000)", "J/A+AS/145/111 : HDF-South catalogue of galaxies (Volonteri+, 2000)", "J/AJ/119/486 : HDF-South: STIS imaging (Gardner+, 2000)", "J/AJ/122/2205 : HDF-South K photometric redshift catalog (Rudnick+, 2001)"], "keyword_cds": "Galaxy catalogs ; Photometry, UBVRIJKLMNH", "keyword_pub": "cosmology: observations - galaxies: evolution - galaxies: statistics", "abstract": ["We present a deep multicolor (U, B, V, I, Js, H, Ks) catalog of", "galaxies in the Hubble Deep Field South, based on observations", "obtained with the HST WFPC2 (UBVI) in 1998 and VLT-ISAAC (Js, H, Ks)", "in 1999. The photometric procedures were tuned to derive a catalog", "optimized for the estimation of photometric redshifts. In particular", "we adopted a \"conservative\" detection threshold, which resulted in a", "list of 1611 objects. The behavior of the observed source counts is in", "general agreement with the previous results of Casertano et al. (2000,", "Cat. ) in the Hubble Deep Field South and Williams et", "al. (1996, Cat. ) in the Hubble Deep Field North, while", "the corresponding counts in the Hubble Deep Field North provided by", "Fernandez-Soto, Lanzetta, & Yahil (1999, Cat. ) are", "systematically lower by a factor 1.5 beyond I_AB_=26."], "doi_pub": ["10.1086/323544"], "orcid_pub": ["0000-0002-5057-135X"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table3.dat", "desc": "The Object Catalog for the HDF-S WFPC2 Field ", "columns": [{"name": "[VCS2001]", "desc": "Identification number "}, {"name": "Xpix", "desc": "X pixel position in the WFPC2 image "}, {"name": "Ypix", "desc": "Y pixel position in the WFPC2 image "}, {"name": "RAh", "desc": "Right Ascension (J2000) "}, {"name": "RAm", "desc": "Right Ascension (J2000) "}, {"name": "RAs", "desc": "Right Ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Imag", "desc": "AB magnitude in the I band "}]}, {"name": "table5.dat", "desc": "HDF-S U-Dropouts ", "columns": [{"name": "[VCS2001]", "desc": "Identification number "}, {"name": "Imag", "desc": "AB magnitude in the I band ((F814W filter) "}, {"name": "B-I", "desc": "AB (B-I) color "}, {"name": "U-B", "desc": "AB (U-B) color "}, {"name": "Xpix", "desc": "X pixel position in the WFPC2 image "}, {"name": "Ypix", "desc": "Y pixel position in the WFPC2 image "}, {"name": "RAh", "desc": "Right Ascension (J2000) "}, {"name": "RAm", "desc": "Right Ascension (J2000) "}, {"name": "RAs", "desc": "Right Ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}]}, {"name": "table6.dat", "desc": "HDF-S B Dropouts ", "columns": [{"name": "[VCS2001]", "desc": "Identification number "}, {"name": "Imag", "desc": "AB magnitude in the I band "}, {"name": "V-I", "desc": "(V-I) AB colour index "}, {"name": "B-V", "desc": "(B-V) AB colour index "}, {"name": "Xpos", "desc": "X position "}, {"name": "Ypos", "desc": "Y position "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}]}, {"name": "table7.dat", "desc": "A list of EROs in the HDF-S with (I-K)_AB_>2.7 ", "columns": [{"name": "[VCS2001]", "desc": "Identification number (1) "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "Kmag", "desc": "K AB magnitude "}, {"name": "Imag", "desc": "? I AB magnitude "}, {"name": "l_I-K", "desc": "Limit flag on I-K "}, {"name": "I-K", "desc": "(I-K) AB magnitude "}, {"name": "n_I-K", "desc": "[*] *: I-K is an upper limit in the infrared bands"}, {"name": "MType", "desc": "Morphology (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_127_3034"}} {"id": "J/AJ/127/3034", "title_cds": "Proper-motion catalog combining USNO-B and SDSS", "title_create": "Munn+, 2004", "year": "2004", "author": "Munn J.A., Monet D.G., Levine S.E., Canzian B., Pier J.R., Harris H.C., Lupton R.H., Ivezic Z., Hindsley R.B., Hennessy G.S., Schneider D.P., Brinkmann J.", "title_pub": "An improved proper-motion catalog combining USNO-B and the Sloan Digital Sky Survey.", "first_author": "Munn J.A.", "ref_biblio": [""], "bibcode": ["2004AJ....127.3034M"], "keyword_cds": "", "keyword_pub": "astrometry - catalogs", "mission": "", "abstract": ["An improved proper-motion catalog is presented, combining the USNO-B", "and Sloan Digital Sky Survey (SDSS) catalogs in the area of sky", "covered by SDSS Data Release 1 (DR1; 2099 deg^2^). USNO-B positions are", "recalibrated using SDSS galaxies, and proper motions are recomputed", "including both the USNO-B and SDSS positions. Statistical errors in", "the USNO-B proper motions are decreased by roughly 20%-30%, systematic", "errors are greatly reduced, and the proper motions are placed on an", "absolute reference frame. Requiring a match to an SDSS object removes", "the large number of false high proper motion objects in USNO-B. The", "resultant catalog is 90% complete to g<19.7, with statistical errors", "in the component proper motions of roughly 3-3.5mas/yr, substantially", "smaller systematic errors, and a contamination rate of less than 0.5%.", "A number of studies are currently underway using proper motions from", "this catalog. The catalog is available via ftp."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/383292"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_128_330"}} {"id": "J/AJ/128/330", "title_cds": "UBVRI photometry and spectroscopy in Roslund 4", "title_create": "Delgado+, 2004", "year": "2004", "author": "Delgado A.J., Miranda L.F., Fernandez M., Alfaro E.J.", "title_pub": "Photometric and spectroscopic study of stars in the field of the young open cluster Roslund 4.", "first_author": "Delgado A.J.", "ref_biblio": [""], "bibcode": ["2004AJ....128..330D"], "keyword_cds": "", "keyword_pub": "H II regions ; ISM: Herbig-Haro objects ; open clusters and associations: individual (Roslund 4); stars: emission-line, Be; stars: fundamental parameters; stars: pre-main sequence", "description": ["Images of Roslund 4 were obtained on 2003 June 30 with the 1.5m", "telescope at the Observatorio de Sierra Nevada (OSN, Granada).", "3 narrow-band filters were used: H{alpha} (656.3nm, FWHM=5.3nm),", "SII (672.3nm, FWHM=5nm), and a continuum filter (665.2nm, FWHM=5nm).", "The UBVRI photometric observations were carried out in 2000 August,", "and were calbirated wo standard fields of the Landolt catalog (1992,", "Cat. II/183)", "The spectra were taken on the nights of 2001 August 11 and 12 with the", "ISIS spectrograph attached to the WHT telescope at the ORM in La", "Palma. Detectors EEV12 and TeK4 were mounted in the blue and red arms,", "respectively. The wavelength ranges 350-500 and 635-675nm were", "observed at respective resolutions R = 10,000 and 16,000."], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/421742"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_129_2562"}} {"id": "J/AJ/129/2562", "title_cds": "NYU-VAGC catalog", "title_create": "Blanton+, 2005", "year": "2005", "author": "Blanton M.R., Schlegel D.J., Strauss M.A., Brinkmann J., Finkbeiner D., Fukugita M., Gunn J.E., Hogg D.W., Ivezic Z., Knapp G.R., Lupton R.H., Munn J.A., Schneider D.P., Tegmark M., Zehavi I.", "title_pub": "New York University Value-Added Galaxy Catalog: a galaxy catalog based on new public surveys.", "first_author": "Blanton M.R.", "ref_biblio": [""], "bibcode": ["2005AJ....129.2562B"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/429803"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_143_57"}} {"id": "J/AJ/143/57", "title_cds": "New RVs from the spectroscopic survey BRAVA (II)", "title_create": "Kunder+, 2012", "year": "2012", "author": "Kunder A., Koch A., Rich R.M., De Propris R., Howard C.D., Stubbs S.A., Johnson C.I., Shen J., Wang Y., Robin A.C., Kormendy J., Soto M., Frinchaboy P., Reitzel D.B., Zhao H., Origlia L.", "title_pub": "The bulge radial velocity assay (BRAVA). II. Complete sample and data release.", "first_author": "Kunder A.", "ref_biblio": [""], "bibcode": ["2012AJ....143...57K"], "see_also": ["VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "J/A+A/546/A57 : Spectroscopy of 400 Bulge red giants (Uttenthaler+, 2012)", "J/ApJ/733/L47 : Galaxy bulge types within 11Mpc (Fisher+, 2011)", "J/ApJ/732/108 : Abundances of 92 giants in Plaut's window (Johnson+, 2011)", "J/ApJ/691/1387 : Spectroscopy of the Galactic bar. I. (Rangwala+, 2009)", "J/A+A/486/177 : Bulge field stars from FLAMES-GIRAFFE (Zoccali+, 2008)", "J/MNRAS/348/1439 : OGLE II Galactic center proper motions (Sumi+, 2004)", "J/AJ/118/895 : Milky way and stellar distributions (Tiede+ 1999)", "J/MNRAS/246/54 : Late-type giants in Baade's window (Sharples+ 1990)", "J/AJ/89/636 : Giant M stars in Baade's Window (Blanco+, 1984)", "http://irsa.ipac.caltech.edu/ : NASA/IPAC Infrared Science Archive (IRSA)", "http://brava.astro.ucla.edu/ : The Bulge Radial Velocity Assay at University"], "keyword_cds": "Milky Way ; Stars, M-type ; Stars, giant ; Spectroscopy ; Radial velocities ; Velocity dispersion", "keyword_pub": "Galaxy: center - stars: abundances - stars: distances - stars: Population II - surveys", "abstract": ["We present new radial velocity measurements from the Bulge Radial", "Velocity Assay, a large-scale spectroscopic survey of M-type giants in", "the Galactic bulge/bar region. The sample of ~4500 new radial", "velocities, mostly in the region -10{deg}"], "bibcode": ["2017AJ....153...10M"], "see_also": ["J/ApJS/219/19 : Nearby white dwarfs from SUPERBLINK (Limoges+, 2015)", "J/MNRAS/449/3966 : Ultracool white dwarfs (Gianninas+, 2015)", "J/ApJ/730/128 : Spectroscopy of DA WD from the SDSS-DR4 (Tremblay+, 2011)", "J/ApJ/714/1037 : White dwarfs from the Kiso survey (Limoges+, 2010)", "J/ApJS/190/77 : Detailed analysis of cool WDs in the SDSS (Kilic+, 2010)", "J/A+A/466/627 : Parameters of DA white dwarfs in SDSS-DR1 (Hu+, 2007)", "J/AJ/132/1221 : VJHK and SDSS photometry of DA white dwarfs (Holberg+, 2006)", "J/AJ/131/582 : Cool white dwarfs in the SDSS (Kilic+, 2006)", "J/ApJS/156/47 : DA white dwarfs from Palomar Green Survey (Liebert+, 2005)", "J/ApJ/607/426 : Catalog of white dwarfs in SDSS-DR1 (Kleinman+, 2004)", "J/AJ/125/2621 : SDSS WD-M binary parameters (Raymond+, 2003)", "J/MNRAS/335/673 : DA white dwarfs in 2dF QSO Redshift Survey (Vennes+, 2002)", "J/ApJS/133/413 : BVRIJHK photometry of cool white dwarfs (Bergeron+, 2001)"], "keyword_cds": "Stars, dwarfs", "keyword_pub": "stars: luminosity function, mass function - white dwarfs", "abstract": ["A catalog of 8472 white dwarf (WD) candidates is presented, selected", "using reduced proper motions from the deep proper motion catalog of", "Munn et al. Candidates are selected in the magnitude range 16"], "bibcode": ["1963AJ.....68..319M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["A catalogue of spectral types and infra-red magnitudes for 920 stars", "M5 and later in an area of 9 square degrees surrounding S.A. 158", "(l=3.9deg, b=-9.0deg) is given. These data, together with similar", "unpublished data for 7069 stars nearer the galactic equator in the", "same general direction, have been analyzed for space density. The", "number of stars per 10^6^pc^3^ appears to be relatively constant", "at about 0.2 in a stratum 1kpc thick south of the galactic plane.", "Superposed on this basic layer and beginning at approximately 6kpc", "from the sun is a concentration of stars in which the density rises to", "5 or 6 times that in the basic stratum. The negative density gradient", "perpendicular to the galactic plane near the galactic center appears", "to be quite high."], "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/108980"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_69_104"}} {"id": "J/AJ/69/104", "title_cds": "Stellar space density near selected area 158", "title_create": "McCuskey, 1964", "year": "1964", "author": "McCuskey S. W.", "title_pub": "Stellar space density near selected area 158", "first_author": "McCuskey S. W.", "ref_biblio": [""], "bibcode": ["1964AJ.....69..104M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["Spectral types and photographic magnitudes for 1684 stars in", "25.2sq.deg surrounding S.A.158 are presented in a catalogue and", "identification charts. The matnitude limit of the data is about", "m_pg_=12. Color indices approximately on the (B,V) system are given", "for 275 stars. Stellar space densities are presented as a function", "of distance in table VII and Fig.3. The early A stars decrease by a", "factor of 10 between 100 and 2000pc from the sun. The yellow-red giant", "stars have approximately a constant density in this distance interval.", "A comparison of the density functions with those for the galactic", "anticenter is shown in Fig.4. General luminosity functions computed", "from the above data have mean values of log{phi}(M) for 0"], "bibcode": ["1968AJ.....73..590D"], "see_also": ["II/221 : LF"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/110666"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_76_412"}} {"id": "J/AJ/76/412", "title_cds": "UBV sequences for QSOs", "title_create": "Angione+, 1971", "year": "1971", "author": "Angione R.J.", "title_pub": "Photoelectric sequences for the brighter QSO's.", "first_author": "Angione R.J.", "ref_biblio": [""], "bibcode": ["1971AJ.....76..412A"], "keyword_cds": "Photometry, UBV ; QSOs", "keyword_pub": "", "mission": "", "description": ["UBV photoelectric sequences were measured for 22 of the brighter QSOs", "and four other objects. The results and finding charts were used to", "identify the stars observed.", "The attached plain-text list shows coordinates for stars in"], "doi_pub": ["10.1086/111136"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "angione71.dat", "desc": "Positions and photometry of stars observed ", "columns": [{"name": "Field", "desc": "File name (QSO or AGN name) "}, {"name": "Seq", "desc": "[A-G' ] Star sequence "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[UGAMS] Source of position "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "B-V", "desc": "Johnson B-V magnitude "}, {"name": "U-B", "desc": "? Johnson U-B magnitude "}, {"name": "Comments", "desc": "Additional comments, from B. Skiff. "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_78_687"}} {"id": "J/AJ/78/687", "title_cds": "Southern stars of astrophysical interest", "title_create": "Bidelman+, 1973", "year": "1973", "author": "Bidelman W.P., Macconnell D.J.", "title_pub": "The brighter stars of astrophysical interest in the southern sky.", "first_author": "Bidelman W.P.", "ref_biblio": [""], "bibcode": ["1973AJ.....78..687B"], "see_also": ["III/46 : Ap and Am Stars (Bertaud+ 1974; Bidelman+ 1973)"], "keyword_cds": "", "keyword_pub": "", "mission": "", "doi_pub": ["10.1086/111475"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "bidmac.dat", "desc": "The catalog of stars of astrophysical interest in the southern sky (Tables III to X)", "columns": [{"name": "Name", "desc": "Star name (1) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[UTMG] Source of position "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "SpType", "desc": "MK spectral type "}, {"name": "Remarks", "desc": "Remartks and notes by B. Skiff "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_79_107"}} {"id": "J/AJ/79/107", "title_cds": "Positions and Identifications in Stock 2", "title_create": "Mccuskey+, 1974", "year": "1974", "author": "Mccuskey S.W.", "title_pub": "The space density of A stars in a region in Cassiopeia.", "first_author": "Mccuskey S.W.", "ref_biblio": [""], "bibcode": ["1974AJ.....79..107M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "description": ["This list shows accarute coordinates and identifications for about 440", "stars in the region of the open cluster Stock 2 observed by McCuskey.", "Many of the stars are present in SIMBAD only by name, lacking", "coordinates altogether. I used the published charts in combination", "with computer screen-plots of stars to get coordinates in addition to", "VizieR and SIMBAD.", "The table shows the names, coordinates (nearly all from Tycho-2),", "Tycho-2 numbers, plus HD, BD, and AGK numbers as available. Many of", "the BD names were omitted by McCuskey. I copy McCuskey's photographic", "V magnitudes rounded to 0.1-mag precision---rms scatter is ~0.2 mag", "despite the claims in the text. Finally his spectral types, which", "appear to be reliable. The remarks include those given by McCuskey as", "well as descriptions of of double stars etc.", "There is much overlap in this region with spectral surveys by the", "Marseilles group, the Kiev group, Brodskaya, Stock's original cluster", "paper, and others. A few stars are included that are in the region of", "clusters besides Stock 2: NGC 743, Markarian 6, and IC 1805, among", "those I noticed.", "Additional photoelectric photometry and slit-spectra for many of the", "same stars are given in the companion paper by Pesch & McCuskey", "(1974AJ.....79..16P)."], "curator": "Francois Ochsenbein [CDS]", "alias": ["[M74]"], "doi_pub": ["10.1086/111537"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_80_208"}} {"id": "J/AJ/80/208", "title_cds": "Souther Stars embedded in nebulosity", "title_create": "van den Bergh+, 1975", "year": "1975", "author": "van den Bergh S., Herbst W.", "title_pub": "Catalogue of southern stars embedded in nebulosity.", "first_author": "van den Bergh S.", "ref_biblio": [""], "bibcode": ["1975AJ.....80..208V"], "see_also": ["VII/21 : Catalogue of Reflection Nebulae (Van den Bergh, 1966)"], "keyword_cds": "Nebulae ; Milky Way", "description": ["A survey of the Milky Way southward of the Palomar Sky Survey for the", "identification of reflection nebulae was carried out at the Cerro", "Tololo Inter-American Observatory in Chile. Plates in blue light were", "obtained at the Curtis Schmidt telescope covering a strip of plus or", "minus six degrees of the galactic equator. Red sensitive plates for", "comparison were also obtained with the same telescope covering the", "same area near the galactic plane. Observatory staff members and some", "students of the University of Toronto, Canada assisted in identifying", "stars embedded in nebulosity as shown by the plates. Although this", "catalogue roughly complements the Catalogue of Reflection Nebulae of", "van den Berg (1966AJ.....71..990V, Cat. ), the region here", "surveyed is more narrowly confined to the galactic equator."], "alias": ["VDBH", "BHe"], "doi_pub": ["10.1086/111733"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "bhe.dat", "desc": "The Catalogue (Table I of publication) ", "columns": [{"name": "BHe", "desc": "BHe id number and components as (a, b, c) "}, {"name": "IDs", "desc": "Alternate designation "}, {"name": "RAh", "desc": "Right Ascension B1950 (hours) "}, {"name": "RAm", "desc": "Right Ascension B1950 (minutes) "}, {"name": "DE-", "desc": "Declination B1950 (sign) "}, {"name": "DEd", "desc": "Declination B1950 (degrees) "}, {"name": "DEm", "desc": "Declination B1950 (minutes) "}, {"name": "Type", "desc": "Type of nebula, see Note (1) "}, {"name": "u_Type", "desc": "Uncertainty flag (:) on Type "}, {"name": "SurfBr", "desc": "Surface brightness from blue plates, Note (2) "}, {"name": "u_SurfBr", "desc": "Uncertainty flag (:) on SurfBr "}, {"name": "Color", "desc": "Coded reference to colors, see Note (3) "}, {"name": "u_Color", "desc": "Uncertainty flag (:) on Color "}, {"name": "Absorb", "desc": "Absorption in field of nebula, see Note (4) "}, {"name": "u_Absorb", "desc": "Uncertainty flag (:) on Absorb "}, {"name": "BDiaMax", "desc": "? Maximum diameter observed on blue plates "}, {"name": "u_BDiaMax", "desc": "Uncertainty flag (:) on BDiaMax "}, {"name": "RDiaMax", "desc": "? Maximum diameter observed on red plates "}, {"name": "u_RDiaMax", "desc": "Uncertainty flag (:) on RDiaMax "}, {"name": "Rem", "desc": "Note flag (*) detailed in file \"notes.dat\" "}]}, {"name": "notes.dat", "desc": "Full notes of publication for Table I ", "columns": [{"name": "BHe", "desc": "BHe id descriptor, repeated if several lines "}, {"name": "Text", "desc": "Text of note "}, {"name": "Flag", "desc": "'*' if note continues on next line "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_81_350"}} {"id": "J/AJ/81/350", "title_cds": "Dwarf late-type stars in the NGP", "title_create": "Sanduleak+, 1976", "year": "1976", "author": "Sanduleak N.", "title_pub": "Catalog of probable dwarf stars of type M3 and later in the direction of the North Galactic Pole.", "first_author": "Sanduleak N.", "ref_biblio": [""], "bibcode": ["1976AJ.....81..350S"], "keyword_cds": "Stars, late-type ; Galactic pole, north", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/111894"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_82_345"}} {"id": "J/AJ/82/345", "title_cds": "OB stars in the Coalsack region", "title_create": "Muzzio+, 1977", "year": "1977", "author": "Muzzio J.C., Orsatti A.M.", "title_pub": "Searches for faint OB stars in the Southern Milky Way. I. The Coalsack region.", "first_author": "Muzzio J.C.", "ref_biblio": [""], "bibcode": ["1977AJ.....82..345M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/112056"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_82_474"}} {"id": "J/AJ/82/474", "title_cds": "OB stars in the Vela region", "title_create": "Muzzio+, 1977", "year": "1977", "author": "Muzzio J.C., Orsatti A.M.", "title_pub": "Searches for faint OB stars in the Southern Milky Way. II. The Vela region.", "first_author": "Muzzio J.C.", "ref_biblio": [""], "bibcode": ["1977AJ.....82..474M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/112076"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_90_418"}} {"id": "J/AJ/90/418", "title_cds": "Galaxies redshifts", "title_create": "Koo+, 1985", "year": "1985", "author": "Koo D.C.", "title_pub": "Optical multicolors : a poor person's z machine for galaxies.", "first_author": "Koo D.C.", "ref_biblio": [""], "bibcode": ["1985AJ.....90..418K"], "keyword_cds": "Redshifts ; Galaxies, photometry", "abstract": ["We explore the feasibility, limits, accuracy, and uncertainties of", "using optical broadband colors in the form of twocolor plots to", "measure the redshifts of faint galaxies. Comparison of redshifts from", "slit spectra and 4-m photographic UBVI photometry of 100 faint", "galaxies confirms that colors do yield redshifts. These galaxies of", "17-23mag in B span a wide range of intrinsic color and are thus", "unlike previous samples of faint galaxies that were largely radio or", "cluster galaxies of early (red) type. For redshifts less than 0.35,", "two-thirds of the color redshifts agree with the spectroscopic values", "to within +/-0.04 in z; for higher redshifts to z of 0.6, the errors", "increase to +/-0.06. These accuracies were achieved for blue as well", "as red galaxies, and ensure that multicolors-can serve as a poor", "person's redshift machine to study distant galaxies in clusters and", "the field."], "doi_pub": ["10.1086/113748"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table4.dat", "desc": "Redshifts and multicolor photometry ", "columns": [{"name": "Seq", "desc": "[1/116]+ Sequential number "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "zUF", "desc": "Redshift determined from UF plots "}, {"name": "zUJFN", "desc": "? Redshift determined from UJFN plots "}, {"name": "J+mag", "desc": "J^+^ magnitude (1) "}, {"name": "U+-J+", "desc": "U^+^-J^+^ colour index (1) "}, {"name": "J+-F+", "desc": "J^+^-F^+^ colour index (1) "}, {"name": "F+-N+", "desc": "? F^+^-N^+^ colour index (1) "}, {"name": "Set", "desc": "Set number "}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "Group", "desc": "Group (I, II or III) "}, {"name": "Seq", "desc": "Sequential number "}, {"name": "Note", "desc": "Text of the note (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_91_530"}} {"id": "J/AJ/91/530", "title_cds": "BV photometry of faint galaxies", "title_create": "Peterson+, 1986", "year": "1986", "author": "Peterson C.J., Baumgart C.W.", "title_pub": "Blue and visual photometry of the Rubin et al. (1976) sample of faint galaxies", "first_author": "Peterson C.J.", "ref_biblio": [""], "bibcode": ["1986AJ.....91..530P"], "keyword_cds": "Galaxies, photometry ; Photometry, UBV", "abstract": ["Blue and visual multiaperture photoelectric photometry of 112 faint", "spiral galaxies from the list of Rubin et al. (1976AJ.....81..687R) is", "presented. We briefly compare total galaxy magnitudes [for an", "aperture/diameter ratio of 1.0 according to the precepts of Graham", "(1976AJ.....81..681G)] with the photographic magnitudes of the Zwicky", "et al. (1961-1968, Cat. ) Catalogue of Galaxies and Clusters of", "Galaxies. From a reanalysis for the motion of the Local Group, we find", "that use of the new galaxy magnitudes increases the difference between", "the motion vector derived from Rubin et al. and the motions derived", "from other sample galaxies and that implied by the anisotropy of the", "cosmic background radiation."], "doi_pub": ["10.1086/114032"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Kitt Peak photoelectric BV photometry of Rubin et al. (1976AJ.....81..687R) Sc I galaxies", "columns": [{"name": "Galaxy", "desc": "Galaxy designation (1) "}, {"name": "Vmag0.46", "desc": "? V magnitude over circular area of 0.46' "}, {"name": "u_Vmag0.46", "desc": "Uncertainty flag on Vmag0.46 "}, {"name": "Vmag0.94", "desc": "? V magnitude over circular area of 0.94' "}, {"name": "u_Vmag0.94", "desc": "Uncertainty flag on Vmag0.94 "}, {"name": "n_Vmag0.94", "desc": "[*] Note on Vmag0.94 (2) "}, {"name": "Vmag1.39", "desc": "? V magnitude over circular area of 1.39' "}, {"name": "u_Vmag1.39", "desc": "Uncertainty flag on Vmag1.39 "}, {"name": "n_Vmag1.39", "desc": "[*] Note on Vmag1.39 (2) "}, {"name": "Vmag1.87", "desc": "? V magnitude over circular area of 1.87' "}, {"name": "u_Vmag1.87", "desc": "Uncertainty flag on Vmag1.87 "}, {"name": "n_Vmag1.87", "desc": "[*] Note on Vmag1.87 (2) "}, {"name": "B-V0.46", "desc": "? B-V colour index over circular area of 0.46' "}, {"name": "u_B-V0.46", "desc": "Uncertainty flag on B-V0.46 "}, {"name": "B-V0.94", "desc": "? B-V colour index over circular area of 0.94' "}, {"name": "u_B-V0.94", "desc": "Uncertainty flag on B-V0.94 "}, {"name": "n_B-V0.94", "desc": "[*] Note on B-V0.94 (2) "}, {"name": "B-V1.39", "desc": "? B-V colour index over circular area of 1.39' "}, {"name": "u_B-V1.39", "desc": "Uncertainty flag on B-V1.39 "}, {"name": "n_B-V1.39", "desc": "[*] Note on B-V1.39 (2) "}, {"name": "B-V1.87", "desc": "? B-V colour index over circular area of 1.87' "}, {"name": "u_B-V1.87", "desc": "Uncertainty flag on B-V1.87 "}, {"name": "n_B-V1.87", "desc": "[*] Note on B-V1.87 (2) "}, {"name": "Nnights", "desc": "Number of separate nights on which the galaxy was observed"}, {"name": "Notes", "desc": "[G1234567] Notes (3) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_94_106"}} {"id": "J/AJ/94/106", "title_cds": "H{alpha} survey of rho Oph complex", "title_create": "Wilking+, 1987", "year": "1987", "author": "Wilking B.A., Schwartz R.D., Blackwell J.H.", "title_pub": "An H-alpha emission-line survey of the rho Ophiuchi dark cloud complex.", "first_author": "Wilking B.A.", "ref_biblio": [""], "bibcode": ["1987AJ.....94..106W"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/114452"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_95_739"}} {"id": "J/AJ/95/739", "title_cds": "Early-G dwarf stars towards SGP", "title_create": "Corbally+, 1988", "year": "1988", "author": "Corbally C.J., Garrison R.F.", "title_pub": "A search for early-G dwarf stars towards the South Galactic Pole.", "first_author": "Corbally C.J.", "ref_biblio": [""], "bibcode": ["1988AJ.....95..739C"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/114671"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_95_745"}} {"id": "J/AJ/95/745", "title_cds": "G dwarf stars at NGP", "title_create": "Corbally+, 1988", "year": "1988", "author": "Corbally C.J., Garrison R.F.", "title_pub": "A search for early-G dwarf stars the North Galactic Pole.", "first_author": "Corbally C.J.", "ref_biblio": [""], "bibcode": ["1988AJ.....95..745C"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/114672"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_99_1488"}} {"id": "J/AJ/99/1488", "title_cds": "UBVRI sequences in the Magellanic Clouds", "title_create": "Alcaino+, 1990", "year": "1990", "author": "Alcaino G., Alvarado F., Wenderoth E., Liller W.", "title_pub": "Photoelectric UBVRI sequences in the Magellanic Cloud clusters Lindsay 1, NGC 339, NGC 361, and NGC 1466.", "first_author": "Alcaino G.", "ref_biblio": [""], "bibcode": ["1990AJ.....99.1488A"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/115433"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_99_1501"}} {"id": "J/AJ/99/1501", "title_cds": "UBVRI sequences in globulars", "title_create": "Alvarado+, 1990", "year": "1990", "author": "Alvarado F., Wenderoth E., Alcaino G., Liller W.", "title_pub": "Photoelectric UBVRI sequences in the galactic globular clusters NGC 6752 and NGC 6864.", "first_author": "Alvarado F.", "ref_biblio": [""], "bibcode": ["1990AJ.....99.1501A"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/115435"], "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_159_27"}} {"id": "J/AJ/159/27", "title_cds": "LCs of the Manwe-Thorondor eclipsing system", "title_create": "Rabinowitz+, 2020", "year": "2020", "author": "Rabinowitz D.L., Benecchi S.D., Grundy W.M., Verbiscer A.J., Thirouin A.", "title_pub": "The complex rotational light curve of (385446) Manwe-Thorondor, a multicomponent eclipsing system in the Kuiper Belt.", "first_author": "Rabinowitz D.L.", "ref_biblio": [""], "bibcode": ["2020AJ....159...27R"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "B/astorb : Orbits of Minor Planets (Bowell+, 2014)", "J/A+A/380/347 : BVRI photometry of 27 Kuiper Belt Objects (Delsanti+, 2001)", "J/A+A/407/1139 : RVB photometry Kuiper-Belt obj. 1999 TD10 (Rousselot+, 2003)", "J/AJ/127/3023 : R magnitudes Kuiper Belt object 2001QG298 (Sheppard+, 2004)", "J/AJ/135/55 : NIR spectra Centaurs & Kuiper Belt objects (Barkume+, 2008)", "J/A+A/509/A94 : Lightcurves of 14 NEAs (Kwiatkowski+, 2010)", "J/A+A/511/A49 : Lightcurves of 12 NEAs (Kwiatkowski+, 2010)", "J/ApJ/720/1691 : Observations of the distant Kuiper belt (Schwamb+, 2010)", "J/A+A/546/A86 : R absolute magnitudes Kuiper Belt objects (Peixinho+, 2012)", "J/ApJ/749/10 : SDSS observations of Kuiper belt objects (Ofek, 2012)", "J/A+A/556/A8 : 100 asteroids rotational parameters (Lhotka+, 2013)", "J/A+A/562/A48 : Light curves of asteroid (25143) Itokawa (Lowry+, 2014)", "J/ApJS/227/20 : Rotation periods of asteroids using iPTF (Chang+, 2016)", "J/AJ/154/62 : Orbital parameters of Kuiper Belt objects (Volk+, 2017)", "J/AJ/154/241 : Photometry Kuiper Belt object: 2002 CC249 (Thirouin+, 2017)", "J/A+A/627/A172 : Near-Earth asteroid (1917) Cuyo opt. & IR obs. (Rozek+,2019)", "J/AJ/157/228 : Cold Classical TNOs LCs & rot. properties (Thirouin+,2019)"], "keyword_cds": "Minor planets; Solar system; Photometry, ugriz; Magnitudes, absolute", "keyword_pub": "Kuiper belt ; Light curves ; Small solar system bodies", "abstract": ["Kuiper Belt Object (385446) Manwe-Thorondor is a multiobject system", "with mutual events predicted to occur from 2014 to 2019. To detect the", "events, we observed the system at 4 epochs (UT 2016 August 25 and 26,", "2017 July 22 and 25, 2017 November 9, and 2018 October 6) in g, r, and", "VR bands using the 4m SOAR and the 8.1m Gemini South telescopes at", "Cerro Pachon, Chile, and Lowell Observatory's 4.3m Discovery Channel", "Telescope at Happy Jack, Arizona. These dates overlap the uncertainty", "range ({+/-}0.5 day) for four inferior events (Thorondor eclipsing", "Manwe). We clearly observe variability for the unresolved system with", "a double-peaked period 11.88190{+/-}0.00005hr and ~0.5mag amplitude", "together with much longer-term variability. Using a multicomponent", "model, we simultaneously fit our observations and earlier photometry", "measured separately for Manwe and Thorondor with the Hubble Space", "Telescope. Our fit suggests Manwe is bilobed, close to the \"barbell\"", "shape expected for a strengthless body with density ~0.8g/cm^3^ in", "hydrostatic equilibrium. For Manwe, we thereby derive maximum width to", "length ratio ~0.30, surface area equivalent to a sphere of diameter", "190km, geometric albedo 0.06, mass 1.4x1018kg, and spin axis oriented", "~75deg from Earth's line of sight. Changes in Thorondor's brightness", "by ~0.6mag with a ~300day period may account for the system's", "long-term variability. Mutual events with unexpectedly shallow depth", "and short duration may account for residuals to the fit. The system is", "complex, providing a challenging puzzle for future modeling efforts."], "description": ["The epoch 1 observations reported here were obtained in the Sloan", "Digital Sky Survey (SDSS) r and g bands on two consecutive nights", "(2016 August 25 and 26 UT) using the SOAR Optical Imager on the 4m", "SOAR telescope at Cerro Pachon, Chile. The imager pixel scale was", "0.154\".", "The epoch 2 observations were obtained in SDSS r and g bands on 2017", "July 22 and 25 UT using the GMOS-S imager on the 8.1m Gemini South", "telescope at Cerro Pachon, Chile. The imager pixel scale was 0.16\".", "The epoch 3 observations were obtained on 2017 November 9 UT in r band", "using the Large Monolithic Imager (LMI) on Lowell Observatory's", "Discovery Channel Telescope (DCT) at Happy Jack AZ. The LMI pixel", "scale was 0.24\".", "The epoch 4 observations were obtained on 2018 October 6 UT in a wide", "VR band, again using the LMI on the DCT.", "Table2 lists the observing circumstances for each epoch.", "Table 4 lists resolved photometry of Manwe and Thorondor previously", "obtained with the HST Wide-Field Planetary Camera2 (WFPC2) in the", "F606W band at seven different epochs from 2007 to 2013.", "Grundy+ (2014Icar..237....1G) report magnitudes for Manwe and", "Thorondor derived from these data after transforming F606W to V band", "and averaging the results from each epoch. Here we present the", "measurements without transformation or averaging."], "type": ["OC"], "doi_pub": ["10.3847/1538-3881/ab59d4"], "data": "f-v", "date_creation": "30-Mar-2020", "last_update": "16-Apr-2020", "catid": "51590027", "date_update": "18-Oct-2022", "tables": [{"name": "table1.dat", "desc": "*Binary orbital parameters for Manwe-Thorondor ", "columns": [{"name": "Per", "desc": "Manwe-Thorondor orbital period "}, {"name": "e_Per", "desc": "Error on Per "}, {"name": "a", "desc": "Manwe-Thorondor semi-major axis "}, {"name": "e_a", "desc": "Error on a "}, {"name": "e", "desc": "Manwe-Thorondor eccentricity "}, {"name": "e_e", "desc": "Error on e "}, {"name": "Msys", "desc": "System mass "}, {"name": "e_Msys", "desc": "Error on M "}, {"name": "inc", "desc": "Manwe-Thorondor inclination "}, {"name": "e_inc", "desc": "Error on inc "}, {"name": "Omega", "desc": "Manwe-Thorondor ascending node "}, {"name": "e_Omega", "desc": "Error on Omega "}]}, {"name": "table2.dat", "desc": "Observing circumstances ", "columns": [{"name": "Epoch", "desc": "[1/4] Epoch number "}, {"name": "Date", "desc": "UT observation date "}, {"name": "Tel", "desc": "Telescope used: DCT, Gemini and SOAR, 2 occurrences for each"}, {"name": "Filt", "desc": "Filter used: VR 1 occurrences, g 4 occurrences and r 5 occurrences"}, {"name": "Obs.start", "desc": "UT start time of the observation "}, {"name": "Obs.end", "desc": "UT end time of the observation "}, {"name": "Midpt", "desc": "UT event midpoint (1) "}, {"name": "Depth", "desc": "[0.05/0.66]? Event depth (1) "}, {"name": "theta", "desc": "[0.4/1.1] Solar phase angle ({Theta}) "}, {"name": "rhel", "desc": "[43.4/43.7] Heliocentric distance (r_hel_) "}, {"name": "rgeo", "desc": "[42/43] Geocentric distance (r_geo_) "}]}, {"name": "table3.dat", "desc": "Photometric observations of Manwe-Thorondor ", "columns": [{"name": "Tel", "desc": "Telescope used (1) "}, {"name": "JD", "desc": "[7625/8398] Julian Date of observation, JD-2450000 "}, {"name": "Filt", "desc": "Filter used: \"VR\" 34 occurrences, \"g\" 43 occurrences or \"r\" 148 occurrences"}, {"name": "omag", "desc": "[21.7/24.6] Observed magnitude in Filt "}, {"name": "e_omag", "desc": "[0.02/0.25] Uncertainty in omag "}, {"name": "Exp", "desc": "[150/600] Exposure time "}, {"name": "O-C", "desc": "[-0.28/0.31] Fit Residuals "}]}, {"name": "table4.dat", "desc": "F606W-band photometry of Manwe-Thorondor with HST ", "columns": [{"name": "Obs.Y", "desc": "[2007/2013] Year of observation, UT "}, {"name": "Obs.M", "desc": "Month of observation, UT "}, {"name": "Obs.D", "desc": "[4/26] Day of observation, UT "}, {"name": "JD", "desc": "[4306/6618] Julian date of observation, JD-2450000"}, {"name": "Mmag", "desc": "[23.2/24.1] Manwe HST/WFPC2 F606W magnitude "}, {"name": "f_Mmag", "desc": "[*] *: rejected measurement "}, {"name": "e_Mmag", "desc": "[0.05/0.11] Uncertainty in Mmag "}, {"name": "Tmag", "desc": "[24.2/26.1]? Thorondor HST/WFPC2 F606W magnitude "}, {"name": "f_Tmag", "desc": "[*] *: rejected measurement "}, {"name": "e_Tmag", "desc": "[0.05/0.69]? Uncertainty in Tmag "}, {"name": "M*mag", "desc": "[22.9/23.5] Pseudo magnitude for Manwe+Thorondor (1)"}, {"name": "f_M*mag", "desc": "[*] *: rejected measurement "}, {"name": "theta", "desc": "[0.08/1.21] Solar phase angle of the Manwe/Thorondor system ({Theta})"}, {"name": "Sep", "desc": "[0.03/0.33] Separation ({Delta}) "}]}, {"name": "table6.dat", "desc": "Multicomponent model parameters ", "columns": [{"name": "DiamM", "desc": "Diameter of sphere with equivalent area as Manwe"}, {"name": "DiamMVol", "desc": "Diameter of sphere with equivalent volume as Manwe"}, {"name": "DiamT", "desc": "Diameter of Thorondor "}, {"name": "MM", "desc": "Mass of Manwe "}, {"name": "MT/MM", "desc": "Upper limit to Thorondor/Manwe mass ratio (1) "}, {"name": "pM", "desc": "Albedo of Manwe "}, {"name": "pT", "desc": "Albedo of Thorondor "}, {"name": "beta", "desc": "Linear dependence on solar phase angle ({beta}) "}, {"name": "PerM", "desc": "Rotation period of Manwe "}, {"name": "t1", "desc": "Reference Julian date for absolute magnitudes "}, {"name": "rho", "desc": "Average density of the Manwe/Thorondor system ({rho})"}, {"name": "epsT", "desc": "Julian date of minimum brightness for Thorondor ({epsilon}_T_)"}, {"name": "OmegaM", "desc": "Ascending node of Manwe's equator ({Omega}) (2) "}, {"name": "incM", "desc": "Inclination of Manwe's equator (2) "}, {"name": "RotM", "desc": "Rotation angle of Manwe's long axis ({mu}) (3) "}, {"name": "aM", "desc": "Average angle between Manwe's spin and Manwe-Earth direction (<{alpha}_M_>)"}, {"name": "PerT", "desc": "Rotation period of Thorondor (single-peaked) "}, {"name": "AmpT", "desc": "Light-curve amplitude of Thorondor (peak-to-peak)"}, {"name": "gMAG", "desc": "Absolute g-band magnitude of Manwe/Thorondor (H_g_) at epoch t1"}, {"name": "rMAG", "desc": "Absolute r-band magnitude of Manwe/Thorondor (H_r_) at epoch t1"}, {"name": "MMAG", "desc": "Absolute F606W-band magnitude of Manwe (H_M_) at epoch t1"}, {"name": "TMAG", "desc": "Absolute F606W-band magnitude of Thorondor (H_T_) at epoch t1"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_159_28"}} {"id": "J/AJ/159/28", "title_cds": "Short Title", "title_create": "Abushattal+, 2020", "year": "2020", "author": "Abushattal A.A., Docobo J.A., Campo P.P.", "title_pub": "The most probable 3D orbit for spectroscopic binaries.", "first_author": "Abushattal A.A.", "ref_biblio": [""], "bibcode": ["2020AJ....159...28A"], "keyword_cds": "", "keyword_pub": "Binary stars; Spectroscopic binary stars; Visual binary stars Fundamental parameters of stars", "mission": "", "abstract": ["Binary stars are a very important source of astronomical information. Those short-period binaries observed by means of both spectroscopy and interferometry can provide, through their corresponding orbits, precise values regarding individual masses as well as orbital parallaxes. For this reason, it is fundamental to attempt to optically resolve double-lined spectroscopic binaries. In the present article, we used the elaboration of a specific algorithm in order to determine the necessary telescope aperture to resolve a concrete spectroscopic binary. To that end, using available photometric and spectroscopic information, we established a 3D model for each spectroscopic binary with an orbit from which we deduced the most probable maximum and minimum separations between the components. In this manner, using the obtained calibrations in our study, we also deduced different physical parameters of the components of each system. The methodology presented here was tested satisfactorily with a list of spectroscopic binaries that had been optically resolved and that have both the spectroscopic and visual orbits."], "object": [], "curator": "Coralie Fix [CDS]", "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_159_217"}} {"id": "J/AJ/159/217", "title_cds": "Simulation of Nodal precession in planet pairs", "title_create": "Bailey+, 2020", "year": "2020", "author": "Bailey N., Fabrycky D.", "title_pub": "Nodal precession in closely spaced planet pairs.", "first_author": "Bailey N.", "ref_biblio": [""], "bibcode": ["2020AJ....159..217B"], "see_also": ["J/ApJS/208/22 : Transit timing variation for 12 planetary pairs (Xie, 2013)", "J/ApJ/790/146 : Planets in Kepler's multi-transiting systems (Fabrycky+, 2014)", "J/ApJS/210/25 : Transit timing variation 15 planetary pairs. II. (Xie, 2014)", "J/A+A/573/A124 : Kepler-117 (KOI-209) transit-timing variations (Bruno+, 2015)", "J/MNRAS/448/1044 : Simulation data 50 planetary model systems (Hansen+, 2015)"], "keyword_cds": "Exoplanets; Models; Binaries, orbits", "keyword_pub": "Analytical mathematics ; Ascending node ; Celestial mechanics ; Exoplanet systems ; Exoplanet dynamics ; N-body simulations ; Orbits ; Three-body problem", "abstract": ["Planet-planet perturbations can cause planet's orbital elements to", "change on secular timescales. Previous work has evaluated the nodal", "precession rate for planets in the limit of low {alpha} (semimajor", "axis ratio; 0<{alpha}<=1). Our simulations show that systems at high", "{alpha} (or low period ratio), similar to multiplanet systems found in", "the Kepler survey, have a nodal precession rate that is more strongly", "dependent on eccentricity and inclination. We present a complete", "expansion of the nodal precession rate to fourth order in the", "disturbing function and show that this analytical solution much better", "describes the simulated N-body behavior of high-{alpha} planet pairs;", "at {alpha}~0.5, the higher-order solution, on average, reduces the", "median analytical error by a factor of 7.5 from linear theory and 6.2", "from a similar expansion assuming low {alpha}. We set limits on", "eccentricity and inclination where the theory is precisely validated", "by N-body integrations, which can be useful in future secular", "treatments of planetary systems."], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "tableB1.dat", "desc": "Restricted Simulations Data ", "columns": [{"name": "Per-b", "desc": "[3.4834] Inner planet period "}, {"name": "Per-c", "desc": "[6.16/174.2] Outer planet period "}, {"name": "/Per", "desc": "[1.77/50] Period ratio "}, {"name": "e-b0", "desc": "[2.09E-16/0.07] Inner planet initial eccentricity"}, {"name": "e-c0", "desc": "[0/0.1] Outer planet initial eccentricity "}, {"name": "i-b0", "desc": "[0] Inner planet initial inclination "}, {"name": "i-c0", "desc": "[0.008/0.42] Outer planet initial inclination "}, {"name": "omega-b0", "desc": "[0.827767955] Inner planet initial argument of pericenter ({omega}_1.0_})"}, {"name": "omega-c0", "desc": "[1.0943632214] Outer planet initial argument of pericenter ({omega}_2.0_})"}, {"name": "Pern-c", "desc": "[106185/966743333] Outer planet nodal precession period fitted from simulation"}, {"name": "e_Pern-c", "desc": "[0.002/45] Standard deviation in Pern-c "}, {"name": "Texp", "desc": "[107270/17417020] Time period used to fit nodal precession period (1)"}, {"name": "Tsim", "desc": "[107270/17417020] Total time simulated "}, {"name": "Per-LL", "desc": "[211025/961145944] Analytical nodal precession period from Laplace-Lagrange linear theory"}, {"name": "Per-2nd", "desc": "[120427/966445072] Analytical nodal precession period from 2nd order expansion"}, {"name": "Per-4th", "desc": "[107816/966631850] Analytical nodal precession period from 4th order expansion"}, {"name": "figs", "desc": "? Figures where this data appears "}]}, {"name": "tableB2.dat", "desc": "Unrestricted Simulations Data ", "columns": [{"name": "Per-b", "desc": "[6.2448] Inner planet period "}, {"name": "Per-c", "desc": "[11.05/312.3] Outer planet period "}, {"name": "/Per", "desc": "[1.77/50] Period ratio "}, {"name": "e-b0", "desc": "[2.95E-7/0.9] Inner planet initial eccentricity "}, {"name": "e-c0", "desc": "[3E-7/0.9] Outer planet initial eccentricity "}, {"name": "i-b0", "desc": "[0.004/0.42] Inner planet initial inclination "}, {"name": "i-c0", "desc": "[0.001/0.23] Outer planet initial inclination "}, {"name": "omega-b0", "desc": "[-3.08/3.1] Inner planet initial argument of pericenter"}, {"name": "omega-c0", "desc": "[-1.49/2.99] Outer planet initial argument of pericenter"}, {"name": "Pern-b", "desc": "[100004/999564] Inner planet nodal precession period fitted from simulation"}, {"name": "e_Pern-b", "desc": "[0.002/999] Standard deviation in Pern-b "}, {"name": "Pern-c", "desc": "[100004/999586] Outer planet nodal precession period fitted from simulation"}, {"name": "e_Pern-c", "desc": "[0.002/993] Standard deviation in pern-c "}, {"name": "Texp", "desc": "[24.9/2547874657] Time period used to fit nodal precession period (1)"}, {"name": "Tsim", "desc": "[1105326/2547874657] Total time simulated "}, {"name": "Per-LL", "desc": "[141883/520413421] Analytical nodal precession0 period from Laplace-Lagrange linear theory"}, {"name": "Per-2nd", "desc": "[54154/600384597] Analytical nodal precession period from 2nd order expansion"}, {"name": "Per-4th", "desc": "[1696/612881431] Analytical nodal precession period from 4th order expansion"}, {"name": "figs", "desc": "? Figures where this data appears "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_160_57"}} {"id": "J/AJ/160/57", "title_cds": "IR spectra of planetary-mass brown dwarfs in IC 348", "title_create": "Luhman+, 2020", "year": "2020", "author": "Luhman+, Luhman K.L., Hapich C.J.", "title_pub": "New candidates for planetary-mass brown dwarfs in IC 348.", "first_author": "Luhman+", "ref_biblio": [""], "bibcode": ["2020AJ....160...57L"], "see_also": ["II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "II/314 : UKIDSS-DR8 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "J/A+A/337/403 : Low-mass stars evolutionary models (Baraffe+ 1998)", "J/ApJ/541/977 : HST observations of low-mass stars in IC 348 (Najita+, 2000)", "J/ApJ/593/1093 : IC 348 membership (Luhman+, 2003)", "J/ApJ/597/555 : IR photometry of IC 348 young brown dwarfs (Mainzer+, 2003)", "J/MNRAS/434/806 : Pre-main-sequence isochrones. II. SFR (Bell+, 2013)", "J/ApJ/810/158 : M,L,T dwarfs fundamental parameters & SEDs (Filippazzo+,2015)", "J/AJ/154/134 : Planetary-mass brown dwarfs in the Taurus SFR (Esplin+, 2017)", "J/AJ/154/46 : Proper motions and photo. for members of Cha I (Esplin+,2017)", "J/AJ/153/46 : Spectroscopy of candidate members in Taurus (Luhman+, 2017)", "J/ApJ/865/73 : GOBELINS. V. Kinematics of Perseus (Ortiz-Leon+, 2018)", "J/AJ/158/54 : Taurus memb. from stellar to planetary masses (Esplin+, 2019)"], "keyword_cds": "Clusters, open; Star Forming Region; Stars, brown dwarf; Spectra, infrared; Spectral types", "keyword_pub": "Brown dwarfs ; Star-forming regions ; Initial mass function ; Hubble Space Telescope", "abstract": ["We have used infrared images obtained with the Wide Field Camera 3 on", "board the Hubble Space Telescope to search for planetary-mass brown", "dwarfs in the star-forming cluster IC348. In those images, we have", "identified 12 objects that have colors indicative of spectral types", "later than M8, corresponding to masses of <~30MJup at the age of", "IC348. The four brightest candidates have been observed with", "spectroscopy, all of which are confirmed to have late types. Two of", "those candidates appear to be young, and thus are likely members of", "the cluster, while the ages and membership of the other two candidates", "are uncertain. One of the former candidates is the faintest known", "member of IC348 in extinction-corrected Ks and is expected to have a", "mass of 4-5MJup based on evolutionary models and an assumed age of", "3Myr. Four of the remaining eight candidates have ground-based", "photometry that further supports their candidacy as brown dwarfs, some", "of which are fainter (and potentially less massive) than the known", "members."], "description": ["IC348 was observed with the IR channel of Hubble's Wide Field Camera 3", "(WFC3) on several dates between 2016 December and 2017 February", "through program 14626 (M. Barsony). The camera contains a 1024x1024", "HgCdTe array in which the pixels have dimensions of ~0.135\"x0.121\".", "The inner 1014x1014 portion of the array detects light, which", "corresponds to a field of view of 136\"x123\".the total exposure times", "were 250 or 275 s for a given field and filter. WFC3 observed 48", "fields through three filters, consisting of F125W (1.1-1.4{mu}m),", "F139M (1.35-1.41{mu}m), and F160W (1.4-1.69{mu}m)."], "type": ["OC"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Candidate members of IC 348 ", "columns": [{"name": "ID", "desc": "IC 348 IRS position-based identifier "}, {"name": "LRL", "desc": "[21460/91235] LRL designation (1) "}, {"name": "SpT", "desc": "Spectral Type "}, {"name": "Ak", "desc": "[0.1/0.2]? K band reddening "}, {"name": "Young?", "desc": "Young according to spectral features? "}, {"name": "m125", "desc": "[18.82/22.13] HST/WFPC3 F125W magnitude "}, {"name": "e_m125", "desc": "[0.02/0.03] Uncertainty in m125 "}, {"name": "m139", "desc": "[18.95/21.62] HST/WFPC3 F139M magnitude "}, {"name": "e_m139", "desc": "[0.02/0.09] Uncertainty in m139 "}, {"name": "m160", "desc": "[18.12/20.94] HST/WFPC3 F160W magnitude "}, {"name": "e_m160", "desc": "[0.02/0.02] Uncertainty in m160 "}, {"name": "Jmag", "desc": "[18.77/21.66]? J band magnitude (2) "}, {"name": "e_Jmag", "desc": "[0.02/0.12]? Uncertainty in Jmag (2) "}, {"name": "Hmag", "desc": "[17.77/20.0]? H band magnitude (2) "}, {"name": "e_Hmag", "desc": "[0.02/0.12]? Uncertainty in Hmag (2) "}, {"name": "Ksmag", "desc": "[16.98/19.09]? Ks band magnitude (2) "}, {"name": "e_Ksmag", "desc": "[0.02/0.06]? Uncertainty in Ksmag (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_160_265"}} {"id": "J/AJ/160/265", "title_cds": "", "title_create": "Hu+, 2020", "year": "2020", "author": "Hu Z., Tak H.", "title_pub": "Modeling stochastic variability in multiband time-series data.", "first_author": "Hu Z.", "ref_biblio": [""], "see_also": ["J/ApJ/698/895 : Variations in QSOs optical flux (Kelly+, 2009)", "J/ApJ/747/107 : QSO Candidates in the MACHO LMC database (Kim+, 2012)", "J/A+A/540/A132 : Optical follow-up of Q0957+561 in 2005-2010 (Shalyapin+, 2012)", "J/ApJ/806/129 : Space telescope RM project. II. Swift data (Edelson+, 2015)"], "keyword_cds": "", "keyword_pub": "Astrostatistics ; Interdisciplinary astronomy ; Astrostatistics tools", "abstract": ["In preparation for the era of time-domain astronomy with upcoming", "large-scale surveys, we propose a state-space representation of a", "multivariate damped random walk process as a tool to analyze", "irregularly-spaced multifilter light curves with heteroscedastic", "measurement errors. We adopt a computationally efficient and scalable", "Kalman filtering approach to evaluate the likelihood function, leading", "to maximum O(k^3^n) complexity, where k is the number of available", "bands and n is the number of unique observation times across the k", "bands. This is a significant computational advantage over a commonly", "used univariate Gaussian process that can stack up all multiband light", "curves in one vector with maximum O(k^3^n^3^) complexity. Using", "such efficient likelihood computation, we provide both maximum", "likelihood estimates and Bayesian posterior samples of the model", "parameters. Three numerical illustrations are presented: (I) analyzing", "simulated five-band light curves for a comparison with independent", "single-band fits; (II) analyzing five-band light curves of a quasar", "obtained from the Sloan Digital Sky Survey Stripe 82 to estimate", "short-term variability and timescale; (III) analyzing gravitationally", "lensed g- and r-band light curves of Q0957+561 to infer the time", "delay. Two R packages, Rdrw and timedelay, are publicly available to", "fit the proposed models."], "object": ["10 01 20.69 +55 53 55.6 QSO0957+561 = 8C 0958+561"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "fig7.dat", "desc": "Light curves of doubly-lensed quasar Q0957+561 ", "columns": [{"name": "Band", "desc": "SDSS band; g or r "}, {"name": "Comp", "desc": "Lensed image component; A or B "}, {"name": "MJD", "desc": "[3443/4249] Modified Julian Date MJD-50000 "}, {"name": "mag", "desc": "[16.8/17.4] Apparent magnitude in Band "}, {"name": "e_mag", "desc": "[8.1E-03/1.6E-02] Uncertainty in mag "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_161_88"}} {"id": "J/AJ/161/88", "title_cds": "Short Title", "title_create": "Popkov+, 2021", "year": "2021", "author": "Popkov A.V., Kovalev Y.Y., Petrov L.Y., Kovalev Y.A.", "title_pub": "Parsec-scale properties of steep and flat-spectrum extragalactic radio sources from a VLBA survey of a complete north polar cap sample.", "first_author": "Popkov A.V.", "ref_biblio": [""], "bibcode": ["2021AJ....161...88P"], "keyword_cds": "", "keyword_pub": "Galaxy jets; Active galactic nuclei; Radio astrometry; Radio astronomy Radio continuum emission; Radio sources Very long baseline interferometry; Radio interferometry", "mission": "", "abstract": ["We observed with the Very Long Baseline Array (VLBA) at 2.3 and 8.6 GHz a complete flux-density-limited sample of 482 radio sources with decl. > +75{deg} brighter than 200 mJy at 1.4 GHz drawn from the NVSS catalog. A total of 34% of the sources show parsec-scale emission above the flux density detection limit of 30 mJy; their accurate positions and parsec-scale structure parameters are determined. Among all the sources detected at least at the shortest VLBA baselines, the majority, or 72%, have a steep single-dish spectrum. The fraction of the sources with a detectable parsec-scale structure is above 95% among the flat-spectrum objects and close to 25% among the steep-spectrum objects. We identified 82 compact steep-spectrum source candidates, which make up 17% of the sample; most of them are reported for the first time. The compactness and the brightness temperature of the sources in our sample show a positive correlation with single-dish and VLBA spectral indices. All the sources with a significant 8 GHz variability were detected by the VLBA snapshot observations, which independently confirmed their compactness. We demonstrated that 54% of the sources detected by the VLBA at 2.3 GHz in our sample have a steep VLBA spectrum. The compact radio emission of these sources is likely dominated by optically thin jets or mini-lobes, not by an opaque jet core. These results show that future VLBI surveys aimed at searching for new sources with parsec-scale structure should include not only flat-spectrum sources but also steep-spectrum ones in order to reach an acceptable level of completeness."], "object": [], "curator": "Coralie Fix [CDS]", "data": "", "date_update": "18-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_161_254"}} {"id": "J/AJ/161/254", "title_cds": "", "title_create": "Smith+, 2021", "year": "2021", "author": "Smith V.V., Bizyaev D., Cunha K., Shetrone M.D., Souto D., Allende Prieto C., Masseron T., Meszaros S., Jonsson H., Hasselquist S., Osorio Y., Garcia-Hernandez D.A., Plez B., Beaton R.L., Holtzman J., Majewski S.R., Stringfellow G.S., Sobeck J.", "title_pub": "The APOGEE Data Release 16 spectral line list.", "first_author": "Smith V.V.", "ref_biblio": [""], "bibcode": ["2021AJ....161..254S"], "see_also": ["III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)", "VI/119 : High accuracy computed water line list - BT2 (Barber+, 2006)", "J/ApJS/95/535 : Infrared CO line list for X 1{Sigma}+ state (Goorvitch, 1994)", "J/A+A/363/1081 : Non-linear limb-darkening law for LTE models (Claret 2000)", "J/A+A/548/A55 : C and O isotopic ratios in Arcturus and Aldebaran (Abia+,2012)", "J/ApJS/214/26 : Line lists for CN isotopes transitions (Sneden+, 2014)", "J/ApJS/221/24 : SDSS-III APOGEE H-band spectral line lists (Shetrone+, 2015)", "J/AJ/151/144 : ASPCAP weights for 15 APOGEE chemical elements (Garcia+, 2016)", "J/ApJ/824/75 : Abundances in 23 open clusters. I. (Overbeek+, 2016)", "J/MNRAS/473/5324 : ExoMol line lists. XXIV. SiH (Yurchenko+, 2018)", "J/MNRAS/480/3397 : ExoMol line lists XXXI: C_2_ (Yurchenko+, 2018)"], "keyword_cds": "", "keyword_pub": "High resolution spectroscopy ; Atomic spectroscopy ; Molecular spectroscopy ; Spectroscopy", "abstract": ["The updated H-band spectral-line list (from {lambda}15000-17000)", "adopted by the Apache Point Observatory Galactic Evolution Experiment", "(APOGEE) for the SDSS-IV Data Release 16 (DR16) is presented in this", "work. The APOGEE line list is a combination of atomic and molecular", "lines, with data drawn from laboratory, theoretical, and astrophysical", "sources. Oscillator strengths and damping constants are adjusted using", "high signal-to-noise, high-resolution spectra of the Sun, and {alpha}Boo (Arcturus), as \"standard stars.\" Updates to the DR16 line list, as", "compared to the previous DR14 version, include the addition of", "molecular H2O and FeH lines, as well as a much larger (by a factor of", "~4) atomic line list, including a significantly greater number of", "transitions with hyperfine splitting. More recent references and line", "lists for the crucial molecules, CO and OH, as well as for C2 and SiH,", "are also included. In contrast to DR14, DR16 contains measurable lines", "from the heavy neutron-capture elements cerium (as CeII), neodymium", "(as NdII), and ytterbium (as YbII), as well as one line from", "rubidium (as RbI), which may be detectable in a small fraction of", "APOGEE red giants."], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table5.dat", "desc": "Global mask to remove regions of the spectra not fit well in Arcturus or the Sun by the line-fitting code", "columns": [{"name": "Wave", "desc": "[15148/16938] Wavelength, air "}, {"name": "Mask", "desc": "[0/1] Mask Value "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_161_256"}} {"id": "J/AJ/161/256", "title_cds": "MYSST. I. HST F555W and F814W obs. of N44 in LMC", "title_create": "Ksoll+, 2021", "year": "2021", "author": "Ksoll V.F., Gouliermis D., Sabbi E., Ryon J.E., Robberto M., Gennaro M., Klessen R.S., Koethe U., De Marchi G., Chen C.-H.R., Cignoni M., Dolphin A.E.", "title_pub": "Measuring Young Stars in Space and Time. I. The photometric catalog and extinction properties of N44.", "first_author": "Ksoll V.F.", "ref_biblio": [""], "bibcode": ["2021AJ....161..256K"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/ApJ/452/210 : UBV photometry in LH 47/48 (Oey+ 1995)", "J/AcA/49/223 : BVI photometry of OGLE LMC Cepheids (Udalski+, 1999)", "J/AcA/49/437 : BVI photometry of OGLE SMC Cepheids (Udalski+, 1999)", "J/AJ/128/1606 : Magellanic Clouds Photometric Survey: the LMC (Zaritsky+, 2004)", "J/ApJ/695/511 : Young massive stars in LHA 120-N 44 (Chen+, 2009)", "J/A+A/530/A115 : Rotating massive MS stars evolutionary models (Brott+, 2011)", "J/ApJ/738/137 : HST VI stars in Shapley Constellation III (Gouliermis+, 2011)", "J/ApJS/197/16 : CO observations of LMC molecular clouds (MAGMA). (Wong+, 2011)", "J/A+A/542/A66 : YSOs in 9 LMC star forming regions (Carlson+, 2012)", "J/ApJ/755/154 : Mass accretion rates from HST in the ONC (Manara+, 2012)", "J/A+A/553/A24 : Models for rotating stars (Georgy+, 2013)", "J/ApJS/207/10 : HST Treasury Program on the ONC (Robberto+, 2013)", "J/ApJS/222/11 : Hubble Tarantula Treasury Project (HTTP). III. (Sabbi+, 2016)", "J/MNRAS/472/1760 : Hierarchical formation of Westerlund 1 (Gennaro+, 2017)", "J/ApJ/854/154 : N159 ^12^CO and ^13^CO (2-1) clumps (Nayak+, 2018)", "J/MNRAS/476/1213 : Ages for stars in 19 clusters (Getman+, 2018)", "http://archive.stsci.edu/hlsp/mysst : MYSST data on MAST"], "keyword_cds": "Photometry, HST; Magellanic Clouds; Star Forming Region; Surveys; Optical", "keyword_pub": "Pre-main sequence stars; Large Magellanic Cloud; Star-forming regions HST photometry; Young star clusters; Low mass stars; Surveys", "abstract": ["In order to better understand the role of high-mass stellar feedback", "in regulating star formation in giant molecular clouds, we carried out", "a Hubble Space Telescope (HST) Treasury Program Measuring Young Stars", "in Space and Time (MYSST) targeting the star-forming complex N44 in", "the Large Magellanic Cloud (LMC). Using the F555W and F814W broadband", "filters of both the ACS and WFC3/UVIS, we built a photometric catalog", "of 461684 stars down to m_F555W_~29mag and m_F814W_~28mag,", "corresponding to the magnitude of an unreddened 1Myr pre-main-sequence", "star of ~0.09M_{sun}_ at the LMC distance. In this first paper we", "describe the observing strategy of MYSST and the data reduction", "procedure and present the photometric catalog. We identify multiple", "young stellar populations tracing the gaseous rim of N44's", "superbubble, together with various contaminants belonging to the LMC", "field population. We also determine the reddening properties from the", "slope of the elongated red clump (RC) feature by applying the", "machine-learning algorithm RANSAC, and we select a set of", "upper-main-sequence stars as primary probes to build an extinction", "map, deriving a relatively modest median extinction A_F555W_~0.77mag.", "The same procedure applied to the RC provides A_F555W_~0.68 mag."], "description": ["The Hubble Space Telescope (HST) Treasury Program Measuring Young", "Stars in Space and Time (MYSST; GO-14689, P.I. Gouliermis) is a deep,", "high spatial resolution HST survey of the star-forming complex N44", "located in the LMC. It covers the large superbubble of N44, as well as", "the region south of it, with a field of view (FOV) of", "12.2x14.7arcmin^2^. The survey provides observations in two broadband", "filters, F555W and F814W, with the Advanced Camera for Surveys (ACS)", "and Wide Field Camera 3 (WFC3, UVIS channel) instruments of HST."], "alias": ["MYSST"], "type": ["OC"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "catalog.dat", "desc": "MYSST photometric catalog ", "columns": [{"name": "---", "desc": "[MYSST] "}, {"name": "MYSST", "desc": "MYSST identifier (HHMMSS.ss+DDMMSS.ss; J2000) "}, {"name": "Xpos", "desc": "[87/28804] Pixel coordinate X in WFC3/UVIS reference image"}, {"name": "Ypos", "desc": "[213/26257] Pixel coordinate Y in WFC3/UVIS reference image"}, {"name": "RAdeg", "desc": "[80.3/81.16] Right ascension (J2000) "}, {"name": "DEdeg", "desc": "[-68.13/-67.84] Declination (J2000) "}, {"name": "Chi2", "desc": "[0.5/19.3] Chi squared PSF fit quality for combined data"}, {"name": "SNR", "desc": "[4/4358] S/N for combined data "}, {"name": "shrp", "desc": "[-0.74/0.34] Sharpness for combined data "}, {"name": "rnd", "desc": "[0/10] Roundness for combined data "}, {"name": "mjaxdir", "desc": "[0/175] Direction of major axis (if not round) for combined data"}, {"name": "crwd", "desc": "[0/2.8] Crowding for combined data "}, {"name": "Type", "desc": "[1] DOLPHOT object type (always \"1\" = bright star)"}, {"name": "F555Wmag", "desc": "[13.94/29.31] HST F555W band magnitude "}, {"name": "e_F555Wmag", "desc": "[0.001/0.22] Uncertainty in F555Wmag "}, {"name": "Chi2F555", "desc": "[0.3/204] {chi}^2^ PSF fit quality for F555W "}, {"name": "SNR555", "desc": "[4.9/1871] Signal-to-noise ratio for F555W "}, {"name": "shrp555", "desc": "[-0.7/0.3] Sharpness for F555W "}, {"name": "rnd555", "desc": "[-1.12/9.16] Roundness for F555W "}, {"name": "crwd555", "desc": "[0/0.25] Crowding for F555W "}, {"name": "q_F555Wmag", "desc": "[0/3] Photometry quality flag for F555Wmag (0=good) (1)"}, {"name": "F814Wmag", "desc": "[13.02/28.2] HST F814W band magnitude "}, {"name": "e_F814Wmag", "desc": "[0.001/0.22] Uncertainty on the F814Wmag "}, {"name": "Chi2F814", "desc": "[0.1/219] {chi}^2^ PSF fit quality for F814W "}, {"name": "SNR814", "desc": "[5/2171] Signal-to-noise ratio for F814W "}, {"name": "shrp814", "desc": "[-0.7/0.3] Sharpness for F814W "}, {"name": "rnd814", "desc": "[-1.85/9.62] Roundness for F814W "}, {"name": "crwd814", "desc": "[0/0.25] Crowding for F814W "}, {"name": "q_F814Wmag", "desc": "[0/3] Photometry quality flag for F814Wmag (0=good) (1)"}, {"name": "Orgn", "desc": "[0/4] Photometry origin flag (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_163_91"}} {"id": "J/AJ/163/91", "title_cds": "", "title_create": "Judkovsky+, 2022", "year": "2022", "author": "Judkovsky Y., Ofir A., Aharonson O.", "title_pub": "Physical Properties and Impact Parameter Variations of Kepler Planets from Analytic Light-curve Modeling.", "first_author": "Judkovsky Y.", "ref_biblio": [""], "bibcode": ["2022AJ....163...91J"], "see_also": ["I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/A+A/363/1081 : Non-linear limb-darkening law for LTE models (Claret 2000)", "J/ApJ/634/625 : Radial velocities and photometry of GJ 876 (Rivera+, 2005)", "J/ApJS/197/8 : Keplers candidate multiple transiting planets (Lissauer+, 2011)", "J/ApJ/750/114 : Kepler TTVs. IV. 4 multiple-planet systems (Fabrycky+, 2012)", "J/MNRAS/421/2342 : 4 Kepler systems transit timing observation (Steffen+, 2012)", "J/A+A/555/A58 : New Kepler planetary candidates (Ofir+, 2013)", "J/ApJ/790/146 : Planets in Kepler's multi-transiting systems (Fabrycky+, 2014)", "J/ApJ/787/80 : 139 Kepler planets transit time variations (Hadden+, 2014)", "J/ApJS/210/20 : Small Kepler planets radial velocities (Marcy+, 2014)", "J/ApJS/210/25 : Transit timing variation for 15 planetary pairs II. (Xie, 2014)", "J/A+A/573/A124 : Kepler-117 (KOI-209) transit-timing variations (Bruno+, 2015)", "J/ApJS/225/9 : Kepler TTVs IX. The full long-cadence data set (Holczer+, 2016)", "J/AJ/154/109 : California-Kepler Survey. III. Planet radii (Fulton+, 2017)", "J/AJ/154/5 : Transit timing variations of 145 Kepler planets (Hadden+, 2017)", "J/A+A/605/A72 : Planetary systems AMD-stability (Laskar+, 2017)", "J/A+A/618/A41 : Photometry of Kepler-9b and c transits (Freudenthal+, 2018)", "J/AJ/156/264 : California-Kepler Survey VII. Planet radius gap (Fulton+, 2018)", "J/ApJS/234/9 : A spectral approach to transit timing variations (Ofir+, 2018)", "J/AJ/155/48 : California-Kepler Survey. V. Masses and radii (Weiss+, 2018)", "J/AJ/157/145 : HIRES RVs of three compact, multiplanet systems (Mills+, 2019)", "J/AJ/159/280 : Gaia-Kepler stellar properties cat.I. KIC stars (Berger+, 2020)", "J/ApJ/890/23 : NUV and FUV measurements of planet host stars (Loyd+, 2020)", "J/AJ/161/246 : Tansit time variations for 12 exoplanets (Jontof-Hutter+, 2021)"], "keyword_cds": "", "keyword_pub": "Exoplanets ; Transits ; Planetary science", "abstract": ["We apply AnalyticLC, an analytic model described in an accompanying", "paper, to interpret Kepler data of systems that contain two or three", "transiting planets. We perform tests to verify that the obtained", "solutions agree with full N-body integrations, and that the number of", "model parameters is statistically justified. We probe non-co-planar", "interactions via impact parameter variations (TbVs), enabled by our", "analytic model. The subset of systems with a valid solution includes", "54 systems composed of 140 planets, more than half of which are", "without previously reported mass constraints. Overall we provide: (I)", "estimates of physical and orbital properties for all systems analyzed;", "(II) 102 planets with mass detections significant to better than", "3{sigma}, 43 of which have masses below 5M{Earth}; and (III) 35 TbVs", "significant to better than 3{sigma}. We focus on select systems", "showing strong TbVs, which can result from either interaction among", "the known transiting planets, or with a nontransiting object, and", "provide: (IV) a method to constrain the parameters of such unseen", "companions. These results are enabled by an accurate 3D photodynamical", "model, of a kind expected to become increasingly important for", "modeling multidecade photometric and composite (radial velocity,", "astrometry) data sets."], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "tablea1.dat", "desc": "Physical and orbital elements of our solutions that pass all tests", "columns": [{"name": "Adopted", "desc": "Adopted solution "}, {"name": "ID", "desc": " "}, {"name": "KeplerName", "desc": "kepler name "}, {"name": "KOI", "desc": "KOI "}, {"name": "P", "desc": "mean orbital period "}, {"name": "mu", "desc": "planet-to-star mass ratio "}, {"name": "mu_ErrPos", "desc": " "}, {"name": "mu_ErrNeg", "desc": " "}, {"name": "mp", "desc": "absolute planet mass; derived from mu and literature stellar mass "}, {"name": "mp_ErrPos", "desc": " "}, {"name": "mp_ErrNeg", "desc": " "}, {"name": "rho_p", "desc": "absolute planet density; derived from RhoRel and literature stellar density "}, {"name": "rho_p_ErrPos", "desc": " "}, {"name": "rho_p_ErrNeg", "desc": " "}, {"name": "Rp", "desc": "absolute planet radius; derived from ror and literature stellar radius "}, {"name": "Rp_ErrPos", "desc": " "}, {"name": "Rp_ErrNeg", "desc": " "}, {"name": "dex", "desc": "eccentricity difference to preceding planet; x is pointing at the observer "}, {"name": "dex_ErrPos", "desc": " "}, {"name": "dex_ErrNeg", "desc": " "}, {"name": "dey", "desc": "eccentricity difference to preceding planet; y is the direction perpendicular to the line of sight pointing with the planets motion along transit "}, {"name": "dey_ErrPos", "desc": " "}, {"name": "dey_ErrNeg", "desc": " "}, {"name": "Ix", "desc": "Ix=I*cos(Omega) is the inclination component corresponding to the inclination around to the line of sight (\"roll angle\") "}, {"name": "Ix_ErrPos", "desc": " "}, {"name": "Ix_ErrNeg", "desc": " "}, {"name": "Iy", "desc": "Iy=I*sin(Omega) is the inclination component corresponding to the inclination relative to the line of sight "}, {"name": "Iy_ErrPos", "desc": " "}, {"name": "Iy_ErrNeg", "desc": " "}]}, {"name": "tablea2.dat", "desc": "Light curve, transit, and MMR proximity parameters of all analyzed planets", "columns": [{"name": "Adopted", "desc": "Adopted solution "}, {"name": "id", "desc": " "}, {"name": "KeplerName", "desc": "kepler name "}, {"name": "KOI", "desc": "KOI "}, {"name": "P", "desc": "mean orbital period "}, {"name": "TTVStd", "desc": "best model TTV std "}, {"name": "J", "desc": "J of the nearest first-order resonance J:J-1 with the planet from the inside. If the planet is innermost, the value is 0. "}, {"name": "Delta", "desc": "normalized distance from the J:J-1 resonance with the planet from the inside. If the planet is innermost, the value is 0. "}, {"name": "SuperPeriod", "desc": "super-period of the J:J-1 resonance with the planet from the inside. If the planet is innermost, the value is 0. "}, {"name": "T0", "desc": "transit duration at first data time stamp "}, {"name": "T0_ErrPos", "desc": " "}, {"name": "T0_ErrNeg", "desc": " "}, {"name": "Tau0", "desc": "ingress-egress time at first data time stamp "}, {"name": "Tau0_ErrPos", "desc": " "}, {"name": "Tau0_ErrNeg", "desc": " "}, {"name": "b0", "desc": "impact parameter at BKJD=0 "}, {"name": "b0_ErrPos", "desc": " "}, {"name": "b0_ErrNeg", "desc": " "}, {"name": "dbdt", "desc": "db/dt median "}, {"name": "dbdt_ErrPos", "desc": "db/dt positive error bar "}, {"name": "dbdt_ErrNeg", "desc": "db/dt negative error bar "}]}, {"name": "tablea3.dat", "desc": "Stellar parameters of the systems for which valid dynamical solutions were found", "columns": [{"name": "KOI", "desc": "KOI "}, {"name": "Star", "desc": "Star name "}, {"name": "KIC", "desc": "KIC "}, {"name": "Source", "desc": "Stellar m,R source "}, {"name": "u1", "desc": "first limb-darkening coeff, taken from nexi "}, {"name": "u2", "desc": "second limb-darkening coeff, taken from nexi "}, {"name": "ms", "desc": "absolute stellar mass "}, {"name": "ms_ErrPos", "desc": "absolute stellar mass positive error bar "}, {"name": "ms_ErrNeg", "desc": "absolute stellar mass negative error bar "}, {"name": "Rs", "desc": "absolute stellar radius; taken from literature "}, {"name": "Rs_ErrPos", "desc": " "}, {"name": "Rs_ErrNeg", "desc": " "}]}, {"name": "tablea4.dat", "desc": "Planets with significant impact parameter variations ", "columns": [{"name": "Adopted", "desc": "Adopted solution "}, {"name": "KeplerName", "desc": "kepler name "}, {"name": "KOI", "desc": "KOI "}, {"name": "P", "desc": "mean orbital period "}, {"name": "Npl", "desc": "model number of planets "}, {"name": "Position", "desc": "planet position within the system, from inside to outside "}, {"name": "b0", "desc": "impact parameter at BKJD=0 "}, {"name": "b0_ErrPos", "desc": " "}, {"name": "b0_ErrNeg", "desc": " "}, {"name": "dbdt", "desc": "db/dt median "}, {"name": "dbdt_ErrPos", "desc": "db/dt positive error bar "}, {"name": "dbdt_ErrNeg", "desc": "db/dt negative error bar "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_163_239"}} {"id": "J/AJ/163/239", "title_cds": "Globular cluster with ZTF; 1209 RR Lyrae", "title_create": "Ngeow+, 2022", "year": "2022", "author": "Ngeow C.-C., Bhardwaj A., Dekany R., Duev D.A., Graham M.J., Groom S.L., Mahabal A.A., Masci F.J., Medford M.S., Riddle R.", "title_pub": "Zwicky Transient Facility and Globular Clusters; The RR Lyrae.", "first_author": "Ngeow C.-C.", "ref_biblio": [""], "bibcode": ["2022AJ....163..239N"], "see_also": ["II/371 : The Dark Energy Survey (DES): Data Release 2 (Abott+, 2021)", "V/150 : Updated catalog of variable stars in globular clusters (Clement+ 2017)", "J/AJ/108/1786 : Blue stragglers and variable stars in M3 (Guhathakurta+, 1994)", "J/ApJ/463/26 : VI photometry of 29 Cepheids in M101. (Kelson+ 1996)", "J/AJ/130/2140 : Abundances and velocities in globular clusters (Pritzl+, 2005)", "J/MNRAS/372/1657 : BVI(c) light curves of variables in M3 (Benko+, 2006)", "J/MNRAS/371/1503 : Synthetic photometry of RR Lyr (Marconi+, 2006)", "J/A+A/474/121 : Galactic globular cluster 2MASSGC02 JKs phot (Borissova+, 2007)", "J/ApJ/708/717 : Light curve templates of RR Lyrae stars (Sesar+, 2010)", "J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012)", "J/ApJ/763/32 : Galactic halo RRab stars from CSS (Drake+, 2013)", "J/AcA/63/91 : V-band light curves of variables in M80 (Kopacki, 2013)", "J/MNRAS/439/3765 : RR Lyrae in 15 Galactic globular clusters (Dambis+, 2014)", "J/ApJ/814/71 : Carina project IX; UBVI data Carina variables (Coppola+, 2015)", "J/A+A/573/A13 : Metal abundances in 6 globular cluster (Dias+, 2015)", "J/AJ/151/88 : LMC NIR Synoptic Survey II Wesenheit relation (Bhardwaj+, 2016)", "J/AJ/152/170 : RRLs in globulars. IV. UBVRI phot. in Omega Cen (Braga+, 2016)", "J/A+A/590/A9 : RGB stars in Galactic GC stellar parameters (Dias+, 2016)", "J/ApJ/841/84 : Theoretical framework for RR Lyrae II. MIR data (Neeley+, 2017)", "J/AJ/153/204 : RR Lyrae stars from the PS1 3{pi} survey (Sesar+, 2017)", "J/AJ/154/85 : CTIO/DECam photometry of RR Lyrae stars in M5 (Vivas+, 2017)", "J/AJ/156/241 : A 1st catalog variable stars measured by ATLAS (Heinze+, 2018)", "J/ApJ/861/23 : RR Lyrae variables in the Crater II dwarf galaxy (Joo+, 2018)", "J/MNRAS/481/1195 : Gaia DR2 RRLyrae stars as standard candles (Muraveva+, 2018)", "J/A+A/619/A13 : 28 distant globular clusters CaT metallicities (Vasquez+, 2018)", "J/ApJ/883/11 : Magellan/IMACS spectra of Crater II & Hercules (Fu+, 2019)", "J/AJ/160/220 : NIR light curve of 234 RR Lyrae in Messier 3 (Bhardwaj+, 2020)", "J/ApJ/896/L43 : Cepheids HST amplitudes in V- and H-band (Riess+, 2020)", "J/ApJ/896/43 : Cepheids HST amplitudes in V- and H-band (Riess+, 2020)", "J/AJ/162/63 : ZTF light curve 51 stars in 12 globular clusters (Ngeow+, 2021)"], "keyword_cds": "Clusters, globular; Stars, variable; Photometry, RI; Reddening", "keyword_pub": "Globular star clusters ; RR Lyrae variable stars ; Distance indicators ; Wide-field telescopes ; Sky surveys", "abstract": ["Based on time-series observations collected from the Zwicky Transient", "Facility (ZTF), we derived period-luminosity-metallicity (PLZ) and", "period-Wesenheit-metallicity (PWZ) relations for RR Lyrae located in", "globular clusters. We have applied various selection criteria to", "exclude RR Lyrae with problematic or spurious light curves. These", "selection criteria utilized information on the number of data points", "per light curve, amplitudes, colors, and residuals on the", "period-luminosity and/or period-Wesenheit relations. Due to blending,", "a number of RR Lyrae in globular clusters were found to be anomalously", "bright and have small amplitudes of their ZTF light curves. We used", "our final sample of ~750 RR Lyrae in 46 globular clusters covering a", "wide metallicity range (-2.36dex<[Fe/H]<-0.54dex) to derive PLZ and", "PWZ relations in the gri bands. In addition, we have also derived the", "period-color-metallicity and, for the first time, the", "period-Q-index-metallicity relations, where the Q-index is", "extinction-free by construction. We have compared our various", "relations to empirical and theoretical relations available in the", "literature and found a good agreement with most studies. Finally, we", "applied our derived PLZ relation to a dwarf galaxy, Crater II, and", "found that its true distance modulus should be larger than the most", "recent determination."], "description": ["The Zwicky Transient Facility (ZTF) is a dedicated time-domain", "wide-field synoptic sky survey aimed at exploring the transient", "universe. It utilizes the Palomar 48inch Samuel Oschin Schmidt", "telescope together with a new mosaic CCD camera that provides a field", "of view of 47deg^2^ to observe the northern sky in customized gri", "filters. The ZTF gri-band light curves were extracted for our sample", "of RR Lyrae from the point-spread function (PSF) catalogs available", "from both the ZTF Public Data Release 7 (including both public and", "Caltech data) and the partner surveys until 2021 September 30."], "type": ["OC"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table3.dat", "desc": "Periods, mean magnitudes, amplitudes and reddenings for our sample of RR Lyrae", "columns": [{"name": "Name", "desc": "Name of the RR Lyrae in globular cluster "}, {"name": "Type", "desc": "Either RR0 or RR1 "}, {"name": "Per", "desc": "[0.21/0.96] Period in days "}, {"name": "gmag", "desc": "[12.15/20.76]? Mean g band magnitude (1) "}, {"name": "ampg", "desc": "[0.01/3.375]? Amplitude in g band (1) "}, {"name": "Ng", "desc": "[0/1385] Number of data points in g band (2) "}, {"name": "rmag", "desc": "[11.47/68.47]? Mean r band magnitude (1) "}, {"name": "ampr", "desc": "[0.009/102.6]? Amplitude in r band (1) "}, {"name": "Nr", "desc": "[0/1415] Number of data points in r band (2) "}, {"name": "imag", "desc": "[11.06/20.33]? Mean i band magnitude (1) "}, {"name": "ampi", "desc": "[0.01/1.1]? Amplitude in i band (1) "}, {"name": "Ni", "desc": "[0/428] Number of data points in i band (2) "}, {"name": "E", "desc": "[0.0/2.029] Reddening from Bayestar19 map (3) "}, {"name": "e_E", "desc": "[0.0/0.021] Error in reddening "}, {"name": "Flag", "desc": "Flags (4) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_163_207"}} {"id": "J/AJ/163/207", "title_cds": "67 binary stars with exoplanet(s) from Gaia EDR3", "title_create": "Christian+, 2022", "year": "2022", "author": "Christian S., Vanderburg A., Becker J., Yahalomi D.A., Pearce L., Zhou G., Collins K.A., Kraus A.L., Stassun K.G., de Beurs Z., Ricker G.R., Vanderspek R.K., Latham D.W., Winn J.N., Seager S., Jenkins J.M., Abe L., Agabi K., Amado P.J., Baker D., Barkaoui K., Benkhaldoun Z., Benni P., Berberian J., Berlind P., Bieryla A., Esparza-Borges E., Bowen M., Brown P., Buchhave L.A., Burke C.J., Buttu M., Cadieux C., Caldwell D.A., Charbonneau D., Chazov N., Chimaladinne S., Collins K.I., Combs D., Conti D.M., Crouzet N., de Leon J.P., Deljookorani S., Diamond B., Doyon R., Dragomir D., Dransfield G., Essack Z., Evans P., Fukui A., Gan T., Esquerdo G.A., Gillon M., Girardin E., Guerra P., Guillot T., Habich E.K. K, Henriksen A., Hoch N., Isogai K.I., Jehin E., Jensen E.L.N., Johnson M.C., Livingston J.H., Kielkopf J.F., Kim K., Kawauchi K., Krushinsky V., Kunzle V., Laloum D., Leger D., Lewin P., Mallia F., Massey B., Mori M., McLeod K.K., Mekarnia D., Mireles I., Mishevskiy N., Tamura M., Murgas F., Narita N., Naves R., Nelson P., Osborn H.P., Palle E., Parviainen H., Plavchan P., Pozuelos F.J., Rabus M., Relles H.M., Rodriguez Lopez C., Quinn S.N., Schmider F.-X., Schlieder J.E., Schwarz R.P., Shporer A., Sibbald L., Srdoc G., Stibbards C., Stickler H., Suarez O., Stockdale C., Tan T.-G., Terada Y., Triaud A., Tronsgaard R., Waalkes W.C., Wang G., Watanabe N., Wenceslas M.-S., Wingham G., Wittrock J., Ziegler C.", "title_pub": "A Possible Alignment Between the Orbits of Planetary Systems and their Visual Binary Companions.", "first_author": "Christian S.", "ref_biblio": [""], "bibcode": ["2022AJ....163..207C"], "see_also": ["B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2020)", "I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "III/279 : RAVE 5th data release (Kunder+, 2017)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)", "I/350 : Gaia EDR3 (Gaia Collaboration, 2020)", "VI/120 : High-resolution synthetic stellar library (Coelho+, 2005)", "VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "J/AJ/101/625 : Radial velocities of NGP wide binaries (Latham+, 1991)", "J/A+A/464/377 : HIP binaries with radial velocities (Frankowski+, 2007)", "J/MNRAS/406/2559 : BVRI light curves of GSC2314-0530 (Dimitrov+, 2010)", "J/ApJ/709/L114 : Protoplanetary disks in PMS binaries (Duchene, 2010)", "J/ApJS/190/1 : A survey of stellar families (Raghavan+, 2010)", "J/A+A/530/A138 : Geneva-Copenhagen survey re-analysis (Casagrande+, 2011)", "J/ApJ/738/170 : False positive Kepler planet candidates (Morton+, 2011)", "J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)", "J/AJ/148/54 : The Hypatia Catalog ((Hinkel+, 2014)", "J/ApJ/808/187 : Metallicities of KIC stars without planets (Buchhave+, 2015)", "J/MNRAS/455/4212 : Pan-STARRS 1: occurrence in the Kepler field (Dacon+, 2016)", "J/AJ/152/8 : Impact stellar multiplicity planetary systems I (Kraus+, 2016)", "J/ApJ/818/73 : Study of protostars in Perseus molecular cloud (Tobin+, 2016)", "J/AJ/154/107 : California-Kepler Survey. I. 1305 stars (Petigura+, 2017)", "J/ApJ/859/21 : ALMA survey of Lupus protoplanetary disks II. (Ansdell+, 2018)", "J/ApJS/239/2 : Simulated exoplanets from TESS list targets (Barclay+, 2018)", "J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018)", "J/MNRAS/483/3196 : GALAH carbon-enhanced stars & CEMP candidates (Cotar+, 2019)", "J/AJ/157/78 : Double & multiple star system GaiaDR2 (Jimenez-Esteban+, 2019)", "J/ApJ/871/63 : How to constrain M dwarf. II. Nearby binaries (Mann+, 2019)", "J/MNRAS/490/5088 : Stellar companions of exoplanet host stars (Mugrauer, 2019)", "J/MNRAS/492/1164 : Abundances of Gaia DR2 wide binaries (Hawkins+, 2020)", "J/AN/341/996 : Stellar companions of (C)TOIs (Mugrauer+, 2020)", "J/AJ/159/19 : SOAR TESS survey. I. (Ziegler+, 2020)", "J/ApJS/254/39 : Exoplanet candidates from TESS first 2yr obs (Guerrero+, 2021)", "J/AJ/162/192 : SOAR TESS survey II Impact stellar companions (Ziegler+, 2021)"], "keyword_cds": "Exoplanets; Stars, double and multiple; Photometry, UBVRIJKLMNH; Proper motions; Radial velocities; Abundances, [Fe/H]; Effective temperatures; Positional data; Parallaxes, trigonometric", "keyword_pub": "Star-planet interactions ; Circumstellar disks ; Exoplanet evolution ; Wide binary stars ; Visual binary stars", "abstract": ["Astronomers do not have a complete picture of the effects of", "wide-binary companions (semimajor axes greater than 100au) on the", "formation and evolution of exoplanets. We investigate these effects", "using new data from Gaia Early Data Release 3 and the Transiting", "Exoplanet Survey Satellite mission to characterize wide-binary systems", "with transiting exoplanets. We identify a sample of 67 systems of", "transiting exoplanet candidates (with well-determined, edge-on orbital", "inclinations) that reside in wide visual binary systems. We derive", "limits on orbital parameters for the wide-binary systems and measure", "the minimum difference in orbital inclination between the binary and", "planet orbits. We determine that there is statistically significant", "difference in the inclination distribution of wide-binary systems with", "transiting planets compared to a control sample, with the probability", "that the two distributions are the same being 0.0037. This implies", "that there is an overabundance of planets in binary systems whose", "orbits are aligned with those of the binary. The overabundance of", "aligned systems appears to primarily have semimajor axes less than", "700au. We investigate some effects that could cause the alignment and", "conclude that a torque caused by a misaligned binary companion on the", "protoplanetary disk is the most promising explanation."], "type": ["GCC"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "tableb1.dat", "desc": "Binaries with exoplanets ", "columns": [{"name": "Index", "desc": "[0/66] Internal index number "}, {"name": "EDR3-1", "desc": "Host GAIA EDR3 designation "}, {"name": "EDR3-2", "desc": "Companion GAIA EDR3 designation "}, {"name": "RAdeg", "desc": "[12/360]? Host GAIA EDR3 Right Ascension (J2016)"}, {"name": "RAdeg-2", "desc": "[12/360]? Companion GAIA EDR3 Right Ascension (J2016)"}, {"name": "DEdeg", "desc": "[-89/83]? Host GAIA EDR3 Declination (J2016) "}, {"name": "DEdeg-2", "desc": "[-89/83]? Companion GAIA EDR3 Declination (J2016)"}, {"name": "pmRA-1", "desc": "[-404/213] Host GAIA EDR3 proper motion along RA"}, {"name": "e_pmRA-1", "desc": "[0.009/0.04] Uncertainty in pmRA-1 "}, {"name": "pmRA-2", "desc": "[-400/213] Companion GAIA EDR3 proper motion along RA"}, {"name": "e_pmRA-2", "desc": "[0.01/0.2] Uncertainty in pmRA-2 "}, {"name": "pmDE-1", "desc": "[-381/192] Host GAIA EDR3 proper motion along DE"}, {"name": "e_pmDE-1", "desc": "[0.01/0.04] Uncertainty in pmDE1 "}, {"name": "pmDE-2", "desc": "[-381/192] Companion GAIA EDR3 proper motion along DE"}, {"name": "e_pmDE-2", "desc": "[0.01/0.2] Uncertainty in pmDE2 "}, {"name": "RVel-1", "desc": "[-61.4/79.2]? Host GAIA EDR3 radial velocity "}, {"name": "e_RVel-1", "desc": "[0.2/2]? Uncertainty in RVel-1 "}, {"name": "RVel-2", "desc": "[-46.1/46.9]? Companion GAIA EDR3 radial velocity"}, {"name": "e_RVel-2", "desc": "[0.2/4]? Uncertainty in RVel-2 "}, {"name": "[Fe/H]-1", "desc": "[-0.61/0.48]? Host metallicity (1) "}, {"name": "e_[Fe/H]-1", "desc": "[0.02/0.3]? Uncertainty in [Fe/H]-1 "}, {"name": "[Fe/H]-2", "desc": "[-0.35/0.22]? ? Companion metallicity (1) "}, {"name": "e_[Fe/H]-2", "desc": "[0.08/0.1]? Uncertainty in [Fe/H]-2 "}, {"name": "logg-1", "desc": "[3.76/4.81]? Host log surface gravity (1) "}, {"name": "e_logg-1", "desc": "[0.06/0.4]? Uncertainty in log(g)-1 "}, {"name": "logg-2", "desc": "[4.05/4.69]? Companion surface gravity (1) "}, {"name": "e_logg-2", "desc": "[0.1/0.2]? Uncertainty in log(g)-2 "}, {"name": "Teff-1", "desc": "[4086/5982]? Host effective temperature (1) "}, {"name": "e_Teff-1", "desc": "[34/275]? Uncertainty in Teff-1 "}, {"name": "Teff-2", "desc": "[3309/5547]? Companion effective temperature (1)"}, {"name": "e_Teff-2", "desc": "[64/157]? Uncertainty in Teff-2 "}, {"name": "Gmag-1", "desc": "[7.06/14.7] Host GAIA EDR3 G band magnitude "}, {"name": "Gmag-2", "desc": "[9.39/18.5] Companion GAIA EDR3 G band mage "}, {"name": "Bpmag-1", "desc": "[7.37/16.3] Host GAIA EDR3 Blue passband mag "}, {"name": "Bpmag-2", "desc": "[9.91/20.3]? Companion GAIA EDR3 Blue passband magnitude"}, {"name": "Rpmag-1", "desc": "[6.64/13.5] Host GAIA EDR3 Red passband mag "}, {"name": "Rpmag-2", "desc": "[8.7/17.2]? Companion GAIA EDR3 Red passband magnitude"}, {"name": "Jmag-1", "desc": "[5.82/11] Host 2MASS J band magnitude "}, {"name": "Jmag-2", "desc": "[6.11/11.9] Companion 2MASS J band magnitude "}, {"name": "Hmag-1", "desc": "[5.87/11.3] Host 2MASS H band magnitude "}, {"name": "Hmag-2", "desc": "[7.03/14.3]? Companion 2MASS H band magnitude "}, {"name": "Ksmag-1", "desc": "[7.63/15.2]? Host 2MASS Ks band magnitude "}, {"name": "Ksmag-2", "desc": "[7.19/14.6]? Companion 2MASS Ks band mag "}, {"name": "plx", "desc": "[5.32/45.5] GAIA EDR3 parallax (2) "}, {"name": "e_plx", "desc": "[37/1715]? Uncertainty in plx "}, {"name": "TIC-1", "desc": "Host TESS Input Catalog Identifier "}, {"name": "TIC-2", "desc": "Companion TESS Input Catalog Identifier "}, {"name": "Inc", "desc": "[34/166] System inclination (3) "}, {"name": "e_Inc", "desc": "[7/152] 5th percentile boundary in Inc "}, {"name": "B_Inc", "desc": "[63/176] 95th percentile boundary in Inc "}, {"name": "e", "desc": "[0.13/0.98] System eccentricity (3) "}, {"name": "b_e", "desc": "[0.01/0.9] 5th percentile boundary in e "}, {"name": "B_e", "desc": "[0.4/1] 95th percentile boundary in e "}, {"name": "MajAxis", "desc": "[79.3/50611] System semi-major axis (3) "}, {"name": "b_MajAxis", "desc": "[46/29454] 5th percentile boundary in MajAxis "}, {"name": "B_MajAxis", "desc": "[260/154240] 95th percentile boundary in MajAxis"}, {"name": "AscNode", "desc": "[-166/180] System longitude of ascending node (3)"}, {"name": "b_AscNode", "desc": "[-340/45] 5th percentile boundary in AscNode "}, {"name": "B_AscNode", "desc": "[10/355] 95th percentile boundary in AscNode "}, {"name": "ArgPer", "desc": "[69.6/182] System argument of periastron (3) "}, {"name": "b_ArgPer", "desc": "[7/40] 5th percentile boundary in ArgPer "}, {"name": "B_ArgPer", "desc": "[159/353] 95th percentile boundary in ArgPer "}, {"name": "PBin", "desc": "[809/8859400] System orbital period "}, {"name": "b_PBin", "desc": "[360/3933200] 5th percentile boundary in Pbin (3)"}, {"name": "B_PBin", "desc": "[5289/47134000] 95th percentile boundary in Pbin (3)"}, {"name": "Peri", "desc": "[-8689800/1742] Epoch of Periastron Passage "}, {"name": "b_Peri", "desc": "[-46934000/-1430] 5th percentile boundary in Peri"}, {"name": "B_Peri", "desc": "[-3776100/1888] 95th percentile boundary in Peri"}, {"name": "M-1", "desc": "[0.25/1.4] Host stellar mass "}, {"name": "e_M-1", "desc": "[0.006/0.2] Uncertainty in M-1 "}, {"name": "M-2", "desc": "[0.1/1.37] Companion stellar mass "}, {"name": "e_M-2", "desc": "[0.002/0.08] Uncertainty in M-2 "}, {"name": "Pp1", "desc": "[0.3/211]? 1st Planetary period "}, {"name": "e_Pp1", "desc": "[8e-07/0.2]? Uncertainty in Pp1 "}, {"name": "Pp2", "desc": "[0.4/63.4]? 2nd Planetary period "}, {"name": "e_Pp2", "desc": "[2e-07/0.008]? Uncertainty in Pp2 "}, {"name": "Pp3", "desc": "[5.9/6]? 3rd Planetary period mass "}, {"name": "e_Pp3", "desc": "[8e-05/9e-05]? Uncertainty in Pp3 "}, {"name": "Pp4", "desc": "[37.9/38]? 4th Planetary period mass "}, {"name": "e_Pp4", "desc": "[0.0007/0.0008]? Uncertainty in Pp4 "}, {"name": "Rp1", "desc": "[1.06/17.2]? 1st Planetary radius "}, {"name": "e_Rp1", "desc": "[0.1/6]? Uncertainty in Rp1 "}, {"name": "Rp2", "desc": "[0.55/15.3]? 2nd Planetary radius "}, {"name": "e_Rp2", "desc": "[0.09/7]? Uncertainty in Rp2 "}, {"name": "Rp3", "desc": "[1.32/2.88]? Third Planetary radius "}, {"name": "e_Rp3", "desc": "[0.2/2]? Uncertainty in Rp3 "}, {"name": "Rp4", "desc": "[0.99/3.33]? 4th Planetary radius "}, {"name": "e_Rp4", "desc": "[1/2]? Uncertainty in Rp4 "}]}, {"name": "tablec1.dat", "desc": "Control sample ", "columns": [{"name": "Index", "desc": "[0/687] Internal index number "}, {"name": "EDR3-1", "desc": "Host GAIA EDR3 designation "}, {"name": "EDR3-2", "desc": "Companion GAIA EDR3 designation "}, {"name": "RAdeg", "desc": "[0/360] Host GAIAEDR3 Right Ascension (J2016) "}, {"name": "RAdeg-2", "desc": "[0/360] Companion GAIA EDR3 Right Ascension (J2016)"}, {"name": "DEdeg", "desc": "[-89/90] Host GAIA EDR3 Declination (J2016) "}, {"name": "DEdeg-2", "desc": "[-89/90] Companion GAIA EDR3 Declination (J2016)"}, {"name": "pmRA-1", "desc": "[-565/884] Host GAIA EDR3 proper motion along RA"}, {"name": "e_pmRA-1", "desc": "[0.006/0.09] Uncertainty in pmRA-1 "}, {"name": "pmRA-2", "desc": "[-545/885] Companion GAIA EDR3 proper motion along RA"}, {"name": "e_pmRA-2", "desc": "[0.006/0.4] Uncertainty in pmRA-2 "}, {"name": "pmDE-1", "desc": "[-536/1096] Host GAIA EDR3 proper motion along DE"}, {"name": "e_pmDE-1", "desc": "[0.007/0.09] Uncertainty in pmDE1 "}, {"name": "pmDE-2", "desc": "[-5450/1094] Companion GAIA EDR3 proper motion along DE"}, {"name": "e_pmDE-2", "desc": "[0.008/0.4] Uncertainty in pmDE2 "}, {"name": "RVel-1", "desc": "[-163/313]? Host GAIA EDR3 radial velocity "}, {"name": "e_RVel-1", "desc": "[0.1/16]? Uncertainty in RVel-1 "}, {"name": "RVel-2", "desc": "[-170/79]? Companion GAIAEDR3 radial velocity "}, {"name": "e_RVel-2", "desc": "[0.1/11]? Uncertainty in RVel-2 "}, {"name": "[Fe/H]-1", "desc": "[-0.99/0.84]? Host metallicity (1) "}, {"name": "e_[Fe/H]-1", "desc": "[0.01/0.3]? Uncertainty in [Fe/H]-1 "}, {"name": "[Fe/H]-2", "desc": "[-0.79/0.36]? Companion metallicity (1) "}, {"name": "e_[Fe/H]-2", "desc": "[0.009/0.2]? Uncertainty in [Fe/H]-2 "}, {"name": "logg-1", "desc": "[3.36/4.81]? Host log surface gravity (1) "}, {"name": "e_logg-1", "desc": "[0.02/0.4]? Uncertainty in log(g)-1 "}, {"name": "logg-2", "desc": "[3.55/4.79]? Companion surface gravity (1) "}, {"name": "e_logg-2", "desc": "[0.01/0.3]? Uncertainty in log(g)-2 "}, {"name": "Teff-1", "desc": "[3924/7418]? Host effective temperature (1) "}, {"name": "e_Teff-1", "desc": "[12.55/317.0]? Uncertainty in Teff-1 "}, {"name": "Teff-2", "desc": "[3902/6376]? Companion effective temperature (1)"}, {"name": "e_Teff-2", "desc": "[11/105]? Uncertainty in Teff-2 "}, {"name": "Gmag-1", "desc": "[5.4/15.7] Host GAIA EDR3 G band magnitude "}, {"name": "Gmag-2", "desc": "[6.41/19.6] Companion GAIA EDR3 G band ma "}, {"name": "Bpmag-1", "desc": "[5.77/17] Host GAIA EDR3 Blue passband ma "}, {"name": "Bpmag-2", "desc": "[6.75/20.9] Companion GAIA EDR3 Blue passband magnitude"}, {"name": "Rpmag-1", "desc": "[4.97/14.6] Host GAIA EDR3 Red passband mag "}, {"name": "Rpmag-2", "desc": "[5.96/19.1] Companion GAIA EDR3 Red passband magnitude"}, {"name": "Jmag-1", "desc": "[4.05/12.3]? Host 2MASS J band magnitude "}, {"name": "Jmag-2", "desc": "[3.94/13.1]? Companion 2MASS J band magnitude "}, {"name": "Hmag-1", "desc": "[3.34/12.5]? Host 2MASS H band magnitude "}, {"name": "Hmag-2", "desc": "[5.05/16.8]? Companion 2MASS H band magnitude "}, {"name": "Ksmag-1", "desc": "[6.41/17]? Host 2MASS Ks band magnitude "}, {"name": "Ksmag-2", "desc": "[6.14/17.7]? Companion 2MASS Ks band mag "}, {"name": "plx", "desc": "[5.04/53.4] GAIA EDR3 parallax (2) "}, {"name": "e_plx", "desc": "[39/1889] Uncertainty in plx "}, {"name": "TIC-1", "desc": "Host TESS Input Catalog Identifier "}, {"name": "TIC-2", "desc": "Companion TESS Input Catalog Identifier "}, {"name": "Inc", "desc": "[11.6/170] System inclination (3) "}, {"name": "e_Inc", "desc": "[3.26/159] 5th percentile boundary in Inc "}, {"name": "B_Inc", "desc": "[21.9/177] 95th percentile boundary in Inc "}, {"name": "e", "desc": "[0.07/1] System eccentricity (3) "}, {"name": "b_e", "desc": "[0.005/1] 5th percentile boundary in e "}, {"name": "B_e", "desc": "[0.3/1] 95th percentile boundary in e "}, {"name": "MajAxis", "desc": "[0.003/237421] System semi-major axis (3) "}, {"name": "b_MajAxis", "desc": "[0.0003/105751] 5th percentile boundary in MajAxis"}, {"name": "B_MajAxis", "desc": "[0.008/537841] 95th percentile boundary in MajAxis"}, {"name": "AscNode", "desc": "[-180/180] System longitude of ascending node (3)"}, {"name": "b_AscNode", "desc": "[-360/26] 5th percentile boundary in AscNode "}, {"name": "B_AscNode", "desc": "[-17/357] 95th percentile boundary in AscNode "}, {"name": "ArgPer", "desc": "[174/184] System argument of periastron (3) "}, {"name": "b_ArgPer", "desc": "[5/47] 5th percentile boundary in ArgPer "}, {"name": "B_ArgPer", "desc": "[292/353] 95th percentile boundary in ArgPer "}, {"name": "PBin", "desc": "[3e-05/56807000] System orbital period "}, {"name": "b_PBin", "desc": "[6e-06/25820000] 5th percentile boundary in Pbin (3)"}, {"name": "B_PBin", "desc": "[0.0007/296140000] 95th percentile boundary in Pbin (3)"}, {"name": "Peri", "desc": "[-21917000/2016] Epoch of Periastron Passage "}, {"name": "b_Peri", "desc": "[-117160000/2016] 5th percentile boundary in Peri"}, {"name": "B_Peri", "desc": "[-9572500/2016] 95th percentile boundary in Peri"}, {"name": "M-1", "desc": "[0.16/1.69] Host stellar mass "}, {"name": "e_M-1", "desc": "[0.004/0.2] Uncertainty in M-1 "}, {"name": "M-2", "desc": "[0.09/1.31] Companion stellar mass "}, {"name": "e_M-2", "desc": "[1e-05/0.2] Uncertainty in M-2 "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_163_219"}} {"id": "J/AJ/163/219", "title_cds": "Gaia DR2 stellar flybys in the Sco-Cen OB association", "title_create": "Ma+, 2022", "year": "2022", "author": "Ma Y., De Rosa R.J., Kalas P.", "title_pub": "Search for Stellar Flybys in the Sco-Cen OB Association with the Gaia DR2.", "first_author": "Ma Y.", "ref_biblio": [""], "bibcode": ["2022AJ....163..219M"], "see_also": ["B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2020)", "III/190 : WEB Catalog of Radial Velocities (Duflot+ 1995)", "III/254 : 2nd Cat. Radial Velocities with Astrometric Data (Kharchenko+, 2007)", "III/272 : RAVE 4th data release (Kordopatis+, 2013)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/A+AS/118/231 : Velocities & rotation of CP stars (Levato+, 1996)", "J/AJ/117/354 : OB associations from Hipparcos (de Zeeuw+, 1999)", "J/A+A/356/541 : T Tauri stars in the Sco-Cen OB association (Koehler+, 2000)", "J/A+A/460/695 : Search for Associations Containing Young stars (Torres+, 2006)", "J/AN/328/889 : Mean Radial Velocities of open clusters (Kharchenko+, 2007)", "J/A+A/480/L33 : Radial velocities of HD 4113 and HD 156846 (Tamuz+, 2008)", "J/A+A/524/A25 : Radial Velocities on 6 exoplanet host stars (Triaud+, 2010)", "J/ApJ/738/122 : ScoCen debris disks Around F- and G-type stars (Chen+, 2011)", "J/ApJ/745/56 : Upper Sco members rotational velocities (Dahm+, 2012)", "J/ApJ/758/31 : IR photometry for members of Upper Sco (Luhman+, 2012)", "J/AJ/144/8 : Spectro. of ~100 G/K/M-type Sco-Cen complex memb (Song+, 2012)", "J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013)", "J/ApJ/785/47 : Sources around target stars Upper Scorpius (Lafreniere+, 2014)", "J/A+A/573/A126 : VLT/NaCo Large program I. Sample (Desidera+, 2015)", "J/ApJ/827/142 : ALMA observations of GKM stars in Upper Sco (Barenfeld+, 2016)", "J/ApJS/225/15 : IR excess stars from Tycho-2 and AllWISE (Cotten+, 2016)", "J/MNRAS/461/794 : Scorpius-Centaurus K-Type Stars (Pecaut+, 2016)", "J/ApJ/840/87 : Young star systems observed with SALT (Riedel+, 2017)", "J/A+A/616/A37 : Close encounters to the Sun in Gaia DR2 (Bailer-Jones+, 2018)", "J/ApJ/856/23 : BANYAN. XI. The BANYAN {Sigma} algorithm (Gagne+, 2018)", "J/AJ/156/194 : Orbits double-lined pairs in multiple stars (Tokovinin, 2018)", "J/A+A/623/A112 : The Sco OB2 population from Gaia DR2 data (Damiani+, 2019)", "J/AJ/157/78 : Double &multiple star systems GaiaDR2 (Jimenez-Esteban+, 2019)", "J/A+A/640/A73 : pi Men radial velocity curves (De Rosa+, 2020)", "J/AJ/160/24 : Circumstellar dust of 104 stars with GPIES (Esposito+, 2020)", "J/A+A/633/A82 : Disks around T Tauri stars with SPHERE. II. (Garufi+, 2020)", "J/ApJS/247/66 : SUPERWIDE: wide binaries in Gaia & SUPERBLINK (Hartman+, 2020)", "J/A+A/636/A116 : VLTI/PIONIER images of 15 Herbig Ae/Be stars (Kluska+, 2020)", "J/AJ/160/44 : Upper Scorpius spectroscopy and photometry (Luhman+, 2020)"], "keyword_cds": "Associations, stellar; Stars, masses; Radial velocities", "keyword_pub": "Celestial mechanics ; Close encounters ; Debris disks ; Circumstellar disks", "abstract": ["High-contrast imaging studies of debris disks have revealed a", "significant diversity in their morphologies, including large-scale", "asymmetries. Theories involving stellar flybys, an external source of", "gravitational disturbance, have offered a plausible explanation for", "the origin of these morphological variations. Our study is an", "experiment to gain empirical evidence that has been lacking from such", "theories. We explore this paradigm by using astrometric and radial", "velocity measurements from the Gaia DR2 and ground-based observations", "to trace the trajectories of 625 stars in the Sco-Cen OB association", "from 5Myr in the past to 2Myr in the future. We identified 119 stars", "that had at least one past flyby event occurring within one Hill", "radius, and 23 of these experienced flybys within 0.5 Hill radii. We", "found no evidence of a significant correlation between the presence of", "flyby events and infrared excess detections, although the sample is", "not uniformly sensitive to infrared excess emission. Ten stars that", "had past flyby events host resolved circumstellar disks that appear", "relatively symmetric in the existing data except for the circumbinary", "disk surrounding HD106906. We determined the trajectory and relative", "velocity of each of these flyby events and compared these to the", "geometry of the spatially resolved disks. Future work is needed to", "measure the kinematics of lower-mass stars and to improve sensitivity", "to circumstellar disks for the entire sample."], "object": ["16 15 -24.2 Sco-Cen = NAME Upper Sco-Cen", "16 12 -23.4 USCO = NAME Upper Sco Association"], "type": ["GCC"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Events identified from Sco-Cen sample ", "columns": [{"name": "Star1", "desc": "Star 1 identifier "}, {"name": "Star2", "desc": "Star 2 identifier "}, {"name": "RVel", "desc": "? Simulated radial velocity (1) "}, {"name": "Tca", "desc": "Time of closest approach "}, {"name": "e_Tca", "desc": "Lower uncertainty in tca "}, {"name": "E_Tca", "desc": "Upper uncertainty in tca "}, {"name": "Dca", "desc": "Distance of closest approach "}, {"name": "e_Dca", "desc": "Lower uncertainty in dca "}, {"name": "E_Dca", "desc": "Upper uncertainty in dca "}, {"name": "dca/RH-T", "desc": "Ratio of closet approach to target Hill radius "}, {"name": "e_dca/RH-T", "desc": "Lower uncertainty in dca/RH,T "}, {"name": "E_dca/RH-T", "desc": "Upper uncertainty in dca/RH,T "}, {"name": "dca/RH-F", "desc": "Ratio of closet approach to flyby Hill radius "}, {"name": "e_dca/RH-F", "desc": "Lower uncertainty in dca/RH,F "}, {"name": "E_dca/RH-F", "desc": "Upper uncertainty in dca/RH,F "}, {"name": "Cat", "desc": "Category (2) "}, {"name": "IREx?", "desc": "Infrared excess detected (3) "}]}, {"name": "table3.dat", "desc": "Events identified from USCO sample ", "columns": [{"name": "Star1", "desc": "Star 1 identifier "}, {"name": "Star2", "desc": "Star 2 identifier "}, {"name": "RVel", "desc": "? Simulated radial velocity (1) "}, {"name": "Tca", "desc": "Time of closest approach "}, {"name": "e_Tca", "desc": "Lower uncertainty in tca "}, {"name": "E_Tca", "desc": "Upper uncertainty in tca "}, {"name": "Dca", "desc": "Distance of closest approach "}, {"name": "e_Dca", "desc": "Lower uncertainty in dca "}, {"name": "E_Dca", "desc": "Upper uncertainty in dca "}, {"name": "dca/RH-T", "desc": "Ratio of closet approach to target Hill radius "}, {"name": "e_dca/RH-T", "desc": "Lower uncertainty in dca/RH,T "}, {"name": "E_dca/RH-T", "desc": "Upper uncertainty in dca/RH,T "}, {"name": "dca/RH-F", "desc": "Ratio of closet approach to flyby Hill radius "}, {"name": "e_dca/RH-F", "desc": "Lower uncertainty in dca/RH,F "}, {"name": "E_dca/RH-F", "desc": "Upper uncertainty in dca/RH,F "}, {"name": "Cat", "desc": "Category (2) "}, {"name": "IREx?", "desc": "Infrared excess detected (3) "}]}, {"name": "table4.dat", "desc": "Events involving candidates and field stars with d_ca_<1pc and v_rel_<10km/s", "columns": [{"name": "Star1", "desc": "Star 1 identifier (1) "}, {"name": "Star2", "desc": "Star 2 identifier (1) "}, {"name": "Tca", "desc": "[-2.43/2.05] Time of closest approach "}, {"name": "e_Tca", "desc": "[0.01/2.28] Lower uncertainty in tca "}, {"name": "E_Tca", "desc": "[0.01/2.28] Upper uncertainty in tca "}, {"name": "Dca", "desc": "[0.02/0.99] Distance of closest approach "}, {"name": "e_Dca", "desc": "[0.01/0.68] Lower uncertainty in dca "}, {"name": "E_Dca", "desc": "[0.02/2.39] Upper uncertainty in dca "}, {"name": "Vrel", "desc": "[0.71/9.98] Flyby star's velocity vector (2) "}, {"name": "e_Vrel", "desc": "[0.1/5.84] Lower uncertainty in Vrel "}, {"name": "E_Vrel", "desc": "[0.16/9.34] Upper uncertainty in Vrel "}, {"name": "Cat", "desc": "Category (3) "}]}, {"name": "table5.dat", "desc": "Simulated Potential Flyby events from USCO sample ", "columns": [{"name": "Star1", "desc": "Star 1 identifier "}, {"name": "Star2", "desc": "Star 2 identifier "}, {"name": "RVel", "desc": "? Simulated radial velocity (1) "}, {"name": "Tca", "desc": "Time of closest approach "}, {"name": "e_Tca", "desc": "Lower uncertainty in tca "}, {"name": "E_Tca", "desc": "Upper uncertainty in tca "}, {"name": "Dca", "desc": "Distance of closest approach "}, {"name": "e_Dca", "desc": "Lower uncertainty in dca "}, {"name": "E_Dca", "desc": "Upper uncertainty in dca "}, {"name": "dca/RH-T", "desc": "Ratio of closet approach to target Hill radius "}, {"name": "e_dca/RH-T", "desc": "Lower uncertainty in dca/RH,T "}, {"name": "E_dca/RH-T", "desc": "Upper uncertainty in dca/RH,T "}, {"name": "dca/RH-F", "desc": "Ratio of closet approach to flyby Hill radius "}, {"name": "e_dca/RH-F", "desc": "Lower uncertainty in dca/RH,F "}, {"name": "E_dca/RH-F", "desc": "Upper uncertainty in dca/RH,F "}, {"name": "Cat", "desc": "Category (2) "}, {"name": "IREx?", "desc": "Infrared excess detected (3) "}]}, {"name": "table6.dat", "desc": "RV measurements of 462 Sco-Cen stars ", "columns": [{"name": "Target", "desc": "Target identifier "}, {"name": "Gaia", "desc": "Gaia DR2 identifier "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Mass", "desc": "? Stellar mass "}, {"name": "SubGrp", "desc": "? Subgroup (1) "}, {"name": "GRVel", "desc": "? Gaia DR2 radial velocity "}, {"name": "e_GRVel", "desc": "? Uncertainty in GRVel "}, {"name": "RVel", "desc": "? Literature radial velocity "}, {"name": "e_RVel", "desc": "? Uncertainty in RVel "}, {"name": "r_RVel", "desc": "ADS bibcode reference for RVel "}]}, {"name": "table7.dat", "desc": "RV measurements of USCO sample ", "columns": [{"name": "Target", "desc": "Target identifier "}, {"name": "Gaia", "desc": "Gaia DR2 identifier "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Mass", "desc": "? Stellar mass "}, {"name": "SubGrp", "desc": "? Subgroup (1) "}, {"name": "GRVel", "desc": "? Gaia DR2 radial velocity "}, {"name": "e_GRVel", "desc": "? Uncertainty in GRVel "}, {"name": "RVel", "desc": "? Literature radial velocity "}, {"name": "e_RVel", "desc": "? Uncertainty in RVel "}, {"name": "r_RVel", "desc": "ADS bibcode reference for RVel "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_163_244"}} {"id": "J/AJ/163/244", "title_cds": "", "title_create": "Christiansen+, 2022", "year": "2022", "author": "Christiansen J.L., Bhure S., Zink J.K., Hardegree-Ullman K.K., Adkins B.D., Hedges C., Morton T.D., Bieryla A., Ciardi D.R., Cochran W.D., Dressing C.D., Everett M.E., Isaacson H., Livingston J.H., Ziegler C., Berlind P., Calkins M.L., Esquerdo G.A., Latham D.W., Endl M., MacQueen P.J., Fulton B.J., Hirsch L.A., Howard A.W., Weiss L.M., Allen B.E., Berberyann A., Ciardi K.N., Dunlavy A., Glassford S.H., Dai F., Hirano T., Tamura M., Beichman C., Gonzales E.J., Schlieder J.E., Barclay T., Crossfield I.J.M., Gilbert E.A., Matthews E.C., Giacalone S., Petigura E.A.", "title_pub": "Scaling K2. V. Statistical Validation of 60 New Exoplanets From K2 Campaigns 2-18.", "first_author": "Christiansen J.L.", "bibcode": [""], "bibcode": ["2022AJ....163..250Y"], "see_also": ["B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)", "II/287 : Northern Sky Variability Survey (NSVS) (Wozniak+, 2004)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "V/146 : LAMOST DR1 catalogs (Luo+, 2015)", "J/AJ/106/2096 : Limb-darkening coefficients in binaries (Van Hamme 1993)", "J/A+A/311/523 : Photometry of W UMa (Maceroni+, 1996)", "J/AcA/48/35 : All Sky Automated Survey variable stars (Pojmamski 1998)", "J/AJ/119/1901 : ROTSE all-sky surveys for variable stars (Akerlof+, 2000)", "J/A+A/406/535 : Hamburg/RASS Cat. of optical ident. V3.0 (Zickgraf+, 2003)", "J/AcA/54/207 : Ephemerids of eclipsing binaries (Kreiner, 2004)", "J/ApJ/629/1055 : Evolution of close binary systems (Yakut+, 2005)", "J/other/IBVS/5731 : Minima and maxima of 816 variables (Hubscher+, 2006)", "J/AcA/58/405 : ASAS eclipsing binaries RASS counterpart (Szczygiel+, 2008)", "J/AJ/138/466 : NSVS variables automated classification (Hoffman+, 2009)", "J/other/IBVS/5874 : Minima and maxima of 299 variables (Hubscher+, 2009)", "J/other/RAA/9.1035 : RV light curves of 1RXS J201607.0+251645 (Li+, 2009)", "J/AJ/138/680 : BVI TX Cnc light curves (Zhang+, 2009)", "J/other/IBVS/5959 : Minima and maxima of 436 variables (Huebscher+, 2011)", "J/AJ/146/35 : BVR light curves of DZ Psc (Yang+, 2013)", "J/MNRAS/430/2029 : Initial masses of WUMa type contact binaries (Yildiz+, 2013)", "J/AJ/148/126 : Light curves of four overcontact binaries (Caliskan+, 2014)", "J/AJ/147/50 : Differential BVRI light curves of DV Psc (Pi+, 2014)", "J/other/NewA/36.50 : V873 Per BVR light curves (Kriwattanawong+, 2015)", "J/AJ/151/68 : Kepler Mission. VII. Eclipsing binaries in DR3 (Kirk+, 2016)", "J/AJ/154/260 : 3 short-period eclipsing binaries BVRI photometry (Pi+, 2017)", "J/ApJS/249/18 : The ZTF catalog of periodic variable stars (Chen+, 2020)", "J/other/RAA/20.163 : Contact binaries in LAMOST DR7 (Qian+, 2020)", "J/AJ/160/104 : EpsilonCrA components radial&orbital velocity (Rucinski, 2020)", "J/ApJS/254/10 : Compilation of W UMa stars (Latkovic+, 2021)", "J/AJ/162/63 : ZTF lightcurve 51 stars in 12 globular clusters (Ngeow+, 2021)", "J/AJ/161/221 : Photometry & spectroscopy of 4 binaries stars (Panchal+, 2021)"], "keyword_cds": "Stars, double and multiple; Binaries, eclipsing; Photometry, UBVRI", "keyword_pub": "Eclipsing binary stars", "abstract": ["We presented new photometry for four short-period late-type binaries,", "observed by three small telescopes in China from 2020 September to", "2021 December. Seven sets of light curves (including the TESS data for", "FY Boo) were analyzed by using the W-D method. Three binaries (V0576", "Peg, V0873 Per, and FY Boo) are W-type binaries with q~2.5, while KW", "Psc is an A-type binary with q~0.43. Max.I-Max.II is up to 10% of", "variable light amplitude for the asymmetric light curves, which are", "modeled by a dark spot on the surface of the more massive component.", "Photometric results imply the existence of movement and evolution of", "the cool spot. From the temperature-luminosity and mass-luminosity", "diagrams, the more massive components are a bit evolved main-sequence", "stars, while the less massive ones are oversized and overluminous", "owing to energy exchange. Orbital period analyses indicate that the", "cyclic oscillations occur in the (O-C) curves. Their modulated periods", "approach 11yr, which may preferably result from the magnetic activity", "cycle for four late-type contact binaries. With angular momentum loss", "through magnetic braking, these short-period contact binaries may", "evolve into deep-contact configurations."], "description": ["New observations of four contact binaries were performed on 14 nights", "in 2020 and 2021 by using the 60cm, the 80cm, and the 85cm telescopes", "at the Xinglong station (XLs) of National Astronomical Observatories,", "Chinese Academy of Sciences (NAOC). All three telescopes are equipped", "with the standard UBVRcIc multicolor photometric systems."], "object": ["23 10 59.53 +21 42 43.2 V0576 Peg = RX J2311.0+2142", "22 58 31.81 +05 52 24.0 KW Psc = ASAS J225832+0552.4", "02 47 08.22 +41 22 31.9 V0873Per = V* V873 Per", "13 46 51.81 +22 57 14.1 FY Boo = V* FY Boo"], "type": ["OC"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table4.dat", "desc": "Seventeen light minimum times for V0576 Peg ", "columns": [{"name": "HJD", "desc": "Heliocentric Julian Date "}, {"name": "e_HJD", "desc": "? Error on HJD "}, {"name": "Epoch", "desc": "Epoch time "}, {"name": "Met", "desc": "Method used "}, {"name": "Min", "desc": "Minimum eclipse-depth (I or II) "}, {"name": "O-Ci", "desc": "Initial residual "}, {"name": "O-Cf", "desc": "? Final residual "}, {"name": "Ref", "desc": "References used "}]}, {"name": "table6.dat", "desc": "All collected light minimum times for KW Psc ", "columns": [{"name": "HJD", "desc": "Heliocentric Julian Date "}, {"name": "e_HJD", "desc": "? Error on HJD "}, {"name": "Epoch", "desc": "Epoch time "}, {"name": "Met", "desc": "Method used "}, {"name": "Min", "desc": "Minimum eclipse-depth (I or II) "}, {"name": "O-Ci", "desc": "Initial residual "}, {"name": "O-Cf", "desc": "? Final residual "}, {"name": "Ref", "desc": "References used "}]}, {"name": "table7.dat", "desc": "All available eclipse times of minimum light for V0873 Per", "columns": [{"name": "HJD", "desc": "Heliocentric Julian Date "}, {"name": "e_HJD", "desc": "? Error on HJD "}, {"name": "Epoch", "desc": "Epoch time "}, {"name": "Met", "desc": "Method used "}, {"name": "Min", "desc": "Minimum eclipse-depth (I or II) "}, {"name": "O-Ci", "desc": "Initial residual "}, {"name": "O-Cf", "desc": "? Final residual "}, {"name": "Ref", "desc": "References used "}]}, {"name": "table8.dat", "desc": "All compiled light minimum times for FY Boo ", "columns": [{"name": "HJD", "desc": "Heliocentric Julian Date "}, {"name": "e_HJD", "desc": "? Error on HJD "}, {"name": "Epoch", "desc": "Epoch time "}, {"name": "Met", "desc": "Method used "}, {"name": "Min", "desc": "Minimum eclipse-depth (I or II) "}, {"name": "O-Ci", "desc": "Initial residual "}, {"name": "O-Cf", "desc": "? Final residual "}, {"name": "Ref", "desc": "References used "}]}, {"name": "refs.dat", "desc": "References used in this work ", "columns": [{"name": "Ref", "desc": "Reference code "}, {"name": "Autor", "desc": "Main autor "}, {"name": "BIB", "desc": "BIBcode "}, {"name": "Cat.", "desc": "Catalog in Vizier "}, {"name": "Note", "desc": "Additional note or comment "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_163_276"}} {"id": "J/AJ/163/276", "title_cds": "X-band observation of compact radio sources in M17", "title_create": "Yanza+, 2022", "year": "2022", "author": "Yanza V., Masque J.M., Dzib S.A., Rodriguez L.F., Medina S.-N.X., Kurtz S., Loinard L., Trinidad M.A., Menten K.M., Rodriguez-Rico C.A.", "title_pub": "The Population of Compact Radio Sources in M17.", "first_author": "Yanza V.", "ref_biblio": [""], "bibcode": ["2022AJ....163..276Y"], "see_also": ["J/ApJ/574/258 : X-ray-emitting young stars in Orion nebula (Feigelson+, 2002)", "J/ApJ/613/393 : X-ray and radio sources in {rho} Oph Core A (Gagne+, 2004)", "J/ApJS/169/353 : Chandra sources in M17 (Broos+, 2007)", "J/ApJ/696/1278 : The extended star-forming environment of M17 (Povich+, 2009)", "J/ApJ/775/63 : Gould's Belt VLA Survey. I. Ophiuchus complex (Dzib+, 2013)", "J/A+A/560/A76 : Catalog of stellar clusters in inner Galaxy (Morales+, 2013)", "J/ApJ/790/49 : Gould's Belt VLA survey. III. Orion region (Kounkel+, 2014)", "J/ApJ/801/91 : Gould's Belt Very Large Array survey. IV. Taurus (Dzib+, 2015)", "J/ApJ/805/9 : Gould's Belt VLA Survey II. Serpens region (Ortiz-Leon+, 2015)", "J/A+A/588/A97 : Continuum sources from the THOR survey (Bihr+, 2016)", "J/ApJ/822/93 : Population of compact radio sources in ONC (Forbrich+, 2016)", "J/ApJ/818/116 : Gould's Belt VLA survey. V. Perseus region (Pech+, 2016)", "J/ApJ/834/142 : Gould's Belt Distances Survey. II. OMC (Kounkel+, 2017)", "J/A+A/610/A27 : Compact radio sources in NGC 6334D to F (Medina+, 2018)", "J/A+A/619/A124 : THOR survey in northern Galactic plane (Wang+, 2018)", "J/A+A/627/A175 : GLOSTAR. Radio Source Catalogue I (Medina+ 2019)", "J/ApJ/906/24 : A VLBA Survey of Radio Stars in the ONC. II. (Dzib+, 2021)", "J/ApJ/906/23 : A VLBA Survey of radio stars in the ONC. I. (Forbrich+, 2021)"], "keyword_cds": "Star Forming Region; YSOs; Radio sources; Parallaxes, trigonometric", "keyword_pub": "Star forming regions ; Young stellar objects ; Radio source catalogs", "abstract": ["We present a catalog of radio sources of the M17 region based on deep", "X-band radio observations centered at 10GHz obtained with the Jansky", "Very Large Array in the A configuration. We detect a total of 194", "radio sources, 12 of them extended and 182 compact. We find that a", "significant fraction (at least 40% in our catalog) have suspected", "gyrosynchrotron emission associated with stellar coronal emission. By", "comparing the radio luminosities of our sources with their X-ray", "counterparts, when available, we find that they are underluminous in", "X-rays with respect to the Gudel-Benz relation, but a correlation with", "a similar slope is obtained provided that only sources with evident", "nonthermal nature are selected from the sample compiled for the Orion", "Nebula Cluster (ONC) and M17. The comparison of M17 with the ONC and", "NGC 6334D-F leads to a similar luminosity function for the three", "regions, at least for the more luminous sources. However, the radio", "sources in M17 are three times more numerous compared to the other", "regions at a given luminosity and their spatial distribution differs", "from that of Orion. Moreover, an arc-shaped structure of 40\" in extent", "is observed in our map, identified previously as an ionizing front,", "with the cometary hypercompact source UC1 at its focus. Archival 1mm", "ALMA data reveals compact emission coincident with the radio", "wavelength peak, possibly associated with a protostellar disk of the", "massive star exciting UC1."], "description": ["The Very Large Array (VLA) data were taken using the most extended A", "configuration in the X-band (8-12GHz) toward the M17 star-forming", "region. The observations were made in three epochs with a total", "observation time of 4hr (1hr on 2018 May 3, 1hr on May 4, and 2hr on", "May 8). The data were taken using the 3bit sampling mode with an", "integration time set to 2s."], "object": ["18 20 47 -16 10.3 M17 = NGC 6618"], "type": ["OC"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Extended sources in M17 region from the final map ", "columns": [{"name": "Seq", "desc": "[1/12] Sequential number ID "}, {"name": "RAh", "desc": "[18] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "[20] Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "[24/31] Second ofright ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[16] Degree of declination (J2000) "}, {"name": "DEm", "desc": "[7/13] Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "Fpeak", "desc": "[57/560] Flux density at peak "}, {"name": "e_Fpeak", "desc": "[7/45] Error on Speak "}, {"name": "Fint", "desc": "[887/101425] Integrated flux "}, {"name": "e_Fint", "desc": "[109/7245] Error on Sint "}, {"name": "Area", "desc": "[0.4/40.3] Angular area "}]}, {"name": "table3.dat", "desc": "Distances of the Gaia counterparts of the CRSs ", "columns": [{"name": "Seq", "desc": "[6/170] Sequential number ID "}, {"name": "plx", "desc": "[0.52/1.01] Parallax from Gaia "}, {"name": "e_plx", "desc": "[0.1/0.6] Error on plx "}, {"name": "Dist", "desc": "[0.99/1.92] Gaia distances "}, {"name": "e_Dist", "desc": "[0.19/0.98] Error on Dist "}]}, {"name": "table4.dat", "desc": "*Spectral Indices of the CRSs ", "columns": [{"name": "Seq", "desc": "[22/161] Sequential number ID "}, {"name": "F9", "desc": "[164/92486] Flux at 9GHz "}, {"name": "e_F9", "desc": "[12/4626] Error on S9 "}, {"name": "F11", "desc": "[138/111808] Flux at 11GHz "}, {"name": "e_F11", "desc": "[9/5591] Error on F11 "}, {"name": "SI", "desc": "[-2.3/1] Spectral index "}, {"name": "e_SI", "desc": "[0.3/0.5] Error on SI "}]}, {"name": "table8.dat", "desc": "Parameters of the CRSs with their counterparts at other wavelengths", "columns": [{"name": "Seq", "desc": "[1/182] Sequential number ID "}, {"name": "RAh", "desc": "[18] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "[20] Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "[16/45] Second of right ascension (J2000) "}, {"name": "e_RAs", "desc": "[0.001/0.002] Error on RAs "}, {"name": "DE-", "desc": "[-] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[16] Degree of declination (J2000) "}, {"name": "DEm", "desc": "[7/14] Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "e_DEs", "desc": "Error on DEs "}, {"name": "Fpeak", "desc": "[25/18582] Flux at peak "}, {"name": "e_Fpeak", "desc": "[5/1003] Error on Fpeak "}, {"name": "Fint", "desc": "[25/97836] Integrated flux "}, {"name": "e_Fint", "desc": "[5/5092] Error on Fint "}, {"name": "Xray", "desc": "X-ray counterparts from Chandra; Broos+, 2007, J/ApJS/169/353"}, {"name": "IR", "desc": "IR counterparts from Two Micron All-Sky Survey (1)"}, {"name": "Opt", "desc": "Optical counterparts from Gaia DR2 "}, {"name": "Radio", "desc": "Catalog number in Rodriguez+, 2012ApJ...755..152R"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_163_278"}} {"id": "J/AJ/163/278", "title_cds": "Stellar populations in IC 2602 and IC 2391", "title_create": "Nisak+, 2022", "year": "2022", "author": "Nisak A.H., White R.J., Yep A., Henry T.J., Paredes L., James H.-S., Jao W.-C.", "title_pub": "Mapping out the Stellar Populations of IC 2602 and IC 2391.", "first_author": "Nisak A.H.", "ref_biblio": [""], "bibcode": ["2022AJ....163..278N"], "see_also": ["B/simbad : Simbad objects catalogue (M.Wenger 2000)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "J/A+AS/126/81 : IC 2602 VRI photometry (Foster+ 1997)", "J/A+AS/126/357 : Members of IC 2391 (Rolleston+ 1997)", "J/ApJS/134/103 : Low-mass members of IC 2391 (Barrado y Navascues+, 2001)", "J/A+A/372/862 : Lithium abundances in IC 2602 and IC 2391 (Randich+, 2001)", "J/A+A/410/671 : X-ray emission in cool main sequence stars (Messina+, 2003)", "J/MNRAS/355/959 : Proper motions of IC 2391 possible members (Dodd+, 2004)", "J/A+A/461/509 : Membership and spectroscopy of IC 2391 (Platais+, 2007)", "J/AJ/133/2524 : Spectra of young nearby stars (White+, 2007)", "J/ApJ/706/1484 : Photometry and spectroscopy in IC 2391 (Boudreault+, 2009)", "J/A+A/501/553 : Equivalent widths of IC 2602 & IC 2391 stars (D'Orazi+, 2009)", "J/A+A/498/949 : Velocities of 1253 F-K dwarfs in clusters (Mermilliod+, 2009)", "J/MNRAS/399/2146 : Orbits of open clusters in the Galaxy (Wu+, 2009)", "J/MNRAS/431/1005 : IC 2391 and Argus young stars (de Silva+, 2013)", "J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013)", "J/AJ/147/69 : Radial velocities in Be 44, Be 81, and NGC 6802 (Hayes+, 2014)", "J/MNRAS/458/4530 : Chandra Galactic Bulge Survey (Wevers+, 2016)", "J/AJ/153/128 : WOCS. LXXV. Hyades&Praesepe stellar Li data (Cummings+, 2017)", "J/A+A/608/A95 : GES: multi-line spectroscopic binary candidates (Merle+, 2017)", "J/A+A/601/A70 : GES: pre-main-sequence clusters [Fe/H] (Spina+, 2017)", "J/ApJ/836/77 : Library of high-S/N optical spectra of FGKM stars (Yee+, 2017)", "J/A+A/618/A93 : Gaia DR2 open clusters in the Milky Way (Cantat-Gaudin+, 2018)", "J/A+A/616/A10 : 46 open cluster GaiaDR2 HR diagrams (Gaia Collaboration, 2018)", "J/ApJ/856/23 : BANYAN. XI. The BANYAN {Sigma} algorithm (Gagne+, 2018)", "J/A+A/612/A99 : Gaia-ESO Survey in 7 open star cluster fields (Randich+, 2018)", "J/AJ/157/85 : The CIDA Variability Survey of Orion OB1. II. (Briceno+, 2019)", "J/AJ/158/163 : Li abundance values for stars in NGC 6819 (Deliyannis+, 2019)", "J/AJ/158/54 : New Taurus members stellar to planetary masses (Esplin+, 2019)", "J/A+A/628/A66 : alpha Persei, Pleiades and Praesepe clusters (Lodieu+, 2019)", "J/A+A/643/A71 : Members for 20 open clusters (Gutierrez Albarran+, 2020)", "J/AJ/160/44 : Upper Scorpius spectroscopy and photometry (Luhman+, 2020)", "J/AJ/162/176 : The solar neighborhood. XLVIII. (Paredes+, 2021)"], "keyword_cds": "Clusters, open; Spectra, optical; Parallaxes, trigonometric; Proper motions; Abundances, [Fe/H]; Effective temperatures", "keyword_pub": "Open star clusters ; Young star clusters", "abstract": ["IC2391 and IC2602 are important benchmarks for testing early star and", "planet evolution theories, both structural and dynamical, because they", "are the nearest open clusters with ages of ~50Myr. We refine", "membership lists for these clusters by identifying candidate members", "using Gaia DR2 kinematic and distance information. We identify 451", "candidate members of IC2602 and 350 candidate members of IC2391. If", "confirmed, this would increase the known populations of these clusters", "by 275% and 130%, respectively. We use CHIRON on the CTIO/SMARTS 1.5m", "telescope via fiber mode which yields a resolution of 27400 to acquire", "high-resolution spectra of 26 new candidate cluster members brighter", "than G=13 magnitude, as well as an additional 12 previously known", "members. Measures of lithium, H{alpha}, stellar properties (Teff,", "logg, [Fe/H]), radial velocities, and vsini values from these spectra", "are used to confirm cluster membership. We find that 37 of 38 stars we", "observe are bona fide cluster members, of which four are new candidate", "photometric binaries and 10 are new candidate spectroscopic binaries."], "description": ["We obtain spectra for all 26 bright (G<13) candidate members newly", "identified in this study to confirm cluster membership. We also", "observe 12 previously known (also with G<13) cluster members to check", "the reliability of our analysis techniques. We obtain single-epoch", "1200s exposures for each star using the CHIRON echelle spectrograph on", "the Cerro Tololo Inter-American Observatory Small and Moderate", "Aperture Research Telescope System CTIO/SMARTS 1.5m telescope. The", "stars are observed in fiber mode, which covers 4500-8900{AA} over 62", "spectral orders at a resolving power of R~27400."], "object": ["08 41 10 -52 59.5 IC 2391 = IC 2391", "10 42 27 -64 25.6 IC 2602 = IC 2602"], "type": ["OC"], "data": "", "date_update": "18-Oct-2022", "tables": [{"name": "table3.dat", "desc": "Measurements for 26 new candidate members of IC 2602 and IC 2391", "columns": [{"name": "Cluster", "desc": "Cluster identifier "}, {"name": "ID", "desc": "Internal identifier "}, {"name": "f_ID", "desc": "l Flag on ID (G1) "}, {"name": "2MASS", "desc": "2MASS identifier "}, {"name": "RVel", "desc": "[-26.7/56] Radial velocity from CHIRON "}, {"name": "e_RVel", "desc": "[0.09/0.3] Error on RVel "}, {"name": "vsini", "desc": "[4.6/27.2] Rotational velocity from CHIRON "}, {"name": "e_vsini", "desc": "[0.7/6.6] Error on vsini "}, {"name": "l_EW-Li", "desc": "[<] Limit flag on EW-Li "}, {"name": "EW-Li", "desc": "[0.01/0.35] CHIRON Equivalent Width for Li-line ({AA})"}, {"name": "e_EW-Li", "desc": "[0.01/0.03] Error on EW-Li "}, {"name": "EW-Ha", "desc": "[-1.3/0.93] CHIRON Equivalent Width for H{alpha}-line ({AA})"}, {"name": "e_EW-Ha", "desc": "[0.01/0.05] Error on EW-Ha "}, {"name": "Teff", "desc": "[3257/6465] Effective temperature from SpecMatch "}, {"name": "e_Teff", "desc": "[70/110] Error on Teff "}, {"name": "logg", "desc": "[3.86/4.86] Surface gravity from SpecMatch "}, {"name": "e_logg", "desc": "[0.12] Error on logg "}, {"name": "Fe/H", "desc": "[-0.53/0.19] Metallicity from SpecMatch "}, {"name": "e_Fe/H", "desc": "[0.09] Error on Fe/H "}]}, {"name": "table4.dat", "desc": "Measurements for 12 known members of IC 2602 and IC 2391", "columns": [{"name": "Cluster", "desc": "Cluster identifier "}, {"name": "ID", "desc": "Internal identifier "}, {"name": "f_ID", "desc": "Flag on ID (G1) "}, {"name": "RVel", "desc": "[13.8/39.9] Radial velocity "}, {"name": "e_RVel", "desc": "[0.1/0.2] Error on RVel "}, {"name": "RVel-l", "desc": "[13.8/31.7] Radial velocity from Litterature "}, {"name": "r_RVel-l", "desc": "Reference used for RVel-l (1) "}, {"name": "vsini", "desc": "[7.8/20.8] Rotational velocity "}, {"name": "e_vsini", "desc": "[0.6/2] Error on vsini "}, {"name": "l-vsini-l", "desc": "[<] Limit flag on vsini-l "}, {"name": "vsini-l", "desc": "[8/20.7] Rotational velocity from litterature "}, {"name": "r_vsini-l", "desc": "Reference used for vsini-l (1) "}, {"name": "EW-Li", "desc": "[0.07/0.36] Equivalent Width for Li-line ({AA}) "}, {"name": "e_EW-Li", "desc": "[0/0.02] Error on EW-Li "}, {"name": "EW-Ha", "desc": "[-0.12/0.91] Equivalent Width for H{alpha}-line ({AA})"}, {"name": "e_EW-Ha", "desc": "[0.01/0.02] Error on EW-Ha "}, {"name": "Teff", "desc": "[4614/6150] Effective temperature "}, {"name": "e_Teff", "desc": "[110] Error on Teff "}, {"name": "Teff-l", "desc": "[4520/5900]? Effective temperature from litterature"}, {"name": "r_Teff", "desc": "Reference used for Teff (1) "}, {"name": "logg", "desc": "[4.09/4.6] Surface gravity "}, {"name": "e_logg", "desc": "[0.12] Error on logg "}, {"name": "Fe/H", "desc": "[-0.54/0.15] Metallicity "}, {"name": "e_Fe/H", "desc": "[0.09] Error on Fe/H "}]}, {"name": "tablea1.dat", "desc": "Refined membership list of IC 2391 ", "columns": [{"name": "GAIA", "desc": "Gaia DR2 identifier "}, {"name": "2MASS", "desc": "2MASS identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2015.5) "}, {"name": "DEdeg", "desc": "Declination (J2015.5) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2015.5) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2015.5) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2015.5) "}, {"name": "DE-", "desc": "Sign of Declination (J2015.5) "}, {"name": "DEd", "desc": "Degree of Declination (J2015.5) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2015.5) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2015.5) "}, {"name": "plx", "desc": "Gaia DR2 parallax "}, {"name": "e_plx", "desc": "Mean error in plx "}, {"name": "pmRA", "desc": "Gaia DR2 Proper motion in Right Ascension "}, {"name": "e_pmRA", "desc": "Mean error in pmRA "}, {"name": "pmDE", "desc": "Proper motion in Declination "}, {"name": "e_pmDE", "desc": "Mean error in pmDE "}, {"name": "Gmag", "desc": "Gaia G apparent magnitude "}, {"name": "BP-RP", "desc": "? Gaia BP-RP color "}]}, {"name": "tablea2.dat", "desc": "Refined membership List of IC 2602 ", "columns": [{"name": "GAIA", "desc": "Gaia DR2 identifier "}, {"name": "2MASS", "desc": "2MASS identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2015.5) "}, {"name": "DEdeg", "desc": "Declination (J2015.5) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2015.5) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2015.5) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2015.5) "}, {"name": "DE-", "desc": "Sign of Declination (J2015.5) "}, {"name": "DEd", "desc": "Degree of Declination (J2015.5) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2015.5) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2015.5) "}, {"name": "plx", "desc": "Gaia DR2 parallax "}, {"name": "e_plx", "desc": "Mean error in plx "}, {"name": "pmRA", "desc": "Gaia DR2 Proper motion in Right Ascension "}, {"name": "e_pmRA", "desc": "Mean error in pmRA "}, {"name": "pmDE", "desc": "Proper motion in Declination "}, {"name": "e_pmDE", "desc": "Mean error in pmDE "}, {"name": "Gmag", "desc": "Gaia G apparent magnitude "}, {"name": "BP-RP", "desc": "? Gaia BP-RP color "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_163_293"}} {"id": "J/AJ/163/293", "title_cds": "The TESS-Keck Survey. XI. TOI-1246 RVel", "title_create": "Turtelboom+, 2022", "year": "2022", "author": "Turtelboom E.V., Weiss L.M., Dressing C.D., Nowak G., Palle E., Beard C., Blunt S., Brinkman C., Chontos A., Claytor Z.R., Dai F., Dalba P.A., Giacalone S., Gonzales E., Harada C.K., Hill M.L., Holcomb R., Korth J., Lubin J., Masseron T., MacDougall M., Mayo A.W., Mocnik T., Akana Murphy J.M., Polanski A.S., Rice M., Rubenzahl R.A., Scarsdale N., Stassun K.G., Tyler D.B., Van Zandt J., Crossfield I.J.M., Deeg H.J., Fulton B., Gandolfi D., Howard A.W., Huber D., Isaacson H., Kane S.R., Lam K.W.F., Luque R., Martin E.L., Morello G., Orell-Miquel J., Petigura E.A., Robertson P., Roy A., Van Eylen V., Baker D., Belinski A.A., Bieryla A., Ciardi D.R., Collins K.A., Cutting N., Della-Rose D.J., Ellingsen T.B., Furlan E., Gan T., Gnilka C.L., Guerra P., Howell S.B., Jimenez M., Latham D.W., Lariviere M., Lester K.V., Lillo-Box J., Luker L., Mann C.R., Plavchan P.P., Safonov B., Skinner B., Strakhov I.A., Wittrock J.M., Caldwell D.A., Essack Z., Jenkins J.M., Quintana E.V., Ricker G.R., Vanderspek R., Seager S., Winn J.N.", "title_pub": "The TESS-Keck Survey. XI. Mass Measurements for Four Transiting Sub-Neptunes Orbiting K Dwarf TOI-1246.", "first_author": "Turtelboom E.V.", "ref_biblio": [""], "bibcode": ["2022AJ....163..293T"], "see_also": ["I/259 : The Tycho-2 Catalogue (Hog+ 2000)", "VI/120 : High-resolution synthetic stellar library (Coelho+, 2005)", "J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)", "J/ApJ/720/1118 : i-band photometry of HAT-P-16 (Buchhave+, 2010)", "J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010)", "J/other/A+ARV/18.67 : Accurate masses and radii of normal stars (Torres+, 2010)", "J/AJ/142/19 : Speckle observations of KOI (Howell+, 2011)", "J/A+A/546/A27 : Radial velocity and photometry for GJ3470 (Bonfils+, 2012)", "J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)", "J/MNRAS/426/739 : Velocities for seven transiting hot Jupiters (Hellier+, 2012)", "J/A+A/546/A10 : Multiplicity transiting planet-host stars (Lillo-Box+, 2012)", "J/MNRAS/421/2342 : 4 Kepler systems transit timing observation (Steffen+, 2012)", "J/MNRAS/432/1203 : Rotation periods of M-dwarf stars (McQuillan+, 2013)", "J/ApJ/776/67 : Rotational tracks (van Saders+, 2013)", "J/ApJ/790/146 : Planets in Kepler's multi-transiting systems (Fabrycky+, 2014)", "J/ApJ/785/15 : Transit times Kepler-79's known planets (Jontof-Hutter+, 2014)", "J/A+A/566/A103 : Kepler planet host candidates imaging (Lillo-Box+, 2014)", "J/ApJ/784/45 : Kepler's multiple planet candidates. III. (Rowe+, 2014)", "J/ApJS/210/25 : Transit timing variation 15 planetary pairs. II. (Xie, 2014)", "J/ApJ/822/86 : False positive probabilities Q1-Q17 DR24 KOIs (Morton+, 2016)", "J/AJ/152/180 : Bolometric fluxes eclipsing binaries Tycho-2 (Stassun+, 2016)", "J/ApJ/825/19 : Mass-radius relationship planets with Rp<4 (Wolfgang+, 2016)", "J/ApJ/834/17 : Mass & radius of planets, moons, low mass stars (Chen+, 2017)", "J/A+A/600/A30 : Limb-darkening for TESS satellite (Claret, 2017)", "J/A+A/608/A35 : K2-18 HARPS time-series (Cloutier+, 2017)", "J/AJ/154/109 : California-Kepler Survey. III. Planet radii (Fulton+, 2017)", "J/AJ/153/71 : Kepler follow-up observation program I Imaging (Furlan+, 2017)", "J/AJ/154/5 : Transit timing variations 145 Kepler planets (Hadden+, 2017)", "J/AJ/154/107 : California-Kepler Survey. I. 1305 stars (Petigura+, 2017)", "J/AJ/153/136 : Planets & their host stars with Gaia plxes (Stassun+, 2017)", "J/A+A/618/A142 : Radial velocity for GJ 1132 (Bonfils+, 2018)", "J/AJ/156/102 : TESS Input Catalog and Candidate Target List (Stassun+, 2018)", "J/AJ/155/48 : California-Kepler Survey. V. Masses and radii (Weiss+, 2018)", "J/AJ/157/242 : Updated study of potential targets for Ariel (Edwards+, 2019)", "J/ApJ/876/L24 : HARPS radial velocities of host star HD15337 (Gandolfi+, 2019)", "J/ApJS/250/20 : Rotation periods in TESS objects of interest (Canto+, 2020)", "J/AJ/159/120 : Transit time of K2-146b and K2-146c with K2 & HPF (Lam+, 2020)", "J/AJ/159/57 : HST spectroscopic LCs Kepler 51b & 51d (Libby-Roberts+, 2020)", "J/A+A/640/A48 : K2-32 and K2-233 light and RV curves (Lillo-Box+, 2020)", "J/A+A/646/A157 : HD 108236 CHEOPS light curves (Bonfanti+, 2021)", "J/A+A/653/A41 : L 98-59 (TOI-175) ESPRESSO observations (Demangeon+, 2021)", "J/ApJS/254/39 : Exoplanet candidates from TESS first 2yr obs (Guerrero+, 2021)", "J/AJ/162/216 : Occurrence rates systems with a Venus-like planet (He+, 2021)", "J/A+A/649/A26 : TOI-178 six transiting planets (Leleu+, 2021)", "J/AJ/162/75 : Speckle obs. TESS exoplanet host stars. II. (Lester+, 2021)", "J/AJ/161/56 : The TESS-Keck Survey. II. RVs of TOI-561 (Weiss+, 2021)", "J/AJ/162/55 : 65 Transit-timing variation planets properties (Yee+, 2021)"], "keyword_cds": "Stars, K-type; Exoplanets; Spectra, optical; Radial velocities", "keyword_pub": "Exoplanet astronomy ; Mini Neptunes ; Exoplanets ; Radial velocity ; Transits ; Transit photometry ; Transit timing variation method ; Exoplanet systems", "abstract": ["Multiplanet systems are valuable arenas for investigating exoplanet", "architectures and comparing planetary siblings. TOI-1246 is one such", "system, with a moderately bright K-dwarf (V=11.6, K=9.9) and four", "transiting sub-Neptunes identified by TESS with orbital periods of", "4.31, 5.90, 18.66, and 37.92days. We collected 130 radial velocity", "observations with Keck/HIRES and TNG/HARPS-N to measure planet masses.", "We refit the 14 sectors of TESS photometry to refine planet radii", "(2.97{+/-}0.06R{Earth}, 2.47{+/-}0.08R{Earth}, 3.46{+/-}0.09R{Earth},", "and 3.72{+/-}0.16R{Earth}) and confirm the four planets. We find that", "TOI-1246 e is substantially more massive than the three inner planets", "(8.1{+/-}1.1M{Earth}, 8.8{+/-}1.2M{Earth}, 5.3{+/-}1.7M{Earth}, and", "14.8{+/-}2.3M{Earth}). The two outer planets, TOI-1246d and TOI-1246e,", "lie near to the 2:1 resonance (Pe/Pd=2.03) and exhibit transit-timing", "variations. TOI-1246 is one of the brightest four-planet systems,", "making it amenable for continued observations. It is one of only five", "systems with measured masses and radii for all four transiting", "planets. The planet densities range from 0.70{+/-}0.24 to", "3.21{+/-}0.44g/cm^3^, implying a range of bulk and atmospheric", "compositions. We also report a fifth planet candidate found in the RV", "data with a minimum mass of 25.6{+/-}3.6M{Earth}. This planet", "candidate is exterior to TOI-1246e, with a candidate period of", "93.8days, and we discuss the implications if it is confirmed to be", "planetary in nature."], "description": ["TESS-Keck Survey (TKS) obtained high-resolution spectra of TOI-1246", "using the High Resolution Echelle Spectrograph (HIRES) spectrograph on", "the Keck I telescope on Maunakea. We collected 100 spectra between", "2019 November and 2021 October. HIRES operates between 360 and 800nm,", "and TOI-1246 was observed using the red cross-disperser, C2 decker", "(14\"x0.861\", R=60000), and with a median exposure time of 1004s.", "A further 28 high-resolution spectra of TOI-1246 were collected using", "the HARPS-N instrument installed at the Telescopio Nazionale Galileo", "(TNG) of Roque de los Muchachos Observatory in La Palma, Spain. These", "observations were taken between 2020 February and 2021 September. The", "exposure time was set to 1800-3600s, based on weather conditions and", "scheduling constraints, leading to a signal-to-noise ratio per pixel", "of 25-56 at 5500{AA}."], "object": ["16 44 27.96 +70 25 46.7 TOI-1246 = TOI-1246 (P=93.8d)"], "type": ["OC"], "data": "", "date_update": "19-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Radial velocities & spectral activity indicators measured from Keck/HIRES and TNG/HARPS-N", "columns": [{"name": "BJD", "desc": "[2458896/2459633] Barycentric Julian Date (BJD_TBD_) "}, {"name": "RVel", "desc": "[-17.9/15.8] Radial velocity "}, {"name": "e_RVel", "desc": "[1/3] Error on RVel "}, {"name": "SI", "desc": "[0/0.19] Spectral index "}, {"name": "e_SI", "desc": "[0.001/0.02] Error on SI "}, {"name": "Inst", "desc": "Instrument used; HARPS or HIRES "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_164_17"}} {"id": "J/AJ/164/17", "title_cds": "GJ 1243 flares properties with Kepler and TESS", "title_create": "Mendoza+, 2022", "year": "2022", "author": "Mendoza G.T., Davenport J.R.A., Agol E., Jackman J.A.G., Hawley S.L.", "title_pub": "Llamaradas Estelares; Modeling the Morphology of White-light Flares.", "first_author": "Mendoza G.T.", "ref_biblio": [""], "bibcode": ["2022AJ....164...17M"], "see_also": ["J/AJ/141/50 : White-light flares on cool stars from Kepler (Walkowicz+, 2011)", "J/ApJS/207/15 : M dwarf flare spectra (Kowalski+, 2013)", "J/ApJS/209/5 : Superflares of Kepler stars. I. (Shibayama+, 2013)", "J/ApJS/211/9 : Variability in UV line emission of F-M stars (Loyd+, 2014)", "J/ApJ/829/23 : Stellar flares from Q0-Q17 Kepler LCs (Davenport, 2016)", "J/A+A/590/A11 : BVRI light curves of V374 Peg (Vida+, 2016)", "J/MNRAS/474/2094 : Inferring probabilistic stellar Prot (Angus+, 2018)", "J/MNRAS/483/5045 : R-band light-curve properties SN Ia (Papadogiannakis+, 2019)", "J/ApJ/876/115 : Optical follow-up of ASAS-SN M dwarf flares (Schmidt+, 2019)", "J/AJ/157/234 : ACRONYM. III. Candidate young low-mass stars (Schneider+, 2019)"], "keyword_cds": "Stars, M-type; Stars, flare; Optical", "keyword_pub": "M dwarf stars ; Stellar flares ; Starspots", "abstract": ["Stellar variability is a limiting factor for planet detection and", "characterization, particularly around active M-type stars. Here we", "revisit one of the most active stars from the Kepler mission, the M4", "star GJ1243, and use a sample of 414 flare events from 11 months of", "1-minute cadence light curves to study the empirical morphology of", "white-light stellar flares. We use a Gaussian process detrending", "technique to account for the underlying starspots. We present an", "improved analytic, continuous flare template that is generated by", "stacking the flares onto a scaled time and amplitude and uses a Markov", "Chain Monte Carlo analysis to fit the model. Our model is defined", "using classical flare events but can also be used to model complex,", "multipeaked flare events. We demonstrate the utility of our model", "using TESS data at the 10minute, 2minute, and 20s cadence modes. Our", "new flare model code is made publicly available on GitHub."], "description": ["We studied the morphology of GJ1243 flares in both the Kepler and TESS", "data sets. The data set of 133 flare events detected by Tansiting", "Exoplanet Survey Satellite (TESS) allowed us to test our updated", "analytic flare template using a new data set. We see more scatter in", "the 2minute TESS sample in comparison to the 1minute Kepler data due", "to cadence and signal-to-noise ratio differences but find that our", "updated flare template is able to model the flares from a different", "data set."], "object": ["19 51 09.32 +46 29 00.2 GJ 1243 = G 208-42"], "type": ["OC"], "data": "", "date_update": "20-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Classical flare properties ", "columns": [{"name": "Tpeak", "desc": "[539/1736] Peak time, days "}, {"name": "FWHM", "desc": "[0.0002/0.02] Full time width at half the max of the flux"}, {"name": "Amp", "desc": "[0.003/0.48] Amplitude, relative units "}, {"name": "e_Tpeak", "desc": "Uncertainty in tpeak "}, {"name": "e_FWHM", "desc": "Uncertainty in FWHM "}, {"name": "e_Amp", "desc": "[0.0002/0.05] Uncertainty in Amp "}, {"name": "Inst", "desc": "Source; Kepler or TESS "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_164_20"}} {"id": "J/AJ/164/20", "title_cds": "RGB radial velocities in M31 northeast shelf fields", "title_create": "Escala+, 2022", "year": "2022", "author": "Escala I., Gilbert K.M., Fardal M., Guhathakurta P., Sanderson R.E., Kalirai J.S., Mobasher B.", "title_pub": "Kinematics and Metallicity of Red Giant Branch Stars in the Northeast Shelf of M31.", "first_author": "Escala I.", "ref_biblio": [""], "bibcode": ["2022AJ....164...20E"], "see_also": ["J/MNRAS/369/120 : Kinematic survey of planetary nebulae in M31 (Merrett+, 2006)", "J/ApJ/663/960 : Radial velocities of Leo I stars (Sohn+, 2007)", "J/ApJ/748/29 : Spectroscopy of M87 globular clusters (Romanowsky+, 2012)", "J/ApJ/752/45 : SPLASH Stellar spectroscopy of M31 satellites (Tollerud+, 2012)", "J/ApJ/765/28 : CFHTLS galaxies with faint tidal features (Atkinson+, 2013)", "J/MNRAS/442/3544 : Kinematic tracers in Umbrella galaxy (Foster+, 2014)", "J/ApJS/215/9 : PHAT X. UV-IR photometry of M31 stars (Williams+, 2014)", "J/ApJ/868/55 : Large-scale structure M31 halo. II. PAndAS (McConnachie+, 2018)", "J/ApJ/883/128 : alpha & Fe abundances in giant stellar stream (Gilbert+, 2019)", "J/ApJ/889/177 : RGB abundances in disk, stream & halo of M31 (Escala+, 2020)", "J/ApJ/902/51 : Abundances for M31 RGB stars from Keck/DEIMOS (Escala+, 2020)"], "keyword_cds": "Stars, giant; Spectra, optical; Radial velocities", "keyword_pub": "Galaxy structure ; Andromeda Galaxy ; Galaxy mergers ; Galaxy dynamics", "abstract": ["We obtained Keck/DEIMOS spectra of 556 individual red giant branch", "stars in four spectroscopic fields spanning 13-31 projected kpc along", "the northeast (NE) shelf of M31. We present the first detection of a", "complete wedge pattern in the space of projected M31-centric radial", "distance versus line-of-sight velocity for this feature, which", "includes the returning stream component of the shelf. This wedge", "pattern agrees with expectations of a tidal shell formed in a radial", "merger and provides strong evidence in favor of predictions of Giant", "Stellar Stream (GSS) formation models in which the NE shelf originates", "from the second orbital wrap of the tidal debris. The observed", "concentric wedge patterns of the NE, west (W), and southeast (SE)", "shelves corroborate this interpretation independently of the models.", "We do not detect a kinematical signature in the NE shelf region", "corresponding to an intact progenitor core, favoring GSS formation", "models in which the progenitor is completely disrupted. The shelf's", "photometric metallicity ([Fe/H]_phot_) distribution implies that it is", "dominated by tidal material, as opposed to the phase-mixed stellar", "halo or the disk. The metallicity distribution", "([Fe/H]_phot_=-0.42{+/-}0.01) also matches the GSS, and consequently", "the W and SE shelves, further supporting a direct physical association", "between the tidal features."], "description": ["We observed five slit masks targeting M31's northeast (NE) shelf with", "the DEep Imaging Multi-Object Spectrograph (DEIMOS) instrument on Keck", "II as part of the Spectroscopic and Photometric Landscape of", "Andromeda's Stellar Halo (SPLASH) survey. We utilized the 1200line/mm", "grating, which has a spectral dispersion of 0.33{AA}/pixel, with the", "OG550 order-blocking filter and a central wavelength of 7800{AA} for", "our science configuration. The spectroscopic fields were observed in", "fall 2011 with ~1hr exposures."], "object": ["00 42 44.33 +41 16 07.5 M 31 = M 31"], "type": ["OC"], "data": "", "date_update": "21-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Catalog of velocity measurements for M31 RGB stars in the northeast shelf fields", "columns": [{"name": "ID", "desc": "Object identifier "}, {"name": "RAh", "desc": "[00] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[47/53] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[41/42] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Vmag", "desc": "[22.1/24.4] Extinction-corrected V-band Vega magnitude"}, {"name": "Imag", "desc": "[20.1/22.4] Extinction-corrected I-band Vega magnitude"}, {"name": "e_Vmag", "desc": "[0.01/0.2] Uncertainty in Vmag "}, {"name": "e_Imag", "desc": "[0.01/0.2] Uncertainty in Imag "}, {"name": "RVel", "desc": "[-541/-100] Heliocentric velocity (1) "}, {"name": "e_RVel", "desc": "[2/21] Uncertainty in RVel "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_164_21"}} {"id": "J/AJ/164/21", "title_cds": "K2-139 G-band photometry with CHEOPS", "title_create": "Smith+, 2022", "year": "2022", "author": "Smith A.M.S., Csizmadia S.", "title_pub": "A CHEOPS Search for Massive, Long-period Companions to the Warm Jupiter K2-139b.", "first_author": "Smith A.M.S.", "ref_biblio": [""], "bibcode": ["2022AJ....164...21S"], "see_also": ["J/A+A/643/A94 : CHEOPS WASP-189 b transit light curve (Lendl+, 2020)", "J/A+A/646/A157 : HD 108236 CHEOPS light curves (Bonfanti+, 2021)", "J/A+A/653/A173 : CHEOPS 55 Cnc light curve (Morris+, 2021)", "J/MNRAS/506/3810 : 7 transiting exoplanets CHEOPS light curves (Borsato+, 2021)", "J/other/ExA/51.109 : Transit KELT-11b observed by CHEOPS (Benz+, 2021)", "J/other/NatAs/5.775 : nu2 Lupi CHEOPS light curves (Delrez+, 2021)", "J/other/RNAAS/5.13 : CHEOPS limb & gravity-darkening coefficient (Claret, 2021)", "J/A+A/657/A52 : CHEOPS transit light curves of WASP-103 b (Barros+, 2022)", "J/A+A/659/A74 : CHEOPS phase curve of WASP-189 b (Deline+, 2022)", "J/A+A/659/L7 : AU Mic b and c transits with CHEOPS (Szabo+, 2022)", "J/A+A/664/L15 : Quaoar stellar occultation observed by CHEOPS (Morgado+, 2022)", "J/MNRAS/511/4551 : TOI-561 CHEOPS light curves (Lacedelli+, 2022)", "J/MNRAS/514/77 : CHEOPS Early Science observations (Maxted+, 2022)"], "keyword_cds": "Stars, K-type; Exoplanets; Photometry, G band", "keyword_pub": "Extrasolar gaseous giant planets; Exoplanet astronomy; Exoplanets", "abstract": ["K2-139b is a warm Jupiter with an orbital period of 28.4days, but only", "three transits of this system have previously been observed-in the", "long-cadence mode of K2-limiting the precision with which the orbital", "period can be determined and future transits predicted. We report", "photometric observations of four transits of K2-139b with ESA's", "CHaracterising ExOPlanet Satellite (CHEOPS), conducted with the goal", "of measuring the orbital obliquity via spot-crossing events. We", "jointly fit these CHEOPS data alongside the three previously-published", "transits from the K2 mission, considerably increasing the precision of", "the ephemeris of K2-139b. The transit times for this system can now be", "predicted for the next decade with a 1{sigma} precision less than 10", "minutes, compared to over one hour previously, allowing the efficient", "scheduling of observations with Ariel. We detect no significant", "deviation from a linear ephemeris, allowing us to exclude the presence", "of a massive outer planet orbiting with a period less than 150 days,", "or a brown dwarf with a period less than one year. We also determine", "the scaled semimajor axis, the impact parameter, and the stellar limb", "darkening with improved precision. This is driven by the shorter", "cadence of the CHEOPS observations compared to that of K2, and", "validates the subexposure technique used for analyzing long-cadence", "photometry. Finally, we note that the stellar spot configuration has", "changed from the epoch of the K2 observations; unlike the K2 transits,", "we detect no evidence of spot-crossing events in the CHEOPS data."], "description": ["CHaracterising ExOPlanet Satellite (CHEOPS) is a small (0.32m", "diameter) telescope designed for high-precision monoband photometry of", "individual exoplanetary systems. We observed two consecutive transits", "in 2020 June and July, and a second pair of consecutive transits in", "2021 June and July. Each \"visit\" consisted of seven consecutive orbits", "of the CHEOPS satellite, or around 11.5hr. With a G-band magnitude of", "11.5, K2-139 is a relatively faint target for CHEOPS, and therefore an", "exposure time of 60s was used."], "object": ["19 16 15.97 -17 54 38.4 K2-139 = K2-139 (P=28.38282d)"], "type": ["OC"], "data": "", "date_update": "21-Oct-2022", "tables": [{"name": "table2.dat", "desc": "CHEOPS light curve of K2-139 ", "columns": [{"name": "BJD", "desc": "[9028/9398] Barycentric Julian Date at TDB; BJD-2450000"}, {"name": "Flux", "desc": "[0.97/1.02] Relative flux "}, {"name": "e_Flux", "desc": "[0.0007/0.0009] Error on Flux "}, {"name": "Roll", "desc": "[19.3/344] Spacecraft roll angle "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_164_25"}} {"id": "J/AJ/164/25", "title_cds": "Velocity data for 148590 stars in the Kepler field", "title_create": "Angus+, 2022", "year": "2022", "author": "Angus R., Price-Whelan A.M., Zinn J.C., Bedell M., Lu Y., Foreman-Mackey D.", "title_pub": "The 3D Galactocentric Velocities of Kepler Stars; Marginalizing Over Missing Radial Velocities.", "first_author": "Angus R.", "ref_biblio": [""], "bibcode": ["2022AJ....164...25A"], "see_also": ["I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)", "V/117 : Geneva-Copenhagen Survey of Solar neighbourhood (Holmberg+, 2007)", "V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)", "V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)", "J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)", "J/A+A/530/A138 : Geneva-Copenhagen survey re-analysis (Casagrande+, 2011)", "J/ApJ/821/93 : Rotation & Galactic kinematics of mid M dwarfs (Newton+, 2016)", "J/AJ/153/257 : Comoving stars in Gaia DR1 (Oh+, 2017)", "J/AJ/158/190 : Main sequence hot Jupiter hosts good astrometry (Hamer+, 2019)", "J/AJ/157/231 : MLSDSS-GaiaDR2 sample of M and L dwarfs (Kiman+, 2019)", "J/ApJ/878/21 : Vertical motions APOGEE & Gaia red clump stars (Ting+, 2019)", "J/ApJS/245/34 : Abundances for 6 million stars from LAMOST DR5 (Xiang+, 2019)", "J/AJ/160/90 : Stellar parameters for 13196 Kepler dwarfs (Angus+, 2020)", "J/ApJ/888/43 : APOGEE-Kepler Cool Dwarf star ages (Claytor+, 2020)", "J/ApJ/904/140 : Ruprecht 147 members & rot. for 5 other cl. (Curtis+, 2020)", "J/AJ/161/189 : Gyro-kinematic ages for ~30000 Kepler stars (Lu+, 2021)"], "keyword_cds": "Milky Way; Stars, late-type; Proper motions; Radial velocities Parallaxes, trigonometric", "keyword_pub": "Milky Way dynamics ; Late-type stars ; Solar neighborhood ; Stellar properties ; Stellar ages", "abstract": ["Precise Gaia measurements of positions, parallaxes, and proper motions", "provide an opportunity to calculate 3D positions and 2D velocities", "(i.e., 5D phase-space) of Milky Way stars. Where available,", "spectroscopic radial velocity (RVel) measurements provide full 6D", "phase-space information, however there are now and will remain many", "stars without RV measurements. Without an RVel it is not possible to", "directly calculate 3D stellar velocities; however, one can infer 3D", "stellar velocities by marginalizing over the missing RV dimension. In", "this paper, we infer the 3D velocities of stars in the Kepler field in", "Cartesian Galactocentric coordinates (vx, vy, vz). We directly", "calculate velocities for around a quarter of all Kepler targets, using", "RV measurements available from the Gaia, LAMOST, and APOGEE", "spectroscopic surveys. Using the velocity distributions of these stars", "as our prior, we infer velocities for the remaining three quarters of", "the sample by marginalizing over the RV dimension. The median", "uncertainties on our inferred vx, vy, and vz velocities are around 4,", "18, and 4km/s, respectively. We provide 3D velocities for a total of", "148590 stars in the Kepler field. These 3D velocities could enable", "kinematic age-dating, Milky Way stellar population studies, and other", "scientific studies using the benchmark sample of well-studied Kepler", "stars. Although the methodology used here is broadly applicable to", "targets across the sky, our prior is specifically constructed from and", "for the Kepler field. Care should be taken to use a suitable prior", "when extending this method to other parts of the Galaxy."], "type": ["GCC"], "data": "", "date_update": "21-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Velocities and kinematic information for stars in the Kepler field", "columns": [{"name": "Seq", "desc": "[0/148589] Sequential number identifier "}, {"name": "KIC", "desc": "Kepler Input catalog identifier "}, {"name": "Gaia", "desc": "Gaia EDR3 identifier "}, {"name": "RAdeg", "desc": "[279/302] Gaia EDR3 right ascension (ICRS) "}, {"name": "e_RAdeg", "desc": "[0.006/0.1] Uncertainty in RAdeg "}, {"name": "DEdeg", "desc": "[36/53] Gaia EDR3 declination (ICRS) "}, {"name": "e_DEdeg", "desc": "[0.007/0.1] Uncertainty in DEdeg "}, {"name": "plx", "desc": "[0.09/18.6] Gaia EDR3 parallax "}, {"name": "e_plx", "desc": "[0.007/0.1] Uncertainty in plx "}, {"name": "Dist", "desc": "[53/18256]? Distance; Bailer-Jones+, 2021, I/352"}, {"name": "b_Dist", "desc": "[53/14207]? Lower bound on Dist "}, {"name": "B_Dist", "desc": "[53/23570]? Upper bound on Dist "}, {"name": "pmRA", "desc": "[-37.7/40.3] Gaia EDR3 proper motion in RA "}, {"name": "e_pmRA", "desc": "[-38/41] Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-39.2/38.7] Gaia EDR3 proper motion in DE "}, {"name": "e_pmDE", "desc": "[-40/39] Uncertainty in pmDE "}, {"name": "RVel-DR2", "desc": "[-393/107]? Gaia DR2 radial velocity "}, {"name": "e_RVel-DR2", "desc": "[0.1/20]? Uncertainty in RVel-DR2 "}, {"name": "RVel-apo", "desc": "[-589/71]? APOGEE DR16 radial velocity "}, {"name": "e_RVel-apo", "desc": "[0.0005/2]? Uncertainty in RVel-apo "}, {"name": "RVel-lam", "desc": "[-403.0/94.0]? LAMOST DR5 radial velocity "}, {"name": "e_RVel-lam", "desc": "[1/89]? Uncertainty in RVel-lam "}, {"name": "vx-calc", "desc": "[-838/1421]? vx velocity calculated using RVel "}, {"name": "vx-inf", "desc": "[-307/387] vx velocity sample, inferred without RVel"}, {"name": "e_vx-inf", "desc": "[2/18] Standard deviation of vx "}, {"name": "vy-calc", "desc": "[-312/621]? vy velocity calculated using RVel "}, {"name": "vy-inf", "desc": "[115/289] vy velocity sample, inferred without RVel"}, {"name": "e_vy-inf", "desc": "[20/26] Standard deviation of vy "}, {"name": "vz-calc", "desc": "[-714/1090]? zx velocity calculated using RVel "}, {"name": "vz-inf", "desc": "[-192/194] vz velocity sample, inferred without RVel"}, {"name": "e_vz-inf", "desc": "[2/11] Standard deviation of vz "}, {"name": "vxvy", "desc": "[28/225] covariance between vx and vy samples "}, {"name": "vxvz", "desc": "[-25/97] covariance between vx and vz samples "}, {"name": "vxlnd", "desc": "[-0.6/2] covariance between vx and ln(distance) samples"}, {"name": "vyvz", "desc": "[54.3/206] covariance between vy & vz samples "}, {"name": "vylnd", "desc": "[-0.35/0.16] covariance between vy and ln(distance) samples"}, {"name": "vzlnd", "desc": "[-0.38/0.35] covariance between vz and ln(distance) samples"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_164_26"}} {"id": "J/AJ/164/26", "title_cds": "102 hot Jupiters isochrone analyse & stellar modeling", "title_create": "Hamer+, 2022", "year": "2022", "author": "Hamer J.H., Schlaufman K.C.", "title_pub": "Evidence for the Late Arrival of Hot Jupiters in Systems with High Host-star Obliquities.", "first_author": "Hamer J.H.", "ref_biblio": [""], "bibcode": ["2022AJ....164...26H"], "see_also": ["B/simbad : Simbad objects catalogue (M.Wenger 2000)", "I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "II/335 : Revised catalog of GALEX UV sources (Bianchi+ 2017)", "VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "J/ApJ/651/L49 : Upper Sco OB association IRAC observations (Carpenter+, 2006)", "J/ApJ/683/1076 : Transits of exoplanet XO-3b (Winn+, 2008)", "J/ApJ/707/446 : HAT-P-13 photometry follow-up (Bakos+, 2009)", "J/ApJ/706/785 : HAT-P-12 light curve (Hartman+, 2009)", "J/ApJ/704/1107 : Transiting planet candidates HATNet field 205 (Latham+, 2009)", "J/A+A/502/391 : WASP-13b photometry and radial velocities (Skillen+, 2009)", "J/A+A/502/395 : WASP-11b (West+, 2009)", "J/ApJ/700/302 : Relative photometry of XO-3 (Winn+, 2009)", "J/ApJ/709/159 : Relative Ic photometry of WASP-17 (Anderson+, 2010)", "J/A+A/519/A98 : Transit of exoplanet WASP-21b (Bouchy+, 2010)", "J/ApJ/720/1118 : i-band photometry of HAT-P-16 (Buchhave+, 2010)", "J/ApJ/725/2017 : Sloan i-band light curve of HAT-P-24 (Kipping+, 2010)", "J/A+A/520/A56 : WASP-26b RV and photometric data (Smalley+, 2010)", "J/ApJ/715/458 : Differential photometry of HAT-P-14 (Torres+, 2010)", "J/A+A/524/A25 : Radial Velocities on 6 exoplanet host stars (Triaud+, 2010)", "J/A+A/534/A16 : WASP-22 & WASP-26 photometry and velocities (Anderson+, 2011)", "J/ApJ/742/116 : Photometry of 4 massive transiting exoplanets (Bakos+, 2011)", "J/A+A/525/A54 : Transits of WASP-38b (Barros+, 2011)", "J/A+A/531/A40 : Transits of WASP-39b (Faedi+, 2011)", "J/ApJ/726/52 : HAT-P-18 and HAT-P-19 follow-up (Hartman+, 2011)", "J/A+A/527/L11 : HAT-P-6 radial velocity curve (Hebrard+, 2011)", "J/ApJ/735/24 : HAT-P-30 follow-up photometry (Johnson+, 2011)", "J/AJ/141/63 : Relative radial velocities of HAT-P-4 & HAT-P-14 (Winn+, 2011)", "J/ApJ/757/18 : Radial velocities 16 hot Jupiter host stars (Albrecht+, 2012)", "J/AJ/144/19 : Follow-up photometry HAT-P-34 through HAT-P-37 (Bakos+, 2012)", "J/MNRAS/423/1503 : RV curves of WASP-16, 25 and 31 (Brown+, 2012)", "J/ApJ/750/84 : Follow-up photometry and velocity of Qatar 2 (Bryan+, 2012)", "J/AJ/144/139 : HAT-P-39, HAT-P-40, and HAT-P-41 follow-up (Hartman+, 2012)", "J/MNRAS/426/739 : Velocities for seven transiting hot Jupiters (Hellier+, 2012)", "J/ApJ/745/19 : Binary systems in Taurus-Auriga (Kraus+, 2012)", "J/A+A/544/A72 : WASP-42 and WASP-49 photometry and velocities (Lendl+, 2012)", "J/A+A/547/A61 : WASP78 and WASP79 RV and photometric data (Smalley+, 2012)", "J/A+A/552/A82 : WASP-64b and WASP-72b light curves (Gillon+, 2013)", "J/A+A/549/A134 : 4 new WASP transiting close-in giant planets (Hebrard+, 2013)", "J/A+A/556/A150 : SWEETCat I. Stellar parameters for host stars (Santos+, 2013)", "J/A+A/552/A120 : WASP-71b light curve (Smith+, 2013)", "J/A+A/551/A80 : WASP-80 photometric and radial velocity data (Triaud+, 2013)", "J/MNRAS/445/1114 : WASP-69b, WASP-70Ab and WASP-84b (Anderson+, 2014)", "J/A+A/562/L3 : WASP-103b radial velocities and light curves (Gillon+, 2014)", "J/A+A/572/A49 : WASP-94AB photo. & radial velocities (Neveu-VanMalle+, 2014)", "J/AJ/150/12 : Radial velocity of HD 33643 (Bieryla+, 2015)", "J/A+A/575/A111 : GAPS V: Global analysis of the XO-2 system (Damasso+, 2015)", "J/AJ/150/85 : Photometry and spectroscopy of HAT-P-56 (Huang+, 2015)", "J/A+A/579/A136 : HAT-P-36 and WASP-11/HAT-P-10 light curves (Mancini+, 2015)", "J/ApJ/801/3 : Rotation periods for Q3-Q14 KOIs (Mazeh+, 2015)", "J/MNRAS/450/1760 : Transiting planet WASP-6b (Tregloan-Reed+, 2015)", "J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016)", "J/A+A/594/A50 : K2-30 b and K2-34 b K2 light curves (Lillo-Box+, 2016)", "J/AJ/152/127 : Sloan i follow-up light curves of HATS-18 (Penev+, 2016)", "J/MNRAS/457/4205 : WASP-22, WASP-41, WASP-42, WASP-55 (Southworth+, 2016)", "J/A+A/585/A126 : 3 irradiated & bloated hot Jupiters RV and phot. (West+, 2016)", "J/A+A/608/A135 : Na detection in WASP-69b atmosphere (Casasayas-Barris+, 2017)", "J/A+A/599/A3 : WASP 127, 136 and 138 RV and light curves (Lam+, 2017)", "J/AJ/154/107 : California-Kepler Survey. I. 1305 stars (Petigura+, 2017)", "J/ApJS/237/38 : Extended abundance analysis of KOIs (Brewer+, 2018)", "J/ApJ/860/109 : Keck HIRES obs. 245 subgiants (retired Astars) (Ghezzi+, 2018)", "J/A+A/613/A41 : 5 exoplanet light and RV curves (Mancini+, 2018)", "J/AJ/155/165 : Dissipation exoplanet hosts from tidal spin-up (Penev+, 2018)", "J/A+A/620/A58 : SWEET-Cat updated (Sousa+, 2018)", "J/AJ/158/190 : Main sequence hot Jupiter hosts good astrometry (Hamer+, 2019)", "J/AJ/158/197 : Radial velocities & light curves of KELT-24 (Rodriguez+, 2019)", "J/AJ/157/141 : Radial velocity and light curves of WASP-190 (Temple+, 2019)", "J/AJ/158/141 : Differential photo. & RVs of HAT-P-69 & HAT-P-70 (Zhou+, 2019)", "J/A+A/635/A205 : Ultra-hot Jupiter WASP-121b transits (Bourrier+, 2020)", "J/A+A/640/A32 : WASP-148 velocity curve (Hebrard+, 2020)", "J/A+A/642/A50 : WASP-74 griz_s_ light curves (Luque+, 2020)", "J/AJ/160/214 : 130 Stellar ages & planetary orbital prop. (Safsten+, 2020)", "J/AJ/161/68 : Obliquities of 150 hot Kepler hosting stars (Louden+, 2021)", "J/A+A/649/A3 : Gaia EDR 3 photometric passbands (Riello+, 2021)", "J/A+A/653/A160 : Updated radial velocities from Gaia DR2 (Seabroke+, 2021)", "J/AJ/163/159 : Species abundances in WASP-77A (Reggiani+, 2022)", "J/AJ/163/158 : BRV light curve of XO-3 (Worku+, 2022)"], "keyword_cds": "Exoplanets; Spectroscopy; Photometry, UBVRIJKLMNH; Stars, ages; Stars, masses; Effective temperatures; Extinction", "keyword_pub": "Exoplanet dynamics ; Exoplanet tides ; Exoplanet evolution ; Exoplanet systems ; Exoplanets ; Stellar ages ; Stellar kinematics ; Tidal interaction ; Star-planet interactions", "abstract": ["It has been shown that hot Jupiters systems with massive, hot stellar", "primaries exhibit a wide range of stellar obliquities. On the other", "hand, hot Jupiter systems with low-mass, cool primaries often have", "stellar obliquities close to zero. Efficient tidal interactions", "between hot Jupiters and the convective envelopes present in", "lower-mass main-sequence stars have been a popular explanation for", "these observations. If this explanation is accurate, then aligned", "systems should be older than misaligned systems. Likewise, the", "convective envelope mass of a hot Jupiter's host star should be an", "effective predictor of its obliquity. We derive homogeneous stellar", "parameters-including convective envelope masses-for hot Jupiter host", "stars with high-quality sky-projected obliquity inferences. Using a", "thin-disk stellar population's Galactic velocity dispersion as a", "relative age proxy, we find that hot Jupiter host stars with", "larger-than-median obliquities are older than hot Jupiter host stars", "with smaller-than-median obliquities. The relative age difference", "between the two populations is larger for hot Jupiter host stars with", "smaller-than-median fractional convective envelope masses and is", "significant at the 3.6{sigma} level. We identify stellar mass, not", "convective envelope mass, as the best predictor of stellar obliquity", "in hot Jupiter systems. The best explanation for these observations is", "that many hot Jupiters in misaligned systems arrived in the close", "proximity of their host stars long after their parent protoplanetary", "disks dissipated. The dependence of observed age offset on convective", "envelope mass suggests that tidal realignment contributes to the", "population of aligned hot Jupiters orbiting stars with convective", "envelopes."], "description": ["We retrieve all known hot Jupiters from the NASA Exoplanet Archive as", "of 2022 February 15 following the definition P<10days and Mpl>0.1MJup.", "The data queried from the NASA Exoplanet Archive include Gaia DR2 for", "the hot Jupiter host stars. Next, we use the Gaia EDR3 neighbourhood", "table provided by the Gaia Archive.", "We then obtain the photometry for our sample of hot Jupiter hosts to", "enable us to fit MESA Isochrones & Stellar Tracks (MIST) isochrones to", "our data. We query the Gaia Archive for the Gaia DR2 photometry of our", "hosts.", "We use the Gaia crossmatch best neighbor tables to identify the", "corresponding AllWISE, Wide-field Infrared Survey Explorer (WISE), Two", "Micron All Sky Survey (2MASS), SDSS DR13, and SkyMapper Data Release 2", "identifiers. We query Galaxy Evolution Explorer (GALEX) on VizieR", "using the Gaia EDR3 designations of our host stars."], "type": ["GCC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "*Isochrone analysis input data and stellar modeling output data", "columns": [{"name": "Name", "desc": "Planet's host star name "}, {"name": "plx", "desc": "[0.98/50.6] Gaia EDR3 parallax "}, {"name": "e_plx", "desc": "[0.008/0.2] Error on plx "}, {"name": "AVmag", "desc": "[0/0.54] Extinction in V band from dust map "}, {"name": "e_AVmag", "desc": "[0/0.5] Error on extinction in AVmag "}, {"name": "Teff", "desc": "[4143/10170]? Effective temperature from spectroscopy"}, {"name": "e_Teff", "desc": "[7/480]? Error on Teff "}, {"name": "logg", "desc": "[3.92/4.8]? Surface gravity from spectroscopy "}, {"name": "e_logg", "desc": "[0.01/0.7]? Error on logg "}, {"name": "[Fe/H]", "desc": "[-0.41/0.5]? Metallicity from spectroscopy "}, {"name": "e_[Fe/H]", "desc": "[0.01/0.1]? Error on [Fe/H] "}, {"name": "NUVmag", "desc": "[12.9/21.9]? GALEX NUV magnitude "}, {"name": "e_NUVmag", "desc": "[0.002/0.4]? Error on NUVmag "}, {"name": "umag", "desc": "[9.38/17]? SDSS or SkyMapper u band magnitude "}, {"name": "e_umag", "desc": "[0.003/0.04]? Error on umag "}, {"name": "vmag", "desc": "[8.72/16.2]? SkyMapper v band magnitude "}, {"name": "e_vmag", "desc": "[0.003/0.02]? Error on vmag "}, {"name": "gmag", "desc": "[9.85/15.5]? SDSS or SkyMapper g band magnitude"}, {"name": "e_gmag", "desc": "[0.004/0.04]? Error on gmag "}, {"name": "rmag", "desc": "[9.58/14.8]? SDSS or SkyMapper r band magnitude"}, {"name": "e_rmag", "desc": "[0.004/0.02]? Error on rmag "}, {"name": "imag", "desc": "[9.42/14.6]? SDSS or SkyMapper i band magnitude"}, {"name": "e_imag", "desc": "[0.004/0.03]? Error on imag "}, {"name": "zmag", "desc": "[10.4/14.5]? SDSS or SkyMapper z band magnitude"}, {"name": "e_zmag", "desc": "[0.003/0.03]? Error on zmag "}, {"name": "BPmag", "desc": "[7.61/15.3] Gaia DR2 BP mean magnitude "}, {"name": "e_BPmag", "desc": "[0.002/0.01] Error on BPmag "}, {"name": "Gmag", "desc": "[7.41/14.9] Gaia DR2 G mean magnitude "}, {"name": "e_Gmag", "desc": "[0.0003/0.002] Error on Gmag "}, {"name": "RPmag", "desc": "[6.8/14.2] Gaia DR2 RP mean magnitude "}, {"name": "e_RPmag", "desc": "[0.002/0.01] Error on RPmag "}, {"name": "Jmag", "desc": "[6.07/13.5]? 2MASS J magnitude "}, {"name": "e_Jmag", "desc": "[0.01/0.05]? Error on Jmagn "}, {"name": "Hmag", "desc": "[5.58/13.09]? 2MASS H magnitude "}, {"name": "e_Hmag", "desc": "[0.01/0.06]? Error on Hmag "}, {"name": "Kmag", "desc": "[5.54/13.1]? 2MASS K magnitude "}, {"name": "e_Kmag", "desc": "[0.01/0.04]? Error on Kmag "}, {"name": "W1mag", "desc": "[7.46/13]? AllWISE or WISE W1 magnitude "}, {"name": "e_W1mag", "desc": "[0.02/0.1]? Error on W1mag "}, {"name": "W2mag", "desc": "[7.12/13]? AllWISE or WISE W2 magnitude "}, {"name": "e_W2mag", "desc": "[0.01/0.04]? Error on W2mag "}, {"name": "Age", "desc": "[126918579/13059983270] Stellar age from isochrone analysis"}, {"name": "e_Age", "desc": "[18199649/1924875180] Lower uncertainty Age "}, {"name": "E_Age", "desc": "[7706714/1776789285] Upper uncertainty on Age "}, {"name": "[Fe/H]-i", "desc": "[-0.31/0.57] Stellar metallicity from isochrone analysis"}, {"name": "e_[Fe/H]-i", "desc": "[0.004/0.05] Lower uncertainty on [Fe/H]-i "}, {"name": "E_[Fe/H]-i", "desc": "[0.003/0.05] Upper uncertainty on [Fe/H]-i "}, {"name": "Mass", "desc": "[0.61/2.36] Stellar mass from isochrone analysis"}, {"name": "e_Mass", "desc": "[0.001/0.06] Lower uncertainty on Mass "}, {"name": "E_Mass", "desc": "[0.002/0.06] Upper uncertainty on Mass "}, {"name": "Rad", "desc": "[0.6/2.33] Stellar radius from isochrone analysis"}, {"name": "e_Rad", "desc": "[0.001/0.04] Lower uncertainty on Rad "}, {"name": "E_Rad", "desc": "[0.0009/0.05] Upper uncertainty on Rad "}, {"name": "Teff-i", "desc": "[4096/9711] Stellar effective temperature from isochrone analysis"}, {"name": "e_Teff-i", "desc": "[1/118] Lower uncertainty on Teff-i "}, {"name": "E_Teff", "desc": "[2/177] Upper uncertainty on Teff-i "}, {"name": "logg-i", "desc": "[3.94/4.66] Stellar surface gravity from isochrone analysis"}, {"name": "e_logg-i", "desc": "[0.001/0.03] Lower uncertainty on logg-i "}, {"name": "E_logg-i", "desc": "[0.002/0.03] Upper uncertainty on logg-i "}, {"name": "AVmag-i", "desc": "[0.0006/0.63] Extinction in V band from isochrone analysis"}, {"name": "e_AVmag-i", "desc": "[0.0005/0.07] Lower uncertainty on AVmag-i "}, {"name": "E_AVmag-i", "desc": "[0.0004/0.06] Upper uncertainty on AVmag-i "}, {"name": "fMass", "desc": "[0/0.73] Fraction of stellar mass in surface convective envelope"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_164_34"}} {"id": "J/AJ/164/34", "title_cds": "Short Title", "title_create": "Morales+, 2022", "year": "2022", "author": "Morales L.M., Sandquist E.L., Schaefer G.H., Farrington C.D., Klement R., Bedin L.R., Libralato M., Malavolta L., Nardiello D., Orosz J.A., Monnier J.D., Kraus S., Le Bouquin J.-B., Anugu N., Ten Brummelaar T., Davies C.L., Ennis J., Gardner T., Lanthermann C.", "title_pub": "The Interferometric Binary {epsilon} Cnc in Praesepe: Precise Masses and Age.", "first_author": "Morales L.M.", "ref_biblio": [""], "bibcode": ["2022AJ....164...34M"], "keyword_cds": "", "keyword_pub": "Open star clusters; Spectroscopic binary stars; White dwarf stars Stellar evolution; Long baseline interferometry", "mission": "", "abstract": ["We observe the brightest member of the Praesepe cluster, \u03f5 Cnc, to precisely measure the characteristics of the stars in this binary system, en route to a new measurement of the cluster's age. We present spectroscopic radial velocity measurements and interferometric observations of the sky-projected orbit to derive the masses, which we find to be M_1_/M_\u2299_ = 2.420 \u00b1 0.008 and M_2_/M_\u2299_ = 2.226 \u00b1 0.004. We place limits on the color-magnitude positions of the stars by using spectroscopic and interferometric luminosity ratios while trying to reproduce the spectral energy distribution of \u03f5 Cnc. We reexamine the cluster membership of stars at the bright end of the color-magnitude diagram using Gaia data and literature radial velocity information. The binary star data are consistent with an age of 637 \u00b1 19 Myr, as determined from MIST model isochrones. The masses and luminosities of the stars appear to select models with the most commonly used amount of convective core overshooting."], "object": [], "curator": "Coralie Fix [CDS]", "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AJ_164_36"}} {"id": "J/AJ/164/36", "title_cds": "", "title_create": "Zacharias+, 2022", "year": "2022", "author": "Zacharias N., Makarov V.V., Finch C.T., Harris H.C., Munn J.A., Subasavage J.P.", "title_pub": "USNO Bright Star Catalog, Version 1.", "first_author": "Zacharias N.", "ref_biblio": [""], "bibcode": ["2022AJ....164...36Z"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/A+A/397/997 : Hipparcos red stars (Platais+, 2003)", "J/A+A/399/1167 : Hipparcos Variability-Induced Movers (Pourbaix+, 2003)", "J/AJ/129/2420 : Proper motion derivatives of binaries (Makarov+, 2005)", "J/AJ/131/2967 : {alpha} Persei open cluster members (Makarov+, 2006)", "J/A+A/623/A72 : Binarity of Hipparcos stars Gaia pm anomaly (Kervella+, 2019)", "J/ApJS/254/42 : Hipparcos-Gaia (EDR3) Catalog of Accelerations (Brandt, 2021)", "J/AJ/163/131 : USNO-UBAD catalog of bright stars (Munn+, 2022)"], "keyword_cds": "", "keyword_pub": "Astrometry ; Catalogs ; Proper motions ; Trigonometric parallax ; Astrometric binary stars", "abstract": ["The U.S. Naval Observatory (USNO) Bright Star Catalog (UBSC) is a new", "astrometric catalog of the 1423 brightest stars covering the entire", "sky, which is published online. It is nearly complete to V=3mag except", "for three stellar systems. A combined astrometric solution of the", "Hipparcos Intermediate Astrometry Data and two dedicated ground-based", "campaigns in 2013-2020 is the basis for this catalog. The astrometric", "parameters for each star include position coordinates, parallax, and", "proper motion components, and their covariances on the Hipparcos mean", "epoch 1991.25. 64% of the catalog are flagged as known or suspected", "double or binary stars. UBSC lists 68 stars missing in Gaia EDR3 and", "another 114 stars without Gaia parallaxes or proper motions. The", "formal precision achieved for proper motions is comparable to that of", "Gaia."], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "*The USNO Bright Star Catalog ", "columns": [{"name": "HIP", "desc": "Hipparcos identifier "}, {"name": "Hpmag", "desc": "[-0.56/7.98] Hipparcos apparent magnitude "}, {"name": "B-V", "desc": "[-0.27/3.34] The (B-V) color from Hipparcos "}, {"name": "Bin", "desc": "[0/7] Binarity/perturbed flag (1) "}, {"name": "Source", "desc": "[1/3] Source flag (2) "}, {"name": "Num", "desc": "[23/628] Number of observational equations in HUU "}, {"name": "chi2", "desc": "[22/910911] The {chi}^2^ of residuals "}, {"name": "MAD", "desc": "[0.32/26.9] MAD of residuals * 1.5 "}, {"name": "RAdeg", "desc": "[0/360] Right Ascension in decimal degrees "}, {"name": "DEdeg", "desc": "[-85/78] Declination in decimal degrees "}, {"name": "plx", "desc": "[-329/311] Parallax "}, {"name": "pmRA", "desc": "[-1722/2221] Proper motion along RA "}, {"name": "pmDE", "desc": "[-2000/1165] Proper motion along DE "}, {"name": "e_RAdeg", "desc": "[0.2/2] Uncertainty in RAdeg "}, {"name": "e_DEdeg", "desc": "[0.2/0.8] Uncertainty in DEdeg "}, {"name": "e_plx", "desc": "[0.3/2] Uncertainty in plx "}, {"name": "e_pmRA", "desc": "[0.03/0.9] Uncertainty in pmRA "}, {"name": "e_pmDE", "desc": "[0.03/0.7] Uncertainty in pmDE "}, {"name": "c12", "desc": "[-0.32/0.32] Covariance c12 value "}, {"name": "c13", "desc": "[-0.55/0.53] Covariance c13 value "}, {"name": "c14", "desc": "[-0.25/0.1] Covariance c14 value "}, {"name": "c15", "desc": "[-0.14/0.12] Covariance c15 value "}, {"name": "c23", "desc": "[-0.44/0.19] Covariance c23 value "}, {"name": "c24", "desc": "[-0.1/0.07] Covariance c24 value "}, {"name": "c25", "desc": "[-0.18/0.12] Covariance c25 value "}, {"name": "c34", "desc": "[-0.11/0.14] Covariance c34 value "}, {"name": "c35", "desc": "[-0.09/0.11] Covariance c35 value "}, {"name": "c45", "desc": "[-0.08/0.14] Covariance c45 value "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AN_298_167"}} {"id": "J/AN/298/167", "title_cds": "UBV sequence in NGC 5823", "title_create": "Schnur+, 1977", "year": "1977", "author": "Schnur G.F.O.", "title_pub": "Two UBV sequences, North and South of the galactic cluster NGC 5823.", "first_author": "Schnur G.F.O.", "ref_biblio": [""], "bibcode": ["1977AN....298..167S"], "keyword_cds": "Photometry, UBV ; Clusters, open", "keyword_pub": "", "description": ["Attached is a plain-text list for the two UBV sequences"], "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1002/asna.19772980307"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AZh_93_968"}} {"id": "J/AZh/93/968", "title_cds": "OCARS catalog second version", "title_create": "Malkin, 2016", "year": "2016", "author": "Malkin Z.M.", "title_pub": "The second version of the OCARS Catalog of Optical Characteristics of Astrometric Radio Sources.", "first_author": "Malkin Z.M.", "ref_biblio": [""], "bibcode": ["2016AZh....93..968M", "2016ARep...60..996M"], "see_also": ["J/A+A/583/A75 : Large Quasar Astrometric Catalogue 3 (LQAC-3) (Souchay+, 2015)", "http://www.gao.spb.ru/english/as/ac_vlbi/ : OCARS Home Page"], "keyword_cds": "Radio sources ; Photometry, UBVRI ; Photometry, SDSS", "abstract": ["A new version of the Optical Characteristics of Astrometric Radio", "Sources (OCARS) catalog is presented. The catalog includes a list of", "radio sources observed in astrometric and geodetic VLBI programs since", "1979, their redshifts, photometric data in 13 bands in the visible and", "near infrared, and a table indicating identifications between the OCARS", "objects and objects in other catalogs. The main sources of information", "for the OCARS catalog are the NED and SIMBAD databases, as well as a", "variety of publications. Targeted observing programs designed to", "supplement the optical data for the astrometric radio sources have", "also been organized. The catalog currently contains 9956 sources, of", "which 5449 have redshifts and 7473 have photometric data. The catalog", "is updated, on average, once every several weeks, and is continuously", "augmented with new sources and new optical data."], "description": ["Unlike the first version, supported in 2007-2015, the second version", "of the OCARS catalog includes three files:", "ocars.txt is the main file containing the source coordinates, source", "types, redshifts, and approximate magnitudes, together with commentary;", "this file corresponds to the first version of the OCARS catalog;", "ocars_m.txt contains photometric data in the 13 uUBgV rRiIzJHK bands;", "ocars_n.txt contains a table of corresponding source names in various", "catalogs; currently, only cross-identifications with IVS programs4 and", "the LQAC catalog [9] are included;", "The list of objects included in the OCARS catalog is formed from", "various astrometric and geodeticVLBI programs and catalogs in the", "following order:", "- sources in the ICRF2 [2];", "- other sources observed in the framework of IVS programs;", "- sources from the NASA Goddard VLBI group catalog5 ;", "- sources from the RFC catalog,6 which is the most complete", "astrometric catalog of radio sources, is updated each quarter, and", "contributed more than half the OCARS objects; the latest version of", "OCARS used the RFC-2016a catalog based on observations obtained in", "1980-2015 as part of IVS and other radio astrometric programs", "[19-31];", "- sources from the literature.", "Optical Characteristics of Astrometric Radio Sources (OCARS)", "~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~", "Last revised: 27-NOV-2016", "Latest update:", "- removed 30+ RFC sources not identified in NED and optics", "- removed rather long detailed statistics table, which seems to be not", "interested for most of users; it is always available on request", "- a few additions and amendments", "E-mail alerts about updates are available on request.", "URL of this file is http://www.gao.spb.ru/english/as/ac_vlbi/ocars.txt", "Supplement files:", "Optical and IR magnitudes:", "http://www.gao.spb.ru/english/as/ac_vlbi/ocars_m.txt", "Cross-identification table:", "http://www.gao.spb.ru/english/as/ac_vlbi/ocars_n.txt", "OCARS catalog in CSV format:", "http://www.gao.spb.ru/english/as/ac_vlbi/ocars.csv", "Please send comments and requests to Zinovy Malkin, malkin(at)gao.spb.ru", "----------------------------------------------------------------------------", "The Second Version of the OCARS Catalog of Optical Characteristics of", "Astrometric Radio Sources. Astronomy Reports, 2016, Vol. 60, No. 11,", "pp. 996-1005. DOI: 10.1134/S1063772916110032 If you use OCARS catalog", "in your work, please cite this publication.", "----------------------------------------------------------------------", "Brief OCARS statistics (detailed statistics is available on request)", "~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~", "Total number of sources 11375", "+30...+90 3320 ( 29.2%)", "-30...+30 6233 ( 54.8%)", "-90...-30 1822 ( 16.0%)", "Number of sources with known type 6284 ( 55.2%)", "AGN 4704 ( 74.9%)", "quasars 3027 ( 64.3%)", "BL Lac 992 ( 21.1%)", "Seyfert 384 ( 8.2%)", "blazars 89 ( 1.9%)", "radio galaxies 1580 ( 25.1%)", "Number of sources with redshift info 5845 ( 51.4%)", "+30...+90 1803 ( 30.8%)", "-30...+30 3329 ( 57.0%)", "-90...-30 713 ( 12.2%)", "unreliable 868 ( 14.9%)", "Number of sources with known magnitude 8133 ( 71.5%)", "+30...+90 2380 ( 29.3%)", "-30...+30 4481 ( 55.1%)", "-90...-30 1272 ( 15.6%)", "Number of sources with both z and magnitude info 5803 ( 51.0%)"], "alias": ["OCARS"], "type": ["CCC"], "data": "", "date_creation": "26-Jan-2017", "date_update": "28-Feb-2017", "tables": [{"name": "ocars.dat", "desc": "OCARS catalog (13/12/2016 version) ", "columns": [{"name": "OCARS", "desc": "OCARS name (HHMM+DDd) "}, {"name": "RAh", "desc": "Right accession (J2000.0) "}, {"name": "RAm", "desc": "Right accession (J2000.0) "}, {"name": "RAs", "desc": "Right accession (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "z", "desc": "? Redshift "}, {"name": "f_z", "desc": "[abcde] Redshift flag (1) "}, {"name": "mag", "desc": "? Optical or NIR magnitude (2) "}, {"name": "Band", "desc": "Band for which magnitude was measured magnitude without a band index is an indicative, primarily NED, value usually related to the V or B bands; it is kept in this file only and not repeated in ocars_m.dat"}, {"name": "Type", "desc": "Object primary type (3) "}, {"name": "Ref", "desc": "Position reference (4) "}, {"name": "n_z", "desc": "[*] * shows that redshift is taken not from NED (see corresponding notes)"}, {"name": "Notes", "desc": "Object names and notes (5) "}]}, {"name": "ocars_m.dat", "desc": "Optical and IR magnitudes of astrometric radio sources from the OCARS catalog (13/12/2016 version)", "columns": [{"name": "OCARS", "desc": "OCARS source name (HHMM+DDd) "}, {"name": "umag", "desc": "? SDSS u magnitude "}, {"name": "u_umag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Umag", "desc": "? U magnitude "}, {"name": "Bmag", "desc": "? B magnitude "}, {"name": "u_Bmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "gmag", "desc": "? SDSS g magnitude "}, {"name": "u_gmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Vmag", "desc": "? V magnitude "}, {"name": "u_Vmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "rmag", "desc": "? SDSS r magnitude "}, {"name": "u_rmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Rmag", "desc": "? R magnitude "}, {"name": "u_Rmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "imag", "desc": "? SDSS i magnitude "}, {"name": "u_imag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Imag", "desc": "? I magnitude "}, {"name": "u_Imag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "zmag", "desc": "? SDSS z magnitude "}, {"name": "u_zmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Jmag", "desc": "? J magnitude "}, {"name": "u_Jmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Hmag", "desc": "? H magnitude "}, {"name": "u_Hmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Kmag", "desc": "? K magnitude "}, {"name": "u_Kmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Gmag", "desc": "? Gaia G magnitude "}, {"name": "Notes", "desc": "Notes "}]}, {"name": "ocars_n.dat", "desc": "Cross-identification table between the OCARS and other catalogs (13/12/2016 version)", "columns": [{"name": "OCARS", "desc": "OCARS source name (HHMM+DDd) "}, {"name": "IVS", "desc": "IVS name (source name used in IVS schedules and databases)"}, {"name": "LQAC", "desc": "LQAC name (LQAC_NNN_NNN_NNN) (from Souchay et al., 2015, Cat. J/A+A/583/A75)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AcA_62_o.1"}} {"id": "J/AcA/62/1", "title_cds": "OGLE-III. Magellanic Clouds stellar proper motions", "title_create": "Poleski+, 2012", "year": "2012", "author": "Poleski R., Soszynski I., Udalski A., Szymanski M.K., Kubiak M., Pietrzynski G., Wyrzykowski L., Ulaczyk K.", "title_pub": "The Optical Gravitational Lensing Experiment. The catalog of stellar proper motions toward the Magellanic Clouds.", "first_author": "Poleski R.", "ref_biblio": [""], "bibcode": ["2012AcA....62....1P"], "see_also": ["J/MNRAS/327/601 : OGLE-II High proper motion stars (Eyer+, 2001)", "J/AcA/52/143 : OGLE high proper motion stars towards MC (Soszynski+, 2002)", "J/AcA/59/1 : LMC RR Lyrae stars VI light curves (Soszynski+, 2009)", "J/AcA/59/239 : LMC long-period variables VI light curves (Soszynski+, 2009)", "J/AcA/60/1 : LMC delta Scuti stars VI light curves (Poleski+, 2010)", "J/AcA/60/17 : SMC classical Cepheids VI light curves (Soszynski+, 2010)", "J/AcA/60/165 : SMC RR Lyrae VI light curves (Soszynski+, 2010)", "J/AcA/61/103 : LMC eclipsing binaries VI light curves (Szymanski+, 2011)", "J/AcA/61/199 : OGLE3 Magellanic Clouds high pm stars (Poleski+, 2011)", "J/AcA/61/217 : SMC long-period variables VI light curves (Soszynski+, 2011)"], "keyword_cds": "Surveys ; Magellanic Clouds ; Proper motions", "keyword_pub": "Astrometry - Catalogs - Stars: kinematics and dynamics - binaries: visual - globular clusters: individual: 47 Tuc", "abstract": ["We present a catalog of over 6.2 million stars with measured proper", "motions. All these stars are observed in the direction of the", "Magellanic Clouds within the brightness range 12"], "bibcode": ["2016AcA....66..255S"], "keyword_cds": "Surveys ; Magellanic Clouds ; Associations, stellar", "keyword_pub": "catalogs - surveys - Magellanic Clouds - galaxies: clusters: general", "abstract": ["The Magellanic System (MS), consisting of the LargeMagellanic Cloud", "(LMC), the SmallMagellanic Cloud (SMC) and the Magellanic Bridge", "(MBR), contains diverse sample of star clusters. Their spatial", "distribution, ages and chemical abundances may provide important", "information about the history of formation of the whole System. We use", "deep photometric maps derived from the images collected during the", "fourth phase of the Optical Gravitational Lensing Experiment (OGLE-IV)", "to construct the most complete catalog of star clusters in the Large", "Magellanic Cloud using the homogeneous photometric data. In this paper", "we present the collection of star clusters found in the area of about", "225 square degrees in the outer regions of the LMC. Our sample", "contains 679 visually identified star cluster candidates, 226 of which", "were not listed in any of the previously published catalogs. The new", "clusters are mainly young small open clusters or clusters similar to", "associations."], "description": ["The photometric data of the LMC fields analyzed in this paper come", "from the images gathered during the first five years (2010\u20132015) of", "the fourth phase of the OGLE project (OGLE-IV, Udalski, Szyma\u00b4nski", "and Szyma\u00b4nski 2015). The project has been conducted on the 1.3-meter", "Warsaw Telescope at the Las Campanas Observatory, equipped with the", "32-chip mosaic CCD camera, covering 1.4 square degree field with", "0.26\" per pixel scale (see the aforementioned paper for the", "details of the OGLE-IV hardware setup, observational strategy and", "photometric reductions pipeline)."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "20-Apr-2018"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_AcA_66_269"}} {"id": "J/AcA/66/269", "title_cds": "Short Title", "title_create": "Skowron+, 2016", "year": "2016", "author": "Skowron D.M., Soszynski I., Udalski A., Szymanski M.K., Pietrukowicz P., Skowron J., Poleski R., Wyrzykowski L., Ulaczyk K., Kozlowski S., Mroz P., Pawlak M.", "title_pub": "OGLE-ing the Magellanic System: Photometric metallicity from fundamental mode RR Lyrae stars.", "first_author": "Skowron D.M.", "ref_biblio": [""], "bibcode": ["2016AcA....66..269S"], "keyword_cds": "Surveys ; Magellanic Clouds", "keyword_pub": "stars: abundances \u2013 stars: statistics \u2013 stars: variables: RR Lyr \u2013 galaxies: abundances \u2013 Magellanic Clouds", "abstract": ["In an era of extensive photometric observations, the catalogs of RR", "Lyr type variable stars number tens of thousands of objects. The", "relation between the iron abundance [Fe/H] and the Fourier parameters", "of the stars light curve allows us to investigate mean metallicities", "and metallicity gradients in various stellar environments,", "independently of time-consuming spectroscopic observations. In this", "paper we use almost 6500 V- and I-band light curves of fundamental", "mode RR Lyr stars from the OGLE-IV survey to provide a relation", "between the V- and I-band phase parameter {phi}_31_ used to estimate", "[Fe/H]. The relation depends on metallicity, which limits its", "applicability. We apply this relation to metallicity formulae", "developed for the Johnson V- and the Kepler Kp-band to obtain the", "relation between [Fe/H] and {phi}_31_ for the I-band photometry. Last,", "we apply the new relation of Nemec to the OGLE-IV fundamental mode RR", "Lyr stars data and construct a metallicity map of the Magellanic", "Clouds. Median [Fe/H] is -1.39+/-0.44dex for the LMC and", "-1.77+/-0.48dex for the SMC, on the Jurcsik metallicity scale. We also", "find a metallicity gradient within the LMC with a slope of", "-0.029+/-0.002dex/kpc in the inner 5kpc and -0.030+/-0.003dex/kpc", "beyond 8kpc, and no gradient in-between (-0.019+/-0.002dex/kpc", "integrally). We do not observe a metallicity gradient in the SMC,", "although we show that the metal-rich RRab stars are more concentrated", "toward the SMC center than the metal-poor."], "description": ["For the purpose of this study we used the OGLE-IV RRab sample that", "consists of 27 258 stars in the Galactic bulge (Soszynski et al. 2014.", "Cat. J/AcA/64/177) and 27 081 in the LMC (Soszynski et al.,", "2016AcA....66..131S). We do not include the SMC RRL sample because of", "smaller number of observations in the V-band."], "object": [], "curator": "Patricia Vannier [CDS]", "orcid_pub": ["0000-0002-2335-1730", "0000-0002-2335-1730"], "data": "", "date_update": "19-Feb-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_116_592"}} {"id": "J/ApJ/116/592", "title_cds": "Cygnus photometry", "title_create": "Macrae+, 1952", "year": "1952", "author": "Macrae D.A.", "title_pub": "Stellar spectra and colors in Cygnus at galactic latitude +14 deg.", "first_author": "Macrae D.A.", "ref_biblio": [""], "bibcode": ["1952ApJ...116..592M"], "keyword_cds": "MK spectral classification; Magnitudes, photographic", "keyword_pub": "", "abstract": ["Photographic magnitudes, colors, and spectral types of 938 stars to", "limiting magnitude 12.7 are given in table3. The photometric data,", "obtained from plates taken with the Burrell telescope, are based on a", "sequence of stars in the field for which magnitudes and colors were", "determined by photoelectric means. Luminosity classes have been", "assigned to stars brighter than 11.2. A few stars of special interest", "are discussed, including one which is similar to BD+28 4211 (Op), a", "new carbon star, and three new variables, one of which is an S-type", "star."], "object": [], "alias": ["ILF-1"], "doi_pub": ["10.1086/145652"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table3.dat", "desc": " ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_119_188"}} {"id": "J/ApJ/119/188", "title_cds": "Positions and Identifications of stars in NGC 2287", "title_create": "Cox+, 1954", "year": "1954", "author": "Cox A.N.", "title_pub": "A study of the galactic cluster NGC 2287.", "first_author": "Cox A.N.", "ref_biblio": [""], "bibcode": ["1954ApJ...119..188C"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["Magnitudes and colours of 106 stars in the region od NGC 2287 (M41)", "were observed with a photoelectric photometer mounted on the 24-inch", "(133cm) Victoria telescope at the Royal Observatory, Cape of Good", "Hope. Spectral types and radial velocities were found for 22 cluster", "stars from low-dispersion spectra obtained at the McDonald", "Observatory."], "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/145809"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_120_129"}} {"id": "J/ApJ/120/129", "title_cds": "Carbon stars near the Galactic Plane", "title_create": "Nassau+, 1954", "year": "1954", "author": "Nassau J.J., Blanco V.M.", "title_pub": "Carbon stars at the galactic equator in a zone 4 degrees wide", "first_author": "Nassau J.J.", "ref_biblio": [""], "bibcode": ["1954ApJ...120..129N"], "keyword_cds": "Stars, carbon", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["CASE"], "doi_pub": ["10.1086/145888"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_125_195"}} {"id": "J/ApJ/125/195", "title_cds": "Carbon stars in Milky Way zones", "title_create": "Nassau+, 1957", "year": "1957", "author": "Nassau J.J., Blanco V.M.", "title_pub": "Carbon stars in two northern Milky Way zones.", "first_author": "Nassau J.J.", "ref_biblio": [""], "bibcode": ["1957ApJ...125..195N"], "keyword_cds": "Stars, carbon", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/146293"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_128_267"}} {"id": "J/ApJ/128/267", "title_cds": "Feige's list of underluminous hot stars", "title_create": "Feige+, 1958", "year": "1958", "author": "Feige J.", "title_pub": "A search for underluminous hot stars.", "first_author": "Feige J.", "ref_biblio": [""], "bibcode": ["1958ApJ...128..267F"], "keyword_cds": "Stars, blue", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/146541"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_176_623"}} {"id": "J/ApJ/176/623", "title_cds": "Suspected supergiant M stars", "title_create": "Albers+, 1972", "year": "1972", "author": "Albers H.", "title_pub": "Infrared surveys of the Southern Milky Way. II. Suspected supergiant M stars.", "first_author": "Albers H.", "ref_biblio": [""], "bibcode": ["1972ApJ...176..623A"], "keyword_cds": "Stars, supergiant ; Stars, late-type", "abstract": ["An infrared objective-prism survey has been carried out along the", "Southern Milky Way, suspected M-type supergiants habe been selected", "from the presence of a CN absorption feature at 790nm. A calalog of", "170 M stars showing this feature is given."], "description": ["Accurate positions from Brian Skuff (Lowell Obs.)"], "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/151664"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_241_486"}} {"id": "J/ApJ/241/486", "title_cds": "Absolute magnitudes in 116 nearby Abell clusters", "title_create": "Hoessel+, 1980", "year": "1980", "author": "Hoessel J.G., Gunn J.E., Thuan T.X.", "title_pub": "The photometry properties of brightest cluster galaxies. I. Absolute magnitudes in 116 nearby Abell clusters.", "first_author": "Hoessel J.G.", "ref_biblio": [""], "bibcode": ["1980ApJ...241..486H"], "see_also": ["VII/87 : Data on 1889 Abell's clusters of galaxies (Leir+ 1977)", "J/ApJ/566/103 : VIK' photometry and redshifts of galaxy clusters (Nelson+ 2002)"], "keyword_cds": "Clusters, galaxy ; Magnitudes, absolute ; Redshifts", "keyword_pub": "cosmology - galaxies: clusters of - galaxies: photometry - galaxies: structure", "abstract": ["Two-color aperture photometry of the brightest galaxies in a complete", "sample of nearby Abeil clusters is presented. The results are used to", "anchor the bright end of the Hubble diagram; essentially the entire", "formal error for this method is then due to the sample of distant", "clusters used. New determinations of the systematic trend of galaxy", "absolute magnitude with the cluster properties of richness and", "Bautz-Morgan type are derived. When these new results are combined", "with the Gunn and Oke data on high-redshift clusters, a formal value", "(without accounting for any evolution) of q_0_=-0.55+/-0.45 (1{sigma})", "is found."], "doi_pub": ["10.1086/158363"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Observed Properties of the Low-Redshift Sample ", "columns": [{"name": "Abell", "desc": "Abell designation (ANNNN) "}, {"name": "RA1h", "desc": "Right ascension (B1950.0) "}, {"name": "RA1m", "desc": "Right ascension (B1950.0) "}, {"name": "RA1s", "desc": "Right ascension (B1950.0) "}, {"name": "DE1-", "desc": "Declination sign (B1950.0) "}, {"name": "DE1d", "desc": "Declination (B1950.0) "}, {"name": "DE1m", "desc": "Declination (B1950.0) "}, {"name": "DE1s", "desc": "Declination (B1950.0) "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "cz", "desc": "? Heliocentric radial velocity "}, {"name": "z", "desc": "? Redshift "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "R", "desc": "Abell richness class "}, {"name": "D", "desc": "Abell distance class "}, {"name": "BM", "desc": "BM type (from Leir & van den Bergh, 1977, Cat. )"}, {"name": "logz", "desc": "? log of redshift "}, {"name": "2gam", "desc": "? Observation angular diameter "}, {"name": "radius", "desc": "? Physical radius "}, {"name": "gmag", "desc": "? g magnitude "}, {"name": "g-r", "desc": "? g-r colour index "}, {"name": "Apcor", "desc": "? Aperture correction "}, {"name": "Rcorr", "desc": "? Corrected Radius "}, {"name": "VImag", "desc": "? VI (visual intrinsic) magnitude "}, {"name": "VIMAG", "desc": "? Absolute VI magnitude "}, {"name": "Obs", "desc": "Type and number of observations (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_253_485"}} {"id": "J/ApJ/253/485", "title_cds": "High-latitude HEAO 1 A-2 sources X-ray sample", "title_create": "Piccinotti+, 1982", "year": "1982", "author": "Piccinotti G., Mushotzky R.F., Boldt E.A., Holt S.S., Marshall F.E., Serlemitsos P.J., Shafer R.A.", "title_pub": "A complete X-ray sample of the high-latitude (|b|>20{deg}) sky from HEAO 1 A-2: log N-log S and luminosity functions.", "first_author": "Piccinotti G.", "ref_biblio": [""], "bibcode": ["1982ApJ...253..485P"], "keyword_cds": "Clusters, galaxy ; X-ray sources ; Redshifts", "keyword_pub": "Galaxies, cluster of - luminosity function - X-ray sources", "abstract": ["The HEAO 1 experiment A-2 has performed a complete X-ray survey of the", "8.2sr of the sky at |b|>20{deg} down to a limiting sensitivity of", "~3.1x10^-11^ergs/cm^2^/s in the 2-10keV band. Of the 85 detected", "sources (excluding the LMC and SMC sources), 17 have been identified", "with galactic objects, 61 have been identified with extragalactic", "objects, and 7 remain unidentified. The log N -log S relation for the", "nongalactic objects is well fitted by the Euclidean relationship. We", "have used the X-ray spectra of these objects to construct the log", "N-log S relation in physical units. The complete sample of identified", "sources has been used to construct X-ray luminosity functions, using", "the absolute maximum likelihood method, for clusters of galaxies and", "active galactic nuclei."], "doi_pub": ["10.1086/159651"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Data on X-ray sources ", "columns": [{"name": "A2Name", "desc": "HEAO A-2 name (HHHMM+DDd) "}, {"name": "A1Name", "desc": "HEAO A-1 Name (1HHHMM+DDd) "}, {"name": "Flux1", "desc": "1st Scan flux, in R15ct/s (1) "}, {"name": "e_Flux1", "desc": "rms uncertainty on Flux1 "}, {"name": "l_Flux2", "desc": "Limit flag on Flux2 "}, {"name": "Flux2", "desc": "2nd Scan flus, in R15ct/s (1) "}, {"name": "e_Flux2", "desc": "? rms uncertainty on Flux2 "}, {"name": "OName", "desc": "Optical identification "}, {"name": "RAh", "desc": "Right ascension (1950.0) "}, {"name": "RAm", "desc": "Right ascension (1950.0) "}, {"name": "RAs", "desc": "Right ascension (1950.0) "}, {"name": "DE-", "desc": "Declination sign (1950.0) "}, {"name": "DEd", "desc": "Declination (1950.0) "}, {"name": "DEm", "desc": "Declination (1950.0) "}, {"name": "DEs", "desc": "Declination (1950.0) "}, {"name": "MType", "desc": "Morphological type (2) "}, {"name": "z", "desc": "? Redshift "}, {"name": "r_z", "desc": "Reference for redshift (3) "}, {"name": "CF", "desc": "Conversion factor, in 10^-11^erg/cm2/(R15ct/s) "}, {"name": "Lum1", "desc": "? 1st Scan luminosity "}, {"name": "Lum2", "desc": "? 2nd Scan luminosity "}, {"name": "Notes", "desc": "? Individual notes (4) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_264_337"}} {"id": "J/ApJ/264/337", "title_cds": "CCD photometry of Abell clusters", "title_create": "Schneider+, 1983", "year": "1983", "author": "Schneider D.P., Gunn J.E., Hoessel J.G.", "title_pub": "CCD photometry of Abell clusters. I. Magnitudes and redshifts for 84 brightest cluster galaxies.", "first_author": "Schneider D.P.", "ref_biblio": [""], "bibcode": ["1983ApJ...264..337S"], "see_also": ["VII/87 : Data on 1889 Abell's clusters of galaxies (Leir+ 1977)", "J/AJ/101/1561 : Isophotometry of ellipticals in Abell clusters (Porter+ 1991)"], "keyword_cds": "Clusters, galaxy ; Photometry, CCD ; Redshifts", "keyword_pub": "cosmology - galaxies: clusters of - galaxies: photometry", "abstract": ["A sample of 84 Abell clusters has been selected to determine how the", "luminosity of the brightest cluster galaxy varies with cluster", "parameters. The clusters are of moderate redshift (0.04"], "bibcode": ["1983ApJ...274..534M"], "keyword_cds": "Galaxy catalogs ; Morphology", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: structure", "abstract": ["We present a catalog of 137 elliptical galaxies south of -17{deg}", "declination which exhibit shell or ripple features at large distances", "from the galaxy or in the outer envelope. Some of these galaxies show", "similar features in the inner envelope when suitable high resolution", "plate material is examined. Very few of the galaxies are associated", "with radio sources. We discuss the environment of shell galaxies, and", "the proportion of ellipticals which have these features. It appears", "that about half of the galaxies with shells are isolated and most of", "the rest are members of small groups. We discuss several individual", "examples which appear to be typical of this class of galaxy and others", "which probably illustrate an evolutionary sequence."], "doi_pub": ["10.1086/161467"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "The Galaxy Catalog ", "columns": [{"name": "[MC83b]", "desc": "Reference name of the object derived from the 1950 coordinates (1)"}, {"name": "n_[MC83b]", "desc": "[*] *: Note in notes.dat file "}, {"name": "Field", "desc": "The ESO/SRC field number (see Holmberg et al., 1974A&AS...18..463H, 1974A&AS...18..491H for the nominal field centers)."}, {"name": "WDist", "desc": "The distance in mm from the eastern edge of the image on the film copies (2)"}, {"name": "NDist", "desc": "The distance in mm from the southern edge of the image on the film copies (2)"}, {"name": "RAh", "desc": "Right ascension (1950) (3) "}, {"name": "RAm", "desc": "Right ascension (1950) (3) "}, {"name": "RAs", "desc": "Right ascension (1950) (3) "}, {"name": "DE-", "desc": "Declination sign (1950) (3) "}, {"name": "DEd", "desc": "Declination (1950) (3) "}, {"name": "DEm", "desc": "Declination (1950) (3) "}, {"name": "DEs", "desc": "Declination (1950) (3) "}, {"name": "Env", "desc": "[IGC] The environment of the sample galaxy (4) "}, {"name": "Com", "desc": "Comments. "}]}, {"name": "table2.dat", "desc": "Supplementary list of galaxies with shells outside main survey", "columns": [{"name": "[MC83b]", "desc": "Reference name of the object derived from the 1950 coordinates (1)"}, {"name": "n_[MC83b]", "desc": "[*] *: Note in notes.dat file "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "RAs", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "DEs", "desc": "? Declination (1950) "}, {"name": "Com", "desc": "Comments. "}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "[MC83b]", "desc": "Reference name of the object "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_301_927"}} {"id": "J/ApJ/301/927", "title_cds": "Stephenson's late M-star catalog", "title_create": "Stephenson+, 1986", "year": "1986", "author": "Stephenson C.B.", "title_pub": "Late M stars found in a hemispheric survey.", "first_author": "Stephenson C.B.", "ref_biblio": [""], "bibcode": ["1986ApJ...301..927S"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Brian Skiff [Lowell Obs.], Francois Ochsenbein [CDS]", "alias": ["StM"], "type": ["OC"], "doi_pub": ["10.1086/163957"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_315_104"}} {"id": "J/ApJ/315/104", "title_cds": "Molecular clouds near Gould belt", "title_create": "Taylor+, 1987", "year": "1987", "author": "Taylor D.K., Dickman R.L., Scoville N.Z.", "title_pub": "Molecular clouds and the Gould belt.", "first_author": "Taylor D.K.", "ref_biblio": [""], "bibcode": ["1987ApJ...315..104T"], "see_also": ["VII/7 : Lynds' Catalogue of Dark Nebulae (LDN) (Lynds 1962)", "VII/191 : Catalogue of Southern Dark Clouds (Hartley+ 1986)", "J/ApJS/95/457 : IRAS images of nearby dark clouds (Wood+ 1994)", "J/A+AS/141/175 : Dark clouds imaging polarimetry (Sen+, 2000)"], "keyword_cds": "Molecular clouds ; Radial velocities", "keyword_pub": "galaxies: Milky Way - galaxies: structure - interstellar: molecules", "abstract": ["We investigate the relationship of the local system of molecular", "clouds to the Gould belt. A careful examination of the National", "Geographic-Palomar Observatory Sky Survey Atlas (POSS) yielded a", "catalog of dark clouds with accurately measured positions as far south", "as {delta}=-27{deg}. From a nonlinear least squares fit to these data,", "along with positions from Feitzinger and Stuwe's catalog of southern", "clouds, we find a subset of dark clouds to be distributed irregularly", "along a curve b=-3.5{deg} + 12.5{deg}sin(l-27.5{deg}) This is similar", "to the distribution of the system of O and B stars used to define the", "system.", "Radial velocities in the J=1->0 transition of carbon monoxide were", "measured for all dark clouds in our catalog using the 14 m antenna of", "the Five College Radio Astronomy Observatory. The velocity", "distribution of those clouds judged to be members of the belt", "population suggests an expansion similar to that seen in the neutral", "atomic hydrogen and OB stars. Similar expansion energies are found for", "both gas constituents, atomic and molecular, as well as for the Gould", "belt stars. The velocity-longitude data for our molecular clouds were", "fitted to a model ring expanding under the influence of Galactic", "differential rotation and interstellar drag, with poor results. We", "discuss the reasons for this.", "Because the similar expansion energies of the stellar, H I, and", "molecular gas constituents of the Gould belt are all approximately", "equal, we suggest that the belt originated in an acceleration of gas", "rather than in a violent impulse such as a blast wave from one or more", "supernovae."], "doi_pub": ["10.1086/165117"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table3.dat", "desc": "Catalog of dark clouds ", "columns": [{"name": "TDS", "desc": "Sequential number "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "RAs", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "DEs", "desc": "Declination (1950) "}, {"name": "RV", "desc": "Spectral line centroid radial velocity "}, {"name": "n_RV", "desc": "[*] *: the observed velocity implies a nonlocal cloud"}, {"name": "Belt", "desc": "Belt (Gal or Gould) "}, {"name": "LDN", "desc": "? Lynds (Cat. ) number "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_381_33"}} {"id": "J/ApJ/381/33", "title_cds": "VRI photometry of Cl 1358+6245", "title_create": "Fabricant+, 1991", "year": "1991", "author": "Fabricant D.G., McClintock J.E., Bautz M.", "title_pub": "Galaxy evolution in distant, X-ray selected clusters of galaxies. I. Cl 1358+6245.", "first_author": "Fabricant D.G.", "ref_biblio": [""], "bibcode": ["1991ApJ...381...33F"], "see_also": ["J/ApJ/498/195 : Spectroscopic survey of CL 1358+62 (Fisher+ 1998)", "J/ApJ/500/714 : Color-magnitude relation in CL 1358+62 (Van Dokkum+ 1998)", "J/ApJ/539/577 : Galaxy morphologies Cl 1358+62 (Fabricant+, 2000)"], "keyword_cds": "Clusters, galaxy ; X-ray sources ; Photometry, VRI", "keyword_pub": "galaxies: clustering - galaxies: photometry - galaxies: structure - galaxies: X-rays", "abstract": ["A photometric and spectroscopic survey of a cluster of galaxies at", "z=0.327 is presented. We have obtained V, R, and I photometry of 288", "stars and galaxies in a region 5.7'x6.5' which is approximately", "centered on the dominant galaxy at the cluster center. The photometry", "is complete to rest band M_V_=-19.5 (19kpc diameter aperture). We have", "obtained the spectra of 70 galaxies which lie within ~2' (~R_30_) of", "the cluster center, to a magnitude limit of M_V_~- 20.5; ~90% of these", "galaxies are cluster members. The large velocity dispersion of the", "cluster, 1125^+126^_-94_ km/s, is consistent with its high X-ray", "luminosity, ~7x10^44^erg/s (0.2-4.5 keV)."], "doi_pub": ["10.1086/170626"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table5.dat", "desc": "Photometric results ", "columns": [{"name": "[FMB91]", "desc": "Sequential number "}, {"name": "RAh", "desc": "Right ascension (B1950) "}, {"name": "RAm", "desc": "Right ascension (B1950) "}, {"name": "RAs", "desc": "Right ascension (B1950) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) "}, {"name": "DEm", "desc": "Declination (B1950) "}, {"name": "DEs", "desc": "Declination (B1950) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "V-R", "desc": "V-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "Type", "desc": "[sg] Classification "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_411_501"}} {"id": "J/ApJ/411/501", "title_cds": "I-band selected galaxy sample", "title_create": "Lilly, 1993", "year": "1993", "author": "Lilly S.J.", "title_pub": "A deep I-band selected galaxy sample : implications for galaxy evolution.", "first_author": "Lilly S.J.", "ref_biblio": [""], "bibcode": ["1993ApJ...411..501L"], "keyword_cds": "Infrared sources ; Galaxies, IR ; Redshifts ; Equivalent widths", "keyword_pub": "galaxies: distances and redshifts - galaxies: evolution - galaxies: formation - infrared: galaxies", "abstract": ["New spectroscopic observations of statistically complete sample of 50", "very faint I-band selected galaxies with I_AB_<22.5 show that,", "although they extend out to z~1, the redshifts are generally low,", "_obs_~0.5+/-0.1."], "doi_pub": ["10.1086/172851"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Photometric and spectroscopic data ", "columns": [{"name": "[L93]", "desc": "Identification number "}, {"name": "n_[L93]", "desc": "[fgh] Note (1) "}, {"name": "Xpos", "desc": "X position (2) "}, {"name": "Ypos", "desc": "Y position (2) "}, {"name": "Imag3", "desc": "I_AB_ magnitude in 3\" diameter aperture "}, {"name": "ImagISO", "desc": "I_AB_ magnitude in circular isophotal aperture to {mu}_AB_(I)=28"}, {"name": "z", "desc": "? Redshift "}, {"name": "n_z", "desc": "[s] s: star "}, {"name": "Q", "desc": "[A-D] Quality class (3) "}, {"name": "(V-I)", "desc": "(V-I)_AB_ colour index (4) "}, {"name": "l_EW0", "desc": "Limit flag on EW0 "}, {"name": "EW0", "desc": "? Rest-of frame equivalent width of [O II] 3727{AA}"}, {"name": "Obs", "desc": "Year of the observing season when spectroscopic observations made"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_412_479"}} {"id": "J/ApJ/412/479", "title_cds": "Intracluster gas temperatures catalog", "title_create": "David+, 1993", "year": "1993", "author": "David L.P., Slyz A., Jones C., Forman W., Vrtilek S.D.", "title_pub": "A catalog of intracluster gas temperatures.", "first_author": "David L.P.", "ref_biblio": [""], "bibcode": ["1993ApJ...412..479D"], "see_also": ["IX/13 : The 2E Catalogue (Harris+ 1994)"], "keyword_cds": "Clusters, galaxy ; X-ray sources ; Redshifts", "keyword_pub": "catalogs - galaxies: clustering - intergalactic medium - X-rays: galaxies", "abstract": ["We have searched the Einstein Monitor Proportional Counter (MPC) data", "base for observations of clusters of galaxies. By coadding the MPC", "spectra obtained during all pointed observations of clusters with IPC", "count rates greater than 0.1 counts/s, we have obtained sufficient", "photon statistics to estimate the X-ray temperature of 84 clusters.", "Combining the MPC results with EXOSAT and Ginga results reported in", "the literature yields a combined sample of 104 clusters with known", "X-ray temperatures. One of the best studied X-ray correlations between", "clusters is that between their X-ray luminosity and gas temperature.", "We show that the best-fit power-law relation for our combined cluster", "sample can be explained by the observed increase in the gas-to-stellar", "mass ratio between low- and high-temperature clusters. The statistical", "significance of any evolution in our combined X-ray sample has been", "examined and compared with the statistical properties of clusters", "culled from optical catalogs. We find that there is strong evidence", "for a decrease in the X-ray luminosity of optically rich clusters", "beyond z approximately about 0.06. This result is used to estimate the", "normalization of the primordial power spectrum of density", "fluctuations."], "doi_pub": ["10.1086/172936"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Combined Cluster Sample ", "columns": [{"name": "Cluster", "desc": "Cluster designation "}, {"name": "Notes", "desc": "[abc] Notes (1) "}, {"name": "n_Cluster", "desc": "[*] Note on cluster (2) "}, {"name": "z", "desc": "Redshift (3) "}, {"name": "NH", "desc": "Hydrogen column density "}, {"name": "T", "desc": "? Temperature "}, {"name": "u_T", "desc": "Uncertainty flag on T "}, {"name": "l_E_T", "desc": "Limit flag on E_T (rms error in E_T) "}, {"name": "E_T", "desc": "? 1{sigma} error on T (upper limit) "}, {"name": "e_T", "desc": "? 1{sigma} error on T (lower limit) "}, {"name": "l_E90T", "desc": "Limit flag on E90T "}, {"name": "E90T", "desc": "? 90% confidence limit on T (upper limit) "}, {"name": "e90T", "desc": "? 90% confidence limit on T (lower limit) "}, {"name": "F2-10kev", "desc": "Flux at 2-10keV "}, {"name": "L2-10kev", "desc": "Luminosity at 2-10keV "}, {"name": "Lbol", "desc": "Bolometric luminosity "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_459_L27"}} {"id": "J/ApJ/459/L27", "title_cds": "R136 population", "title_create": "Hunter+ 1996", "year": "1996", "author": "Hunter D.A., O'Neil E.J.JR., Lynds R., Shaya E.J., Groth E.J., Holtzman J.A", "title_pub": "The intermediate-mass population in the core of the R136 star cluster.", "first_author": "Hunter D.A.", "ref_biblio": [""], "bibcode": ["1996ApJ...459..L27H\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "stars: formation - stars: luminosity function, mass function - galaxies: star clusters", "abstract": ["R136, the compact, luminous star cluster at the center of the", "30 Doradus nebula represents an extreme mode of star formation. Yet it", "is unique among these kinds of objects in that it can be resolved into", "individual stars and the star formation process probed through the", "stellar products. In a previous paper we reported on a study of the", "intermcdiate stellar mass population in R136 and derived a stellar", "initial mass function (IMF) for intermediate-mass stars in the region", "0.5 to 4.7pc from the center of the cluster. We have now obtained", "Hubble Space Telescope images designed to probe the stellar population", "in the core (<0.5pc) of the cluster. We have measured the IMF for", "stars 5-15M_{sun}_ at radii 0.11-0.34pc, and for 4-15M_{sun}_ at", "0.34-0.46pc. Beyond 0.46pc we measure stars in mass bins from", "2.8-15M_{sun}_, as before. The slope of the stellar IMF heyond 0.5pc", "is found to be -1.0+/-0.1, which is within a few sigma of the value", "measured previously for the same annulus. The slopes of the IMFs", "become shallower at smaller radii but the uncertainties do not rule", "out an IMF that is constant with cluster radius. The lower stellar", "mass limit is 5M_{sun}_. in the cluster core. Thus R136 is found to", "be similar to less concentrated OB associations even into 0.1pc from", "the center of the cluster."], "object": ["05 38 42.8 -69 06 03 RMC 136 = HD 38268"], "curator": "James Marcout, Patricia Bauer [CDS]", "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_472_509"}} {"id": "J/ApJ/472/509", "title_cds": "Lyman-alpha Forest in Q0000-26", "title_create": "Lu+ 1996", "year": "1996", "author": "Lu L., Sargent W.L.W., Womble D.S., Takada-Hidai M.", "title_pub": "The Lyman-alpha Forest at z about 4: Keck HIRES Observations of Q0000-26", "first_author": "Lu L.", "ref_biblio": [""], "bibcode": ["1996ApJ...472..509L"], "keyword_cds": "QSOs ; Redshifts ; Spectroscopy", "abstract": ["This file contains the list of absorption lines found in the spectrum", "of the z_em_=4.1 quasar Q0000-26 obtained with the 10m Keck I", "telescope. The spectrum has a resolution of 6.6km/s, with typical", "signal-to-noise ratio 25-35 per resolution element. The absorption", "lines found in the Lyman-alpha forest region has been deblended using", "the Voigt profile fitting routine VPFIT from Robert Carswell and", "colleagues; redshift, column density, and Doppler width are provided", "for each line in the list."], "object": ["00 03 22.91 -26 03 16.8 QSO 0000-26 = QSO J0003-2603"], "doi_pub": ["10.1086/526756"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "lu1.dat", "desc": "Measured wavelengths ", "columns": [{"name": "No", "desc": "Running number "}, {"name": "lambda", "desc": "Wavelength "}, {"name": "ID", "desc": "Element identification "}, {"name": "z", "desc": "Redshift "}, {"name": "e_z", "desc": "Mean error of z "}, {"name": "b", "desc": "Effective radial velocity dispersion "}, {"name": "e_b", "desc": "Mean error of b "}, {"name": "logN", "desc": "logN (column density) "}, {"name": "e_logN", "desc": "Mean error of logN "}, {"name": "Note", "desc": "? Note detailed in file \"notes.dat\" "}]}, {"name": "lu2.dat", "desc": "Redshifts ", "columns": [{"name": "No", "desc": "? Running number "}, {"name": "lambda", "desc": "? Wavelength "}, {"name": "lam_obs", "desc": "? Observed wavelength "}, {"name": "e_lambda", "desc": "? Mean error of observed wavelength "}, {"name": "ID", "desc": "Element identification "}, {"name": "z", "desc": "? Redshift "}, {"name": "Note", "desc": "? Note detailed in file \"notes.dat\" "}]}, {"name": "notes.dat", "desc": "Notes ", "columns": [{"name": "NoteNo", "desc": "[1,10]+= Note number "}, {"name": "---", "desc": "[=] "}, {"name": "Text", "desc": "Text of note "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_478_124"}} {"id": "J/ApJ/478/124", "title_cds": "NGC 1818 stellar population", "title_create": "Hunter+, 1998", "year": "1998", "author": "Hunter D.A., Light R.M., Holtzman J.A., Lynds R., O'Neil E.J., Grillmair C.J.", "title_pub": "The intermediate-mass stellar population of the Large Magellanic Cloud cluster NGC 1818 and the universality of the stellar initial mass function.", "first_author": "Hunter D.A.", "ref_biblio": [""], "bibcode": ["1998ApJ...478..124H\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "James Marcout, Patricia Bauer [CDS]", "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_485_447"}} {"id": "J/ApJ/485/447", "title_cds": "Evidence of substructure in A3558", "title_create": "Dantas+ 1997", "year": "1997", "author": "Dantas C.C., de Carvalho R.R., Capelato H.V., Mazure A.", "title_pub": "Evidence of substructure in the cluster of galaxies A3558", "first_author": "Dantas C.C.", "ref_biblio": [""], "bibcode": ["1997ApJ...485..447D"], "keyword_cds": "Clusters, galaxy ; Photometry ; Radial velocities", "keyword_pub": "catalogs - galaxies: clusters: individual (A3558) - galaxies: distances and redshifts - galaxies: elliptical and lenticular, cD - galaxies: photometry", "abstract": ["We investigate the dynamical properties of the cluster of galaxies", "A3558 (Shapley 8). Studying a region of 1deg^2^(~3Mpc^2^) centered on", "the cluster cD galaxy, we have obtained a statistically complete", "photometric catalog with positions and magnitudes of 1421 galaxies", "(down to a limiting magnitude of B~21). This catalog has been matched", "to the recent velocity data obtained by Mazure et al. (1997, in prep)", "and from the literature, yielding a radial velocity catalog containing", "322 galaxies. We analyze the resulting catalog in search of", "substructure, using different statistical techniques. This analysis", "shows that the position/velocity space distribution of galaxies shows", "significant substructure. A central bimodal core, detected previously", "in a preliminary study by Dantas, de Carvalho, & Capelato (1994, in", "Proc. 29th Rencontre de Moriond, Clusters of Galaxies, p. 385) and by", "an analysis of the X-ray emission map by Slezak, Durret, & Gerbal", "(1994AJ....108.1996S), is confirmed using the adaptive kernel", "technique and wavelet analysis. We show that this central bimodal", "substructure is nevertheless composed of a projected feature,", "kinematically unrelated to the cluster, plus a group of galaxies", "probably in its initial merging phase into a relaxed core. The cD", "galaxy's velocity offset with respect to the average cluster redshift,", "reported earlier by several authors, is completely eliminated as a", "result of our dynamical analysis. The untangling of the relaxed core", "component also allows a better, more reliable determination of the", "central velocity dispersion, which in turn eliminates the \"Beta", "problem\" for A3558. The cluster also shows a \"preferential\"", "distribution of subclumps coinciding with the direction of the", "major-axis position angle of the cD galaxy and of the central X-ray", "emission ellipsoidal distribution, in agreement with the anisotropic", "merger scenario described by West (1994MNRAS.268...79W) ."], "doi_pub": ["10.1086/304458"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table.dat", "desc": "A3558 Photometric Galaxy Catalogue ", "columns": [{"name": "Num", "desc": "Galaxy number "}, {"name": "RAh", "desc": "Right Ascension (J2000) "}, {"name": "RAm", "desc": "Right Ascension (J2000) "}, {"name": "RAs", "desc": "Right Ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "SuArea", "desc": "? Surface area "}, {"name": "e", "desc": "Ellipticity "}, {"name": "SuBr", "desc": "Surface brightness "}, {"name": "CI", "desc": "Color Index "}, {"name": "Vel", "desc": "? Velocity "}, {"name": "e_Vel", "desc": "? Velocity error "}, {"name": "Note", "desc": "Notes (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_498_77"}} {"id": "J/ApJ/498/77", "title_cds": "Ly{alpha} absorption systems. III.", "title_create": "Chen+, 1998", "year": "1998", "author": "Chen H.-W., Lanzetta K.M., Webb J.K., Barcons X.", "title_pub": "The gaseous extent of galaxies and the origin of Ly{alpha} absorption systems. III. Hubble space telescope imaging of Ly{alpha}-absorbing galaxies at z < 1.", "first_author": "Chen H.-W.", "ref_biblio": [""], "bibcode": ["1998ApJ...498...77C"], "see_also": ["J/ApJ/559/654 : Ly{alpha} absorption systems V. (Chen+, 2001)"], "keyword_cds": "QSOs ; Redshifts ; Equivalent widths", "keyword_pub": "galaxies: clusters: general - galaxies: distances and redshifts - quasars: absorption lines", "abstract": ["We present initial results of a program to obtain and analyze Hubble", "Space Telescope (HST) Wide Field Planetary Camera 2 images of galaxies", "identified in an imaging and spectroscopic survey of faint galaxies in", "fields of HST spectroscopic target QSOs. We measure properties of 87", "galaxies, of which 33 are associated with corresponding Ly absorption", "systems and 24 do not produce corresponding Ly{alpha} absorption lines", "to within sensitive upper limits. Considering only galaxy and absorber", "pairs that are likely to be physically associated and excluding galaxy", "and absorber pairs within 3000km/s of the background QSOs leaves 26", "galaxy and absorber pairs and seven galaxies that do not produce", "corresponding Ly{alpha} absorption lines to within sensitive upper", "limits. Redshifts of the galaxy and absorber pairs range from 0.0750", "to 0.8912 with a median of 0.3718, and impact parameter separations of", "the galaxy and absorber pairs range from 12.4 to 157.4h^-1^kpc with a", "median of 62.4h^-1^kpc."], "doi_pub": ["10.1086/305554"], "orcid_pub": ["0000-0001-8813-4182"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Journal of observations ", "columns": [{"name": "Field", "desc": "Field designation "}, {"name": "RAh", "desc": "Right ascension (B1950.0) "}, {"name": "RAm", "desc": "Right ascension (B1950.0) "}, {"name": "RAs", "desc": "Right ascension (B1950.0) "}, {"name": "DE-", "desc": "Declination sign (B1950.0) "}, {"name": "DEd", "desc": "Declination (B1950.0) "}, {"name": "DEm", "desc": "Declination (B1950.0) "}, {"name": "DEs", "desc": "Declination (B1950.0) "}, {"name": "Zem", "desc": "Emission redshift "}, {"name": "Filter", "desc": "Filter "}, {"name": "TExp", "desc": "Exposition time "}, {"name": "Date", "desc": "Observation date "}]}, {"name": "table2.dat", "desc": "Journal of archival observations ", "columns": [{"name": "Field", "desc": "Field designation "}, {"name": "RAh", "desc": "Right ascension (B1950.0) "}, {"name": "RAm", "desc": "Right ascension (B1950.0) "}, {"name": "RAs", "desc": "Right ascension (B1950.0) "}, {"name": "DE-", "desc": "Declination sign (B1950.0) "}, {"name": "DEd", "desc": "Declination (B1950.0) "}, {"name": "DEm", "desc": "Declination (B1950.0) "}, {"name": "DEs", "desc": "Declination (B1950.0) "}, {"name": "Zem", "desc": "Emission redshift "}, {"name": "Filter", "desc": "Filter "}, {"name": "TExp", "desc": "Exposition time "}, {"name": "Date", "desc": "Observation date "}]}, {"name": "table4.dat", "desc": "Galaxies and Absorption Systems ", "columns": [{"name": "Field", "desc": "Galaxy field name (1) "}, {"name": "oRA", "desc": "Right Ascension offset from the QSO (1) "}, {"name": "oDE", "desc": "Declination offset from the QSO (1) "}, {"name": "z", "desc": "Galaxy redshift "}, {"name": "Rho", "desc": "Impact parameter in units of kpc/h "}, {"name": "DRad", "desc": "? Effective disk radius in units of kpc/h "}, {"name": "BRad", "desc": "? Effective bulge radius in units of kpc/h "}, {"name": "l_D/B", "desc": "Limit flag in D/B "}, {"name": "D/B", "desc": "? Disk to Bulge ratio "}, {"name": "Alpha", "desc": "? Orientation angle "}, {"name": "Inc", "desc": "? Inclination angle "}, {"name": "b/a", "desc": "? Bulge axis ratio "}, {"name": "Wmag", "desc": "? The WFPC2 apparent magnitude "}, {"name": "SB", "desc": "? Rest-frame B band mean surface brightness "}, {"name": "BMag", "desc": "? Absolute B band magnitude minus 5*log[h] "}, {"name": "zabs", "desc": "? Absorber redshift "}, {"name": "l_EqWLya", "desc": "Limit flag on EqWLya "}, {"name": "EqWLya", "desc": "? Ly{alpha} rest-frame equivalent width (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_505_L7"}} {"id": "J/ApJ/505/L7", "title_cds": "5 BAL QSO discovery", "title_create": "Brotherton+, 1998", "year": "1998", "author": "Brotherton M.S., van Breugel W., Smith R.J., Boyle B.J., Shanks T., Croom S.M., Miller L., Becker R.H.", "title_pub": "Discovery of radio-loud broad absorption line quasars using ultraviolet excess and deep radio selection.", "first_author": "Brotherton M.S.", "ref_biblio": [""], "bibcode": ["1998ApJ...505L...7B"], "keyword_cds": "QSOs ; Photometry ; Equivalent widths ; Redshifts", "keyword_pub": "quasar: absorption lines - quasar: emission lines - galaxies: general", "abstract": ["We report the discovery of five broad absorption line (BAL) QSOs in a", "complete sample of 111 ultraviolet excess (UVX) QSO candidates also", "detected in the NRAO VLA Sky Survey. All five BAL QSOs, which include", "two high-ionization BAL QSOs and three low-ionization BAL QSOs, are", "formally radio loud. Of QSOs with z>0.4, 3%+/-2% show low-ionization", "BALs, and of QSOs with z>1.5 , all radio loud, 9%+/-5% show BALs;", "these frequencies are consistent with those of optical surveys. While", "the first reported radio-loud BAL QSO, FIRST J155633.8+351758, is", "likely to be heavily dust reddened and thus less radio loud than", "indicated by its observed radio-to-optical luminosity, these QSOs are", "UVX-selected and probably free of significant dust along the line of", "sight. We point out unusual features in two of the BAL QSOs and", "discuss the significance finding these heretofore rare objects."], "doi_pub": ["10.1086/311599"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Radio-loud UVX BAL QSO properties ", "columns": [{"name": "UN", "desc": "Quasar name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "z", "desc": "Redshift "}, {"name": "Bjmag", "desc": "B_j_ magnitude (1) "}, {"name": "U-Bj", "desc": "U-Bj colour index (1) "}, {"name": "Bj-R", "desc": "Bj-R colour index (1) "}, {"name": "BMAG", "desc": "Absolute B magnitude (2) "}, {"name": "S1400MHz", "desc": "Flux density at 1400MHz "}, {"name": "e_S1400MHz", "desc": "rms uncertainty on S1400MHz "}, {"name": "logL1400MHz", "desc": "Luminosity at 1400MHz "}, {"name": "logR*", "desc": "Formal measure of radio loudness (2) (3) "}]}, {"name": "tables.tex", "desc": "LaTeX version of the tables ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_520_491"}} {"id": "J/ApJ/520/491", "title_cds": "Superclustering in Aquarius", "title_create": "Batuski+, 1999", "year": "1999", "author": "Batuski D.J., Miller C.J., Slinglend K.A., Balkowski C., Maurogordato S., Cayatte V., Felenbok P., Olowin R.", "title_pub": "Discovery of extreme examples of superclustering in Aquarius.", "first_author": "Batuski D.J.", "ref_biblio": [""], "bibcode": ["1999ApJ...520..491B"], "see_also": ["VII/4 : Abell and Zwicky Clusters of Galaxies (Abell+ 1974)", "VII/110 : Rich Clusters of Galaxies (Abell+ 1989)"], "keyword_cds": "Clusters, galaxy ; Radial velocities", "keyword_pub": "galaxies: clusters: general - galaxies: distances and redshifts", "abstract": ["The results of spectroscopic observations of 46 R>=1 clusters of", "galaxies from the Abell (Cat. ) and Abell, Corwin, & Olowin", "(hereafter ACO, Cat. ) catalogs are presented. The", "observations were conducted at the ESO 3.6 m telescope with the", "Meudon-ESO Fibre Optics Spectrograph (MEFOS) multiple-fiber", "spectrograph. Thirty-nine of the clusters lie in a 10{deg}x45{deg}", "strip of sky that contains two supercluster candidates (in Aquarius", "and Eridanus)."], "doi_pub": ["10.1086/307484"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Abell/ACO clusters observed in 10{deg} square Centered on Aquarius supercluster", "columns": [{"name": "ACO", "desc": "Cluster name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "HV", "desc": "(R+1)-weighted heliocentric velocity (1) "}, {"name": "n_HV", "desc": "[e] HV is the emission-line velocity "}, {"name": "e_HV", "desc": "rms uncertainty on HV "}, {"name": "Em", "desc": "? Object number if the subject galaxy has an emission-line velocity"}, {"name": "Note", "desc": "[ae] Note (2) "}, {"name": "Comm", "desc": "Comments "}]}, {"name": "table2.dat", "desc": "Other Abell/ACO clusters observed within 10{deg}x45{deg} strip", "columns": [{"name": "ACO", "desc": "Cluster name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "HV", "desc": "(R+1)-weighted heliocentric velocity (1) "}, {"name": "n_HV", "desc": "[e] HV is the emission-line velocity "}, {"name": "e_HV", "desc": "rms uncertainty on HV "}, {"name": "Em", "desc": "? Object number if the subject galaxy has an emission-line velocity"}, {"name": "Note", "desc": "[ae] Note (2) "}, {"name": "Comm", "desc": "Comments "}]}, {"name": "table3.dat", "desc": "Abell/ACO galaxies in Grus-Indus sample ", "columns": [{"name": "ACO", "desc": "Cluster name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "HV", "desc": "(R+1)-weighted heliocentric velocity (1) "}, {"name": "n_HV", "desc": "[e] HV is the emission-line velocity "}, {"name": "e_HV", "desc": "rms uncertainty on HV "}, {"name": "Em", "desc": "? Object number if the subject galaxy has an emission-line velocity"}, {"name": "Note", "desc": "[ae] Note (2) "}, {"name": "Comm", "desc": "Comments "}]}, {"name": "table4.dat", "desc": "Emission-line galaxy velocities ", "columns": [{"name": "ACO", "desc": "ACO name "}, {"name": "Em", "desc": "Object number "}, {"name": "Note", "desc": "[ae] Note "}, {"name": "Vem", "desc": "Emission-line velocity "}, {"name": "e_Vem", "desc": "rms uncertainty on Vem "}, {"name": "Lines", "desc": "Lines found (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_521_155"}} {"id": "J/ApJ/521/155", "title_cds": "New Cepheids and distance to NGC 4535", "title_create": "Macri+, 1999", "year": "1999", "author": "Macri L.M., Huchra J.P., Stetson P.B., Silbermann N.A., Freedman W.L., Kennicutt R.C., Mould J.R., Madore B.F., Bresolin F., Ferrarese L., Ford H.C., Graham J.A., Gibson B.K., Han M., Harding P., Hill R.J., Hoessel J.G., Hughes S.M.G., Kelson D.D., Illingworth G.D., Phelps R.L., Prosser C.F., Rawson D.M., Saha A., Sakai S., Turner A.", "title_pub": "The extragalactic distance scale key project. XVIII. The discovery of Cepheids and a new distance to NGC 4535 using the Hubble space telescope.", "first_author": "Macri L.M.", "ref_biblio": [""], "bibcode": ["1999ApJ...521..155M"], "see_also": ["J/ApJ/463/26 : Extragalactic Distance Scale Key Project. III (Kelson+ 1996)", "J/ApJ/507/655 : VI photometry of new Cepheids in NGC 2541 (Ferrarese+, 1998)", "J/ApJ/508/491 : M101 Cepheids (Stetson+, 1998)", "J/ApJ/523/540 : VI photometry of new Cepheids in NGC 3319 (Sakai+, 1999)", "J/ApJ/529/723 : VI photometry of Cepheids (Gibson+, 2000)"], "keyword_cds": "Stars, variable ; Photometry", "keyword_pub": "Cepheids - distance scale - galaxies: distances and redshifts - galaxies: individual (NGC 4535)", "abstract": ["We report on the discovery of Cepheids in the Virgo spiral galaxy NGC", "4535, based on observations made with the Wide Field and Planetary", "Camera 2 on board the Hubble Space Telescope (HST). NGC 4535 is one of", "18 galaxies observed as a part of The HST Key Project on the", "Extragalactic Distance Scale, which aims to measure the Hubble", "constant to 10% accuracy. NGC 4535 was observed over 13 epochs using", "the F555W filter, and over 9 epochs using the F814W filter. The HST", "F555W and F814W data were transformed to the Johnson V and", "Kron-Cousins I magnitude systems, respectively. Photometry was", "performed using two independent programs, DoPHOT and DAOPHOT", "II/ALLFRAME. Period-luminosity relations in the V and I bands were", "constructed using 39 high-quality Cepheids present in our set of 50", "variable candidates. We obtain a distance modulus of 31.02+/-0.26mag,", "corresponding to a distance of 16.0+/-1.9Mpc. Our distance estimate is", "based on values of {mu}_0_=18.50+/-0.10mag and E(V-I)=0.13mag for the", "distance modulus and reddening of the LMC, respectively."], "doi_pub": ["10.1086/307541"], "orcid_pub": ["0000-0002-1775-4859"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Cepheid candidates - coordinates and classification ", "columns": [{"name": "[MHS99]", "desc": "Cepheid candidate number (CNN) "}, {"name": "Chip", "desc": "Chip number "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "Grade", "desc": "Quality grade (1) "}, {"name": "n_Grade", "desc": "[*] Stars used in the final fits (2) "}]}, {"name": "table3.dat", "desc": "Cepheid candidates - mean properties ", "columns": [{"name": "[MHS99]", "desc": "Cepheid candidate number (CNN) "}, {"name": "PerA", "desc": "Allframe period "}, {"name": "e_PerA", "desc": "rms uncertainty on PerA "}, {"name": "A", "desc": "Allframe average V magnitude "}, {"name": "e_A", "desc": "rms uncertainty on A "}, {"name": "A", "desc": "Allframe average I magnitude "}, {"name": "e_A", "desc": "rms uncertainty on A "}, {"name": "PerD", "desc": "DoPHOT period "}, {"name": "e_PerD", "desc": "rms uncertainty on PerD "}, {"name": "D", "desc": "DoPHOT average V magnitude "}, {"name": "e_D", "desc": "rms uncertainty on D "}, {"name": "D", "desc": "DoPHOT average I magnitude "}, {"name": "e_D", "desc": "rms uncertainty on D "}]}, {"name": "taba3-6.dat", "desc": "Secondary photometry stars for PC1, WF1, WF2 and WF3 ", "columns": [{"name": "Chip", "desc": "Chip (PC1, WF1, WF2 or WF3) "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "A", "desc": "Allframe average V magnitude "}, {"name": "e_A", "desc": "rms uncertainty on A "}, {"name": "A", "desc": "Allframe average I magnitude "}, {"name": "e_A", "desc": "rms uncertainty on A "}, {"name": "D", "desc": "DoPHOT average V magnitude "}, {"name": "e_D", "desc": "rms uncertainty on D "}, {"name": "D", "desc": "DoPHOT average I magnitude "}, {"name": "e_D", "desc": "rms uncertainty on D "}]}, {"name": "taba7-10.dat", "desc": "DoPHOT and ALLFRAME photometry ", "columns": [{"name": "[MHS99]", "desc": "Cepheid candidate number (CNN) "}, {"name": "HJD", "desc": "Heliocentric Julian date "}, {"name": "Filt", "desc": "Filter (1) "}, {"name": "mag", "desc": "Magnitude in Filt band "}, {"name": "e_mag", "desc": "rms uncertainty on mag "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_522_983"}} {"id": "J/ApJ/522/983", "title_cds": "M80 blue straggler stars", "title_create": "Ferraro+, 1999", "year": "1999", "author": "Ferraro F.R., Paltrinieri B., Rood R.T., Dorman B.", "title_pub": "Blue straggler stars: the spectacular population in M80.", "first_author": "Ferraro F.R.", "ref_biblio": [""], "bibcode": ["1999ApJ...522..983F"], "keyword_cds": "Stars, blue ; Photometry, ultraviolet", "keyword_pub": "blue stragglers - globular clusters: individual (M80) - stars: evolution - ultraviolet: stars", "mission": "HST", "abstract": ["Using Hubble Space Telescope WFPC2 observations in two ultraviolet", "(UV) filters (F225W and F336W) of the central region of the", "high-density Galactic globular cluster (GGC) M80, we have identified", "305 blue straggler stars (BSS), which represents the largest and most", "concentrated population of BSS ever observed in a GGC. We also", "identify the largest clean sample of evolved BSS yet found. The high", "stellar density alone cannot explain the BSS, and we suggest that in", "M80 we are witnessing a transient dynamical state, during which", "stellar interactions are delaying the core-collapse process leading to", "an exceptionally large population of collisional BSS."], "object": ["16 17 02.5 -22 58 30 M 80 = NGC 6093"], "doi_pub": ["10.1086/307700"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "The BSS population in M 80 ", "columns": [{"name": "Name", "desc": "BSS number (BSS NNN) (Cl* NGC 6093 BSS NNN in Simbad) (1)"}, {"name": "FPR", "desc": "FPR (1999ApJ...522..983F) identification number (Cl* NGC 6093 FPR NNNNN in Simbad)"}, {"name": "m255", "desc": "m_255_ UV magnitude "}, {"name": "Umag", "desc": "U magnitude "}, {"name": "Xpos", "desc": "X position (2) "}, {"name": "Ypos", "desc": "Y position (2) "}]}, {"name": "table2.dat", "desc": "The E-BSS population in M 80 ", "columns": [{"name": "EBSS", "desc": "E-BSS number (E-BSS NN) (Cl* NGC 6093 EBSS NN in Simbad)"}, {"name": "FPR", "desc": "FPR (1999ApJ...522..983F) identification number (Cl* NGC 6093 FPR NNNNN in Simbad)"}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "Umag", "desc": "U magnitude "}, {"name": "Xpos", "desc": "X position (1) "}, {"name": "Ypos", "desc": "Y position (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_523_87"}} {"id": "J/ApJ/523/87", "title_cds": "Shakhbazian compact galaxy groups", "title_create": "Tovmassian+, 1999", "year": "1999", "author": "Tovmassian H.M., Chavushyan V.H., Verkhodanov O.V., Tiersch H.", "title_pub": "Radio emission of Shakhbazian compact galaxy groups.", "first_author": "Tovmassian H.M.", "ref_biblio": [""], "bibcode": ["1999ApJ...523...87T"], "see_also": ["VII/89 : Compact groups of compact galaxies (Shakhbazian+ 1973-1979)", "VIII/59 : The FIRST Survey, version 1999Jul (White+ 1999)", "J/AJ/115/1693 : NRAO VLA Sky Survey (NVSS) (Condon+, 1998)"], "keyword_cds": "Clusters, galaxy ; Radio sources", "keyword_pub": "galaxies: clusters: general - radio continuum: galaxies - submillimeter - surveys", "abstract": ["We detect 353 radio sources from the NRAO VLA Sky Survey (NVSS, Cat.", ") and the FIRST Survey (Cat. ) within the", "areas of 179 Shakhbazian compact groups (ShCGs, Cat. ) of", "galaxies. Ninety-three of them are identified with galaxies in", "74 ShCGs. Six radio sources have complex structure. The radio spectra", "of 22 sources are determined. Radio luminosities of galaxies in ShCGs", "are in general higher than those of galaxies in Hickson compact groups", "(HCGs). A comparison of radio (at 1.4GHz) and FIR (at 60{mu}m) fluxes", "of ShCG galaxies with those of HCG galaxies shows that galaxies in", "ShCGs are relatively stronger emitters at radio wavelengths, while", "galaxies in HCGs have relatively stronger FIR emission. The reasons", "for such differences are discussed"], "doi_pub": ["10.1086/307726"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "List of radio identifications ", "columns": [{"name": "ShCG.G-xy", "desc": "Shakhbazian designation of the group and number of the galaxy (as labeled in the original ShCG finding charts) (1)"}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Name", "desc": "Identified radio source "}, {"name": "RArh", "desc": "Radio source right ascension (J2000) "}, {"name": "RArm", "desc": "Radio source right ascension (J2000) "}, {"name": "RArs", "desc": "Radio source right ascension (J2000) "}, {"name": "DEr-", "desc": "Radio source declination sign (J2000) "}, {"name": "DErd", "desc": "Radio source declination (J2000) "}, {"name": "DErm", "desc": "Radio source declination (J2000) "}, {"name": "DErs", "desc": "Radio source declination (J2000) "}, {"name": "S1.4GHz", "desc": "1.4GHz radio source flux density "}]}, {"name": "table2.dat", "desc": "Radio spectral indices ", "columns": [{"name": "ShCG.G-xy", "desc": "Shakhbazian designation (1) "}, {"name": "SI", "desc": "Radio spectral index "}]}, {"name": "table3.dat", "desc": "Radio luminosities ", "columns": [{"name": "ShCG.G-xy", "desc": "Shakhbazian designation (1) "}, {"name": "z", "desc": "Redshift "}, {"name": "logP1.4GHz", "desc": "Radio luminosity at 1.4GHz "}]}, {"name": "table4.dat", "desc": "List of HCG radio identifications ", "columns": [{"name": "Shk", "desc": "Shakhbazian designation (1) "}, {"name": "MType", "desc": "Morphological type "}, {"name": "Name", "desc": "Radio source designation "}, {"name": "F1.4", "desc": "1.4GHz flux "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_567_12"}} {"id": "J/ApJ/567/12", "title_cds": "Short Title", "title_create": "Author+, ", "title_pub": "Title of the paper", "first_author": "Authors", "author": "Authors", "ref_biblio": [""], "bibcode": ["2019ApJ...567...12.\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Coralie Fix [CDS]", "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_616_1284"}} {"id": "J/ApJ/616/1284", "title_cds": "Automated classification of ROSAT sources", "title_create": "McGlynn+, 2004", "year": "2004", "author": "McGlynn T.A., Suchkov A.A., Winter E.L., Hanisch R.J., White R.L., Ochsenbein F., Derriere S., Voges W., Corcoran M.F., Drake S.A., Donahue M.", "title_pub": "Automated classification of ROSAT sources using heterogeneous multiwavelength source catalogs.", "first_author": "McGlynn T.A.", "ref_biblio": [""], "bibcode": ["2004ApJ...616.1284M"], "see_also": ["http://heasarc.gsfc.nasa.gov/classx/classx_classes/index.html :", "IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)", "IX/29 : ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000)", "IX/31 : The WGACAT version of ROSAT sources (White+ 2000)"], "keyword_cds": "X-ray sources", "keyword_pub": "methods: statistical - surveys - X-rays: binaries - X-rays: general - X-rays: stars", "abstract": ["We describe an online system for automated classification of X-ray", "sources, ClassX, and we present preliminary results of classification", "of the three major catalogs of ROSAT sources, ROSAT All-Sky Survey", "(RASS) Bright Source Catalog (Cat. ), RASS Faint Source Catalog", "(Cat. ), and WGACAT (Cat. ), into six class categories:", "stars, white dwarfs, X-ray binaries, galaxies, active galactic nuclei,", "and clusters of galaxies. ClassX is based on a machine-learning", "technology. It represents a system of classifiers, each classifier", "consisting of a considerable number of oblique decision trees. These", "trees are built as the classifier is \"trained\" to recognize various", "classes of objects using a training sample of sources of known object", "types. Each source is characterized by a preselected set of", "parameters, or attributes; the same set is then used as the classifier", "conducts classification of sources of unknown identity. The ClassX", "pipeline features an automatic search for X-ray source counterparts", "among heterogeneous data sets in online data archives using Virtual", "Observatory protocols; it retrieves from those archives all the", "attributes required by the selected classifier and inputs them to the", "classifier. The user input to ClassX is typically a file with target", "coordinates, optionally complemented with target IDs. The output", "contains the class name, attributes, and class probabilities for all", "classified targets."], "doi_pub": ["10.1086/424955"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table5a.dat", "desc": "Classification of RASS BSC by the RASS-X classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table5b.dat", "desc": "Classification of RASS BSC by the RASS-XOR classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table5c.dat", "desc": "Classification of RASS BSC by the WGACAT-X classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table5d.dat", "desc": "Classification of RASS BSC by the WGACAT-XOR classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table6a.dat", "desc": "Classification of WGACAT by the RASS-X classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table6b.dat", "desc": "Classification of WGACAT by the RASS-XOR classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table6c.dat", "desc": "Classification of WGACAT by the WGACAT-X classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table6d.dat", "desc": "Classification of WGACAT by the WGACAT-XOR classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table7a.dat", "desc": "Classification of RASS FSC by the RASS-X classifier ", "columns": [{"name": "Seq", "desc": "Sequential number of source in RASS FSC "}]}, {"name": "table7b.dat", "desc": "Classification of RASS FSC by the RASS-XOR classifier ", "columns": [{"name": "Seq", "desc": "Sequential number of source in RASS FSC "}]}, {"name": "table7c.dat", "desc": "Classification of RASS FSC by the WGACAT-X classifier ", "columns": [{"name": "Seq", "desc": "Sequential number of source in RASS FSC "}]}, {"name": "table7d.dat", "desc": "Classification of RASS FSC by the WGACAT-XOR classifier ", "columns": [{"name": "Seq", "desc": "Sequential number of source in RASS FSC "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_654_499"}} {"id": "J/ApJ/654/499", "title_cds": "H-rich white dwarfs spectropolarimetric survey", "title_create": "Kawka+, 2007", "year": "2007", "author": "Kawka A., Vennes S., Schmidt G.D., Wickramasinghe D.T., Koch R.", "title_pub": "Spectropolarimetric survey of hydrogen-rich white dwarf stars.", "first_author": "Kawka A.", "ref_biblio": [""], "bibcode": ["2007ApJ...654..499K"], "keyword_cds": "", "keyword_pub": "magnetic fields - white dwarfs", "mission": "", "abstract": ["We have conducted a survey of 61 southern white dwarfs searching for", "magnetic fields using Zeeman spectropolarimetry. Our objective is to", "obtain a magnetic field distribution for these objects and, in", "particular, to find white dwarfs with weak fields. We found one", "possible candidate (WD 0310688) that may have a weak magnetic field of", "-6.1+/-2.2kG. Next, we determine the fraction and distribution of", "magnetic white dwarfs in the solar neighborhood and investigate the", "probability of finding more of these objects based on the current", "incidence of magnetism in white dwarfs within 20 pc of the Sun. We", "have also analyzed the spectra of the white dwarfs to obtain effective", "temperatures and surface gravities."], "description": ["The data for the survey of magnetic fields in southern white dwarfs", "were acquired using the 74 inch (1.88 m) telescope at the Mount", "Stromlo Observatory with the Steward Observatory CCD", "Spectropolarimeter. The observations were conducted on 2000 October", "27-29, November 3, 5, and 25-26, and December 14, 23-28, and 31 and", "2001 January 1, 18-20, and 27 and February 17, 18, 21, 22, and 25."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/509072"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_702_506"}} {"id": "J/ApJ/702/506", "title_cds": "The Clowes-Campusano LQG Survey. I.", "title_create": "Haberzettl+, 2009", "year": "2009", "author": "Haberzettl L., Williger G.M., Lauroesch J.T., Haines C.P., Valls-Gabaud D., Harris K.A., Koekemoer A.M., Loveday J., Campusano L.E., Clowes R.G., Dave R., Graham M.J., Sochting I.K.", "title_pub": "The Clowes-Campusano Large Quasar Group Survey. I. GALEX selected sample of Lyman break galaxies at z~1.", "first_author": "Haberzettl L.", "ref_biblio": [""], "bibcode": ["2009ApJ...702..506H"], "see_also": ["VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)", "II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)", "J/A+A/533/A142 : UV-to-IR fluxes of Hickson compact groups (Bitsakis+, 2011)", "J/MNRAS/403/683 : GALEX Arecibo SDSS survey (GASS) (Catinella+, 2010)", "J/ApJ/697/1410 : Lyman break galaxies at z~1.8-2.8 (Ly+, 2009)", "J/MNRAS/392/19 : The 2dF-SDSS QSO survey (Croom+, 2009)", "J/MNRAS/380/986 : Lyman-break galaxies from GALEX (Burgarella+, 2007)", "J/AJ/133/1780 : GALEX/SDSS quasar catalog (Trammell+, 2007)", "J/MNRAS/249/218 : Group of quasars (Clowes+, 1991)", "http://www.sdss.org/ : SDSS web site"], "keyword_cds": "Galaxies, optical ; Redshifts ; Surveys ; Ultraviolet ; Photometry, SDSS", "keyword_pub": "galaxies: distances and redshifts - galaxies: evolution - large-scale structure of universe - quasars: general", "abstract": ["The nature of galaxy structures on large scales is a key observational", "prediction for current models of galaxy formation. The Sloan Digital", "Sky Survey (SDSS) and the 2dF galaxy survey have revealed a number of", "structures on 40-150h^-1^Mpc scales at low redshifts, and some even", "larger ones. To constrain galaxy number densities, luminosities, and", "stellar populations in large structures at higher redshift, we have", "investigated two sheet-like structures of galaxies at z=0.8 and 1.3", "spanning 150h^-1^ comoving Mpc embedded in large quasar groups (LQGs)", "extending over at least 200h^-1^Mpc. We present first results of an", "analysis of these sheet-like structures using two contiguous 1{deg}", "Galaxy Evolution Explorer (GALEX) fields (FUV and NUV)", "cross-correlated with optical data from the SDSS. We derive a sample", "of 462 Lyman break galaxy (LBG) candidates coincident with the sheets.", "Using the GALEX and SDSS data, we show that the overall average", "spectral energy distribution of a LBG galaxy at z~1 is flat (in", "f_{lambda}_) in the rest-frame wavelength range from 1500{AA} to", "4000{AA}, implying evolved populations of stars in the LBGs. From the", "luminosity functions we get indications for overdensities in the two", "LQGs compared to their foreground regions."], "description": ["We observed part of the Clowes-Campusano Large Quasar Group (CCLQG),", "it contains at least 18 bright quasars at 1.2 in Simbad)"}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "FUVmag", "desc": "?=99 GALEX FUV band (1538.6{AA}) magnitude "}, {"name": "e_FUVmag", "desc": "?=99 Error in FUVmag "}, {"name": "NUVmag", "desc": "GALEX NUV band (2315.7{AA}) magnitude "}, {"name": "e_NUVmag", "desc": "Error in NUVmag "}, {"name": "umag", "desc": "SDSS-DR5 u band magnitude "}, {"name": "e_umag", "desc": "Error in umag "}, {"name": "gmag", "desc": "SDSS-DR5 g band magnitude "}, {"name": "e_gmag", "desc": "Error in gmag "}, {"name": "rmag", "desc": "SDSS-DR5 r band magnitude "}, {"name": "e_rmag", "desc": "Error in rmag "}, {"name": "imag", "desc": "SDSS-DR5 i band magnitude "}, {"name": "e_imag", "desc": "Error in imag "}, {"name": "zmag", "desc": "SDSS-DR5 z band magnitude "}, {"name": "e_zmag", "desc": "Error in zmag "}, {"name": "z", "desc": "Photometric redshift "}, {"name": "e_z", "desc": "Error in z "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_716_398"}} {"id": "J/ApJ/716/398", "title_cds": "The 1998 november 14 Saturn occultation. I.", "title_create": "Harrington+, 2010", "year": "2010", "author": "Harrington J., French R.G.", "title_pub": "The 1998 november 14 occulaion of GSC 0622-00345 by Saturn. I. Techniques for ground-based stellar occultations", "first_author": "Harrington J.", "ref_biblio": [""], "bibcode": ["2010ApJ...716..398H"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Greg Schwarz [AAS], Emmanuelle Perret [CDS]", "doi_pub": ["10.1088/0004-637X/716/1/398"], "orcid_pub": ["0000-0002-8955-8531"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_750_90"}} {"id": "J/ApJ/750/90", "title_cds": "Short Title", "title_create": "Kucas+, 2012", "year": "2012", "author": "Kucas S., Karazija R., Momkauskaite A.", "title_pub": "Cascades after k-vacancy production in atoms and ions of light elements.", "first_author": "Kucas S.", "ref_biblio": [""], "bibcode": ["2012ApJ...750...90K"], "keyword_cds": "", "keyword_pub": "atomic data - atomic processes - radiation mechanisms: general - X-rays: general", "abstract": ["The results of detailed level-by-level calculations of Auger and", "radiative cascades after K-vacancy production are presented for the", "astrophysically important elements, namely Ne, Mg, Si, S, and Ar.", "Calculations are performed using the single-configuration,", "quasi-relativistic approximation. The whole isonuclear sequence of", "ions for a given element is considered. For the first time, the", "dependence of the cascade on the initial vacancy state is", "investigated. The populations are presented not only for the levels of", "the final configurations, but also for the levels of the excited", "configurations after the Auger transitions. An intense characteristic", "emission can be observed from such levels."], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/750/2/90"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_768_42"}} {"id": "J/ApJ/768/42", "title_cds": "Short Title", "title_create": "Cubillos+, 2013", "year": "2013", "author": "Cubillos P., Harrington J., Madhusudhan N., Stevenson K.B., Hardy R.A., Blecic J., Anderson D.R., Hardin M., Campo C.J.", "title_pub": "WASP-8b: characterization of a cool and eccentric exoplanet with Spitzer.", "first_author": "Cubillos P.", "ref_biblio": [""], "bibcode": ["2013ApJ...768...42C"], "keyword_cds": "", "keyword_pub": "planetary systems; stars: individual: WASP-8; techniques: photometric", "abstract": ["WASP-8b has 2.18 times Jupiter's mass and is on an eccentric (e=0.31)", "8.16 day orbit. With a time-averaged equilibrium temperature of 948K,", "it is one of the least-irradiated hot Jupiters observed with the", "Spitzer Space Telescope. We have analyzed six photometric light curves", "of WASP-8b during secondary eclipse observed in the 3.6, 4.5, and", "8.0um Infrared Array Camera bands. The eclipse depths are", "0.113%+/-0.018%, 0.069%+/-0.007%, and 0.093%+/-0.023%, respectively,", "giving respective brightness temperatures of 1552, 1131, and 938K. We", "characterized the atmospheric thermal profile and composition of the", "planet using a line-by-line radiative transfer code and a Markov-chain", "Monte Carlo sampler. The data indicated no thermal inversion,", "independently of any assumption about chemical composition. We noted", "an anomalously high 3.6{mu}m brightness temperature (1552K); by", "modeling the eccentricity-caused thermal variation, we found that this", "temperature is plausible for radiative timescales less than ~10^2^hr.", "However, as no model spectra fit all three data points well, the", "temperature discrepancy remains as an open question."], "object": [], "curator": "Greg Schwarz [AAS], Emmanuelle Perret [CDS]", "doi_pub": ["10.1088/0004-637X/768/1/42"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_779_5"}} {"id": "J/ApJ/779/5", "title_cds": "Short Title", "title_create": "Blecic+, 2013", "year": "2013", "author": "Blecic J., Harrington J., Madhusudhan N., Stevenson K.B., Hardy R.A., Cubillos P.E., Hardin M., Campo C.J., Bowman W.C., Nymeyer S., Loredo T.J., Anderson D.R., Maxted P.F.L.", "title_pub": "Thermal emission of WASP-14b revealed with three Spitzer eclipses.", "first_author": "Blecic J.", "ref_biblio": [""], "bibcode": ["2013ApJ...779....5B"], "keyword_cds": "", "keyword_pub": "eclipses; planets and satellites: atmospheres; planets and satellites: individual: WASP-14b; techniques: photometric", "abstract": ["Exoplanet WASP-14b is a highly irradiated, transiting hot Jupiter.", "Joshi et al. calculate an equilibrium temperature (T_eq_) of 1866K for", "zero albedo and reemission from the entire planet, a mass of 7.3+/-0.5", "Jupiter masses (M_J_), and a radius of 1.28+/-0.08 Jupiter radii", "(R_J_). Its mean density of 4.6g/cm3 is one of the highest known for", "planets with periods less than three days. We obtained three secondary", "eclipse light curves with the Spitzer Space Telescope. The eclipse", "depths from the best jointly fit model are 0.224%+/-0.018% at 4.5{mu}m", "and 0.181%+/-0.022% at 8.0{mu}m. The corresponding brightness", "temperatures are 2212+/-94K and 1590+/-116K. A slight ambiguity", "between systematic models suggests a conservative 3.6{mu}m eclipse", "depth of 0.19%+/-0.01% and brightness temperature of 2242+/-55K.", "Although extremely irradiated, WASP-14b does not show any distinct", "evidence of a thermal inversion. In addition, the present data", "nominally favor models with day-night energy redistribution less than", "~30%. The current data are generally consistent with oxygen-rich as", "well as carbon-rich compositions, although an oxygen-rich composition", "provides a marginally better fit. We confirm a significant", "eccentricity of e=0.087+/-0.002 and refine other orbital parameters."], "curator": "Greg Schwarz [AAS], Emmanuelle Perret [CDS]", "doi_pub": ["10.1088/0004-637X/779/1/5"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_781_116"}} {"id": "J/ApJ/781/116", "title_cds": "Short Title", "title_create": "Blecic+, 2014", "year": "2014", "author": "Blecic J., Harrington J., Madhusudhan N., Stevenson K.B., Hardy R.A., Cubillos P.E., Hardin M., Bowman O., Nymeyer S., Anderson D.R., Hellier C., Smith A.M.S., Cameron A.C.", "title_pub": "Spitzer observations of the thermal emission from WASP-43b.", "first_author": "Blecic J.", "ref_biblio": [""], "bibcode": ["2014ApJ...781..116B"], "keyword_cds": "", "keyword_pub": "eclipses - planets and satellites: atmospheres - planets and satellites: individual: WASP-43b - techniques: photometric", "abstract": ["WASP-43b is one of the closest-orbiting hot Jupiters, with a semimajor", "axis of a=0.01526+/-0.00018AU and a period of only 0.81days. However,", "it orbits one of the coolest stars with a hot Jupiter", "(T_*_=4520+/-120K), giving the planet a modest equilibrium temperature", "of T_eq_=1440+/-40K, assuming zero Bond albedo and uniform planetary", "energy redistribution. The eclipse depths and brightness temperatures", "from our jointly fit model are 0.347%+/-0.013% and 1670+/-23K at", "3.6{mu}m and 0.382%+/-0.015% and 1514+/-25K at 4.5{mu}m. The eclipse", "timings improved the estimate of the orbital period, P, by a factor of", "three (P=0.81347436+/-1.4x10^-7^days) and put an upper limit on the", "eccentricity (e=0.010_-0.007_^+0.010^). We use our Spitzer eclipse", "depths along with four previously reported ground-based photometric", "observations in the near-infrared to constrain the atmospheric", "properties of WASP-43b. The data rule out a strong thermal inversion", "in the dayside atmosphere of WASP-43b. Model atmospheres with no", "thermal inversions and fiducial oxygen-rich compositions are able to", "explain all the available data. However, a wide range of metallicities", "and C/O ratios can explain the data. The data suggest low day-night", "energy redistribution in the planet, consistent with previous studies,", "with a nominal upper limit of about 35% for the fraction of energy", "incident on the dayside that is redistributed to the nightside."], "description": ["We observed two secondary eclipses (on 2011 Jul 30 with channel", "1-3.6{mu}m, and on 2011 Jul 29 with channel 2-4.5{mu}m) of WASP-43b", "with the Spitzer IRAC camera in subarray mode (Program ID 70084)"], "object": [], "curator": "Sylvain Guehenneux [CDS]", "doi_pub": ["10.1088/0004-637X/781/2/116"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_786_133"}} {"id": "J/ApJ/786/133", "title_cds": "Short Title", "title_create": "Yu+, 2014", "year": "2014", "author": "Yu S., Pearson J.C.", "title_pub": "Terahertz measurements of the hot hydronium ion with an extended negative glow discharge.", "first_author": "Yu S.", "ref_biblio": [""], "bibcode": ["2014ApJ...786..133Y"], "keyword_cds": "", "keyword_pub": "ISM: molecules; line: identification; molecular data techniques: spectroscopic", "mission": "", "abstract": ["Terahertz absorption spectroscopy was employed to detect the ground-state inversion transitions of the hydronium ion (H_3_O^+^). The highly excited ions were created with an extended negative glow discharge through a gas mixture of 1 mtorr of H_2_O, 2 mtorr of H_2_, and 12 mtorr of Ar, which allowed observation of transitions with J and K up to 12. In total, 47 transitions were measured in the 0.9-2.0 THz region and 22 of these were observed for the first time. The experimental uncertainties range from 100 to 300 kHz, which are much better than the range 0.3-1.2 MHz reported in previous work. Differences of up to 25.6 MHz were found between the observed positions and the catalog values that have been used for Herschel data analysis of observations of Sagittarius B2(N), NGC 4418, and Arp 220. The new and improved measurements were fit to experimental accuracies with an updated Hamiltonian, and better H_3_O^+^ predictions are reported to support the proper analysis of astronomical observations by high-resolution", "spectroscopy telescopes, such as Herschel, SOFIA, and ALMA."], "object": [], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/786/2/133"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_787_166"}} {"id": "J/ApJ/787/166", "title_cds": "Short Title", "title_create": "Aliu+, 2014", "year": "2014", "author": "Aliu E., Archambault S., Aune T., Behera B., Beilicke M., Benbow W., Berger K., Bird R., Buckley J.H., Bugaev V., Cardenzana J.V., Cerruti M., Chen X., Ciupik L., Collins-hughes E., Connolly M.P., Cui W., Dumm J., Dwarkadas V.V., Errando M., Falcone A., Federici S., Feng Q., Finley J.P., Fleischhack H., Fortin P., Fortson L., Furniss A., Galante N., Gall D., Gillanders G.H., Griffin S., Griffiths S.T., Grube J., Gyuk G., Hanna D., Holder J., Hughes G., Humensky T.B., Kaaret P., Kertzman M., Khassen Y., Kieda D., Krennrich F., Kumar S., Lang M.J., Madhavan A.S., Maier G., Mccann A.J., Meagher K., Millis J., Moriarty P., Mukherjee R., Nieto D., De Bhroithe A.O., Ong R.A., Otte A.N., Pandel D., Park N., Pohl M., Popkow A., Prokoph H., Quinn J., Ragan K., Rajotte J., Ratliff G., Reyes L.C., Reynolds P.T., Richards G.T., Roache E., Rousselle J., Sembroski G.H., Shahinyan K., Sheidaei F., Smith A.W., Staszak D., Telezhinsky I., Tsurusaki K., Tucci J.V., Tyler J., Varlotta A., Vassiliev V.V., Vincent S., Wakely S.P., Ward J.E., Weinstein A., Welsing R., Wilhelm A.", "title_pub": "Investigating the TeV morphology of MGRO J1908+06 with VERITAS.", "first_author": "Aliu E.", "ref_biblio": [""], "bibcode": ["2014ApJ...787..166A"], "keyword_cds": "", "keyword_pub": "gamma rays: general gamma-ray burst: individual: (\\objac{@3946220}{MGRO J1908+06}{19 08 42.0000 +06 11 00.000},\\objac{@3946220}{VER J1907+062}{19 08 42.0000 +06 11 00.000}) pulsars: individual: \\objac{@2689987}{PSR J1907+0602}{19 07 54.7400 +06 02 16.900} ISM: supernova remnants", "mission": "", "abstract": ["We report on deep observations of the extended TeV gamma-ray source MGRO J1908+06 made with the VERITAS very high energy gamma-ray observatory. Previously, the TeV emission has been attributed to the pulsar wind nebula (PWN) of the Fermi-LAT pulsar PSR J1907+0602. We detect MGRO J1908+06 at a significance level of 14 standard deviations (14{sigma}) and measure a photon index of 2.20+/-0.10_stat_+/- 0.20_sys_. The TeV emission is extended, covering the region near PSR J1907+0602 and also extending toward SNR G40.5-0.5. When fitted with a two-dimensional Gaussian, the intrinsic extension has a standard deviation of {sigma}_src_= 0.{deg}44+/-0.{deg}02. In contrast to other TeV PWNe of similar age in which the TeV spectrum softens with distance from the pulsar, the TeV spectrum measured near the pulsar location is consistent with that measured at a position near the rim of G40.5-0.5, 0.{deg}33 away."], "object": [], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/787/2/166"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_793_127"}} {"id": "J/ApJ/793/127", "title_cds": "Short Title", "title_create": "Vogt+, 2014", "year": "2014", "author": "Vogt F.P.A., Dopita M.A., Kewley L.J., Sutherland R.S., Scharwachter J., Basurah H.M., Ali A., Amer M.A.", "title_pub": "Galaxy emission line classification using three-dimensional line ratio diagrams.", "first_author": "Vogt F.P.A.", "ref_biblio": [""], "bibcode": ["2014ApJ...793..127V"], "keyword_cds": "", "keyword_pub": "galaxies: abundances - galaxies: general - galaxies: Seyfert - galaxies: starburst - H II regions - ISM: lines and bands", "abstract": ["Two-dimensional (2D) line ratio diagnostic diagrams have become a key", "tool in understanding the excitation mechanisms of galaxies. The", "curves used to separate the different regions--H II-like or excited by", "an active galactic nucleus (AGN)--have been refined over time but the", "core technique has not evolved significantly. However, the", "classification of galaxies based on their emission line ratios really", "is a multi-dimensional problem. Here we exploit recent software", "developments to explore the potential of three-dimensional (3D) line", "ratio diagnostic diagrams. We introduce the ZQE diagrams, which are a", "specific set of 3D diagrams that separate the oxygen abundance and the", "ionization parameter of H II region-like spectra and also enable us to", "probe the excitation mechanism of the gas. By examining these new 3D", "spaces interactively, we define the ZE diagnostics, a new set of 2D", "diagnostics that can provide the metallicity of objects excited by hot", "young stars and that cleanly separate H II region-like objects from", "the different classes of AGNs. We show that these ZE diagnostics are", "consistent with the key log [N II]/H{alpha} versus log [O III]/H{beta}", "diagnostic currently used by the community. They also have the", "advantage of attaching a probability that a given object belongs to", "one class or the other. Finally, we discuss briefly why ZQE diagrams", "can provide a new way to differentiate and study the different classes", "of AGNs in anticipation of a dedicated follow-up study."], "curator": "Prepared by [AAS], Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/793/2/127"], "orcid_pub": ["0000-0002-9665-2788"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_794_145"}} {"id": "J/ApJ/794/145", "title_cds": "Short Title", "title_create": "Savcheva+, 2014", "year": "2014", "author": "Savcheva A.S., West A.A., Bochanski J.J.", "title_pub": "A new sample of cool subdwarfs from SDSS: properties and kinematics.", "first_author": "Savcheva A.S.", "ref_biblio": [""], "bibcode": ["2014ApJ...794..145S"], "keyword_cds": "", "keyword_pub": "stars: late-type; stars: low-mass; stars: statistics; subdwarfs", "mission": "", "abstract": ["We present a new sample of M subdwarfs compiled from the seventh data release of the Sloan Digital Sky Survey. With 3517 new subdwarfs, this new sample significantly increases the number of spectroscopically confirmed low-mass subdwarfs. This catalog also includes 905 extreme and 534 ultra sudwarfs. We present the entire catalog, including observed and derived quantities, and template spectra created from co-added subdwarf spectra. We show color-color and reduced proper motion diagrams of the three metallicity classes, which are shown to separate from the disk dwarf population. The extreme and ultra subdwarfs are seen at larger values of reduced proper motion, as expected for more dynamically heated populations. We determine 3D kinematics for all of the stars with proper motions. The color-magnitude diagrams show a clear separation of the three metallicity classes with the ultra and extreme subdwarfs being significantly closer to the main sequence than the ordinary subdwarfs. All subdwarfs lie below (fainter)", "and to the left (bluer) of the main sequence. Based on the average (U, V, W) velocities and their dispersions, the extreme and ultra subdwarfs likely belong to the Galactic halo, while the ordinary subdwarfs are likely part of the old Galactic (or thick) disk. An extensive activity analysis of subdwarfs is performed using H{alpha} emission, and 208 active subdwarfs are found. We show that while the activity fraction of subdwarfs rises with spectral class and levels off at the latest spectral classes, consistent with the behavior of M dwarfs, the extreme and ultra subdwarfs are basically flat."], "object": [], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/794/2/145"], "orcid_pub": ["0000-0002-5598-046X"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_794_165"}} {"id": "J/ApJ/794/165", "title_cds": "Short Title", "title_create": "Storm+, 2014", "year": "2014", "author": "Storm S., Mundy L.G., Fernandez-lopez M., Lee K.I., Looney L.W., Teuben P., Rosolowsky E., Arce H.G., Ostriker E.C., Segura-cox D.M., Pound M.W., Salter D.M., Volgenau N.H., Shirley Y.L., Chen C.-Y., Gong H., Plunkett A.L., Tobin J.J., Kwon W., Isella A., Kauffmann J., Tassis K., Crutcher R.M., Gammie C.F., Testi L.", "title_pub": "CARMA large area star formation survey: project overview with analysis of dense gas structure and kinematics in Barnard 1.", "first_author": "Storm S.", "ref_biblio": [""], "bibcode": ["2014ApJ...794..165S"], "keyword_cds": "", "keyword_pub": "ISM: clouds; ISM: kinematics and dynamics; ISM: molecules ISM: structure; stars: formation", "mission": "", "abstract": ["We present details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N_2_H^+^, HCO^+^, and HCN (J = 1 --> 0 transitions) across over 800 square arcminutes of the Perseus and Serpens Molecular Clouds. The observations have angular resolution near 7'' and spectral resolution near 0.16 km/s. We imaged ~150 square arcminutes of Barnard 1, focusing on the main core, and the B1 Ridge and clumps to its southwest. N_2_H^+^ shows the strongest emission, with morphology similar to cool dust in the region, while HCO^+^ and HCN trace several molecular outflows from a collection of protostars in the main core. We identify a range of kinematic complexity, with N_2_H^+^ velocity dispersions ranging from ~0.05 to 0.50 km/s across the field. Simultaneous continuum mapping at 3 mm reveals six compact object detections, three of which are new detections. A new, non-binary dendrogram algorithm is used to analyze", "dense gas structures in the N_2_H^+^ position-position-velocity (PPV) cube. The projected sizes of dendrogram-identified structures range from about 0.01 to 0.34 pc. Size-linewidth relations using those structures show that non-thermal line-of-sight velocity dispersion varies weakly with projected size, while rms variation in the centroid velocity rises steeply with projected size. Comparing these relations, we propose that all dense gas structures in Barnard 1 have comparable depths into the sky, around 0.1-0.2 pc; this suggests that overdense, parsec-scale regions within molecular clouds are better described as flattened structures rather than spherical collections of gas. Science-ready PPV cubes for Barnard 1 molecular emission are available for download."], "object": [], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/794/2/165"], "orcid_pub": ["0000-0001-9401-1357"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_797_42"}} {"id": "J/ApJ/797/42", "title_cds": "Short Title", "title_create": "Cubillos+, 2014", "year": "2014", "author": "Cubillos P., Harrington J., Madhusudhan N., Foster A.S.D., Lust N.B., Hardy R.A., Bowman M.O.", "title_pub": "A Spitzer five-band analysis of the jupiter-sized planet TrES-1.", "first_author": "Cubillos P.", "ref_biblio": [""], "bibcode": ["2014ApJ...797...42C"], "keyword_cds": "", "keyword_pub": "planetary systems - stars: individual: TrES-1 - techniques: photometric", "abstract": ["With an equilibrium temperature of 1200 K, TrES-1 is one of the", "coolest hot Jupiters observed by Spitzer. It was also the first planet", "discovered by any transit survey and one of the first exoplanets from", "which thermal emission was directly observed. We analyzed all Spitzer", "eclipse and transit data for TrES-1 and obtained its eclipse depths", "and brightness temperatures in the 3.6 {mu}m (0.083%+/-0.024%,", "1270+/-110 K), 4.5 {mu}m (0.094%+/-0.024%, 1126+/-90 K), 5.8 {mu}m", "(0.162%+/-0.042%, 1205+/-130 K), 8.0 {mu}m (0.213%+/-0.042%,", "1190+/-130 K), and 16 {mu}m (0.33%+/-0.12%, 1270+/-310 K) bands. The", "eclipse depths can be explained, within 1{sigma} errors, by a standard", "atmospheric model with solar abundance composition in chemical", "equilibrium, with or without a thermal inversion. The combined", "analysis of the transit, eclipse, and radial-velocity ephemerides", "gives an eccentricity of e = 0.033_-0.031_^+0.015^, consistent with a", "circular orbit. Since TrES-1's eclipses have low signal-to-noise", "ratios, we implemented optimal photometry and differential-evolution", "Markov Chain Monte Carlo (MCMC) algorithms in our Photometry for", "Orbits, Eclipses, and Transits pipeline. Benefits include higher", "photometric precision and ~10 times faster MCMC convergence, with", "better exploration of the phase space and no manual parameter tuning."], "object": ["19 04 09.84 +36 37 57.5 TrES-1 = NAME TrES-1b"], "curator": "Prepared by [AAS], Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/797/1/42"], "orcid_pub": ["0000-0002-1347-2600"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_81_187"}} {"id": "J/ApJ/81/187", "title_cds": "Spectral Types of 4179 stars", "title_create": "Adams+, 1935", "year": "1935", "author": "Adams W.S., Joy A.H., Humason M.L., Brayton A.M.", "title_pub": "The spectroscopic absolute magnitudes and parallaxes of 4179 stars.", "first_author": "Adams W.S.", "ref_biblio": [""], "bibcode": ["1935ApJ....81..187A"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/143628"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_827_52"}} {"id": "J/ApJ/827/52", "title_cds": "Census of YSOs in IC 348 and NGC 1333", "title_create": "Luhman+, 2016", "year": "2016", "author": "Luhman K.L., Esplin T.L., Loutrel N.P.", "title_pub": "A census of young stars and brown dwarfs in IC 348 and NGC 1333.", "first_author": "Luhman K.L.", "ref_biblio": [""], "bibcode": ["2016ApJ...827...52L"], "see_also": ["II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "J/AJ/150/175 : YSOVAR: infrared photometry in NGC 1333 (Rebull+, 2015)", "J/AJ/150/40 : The Spitzer c2d survey of clouds. XII. Perseus (Young+, 2015)", "J/ApJ/807/27 : IN-SYNC III. Radial velocities of IC348 stars (Cottaar+, 2015)", "J/ApJ/799/136 : IN-SYNC. II. Candidate young stars in NGC 1333 (Foster+, 2015)", "J/ApJ/787/107 : Spatial structure of young stellar clusters. I. (Kuhn+, 2014)", "J/ApJ/786/29 : Catalog of distances to molecular clouds (Schlafly+, 2014)", "J/MNRAS/437/906 : Cl* IC 348 H 254 VRI light curves (Ripepi+, 2014)", "J/MNRAS/434/806 : Pre-main-sequence isochrones. II. SFR (Bell+, 2013)", "J/AJ/145/66 : Spitzer light curves of YSOs in IC 348 (Flaherty+, 2013)", "J/ApJ/744/6 : SONYC census of very low-mass NGC1333 objects (Scholz+, 2012)", "J/A+A/537/A135 : X-ray view of IC348 (Stelzer+, 2012)", "J/AJ/140/1214 : NIR spectroscopic survey of class I YSOs (Connelley+, 2010)", "J/AJ/140/266 : NGC 1333 X-ray luminous YSOs properties (Winston+, 2010)", "J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)", "J/AJ/138/703 : Deep MIPS observations of IC 348 nebula (Currie+, 2009)", "J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009)", "J/AJ/136/1372 : Very low-mass YSOs in NGC 1333 (Oasa+, 2008)", "J/ApJ/674/336 : Spitzer observations of NGC 1333 (Gutermuth+, 2008)", "J/ApJ/667/308 : Weak-line T Tauri in Spitzer c2d Survey. II. (Cieza+, 2007)", "J/AJ/134/411 : Properties of IC 348 members (Muench+, 2007)", "J/AJ/131/1574 : Infrared photometry of IC348 members (Lada+, 2006)", "J/AJ/127/1131 : NGC 1333 low-mass stars infrared photometry (Wilking+, 2004)", "J/ApJ/597/555 : IR photometry of IC 348 young brown dwarfs (Mainzer+, 2003)", "J/ApJ/593/1093 : IC 348 membership (Luhman+, 2003)", "J/A+A/401/543 : XMM-Newton observations of NGC 1333 (Preibisch, 2003)", "J/ApJ/575/354 : Young stellar objects in the NGC 1333 (Getman+, 2002)", "J/AJ/122/866 : X-ray sources in IC 348 from Chandra (Preibisch+, 2001)", "J/ApJ/541/977 : HST observations of low-mass stars in IC 348 (Najita+, 2000)", "J/ApJ/525/466 : Young low-mass stars & brown dwarfs in IC 348 (Luhman+, 1999)", "J/A+AS/137/305 : IC 348 proper motion catalogue (Scholz+, 1999)", "J/ApJ/497/736 : The young cluster IC 348. (Herbig, 1998)", "J/AJ/111/1964 : JHK photometry of NGC1333 (Lada+, 1996)", "J/A+AS/106/165 : Near-IR imaging photometry of NGC 1333 (Aspin+ 1994)"], "keyword_cds": "Clusters, open ; Spectra, infrared ; Photometry, infrared ; YSOs ; Cross identifications ; Proper motions ; Spectral types", "keyword_pub": "brown dwarfs; protoplanetary disks; stars: formation; stars: low-mass; stars: luminosity function, mass function; stars: pre-main sequence", "abstract": ["We have obtained optical and near-infrared spectra of candidate", "members of the star-forming clusters IC 348 and NGC 1333. We classify", "100 and 42 candidates as new members of the clusters, respectively,", "which brings the total numbers of known members to 478 and 203. We", "also have performed spectroscopy on a large majority of the previously", "known members of NGC 1333 in order to provide spectral classifications", "that are measured with the same scheme that has been applied to IC 348", "in previous studies. The new census of members is nearly complete for", "Ks<16.8 at A_J_<1.5 in IC 348 and for Ks<16.2 at A_J_<3 in NGC 1333,", "which correspond to masses of >~0.01M_{sun}_ for ages of 3Myr", "according to theoretical evolutionary models. The faintest known", "members extend below these completeness limits and appear to have", "masses of ~0.005M_{sun}_. In extinction-limited samples of cluster", "members, NGC 1333 exhibits a higher abundance of objects at lower", "masses than IC 348. It would be surprising if the initial mass", "functions of these clusters differ significantly given their similar", "stellar densities and formation environments. Instead, it is possible", "that average extinctions are lower for less massive members of", "star-forming clusters, in which case extinction-limited samples could", "be biased in favor of low-mass objects in the more heavily embedded", "clusters like NGC 1333. In the Hertzsprung-Russell diagram, the median", "sequences of IC 348 and NGC 1333 coincide with each other for the", "adopted distances of 300 and 235pc, which would suggest that they have", "similar ages. However, NGC 1333 is widely believed to be younger than", "IC 348 based on its higher abundance of disks and protostars and its", "greater obscuration. Errors in the adopted distances may be", "responsible for this discrepancy."], "description": ["We have made use of several X-ray to IR imaging surveys of IC 348 and", "NGC 1333 for identifying candidate members.", "See section 3.1 for the details.", "Unpublished images from WIRCam are also available for NGC 1333. We", "reduced all of the WIRCam images in JHKs that are available for IC 348", "and NGC 1333 from the CFHT archive, which were obtained through", "programs 07BH20 (K. Allers), 07BH12 (B. Biller), 09BD95 (L. Albert),", "O6BF23, 08BF98, and 09BF50 (J. Bouvier). The data from O6BF23 were", "those in IC 348 analyzed by Alves de Oliveira+ (2013A&A...549A.123A).", "We also reduced the Suprime-Cam images from Scholz+", "(2009ApJ...702..805S), which were retrieved from the Subaru Telescope", "data archive.", "We have obtained spectra of 152 candidate members of IC 348 and 16", "previously known members.", "We observed 130 sources with the near-IR spectrograph SpeX (R=150) at", "the NASA Infrared Telescope Facility (IRTF).", "We performed optical spectroscopy on 15 candidates (8 new members, 7", "non-members) and six known members (LRL 141, LRL 174, LRL 294, LRL", "334, LRL 366, LRL 10094) with the Inamori Magellan Areal Camera and", "Spectrograph (IMACS) on the Magellan I telescope at Las Campanas", "Observatory.", "We used the near-IR camera on the Keck I telescope (NIRC) to obtain", "low-resolution (~100) spectra of one candidate (LRL 6005) and two", "known members (LRL 1050, LRL 2103).", "We observed two and 12 candidates with the Gemini Near-Infrared Imager", "(NIRI, R=500) and the Gemini Near-Infrared Spectrograph (GNIRS, R=800),", "respectively, at the Gemini North telescope.", "In NGC 1333, we have performed spectroscopy on 55 candidate members", "and 124 known members with SpeX and 14 candidates with GNIRS.", "See section 4 for further details."], "type": ["OC"], "doi_pub": ["10.3847/0004-637X/827/1/52"], "orcid_pub": ["0000-0003-2822-2951"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Members of IC 348 ", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[42/45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31/32] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "---", "desc": "[LRL] "}, {"name": "LRL", "desc": "Name based on Luhman+ (1998ApJ...508..347L) running IDs (1)"}, {"name": "---", "desc": "<[EDJ2009] NNN> in Simbad "}, {"name": "[EDJ2009]", "desc": "? Name from Evans+ (2009, J/ApJS/181/321) "}, {"name": "---", "desc": "[CXOU] "}, {"name": "CXOU", "desc": "Name from Stelzer+ (2012, J/A+A/537/A135) "}, {"name": "A13", "desc": "Name from Alves de Oliveira+ (2013A&A...549A.123A)"}, {"name": "ONames", "desc": "Other source names "}, {"name": "SpT", "desc": "MK spectral type(s) "}, {"name": "r_SpT", "desc": "Spectral type reference (2) "}, {"name": "Spph", "desc": "Spectrograph for spectral classification (G2) "}, {"name": "Date", "desc": "Date of spectroscopy "}, {"name": "ASpT", "desc": "Adopted spectral type "}, {"name": "Aj", "desc": "[0/8]? Extinction in J band "}, {"name": "IRexc", "desc": "[yes/no ] IR excess? (3) "}, {"name": "pmRA", "desc": "[-3.5/9.4]? Proper motion in Right Ascension "}, {"name": "e_pmRA", "desc": "[0.1/6]? Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-7.9/2.6]? Proper motion in Declination "}, {"name": "e_pmDE", "desc": "[0.1/6.6]? Uncertainty in pmDE "}, {"name": "Jmag", "desc": "[6.7/20.5]? J magnitude "}, {"name": "e_Jmag", "desc": "[0.02/0.2]? Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[6.6/19]? H magnitude "}, {"name": "e_Hmag", "desc": "[0.02/0.08]? Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[6.5/18.6]? Ks magnitude "}, {"name": "e_Ksmag", "desc": "[0.01/0.2]? Uncertainty in Ksmag "}, {"name": "Ref", "desc": "JHK references (G3) "}]}, {"name": "table2.dat", "desc": "Members of NGC 1333 ", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[28/30] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[30/31] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "S74", "desc": "Name from Strom+ (1974ApJ...191..111S) "}, {"name": "---", "desc": "[ASR] "}, {"name": "ASR", "desc": "? Name from Aspin+ (1994, J/A+AS/106/165) "}, {"name": "---", "desc": "<[LAL96] NNN> in Simbad "}, {"name": "[LAL96]", "desc": "? Name from Lada+ (1996, J/AJ/111/1964) "}, {"name": "---", "desc": "<[GFT2002] NNN> in Simbad "}, {"name": "[GFT2002]", "desc": "? Name from Getman+ (2002, J/ApJ/575/354) "}, {"name": "---", "desc": "[MBO] "}, {"name": "MBO", "desc": "? Name from Wilking+ (2004, J/AJ/127/1131) "}, {"name": "---", "desc": "<[GMM2008] NNN> in Simbad "}, {"name": "[GMM2008]", "desc": "? Name from Gutermuth+ (2008, J/ApJ/674/336) "}, {"name": "---", "desc": "<[OTS2008]> in Simbad "}, {"name": "[OTS2008]", "desc": "Name(s) from Oasa+ (2008, J/AJ/136/1372) "}, {"name": "---", "desc": "<[EDJ2009] NNN> in Simbad "}, {"name": "[EDJ2009]", "desc": "? Name from Evans+ (2009, J/ApJS/181/321) "}, {"name": "S09", "desc": "Name from Scholz+ (2009ApJ...702..805S) "}, {"name": "---", "desc": "<[WMW2010] NNN> in Simbad "}, {"name": "[WMW2010]", "desc": "? Name from Winston+ (2010, J/AJ/140/266) "}, {"name": "---", "desc": "[SSTYSV] "}, {"name": "SSTYSV", "desc": "Name from Rebull+ (2015, J/AJ/150/175) "}, {"name": "ONames", "desc": "Other source names "}, {"name": "SpT", "desc": "MK spectral type(s) "}, {"name": "r_SpT", "desc": "Spectral type reference (1) "}, {"name": "Spph", "desc": "Spectrograph for spectral classification (G2) "}, {"name": "Date", "desc": "Date of spectroscopy "}, {"name": "ASpT", "desc": "Adopted spectral type "}, {"name": "Aj", "desc": "[0/14]? Extinction in J band "}, {"name": "IRexc", "desc": "IR excess? (2) "}, {"name": "MmEv", "desc": "Membership evidence (3) "}, {"name": "pmRA", "desc": "[-8.9/8.4]? Proper motion in right ascension "}, {"name": "e_pmRA", "desc": "[0/6.8]? Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-7.8/3.4]? Proper motion in declination "}, {"name": "e_pmDE", "desc": "[0/7.4]? Uncertainty in pmDE "}, {"name": "Jmag", "desc": "[8.1/20.8]? J magnitude "}, {"name": "e_Jmag", "desc": "[0.02/0.2]? Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[7.7/19.1]? H magnitude "}, {"name": "e_Hmag", "desc": "[0.02/0.08]? Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[7.1/18.2]? Ks magnitude "}, {"name": "e_Ksmag", "desc": "[0.02/0.2]? Uncertainty in Ksmag "}, {"name": "Ref", "desc": "JHK reference (G3) "}]}, {"name": "table3.dat", "desc": "Field stars in spectroscopic samples for IC 348 and NGC 1333", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[28/45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31/32] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Flag", "desc": "[y] Proper Motion Flag (1) "}, {"name": "SpT", "desc": "MK Spectral Type(s) "}, {"name": "r_SpT", "desc": "Spectral type reference(s) (2) "}, {"name": "Inst", "desc": "Telescope/Instrument "}, {"name": "Date", "desc": "Date of spectroscopy "}]}, {"name": "table4.dat", "desc": "Candidate members of IC 348 ", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[43/45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31/32] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "L98", "desc": "[596/54532] Name based on Luhman+ (1998ApJ...508..347L) running IDs; in Simbad"}, {"name": "Select", "desc": "Basis of Selection (1) "}, {"name": "Jmag", "desc": "[18.4/20.8]? WIRCam J magnitude, this work "}, {"name": "e_Jmag", "desc": "[0.03/0.07]? Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[16.4/19.8] WIRCam H magnitude, this work "}, {"name": "e_Hmag", "desc": "[0.03/0.1] Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[14.8/18.5] WIRCam Ks magnitude, this work "}, {"name": "e_Ksmag", "desc": "[0.03/0.04] Uncertainty in Ksmag "}]}, {"name": "table5.dat", "desc": "Candidate Members of NGC 1333 ", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[28/29] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[12/29] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "S74", "desc": "Name from Strom+ (1974ApJ...191..111S) "}, {"name": "---", "desc": "[ASR] "}, {"name": "ASR", "desc": "? Name from Aspin+ (1994, J/A+AS/106/165) "}, {"name": "---", "desc": "<[LAL96] NNN> in Simbad "}, {"name": "[LAL96]", "desc": "? Name from Lada+ (1996, J/AJ/111/1964) "}, {"name": "---", "desc": "[MBO] "}, {"name": "MBO", "desc": "? Name from Wilking+ (2004, J/AJ/127/1131) "}, {"name": "---", "desc": "<[GMM2008] NNN> in Simbad "}, {"name": "[GMM2008]", "desc": "? Name from Gutermuth+ (2008, J/ApJ/674/336) "}, {"name": "---", "desc": "<[OTS2008] NNN> in Simbad "}, {"name": "[OTS2008]", "desc": "? Name from Oasa+ (2008, J/AJ/136/1372) "}, {"name": "---", "desc": "<[EDJ2009] NNN> in Simbad "}, {"name": "[EDJ2009]", "desc": "? Name from Evans+ (2009, J/ApJS/181/321) "}, {"name": "---", "desc": "<[WMW2010] NNN> in Simbad "}, {"name": "[WMW2010]", "desc": "? Name from Winston+ (2010, J/AJ/140/266) "}, {"name": "---", "desc": "[SSTYSV] "}, {"name": "SSTYSV", "desc": "Name from Rebull+ (2015, J/AJ/150/175) "}, {"name": "Select", "desc": "Basis of selection (1) "}, {"name": "Jmag", "desc": "[11.2/21.6]? J magnitude "}, {"name": "e_Jmag", "desc": "[0.02/0.2]? Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[10.1/19.7]? H magnitude "}, {"name": "e_Hmag", "desc": "[0.03/0.2]? Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[9.5/19] Ks magnitude "}, {"name": "e_Ksmag", "desc": "[0.02/0.04] Uncertainty in Ksmag "}, {"name": "Ref", "desc": "JHK reference (G3) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_829_89"}} {"id": "J/ApJ/829/89", "title_cds": "Short Title", "title_create": "Barnes+, 2016", "year": "2016", "author": "Barnes G., Leka K.D., Schrijver C.J., Colak T., Qahwaji R., Ashamari O.W., Yuan Y., Zhang J., McAteer R.T.J., Bloomfield D.S., Higgins P.A., Gallagher P.T., Falconer D.A., Georgoulis M.K., Wheatland M.S., Balch C., Dunn T., Wagner E.L.", "title_pub": "A comparison of flare forecasting methods. I. Results from the \"all-clear\" workshop.", "first_author": "Barnes G.", "ref_biblio": [""], "bibcode": ["2016ApJ...829...89B"], "keyword_cds": "", "keyword_pub": "methods: statistical; Sun: flares; Sun: magnetic fields", "abstract": ["Solar flares produce radiation that can have an almost immediate", "effect on the near-Earth environment, making it crucial to forecast", "flares in order to mitigate their negative effects. The number of", "published approaches to flare forecasting using photospheric magnetic", "field observations has proliferated, with varying claims about how", "well each works. Because of the different analysis techniques and data", "sets used, it is essentially impossible to compare the results from", "the literature. This problem is exacerbated by the low event rates of", "large solar flares. The challenges of forecasting rare events have", "long been recognized in the meteorology community, but have yet to be", "fully acknowledged by the space weather community. During the", "interagency workshop on \"all clear\" forecasts held in Boulder, CO in", "2009, the performance of a number of existing algorithms was compared", "on common data sets, specifically line-of-sight magnetic field and", "continuum intensity images from the Michelson Doppler Imager, with", "consistent definitions of what constitutes an event. We demonstrate", "the importance of making such systematic comparisons, and of using", "standard verification statistics to determine what constitutes a good", "prediction scheme. When a comparison was made in this fashion, no one", "method clearly outperformed all others, which may in part be due to", "the strong correlations among the parameters used by different methods", "to characterize an active region. For M-class flares and above, the", "set of methods tends toward a weakly positive skill score (as measured", "with several distinct metrics), with no participating method proving", "substantially better than climatological forecasts."], "doi_pub": ["10.3847/0004-637X/829/2/89"], "orcid_pub": ["0000-0003-3571-8728"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "27769.dat", "desc": "Forecasts for events with at least one C1.0 or greater flare within 24hr after the observation", "columns": [{"name": "ID", "desc": "Identifier of the data source: date, time, number of active regions and active region number"}, {"name": "Event", "desc": "yes=1, no=0 "}, {"name": "MCD1", "desc": "Part of Maximum Common Dataset #1: yes=1,no=0 "}, {"name": "MCD2", "desc": "Part of Maximum Common Dataset #2: yes=1,no=0 "}, {"name": "Beff", "desc": "Forecast probability for B_eff "}, {"name": "ASAP", "desc": "Forecast probability for ASAP "}, {"name": "BBSO", "desc": "Forecast probability for BBSO "}, {"name": "WLSG2", "desc": "? Forecast probability for WL_SG2 (blank value when NaN)"}, {"name": "NWRAMAG", "desc": "Forecast probability for NWRA MAG 2-var "}, {"name": "log(R)", "desc": "Forecast probability for log(R) "}, {"name": "GCD", "desc": "Forecast probability for GCD "}, {"name": "NWRAMCT", "desc": "Forecast probability for NWRA MCT 2-var "}, {"name": "SMART2", "desc": "Forecast probability for SMART2 "}, {"name": "EventS", "desc": "Forecast probability for Event Statistics, 10 prior"}, {"name": "McIntosh", "desc": "? Forecast probability for McIntosh (blank value when NaN)"}]}, {"name": "27825.dat", "desc": "Forecasts for events with at least one M1.0 or greater flare within 12hr after the observation", "columns": [{"name": "ID", "desc": "Identifier of the data source: date, time, number of active regions and active region number"}, {"name": "Event", "desc": "yes=1, no=0 "}, {"name": "MCD1", "desc": "Part of Maximum Common Dataset #1: yes=1,no=0 "}, {"name": "MCD2", "desc": "Part of Maximum Common Dataset #2: yes=1,no=0 "}, {"name": "Beff", "desc": "Forecast probability for B_eff "}, {"name": "ASAP", "desc": "Forecast probability for ASAP "}, {"name": "BBSO", "desc": "Forecast probability for BBSO "}, {"name": "WLSG2", "desc": "? Forecast probability for WL_SG2 (blank value when NaN)"}, {"name": "NWRAMAG", "desc": "Forecast probability for NWRA MAG 2-var "}, {"name": "log(R)", "desc": "Forecast probability for log(R) "}, {"name": "GCD", "desc": "Forecast probability for GCD "}, {"name": "NWRAMCT", "desc": "Forecast probability for NWRA MCT 2-var "}, {"name": "SMART2", "desc": "Forecast probability for SMART2 "}, {"name": "EventS", "desc": "Forecast probability for Event Statistics, 10 prior"}, {"name": "McIntosh", "desc": "? Forecast probability for McIntosh (blank value when NaN)"}]}, {"name": "27847.dat", "desc": "Forecasts for events with at least one M5.0 or greater flare within 12hr after the observation", "columns": [{"name": "ID", "desc": "Identifier of the data source: date, time, number of active regions and active region number"}, {"name": "Event", "desc": "yes=1, no=0 "}, {"name": "MCD1", "desc": "Part of Maximum Common Dataset #1: yes=1,no=0 "}, {"name": "MCD2", "desc": "Part of Maximum Common Dataset #2: yes=1,no=0 "}, {"name": "Beff", "desc": "Forecast probability for B_eff "}, {"name": "ASAP", "desc": "Forecast probability for ASAP "}, {"name": "BBSO", "desc": "Forecast probability for BBSO "}, {"name": "WLSG2", "desc": "? Forecast probability for WL_SG2 (blank value when NaN)"}, {"name": "NWRAMAG", "desc": "Forecast probability for NWRA MAG 2-var "}, {"name": "log(R)", "desc": "Forecast probability for log(R) "}, {"name": "GCD", "desc": "Forecast probability for GCD "}, {"name": "NWRAMCT", "desc": "Forecast probability for NWRA MCT 2-var "}, {"name": "SMART2", "desc": "Forecast probability for SMART2 "}, {"name": "EventS", "desc": "Forecast probability for Event Statistics, 10 prior"}, {"name": "McIntosh", "desc": "? Forecast probability for McIntosh (blank value when NaN)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_833_58"}} {"id": "J/ApJ/833/58", "title_cds": "Short Title", "title_create": "Hodges-Kluck+, 2016", "year": "2016", "author": "Hodges-Kluck E., Cafmeyer J., Bregman J.N.", "title_pub": "Ultraviolet halos around spiral galaxies. I. Morphology.", "first_author": "Hodges-Kluck E.", "ref_biblio": [""], "bibcode": ["2016ApJ...833...58H"], "keyword_cds": "", "keyword_pub": "dust, extinction; galaxies: halos; ultraviolet: galaxies", "abstract": ["We examine ultraviolet halos around a sample of highly inclined", "galaxies within 25 Mpc to measure their morphology and luminosity.", "Despite contamination from galactic light scattered into the wings of", "the point-spread function, we find that ultraviolet (UV) halos occur", "around each galaxy in our sample. Around most galaxies the halos form", "a thick, diffuse disk-like structure, but starburst galaxies with", "galactic superwinds have qualitatively different halos that are more", "extensive and have filamentary structure. The spatial coincidence of", "the UV halos above star-forming regions, the lack of consistent", "association with outflows or extraplanar ionized gas, and the strong", "correlation between the halo and galaxy UV luminosity suggest that the", "UV light is an extragalactic reflection nebula. UV halos may thus", "represent 10^6^-10^7^M_{sun}_ of dust within 2-10kpc of the disk,", "whose properties may change with height in starburst galaxies."], "doi_pub": ["10.3847/1538-4357/833/1/58"], "orcid_pub": ["0000-0002-2397-206X"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table9.dat", "desc": "Swift Mrk 501 observations ", "columns": [{"name": "uvm2", "desc": "Swift/UVOT uvm2 band observation identifier "}, {"name": "uvw1", "desc": "Swift/UVOT uvw1 band observation identifier "}, {"name": "uvw2", "desc": "Swift/UVOT uvw2 band observation identifier "}]}, {"name": "table10.dat", "desc": "All Swift and GALEX observations ", "columns": [{"name": "Name", "desc": "Galaxy identifier "}, {"name": "FUV", "desc": "GALEX/FUV observation identifier "}, {"name": "NUV", "desc": "GALEX/NUV observation identifier "}, {"name": "uvm2", "desc": "Swift/UVOT uvm2 band observation identifier "}, {"name": "uvw1", "desc": "Swift/UVOT uvw1 band observation identifier "}, {"name": "uvw2", "desc": "Swift/UVOT uvw2 band observation identifier "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_839_20"}} {"id": "J/ApJ/839/20", "title_cds": "Spectroscopy of stars along the LoS of Crater2", "title_create": "Caldwell+, 2017", "year": "2017", "author": "Caldwell N., Walker M.G., Mateo M., Olszewski E.W., Koposov S., Belokurov V., Torrealba G., Geringer-sameth A., Johnson C.I.", "title_pub": "Crater 2: an extremely cold dark matter halo.", "first_author": "Caldwell N.", "ref_biblio": [""], "bibcode": ["2017ApJ...839...20C"], "see_also": ["J/A+A/459/423 : VI and [Fe/H] of Fornax dSph RGB stars (Battaglia+, 2006)", "J/MNRAS/380/281 : Faint galactic satellites spectrosc. survey (Martin+, 2007)", "J/AJ/136/2050 : SEGUE stellar parameter pipeline. II. (Lee+, 2008)", "J/ApJ/675/201 : Radial velocities of stars near Leo I (Mateo+, 2008)", "J/MNRAS/397/1748 : Spectroscopic study of Segue 2 (Belokurov+, 2009)", "J/AJ/137/94 : Star clusters in M31 (Caldwell+, 2009)", "J/AJ/137/3100 : Radial velocities of 4 dSph galaxies (Walker+, 2009)", "J/ApJ/694/L144 : Spectroscopic study of Leo V dSph (Walker+, 2009)", "J/ApJS/191/352 : Abundances in stars of MW dwarf satellites (Kirby+, 2010)", "J/ApJ/736/146 : Radial velocities of stars in Bootes I (Koposov+, 2011)", "J/ApJ/733/46 : Velocity measurements in Segue 1 (Simon+, 2011)", "J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)", "J/ApJ/768/172 : Kinematic analysis of red giant in M31 dSphs (Collins+, 2013)", "J/ApJ/779/102 : Metallicities of RGB stars in dwarf galaxies (Kirby+, 2013)", "J/ApJ/801/74 : Dark matter profiles in dwarf gal. (Geringer-Sameth+, 2015)", "J/MNRAS/448/2717 : Bayesian analysis of resolved stellar spectra", "J/MNRAS/453/690 : Fornax VST ATLAS catalogue (Bate+, 2015)", "J/MNRAS/469/621 : VST ATLAS white dwarf candidates (Gentile Fusillo+, 2017)", "http://astro.dur.ac.uk/Cosmology/vstatlas/ : VST ATLAS survey home page"], "keyword_cds": "Stars, giant ; Photometry, SDSS ; Abundances, [Fe/H]", "keyword_pub": "galaxies: dwarf; galaxies: individual (Crater 2); galaxies: kinematics and dynamics; Local Group; methods: data analysis techniques: spectroscopic", "abstract": ["We present results from MMT/Hectochelle spectroscopy of 390 red giant", "candidate stars along the line of sight to the recently discovered", "Galactic satellite Crater 2. Modeling the joint distribution of", "stellar positions, velocities, and metallicities as a mixture of", "Crater 2 and Galactic foreground populations, we identify ~62 members", "of Crater 2, for which we resolve a line-of-sight velocity dispersion", "of {sigma}_Vlos_=2.7_-0.3_^+0.3^km/s and a mean velocity of", "=87.5_-0.4_^+0.4^km/s (solar rest frame). We also resolve a", "metallicity dispersion of {sigma}_[Fe/H]_=0.22_-0.03_^+0.04^dex and a", "mean of <[Fe/H]>=-1.98_-0.1_^+0.1^dex that is 0.28+/-0.14dex poorer", "than estimated from photometry. Despite Crater 2's relatively large", "size (projected halflight radius R_h_~1kpc) and intermediate", "luminosity (M_V_~-8), its velocity dispersion is the coldest that has", "been resolved for any dwarf galaxy. These properties make Crater 2 the", "most extreme low-density outlier in dynamical as well as structural", "scaling relations among the Milky Way's dwarf spheroidals. Even so,", "under assumptions of dynamical equilibrium and negligible", "contamination by unresolved binary stars, the observed velocity", "distribution implies a gravitationally dominant dark matter halo, with", "a dynamical mass of 4.4_-0.9_^+1.2^x10^6^M_{sun}_ and a mass-to-light", "ratio of 53_-11_^+15^M_{sun}_/L_V,{sun}_ enclosed within a radius of", "~1kpc, where the equivalent circular velocity is 4.3_-0.5_^+0.5^ km/s."], "description": ["We observed Crater 2 using the Hectochelle multi-object fiber", "spectrograph on the 6.5m MMT on Mt. Hopkins, Arizona.", "On the nights of 2016 April 27 and 30 and May 11, we used", "Hectochelle's \"RV31\" filter to observe the spectral range of", "5150-5300{AA}. The effective resolution is R~32000.", "We selected red giant branch (RGB) candidates from the photometric", "catalog provided by the VLT Survey Telescope (VST) ATLAS survey", "(Shanks+ 2015MNRAS.451.4238S)."], "object": ["11 49 14 -18 24.8 Crater 2 = NAME Crater 2 (=87.5km/s)"], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aa688e"], "orcid_pub": ["0000-0003-2352-3202"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Hectochelle Stellar Spectroscopy of Crater 2 ", "columns": [{"name": "ID", "desc": "Object identifier (Cra2-NNN) "}, {"name": "RAh", "desc": "[11] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[46/55] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[17/18] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "gmag", "desc": "[17/20.3] The g band magnitude from the VST-ATLAS catalog (SDSS AB system??)"}, {"name": "imag", "desc": "[16/20.1] The i band magnitude from the VST-ATLAS catalog (SDSS AB system??)"}, {"name": "HJD", "desc": "Heliocentric Julian Date; JD-2450000 "}, {"name": "S/N", "desc": "[0.2/18.1] Median signal-to-Noise per pixel "}, {"name": "Vlos", "desc": "[-73/370] Heliocentric rest frame line-of-sight velocity"}, {"name": "e_Vlos", "desc": "[0.3/4] Uncertainty in vlos "}, {"name": "Teff", "desc": "[4428/7309] Effective temperature "}, {"name": "e_Teff", "desc": "[25/1085] Uncertainty in Teff "}, {"name": "log(g)", "desc": "[1/6] Log surface gravity "}, {"name": "e_log(g)", "desc": "[0.06/1.4] Uncertainty in log(g) "}, {"name": "[Fe/H]", "desc": "[-3.2/1.4] Metallicity "}, {"name": "e_[Fe/H]", "desc": "[0.04/1.1] Uncertainty in [Fe/H] "}]}, {"name": "spectra.dat", "desc": "Summary of individual spectroscopic targets; table added by CDS", "columns": [{"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "FileName", "desc": "Name of the FITS file in subdirectory spectra "}]}, {"name": "spectra/*", "desc": "Individual fits files for all individual spectroscopic targets (and \"README\" file)", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_839_6"}} {"id": "J/ApJ/839/6", "title_cds": "NGC 6946 giant molecular cloud in ^12^CO (2-1)", "title_create": "Wu+, 2017", "year": "2017", "author": "Wu Y.-L., Sakamoto K., Pan H.-A.", "title_pub": "Submillimeter Array ^12^CO (2-1) imaging of the NGC 6946 giant molecular clouds.", "first_author": "Wu Y.-L.", "ref_biblio": [""], "bibcode": ["2017ApJ...839....6W"], "see_also": ["J/ApJ/551/852 : FCRAO CO survey of the outer Galaxy (Heyer+, 2001)", "J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)", "J/ApJ/661/830 : Giant molecular clouds of M33 (Rosolowsky+, 2007)", "J/ApJ/669/525 : VRI photometric standards for NGC 6946 (Welch+, 2007)", "J/ApJ/686/948 : CO in extragalactic giant molecular clouds (Bolatto+, 2008)", "J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008)", "J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008)", "J/ApJS/177/465 : X-ray variability in NGC 6946, NGC4485/90 (Fridriksson+, 2008)", "J/ApJ/699/1092 : Giant molecular clouds (SRBY) (Heyer+, 2009)", "J/ApJS/197/16 : CO observations of LMC molecular clouds (MAGMA). (Wong+, 2011)", "J/A+A/542/A108 : Giant molecular clouds in M33 (Gratier+, 2012)", "J/A+A/545/A43 : HII regions in NGC 628 and NGC 6946 (Cedres+, 2012)", "J/A+A/552/A19 : Radio-farIR correlation in NGC 6946 (Tabatabaei+, 2013)", "J/ApJ/772/107 : GMCs in nearby galaxies (Donovan Meyer+, 2013)", "J/ApJ/784/3 : The PAWS catalogs of GMCs and islands in M51 (Colombo+, 2014)", "J/ApJ/803/16 : GMCs in NGC4526 based on ^12^CO (Utomo+, 2015)"], "keyword_cds": "Molecular clouds ; Interstellar medium ; Millimetric/submm sources", "keyword_pub": "galaxies: individual (NGC 6946); galaxies: ISM; galaxies: spiral; ISM: clouds", "abstract": ["We present a ^12^CO (2-1) mosaic map of the spiral galaxy NGC 6946 by", "combining data from the Submillimeter Array and the IRAM 30m", "telescope. We identify 390 giant molecular clouds (GMCs) from the", "nucleus to 4.5kpc in the disk. GMCs in the inner 1kpc are generally", "more luminous and turbulent, some of which have luminosities", ">10^6^K.km/s.pc^2^ and velocity dispersions >10km/s. Large-scale", "bar-driven dynamics likely regulate GMC properties in the nuclear", "region. Similar to the Milky Way and other disk galaxies, GMC mass", "function of NGC 6946 has a shallower slope (index > -2) in the inner", "region, and a steeper slope (index < -2) in the outer region. This", "difference in mass spectra may be indicative of different cloud", "formation pathways: gravitational instabilities might play a major", "role in the nuclear region, while cloud coalescence might be dominant", "in the outer disk. Finally, the NGC 6946 clouds are similar to those", "in M33 in terms of statistical properties, but they are generally less", "luminous and turbulent than the M51 clouds."], "description": ["We performed a 10-pointing ^12^CO(2-1) mosaic of NGC 6946 between 2010", "June and October in the compact (CMP) and extended (EXT) array", "configurations of the Submillimeter Array (SMA), with baselines", "ranging from 6 to 180m. We also acquired complementary data with the", "sub-compact configuration (SUB) in 2012.", "We also use the IRAM 30m ^12^CO(2-1) cube of NGC 6946 presented by", "Leroy+ (2009AJ....137.4670L)."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aa68de"], "orcid_pub": ["0000-0002-4392-1446"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table3.dat", "desc": "NGC 6946 giant molecular cloud catalog ", "columns": [{"name": "Seq", "desc": "Cloud ID "}, {"name": "oRA", "desc": "Right Ascension offset w.r.t. the galactic center (1)"}, {"name": "oDE", "desc": "Declination offset w.r.t. the galactic center (1)"}, {"name": "Velc", "desc": "[-48/174] Central velocity of the cloud "}, {"name": "Rad", "desc": "[13/213] Cloud radius "}, {"name": "e_Rad", "desc": "[6/154] Uncertainty in cloud radius "}, {"name": "sigv", "desc": "[0.5/42.5] Velocity dispersion "}, {"name": "e_sigv", "desc": "[0.5/55] Uncertainty in sigv "}, {"name": "Lum", "desc": "[1.6/702] Luminosity "}, {"name": "e_Lum", "desc": "[0.7/1912] Uncertainty in luminosity "}, {"name": "Mlum", "desc": "[0.2/40.2] Luminosity mass (2) "}, {"name": "e_Mlum", "desc": "[0.1/110] Uncertainty in luminosity mass "}, {"name": "Mvir", "desc": "[0.1/1517] Virial mass "}, {"name": "e_Mvir", "desc": "[0.3/1684] Uncertainty in virial mass "}, {"name": "T", "desc": "[1.7/18.1] Peak temperature "}, {"name": "S/N", "desc": "[5/55] Signal-to-noise ratio "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_847_20"}} {"id": "J/ApJ/847/20", "title_cds": "GMOS spectrosc. obs. of 0.3"], "bibcode": ["2017ApJ...847...20W"], "see_also": ["J/ApJS/94/687 : Old stellar populations. V. (Worthey+, 1994)", "J/MNRAS/276/1341 : Spectroscopy of E and S0 galaxies (Jorgensen+, 1995)", "J/ApJS/111/377 : H{gamma} & H{delta} absorption features (Worthey+ 1997)", "J/A+A/432/381 : VLT spectroscopic survey of RX J0152.7-1357 (Demarco+, 2005)", "J/ApJ/621/673 : Line indices for 124 early-type galaxies (Thomas+, 2005)", "J/ApJ/633/174 : Spheroidals and bulge dominated galaxies (Treu+, 2005)", "J/AJ/131/1288 : Composite spectra of early-type galaxies (Bernardi+, 2006)", "J/MNRAS/382/109 : Massive galaxies in Extended Groth Strip (Trujillo+, 2007)", "J/ApJS/184/271 : Photometry of galaxies in 3 clusters (Chiboucas+, 2009)", "J/ApJ/725/1252 : Confirmed members of RX J0152.7-1357 (Demarco+, 2010)", "J/A+A/524/A6 : Evolution of spectral early-type galaxies (Saglia+, 2010)", "J/AJ/145/77 : Imaging & spectrosc. in 3 galaxy clusters (Jorgensen+, 2013)", "J/ApJ/788/72 : Observed sample of z~0.7 massive galaxies (Gallazzi+, 2014)", "J/AJ/148/117 : Imaging and spectroscopy in Lynx W (Jorgensen+, 2014)", "J/A+A/597/A122 : Cluster & field elliptical gal. at z~1.3 (Saracco+, 2017)"], "keyword_cds": "Galaxies, spectra ; Redshifts ; Velocity dispersion ; Optical ; Equivalent widths", "keyword_pub": "galaxies: evolution ; galaxies: stellar content", "abstract": ["We analyze the stellar populations and evolutionary history of", "bulge-dominated field galaxies at redshifts 0.3"], "bibcode": ["2017ApJ...850...89G"], "see_also": ["B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)", "J/MNRAS/372/1315 : UBVRI photometry of SN 2004et (Sahu+, 2006)", "J/MNRAS/394/2266 : SN 2005cs one-year photometry (Pastorello+, 2009)", "J/MNRAS/395/1409 : Type II-P SN progenitor constraints (Smartt+, 2009)", "J/ApJ/708/661 : SDSS-II SN Survey: SN.II-P standardization (D'Andrea+, 2010)", "J/AJ/139/519 : Carnegie supernova project. SNe Ia (Contreras+, 2010)", "J/AJ/139/120 : Low-redshift Type-Ia supernovae (Folatelli+, 2010)", "J/AJ/142/156 : The CSP (DR2): photometry of SNe Ia (Stritzinger+, 2011)", "J/MNRAS/433/1871 : UBVRI griz light curves of SN 2012aw (Bose+, 2013)", "J/ApJ/773/53 : Type Ia SNe spectroscopy by the CSP (Folatelli+, 2013)", "J/ApJ/763/42 : X-ray emission from 28 SNe (IIn, Ibn, SLSN-I) (Ofek+, 2013)", "J/A+A/555/A142 : Spectra of 5 Type II supernovae (Inserra+, 2013)", "J/A+A/559/A114 : Updated O3N2 and N2 abundance indicators (Marino+, 2013)", "J/A+A/555/A10 : Light curves of 5 type IIn supernovae (Taddia+, 2013)", "J/MNRAS/442/844 : BVRI light curves of type II-P supernovae (Faran+, 2014)", "J/MNRAS/438/L101 : First month on SN 2013ej (Valenti+, 2014)", "J/ApJ/788/154 : Palomar Transient Factory SNe IIn photometry (Ofek+, 2014)", "J/ApJ/789/104 : SNe IIn observations and properties (Ofek+, 2014)", "J/ApJ/799/208 : Type IIP supernovae from Pan-STARRS1 (Sanders+, 2015)", "J/ApJ/799/215 : 26 type II-Plateau supernovae parameters (Pejcha+, 2015)", "J/ApJ/807/169 : SN IIn catalog with Fermi LAT (Ackermann+, 2015)", "J/ApJ/827/90 : Spectroscopy of SNe Ib, IIb and Ic (Liu+, 2016)", "J/A+A/587/L7 : Metallicity from Type II SN from (i)PTF (Taddia+, 2016)", "J/A+A/589/A110 : SN II in host HII regions (Anderson+, 2016)", "J/AJ/151/33 : UBVRIz LCs of 51 Type II supernovae (Galbany+, 2016)", "J/MNRAS/459/3939 : Type II supernova light curves (Valenti+, 2016)", "J/ApJ/835/166 : SNe type II from CSP-I, SDSS-II, and SNLS (de Jaeger+, 2017)", "J/ApJS/233/6 : SNe II light curves + spectra from the CfA (Hicken+, 2017)", "J/A+A/611/A25 : Updated Type II supernova Hubble diagram (Gall+, 2018)", "http://csp.obs.carnegiescience.edu/ : The Carnegie Supernova Project home", "http://sngroup.oapd.inaf.it/ : Padova-Asiago Supernova Group"], "keyword_cds": "Supernovae; Radial velocities; Spectra, optical", "keyword_pub": "supernovae: general ; surveys ; techniques: photometric ; techniques: spectroscopic", "abstract": ["We present 888 visual-wavelength spectra of 122 nearby type II", "supernovae (SNe II) obtained between 1986 and 2009, and ranging", "between 3 and 363 days post-explosion. In this first paper, we outline", "our observations and data reduction techniques, together with a", "characterization based on the spectral diversity of SNe II. A", "statistical analysis of the spectral matching technique is discussed", "as an alternative to nondetection constraints for estimating SN", "explosion epochs. The time evolution of spectral lines is presented", "and analyzed in terms of how this differs for SNe of different", "photometric, spectral, and environmental properties: velocities,", "pseudo-equivalent widths, decline rates, magnitudes, time durations,", "and environment metallicity. Our sample displays a large range in", "ejecta expansion velocities, from ~9600 to ~1500km/s at 50 days", "post-explosion with a median H_{alpha}_ value of 7300km/s. This is", "most likely explained through differing explosion energies.", "Significant diversity is also observed in the absolute strength of", "spectral lines, characterized through their pseudo-equivalent widths.", "This implies significant diversity in both temperature evolution", "(linked to progenitor radius) and progenitor metallicity between", "different SNe II. Around 60% of our sample shows an extra absorption", "component on the blue side of the H_{alpha}_ P-Cygni profile", "(\"Cachito\" feature) between 7 and 120 days since explosion. Studying", "the nature of Cachito, we conclude that these features at early times", "(before ~35 days) are associated with SiII{lambda}6355, while past the", "middle of the plateau phase they are related to high velocity (HV)", "features of hydrogen lines."], "description": ["The data presented here were obtained with a large variety of", "instruments and telescopes, as shown in Table 6.", "The majority of our spectra cover the range of ~3800 to ~9500{AA}. The", "observations were performed with the Cassegrain spectrographs at 1.5m", "and 4.0m telescopes at Cerro Tololo, with the Wide Field CCD Camera", "(WFCCD) at the 2.5m du Pont Telescope, the Low Dispersion Survey", "Spectrograph (LDSS2) on the Magellan Clay 6.5m telescope and the", "Inamori Magellan Areal Camera and Spectrograph (IMACS) on the Magellan", "Baade 6.5m telescope at Las Campanas Observatory. At La Silla, the", "observations were carried out with the ESO Multi-Mode Instrument", "(EMMI) in medium resolution spectroscopy mode (at the NTT) and the ESO", "Faint Object Spectrograph and Camera (EFOSC) at the NTT and 3.6m", "telescopes. We also have three spectra for SN 2006ee obtained with the", "Boller & Chivens CCD spectrograph at the Hiltner 2.4m Telescope of the", "MDM Observatory.", "A total of 888 spectra obtained between 1986 and 2009 and ranging", "between 3 and 363 days post-explosion have been analyzed."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aa8f52"], "orcid_pub": ["0000-0002-7252-4351"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "SN II sample ", "columns": [{"name": "SN", "desc": "Supernova identifier "}, {"name": "Host", "desc": "Host galaxy identifier "}, {"name": "HRV", "desc": "[227/23100] Galaxy heliocentric recession velocity (1)"}, {"name": "f_SN", "desc": "[1/3]? Source flags (2) "}, {"name": "Type", "desc": "Host galaxy morphological Hubble types (1) "}, {"name": "E(B-V)", "desc": "[0.01/0.6] Schlafly & Finkbeiner (2011ApJ...737..103S) reddening due to dust"}]}, {"name": "table6.dat", "desc": "Spectroscopic observations information ", "columns": [{"name": "---", "desc": "[SN] "}, {"name": "SN", "desc": "Supernova identifier "}, {"name": "UTDate", "desc": "UT date of the observation, YYYY-MM-DD "}, {"name": "JD", "desc": "Julian date of observation "}, {"name": "Phase", "desc": "[3/363] Phase, in days, since explosion "}, {"name": "Tel", "desc": "Telescope code (1) "}, {"name": "Inst", "desc": "Instrument code (2) "}, {"name": "Wmin", "desc": "[2903/10603] Min Wavelength range covered, in angstroms"}, {"name": "Wmax", "desc": "[4988/26935] Max Wavelength range covered, in angstroms"}, {"name": "Res", "desc": "[0.5/39]? Spectral resolution, angstroms, from arc-lamp lines"}, {"name": "Exp", "desc": "Total exposure time, (sequence x) seconds "}, {"name": "Airmass", "desc": "[1/5.6]? Airmass at the middle of the observation "}, {"name": "flag", "desc": "[cs] Spectrum flag (3) "}, {"name": "FileName", "desc": "Name of the FITS file in subdirectory Sp; column added by CDS"}]}, {"name": "table7.dat", "desc": "Explosion epoch estimations comparison ", "columns": [{"name": "SN", "desc": "Supernova identifier "}, {"name": "JD", "desc": "? Reduced Julian date of the spectrum used to match; JD-2400000 (1)"}, {"name": "SNID", "desc": "Best Match SN template identifier (2) "}, {"name": "dt-max", "desc": "[-7/101]? Days from maximum of the template used to match"}, {"name": "dt-exp", "desc": "[3/111]? Days from explosion of the template used to match"}, {"name": "dt-avg", "desc": "[4/93]? Average obtained from the days from explosion (1)"}, {"name": "MJD-exp1", "desc": "? Explosion date obtained with matching technique (1)"}, {"name": "e_MJD-exp1", "desc": "[3/17]? Uncertainty in MJD-exp1 "}, {"name": "MJD-nod", "desc": "? Non-detection date of the SN, Modified Julian Date (1)(3)"}, {"name": "MJD-dis", "desc": "? Discovery date of the SN, Modified Julian Date (1)(3)"}, {"name": "MJD-exp2", "desc": "? Explosion date obtained from MJD-nod and MJD-dis (1)(3)"}, {"name": "e_MJD-exp2", "desc": "[1/99]? Uncertainty in MJD-exp2 "}, {"name": "diff", "desc": "[-16/65]? Difference in MJD-exp1 and MJD-exp2 (1)(3)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_857_116"}} {"id": "J/ApJ/857/116", "title_cds": "Star cluster populations of nuclear ring galaxies", "title_create": "Ma+, 2018", "year": "2018", "author": "Ma C., de Grijs R., Ho L.C.", "title_pub": "Connections between star cluster populations and their host galaxy nuclear rings.", "first_author": "Ma C.", "ref_biblio": [""], "bibcode": ["2018ApJ...857..116M"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "J/AJ/118/2071 : ESO 565-11 UBVI(c) photometry (Buta+, 1999)", "J/AJ/121/3048 : Multicolor photometry in NGC 1512 and NGC 5248 (Maoz+, 2001)", "J/AJ/123/1411 : UBVIHalpha phot. of NGC 4314 star clusters (Benedict+, 2002)", "J/MNRAS/355/1251 : Bar-induced strengths in spiral gal. (Laurikainen+, 2004)", "J/AJ/127/1982 : HST UBVI photometry of NGC 3081 inner regions (Buta+, 2004)", "J/AJ/129/2138 : Centers of early-type galaxies with HST (Lauer+, 2005)", "J/ApJ/659/1176 : Study of bars in 180 spiral galaxies (Marinova+, 2007)", "J/ApJS/174/337 : Star formation in nuclear rings (Mazzuca+, 2008)", "J/ApJ/703/1672 : Far-IR and H{alpha} fluxes in galaxies (Kennicutt+, 2009)", "J/MNRAS/431/2917 : NGC5253 star clusters age and mass (de Grijs+, 2013)", "J/A+A/551/A81 : NGC 6951 intensity and velocity maps (van der Laan+, 2013)", "J/ApJS/216/6 : Opt-NIR HST photometry of cluster cand. in M82 (Li+, 2015)", "J/MNRAS/451/3173 : Circumnuclear star-forming regions (Alvarez-Alvarez+, 2015)", "J/MNRAS/465/2820 : NGC 6951 & NGC 1512 clusters HST photom. (de Grijs+, 2017)"], "keyword_cds": "Galaxies, IR; Photometry, HST; Photometry, infrared; Morphology; Clusters, globular; Photometry, UBVRI", "keyword_pub": "galaxies: evolution ; galaxies: individual (NGC 1512) ; galaxies: star clusters: general ; galaxies: star formation ; globular clusters: general", "abstract": ["Nuclear rings are excellent laboratories for probing diverse phenomena", "such as the formation and evolution of young massive star clusters and", "nuclear starbursts, as well as the secular evolution and dynamics of", "their host galaxies. We have compiled a sample of 17 galaxies with", "nuclear rings, which are well resolved by high-resolution Hubble and", "Spitzer Space Telescope imaging. For each nuclear ring, we identified", "the ring star cluster population, along with their physical properties", "(ages, masses, and extinction values). We also determined the", "integrated ring properties, including the average age, total stellar", "mass, and current star formation rate (SFR). We find that Sb-type", "galaxies tend to have the highest ring stellar mass fraction with", "respect to the host galaxy, and this parameter is correlated with the", "ring's SFR surface density. The ring SFRs are correlated with their", "stellar masses, which is reminiscent of the main sequence of", "star-forming galaxies. There are striking correlations between", "star-forming properties (i.e., SFR and SFR surface density) and", "nonaxisymmetric bar parameters, appearing to confirm previous", "inferences that strongly barred galaxies tend to have lower ring SFRs,", "although the ring star formation histories turn out to be", "significantly more complicated. Nuclear rings with higher stellar", "masses tend to be associated with lower cluster mass fractions, but", "there is no such relation for the ages of the rings. The two youngest", "nuclear rings in our sample, NGC 1512 and NGC 4314, which have the", "most extreme physical properties, represent the young extremity of the", "nuclear ring age distribution."], "description": ["From our initial sample of 108 galaxies (mainly from Comeron+", "2010MNRAS.402.2462C) exhibiting nuclear rings, we selected those that", "had been observed and resolved by any HST camera, including the Wide", "Field Camera 3, the Wide Field and Planetary Camera 2, the Advanced", "Camera for Surveys, the Near-Infrared Camera and Multi-Object", "Spectrometer, and the Faint Object Camera. The final sample consists", "of 17 galaxies, for which we have included the relevant information in", "Table 1.", "From the Spitzer Heritage Archive, we downloaded any available", "broadband infrared images (post-basic calibrated data, with a pixel", "scale of 0.6\") observed with the Spitzer/Infrared Array Camera."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aab6b4"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Observed filter sets and basic galactic parameters of our target galaxies", "columns": [{"name": "Galaxy", "desc": "Host galaxy name "}, {"name": "Type", "desc": "Hubble Type (1) "}, {"name": "DM", "desc": "[27.5/34.3] Distance Modulus (1) "}, {"name": "Filters", "desc": "Filters "}, {"name": "Qg", "desc": "[0.02/0.5]? non-axisymmetric bar parameter, Comeron et al. (2010MNRAS.402.2462C)"}]}, {"name": "table2.dat", "desc": "*Derived NGC 1512 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table3.dat", "desc": "Basic parameters of the ring star cluster populations ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name "}, {"name": "Nclus", "desc": "[27/1064] Number of clusters in the final selected ring cluster population"}, {"name": "f", "desc": "[0.1/1] Ratio, initial to final cluster population (1)"}, {"name": "", "desc": "[7/3020] Ring cluster surface density "}, {"name": "Lim", "desc": "Limiting master filter used for the cluster selection"}, {"name": "omagLim", "desc": "[20.4/24.1] Magnitude 90% completeness limit in filter Lim"}, {"name": "logAge", "desc": "[7.4/9] log Average age of the ring cluster sample"}, {"name": "logMass", "desc": "[4.4/7.2] log Average mass of the ring cluster sample"}, {"name": "logMtot", "desc": "[5.4/7.4] log Total mass of YMCs (2) "}]}, {"name": "table4.dat", "desc": "Integrated nuclear ring properties derived in this paper", "columns": [{"name": "Galaxy", "desc": "Host galaxy name "}, {"name": "logAge", "desc": "[7.5/9.8] Log of best-fitting age "}, {"name": "e_logAge", "desc": "[0.06/3.6] Lower uncertainty in logAge "}, {"name": "E_logAge", "desc": "[0.06/1.6] Upper uncertainty in logAge "}, {"name": "logMass", "desc": "[7.1/10] Log of total stellar mass "}, {"name": "e_logMass", "desc": "[0.06/0.4] Lower uncertainty in logAge "}, {"name": "E_logMass", "desc": "[0.05/0.2] Upper uncertainty in logAge "}, {"name": "SFR", "desc": "[0.04/2.4]? Current SFR for the past 10Myr"}, {"name": "e_SFR", "desc": "[0.006/0.4]? Uncertainty for SFR "}, {"name": "SFRD", "desc": "[0.02/0.8]? Surface density "}, {"name": "e_SFRD", "desc": "[0.005/0.1]? Uncertainty for SFRD "}]}, {"name": "table5.dat", "desc": "Multi-band photometry of the ESO 565-11 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/241] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F255W", "desc": "[17.4/26.6]?=100 Integrated apparent HST/WFPC2 F255W magnitude"}, {"name": "e_F255W", "desc": "[0.1/10]?=10 Uncertainty F255W "}, {"name": "F336W", "desc": "[17.8/28.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.07/6]?=10 Uncertainty in F336W "}, {"name": "F439W", "desc": "[17.9/27.2]?=100 Integrated apparent HST/WFPC2 F439W magnitude"}, {"name": "e_F439W", "desc": "[0.06/7.2]?=10 Uncertainty in F439W "}, {"name": "F555W", "desc": "[18.4/27]?=100 Integrated apparent HST/WFPC2 F555W magnitude"}, {"name": "e_F555W", "desc": "[0.04/2.3]?=10 Uncertainty in F555W "}, {"name": "F814W", "desc": "[18.6/30.4]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/10]?=10 Uncertainty in F814W "}]}, {"name": "table6.dat", "desc": "Derived ESO 565-11 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table7.dat", "desc": "Multi-band photometry of the IC 342 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/1063] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F275W", "desc": "[16.3/25.1]?=100 Integrated apparent HST/WFC3 F275W magnitude"}, {"name": "e_F275W", "desc": "[0.05/3]?=10 Uncertainty in F275W "}, {"name": "F336W", "desc": "[15.9/28.4]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.03/9]?=10 Uncertainty in F336W "}, {"name": "F438W", "desc": "[16/27.7]?=100 Integrated apparent HST/WFC3 F438W magnitude"}, {"name": "e_F438W", "desc": "[0.02/6]?=10 Uncertainty in F438W "}, {"name": "F547M", "desc": "[16.2/29.3]?=100 Integrated apparent HST/WFC3 F547M magnitude"}, {"name": "e_F547M", "desc": "[0.02/6.3]?=10 Uncertainty in F547M "}, {"name": "F814W", "desc": "[16.9/28.6]?=100 Integrated apparent HST/WFC3 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.01/10]?=10 Uncertainty in F814W "}]}, {"name": "table8.dat", "desc": "Derived IC 342 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table9.dat", "desc": "Multi-band photometry of the NGC 1097 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/1063] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F275W", "desc": "[16.3/25.1]?=100 Integrated apparent HST/WFC3 F275W magnitude"}, {"name": "e_F275W", "desc": "[0.05/3]?=10 Uncertainty in F275W "}, {"name": "F336W", "desc": "[15.9/28.4]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.03/9]?=10 Uncertainty in F336W "}, {"name": "F438W", "desc": "[16/27.7]?=100 Integrated apparent HST/WFC3 F438W magnitude"}, {"name": "e_F438W", "desc": "[0.02/6]?=10 Uncertainty in F438W "}, {"name": "F547M", "desc": "[16.2/29.3]?=100 Integrated apparent HST/WFC3 F547M magnitude"}, {"name": "e_F547M", "desc": "[0.02/6.3]?=10 Uncertainty in F547M "}, {"name": "F814W", "desc": "[16.9/28.6]?=100 Integrated apparent HST/WFC3 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.01/10]?=10 Uncertainty in F814W "}]}, {"name": "table10.dat", "desc": "Derived NGC 1097 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table11.dat", "desc": "Multi-band photometry of the NGC 1326 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/241] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F255W", "desc": "[17.4/26.6]?=100 Integrated apparent HST/WFPC2 F255W magnitude"}, {"name": "e_F255W", "desc": "[0.1/10]?=10 Uncertainty F255W "}, {"name": "F336W", "desc": "[17.8/28.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.07/6]?=10 Uncertainty in F336W "}, {"name": "F439W", "desc": "[17.9/27.2]?=100 Integrated apparent HST/WFPC2 F439W magnitude"}, {"name": "e_F439W", "desc": "[0.06/7.2]?=10 Uncertainty in F439W "}, {"name": "F555W", "desc": "[18.4/27]?=100 Integrated apparent HST/WFPC2 F555W magnitude"}, {"name": "e_F555W", "desc": "[0.04/2.3]?=10 Uncertainty in F555W "}, {"name": "F814W", "desc": "[18.6/30.4]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/10]?=10 Uncertainty in F814W "}]}, {"name": "table12.dat", "desc": "Derived NGC 1326 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table13.dat", "desc": "Multi-band photometry of the NGC 1672 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/301] ID number "}, {"name": "RAdeg", "desc": "[71.42/71.44] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[4] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[41.7/43.5] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-59.3/-59.2] Declination in decimal degrees (J2000)"}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[59] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[14] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[44/55] Arcsecond of Declination (J2000) "}, {"name": "F330W", "desc": "[16.4/30.3]?=100 Integrated apparent HST/ACS_HRC F330W magnitude"}, {"name": "e_F330W", "desc": "[0.04/5]?=10 Uncertainty in F330W "}, {"name": "F435W", "desc": "[16.9/26.4]?=100 Integrated apparent HST/ACS F435W magnitude"}, {"name": "e_F435W", "desc": "[0.03/5.5]?=10 Uncertainty in F435W "}, {"name": "F550M", "desc": "[17.32/24.8]?=100 Integrated apparent HST/ACS F550M magnitude"}, {"name": "e_F550M", "desc": "[0.04/5.6]?=10 Uncertainty in F550M "}, {"name": "F606W", "desc": "[17.4/25.7]?=100 Integrated apparent HST/ACS F606W magnitude"}, {"name": "e_F606W", "desc": "[0.02/10]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[17.8/26.5]?=100 Integrated apparent HST/ACS F814W magnitude"}, {"name": "e_F814W", "desc": "[0.03/3.6]?=10 Uncertainty in F814W "}]}, {"name": "table14.dat", "desc": "Derived NGC 1672 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table15.dat", "desc": "Multi-band photometry of the NGC 2997 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/250] ID number "}, {"name": "RAdeg", "desc": "[146.4/146.5] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[9] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[38/39.4] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-31.2/-31.1] Declination in decimal degrees (J2000)"}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[11] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[20/35] Arcsecond of Declination (J2000) "}, {"name": "F220W", "desc": "[17.9/29.8]?=100 Integrated apparent HST/ACS_HRC F220W magnitude"}, {"name": "e_F220W", "desc": "[0.1/8.2]?=10 Uncertainty in F220W "}, {"name": "F330W", "desc": "[18.4/29]?=100 Integrated apparent HST/ACS_HRC F330W magnitude"}, {"name": "e_F330W", "desc": "[0.09/9]?=10 Uncertainty in F330W "}, {"name": "F336W", "desc": "[18.4/36.2]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.09/6.4]?=10 Uncertainty in F336W "}, {"name": "F555W", "desc": "[19.2/31.3]?=100 Integrated apparent HST F555W magnitude"}, {"name": "e_F555W", "desc": "[0.05/2]?=10 Uncertainty in F555W "}, {"name": "F606W", "desc": "[19.8/28.5]?=100 Integrated apparent HST F606W magnitude"}, {"name": "e_F606W", "desc": "[0.03/6.8]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[20.3/28.3]?=100 Integrated apparent HST F814W magnitude"}, {"name": "e_F814W", "desc": "[0.05/4.1]?=10 Uncertainty in F814W "}]}, {"name": "table16.dat", "desc": "Derived NGC 2997 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table17.dat", "desc": "Multi-band photometry of the NGC 3081 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/241] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F255W", "desc": "[17.4/26.6]?=100 Integrated apparent HST/WFPC2 F255W magnitude"}, {"name": "e_F255W", "desc": "[0.1/10]?=10 Uncertainty F255W "}, {"name": "F336W", "desc": "[17.8/28.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.07/6]?=10 Uncertainty in F336W "}, {"name": "F439W", "desc": "[17.9/27.2]?=100 Integrated apparent HST/WFPC2 F439W magnitude"}, {"name": "e_F439W", "desc": "[0.06/7.2]?=10 Uncertainty in F439W "}, {"name": "F555W", "desc": "[18.4/27]?=100 Integrated apparent HST/WFPC2 F555W magnitude"}, {"name": "e_F555W", "desc": "[0.04/2.3]?=10 Uncertainty in F555W "}, {"name": "F814W", "desc": "[18.6/30.4]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/10]?=10 Uncertainty in F814W "}]}, {"name": "table18.dat", "desc": "Derived NGC 3081 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table19.dat", "desc": "Multi-band photometry of the NGC 3351 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/447] ID number "}, {"name": "RAdeg", "desc": "[160.9/161] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[10] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[43] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[57.3/58.3] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[11.7/11.8] Declination, decimal degrees (J2000) "}, {"name": "DEd", "desc": "[11] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[42] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[5/21] Arcsecond of Declination (J2000) "}, {"name": "F275W", "desc": "[15.6/27.2]?=100 Integrated apparent HST/WFC3 F275W magnitude"}, {"name": "e_F275W", "desc": "[0.04/9]?=10 Uncertainty in F275W "}, {"name": "F336W", "desc": "[16/36.1]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.03/10]?=10 Uncertainty in F336W "}, {"name": "F438W", "desc": "[16.5/27]?=100 Integrated apparent HST/WFC3 F438W magnitude"}, {"name": "e_F438W", "desc": "[0.03/9]?=10 Uncertainty in F438W "}, {"name": "F450W", "desc": "[16.7/27]?=100 Integrated apparent HST/WFPC2 F450W magnitude"}, {"name": "e_F450W", "desc": "[0.02/10]?=10 Uncertainty in F450W "}, {"name": "F555W", "desc": "[17/25.8]?=100 Integrated apparent HST F555W magnitude"}, {"name": "e_F555W", "desc": "[0.02/4.4]?=10 Uncertainty in F555W "}, {"name": "F606W", "desc": "[17.6/27]?=100 Integrated apparent HST F606W magnitude"}, {"name": "e_F606W", "desc": "[0.03/4]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[18.4/27.1]?=100 Integrated apparent HST F814W magnitude"}, {"name": "e_F814W", "desc": "[0.03/4.1]?=10 Uncertainty in F814W "}]}, {"name": "table20.dat", "desc": "Derived NGC 3351 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table21.dat", "desc": "Multi-band photometry of the NGC 4303 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/142] ID number "}, {"name": "RAdeg", "desc": "[185.4/185.5] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[12] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[21] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[54.7/55.2] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[4.472/4.475] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[4] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[28] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[21.8/28.6] Arcsecond of Declination (J2000) "}, {"name": "F330W", "desc": "[18.6/25.5]?=100 Integrated apparent HST/ACS_HRC F330W magnitude"}, {"name": "e_F330W", "desc": "[0.1/2.4]?=10 Uncertainty in F330W "}, {"name": "F555W", "desc": "[19.7/25.7]?=100 Integrated apparent HST/ACS F555W magnitude"}, {"name": "e_F555W", "desc": "[0.07/3.5]?=10 Uncertainty in F555W "}, {"name": "F814W", "desc": "[20/25.4]?=100 Integrated apparent HST/ACS F814W magnitude"}, {"name": "e_F814W", "desc": "[0.05/2.5]?=10 Uncertainty in F814W "}]}, {"name": "table22.dat", "desc": "Derived NGC 4303 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table23.dat", "desc": "Multi-band photometry of the NGC 4314 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/208] ID number "}, {"name": "RAdeg", "desc": "[185.631/185.636] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[12] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[22] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[31.4/32.6] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[29.893/29.898] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[29] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[53] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[35.7/51.7] Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[17.5/27.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.06/7.2]?=10 Uncertainty in F336W "}, {"name": "F439W", "desc": "[17.9/25.4]?=100 Integrated apparent HST/WFPC2 F439W magnitude"}, {"name": "e_F439W", "desc": "[0.06/1.8]?=10 Uncertainty in F439W "}, {"name": "F569W", "desc": "[18.6/26.1]?=100 Integrated apparent HST/WFPC2 F569W magnitude"}, {"name": "e_F569W", "desc": "[0.04/1.6]?=10 Uncertainty in F569W "}, {"name": "F606W", "desc": "[18.8/26.6]?=100 Integrated apparent HST/WFPC2 F606W magnitude"}, {"name": "e_F606W", "desc": "[0.03/2]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[19.4/28.3]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/6]?=10 Uncertainty in F814W "}]}, {"name": "table24.dat", "desc": "Derived NGC 4314 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table25.dat", "desc": "Multi-band photometry of the NGC 6782 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/44] ID number "}, {"name": "RAdeg", "desc": "[290.98/291] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[19] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[23] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[57/58.5] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-59.93/-59.92] Declination in decimal degrees (J2000)"}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[59] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[55] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[16/26.2] Arcsecond of Declination (J2000) "}, {"name": "F255W", "desc": "[18/24.3]?=100 Integrated apparent HST/WFPC2 F255W magnitude"}, {"name": "e_F255W", "desc": "[0.2/7.6]?=10 Uncertainty in F255W "}, {"name": "F300W", "desc": "[18.2/24.5]?=100 Integrated apparent HST/WFPC2 F300W magnitude"}, {"name": "e_F300W", "desc": "[0.09/5.5]?=10 Uncertainty in F300W "}, {"name": "F450W", "desc": "[18/23.7]?=100 Integrated apparent HST/WFPC2 F450W magnitude"}, {"name": "e_F450W", "desc": "[0.06/4.1]?=10 Uncertainty in F450W "}, {"name": "F606W", "desc": "[17.5/24.4]?=100 Integrated apparent HST/WFPC2 F606W magnitude"}, {"name": "e_F606W", "desc": "[0.04/6.6]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[17.4/24.6]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/2.7]?=10 Uncertainty in F814W "}]}, {"name": "table26.dat", "desc": "Derived NGC 6782 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table27.dat", "desc": "*Derived NGC 6951 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table28.dat", "desc": "Multi-band photometry of the NGC 7217 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/115] ID number "}, {"name": "RAdeg", "desc": "[331.96/331.98] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[22] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[7] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[51.4/53.3] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[31.35/31.37] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[31] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[21] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[23/43.2] Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[21.4/28.6]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.3/5.6]?=10 Uncertainty in F336W "}, {"name": "F450W", "desc": "[21.3/26]?=100 Integrated apparent HST/WFPC2 F450W magnitude"}, {"name": "e_F450W", "desc": "[0.1/1.3]?=10 Uncertainty in F450W "}, {"name": "F547M", "desc": "[19.7/27.3]?=100 Integrated apparent HST/WFPC2 F547M magnitude"}, {"name": "e_F547M", "desc": "[0.06/9.5]?=10 Uncertainty in F547M "}, {"name": "F814W", "desc": "[21.7/29.3]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.09/1.6]?=10 Uncertainty in F814W "}]}, {"name": "table29.dat", "desc": "Derived NGC 7217 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table30.dat", "desc": "Multi-band photometry of the NGC 7469 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/56] ID number "}, {"name": "RAdeg", "desc": "[345.814/345.816] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[23] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[3] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[15.5/16] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[8.873/8.875] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[8] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[52] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[25.5/28.7] Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[16.7/23.5]?=100 Integrated apparent HST F336W magnitude"}, {"name": "e_F336W", "desc": "[0.04/1.1]?=10 Uncertainty in F336W "}, {"name": "F435W", "desc": "[17/25.5]?=100 Integrated apparent HST/ACS F435W magnitude"}, {"name": "e_F435W", "desc": "[0.02/1.6]?=10 Uncertainty in F435W "}, {"name": "F550M", "desc": "[17.6/23]?=100 Integrated apparent HST/ACS F550M magnitude"}, {"name": "e_F550M", "desc": "[0.03/0.5]?=10 Uncertainty in F550M "}, {"name": "F606W", "desc": "[18/26.3]?=100 Integrated apparent HST F606W magnitude"}, {"name": "e_F606W", "desc": "[0.02/4]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[18.6/25.2]?=100 Integrated apparent HST F814W magnitude"}, {"name": "e_F814W", "desc": "[0.02/1.5]?=10 Uncertainty in F814W "}]}, {"name": "table31.dat", "desc": "Derived NGC 7469 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table32.dat", "desc": "Multi-band photometry of the NGC 7742 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/270] ID number "}, {"name": "RAdeg", "desc": "[356.062/356.07] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[23] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[44] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[14.9/16.6] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[10.76/10.78] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[10] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[45/46] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[18.6/29.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.1/8.1]?=10 Uncertainty in F336W "}, {"name": "F555W", "desc": "[19.4/26]?=100 Integrated apparent HST/WFPC2 F555W magnitude"}, {"name": "e_F555W", "desc": "[0.05/10]?=10 Uncertainty in F555W "}, {"name": "F675W", "desc": "[19.6/29.3]?=100 Integrated apparent HST/WFPC2 F675W magnitude"}, {"name": "e_F675W", "desc": "[0.05/5]?=10 Uncertainty in F675W "}, {"name": "F814W", "desc": "[20.4/28.2]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.07/9]?=10 Uncertainty in F814W "}]}, {"name": "table33.dat", "desc": "Derived NGC 7742 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table34.dat", "desc": "Multi-band photometry of the UGC 3789 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/80] ID number "}, {"name": "RAdeg", "desc": "[41.584/41.587] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[2] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[46] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[20.2/20.7] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-30.28/-30.27] Declination in decimal degrees (J2000)"}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[30] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[16] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[25/33] Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[19.3/26.5]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.1/4]?=10 Uncertainty in F336W "}, {"name": "F438W", "desc": "[19.4/26.7]?=100 Integrated apparent HST/WFC3 F438W magnitude"}, {"name": "e_F438W", "desc": "[0.1/8.2]?=10 Uncertainty in F438W "}, {"name": "F814W", "desc": "[20.7/27.3]?=100 Integrated apparent HST/WFC3 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.1/3.1]?=10 Uncertainty in F814W "}]}, {"name": "table35.dat", "desc": "Derived UGC 3789 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_862_57"}} {"id": "J/ApJ/862/57", "title_cds": "", "title_create": "Takeda+, 2018", "year": "2018", "author": "Takeda Y., Hashimoto O., Honda S.", "title_pub": "Spectroscopic Determination of Capella's Photospheric Abundances: Possible Influence of Stellar Activity.", "first_author": "Takeda Y.", "bibcode": [""], "bibcode": ["2018ApJ...863...59E"], "see_also": ["B/eso : ESO Science Archive Catalog (ESO, 1991-2019)", "J/ApJ/633/871 : Positions & photometry of HII knots in M51 (Calzetti+, 2005)", "J/ApJ/642/158 : IRAC flux densities in IC2163 and NGC2207 (Elmegreen+, 2006)", "J/ApJ/656/770 : Mid-IR spectrum of star-forming galaxies (Smith+, 2007)", "J/ApJ/669/959 : Warm molecular hydrogen in SINGS galaxies (Roussel+, 2007)", "J/AJ/133/791 : Spitzer phot. of normal+interacting galaxies (Smith+, 2007)", "J/ApJ/693/1821 : The Spitzer infrared nearby galaxies survey (Dale+, 2009)", "J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)", "J/A+A/505/405 : A catalogue of Spitzer dark clouds (Peretto+, 2009)", "J/ApJ/716/942 : Bulges of nearby galaxies with Spitzer (Fisher+, 2010)", "J/ApJ/772/107 : Giant molecular clouds in nearby gal. (Donovan Meyer+, 2013)", "J/MNRAS/432/2182 : FIR bright sources of M83 (Foyle+, 2013)", "J/A+A/551/A81 : NGC 6951 intensity and velocity maps (van der Laan+, 2013)", "J/A+A/553/A54 : M100 (NGC4321) HII region IRAC photometry (Chan+, 2013)", "J/ApJ/784/3 : PAWS catalogs of GMCs and islands in M51 (Colombo+, 2014)", "J/ApJS/212/18 : An atlas of UV-to-MIR galaxy SEDs (Brown+, 2014)", "J/A+A/569/A11 : G35.20-0.74N data cubes (Sanchez-Monge+, 2014)", "J/A+A/582/A86 : Catalogue of features in the S4G (Herrera-Endoqui+, 2015)", "J/ApJ/841/37 : Tori in AGNs through Spitzer/IRS (Gonzalez-Martin+, 2017)", "J/ApJ/858/90 : Radial profiles of 5 nearby galaxies (Gallagher+, 2018)", "J/A+A/609/A123 : SABOCA imaging of G304.74+01.32 (Miettinen, 2018)", "J/ApJS/234/18 : GALEX/S4G surface brightness profiles. I. (Bouquin+, 2018)", "J/ApJS/234/35 : Stellar pop. synthesis of clumps (Zaragoza-Cardiel+, 2018)", "http://irsa.ipac.caltech.edu/Missions/spitzer.html : IRSA Spitzer home page"], "keyword_cds": "Galaxies, nearby; Photometry, infrared; Interstellar medium", "keyword_pub": "galaxies: ISM; galaxies: spiral; galaxies: star formation; ISM: structure; stars: formation", "abstract": ["Spitzer Space Telescope Infrared Array Camera (IRAC) images of M100", "show numerous long filaments with regularly spaced clumps, suggesting", "the associated cloud complexes formed by large-scale gravitational", "instabilities in shocked and accumulated gas. Optical images give no", "hint of this underlying regularity. The typical spacing between", "near-infrared clumps is ~410pc, which is ~3 times the clump diameter,", "consistent with the fastest growing mode in a filament of critical", "line density. The IRAC magnitudes and colors of several hundred clumps", "are measured in the most obvious 27 filaments and elsewhere. The clump", "colors suggest that the dust is associated with diffuse gas,", "polycyclic aromatic hydrocarbon emission, and local heating from star", "formation. Neighboring clumps on the same filament have similar", "magnitudes. The existence of many clumps all along the filament", "lengths suggests that the ages of the filaments are uniform. The", "observations support a model where interstellar gas is systematically", "accumulated over lengths exceeding several kpc, forming spiral-like", "filaments that spontaneously collapse into giant clouds and stellar", "complexes. Optical wavelengths show primarily the irregular dust", "debris, HII regions, and lingering star formation downstream from", "these primal formation sites."], "description": ["The Spitzer image of M100 was examined for small bright clumps with", "central peaks and red colors. The position and flux of each clump were", "first measured in four IRAC bands."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aacf9a"], "orcid_pub": ["0000-0002-1723-6330"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Clumps in filaments with background annulus subtracted", "columns": [{"name": "Seq", "desc": "[1/27] Filament sequential running number "}, {"name": "Fig4", "desc": "Symbol, Color in Figure 4 "}, {"name": "RAh", "desc": "[12] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[22/23] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of Declination (J2000) "}, {"name": "DEd", "desc": "[15] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[47/51] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "3.6mag", "desc": "[14.8/24] Spitzer/IRAC 3.6 band magnitude "}, {"name": "e_3.6mag", "desc": "[0.2/2.4] Uncertainty in 3.6mag "}, {"name": "4.5mag", "desc": "[14.5/22.5] Spitzer/IRAC 4.5 band magnitude "}, {"name": "e_4.5mag", "desc": "[0.2/6.4] Uncertainty in 4.5mag "}, {"name": "5.8mag", "desc": "[12.6/20.4] Spitzer/IRAC 5.8 band magnitude "}, {"name": "e_5.8mag", "desc": "[0.1/1.3] Uncertainty in 5.8mag "}, {"name": "8.0mag", "desc": "[10.9/17.8] Spitzer/IRAC 8.0 band magnitude "}, {"name": "e_8.0mag", "desc": "[0.1/1.4] Uncertainty in 8.0mag "}]}, {"name": "table2.dat", "desc": "Clumps in filaments with interclump subtracted ", "columns": [{"name": "Seq", "desc": "[1/27] Filament sequential running number "}, {"name": "Fig4", "desc": "Symbol, Color in Figure 4 "}, {"name": "RAh", "desc": "[12] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[22/23] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of Declination (J2000) "}, {"name": "DEd", "desc": "[15] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[47/51] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "3.6mag", "desc": "[14.8/24] Spitzer/IRAC 3.6 band magnitude "}, {"name": "e_3.6mag", "desc": "[0.2/2.4] Uncertainty in 3.6mag "}, {"name": "4.5mag", "desc": "[14.5/22.5] Spitzer/IRAC 4.5 band magnitude "}, {"name": "e_4.5mag", "desc": "[0.2/6.4] Uncertainty in 4.5mag "}, {"name": "5.8mag", "desc": "[12.6/20.4] Spitzer/IRAC 5.8 band magnitude "}, {"name": "e_5.8mag", "desc": "[0.1/1.3] Uncertainty in 5.8mag "}, {"name": "8.0mag", "desc": "[10.9/17.8] Spitzer/IRAC 8.0 band magnitude "}, {"name": "e_8.0mag", "desc": "[0.1/1.4] Uncertainty in 8.0mag "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_863_91"}} {"id": "J/ApJ/863/91", "title_cds": "Co-moving catalog reorganized with BANYAN & Gaia", "title_create": "Faherty+, 2018", "year": "2018", "author": "Faherty J.K., Bochanski J.J., Gagne J., Nelson O., Coker K., Smithka I., Desir D., Vasquez C.", "title_pub": "New and known moving groups and clusters identified in a Gaia co-moving catalog.", "first_author": "Faherty J.K.", "ref_biblio": [""], "bibcode": ["2018ApJ...863...91F"], "see_also": ["B/mk : Catalogue of Stellar Spectral Classifications (Skiff, 2009-)", "IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)", "IX/29 : ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000)", "I/259 : The Tycho-2 Catalogue (Hog+ 2000)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "I/298 : LSPM-North Catalog (Lepine+ 2005)", "II/328 : AllWISE Data Release (Cutri+ 2013)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/ApJS/101/117 : UBVRIJHKLMNQ photometry in Taurus-Auriga (Kenyon+ 1995)", "J/AJ/130/1247 : High proper motion stars in the DSS. III (Lepine+, 2005)", "J/AJ/133/889 : Faint companions of Hipparcos stars (Lepine+, 2007)", "J/AJ/139/2566 : SLoWPoKES catalog (Dhital+, 2010)", "J/ApJS/192/2 : A Bayesian search for binaries in Hipparcos (Shaya+, 2011)", "J/MNRAS/435/1325 : Membership of the {epsilon} Cha association (Murphy+, 2013)", "J/A+A/566/A132 : Teff and L for stars in 7 open clusters (Silaj+, 2014)", "J/MNRAS/454/593 : Young moving groups in solar neighbourhood (Bell+, 2015)", "J/ApJ/799/155 : Sub-stellar companions in Taurus (Daemgen+, 2015)", "J/AJ/150/57 : SLoWPoKES-II catalog (Dhital+, 2015)", "J/ApJS/219/33 : BANYAN. VII. Candidate YMG members from BASS (Gagne+, 2015)", "J/MNRAS/447/1267 : Low-mass members of the Octans association (Murphy+, 2015)", "J/ApJ/801/L10 : XO-2N and XO-2S equivalent widths (Teske+, 2015)", "J/ApJS/225/10 : Kinematic analysis of M7-L8 dwarfs (Faherty+, 2016)", "J/ApJ/830/44 : X-ray LFs of M37 low-mass stars (Nunez+, 2016)", "J/MNRAS/461/794 : Scorpius-Centaurus K-Type Stars (Pecaut+, 2016)", "J/A+A/595/A22 : 9 new open clusters within 500pc from the Sun (Roser+, 2016)", "J/MNRAS/472/675 : Wide binaries in Tycho-Gaia: search method (Andrews+, 2017)", "J/A+A/601/A19 : Gaia DR1 open cluster members (Gaia Collaboration+, 2017)", "J/AJ/153/259 : GAMBLES extension of the SLoWPoKES catalog (Oelkers+, 2017)", "J/AJ/153/257 : Comoving stars in Gaia DR1 (Oh+, 2017)", "J/AJ/155/149 : Co-moving stars observed by Gaia (Bochanski+, 2018)", "J/ApJ/856/23 : BANYAN. XI. The BANYAN {Sigma} algorithm (Gagne+, 2018)", "J/ApJ/860/43 : BANYAN. XII. New members from Gaia-Tycho data (Gagne+, 2018)", "J/ApJ/862/138 : BANYAN. XIII. Young assoc. with Gaia DR2 (Gagne+, 2018)"], "keyword_cds": "Photometry, infrared ; Proper motions ; Associations, stellar ; Radial velocities ; Spectral types ; Ultraviolet ; X-ray sources ; Parallaxes, trigonometric ; Optical", "keyword_pub": "methods: data analysis; proper motions; stars: kinematics and dynamics; open clusters and associations: general; binaries: general", "abstract": ["We present a reorganization of the Oh+ (2017, J/AJ/153/257) wide,", "comoving catalog of 4555 groups of stars (10606 individual objects)", "identified in the Tycho Gaia Astrometric Survey (TGAS) into new and", "known coevolving groups of stars in the Milky Way. We use the BANYAN", "{Sigma} kinematic analysis tool to identify 1015 individual stars in", "the Oh+ catalog that yielded a >80% probability in 1 of 27 known", "associations (e.g., the AB Doradus moving group, Columba, Upper", "Scorpius) in the vicinity of the Sun. Among the 27 groups uncovered by", "Oh+ that had >10 connected components, we find that 4 are newly", "discovered. We use a combination of Tycho, Gaia, Two micron All Sky", "catalog, Wide Field Infrared Survey Explorer Mission, Galaxy Evolution", "Explorer, and Rontgen Satellite photometry as well as Gaia parallaxes", "to determine that these new groups are likely older than the Pleiades", "but younger than ~1Gyr. Using isochrone fitting, we find that the", "majority of these new groups have solar-type stars and solar-type", "metallicity. Among the 35 Oh+ groups with five to nine members, we", "find that 19 also appear new and comoving, with Oh+ Group 30 is", "particularly exciting as it is well within 100pc (range of 77-90pc)", "and also appears to be older than the Pleiades. For known star-forming", "regions, open clusters, and moving groups identified by Oh+, we find", "that the majority were broken up into pieces over several Oh+ groups", "(e.g., Lower Centaurus Crux members are spread over 26 Oh+ groups);", "however, we found no correlation with positions of the groups on", "color-magnitude diagrams, and therefore no substructure of the", "association correlated with the Oh+ designated group. We find that", "across the 27 groups tested by BANYAN {Sigma} there were 400 new", "members to 20 different associations uncovered by Oh+ that require", "further vetting."], "type": ["CCC"], "doi_pub": ["10.3847/1538-4357/aac76e"], "orcid_pub": ["0000-0001-6251-0573"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Oh+ (Oh17; 2017, J/AJ/153/257) with spectral type and T_eff_", "columns": [{"name": "Name", "desc": "Object identifier; Tycho or Hipparcos "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) (G1) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) (G1) "}, {"name": "SpType", "desc": "Spectral type (G1) "}, {"name": "Teff", "desc": "[2800/32000]? Effective temperature (G1) "}, {"name": "Assoc", "desc": "BANYAN group designation (G2) "}, {"name": "Prob", "desc": "[0/100] BANYAN membership probability (1) "}, {"name": "Group", "desc": "[0/4554] Oh17 group number (G3) "}]}, {"name": "table2.dat", "desc": "Oh17 with photometry ", "columns": [{"name": "Name", "desc": "Object identifier; Tycho or Hipparcos "}, {"name": "SpType", "desc": "Spectral type (G1) "}, {"name": "Bmag", "desc": "[0.02/19.6]? Tycho B band magnitude "}, {"name": "Vmag", "desc": "[0.02/18.2]? Tycho V band magnitude "}, {"name": "l_Jmag", "desc": "Upper limit flag on Jmag "}, {"name": "Jmag", "desc": "[-27.2/16.8]? 2MASS J band magnitude "}, {"name": "e_Jmag", "desc": "[0/10]? Uncertainty in Jmag "}, {"name": "l_Hmag", "desc": "Upper limit flag on Hmag "}, {"name": "Hmag", "desc": "[0.02/11.3]? 2MASS H band magnitude "}, {"name": "e_Hmag", "desc": "[0/10]? Uncertainty in Hmag "}, {"name": "l_Ksmag", "desc": "Upper limit flag on Ksmag "}, {"name": "Ksmag", "desc": "[0/11.3]? 2MASS Ks band magnitude "}, {"name": "e_Ksmag", "desc": "[0/10]? Uncertainty in Ksmag "}, {"name": "l_W1mag", "desc": "Upper limit flag on W1mag "}, {"name": "W1mag", "desc": "[0/19.5]? WISE 3.4 micron band magnitude "}, {"name": "e_W1mag", "desc": "[0.01/18.4]? Uncertainty in W1mag "}, {"name": "l_W2mag", "desc": "Upper limit flag on W2mag "}, {"name": "W2mag", "desc": "[0.02/16] WISE 4.6 micron band magnitude "}, {"name": "e_W2mag", "desc": "[0/10]? Uncertainty in W2mag "}, {"name": "l_W3mag", "desc": "Upper limit flag on W3mag "}, {"name": "W3mag", "desc": "[-0.4/13]? WISE 12 micron band magnitude "}, {"name": "e_W3mag", "desc": "[0.01/10]? Uncertainty in W3mag "}, {"name": "l_W4mag", "desc": "Upper limit flag on W4mag "}, {"name": "W4mag", "desc": "[-3.3/11.5]? WISE 22 micron band magnitude "}, {"name": "e_W4mag", "desc": "[0/8.7]? Uncertainty in W4mag "}]}, {"name": "table3.dat", "desc": "Oh17 with photometry (cont) ", "columns": [{"name": "Name", "desc": "Object identifier; Tycho or Hipparcos "}, {"name": "SpType", "desc": "Spectral type (G1) "}, {"name": "NUVmag", "desc": "[9.8/21.8]? GALEX NUV band magnitude "}, {"name": "e_NUVmag", "desc": "[0/0.5]? Uncertainty in NUVmag "}, {"name": "FUVmag", "desc": "[10.7/24.3]? GALEX FUV band magnitude "}, {"name": "e_FUVmag", "desc": "[0/2.2]? Uncertainty in FUVmag "}, {"name": "1RXS", "desc": "ROSAT bright identifier (JHHMMSS.s+DDMMs) "}, {"name": "logLBx", "desc": "[27.6/31.7]? log bright X-ray luminosity; in erg/s units"}, {"name": "e_logLBx", "desc": "[0.03/0.5]? Uncertainty in logLBx; ergs/s "}, {"name": "1RXSf", "desc": "ROSAT faint identifier (JHHMMSS.s+DDMMs) "}, {"name": "logLFx", "desc": "[27.3/31]? log faint X-ray luminosity; ergs/s "}, {"name": "e_logLFx", "desc": "[0.1/1.6]? Uncertainty in logLFx; ergs/s "}, {"name": "Group", "desc": "[0/4554] Oh17 group number (G3) "}, {"name": "Assoc", "desc": "BANYAN group designation (G2) "}, {"name": "Prob", "desc": "[0/100] BANYAN group membership probability "}]}, {"name": "table4.dat", "desc": "Oh+ (Oh17; 2017, J/AJ/153/257) sample with BANYAN {Sigma} input of known members", "columns": [{"name": "Name", "desc": "Object identifier; Tycho or Hipparcos "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) (G1) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) (G1) "}, {"name": "pmRA", "desc": "[-248/226.4] Proper motion along RA "}, {"name": "e_pmRA", "desc": "[0.01/4.7] Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-320.4/271.6] Proper motion along DE "}, {"name": "e_pmDE", "desc": "[0.01/2.7] Uncertainty in pmDE "}, {"name": "plx", "desc": "[5.7/63.4] Parallax "}, {"name": "e_plx", "desc": "[0.2/1] Uncertainty in plx "}, {"name": "RVel", "desc": "[-4.4/42.8]? Radial velocity "}, {"name": "e_RVel", "desc": "[0.8/8.3]? Uncertainty in RVel "}, {"name": "B-Grp", "desc": "BANYAN nearby group(s) designation "}, {"name": "Prob", "desc": "[81/100] BANYAN nearby membership probability "}, {"name": "Group", "desc": "[2/4103] Oh17 group number (G3) "}, {"name": "Known", "desc": "Object type (1) "}, {"name": "K-Grp", "desc": "Corresponding group(s) of investigation to Known"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_872_16"}} {"id": "J/ApJ/872/16", "title_cds": "Integrated star formation law revisited. I.", "title_create": "de los Reyes+, 2019", "year": "2019", "author": "de los Reyes M.A.C., Kennicutt R.C.", "title_pub": "Revisiting the integrated star formation law. I. Non-starbursting galaxies.", "first_author": "de los Reyes M.A.C.", "ref_biblio": [""], "bibcode": ["2019ApJ...872...16D"], "see_also": ["II/328 : AllWISE Data Release (Cutri+ 2013)", "VII/155 : Third Reference Cat. of Bright Galaxies (RC3) (de Vaucouleurs+ 1991)", "J/A+AS/115/407 : Short WSRT HI observations of spiral galaxies (Rhee+, 1996)", "J/A+A/324/877 : HI properties of spiral & irregular galaxies (Broeils+, 1997)", "J/A+A/370/765 : HI synthesis observations in UMa cluster (Verheijen+, 2001)", "J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)", "J/A+A/442/137 : HI observations of WHISP disk galaxies (Noordermeer+, 2005)", "J/ApJS/164/81 : Spectrophotometry of nearby galaxies (Moustakas+, 2006)", "J/PASP/119/994 : MIPS 24um calibrators (Engelbracht+, 2007)", "J/ApJS/173/185 : GALEX UV atlas of nearby galaxies (Gil de Paz+, 2007)", "J/ApJ/671/333 : Aperture photometry in NGC 5194 (Kennicutt+, 2007)", "J/ApJS/173/538 : XUV-Disk galaxies in the Local Universe (Thilker+, 2007)", "J/ApJS/178/247 : H{alpha} and [NII] survey in local 11 Mpc (Kennicutt+, 2008)", "J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008)", "J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008)", "J/ApJ/703/517 : The Spitzer Local Volume Legacy: IR photometry (Dale+, 2009)", "J/ApJ/706/599 : H{alpha} and UV SFR in the local volume (Lee+, 2009)", "J/ApJS/190/233 : Spectroscopy & abundances of SINGS gal. (Moustakas+, 2010)", "J/PASP/122/1397 : Spitzer Survey of Stellar Structure in Gal. (Sheth+, 2010)", "J/ApJS/192/6 : A GALEX UV imaging survey of nearby galaxies (Lee+, 2011)", "J/ApJ/733/87 : Star formation efficiency in galaxies (Shi+, 2011)", "J/MNRAS/414/940 : ATLAS3D project. IV. (Young+, 2011)", "J/MNRAS/423/197 : MIPS photometry for Herschel SAG2 Programs (Bendo+, 2012)", "J/A+A/544/A101 : GALEX obs. of Herschel Reference Survey (Cortese+, 2012)", "J/AJ/144/134 : LITTLE THINGS survey of nearby dwarf galaxies (Hunter+, 2012)", "J/ApJ/771/59 : S^4^G face-on gal. surface brightnesses (Munoz-Mateos+, 2013)", "J/A+A/564/A65 : Cold gas data of Herschel Reference Survey (Boselli+, 2014)", "J/MNRAS/445/899 : LVL SEDs and physical properties (Cook+, 2014)", "J/A+A/566/A71 : HI study of 18 nearby dwarf galaxies (Lelli+, 2014)", "J/A+A/569/A124 : GUViCS. Ultraviolet Source Catalogs (Voyer+, 2014)", "J/ApJS/220/6 : Updated catalog of GALEX nearby galaxies (Bai+, 2015)", "J/ApJ/805/31 : IR-Rad luminosities & surface densities of gal. (Liu+, 2015)"], "keyword_cds": "Galaxies, photometry; Ultraviolet; Infrared; Abundances; References; Radio sources", "keyword_pub": "galaxies: dwarf ; galaxies: spiral ; galaxies: star formation", "abstract": ["We use new and updated gas- and dust-corrected star formation rate", "(SFR) surface densities to revisit the integrated star formation law", "for local \"quiescent\" spiral, dwarf, and low surface brightness", "galaxies. Using UV-based SFRs with individual IR-based dust", "corrections, we find that \"normal\" spiral galaxies alone define a", "tight {Sigma}_(HI+H2)-{Sigma}_SFR_ relation described by an", "n=1.41_-0.07_^+0.07^ power law with a dispersion of 0.28_-0.02_^+0.02^", "(errors reflect fitting and statistical uncertainties). The SFR", "surface densities are only weakly correlated with HI surface", "densities alone, exhibiting a stronger and roughly linear correlation", "with H_2_ surface densities, similar to what is seen in spatially", "resolved measurements of disks. However, many dwarf galaxies lie below", "the star formation law defined by spirals, suggesting a low-density", "threshold in the integrated star formation law. We consider", "alternative scaling laws that better describe both spirals and dwarfs.", "Our improved measurement precision also allows us to determine that", "much of the scatter in the star formation law is intrinsic, and we", "search for correlations between this intrinsic scatter and secondary", "physical parameters. We find that dwarf galaxies exhibit second-order", "correlations with the total gas fraction, stellar mass surface", "density, and dynamical time, which may explain much of the scatter in", "the star formation law. Finally, we discuss various systematic", "uncertainties that should be kept in mind when interpreting any study", "of the star formation law, particularly the X(CO) conversion factor", "and the diameter chosen to define the star-forming disk in a galaxy."], "type": ["CCC"], "doi_pub": ["10.3847/1538-4357/aafa82"], "orcid_pub": ["0000-0002-4739-046X"], "data": "f-v", "date_creation": "10-Aug-2020", "xmatch": "J/ApJ/872/16/sample", "last_update": "12-Oct-2020", "catid": "18720016", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "General properties of sample ", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Dist", "desc": "[0.5/75.4]? Distance (1) "}, {"name": "Bmag", "desc": "[4.16/15.8]? Apparent B-band (AB) magnitude (2)"}, {"name": "e_Bmag", "desc": "[0.04/0.99]? Mean error on Bmag (2) "}, {"name": "B-V", "desc": "[0.21/1.07]? B-V color index (2) "}, {"name": "e_B-V", "desc": "[0.01/0.19]? Mean error B-V (2) "}, {"name": "MType", "desc": "Galaxy type; s=spiral, d=dwarf "}, {"name": "PA", "desc": "[-75/203] Position angle (2) "}, {"name": "E(B-V)", "desc": "[0.01/0.8] Reddening E(B-V) (3) "}, {"name": "Diam25", "desc": "[25/11433]? D25 diameter (2) "}, {"name": "DiamHa", "desc": "[8/5940] D(Halpha) diameter (4) "}, {"name": "b/a", "desc": "[0.1/1.0]? Axis ratio measured from B-band isophotes (2)"}]}, {"name": "table2.dat", "desc": "UV photometric data ", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "l_UVmag", "desc": "[0/1] Upper limit flag on UVmag; 1=yes, 0=no "}, {"name": "UVmag", "desc": "[8.2/20.7]? GALEX apparent UV magnitude "}, {"name": "e_UVmag", "desc": "[0.1/1]? Mean error on UVmag "}, {"name": "r_UVmag", "desc": "[401/408]? Reference for UVmag (see refs.dat file) "}, {"name": "tUV", "desc": "[87/21177.4]? Exposure time (5) "}, {"name": "Tile", "desc": "GALEX tile name (5) "}, {"name": "f_UVmag", "desc": "[0/1]? NUV flag; 1=only NUV available; 0=FUV used (5)"}]}, {"name": "table3.dat", "desc": "IR photometric data ", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "l_IRflux", "desc": "[0/1] Upper limit flag on IR flux; 1=yes, 0=no "}, {"name": "IRflux", "desc": "[1.9e-05/139]? 24um IR flux density "}, {"name": "e_IRflux", "desc": "[0.0001/23]? Mean error on IRflux "}, {"name": "r_IRflux", "desc": "[301/404] Reference for IRflux (see refs.dat file)"}, {"name": "tIR", "desc": "[146.8/1404.7]? Exposure time (s) (6) "}, {"name": "Survey", "desc": "For Spitzer MIPS images, name of survey (7) "}, {"name": "Nfr", "desc": "[99/558]? For AllWISE images, number of frames "}, {"name": "CoaddID", "desc": "For AllWISE images, the co-add ID "}]}, {"name": "table4.dat", "desc": "SFRs, gas masses, and SFR and gas surface densities; from erratum published in 2019, ApJ, 878, 74", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "l_logSFR", "desc": "[0/1]? Upper limit flag on logSFR (1=yes)"}, {"name": "logSFR", "desc": "[-4.5/1.5]? Log uncorrected SFR "}, {"name": "e_logSFR", "desc": "[0.02/0.4]? Mean error on logSFR "}, {"name": "l_logSFRc", "desc": "[0/1]? Upper limit flag on logSFRc (1=yes)"}, {"name": "logSFRc", "desc": "[-5.4/1.5]? Log dust-corrected SFR "}, {"name": "e_logSFRc", "desc": "[0.02/0.5]? Mean error on logSFRcorr "}, {"name": "logSigSFRc", "desc": "[-5.7/1.2]? Log dust-corrected SFR surface density"}, {"name": "logSigHI", "desc": "[-0.3/1.5]? Log HI surface density (8) "}, {"name": "r_logSigHI", "desc": "Reference for logSigHI (see refs.dat file)"}, {"name": "l_logSigH2", "desc": "[0/1] Upper limit flag on logSigH2 (1=yes)"}, {"name": "logSigH2", "desc": "[-1.3/3.5]? Log H2 surface density (8) "}, {"name": "r_logSigH2", "desc": "Reference for logSigH2 (see refs.dat file)"}]}, {"name": "table5.dat", "desc": "Other properties of sample ", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "Mass", "desc": "[5.8/11.5]? Log stellar mass "}, {"name": "r_Mass", "desc": "[501/503]? Reference for stellar mass (see refs.dat file)"}, {"name": "Z", "desc": "[7.3/9.2]? Gas-phase metallicity; 12+log[O/H]"}, {"name": "r_Z", "desc": "[601/605]? Reference for Z (see refs.dat file)"}, {"name": "C42", "desc": "[1.7/6.7]? Concentration index "}, {"name": "tDyn", "desc": "[0.2/17.4]? Dynamical time (9) "}, {"name": "vRot", "desc": "[0.6/43]? Rotational velocity (9) "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "[1/605] Reference code "}, {"name": "Auth", "desc": "First author's name(s) "}, {"name": "BibCode", "desc": "Bibcode of the reference "}, {"name": "Comm", "desc": "Comment "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_872_89"}} {"id": "J/ApJ/872/89", "title_cds": "Solar energetic particle (SEP) events with GOES", "title_create": "Kahler+, 2019", "year": "2019", "author": "Kahler S.W., Ling A.G.", "title_pub": "Suprathermal ion backgrounds of solar energetic particle events.", "first_author": "Kahler S.W.", "ref_biblio": [""], "bibcode": ["2019ApJ...872...89K"], "see_also": ["J/ApJ/709/1238 : Solar Coronal Mass Ejection (Yeates+, 2010)", "J/ApJ/757/94 : Solar flares observed with GOES and AIA (Aschwanden, 2012)", "J/ApJ/759/69 : Solar electron events 1995-2005 with WIND/3DP (Wang+, 2012)", "J/ApJ/774/L27 : Solar flares predictors (Yang+, 2013)", "J/A+A/574/A37 : Movies of 2012-10-16 solar flare (Dalmasse+, 2015)", "J/ApJ/831/105 : Global energetics of solar flares. IV. CME (Aschwanden, 2016)", "J/ApJ/845/36 : Complex network for solar active regions (Daei+, 2017)", "J/ApJ/847/115 : The solar flare complex network (Gheibi+, 2017)", "J/ApJ/868/124 : ICMEs events from 1998 to 2011 with ACE and WIND (Feng+, 2018)", "J/A+A/640/A17 : GLE integral intensities (Usoskin+, 2020)", "http://umbra.nascom.nasa.gov/SEP : : Solar Proton Events list from NOAA", "http://st4a.stelab.nagoya-u.ac.jp/hinode_flare/ : Hinode Flare Catalog", "http://www.lmsal.com/hek/index.html : Heliophysics Events Knowledgebase"], "keyword_cds": "Sun; Stars, flare", "keyword_pub": "acceleration of particles ; Sun: coronal mass ejections (CMEs) ; Sun: flares ; Sun: particle emission", "abstract": ["Gradual solar energetic particle (SEP) events result from the", "acceleration of low-energy suprathermal seed particles to high", "(E>10MeV/nuc) energies by shocks driven by coronal mass ejections", "(CMEs). Several studies suggest connections between suprathermal", "particles measured in situ at 1au and the seed particles accelerated", "near the Sun to E>10MeV. We correlate E>10MeV SEP event peak", "intensities (Ip) with suprathermal H and He intensities at each of two", "energies averaged over four periods around the SEP onsets in the", "Geostationary Operational Environmental Satellite spacecraft during", "the period of 1998-2016. The 201 SEP events are sorted into four", "groups by their associated solar source longitudes and are further", "separated between events in transient CMEs and in normal solar wind", "(SW). The mean Ip in CME SW that is larger than in normal SW that was", "found earlier is confirmed. The suprathermals significantly correlate", "(correlation coefficients CCs~0.4-0.6) with the SEP Ip from the 0{deg}", "to W40{deg} range, but only weakly (CC~0.0-0.3) with SEP events from", "the well-connected W41{deg} to W83{deg} range. Eastern hemisphere SEP", "intensities are uncorrelated (CC~0.0) with suprathermals in normal SW", "but are well correlated (CC~0.4-0.7) for those in transient CME SW,", "which we interpret with a simple model involving perpendicular shock", "acceleration of the suprathermals. The in situ B field magnitude shows", "no correlation with SEP intensities for any longitude range or", "timescale. These results confirm that tracking suprathermal", "intensities at 1 au can be useful in forecasting the Ip of SEP events."], "description": ["We compiled a list of E>10MeV solar energetic particle (SEP) events", "observed with the Energetic Particle Sensors on board the", "Geostationary Operational Environmental Satellite (GOES) from 1998", "through 2016. See Section 2 for further details."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "E>10MeV solar energetic particle (SEP) events ", "columns": [{"name": "Event.Y", "desc": "[1998/2016] Year of the event (1) "}, {"name": "Event.M", "desc": "Month of the event "}, {"name": "Event.D", "desc": "Day of the event "}, {"name": "---", "desc": "[/] "}, {"name": "Onset", "desc": "Hour of event onset (unit????) "}, {"name": "Ip", "desc": "[1.4/8000] Peak intensity (2) "}, {"name": "Time", "desc": "UT time of flare peak; Day/hour "}, {"name": "Loc", "desc": "Location of flare "}, {"name": "CME", "desc": "Coronal Mass Ejection Solar Wind event? Y=yes "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_872_206"}} {"id": "J/ApJ/872/206", "title_cds": "Blue horizontal branch stars in the VVV data", "title_create": "Montenegro+, 2019", "year": "2019", "author": "Montenegro K., Minniti D., Alonso-Garcia J., Hempel M., Saito R.K., Beers T.C., Brown D.", "title_pub": "VVV Survey of blue horizontal branch stars in the bulge-halo transition region of the Milky Way.", "first_author": "Montenegro K.", "ref_biblio": [""], "bibcode": ["2019ApJ...872..206M"], "see_also": ["B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "II/337 : VISTA Variables in the Via Lactea Survey DR1 (Saito+, 2012)", "II/348 : VISTA Variable in the Via Lactea Survey DR2 (Minniti+, 2017)", "II/364 : VIRAC. The VVV Infrared Astrometric Catalogue (Smith+, 2019)", "J/AJ/87/1515 : UBV photometry of AB stars in halo (Pier, 1982)", "J/ApJS/67/461 : Candidate field horizontal-branch stars catalog (Beers+, 1988)", "J/ApJS/103/433 : Horizontal-branch and A-type star catalog. II (Beers+ 1996)", "J/A+A/431/143 : Field HB stars in the Galaxy (Christlieb+, 2005)", "J/ApJS/168/277 : HK-Survey field horizontal-branch candidates (Beers+, 2007)", "J/AJ/135/564 : Photometry and spectroscopy of BHB candidates (Brown+, 2008)", "J/ApJ/684/1143 : BHB candidates in the Milky Way (Xue+, 2008)", "J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009)", "J/A+A/522/A88 : Photometric identification of BHB stars (Smith+, 2010)", "J/AJ/141/83 : Kepler Mission. I. Eclipsing binaries in DR1 (Prsa+, 2011)", "J/ApJ/731/119 : BHB candidates in Sagittarius stream (Ruhland+, 2011)", "J/AJ/149/99 : VVV globulars. I. 2MASS-GC02, Terzan 10 (Alonso-Garcia+, 2015)", "J/A+A/591/A145 : VVV Survey outer bulge RRab stars (Gran+, 2016)", "J/A+A/587/A124 : Metal-poor stars towards the Galactic bulge (Koch+, 2016)", "http://horus.roe.ac.uk/vsa/ : VSA - VISTA Science Archive"], "keyword_cds": "Binaries, eclipsing; Milky Way; Stars, horizontal branch; Photometry, infrared", "keyword_pub": "binaries: eclipsing ; Galaxy: bulge ; stars: horizontal-branch", "abstract": ["We characterize the population of blue horizontal branch (BHB) stars", "in the bulge-halo transition region of the Milky Way using the VISTA", "Variables in the Via Lactea (VVV) ESO Public Survey data. The", "selection of BHB stars is made using the globular cluster M22 as a", "reference standard and constructing color-magnitude and color-color", "diagrams with specific cuts in the ZYJHKs near-infrared passbands. A", "total of 12554 BHB stars were detected, in a region within", "-10.0{deg}<=lw=10.2{deg} and -10.2{deg}<=b<=-8.0{deg}. We provide", "accurate coordinates and near-IR photometry for this sample of BHB", "stars. We searched for overdensities of stars with sizes similar to", "those of known globular clusters and stellar streams. By comparing", "real data with Monte Carlo simulations, we conclude that the few", "overdensities detected are of low significance. We also constructed", "Ks-band light curves for the BHB stars to study their variability.", "Taking an average of 52 epochs to calculate periods and amplitudes, we", "identify hundreds of candidate eclipsing binaries and a dozen", "pulsating stars. Finally, we made some comparisons with results", "obtained in a previous study for RR Lyrae variable stars in this same", "region."], "description": ["The VISTA Variables in the Via Lactea (VVV) is a public near-IR survey", "of the inner Milky Way (Minniti+ 2010NewA...15..433M ;", "Catelan+ 2011rrls.conf..145C and Saito+ 2012A&A...537A.107S), whose", "coordinates have subarcsecond accuracy (Smith+ 2018, II/364), a", "necessary requirement in this high stellar density region. The VVV", "observations were taken with the near-IR camera VIRCAM at the 4m", "Visible and Infrared Survey Telescope for Astronomy (VISTA) located at", "ESO Cerro Paranal Observatory.", "The observations are made using the ZYJHKs filters and consist of two", "epochs in ZYJH, taken at the beginning and the end of the survey, in", "years 2010 and 2015, respectively, plus multiple epochs in the Ks", "band. The Ks-band variability campaign was carried out between 2010", "and 2016, obtaining a total of about 75 observations per field in the", "VVV bulge area.", "We search for variability by constructing light curves of all the blue", "horizontal branch (BHB) stars in our sample. See Section 4."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Complete parameters for the first category eclipsing binaries", "columns": [{"name": "---", "desc": "[VVV] "}, {"name": "VVV", "desc": "[515455684844/515723445466] VVV survey identifier number"}, {"name": "RAh", "desc": "[17/18] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[23/42] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Per", "desc": "[0.1/18.2] Binary period "}, {"name": "KsAmp", "desc": "[0.15/1.1] The K_s_ band amplitude "}, {"name": "Zmag", "desc": "[13.2/16.8] Apparent Z band magnitude "}, {"name": "Ymag", "desc": "[13.3/17.2] Apparent Y band magnitude "}, {"name": "Jmag", "desc": "[13/16.8] Apparent J band magnitude "}, {"name": "Hmag", "desc": "[12.8/16.6] Apparent H band magnitude "}, {"name": "Ksmag", "desc": "[12.8/16.7] Apparent K_s_ band magnitude "}, {"name": "Class", "desc": "Classification code (1) "}]}, {"name": "table3.dat", "desc": "Complete parameters for the second category of eclipsing binaries", "columns": [{"name": "---", "desc": "[VVV] "}, {"name": "VVV", "desc": "[515455684844/515723445466] VVV survey identifier number"}, {"name": "RAh", "desc": "[17/18] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[23/42] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Per", "desc": "[0.1/18.2] Binary period "}, {"name": "KsAmp", "desc": "[0.15/1.1] The K_s_ band amplitude "}, {"name": "Zmag", "desc": "[13.2/16.8] Apparent Z band magnitude "}, {"name": "Ymag", "desc": "[13.3/17.2] Apparent Y band magnitude "}, {"name": "Jmag", "desc": "[13/16.8] Apparent J band magnitude "}, {"name": "Hmag", "desc": "[12.8/16.6] Apparent H band magnitude "}, {"name": "Ksmag", "desc": "[12.8/16.7] Apparent K_s_ band magnitude "}, {"name": "Class", "desc": "Classification code (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_907_69"}} {"id": "J/ApJ/907/69", "title_cds": "", "title_create": "Liggins+, 2021", "year": "2021", "author": "Liggins F.S., Pickering J.C., Nave G., Kramida A., Gamrath S., Quinet P.", "title_pub": "New Ritz Wavelengths and Transition Probabilities of Parity-forbidden [MnII] lines of astrophysical interest", "first_author": "Liggins F.S.", "ref_biblio": [""], "bibcode": ["2021ApJ...907...69L"], "see_also": ["J/A+A/419/215 : Emission lines of strontium filament near eta Car (Hartman+, 2004)", "J/ApJS/205/14 : Energy levels and spectral lines of MnII (Kramida+, 2013)", "J/A+A/580/A10 : New MnII energy levels (Castelli+, 2015)"], "keyword_cds": "", "keyword_pub": "Atomic data benchmarking ; Atomic physics ; Line positions ; Spectral line lists ; Line intensities ; Laboratory astrophysics ; Theoretical techniques ; High resolution spectroscopy ; Atomic spectroscopy", "abstract": ["We report a comprehensive list of accurate Ritz wavelengths and", "calculated transition probabilities for parity-forbidden [Mn ii]", "lines. Ritz wavelengths have been derived from experimentally", "established energy level values resulting from an extensive analysis", "of a high-resolution Fourier-transform emission spectrum of singly", "ionized manganese. Our analysis includes transitions between all known", "metastable and other long-lived levels of Mn ii giving a total of 1130", "[Mn ii] Ritz wavelengths. Our entire list of derived Ritz wavelengths", "for [Mn ii] lines ranges between 237 nm and 170 {mu}m (42,125-58", "cm-1). The accurate Ritz wavelengths and calculated transition", "probabilities for forbidden lines in this paper are useful in the", "study and diagnostics of nebulae and other low-density astrophysical", "plasmas."], "object": [], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "nothing ", "columns": [{"name": "Trans", "desc": "Description of Trans "}, {"name": "Parity", "desc": "Description of Parity "}, {"name": "DeltaJ", "desc": "Description of DeltaJ "}, {"name": "Restrictions", "desc": "Description of Restrictions "}]}, {"name": "table2.dat", "desc": "[Mn II] lines from the a5S, a5D, a5P, a5G, and b5D levels sorted by wavenumber ", "columns": []}, {"name": "table3.dat", "desc": "[Mn II] lines sorted by wavenumber ", "columns": [{"name": "Air-wl", "desc": "[237.31485/1981.0725]? Air wavelength (1) "}, {"name": "Vac-wl", "desc": "[237.38731/170448.0] Vacuum wavelength "}, {"name": "u_Vac-wl", "desc": "[1.3e-05/4.0] Uncertainty in air and vacuum wavelengths "}, {"name": "Waveno", "desc": "[58.6689/42125.252] Wavenumber "}, {"name": "u_Waveno", "desc": "[0.0003/0.03] Uncertainty in wavenumber "}, {"name": "low-config", "desc": "Lower energy level configuration and term "}, {"name": "upp-config", "desc": "Upper energy level configuration and term "}, {"name": "low-enval", "desc": "[0.0/59537.452] Lower energy level value (3) "}, {"name": "upp-enval", "desc": "[9472.9914/72648.936] Upper energy level value (3) "}, {"name": "BF", "desc": "[0.0004/1.0] Branching fraction "}, {"name": "A", "desc": "Transition rate "}, {"name": "u_A", "desc": "[1/80] Uncertainty in transition rate "}, {"name": "Type", "desc": "Type: M1 or E2 (2) "}, {"name": "Flag", "desc": "Flag (4) "}, {"name": "A-M1-NIST", "desc": "NIST M1 transition rate "}, {"name": "A-M1-Mons", "desc": "Mons M1 transition rate "}, {"name": "A-M1-Kurucz", "desc": "Kurucz M1 transition rate "}, {"name": "A-E2-NIST", "desc": "NIST E2 transition rate "}, {"name": "A-E2-Mons", "desc": "Mons E2 transition rate "}, {"name": "A-E2-Kurucz", "desc": "Kurucz E2 transition rate "}, {"name": "A-M1+E2-NIST", "desc": "NIST M1+E2 transition rate "}, {"name": "A-M1+E2-Mons", "desc": "Mons M1+E2 transition rate "}, {"name": "A-M1+E2-Kurucz", "desc": "Kurucz M1+E2 transition rate "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_907_112"}} {"id": "J/ApJ/907/112", "title_cds": "", "title_create": "Lee+, 2021", "year": "2021", "author": "Lee A.J., Freedman W.L., Madore B.F., Owens K.A., Monson A.J., Hoyt T.J.", "title_pub": "The Astrophysical Distance Scale. III. Distance to the Local Group Galaxy WLM Using Multiwavelength Observations of the Tip of the Red Giant Branch, Cepheids, and JAGB Stars.", "first_author": "Lee A.J.", "ref_biblio": [""], "bibcode": ["2021ApJ...907..112L"], "see_also": ["J/AJ/134/594 :\tAraucaria project: Cepheids in WLM galaxy (Pietrzynski+, 2007)"], "keyword_cds": "", "keyword_pub": "Distance indicators ; Population II stars ; Asymptotic giant branch stars ; Carbon stars ; Observational cosmology ; Hubble constant ; Cepheid variable stars", "abstract": ["The local determination of the Hubble constant sits at a crossroad.", "Current estimates of the local expansion rate of the universe differ", "by about 1.7{sigma}, derived from the Cepheid- and TRGB-based", "calibrations, applied to Type Ia supernovae. To help elucidate", "possible sources of systematic error causing the tension, we show in", "this study the recently developed distance indicator, the J-region", "Asymptotic Giant Branch (JAGB) method, can serve as an independent", "cross-check and comparison with other local distance indicators.", "Furthermore, we make the case that the JAGB method has substantial", "potential as an independent, precise, and accurate calibrator of Type", "Ia supernovae for the determination of H0. Using the Local Group", "galaxy Wolf-Lundmark-Melotte (WLM), we present distance comparisons", "between the JAGB method, a TRGB measurement at near-infrared (JHK)", "wavelengths, a TRGB measurement in the optical I band, and a", "multiwavelength Cepheid period-luminosity relation determination. We", "find {mu}_0_(JAGB)=24.97{+/-}0.02(stat){+/-}0.04(sys)mag", "{mu}_0_(TRGB_NIR_)=24.98{+/-}0.04(stat){+/-}0.07(sys)mag", "{mu}_0_(TRGB_F814W_=24.93{+/-}0.02(stat){+/-}0.06(sys)mag", "{mu}_0_(Cepheids)=24.98{+/-}0.03(stat){+/-}0.04(sys)mag. All four", "methods are in good agreement, confirming the local self-consistency", "of the four distance scales at the 3% level and adding confidence that", "the JAGB method is as accurate and as precise a distance indicator as", "either of the other three astrophysically based methods."], "description": ["Ground-based VI data of WLM were obtained at the Inamori-Magellan", "Areal Camera and Spectrograph (IMACS) on the 6.5m Magellan-Baade", "telescope using the f/4 imaging mode at Las Campanas Observatory on", "2019 November 16. The field has a dimension of 15.4x15.4'at a scale of", "0.111\"/pixel.", "Ground-based JHK data were taken at the 6.5m Magellan-Baade telescope", "at Las Campanas Observatory with the FourStar Infrared Camera. The", "FourStar imager has a field of view of 10.8x10.8' and a resolution of", "0.159\"/pixel."], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "ceph01.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_01 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph02.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_02 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph03.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_03 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band 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magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph51.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_51 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph52.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_52 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph53.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_53 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph54.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_54 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph55.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_55 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph56.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_56 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph57.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_57 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph58.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_58 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph59.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_59 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}, {"name": "ceph60.dat", "desc": "GLOESS-fit light curves in VIJHK for Ceph_60 ", "columns": [{"name": "JD", "desc": "Julian Date "}, {"name": "Imag", "desc": "?=99.99 I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.99 I-band magnitude error "}, {"name": "Vmag", "desc": "?=99.99 V-band magnitude "}, {"name": "e_Vmag", "desc": "?=9.99 V-band magnitude error "}, {"name": "Jmag", "desc": "?=99.99 J-band magnitude "}, {"name": "e_Jmag", "desc": "?=9.99 J-band magnitude error "}, {"name": "Hmag", "desc": "?=99.99 H-band magnitude "}, {"name": "e_Hmag", "desc": "?=9.99 H-band magnitude error "}, {"name": "Kmag", "desc": "?=99.99 K-band magnitude "}, {"name": "e_Kmag", "desc": "?=9.99 K-band magnitude error "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_871_103"}} {"id": "J/ApJ/871/103", "title_cds": "Catalog of 563 stars in the Galactic Center", "title_create": "Gautam+, 2019", "year": "2019", "author": "Gautam A.K., Do T., Ghez A.M., Morris M.R., Martinez G.D., Hosek M.W., Lu J.R., Sakai S., Witzel G., Jia S., Becklin E.E., Matthews K.", "title_pub": "An adaptive optics survey of stellar variability at the Galactic center.", "first_author": "Gautam A.K.", "ref_biblio": [""], "bibcode": ["2019ApJ...871..103G"], "see_also": ["J/ApJ/470/864 : JHKL photometry of the Galactic Center (Blum+, 1996)", "J/ApJ/523/248 : Variable stars in the Galactic center (Ott+, 1999)", "J/A+A/373/608 : Early-type stars towards Galactic Center. II. (Dufton+,2001)", "J/A+A/426/81 : Kinematic analysis of the Minispiral (Paumard+, 2004)", "J/A+A/433/117 : L- & M-band imaging of the Galactic Center (Viehmann+, 2005)", "J/MNRAS/370/1979 : JHKs photometry T2Cs in globular clusters (Matsunaga+, 2006)", "J/ApJ/643/1011 : Early-type stars in the center of the Galaxy (Paumard+,2006)", "J/ApJ/659/1241 : Stellar variability in Galactic Center (Rafelski+, 2007)", "J/ApJ/697/1741 : Warped disks of YSOs in Galactic center (Bartko+, 2009)", "J/ApJ/703/1323 : Spectroscopy of stars in Galaxy's nuclear cluster (Do+ 2009)", "J/MNRAS/399/1709 : Near-infrared survey of Miras (Matsunaga+, 2009)", "J/ApJ/723/1195 : SAGE AGB candidates (Riebel+, 2010)", "J/A+A/511/A18 : NIR observations of stars near SgrA* (Schoedel+, 2010)", "J/ApJ/725/331 : Astrometry in the Galactic Center (Yelda+, 2010)", "J/A+A/537/A146 : Stellar models (rotation 0.8"], "bibcode": ["2020ApJ...899..130S"], "see_also": ["II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "II/314 : UKIDSS-DR8 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/ApJ/454/151 : OB Associations of the Northern Milky Way (Massey+ 1995)", "J/ApJ/733/L8 : Optical and IR photometry of [KOS94] HA11 (Kun+, 2011)", "J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012)", "J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013)"], "keyword_cds": "Stars, variable; Photometry, VRI", "keyword_pub": "Star formation ; Accretion ; Protoplanetary disks ; Eruptive variable stars", "abstract": ["We present optical-infrared photometric and spectroscopic observations", "of Gaia 18dvy, located in the Cygnus OB3 association at a distance of", "1.88kpc. Gaia 18dvy was noted by the Gaia alerts system when its light", "curve exhibited a ~4mag rise in 2018-2019. The brightening was also", "observable at mid-infared wavelengths. The infrared colors of Gaia", "18dvy became bluer as the outburst progressed. Its optical and", "near-infrared spectroscopic characteristics in the outburst phase are", "consistent with those of bona fide FU Orionis-type young eruptive", "stars. The progenitor of the outburst is probably a low-mass K-type", "star with an optical extinction of ~3mag. A radiative transfer", "modeling of the circumstellar structure, based on the quiescent", "spectral energy distribution, indicates a disk with a mass of", "4x10^-3^M{sun}. Our simple accretion disk modeling implies that the", "accretion rate had been exponentially increasing for more than 3yr", "until mid-2019, when it reached a peak value of 6.9x10^-6^M{sun}/yr.", "In many respects, Gaia 18dvy is similar to the FU Ori-type object HBC722."], "description": ["We observed Gaia 18dvy in the BVR_C_I_C_ bands between 2019 June and", "December using the 60/90/180cm Schmidt telescope at the Konkoly", "Observatory (Hungary).", "Gaia 18dvy was also observed with the Schmidt-Teleskop-Kamera of", "University Observatory Jena in the Bessell V, R, and I bands. Each", "night, two frames (60s) were taken in each filter.", "Gaia 18dvy was also monitored with the Las Cumbres Observatory network", "of robotic telescopes. About 200 images have been obtained in V and", "I_C_.", "We monitored Gaia 18dvy at optical wavelengths using the Optical", "Infrared Coordination Network for Astronomy (OPTICON) Time-Domain", "Follow-up Network since 2019 February."], "object": ["20 05 06.03 +36 29 13.6 Gaia 18dvy = 2MASS J20050603+3629135"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Follow-up photometry ", "columns": [{"name": "MJD", "desc": "[8541/8830] Modified Julian Date; JD-2400000.5 "}, {"name": "Band", "desc": "Photometry band "}, {"name": "mag", "desc": "[5.75/17.93] Magnitude measured in the band "}, {"name": "e_mag", "desc": "[0/0.48] Uncertainty for magnitude "}, {"name": "Instr", "desc": "Telescope used for measuring the magnitude (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_875_111"}} {"id": "J/ApJ/875/111", "title_cds": "HST/COS spectra toward HeII-transparent QSOs", "title_create": "Worseck+, 2019", "year": "2019", "author": "Worseck G., Davies F.B., Hennawi J.F., Prochaska J.X.", "title_pub": "The evolution of the HeII-ionizing background at redshifts 2.3"], "bibcode": ["2019ApJ...875..111W"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "VII/286 : SDSS quasar catalog, fourteenth data release (Paris+, 2018)", "J/ApJ/596/768 : Optical depths in 19 QSOs (Schaye+, 2003)", "J/ApJ/690/1181 : UV-bright quasars (Syphers+, 2009)", "J/ApJS/185/20 : UV-bright quasars (Syphers+, 2009)", "J/ApJ/728/23 : GALEX UV-bright high-redshift quasars (Worseck+, 2011)", "J/ApJS/206/4 : SEDs for luminous QSOs (Krawczyk+, 2013)", "J/ApJ/768/105 : z~5 QSO lum. function from SDSS Stripe 82 (McGreer+, 2013)", "J/ApJ/814/40 : Nearby galaxy filaments with UV obs. (Wakker+, 2015)", "J/ApJ/818/113 : HST observations of QSOs with medium spectra (Neeleman+, 2016)", "J/ApJ/837/106 : UV bckg photoionization & photoheating rates (Onorbe+, 2017)", "J/ApJ/847/81 : HeII photoionization rates of quasars (Schmidt+, 2017)", "J/ApJS/230/6 : HST/COS & STIS absorption-line spectrosc. II. (Keeney+, 2017)", "J/ApJ/863/92 : LAE cand. at z~5.7 in the QSO J0148+0600 field (Becker+, 2018)", "J/AJ/155/131 : z~5 QSO luminosity function from the CFHTLS (McGreer+, 2018)", "J/ApJ/852/22 : Ly{alpha} forest power spectrum at 1.8~3 HeII sightlines at", "z>3.5, and study the redshift evolution and sightline-to-sightline", "variance of {tau}_eff_ in 24 HeII sightlines. We confirm an increase", "of the median {tau}_eff_ from ~2 at z=2.7 to {tau}_eff_>~5 at z>3, and", "a scatter in {tau}_eff_ that increases with redshift. The z>3.5 HeII", "absorption is predominantly saturated, but isolated narrow", "({Delta}v<650km/s) transmission spikes indicate patches of reionized", "helium. We compare our measurements to predictions for a range of UV", "background models applied to outputs of a large-volume (146 comoving", "Mpc)^3^ hydrodynamical simulation by forward-modeling our sample's", "quality and size. At z>2.74, the variance in {tau}_eff_ significantly", "exceeds expectations for a spatially uniform UV background, but is", "consistent with a fluctuating radiation field sourced by variations in", "the quasar number density and the mean free path in the", "post-reionization IGM. We develop a method to infer the approximate", "median HeII photoionization rate {Gamma}_HeII_ of a fluctuating UV", "background from the median {tau}_eff_, finding a factor ~5 decrease in", "{Gamma}_HeII_ between z~2.6 and z~3.1. At z~3.1,", "{Gamma}_HeII_=[9.1_-1.2_^+1.1^(stat)_-3.4_^+2.4^(sys)]x10^-16^s^-1^", "corresponds to a median HeII fraction of ~2.5%, indicating that our", "data probe the tail end of HeII reionization."], "description": ["Target selection was performed mainly by applying color cuts to", "combined catalogs of wide-field multiwavelength photometry. The quasar", "candidates were verified with low-resolution (R~200) optical", "spectroscopy, mainly with the Calar Alto Faint Object Spectrograph", "(CAFOS) at the Calar Alto 2.2m telescope and the Kast spectrometer at", "the Lick 3m Shane Telescope during several campaigns (2010-2015).", "Unambiguous redshifts were measured from broad emission lines", "(typically HI Ly{alpha} and CIV).", "In HST Cycles 20 and 22, we used the FUV-sensitive Cosmic Origins", "Spectrograph (COS) to obtain follow-up spectroscopy of eight", "3.12.7 quasars ", "columns": [{"name": "ID", "desc": "Quasar identifier "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "zEm", "desc": "[2.7/4] Quasar emission redshift "}, {"name": "PID", "desc": "[9350/13875] HST Program identifier "}, {"name": "Inst", "desc": "Instrument "}, {"name": "R", "desc": "[1000/16000] Spectral resolution at {lambda}=1150{AA} (R={lambda}/FWHM)"}, {"name": "Exp", "desc": "[4739/50993] Exposure time "}, {"name": "S/N", "desc": "[0/19] Signal-to-Noise ratio per pixel (1) "}, {"name": "F1500", "desc": "[0.5/21.6] Continuum flux density at 1500 Angstroms; in units of 10^-16^erg/cm^2^/s/{AA}"}, {"name": "alpha", "desc": "[-7.4/-0.4] Power-law spectral index (2) "}, {"name": "zAbs", "desc": "[0.13/0.9]? Intervening H I absorber redshift "}, {"name": "l_logNHI", "desc": "[<=~ ] Limit or uncertainty flag on logNHI "}, {"name": "logNHI", "desc": "[15.8/21.2]? Log intervening HI absorber column density"}, {"name": "f_logNHI", "desc": "b = blend "}, {"name": "Ref", "desc": "Data reference code (3) "}]}, {"name": "table5.dat", "desc": "Cumulative distributions of {tau}_eff_ in redshift ranges", "columns": [{"name": "zmin", "desc": "[2.3/3.7] Minimum redshift of the taueff subsample "}, {"name": "zmax", "desc": "[2.5/4] Maximum redshift of the taueff subsample "}, {"name": "taueff", "desc": "[1/6] Effective optical depth value ({tau}_eff_) "}, {"name": "F", "desc": "[0/1] Cumulative distribution function of taueff (F(<{tau}_eff_))"}, {"name": "l_taueff", "desc": "[0/1]? Limit flag on taueff (1) "}]}, {"name": "table7.dat", "desc": "Measured {tau}_eff_ in new or reanalyzed spectra (Table 1)", "columns": [{"name": "ID", "desc": "Quasar identifier "}, {"name": "z", "desc": "[2.56/3.84] Redshift "}, {"name": "taueff", "desc": "[1/6] Effective optical depth value ({tau}_eff_) "}, {"name": "E_taueff", "desc": "[0.02/1.2]? Upper statistical uncertainty in taueff (1)"}, {"name": "e_taueff", "desc": "[0/0.7] Lower statistical uncertainty in taueff "}, {"name": "upSys", "desc": "[0/1.4] Upper systematic uncertainty in taueff "}, {"name": "loSys", "desc": "[0/0.3] Lower systematic uncertainty in taueff "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_885_105"}} {"id": "J/ApJ/885/105", "title_cds": "", "title_create": "Rangelov+, 2019", "year": "2019", "author": "Rangelov+, Rangelov B., Montmerle T., Federman S.R., Boisse P., Gabici S.", "title_pub": "Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur Revisited.", "first_author": "Rangelov+", "bibcode": [""], "bibcode": ["2020ApJ...890...24V"], "see_also": ["VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)", "J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)", "J/MNRAS/401/1521 : Stellar masses of Lyman break gal. at z~3 (Magdis+, 2010)", "J/ApJ/719/763 : Millimeter-wave sources in the SPT survey (Vieira+, 2010)", "J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011)", "J/ApJ/745/95 : Herschel FIR & submm photom. of KINGFISH sample (Dale+, 2012)", "J/ApJ/783/84 : ALMA obs. in 107 galaxies at z=0.2-2.5 (Scoville+, 2014)", "J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014)", "J/ApJ/829/93 : CO, [CI] & [NII] lines from Herschel sp. (Kamenetzky+, 2016)", "J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)", "J/ApJS/225/27 : 3D-HST Survey: grism spectra master catalog (Momcheva+, 2016)", "J/MNRAS/465/1789 : SCUBA-2 Cosmology Legacy Survey (Geach+, 2017)", "J/ApJS/230/1 : Herschel SPIRE/FTS 194-671um survey of GOALS LIRGs (Lu+, 2017)", "J/A+A/608/A144 : Strongly lensed submm galaxies CO spectra (Yang+, 2017)", "J/A+A/609/A30 : Monochromatic conversion factors to LIR (Schreiber+, 2018)", "J/A+A/628/A23 : SPT0346-52 CO and H2O ALMA images (Apostolovski+, 2019)", "J/A+A/628/A104 : [ESS2003] Q2343-BX610 reduced PdBI spectra (Brisbin+, 2019)", "J/ApJS/244/40 : A3COSMOS. I. ALMA continuum photometry catalogs (Liu+, 2019)"], "keyword_cds": "Galaxies, radio; Carbon monoxide; Redshifts; Infrared; Interstellar medium; Millimetric/submm sources", "keyword_pub": "Galaxy evolution ; High-redshift galaxies ; Starburst galaxies ; Ultraluminous infrared galaxies ; Submillimeter astronomy ; Interstellar medium ; Star formation", "abstract": ["We report Atacama Large Millimeter Array observations of the neutral", "atomic carbon transitions [CI] and multiple CO lines in a sample of", "~30 main-sequence galaxies at z~1, including novel information on", "[CI](^3^P_2_-^3^P_1_) and CO (7-6) for 7 of such normal objects. We", "complement our observations with a collection of >200 galaxies with", "coverage of similar transitions, spanning the z=0-4 redshift interval", "and a variety of ambient conditions from local to high-redshift", "starbursts. We find systematic variations in the [CI]/IR and", "[CI]/high-J_upper_ (J_upper_=7) CO luminosity ratios among the various", "samples. We interpret these differences as increased dense molecular", "gas fractions and star formation efficiencies in the strongest", "high-redshift starbursts with respect to normal main-sequence", "galaxies. We further report constant", "L'_[CI]^3^P_2_-^3^P_1_/L'_[CI]^3^P_1_-^3^P_0_ ratios across the galaxy", "populations and redshifts, suggesting that gas temperatures T_exc_", "traced by [CI] do not strongly vary. We find only a mild correlation", "with T_dust_ and that, generally, T_exc_<~Tdust. We fit the line", "ratios with classical photodissociation region models, retrieving", "consistently larger densities and intensities of the UV radiation", "fields in submillimeter galaxies than in main-sequence and local", "objects. However, these simple models fall short in representing the", "complexity of a multiphase interstellar medium and should be treated", "with caution. Finally, we compare our observations with the Santa Cruz", "semi-analytical model of galaxy evolution, recently extended to", "simulate submillimeter emission. While we confirm the success in", "reproducing the CO lines, we find systematically larger [CI]", "luminosities at fixed IR luminosity than predicted theoretically. This", "highlights the necessity of improving our understanding of the", "mechanisms regulating the [CI] emission on galactic scales. We release", "our data compilation to the community."], "description": ["The galaxies we study here largely overlap with the sample of", "main-sequence galaxies presented in V18 (Valentino+ 2018ApJ...869...27V).", "In this work, we also present new observations of the", "[CI](^3^P_2_-^3^P_1_) and CO (7-6) transitions for 7 objects from V18", "observed during ALMA Cycle 6 (Project ID: 2018.1.00635.S,", "PI: F. Valentino) in Band 7.", "We further add recent observations of main-sequence galaxies from", "other papers, see Section 2. In total we retrieve information about", "[CI] emission in 217 galaxies. Our collection refers to published", "material prior to May 2019, to the best of our knowledge."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "highz.dat", "desc": "High-redshift sample data ", "columns": [{"name": "ID", "desc": "Identifier "}, {"name": "z", "desc": "[0.84/6.42] Spectroscopic redshift (zspec) "}, {"name": "muDust", "desc": "[1/80]?=- Magnification factor for lensed sources from dust (MagnificationFactor_dust)"}, {"name": "e_muDust", "desc": "[0/20]?=- MuDust uncertainty (e_MagnificationFactor_dust)"}, {"name": "muGas", "desc": "[1/80]?=- Magnification factor for lensed sources from molecular gas (MagnificationFactor_gas)"}, {"name": "e_muGas", "desc": "[0/20]?=- MuGas uncertainty (e_MagnificationFactor_gas)"}, {"name": "LIR", "desc": "[4.4e+10/3.5e+14] Total IR luminosity integrated within 8-1000um"}]}, {"name": "local.dat", "desc": "Local sample data ", "columns": [{"name": "ID", "desc": "Identifier (ID) "}, {"name": "Dist", "desc": "[0.7/289.7] Distance (Distance_Mpc) "}, {"name": "z", "desc": "[-0.0012/0.07] Spectroscopic redshift (zspec) "}, {"name": "LIR", "desc": "[4.7e+7/3.2e+12] Total IR luminosity integrated within 8-1000um"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_890_L22"}} {"id": "J/ApJ/890/L22", "title_cds": "VLA obs. of methanol emissions in G358.93-0.03", "title_create": "Chen+, 2020", "year": "2020", "author": "Chen X., Sobolev A.M., Breen S.L., Shen Z.-Q., Ellingsen S.P., Macleod G.C., Li B., Voronkov M.A., Kaczmarek J.F., Zhang J., Ren Z.-Y., Wang J., Linz H., Hunter T.R., Brogan C., Sugiyama K., Burns R.A., Menten K., Sanna A., Stecklum B., Hirota T., Kim K.-T., Chibueze J., Van Den Heever S.P.", "title_pub": "^13^CH_3_OH masers associated with a transient phenomenon in a high-mass young stellar object.", "first_author": "Chen X.", "ref_biblio": [""], "bibcode": ["2020ApJ...890L..22C"], "see_also": ["J/A+A/403/1095 : 6.7GHz methanol masers survey of low-mass YSO (Minier+, 2003)", "J/A+A/428/1019 : Rest frequencies of methanol maser lines (Mueller+, 2004)", "J/ApJS/206/9 : New EGOs from Spitzer GLIMPSE II survey. I. (Chen+, 2013)", "J/MNRAS/439/2584 : Southern methanol masers at 36 and 44GHz (Voronkov+, 2014)", "J/ApJ/854/170 : Methanol (CH_3_OH) and OH masers in NGC 6334I (Hunter+, 2018)"], "keyword_cds": "Masers; YSOs; Radio lines; Molecular data", "keyword_pub": "Interstellar masers; Interstellar molecules; Stellar accretion disks Star formation; Astrophysical masers", "abstract": ["We report the first detection of isotopic methanol (^13^CH_3_OH) maser", "emission in interstellar space. The emission was detected toward the", "high-mass young stellar object G358.93-0.03 during monitoring of a", "flare in the 6.7GHz methanol (CH_3_OH) maser emission in this source.", "We find that the spectral and spatial distribution of the ^13^CH_3_OH", "masers differs from the CH_3_OH masers imaged at the same epoch,", "contrary to expectations from similarity of their pumping. This", "conclusively demonstrates that isotopic methanol masers are bright", "under different physical conditions and suggests that they can provide", "additional, complementary information to the CH_3_OH masers from the", "same source. We detect a rapid decay of the ^13^CH_3_OH maser lines", "suggesting that they are transient phenomena (masing for only a few", "months), likely associated with rapid changes in radiation field due", "to an accretion burst induced by massive disk fragmentation. Changes", "in the line flux density are faster than required to achieve", "equilibrium in the energy level populations, indicating that the", "pumping of these masers is likely variable."], "description": ["The first observation of the 5_1_-6_0_ A^+^ (14.300GHz) and", "2_0_-3_-1_ E (14.782GHz) ^13^CH_3_OH transitions toward G358.93-0.03", "were undertaken with the Shanghai 65m Tianma Radio Telescope (TMRT) on", "2019 March 14. Monitoring observations of the two transitions were", "performed using the TMRT during 2019 April 2-15.", "VLA B-array observations of ^13^CH_3_OH in the 5_1_-6_0_ A^+^ and", "2_0_-3_-1_ E transitions, and CH_3_OH in the 2_0_-3-_-1_ E (12.178GHz)", "and 16_5_-17_4_ E (12.229GHz) transitions were made on 2019 March 24.", "Australia Telescope Compact Array (ATCA) observations of the 35.171GHz", "9_2_-10_1_ A^+^ transition of ^13^CH_3_OH were conducted as part of a", "series of spectral line observations on 2019 March 7", "(Breen+ 2019ApJ...876L..25B)."], "object": ["17 43 10.02 -29 51 45.8 G358.931-00.030 = MMB G358.931-00.030"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Parameters measured from the Gaussian fitting to maser spots at the ^13^CH_3_OH and CH_3_OH transitions detected from the VLA observations", "columns": [{"name": "Freq", "desc": "[12.178/14.782] Frequency "}, {"name": "Trans", "desc": "Transition (CH_3_OH or ^13^CH_3_OH) "}, {"name": "Vel", "desc": "[-19.14/-14.72] Spot velocity "}, {"name": "Flux", "desc": "[0.12/709.4] Peak flux density "}, {"name": "X", "desc": "X position (1) "}, {"name": "e_X", "desc": "[0.002/0.02] Uncertainty in X "}, {"name": "Y", "desc": "Y position (1) "}, {"name": "e_Y", "desc": "[0.003/0.03] Uncertainty in Y "}, {"name": "Tb", "desc": "[0.2/1083] Maser spot lower brightness temperature limit"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_890_97"}} {"id": "J/ApJ/890/97", "title_cds": "Multiwavelength obs. of Mrk421 in 2010 February", "title_create": "Abeysekara+, 2020", "year": "2020", "author": "Abeysekara A.U., Benbow W., Bird R., Brill A., Brose R., Buchovecky M., Buckley J.H., Christiansen J.L., Chromey A.J., Daniel M.K., Dumm J., Falcone A., Feng Q., Finley J.P., Fortson L., Furniss A., Galante N., Gent A., Gillanders G.H., Giuri C., Gueta O., Hassan T., Hervet O., Holder J., Hughes G., Humensky T.B., Johnson C.A., Kaaret P., Kar P., Kelley-Hoskins N., Kertzman M., Kieda D., Krause M., Krennrich F., Kumar S., Lang M.J., Moriarty P., Mukherjee R., Nelson T., Nieto D., Nievas-rosillo M., O'brien S., Ong R.A., Otte A.N., Park N., Petrashyk A., Pichel A., Pohl M., Prado R.R., Pueschel E., Quinn J., Ragan K., Reynolds P.T., Richards G.T., Roache E., Rovero A.C., Rulten C., Sadeh I., Santander M., Sembroski G.H., Shahinyan K., Stevenson B., Sushch I., Tyler J., Vassiliev V.V., Wakely S.P., Weinstein A., Wells R.M., Wilcox P., Wilhelm A., Williams D.A., Zitzer B., (the Veritas Collaboration), Acciari V.A., Ansoldi S., Antonelli L.A., Arbet Engels A., Baack D., Babic A., Banerjee B., Barres De Almeida U., Barrio J.A., Becerra Gonzalez J., Bednarek W., Bellizzi L., Bernardini E., Berti A., Besenrieder J., Bhattacharyya W., Bigongiari C., Biland A., Blanch O., Bonnoli G., Busetto G., Carosi R., Ceribella G., Chai Y., Cikota S., Colak S.M., Colin U., Colombo E., Contreras J.L., Cortina J., Covino S., D'Elia V., Da Vela P., Dazzi F., De Angelis A., De Lotto B., Delfino M., Delgado J., Di Pierro F., Do Souto Espinera E., Dominis Prester D., Dorner D., Doro M., Einecke S., Elsaesser D., Fallah Ramazani V., Fattorini A., Fernandez-barral A., Ferrara G., Fidalgo D., Foffano L., Fonseca M.V., Font L., Fruck C., Galindo D., Gallozzi S., Garcia Lopez R.J., Garczarczyk M., Gasparyan S., Gaug M., Godinovic N., Green D., Guberman D., Hadasch D., Hahn A., Herrera J., Hoang J., Hrupec D., Inoue S., Ishio K., Iwamura Y., Kubo H., Kushida J., Lamastra A., Lelas D., Leone F., Lindfors E., Lombardi S., Longo F., Lopez M., Lopez-Coto R., Lopez-oramas A., Machado De Oliveira Fraga B., Maggio C., Majumdar P., Makariev M., Mallamaci M., Maneva G., Manganaro M., Mannheim K., Maraschi L., Mariotti M., Martinez M., Masuda S., Mazin D., Miceli D., Minev M., Miranda J.M., Mirzoyan R., Molina E., Moralejo A., Morcuende D., Moreno V., Moretti E., Munar-Adrover P., Neustroev V., Niedzwiecki A., Nievas Rosillo M., Nigro C., Nilsson K., Ninci D., Nishijima K., Noda K., Nogues L., Nothe M., Paiano S., Palacio J., Palatiello M., Paneque D., Paoletti R., Paredes J.M., Penil P., Peresano M., Persic M., Prada Moroni P.G., Prandini E., Puljak I., Rhode W., Ribo M., Rico J., Righi C., Rugliancich A., Saha L., Sahakyan N., Saito T., Satalecka K., Schweizer T., Sitarek J., Snidaric I., Sobczynska D., Somero A., Stamerra A., Strom D., Strzys M., Sun S., Suric T., Tavecchio F., Temnikov P., Terzic T., Teshima M., Torres-Alba N., Tsujimoto S., Van Scherpenberg J., Vanzo G., Vazquez Acosta M., Vovk I., Will M., Zaric D., (the Magic Collaboration), Aller H.D., Aller M.F., Carini M.T., Horan D., Jordan B., Jorstad S.G., Kurtanidze O.M., Kurtanidze S.O., Lahteenmaki A., Larionov V.M., Larionova E.G., Madejski G., Marscher A.P., Max-Moerbeck W., Moody J.W., Morozova D.A., Nikolashvili M.G., Raiteri C.M., Readhead A.C.S., Richards J.L., Sadun A.C., Sakamoto T., Sigua L.A., Smith P.S., Talvikki H., Tammi J., Tornikoski M., Troitsky I.S., Villata M., (the Multiwavelength Partners)", "title_pub": "The great Markarian 421 flare of 2010 February: multiwavelength variability and correlation studies.", "first_author": "Abeysekara A.U.", "ref_biblio": [""], "bibcode": ["2020ApJ...890...97A"], "see_also": ["J/A+AS/132/305 : Extragal. radio sources at 22, 37 and 87GHz (Terasranta+ 1998)", "J/AJ/130/2473 : Fine-scale structure in 250 sources at 15GHz (Kovalev+, 2005)", "J/A+A/445/441 : SED of BL Lacertae objects (Nieppola+, 2006)", "J/ApJ/690/163 : The first Swift UV-Opt GRB afterglow catalog (Roming+, 2009)", "J/ApJ/722/520 : Gamma-ray light curves of Fermi blazars (Abdo+, 2010)", "J/A+A/531/A123 : Optical light curve of PKS 2155-304 (Kastendieck+, 2011)", "J/ApJS/194/29 : Observations of blazars at 15GHz (Richards+, 2011)", "J/A+A/539/A149 : Multiwavelength view of blazar PKS2155-304 (Abramowski+, 2012)", "J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)", "J/A+A/576/A126 : The 2009 multiwavelength campaign on Mrk421 (Aleksic+, 2015)", "J/A+A/578/A22 : Mrk421 in March 2010 (Aleksic+, 2015)", "J/A+A/573/A50 : Multiwavelength obs. of Mrk 501 in 2008 (Aleksic+, 2015)", "J/ApJ/846/98 : Jet kinematics of blazars at 43GHz with VLBA (Jorstad+, 2017)", "J/ApJ/858/68 : Mrk421 Swift obs. in selected epochs. II. (Kapanadze+, 2018)", "J/ApJS/234/12 : MOJAVE XV. VLBA 15GHz obs. of AGN jets (Lister+, 2018)", "J/ApJ/853/68 : Multi-epoch VLBA imaging of 20 Tev blazars (Piner+, 2018)"], "keyword_cds": "BL Lac objects; Gamma rays; Photometry, VRI", "keyword_pub": "BL Lacertae objects; Blazars; High energy astrophysics Relativistic jets; Markarian galaxies; Gamma-ray astronomy Time domain astronomy", "abstract": ["We report on variability and correlation studies using multiwavelength", "observations of the blazar Mrk 421 during the month of 2010 February,", "when an extraordinary flare reaching a level of ~27 Crab Units above", "1TeV was measured in very high energy (VHE) {gamma}-rays with the Very", "Energetic Radiation Imaging Telescope Array System (VERITAS)", "observatory. This is the highest flux state for Mrk 421 ever observed", "in VHE {gamma}-rays. Data are analyzed from a coordinated campaign", "across multiple instruments, including VHE {gamma}-ray (VERITAS, Major", "Atmospheric Gamma-ray Imaging Cherenkov), high-energy {gamma}-ray", "(Fermi-LAT), X-ray (Swift, Rossi X-ray Timing Experiment, MAXI),", "optical (including the GASP-WEBT collaboration and polarization data),", "and radio (Metsahovi, Owens Valley Radio Observatory, University of", "Michigan Radio Astronomy Observatory). Light curves are produced", "spanning multiple days before and after the peak of the VHE flare,", "including over several flare \"decline\" epochs. The main flare", "statistics allow 2 minute time bins to be constructed in both the VHE", "and optical bands enabling a cross-correlation analysis that shows", "evidence for an optical lag of ~25-55 minutes, the first time-lagged", "correlation between these bands reported on such short timescales.", "Limits on the Doppler factor ({delta}>=33) and the size of the", "emission region ({delta}^-1^R_B_<~3.8x10^13^cm) are obtained from the", "fast variability observed by VERITAS during the main flare. Analysis", "of 10 minute binned VHE and X-ray data over the decline epochs shows", "an extraordinary range of behavior in the flux-flux relationship, from", "linear to quadratic to lack of correlation to anticorrelation. Taken", "together, these detailed observations of an unprecedented flare seen", "in Mrk 421 are difficult to explain with the classic single-zone", "synchrotron self-Compton model."], "description": ["The very high energy (VHE) {gamma}-ray data comprise both the Major", "Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) and Very Energetic", "Radiation Imaging Telescope Array System (VERITAS) observations.", "Starting with the MAGIC observatory, data were taken on Mrk421 between", "MJD 55234 and 55240 (2010 February 7 and 13). VERITAS picked up the", "observations between MJD 55244 and 55247 (2010 February 17 and 20). As", "soon as VERITAS began taking Mrk 421 data on MJD 55244, VERITAS", "observed a remarkable flare. The VERITAS array is located at 1300m", "above sea level in Arizona at the Fred Lawrence Whipple Observatory.", "See Section 2.1.", "Events belonging to the Source data class with energies between 100MeV", "and 100GeV (HE) were selected and analyzed for the MJD 55230 to 55255", "Fermi-LAT observations. See Section 2.2.", "We obtained X-ray data over the period of interest from three", "different observatories: MAXI, the Rossi X-ray Timing Experiment", "(RXTE; ObsIDs: 95386 and 95133), and Swift/XRT (ObsIDs: 31630 and 30352).", "See Section 2.3.", "The UVOT on board Swift also obtained data during each observation in", "one of three UV filters (UVW2, UVM2, or UVW1) for a total of 59", "exposures. All of the data taken between 2010 February 7 and 20 were", "analyzed.", "The optical fluxes reported in this paper were obtained within the", "GASP-WEBT program (e.g., Villata+ 2008A&A...481L..79V and", "2009A&A...504L...9V), with the optical telescopes at Abastumani, Roque", "de los Muchachos (KVA), Crimean, and Lowell (Perkins) observatories.", "Additional observations were performed with the Goddard Robotic", "Telescope (GRT), Galaxy View, and New Mexico Skies.", "Additionally, high-cadence, 2 minute exposure optical R-band", "observations nearly simultaneous with VERITAS were obtained on 2010", "February 17 with the 1.3m Robotically Controlled Telescope (RCT)", "located at Kitt Peak National Observatory. The RCT observations", "started ~50 minutes after the beginning of the VERITAS observations", "and ended ~15 minutes after VERITAS stopped observing.", "Optical polarization observations of Mrk 421 were made during the HE", "monitoring campaign by the Steward Observatory 2.3m Bok Telescope on", "Kitt Peak, Arizona. The source was observed on seven consecutive", "nights from 2010 February 13 (MJD 55240) through 2010 February 19 (MJD", "55246) using the SPOL imaging/spectropolarimeter.", "See Section 2.4.", "Contemporaneous radio data were taken with the 40m Owens Valley Radio", "Observatory (OVRO) telescope at 15GHz, the 26m University of Michigan", "Radio Astronomy Observatory (UMRAO) at 14 and 8GHz, and the 14m", "Metsahovi Radio Observatory at 37GHz.", "See Section 2.5."], "object": ["11 04 27.31 +38 12 31.8 Mrk 421 = 3FHL J1104.4+3812"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "fig1-vhe.dat", "desc": "VHE VERITAS and MAGIC observations ", "columns": [{"name": "MJD", "desc": "[55230.1/55255.2] Time "}, {"name": "e_MJD", "desc": "[0.01/1] Time binsize "}, {"name": "Flux", "desc": "[1.6e-10/2.6e-9] Flux in photons/cm2/s "}, {"name": "e_Flux", "desc": "[2e-12/1.4e-10] Flux uncertainty "}]}, {"name": "fig1-he.dat", "desc": "HE Fermi-LAT observations? ", "columns": [{"name": "MJD", "desc": "[55230.1/55255.2] Time "}, {"name": "e_MJD", "desc": "[0.01/1] Time binsize "}, {"name": "Flux", "desc": "[1.6e-10/2.6e-9] Flux in photons/cm2/s "}, {"name": "e_Flux", "desc": "[2e-12/1.4e-10] Flux uncertainty "}]}, {"name": "fig1-maxi.dat", "desc": "Hard X-ray MAXI observations? ", "columns": [{"name": "MJD", "desc": "[55230.1/55255.2] Modified Julian Date "}, {"name": "e_MJD", "desc": "[0.01/1] Time binsize "}, {"name": "Rate", "desc": "[1.6e-10/2.6e-9] Flux in photons/s "}, {"name": "e_Rate", "desc": "[2e-12/1.4e-10] Flux uncertainty "}]}, {"name": "fig1-rxte.dat", "desc": "X-ray RXTE observations ", "columns": [{"name": "MJD", "desc": "[55230.1/55255.2] Time "}, {"name": "e_MJD", "desc": "[0.01/1] Time binsize "}, {"name": "Flux", "desc": "[1.6e-10/2.6e-9] X-ray flux in erg/cm2/s "}, {"name": "e_Flux", "desc": "[2e-12/1.4e-10] Flux uncertainty or negative error on Flux"}, {"name": "E_Flux", "desc": "[1.7e-12/1.4e-11]? Positive error on Flux "}]}, {"name": "fig1-xrt.dat", "desc": "X-ray Swift-XRT observations ", "columns": [{"name": "MJD", "desc": "[55230.1/55255.2] Time "}, {"name": "e_MJD", "desc": "[0.01/1] Time binsize "}, {"name": "Flux", "desc": "[1.6e-10/2.6e-9] X-ray flux in erg/cm2/s "}, {"name": "e_Flux", "desc": "[2e-12/1.4e-10] Flux uncertainty or negative error on Flux"}, {"name": "E_Flux", "desc": "[1.7e-12/1.4e-11]? Positive error on Flux "}]}, {"name": "fig1-uvw2.dat", "desc": "Swift-UVOT UVW2 observations ", "columns": []}, {"name": "fig1-uvm2.dat", "desc": "Swift-UVOT UVM2 observations ", "columns": []}, {"name": "fig1-uvw1.dat", "desc": "Swift-UVOT UVW1 observations ", "columns": []}, {"name": "fig1-opt.dat", "desc": "Optical observations in R-band ", "columns": [{"name": "MJD", "desc": "[55228.4/55255.2] Modified Julian Date of observation (OPT_TIME)"}, {"name": "Flux", "desc": "[7.8/24.11] R-band flux density (OPT_FLUXD) "}, {"name": "e_Flux", "desc": "[0.02/1.3] Flux uncertainty (OPT_FLUXD_ERR) "}, {"name": "Inst", "desc": "Optical instrument (OPT_INSTR) (1) "}]}, {"name": "fig1-rad.dat", "desc": "Radio observations ", "columns": [{"name": "MJD", "desc": "[55228.4/55255.2] Modified Julian Date of observation (RADIO_TIME)"}, {"name": "Flux", "desc": "[7.8/24.11] Radio flux density in Freq (RADIO_FLUXD)"}, {"name": "e_Flux", "desc": "[0.02/1.3] Flux uncertainty (RADIO_FLUXD_ERR) "}, {"name": "Inst", "desc": "Radio instrument (RADIO_INSTR) (1) "}, {"name": "Freq", "desc": "Frequence of observation (RADIO_INSTR2) "}]}, {"name": "fig1-pol.dat", "desc": "Steward SPOL observations ", "columns": [{"name": "MJD", "desc": "[55240.8/55246.8] Modified Julian Date of observation (POL_TIME)"}, {"name": "Pol", "desc": "[1/3.5] Polarization (PPOL) "}, {"name": "e_Pol", "desc": "[0.02/0.03] Pol uncertainty (PPOL_ERR) "}, {"name": "PA", "desc": "[125.8/155.1] Polarization angle "}, {"name": "e_PA", "desc": "[0.2/0.6] PA uncertainty "}]}, {"name": "fig2_1.dat", "desc": "2 minute bins light curve for VERITAS Mrk421 data above 110GeV for the first 2.33hr of observations on MJD 55244", "columns": [{"name": "MJD", "desc": "[55244.3/55244.4] Modified Julian Date of observation (VER_2min_TIME)"}, {"name": "e_MJD", "desc": "[0.0013888] MJD uncertainty (always \"0.0013888\")"}]}, {"name": "fig2_2.dat", "desc": "5 minute bins light curve for VERITAS Mrk421 data above 110GeV for the first 2.33hr of observations on MJD 55244", "columns": [{"name": "MJD", "desc": "[55244.3/55244.4] Modified Julian Date of observation (VER_5min_TIME)"}, {"name": "e_MJD", "desc": "[0.00347222] MJD uncertainty (always \"0.00347222\")"}]}, {"name": "fig4r.dat", "desc": "RCT optical R-band photometry during MJD 55244 ", "columns": [{"name": "MJD", "desc": "Modified Julian Date (RCT_TIME) "}, {"name": "Bin", "desc": "[0.0013888] RCT time binsize (always \"0.0013888\") (RCT_TIME_BINSIZE)"}, {"name": "FR", "desc": "[17.98/20.33] RCT R-band flux density (RCT_FLUXD) "}, {"name": "e_FR", "desc": "[0.34/0.38] FR uncertainty (RCT_FLUXD_ERR) "}]}, {"name": "fig4gev.dat", "desc": "VERITAS >420GeV data during MJD 55244 ", "columns": [{"name": "MJD", "desc": "Modified Julian Date (VER_TIME) "}, {"name": "Bin", "desc": "[0.0013888] VERITAS time binsize (always \"0.0013888\") (VER_TIME_BINSIZE)"}, {"name": "Flux", "desc": "[4.6e-6/1.5e-5] VERITAS >420GeV flux (VER_FLUX) "}, {"name": "e_Flux", "desc": "[6.9e-7/2.1e-6] Flux uncertainty (VER_FLUX_ERR) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_902_62"}} {"id": "J/ApJ/902/62", "title_cds": "WR 121-16: a new Wolf-Rayet WN/C star in the MW", "title_create": "Zhang+, 2020", "year": "2020", "author": "Zhang W., Todt H., Wu H., Shi J., Hsia C.-H., Wu Y., Wu C., Zhao Y., Zhang T., Hou Y.", "title_pub": "A new transition Wolf-Rayet WN/C star in the Milky Way.", "first_author": "Zhang W.", "ref_biblio": [""], "bibcode": ["2020ApJ...902...62Z"], "see_also": ["III/215 : 7th Catalog of Galactic Wolf-Rayet stars (van der Hucht, 2001)", "I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)", "V/146 : LAMOST DR1 catalogs (Luo+, 2015)", "J/MNRAS/381/418 : Wolf-Rayet population in NGC 1313 (Hadfield+, 2007)", "J/ApJ/764/21 : Stellar evolutionary models with 13-120Msun (Chieffi+, 2013)"], "keyword_cds": "Stars, Wolf-Rayet; Spectra, optical", "keyword_pub": "Wolf-Rayet stars ; Massive stars ; Stellar distance ; Galaxy stellar content", "abstract": ["We report the discovery of a new transition type Wolf-Rayet (W-R) WN/C", "star in the Galaxy. According to its coordinates", "RAJ2000=18:51:39.7,DEJ2000=-05:34:51.1, and the distance", "(7.11_-1.22_^+1.56^kpc away from Earth) inferred from the second Gaia", "data release, it is found that W-R 121-16 is located in the Far 3kpc", "Arm, and it is 3.75kpc away from the Galactic Center. The optical", "spectra obtained by the Large Sky Area Multi-Object Fiber", "Spectroscopic Telescope and the 2.16m telescope, both located at the", "Xinglong Observatory in China, indicate that this is a W-R star of the", "transitional WN7o/WC subtype. A current stellar mass of about", "7.1_-1.1_^+1.7^M_{sun}_, a mass- loss rate of", "dM/dt=10^-4.97^(_-0.20_^+0.16^)M_{sun}_/yr, a bolometric luminosity of", "log L/L_{sun}_=4.88_-0.15_^+0.17^, and a stellar temperature of", "T_*_=47_-5_^+9^kK are derived by fitting the observed spectrum with a", "specific Potsdam W-R model. The magnitude in V-band varies between", "13.95 and 14.14mag, while no period is found. Based on the optical", "spectra, the time domain data, and the indices of the astrometric", "solution of the Gaia data, W-R 121-16 is likely a transitional WN/C", "single star rather than a WN+WC binary."], "description": ["The LAMOST low-resolution (R~1800) spectrum of WR 121-16 obtained on", "2014 September 9, with an exposure time of 1800s, shows strong", "nitrogen lines, such as NIII{lambda}4634-{lambda}4641 blend,", "NIV{lambda}4057, {lambda}7109, {lambda}7123. The HeI and HeII lines", "are also strong. The CIV{lambda}5808 line is strong, while", "CIII{lambda}5696 line cannot be detected.", "We also carried out the followup observations using the BAO Faint", "Object Spectrograph and Camera (BFOSC) on the 2.16m telescope at the", "Xinglong Observatory in China on 2019 October 30 and 31, with an", "exposure time of 1200s on each night (spectral coverage roughly from", "3250 to 8850{AA} with a resolving power R~1600)."], "object": ["18 51 39.71 -05 34 51.1 WR 121-16 = ASASSN-V J185139.71-053451.1"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "bfosc30.dat", "desc": "BFOSC/2.16m telescope spectrum from 2019-10-30 ", "columns": [{"name": "lambda", "desc": "[3241.8/8850.6] Wavelength in Angstroms "}, {"name": "Flux", "desc": "[-2.4/3.4] Flux in 10^-14^erg/s/cm^2^/{AA} "}]}, {"name": "bfosc31.dat", "desc": "BFOSC/2.16m telescope spectrum from 2019-10-31 ", "columns": [{"name": "lambda", "desc": "[3241.8/8850.6] Wavelength in Angstroms "}, {"name": "Flux", "desc": "[-2.4/3.4] Flux in 10^-14^erg/s/cm^2^/{AA} "}]}, {"name": "lamost.dat", "desc": "LAMOST spectrum from 2014-09-09 ", "columns": [{"name": "lambda", "desc": "[3698.9/9096.7] Wavelength in Angstroms "}, {"name": "Flux", "desc": "[0.23/6.27]?=0 Flux in 10^-14^erg/s/cm^2^/{AA}"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_879_125"}} {"id": "J/ApJ/879/125", "title_cds": "", "title_create": "Zucker+, 2019", "year": "2019", "author": "Zucker C., Speagle J.S., Schlafly E.F., Green G.M., Finkbeiner D.P., Goodman A.A., Alves J.", "title_pub": "A Large Catalog of Accurate Distances to Local Molecular Clouds: The Gaia DR2 Edition.", "first_author": "Zucker C.", "bibcode": [""], "bibcode": ["2019ApJ...884L..42K"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "V/153 : LAMOST DR4 catalogs (Luo+, 2018)", "J/ApJS/192/2 : A Bayesian search for binaries in Hipparcos (Shaya+, 2011)", "J/other/RAA/11.924 : Atmospheric parameters for 771 stars (Wu+, 2011)", "J/AJ/144/102 : Wide companions to Hipparcos stars (Tokovinin+, 2012)", "J/A+A/583/A85 : Binaries in beta Pic moving group (Alonso-Floriano+, 2015)", "J/MNRAS/472/675 : Wide bin. in Tycho-Gaia: search method (Andrews+, 2017)", "J/AJ/153/259 : GAMBLES extension of the SLoWPoKES cat. (Oelkers+, 2017)", "J/AJ/153/257 : Comoving stars in Gaia DR1 (Oh+, 2017)", "J/MNRAS/473/5393 : Wide binaries in Tycho-Gaia (Andrews+, 2018)", "J/AJ/155/149 : Co-moving stars observed by Gaia (Bochanski+, 2018)", "J/AJ/157/78 : Multiple star syst. from Gaia DR2 (Jimenez-Esteban+, 2019)"], "keyword_cds": "Stars, double and multiple; Abundances, [Fe/H]; Proper motions; Radial velocities; Stars, distances", "keyword_pub": "Galaxy: evolution ; Galaxy: kinematics and dynamics ; open clusters and associations: general", "abstract": ["It is challenging to reliably identify stars that were born together", "outside of actively star-forming regions and bound stellar systems.", "However, conatal stars should be present throughout the Galaxy, and", "their demographics can shed light on the clustered nature of star", "formation and the dynamical state of the disk. In previous work we", "presented a set of simulations of the Galactic disk that followed the", "clustered formation and dynamical evolution of 4 billion individual", "stars over the last 5Gyr. The simulations predict that a high fraction", "of comoving stars with physical and 3D velocity separation of", "{Delta}r<20pc and {Delta}v<1.5km/s are conatal. In this Letter, we use", "Gaia DR2 and LAMOST DR4 data to identify and study comoving pairs. We", "find that the distribution of relative velocities and separations of", "pairs in the data is in good agreement with the predictions from the", "simulation. We identify 111 comoving pairs in the solar neighborhood", "with reliable astrometric and spectroscopic measurements. These pairs", "show a strong preference for having similar metallicities when", "compared to random field pairs. We therefore conclude that these pairs", "were very likely born together. The simulations predict that conatal", "pairs are born in clusters that follow the overall cluster mass", "function and in relatively young (<1Gyr) star clusters. Gaia will", "eventually deliver well-determined metallicities for the brightest", "stars, enabling the identification of thousands of conatal pairs due", "to disrupting star clusters in the solar neighborhood."], "type": ["CCC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "star1.dat", "desc": "Co-moving pairs in Gaia DR2 + LAMOST DR4 -- primary star data", "columns": [{"name": "Gaia", "desc": "Gaia DR2 identifier (gidp) "}, {"name": "Xgal", "desc": "[-8.96/-7.68] Galactocentric X (xp) "}, {"name": "Ygal", "desc": "[-0.37/0.58] Galactocentric Y (yp) "}, {"name": "Zgal", "desc": "[-0.37/0.52] Galactocentric Z (zp) "}, {"name": "VX", "desc": "[-61.9/74.6] Galactocentric VX (vxp) "}, {"name": "VY", "desc": "[189.9/280.1] Galactocentric VY (vyp) "}, {"name": "VZ", "desc": "[-34.5/25.6] Galactocentric VZ (vzp) "}, {"name": "RAdeg", "desc": "[0.3/358.8] Right ascension (J2000) (rap) "}, {"name": "DEdeg", "desc": "[-7.4/57.8] Declination (J2000) (decp) "}, {"name": "plx", "desc": "[1/10.7] Parallax (parallaxp) "}, {"name": "pmRA", "desc": "[-70/352] Proper motion in right ascension (pmrap)"}, {"name": "pmDE", "desc": "[-76/50] Proper motion in declination (pmdecp) "}, {"name": "RV", "desc": "[-67/52] Radial velocity (rvp) "}, {"name": "Gmag", "desc": "[9/13.3] Gaia G-band magnitude (Gmagp) "}, {"name": "BP-RP", "desc": "[0.4/1.8] BP-RP color index (bp_rpp) "}, {"name": "obsid", "desc": "LAMOST observation ID (obsidp) "}, {"name": "snru", "desc": "[0.3/203] SNR in u-band (snrup) "}, {"name": "snrg", "desc": "[14/598] SNR in g-band (snrgp) "}, {"name": "snrr", "desc": "[34/999] SNR in r-band (snrrp) "}, {"name": "snri", "desc": "[40/999] SNR in i-band (snrip) "}, {"name": "snrz", "desc": "[24/999] SNR in z-band (snrzp) "}, {"name": "Teff", "desc": "[3901/7580] LAMOST effective temperature (teffp)"}, {"name": "e_Teff", "desc": "[8/287] Teff uncertainty (teff_errp) "}, {"name": "logg", "desc": "[2.7/4.9] Log of surface gravity (loggp) "}, {"name": "[Fe/H]", "desc": "[-0.7/0.6] Metallicity (fehp) "}, {"name": "e_[Fe/H]", "desc": "[0.007/0.3] Uncertainty in [Fe/H] (feherrp) "}, {"name": "Sep", "desc": "[0.002/0.02] 3D separation (dr) "}, {"name": "delV", "desc": "[0.3/1.5] 3D velocity difference (dv) "}, {"name": "Conn", "desc": "[2] Connectivity (2=mutually exclusive) "}, {"name": "dfeh", "desc": "[0.002/0.9] Difference in [Fe/H] for pair (dfeh)"}, {"name": "dteff", "desc": "[1.4/198.3] Difference in effective temperature for pair (dteff)"}, {"name": "RUWE", "desc": "[0.7/1.7] Re-normalised unit weight error "}, {"name": "Nvis", "desc": "[8/21] Number of visibility periods (nvs) "}, {"name": "Nrvt", "desc": "[3/27] Number of radial velocity transits (rvnbs)"}, {"name": "Dist", "desc": "[93/878] Distance to star (dists) "}]}, {"name": "star2.dat", "desc": "Co-moving pairs in Gaia DR2 + LAMOST DR4 -- secondary star data", "columns": [{"name": "Gaia", "desc": "Gaia DR2 identifier (gidp) "}, {"name": "Xgal", "desc": "[-8.96/-7.68] Galactocentric X (xp) "}, {"name": "Ygal", "desc": "[-0.37/0.58] Galactocentric Y (yp) "}, {"name": "Zgal", "desc": "[-0.37/0.52] Galactocentric Z (zp) "}, {"name": "VX", "desc": "[-61.9/74.6] Galactocentric VX (vxp) "}, {"name": "VY", "desc": "[189.9/280.1] Galactocentric VY (vyp) "}, {"name": "VZ", "desc": "[-34.5/25.6] Galactocentric VZ (vzp) "}, {"name": "RAdeg", "desc": "[0.3/358.8] Right ascension (J2000) (rap) "}, {"name": "DEdeg", "desc": "[-7.4/57.8] Declination (J2000) (decp) "}, {"name": "plx", "desc": "[1/10.7] Parallax (parallaxp) "}, {"name": "pmRA", "desc": "[-70/352] Proper motion in right ascension (pmrap)"}, {"name": "pmDE", "desc": "[-76/50] Proper motion in declination (pmdecp) "}, {"name": "RV", "desc": "[-67/52] Radial velocity (rvp) "}, {"name": "Gmag", "desc": "[9/13.3] Gaia G-band magnitude (Gmagp) "}, {"name": "BP-RP", "desc": "[0.4/1.8] BP-RP color index (bp_rpp) "}, {"name": "obsid", "desc": "LAMOST observation ID (obsidp) "}, {"name": "snru", "desc": "[0.3/203] SNR in u-band (snrup) "}, {"name": "snrg", "desc": "[14/598] SNR in g-band (snrgp) "}, {"name": "snrr", "desc": "[34/999] SNR in r-band (snrrp) "}, {"name": "snri", "desc": "[40/999] SNR in i-band (snrip) "}, {"name": "snrz", "desc": "[24/999] SNR in z-band (snrzp) "}, {"name": "Teff", "desc": "[3901/7580] LAMOST effective temperature (teffp)"}, {"name": "e_Teff", "desc": "[8/287] Teff uncertainty (teff_errp) "}, {"name": "logg", "desc": "[2.7/4.9] Log of surface gravity (loggp) "}, {"name": "[Fe/H]", "desc": "[-0.7/0.6] Metallicity (fehp) "}, {"name": "e_[Fe/H]", "desc": "[0.007/0.3] Uncertainty in [Fe/H] (feherrp) "}, {"name": "Sep", "desc": "[0.002/0.02] 3D separation (dr) "}, {"name": "delV", "desc": "[0.3/1.5] 3D velocity difference (dv) "}, {"name": "Conn", "desc": "[2] Connectivity (2=mutually exclusive) "}, {"name": "dfeh", "desc": "[0.002/0.9] Difference in [Fe/H] for pair (dfeh)"}, {"name": "dteff", "desc": "[1.4/198.3] Difference in effective temperature for pair (dteff)"}, {"name": "RUWE", "desc": "[0.7/1.7] Re-normalised unit weight error "}, {"name": "Nvis", "desc": "[8/21] Number of visibility periods (nvs) "}, {"name": "Nrvt", "desc": "[3/27] Number of radial velocity transits (rvnbs)"}, {"name": "Dist", "desc": "[93/878] Distance to star (dists) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_909_106"}} {"id": "J/ApJ/909/106", "title_cds": "R-band LC and spectrum of a superstellar flare", "title_create": "Xin+, 2021", "year": "2021", "author": "Xin L.P., Li H.L., Wang J., Han X.H., Xu Y., Meng X.M., Cai H.B., Huang L., Lu X.M., Qiu Y.L., Wang X.G., Liang E.W., Dai Z.G., Wang X.Y., Wu C., Zhang J.B., Li G.W., Turpin D., Feng Q.C., Deng J.S., Sun S.S., Zheng T.C., Yang Y.G., Wei J.Y.", "title_pub": "A {Delta}R~9.5mag superflare of an ultracool star detected by the SVOM/GWAC system.", "first_author": "Xin L.P.", "ref_biblio": [""], "bibcode": ["2021ApJ...909..106X"], "see_also": ["V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)", "I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)", "J/A+A/333/231 : O-M stars model atmospheres (Bessell+ 1998)", "J/A+A/487/293 : Em. lines in a giant flare of CN Leo (Fuhrmeister+, 2008)", "J/AJ/141/97 : SDSS DR7 M dwarfs (West+, 2011)", "J/MNRAS/435/2161 : Catalogue of bright (K<9) M dwarfs (Frith+, 2013)", "J/ApJS/207/15 : M dwarf flare spectra (Kowalski+, 2013)", "J/ApJ/794/120 : Sloan Digital Sky Survey coadd. Stripe 82 (Annis+, 2014)", "J/AJ/149/158 : The BUD sample. I. L dwarf activity sample (Schmidt+, 2015)", "J/ApJ/829/23 : Stellar flares from Q0-Q17 Kepler LCs (Davenport, 2016)", "J/ApJ/858/55 : K2 ultracool dwarfs survey. III. Flares (Paudel+, 2018)", "J/A+A/623/A127 : Homogeneous sample of 34000 M7-M9.5 dwarfs (Ahmed+, 2019)", "J/ApJ/876/115 : Optical follow-up of ASAS-SN M dwarf flares (Schmidt+, 2019)"], "keyword_cds": "Stars, flare; Photometry, RI; Spectra, optical", "keyword_pub": "Flare stars ; M dwarf stars ; Stellar flares ; Spectroscopy", "abstract": ["We report the detection and follow-up of a superstellar flare", "GWAC181229A with an amplitude of {Delta}R~9.5mag on an M9-type star by", "SVOM/GWAC and the dedicated follow-up telescopes. The estimated", "bolometric energy Ebol is (5.56-9.25)x10^34^erg, which makes the event", "one of the most powerful flares seen on ultracool stars. The magnetic", "strength is inferred to be 3.6-4.7kG. Thanks to sampling with a", "cadence of 15s, a new component near the peak time with a very steep", "decay is detected in the R-band light curve, followed by the", "two-component flare template given by Davenport+ (2014ApJ...797..122D).", "An effective temperature of 5340+/-40K is measured by fitting a", "blackbody shape to the spectrum in the shallower phase during the", "flare. The filling factors of the flare are estimated to be ~30% and", "19% at the peak time and at 54 minutes after the first detection. The", "detection of this particular event with large amplitude, huge emitted", "energy, and a new component demonstrates that high-cadence sky", "monitoring cooperation with fast follow-up observations is very", "important for understanding the violent magnetic activity."], "description": ["On 2018 December 29 UT10:42:51, an alert was generated by the", "Ground-based Wide Angle Cameras (GWAC) online pipelines for a very", "bright optical transient (GWAC 181229A) during a survey for one", "predefined field from 10:03:07.8 to 14:55:21.0 UT on the same night.", "The GWAC system located at Xinglong observatory of the National", "Astronomical Observatories of China (NAOC) is an optical transient", "survey that images the sky in the optical down to R~16.0mag.", "When the flare was triggered by the GWAC real-time pipeline, it was", "immediately followed-up by the Guangxi-NAOC 60cm optical telescope", "(F60A) in the standard Johnson-Cousins R band. See Section 3.1.", "One long-slit spectrum was obtained by the NAOC 2.16m telescope by", "using the Beijing Faint Object Spectrograph and Camera (BFOSC) via a", "Target of Opportunity request. The observation start time for the", "spectrum was at 11:21:51.0 UT, 39 minutes after the trigger time. The", "exposure time was 30 minutes. The spectral resolution is ~10{AA} for a", "wavelength coverage of 3850-8000{AA}. See Section 3.2."], "object": ["01 33 33.08 +00 32 23.0 GWAC 181229A = GWAC 181229A"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "fig2.dat", "desc": "R-band light curve of GWAC181229A ", "columns": [{"name": "JD", "desc": "Julian Date of the observation "}, {"name": "Exp", "desc": "[10/150] Exposure time "}, {"name": "Rmag", "desc": "[13.49/19.1] Apparent R band magnitude "}, {"name": "e_Rmag", "desc": "[0.03/0.6] Uncertainty in Rmag "}, {"name": "Tel", "desc": "Telescope code (1) "}]}, {"name": "fig6.dat", "desc": "The spectrum obtained by the 2.16m telescope at Xinglong observatory, China", "columns": [{"name": "lambda", "desc": "[3731.84/8691.75] Wavelength; Angstroms "}, {"name": "Flux", "desc": "[-3.42e-16/1.6e-15] Flux; in erg/s/cm^2^/Angstrom units"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_896_173"}} {"id": "J/ApJ/896/173", "title_cds": "", "title_create": "Phillips+, 2020", "year": "2020", "author": "Phillips C.L., Bowler B.P., Mace G., Liu M.C., Sokal K.", "title_pub": "2MASS J04435686+3723033 B: A Young Companion at the Substellar Boundary with Potential Membership in the.", "first_author": "Phillips C.L.", "bibcode": [""], "bibcode": ["2021ApJ...912...19D"], "see_also": ["I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)", "J/AJ/99/1079 : Nova rate in NGC 5128 (Ciardullo+, 1990)", "J/AJ/134/2340 : Membership of Praesepe & Coma Berenices (Kraus+, 2007)", "J/ApJS/187/275 : Photometric histories of recurrent novae (Schaefer, 2010)", "J/AJ/140/34 : Classification of nova light curves (Strope+, 2010)", "J/ApJ/743/156 : NEOWISE obs. of NEOs: preliminary results (Mainzer+, 2011)", "J/A+A/554/A123 : Near-IR catalog of novae in VVV survey area (Saito+, 2013)", "J/ApJ/792/30 : NEOWISE magnitudes for near-Earth objects (Mainzer+, 2014)", "J/ApJS/227/1 : HST survey for novae in M87. I. VI LCs (Shara+, 2016)", "J/MNRAS/465/3039 : Eruptive variable protostars from VVV EW (Contreras+, 2017)", "J/MNRAS/465/3011 : VVV high amplitude NIR var. stars (Contreras Pena+, 2017)", "J/ApJ/834/196 : Galactic novae with m<=10 from 1900 to 2015 (Shafter, 2017)", "J/ApJ/905/58 : The local universe. I. Ca-rich gap transients (De+, 2020)", "J/ApJ/910/120 : Dwarf nova outbursts detected by ASAS-SN (Kawash+, 2021)"], "keyword_cds": "Novae; Photometry, infrared; Surveys; Spectra, optical; Spectra, infrared;", "keyword_pub": "Classical novae ; Novae ; Cataclysmic variable stars ; White dwarf stars ; Interstellar dust extinction", "abstract": ["The nova rate in the Milky Way remains largely uncertain, despite its", "vital importance in constraining models of Galactic chemical evolution", "as well as understanding progenitor channels for Type Ia supernovae.", "The rate has been previously estimated to be in the range of", "~10-300yr^-1^, either based on extrapolations from a handful of very", "bright optical novae or the nova rates in nearby galaxies; both", "methods are subject to debatable assumptions. The total discovery rate", "of optical novae remains much smaller (~5-10/yr) than these estimates,", "even with the advent of all-sky optical time-domain surveys. Here, we", "present a systematic sample of 12 spectroscopically confirmed Galactic", "novae detected in the first 17 months of Palomar Gattini-IR (PGIR), a", "wide-field near-infrared time-domain survey. Operating in the J band", "(~1.2{mu}m), which is significantly less affected by dust extinction", "compared to optical bands, the extinction distribution of the PGIR", "sample is highly skewed to a large extinction values (>50% of events", "obscured by A_V_>~5mag). Using recent estimates for the distribution", "of Galactic mass and dust, we show that the extinction distribution of", "the PGIR sample is commensurate with dust models. The PGIR extinction", "distribution is inconsistent with that reported in previous optical", "searches (null-hypothesis probability <0.01%), suggesting that a large", "population of highly obscured novae have been systematically missed in", "previous optical searches. We perform the first quantitative", "simulation of a 3{pi} time-domain survey to estimate the Galactic nova", "rate using PGIR, and derive a rate of ~43.7_-8.7_^+19.5^yr^-1^. Our", "results suggest that all-sky near-infrared time-domain surveys are", "well poised to uncover the Galactic nova population."], "description": ["In this paper, we present a sample of 12 spectroscopically confirmed", "novae detected in the first 17 months -- between 2019 July 2 (the", "start date of the survey when the reference image construction was", "completed) and 2020 November 30 (the end of the 2020 Galactic bulge", "season in the northern hemisphere) -- of the Palomar Gattini-IR (PGIR)", "NIR time-domain survey (Moore & Kasliwal 2019NatAs...3..109M and De+", "2020PASP..132b5001D). PGIR is a robotic, wide-field time-domain survey", "at the Palomar Observatory using a 25deg^2^ J-band camera to survey", "the entire northern visible sky ({delta}>-28.9{deg}; ~15000deg^2^) at", "a cadence of ~2 nights.", "In order to determine spectroscopic classifications of confirmed", "novae, we obtained medium resolution optical and IR spectroscopic", "follow-up (see Figure 3) using the Palomar 200 inch telescope (P200)", "using the optical Double Spectrograph (DBSP) and NIR Triple", "spectrograph (TSpec) at the Palomar Observatory, the NASA Infrared", "Telescope Facility (IRTF) and Keck I telescopes at Maunakea, and the", "Australian National University 2.3m telescope at Siding Spring", "Observatory (SSO) using the Wide-field Spectrograph (WiFeS).", "The IRTF data were acquired with the SpeX instrument in the SXD mode", "(~0.7-2.5um) as part of programs 2020A111 and 2020B087 (PI: K. De).", "The Keck spectrum of PGIR 20ekz was acquired using the Low Resolution", "Imaging Spectrometer (LRIS)."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "*Summary of novae detected in the first 17 months of the PGIR survey (see the Appendix for details)", "columns": [{"name": "---", "desc": "[PGIR] "}, {"name": "PGIR", "desc": "PGIR name "}, {"name": "Name", "desc": "Name of the nova "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "MJD", "desc": "[58685.2/59180.3] Modified Julian Date, first detection (1)"}, {"name": "Jmag", "desc": "[6.22/12.07] Peak J-band Vega magnitude (2) "}, {"name": "e_Jmag", "desc": "[0.01/0.03] Uncertainty on the Jmag "}, {"name": "phCl", "desc": "Photometric class of the nova based on classification schemes of"}, {"name": "J/AJ/140/34", "desc": " "}, {"name": "spCl", "desc": "Spectroscopic class of the nova based on classification schemes of"}]}, {"name": "lcs/*", "desc": "Individual light curve in ASCII format ", "columns": [{"name": "JD", "desc": "Julian Date of observation "}, {"name": "l_Jmag", "desc": "5 sigma upper limit "}, {"name": "Jmag", "desc": "[6.2/14.8] PGIR J band magnitude "}, {"name": "e_Jmag", "desc": "[0/0.21]?=-99 Uncertainty in Jmag "}]}, {"name": "sp/*", "desc": "Individual spectrum in ASCII format ", "columns": [{"name": "lambda", "desc": "[3081/25704] Wavelength "}, {"name": "Flux", "desc": "[-1.8e+1/5e+4]?=- Flux in erg/s/cm^2^/{AA} units"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_888_L9"}} {"id": "J/ApJ/888/L9", "title_cds": "Chemical homogeneity of 14 wide binary star systems", "title_create": "Nagar+, 2020", "year": "2020", "author": "Nagar T., Spina L., Karakas A.I.", "title_pub": "The chemical signatures of planetary engulfment events in binary systems.", "first_author": "Nagar T.", "ref_biblio": [""], "bibcode": ["2020ApJ...888L...9N"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/A+A/420/683 : Equivalent widths of 23 wide binaries (Desidera+, 2004)", "J/ApJ/709/447 : Chemical composition of OGLE-2007-BLG-514S (Epstein+, 2010)", "J/A+A/561/A7 : High-precision abund. for stars with planets (Ramirez+, 2014)", "J/ApJ/791/14 : 18 Sco atomic data and equivalent widths (Melendez+, 2014)", "J/ApJ/795/23 : Line list for stellar chemical abundances (Bedell+, 2014)", "J/ApJ/801/L10 : XO-2N and XO-2S equivalent widths (Teske+, 2015)", "J/A+A/583/A135 : XO-2N and XO-2S spectra (Biazzo+, 2015)", "J/ApJ/819/19 : Equivalent widths of WASP-94A and WASP-94B (Teske+, 2016)", "J/A+A/588/A81 : Line list and abundances of the binary zet2 Ret (Saffe+, 2016)", "J/A+A/589/A17 : Abundances of solar twin HIP 100963 (Yana Galarza+, 2016)", "J/AJ/152/167 : Radial velocities of HD 133131A and HD 133131B (Teske+, 2016)", "J/A+A/604/L4 : HAT-P-4 & TYC 2569-744-1 abundances and spectra (Saffe+, 2017)", "J/MNRAS/474/2580 : Evolution of neutron-capture elements (Spina+, 2018)", "J/A+A/614/A138 : HD 80606/80607 equivalent widths (Lui+, 2018)", "J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018)", "J/ApJ/865/68 : Abundances for 79 Sun-like stars within 100pc (Bedell+, 2018)", "J/A+A/618/A132 : PMS stars evolutionary models. II (Kunitomo+, 2018)"], "keyword_cds": "Abundances; Stars, double and multiple; Exoplanets; Equivalent widths; Abundances, peculiar", "keyword_pub": "Chemical abundances; Stellar abundances; Wide binary stars; Exoplanets Chemically peculiar stars", "abstract": ["Planetary engulfment events involve the chemical assimilation of a", "planet into a star's external layer. This can cause a change in the", "chemical pattern of the stellar atmosphere in a way that mirrors the", "composition of the rocky object engulfed, with the refractory elements", "being more abundant than the volatiles. Due to these stellar chemical", "changes, planetary engulfment events can render the process of", "chemical tagging potentially inaccurate. A line-by-line differential", "analysis of twin stars in wide binary systems allows us to test the", "chemical homogeneity of these associations with typical individual", "stellar FeI uncertainties of 0.01dex and eventually unveil chemical", "anomalies that could be attributed to planetary engulfment events. Out", "of the 14 systems analyzed here, we report the discovery of the most", "chemically inhomogeneous system to date (HIP 34407/HIP 34426). The", "median difference in abundances of refractory elements within the pair", "is 0.19dex and the trend between the differential abundances and", "condensation temperature suggests that the anomaly is likely due to a", "planetary engulfment event. Within our sample, five other chemically", "anomalous systems are found."], "description": ["Eight binary systems were observed by the Ultraviolet and Visual", "Echelle Spectrograph (UVES) on the Very Large Telescope of the", "European Southern Observatory. The observations have been performed", "with a resolving power R~85000 and a wavelength coverage between 330", "and 680nm.", "Another six pairs have been observed with the High Dispersion", "Spectrograph (HDS) on the Subaru telescope. For the latter we have", "used a R~80000 and the Yc standard setup which covers the 439-705nm", "spectral range.", "Solar spectra have been acquired both with UVES (S/N~350) and HDS", "(S/N~400) using the same instrument configurations."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Target selection ", "columns": [{"name": "Star", "desc": "Star observed "}, {"name": "Plx", "desc": "[4.5/36.1] Gaia DR2 Parallax "}, {"name": "e_Plx", "desc": "[0.04/0.5] Gaia DR2 Parallax error "}, {"name": "pmRA", "desc": "[-451/67] Gaia DR2 proper motion in RA "}, {"name": "e_pmRA", "desc": "[0.05/2.2] pmRA uncertainty "}, {"name": "pmDE", "desc": "[-214/145] Gaia DR2 proper motion in DEC "}, {"name": "e_pmDE", "desc": "[0.04/3] pmDE uncertainty "}, {"name": "RVel", "desc": "[-33.1/47.8]? Gaia DR2 Radial velocity "}, {"name": "e_RVel", "desc": "[0.1/1.1]? Gaia DR2 Radial velocity, error "}, {"name": "SNR", "desc": "[300/400] spectrum signal-to-noise "}, {"name": "Inst", "desc": "Instrument (VLT/UVES or Subaru/HDS) "}]}, {"name": "table2.dat", "desc": "Equivalent width measurements (data per objects in columns)", "columns": [{"name": "lambda", "desc": "Wavelength, Angstroms "}, {"name": "Species", "desc": "Species "}, {"name": "EP", "desc": "Excitation potential "}, {"name": "loggf", "desc": "log, statistical weight*oscillator strength "}, {"name": "EW-Sun-UVES", "desc": "? Equivalent Width, Sun-UVES m{AA} "}, {"name": "EW-HIP58298B", "desc": "? Equivalent Width, HIP58298B m{AA} "}, {"name": "EW-HIP44858", "desc": "? Equivalent Width, HIP44858 m{AA} "}, {"name": "EW-HIP39409B", "desc": "? Equivalent Width, HIP39409B m{AA} "}, {"name": "EW-HIP34407", "desc": "? Equivalent Width, HIP34407 m{AA} "}, {"name": "EW-HIP49520A", "desc": "? Equivalent Width, HIP49520A m{AA} "}, {"name": "EW-HIP47836", "desc": "? Equivalent Width, HIP47836 m{AA} "}, {"name": "EW-BD+132311A", "desc": "? Equivalent Width, BD+132311A m{AA} "}, {"name": "EW-HIP47839", "desc": "? Equivalent Width, HIP47839 m{AA} "}, {"name": "EW-HIP44862", "desc": "? Equivalent Width, HIP44862 m{AA} "}, {"name": "EW-HIP58298A", "desc": "? Equivalent Width, HIP58298A m{AA} "}, {"name": "EW-HR4443", "desc": "? Equivalent Width, HR4443 m{AA} "}, {"name": "EW-HR4444", "desc": "? Equivalent Width, HR4444 m{AA} "}, {"name": "EW-HIP39409A", "desc": "? Equivalent Width, HIP39409A m{AA} "}, {"name": "EW-HIP34426", "desc": "? Equivalent Width, HIP34426 m{AA} "}, {"name": "EW-BD+132311B", "desc": "? Equivalent Width, BD+132311B m{AA} "}, {"name": "EW-HIP49520B", "desc": "? Equivalent Width, HIP49520B m{AA} "}, {"name": "EW-Sun-HDS", "desc": "? Equivalent Width, Sun-HDS m{AA} "}, {"name": "EW-HIP70386A", "desc": "? Equivalent Width, HIP70386A m{AA} "}, {"name": "EW-HD103432", "desc": "? Equivalent Width, HD103432 m{AA} "}, {"name": "EW-HD105422", "desc": "? Equivalent Width, HD105422 m{AA} "}, {"name": "EW-HIP70269B", "desc": "? Equivalent Width, HIP70269B m{AA} "}, {"name": "EW-HD111484B", "desc": "? Equivalent Width, HD111484B m{AA} "}, {"name": "EW-HD124913B", "desc": "? Equivalent Width, HD124913B m{AA} "}, {"name": "EW-HD98744", "desc": "? Equivalent Width, HD98744 m{AA} "}, {"name": "EW-HIP70386B", "desc": "? Equivalent Width, HIP70386B m{AA} "}, {"name": "EW-HD103431", "desc": "? Equivalent Width, HD103431 m{AA} "}, {"name": "EW-HD98745", "desc": "? Equivalent Width, HD98745 m{AA} "}, {"name": "EW-HD105421", "desc": "? Equivalent Width, HD105421 m{AA} "}, {"name": "EW-HIP70269A", "desc": "? Equivalent Width, HIP70269A m{AA} "}, {"name": "EW-HD111484A", "desc": "? Equivalent Width, HD111484A m{AA} "}, {"name": "EW-HD124913A", "desc": "? Equivalent Width, HD124913A m{AA} "}]}, {"name": "table3.dat", "desc": "Stellar parameters ", "columns": [{"name": "Star", "desc": "Star observed "}, {"name": "Teff", "desc": "[5515/6295] Effective temperature "}, {"name": "e_Teff", "desc": "[5/31] Uncertainty in Teff "}, {"name": "logg", "desc": "[3.97/4.53] Surface gravity, log "}, {"name": "e_logg", "desc": "[0.02/0.09] Uncertainty in logg "}, {"name": "Fe/H", "desc": "[-0.51/0.13] Metallicity "}, {"name": "e_Fe/H", "desc": "[0.005/0.02] Uncertainty in Fe/H "}, {"name": "Vt", "desc": "[0.85/1.82] Microturbulent velocity "}, {"name": "e_Vt", "desc": "[0.01/0.06] Uncertainty in Vt "}]}, {"name": "ews.dat", "desc": "Equivalent width measurements (data per objects in rows)", "columns": [{"name": "Star", "desc": "Star observed "}, {"name": "lambda", "desc": "[3365.18/7113.2] Wavelength in Angstrom units "}, {"name": "Ion", "desc": "[6/107] Species "}, {"name": "EP", "desc": "[0/8.7] Excitation potential "}, {"name": "loggf", "desc": "[-6.2/0.6] log, statistical weight*oscillator strength"}, {"name": "EW", "desc": "[1/144]? Equivalent Width in m{AA} units "}]}, {"name": "table4.dat", "desc": "Differential abundances relative to the Sun ", "columns": [{"name": "Star", "desc": "Star Observed "}, {"name": "[CI]", "desc": "[-0.36/-0.016] Differential abundance, Sun, [CI] "}, {"name": "o_[CI]", "desc": "[2/4] Number of lines, [CI] "}, {"name": "e_[CI]", "desc": "[0.01/0.06] Uncertainty, [CI] "}, {"name": "[CH]", "desc": "? Differential abundance, Sun, [CH] "}, {"name": "o_[CH]", "desc": "? Number of lines, [CH] "}, {"name": "e_[CH]", "desc": "? Uncertainty, [CH] "}, {"name": "[NH]", "desc": "? Differential abundance, Sun, [NH] "}, {"name": "o_[NH]", "desc": "? Number of lines, [NH] "}, {"name": "e_[NH]", "desc": "? Uncertainty, [NH] "}, {"name": "[OI]", "desc": "[-0.14/0.03]? Differential abundance, Sun, [OI] "}, {"name": "o_[OI]", "desc": "[1]? Number of lines, [OI] "}, {"name": "e_[OI]", "desc": "[0/0.03]? Uncertainty, [OI] "}, {"name": "[NaI]", "desc": "Differential abundance, Sun, [NaI] "}, {"name": "o_[NaI]", "desc": "Number of lines, [NaI] "}, {"name": "e_[NaI]", "desc": "Uncertainty, [NaI] "}, {"name": "[MgI]", "desc": "Differential abundance, Sun, [MgI] "}, {"name": "o_[MgI]", "desc": "Number of lines, [MgI] "}, {"name": "e_[MgI]", "desc": "Uncertainty, [MgI] "}, {"name": "[AlI]", "desc": "[-0.53/0.04] Differential abundance, Sun, [AlI] "}, {"name": "o_[AlI]", "desc": "[2] Number of lines, [AlI] "}, {"name": "e_[AlI]", "desc": "[0.003/0.08] Uncertainty, [AlI] "}, {"name": "[SiI]", "desc": "[-0.42/0.11] Differential abundance, Sun, [SiI] "}, {"name": "o_[SiI]", "desc": "[12/13] Number of lines, [SiI] "}, {"name": "e_[SiI]", "desc": "[0.003/0.013] Uncertainty, [SiI] "}, {"name": "[SI]", "desc": "Differential abundance, Sun, [SI] "}, {"name": "o_[SI]", "desc": "Number of lines, [SI] "}, {"name": "e_[SI]", "desc": "Uncertainty, [SI] "}, {"name": "[CaI]", "desc": "[-0.44/0.16] Differential abundance, Sun, [CaI] "}, {"name": "o_[CaI]", "desc": "[10/11] Number of lines, [CaI] "}, {"name": "e_[CaI]", "desc": "[0.006/0.024] Uncertainty, [CaI] "}, {"name": "[ScII]", "desc": "Differential abundance, Sun, [ScII] "}, {"name": "o_[ScII]", "desc": "Number of lines, [ScII] "}, {"name": "e_[ScII]", "desc": "Uncertainty, [ScII] "}, {"name": "[TiI]", "desc": "[-0.42/0.09] Differential abundance, Sun, [TiI] "}, {"name": "o_[TiI]", "desc": "[14/17] Number of lines, [TiI] "}, {"name": "e_[TiI]", "desc": "[0.006/0.03] Uncertainty, [TiI] "}, {"name": "[TiII]", "desc": "[-0.43/0.09] Differential abundance, Sun, [TiII] "}, {"name": "o_[TiII]", "desc": "[8/13] Number of lines, [TiII] "}, {"name": "e_[TiII]", "desc": "[0.008/0.05] Uncertainty, [TiII] "}, {"name": "[VI]", "desc": "Differential abundance, Sun, [VI] "}, {"name": "o_[VI]", "desc": "Number of lines, [VI] "}, {"name": "e_[VI]", "desc": "Uncertainty, [VI] "}, {"name": "[CrI]", "desc": "[-0.6/0.11] Differential abundance, Sun, [CrI] "}, {"name": "o_[CrI]", "desc": "[10/12] Number of lines, [CrI] "}, {"name": "e_[CrI]", "desc": "[0.006/0.04] Uncertainty, [CrI] "}, {"name": "[CrII]", "desc": "Differential abundance, Sun, [CrII] "}, {"name": "o_[CrII]", "desc": "Number of lines, [CrII] "}, {"name": "e_[CrII]", "desc": "Uncertainty, [CrII] "}, {"name": "[MnI]", "desc": "Differential abundance, Sun, [MnI] "}, {"name": "o_[MnI]", "desc": "Number of lines, [MnI] "}, {"name": "e_[MnI]", "desc": "Uncertainty, [MnI] "}, {"name": "[FeI]", "desc": "[-0.51/0.13] Differential abundance, Sun, [FeI] "}, {"name": "o_[FeI]", "desc": "[81/91] Number of lines, [FeI] "}, {"name": "e_[FeI]", "desc": "[0.005/0.021] Uncertainty, [FeI] "}, {"name": "[FeII]", "desc": "[-0.51/0.14] Differential abundance, Sun, [FeII] "}, {"name": "o_[FeII]", "desc": "[13/17] Number of lines, [FeII] "}, {"name": "e_[FeII]", "desc": "[0.009/0.04] Uncertainty, [FeII] "}, {"name": "[CoI]", "desc": "Differential abundance, Sun, [CoI] "}, {"name": "o_[CoI]", "desc": "Number of lines, [CoI] "}, {"name": "e_[CoI]", "desc": "Uncertainty, [CoI] "}, {"name": "[NiI]", "desc": "[-0.53/0.08] Differential abundance, Sun, [NiI] "}, {"name": "o_[NiI]", "desc": "[16/18] Number of lines, [NiI] "}, {"name": "e_[NiI]", "desc": "[0.004/0.022] Uncertainty, [NiI] "}, {"name": "[CuI]", "desc": "Differential abundance, Sun, [CuI] "}, {"name": "o_[CuI]", "desc": "Number of lines, [CuI] "}, {"name": "e_[CuI]", "desc": "Uncertainty, [CuI] "}, {"name": "[ZnI]", "desc": "[-0.49/0.13] Differential abundance, Sun, [ZnI] "}, {"name": "o_[ZnI]", "desc": "[2] Number of lines, [ZnI] "}, {"name": "e_[ZnI]", "desc": "[0.005/0.13] Uncertainty, [ZnI] "}, {"name": "[YII]", "desc": "Differential abundance, Sun, [YII] "}, {"name": "o_[YII]", "desc": "Number of lines, [YII] "}, {"name": "e_[YII]", "desc": "Uncertainty, [YII] "}, {"name": "[ZrII]", "desc": "[-0.53/0.12]? Differential abundance, Sun, [ZrII]"}, {"name": "o_[ZrII]", "desc": "[1]? Number of lines, [ZrII] "}, {"name": "e_[ZrII]", "desc": "[0.008/0.03]? Uncertainty, [ZrII] "}, {"name": "[BaII]", "desc": "[-0.61/0.26] Differential abundance, Sun, [BaII] "}, {"name": "o_[BaII]", "desc": "[3] Number of lines, [BaII] "}, {"name": "e_[BaII]", "desc": "[0.008/0.07] Uncertainty, [BaII] "}]}, {"name": "table5.dat", "desc": "Differential abundances within each pair ", "columns": [{"name": "[CI]", "desc": "Differential abundance, pair, [CI] "}, {"name": "o_[CI]", "desc": "Number of lines, [CI] "}, {"name": "e_[CI]", "desc": "Uncertainty, [CI] "}, {"name": "[CH]", "desc": "? Differential abundance, pair, [CH] "}, {"name": "o_[CH]", "desc": "? Number of lines, [CH] "}, {"name": "e_[CH]", "desc": "? Uncertainty, [CH] "}, {"name": "[OI]", "desc": "? Differential abundance, pair, [OI] "}, {"name": "o_[OI]", "desc": "? Number of lines, [OI] "}, {"name": "e_[OI]", "desc": "? Uncertainty, [OI] "}, {"name": "[NH]", "desc": "? Differential abundance, pair, [NH] "}, {"name": "o_[NH]", "desc": "? Number of lines, [NH] "}, {"name": "e_[NH]", "desc": "? Uncertainty, [NH] "}, {"name": "[NaI]", "desc": "Differential abundance, pair, [NaI] "}, {"name": "o_[NaI]", "desc": "Number of lines, [NaI] "}, {"name": "e_[NaI]", "desc": "Uncertainty, [NaI] "}, {"name": "[MgI]", "desc": "Differential abundance, pair, [MgI] "}, {"name": "o_[MgI]", "desc": "Number of lines, [MgI] "}, {"name": "e_[MgI]", "desc": "Uncertainty, [MgI] "}, {"name": "[AlI]", "desc": "Differential abundance, pair, [AlI] "}, {"name": "o_[AlI]", "desc": "Number of lines, [AlI] "}, {"name": "e_[AlI]", "desc": "Uncertainty, [AlI] "}, {"name": "[SiI]", "desc": "Differential abundance, pair, [SiI] "}, {"name": "o_[SiI]", "desc": "Number of lines, [SiI] "}, {"name": "e_[SiI]", "desc": "Uncertainty, [SiI] "}, {"name": "[SI]", "desc": "Differential abundance, pair, [SI] "}, {"name": "o_[SI]", "desc": "Number of lines, [SI] "}, {"name": "e_[SI]", "desc": "Uncertainty, [SI] "}, {"name": "[CaI]", "desc": "Differential abundance, pair, [CaI] "}, {"name": "o_[CaI]", "desc": "Number of lines, [CaI] "}, {"name": "e_[CaI]", "desc": "Uncertainty, [CaI] "}, {"name": "[ScII]", "desc": "Differential abundance, pair, [ScII] "}, {"name": "o_[ScII]", "desc": "Number of lines, [ScII] "}, {"name": "e_[ScII]", "desc": "Uncertainty, [ScII] "}, {"name": "[TiI]", "desc": "Differential abundance, pair, [TiI] "}, {"name": "o_[TiI]", "desc": "Number of lines, [TiI] "}, {"name": "e_[TiI]", "desc": "Uncertainty, [TiI] "}, {"name": "[TiII]", "desc": "Differential abundance, pair, [TiII] "}, {"name": "o_[TiII]", "desc": "Number of lines, [TiII] "}, {"name": "e_[TiII]", "desc": "Uncertainty, [TiII] "}, {"name": "[VI]", "desc": "Differential abundance, pair, [VI] "}, {"name": "o_[VI]", "desc": "Number of lines, [VI] "}, {"name": "e_[VI]", "desc": "Uncertainty, [VI] "}, {"name": "[CrI]", "desc": "Differential abundance, pair, [CrI] "}, {"name": "o_[CrI]", "desc": "Number of lines, [CrI] "}, {"name": "e_[CrI]", "desc": "Uncertainty, [CrI] "}, {"name": "[CrII]", "desc": "Differential abundance, pair, [CrII] "}, {"name": "o_[CrII]", "desc": "Number of lines, [CrII] "}, {"name": "e_[CrII]", "desc": "Uncertainty, [CrII] "}, {"name": "[MnI]", "desc": "Differential abundance, pair, [MnI] "}, {"name": "o_[MnI]", "desc": "Number of lines, [MnI] "}, {"name": "e_[MnI]", "desc": "Uncertainty, [MnI] "}, {"name": "[FeI]", "desc": "Differential abundance, pair, [FeI] "}, {"name": "o_[FeI]", "desc": "Number of lines, [FeI] "}, {"name": "e_[FeI]", "desc": "Uncertainty, [FeI] "}, {"name": "[FeII]", "desc": "Differential abundance, pair, [FeII] "}, {"name": "o_[FeII]", "desc": "Number of lines, [FeII] "}, {"name": "e_[FeII]", "desc": "Uncertainty, [FeII] "}, {"name": "[CoI]", "desc": "Differential abundance, pair, [CoI] "}, {"name": "o_[CoI]", "desc": "Number of lines, [CoI] "}, {"name": "e_[CoI]", "desc": "Uncertainty, [CoI] "}, {"name": "[NiI]", "desc": "Differential abundance, pair, [NiI] "}, {"name": "o_[NiI]", "desc": "Number of lines, [NiI] "}, {"name": "e_[NiI]", "desc": "Uncertainty, [NiI] "}, {"name": "[CuI]", "desc": "Differential abundance, pair, [CuI] "}, {"name": "o_[CuI]", "desc": "Number of lines, [CuI] "}, {"name": "e_[CuI]", "desc": "Uncertainty, [CuI] "}, {"name": "[ZnI]", "desc": "Differential abundance, pair, [ZnI] "}, {"name": "o_[ZnI]", "desc": "Number of lines, [ZnI] "}, {"name": "e_[ZnI]", "desc": "Uncertainty, [ZnI] "}, {"name": "[YII]", "desc": "Differential abundance, pair, [YII] "}, {"name": "o_[YII]", "desc": "Number of lines, [YII] "}, {"name": "e_[YII]", "desc": "Uncertainty, [YII] "}, {"name": "[ZrII]", "desc": "? Differential abundance, pair, [ZrII] "}, {"name": "o_[ZrII]", "desc": "? Number of lines, [ZrII] "}, {"name": "e_[ZrII]", "desc": "? Uncertainty, [ZrII] "}, {"name": "[BaII]", "desc": "Differential abundance, pair, [BaII] "}, {"name": "o_[BaII]", "desc": "Number of lines, [BaII] "}, {"name": "e_[BaII]", "desc": "Uncertainty, [BaII] "}, {"name": "Star1", "desc": "Pair Star 1 "}, {"name": "Star2", "desc": "Pair Star 2 "}]}, {"name": "table6.dat", "desc": "Parameters for the chemical homogeneity test ", "columns": [{"name": "Star1", "desc": "Star #1 observed "}, {"name": "Star2", "desc": "Star #2 observed "}, {"name": "chi2-red", "desc": "reduced chi-square, equation 1 "}, {"name": "chi2-survey", "desc": "[0.06/12.1] reduced chi-square, survey "}, {"name": "sigma-x", "desc": "[0.28/0.3] Uncertainty in differential abundance"}, {"name": "slope", "desc": "? Slope, {Delta}[X/H] vs T_Cond_, 10-6[dex]/K"}, {"name": "e_slope", "desc": "? Uncertainty in slope "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_894_27"}} {"id": "J/ApJ/894/27", "title_cds": "Rapidly evolving transients from the HSC SSP survey", "title_create": "Tampo+, 2020", "year": "2020", "author": "Tampo Y., Tanaka M., Maeda K., Yasuda N., Tominaga N., Jiang J.-A., Moriya T.J., Morokuma T., Suzuki N., Takahashi I., Kokubo M., Kawana K.", "title_pub": "Rapidly evolving transients from the Hyper Suprime-Cam SSP Transient Survey.", "first_author": "Tampo Y.", "ref_biblio": [""], "bibcode": ["2020ApJ...894...27T"], "see_also": ["V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)", "J/ApJ/673/999 : Supernova and host galaxies metallicities (Prieto+, 2008)", "J/ApJS/184/218 : The zCOSMOS 10k-bright spectroscopic sample (Lilly+, 2009)", "J/A+A/523/A7 : Light curves of type Ia supernovae in SNLS (Guy+, 2010)", "J/A+A/559/A14 : VIMOS VLT Deep Survey final data release (Le Fevre+, 2013)", "J/A+A/568/A22 : Joint analysis of the SDSS-II and SNLS SNe Ia (Betoule+, 2014)", "J/ApJ/794/23 : Pan-STARRS1 transients optical photometry (Drout+, 2014)", "J/AJ/148/13 : Redshifts of 65 CANDELS supernovae (Rodney+, 2014)", "J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014)", "J/A+A/584/A62 : SUDARE VST-OmegaCAM search supernova rates (Cappellaro+, 2015)", "J/ApJ/819/35 : LCs of four transients from PTF & SNLS (Arcavi+, 2016)", "J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)", "J/ApJS/225/27 : 3D-HST Survey: grism spectra master catalog (Momcheva+, 2016)", "J/ApJ/851/107 : iPTF 16asu photometry follow-up (Whitesides+, 2017)", "J/ApJ/887/169 : UV-Opt light curves of the type Ic SN 2018gep (Ho+, 2019)", "http://hsc-release.mtk.nao.ac.jp/doc/index.php/database/ : HSC SSP database"], "keyword_cds": "Supernovae; Photometry, ugriz; Surveys; Redshifts", "keyword_pub": "Supernovae", "abstract": ["Rapidly evolving transients form a new class of transients that show", "shorter timescales of light curves than those of typical core-collapse", "and thermonuclear supernovae. We performed a systematic search for", "rapidly evolving transients using deep data taken with the Hyper", "Suprime-Cam Subaru Strategic Program Transient Survey. By measuring", "the timescales of the light curves of 1824 transients, we identified", "five rapidly evolving transients. Our samples are found in a wide", "range of redshifts (0.3<=z<=1.5) and peak absolute magnitudes", "(-17>=M_i_>=-20). The light-curve properties are similar to those of", "the previously discovered rapidly evolving transients. They show a", "relatively blue spectral energy distribution, with the best-fit", "blackbody of 8000-18000K. We show that some of the transients require", "power sources other than the radioactive decays of ^56^Ni because of", "their high peak luminosities and short timescales. The host galaxies", "of all of the samples are star-forming galaxies, suggesting a massive", "star origin for the rapidly evolving transients. The event rate is", "roughly estimated to be ~4000 events yr^-1^ Gpc^-3^, which is about 1%", "of core-collapse supernovae."], "description": ["We use the observational data from the Hyper Suprime-Cam Subaru", "Strategic Program Transient Survey (HSC-SSP Transient Survey;", "Aihara+ 2018PASJ...70S...4A & Yasuda+ 2019PASJ...71...74Y). The survey", "around the COSMOS field was performed over six months from 2016", "November to 2017 April, covering the 1.77deg^2^ Ultra-Deep layer and", "the 5.78deg^2^ Deep layer, with the cadence of 7-10 days using the g,", "r, i, z and y bands."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "sample.dat", "desc": "Basic observational information (Table 1) and photometric properties (Table 3) of the rapidly evolving transients from the HSC-SSP Transient Survey and properties of the host galaxies (Table 4)", "columns": [{"name": "Name", "desc": "Name of the transient "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "z", "desc": "[0.33/1.5] Redshift "}, {"name": "e_z", "desc": "[0.01/0.06]? Lower uncertainty in z "}, {"name": "E_z", "desc": "[0.01/0.07]? Upper uncertainty in z "}, {"name": "n_z", "desc": "Spectroscopic or photometric redshift "}, {"name": "r_z", "desc": "Photometric redshift reference (1) "}, {"name": "iMag", "desc": "[-19.76/-17.35] Peak i-band absolute magnitude "}, {"name": "e_iMag", "desc": "[0.02/0.11] iMag uncertainty "}, {"name": "trise", "desc": "[1.37/5.11] i-band rise time t_1/2,rise_ (2) "}, {"name": "e_trise", "desc": "[0.08/0.7] trise uncertainty "}, {"name": "tdec", "desc": "[5/16] i-band decline time t_1/2,decline_ (2) "}, {"name": "e_tdec", "desc": "[0.06/2] tdec uncertainty "}, {"name": "Temp", "desc": "[8100/17400] Blackbody temperature at the i-band peak"}, {"name": "e_Temp", "desc": "[1300/3700] Temp uncertainty "}, {"name": "zGal", "desc": "[0.33/1.5] Host galaxy redshift "}, {"name": "SFR", "desc": "[0.39/8.3] Host star formation rate "}, {"name": "Offset", "desc": "[0.4/25.7] Offset of the transient from the center of the host galaxy"}]}, {"name": "table2.dat", "desc": "Log of photometric observations for our sample ", "columns": [{"name": "Name", "desc": "HSC-SSP Transient Survey name "}, {"name": "MJD", "desc": "[57715.5/57924.3] Modified Julian Date (JD-2400000.5), mid-observation"}, {"name": "l_mag", "desc": "3{sigma} upper limit flag "}, {"name": "mag", "desc": "[23/27.7] Observed magnitude in Filter "}, {"name": "e_mag", "desc": "[0.01/0.2]? Uncertainty in mag "}, {"name": "Filt", "desc": "Filter (g, r, i or z) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_897_10"}} {"id": "J/ApJ/897/10", "title_cds": "Doppler factor estimation for 350 blazars", "title_create": "Zhang+, 2020", "year": "2020", "author": "Zhang L., Chen S., Xiao H., Cai J., Fan J.", "title_pub": "Doppler Factor Estimation for Fermi Blazars.", "first_author": "Zhang L.", "ref_biblio": [""], "bibcode": ["2020ApJ...897...10Z"], "see_also": ["VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)", "J/A+A/436/799 : X & gamma-ray fluxes of {gamma}-ray-loud blazars (Fan+, 2005)", "J/ApJ/715/429 : First Fermi-LAT AGN catalog (1LAC) (Abdo+, 2010)", "J/ApJS/188/405 : Fermi-LAT first source catalog (1FGL) (Abdo+, 2010)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/ApJ/748/49 : Optical spectroscopy of 1LAC broad-line blazars (Shaw+, 2012)", "J/other/RAA/13.259 : {gamma}-ray Doppler factor for Fermi blazars (Fan+, 2013)", "J/other/RAA/14.1135 : Doppler factor for a Fermi blazar sample (Fan+, 2014)", "J/other/Nat/515.376 : Power of relativistic jets in blazars (Ghisellini+, 2014)", "J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)", "J/ApJ/810/14 : Third catalog of LAT-detected AGNs (3LAC) (Ackermann+, 2015)", "J/ApJS/226/20 : X-ray, opt. & radio SEDs of Fermi blazars (Fan+, 2016)", "J/ApJ/835/L38 : Fermi blazars with Doppler factors (Fan+, 2017)", "J/ApJS/235/39 : Jet properties of {gamma}-ray-loud 3FGL AGNs (Chen, 2018)", "J/A+A/615/A167 : Catalog of NLS1s galaxies in 6dFGS survey (Chen+, 2018)", "J/AJ/155/90 : 1996-2009 optical photom. monitoring for 3C 66A (Fan+, 2018)", "J/ApJ/866/137 : Bright blazars variability brightness temp. (Liodakis+, 2018)", "J/ApJS/247/33 : The Fermi LAT fourth source catalog (4FGL) (Abdollahi+, 2020)"], "keyword_cds": "BL Lac objects; QSOs; Gamma rays; Redshifts", "keyword_pub": "Active galactic nuclei ; Blazars ; High energy astrophysics ; Jets", "abstract": ["In this work, we exploit the luminosity of the broad-line region (BLR)", "for 50 Fermi blazars through matching the coordinates between the", "Sloan Digital Sky Survey catalog, Fermi Large Area Telescope Third", "Source Catalog, and the Fermi Large Area Telescope Fourth Source", "Catalog and fitting their emission lines. In total, we collected a", "sample of 350 blazars with broad-line emissions including 50 new", "objects and 300 blazars from published works to revisit the", "correlation between the {gamma}-ray luminosity and the broad-line", "luminosity, and proposed a new method to estimate the Doppler factors", "based on the correlation between the radiative power of the jet and", "luminosity of the BLR. We come to following conclusions. (1) For the", "50 Fermi blazars, their broad-line luminosity (log LBLR) ranges from", "41.82-45.2erg/s with a mean value of 44.39erg/s. (2) The Doppler", "factor ({delta}) ranges from {delta}=0.35 to {delta}=85.66 with a mean", "value of 12.54, which is consistent with the results in the", "literature. (3) There are positive correlations between {gamma}-ray", "luminosity and broad-line luminosity, and between {gamma}-ray", "luminosity and the Doppler factor."], "description": ["In this paper, we obtained emission-line luminosity for 50 Fermi", "blazars by matching Sloan Digital Sky Survey (SDSS) with Fermi Large", "Area Telescope DR3 (3FGL) and Fermi Large Area Telescope DR4 (4FGL)", "and compiled emission-line luminosity for 300 Fermi blazars from the", "literature and got a sample of 350 Fermi blazars. We revisited the", "correlation between {gamma}-rays and emission-line luminosity, and", "proposed a new method to estimate the Doppler factor for Fermi", "blazars."], "type": ["GCC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Blazar sample ", "columns": [{"name": "Name", "desc": "Blazar name "}, {"name": "OName", "desc": "Other name "}, {"name": "z", "desc": "[0.03/3.104] Redshift "}, {"name": "Class", "desc": "Classification (1) "}, {"name": "Cts", "desc": "[7.5e-11/9.9e-8] {gamma}-ray photon flux, 1-100GeV"}, {"name": "alpha", "desc": "[1.75/3.1] photon spectral index "}, {"name": "logLgamma", "desc": "[43.8/48.6] log, {gamma}-ray luminosity, 1-100GeV, erg/s"}, {"name": "logLBLR", "desc": "[41.7/46.5] log, broad-line region luminosity, erg/s"}, {"name": "r_logLBLR", "desc": "References for logLBLR (2) "}, {"name": "delta", "desc": "[0.35/85.66] Doppler factor, this work "}]}, {"name": "table3.dat", "desc": "List of sources with Doppler factors ", "columns": [{"name": "Name", "desc": "Blazar name "}, {"name": "OName", "desc": "Other name "}, {"name": "delta-ALL", "desc": "[0.35/85.66]? Doppler factor, this work "}, {"name": "delta-G14", "desc": "[5/18]? Doppler factor, Ghisellini+, 2014, J/other/Nat/515.376"}, {"name": "delta-L18", "desc": "[0.23/88.44]? Doppler factor, Liodakis+, 2018, J/ApJ/866/137"}, {"name": "delta-C18", "desc": "[1.3/94.0]? Doppler factor, Chen+, 2018, J/ApJS/235/39"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_908_8"}} {"id": "J/ApJ/908/8", "title_cds": "", "title_create": "Calahan+, 2021", "year": "2021", "author": "Calahan J.K., Bergin E., Zhang Ke, Teague R., Cleeves I., Bergner J., Blake G.A., Cazzoletti P., Guzman V., Hogerheijde M. R, Huang J., Kama M., Loomis R., Oberg K., Qi C., van Dishoeck E.F., van Scheltinga J.T., Walsh C., Wilner D.", "title_pub": "The TW Hya Rosetta Stone Project. III. Resolving the Gaseous Thermal Profile of the Disk.", "first_author": "Calahan J.K.", "bibcode": [""], "bibcode": ["2021ApJ...908...51F"], "see_also": ["I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)", "J/MNRAS/446/3895 : The rising light curves of Type Ia supernovae (Firth+, 2015)", "J/ApJ/799/105 : KELT light curve of the M82 SN 2014J (Siverd+, 2015)", "J/ApJ/853/62 : Optical and NIR spectra and LCs of SN2016ija (Tartaglia+, 2018)", "J/ApJ/870/L1 : K2 observations type Ia supernova SN2018oh (Dimitriadis+, 2019)", "J/ApJ/883/111 : UV-Opt LCs of ASASSN-19bt detected by TESS (Holoien+, 2019)", "J/ApJ/870/13 : K2 light curve analysis of ASASSN-18bt (Shappee+, 2019)", "J/ApJ/886/152 : ZTF early observations of Type Ia SNe. I. LCs (Yao+, 2019)", "J/ApJ/893/143 : UBVRIJHK & spec. obs. of type Ia SN2019ein (Kawabata+, 2020)", "J/A+A/634/A37 : TURTLS Light curves of ^56^Ni distributions (Magee+, 2020)", "J/ApJ/898/56 : UVOT, ZTF gri LCs & spectra of SN Ia 2019yvq (Miller+, 2020)", "J/ApJ/902/47 : ZTF early obs. of type Ia SNe. II. Rise time (Miller+, 2020)", "J/ApJ/897/159 : Type Ia supernova SN2019ein UBVgri photo. (Pellegrino+, 2020)"], "keyword_cds": "Supernovae; Photometry, VRI", "keyword_pub": "Type Ia supernovae ; Supernovae", "abstract": ["We present the early-time light curves of Type Ia supernovae (SNeIa)", "observed in the first six sectors of Transiting Exoplanet Survey", "Satellite (TESS) data. Ten of these SNe were discovered by ASAS-SN,", "seven by ATLAS, six by ZTF, and one by Gaia. For nine of these objects", "with sufficient dynamic range (>3.0mag from detection to peak), we fit", "power-law models and searched for signatures of companion stars. We", "found a diversity of early-time light-curve shapes, although most of", "our sources are consistent with fireball models where the flux", "increases as {prop}t2. Three SNe displayed a flatter rise with flux", "{prop}t. We did not find any obvious evidence for additional", "structures, such as multiple power-law components, in the early rising", "light curves. For assumptions about the SN properties and the observer", "viewing angle (ejecta mass of 1.4M{sun}, expansion velocity of", "104km/s, opacity of 0.2cm^2^/g, and viewing angle of 45{deg}) and a", "further assumption that any companion stars would be in Roche lobe", "overflow, it is possible to place upper limits on the radii of any", "companion stars. Six of the nine SNe had complete coverage of the", "early-time light curves, and we placed upper limits on the radii of", "companion stars of <~32R{sun} for these SNe, <~20R{sun} for five of", "the six, and <~4R{sun} for two of the six. The small sample size did", "not allow us to put limits on the occurrence rate of companion stars", "in the progenitors of SNe Ia. However, we expect that TESS observed", "enough SNe in its two-year primary mission (26 sectors) to either", "detect the signature of a large companion (R>20R{sun}) or constrain", "the occurrence rate of such systems, at least for the fiducial SN", "properties adopted here. We also show that TESS is capable of", "detecting emission from a 1R{sun} companion for an SN Ia within 50Mpc", "and has a reasonable chance of doing so after about six years."], "description": ["Transiting Exoplanet Survey Satellite (TESS) observes in a single", "broadband filter ranging from about 600 to 1000nm with an effective", "wavelength of 800nm."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/abcd42"], "orcid_pub": ["0000-0002-9113-7162"], "data": "f", "date_creation": "27-Jul-2022", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Properties of the supernova sample ", "columns": [{"name": "SN", "desc": "Super Nova identifier "}, {"name": "TNS", "desc": "Discovery survey identifier "}, {"name": "mag", "desc": "[14.9/19.2]? Apparent peak magnitude "}, {"name": "Dmag", "desc": "[0.59/4.89]? Differential magnitude "}, {"name": "MAG", "desc": "[-20.9/-16.3]? Absolute magnitude (1) "}, {"name": "e_MAG", "desc": "[0.09/2]? Error in MAG "}, {"name": "vLv", "desc": "[3.7e+45/3.3e+47]? Luminosity "}, {"name": "z", "desc": "[0.01/0.09] Redshift "}, {"name": "B-V", "desc": "[0.005/0.3] E(B-V) color "}, {"name": "Discov", "desc": "Discorvery reference "}, {"name": "Class", "desc": "Classification reference "}, {"name": "Note1", "desc": "X = fit with a power law to characterize the early light curve (see section 4)"}, {"name": "Note2", "desc": "X = searched for signatures of companion stars (section 5)"}, {"name": "Note3", "desc": "X = flux calibrated across two sectors using a joint fit to both data sets (section 3)"}, {"name": "Note4", "desc": "X = near strong scattered light backgrounds at the time of first light"}, {"name": "Note5", "desc": "X = affected by pixels with enhanced sensitivity from \"straps\""}, {"name": "Note6", "desc": "X = near bright stars and required detrending "}]}, {"name": "table2.dat", "desc": "TESS supernova light curves ", "columns": [{"name": "SN", "desc": "Supernova identifier "}, {"name": "TNS", "desc": "Discovery survey identifier "}, {"name": "BJD", "desc": "[1325/1491] Barycentric Julian Date JD-2457000.0 "}, {"name": "Flux", "desc": "[-30/168] Observed flux "}, {"name": "e_Flux", "desc": "[0.8/5] Uncertainty in Flux "}, {"name": "Asteroid", "desc": "[0/1] Asteroid flag (1) "}]}, {"name": "table5.dat", "desc": "*TESS light curves ", "columns": [{"name": "Time", "desc": "[0.001/17] Time since explosion "}, {"name": "Flux50", "desc": "[0.006/21.7] 50R* companion model flux "}, {"name": "mag50", "desc": "[17/25.9] 50R* companion model apparent magnitude "}, {"name": "Flux25", "desc": "[0.005/12.9] 25R* companion model flux "}, {"name": "mag25", "desc": "[17.6/26.1] 25R* companion model apparent magnitude"}, {"name": "Flux10", "desc": "[0.004/6.42] 10R* companion model flux "}, {"name": "mag10", "desc": "[18.4/26.3] 10R* companion model apparent magnitude"}, {"name": "Flux5", "desc": "[0.003/3.78] 5R* companion model flux "}, {"name": "mag5", "desc": "[18.9/26.5] 5R* companion model apparent magnitude "}, {"name": "Flux1", "desc": "[0.002/1.13] 1R* companion model flux "}, {"name": "mag1", "desc": "[20.3/27] 1R* companion model apparent magnitude "}, {"name": "Flux0.5", "desc": "[0.002/0.67] 0.5R* companion model flux "}, {"name": "mag0.5", "desc": "[20.8/27.2] 0.5R* companion model apparent magnitude"}, {"name": "Flux0.1", "desc": "[0.0004/0.2] 0.1R* companion model flux "}, {"name": "mag0.1", "desc": "[22.2/28.9] 0.1R* companion model apparent magnitude"}]}, {"name": "refs.dat", "desc": "References used for table1 ", "columns": [{"name": "Ref", "desc": "Reference code "}, {"name": "Autor", "desc": "Main autor "}, {"name": "BIB", "desc": "BIBcode "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_903_296"}} {"id": "J/ApJ/903/296", "title_cds": "Short Title", "title_create": "Author+, ", "title_pub": "Title of the paper", "first_author": "Authors", "author": "Authors", "ref_biblio": [""], "bibcode": ["2022ApJ...903..296.\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Coralie Fix [CDS]", "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_905_44"}} {"id": "J/ApJ/905/44", "title_cds": "Horizontal branch stars of globular cluster NGC 1851", "title_create": "Singh+, 2020", "year": "2020", "author": "Singh G., Sahu S., Subramaniam A., Yadav R.K.S.", "title_pub": "Peculiarities in the horizontal branch stars of globular cluster NGC 1851: discovery of a blue straggler companion to an EHB star.", "first_author": "Singh G.", "ref_biblio": [""], "bibcode": ["2020ApJ...905...44S"], "see_also": ["II/312 : GALEX-DR5 (GR5) sources from AIS and MIS (Bianchi+ 2011)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "II/370 : XMM-OM Serendipitous Source Survey Cat. (XMM-SUSS5.0) (Page+, 2021)", "VII/195 : Globular Clusters in the Milky Way (Harris, 1996)", "VII/202 : Globular Clusters in the Milky Way (Harris, 1997)", "J/ApJ/562/368 : UV photometry in NGC 2808 (Brown+, 2001)", "J/AJ/133/1658 : ACS survey of galactic globular clusters (Sarajedini+, 2007)", "J/A+A/492/277 : Analysis of Collinder 69 stars with VOSA (Bayo+, 2008)", "J/ApJ/677/1069 : Blue stragglers in NGC 6388 (Dalessandro+, 2008)", "J/A+A/539/A19 : Horizontal branch stars in NGC 1851 (Gratton+, 2012)", "J/AJ/148/27 : Photom. in globular clusters. I. NGC 1851 (Cummings+, 2014)", "J/AJ/150/176 : JK phot. of 12 galactic globular clusters (Cohen+, 2015)", "J/A+A/616/A12 : Gaia DR2 sources in GC and dSph (Gaia Collaboration+, 2018)", "J/AJ/157/109 : Stellar proper motions in Orion Nebula Cluster (Kim+, 2019)", "J/A+A/627/A34 : GC hot UV-bright stars model spectra (Moehler+, 2019)", "J/MNRAS/485/3042 : UBVRI photometry in 48 globular clusters (Stetson+, 2019)"], "keyword_cds": "Abundances, [Fe/H]; Clusters, globular; Stars, horizontal branch; Stars, diameters; Ultraviolet; Effective temperatures", "keyword_pub": "Globular star clusters ; Blue straggler stars ; Horizontal branch stars ; Hertzsprung Russell diagram", "abstract": ["We present a study of far-UV (FUV) bright horizontal branch (HB) stars", "to understand the peculiarities seen in the HB sequence of the", "globular cluster NGC 1851, using ground- and space-based", "multiwavelength data. Optical and UV color-magnitude diagrams are used", "to classify HB stars and their membership from Hubble Space Telescope", "and Gaia DR2 data. The spectral energy distributions (SEDs) of the hot", "HB stars located from the core to tidal radii are constructed. The", "SEDs reveal that the HB stars near the \"Grundahl jump\" show a decrease", "in the FUV flux when atmospheric models of cluster metallicity are", "used for fitting, but a better fit is found with higher-metallicity", "models, as expected due to atmospheric diffusion. We report on four", "particularly interesting extreme HB (EHB) stars, two each in the inner", "and outer regions. We detect a subluminous EHB and \"blue-hook\"", "candidates with temperatures T_eff_~25000K and 31000K, respectively.", "We found an EHB star (T_eff_~17000K) with a radius that lies between", "the BHB and normal EHB stars. The most peculiar of our EHB stars", "(T_eff_~28000K) is found to be a photometric binary to a blue", "straggler star (BSS; T_eff_~7000K), which is an important target for", "spectroscopic study. This discovery of the candidate EHB+BSS binary", "system could help to explain the mass loss in the red giant branch", "phase, leading to the formation of EHB stars."], "description": ["In the dense central region of the globular cluster NGC1851 (r<=80\"),", "we use the Hubble Space Telescope (HST) data in the astrophotometric", "catalog of Nardiello+ (2018MNRAS.481.3382N), a part of the HST UV", "Legacy Survey of Galactic Globular Clusters.", "The FUV and near-UV (NUV) data used for the analysis are obtained from", "the UVIT instrument on board the AstroSat satellite. UVIT/AstroSat is", "primarily an imaging instrument that consists of twin 38cm telescopes.", "It provides imaging in the FUV (130-180nm) and NUV (200-300nm)", "channels simultaneously with a circular field of view ~28'. The", "angular resolution of UVIT/AstroSat is <1.8\" in the FUV and NUV", "channels. For this cluster, the observations were performed in three", "filters: F148W, F169M, and N279N, as a part of the performance", "verification (PV) phase during 2016 March 19-21. The details of data", "acquisition and reduction procedures are provided in", "Subramaniam+ (2017AJ....154..233S).", "For the complementary UV data in the outer region (80\"<=r<=r_t_), we", "used the Ultraviolet/Optical Telescope (UVOT) data. UVOT/Swift is a", "modified Richey-Chretien telescope on board the Swift spacecraft. It", "provides an FOV of about 17'x17' with an angular resolution of 2.3\".", "To cover the optical wavelength in the outer region, we used Stetson's", "UBVRI photometric catalog (Stetson+ 2019, J/MNRAS/485/3042).", "We used Gaia DR2 (I/345) data to compute the membership of stars", "located in the regions outside the HST region (see Section 3)."], "object": ["05 14 06.76 -40 02 47.6 NGC 1851 = GCl 9"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "*SED fit parameters of the FUV bright blue horizontal branch (BHB) and BHBd stars for a varying metallicity", "columns": [{"name": "Name", "desc": "Star identifier "}, {"name": "f_Name", "desc": "a: stars having spectroscopic determination of temperatures (Gratton+ 2012, J/A+A/539/A19)"}, {"name": "RAdeg", "desc": "[78.42/78.6] Right ascension (J2000) "}, {"name": "DEdeg", "desc": "[-40.16/-39.9] Declination (J2000) "}, {"name": "[Fe/H]", "desc": "[-1.5/0.5] Log of Fe/H abundance "}, {"name": "Teff", "desc": "[7000/31000] Effective temperature derived from the SED fitting"}, {"name": "e_Teff", "desc": "[500] Teff uncertainty "}, {"name": "Rad", "desc": "[0.16/4.3] Radius derived from the SED fitting "}, {"name": "e_Rad", "desc": "[0.01/0.2] Rad uncertainty "}, {"name": "Lum", "desc": "[2.95/51] Luminosity derived from the SED fitting"}, {"name": "e_Lum", "desc": "[0.13/1.3] Lum uncertainty "}, {"name": "rChi2", "desc": "[2/480]? Reduced {chi}^2^ "}, {"name": "Nfit", "desc": "[7/20]? The number of points considered in fitting the SED"}]}, {"name": "table3.dat", "desc": "SED fit parameters of the extreme horizontal branch (EHB) stars with a varying metallicity", "columns": [{"name": "Name", "desc": "Star identifier "}, {"name": "f_Name", "desc": "a: stars having spectroscopic determination of temperatures (Gratton+ 2012, J/A+A/539/A19)"}, {"name": "RAdeg", "desc": "[78.42/78.6] Right ascension (J2000) "}, {"name": "DEdeg", "desc": "[-40.16/-39.9] Declination (J2000) "}, {"name": "[Fe/H]", "desc": "[-1.5/0.5] Log of Fe/H abundance "}, {"name": "Teff", "desc": "[7000/31000] Effective temperature derived from the SED fitting"}, {"name": "e_Teff", "desc": "[500] Teff uncertainty "}, {"name": "Rad", "desc": "[0.16/4.3] Radius derived from the SED fitting "}, {"name": "e_Rad", "desc": "[0.01/0.2] Rad uncertainty "}, {"name": "Lum", "desc": "[2.95/51] Luminosity derived from the SED fitting"}, {"name": "e_Lum", "desc": "[0.13/1.3] Lum uncertainty "}, {"name": "rChi2", "desc": "[2/480]? Reduced {chi}^2^ "}, {"name": "Nfit", "desc": "[7/20]? The number of points considered in fitting the SED"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_905_52"}} {"id": "J/ApJ/905/52", "title_cds": "Extreme variability QSOs from SDSS DR16", "title_create": "Guo+, 2020", "year": "2020", "author": "Guo H., Peng J., Zhang K., Burke C.J., Liu X., Sun M., Wang S., Kong M., Sheng Z., Wang T., He Z., Gu M.", "title_pub": "High-redshift extreme variability quasars from Sloan Digital Sky Survey multiepoch spectroscopy.", "first_author": "Guo H.", "ref_biblio": [""], "bibcode": ["2020ApJ...905...52G"], "see_also": ["VIII/92 : The FIRST Survey Catalog, Version 2014Dec17 (Helfand+ 2015)", "V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)", "J/ApJ/633/638 : Variable quasar sample from SDSS (Wilhite+, 2005)", "J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006)", "J/ApJ/641/78 : CIV variability in 105 SDSS quasars (Wilhite+, 2006)", "J/ApJ/679/962 : Quasars with strong nitrogen emission lines (Jiang+, 2008)", "J/ApJ/680/169 : SDSS DR5 virial black hole masses (Shen+, 2008)", "J/ApJ/696/870 : Catalina Real-time Transient Survey (CRTS) (Drake+, 2009)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/ApJS/201/23 : Spectroscopy of 88 z<0.7 SDSS QSOs (Eracleous+, 2012)", "J/ApJ/753/125 : NIR spectroscopy follow-up of 60 SDSS-DR7 QSOs (Shen+, 2012)", "J/ApJ/763/32 : Galactic halo RRab stars from CSS (Drake+, 2013)", "J/ApJ/789/140 : SDSS quasars balmer emission lines (Liu+, 2014)", "J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)", "J/ApJS/217/26 : Lick AGN monitoring 2011: light curves (Barth+, 2015)", "J/ApJS/216/4 : SDSS-RM project: technical overview (Shen+, 2015)", "J/ApJ/821/33 : Broad H{beta} emission line in Seyfert galaxies (Runco+, 2016)", "J/ApJ/859/8 : SDSS J120414.37+351800.5 quasar opt. photometry (Liu+, 2018)", "J/ApJ/854/160 : SDSS&DES long-term extreme variability QSOs (Rumbaugh+, 2018)", "J/ApJ/874/8 : Follow-up sp. of SDSS changing-look QSOs (Macleod+, 2019)", "J/ApJS/241/34 : The SDSS Reverberation Mapping (SDSS-RM) project (Shen+, 2019)", "J/ApJ/883/94 : Optical and UV follow-up of 1ES 1927+654 (Trakhtenbrot+, 2019)"], "keyword_cds": "QSOs; Spectra, optical; Redshifts; Equivalent widths; Black holes; Radio sources", "keyword_pub": "Active galactic nuclei ; Quasars ; Black hole physics ; Spectroscopy ; Time domain astronomy", "abstract": ["We perform a systematic search for high-redshift (z>1.5) extreme", "variability quasars (EVQs) using repeat spectra from the Sixteenth", "Data Release of the Sloan Digital Sky Survey, which provides a", "baseline spanning up to ~18yr in the observed frame. We compile a", "sample of 348 EVQs with a maximum continuum variability at rest frame", "1450{AA} of more than 100% (i.e., {delta}V=(Max-Min)/Mean>1). The EVQs", "show a range of emission-line variability, including 23 where at least", "one line in our redshift range disappears below detectability, which", "can then be seen as analogous to low-redshift changing-look quasars", "(CLQs). Importantly, spurious CLQs caused by problematic SDSS spectral", "flux calibration, e.g., fiber-drop issue, have been rejected. The", "similar properties (e.g., continuum/line, difference-composite spectra", "and Eddington ratio) of normal EVQs and CLQs imply that they are", "basically the same physical population with analogous intrinsic", "variability mechanisms, as a tail of a continuous distribution of", "normal quasar properties. In addition, we find no reliable evidence", "(<=1{sigma}) to support that CLQs are a subset of EVQs with less", "efficient accretion. Finally, we also confirm the antibreathing of CIV", "(i.e., the line width increases as luminosity increases) in EVQs and", "find that in addition to the ~0.4dex systematic uncertainty in", "single-epoch CIV virial black hole mass estimates, an extra scatter of", "~0.3dex will be introduced by extreme variability."], "description": ["All the spectra in this work are obtained from the public Sixteenth", "Data Release of Sloan Digital Sky Survey (SDSS DR16) database", "(Ahumada+, 2020, V/154)."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/abc2ce"], "orcid_pub": ["0000-0001-8416-7059"], "data": "f-v", "date_creation": "21-Jun-2022", "xmatch": "J/ApJ/905/52/table3", "last_update": "05-Sep-2022", "catid": "19050052", "date_update": "24-Oct-2022", "tables": [{"name": "table3.dat", "desc": "Catalog ", "columns": [{"name": "GroupID", "desc": "[10859/292717] SDSS DR16 repeat catalog object identifier"}, {"name": "Plate", "desc": "[309/11703] SDSS spectroscopic plate number "}, {"name": "MJD", "desc": "[51792/58543] Modified Julian Date of spectroscopic observation"}, {"name": "Fiber", "desc": "[2/1000] SDSS spectroscopic fiber number "}, {"name": "RAdeg", "desc": "Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-8.5/65.6] Declination (J2000) "}, {"name": "z", "desc": "[1.5/4] Spectroscopic redshift "}, {"name": "Nep", "desc": "[2/23] Number of spectroscopic observations "}, {"name": "FIRST", "desc": "[-1/1] FIRST detection code (1=detected; -1=out of FIRST footprint)"}, {"name": "F1.4GHz", "desc": "[0.7/160]?=-1 Observed FIRST 20cm flux density"}, {"name": "Flag", "desc": "[-1/1] Brightest/faintest epoch flag (1=brightest or -1=faintest epoch)"}, {"name": "1450avg", "desc": "[1/2.1] Rest frame 1450{AA} continuum variability (1)"}, {"name": "F1450", "desc": "[-0.007/122] Rest frame 1450{AA} flux density; erg/s/cm^2^/{AA}"}, {"name": "SN1450", "desc": "[-0.012/26] Signal-to-Noise at 1450{AA} "}, {"name": "SNCIV", "desc": "[0.1/57.2] Signal-to-Noise of CIV line "}, {"name": "L1350", "desc": "[-1/47.2] Log monochromatic 1350{AA} luminosity; erg/s"}, {"name": "e_L1350", "desc": "[0/0.3]?=-1 Uncertainty in L1350 "}, {"name": "FWHM-civ", "desc": "[1199/13274] Whole CIV line Full-Width at Half-Maximum"}, {"name": "e_FWHM-civ", "desc": "[0.2/7636]?=-1 Uncertainty in FWHM-civ "}, {"name": "EW-civ", "desc": "[13.6/283.8] Rest frame broad CIV equivalent width; in Angstroms"}, {"name": "e_EW-civ", "desc": "[0/89.6]?=-1 Uncertainty in EW-civ "}, {"name": "BH-civ", "desc": "[7.2/9.8]?=-1 Log virial BH mass from CIV (2)"}, {"name": "e_BH-civ", "desc": "[0.001/1.2]?=-1 Uncertainty in BH-civ "}, {"name": "BH-mean", "desc": "[7.4/10]?=-1 Log adopted fiducial virial BH mass (3)"}, {"name": "e_BH-mean", "desc": "[0.002/1.2]?=-1 Uncertainty in BH-mean "}, {"name": "LogEdd", "desc": "[-2.1/0.3]?=-999 Log Eddington ratio based on logMBHa"}, {"name": "chi2", "desc": "[1.4/33] Reduced {chi}^2^ for CIV line fitting"}, {"name": "Type", "desc": "[0/1] Type (0=changing-look quasar (CLQ); 1=extreme variability quasar (EVQ), 650 occurrences)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_910_132"}} {"id": "J/ApJ/910/132", "title_cds": "R Coronae Borealis stars. I. IR LCs & sp.", "title_create": "Karambelkar+, 2021", "year": "2021", "author": "Karambelkar V.R., Kasliwal M.M., Tisserand P., De K., Anand S., Ashley M.C.B., Delacroix A., Hankins M., Jencson J.E., Lau R.M., McKenna D., Moore A., Ofek E.O., Smith R.M., Soria R., Soon J., Tinyanont S., Travouillon T., Yao Y.", "title_pub": "Census of R Coronae Borealis stars. I. Infrared light curves from Palomar Gattini IR.", "first_author": "Karambelkar V.R.", "ref_biblio": [""], "bibcode": ["2021ApJ...910..132K"], "see_also": ["I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)", "J/A+A/353/287 : The R CrB stars (Asplund+, 2000)", "J/A+A/461/183 : Variability of classical T Tauri (Grankin+, 2007)", "J/PASP/123/1149 : NSV 11154 BVRI light curves (Kijbunchoo+, 2011)", "J/A+A/539/A51 : Catalogue enriched with R CrB stars (Tisserand, 2012)", "J/MNRAS/453/133 : WISE view of RV Tauri stars (Gezer+, 2015)", "J/AJ/156/148 : Multiwavelength photometry of RCB stars (Montiel+, 2018)", "J/AJ/159/61 : Optical LCs & sp. of the RCB star ZTF18abhjrcf (Lee+, 2020)", "J/A+A/635/A14 : New R Coronae Borealis stars (Tisserand+, 2020)", "J/ApJ/901/L7 : NIR obs. of SGR 1935+215 with PGIR (De+, 2020)"], "keyword_cds": "Stars, variable; Photometry, infrared; Spectra, infrared ; Effective temperatures; Surveys", "keyword_pub": "R Coronae Borealis variable stars ; Hydrogen deficient stars ; Near infrared astronomy ; Time domain astronomy", "abstract": ["We are undertaking the first systematic infrared (IR) census of", "R Coronae Borealis (RCB) stars in the Milky Way, beginning with IR", "light curves from the Palomar Gattini IR (PGIR) survey. The PGIR is a", "30cm J-band telescope with a 25deg2 camera that is surveying", "18000deg^2^ of the northern sky ({delta}>-28{deg}) at a cadence of 2d.", "We present PGIR light curves for 922 RCB candidates selected from a", "mid-IR color-based catalog. Of these 922, 149 are promising RCB", "candidates, as they show pulsations or declines similar to RCB stars.", "The majority of the candidates that are not RCB stars are either", "long-period variables (LPVs) or RV Tauri stars. We identify IR", "color-based criteria to better distinguish between RCB stars and LPVs.", "As part of a pilot spectroscopic run, we obtain NIR spectra for 26 of", "the 149 promising candidates and spectroscopically confirm 11 new RCB", "stars. We detect strong HeI{lambda}10830 features in the spectra of", "all RCB stars, likely originating within high-velocity (200-400km/s)", "winds in their atmospheres. Nine of these RCB stars show ^12^C^16^O", "and ^12^C^18^O molecular absorption features, suggesting that they are", "formed through a white dwarf merger. We detect quasiperiodic", "pulsations in the light curves of five RCB stars. The periods range", "between 30 and 125 days and likely originate from the strange-mode", "instability in these stars. Our pilot run results motivate a dedicated", "IR spectroscopic campaign to classify all RCB candidates."], "description": ["The Palomar Gattini IR (PGIR) is a 25deg^2^ J-band camera on a 30cm", "telescope located atop Mt. Palomar. The PGIR was commissioned in", "2018 September and commenced survey operations in 2019 July.", "Our source catalog comes from the Tisserand+ (2020, J/A+A/635/A14)", "list of 2194 Galactic R Coronae Borealis (RCB) candidates selected", "based on their Wide-field Infrared Survey Explorer (WISE) colors. We", "performed forced aperture photometry using a 3 pixel (~13\") aperture", "on all J-band PGIR images since 2018 November at the locations of", "these candidates to generate light curves for each of them. The", "average cadence between observations is ~2days. The baseline of", "observations is ~500days.", "We used Triplespec, a medium-resolution (R~2700) JHK-band spectrograph", "on the 200 inch Hale telescope at Mt. Palomar. We observed eight known", "RCB stars and 21 candidates on 2019 October 23 and three additional", "candidates on 2020 February 3. We further observed seven more", "candidates on 2020 June 28 with the Spex spectrograph (R~1500) on the", "NASA Infrared Telescope Facility (IRTF) at Maunakea. The IRTF", "observations were acquired as part of program 2020A111 (PI: K. De).", "See Section 4."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Light curve (LC) based priorities, sub-classifications and IR color based priorities for spectroscopic followup of candidates in Tisserand+ (2020, J/A+A/635/A14)", "columns": [{"name": "ID", "desc": "[1/4175] WISE-ToI designation, Tisserand+ (2020, J/A+A/635/A14)"}, {"name": "RAdeg", "desc": "Right Ascension (J2000) (degrees) "}, {"name": "DEdeg", "desc": "[-76.7/75.51] Declination (J2000) (degrees) "}, {"name": "cPrior", "desc": "IR color based priority (see Section 3) "}, {"name": "LCPrior", "desc": "PGIR light curve based priority (1) "}, {"name": "LCsubCl", "desc": "PGIR lightcurve based sub-class "}, {"name": "N", "desc": "n = The 11 newly identified RCB star (see Table 2); column added by CDS"}, {"name": "FileName", "desc": "Name of the light curve for the RCB candidates in subdirectory \"lcs\" in CSV format; column added by CDS"}]}, {"name": "lcs/*", "desc": "Individual light curve for the 1209 RCB candidates in CSV format", "columns": []}, {"name": "table3.dat", "desc": "Properties derived from the spectra of RCB stars ", "columns": [{"name": "Name", "desc": "RCB star identifier "}, {"name": "RV", "desc": "[-170/430]? Radial velocity (1) "}, {"name": "e_RV", "desc": "[20/50]? RV uncertainty "}, {"name": "Teff", "desc": "[4730/5790]? Effective temperature (2) "}, {"name": "e_Teff", "desc": "[130/400]? Lower uncertainty on Teff "}, {"name": "E_Teff", "desc": "[140/360]? Upper uncertainty on Teff "}, {"name": "Tdust", "desc": "[770/920]? Dust temperature "}, {"name": "e_Tdust", "desc": "[35/60]? Lower uncertainty on Tdust "}, {"name": "E_Tdust", "desc": "[25/45]? Upper uncertainty on Tdust "}, {"name": "tauV", "desc": "[0.36/2.21]? Optical depth (2) "}, {"name": "e_tauV", "desc": "[0.04/0.46]? Lower uncertainty on tauV "}, {"name": "E_tauV", "desc": "[0.05/0.25]? Upper uncertainty on tauV "}, {"name": "l_Teffir", "desc": "Limit flag on Teffir "}, {"name": "Teffir", "desc": "[4750/6250]? Effective temperature (3) "}, {"name": "---", "desc": "[-] "}, {"name": "Teffir2", "desc": "[5750]? Upper range of Teffir "}, {"name": "l_O16/O18", "desc": "Limit flag on O16/O18 "}, {"name": "O16/O18", "desc": "[0.5/10]? O16 to O18 ratio (3) "}, {"name": "---", "desc": "[-] "}, {"name": "O16/O18b", "desc": "[2/50]? Upper range of O16/O18 "}, {"name": "FileName", "desc": "Name of the FITS file in subdirectory \"sp\"; column added by CDS"}]}, {"name": "sp/*", "desc": "Medium resolution NIR spectra for the 19 RCB stars in FITS format", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_910_139"}} {"id": "J/ApJ/910/139", "title_cds": "Feedback from outflows in AGNs. III. Mrk78", "title_create": "Revalski+, 2021", "year": "2021", "author": "Revalski M., Meena B., Martinez F., Polack G.E., Crenshaw D.M., Kraemer S.B., Collins N.R., Fischer T.C., Schmitt H.R., Schmidt J., Maksym W.P., Rafelski M.", "title_pub": "Quantifying feedback from narrow line region outflows in nearby active galaxies. III. Results for the Seyfert 2 galaxies Markarian 3, Markarian 78, and NGC 1068.", "first_author": "Revalski M.", "ref_biblio": [""], "bibcode": ["2021ApJ...910..139R"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "J/A+A/442/137 : HI observations of WHISP disk galaxies (Noordermeer+, 2005)", "J/ApJ/661/L143 : Star formation rate in Seyfert galaxies (Wang+, 2007)", "J/ApJ/676/184 : Peculiar motion away from the Local Void (Tully+, 2008)", "J/A+A/564/A125 : AGN Torus model comparison of AGN in CDFS (Buchner+, 2014)", "J/MNRAS/480/2302 : Extended emission-line regions of obscured AGN (Sun+, 2018)", "J/MNRAS/486/4290 : AGN-driven winds through IR emission. II. (Baron+, 2019)", "J/A+A/630/A59 : ALMA datacubes for 48 QSOs (Bischetti+, 2019)", "J/A+A/622/A146 : MAGNUM survey galaxies images (Mingozzi+, 2019)", "J/MNRAS/492/3073 : CALIFA galaxies hosting an AGN (Lacerda+, 2020)", "J/ApJ/902/26 : HST opt. & H-band obs. of Cepheids in NGC4151 (Yuan+, 2020)"], "keyword_cds": "Galaxies, Seyfert; Active gal. nuclei; Spectra, optical", "keyword_pub": "Active galaxies ; Active galactic nuclei ; AGN host galaxies ; Emission line galaxies ; Seyfert galaxies ; Markarian galaxies ; Supermassive black holes ; Galaxy kinematics ; Galaxy winds ; Interstellar medium wind", "abstract": ["Outflows of ionized gas driven by active galactic nuclei (AGN) may", "significantly impact the evolution of their host galaxies. However,", "determining the energetics of these outflows is difficult with", "spatially unresolved observations that are subject to strong global", "selection effects. We present part of an ongoing study using Hubble", "Space Telescope and Apache Point Observatory spectroscopy and imaging", "to derive spatially resolved mass outflow rates and energetics for", "narrow-line region outflows in nearby AGN that are based on", "multi-component photoionization models to account for spatial", "variations in gas ionization, density, abundances, and dust content.", "This expanded analysis adds Mrk 3, Mrk 78, and NGC 1068, doubling our", "earlier sample. We find that the outflows contain total ionized gas", "masses of M~10^5.5^-10^7.5^M_{sun}_ and reach peak velocities of", "v~800-2000km/s. The outflows reach maximum mass outflow rates of", "dM/dt_out_3-12M_{sun}_/yr and encompass total kinetic energies of", "E~10^54^-10^56^erg. The outflows extend to radial distances of", "r~0.1-3kpc from the nucleus, with the gas masses, outflow energetics,", "and radial extents positively correlated with AGN luminosity. The", "outflow rates are consistent with in situ ionization and acceleration", "where gas is radiatively driven at multiple radii. These radial", "variations indicate that spatially resolved observations are essential", "for localizing AGN feedback and determining the most accurate outflow", "parameters."], "description": ["The archival HST spectroscopy and [OIII] imaging used in this study", "were obtained with the Space Telescope Imaging Spectrograph (STIS),", "Wide Field and Planetary Camera 2 (WFPC2), and Faint Object Camera", "(FOC). We retrieved calibrated data (DOI:10.17909/t9-4581-8p50) from", "the Mikulski Archive at the Space Telescope Science Institute (MAST).", "To investigate jet-gas interactions within the narrow line region", "(NLR), Mrk 78 was observed extensively with HST/STIS using the G140L,", "G430L, G430M, and G750M gratings with a 52\"x0.2\" slit (Prog ID 7404,", "PI: M. Whittle).", "For [OIII] imaging, we use FOC observations through the F502M filter", "with F550M for continuum subtraction (Program ID 5140, PI: F. Macchetto).", "We observed Mrk 78 with the Dual Imaging Spectrograph (DIS) on the", "Apache Point Observatory (APO) 3.5m telescope to obtain deep", "spectroscopy of the ionized gas outside of the narrow HST slits.", "See Section 2.2."], "object": ["07 42 41.70 +65 10 37.4 Mrk 78 = LEDA 21624"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table4.dat", "desc": "Mrk 78 HST STIS flux-weighted average emission line ratios", "columns": [{"name": "Pos", "desc": "[-3.2/3.2] Spatial distance from nucleus (G1) "}, {"name": "Ne5-3426", "desc": "[0.5/3.2]? The [NeV] 3426{AA} line ratio (G2) "}, {"name": "e_Ne5-3426", "desc": "[0.29/3.2]? Uncertainty in Ne5-3426 "}, {"name": "O2-3727", "desc": "[1.5/6.8]? The [OII] 3727{AA} line ratio (G2) "}, {"name": "e_O2-3727", "desc": "[0.4/4.6]? Uncertainty in O2-3727 "}, {"name": "Ne3-3869", "desc": "[0.58/5]? The [NeIII] 3869{AA} line ratio (G2) "}, {"name": "e_Ne3-3869", "desc": "[0.3/5]? Uncertainty in Ne3-3869 "}, {"name": "He+Ne3", "desc": "[0.28/1.5]? The H{epsilon}+[NeIII]3969{AA} line ratio (G2)"}, {"name": "e_He+Ne3", "desc": "[0.19/1.2]? Uncertainty in He+Ne3 "}, {"name": "S2-4074", "desc": "[0.24/0.8]? The [SII] 4074{AA} line ratio (G2) "}, {"name": "e_S2-4074", "desc": "[0.13/0.8]? Uncertainty in S2-4074 "}, {"name": "Hd", "desc": "[0.2/1.4]? The H{delta} line ratio (G2) "}, {"name": "e_Hd", "desc": "[0.18/1.4]? Uncertainty in Hd "}, {"name": "Hg", "desc": "[0.28/1.1]? The H{gamma} line ratio (G2) "}, {"name": "e_Hg", "desc": "[0.16/1]? Uncertainty in Hg "}, {"name": "O3-4363", "desc": "[0.16/0.9]? The [OIII] 4363{AA} line ratio (G2) "}, {"name": "e_O3-4363", "desc": "[0.06/0.7]? Uncertainty in O3-4363 "}, {"name": "He2-4686", "desc": "[0.14/0.7]? The HeII 4686{AA} line ratio (G2) "}, {"name": "e_He2-4686", "desc": "[0.07/0.7]? Uncertainty in He2-4686 "}, {"name": "Hb", "desc": "[1] The H{beta} line ratio (G2) "}, {"name": "e_Hb", "desc": "[0.16/1] Uncertainty in Hb "}, {"name": "O3-4959", "desc": "[2/6.2] The [OIII] 4959{AA} line ratio (G2) "}, {"name": "e_O3-4959", "desc": "[0.57/5.7] Uncertainty in O3-4959 "}, {"name": "O3-5007", "desc": "[6/18] The [OIII] 5007{AA} line ratio (G2) "}, {"name": "e_O3-5007", "desc": "[1.7/16] Uncertainty in O3-5007 "}, {"name": "O1-6300", "desc": "[0.15/1.1]? The [OI] 6300{AA} line ratio (G2) "}, {"name": "e_O1-6300", "desc": "[0.13/1.1]? Uncertainty in O1-6300 "}, {"name": "O1-6363", "desc": "[0.09/0.11]? The [OI] 6363{AA} line ratio (G2) "}, {"name": "e_O1-6363", "desc": "[0.04/0.07]? Uncertainty in O1-6363 "}, {"name": "N2-6548", "desc": "[0.54/1]? The [NII] 6548{AA} line ratio (G2) "}, {"name": "e_N2-6548", "desc": "[0.13/0.9]? Uncertainty in N2-6548 "}, {"name": "Ha", "desc": "[2/2.9] The H{alpha} line ratio (G2) "}, {"name": "e_Ha", "desc": "[0.7/2.9] Uncertainty in Ha "}, {"name": "N2-6584", "desc": "[1/2.8]? The [NII] 6584{AA} line ratio (G2) "}, {"name": "e_N2-6584", "desc": "[0.38/2.7]? Uncertainty in N2-6584 "}, {"name": "S2-6716", "desc": "[0.3/1.5]? The [SII] 6716{AA} line ratio (G2) "}, {"name": "e_S2-6716", "desc": "[0.1/1.5]? Uncertainty in S2-6716 "}, {"name": "S2-6731", "desc": "[0.38/2.7]? The [SII] 6731{AA} line ratio (G2) "}, {"name": "e_S2-6731", "desc": "[0.12/2.7]? Uncertainty in S2-6731 "}, {"name": "FHb", "desc": "[0.04/42.6] The H{beta} line flux; erg/s/cm^2^ "}, {"name": "e_FHb", "desc": "[0.03/23] Uncertainty in FHb "}]}, {"name": "table4a.dat", "desc": "Mrk 78 HST STIS observed emission line ratios from slits A-D", "columns": [{"name": "Slit", "desc": "[A-D] Slit identifier "}, {"name": "Pos", "desc": "[-3.5/3.2] Spatial distance from nucleus (G1) "}, {"name": "Ne5-3426", "desc": "[0.29/2.4]? The [NeV] 3426{AA} line ratio (G2) "}, {"name": "e_Ne5-3426", "desc": "[0.1/2.2]? Uncertainty in Ne5-3426 (G2) "}, {"name": "O1-3727", "desc": "[0.67/5.7]? The [OI] 3727{AA} line ratio (G2) "}, {"name": "e_O1-3727", "desc": "[0.1/6.2]? Uncertainty in O1-3727 (G2) "}, {"name": "Ne3-3869", "desc": "[0.3/2.3]? The [NeIII]3869{AA} line ratio (G2) "}, {"name": "e_Ne3-3869", "desc": "[0.1/2.3]? Uncertainty in Ne3-3869 (G2) "}, {"name": "He+Ne3", "desc": "[0.16/1]? The H{epsilon}+[NeIII]3969{AA} line ratio (G2)"}, {"name": "e_He+Ne3", "desc": "[0.07/1.2]? Uncertainty in He+Ne3 (G2) "}, {"name": "S2-4074", "desc": "[0.2/0.7]? The [SII] 4074{AA} line ratio (G2) "}, {"name": "e_S2-4074", "desc": "[0.1/0.7]? Uncertainty in S2-4074 (G2) "}, {"name": "Hd", "desc": "[0.18/1.4]? The H{delta} line ratio (G2) "}, {"name": "e_Hd", "desc": "[0.13/1.8]? Uncertainty in Hd (G2) "}, {"name": "Hg", "desc": "[0.2/1.2]? The H{gamma} line ratio (G2) "}, {"name": "e_Hg", "desc": "[0.08/1.7]? Uncertainty in Hg (G2) "}, {"name": "O3-4363", "desc": "[0.1/1.4]? The [OIII] 4363{AA} line ratio (G2) "}, {"name": "e_O3-4363", "desc": "[0.05/2.8]? Uncertainty in O3-4363 (G2) "}, {"name": "He2-4686", "desc": "[0.1/0.9]? The HeII 4686{AA} line ratio (G2) "}, {"name": "e_He2-4686", "desc": "[0.06/1.1]? Uncertainty in He2-4686 (G2) "}, {"name": "Hb", "desc": "[1]? The H{beta} line ratio (G2) "}, {"name": "e_Hb", "desc": "[0.06/0.99]? Uncertainty in Hb (G2) "}, {"name": "O3-4959", "desc": "[1.46/8.6]? The [OIII]4959{AA} line ratio (G2) "}, {"name": "e_O3-4959", "desc": "[0.24/8.6]? Uncertainty in O3-4959 (G2) "}, {"name": "O3-5007", "desc": "[4.4/26]? The [OIII] 5007{AA} line ratio (G2) "}, {"name": "e_O3-5007", "desc": "[0.7/26]? Uncertainty in O3-5007 (G2) "}, {"name": "O1-6300", "desc": "[0.15/2.4]? The [OI] 6300{AA} line ratio (G2) "}, {"name": "e_O1-6300", "desc": "[0.14/4]? Uncertainty in O1-6300 (G2) "}, {"name": "O1-6363", "desc": "[0.23/0.6]? The [OI] 6363{AA} line ratio (G2) "}, {"name": "e_O1-6363", "desc": "[0.1/0.9]? Uncertainty in O1-6363 (G2) "}, {"name": "N2-6548", "desc": "[0.58/6.3]? The [NII] 6548{AA} line ratio (G2) "}, {"name": "e_N2-6548", "desc": "[0.1/6.3]? Uncertainty in N2-6548 (G2) "}, {"name": "Ha", "desc": "[1.59/21.1]? The H{alpha} line ratio (G2) "}, {"name": "e_Ha", "desc": "[0.5/21]? Uncertainty in Ha (G2) "}, {"name": "N2-6584", "desc": "[0.96/18.5]? The [NII]6584{AA} line ratio (G2) "}, {"name": "e_N2-6584", "desc": "[0.3/18.4]? Uncertainty in N2-6584 (G2) "}, {"name": "S2-6716", "desc": "[0.48/4.2]? The [SII] 6716{AA} line ratio (G2) "}, {"name": "e_S2-6716", "desc": "[0.18/3.9]? Uncertainty in S2-6716 (G2) "}, {"name": "S2-6731", "desc": "[0.5/4.5]? The [SII] 6731{AA} line ratio (G2) "}, {"name": "e_S2-6731", "desc": "[0.2/3.6]? Uncertainty in S2-6731 (G2) "}]}, {"name": "table4b.dat", "desc": "Mrk 78 HST STIS reddening-corrected emission line ratios from slits A-D", "columns": [{"name": "Slit", "desc": "[A-D] Slit identifier "}, {"name": "Pos", "desc": "[-3.5/3.2] Spatial distance from nucleus (G1) "}, {"name": "Ne5-3426", "desc": "[0.48/4.4]? The [NeV] 3426{AA} line ratio (1) "}, {"name": "e_Ne5-3426", "desc": "[0.2/5.5]? Uncertainty in Ne5-3426 (1) "}, {"name": "O1-3727", "desc": "[1/11.7]? The [OI] 3727{AA} line ratio (1) "}, {"name": "e_O1-3727", "desc": "[0.2/11]? Uncertainty in O1-3727 (1) "}, {"name": "Ne3-3869", "desc": "[0.4/5.1]? The [NeIII] 3869{AA} line ratio (1) "}, {"name": "e_Ne3-3869", "desc": "[0.15/7.6]? Uncertainty in Ne3-3869 (1) "}, {"name": "He+Ne3", "desc": "[0.2/2]? The H{epsilon}+[NeIII]3969{AA} line ratio (1)"}, {"name": "e_He+Ne3", "desc": "[0.1/1.6]? Uncertainty in He+Ne3 (1) "}, {"name": "S2-4074", "desc": "[0.24/1.1]? The [SII] 4074{AA} line ratio (1) "}, {"name": "e_S2-4074", "desc": "[0.13/1]? Uncertainty in S2-4074 (1) "}, {"name": "Hd", "desc": "[0.2/1.4]? The H{delta} line ratio (1) "}, {"name": "e_Hd", "desc": "[0.15/1.8]? Uncertainty in Hd (1) "}, {"name": "Hg", "desc": "[0.24/1.3]? The H{gamma} line ratio (1) "}, {"name": "e_Hg", "desc": "[0.1/2.2]? Uncertainty in Hg (1) "}, {"name": "O3-4363", "desc": "[0.12/1.7]? The [OIII] 4363{AA} line ratio (1) "}, {"name": "e_O3-4363", "desc": "[0.05/3.6]? Uncertainty in O3-4363 (1) "}, {"name": "He2-4686", "desc": "[0.1/1]? The HeII 4686{AA} line ratio (1) "}, {"name": "e_He2-4686", "desc": "[0.06/1.1]? Uncertainty in He2-4686 (1) "}, {"name": "Hb", "desc": "[1]? The H{beta} line ratio (1) "}, {"name": "e_Hb", "desc": "[0.06/1]? Uncertainty in Hb (1) "}, {"name": "O3-4959", "desc": "[1.46/8.1]? The [OIII] 4959{AA} line ratio (1) "}, {"name": "e_O3-4959", "desc": "[0.23/8.1]? Uncertainty in O3-4959 (1) "}, {"name": "O3-5007", "desc": "[4.4/23.7]? The [OIII] 5007{AA} line ratio (1) "}, {"name": "e_O3-5007", "desc": "[0.7/23.7]? Uncertainty in O3-5007 (1) "}, {"name": "O1-6300", "desc": "[0.1/1.5]? The [OI] 6300{AA} line ratio (1) "}, {"name": "e_O1-6300", "desc": "[0.1/2.1]? Uncertainty in O1-6300 (1) "}, {"name": "O1-6363", "desc": "[0.09/0.5]? The [OI] 6363{AA} line ratio (1) "}, {"name": "e_O1-6363", "desc": "[0.04/0.7]? Uncertainty in O1-6363 (1) "}, {"name": "N2-6548", "desc": "[0.4/1.2]? The [NII] 6548{AA} line ratio (1) "}, {"name": "e_N2-6548", "desc": "[0.09/1]? Uncertainty in N2-6548 (1) "}, {"name": "Ha", "desc": "[1.59/2.92]? The H{alpha} line ratio (1) "}, {"name": "e_Ha", "desc": "[0.45/4]? Uncertainty in Ha (1) "}, {"name": "N2-6584", "desc": "[0.89/3.3]? The [NII] 6584{AA} line ratio (1) "}, {"name": "e_N2-6584", "desc": "[0.27/3.5]? Uncertainty in N2-6584 (1) "}, {"name": "S2-6716", "desc": "[0.25/1.5]? The [SII] 6716{AA} line ratio (1) "}, {"name": "e_S2-6716", "desc": "[0.1/1.8]? Uncertainty in S2-6716 (1) "}, {"name": "S2-6731", "desc": "[0.3/2.7]? The [SII] 6731{AA} line ratio (1) "}, {"name": "e_S2-6731", "desc": "[0.1/3.7]? Uncertainty in S2-6731 (1) "}, {"name": "E(B-V)", "desc": "[0/1.9]? The (B-V) color excess "}, {"name": "e_E(B-V)", "desc": "[0.1/0.8]? Uncertainty in E(B-V) "}, {"name": "Hbc", "desc": "[0.03/20]? Extinction-corrected H{beta} line flux; in erg/s/cm^2^"}, {"name": "e_Hbc", "desc": "[0.02/18]? Uncertainty in Hbc "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_910_160"}} {"id": "J/ApJ/910/160", "title_cds": "Fermi LAT sources observed with the GMRT", "title_create": "Bhattacharyya+, 2021", "year": "2021", "author": "Bhattacharyya B., Roy J., Johnson T.J., Ray P.S., Freire P.C.C., Gupta Y., Bhattacharya D., Kaninghat A., Stappers B.W., Ferrara E.C., Sengupta S., Rathour R.S., Kerr M., Smith D.A., Parkinson P.M.S., Ransom S.M., Michelson P.F.", "title_pub": "Discovery and timing of three millisecond pulsars in radio and gamma-rays with the Giant Metrewave Radio Telescope and Fermi Large Area Telescope.", "first_author": "Bhattacharyya B.", "ref_biblio": [""], "bibcode": ["2021ApJ...910..160B"], "see_also": ["B/psr : ATNF Pulsar Catalogue (Manchester+, 2005)", "J/ApJS/188/405 : Fermi-LAT first source catalog (1FGL) (Abdo+, 2010)", "J/ApJ/753/83 : Associations to 1FGL sources (Ackermann+, 2012)", "J/ApJS/199/31 : Fermi LAT second source catalog (2FGL) (Nolan+, 2012)", "J/ApJS/208/17 : 2nd Fermi LAT cat. of gamma-ray pulsars (2PC) (Abdo+, 2013)", "J/ApJS/209/34 : The first Fermi-LAT >10GeV catalog (1FHL) (Ackermann+, 2013)", "J/ApJS/232/18 : The third Fermi-LAT >10GeV catalog (3FHL) (Ajello+, 2017)", "J/ApJS/247/33 : The Fermi LAT fourth source catalog (4FGL) (Abdollahi+, 2020)"], "keyword_cds": "Pulsars; Gamma rays; Radio sources", "keyword_pub": "High energy astrophysics ; High time resolution astrophysics ; Millisecond pulsars ; Radio astronomy ; Gamma-ray astronomy ; Binary pulsars", "abstract": ["We performed deep observations to search for radio pulsations in the", "directions of 375 unassociated Fermi Large Area Telescope {gamma}-ray", "sources using the Giant Metrewave Radio Telescope (GMRT) at 322 and", "607MHz. In this paper we report the discovery of three millisecond", "pulsars (MSPs), PSR J0248+4230, PSR J1207-5050, and PSR J1536-4948. We", "conducted follow-up timing observations for ~5yr with the GMRT and", "derived phase-coherent timing models for these MSPs. PSR J0248+4230", "and J1207-5050 are isolated MSPs having periodicities of 2.60ms and", "4.84ms. PSR J1536-4948 is a 3.07ms pulsar in a binary system with an", "orbital period of ~62 days about a companion of a minimum mass of", "0.32M_{sun}_. We also present multifrequency pulse profiles of these", "MSPs from the GMRT observations. PSR J1536-4948 is an MSP with an", "extremely wide pulse profile having multiple components. Using the", "radio timing ephemeris we subsequently detected {gamma}-ray pulsations", "from these three MSPs, confirming them as the sources powering the", "{gamma}-ray emission. For PSR J1536-4948 we performed combined", "radio-{gamma}-ray timing using ~11.6yr of {gamma}-ray pulse times of", "arrival (TOAs) along with the radio TOAs. PSR J1536-4948 also shows", "evidence for pulsed {gamma}-ray emission out to above 25GeV,", "confirming earlier associations of this MSP with a >=10GeV point", "source. The multiwavelength pulse profiles of all three MSPs offer", "challenges to models of radio and {gamma}-ray emission in pulsar", "magnetospheres."], "description": ["As part of a broader effort coordinated by the Fermi PSC, we selected", "sources from early versions of the Fermi-LAT catalogs (Abdo+ 2010,", "J/ApJS/188/405 and Nolan+ 2012, J/ApJS/199/31), analyses of sources", "that were not associated with likely {gamma}-ray-emitting counterparts", "and were visible from the Giant Metrewave Radio Telescope (GMRT).", "The search observations were performed between 2010 November and 2013", "September with the GMRT Software Backend (GSB), producing simultaneous", "incoherent and coherent beam filter-bank outputs of 512x0.0651MHz", "sampled every 61.44us. Details of the observational configuration are", "described in Bhattacharyya+ (2013ApJ...773L..12B)."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table4.dat", "desc": "Summary of the GMRT observations ", "columns": [{"name": "ID", "desc": "Source designation "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "MJD", "desc": "[55521.59/56552.14] Observing epoch (MJD) "}, {"name": "Freq", "desc": "[322/607] Observed frequency "}, {"name": "Dur", "desc": "[3/150] Duration "}, {"name": "Smin", "desc": "[0.2/4.9] 10{sigma} detection limit (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_910_151"}} {"id": "J/ApJ/910/151", "title_cds": "KMTNet BVi photometry of SNIa KSP-OT-201509b", "title_create": "Moon+, 2021", "year": "2021", "author": "Moon D.-S., Ni Y.Qi, Drout M.R., Gonzalez-Gaitan S., Afsariardchi N., Park H.S., Lee Y., Kim S.C., Antoniadis J., Kim D.-J., Lee Y.", "title_pub": "Rapidly declining hostless type Ia supernova KSP-OT-201509b from the KMTNet Supernova Program: transitional nature and constraint on ^56^Ni distribution and progenitor type.", "first_author": "Moon D.-S.", "ref_biblio": [""], "bibcode": ["2021ApJ...910..151M"], "see_also": ["J/MNRAS/383/1485 : BVRI light curves of SN 2003jd (Valenti+, 2008)", "J/AJ/139/519 : Carnegie supernova project. SNe Ia (Contreras+, 2010)", "J/MNRAS/412/1441 : SNe luminosity functions (Li+, 2011)", "J/MNRAS/448/1345 : YJK for Type Ia supernovae (Dhawan+, 2015)", "J/A+A/578/A9 : Optical and NIR spectra of SN iPTF13ebh (Hsiao+, 2015)", "J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. (Riess+, 2016)", "J/ApJ/826/144 : Follow-up observations of SNIa ASASSN-14lp (Shappee+, 2016)", "J/ApJ/836/60 : Bgri light curves of PTF11kmb and PTF12bho (Lunnan+, 2017)", "J/ApJ/869/56 : Updated calibration of CSP-I SNe Ia sample (Burns+, 2018)", "J/ApJ/881/22 : BVI phot. of TypeII SN KSP-SN-2016kf (Afsariardchi+, 2019)", "J/ApJ/870/L1 : K2 obs. of type Ia supernova SN 2018oh (Dimitriadis+, 2019)", "J/A+A/627/A174 : Early light curve of SN 2013gy (Holmbo+, 2019)", "J/MNRAS/483/628 : SN Ia properties using bolometric LCs (Scalzo+, 2019)", "J/ApJ/870/13 : K2 LC alternative analysis of ASASSN-18bt (Shappee+, 2019)", "J/A+A/634/A37 : TURTLS Light curves of ^56^Ni distributions (Magee+, 2020)", "J/ApJ/898/56 : UVOT, ZTF gri LCs & sp. of the SN Ia 2019yvq (Miller+, 2020)", "J/ApJ/908/51 : TESS early LCs of type Ia Supernovae (Fausnaugh+, 2021)"], "keyword_cds": "Supernovae; Photometry, UBVRI", "keyword_pub": "Type Ia supernovae ; Supernovae", "abstract": ["We report the early discovery and multicolor (BVI) high-cadence", "light-curve analyses of the rapidly declining sub-Chandrasekhar Type", "Ia supernova KSP-OT-201509b (= AT 2015cx) from the KMTNet Supernova", "Program. The Phillips and color stretch parameters of KSP-OT-201509b", "are {Delta}M_B,15_~1.62mag and s_BV_~0.54, respectively, at an", "inferred redshift of 0.072. These, together with other measured", "parameters (such as the strength of the secondary I-band peak, colors,", "and luminosity), identify the source to be a rapidly declining Type Ia", "of a transitional nature that is closer to Branch-normal than", "91bg-like. Its early light-curve evolution and bolometric luminosity", "are consistent with those of homologously expanding ejecta powered by", "radioactive decay and a Type Ia SN explosion with 0.32+/-0.01M_{sun}_", "of synthesized ^56^Ni mass, 0.84+/-0.12M_{sun}_ of ejecta mass, and", "(0.61+/-0.14)x10^51^erg of ejecta kinetic energy. While its B-V and", "V-I colors evolve largely synchronously with the changes in the I-band", "light curve, as found in other supernovae, we also find the presence", "of an early redward evolution in V-I prior to -10 days since peak. The", "bolometric light curve of the source is compatible with a stratified", "^56^Ni distribution extended to shallow layers of the exploding", "progenitor. Comparisons between the observed light curves and those", "predicted from ejecta-companion interactions clearly disfavor Roche", "lobe-filling companion stars at large separation distances, thus", "supporting a double-degenerate scenario for its origin. The lack of", "any apparent host galaxy in our deep stack images reaching a", "sensitivity limit of ~28mag/arcsec^2^ makes KSP-OT-201509b a hostless", "Type Ia supernova and offers new insights into supernova host galaxy", "environments."], "description": ["We conducted high-cadence, multicolor (BVI) monitoring observations of", "a 2{deg}x2{deg} field containing the galaxy NGC 300 in the direction", "of the south Galactic pole using the Korea Microlensing Telescope", "Network (KMTNet) as part of its KMTNet Supernova Program (KSP;", "Moon+ 2016SPIE.9906E..4IM and Afsariardchi+ 2019, J/ApJ/881/22). The", "initial phase of the monitoring started in 2015 July during the", "commissioning test period of the KMTNet and continued until", "2017 August 9. The KMTNet operates three wide-field 1.6m telescopes", "located at the Cerro Tololo Inter-American Observatory (CTIO; Chile),", "the South African Astronomical Observatory (SAAO), and the Siding", "Spring Observatory (SSO; Australia). We obtained about 2460 images of", "the field with 60s exposure time for each of the Johnson-Cousins BVI", "bands, and the mean cadence of our observations within the monitoring", "period was approximately 3.5hr for each band.", "The BV-band magnitudes of KSP-OT-201509b presented in this paper are", "in the Vega magnitude system, while its I-band magnitudes are in the", "AB system. See Section 2."], "object": ["00 57 03.19 -37 02 23.6 KSP-OT-201509b = AT 2015cx"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Observed KMTNet BVi magnitudes of KSP-OT-201509b ", "columns": [{"name": "MJD", "desc": "[57289.89/57359.48] Time, Modified Julian Date (JD-2400000.5)"}, {"name": "omag", "desc": "[18.37/22.18] Observed magnitude in Filt (1) "}, {"name": "e_omag", "desc": "[0.016/0.5] Uncertainty in omag "}, {"name": "Filt", "desc": "[BVi] Band "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_12"}} {"id": "J/ApJ/911/12", "title_cds": "HST opt-NIR obs. of Cepheids in NGC5584", "title_create": "Javanmardi+, 2021", "year": "2021", "author": "Javanmardi B., Merand A., Kervella P., Breuval L., Gallenne A., Nardetto N., Gieren W., Pietrzynski G., Hocde V., Borgniet S.", "title_pub": "Inspecting the Cepheid distance ladder: the Hubble Space Telescope distance to the SN Ia host galaxy NGC 5584.", "first_author": "Javanmardi B.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...12J"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "J/AJ/128/2815 : ARAUCARIA project: NGC 6822 Cepheid var. (Pietrzynski+, 2004)", "J/ApJ/627/579 : Photometry of variables in NGC 3370 (Riess+, 2005)", "J/AcA/58/163 : VI light curves of LMC classical Cepheids (Soszynski+, 2008)", "J/ApJ/699/539 : Cepheids in SN-Ia host galaxies (Riess+, 2009)", "J/ApJ/738/27 : Galactic HII regions RRL and continuum data (Balser+, 2011)", "J/AJ/149/117 : LMC infrared survey. I. Photometry of Cepheids (Macri+, 2015)", "J/A+A/584/A80 : Pulsation model data for delta Cep and eta Aql (Merand+, 2015)", "J/ApJ/830/10 : >20yrs of HST obs. of Cepheids (Hoffmann+, 2016)", "J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. (Riess+, 2016)", "J/A+A/605/A79 : TGAS Cepheids and RR Lyrae stars (Gaia Collaboration+, 2017)", "J/ApJ/869/56 : Updated calibration of the CSP-I SNe Ia sample (Burns+, 2018)", "J/A+A/620/A99 : SMC Cepheids K-band and RV curves (Gieren+, 2018)", "J/A+A/619/A8 : Cepheid period-luminosity-metallicity (Groenewegen, 2018)", "J/ApJ/867/108 : Stellar masses & rest-frame u-g colors of SNIa (Jones+, 2018)", "J/A+A/615/A68 : Type Ia supernova luminosities (Roman+, 2018)", "J/ApJ/885/161 : 90 cepheid candidates nearby NGC 6814 (Bentz+, 2019)", "J/A+A/631/A37 : Classical Cepheids consistent RVs (Borgniet+, 2019)", "J/A+A/622/A60 : Gaia DR2 misclassified RR Lyrae list (Clementini+, 2019)", "J/A+A/622/A164 : Radial velocity curves of 11 Cepheids (Gallenne+, 2019)", "J/A+A/623/A72 : Binarity of HIP stars from Gaia pm anomaly (Kervella+, 2019)", "J/A+A/623/A117 : Gal. Cepheids & RR Lyrae multiplicity. II (Kervella+, 2019)", "J/ApJ/876/85 : HST observations for LMC Cepheids (Riess+, 2019)", "J/A+A/625/A14 : Reclassification of Cepheids in the Gaia DR2 (Ripepi+, 2019)", "J/A+A/641/A79 : FEDReD. Extinction map with 2MASS & Gaia DR2 (Hottier+, 2020)", "J/ApJ/889/5 : HST obs. of Mira var. in the SNIa host NGC1559 (Huang+, 2020)", "J/ApJ/896/L43 : Cepheids HST amplitudes in V- and H-band (Riess+, 2020)"], "keyword_cds": "Photometry, HST; Photometry, UBVRI; Stars, variable; Galaxies, nearby; Supernovae", "keyword_pub": "Observational cosmology ; Cosmological parameters ; Hubble constant ; Cepheid distance ; Galaxies ; Type Ia supernovae ; Variable stars ; Photometry ; Light curves ; Stellar photometry ; Astronomy data analysis ; Galaxy distances", "abstract": ["The current tension between the direct and the early-universe", "measurements of the Hubble constant, H_0_, requires detailed scrutiny", "of all the data and methods used in the studies on both sides of the", "debate. The Cepheids in the Type Ia supernova (SN Ia) host galaxy", "NGC5584 played a key role in the local measurement of H_0_. The SH0ES", "(Supernovae H_0_ for the Equation of State) project used the", "observations of this galaxy to derive a relation between the Cepheids'", "periods and ratios of their amplitudes in different optical bands of", "the Hubble Space Telescope and used these relations to analyze the", "light curves of the Cepheids in around half of the current sample of", "local SN Ia host galaxies. In this work, we present an independent", "detailed analysis of the Cepheids in NGC5584. We employ different", "tools for our photometric analysis and a completely different method", "for our light-curve analysis, and we do not find a systematic", "difference between our period and mean magnitude measurements compared", "to those reported by SH0ES. By adopting a period-luminosity relation", "calibrated by the Cepheids in the Milky Way, we measure a distance", "modulus {mu}=31.810+/-0.047 (mag), which is in agreement with", "{mu}=31.786+/-0.046 (mag) measured by SH0ES. In addition, the", "relations we find between the periods and amplitude ratios of the", "Cepheids in NGC5584 are significantly tighter than those of SH0ES, and", "their potential impact on the direct H0 measurement will be", "investigated in future studies."], "description": ["We obtain the data of NGC 5584 from the Mikulski Archive for Space", "Telescopes (MAST) database. NGC 5584 has been observed by the Wide", "Field Camera 3 (WFC3) between 2010 January and April with the purpose", "of measuring a Cepheid distance to the SN Ia SN 2007af hosted by this", "galaxy (PI: Adam Riess, Cycle: 17, Proposal ID: 11570).", "NGC 5584 has been observed in 13 epochs (in total 45540s) in the F555W", "band, 6 of which are also accompanied by F814W observations (in total", "14400s). In 12 of these epochs, this galaxy has also been observed in", "the F350LP band (in total 15000sc). In addition, NGC 5584 has also", "been observed with the WFC3/IR channel with the F160W or the H band in", "two epochs (in total 4929s)."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Our measurements for the photometric properties of the Cepheids in NGC 5584", "columns": [{"name": "ID", "desc": "[82928/1073816] Identifier (1) "}, {"name": "RAdeg", "desc": "[215.57/215.62] Right ascension (J2000) (1) "}, {"name": "DEdeg", "desc": "[-0.41/-0.36] Declination (J2000) (1) "}, {"name": "Umag", "desc": "[25/27.98] HST WFC3/UVIS F350LP band magnitude "}, {"name": "e_Umag", "desc": "[0.008/0.12] Uncertainty on F350LP "}, {"name": "Uamp", "desc": "[0.15/0.45] F350LP amplitude "}, {"name": "Vmag", "desc": "[25.24/28.27] HST WFC3/UVIS F555W band magnitude "}, {"name": "e_Vmag", "desc": "[0.01/0.2] Uncertainty on the Vmag "}, {"name": "Vamp", "desc": "[0.18/0.5] Vmag amplitude "}, {"name": "Imag", "desc": "[24.18/27.23] HST WFC3/UVIS F814W band magnitude "}, {"name": "e_Imag", "desc": "[0.009/0.2] Uncertainty on the Imag "}, {"name": "Iamp", "desc": "[0.1/0.32] Imag amplitude "}, {"name": "Hmag", "desc": "[23.13/26.24]? HST WFC3/IR F160W band magnitude "}, {"name": "e_Hmag", "desc": "[0.013/0.3]? Uncertainty on the Hmag "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_20"}} {"id": "J/ApJ/911/20", "title_cds": "Power sp. density analysis of time series. II.", "title_create": "Tarnopolski+, 2021", "year": "2021", "author": "Tarnopolski M., Marchenko V.", "title_pub": "A comprehensive power spectral density analysis of astronomical time series. II. The Swift/BAT long gamma-ray bursts.", "first_author": "Tarnopolski M.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...20T"], "see_also": ["J/ApJS/166/298 : Sp. cat. of bright BATSE gamma-ray bursts (Kaneko+, 2006)", "J/MNRAS/431/3608 : BeppoSAX/GRBM and Fermi/GBM long GRBs (Dichiara+, 2013)", "J/ApJ/777/132 : A search for progenitors of short GRBs (Dichiara+, 2013)", "J/ApJS/211/13 : The second Fermi/GBM GRB catalog (4yr) (von Kienlin+, 2014)", "J/A+A/589/A97 : GRBs Ep and Fourier PDS slope correlation (Dichiara+, 2016)", "J/A+A/589/A98 : Swift GRBs individual power density sp. (Guidorzi+, 2016)", "J/ApJ/829/7 : 3rd Swift/BAT GRB catalog (past ~11yrs) (BAT3) (Lien+, 2016)", "J/ApJ/867/131 : Blazar cand. behind the Magellanic Clouds (Zywucka+, 2018)", "J/ApJ/896/20 : Swift BAT gamma-ray burst durations (Jespersen+, 2020)", "J/ApJ/896/L20 : Swift BAT gamma-ray burst durations (Jespersen+, 2020)", "J/ApJ/893/46 : The fourth Fermi-GBM GRB catalog: 10yrs (von Kienlin+, 2020)"], "keyword_cds": "GRB; Photometry; Redshifts", "keyword_pub": "Gamma-ray bursts ; Astrostatistics ; Astronomy data analysis ; Light curves", "abstract": ["We have investigated the prompt light curves of long gamma-ray bursts", "(GRBs) from the Swift/BAT catalog. We aimed to characterize their", "power spectral densities (PSDs), search for quasiperiodic oscillations", "(QPOs), and conduct novel analyses directly in the time domain. We", "analyzed the PSDs using Lomb-Scargle periodograms, and searched for", "QPOs using wavelet scalograms. We also attempted to classify the GRBs", "using the Hurst exponent, H, and the A-T plane. The PSDs fall into", "three categories: power law (PL; P(f){propto}1/f^{beta}^) with index", "{beta}{in}(0,2), PL with a non-negligible Poisson noise level (PLC)", "with {beta}{in}(1,3), and a smoothly broken PL (with Poisson noise", "level) yielding high-frequency index {beta}2{in}(2,6). The latter", "yields break timescales of the order of 1-100s. The PL and PLC models", "are broadly consistent with fully developed turbulence, {beta}=5/3.", "For an overwhelming majority of GRBs (93%), H>0.5, implying ubiquity", "of the long-term memory. We find no convincing substructure in the A-T", "plane. Finally, we report on 34 new QPOs, with one or more constant", "leading periods, as well as several chirping signals. The presence of", "breaks and QPOs suggests the existence of characteristic timescales", "that in at least some GRBs might be related to the dynamical", "properties of plasma trajectories in the accretion disks powering the", "relativistic jets."], "description": ["The mask-weighted, background-subtracted light curves (LCs), in a 64ms", "binning and covering the total energy range 15-350keV, were downloaded", "from the Swift/BAT catalog (Lien+ 2016, J/ApJ/829/7). The portions of", "the LCs within respective T_100_ intervals were extracted. We focus on", "long gamma-ray bursts (GRBs) with a sufficient number of points to", "conduct a meaningful time series and power spectral density (PSD)", "analysis. We therefore utilized LCs with more than 50 points, i.e.,", "with T_100_>3.2s. We excluded confirmed short GRBs with extended", "emission. We ended with 1160 GRBs in our sample."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Time series and power spectral density (PSD) properties of the gamma-ray bursts (GRBs)", "columns": [{"name": "Seq", "desc": "[1/1354] Consecutive number of the GRB in the sample (reverse chronological order)"}, {"name": "---", "desc": "[GRB] "}, {"name": "GRB", "desc": "Identifying name of the GRB, according to the Swift catalog"}, {"name": "---", "desc": "[-] "}, {"name": "m_GRB", "desc": "? Multiple index component on GRB140716A (following the Swift catalog)"}, {"name": "T90", "desc": "[0/811]? Duration of the GRB "}, {"name": "betaPL", "desc": "[-0.3/2.1]? Exponent beta of the pure PL fit"}, {"name": "e_betaPL", "desc": "[0/0.06]? Uncertainty of the exponent beta of the pure PL fit"}, {"name": "betaPLC", "desc": "[0.4/12.4]? Exponent beta of the PL plus Poisson noise (PLC) fit"}, {"name": "e_betaPLC", "desc": "[0/7.3]? Uncertainty of the exponent beta of the PL plus Poisson noise (PLC) fit"}, {"name": "beta1SBPL", "desc": "[-7.8/1.91]? Low-frequency exponent beta1 of the SBPL fit"}, {"name": "e_beta1SBPL", "desc": "[0/2.9]? Uncertainty of the low-frequency exponent beta1 of the SBPL fit"}, {"name": "beta2SBPL", "desc": "[0.98/15.32]? High-frequency exponent beta2 of the SBPL fit"}, {"name": "e_beta2SBPL", "desc": "[0/9.7]? Uncertainty of the high-frequency exponent beta2 of the SBPL fit"}, {"name": "Tbreak", "desc": "[0.6/409]? Break time scale of the SBPL fit "}, {"name": "e_Tbreak", "desc": "[0.01/448]? Uncertainty of the break time scale of the SBPL fit"}, {"name": "MVTS", "desc": "[0.17/61.1]? Minimum variability time scale "}, {"name": "e_MVTS", "desc": "[0/48]? Uncertainty of the minimum variability time scale"}, {"name": "H", "desc": "[0.09/0.95]? Hurst exponent "}, {"name": "e_H", "desc": "[0.03/0.8]? Uncertainty of the Hurst exponent"}, {"name": "HPL", "desc": "[0/1]? Hurst exponent inferred from the index betaPL"}, {"name": "e_HPL", "desc": "[0/0.03]? Uncertainty of the Hurst exponent inferred from the index betaPL"}, {"name": "z", "desc": "[0.013/9.4]? Redshift "}, {"name": "Epeak", "desc": "[32.7/4728]? Peak energy of the spectral model"}, {"name": "e_Epeak", "desc": "[1/918]? Uncertainty of the peak energy of the spectral model"}, {"name": "logLiso", "desc": "[49.8/54.2]? Logarithm of the peak isotropic luminosity, erg/s"}, {"name": "e_logLiso", "desc": "[0.01/0.3]? Uncertainty of the logarithm of the peak isotropic luminosity"}]}, {"name": "table2.dat", "desc": "Identified quasiperiodic oscillations (QPOs) ", "columns": [{"name": "Seq", "desc": "[6/1335] Number as in Table 1 "}, {"name": "---", "desc": "[GRB] "}, {"name": "GRB", "desc": "GRB name "}, {"name": "Per", "desc": "Period(s) (1) "}, {"name": "Comm", "desc": "Comment (2) "}, {"name": "f_Comm", "desc": "Flag on Comm (3) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_21"}} {"id": "J/ApJ/911/21", "title_cds": "", "title_create": "Barsanti+, 2021", "year": "2021", "author": "Barsanti S., Owers M.S., McDermid R.M., Bekki K., Bryant J.J., Croom S.M., Oh S., Robotham A.S.G., Scott N., van de Sande J.", "title_pub": "The colors of bulges and disks in the core and outskirts of galaxy clusters.", "first_author": "Barsanti S.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...21B"], "see_also": ["II/350 : VLT Survey Telescope ATLAS (Shanks+, 2015)", "V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)", "J/ApJ/542/673 : Morphological types of galaxies in clusters (Fasano+, 2000)", "J/MNRAS/329/87 : 2dF Galaxy z Survey: gal. clusters (de Propris+, 2002)", "J/MNRAS/366/645 : LARCS. 11 X-ray luminous clusters (Pimbblet+, 2006)", "J/ApJ/671/1503 : Cl 0024+16 and MS 0451-03 spectrophotometry (Moran+, 2007)", "J/MNRAS/393/1531 : BUDDA structural properties of galaxies (Gadotti+, 2009)", "J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies (Simard+, 2011)", "J/MNRAS/440/1690 : Bulge and disc colours of ETG in Coma (Head+, 2014)", "J/ApJS/210/3 : SDSS bulge, disk & total stellar masses (Mendel+, 2014)", "J/MNRAS/446/3943 : galaxies 2D phot. decompositions in SDSS-DR7 (Meert+, 2015)", "J/MNRAS/455/2440 : Gal. 2D phot. decompositions in r, g & i (Meert+, 2016)", "J/MNRAS/481/5580 : Formation sequence of S0 galaxies (Fraser-McKelvie+, 2018)"], "keyword_cds": "", "keyword_pub": "Galaxy clusters ; Galaxy evolution ; Galaxy structure ; Redshift surveys ; Galaxy colors", "abstract": ["The role of the environment on the formation of S0 galaxies is still", "not well understood, specifically in the outskirts of galaxy clusters.", "We study eight low-redshift clusters, analyzing galaxy members up to", "cluster-centric distances of ~2.5R_200_. We perform 2D photometric", "bulge-disk decomposition in the g, r, and i bands from which we", "identify 469 double-component galaxies. We separately analyze the", "colors of the bulges and disks and their dependence on the projected", "cluster-centric distance and local galaxy density. For our sample of", "cluster S0 galaxies, we find that bulges are redder than their", "surrounding disks, show a significant color-magnitude trend, and have", "colors that do not correlate with environment metrics. On the other", "hand, the disks associated with our cluster S0s become significantly", "bluer with increasing cluster-centric radius but show no evidence for", "a color-magnitude relation. The disk color-radius relation is mainly", "driven by galaxies in the cluster core at 0<=R/R_200_<0.5. No", "significant difference is found for the disk colors of backsplash and", "infalling galaxies in the projected phase space (PPS). Beyond R_200_,", "the disk colors do not change with the local galaxy density,", "indicating that the colors of double-component galaxies are not", "affected by preprocessing. A significant color-density relation is", "observed for single-component disk-dominated galaxies beyond R200. We", "conclude that the formation of cluster S0 galaxies is primarily driven", "by cluster core processes acting on the disks, while evidence of", "preprocessing is found for single-component disk-dominated galaxies.", "We publicly release the data from the bulge-disk decomposition."], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table10a.dat", "desc": "2D bulge-disk decomposition for the g-band ", "columns": [{"name": "cataid", "desc": "Catalog ID (G1) "}, {"name": "photo-flag", "desc": "Photometric data survey; SDSS, VST/ATLAS"}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) (G1)"}, {"name": "DEdeg", "desc": "Declination in decimals degrees (J2000) (G1)"}, {"name": "g-psf-model", "desc": "PSF photometric model; Mof=Moffat "}, {"name": "g-psf-fwhm", "desc": "PSF full-width-at-half-maximum "}, {"name": "g-psf-con", "desc": "PSF concentration "}, {"name": "g-psf-axrat", "desc": "PSF axial ratio; minor/major axis "}, {"name": "g-psf-ang", "desc": "PSF position angle of major axis "}, {"name": "g-s-model", "desc": "Single-component photometric model; Ser=Sersic"}, {"name": "g-s-xcen", "desc": "Single-component x-position "}, {"name": "e_g-s-xcen", "desc": "?=-9999999 Error on g-s-xcen "}, {"name": "g-s-ycen", "desc": "Single-component y-position "}, {"name": "e_g-s-ycen", "desc": "?=-9999999 Error on g-s-ycen "}, {"name": "g-s-mag", "desc": "Single-component magnitude "}, {"name": "e_g-s-mag", "desc": "?=-9999999 Error on g-s-mag "}, {"name": "g-s-re", "desc": "Single-component effective radius "}, {"name": "e_g-s-re", "desc": "?=-9999999 Error on g-s-re "}, {"name": "g-s-nser", "desc": "Single-component Sersic index "}, {"name": "e_g-s-nser", "desc": "?=-9999999 Error on g-s-nser "}, {"name": "g-s-axrat", "desc": "Single-component axial ratio; minor/major axis"}, {"name": "e_g-s-axrat", "desc": "?=-1 Error on g-s-axrat "}, {"name": "g-s-ang", "desc": "Single-component position angle of major axis"}, {"name": "e_g-s-ang", "desc": "?=-1 Error on g-s-ang "}, {"name": "g-s-ang-WCS", "desc": "g-s-ang in the World Coordinate System"}, {"name": "g-s-npegged", "desc": "Number of single-component parameters pegged to upper/lower fit limits"}, {"name": "g-s-npegged-warn", "desc": "Number of single-component parameters pegged to upper/lower fit limits within the errors"}, {"name": "g-s-redchisq", "desc": "Reduced chi-square for single-component fit"}, {"name": "g-s-DIC", "desc": "Deviance Information Criterion for single-component fit"}, {"name": "g-s-BIC", "desc": "Bayesian Information Criterion for single-component fit"}, {"name": "g-s-LL", "desc": "Unnormalized Log-Likelihood for single-component fit"}, {"name": "g-s-LML", "desc": "Logarithm of the Marginal Likelihood for single-component fit"}, {"name": "g-d-model1", "desc": "Bulge photometric model (G2) "}, {"name": "g-d-model2", "desc": "Disk photometric model; Exp=exponential"}, {"name": "g-d-xcen12", "desc": "Bulge and Disk x-position "}, {"name": "e_g-d-xcen12", "desc": "?=-9999999 Error on g-d-xcen12 (G3) "}, {"name": "g-d-ycen12", "desc": "Bulge and Disk y-position "}, {"name": "e_g-d-ycen12", "desc": "?=-9999999 Error on g-d-ycen12 (G3) "}, {"name": "g-d-mag1", "desc": "Bulge magnitude "}, {"name": "e_g-d-mag1", "desc": "?=-9999999 Error on g-d-mag1 (G3) "}, {"name": "g-d-mag2", "desc": "Disk magnitude "}, {"name": "e_g-d-mag2", "desc": "?=-9999999 Error on g-d-mag2 (G3) "}, {"name": "g-d-re1", "desc": "Bulge effective radius "}, {"name": "e_g-d-re1", "desc": "?=-9999999 Error on g-d-re1 (G3) "}, {"name": "g-d-re1-up", "desc": "Upper fit limit for g-d-re1 "}, {"name": "g-d-re2", "desc": "Disk effective radius "}, {"name": "e_g-d-re2", "desc": "?=-9999999 Error on g-d-re2 (G3) "}, {"name": "g-d-re2-up", "desc": "Upper fit limit for g-d-re2 "}, {"name": "g-d-nser1", "desc": "Bulge Sersic index "}, {"name": "errg-d-nser1", "desc": "Error on g-d-nser1 (G3) "}, {"name": "g-d-nser2", "desc": "Disk Sersic index "}, {"name": "e_g-d-nser2", "desc": "?=-1 Error on g-d-nser2 (G3) "}, {"name": "g-d-axrat1", "desc": "Bulge axial ratio; minor/major axis "}, {"name": "e_g-d-axrat1", "desc": "?=-1 Error on g-d-axrat1 "}, {"name": "g-d-axrat2", "desc": "Disk axial ratio; minor/major axis "}, {"name": "e_g-d-axrat2", "desc": "?=-1 Error on g-d-axrat2 (G3) "}, {"name": "g-d-ang1", "desc": "Bulge position angle of major axis "}, {"name": "e_g-d-ang1", "desc": "?=-1 Error on g-d-ang1 (G3) "}, {"name": "g-d-ang1-WCS", "desc": "g-d-ang1 in the World Coordinate System"}, {"name": "g-d-ang2", "desc": "Disk position angle of major axis "}, {"name": "e_g-d-ang2", "desc": "?=-1 Error on g-d-ang2 (G3) "}, {"name": "g-d-ang2-WCS", "desc": "g-d-ang2 in the World Coordinate System"}, {"name": "g-d-BT", "desc": "Bulge-to-total flux ratio "}, {"name": "g-d-npegged", "desc": "Number of double-component parameters pegged to upper/lower fit limits"}, {"name": "g-d-npegged-warn", "desc": "Number of double-component parameters pegged to upper/lower fit limits within the errors"}, {"name": "g-d-redchisq", "desc": "Reduced chi-square for double-component fit"}, {"name": "g-d-DIC", "desc": "Deviance Information Criterion for double-component fit"}, {"name": "g-d-BIC", "desc": "Bayesian Information Criterion for double-component fit"}, {"name": "g-d-LL", "desc": "Unnormalized Log-Likelihood for double-component fit"}, {"name": "g-d-LML", "desc": "Logarithm of the Marginal Likelihood for double-component fit"}, {"name": "g-DeltaBIC", "desc": "Bayesian Information Criterion difference; (g-d-BIC)-(g-s-BIC)"}, {"name": "g-LBF", "desc": "Logarithm of Bayes Factor; (g-d-LML)-(g-s-LML)"}]}, {"name": "table10b.dat", "desc": "2D bulge-disk decomposition for the i-band ", "columns": [{"name": "cataid", "desc": "Catalog ID (G1) "}, {"name": "photo-flag", "desc": "Photometric data survey; SDSS, VST/ATLAS"}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) (G1)"}, {"name": "DEdeg", "desc": "Declination in decimals degrees (J2000) (G1)"}, {"name": "i-psf-model", "desc": "PSF photometric model; Mof=Moffat "}, {"name": "i-psf-fwhm", "desc": "PSF full-width-at-half-maximum "}, {"name": "i-psf-con", "desc": "PSF concentration "}, {"name": "i-psf-axrat", "desc": "PSF axial ratio; minor/major axis "}, {"name": "i-psf-ang", "desc": "PSF position angle of major axis "}, {"name": "i-s-model", "desc": "Single-component photometric model; Ser=Sersic"}, {"name": "i-s-xcen", "desc": "Single-component x-position "}, {"name": "e_i-s-xcen", "desc": "?=-9999999 Error on i-s-xcen "}, {"name": "i-s-ycen", "desc": "Single-component y-position "}, {"name": "e_i-s-ycen", "desc": "?=-9999999 Error on i-s-ycen "}, {"name": "i-s-mag", "desc": "Single-component magnitude "}, {"name": "e_i-s-mag", "desc": "?=-9999999 Error on i-s-mag "}, {"name": "i-s-re", "desc": "Single-component effective radius "}, {"name": "e_i-s-re", "desc": "?=-9999999 Error on i-s-re "}, {"name": "i-s-nser", "desc": "Single-component Sersic index "}, {"name": "e_i-s-nser", "desc": "?=-9999999 Error on i-s-nser "}, {"name": "i-s-axrat", "desc": "Single-component axial ratio; minor/major axis"}, {"name": "e_i-s-axrat", "desc": "?=-1 Error on i-s-axrat "}, {"name": "i-s-ang", "desc": "Single-component position angle of major axis"}, {"name": "e_i-s-ang", "desc": "?=-1 Error on i-s-ang "}, {"name": "i-s-ani-WCS", "desc": "i-s-ang in the World Coordinate System"}, {"name": "i-s-npegged", "desc": "Number of single-component parameters pegged to upper/lower fit limits"}, {"name": "i-s-npegged-warn", "desc": "Number of single-component parameters pegged to upper/lower fit limits within the errors"}, {"name": "i-s-redchisq", "desc": "Reduced chi-square for single-component fit"}, {"name": "i-s-DIC", "desc": "Deviance Information Criterion for single-component fit"}, {"name": "i-s-BIC", "desc": "Bayesian Information Criterion for single-component fit"}, {"name": "i-s-LL", "desc": "Unnormalized Loi-Likelihood for single-component fit"}, {"name": "i-s-LML", "desc": "Logarithm of the Marginal Likelihood for single-component fit"}, {"name": "i-d-model1", "desc": "Bulge photometric model (G2) "}, {"name": "i-d-model2", "desc": "Disk photometric model; Exp=exponential"}, {"name": "i-d-xcen12", "desc": "Bulge and Disk x-position "}, {"name": "e_i-d-xcen12", "desc": "?=-9999999 Error on i-d-xcen12 (G3) "}, {"name": "i-d-ycen12", "desc": "Bulge and Disk y-position "}, {"name": "e_i-d-ycen12", "desc": "?=-9999999 Error on i-d-ycen12 (G3) "}, {"name": "i-d-mag1", "desc": "Bulge magnitude "}, {"name": "e_i-d-mag1", "desc": "?=-9999999 Error on i-d-mag1 (G3) "}, {"name": "i-d-mag2", "desc": "Disk magnitude "}, {"name": "e_i-d-mag2", "desc": "?=-9999999 Error on i-d-mag2 (G3) "}, {"name": "i-d-re1", "desc": "Bulge effective radius "}, {"name": "e_i-d-re1", "desc": "?=-9999999 Error on i-d-re1 (G3) "}, {"name": "i-d-re1-up", "desc": "Upper fit limit for i-d-re1 "}, {"name": "i-d-re2", "desc": "Disk effective radius "}, {"name": "e_i-d-re2", "desc": "?=-9999999 Error on i-d-re2 (G3) "}, {"name": "i-d-re2-up", "desc": "Upper fit limit for i-d-re2 "}, {"name": "i-d-nser1", "desc": "Bulge Sersic index "}, {"name": "erri-d-nser1", "desc": "Error on i-d-nser1 (G3) "}, {"name": "i-d-nser2", "desc": "Disk Sersic index "}, {"name": "e_i-d-nser2", "desc": "?=-1 Error on i-d-nser2 (G3) "}, {"name": "i-d-axrat1", "desc": "Bulge axial ratio; minor/major axis "}, {"name": "e_i-d-axrat1", "desc": "?=-1 Error on i-d-axrat1 (G3) "}, {"name": "i-d-axrat2", "desc": "Disk axial ratio; minor/major axis "}, {"name": "e_i-d-axrat2", "desc": "?=-1 Error on i-d-axrat2 (G3) "}, {"name": "i-d-ang1", "desc": "Bulge position angle of major axis "}, {"name": "e_i-d-ang1", "desc": "?=-1 Error on i-d-ang1 (G3) "}, {"name": "i-d-ang1-WCS", "desc": "i-d-ang1 in the World Coordinate System"}, {"name": "i-d-ang2", "desc": "Disk position angle of major axis "}, {"name": "e_i-d-ang2", "desc": "?=-1 Error on i-d-ang2 (G3) "}, {"name": "i-d-ang2-WCS", "desc": "i-d-ang2 in the World Coordinate System"}, {"name": "i-d-BT", "desc": "Bulge-to-total flux ratio "}, {"name": "i-d-npegged", "desc": "Number of double-component parameters pegged to upper/lower fit limits"}, {"name": "i-d-npegged-warn", "desc": "Number of double-component parameters pegged to upper/lower fit limits within the errors"}, {"name": "i-d-redchisq", "desc": "Reduced chi-square for double-component fit"}, {"name": "i-d-DIC", "desc": "Deviance Information Criterion for double-component fit"}, {"name": "i-d-BIC", "desc": "Bayesian Information Criterion for double-component fit"}, {"name": "i-d-LL", "desc": "Unnormalized Loi-Likelihood for double-component fit"}, {"name": "i-d-LML", "desc": "Logarithm of the Marginal Likelihood for double-component fit"}, {"name": "i-DeltaBIC", "desc": "Bayesian Information Criterion difference; (i-d-BIC)-(i-s-BIC)"}, {"name": "i-LBF", "desc": "Logarithm of Bayes Factor; (i-d-LML)-(i-s-LML)"}]}, {"name": "table10c.dat", "desc": "2D bulge-disk decomposition for the r-band ", "columns": [{"name": "cataid", "desc": "Catalog ID (G1) "}, {"name": "photo-flag", "desc": "Photometric data survey; SDSS, VST/ATLAS"}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) (G1)"}, {"name": "DEdeg", "desc": "Declination in decimals degrees (J2000) (G1)"}, {"name": "r-psf-model", "desc": "PSF photometric model; Mof=Moffat "}, {"name": "r-psf-fwhm", "desc": "PSF full-width-at-half-maximum "}, {"name": "r-psf-con", "desc": "PSF concentration "}, {"name": "r-psf-axrat", "desc": "PSF axial ratio; minor/major axis "}, {"name": "r-psf-ang", "desc": "PSF position angle of major axis "}, {"name": "r-s-model", "desc": "Single-component photometric model; Ser=Sersic"}, {"name": "r-s-xcen", "desc": "Single-component x-position "}, {"name": "e_r-s-xcen", "desc": "?=-9999999 Error on r-s-xcen "}, {"name": "r-s-ycen", "desc": "Single-component y-position "}, {"name": "e_r-s-ycen", "desc": "?=-9999999 Error on r-s-ycen "}, {"name": "r-s-mag", "desc": "Single-component magnitude "}, {"name": "e_r-s-mag", "desc": "?=-9999999 Error on r-s-mag "}, {"name": "r-s-re", "desc": "Single-component effective radius "}, {"name": "e_r-s-re", "desc": "?=-9999999 Error on r-s-re "}, {"name": "r-s-nser", "desc": "Single-component Sersic index "}, {"name": "e_r-s-nser", "desc": "?=-9999999 Error on r-s-nser "}, {"name": "r-s-axrat", "desc": "Single-component axial ratio; minor/major axis"}, {"name": "e_r-s-axrat", "desc": "?=-9999999 Error on r-s-axrat "}, {"name": "r-s-ang", "desc": "Single-component position angle of major axis"}, {"name": "e_r-s-ang", "desc": "?=-9999999 Error on r-s-ang "}, {"name": "r-s-anr-WCS", "desc": "r-s-ang in the World Coordinate System"}, {"name": "r-s-npegged", "desc": "Number of single-component parameters pegged to upper/lower fit limits"}, {"name": "r-s-npegged-warn", "desc": "Number of single-component parameters pegged to upper/lower fit limits within the errors"}, {"name": "r-s-redchisq", "desc": "Reduced chi-square for single-component fit"}, {"name": "r-s-DIC", "desc": "Deviance Information Criterion for single-component fit"}, {"name": "r-s-BIC", "desc": "Bayesian Information Criterion for single-component fit"}, {"name": "r-s-LL", "desc": "Unnormalized Lor-Likelihood for single-component fit"}, {"name": "r-s-LML", "desc": "Logarithm of the Marginal Likelihood for single-component fit"}, {"name": "r-d-model1", "desc": "Bulge photometric model (G2) "}, {"name": "r-d-model2", "desc": "Disk photometric model; Exp=exponential"}, {"name": "r-d-xcen12", "desc": "Bulge and Disk x-position "}, {"name": "e_r-d-xcen12", "desc": "?=-9999999 Error on r-d-xcen12 (G3) "}, {"name": "r-d-ycen12", "desc": "Bulge and Disk y-position "}, {"name": "e_r-d-ycen12", "desc": "?=-9999999 Error on r-d-ycen12 (G3) "}, {"name": "r-d-mag1", "desc": "Bulge magnitude "}, {"name": "e_r-d-mag1", "desc": "?=-9999999 Error on r-d-mag1 (G3) "}, {"name": "r-d-mag2", "desc": "Disk magnitude "}, {"name": "e_r-d-mag2", "desc": "?=-9999999 Error on r-d-mag2 (G3) "}, {"name": "r-d-re1", "desc": "Bulge effective radius "}, {"name": "e_r-d-re1", "desc": "?=-9999999 Error on r-d-re1 (G3) "}, {"name": "r-d-re1-up", "desc": "Upper fit limit for r-d-re1 "}, {"name": "r-d-re2", "desc": "Disk effective radius "}, {"name": "e_r-d-re2", "desc": "?=-9999999 Error on r-d-re2 (G3) "}, {"name": "r-d-re2-up", "desc": "Upper fit limit for r-d-re2 "}, {"name": "r-d-nser1", "desc": "Bulge Sersic index "}, {"name": "errir-d-nser1", "desc": "Error on r-d-nser1 (G3) "}, {"name": "r-d-nser2", "desc": "Disk Sersic index "}, {"name": "e_r-d-nser2", "desc": "?=-1 Error on r-d-nser2 (G3) "}, {"name": "r-d-axrat1", "desc": "Bulge axial ratio; minor/major axis "}, {"name": "errr-d-axrat1", "desc": "Error on r-d-axrat1 (G3) "}, {"name": "r-d-axrat2", "desc": "Disk axial ratio; minor/major axis "}, {"name": "errr-d-axrat2", "desc": "Error on r-d-axrat2 (G3) "}, {"name": "r-d-ang1", "desc": "Bulge position angle of major axis "}, {"name": "errr-d-ang1", "desc": "Error on r-d-ang1 (G3) "}, {"name": "r-d-ang1-WCS", "desc": "r-d-ang1 in the World Coordinate System"}, {"name": "r-d-ang2", "desc": "Disk position angle of major axis "}, {"name": "e_r-d-ang2", "desc": "?=-9999999 Error on r-d-ang2 (G3) "}, {"name": "r-d-ang2-WCS", "desc": "r-d-ang2 in the World Coordinate System"}, {"name": "r-d-BT", "desc": "Bulge-to-total flux ratio "}, {"name": "r-d-npegged", "desc": "Number of double-component parameters pegged to upper/lower fit limits"}, {"name": "r-d-npegged-warn", "desc": "Number of double-component parameters pegged to upper/lower fit limits within the errors"}, {"name": "r-d-redchisq", "desc": "Reduced chi-square for double-component fit"}, {"name": "r-d-DIC", "desc": "Deviance Information Criterion for double-component fit"}, {"name": "r-d-BIC", "desc": "Bayesian Information Criterion for double-component fit"}, {"name": "r-d-LL", "desc": "Unnormalized Lor-Likelihood for double-component fit"}, {"name": "r-d-LML", "desc": "Logarithm of the Marginal Likelihood for double-component fit"}, {"name": "r-DeltaBIC", "desc": "Bayesian Information Criterion difference; (r-d-BIC)-(r-s-BIC)"}, {"name": "r-LBF", "desc": "Logarithm of Bayes Factor; (r-d-LML)-(r-s-LML)"}, {"name": "r-ncomp", "desc": "Number of galaxy components (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_28"}} {"id": "J/ApJ/911/28", "title_cds": "MW Project: DR2 \"yellow balls\" in Spitzer", "title_create": "Wolf-Chase+, 2021", "year": "2021", "author": "Wolf-Chase G., Kerton C.R., Devine K., Pouydal A., Mori J., Trujillo L., Cossairt A., Schoultz S., Jayasinghe T., Povich M.", "title_pub": "The Milky Way Project: probing star formation with first results on yellowballs from DR2.", "first_author": "Wolf-Chase G.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...28W"], "see_also": ["II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008)", "J/A+A/275/67 : Velocity Field of the outer Galaxy (Brand+ 1993)", "J/A+A/481/345 : SED evolution in massive YSOs (Molinari+, 2008)", "J/ApJ/720/679 : Optical spectroscopy in Cygnus X region (Beerer+, 2010)", "J/A+A/537/A1 : Infrared fluxes of HII regions and PNe (Anderson+, 2012)", "J/MNRAS/424/2442 : Catalog of bubbles from Milky Way Project (Simpson+, 2012)", "J/A+A/544/A146 : ATLASGAL cold high-mass clumps with NH_3_ (Wienen+, 2012)", "J/ApJS/208/11 : Red MSX Source Survey: massive protostars (Lumsden+, 2013)", "J/ApJS/205/1 : CORNISH project. II. Source catalog (Purcell+, 2013)", "J/ApJS/212/1 : The WISE catalog of Galactic HII regions (Anderson+, 2014)", "J/A+A/565/A75 : ATLASGAL: dust condensations in Gal. plane (Csengeri+, 2014)", "J/ApJ/783/130 : Parallaxes of high mass star forming regions (Reid+, 2014)", "J/ApJ/799/153 : Yellowballs in Milky Way project (Kerton+, 2015)", "J/MNRAS/471/100 : Hi-GAL compact source catalog. -71.0350um "}, {"name": "e_Lratio", "desc": "[1/112] Uncertainty in Lratio "}, {"name": "TBol", "desc": "[18/128] Bolometric temperature (2) "}, {"name": "e_TBol", "desc": "[3.6/26] Uncertainty in TBol "}, {"name": "SDen", "desc": "[0.005/6.9] Surface density "}, {"name": "e_SDen", "desc": "[0.001/2.7] Uncertainty in SDen "}]}, {"name": "table6.dat", "desc": "Pilot region MIR photometry ", "columns": [{"name": "Seq", "desc": "[1153/1670] Yellowball identifier "}, {"name": "F8", "desc": "[0.02/16.67]? Mean 8 micron flux density "}, {"name": "stdF8", "desc": "[0/69]? Normalized standard deviation in F8 (4) "}, {"name": "F12", "desc": "[0/7.7]? Mean 12 micron flux density "}, {"name": "stdF12", "desc": "[0.01/8]? Normalized standard deviation in F12 (4)"}, {"name": "F24", "desc": "[-0.01/13.1]? Mean 24 micron flux density "}, {"name": "stdF24", "desc": "[0.01/2.5]? Normalized standard deviation in F24 (4)"}, {"name": "F70", "desc": "[0.9/2563]? Hi-GAL 70 micron flux density from Elia et al. (2017MNRAS.417..100E)"}, {"name": "e_F70", "desc": "[0.05/90]? Uncertainty in F70 "}, {"name": "Fit", "desc": "[1]? Well-fit by 2D Gaussian model flag? 1=Yes "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_51"}} {"id": "J/ApJ/911/51", "title_cds": "1894-2020 opt-to-NIR photometry of HO Puppis", "title_create": "Lee+, 2021", "year": "2021", "author": "Lee C.-D., Ou J.-Y., Yu P.-C., Ngeow C.-C., Huang P.-C., Ip W.-H., Hambsch F.-J., Sung H.-I., van Roestel J., Dekany R., Drake A.J., Graham M.J., Duev D.A., Kaye S., Kupfer T., Laher R.R., Masci F.J., Mroz P., Neill J.D., Riddle R., Rusholme B., Walters R.", "title_pub": "HO Puppis: not a Be star, but a newly confirmed IW And-type star.", "first_author": "Lee C.-D.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...51L"], "see_also": ["B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "II/264 : ASAS Variable Stars in Southern hemisphere (Pojmanski+, 2002-2005)", "I/305 : The Guide Star Catalog, Version 2.3.2 (GSC2.3) (STScI, 2006)", "II/311 : WISE All-Sky Data Release (Cutri+ 2012)", "I/322 : UCAC4 Catalogue (Zacharias+, 2012)", "II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "II/358 : SkyMapper Southern Sky Survey. DR1.1 (Wolf+, 2018)", "II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)", "I/353 : The Guide Star Catalog, Version 2.4.2 (GSC2.4.2) (STScI, 2020)", "J/A+A/548/A79 : INTEGRAL-OMC optically variable sources (Alfonso-Garzon+, 2012)", "J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)", "J/AJ/153/252 : Phot. variability of BeSS-KELT stars (Labadie-Bartz+, 2017)", "J/AJ/156/241 : First cat. of variable stars measured by ATLAS (Heinze+, 2018)", "J/AJ/155/91 : Be stars in open clusters with PTF/iPTF. I. (Yu+, 2018)", "J/A+A/621/A38 : Gaia catalogue of hot subluminous stars (Geier+, 2019)"], "keyword_cds": "Stars, variable; Photometry, infrared; Optical; Surveys", "keyword_pub": "Dwarf novae ; Be stars ; Sky surveys ; Time series analysis", "abstract": ["HO Puppis (HO Pup) was considered as a Be-star candidate based on its", "{gamma} Cassiopeiae-type light curve, but lacked spectroscopic", "confirmation. Using distance measured from Gaia Data Release 2 and the", "spectral-energy-distribution fit on broadband photometry, the Be-star", "nature of HO Pup is ruled out. Furthermore, based on the", "28700 photometric data points collected from various time-domain", "surveys and dedicated intensive-monitoring observations, the light", "curves of HO Pup closely resemble those of IW And-type stars (as", "pointed out by Kimura+ 2020PASJ...72...22K), exhibiting", "characteristics such as a quasi-standstill phase, brightening, and", "dips. The light curve of HO Pup displays various variability", "timescales, including brightening cycles ranging from 23 to 61days,", "variations with periods between 3.9d and 50min during the", "quasi-standstill phase, and a semiregular ~14d period for the dip", "events. We have also collected time-series spectra (with various", "spectral resolutions), in which Balmer emission lines and other", "spectral lines expected for an IW And-type star were detected (even", "though some of these lines were also expected to be present for Be", "stars). We detect Bowen fluorescence near the brightening phase, and", "that can be used to discriminate between IW And-type stars and Be", "stars. Finally, despite only observing for four nights, the", "polarization variation was detected, indicating that HO Pup has", "significant intrinsic polarization."], "description": ["Time-series photometric data ranging from optical to infrared for HO", "Pup were collected from various survey catalogs, including the ZTF,", "the ASAS-SN, the Digital Access to a Sky Century @ Harvard (DASCH,", "Grindlay+ 2012IAUS..285...29G), the third phase of the All Sky", "Automated Survey (ASAS-3, Pojmanski+ 2002, II/264), the Panoramic", "Survey Telescope and Rapid Response System 3{pi} survey (Pan-STARRS,", "Chambers+ 2016, II/349), the Wide-field Infrared Survey Explorer", "(WISE, Cutri+ 2012, II/311), and observations available via the", "American Association of Variable Star Observers (AAVSO).", "These light-curve data were supplemented with dedicated observations", "taken at the Lulin Observatory with the 0.4m SLT telescope in Taiwan.", "These light curves are listed in Table 1 and cover years from 1894 to", "2020. See Section 2.1.", "Spectroscopic observations with low and high spectral resolutions were", "conducted by P60/SEDM, the 1.8m Optical Telescope at the Bohyunsan", "Optical Astronomy Observatory (BOAO)/Bohyunsan Optical Echelle", "Spectrograph (BOES), CFHT/ESPaDOnS, and P200/DBSP. Additionally,", "polarization was measured on four different nights in late October", "2018 using the TRIPOL2 instrument installed at the Lulin Observatory.", "See Section 2.2."], "object": ["07 33 54.18 -15 45 38.3 HO Pup = V* HO Pup"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Collected light curves with 28700 data points for HO Pup", "columns": [{"name": "MJD", "desc": "[13146.3/58938.6] Modified Julian Date, (JD-2400000.5)"}, {"name": "omag", "desc": "[12.4/16.05] Observed magnitude in Filt "}, {"name": "e_omag", "desc": "[0.001/0.42] Magnitude error "}, {"name": "Filt", "desc": "Filter (BV, grizy, W1, W2) "}, {"name": "r_omag", "desc": "Source of photometry (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_55"}} {"id": "J/ApJ/911/55", "title_cds": "FUSE survey of H_2_ in the Galactic disk", "title_create": "Shull+, 2021", "year": "2021", "author": "Shull J.M., Danforth C.W., Anderson K.L.", "title_pub": "A Far Ultraviolet Spectroscopic Explorer survey of interstellar molecular hydrogen in the Galactic disk.", "first_author": "Shull J.M.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...55S"], "see_also": ["III/274 : Galactic O-Star Spectroscopic Survey (GOSSS) (Sota+, 2014)", "V/116 : Galactic O star catalog (Maiz-apellaniz+, 2004)", "J/ApJS/93/211 : IUE survey of H I Ly{alpha} absorption. I. (Diplas+ 1994)", "J/ApJS/163/282 : Molecular hydrogen column densities (Wakker+, 2006)", "J/ApJS/176/59 : FUSE survey of OVI in the disk of the Milky Way (Bowen+, 2008)", "J/ApJ/711/1236 : Equivalent width of H_2_ from FUSE (Jensen+, 2010)", "J/ApJ/734/65 : CI radial velocities with HST/STIS (Jenkins+, 2011)", "J/A+A/613/A9 : Extinction towards Galactic O stars (Maiz Apellaniz+, 2018)", "J/ApJ/872/55 : OI, GeII, KrI & H abundances from HST UV sp. (Jenkins, 2019)", "J/ApJ/906/73 : Extinction & emission PostPlanck Era (Hensley+, 2021)"], "keyword_cds": "Stars, OB; Ultraviolet; Surveys; Milky Way; Extinction; Molecular data; Interstellar medium; H I data", "keyword_pub": "Diffuse interstellar clouds ; Milky Way disk ; Interstellar molecules ; Ultraviolet astronomy ; Ultraviolet extinction", "abstract": ["We report results from a Far Ultraviolet Spectrographic Explorer", "(FUSE) survey of interstellar molecular hydrogen (H_2_) in the", "Galactic disk toward 139 O-type and early B-type stars at Galactic", "latitudes |b|<=10{deg}, with updated photometric and parallax", "distances. H_2_ absorption is measured using the far-UV Lyman and", "Werner bands, including strong R(0), R(1), and P(1) lines from", "rotational levels J=0 and J=1 and excited states up to J=5 (sometimes", "J=6 and 7). For each sight line, we report column densities N_H2_,", "N_HI_, N(J), and N_H_=N_HI_+2N_H2_ and the molecular fraction", "f_H2_=2N_H2_/N_H_. Our survey extends the 1977 Copernicus H_2_ survey", "up to N_H_~5x10^21^cm^-2^. The lowest rotational states have", "excitation temperatures and rms dispersions =88+/-20K and", "=77+/-18K, suggesting that J=0, 1, 2 are coupled to the gas", "kinetic temperature. Populations of higher-J states exhibit mean", "excitation temperatures =237+/-91K and =304+/-108K,", "produced primarily by UV radiative pumping. Correlations of f_H2_ with", "E(B-V) and N_H_ show a transition to f_H2_>=0.1 at N_H_>~10^21^cm^-2^", "and E(B-V)>~0.2, interpreted with an analytic model of H_2_", "formation-dissociation equilibrium and attenuation of the far-UV", "radiation field by self-shielding and dust opacity. Results of this", "disk survey are compared to previous FUSE studies of H_2_ in", "translucent clouds, at high Galactic latitudes, and in the Magellanic", "Clouds. Using updated distances to the target stars, we find average", "sight-line values =0.20 and =6.07x10^21^cm^-2^/mag."], "description": ["The 139 targets in this survey were drawn primarily from FUSE programs", "designed to study OB stars and interstellar gas in the Milky Way.", "These stars have updated spectral types and both photometric and", "Gaia-DR2 parallax distances determined by", "Shull & Danforth (2019ApJ...882..180S) using new information from the", "Galactic O-star Spectroscopic Survey (GOSS; Maiz Apellaniz+ 2004, V/116)."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Stellar parameters and distances ", "columns": [{"name": "Seq", "desc": "[1/139] Internal target number "}, {"name": "Name", "desc": "Target identifier "}, {"name": "GLON", "desc": "[2.26/355.36] Galactic longitude "}, {"name": "GLAT", "desc": "[-23.23/13.5] Galactic latitude "}, {"name": "Bmag", "desc": "[5.3/10.61] Apparent B band magnitude "}, {"name": "Vmag", "desc": "[5/10.7] Apparent V band magnitude "}, {"name": "E(B-V)", "desc": "[0.02/1.1] The(B-V) color excess "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Dphot", "desc": "[0.2/9.9] Photometric distance (1) "}, {"name": "f_Dphot", "desc": "[b] Flag on Dphot (2) "}, {"name": "l_DGaia", "desc": "Limit flag on DGaia "}, {"name": "DGaia", "desc": "[0.28/14]? Parallax distance (3) "}, {"name": "e_DGaia", "desc": "[0.27/7.7]? Lower limit on DGaia "}, {"name": "E_DGaia", "desc": "[0.29/20.1]? Upper limit on DGaia "}, {"name": "f_DGaia", "desc": "Flag on DGaia (4) "}, {"name": "FUSE", "desc": "FUSE program identifier "}, {"name": "Texp", "desc": "[0.059/31.6] FUSE spectroscopic exposure time "}]}, {"name": "table2.dat", "desc": "HI column density measurements ", "columns": [{"name": "Seq", "desc": "[1/139] Internal target number "}, {"name": "Name", "desc": "Target identifier "}, {"name": "E(B-V)", "desc": "[0.02/1.1] The(B-V) color excess (1) "}, {"name": "logNHI-A", "desc": "[20.5/21.7] Adopted log HI column density (2) "}, {"name": "logNHI-S", "desc": "[20.9/21.5]? log HI column density from Shull & Van Steenberg 1985ApJ...294..599S"}, {"name": "e_logNHI-S", "desc": "[0.05/0.15]? Uncertainty in logNHI-S "}, {"name": "logNHI-D", "desc": "[20.56/21.65]? log HI column density from Diplas & Savage, 1994, J/ApJS/93/211"}, {"name": "e_logNHI-D", "desc": "[0.06/0.23]? Uncertainty in logNHI-D "}, {"name": "logNHI-J", "desc": "[20.55/21.5]? log HI column density from Jenkins 2019, J/ApJ/872/55"}, {"name": "E_logNHI-J", "desc": "[0.03/0.1]? Upper uncertainty in logNHI-J "}, {"name": "e_logNHI-J", "desc": "[0.02/0.13]? Lower uncertainty in logNHI-J "}, {"name": "logNHI-O", "desc": "[20.8/21.6]? Other log HI column density "}, {"name": "e_logNHI-O", "desc": "[0.05/0.3]? Uncertainty in logNHI-O "}, {"name": "r_logNHI-O", "desc": "Reference for logNHI-O (3) "}]}, {"name": "table3.dat", "desc": "Column densities and Doppler parameters ", "columns": [{"name": "Seq", "desc": "[1/139] Internal target number "}, {"name": "Target", "desc": "Target identifier "}, {"name": "f_Target", "desc": "[bc] Flag on Target (1) "}, {"name": "logN0", "desc": "[16.8/21.1]? log J=0 rotational state column density (2)"}, {"name": "E_logN0", "desc": "[0.05/0.15]? Upper uncertainty in logN0 "}, {"name": "e_logN0", "desc": "[0.05/0.15]? Lower uncertainty in logN0 "}, {"name": "logN1", "desc": "[17.3/20.8]? log J=1 rotational state column density (2)"}, {"name": "E_logN1", "desc": "[0.05/0.15]? Upper uncertainty in logN1 "}, {"name": "e_logN1", "desc": "[0.05/0.15]? Lower uncertainty in logN1 "}, {"name": "logN2", "desc": "[14.36/19.64]? log J=2 rotational state column density (2)"}, {"name": "E_logN2", "desc": "[0.03/1.5]? Upper uncertainty in logN2 "}, {"name": "e_logN2", "desc": "[0.04/0.5]? Lower uncertainty in logN2 "}, {"name": "logN3", "desc": "[14.93/18.24]? log J=3 rotational state column density (2)"}, {"name": "E_logN3", "desc": "[0.04/1.9]? Upper uncertainty in logN3 "}, {"name": "e_logN3", "desc": "[0.04/0.8]? Lower uncertainty in logN3 "}, {"name": "logN4", "desc": "[13.95/16.93] log J=4 rotational state column density (2)"}, {"name": "E_logN4", "desc": "[0.02/1.9]? Upper uncertainty in logN4 "}, {"name": "e_logN4", "desc": "[0.02/0.7]? Lower uncertainty in logN4 "}, {"name": "l_logN5", "desc": "Limit flag on logN5 "}, {"name": "logN5", "desc": "[13.88/16.68]? log J=5 rotational state column density (2)"}, {"name": "E_logN5", "desc": "[0.03/1.4]? Upper uncertainty in logN5 "}, {"name": "e_logN5", "desc": "[0.02/0.3]? Lower uncertainty in logN5 "}, {"name": "l_logN6", "desc": "Limit flag on logN6 "}, {"name": "logN6", "desc": "[13.53/15.71]? log J=6 rotational state column density (2)"}, {"name": "E_logN6", "desc": "[0.04/0.2]? Upper uncertainty in logN6 "}, {"name": "e_logN6", "desc": "[0.04/0.2]? Lower uncertainty in logN6 "}, {"name": "b", "desc": "[2.8/20]? Doppler parameter "}, {"name": "E_b", "desc": "[0.3/4.4]? Upper uncertainty in b "}, {"name": "e_b", "desc": "[0.4/3.7]? Lower uncertainty in b "}]}, {"name": "table4.dat", "desc": "Column densities and rotational temperatures ", "columns": [{"name": "Seq", "desc": "[1/139] Internal target number "}, {"name": "Target", "desc": "Target identifier "}, {"name": "logNH2", "desc": "[17.48/21.17] log H2 column density (1) "}, {"name": "T01", "desc": "[40/159] Rotational excitation temperature from N1/N0 ratio (2)"}, {"name": "T02", "desc": "[44/331]? Rotational excitation temperature from N2/N0 ratio (2)"}, {"name": "T24", "desc": "[118/582]? Rotational excitation temperature from N4/N2 ratio (2)"}, {"name": "T35", "desc": "[171/1358]? Rotational excitation temperature from N5/N3 ratio (2)"}, {"name": "logNHI", "desc": "[20.55/21.65] log HI column density (1) "}, {"name": "f_logNHI", "desc": "[*] Flag on logNHI (3) "}, {"name": "logNH", "desc": "[20.55/21.74] log H column density (1) "}, {"name": "Dphot", "desc": "[0.21/9.85] Photometric distance "}, {"name": "nH", "desc": "[0.02/3.9] Mean total hydrogen density along sight line"}, {"name": "fH2", "desc": "[0.0017/0.747] Molecular fraction (4) "}, {"name": "Note", "desc": "[1/3] S/N ratio level (5) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_78"}} {"id": "J/ApJ/911/78", "title_cds": "SILVERRUSH. X. Confirmed LAE galaxies & AGN from HSC", "title_create": "Ono+, 2021", "year": "2021", "author": "Ono Y., Itoh R., Shibuya T., Ouchi M., Harikane Y., Yamanaka S., Inoue A.K., Amagasa T., Miura D., Okura M., Shimasaku K., Iwata I., Taniguchi Y., Fujimoto S., Iye M., Jaelani A.T., Kashikawa N., Kikuchihara S., Kikuta S., Kobayashi M.A.R., Kusakabe H., Lee C.-H., Liang Y., Matsuoka Y., Momose R., Nagao T., Nakajima K., Tadaki K.-I.", "title_pub": "SILVERRUSH X: machine learning-aided selection of 9318 LAEs at z=2.2, 3.3, 4.9, 5.7, 6.6, and 7.0 from the HSC SSP and CHORUS survey data.", "first_author": "Ono Y.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...78O"], "see_also": ["II/357 : The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018)", "VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)", "J/ApJS/176/301 : Subaru/XMM-Newton deep survey IV. (SXDS) (Ouchi+, 2008)", "J/ApJS/184/218 : The zCOSMOS 10k-bright spectroscopic sample (Lilly+, 2009)", "J/ApJ/760/128 : Ly{alpha} from 45.6 quasars follow-up (Banados+, 2016)", "J/ApJS/225/27 : 3D-HST Survey: grism sp. master catalog (Momcheva+, 2016)", "J/ApJ/826/114 : z~3-6 protoclusters in CFHTLS deep fields (Toshikawa+, 2016)", "J/ApJ/819/24 : z>4.5 QSOs with SDSS and WISE. I. Opt. spectra (Wang+, 2016)", "J/A+A/608/A8 : MUSE Hubble Ultra Deep Field Survey. VIII (Leclercq+, 2017)", "J/ApJ/841/111 : C3R2 survey: high-confidence z from DR1 (Masters+, 2017)", "J/A+A/600/A110 : VIMOS Ultra Deep Survey (VUDS) DR1 (Tasca+, 2017)", "J/ApJS/228/24 : GALAH semi-automated classification scheme (Traven+, 2017)", "J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018)", "J/MNRAS/476/3661 : Morphology of SDSS galaxies (Dominguez+, 2018)", "J/ApJS/237/31 : CLAMATO DR1: 3D Ly{alpha} forest tomography (Lee+, 2018)", "J/A+A/619/A136 : VLT/X-SHOOTER spectrum of COLA1 (Matthee+, 2018)", "J/PASJ/70/S10 : GOLDRUSH I. UV magnitudes (Ono+, 2018)", "J/A+A/611/A97 : Phot. quasar candidates in Stripe 82 (Pasquet-Itam+, 2018)", "J/MNRAS/477/2817 : Luminous Ly{alpha} emitters at z~2-3 (Sobral+, 2018)", "J/MNRAS/483/3060 : Candidate massive galaxies at z~4 in DES (Guarnieri+, 2019)", "J/ApJS/243/17 : Strong DES lens cand. from neural networks (Jacobs+, 2019)", "J/ApJ/877/81 : The C3R2 survey: DR2 new sp. redshifts (Masters+, 2019)", "J/A+A/644/A163 : Pan-STARRS lens cand. from neural networks (Canameras+ 2020)", "J/PASJ/72/89 : Hyper Suprime-Cam transients classif. (Takahashi+, 2020)", "J/ApJ/909/27 : Strong gravitational lenses in DESI Surveys (Huang+, 2021)", "J/MNRAS/500/4849 : GALAH emission-line stars (Cotar+, 2021)", "http://hsc.mtk.nao.ac.jp/ssp/data-release/ : HSC SSP data release webpage"], "keyword_cds": "Active gal. nuclei; Galaxies, optical; Redshifts; Surveys", "keyword_pub": "Lyman-alpha galaxies ; High-redshift galaxies ; Convolutional neural networks ; Galaxy evolution ; Galaxy formation", "abstract": ["We present a new catalog of 9318 Ly{alpha} emitter (LAE) candidates at", "z=2.2, 3.3, 4.9, 5.7, 6.6, and 7.0 that are photometrically selected", "by the Systematic Identification of LAEs for Visible Exploration and", "Reionization Research Using Subaru HSC (SILVERRUSH) program with a", "machine learning technique from large area (up to 25.0deg^2^) imaging", "data with six narrowband filters taken by the Subaru Strategic Program", "with Hyper Suprime-Cam and a Subaru intensive program, Cosmic HydrOgen", "Reionization Unveiled with Subaru. We construct a convolutional neural", "network that distinguishes between real LAEs and contaminants with a", "completeness of 94% and a contamination rate of 1%, enabling us to", "efficiently remove contaminants from the photometrically selected LAE", "candidates. We confirm that our LAE catalogs include 177 LAEs that", "have been spectroscopically identified in our SILVERRUSH programs and", "previous studies, ensuring the validity of our machine learning", "selection. In addition, we find that the object-matching rates between", "our LAE catalogs and our previous results are ~80%-100% at bright NB", "magnitudes of <~24mag. We also confirm that the surface number", "densities of our LAE candidates are consistent with previous results."], "description": ["We use data products of the on-going Hyper Suprime-Cam Subaru", "Strategic Program (HSC SSP) survey that were obtained between", "2014-March and 2018-January (Aihara+ 2019PASJ...71..114A).", "Specifically, we use the internal data release of S18A, which is", "basically identical to the version of Public Data Release 2.", "In addition, we use HSC NB data taken by the Cosmic HydrOgen", "Reionization Unveiled with Subaru (CHORUS) program between 2017", "January and 2018 March (Inoue+ 2020PASJ...72..101I)."], "type": ["CCC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "tablea1.dat", "desc": "Spectroscopically confirmed galaxies and AGNs in our Ly{alpha} emitter (LAE) samples", "columns": [{"name": "---", "desc": "[HSC] "}, {"name": "HSC", "desc": "HSC identifier (JHHMMSS+DDMMSS); in Simbad"}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "zsp", "desc": "[2.14/7] Spectroscopic redshift "}, {"name": "gmag", "desc": "[20/33.7]?=99 g-band magnitude with 20 diameter circular aperture"}, {"name": "rmag", "desc": "[20/32.7]?=99 r-band magnitude with 20 diameter circular aperture"}, {"name": "imag", "desc": "[20/30.5]?=99 i-band magnitude with 20 diameter circular aperture"}, {"name": "zmag", "desc": "[19.8/30]?=99 z-band magnitude with 20 diameter circular aperture"}, {"name": "ymag", "desc": "[19.9/29.3]?=99 y band magnitude with 20 diameter circular aperture"}, {"name": "mag", "desc": "[19.1/25.6] Apparent total NB magnitude (See Figure 1 for the NB filters)"}, {"name": "Sample", "desc": "The LAE sample in which the source is selected "}, {"name": "Field", "desc": "Survey field "}, {"name": "Flag", "desc": "[1/2] Galaxy/AGN flag (1=galaxy; 2=AGN) "}, {"name": "Ref", "desc": "Reference (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_81"}} {"id": "J/ApJ/911/81", "title_cds": "H-band polarimetric obs. of the S235 complex", "title_create": "Devaraj+, 2021", "year": "2021", "author": "Devaraj R., Clemens D.P., Dewangan L.K., Luna A., Ray T.P., Mackey J.", "title_pub": "Magnetic fields and star formation around HII regions: the S235 complex.", "first_author": "Devaraj R.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...81D"], "see_also": ["VII/20 : Catalogue of HII Regions (Sharpless 1959)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/ApJ/649/759 : Bubbles in the galactic disk (Churchwell+, 2006)", "J/ApJ/638/293 : 1.1mm sources in the Perseus Molecular Cloud (Enoch+, 2006)", "J/A+A/453/911 : VLA and IR observations of the S235A-B region (Felli+, 2006)", "J/ApJ/653/383 : SCUBA obs. in Orion A South region (Johnstone+, 2006)", "J/A+A/487/993 : MAMBO Mapping of c2d Clouds and Cores (Kauffmann+, 2008)", "J/ApJ/721/137 : The Bolocam Galactic Plane Survey (BGPS) (Bally+, 2010)", "J/ApJS/188/123 : The Bolocam Galactic Plane Survey. II. (Rosolowsky+, 2010)", "J/ApJ/741/21 : Polarization of stars in Taurus (Chapman+, 2011)", "J/MNRAS/414/1526 : Near-IR photometry of Sh 2-235 (Dewangan+, 2011)", "J/ApJ/741/110 : The BGPS. VII. Massive star-forming regions (Dunham+, 2011)", "J/A+A/530/A118 : G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011)", "J/ApJ/759/48 : YSOs in the Galactic HII region Sh2-297 (Mallick+, 2012)", "J/ApJS/208/14 : BGPS. IX. Data release 2. (Ginsburg+, 2013)", "J/A+A/569/L1 : Polarization hole in a starless core (Alves+, 2014)", "J/ApJ/793/126 : L204 - Cloud 3 polarimetry and photometry (Cashman+, 2014)", "J/MNRAS/439/3719 : Embedded clusters infrared photometry (Chavarria+, 2014)", "J/ApJ/783/1 : VRI and H polarization toward Sh 2-29 (Santos+, 2014)", "J/ApJ/838/80 : JHK polarimetry of stars behind bubble N4 (Chen+, 2017)", "J/ApJ/836/199 : IRDC G028.23-00.19 NIR polarimetry analysis (Hoq+, 2017)", "J/ApJ/849/157 : Polarimetry toward IC5146 background stars (Wang+, 2017)", "J/ApJ/867/79 : NIR obs. of GF 9/LDN 1082C field stars (Clemens+, 2018)", "J/ApJS/249/23 : Galactic Plane IR Polarization Survey, DR4 (Clemens+, 2020)"], "keyword_cds": "H II regions; Polarization; Photometry, infrared; Extinction; Stars, distances; Star Forming Region", "keyword_pub": "H II regions ; Magnetic fields ; Interstellar magnetic fields ; Molecular clouds ; Starlight polarization ; Polarimetry", "abstract": ["Magnetic fields are ubiquitous and essential in star formation. In", "particular, their role in regulating formation of stars across diverse", "environments like HII regions needs to be well understood. In this", "study, we present magnetic field properties toward the S235 complex", "using near-infrared (NIR) H-band polarimetric observations, obtained", "with the Mimir and POLICAN instruments. We selected 375 background", "stars in the field through combination of Gaia distances and", "extinctions from NIR colors. The plane-of-sky (POS) magnetic field", "orientations inferred from starlight polarization angles reveal a", "curved morphology tracing the spherical shell of the HII region. The", "large-scale magnetic field traced by Planck is parallel to the", "Galactic plane. We identified 11 dense clumps using 1.1mm dust", "emission, with masses between 33 and 525M_{sun}_. The clump-averaged", "POS magnetic field strengths were estimated to be between 36 and", "121{mu}G, with a mean of ~65{mu}G. The mass-to-flux ratios for the", "clumps are found to be subcritical with turbulent Alfven Mach numbers", "less than 1, indicating a strongly magnetized region. The clumps show", "scaling of magnetic field strength versus density with a power-law", "index of 0.52+/-0.07, similar to ambipolar diffusion models. Our", "results indicate that the S235 complex is a region where stellar", "feedback triggers new stars, and the magnetic fields regulate the rate", "of new star formation."], "description": ["NIR linear polarimetric observations were obtained in the H band", "(1.6um) using two instruments: Mimir and POLICAN.", "The Mimir instrument was located on the 1.8m Perkins telescope outside", "of Flagstaff, AZ. Observations with Mimir were carried out during", "2015-January for seven nights.", "The POLICAN instrument operated on the 2.1m Guillermo Haro", "Astrophysical Observatory (OAGH) telescope in Cananea, Sonora, Mexico.", "Observations with the POLICAN instrument focused on reaching finer", "angular resolutions and signal-to-noise ratios for regions with high", "stellar density. Three subfields of 4x4arcmin^2^ were observed during", "2017 September."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Polarimetric properties of the 623 stars in the S235 complex", "columns": [{"name": "Seq", "desc": "[1/623] Star sequential identifier "}, {"name": "RAdeg", "desc": "[85.1/85.41] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[35.6/35.95] Declination (J2000) "}, {"name": "Hmag", "desc": "[9.18/16.06] Mimir or POLICAN H-band magnitude "}, {"name": "e_Hmag", "desc": "[0/0.08] Uncertainty in Hmag "}, {"name": "Pol", "desc": "[0.2/9.75] debiased Polarization, percent "}, {"name": "e_Pol", "desc": "[0.078/3] Uncertainty in Pol "}, {"name": "PA", "desc": "[1.1/179.8] Equatorial Position Angle "}, {"name": "e_PA", "desc": "[0.97/32] Uncertainty in PA "}, {"name": "Q", "desc": "[-8.85/9.64] equatorial Stokes Q, percent "}, {"name": "e_Q", "desc": "[0.047/3.1] Uncertainty in Q "}, {"name": "U", "desc": "[-9.54/9.5] equatorial Stokes U, percent "}, {"name": "e_U", "desc": "[0.048/3] Uncertainty in U "}]}, {"name": "table3.dat", "desc": "Polarimetric and photometric properties of the 375 foreground-corrected embedded and background stars in the S235 complex", "columns": [{"name": "Seq", "desc": "[1/375] Star sequential identifier (does not match Table 1)"}, {"name": "RAdeg", "desc": "[85.1/85.41] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[35.6/35.95] Declination (J2000) "}, {"name": "Pol", "desc": "[0.04/9.71] Debiased Polarization, percent "}, {"name": "e_Pol", "desc": "[0.08/3] Uncertainty in Pol "}, {"name": "PA", "desc": "[1/179] Equatorial Position Angle "}, {"name": "e_PA", "desc": "[0.98/32] Uncertainty in PA "}, {"name": "Q", "desc": "[-9.03/9.44] Equatorial Stokes Q, percent "}, {"name": "e_Q", "desc": "[0.08/3.04] Uncertainty in Q "}, {"name": "U", "desc": "[-8.69/5.18] Equatorial Stokes U, percent "}, {"name": "e_U", "desc": "[0.08/3] Uncertainty in U "}, {"name": "Jmag", "desc": "[10.58/20.14] 2MASS or UKIDSS J-band magnitude "}, {"name": "e_Jmag", "desc": "[0.003/0.24] Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[10.11/16.95] 2MASS or UKIDSS H-band magnitude "}, {"name": "e_Hmag", "desc": "[0.002/0.12] Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[9.82/15.53] 2MASS or UKIDSS Ks-band magnitude "}, {"name": "e_Ksmag", "desc": "[0.002/0.13] Uncertainty in Ksmag "}, {"name": "Av", "desc": "[-1.13/25.63] Visual extinction "}, {"name": "e_Av", "desc": "[0.03/3] Uncertainty in Av "}, {"name": "rest", "desc": "[1508/5496]?=0 Estimated distance from Bailer-Jones+ 2018, I/347"}, {"name": "b_rest", "desc": "[531/3732]?=0 Lower bound on rest "}, {"name": "B_rest", "desc": "[1750/7997]?=0 Upper bound on rest "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_82"}} {"id": "J/ApJ/911/82", "title_cds": "Sparsity & gas mass fractin of galaxy clusters", "title_create": "Corasaniti+, 2021", "year": "2021", "author": "Corasaniti P.-S., Sereno M., Ettori S.", "title_pub": "Cosmological constraints from galaxy cluster sparsity, cluster gas mass fraction, and baryon acoustic oscillation data.", "first_author": "Corasaniti P.-S.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...82C"], "see_also": ["B/xmm : XMM-Newton Obs. Log (XMM-Newton Science Operation Center, 2012)", "VIII/91 : Planck Catalog of Compact Sources Release 1 (Planck, 2013)", "IX/49 : XXL Survey: First results (Pierre+, 2016)", "IX/52 : XXL Survey. DR2 (Chiappetti+, 2018)", "J/A+A/521/A78 : Velocities in the A2345 cluster (Boschin+, 2010)", "J/ApJS/199/25 : CLASH sources for MACS1149.6+2223 (Postman+, 2012)", "J/ApJS/216/27 : Galaxy clusters in the SPT-SZ survey (Bleem+, 2015)", "J/MNRAS/449/835 : Clustering of SDSS DR7 main galaxy sample. I. (Ross+, 2015)", "J/MNRAS/450/3665 : CoMaLit. III. LC2 catalog (Sereno+, 2015)", "J/A+A/594/A27 : Planck Sunyaev-Zeldovich sources (PSZ2) (Planck+, 2016)", "J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. (Riess+, 2016)", "J/ApJS/224/1 : redMaPPer cluster catalog from DES data (Rykoff+, 2016)", "J/AJ/153/220 : NORAS II. I. First results (Bohringer+, 2017)", "J/MNRAS/465/4914 : R-band light curves of HE 0435-1223 (Bonvin+, 2017)", "J/A+A/601/A145 : Catalogue of cluster members (Foex+, 2017)", "J/A+A/617/A64 : 3D density & temp. profiles of clusters (Bartalucci+, 2018)", "J/ApJ/878/55 : SPT-SZ clusters with optical & X-ray data (Bocquet+, 2019)", "J/A+A/633/A69 : KiDS-VIKING-450 cosmic shear (Hildebrandt+, 2020)", "J/ApJ/890/148 : Concentration-mass relation for XXL clusters (Umetsu+, 2020)", "http://github.com/pierste75/Halo_Sparsity : Halo_Sparsity code"], "keyword_cds": "Clusters, galaxy; Surveys; Redshifts; Optical; X-ray sources", "keyword_pub": "Cosmological parameters from large-scale structure ; Cosmology ; Galaxy clusters", "abstract": ["In recent years, the availability of large, complete cluster samples", "has enabled numerous cosmological parameter inference analyses using", "cluster number counts. These have provided constraints on the cosmic", "matter density {Omega}_m_ and the amplitude of matter density", "fluctuations {sigma}_8_ alternative to that obtained from other", "standard probes. However, systematics uncertainties, such as the mass", "calibration bias and selection effects, may still significantly affect", "these data analyses. Hence, it is timely to explore other proxies of", "galaxy cluster cosmology that can provide cosmological constraints", "complementary to those obtained from cluster number counts. Here we", "use measurements of the cluster sparsity from weak-lensing mass", "estimates of the LC^2^-single and HSC-XXL cluster catalogs to infer", "constraints on a flat {Lambda}CDM model. The cluster sparsity has the", "advantage of being insensitive to selection and mass calibration bias.", "On the other hand, it primarily constrains a degenerate combination of", "{Omega}_m_ and {sigma}_8_ (along approximately constant curves of", "S_8_={sigma}_8_({Omega}_m_/0.3)^0.5^ and, to a lesser extent, the", "reduced Hubble parameter h. Hence, in order to break the internal", "parameter degeneracies, we perform a combined likelihood analysis of", "the cluster sparsity estimates with cluster gas mass fraction", "measurements and BAO data. We find marginal constraints that are", "competitive with those from other standard cosmic probes:", "{Omega}_m_=0.316+/-0.013, {sigma}_8_=0.757+/-0.067 (corresponding to", "S_8_=0.776+/-0.064), and h=0.696+/-0.017 at 1{sigma}. Moreover,", "assuming a conservative Gaussian prior on the mass bias of gas mass", "fraction data, we find a lower limit on the gas depletion factor", "Y_b,500c_>~0.89."], "description": ["We estimate the sparsity of galaxy clusters using lensing mass", "measurements from publicly available cluster catalogs at M500c and", "M200c. In particular, we consider a selected sample of clusters from", "the Literature Catalogs of Lensing Clusters (LC^2^;", "Sereno 2015, J/MNRAS/450/3665) that includes as subsets the PSZ2Lens", "(Sereno+ 2017MNRAS.472.1946S) and the Cluster Lensing and Supernova", "Hubble (CLASH) project (Postman+ 2012, J/ApJS/199/25) catalogs. In", "addition, we consider the Subaru Hyper Suprime-Cam (HSC) lensing mass", "determinations (Umetsu+ 2020, J/ApJ/890/148) of an X-ray-selected", "cluster sample from the XXL-XMM survey (Pierre+ 2016, IX/49), which we", "refer to as the HSC-XXL sample."], "type": ["CCC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Galaxy clusters from the selected LC-single and HSC-XXL catalogs", "columns": [{"name": "Name", "desc": "Galaxy Cluster Name "}, {"name": "z", "desc": "[0.03/1.5] Redshift "}, {"name": "M200c", "desc": "[0.07/57] Weak lensing estimated M200c mass "}, {"name": "e_M200c", "desc": "[0.08/27] Uncertainty in M200c "}, {"name": "M500c", "desc": "[0.05/30] Weak lensing estimated M200c mass "}, {"name": "e_M500c", "desc": "[0.05/12] Uncertainty in M500c "}, {"name": "S200500", "desc": "[1.16/2] Sparsity (see Section 2.1) "}, {"name": "e_S200500", "desc": "[0.04/1.8] Uncertainty in S200500 "}]}, {"name": "table2.dat", "desc": "Galaxy cluster gas mass fractions ", "columns": [{"name": "Name", "desc": "Galaxy Cluster Name "}, {"name": "z", "desc": "[0.047/1.3] Redshift "}, {"name": "fgas", "desc": "[0.02/0.3] Cluster gas mass fraction (see Section 2.3)"}, {"name": "e_fgas", "desc": "[0.005/0.2] Uncertainty in fgas "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_92"}} {"id": "J/ApJ/911/92", "title_cds": "Multiwavelength study for 4FGL J0336.0+7502", "title_create": "Li+, 2021", "year": "2021", "author": "Li K.-L., Jane Yap Y.X., Hui C.Y., Kong A.K.H.", "title_pub": "Revealing a new black widow binary 4FGL J0336.0+7502.", "first_author": "Li K.-L.", "ref_biblio": [""], "bibcode": ["2021ApJ...911...92L"], "see_also": ["J/ApJS/188/405 : Fermi-LAT first source catalog (1FGL) (Abdo+, 2010)", "J/ApJS/199/31 : Fermi LAT second source catalog (2FGL) (Nolan+, 2012)", "J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)", "J/A+A/594/A116 : HI4PI spectra and column density maps (HI4PI team+, 2016)", "J/ApJ/820/8 : 3FGL sources statistical classif. (Saz Parkinson+, 2016)", "J/ApJS/247/33 : The Fermi LAT fourth source catalog (4FGL) (Abdollahi+, 2020)", "J/ApJ/904/49 : 4FGLJ0407.7-5702 optical spectroscopy & LC (Miller+, 2020)", "J/ApJ/902/L46 : Gravitational-wave limits for PSRJ1653-0158 (Nieder+, 2020)"], "keyword_cds": "Pulsars; Binaries, X-ray; Gamma rays; Photometry, VRI", "keyword_pub": "High energy astrophysics ; Gamma-ray sources ; Compact binary stars ; Millisecond pulsars ; X-ray sources", "abstract": ["We report on the discovery of a promising candidate for a black widow", "(BW) millisecond pulsar binary, 4FGL J0336.0+7502, which shows many", "pulsar-like properties in the 4FGL-DR2 catalog. Within the 95% error", "region of the LAT source, we identified an optical counterpart with a", "clear periodicity at P_orb_=3.718178(9)hr using the Bohyunsan 1.8m", "Telescope, the Lulin One-meter Telescope, the Canada-France-Hawaii", "Telescope, and Gemini-North. At the optical position, an X-ray source", "was marginally detected in the Swift/X-Ray Telescope archival data,", "and the detection was confirmed by our Chandra/ACIS DDT observation.", "The spectrum of the X-ray source can be described by a power- law", "model of {Gamma}_x_=1.6+/-0.7 and", "F_0.3-7keV_=3.5_-1.0_^+1.2^x10^-14^erg/cm^2^/s. The X-ray photon index", "and the low X-ray-to-{gamma}-ray flux ratio (i.e., <1%) are both", "consistent with that of many known BW pulsars. There is also a hint of", "an X-ray orbital modulation in the Chandra data, although the", "significance is very low (1.3{sigma}). If the pulsar identity and the", "X-ray modulation are confirmed, it would be the fifth BW millisecond", "pulsar binary that showed an orbitally modulated emission in X-rays."], "description": ["In this paper, we present a multiwavelength study for", "4FGLJ0336.0+7502, which is a new black widow millisecond pulsar binary", "(BW MSP) candidate identified by our unidentified Fermi-LAT sources", "observing campaign.", "The observations include:", "(i) the Fermi-LAT {gamma}-ray properties of 4FGL J0336.0+7502,", "see Section 2;", "(ii) optical photometric observations taken by the Bohyunsan 1.8m", "Telescope on 2019 March 31,", "the Lulin One-meter Telescope (LOT) on 2019 October 17/18,", "2019 November 10, and 2020 January 8/9,", "the Canada-France-Hawaii Telescope (CFHT) on 2017 January 25", "and February 2, and", "a 4hr series of Gemini-North photometric observations", "(PI: Kwan-Lok Li) on 2019 November 28.", "See section 3;", "(iii) four archival Swift/X-Ray Telescope (XRT) observations taken", "between 2012 April 14 and 18 and", "an observation taken on 2020 January 25 with Chandra/ACIS-S;", "see Section 4."], "object": ["03 36 06.0 +75 03 00 4FGL J0336.0+7502 = 1FGL J0334.2+7501"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "fig3.dat", "desc": "Optical light curves of 4FGL J0336.0+7502 ", "columns": [{"name": "BJD", "desc": "Barycentric Julian Date of observation "}, {"name": "omag", "desc": "[20.07/25.49] Observed magnitude "}, {"name": "e_omag", "desc": "[0.004/1.4] Uncertainty in omag "}, {"name": "Inst", "desc": "Instrument (1) "}, {"name": "Filt", "desc": "[gri] Filter "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_108"}} {"id": "J/ApJ/911/108", "title_cds": "Stars of HETDEX. I. RVels & metal-poor stars", "title_create": "Hawkins+, 2021", "year": "2021", "author": "Hawkins K., Zeimann G., Sneden C., Mentuch Cooper E., Gebhardt K., Bond H.E., Carrillo A., Casey C.M., Castanheira B.G., Ciardullo R., Davis D., Farrow D.J., Finkelstein S.L., Hill G.J., Kelz A., Liu C., Shetrone M., Schneider D.P., Starkenburg E., Steinmetz M., Wheeler J.C., The HETDEX Collaboration", "title_pub": "The stars of the HETDEX survey. I. Radial velocities and metal-poor stars from low-resolution stellar spectra.", "first_author": "Hawkins K.", "ref_biblio": [""], "bibcode": ["2021ApJ...911..108H"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "V/146 : LAMOST DR1 catalogs (Luo+, 2015)", "J/AJ/136/2050 : SEGUE stellar parameter pipeline. II. (Lee+, 2008)", "J/AJ/136/2070 : SEGUE stellar param. pipeline. III. (Allende Prieto+, 2008)", "J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009)", "J/AJ/141/89 : SEGUE stellar parameter pipeline. IV. (Smolinski+, 2011)", "J/ApJ/762/26 : Most metal-poor stars. II. Galactic halo stars (Yong+, 2013)", "J/AJ/147/136 : Stars of very low metal abundance. VI. (Roederer+, 2014)", "J/AJ/150/187 : Abundances & stellar parameters of LAMOST stars (Lee+, 2015)", "J/MNRAS/472/2517 : Stellar twins in RAVE with Gaia (Jofre+, 2017)", "J/AJ/155/181 : LAMOST/SP_Ace DR1 catalog (Boeche+, 2018)", "J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018)", "J/ApJS/238/16 : LAMOST-DR3 very metal-poor star catalog (Li+, 2018)", "J/ApJ/868/110 : R-Process Alliance: 1st release in Gal. halo (Sakari+, 2018)", "J/MNRAS/488/2283 : COMBS survey. Galactic Bulge metal-poor stars (Lucey+, 2019)", "J/ApJS/244/27 : Radial velocity measurements in LAMOST-II (Wang+, 2019)", "J/ApJS/245/34 : Abund. for 6 million stars from LAMOST DR5 (Xiang+, 2019)", "J/MNRAS/492/1164 : Abundances of Gaia DR2 wide binaries (Hawkins+, 2020)"], "keyword_cds": "Stars, metal-deficient; Radial velocities; Spectra, optical; Proper motions; Photometry; Surveys", "keyword_pub": "Stellar types ; Catalogs ; Surveys", "abstract": ["The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) is an", "unbiased, massively multiplexed spectroscopic survey, designed to", "measure the expansion history of the universe through low-resolution", "(R~750) spectra of Ly{alpha} emitters. In its search for these", "galaxies, HETDEX will also observe a few times 105 stars. In this", "paper, we present the first stellar value-added catalog within the", "internal second data release of the HETDEX Survey (HDR2). The new", "catalog contains 120,571 low-resolution spectra for 98,736 unique", "stars between 10=16) stars,", "they will be complementary to Gaia. Using t-Distributed Stochastic", "Neighbor Embedding (tSNE), we also demonstrate that the HETDEX spectra", "can be used to determine a star's Teff, and log g and its [Fe/H]. With", "the tSNE projection of the FGK-type stars with HETDEX spectra we also", "identify 416 new candidate metal-poor ([Fe/H]{<}-1dex) stars for", "future study. These encouraging results illustrate the utility of", "future low-resolution stellar spectroscopic surveys."], "description": ["The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) survey is", "currently being carried out on the Hobby-Eberly Telescope (HET), which", "is an 11m telescope with a segmented primary mirror, recently upgraded", "with a 22' field of view and 10m pupil and the Visible Integral-field", "Replicable Unit Spectrograph (VIRUS) instrument (R~750)."], "alias": ["HETDEX"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "The HETDEX-Gaia value-added catalog ", "columns": [{"name": "GaiaDR2", "desc": "Gaia DR2 source identifier "}, {"name": "RAdeg", "desc": "[5.87/335.05] Gaia DR2 right ascension (ICRS) at Ep=2015.5"}, {"name": "DEdeg", "desc": "[-1.11/67.87] Gaia DR2 declination (ICRS) at Ep=2015.5"}, {"name": "Gmag", "desc": "[4.63/21.71] Mean Gaia DR2 G band magnitude "}, {"name": "BP-RP", "desc": "[-1.92/5.1]?=-999 Gaia DR2 (Blue-Red) passband color"}, {"name": "SNR", "desc": "[0/251]?=-999 HETDEX SNR "}, {"name": "RVel", "desc": "[-999/999]?=-999 HETDEX radial velocity "}, {"name": "e_RVel", "desc": "[0.04/1176725]?=-999 Uncertainty in RVel "}, {"name": "Bcor", "desc": "[-30.4/30]?=-999 Barycentric correction for RVel"}, {"name": "e_RAdeg", "desc": "[0.006/91] Uncertainty in RAdeg "}, {"name": "e_DEdeg", "desc": "[0.009/94] Uncertainty in DEdeg "}, {"name": "plx", "desc": "[-18/41]?=-999 Gaia DR2 parallax "}, {"name": "e_plx", "desc": "[0.01/4.6]?=-999 Uncertainty in plx "}, {"name": "pmRA", "desc": "[-869/300]?=-999 Gaia DR2 proper motion along RA"}, {"name": "e_pmRA", "desc": "[0.02/5.1]?=-999 Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-545/296]?=-999 Gaia DR2 proper motion along DE"}, {"name": "e_pmDE", "desc": "[0.02/5.4]?=-999 Uncertainty in pmDE "}, {"name": "Dup", "desc": "Duplicated source? (\"false\" or \"true\") "}, {"name": "GFlux", "desc": "[39/264144000] Mean Gaia DR2 G band flux (1)"}, {"name": "e_GFlux", "desc": "[0.5/771430] Uncertainty in GFlux (1) "}, {"name": "BPFlux", "desc": "[3/163728000]?=-999 Mean Gaia DR2 Blue passband flux (1)"}, {"name": "e_BPFlux", "desc": "[0.06/264439]?=-999 Uncertainty in BPFlux (1)"}, {"name": "BPmag", "desc": "[4.8/24.13]?=-999 Mean Gaia DR2 Blue passband magnitude"}, {"name": "RPFlux", "desc": "[5/124350000]?=-999 Mean Gaia DR2 Red passband flux (1)"}, {"name": "e_RPFlux", "desc": "[0.1/349102]?=-999 Uncertainty in RPFlux (1)"}, {"name": "RPmag", "desc": "[4.5/23]?=-999 Mean Gaia DR2 Red passband magnitude"}, {"name": "GRVel", "desc": "[-279/125]?=-999 Gaia DR2 radial velocity "}, {"name": "e_GRVel", "desc": "[0.1/20]?=-999 Uncertainty in GRVel "}, {"name": "NGRVel", "desc": "[0/87] Number of Gaia DR2 radial velocity epochs"}, {"name": "Teff", "desc": "[3229/9674]?=-999 Gaia DR2 Effective temperature"}, {"name": "AG", "desc": "[0.01/2.8]?=-999 Gaia G band extinction "}, {"name": "E(BP-RP)", "desc": "[0/1.43]?=-999 Estimate of reddening "}, {"name": "Rad", "desc": "[0.5/82]?=-999 Radius "}, {"name": "Lum", "desc": "[0.03/1606]?=-999 Luminosity "}, {"name": "HRVc", "desc": "[1/2]?=-999 Number of HETDEX Radial Velocity CCF Components"}, {"name": "tX", "desc": "[-46/49]?=-999 tSNE X-location (2) "}, {"name": "tY", "desc": "[-39/44]?=-999 tSNE Y-location (2) "}, {"name": "GaiaEDR3", "desc": "Gaia EDR3 source identifier "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_109"}} {"id": "J/ApJ/911/109", "title_cds": "RR Lyrae variable stars in DES Y6", "title_create": "Stringer+, 2021", "year": "2021", "author": "Stringer K.M., Drlica-Wagner A., Macri L., Martinez-Vazquez C.E., Vivas A.K., Ferguson P., Pace A.B., Walker A.R., Neilsen E., Tavangar K., Wester W., Abbott T.M.C., Aguena M., Allam S., Bacon D., Bechtol K., Bertin E., Brooks D., Burke D.L., Carnero Rosell A., Carrasco Kind M., Carretero J., Costanzi M., Crocce M., da Costa L.N., Pereira M.E.S., De Vicente J., Desai S., Diehl H.T., Doel P., Ferrero I., Garcia-Bellido J., Gaztanaga E., Gerdes D.W., Gruen D., Gruendl R.A., Gschwend J., Gutierrez G., Hinton S.R., Hollowood D.L., Honscheid K., Hoyle B., James D.J., Kuehn K., Kuropatkin N., Li T.S., Maia M.A.G., Marshall J.L., Menanteau F., Miquel R., Morgan R., Ogando R.L.C., Palmese A., Paz-Chinchon F., Plazas A.A., Roodman A., Sanchez E., Schubnell M., Serrano S., Sevilla-Noarbe I., Smith M., Soares-Santos M., Suchyta E., Tarle G., Thomas D., To C., Varga T.N., Wilkinson R.D., Zhang Y., The DES Collaboration", "title_pub": "Identifying RR Lyrae variable stars in six years of the Dark Energy Survey.", "first_author": "Stringer K.M.", "ref_biblio": [""], "bibcode": ["2021ApJ...911..109S"], "see_also": ["II/347 : KiDS-ESO-DR3 multi-band source catalog (de Jong+, 2017)", "II/357 : The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)", "VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)", "II/371 : The Dark Energy Survey (DES): Data Release 2 (Abbott+, 2021)", "J/AcA/51/221 : OGLE-II. Cepheids in IC 1613 (Udalski+, 2001)", "J/AJ/123/840 : VI photometry of variable stars in Fornax (Bersier+, 2002)", "J/AJ/127/1158 : QUEST RR Lyrae Survey first catalog (Vivas+, 2004)", "J/AJ/132/714 : QUEST RR Lyrae survey. II. Halo overdensities (Vivas+, 2006)", "J/MNRAS/398/1757 : RR Lyraes in SDSS stripe 82 (Watkins+, 2009)", "J/ApJ/712/1259 : LCID project. II. Variables in IC1613 (Bernard+, 2010)", "J/ApJ/708/717 : Light curve templates of RR Lyrae stars (Sesar+, 2010)", "J/ApJ/731/4 : Galactic halo as seen by the CFHTLS (Sesar+, 2011)", "J/A+A/544/A73 : BVI photometry of Fornax dSph galaxy (de Boer+, 2012)", "J/ApJ/753/106 : Quasar variability with SDSS & POSS imaging (MacLeod+, 2012)", "J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)", "J/ApJ/763/32 : Galactic halo RRab stars from CSS (Drake+, 2013)", "J/ApJ/765/154 : RR Lyrae stars in the Catalina Sky Survey (Drake+, 2013)", "J/AJ/145/160 : Variables in LMC GCs. III. Reticulum (Kuehn+, 2013)", "J/ApJS/213/9 : Catalina Surveys periodic variable stars (Drake+, 2014)", "J/ApJ/788/105 : XSTPS RR Lyrae in the north Galactic cap (Faccioli+, 2014)", "J/ApJ/793/135 : Positions and distances of RR Lyrae stars (Sesar+, 2014)", "J/ApJ/793/62 : Triangulum-Andromeda stellar properties (Sheffield+, 2014)", "J/PASP/126/616 : Variable stars in Leo I dSph (Stetson+, 2014)", "J/ApJ/781/22 : Region I of La Silla QUEST RR Lyrae stars (Zinn+, 2014)", "J/A+A/584/A106 : Catalogues of variable AGNs (Simm+, 2015)", "J/MNRAS/446/2251 : Southern Catalina Survey type-ab RR Lyrae (Torrealba+, 2015)", "J/ApJ/817/73 : QSOs & RR Lyrae in PS1 3{pi} Data (Hernitschek+ 2016)", "J/MNRAS/462/4349 : Variable stars in Sculptor dSph (Martinez-Vazquez+, 2016)", "J/MNRAS/469/3688 : CSS Periodic Variable Star Catalogue (Drake+, 2017)", "J/AJ/154/263 : NIR photometry of 77 RR Lyrae stars (Karczmarek+, 2017)", "J/ApJ/850/137 : ISLAndS project. III. Var. stars (Martinez-Vazquez+, 2017)", "J/AJ/153/204 : RR Lyrae stars from the PS1 3{pi} survey (Sesar+, 2017)", "J/AJ/153/107 : Australian Dark Energy Survey (OzDES) QSO cat. (Tie+, 2017)", "J/AJ/154/85 : CTIO/DECam photometry of RR Lyrae stars in M5 (Vivas+, 2017)", "J/MNRAS/474/4112 : Candidate RR Lyr star streams in inner Galaxy (Mateu+, 2018)", "J/ApJ/855/43 : Distant RR Lyrae stars discovered with HiTS (Medina+, 2018)", "J/MNRAS/480/669 : Variable stars in the SMCNOD (Prudil+, 2018)", "J/A+A/622/A60 : Gaia DR2 misclassified RR Lyrae list (Clementini+, 2019)", "J/A+A/624/A13 : KiDS DR3 QSO catalog (Nakoneczny+, 2019)", "J/ApJ/875/77 : PMs of MW satellites with Gaia & DES (Pace+, 2019)", "J/AJ/158/223 : RR Lyrae members of Pal 5 stream (Price-Whelan+, 2019)", "J/AJ/158/16 : Identification of RR Lyrae stars from DES (Stringer+, 2019)", "J/ApJ/893/47 : MW satellite census. I. DES & PS1 (Drlica-Wagner+, 2020)", "J/A+A/638/A104 : GaiaDR2 cand. RR Lyrae of Sgr stream & dwarf (Ramos+, 2020)", "J/ApJ/892/137 : Spectroscopy of Grus II, Tuc IV and Tuc V (Simon+, 2020)", "http://www.sdss.org/ : SDSS home page", "http://des.ncsa.illinois.edu/releases/other/y6-rrl : DES Y6 RR Lyrae home page"], "keyword_cds": "Stars, variable; Photometry, ugriz; Extinction; Cross identifications", "keyword_pub": "RR Lyrae variable stars ; RRab variable stars ; Milky Way stellar halo ; Milky Way Galaxy", "abstract": ["We present a search for RR Lyrae stars using the full six-year data", "set from the Dark Energy Survey covering ~5000deg^2^ of the southern", "sky. Using a multistage multivariate classification and light-curve", "template-fitting scheme, we identify RR Lyrae candidates with a median", "of 35 observations per candidate. We detect 6971 RR Lyrae candidates", "out to ~335kpc, and we estimate that our sample is >70% complete at", "~150kpc. We find excellent agreement with other wide-area RR Lyrae", "catalogs and RR Lyrae studies targeting the Magellanic Clouds and", "other Milky Way satellite galaxies. We fit the smooth stellar halo", "density profile using a broken-power-law model with fixed halo", "flattening (q=0.7), and we find strong evidence for a break at", "R_0_=32.1_-0.9_^+1.1^kpc with an inner slope of", "n_1_=-2.54_-0.09_^+0.09^ and an outer slope of", "n_2_=-5.42_-0.14_^+0.13^. We use our catalog to perform a search for", "Milky Way satellite galaxies with large sizes and low luminosities.", "Using a set of simulated satellite galaxies, we find that our RR", "Lyrae-based search is more sensitive than those using resolved stellar", "populations in the regime of large (rh>=500pc), low-surface-brightness", "dwarf galaxies. A blind search for large, diffuse satellites yields", "three candidate substructures. The first can be confidently associated", "with the dwarf galaxy Eridanus II. The second has a distance and", "proper motion similar to the ultrafaint dwarf galaxy Tucana II but is", "separated by ~5 deg. The third is close in projection to the globular", "cluster NGC 1851 but is ~10 kpc more distant and appears to differ in", "proper motion."], "description": ["The Dark Energy Survey (DES, see II/371) was a six-year", "optical/near-infrared imaging survey covering ~5000deg^2^ of the", "southern Galactic cap using the Dark Energy Camera (DECam) mounted at", "the prime focus of the 4m Blanco telescope at the Cerro Tololo", "Inter-American Observatory (CTIO). Observations were completed in", "2019-January. DES obtained ~10x90s exposures in five broadband filters,", "grizY.", "As in Stringer+ 2019, J/AJ/158/16, the light curves for this work were", "assembled using the internal DES \"Quick\" release pipeline."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "The Dark Energy Survey (DES) Y6 RRab candidates ", "columns": [{"name": "ID", "desc": "[871765223/1700521769] DES Y6A1 Coadd Object ID "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "[-67/5] Decination, decimal degrees (J2000) "}, {"name": "Ag", "desc": "[0.01/0.55] Extinction, g band (1) "}, {"name": "Ar", "desc": "[0.008/0.4] Extinction, r band (1) "}, {"name": "Ai", "desc": "[0.006/0.3] Extinction, i band (1) "}, {"name": "Az", "desc": "[0.004/0.21] Extinction, z band (1) "}, {"name": "AY", "desc": "[0.004/0.18] Extinction, Y band (1) "}, {"name": "gmag0", "desc": "[14.15/23.44]? Mean g-band magnitude with extinction correction"}, {"name": "rmag0", "desc": "[14.38/23.3]? Mean r-band magnitude with extinction correction"}, {"name": "imag0", "desc": "[14.43/23.2]? Mean i-band magnitude with extinction correction"}, {"name": "zmag0", "desc": "[14.19/23.01]? Mean z-band magnitude with extinction correction"}, {"name": "Ymag0", "desc": "[13.87/22.34]? Mean Y-band magnitude with extinction correction"}, {"name": "Nobs", "desc": "[10/73] Number of Observations "}, {"name": "Per", "desc": "[0.3/1] Best fit period "}, {"name": "Amp", "desc": "[0.14/1.93] Best-fit model amplitude "}, {"name": "mu", "desc": "[13.26/22.61] Best-fit distance modulus "}, {"name": "RF1", "desc": "[0.75/1] Score from first random forest classifier (variability)"}, {"name": "RF2", "desc": "[0.34/1] Score from second random forest classifier (variability)"}, {"name": "RF3", "desc": "[0.6/1] Score from third random forest classifier (template fit)"}, {"name": "GaiaDR2", "desc": "?=-99 Gaia DR2 source_id for cross-matched RRab in Clementini+ (2019, J/A+A/622/A60)"}, {"name": "PS1", "desc": "?=-99 Pan-Starrs PS1 identifier from Sesar+ (2017, J/AJ/153/204) RRab catalog"}, {"name": "CSDR2", "desc": "?=-99 Catalina Surveys DR2 RRab catalog identifier (2)"}, {"name": "DESY3Q2", "desc": "?=-99 DES Y3Q2 identifier from Stringer+ (2019, J/AJ/158/16)"}, {"name": "Sys", "desc": "Association with resolved stellar system "}, {"name": "SysID", "desc": "Star identifier in System from previous study "}, {"name": "r_Sys", "desc": "Reference for star in System (3) "}, {"name": "ACc", "desc": "Anomalous Cepheid candidate (\"True\"=11 occurrences or \"False\")"}]}, {"name": "lcs/*", "desc": "The light curves in CSV format for each RRab candidate", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_138"}} {"id": "J/ApJ/911/138", "title_cds": "Low-mass pre-main-sequence stars in Taurus-Auriga", "title_create": "Nofi+, 2021", "year": "2021", "author": "Nofi L.A., Johns-Krull C.M., Lopez-Valdivia R., Biddle L., Carvalho A.S., Huber D., Jaffe D., Llama J., Mace G., Prato L., Skiff B., Sokal K.R., Sullivan K., Tayar J.", "title_pub": "Projected rotational velocities and fundamental properties of low-mass pre-main-sequence stars in the Taurus-Auriga star-forming region.", "first_author": "Nofi L.A.", "ref_biblio": [""], "bibcode": ["2021ApJ...911..138N"], "see_also": ["II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "J/A+AS/101/485 : Multisite UBVRI photometry in Tau-Aur cloud (Bouvier+ 1993)", "J/ApJS/95/535 : Infrared CO line list for X1{Sigma}+state (Goorvitch, 1994)", "J/A+A/299/89 : COYOTES II (Bouvier+, 1995)", "J/A+AS/145/187 : uvby-{beta} photometry of WTTS (Chavarria-K+, 2000)", "J/A+A/396/513 : Stellar Rotation in the Orion Nebula Cluster (Herbst+, 2002)", "J/ApJ/601/979 : vsini of Orion low-mass stars (Wolff+, 2004)", "J/A+A/430/1005 : VRIH{alpha} photometry of NGC 2264 variables (Lamm+, 2005)", "J/AJ/129/363 : Sp. in Orion Nebula Cluster (Sicilia-Aguilar+, 2005)", "J/A+A/450/681 : Companions to close sp. binaries (Tokovinin+, 2006)", "J/A+A/467/785 : SuperWASP/ROSAT periodic variable stars (Norton+, 2007)", "J/A+A/479/827 : UBVR LCs of weak-line T Tauri stars (Grankin+, 2008)", "J/ApJ/704/531 : The coevality of young binary systems (Kraus+, 2009)", "J/ApJ/745/56 : Upper Sco members rotational velocities (Dahm+, 2012)", "J/ApJ/745/19 : Binary systems in Taurus-Auriga (Kraus+, 2012)", "J/ApJ/745/119 : Close companions to young stars. I. (Nguyen+, 2012)", "J/AJ/143/93 : Rotational velocities in early-M stars (Reiners+, 2012)", "J/ApJS/208/9 : Intrinsic colors & temperatures of PMS stars (Pecaut+, 2013)", "J/ApJ/786/97 : Photospheric properties of T Tauri stars (Herczeg+, 2014)", "J/MNRAS/468/931 : Orion Nebula Cluster members VRI photometry (Messina+, 2017)", "J/MNRAS/480/3739 : Extended main sequence turnoff in open cl. (Bastian+, 2018)", "J/AJ/155/225 : M dwarf stars rot. broadening measurements (Kesseli+, 2018)", "J/AJ/156/271 : The stellar membership of the Taurus SFR (Luhman, 2018)", "J/A+A/615/A76 : Spectroscopic param. of stars (SPECIES). I. (Soto+, 2018)", "J/AJ/156/275 : Rot. evolution of young, binary M dwarfs (Stauffer+, 2018)", "J/AJ/158/54 : New Taurus members (Esplin+, 2019)", "J/ApJ/879/105 : Eff. temperatures of low-mass stars (Lopez-Valdivia+, 2019)", "J/AJ/159/273 : Taurus members & nonmembers with K2 data (Rebull+, 2020)"], "keyword_cds": "Stars, pre-main sequence; Spectra, infrared; Optical; Rotational velocities; Stars, diameters; Effective temperatures", "keyword_pub": "Stellar rotation ; Pre-main-sequence stars ; Low-mass stars ; Fundamental parameters of stars ; High-resolution spectroscopy", "abstract": ["The projected stellar rotational velocity (vsini) is critical for our", "understanding of processes related to the evolution of angular", "momentum in pre-main-sequence stars. We present vsini measurements of", "high-resolution infrared and optical spectroscopy for 70", "pre-main-sequence stars in the Taurus-Auriga star-forming region, in", "addition to effective temperatures measured from line-depth ratios, as", "well as stellar rotation periods determined from optical photometry.", "From the literature, we identified the stars in our sample that show", "evidence of residing in circumstellar disks or multiple systems. The", "comparison of infrared vsini measurements calculated using two", "techniques shows a residual scatter of ~1.8km/s, defining a typical", "error floor for the vsini of pre-main-sequence stars from infrared", "spectra. A comparison of the vsini distributions of stars with and", "without companions shows that binaries/multiples typically have a", "higher measured vsini, which may be caused by contamination by", "companion lines, shorter disk lifetimes in binary systems, or tidal", "interactions in hierarchical triples. A comparison of optical and", "infrared vsini values shows no significant difference regardless of", "whether the star has a disk or not, indicating that CO contamination", "from the disk does not impact vsini measurements above the typical", "~1.8km/s error floor of our measurements. Finally, we observe a lack", "of a correlation between the vsini, presence of a disk, and H-R", "diagram position, which indicates a complex interplay between stellar", "rotation and evolution of pre-main-sequence stars."], "description": ["The infrared spectral observations used to measure the Teff and the", "vsini were obtained using the Immersion GRating INfrared Spectrometer", "(IGRINS) at both the 2.7m Harlan J. Smith Telescope at McDonald", "Observatory, and the 4.3m Lowell Discovery Telescope between 2014", "October and 2018 March. IGRINS is a high-resolution (R~45000)", "near-infrared spectrograph with no moving parts that simultaneously", "records the H and K bands (1.4-2.5um). See Section 2.2.1.", "In addition to the infrared spectroscopy, we also obtained optical", "high-resolution (R~60000) spectra at McDonald Observatory as part of", "the ongoing search for substellar companions to young stars. Starting", "in 2004 and continuing to the present time, spectra have been obtained", "primarily with the McDonald Observatory 2.7m Harlan J. Smith telescope", "coupled to the Robert G. Tull cross-dispersed coude echelle", "spectrograph. A smaller number of stars have been observed with the", "2.1m Otto Struve telescope coupled to the Sandiford echelle cassegrain", "spectrometer. See Section 2.2.2.", "We obtained ground-based photometry for many of our targets, to", "determine stellar rotation periods. Our ground-based photometry comes", "from seasonal V-band monitoring of the sample stars using the Lowell", "0.7m robotic telescope. The stars have generally been observed for", "about ten nights per month from September through March each year", "since 2012, using CCD differential aperture photometry. Additionally,", "we obtained rotation periods for several of our sample targets from", "the K2 long-cadence time-series photometry observed during Campaign 13", "between 2017 March 8 and 2017 May 27 UTC. See Section 2.2.3."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Stellar properties of pre-main sequence stars ", "columns": [{"name": "Name", "desc": "Target name (1) "}, {"name": "n_Name", "desc": "Flag on name (2) "}, {"name": "RAh", "desc": "[4/5] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[14/30] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Kmag", "desc": "[5.3/11.6]? K-band apparent magnitude "}, {"name": "Nir", "desc": "[3/54] Number of infrared observations "}, {"name": "Nop", "desc": "[1/43]? Number of optical observations "}, {"name": "Mult", "desc": "Multiplicity (3) "}, {"name": "Teff", "desc": "[3100/4900]? Effective temperature (4) "}, {"name": "l_vsiniIR", "desc": "Limit flag on vsini-IR "}, {"name": "vsiniIR", "desc": "[4/50]? Infrared vsini (5) "}, {"name": "e_vsiniIR", "desc": "[1.7/3.4]? Infrared vsini uncertainty "}, {"name": "l_vsiniOp", "desc": "Limit flag on vsini-op "}, {"name": "vsiniOp", "desc": "[7/50]? Optical vsini "}, {"name": "e_vsiniOp", "desc": "[0.4/5.1]? Optical vsini uncertainty "}, {"name": "vsini", "desc": "[4/83]? Published vsini (6) "}, {"name": "e_vsini", "desc": "[0.04/4]? Published vsini uncertainty "}, {"name": "Prot", "desc": "[0.7/15.7]? Stellar rotation period "}, {"name": "e_Prot", "desc": "[0.02/0.1]? Period uncertainty "}, {"name": "r_Prot", "desc": "[1/8]? Period reference (7) "}, {"name": "l_Rsini", "desc": "Limit flag on Rsini "}, {"name": "Rsini", "desc": "[0.7/2.1]? Lower limit stellar radius "}, {"name": "e_Rsini", "desc": "[0.05/0.5]? Rsini uncertainty "}, {"name": "Class", "desc": "? Classification (8) "}, {"name": "r_Class", "desc": "[1/4]? Classification reference (9) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_149"}} {"id": "J/ApJ/911/149", "title_cds": "Spectroscopic obs. in ATLAS and Aliqa Uma streams", "title_create": "Li+, 2021", "year": "2021", "author": "Li T.S., Koposov S.E., Erkal D., Ji A.P., Shipp N., Pace A.B., Hilmi T., Kuehn K., Lewis G.F., Mackey D., Simpson J.D., Wan Z., Zucker D.B., Bland-Hawthorn J., Cullinane L.R., Da Costa G.S., Drlica-Wagner A., Hattori K., Martell S.L., Sharma S., The S5 Collaboration", "title_pub": "Broken into pieces: ATLAS and Aliqa Uma as one single stream.", "first_author": "Li T.S.", "ref_biblio": [""], "bibcode": ["2021ApJ...911..149L"], "see_also": ["II/350 : VLT Survey Telescope ATLAS (Shanks+, 2015)", "II/357 : The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/AJ/131/2114 : Radial velocities in Fornax dSph (Walker+, 2006)", "J/A+A/466/181 : BVI photometry of Whiting 1 (Carraro+, 2007)", "J/ApJ/736/146 : Radial velocities of stars in Bootes I (Koposov+, 2011)", "J/AJ/141/175 : Abundances in M15 RGB/RHB stars (Sobeck+, 2011)", "J/ApJ/757/83 : The Blanco Cosmology Survey (BCS) (Desai+, 2012)", "J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)", "J/MNRAS/434/1681 : Extremely metal-poor stars CaII triplet (Carrera+, 2013)", "J/A+A/561/A87 : FLAMES observations of Terzan 8 (Carretta+, 2014)", "J/ApJ/834/57 : MW molecular clouds from ^12^CO (Miville-Deschenes+, 2017)", "J/A+A/616/A10 : Open clusters GaiaDR2 HR diagrams (Gaia Collaboration, 2018)", "J/A+A/616/A12 : Gaia DR2 sources in GC and dSph (Gaia Collaboration+, 2018)", "J/ApJ/866/22 : Spectroscopic analysis of Tuc III stream (Li+, 2018)", "J/MNRAS/481/1195 : Gaia DR2 RRL stars as standard candles (Muraveva+, 2018)", "J/MNRAS/482/5138 : Galactic GC mean PMs & velocities (Baumgardt+, 2019)", "J/AJ/158/223 : RRL members of Pal 5 stellar stream (Price-Whelan+, 2019)", "J/ApJ/885/3 : Membership in 12 stellar streams from DES (Shipp+, 2019)", "J/MNRAS/484/2832 : Proper motions of MW globular clusters (Vasiliev, 2019)", "J/AJ/159/287 : Stellar parameters in Oph Stream with MMT (Caldwell+, 2020)", "J/AJ/160/181 : Chemical abundances in red giants with Magellan (Ji+, 2020)"], "keyword_cds": "Associations, stellar; Abundances, [Fe/H]; Radial velocities; Stars, horizontal branch; Stars, variable; Spectra, optical; Photometry", "keyword_pub": "Tidal disruption ; Stellar kinematics ; Stellar motion ; Stellar associations ; Metallicity ; Stellar abundances ; Dark matter ; Milky Way dark matter halo ; Stellar streams ; Milky Way dynamics", "abstract": ["We present the first spectroscopic measurements of the ATLAS and Aliqa", "Uma streams from the Southern Stellar Stream Spectroscopic Survey", "(S5), in combination with the photometric data from the Dark Energy", "Survey and astrometric data from Gaia. From the coherence of", "spectroscopic members in radial velocity and proper motion, we find", "that these two systems are extremely likely to be one stream with", "discontinuity in morphology and density on the sky (the \"kink\"", "feature). We refer to this entire stream as the ATLAS-Aliqa Uma", "stream, or the AAU stream. We perform a comprehensive exploration of", "the effect of baryonic substructures and find that only an encounter", "with the Sagittarius dwarf ~0.5Gyr ago can create a feature similar to", "the observed \"kink.\" In addition, we also identify two gaps in the", "ATLAS component associated with the broadening in the stream width", "(the \"broadening\" feature). These gaps have likely been created by", "small mass perturbers, such as dark matter halos, as the AAU stream is", "the most distant cold stream known with severe variations in both the", "stream surface density and the stream track on the sky. With the", "stream track, stream distance, and kinematic information, we determine", "the orbit of the AAU stream and find that it has been affected by the", "Large Magellanic Cloud, resulting in a misalignment between the proper", "motion and stream track. Together with the Orphan-Chenab Stream, AAU", "is the second stream pair that has been found to be a single stream", "separated into two segments by external perturbation."], "description": ["The ATLAS and Aliqa Uma streams were observed in 2018 as part of the", "Southern Stellar Stream Spectroscopic Survey (S^5^ program), which", "uses the AAOmega spectrograph on the 3.9m Anglo-Australian Telescope", "(AAT), fed by the Two Degree Field (\"2dF\") fiber positioner facility,", "allowing the acquisition of up to 392 simultaneous spectra of objects", "within a 2{deg} field in diameter on the sky. We refer readers to", "Paper I (Li+ 2019MNRAS.490.3508L) for details on the survey strategy,", "target selection, observation, and reduction of S^5^.", "A total of five AAT fields were observed in Aliqa Uma and 12 fields in", "ATLAS, with a total covered length of the stream of about 34{deg} on", "the sky."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "A total of 96 spectroscopic members in ATLAS stream and Aliqa Uma stream", "columns": [{"name": "Gaia", "desc": "Gaia DR2 source identifier "}, {"name": "RAdeg", "desc": "[9.1/40.4] Gaia DR2 Right Ascension in decimal degrees (ICRS) at Ep=2015.5"}, {"name": "DEdeg", "desc": "[-37.6/-20.4] Gaia DR2 Declination in decimal degrees (ICRS) at Ep=2015.5"}, {"name": "SNR", "desc": "[2.6/77.5] Signal-to-Noise "}, {"name": "Gmag", "desc": "[14.96/19.58] Gaia DR2 G band magnitude "}, {"name": "RVel", "desc": "[-157/-5] Heliocentric radial velocity "}, {"name": "e_RVel", "desc": "[0.6/21] Uncertainty in RVel "}, {"name": "[Fe/H]", "desc": "[-2.71/-1.93]? Metallicity "}, {"name": "e_[Fe/H]", "desc": "[0.1/0.53]? Uncertainty in [Fe/H] "}]}, {"name": "table2.dat", "desc": "Blue horizontal branch (BHB) and RR Lyrae (RRL) members in ATLAS stream and Aliqa Uma stream", "columns": [{"name": "Gaia", "desc": "Gaia DR2 source identifier "}, {"name": "RAdeg", "desc": "[9.97/38.25] Gaia DR2 Right Ascension in decimal degrees (ICRS) at Ep=2015.5"}, {"name": "DEdeg", "desc": "[-35.82/-20.8] Gaia DR2 Declination in decimal degrees (ICRS) at Ep=2015.5"}, {"name": "m-M", "desc": "[16.21/17.29] Distance modulus "}, {"name": "Cl", "desc": "Tracer identifier (1) "}]}, {"name": "table3.dat", "desc": "A total of 25 spectroscopic members in Palca stream, found in the ATLAS-Aliqa Uma (AAU) stream fields", "columns": [{"name": "Gaia", "desc": "Gaia DR2 source identifier "}, {"name": "RAdeg", "desc": "[29.75/39.6] Gaia DR2 Right Ascension in decimal degrees (ICRS) at Ep=2015.5"}, {"name": "DEdeg", "desc": "[-37.86/-31.5] Gaia DR2 Declination in decimal degrees (ICRS) at Ep=2015.5"}, {"name": "SNR", "desc": "[2.9/75.3] Signal-to-Noise "}, {"name": "Gmag", "desc": "[15.44/19.5] Gaia DR2 G band magnitude "}, {"name": "RVel", "desc": "[81/118] Heliocentric radial velocity "}, {"name": "e_RVel", "desc": "[0.6/34] Uncertainty in RVel "}, {"name": "[Fe/H]", "desc": "[-2.21/-1.57]? Metallicity "}, {"name": "e_[Fe/H]", "desc": "[0.1/0.34]? Uncertainty in [Fe/H] "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJ_911_153"}} {"id": "J/ApJ/911/153", "title_cds": "HST 1.60um & 2.05um images of protostars in Orion", "title_create": "Habel+, 2021", "year": "2021", "author": "Habel N.M., Thomas Megeath S., Jon Booker J., Fischer W.J., Kounkel M., Poteet C., Furlan E., Stutz A., Manoj P., Tobin J.J., Nagy Z., Pokhrel R., Watson D.", "title_pub": "An HST survey of protostellar outflow cavities: does feedback clear envelopes?", "first_author": "Habel N.M.", "ref_biblio": [""], "bibcode": ["2021ApJ...911..153H"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "J/A+A/291/943 : Protostellar cores (Ossenkopf+, 1994)", "J/ApJ/566/993 : rho Oph (Lynds 1688) cluster NICMOS imaging (Allen+, 2002)", "J/A+A/462/L17 : Dense cores in interstellar molecular clouds (Alves+, 2007)", "J/A+A/472/187 : 12CO outflows towards submm cores in Perseus (Hatchell+, 2007)", "J/AJ/144/192 : Spitzer survey of Orion A & B. I. YSO catalog (Megeath+, 2012)", "J/AJ/145/94 : Luminosities of protostars from Spitzer (Dunham+, 2013)", "J/ApJ/767/36 : APEX observations of HOPS protostars (Stutz+, 2013)", "J/ApJ/783/6 : Deconvolved Spitzer images of 89 protostars (Velusamy+, 2014)", "J/A+A/584/A91 : Dense cores in Aquila from Herschel (Konyves+, 2015)", "J/ApJS/224/5 : The Herschel Orion Protostar Survey (HOPS) (Furlan+, 2016)", "J/ApJ/821/52 : NIR survey of Spitzer YSOs in Orion MoC (Kounkel+, 2016)", "J/A+A/619/A106 : 3D shape of Orion A from Gaia DR2 (Grossschedl+, 2018)", "J/AJ/156/84 : APOGEE-2 survey of Orion Complex. II. (Kounkel+, 2018)"], "keyword_cds": "YSOs; Molecular clouds; Infrared sources", "keyword_pub": "Protostars ; Stellar feedback ; Molecular clouds ; Near infrared astronomy ; Stellar jets ; Early stellar evolution", "abstract": ["We study protostellar envelope and outflow evolution using Hubble", "Space Telescope NICMOS or WFC3 images of 304 protostars in the Orion", "molecular clouds. These near-IR images resolve structures in the", "envelopes delineated by the scattered light of the central protostars", "with 80au resolution, and they complement the 1.2{mu}m to 870{mu}m", "spectral energy distributions (SEDs) obtained with the Herschel Orion", "Protostar Survey program. Based on their 1.60{mu}m morphologies, we", "classify the protostars into five categories: nondetections, point", "sources without nebulosity, bipolar cavity sources, unipolar cavity", "sources, and irregulars. We find point sources without associated", "nebulosity are the most numerous, and show through monochromatic Monte", "Carlo radiative transfer modeling that this morphology occurs when", "protostars are observed at low inclinations or have low envelope", "densities. We also find that the morphology is correlated with the", "SED-determined evolutionary class, with Class 0 protostars more likely", "to be nondetections, Class I protostars to show cavities, and", "flat-spectrum protostars to be point sources. Using an edge detection", "algorithm to trace the projected edges of the cavities, we fit power", "laws to the resulting cavity shapes, thereby measuring the cavity", "half-opening angles and power-law exponents. We find no evidence for", "the growth of outflow cavities as protostars evolve through the", "Class I protostar phase, in contradiction with previous studies of", "smaller samples. We conclude that the decline of mass infall with time", "cannot be explained by the progressive clearing of envelopes by", "growing outflow cavities. Furthermore, the low star formation", "efficiency inferred for molecular cores cannot be explained by", "envelope clearing alone."], "description": ["The HST observations were assembled from two GO programs and a", "snapshot program. The bulk of the sample was observed in program GO", "11548. The Near Infrared Camera and Multi-Object Spectrometer's", "(NICMOS) F205W and F160W filters were used for a total of 87 orbits in", "August and September of 2008 to image 92 objects in the HOPS catalog.", "After the 2009 June deployment of the Wide Field Camera 3 (WFC3),", "126 orbits were used between 2009 August and 2010 December to observe", "237 HOPS objects with the F160W filter. The observation and reduction", "of these data is described in Kounkel+ (2016, J/ApJ/821/52).", "A subsequent program using WFC3, SNAP 14181, was designed to target", "multiple star-forming regions within 500pc. It completed observations", "during 114 orbits between 2015 December and 2017 September, 10 of", "which imaged 13 objects in the Orion molecular clouds. A final WFC3", "study, program GO 14695, targeted four objects in Orion with weak 24um", "fluxes atypical of protostars. These observations were conducted in", "2016 September with four orbits."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table4.dat", "desc": "All HST sources ", "columns": [{"name": "HOPS", "desc": "[1/410] HOPS identifier "}, {"name": "f_HOPS", "desc": "[4/6]? Flag on HOPS (1) "}, {"name": "RAh", "desc": "[5] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[33/54] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+/-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[0/8] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Class", "desc": "SED class (2) "}, {"name": "Tbol", "desc": "[24.6/1211]? Bolometric temperature (2) "}, {"name": "Inst", "desc": "Instrument (3) "}, {"name": "PS", "desc": "Point source? (4) "}, {"name": "Morph", "desc": "Morphology type from F160W image "}, {"name": "Vol", "desc": "[0.4/37.6]? Percent volume cleared "}, {"name": "Angle", "desc": "[4/50]? Half-opening angle "}, {"name": "Fit", "desc": "[1/6.7]? Power-Law fit "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_102_411"}} {"id": "J/ApJS/102/411", "title_cds": "Neutrino Energy Loss in Stellar Interiors. VII", "title_create": "Itoh+ 1996", "year": "1996", "author": "Itoh N., Hayashi H., Nishikawa A., Kohyama Y.", "title_pub": "Neutrino Energy Loss in Stellar Interiors. VII. Pair, Photo-, Plasma, Bremsstrahlung, and Recombination Neutrino Processes.", "first_author": "Itoh N.", "ref_biblio": [""], "bibcode": ["1996ApJS..102..411I\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "dense matter - elementary particles - methods: numerical - radiation mechanisms: nonthermal - stars: interiors", "abstract": ["The results of the calculations of the neutrino energy-loss rates", "resulting from pair, photo-, plasma, bremsstrahlung, and recombination", "processes are summarized in the form of analytic fitting formulae and", "tables. Care has been taken in order to serve the convenience of the", "users of these results. We have tried to make the present paper as", "self-contained as possible. The contents of the present paper are", "intended to serve as useful physical input data for stellar evolution", "computations. We intend to publish the numerical data and the FORTRAN", "codes for the results of the neutrino energy-loss rates in the CD-ROM", "series of the American Astronomical Society. In the CD-ROM, we intend", "to give three options for the FORTRAN codes. The first option", "comprises the results with analytic fitting formulae only. The", "second option comprises the results with analytic fitting formulae for", "the bremsstrahlung and recombination neutrino processes, and the", "numerical tables for the pair, photo- and plasma neutrino processes", "with a standard quadratic interpolation procedure. In this option,", "the grid of log T for the pair neutrino energy-loss rate is 0.2. The", "third option is a variant of the second option, with the replacement", "of the grid of log T for the pair neutrino energy-loss rate to be", "0.05."], "description": ["The contents of the directories listed below are adequately described", "by the author-supplied documentation, and the manuscript for the paper", "accepted by the Astrophysical Journal Supplement Series. The", "following is directly from the file 'content.doc' supplied by the", "authors."], "curator": "Lee Brotzman [ADS]", "doi_pub": ["10.1086/192264"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_107_175"}} {"id": "J/ApJS/107/175", "title_cds": "Steep-spectrum radio galaxies VLA imaging", "title_create": "Rhee+, 1996", "year": "1996", "author": "Rhee G., Marvel K., Wilson T., Roland J., Bremer M., Jackson N., Webb J.", "title_pub": "VLA imaging of a sample of steep-spectrum radio galaxies.", "first_author": "Rhee G.", "ref_biblio": [""], "bibcode": ["1996ApJS..107..175R\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/192359"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_107_312"}} {"id": "J/ApJS/107/312", "title_cds": "Ordinary Cool Stars in K Band", "title_create": "Wallace+ 1996", "year": "1996", "author": "Wallace L., Hinkle K.", "title_pub": "High Resolution Spectra of Ordinary Cool Stars in the K Band", "first_author": "Wallace L.", "ref_biblio": [""], "bibcode": ["1996ApJS..107..312W"], "keyword_cds": "Stars, late-type ; Spectra, infrared ; Atlases", "keyword_pub": "atlases - infrared: stars - line: identification - stars: late-type", "abstract": ["We present an atlas of high-resolution (R>=45,000) 2.02-2.41um spectra", "of 12 representative stars, a sunspot, three Mira variables, and a", "carbon star. The star sample, MK spectral types from about early-G to", "about mid-M, with luminosity classes dwarf to supergiant. The Mira", "variables are one each of M, S, and C types. All of the spectra have", "been corrected for atmospheric absorption and have the major spectral", "features labeled with responsible absorbers. Spectra and line lists", "are also available on the AAS CD-ROM series Vol. 7. (ApJS, 106, 165)", "The 2.0-2.4 um region includes molecular vibration-rotation", "transitions from the CO first overtone, HF fundamental, and several", "bands of H2O as well as the CN red system, an electronic transition.", "The relative contribution of H2O versus CN in cool star spectra is", "discussed. Atomic features include clean measurable lines of H, C, Na,", "Mg, Al, Si, S, Ca, Sc, Ti, V, and Fe. We discuss temperature and", "luminosity spectral indicators and the effects of blending on these", "indicators at lower spectral resolution."], "doi_pub": ["10.1086/192367"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "tablea1.dat", "desc": "Atomic features ", "columns": [{"name": "Atom", "desc": "Atom designation "}, {"name": "Freq", "desc": "Frequency "}]}, {"name": "tablea2.dat", "desc": "Molecular features ", "columns": [{"name": "band", "desc": "Band designation "}, {"name": "Freq", "desc": "Frequency "}, {"name": "Trans", "desc": "Rotational transition "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_120_335"}} {"id": "J/ApJS/120/335", "title_cds": "Gamma-ray source catalog", "title_create": "Macomb+, 1999", "year": "1999", "author": "Macomb D.J., Gehrels N.", "title_pub": "A general gamma-ray source catalog.", "first_author": "Macomb D.J.", "ref_biblio": [""], "bibcode": ["1999ApJS..120..335M"], "see_also": ["J/ApJS/101/259 : The second EGRET catalog (Thompson+ 1995)", "J/ApJS/107/227 : Supplement to Second EGRET Catalog (Thompson+ 1996)", "J/ApJS/123/79 : Third EGRET catalog (3EG) (Hartman+, 1999)"], "keyword_cds": "Gamma rays", "keyword_pub": "catalog - gamma rays: observations", "abstract": ["The past several years have seen unprecedented growth in the field of", "gamma-ray astronomy. Highly successful missions such as the Compton", "Gamma-Ray Observatory (CGRO) have led to both a great increase in the", "number of detected gamma-ray sources and a more fundamental", "understanding of the basic physical processes involved for those", "sources. New ground-based observatories, the Rossi X-Ray Timing", "Explorer (RXTE), and the SIGMA instrument aboard the GRANAT spacecraft", "have all contributed to this explosion. Detailed observations of", "active galaxies, pulsars, accreting binaries, and diffuse emission", "have had a tremendous impact on our view of the universe. Given that", "new experiments that will provide a similar increase in source numbers", "are several years away, it is a good time to take inventory of the", "state of gamma-ray astronomy. To this end, we have developed a general", "gamma-ray point-source catalog containing 309 objects that summarize", "the field. Gamma-ray astronomy, as we define it, includes photon", "energies from 50 keV to about 1 TeV. While many catalogs concentrate", "on a single type of astronomical object and/or a very restricted", "energy range, the nature of this catalog is somewhat different. The", "large variety of objects and the many orders of magnitude in energy", "space covered by gamma-ray astronomy presents an organizational", "challenge. We focus on two main types of information: a general", "listing of the basic characteristics of each source, and detailed", "tables of a representative sample of high-energy observations. We also", "summarize the gamma-ray instruments whose observations are included in", "the catalog."], "doi_pub": ["10.1086/313182"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1a.dat", "desc": "Gamma-Ray Source Summary ", "columns": [{"name": "Name", "desc": "Source Name "}, {"name": "Type", "desc": "Source type "}, {"name": "GLON", "desc": "Galactic position "}, {"name": "GLAT", "desc": "Galactic position "}, {"name": "RAdeg", "desc": "Celestial position (2000) "}, {"name": "DEdeg", "desc": "Celestial position (2000) "}, {"name": "Dist1", "desc": "? Lower range in distance (galactic sources) "}, {"name": "n_Dist1", "desc": "[-] Indicates an interval of distances "}, {"name": "Dist2", "desc": "? Upper range in distance (galactic sources) "}, {"name": "z", "desc": "? Redshift (extragalactic sources) "}, {"name": "Energy", "desc": "Energy ranges "}, {"name": "Names", "desc": "Alternate Names "}]}, {"name": "table1b.dat", "desc": "Gamma-Ray Source, General informations ", "columns": [{"name": "Name", "desc": "Source name "}, {"name": "Com", "desc": "Comments "}]}, {"name": "table2.dat", "desc": "Source observations ", "columns": [{"name": "Type", "desc": "[A-G] Type of source (G1) "}, {"name": "Name", "desc": "Most common name for the source in the gamma-ray literature"}, {"name": "n_Name", "desc": "[*] when 2 entries for the same observation "}, {"name": "Inst", "desc": "Name of the experiment whose results are described by the current row"}, {"name": "E1", "desc": "Lower energy limit (1) "}, {"name": "E2", "desc": "? Upper energy limit (1) "}, {"name": "l_E2", "desc": "[L] for the observation of a line "}, {"name": "l_Flux", "desc": "limit flag on Flux "}, {"name": "Flux", "desc": "? Flux , over the energy range E1 - E2 (2) "}, {"name": "e_Flux", "desc": "? rms uncertainty on Flux "}, {"name": "f_Flux", "desc": "[)] When fluxes within (...) "}, {"name": "n_Flux", "desc": "Various notes on Flux (units, range,...) (3) "}, {"name": "Norm", "desc": "? Normalisation constant in spectral fit "}, {"name": "e_Norm", "desc": "? rms uncertainty on Normalisation "}, {"name": "f_Norm", "desc": "[)] When Norm within (...) "}, {"name": "n_Norm", "desc": "Various notes on Normalisation "}, {"name": "l_Index", "desc": "Limit flag on Index "}, {"name": "Index", "desc": "? spectral form (4) "}, {"name": "e_Index", "desc": "? rms uncertainty on Index "}, {"name": "f_Index", "desc": "[)] When Index within (...) "}, {"name": "n2_Index", "desc": "[o] when Index is the temperature in keV "}, {"name": "n_Index", "desc": "Notes about the spectral form "}, {"name": "E0", "desc": "? Energy at which the normalization is evaluated"}, {"name": "n_E0", "desc": "Second value of E0 "}, {"name": "Date", "desc": "Calendar dates for the observations. (5) "}, {"name": "r_Name", "desc": "At least, one reference for the observation in question (see \"refs.dat\" file)"}]}, {"name": "refs.dat", "desc": "References to table2.dat ", "columns": [{"name": "Ref", "desc": "Reference number "}, {"name": "Bibcode", "desc": "Simbad bibcode "}, {"name": "Aut", "desc": "Author's names "}, {"name": "Com", "desc": "Comments "}]}, {"name": "table3.dat", "desc": "Observation notes ", "columns": [{"name": "Type", "desc": "[A-G] Type (G1) "}, {"name": "Name", "desc": "Source name "}, {"name": "Inst", "desc": "Name of the experiment "}, {"name": "Notes", "desc": "Text of the note "}]}, {"name": "table4.dat", "desc": "Gamma-ray instruments ", "columns": [{"name": "Inst", "desc": "Name of the experiment "}, {"name": "n_Inst", "desc": "Note on Inst "}, {"name": "TypeInst", "desc": "A brief description of the instrument type, based upon the nature of the photon detection mechanism"}, {"name": "Energy", "desc": "Usually the stated energy range of the experiment in question, independent of the stated energy ranges of the catalog"}, {"name": "Refs", "desc": "One or several pointers to appropriate information"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_121_417"}} {"id": "J/ApJS/121/417", "title_cds": "Compact nuclei in galaxies. I.", "title_create": "Sarajedini+ 1999", "year": "1999", "author": "Sarajedini V.L., Green R.F., Griffiths R.E., Ratnatunga K.", "title_pub": "Compact nuclei in galaxies at moderate redshift. I. Imaging and spectroscopy.", "first_author": "Sarajedini V.L.", "ref_biblio": [""], "bibcode": ["1999ApJS..121..417S"], "see_also": ["http://archive.stsci.edu/mds/mds.cgi : MDS website"], "keyword_cds": "Galaxy catalogs ; Redshifts ; Magnitudes", "keyword_pub": "galaxies: active - galaxies: nuclei - galaxies: starburst - surveys", "mission": "HST", "description": ["In this paper, the first of two for this study, we present the", "selected Hubble Space Telescope imaged galaxies having unresolved", "nuclei and discuss the selection procedure. We also present the", "ground-based spectroscopy for these galaxies as well as the", "photometric redshift predictions for those galaxies without spectra."], "doi_pub": ["10.1086/313199"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "MDS fields ", "columns": [{"name": "MDS", "desc": "Field name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "o_Vmag", "desc": "Number of V exposures "}, {"name": "Vexp", "desc": "Total V exposure time "}, {"name": "o_Imag", "desc": "Number of I exposures "}, {"name": "Iexp", "desc": "Total I exposure time "}, {"name": "Vmag", "desc": "Limiting V integrated galaxy magnitude for fitting galaxies with a three-component model"}, {"name": "Imag", "desc": "Limiting I integrated galaxy magnitude for fitting galaxies with a three-component model"}, {"name": "Ngal", "desc": "Number of galaxies in the I image above this limiting magnitude"}, {"name": "Note", "desc": "[a] Note "}]}, {"name": "table2.dat", "desc": "Model parameters for galaxies containing unresolved nuclei", "columns": [{"name": "ID", "desc": "Identification number "}, {"name": "Name", "desc": "Object name "}, {"name": "Imag", "desc": "I magnitude of the galaxy model "}, {"name": "e_Imag", "desc": "rms uncertainty on Imag "}, {"name": "log(hlr)", "desc": "log of the I filter half-light radius "}, {"name": "e_log(hlr)", "desc": "rms uncertainty on log(hlr) "}, {"name": "V-I", "desc": "V-I galaxy colour index "}, {"name": "e_V-I", "desc": "rms uncertainty on V-I "}, {"name": "B/TI", "desc": "I bulge-to-total measurement "}, {"name": "P/TI", "desc": "I point-source-to-total measurement "}, {"name": "P/TV", "desc": "V point-source-to-total measurement "}, {"name": "V-Ip", "desc": "? V-I colour index of the point source "}, {"name": "e_V-Ip", "desc": "? rms uncertainty on V-Ip "}]}, {"name": "table4.dat", "desc": "Redshift list ", "columns": [{"name": "ID", "desc": "Identification number "}, {"name": "Name", "desc": "Object name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "z", "desc": "Redshift "}, {"name": "u_z", "desc": "[? ] Uncertainty flag on z "}, {"name": "e_z", "desc": "? rms uncertainty on z "}, {"name": "Note", "desc": "[*12] Notes (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_125_35"}} {"id": "J/ApJS/125/35", "title_cds": "ACO clusters redshifts and velocity dispersions", "title_create": "Struble+ 1999", "year": "1999", "author": "Struble M.F., Rood H.J.", "title_pub": "A compilation of redshifts and velocity dispersions for ACO clusters.", "first_author": "Struble M.F.", "ref_biblio": [""], "bibcode": ["1999ApJS..125...35S"], "see_also": ["VII/4 : Abell and Zwicky Clusters of Galaxies (Abell+ 1974)", "VII/110 : Rich Clusters of Galaxies (Abell+ 1989)", "VII/56 : Redshifts for Abell Clusters (Sarazin+ 1982)", "VII/177 : Redshifts and Vel Dispersions for Abell Clusters (Struble+, 1991)"], "keyword_cds": "Clusters, galaxy ; Redshifts ; Velocity dispersion", "keyword_pub": "galaxies: clusters: general - galaxies: distances and redshifts", "abstract": ["We present a compilation of redshifts for 1572 Abell, Corwin, & Olowin", "(ACO, 1989, Cat. ) clusters, referenced to both the", "heliocentric and cosmic background radiation reference frames, and 395", "velocity dispersions corrected to the reference frame of the cluster,", "available from the literature as of 1998 December. We present an", "additional list of 81 ACO clusters with published redshifts which are", "probably those of galaxies or groups superimposed on, or near, the ACO", "cluster position."], "doi_pub": ["10.1086/313274"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Redshifts and velocity dispersions for ACO clusters", "columns": [{"name": "ACO", "desc": "ACO number "}, {"name": "n_ACO", "desc": "[*] *: membership in Abell's (1958, See Cat. ) nonstatistical sample"}, {"name": "zh", "desc": "Adopted heliocentric redshift "}, {"name": "u_zh", "desc": "Uncertainty flag on zh "}, {"name": "a", "desc": "? [2-3] Flag indicating the accuracy of z_h_ in the original references (1)"}, {"name": "zC", "desc": "Redshift with respect to the cosmic background radiation (2)"}, {"name": "l_Nz", "desc": "Limit flag on Nz "}, {"name": "Nz", "desc": "Number of cluster members with published redshift (3)"}, {"name": "sigma", "desc": "? Adopted velocity dispersion in the rest frame of the cluster"}, {"name": "Ref", "desc": "References for redshift and radial velocity (4) "}, {"name": "Note", "desc": "[0nN] Note on comments (5) "}]}, {"name": "table2.dat", "desc": "New and Revised Notes to Table 1 ", "columns": [{"name": "ACO", "desc": "Cluster number "}, {"name": "Note", "desc": "Text of the note (1) "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference number "}, {"name": "BibCode", "desc": "BibCode "}, {"name": "Aut", "desc": "Author's name "}, {"name": "Com", "desc": "Comments "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_130_37"}} {"id": "J/ApJS/130/37", "title_cds": "Analysis of the Ly{alpha} forest at z=0-5. I.", "title_create": "Scott+ 2000", "year": "2000", "author": "Scott J., Bechtold J., Dobrzycki A.", "title_pub": "A uniform analysis of the Ly{alpha} forest at z=0-5. I. The sample and distribution of clouds at z>1.7.", "first_author": "Scott J.", "ref_biblio": [""], "bibcode": ["2000ApJS..130...37S\t(SIMBAD/NED"], "see_also": ["http://lithops.as.arizona.edu/~jill/QuasarSpectra/"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/317339"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_139_199"}} {"id": "J/ApJS/139/199", "title_cds": "Catalog of distances of planetary nebulae", "title_create": "Phillips, 2002", "year": "2002", "author": "Phillips J.P.", "title_pub": "The distances of planetary nebulae: a scale based upon nearby sources.", "first_author": "Phillips J.P.", "ref_biblio": [""], "bibcode": ["2002ApJS..139..199P"], "see_also": ["V/84 : Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker+, 1992)", "IV/24 : Catalogue of Galactic Planetary Nebulae (Kohoutek, 2001)"], "keyword_cds": "Planetary nebulae ; Stars, distances", "keyword_pub": "catalogs - planetary nebulae: general", "description": ["We present a database of standard sources that is as complete as", "possible, and that samples the broadest possible range of nebular", "surface brightnesses and radii.", "We have therefore, in order to achieve this, compiled a list of", "sources having distances D <=1.0 sec b kpc, where b is Galactic", "latitude; that is, of sources located within a cylinder of radius", "R_C_=1kpc, centered upon the Sun. This list is presented in", "table1.dat", "A table of standards having well-defined distances, D>1.0 sec b kpc,", "is given in table2.dat", "We have compared the distances obtained here, and summarized in", "table3.dat, with those of Zhang (1995, Cat. ),", "Cahn et al. (1992A&AS...94..399C), van de Steene & Zijlstra", "(1995A&A...293..541V), and Daub (1982ApJ...260..612D)"], "doi_pub": ["10.1086/338028"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Distances and Emission Characteristics of Nearby Reference Nebulae", "columns": [{"name": "Name", "desc": "Planetary nebula name "}, {"name": "n_Name", "desc": "[*] Note on Name (1) "}, {"name": "GC", "desc": "Galactic coordinates (2) "}, {"name": "Dist", "desc": "Distance "}, {"name": "Rad", "desc": "? Radius "}, {"name": "Tb", "desc": "? 5GHz brightness temperature "}, {"name": "r_Dist", "desc": "Reference code for distance, separated by comma in refs.dat file"}, {"name": "Method", "desc": "Method used "}]}, {"name": "table2.dat", "desc": "Distances and Emission Characteristics of Distant Reference Nebulae", "columns": [{"name": "Name", "desc": "Planetary nebula name "}, {"name": "n_Name", "desc": "[*] Note on Name (1) "}, {"name": "GC", "desc": "Galactic coordinates (2) "}, {"name": "Dist", "desc": "Distance "}, {"name": "Rad", "desc": "? Radius "}, {"name": "Tb", "desc": "? 5GHz brightness temperature "}, {"name": "r_Dist", "desc": "Reference code for distance, separated by comma in refs.dat file"}, {"name": "Method", "desc": "Method used "}]}, {"name": "refs.dat", "desc": "References for tables 1 and 2 ", "columns": [{"name": "Ref", "desc": "Reference code "}, {"name": "BibCode", "desc": "BibCode "}, {"name": "Aut", "desc": "Author's name "}, {"name": "Com", "desc": "Comments "}]}, {"name": "table3.dat", "desc": "Statistical Distances to Planetary Nebula ", "columns": [{"name": "Name", "desc": "Planetary nebula name "}, {"name": "n_Name", "desc": "[*W] Note on Name "}, {"name": "PK", "desc": "PK designation (1) "}, {"name": "n_PK", "desc": "[*] Note on PK (2) "}, {"name": "theta", "desc": "Angular radius of the source "}, {"name": "Tb", "desc": "5GHz brightness temperature "}, {"name": "Dist", "desc": "Distance "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_181_o129"}} {"id": "J/ApJS/181/129", "title_cds": "QUEST1 variability survey (QVS). III.", "title_create": "Rengstorf+, 2009", "year": "2009", "author": "Rengstorf A.W., Thompson D.L., Mufson S.L., Andrews P., Honeycutt R.K., Vivas A.K., Abad C., Adams B., Bailyn C., Baltay C., Bongiovanni A., Briceno C., Bruzual G., Coppi P., Della Prugna F., Emmet W., Ferrin I., Fuenmayor F., Gebhard M., Hernandez J., Magris G., Musser J., Naranjo O., Oemler A., Rosenzweig P., Sabbey C.N., Sanchez Ge., Sanchez Gu., Schaefer B., Schenner H., Sinnott J., Snyder J.A., Sofia S., Stock J., Van Altena W.", "title_pub": "QUEST1 Variability Survey. III: Light Curve Catalog Update", "first_author": "Rengstorf A.W.", "ref_biblio": [""], "bibcode": ["2009ApJS..181..129R"], "see_also": ["II/266 : QUEST1 200k light curve catalog (Rengstorf+, 2004)", "J/AJ/127/1158 : QUEST RR Lyrae Survey first catalog (Vivas+, 2004)", "J/AJ/131/1923 : Known quasars in QUEST Variability Survey (Rengstorf+, 2006)", "J/AJ/132/714 : QUEST RR Lyrae survey. II. Halo overdensities (Vivas+, 2006)"], "keyword_cds": "Surveys ; Photometry ; Stars, variable", "keyword_pub": "catalogs - methods: data analysis - surveys", "abstract": ["This paper reports an update to the QUEST1 (QUasar Equatorial Survey", "Team, Phase 1) Variability Survey (QVS) light curve catalog, which", "links QVS instrumental Light curve magnitude at jdlight curves to", "Sloan Digital Sky Survey (SDSS) objects and photometry. In the time", "since the original QVS catalog release, the overlap between publicly", "available SDSS data and QVS data has increased by 8% in sky coverage", "and 16728 in number of matched objects. The astrometric matching and", "the treatment of SDSS masks have been refined for the updated catalog.", "We report on these improvements and present multiple bandpass light", "curves, global variability information, and matched SDSS photometry", "for 214941 QUEST1 objects."], "description": ["QUEST1 constructed a 16-chip CCD camera to be used on the 1m Schmidt", "telescope at the Llano del Hato National Astronomical Observatory in", "Venezuela. Normally operated in the drift-scan mode, an equatorial", "scan will expose any point on the sky for 143s and result in limiting", "magnitudes of B=18.5, V=19.2, and R=19.5 at S/N=10. These data were", "collected between 1999 February and 2001 April."], "date_update": "24-Oct-2022", "tables": [{"name": "catalog.dat", "desc": "QVS Light Curve Catalog, version 2: Main Table ", "columns": [{"name": "QVS2", "desc": "[1/214941] Unique Running Identifier "}, {"name": "QUEST", "desc": "QUEST Identifier (JHHMMSS.s+DDMMSS.s) "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "GCL", "desc": "Global confidence level (GCL) for variability "}, {"name": "N1", "desc": "Number of data points in r1 light curve "}, {"name": "N2", "desc": "Number of data points in b light curve "}, {"name": "N3", "desc": "Number of data points in r3 light curve "}, {"name": "N4", "desc": "Number of data points in v light curve "}, {"name": "ObjID", "desc": "SDSS DR6 Object ID String "}, {"name": "umag", "desc": "?=00.0 SDSS DR6 u band model magnitude "}, {"name": "gmag", "desc": "?=00.0 SDSS DR6 g band model magnitude "}, {"name": "rmag", "desc": "?=00.0 SDSS DR6 r band model magnitude "}, {"name": "imag", "desc": "?=00.0 SDSS DR6 i band model magnitude "}, {"name": "zmag", "desc": "?=00.0 SDSS DR6 z band model magnitude "}]}, {"name": "bmaglc.dat", "desc": "b band light curves ", "columns": [{"name": "QVS2", "desc": "Unique Running Identifier "}, {"name": "JD01", "desc": "Date of observation 1; JD-2451224.0 "}, {"name": "mag1", "desc": "Light curve magnitude at JD1 "}, {"name": "e_mag1", "desc": "rms uncertainty on mag1 "}, {"name": "JD2", "desc": "Date of observation 2; JD-2451224.0 "}, {"name": "mag2", "desc": "Light curve magnitude at JD2 "}, {"name": "e_mag2", "desc": "rms uncertainty on mag2 "}, {"name": "JD3", "desc": "Date of observation 3; JD-2451224.0 "}, {"name": "mag3", "desc": "Light curve magnitude at JD3 "}, {"name": "e_mag3", "desc": "rms uncertainty on mag3 "}, {"name": "JD4", "desc": "? Date of observation 4; JD-2451224.0 "}, {"name": "mag4", "desc": "? Light curve magnitude at JD4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "JD5", "desc": "? Date of observation 5; JD-2451224.0 "}, {"name": "mag5", "desc": "? Light curve magnitude at JD5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "JD6", "desc": "? Date of observation 6; JD-2451224.0 "}, {"name": "mag6", "desc": "? Light curve magnitude at JD6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "JD7", "desc": "? Date of observation 7; JD-2451224.0 "}, {"name": "mag7", "desc": "? Light curve magnitude at JD7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "JD8", "desc": "? Date of observation 8; JD-2451224.0 "}, {"name": "mag8", "desc": "? Light curve magnitude at JD8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "JD9", "desc": "? Date of observation 9; JD-2451224.0 "}, {"name": "mag9", "desc": "? Light curve magnitude at JD9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "JD10", "desc": "? Date of observation 10; JD-2451224.0 "}, {"name": "mag10", "desc": "? Light curve magnitude at JD10 "}, {"name": "e_mag10", "desc": "? rms uncertainty on mag10 "}, {"name": "JD11", "desc": "? Date of observation 11; JD-2451224.0 "}, {"name": "mag11", "desc": "? Light curve magnitude at JD11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}, {"name": "JD12", "desc": "? Date of observation 12; JD-2451224.0 "}, {"name": "mag12", "desc": "? Light curve magnitude at JD12 "}, {"name": "e_mag12", "desc": "? rms uncertainty on mag12 "}, {"name": "JD13", "desc": "? Date of observation 13; JD-2451224.0 "}, {"name": "mag13", "desc": "? Light curve magnitude at JD13 "}, {"name": "e_mag13", "desc": "? rms uncertainty on mag13 "}, {"name": "JD14", "desc": "? Date of observation 14; JD-2451224.0 "}, {"name": "mag14", "desc": "? Light curve magnitude at JD14 "}, {"name": "e_mag14", "desc": "? rms uncertainty on mag14 "}, {"name": "JD15", "desc": "? Date of observation 15; JD-2451224.0 "}, {"name": "mag15", "desc": "? Light curve magnitude at JD15 "}, {"name": "e_mag15", "desc": "? rms uncertainty on mag15 "}, {"name": "JD16", "desc": "? Date of observation 16; JD-2451224.0 "}, {"name": "mag16", "desc": "? Light curve magnitude at JD16 "}, {"name": "e_mag16", "desc": "? rms uncertainty on mag16 "}, {"name": "JD17", "desc": "? Date of observation 17; JD-2451224.0 "}, {"name": "mag17", "desc": "? Light curve magnitude at JD17 "}, {"name": "e_mag17", "desc": "? rms uncertainty on mag17 "}, {"name": "JD18", "desc": "? Date of observation 18; JD-2451224.0 "}, {"name": "mag18", "desc": "? Light curve magnitude at JD18 "}, {"name": "e_mag18", "desc": "? rms uncertainty on mag18 "}, {"name": "JD19", "desc": "? Date of observation 19; JD-2451224.0 "}, {"name": "mag19", "desc": "? Light curve magnitude at JD19 "}, {"name": "e_mag19", "desc": "? rms uncertainty on mag19 "}, {"name": "JD20", "desc": "? Date of observation 20; JD-2451224.0 "}, {"name": "mag20", "desc": "? Light curve magnitude at JD20 "}, {"name": "e_mag20", "desc": "? rms uncertainty on mag20 "}, {"name": "JD21", "desc": "? Date of observation 21; JD-2451224.0 "}, {"name": "mag21", "desc": "? Light curve magnitude at JD21 "}, {"name": "e_mag21", "desc": "? rms uncertainty on mag21 "}, {"name": "JD22", "desc": "? Date of observation 22; JD-2451224.0 "}, {"name": "mag22", "desc": "? Light curve magnitude at JD22 "}, {"name": "e_mag22", "desc": "? rms uncertainty on mag22 "}, {"name": "JD23", "desc": "? Date of observation 23; JD-2451224.0 "}, {"name": "mag23", "desc": "? Light curve magnitude at JD23 "}, {"name": "e_mag23", "desc": "? rms uncertainty on mag23 "}, {"name": "JD24", "desc": "? Date of observation 24; JD-2451224.0 "}, {"name": "mag24", "desc": "? Light curve magnitude at JD24 "}, {"name": "e_mag24", "desc": "? rms uncertainty on mag24 "}, {"name": "JD25", "desc": "? Date of observation 25; JD-2451224.0 "}, {"name": "mag25", "desc": "? Light curve magnitude at JD25 "}, {"name": "e_mag25", "desc": "? rms uncertainty on mag25 "}, {"name": "JD26", "desc": "? Date of observation 26; JD-2451224.0 "}, {"name": "mag26", "desc": "? Light curve magnitude at JD26 "}, {"name": "e_mag26", "desc": "? rms uncertainty on mag26 "}, {"name": "JD27", "desc": "? Date of observation 27; JD-2451224.0 "}, {"name": "mag27", "desc": "? Light curve magnitude at JD27 "}, {"name": "e_mag27", "desc": "? rms uncertainty on mag27 "}, {"name": "JD28", "desc": "? Date of observation 28; JD-2451224.0 "}, {"name": "mag28", "desc": "? Light curve magnitude at JD28 "}, {"name": "e_mag28", "desc": "? rms uncertainty on mag28 "}, {"name": "JD29", "desc": "? Date of observation 29; JD-2451224.0 "}, {"name": "mag29", "desc": "? Light curve magnitude at JD29 "}, {"name": "e_mag29", "desc": "? rms uncertainty on mag29 "}, {"name": "JD30", "desc": "? Date of observation 30; JD-2451224.0 "}, {"name": "mag30", "desc": "? Light curve magnitude at JD30 "}, {"name": "e_mag30", "desc": "? rms uncertainty on mag30 "}, {"name": "JD31", "desc": "? Date of observation 31; JD-2451224.0 "}, {"name": "mag31", "desc": "? Light curve magnitude at JD31 "}, {"name": "e_mag31", "desc": "? rms uncertainty on mag31 "}, {"name": "JD32", "desc": "? Date of observation 32; JD-2451224.0 "}, {"name": "mag32", "desc": "? Light curve magnitude at JD32 "}, {"name": "e_mag32", "desc": "? rms uncertainty on mag32 "}, {"name": "JD33", "desc": "? Date of observation 33; JD-2451224.0 "}, {"name": "mag33", "desc": "? Light curve magnitude at JD33 "}, {"name": "e_mag33", "desc": "? rms uncertainty on mag33 "}, {"name": "JD34", "desc": "? Date of observation 34; JD-2451224.0 "}, {"name": "mag34", "desc": "? Light curve magnitude at JD34 "}, {"name": "e_mag34", "desc": "? rms uncertainty on mag34 "}, {"name": "JD35", "desc": "? Date of observation 35; JD-2451224.0 "}, {"name": "mag35", "desc": "? Light curve magnitude at JD35 "}, {"name": "e_mag35", "desc": "? rms uncertainty on mag35 "}, {"name": "JD36", "desc": "? Date of observation 36; JD-2451224.0 "}, {"name": "mag36", "desc": "? Light curve magnitude at JD36 "}, {"name": "e_mag36", "desc": "? rms uncertainty on mag36 "}, {"name": "JD37", "desc": "? Date of observation 37; JD-2451224.0 "}, {"name": "mag37", "desc": "? Light curve magnitude at JD37 "}, {"name": "e_mag37", "desc": "? rms uncertainty on mag37 "}, {"name": "JD38", "desc": "? Date of observation 38; JD-2451224.0 "}, {"name": "mag38", "desc": "? Light curve magnitude at JD38 "}, {"name": "e_mag38", "desc": "? rms uncertainty on mag38 "}, {"name": "JD39", "desc": "? Date of observation 39; JD-2451224.0 "}, {"name": "mag39", "desc": "? Light curve magnitude at JD39 "}, {"name": "e_mag39", "desc": "? rms uncertainty on mag39 "}, {"name": "JD40", "desc": "? Date of observation 40; JD-2451224.0 "}, {"name": "mag40", "desc": "? Light curve magnitude at JD40 "}, {"name": "e_mag40", "desc": "? rms uncertainty on mag40 "}, {"name": "JD41", "desc": "? Date of observation 41; JD-2451224.0 "}, {"name": "mag41", "desc": "? Light curve magnitude at JD41 "}, {"name": "e_mag41", "desc": "? rms uncertainty on mag41 "}, {"name": "JD42", "desc": "? Date of observation 42; JD-2451224.0 "}, {"name": "mag42", "desc": "? Light curve magnitude at JD42 "}, {"name": "e_mag42", "desc": "? rms uncertainty on mag42 "}, {"name": "JD43", "desc": "? Date of observation 43; JD-2451224.0 "}, {"name": "mag43", "desc": "? Light curve magnitude at JD43 "}, {"name": "e_mag43", "desc": "? rms uncertainty on mag43 "}]}, {"name": "r1maglc.dat", "desc": "r1 band light curves ", "columns": [{"name": "QVS2", "desc": "Unique Running Identifier "}, {"name": "JD01", "desc": "Date of observation 1; JD-2451224.0 "}, {"name": "mag1", "desc": "Light curve magnitude at JD1 "}, {"name": "e_mag1", "desc": "rms uncertainty on mag1 "}, {"name": "JD2", "desc": "Date of observation 2; JD-2451224.0 "}, {"name": "mag2", "desc": "Light curve magnitude at JD2 "}, {"name": "e_mag2", "desc": "rms uncertainty on mag2 "}, {"name": "JD3", "desc": "Date of observation 3; JD-2451224.0 "}, {"name": "mag3", "desc": "Light curve magnitude at JD3 "}, {"name": "e_mag3", "desc": "rms uncertainty on mag3 "}, {"name": "JD4", "desc": "? Date of observation 4; JD-2451224.0 "}, {"name": "mag4", "desc": "? Light curve magnitude at JD4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "JD5", "desc": "? Date of observation 5; JD-2451224.0 "}, {"name": "mag5", "desc": "? Light curve magnitude at JD5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "JD6", "desc": "? Date of observation 6; JD-2451224.0 "}, {"name": "mag6", "desc": "? Light curve magnitude at JD6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "JD7", "desc": "? Date of observation 7; JD-2451224.0 "}, {"name": "mag7", "desc": "? Light curve magnitude at JD7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "JD8", "desc": "? Date of observation 8; JD-2451224.0 "}, {"name": "mag8", "desc": "? Light curve magnitude at JD8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "JD9", "desc": "? Date of observation 9; JD-2451224.0 "}, {"name": "mag9", "desc": "? Light curve magnitude at JD9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "JD10", "desc": "? Date of observation 10; JD-2451224.0 "}, {"name": "mag10", "desc": "? Light curve magnitude at JD10 "}, {"name": "e_mag10", "desc": "? rms uncertainty on mag10 "}, {"name": "JD11", "desc": "? Date of observation 11; JD-2451224.0 "}, {"name": "mag11", "desc": "? Light curve magnitude at JD11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}, {"name": "JD12", "desc": "? Date of observation 12; JD-2451224.0 "}, {"name": "mag12", "desc": "? Light curve magnitude at JD12 "}, {"name": "e_mag12", "desc": "? rms uncertainty on mag12 "}, {"name": "JD13", "desc": "? Date of observation 13; JD-2451224.0 "}, {"name": "mag13", "desc": "? Light curve magnitude at JD13 "}, {"name": "e_mag13", "desc": "? rms uncertainty on mag13 "}, {"name": "JD14", "desc": "? Date of observation 14; JD-2451224.0 "}, {"name": "mag14", "desc": "? Light curve magnitude at JD14 "}, {"name": "e_mag14", "desc": "? rms uncertainty on mag14 "}, {"name": "JD15", "desc": "? Date of observation 15; JD-2451224.0 "}, {"name": "mag15", "desc": "? Light curve magnitude at JD15 "}, {"name": "e_mag15", "desc": "? rms uncertainty on mag15 "}, {"name": "JD16", "desc": "? Date of observation 16; JD-2451224.0 "}, {"name": "mag16", "desc": "? Light curve magnitude at JD16 "}, {"name": "e_mag16", "desc": "? rms uncertainty on mag16 "}, {"name": "JD17", "desc": "? Date of observation 17; JD-2451224.0 "}, {"name": "mag17", "desc": "? Light curve magnitude at JD17 "}, {"name": "e_mag17", "desc": "? rms uncertainty on mag17 "}, {"name": "JD18", "desc": "? Date of observation 18; JD-2451224.0 "}, {"name": "mag18", "desc": "? Light curve magnitude at JD18 "}, {"name": "e_mag18", "desc": "? rms uncertainty on mag18 "}, {"name": "JD19", "desc": "? Date of observation 19; JD-2451224.0 "}, {"name": "mag19", "desc": "? Light curve magnitude at JD19 "}, {"name": "e_mag19", "desc": "? rms uncertainty on mag19 "}, {"name": "JD20", "desc": "? Date of observation 20; JD-2451224.0 "}, {"name": "mag20", "desc": "? Light curve magnitude at JD20 "}, {"name": "e_mag20", "desc": "? rms uncertainty on mag20 "}, {"name": "JD21", "desc": "? Date of observation 21; JD-2451224.0 "}, {"name": "mag21", "desc": "? Light curve magnitude at JD21 "}, {"name": "e_mag21", "desc": "? rms uncertainty on mag21 "}, {"name": "JD22", "desc": "? Date of observation 22; JD-2451224.0 "}, {"name": "mag22", "desc": "? Light curve magnitude at JD22 "}, {"name": "e_mag22", "desc": "? rms uncertainty on mag22 "}, {"name": "JD23", "desc": "? Date of observation 23; JD-2451224.0 "}, {"name": "mag23", "desc": "? Light curve magnitude at JD23 "}, {"name": "e_mag23", "desc": "? rms uncertainty on mag23 "}, {"name": "JD24", "desc": "? Date of observation 24; JD-2451224.0 "}, {"name": "mag24", "desc": "? Light curve magnitude at JD24 "}, {"name": "e_mag24", "desc": "? rms uncertainty on mag24 "}, {"name": "JD25", "desc": "? Date of observation 25; JD-2451224.0 "}, {"name": "mag25", "desc": "? Light curve magnitude at JD25 "}, {"name": "e_mag25", "desc": "? rms uncertainty on mag25 "}, {"name": "JD26", "desc": "? Date of observation 26; JD-2451224.0 "}, {"name": "mag26", "desc": "? Light curve magnitude at JD26 "}, {"name": "e_mag26", "desc": "? rms uncertainty on mag26 "}, {"name": "JD27", "desc": "? Date of observation 27; JD-2451224.0 "}, {"name": "mag27", "desc": "? Light curve magnitude at JD27 "}, {"name": "e_mag27", "desc": "? rms uncertainty on mag27 "}, {"name": "JD28", "desc": "? Date of observation 28; JD-2451224.0 "}, {"name": "mag28", "desc": "? Light curve magnitude at JD28 "}, {"name": "e_mag28", "desc": "? rms uncertainty on mag28 "}, {"name": "JD29", "desc": "? Date of observation 29; JD-2451224.0 "}, {"name": "mag29", "desc": "? Light curve magnitude at JD29 "}, {"name": "e_mag29", "desc": "? rms uncertainty on mag29 "}, {"name": "JD30", "desc": "? Date of observation 30; JD-2451224.0 "}, {"name": "mag30", "desc": "? Light curve magnitude at JD30 "}, {"name": "e_mag30", "desc": "? rms uncertainty on mag30 "}, {"name": "JD31", "desc": "? Date of observation 31; JD-2451224.0 "}, {"name": "mag31", "desc": "? Light curve magnitude at JD31 "}, {"name": "e_mag31", "desc": "? rms uncertainty on mag31 "}, {"name": "JD32", "desc": "? Date of observation 32; JD-2451224.0 "}, {"name": "mag32", "desc": "? Light curve magnitude at JD32 "}, {"name": "e_mag32", "desc": "? rms uncertainty on mag32 "}, {"name": "JD33", "desc": "? Date of observation 33; JD-2451224.0 "}, {"name": "mag33", "desc": "? Light curve magnitude at JD33 "}, {"name": "e_mag33", "desc": "? rms uncertainty on mag33 "}, {"name": "JD34", "desc": "? Date of observation 34; JD-2451224.0 "}, {"name": "mag34", "desc": "? Light curve magnitude at JD34 "}, {"name": "e_mag34", "desc": "? rms uncertainty on mag34 "}, {"name": "JD35", "desc": "? Date of observation 35; JD-2451224.0 "}, {"name": "mag35", "desc": "? Light curve magnitude at JD35 "}, {"name": "e_mag35", "desc": "? rms uncertainty on mag35 "}, {"name": "JD36", "desc": "? Date of observation 36; JD-2451224.0 "}, {"name": "mag36", "desc": "? Light curve magnitude at JD36 "}, {"name": "e_mag36", "desc": "? rms uncertainty on mag36 "}, {"name": "JD37", "desc": "? Date of observation 37; JD-2451224.0 "}, {"name": "mag37", "desc": "? Light curve magnitude at JD37 "}, {"name": "e_mag37", "desc": "? rms uncertainty on mag37 "}, {"name": "JD38", "desc": "? Date of observation 38; JD-2451224.0 "}, {"name": "mag38", "desc": "? Light curve magnitude at JD38 "}, {"name": "e_mag38", "desc": "? rms uncertainty on mag38 "}, {"name": "JD39", "desc": "? Date of observation 39; JD-2451224.0 "}, {"name": "mag39", "desc": "? Light curve magnitude at JD39 "}, {"name": "e_mag39", "desc": "? rms uncertainty on mag39 "}, {"name": "JD40", "desc": "? Date of observation 40; JD-2451224.0 "}, {"name": "mag40", "desc": "? Light curve magnitude at JD40 "}, {"name": "e_mag40", "desc": "? rms uncertainty on mag40 "}, {"name": "JD41", "desc": "? Date of observation 41; JD-2451224.0 "}, {"name": "mag41", "desc": "? Light curve magnitude at JD41 "}, {"name": "e_mag41", "desc": "? rms uncertainty on mag41 "}, {"name": "JD42", "desc": "? Date of observation 42; JD-2451224.0 "}, {"name": "mag42", "desc": "? Light curve magnitude at JD42 "}, {"name": "e_mag42", "desc": "? rms uncertainty on mag42 "}, {"name": "JD43", "desc": "? Date of observation 43; JD-2451224.0 "}, {"name": "mag43", "desc": "? Light curve magnitude at JD43 "}, {"name": "e_mag43", "desc": "? rms uncertainty on mag43 "}]}, {"name": "r3maglc.dat", "desc": "r3 band light curves ", "columns": [{"name": "QVS2", "desc": "Unique Running Identifier "}, {"name": "JD01", "desc": "Date of observation 1; JD-2451224.0 "}, {"name": "mag1", "desc": "Light curve magnitude at JD1 "}, {"name": "e_mag1", "desc": "rms uncertainty on mag1 "}, {"name": "JD2", "desc": "Date of observation 2; JD-2451224.0 "}, {"name": "mag2", "desc": "Light curve magnitude at JD2 "}, {"name": "e_mag2", "desc": "rms uncertainty on mag2 "}, {"name": "JD3", "desc": "Date of observation 3; JD-2451224.0 "}, {"name": "mag3", "desc": "Light curve magnitude at JD3 "}, {"name": "e_mag3", "desc": "rms uncertainty on mag3 "}, {"name": "JD4", "desc": "? Date of observation 4; JD-2451224.0 "}, {"name": "mag4", "desc": "? Light curve magnitude at JD4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "JD5", "desc": "? Date of observation 5; JD-2451224.0 "}, {"name": "mag5", "desc": "? Light curve magnitude at JD5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "JD6", "desc": "? Date of observation 6; JD-2451224.0 "}, {"name": "mag6", "desc": "? Light curve magnitude at JD6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "JD7", "desc": "? Date of observation 7; JD-2451224.0 "}, {"name": "mag7", "desc": "? Light curve magnitude at JD7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "JD8", "desc": "? Date of observation 8; JD-2451224.0 "}, {"name": "mag8", "desc": "? Light curve magnitude at JD8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "JD9", "desc": "? Date of observation 9; JD-2451224.0 "}, {"name": "mag9", "desc": "? Light curve magnitude at JD9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "JD10", "desc": "? Date of observation 10; JD-2451224.0 "}, {"name": "mag10", "desc": "? Light curve magnitude at JD10 "}, {"name": "e_mag10", "desc": "? rms uncertainty on mag10 "}, {"name": "JD11", "desc": "? Date of observation 11; JD-2451224.0 "}, {"name": "mag11", "desc": "? Light curve magnitude at JD11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}, {"name": "JD12", "desc": "? Date of observation 12; JD-2451224.0 "}, {"name": "mag12", "desc": "? Light curve magnitude at JD12 "}, {"name": "e_mag12", "desc": "? rms uncertainty on mag12 "}, {"name": "JD13", "desc": "? Date of observation 13; JD-2451224.0 "}, {"name": "mag13", "desc": "? Light curve magnitude at JD13 "}, {"name": "e_mag13", "desc": "? rms uncertainty on mag13 "}, {"name": "JD14", "desc": "? Date of observation 14; JD-2451224.0 "}, {"name": "mag14", "desc": "? Light curve magnitude at JD14 "}, {"name": "e_mag14", "desc": "? rms uncertainty on mag14 "}, {"name": "JD15", "desc": "? Date of observation 15; JD-2451224.0 "}, {"name": "mag15", "desc": "? Light curve magnitude at JD15 "}, {"name": "e_mag15", "desc": "? rms uncertainty on mag15 "}, {"name": "JD16", "desc": "? Date of observation 16; JD-2451224.0 "}, {"name": "mag16", "desc": "? Light curve magnitude at JD16 "}, {"name": "e_mag16", "desc": "? rms uncertainty on mag16 "}, {"name": "JD17", "desc": "? Date of observation 17; JD-2451224.0 "}, {"name": "mag17", "desc": "? Light curve magnitude at JD17 "}, {"name": "e_mag17", "desc": "? rms uncertainty on mag17 "}, {"name": "JD18", "desc": "? Date of observation 18; JD-2451224.0 "}, {"name": "mag18", "desc": "? Light curve magnitude at JD18 "}, {"name": "e_mag18", "desc": "? rms uncertainty on mag18 "}, {"name": "JD19", "desc": "? Date of observation 19; JD-2451224.0 "}, {"name": "mag19", "desc": "? Light curve magnitude at JD19 "}, {"name": "e_mag19", "desc": "? rms uncertainty on mag19 "}, {"name": "JD20", "desc": "? Date of observation 20; JD-2451224.0 "}, {"name": "mag20", "desc": "? Light curve magnitude at JD20 "}, {"name": "e_mag20", "desc": "? rms uncertainty on mag20 "}, {"name": "JD21", "desc": "? Date of observation 21; JD-2451224.0 "}, {"name": "mag21", "desc": "? Light curve magnitude at JD21 "}, {"name": "e_mag21", "desc": "? rms uncertainty on mag21 "}, {"name": "JD22", "desc": "? Date of observation 22; JD-2451224.0 "}, {"name": "mag22", "desc": "? Light curve magnitude at JD22 "}, {"name": "e_mag22", "desc": "? rms uncertainty on mag22 "}, {"name": "JD23", "desc": "? Date of observation 23; JD-2451224.0 "}, {"name": "mag23", "desc": "? Light curve magnitude at JD23 "}, {"name": "e_mag23", "desc": "? rms uncertainty on mag23 "}, {"name": "JD24", "desc": "? Date of observation 24; JD-2451224.0 "}, {"name": "mag24", "desc": "? Light curve magnitude at JD24 "}, {"name": "e_mag24", "desc": "? rms uncertainty on mag24 "}, {"name": "JD25", "desc": "? Date of observation 25; JD-2451224.0 "}, {"name": "mag25", "desc": "? Light curve magnitude at JD25 "}, {"name": "e_mag25", "desc": "? rms uncertainty on mag25 "}, {"name": "JD26", "desc": "? Date of observation 26; JD-2451224.0 "}, {"name": "mag26", "desc": "? Light curve magnitude at JD26 "}, {"name": "e_mag26", "desc": "? rms uncertainty on mag26 "}, {"name": "JD27", "desc": "? Date of observation 27; JD-2451224.0 "}, {"name": "mag27", "desc": "? Light curve magnitude at JD27 "}, {"name": "e_mag27", "desc": "? rms uncertainty on mag27 "}, {"name": "JD28", "desc": "? Date of observation 28; JD-2451224.0 "}, {"name": "mag28", "desc": "? Light curve magnitude at JD28 "}, {"name": "e_mag28", "desc": "? rms uncertainty on mag28 "}, {"name": "JD29", "desc": "? Date of observation 29; JD-2451224.0 "}, {"name": "mag29", "desc": "? Light curve magnitude at JD29 "}, {"name": "e_mag29", "desc": "? rms uncertainty on mag29 "}, {"name": "JD30", "desc": "? Date of observation 30; JD-2451224.0 "}, {"name": "mag30", "desc": "? Light curve magnitude at JD30 "}, {"name": "e_mag30", "desc": "? rms uncertainty on mag30 "}, {"name": "JD31", "desc": "? Date of observation 31; JD-2451224.0 "}, {"name": "mag31", "desc": "? Light curve magnitude at JD31 "}, {"name": "e_mag31", "desc": "? rms uncertainty on mag31 "}, {"name": "JD32", "desc": "? Date of observation 32; JD-2451224.0 "}, {"name": "mag32", "desc": "? Light curve magnitude at JD32 "}, {"name": "e_mag32", "desc": "? rms uncertainty on mag32 "}, {"name": "JD33", "desc": "? Date of observation 33; JD-2451224.0 "}, {"name": "mag33", "desc": "? Light curve magnitude at JD33 "}, {"name": "e_mag33", "desc": "? rms uncertainty on mag33 "}, {"name": "JD34", "desc": "? Date of observation 34; JD-2451224.0 "}, {"name": "mag34", "desc": "? Light curve magnitude at JD34 "}, {"name": "e_mag34", "desc": "? rms uncertainty on mag34 "}, {"name": "JD35", "desc": "? Date of observation 35; JD-2451224.0 "}, {"name": "mag35", "desc": "? Light curve magnitude at JD35 "}, {"name": "e_mag35", "desc": "? rms uncertainty on mag35 "}, {"name": "JD36", "desc": "? Date of observation 36; JD-2451224.0 "}, {"name": "mag36", "desc": "? Light curve magnitude at JD36 "}, {"name": "e_mag36", "desc": "? rms uncertainty on mag36 "}, {"name": "JD37", "desc": "? Date of observation 37; JD-2451224.0 "}, {"name": "mag37", "desc": "? Light curve magnitude at JD37 "}, {"name": "e_mag37", "desc": "? rms uncertainty on mag37 "}, {"name": "JD38", "desc": "? Date of observation 38; JD-2451224.0 "}, {"name": "mag38", "desc": "? Light curve magnitude at JD38 "}, {"name": "e_mag38", "desc": "? rms uncertainty on mag38 "}, {"name": "JD39", "desc": "? Date of observation 39; JD-2451224.0 "}, {"name": "mag39", "desc": "? Light curve magnitude at JD39 "}, {"name": "e_mag39", "desc": "? rms uncertainty on mag39 "}, {"name": "JD40", "desc": "? Date of observation 40; JD-2451224.0 "}, {"name": "mag40", "desc": "? Light curve magnitude at JD40 "}, {"name": "e_mag40", "desc": "? rms uncertainty on mag40 "}, {"name": "JD41", "desc": "? Date of observation 41; JD-2451224.0 "}, {"name": "mag41", "desc": "? Light curve magnitude at JD41 "}, {"name": "e_mag41", "desc": "? rms uncertainty on mag41 "}, {"name": "JD42", "desc": "? Date of observation 42; JD-2451224.0 "}, {"name": "mag42", "desc": "? Light curve magnitude at JD42 "}, {"name": "e_mag42", "desc": "? rms uncertainty on mag42 "}, {"name": "JD43", "desc": "? Date of observation 43; JD-2451224.0 "}, {"name": "mag43", "desc": "? Light curve magnitude at JD43 "}, {"name": "e_mag43", "desc": "? rms uncertainty on mag43 "}]}, {"name": "vmaglc.dat", "desc": "v band light curves ", "columns": [{"name": "QVS2", "desc": "Unique Running Identifier "}, {"name": "JD01", "desc": "Date of observation 1; JD-2451224.0 "}, {"name": "mag1", "desc": "Light curve magnitude at JD1 "}, {"name": "e_mag1", "desc": "rms uncertainty on mag1 "}, {"name": "JD2", "desc": "Date of observation 2; JD-2451224.0 "}, {"name": "mag2", "desc": "Light curve magnitude at JD2 "}, {"name": "e_mag2", "desc": "rms uncertainty on mag2 "}, {"name": "JD3", "desc": "Date of observation 3; JD-2451224.0 "}, {"name": "mag3", "desc": "Light curve magnitude at JD3 "}, {"name": "e_mag3", "desc": "rms uncertainty on mag3 "}, {"name": "JD4", "desc": "? Date of observation 4; JD-2451224.0 "}, {"name": "mag4", "desc": "? Light curve magnitude at JD4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "JD5", "desc": "? Date of observation 5; JD-2451224.0 "}, {"name": "mag5", "desc": "? Light curve magnitude at JD5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "JD6", "desc": "? Date of observation 6; JD-2451224.0 "}, {"name": "mag6", "desc": "? Light curve magnitude at JD6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "JD7", "desc": "? Date of observation 7; JD-2451224.0 "}, {"name": "mag7", "desc": "? Light curve magnitude at JD7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "JD8", "desc": "? Date of observation 8; JD-2451224.0 "}, {"name": "mag8", "desc": "? Light curve magnitude at JD8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "JD9", "desc": "? Date of observation 9; JD-2451224.0 "}, {"name": "mag9", "desc": "? Light curve magnitude at JD9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "JD10", "desc": "? Date of observation 10; JD-2451224.0 "}, {"name": "mag10", "desc": "? Light curve magnitude at JD10 "}, {"name": "e_mag10", "desc": "? rms uncertainty on mag10 "}, {"name": "JD11", "desc": "? Date of observation 11; JD-2451224.0 "}, {"name": "mag11", "desc": "? Light curve magnitude at JD11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}, {"name": "JD12", "desc": "? Date of observation 12; JD-2451224.0 "}, {"name": "mag12", "desc": "? Light curve magnitude at JD12 "}, {"name": "e_mag12", "desc": "? rms uncertainty on mag12 "}, {"name": "JD13", "desc": "? Date of observation 13; JD-2451224.0 "}, {"name": "mag13", "desc": "? Light curve magnitude at JD13 "}, {"name": "e_mag13", "desc": "? rms uncertainty on mag13 "}, {"name": "JD14", "desc": "? Date of observation 14; JD-2451224.0 "}, {"name": "mag14", "desc": "? Light curve magnitude at JD14 "}, {"name": "e_mag14", "desc": "? rms uncertainty on mag14 "}, {"name": "JD15", "desc": "? Date of observation 15; JD-2451224.0 "}, {"name": "mag15", "desc": "? Light curve magnitude at JD15 "}, {"name": "e_mag15", "desc": "? rms uncertainty on mag15 "}, {"name": "JD16", "desc": "? Date of observation 16; JD-2451224.0 "}, {"name": "mag16", "desc": "? Light curve magnitude at JD16 "}, {"name": "e_mag16", "desc": "? rms uncertainty on mag16 "}, {"name": "JD17", "desc": "? Date of observation 17; JD-2451224.0 "}, {"name": "mag17", "desc": "? Light curve magnitude at JD17 "}, {"name": "e_mag17", "desc": "? rms uncertainty on mag17 "}, {"name": "JD18", "desc": "? Date of observation 18; JD-2451224.0 "}, {"name": "mag18", "desc": "? Light curve magnitude at JD18 "}, {"name": "e_mag18", "desc": "? rms uncertainty on mag18 "}, {"name": "JD19", "desc": "? Date of observation 19; JD-2451224.0 "}, {"name": "mag19", "desc": "? Light curve magnitude at JD19 "}, {"name": "e_mag19", "desc": "? rms uncertainty on mag19 "}, {"name": "JD20", "desc": "? Date of observation 20; JD-2451224.0 "}, {"name": "mag20", "desc": "? Light curve magnitude at JD20 "}, {"name": "e_mag20", "desc": "? rms uncertainty on mag20 "}, {"name": "JD21", "desc": "? Date of observation 21; JD-2451224.0 "}, {"name": "mag21", "desc": "? Light curve magnitude at JD21 "}, {"name": "e_mag21", "desc": "? rms uncertainty on mag21 "}, {"name": "JD22", "desc": "? Date of observation 22; JD-2451224.0 "}, {"name": "mag22", "desc": "? Light curve magnitude at JD22 "}, {"name": "e_mag22", "desc": "? rms uncertainty on mag22 "}, {"name": "JD23", "desc": "? Date of observation 23; JD-2451224.0 "}, {"name": "mag23", "desc": "? Light curve magnitude at JD23 "}, {"name": "e_mag23", "desc": "? rms uncertainty on mag23 "}, {"name": "JD24", "desc": "? Date of observation 24; JD-2451224.0 "}, {"name": "mag24", "desc": "? Light curve magnitude at JD24 "}, {"name": "e_mag24", "desc": "? rms uncertainty on mag24 "}, {"name": "JD25", "desc": "? Date of observation 25; JD-2451224.0 "}, {"name": "mag25", "desc": "? Light curve magnitude at JD25 "}, {"name": "e_mag25", "desc": "? rms uncertainty on mag25 "}, {"name": "JD26", "desc": "? Date of observation 26; JD-2451224.0 "}, {"name": "mag26", "desc": "? Light curve magnitude at JD26 "}, {"name": "e_mag26", "desc": "? rms uncertainty on mag26 "}, {"name": "JD27", "desc": "? Date of observation 27; JD-2451224.0 "}, {"name": "mag27", "desc": "? Light curve magnitude at JD27 "}, {"name": "e_mag27", "desc": "? rms uncertainty on mag27 "}, {"name": "JD28", "desc": "? Date of observation 28; JD-2451224.0 "}, {"name": "mag28", "desc": "? Light curve magnitude at JD28 "}, {"name": "e_mag28", "desc": "? rms uncertainty on mag28 "}, {"name": "JD29", "desc": "? Date of observation 29; JD-2451224.0 "}, {"name": "mag29", "desc": "? Light curve magnitude at JD29 "}, {"name": "e_mag29", "desc": "? rms uncertainty on mag29 "}, {"name": "JD30", "desc": "? Date of observation 30; JD-2451224.0 "}, {"name": "mag30", "desc": "? Light curve magnitude at JD30 "}, {"name": "e_mag30", "desc": "? rms uncertainty on mag30 "}, {"name": "JD31", "desc": "? Date of observation 31; JD-2451224.0 "}, {"name": "mag31", "desc": "? Light curve magnitude at JD31 "}, {"name": "e_mag31", "desc": "? rms uncertainty on mag31 "}, {"name": "JD32", "desc": "? Date of observation 32; JD-2451224.0 "}, {"name": "mag32", "desc": "? Light curve magnitude at JD32 "}, {"name": "e_mag32", "desc": "? rms uncertainty on mag32 "}, {"name": "JD33", "desc": "? Date of observation 33; JD-2451224.0 "}, {"name": "mag33", "desc": "? Light curve magnitude at JD33 "}, {"name": "e_mag33", "desc": "? rms uncertainty on mag33 "}, {"name": "JD34", "desc": "? Date of observation 34; JD-2451224.0 "}, {"name": "mag34", "desc": "? Light curve magnitude at JD34 "}, {"name": "e_mag34", "desc": "? rms uncertainty on mag34 "}, {"name": "JD35", "desc": "? Date of observation 35; JD-2451224.0 "}, {"name": "mag35", "desc": "? Light curve magnitude at JD35 "}, {"name": "e_mag35", "desc": "? rms uncertainty on mag35 "}, {"name": "JD36", "desc": "? Date of observation 36; JD-2451224.0 "}, {"name": "mag36", "desc": "? Light curve magnitude at JD36 "}, {"name": "e_mag36", "desc": "? rms uncertainty on mag36 "}, {"name": "JD37", "desc": "? Date of observation 37; JD-2451224.0 "}, {"name": "mag37", "desc": "? Light curve magnitude at JD37 "}, {"name": "e_mag37", "desc": "? rms uncertainty on mag37 "}, {"name": "JD38", "desc": "? Date of observation 38; JD-2451224.0 "}, {"name": "mag38", "desc": "? Light curve magnitude at JD38 "}, {"name": "e_mag38", "desc": "? rms uncertainty on mag38 "}, {"name": "JD39", "desc": "? Date of observation 39; JD-2451224.0 "}, {"name": "mag39", "desc": "? Light curve magnitude at JD39 "}, {"name": "e_mag39", "desc": "? rms uncertainty on mag39 "}, {"name": "JD40", "desc": "? Date of observation 40; JD-2451224.0 "}, {"name": "mag40", "desc": "? Light curve magnitude at JD40 "}, {"name": "e_mag40", "desc": "? rms uncertainty on mag40 "}, {"name": "JD41", "desc": "? Date of observation 41; JD-2451224.0 "}, {"name": "mag41", "desc": "? Light curve magnitude at JD41 "}, {"name": "e_mag41", "desc": "? rms uncertainty on mag41 "}, {"name": "JD42", "desc": "? Date of observation 42; JD-2451224.0 "}, {"name": "mag42", "desc": "? Light curve magnitude at JD42 "}, {"name": "e_mag42", "desc": "? rms uncertainty on mag42 "}, {"name": "JD43", "desc": "? Date of observation 43; JD-2451224.0 "}, {"name": "mag43", "desc": "? Light curve magnitude at JD43 "}, {"name": "e_mag43", "desc": "? rms uncertainty on mag43 "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_2_315"}} {"id": "J/ApJS/2/315", "title_cds": "H{alpha} emission stars and nebulae", "title_create": "Henize, 1956", "year": "1956", "author": "Henize K.G.", "title_pub": "Catalogues of H-alpha emission stars and nebulae in the Magellanic Clouds.", "first_author": "Henize K.G.", "ref_biblio": [""], "bibcode": ["1956ApJS....2..315H\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "description": ["H{alpha} emission stars and emission nebulae were discovered on", "objective-prism photographs of the Magellanic Clouds made at the", "Lamount-Hussay Observatory of the University of Michigan.", "The original catalog was divided in 5 tables containing the emission", "stars of the Large Cloud (LHA 120-S), the emission nebulae in the", "Large Cloud (LHA 120-N), the exciting stars in the Large Cloud, the", "emission stars of the Small Cloud (LHA 115-S), and the emission", "nebulae in the Small Cloud (LHA 115-N).", "The accurate positions of these stars were found by Brian Skiff."], "object": [], "curator": "Brian Skiff [Lowell Obs.], Francois Ochsenbein [CDS]", "alias": ["LHA"], "type": ["OC"], "doi_pub": ["10.1086/190025"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_207_6"}} {"id": "J/ApJS/207/6", "title_cds": "YNOGK code for null geodesics in Kerr spacetime", "title_create": "Yang+, 2013", "year": "2013", "author": "Yang X., Wang J.", "title_pub": "YNOGK: a new public code for calculating null geodesics in the Kerr spacetime.", "first_author": "Yang X.", "ref_biblio": [""], "bibcode": ["2013ApJS..207....6Y"], "see_also": ["http://www1.ynao.ac.cn/~yangxl/yxl.html : autho's repository", "J/A+A/561/A127 : YNOGKM code for calculating time-like geodesics (Yang+, 2014)"], "keyword_cds": "Models ; Accretion", "keyword_pub": "accretion, accretion disks; black hole physics; radiative transfer relativistic processes", "abstract": ["Following the work of Dexter & Agol, we present a new public code for", "the fast calculation of null geodesics in the Kerr spacetime. Using", "Weierstrass's and Jacobi's elliptic functions, we express all", "coordinates and affine parameters as analytical and numerical", "functions of a parameter p, which is an integral value along the", "geodesic. This is the main difference between our code and previous", "similar ones. The advantage of this treatment is that the information", "about the turning points does not need to be specified in advance by", "the user, and many applications such as imaging, the calculation of", "line profiles, and the observer-emitter problem, become root-finding", "problems. All elliptic integrations are computed by Carlson's elliptic", "integral method as in Dexter & Agol, which guarantees the fast", "computational speed of our code. The formulae to compute the constants", "of motion given by Cunningham & Bardeen have been extended, which", "allow one to readily handle situations in which the emitter or the", "observer has an arbitrary distance from, and motion state with respect", "to, the central compact object. The validation of the code has been", "extensively tested through applications to toy problems from the", "literature. The source FORTRAN code is freely available for download", "on our Web site http://www1.ynao.ac.cn/~yangxl/yxl.html."], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1088/0067-0049/207/1/6"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_213_12"}} {"id": "J/ApJS/213/12", "title_cds": "SDSS Stripe 82 co-added runs", "title_create": "Jiang+, 2014", "year": "2014", "author": "Jiang L., Fan X., Bian F., McGreer I.D., Strauss M.A., Annis J., Buck Z., Green R., Hodge J.A., Myers A.D., Rafiee A., Richards G.", "title_pub": "The Sloan Digital Sky Survey Stripe 82 imaging data: depth-optimized co-adds over 300 deg^2^ in five filters.", "first_author": "Jiang L.", "ref_biblio": [""], "bibcode": ["2014ApJS..213...12J"], "see_also": ["V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)", "V/141 : Light-Motion Curve Catalogue (LMCC) in Stripe 82 (Bramich+ 2008)", "J/MNRAS/436/3581 : X-ray observations of Stripe 82 (LaMassa+, 2013)", "http://www.sdss.org/ : The SDSS home page", "http://classic.sdss.org/legacy/stripe82.html : Stripe 82 home page"], "keyword_cds": "Atlases ; Surveys ; Observatory log", "keyword_pub": "atlases; catalogs; surveys", "abstract": ["We present and release co-added images of the Sloan Digital Sky Survey", "(SDSS) Stripe 82. Stripe 82 covers an area of ~300deg^2^ on the", "celestial equator, and has been repeatedly scanned 70-90 times in the", "ugriz bands by the SDSS imaging survey. By making use of all available", "data in the SDSS archive, our co-added images are optimized for depth.", "Input single-epoch frames were properly processed and weighted based", "on seeing, sky transparency, and background noise before co-addition.", "The resultant products are co-added science images and their", "associated weight images that record relative weights at individual", "pixels. The depths of the co-adds, measured as the 5{sigma} detection", "limits of the aperture (3.2\" diameter) magnitudes for point sources,", "are roughly 23.9, 25.1, 24.6, 24.1, and 22.8 AB magnitudes in the five", "bands, respectively. They are 1.9-2.2mag deeper than the best SDSS", "single-epoch data. The co-added images have good image quality, with", "an average point-spread function FWHM of ~1\" in the r, i, and z bands.", "We also release object catalogs that were made with SExtractor. These", "co-added products have many potential uses for studies of galaxies,", "quasars, and Galactic structure. We further present and release", "near-IR J-band images that cover ~90deg^2^ of Stripe 82. These images", "were obtained using the NEWFIRM camera on the NOAO 4m Mayall", "telescope, and have a depth of about 20.0-20.5 Vega magnitudes (also", "5{sigma} detection limits for point sources)."], "description": ["Stripe 82 covers 300deg^2^, and was repeatedly scanned 70-90 times", "over roughly 10 years. These Stripe 82 images, when co-added, reach a", "much greater depth than do SDSS single-run data.", "All our data products, including 24060 co-added science images and", "their associated weight images and object catalogs, are released on", "this Web site: http://das.sdss.org/ge/sample/stripe82/."], "type": ["OC"], "doi_pub": ["10.1088/0067-0049/213/1/12"], "orcid_pub": ["0000-0003-4176-6486"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table3.dat", "desc": "SDSS runs used for our co-adds ", "columns": [{"name": "Run", "desc": "[125/7202] SDSS run number "}, {"name": "MJD", "desc": "[51081/54433] Modified Julian Date of observation "}, {"name": "Fst", "desc": "[11/702] Starting field number "}, {"name": "Fend", "desc": "[50/1000] Ending field number "}, {"name": "RAst", "desc": "[-70/54] Starting Right Ascension in decimal degrees"}, {"name": "RAend", "desc": "[-55/87] Ending Right Ascension in decimal degrees "}, {"name": "ID", "desc": "Stripe 82 identifier (N=North or S=South) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_219_26"}} {"id": "J/ApJS/219/26", "title_cds": "OGLE atlas of classical novae. I. Galactic bulge", "title_create": "Mroz+, 2015", "year": "2015", "author": "Mroz P., Udalski A., Poleski R., Soszynski I., Szymanski M.K., Pietrzynski G., Wyrzykowski L., Ulaczyk K., Kozlowski S., Pietrukowicz P., Skowron J.", "title_pub": "OGLE atlas of classical novae. I. Galactic bulge objects.", "first_author": "Mroz P.", "ref_biblio": [""], "bibcode": ["2015ApJS..219...26M"], "see_also": ["B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-2014)", "B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013)", "V/123 : Catalog of Cataclysmic Variables (Downes+ 2001-2006)", "II/213 : OGLE Galactic Bulge periodic variables (Udalski+ 1996)", "J/AcA/64/197 : OGLE-IV 2012-2014 transients (Wyrzykowski+, 2014)", "J/AcA/63/135 : New OGLEIII dwarf novae in Galactic disk (Mroz+, 2013)", "J/A+A/554/A123 : Near-IR catalog of novae in VVV survey area (Saito+, 2013)", "J/ApJ/721/L28 : Red clump stars in Bulge from OGLE-III (Nataf+, 2010)", "J/AJ/140/34 : Classification of nova light curves (Strope+, 2010)", "J/ApJS/187/275 : Photometric histories of recurrent novae (Schaefer, 2010)", "J/MNRAS/387/344 : BVRcIC photometry of V2615 Oph (Munari+, 2008)", "J/PAZh/34/270 : Photometric parameters of Galactic novae (Burlak+, 2008)", "J/AcA/52/217 : OGLE II. VI photometry of Galactic Bulge (Udalski+, 2002)", "J/AJ/99/1079 : Nova rate in NGC 5128 (Ciardullo+, 1990)", "http://ogle.astrouw.edu.pl/ : OGLE home page", "http://ogle.astrouw.edu.pl/ogle4/transients/ : OGLE-IV transients", "http://www.cbat.eps.harvard.edu/nova_list.html : IAU CBAT list of MW novae", "http://asd.gsfc.nasa.gov/Koji.Mukai/novae/novae.html : Koji's list of recent"], "keyword_cds": "Novae ; Stars, variable ; Photometry, VRI", "keyword_pub": "novae, cataclysmic variables; stars: statistics", "abstract": ["Eruptions of classical novae are possible sources of lithium formation", "and gamma-ray emission. Nova remnants can also become Type Ia", "supernovae (SNe Ia). The contribution of novae to these phenomena", "depends on nova rates, which are not well established for the Galaxy.", "Here, we directly measure a Galactic bulge nova rate of", "13.8+/-2.6yr^-1^. This measurement is much more accurate than any", "previous measurement of this kind thanks to many years' monitoring of", "the bulge by the Optical Gravitational Lensing Experiment (OGLE)", "survey. Our sample consists of 39 novae eruptions, ~1/3 of which are", "OGLE-based discoveries. This long-term monitoring allows us to not", "only measure the nova rate but also to study in detail the light", "curves of 39 eruptions and more than 80 post-nova candidates. We", "measured orbital periods for 9 post-novae and 9 novae, and in 14 cases", "we procured the first estimates. The OGLE survey is very sensitive to", "the frequently erupting recurrent novae. We did not find any object", "similar to M31 2008-12a, which erupts once a year. The lack of", "detection indicates that there is only a small number of them in the", "Galactic bulge."], "description": ["All of the data presented in this paper were collected in the course", "of OGLE. The OGLE sky survey began operation in 1992. In the first", "phase, OGLE-I, conducted from 1992 to 1995 with the 1.0 m Swope", "telescope at Las Campanas Observatory (LCO), Chile, 16 Galactic bulge", "fields with a total field of view of about 1 sq. degree were observed.", "In its second phase, OGLE-II, from 1997 to 2000, approximately 30", "million stars from 11 sq. degrees of the Galactic bulge were monitored", "with the dedicated 1.3m Warsaw Telescope (located at LCO). In the", "OGLE-III phase (2001 to 2009), 92 sq. degrees around the Galactic", "center were regularly observed. Currently, the project is in its", "fourth phase, OGLE-IV (since 2010). The OGLE-IV observations analyzed", "here cover 140 sq. degrees of the Galactic bulge. The majority of", "measurements were taken through the I-band filter, closely resembling", "that of the standard Johnson-Cousins system."], "type": ["OC"], "doi_pub": ["10.1088/0067-0049/219/2/26"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "List of nova eruptions recorded by the OGLE survey ", "columns": [{"name": "Name", "desc": "Designation "}, {"name": "f_Name", "desc": "Flag on Name (1) "}, {"name": "OName", "desc": "Other nova name "}, {"name": "RAh", "desc": "[17/18] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Arcminute of right ascension (J2000) "}, {"name": "RAs", "desc": "Arcsecond of right ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[20/36] Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "Field", "desc": "OGLE field "}, {"name": "OGLE", "desc": "OGLE database number "}, {"name": "Date", "desc": "UT date of the eruption "}]}, {"name": "table2.dat", "desc": "Properties of novae recorded by the OGLE survey ", "columns": [{"name": "Name", "desc": "Designation "}, {"name": "Type", "desc": "Light curve type (1) "}, {"name": "Per", "desc": "[0.1/1.6]? Orbital period "}, {"name": "e_Per", "desc": "[/0.0001]? Per uncertainty "}, {"name": "l_ImagPre", "desc": "Limit flag on ImagPre "}, {"name": "ImagPre", "desc": "[13.7/21.5]? OGLE I-band brightness of pre-nova (G1)"}, {"name": "V-IPre", "desc": "[0.6/5]? (V-I) color index of pre-nova "}, {"name": "ImagPst", "desc": "[13.7/21.5]? OGLE I-band brightness of post-nova (G1)"}, {"name": "f_ImagPst", "desc": "[b] b = During decline "}, {"name": "V-IPst", "desc": "[-1.2/3.1]? (V-I) color index of post-nova "}]}, {"name": "table3.dat", "desc": "Likely post-novae: stars showing eclipse-like variability", "columns": [{"name": "Star", "desc": "GCVS identifier "}, {"name": "Name", "desc": "Nova name (Nova XXX YYYYZ) "}, {"name": "RAh", "desc": "[17/18] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Arcminute of right ascension (J2000) "}, {"name": "RAs", "desc": "Arcsecond of right ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[17/39] Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "sep", "desc": "[0.03/7] Distance from SIMBAD position "}, {"name": "Field", "desc": "OGLE field "}, {"name": "OGLE", "desc": "OGLE database number "}, {"name": "Imag", "desc": "[12.4/21.4] OGLE mean I-band brightness (G1) "}, {"name": "Vmag", "desc": "[14.2/22.1]? OGLE mean V-band brightness "}, {"name": "V-I", "desc": "[0.5/5.6]? OGLE mean (V-I) color index "}, {"name": "Type", "desc": "Type of the secondary (MS=main sequence; RG=red giant)"}, {"name": "Per", "desc": "[0.1/0.9]? Orbital period (only for table 3) "}, {"name": "e_Per", "desc": "? Per uncertainty "}]}, {"name": "table4.dat", "desc": "Possible post-novae: old novae counterparts ", "columns": [{"name": "Star", "desc": "GCVS identifier "}, {"name": "Name", "desc": "Nova name (Nova XXX YYYYZ) "}, {"name": "RAh", "desc": "[17/18] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Arcminute of right ascension (J2000) "}, {"name": "RAs", "desc": "Arcsecond of right ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[17/39] Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "sep", "desc": "[0.03/7] Distance from SIMBAD position "}, {"name": "Field", "desc": "OGLE field "}, {"name": "OGLE", "desc": "OGLE database number "}, {"name": "Imag", "desc": "[12.4/21.4] OGLE mean I-band brightness (G1) "}, {"name": "Vmag", "desc": "[14.2/22.1]? OGLE mean V-band brightness "}, {"name": "V-I", "desc": "[0.5/5.6]? OGLE mean (V-I) color index "}, {"name": "Type", "desc": "Type of the secondary (MS=main sequence; RG=red giant)"}, {"name": "Per", "desc": "[0.1/0.9]? Orbital period (only for table 3) "}, {"name": "e_Per", "desc": "? Per uncertainty "}]}, {"name": "phot/*", "desc": "I-band photometry of individual objects ", "columns": [{"name": "HJD", "desc": "Heliocentric Julian Date; JD-2450000 "}, {"name": "Imag", "desc": "?=99.999 OGLE I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.999 Imag uncertainty "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_220_5"}} {"id": "J/ApJS/220/5", "title_cds": "Chandra survey of 3CR extragalactic sources", "title_create": "Massaro+, 2015", "year": "2015", "author": "Massaro F., Harris D.E., Liuzzo E., Orienti M., Paladino R., Paggi A., Tremblay G.R., Wilkes B.J., Kuraszkiewicz J., Baum S.A., O'Dea C.P.", "title_pub": "The Chandra survey of extragalactic sources in the 3CR catalog: X-ray emission from nuclei, jets, and hotspots in the Chandra archival observations.", "first_author": "Massaro F.", "ref_biblio": [""], "bibcode": ["2015ApJS..220....5M"], "see_also": ["B/chandra : The Chandra Archive Log (CXC, 1999-2014)", "VIII/1 : The 3C and 3CR Catalogues (Edge+ 1959-1962)", "J/A+A/575/A80 : FIR photometry of 3CR galaxies (Podigachoski+, 2015)", "J/ApJS/206/12 : Blazars with {gamma}-ray counterparts. I. (D'Abrusco+, 2013)", "J/ApJS/197/24 : Chandra large-scale extragalactic jets. I. (Massaro+, 2011)", "J/ApJ/726/20 : X-ray emission from quasars (Miller+, 2011)", "J/ApJ/704/1586 : BCGs with radio AGN (Sun, 2009)", "J/MNRAS/392/1509 : Distribution of AGNs in galaxy clusters (Gilmour+, 2009)", "J/ApJS/164/307 : NICMOS observations of 3CR radio sources (Madrid+, 2006)", "J/ApJS/177/148 : HST survey of 3CR radio source counterparts II. (Floyd+, 2008)", "J/AJ/130/23 : Spectrophotometry of 3CR lobe-dominated quasars (Aars+, 2005)", "J/A+A/396/397 : Deep cluster survey in Chandra archival data (Boschin+, 2002)", "J/ApJS/122/81 : HST snapshot survey of 3CR radio sources (Martel+, 1999)", "J/PASP/97/932 : 3CR Source Identifications (Spinrad+, 1985)", "http://hea-www.cfa.harvard.edu/XJET/ : XJET home page", "http://www.jb.man.ac.uk/atlas/ : Online atlas of DRAGNs"], "keyword_cds": "Active gal. nuclei ; Radio sources ; X-ray sources ; Redshifts", "keyword_pub": "galaxies: active; radio continuum: galaxies; X-rays: general", "abstract": ["As part of our program to build a complete radio and X-ray database of", "all Third Cambridge catalog extragalactic radio sources, we present an", "analysis of 93 sources for which Chandra archival data are available.", "Most of these sources have already been published. Here we provide a", "uniform re-analysis and present nuclear X-ray fluxes and X-ray", "emission associated with radio jet knots and hotspots using both", "publicly available radio images and new radio images that have been", "constructed from data available in the Very Large Array archive. For", "about 1/3 of the sources in the selected sample, a comparison between", "the Chandra and radio observations was not reported in the literature:", "we find X-ray detections of 2 new radio jet knots and 17 hotspots. We", "also report the X-ray detection of extended emission from the", "intergalactic medium for 15 galaxy clusters."], "description": ["In the present paper, we uniformly analyzed 93 3CR sources observed by", "Chandra that were not reported in our previous investigations (see", "table 2)."], "type": ["OC"], "doi_pub": ["10.1088/0067-0049/220/1/5"], "orcid_pub": ["0000-0002-1704-9850"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Source list of the archival Chandra 3CR radio sources", "columns": [{"name": "3CR", "desc": "3CR name (NNN.N) "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) (1) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) (1) "}, {"name": "DEd", "desc": "Degree of declination (J2000) (1) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "z", "desc": "[0.01/2] Redshift (G1) "}, {"name": "Scale", "desc": "[0.3/8.5] Angular to linear scale factor (G2) "}, {"name": "Dist", "desc": "[72/15097] Luminosity distance D_L_ (G2) "}, {"name": "ObsID", "desc": "[326/15656] Chandra observation ID "}, {"name": "PropID", "desc": "[1600145/14700660] Chandra proposal ID "}, {"name": "Date", "desc": "UT date of Chandra observation "}, {"name": "Mode", "desc": "Data mode (2) "}, {"name": "Time", "desc": "[2/72.1] Live time of Chandra observation "}, {"name": "Ref", "desc": "Reference(s) for the Chandra observation "}]}, {"name": "table4.dat", "desc": "X-Ray emission from radio cores ", "columns": [{"name": "3CR", "desc": "3CR name (NNN.N) "}, {"name": "f_3CR", "desc": "[b] Flag on 3CR (1) "}, {"name": "Ncts", "desc": "[6/20856] net counts "}, {"name": "e_Ncts", "desc": "[2/144] Ncts uncertainty (2) "}, {"name": "ExtR", "desc": "[0.05/1.1] Ext. ratio (3) "}, {"name": "e_ExtR", "desc": "[0.004/0.5]? ExtR uncertainty (2) "}, {"name": "F0.5-1keV", "desc": "[0/699] 0.5-1keV flux in 10^-15^erg/cm^2^/s "}, {"name": "e_F0.5-1keV", "desc": "[0/20] F0.5-1keV uncertainty (4) "}, {"name": "E_F0.5-1keV", "desc": "[0.03]? Second uncertainty on F0.5-1keV (4) "}, {"name": "F1-2keV", "desc": "[0.2/822] 1-2keV flux in 10^-15^erg/cm^2^/s "}, {"name": "e_F1-2keV", "desc": "[0.2/26] F1-2keV uncertainty (4) "}, {"name": "F2-7keV", "desc": "[0.7/2364] Measured X-ray flux between 2 and 7keV in 10^-15^erg/cm^2^/s"}, {"name": "e_F2-7keV", "desc": "[1/97] F2-7keV uncertainty (4) "}, {"name": "F0.5-7keV", "desc": "[4/3022] 0.5-7keV flux in 10^-15^erg/cm^2^/s"}, {"name": "e_F0.5-7keV", "desc": "[1/102] F0.5-7keV uncertainty (4) "}, {"name": "LX", "desc": "[/425] 0.5-7keV X-ray luminosity "}, {"name": "e_LX", "desc": "[/7] LX 1{sigma} uncertainty "}]}, {"name": "table8.dat", "desc": "The current status of the 3CR Chandra observations ", "columns": [{"name": "3CR", "desc": "3CR name (NNN.N) "}, {"name": "m_3CR", "desc": "3CR component letter "}, {"name": "Class", "desc": "Radio-to-optical classification (1) "}, {"name": "z", "desc": "? Redshift (G1) "}, {"name": "f_z", "desc": "[?] ?=Undetermined redshift (2) "}, {"name": "Dist", "desc": "[2.9/21341]? Luminosity distance D_L_ (G2) "}, {"name": "Flag", "desc": "[yes/no ] Cluster flag (3) "}, {"name": "XDet", "desc": "X-ray detection flag(s) (4) "}, {"name": "CFlag", "desc": "[yes/no ] Chandra flag (5) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_221_6"}} {"id": "J/ApJS/221/6", "title_cds": "H2O & CH3OH maser survey of class II methanol masers", "title_create": "Kang+, 2015", "year": "2015", "author": "Kang H., Kim K.-T., Byun D.-Y., Lee S., Park Y.-S.", "title_pub": "Simultaneous observation of water and class I methanol masers toward class II methanol maser sources.", "first_author": "Kang H.", "ref_biblio": [""], "bibcode": ["2015ApJS..221....6K"], "see_also": ["J/other/IJAA/4.571 : Methanol masers in HII regions (Farmer, 2014)", "J/MNRAS/439/2584 : Southern methanol masers at 36 and 44GHz (Voronkov+, 2014)", "J/ApJS/209/25 : H2O + CH_3_OH maser survey of Orion protostars (Kang+, 2013)", "J/ApJ/763/2 : 95GHz methanol masers in molecular outflows (Gan+, 2013)", "J/AZh/89/611 : Class I methanol maser catalog (Bayandina+, 2012)", "J/ApJ/753/50 : 6.7GHz methanol masers. I. NH_3_ lines (Pandian+, 2012)", "J/ApJS/200/5 : 95GHz class I methanol maser survey (Chen+, 2012)", "J/MNRAS/418/1689 : Red MSX water maser and ammonia emissions (Urquhart+, 2011)", "J/ApJS/196/9 : 95GHz methanol maser survey toward GLIMPSE EGOs (Chen+, 2011)", "J/ApJ/702/1615 : CH_3_OH maser survey of EGOs (Cyganowski+, 2009)", "J/ApJ/656/255 : Arecibo methanol maser Galactic Plane Survey (Pandian+, 2007)", "J/MNRAS/359/1498 : Class I and class II methanol masers (Ellingsen+, 2005)", "J/A+A/434/613 : Water maser survey of methanol maser sources (Szymczak+, 2005)", "J/A+A/417/615 : Maser and outflows in UC HII region (Codella+, 2004)", "J/A+A/403/1095 : 6.7GHz methanol masers survey of low-mass YSO (Minier+, 2003)", "J/A+AS/137/43 : OH/H2O masers database (Forster+, 1999)", "J/MNRAS/301/640 : Ultracompact H II regions studies. II. (Walsh+, 1998)"], "keyword_cds": "Masers ; Radio lines ; Millimetric/submm sources ; Surveys", "keyword_pub": "ISM: abundances; ISM: molecules; masers; stars: formation", "abstract": ["We present a simultaneous single-dish survey of 22GHz water masers and", "44 and 95GHz class I methanol masers toward 77 6.7GHz class II", "methanol maser sources, which were selected from the Arecibo methanol", "maser Galactic plane survey catalog. Water maser emission is detected", "in 39 (51%) sources, 15 of which are new detections. Methanol maser", "emission at 44 and 95GHz is found in 25 (32%) and 19 (25%) sources, 21", "and 13 of which, respectively, are newly detected. We find four", "high-velocity (>30km/s) water maser sources, including three dominant", "blue- or redshifted outflows. The 95GHz masers always appear with", "44GHz maser emission. They are strongly correlated with 44GHz masers", "in velocity, flux density, and luminosity, yet they are not correlated", "with either water or 6.7GHz class II methanol masers. The average peak", "flux density ratio of 95GHz masers to 44GHz masers is close to unity,", "which is two times higher than previous estimates. The flux densities", "of class I methanol masers are more closely correlated with the", "associated Bolocam Galactic Plane Survey core mass than those of water", "masers or class II methanol masers. Using the large velocity gradient", "model and assuming unsaturated class I methanol maser emission, we", "derive the fractional abundance of methanol to be in the range", "4.2x10^-8^-2.3x10^-6^, with a median value of 3.3+/-2.7x10^-7^."], "description": ["We selected 77 sources from the Arecibo methanol maser Galactic plane", "survey (AMGPS) catalog of 6.7GHz methanol maser sources (Pandian+,", "2007, J/ApJ/656/255).", "Using the Korean VLBI Network (KVN) 21m telescopes, we performed", "simultaneous surveys of the H_2_O 6_16_-5_23_ (22.23508GHz),", "CH_3_OH 7_0_-6_1_ A^+^ (44.06943GHz), and CH_3_OH 8_0_-7_1_ A^+^", "(95.169463GHz) masers toward the 77 class II methanol maser sources.", "The observations took a total of 18 days to complete and were", "undertaken between 2011 November and 2012 March: 15 days for the", "survey and 3 days for the grid mapping.", "We also observed four sources in the ^13^CO (J=1-0) (110.201353GHz)", "line and one of them in the HCO+ (J=1-0) (89.188523GHz) line using the", "Taeduk Radio Astronomy Observatory (TRAO) 14m telescope on 2014 March 17."], "type": ["OC"], "doi_pub": ["10.1088/0067-0049/221/1/6"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Source summary with detection results ", "columns": [{"name": "Name", "desc": "Source designation (GLL.ll+B.bb) (1) "}, {"name": "f_Name", "desc": "[d] Flag on Name (2) "}, {"name": "RAh", "desc": "[18/19] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[1/18] Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "Fpos", "desc": "[c] Flag on J2000 coordinates (2) "}, {"name": "Vsys", "desc": "[-44.4/94.6] Systemic velocity from the NH3 observation (Pandian+ 2012, J/ApJ/753/50)"}, {"name": "f_Vsys", "desc": "[ef] Flag on Vsys (2) "}, {"name": "Date", "desc": "UT date "}, {"name": "22GHz", "desc": "New 22GHz water maser "}, {"name": "r_22GHz", "desc": "22GHz water maser reference(s) (3) "}, {"name": "44GHz", "desc": "44GHz class I maser reference(s) (3) "}, {"name": "95GHz", "desc": "New 95GHz ClassI maser "}, {"name": "r_95GHz", "desc": "[11/13]? 95GHz ClassI maser reference (3) "}, {"name": "Fig", "desc": "[2/6]? Figure number "}]}, {"name": "table3.dat", "desc": "Line parameters of detected masers ", "columns": [{"name": "Name", "desc": "Source designation (GLL.ll+B.bb) "}, {"name": "Freq", "desc": "[22/95] Frequency "}, {"name": "Sint", "desc": "[0.7/494] Integrated flux density (Gaussian fit)"}, {"name": "e_Sint", "desc": "[0.1/13.2] Sint uncertainty "}, {"name": "Vpk", "desc": "[-16.9/137] Peak velocity "}, {"name": "e_Vpk", "desc": "[0/0.7] Vpk uncertainty "}, {"name": "FWHM", "desc": "[0.2/6.8] Full-width at half-maximum "}, {"name": "e_FWHM", "desc": "[0/2.3] FWHM uncertainty "}, {"name": "Spk", "desc": "[0.8/716.9] Peak flux density (Gaussian fit) "}, {"name": "e_Spk", "desc": "[0.3/4.9] Spk uncertainty "}, {"name": "SintI", "desc": "[0.8/608] Integrated flux density (Integrated fit)"}, {"name": "Vmin", "desc": "[-18.2/135.3] Minimum velocity "}, {"name": "Vmax", "desc": "[-16.6/139.1] Maximum velocity "}, {"name": "SpkI", "desc": "[1.2/714.2] Peak flux density (Integrated fit) "}, {"name": "VpkI", "desc": "[-16.8/137.2] Peak velocity (Integrated fit) "}]}, {"name": "table4.dat", "desc": "Maser luminosities and associated BGPS sources ", "columns": [{"name": "Name", "desc": "Source designation (GLL.ll+B.bb) "}, {"name": "L6.7", "desc": "6.7GHz luminosity (1) "}, {"name": "L22", "desc": "[/0.003]? 22GHz luminosity "}, {"name": "L44", "desc": "[/0.0002]? 44GHz luminosity "}, {"name": "L95", "desc": "[/0.0004]? 95GHz luminosity "}, {"name": "Tkin", "desc": "[14/67.3]? Kinetic temperature (2) "}, {"name": "BGPS", "desc": "BGPS name (GLLL.lll+BB.bbb) "}, {"name": "Sint", "desc": "[0.1/9.6]? Integrated flux density "}, {"name": "NH2", "desc": "[0.5/12.1]? H_2_ column density (T=20K) "}, {"name": "Mgas", "desc": "[41/5800]? M_gas_ value (T_kin_) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_223_29"}} {"id": "J/ApJS/223/29", "title_cds": "The VLT LEGA-C spectroscopic survey", "title_create": "van der Wel+, 2016", "year": "2016", "author": "van der Wel A., Noeske K., Bezanson R., Pacifici C., Gallazzi A., Franx M., Munoz-mateos J.C., Bell E.F., Brammer G., Charlot S., Chauke P., Labbe I., Maseda M.V., Muzzin A., Rix H.-W., Sobral D., van de Sande J., van Dokkum P.G., Wild V., Wolf C.", "title_pub": "The VLT LEGA-C spectroscopic survey: the physics of galaxies at a lookback time of 7 Gyr.", "first_author": "van der Wel A.", "ref_biblio": [""], "bibcode": ["2016ApJS..223...29V"], "see_also": ["J/ApJS/94/687 : Old stellar populations. V. (Worthey+, 1994)", "J/ApJS/111/377 : H{gamma} & H{delta} absorption features (Worthey+ 1997)", "J/ApJ/706/1364 : SINS survey of high-redshift gal. (Forster Schreiber+, 2009)", "J/MNRAS/396/818 : Blue early-type galaxies in Galaxy Zoo (Schawinski+, 2009)", "J/ApJ/724/714 : Velocity dispersions of MS1054-03 & Coma gal. (Holden+, 2010)", "J/ApJ/741/115 : Deep spectroscopy in the GOODS fields (Miller+, 2011)", "J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012)", "J/ApJS/203/24 : Structural param. of galaxies in CANDELS (van der Wel+, 2012)", "J/AJ/145/77 : Imaging & spectrosc. in 3 galaxy clusters (Jorgensen+, 2013)", "J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013)", "J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)", "J/ApJ/788/72 : Observed sample of z~0.7 massive galaxies (Gallazzi+, 2014)", "J/ApJ/799/148 : DEIMOS galaxy sample at z~0.7 (Bezanson+, 2015)", "http://www.mpia.de/home/legac/index.html : LEGA-C survey home page", "http://www.eso.org/rm/api/v1/public/releaseDescriptions/83 : Description of"], "keyword_cds": "Galaxies, spectra ; Redshifts ; Surveys", "keyword_pub": "galaxies: evolution; galaxies: fundamental parameters; galaxies: general; galaxies: stellar content; surveys", "abstract": ["The Large Early Galaxy Census (LEGA-C) is an ESO Public Spectroscopic", "Survey of ~3200K-band selected galaxies at redshifts z=0.6-1.0 with", "stellar masses M*>10^10^M_{sun}_, conducted with VIMOS on ESO's Very", "Large Telescope. The survey is embedded in the COSMOS field", "(RA=10h00,DEC=+2{deg}). The 20hr long integrations produce", "high-signal-to-noise ratio continuum spectra that reveal ages,", "metallicities and velocity dispersions of the stellar populations.", "LEGA-C's unique combination of sample size and depth will enable us", "for the first time to map the stellar content at large lookback time,", "across galaxies of different types and star formation activity.", "Observations started in 2014 December and are planned to be completed", "by mid 2018, with early data releases of the spectra and value-added", "products. In this paper we present the science case, the observing", "strategy, an overview of the data reduction process and data products,", "and a first look at the relationship between galaxy structure and", "spectral properties, as it existed 7Gyr ago."], "description": ["This catalog is the first data release (DR1) from the LEGA-C (Large", "Early Galaxy Census) survey. The VIMOS high-resolution red grating is", "used in combination with the GG475 order separation filter, which", "results in a typical wavelength range of ~6300-8800{AA} at a", "resolution of R=2500 and a dispersion of 0.6{AA}/pix.", "In this release, we provide the data resulting from our first year of", "observations, totaling 892 galaxy spectra for 865 unique galaxies as", "well as a catalog that provides survey IDs, coordinates, and redshifts", "for this first subsample. The data presented here were taken during", "the ESO observing periods 94 and 95, during the runs 194.A-2005(A) to", "194.A-2005(F), with the respective date windows:", "22 Dec 2014 - 27 Dec 2014, 15 Jan 2015 - 25 Jan 2015, 14 Feb 2015 -", "24 Feb 2014, 15 Mar 2015 - 26 Mar 2015, 13 Apr 2015 -", "23 Apr 2015, 12 May 2015 - 22 May 2015.", "The parent sample is the photometric sample from Muzzin+ (2013,", "J/ApJS/206/8). Their UltraVISTA K-band selected catalog is 90%", "complete down to K=23.4 and contains 160070 sources across 1.62deg^2^", "in the COSMOS field (RA=10:00,DE=+2:12; J2000)."], "type": ["OC"], "doi_pub": ["10.3847/0067-0049/223/2/29"], "orcid_pub": ["0000-0002-5027-0135"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "legac_v1.dat", "desc": "Large Early Galaxy Census (LEGA-C) spectroscopic survey, DR1", "columns": [{"name": "[MMS2013]", "desc": "[73754/241460] ID from UltraVISTA (Muzzin+ 2013, J/ApJS/206/8)"}, {"name": "SpID", "desc": "Spectrum unique identifier (mask number+ objID) "}, {"name": "RAdeg", "desc": "[149.7/150.5] Right ascension (J2000) "}, {"name": "DEdeg", "desc": "[2/2.6] Declination (J2000) "}, {"name": "z", "desc": "[0.3/1.4]? Spectroscopic redshift "}, {"name": "FileName", "desc": "FITS file name of the original spectrum "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_228_13"}} {"id": "J/ApJS/228/13", "title_cds": "Short Title", "title_create": "Roming+, 2017", "year": "2017", "author": "Roming P.W.A., Koch T.S., Oates S.R., Porterfield B.L., Bayless A.J., Breeveld A.A., Gronwall C., Kuin N.P.M., Page M.J., De Pasquale M., Siegel M.H., Swenson C.A., Tobler J.M.", "title_pub": "A large catalog of homogeneous ultra-violet/optical GRB afterglows: temporal and spectral evolution.", "first_author": "Roming P.W.A.", "ref_biblio": [""], "bibcode": ["2017ApJS..228...13R"], "keyword_cds": "", "keyword_pub": "catalogs; gamma-ray burst: general", "abstract": ["We present the second Swift Ultra-Violet/Optical Telescope (UVOT)", "gamma-ray burst (GRB) afterglow catalog, greatly expanding on the", "first Swift UVOT GRB afterglow catalog. The second catalog is", "constructed from a database containing over 120,000 independent UVOT", "observations of 538 GRBs first detected by Swift, the High Energy", "Transient Explorer 2 (HETE2), the INTErnational Gamma-Ray Astrophysics", "Laboratory (INTEGRAL), the Interplanetary Network (IPN), Fermi, and", "Astro-rivelatore Gamma a Immagini Leggero (AGILE). The catalog covers", "GRBs discovered from 2005 January 17 to 2010 December 25. Using", "photometric information in three UV bands, three optical bands, and a", "\"white\" or open filter, the data are optimally coadded to maximize the", "number of detections and normalized to one band to provide a detailed", "light curve. The catalog provides positional, temporal, and", "photometric information for each burst, as well as Swift Burst Alert", "Telescope and X-ray Telescope (XRT) GRB parameters. Temporal slopes", "are provided for each UVOT filter. The temporal slope per filter of", "almost half the GRBs are fit with a single power law, but one to three", "breaks are required in the remaining bursts. Morphological comparisons", "with the X-ray reveal that \\sim 75 \\% of the UVOT light curves are", "similar to one of the four morphologies identified by Evans et al.", "(2009). The remaining \\sim 25 \\% have a newly identified morphology.", "For many bursts, redshift- and extinction-corrected UV/optical", "spectral slopes are also provided at 2 x 10^3^, 2 x 10^4^, and 2 x", "10^5^ s."], "doi_pub": ["10.3847/1538-4365/228/2/13"], "orcid_pub": ["0000-0002-5499-953X"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table5.dat", "desc": "Normalized Optimally Coadded (NOC) table ", "columns": [{"name": "Name", "desc": "GRB name (OBJECT) "}, {"name": "Filt", "desc": "UVOT filter used for exposure (uvw2, uvm2, uvwu, b, v, and white) (FILTER)"}, {"name": "Time", "desc": "[63/13649310] Weighted time of the detection as described in M08 (TIME)"}, {"name": "Tstart", "desc": "[58/] MET start time of the data used in the optimal coaddition (TSTART)"}, {"name": "Tstop", "desc": "[68/] MET stop time of the data used in the optimal coaddition (TSTOP)"}, {"name": "Exp", "desc": "[1.5/52183] Total exposure time for the optimally coadded data (EXPOSURE) (1)"}, {"name": "Cts", "desc": "[4/40343] Computed source counts in a coadded image as described in M08 (CSRC)"}, {"name": "e_Cts", "desc": "[2/294] Cts uncertainty (CERR) "}, {"name": "Rate", "desc": "[0/404] Computed coadded source rate calculated using (Cts*Scale)/Exp"}, {"name": "e_Rate", "desc": "[0/29] Source rate error calculated using (e_Cts*Scale)/Exp (RATE_ERR)"}, {"name": "mag", "desc": "[11.3/28.4] Magnitude of the source in the UVOT system computed from RATE (MAG)"}, {"name": "e_mag", "desc": "[0.006/0.6] mag uncertainty (MAG_ERR) "}, {"name": "Flux", "desc": "Flux density based on an average GRB spectrum, in erg/cm^2^/s/{AA} (FLUX)"}, {"name": "e_Flux", "desc": "1{sigma} error in Flux (FLUX_ERR) "}, {"name": "S/N", "desc": "[2/193] Signal-to-noise of the coadded weighted image as described in M08"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_228_14"}} {"id": "J/ApJS/228/14", "title_cds": "Short Title", "title_create": "Chilingarian+, 2017", "year": "2017", "author": "Chilingarian I.V., Zolotukhin I.Y., Katkov I.Y., Melchior A.-L., Rubtsov E.V., Grishin K.A.", "title_pub": "RCSED - A value-added Reference Catalog of Spectral Energy Distributions of 800299 galaxies in 11 ultraviolet, optical, and near-infrared bands: morphologies, colors, ionized gas, and stellar population properties.", "first_author": "Chilingarian I.V.", "keyword_cds": "", "keyword_pub": "catalogs; galaxies: fundamental parameters; galaxies: photometry galaxies: stellar content", "abstract": ["We present RCSED, the value-added Reference Catalog of Spectral Energy", "Distributions of galaxies, which contains homogenized", "spectrophotometric data for 800299 low- and intermediate-redshift", "galaxies (0.007"], "bibcode": ["2017ApJS..230...24B"], "keyword_cds": "", "keyword_pub": "catalogs; Galaxy: stellar content; stars: AGB and post-AGB; stars: early-type; surveys; ultraviolet: general", "abstract": ["The Galaxy Evolution Explorer (GALEX) imaged the sky in two", "ultraviolet (UV) bands, far-UV (FUV, {lambda}_eff_~1528{AA}), and", "near-UV (NUV, {lambda}_eff_~2310{AA}), delivering the first", "comprehensive sky surveys at these wavelengths. The GALEX database", "contains FUV and NUV images, ~500 million source measurements and over", "100000 low-resolution UV spectra. The UV surveys are a unique resource", "for statistical studies of hot stellar objects, z<~2 QSOs,", "star-forming galaxies, nebulae and the interstellar medium, and", "provide a roadmap for planning future UV instrumentation and follow-up", "observing programs. We present science-enhanced, \"clean\" catalogs of", "GALEX UV sources, with useful tags to facilitate scientific", "investigations. The catalogs are an improved and expanded version of", "our previous catalogs of UV sources (BCScat). With respect to BCScat,", "we have patched 640 fields for which the pipeline had improperly", "coadded non-overlapping observations, and we provide a version with a", "larger sky coverage (about 10%) by relaxing the restriction to the", "central area of the GALEX field to 1.1{deg} diameter", "(GUVcat_AIS_fov055), as well as the cleaner, more restrictive version", "using only the 1{deg} central portion of each field as in BCScat", "(GUVcat_AIS_fov050). We added new tags to facilitate selection and", "cleaning of statistical samples for science applications: we flag", "sources within the footprint of extended objects (nearby galaxies,", "stellar clusters) so that these regions can be excluded for estimating", "source density. As in our previous catalogs, in GUVcat duplicate", "measurements of the same source are removed, so that each", "astrophysical object has only one entry. Such a unique-source catalog", "is needed to study the density and distributions of sources, and to", "match UV sources with catalogs at other wavelengths. The catalog", "includes all observations from the All-Sky Imaging Survey (AIS), the", "survey with the largest area coverage, with both FUV and NUV detectors", "exposed: over 28700 fields, made up of a total of 57000 observations", "(\"visits\"). The total area covered, when overlaps are removed and gaps", "are accounted for, is 24790 square degrees for GUVcat_AIS_fov055", "(GUVcat_AIS_fov055) and 22125 square degrees for (GUVcat_AIS_fov050).", "The total numbers of \"unique\" AIS sources (eliminating duplicate", "measurements) are 82,992,086 (GUVcat\\_AIS\\_fov055) and 69,772,677", "(GUVcat\\_AIS\\_fov050). The typical depth of the GUVcat_AIS catalog is", "FUV=19.9, NUV=20.8 AB mag."], "doi_pub": ["10.3847/1538-4365/aa7053"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "List of clusters included in the GUVcat footprint ", "columns": [{"name": "ID", "desc": "Source identifier (1) "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "GLON", "desc": "Galactic longitude in decimal degrees (J2000) "}, {"name": "GLAT", "desc": "Galactic latitude in decimal degrees (J2000) "}, {"name": "R1", "desc": "Angular radius of central part of cluster "}, {"name": "o_R1", "desc": "Number of optical cluster stars (most probable) inside R1"}, {"name": "R0", "desc": "Angular radius of core of cluster "}, {"name": "o_R0", "desc": "Number of optical cluster stars (most probable) inside R0"}, {"name": "Class", "desc": "Cluster classification (2) "}, {"name": "Bd", "desc": "Broad type (3) "}, {"name": "St", "desc": "Cluster status (4) "}, {"name": "Type", "desc": "Cluster type (5) "}]}, {"name": "table3.dat", "desc": "List of galaxies larger than 1' included in the GUVcat footprint", "columns": [{"name": "ID", "desc": "Source identifier "}, {"name": "Type", "desc": "Source type (1) "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "v3k", "desc": "Radial velocity (cz) with respect to CMB radiation (2)"}, {"name": "vlg", "desc": "Radial velocity (cz) with respect to Local Group (2)"}, {"name": "PosAng", "desc": "Position angle (2) "}, {"name": "Inc", "desc": "Inclination "}, {"name": "D25", "desc": "D_25_ diameter in units of arcmin "}, {"name": "e_D25", "desc": "Uncertainty in D25 "}, {"name": "R25", "desc": "Axis ratio (major axis / minor axis) "}, {"name": "e_R25", "desc": "Uncertainty in R25 "}]}, {"name": "table4.dat", "desc": "List of AIS GALEX fields used to construct the GUVcat AIS catalog", "columns": [{"name": "ID", "desc": "Field identifier "}, {"name": "RAdeg", "desc": "Center Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Center Declination (J2000) "}, {"name": "GLON", "desc": "Center Galactic longitude "}, {"name": "GLAT", "desc": "Center Galactic latitude "}, {"name": "FUVexp", "desc": "FUV exposure time "}, {"name": "NUVexp", "desc": "NUV exposure time "}, {"name": "CorV", "desc": "Observation type (1) "}]}, {"name": "table5.dat", "desc": "List of AIS eliminated bad coadds, and their associated visits", "columns": [{"name": "C-ID", "desc": "Coadd identifier (1) "}, {"name": "RAdeg", "desc": "Coadd center Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Coadd center Declination (J2000) "}, {"name": "C-GLON", "desc": "Coadd center Galactic longitude "}, {"name": "C-GLAT", "desc": "Coadd center Galactic latitude "}, {"name": "C-FUVexp", "desc": "Coadd FUV exposure time "}, {"name": "C-NUVexp", "desc": "Coadd NUV exposure time "}, {"name": "V-ID", "desc": "Visit identifier "}, {"name": "RAVdeg", "desc": "Visit center Right Ascension (J2000) "}, {"name": "DEVdeg", "desc": "Visit center Declination (J2000) "}, {"name": "V-FUVexp", "desc": "Visit FUV exposure time "}, {"name": "V-NUVexp", "desc": "Visit NUV exposure time "}, {"name": "Dist", "desc": "Angular distance between Coadd and Visit observations"}, {"name": "GUVcat", "desc": "In GUVcat; G=Yes,N=No "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_231_7"}} {"id": "J/ApJS/231/7", "title_cds": "The VISTA-CFHT Stripe 82 NIR survey (VICS82)", "title_create": "Geach+, 2017", "year": "2017", "author": "Geach J.E., Lin Y.-T., Makler M., Kneib J.-P., Ross N.P., Wang W.-H., Hsieh B.-C., Leauthaud A., Bundy K., McCracken H.J., Comparat J., Caminha G.B., Hudelot P., Lin L., Van Waerbeke L., Pereira M.E.S., Mast D.", "title_pub": "VICS82: the VISTA-CFHT Stripe 82 near-infrared survey.", "first_author": "Geach J.E.", "ref_biblio": [""], "bibcode": ["2017ApJS..231....7G"], "keyword_cds": "Surveys; Photometry, infrared", "keyword_pub": "catalogs; infrared: general; surveys", "abstract": ["We present the VISTA-CFHT Stripe 82 (VICS82) survey: a near-infrared", "(J+K_s_) survey covering 150 square degrees of the Sloan Digital Sky", "Survey (SDSS) equatorial Stripe 82 to an average depth of J=21.9 AB", "mag and K_s_=21.4 AB mag (80% completeness limits; 5{sigma}", "point-source depths are approximately 0.5mag brighter). VICS82", "contributes to the growing legacy of multiwavelength data in the", "Stripe 82 footprint. The addition of near-infrared photometry to the", "existing SDSS Stripe 82 coadd ugriz photometry reduces the scatter in", "stellar mass estimates to {delta}log(M_*_)~0.3dex for galaxies with", "M_*_>10^9^M_{sun}_ at z~0.5, and offers improvement compared to", "optical-only estimates out to z~1, with stellar masses constrained", "within a factor of approximately 2.5. When combined with other", "multiwavelength imaging of the Stripe, including moderate-to-deep", "ultraviolet (GALEX), optical and mid-infrared (Spitzer-IRAC) coverage,", "as well as tens of thousands of spectroscopic redshifts, VICS82 gives", "access to approximately 0.5Gpc^3^ of comoving volume. Some of the main", "science drivers of VICS82 include (a) measuring the stellar mass", "function of L^*^ galaxies out to z~1; (b) detecting", "intermediate-redshift quasars at 2<~z<~3.5; (c) measuring the stellar", "mass function and baryon census of clusters of galaxies, and (d)", "performing cross-correlation experiments of cosmic microwave", "background lensing in the optical/near-infrared that link stellar mass", "to large-scale dark matter structure. Here we define and describe the", "survey, highlight some early science results, and present the first", "public data release, which includes an SDSS-matched catalog as well as", "the calibrated pixel data themselves."], "description": ["The VISTA-CFHT Stripe 82 (VICS82) (VICS82) survey is conducted with", "the CFHT WIRCam instrument and with the Visible Infrared Survey", "Telescope for Astronomy (VISTA) VIRCAM instrument in J- and Ks", "broadband filters.", "The VICS82 coverage of Stripe 82 is a near-contiguous ~150deg^2^", "region defined by the boundaries 3hr and 22.2hr in RA and", "-1<{delta}<1deg in DEC."], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/aa74b6"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "vics82.dat", "desc": "*Full VICS82 catalogue limited to Ks<22 AB mag ", "columns": [{"name": "---", "desc": "[VICS82/blah ] 313,883 sources are identified as \"blah\""}, {"name": "VICS82", "desc": "? VICS82 identifier (JHHMMSS.ss+DDMMSS.s)"}, {"name": "RAdeg", "desc": "[4.3e-7/360] Right ascension (J2000) (ALPHA_J2000)"}, {"name": "DEdeg", "desc": "[-1.3/1.3] Declination (J2000) (DELTA_J2000) "}, {"name": "Img", "desc": "Image file name (IMAGE) "}, {"name": "SNR", "desc": "[-164.5/1e+30] Signal to noise ratio (SNR_WIN)"}, {"name": "mag", "desc": "[5.7/36]?=- Total magnitude (MAG_AUTO) "}, {"name": "magAp1", "desc": "[13.2/37]?=- 1\" aperture magnitude (MAG_APER1)"}, {"name": "magAp1.5", "desc": "[12.3/38.5]?=- 1.5\" aperture magnitude (MAG_APER2)"}, {"name": "magAp2", "desc": "[11.7/41.6]?=- 2\" aperture magnitude (MAG_APER3)"}, {"name": "magAp2.5", "desc": "[11.3/40.8]?=- 2.5\" aperture magnitude (MAG_APER4)"}, {"name": "magAp3", "desc": "[11/39.3]?=- 3\" aperture magnitude (MAG_APER5)"}, {"name": "S/G", "desc": "[2e-5/1] S/G classifier output (1=star) (CLASS_STAR)"}, {"name": "Jmag", "desc": "[7/99]?=- J-band total magnitude (JMAG_AUTO) "}, {"name": "JmagAp1", "desc": "[13.5/99]?=- 1\" aperture J-band magnitude (JMAG_APER1)"}, {"name": "JmagAp1.5", "desc": "[12.6/99]?=- 1.5\" aperture J-band magnitude (JMAG_APER2)"}, {"name": "JmagAp2", "desc": "[12/99]?=- 2\" aperture J-band magnitude (JMAG_APER3)"}, {"name": "JmagAp2.5", "desc": "[11.6/99]?=- 2.5\" aperture J-band magnitude (JMAG_APER4)"}, {"name": "JmagAp3", "desc": "[11.2/99]?=- 3\" aperture J-band magnitude (JMAG_APER5)"}, {"name": "JSNR", "desc": "[-689.5/1e+30]?=- Signal to noise ratio in J (JSNR_WIN)"}, {"name": "objID", "desc": "[8647474690320302162/8647475122531011475]?=- VICS82 objID?? (objID)"}, {"name": "RASdeg", "desc": "? SDSS-DR9 right ascension (J2000) (ra) "}, {"name": "DESdeg", "desc": "? SDSS-DR9 declination (J2000) (dec) "}, {"name": "umag0", "desc": "[11.7/38.5]? Dereddened u-band magnitude (dered_u)"}, {"name": "gmag0", "desc": "[9.9/38.8]? Dereddened g-band magnitude (dered_g)"}, {"name": "rmag0", "desc": "[10.7/38]? Dereddened r-band magnitude (dered_r)"}, {"name": "imag0", "desc": "[10.4/42.7]?=- Dereddened i-band magnitude (dered_i)"}, {"name": "zmag0", "desc": "[11/36.7]?=- Dereddened z-band magnitude (dered_z)"}, {"name": "e_umag", "desc": "[0.002/166]? Model magnitude in u filter, AB scale, uncertainty (modelMagErr_u)"}, {"name": "e_gmag", "desc": "[0.001/192]? Model magnitude in g filter, AB scale, uncertainty (modelMagErr_g)"}, {"name": "e_rmag", "desc": "[0.001/254]? Model magnitude in r filter, AB scale, uncertainty (modelMagErr_r)"}, {"name": "e_imag", "desc": "[0.001/66]?=- Model magnitude in i filter, AB scale, uncertainty (modelMagErr_i)"}, {"name": "e_zmag", "desc": "[0.001/181]?=- Model magnitude in z filter, AB scale, uncertainty (modelMagErr_z)"}, {"name": "SDSS9", "desc": "SDSS DR9 IAU name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "DESdeg2", "desc": "? SDSS DR9 declination (J2000) (DEdeg) "}, {"name": "cl", "desc": "[0/6]?=- Class (1) "}, {"name": "q_mode", "desc": "[0/1] 1 (ou 0??) SDSS clean photometry flag "}, {"name": "flags", "desc": "Flags "}, {"name": "Q", "desc": "[3]?=- Quality of the observation: 3=good (Always \"3\" or blank)"}, {"name": "ObsDate", "desc": "[1998.72/2009.71]? Observing date in decimal years"}, {"name": "pmRA", "desc": "[-727/823]?=- SDSS proper motion in RA "}, {"name": "e_pmRA", "desc": "[2/183]?=- pmRA uncertainty "}, {"name": "pmDE", "desc": "[-1163/920]?=- SDSS proper motion in DEC "}, {"name": "e_pmDE", "desc": "[2/183]?=- pmDE uncertainty "}, {"name": "SpObjID", "desc": "[0/4920432000009434112]?=- SDSS-DR9 SpObjID "}, {"name": "zsp", "desc": "[-0.011/7.1]? SDSS spectroscopic redshift "}, {"name": "e_zsp", "desc": "[-6/10]? Redshift uncertainty "}, {"name": "f_zsp", "desc": "[0/134]?=- Flag on zsp (2) "}, {"name": "spType", "desc": "SDSS source type (3) "}, {"name": "spCl", "desc": "SDSS spectroscopic class (class): GALAXY (69,016 sources),"}, {"name": "sources)", "desc": "or "}, {"name": "sources)", "desc": " "}, {"name": "subClass", "desc": "SDSS spectroscopic subclass (subClass) (4) "}, {"name": "Sep", "desc": "[0.00014/2]? Separation between VICS82 and SDSS DR9 source (angDist)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_234_26"}} {"id": "J/ApJS/234/26", "title_cds": "Short Title", "title_create": "Li+, 2018", "year": "2018", "author": "Li L., Wang Y., Shao L., Wu X.-F., Huang Y.-F., Zhang B., Ryde F., Yu H.-F.", "title_pub": "A large catalog of multiwavelength GRB afterglows. I. Color evolution and its physical implication.", "first_author": "Li L.", "ref_biblio": [""], "bibcode": ["2018ApJS..234...26L"], "see_also": ["J/ApJ/672/449 : GRB 061126 light curves (Perley+, 2008)", "J/ApJ/691/723 : BVIJHKs observations of GRB 080319B (Bloom+, 2009)", "J/ApJ/693/1484 : Early optical afterglow catalog (Cenko+, 2009)", "J/AJ/137/4517 : UVOT light curves of supernovae (Brown+, 2009)", "J/ApJ/702/226 : Swift/UVOT panchromatic obs. of SN 2008D (Modjaz+, 2009)", "J/ApJ/702/489 : ROTSE obs. of gamma-ray burst afterglows (Rykoff+, 2009)", "J/A+A/508/593 : GRB 080710 bright optical/NIR afterglow (Kruehler+, 2009)", "J/MNRAS/406/2473 : Photometry of GRB 071025 (Perley+, 2010)", "J/ApJ/720/862 : Afterglow light curve of GRB 090926A (Rau+, 2010)", "J/ApJ/720/1513 : The afterglows of Swift-era GRBs. I. (Kann+, 2010)", "J/AJ/141/36 : GRB 080607 multi-band light curves (Perley+, 2011)", "J/AJ/141/163 : Ultimate LC of SN 1998bw/GRB 980425 (Clocchiatti+, 2011)", "J/A+A/531/A39 : g'r'i'z'JHKs light curves of GRB 081029 (Nardini+, 2011)", "J/A+A/535/A57 : g'r'i'z'JH light curves of GRB 091127 (Filgas+, 2011)", "J/ApJ/743/154 : Multi-band photom. of GRB 110205A + 110213A (Cucchiara+, 2011)", "J/MNRAS/421/2692 : Optical/near-IR obs. of GRB 080310 (Littlejohns+, 2012)", "J/MNRAS/426/2 : GRB 091018 Optical/NIR photometry (Wiersema+, 2012)", "J/A+A/557/A18 : GRB 120815A afterglow spectra (Kruehler+, 2013)", "J/A+A/560/A70 : GRB 100621A unusual afterglow (Greiner+, 2013)", "J/ApJ/781/37 : Multi-band photometry of GRB 130427A (Perley+, 2014)", "J/A+A/562/A29 : GRB 100814A GROND and UVOT light curves (Nardini+, 2014)", "J/A+A/568/A19 : Photometry of 3 {gamma}-ray burst supernovae (Cano+, 2014)", "J/A+A/568/A75 : GRB 130925A GROND light curves (Greiner+, 2014)", "J/A+A/607/A29 : GRB 120327A afterglow colour variations (Melandri+, 2017)", "http://gcn.gsfc.nasa.gov/ : GCN: The Gamma-ray Coordinates Network home page"], "keyword_cds": "GRB ; Colors ; Optical ; Infrared", "keyword_pub": "methods: statistical; stars: gamma-ray burst; ISM: dust, extinction", "abstract": ["The spectrum of gamma-ray burst (GRB) afterglows can be studied with", "color indices. Here, we present a large comprehensive catalog of 70", "GRBs with multiwavelength optical transient data on which we perform a", "systematic study to find the temporal evolution of color indices. We", "categorize them into two samples based on how well the color indices", "are evaluated. The Golden sample includes 25 bursts mostly observed by", "GROND, and the Silver sample includes 45 bursts observed by other", "telescopes. For the Golden sample, we find that 96% of the color", "indices do not vary over time. However, the color indices do vary", "during short periods in most bursts. The observed variations are", "consistent with effects of (i) the cooling frequency crossing the", "studied energy bands in a wind medium (43%) and in a constant-density", "medium (30%), (ii) early dust extinction (12%), (iii) transition from", "reverse-shock to forward-shock emission (5%), or (iv) an emergent SN", "emission (10%). We also study the evolutionary properties of the mean", "color indices for different emission episodes. We find that 86% of the", "color indices in the 70 bursts show constancy between consecutive", "ones. The color index variations occur mainly during the late GRB-SN", "bump, the flare, and early reverse-shock emission components. We", "further perform a statistical analysis of various observational", "properties and model parameters (spectral index {beta}_o_^CI^,", "electron spectral indices p^CI^, etc.) using color indices. Overall,", "we conclude that ~90% of colors are constant in time and can be", "accounted for by the simplest external forward-shock model, while the", "varying color indices call for more detailed modeling."], "description": ["We extensively compiled as many optical/near-IR (NIR) photometric data", "as possible, detected by ground-based telescopes from both pre-Swift-", "and Swift-era afterglows. We collected observational data from", "published papers and the Gamma-ray Burst Coordinates Networks Circular", "Service (GCN). A total of 70 bursts satisfy our selection criteria", "(from 1997 February 28 to 2015 December)."], "doi_pub": ["10.3847/1538-4365/aaa02a"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Properties of the GRB sample with multicolor light curves", "columns": [{"name": "GRB", "desc": "GRB name (YYMMDDA) "}, {"name": "Filt", "desc": "Filters "}, {"name": "E(B-V)", "desc": "[0.008/1] Galaxy color excess "}, {"name": "beta0", "desc": "[0.1/1.4]? Spectral index {beta}_0_ "}, {"name": "e_beta0", "desc": "[0/0.5]? beta0 uncertainty "}, {"name": "l_Av", "desc": "Limit flag on Av "}, {"name": "Av", "desc": "[0/5]? Host galaxy extinction "}, {"name": "e_Av", "desc": "[0.01/20.6]? Av uncertainty "}, {"name": "f_Av", "desc": "[a] a: Range 0.3-1.5 for 111209A "}, {"name": "r_Av", "desc": "Reference for Av (see refs.dat file) "}, {"name": "z", "desc": "[0.007/5.2]? Redshift "}, {"name": "r_z", "desc": "Reference for z (see refs.dat file) "}, {"name": "Ref", "desc": "References for data sources (see refs.dat file) "}]}, {"name": "table2.dat", "desc": "Color indices of the Golden sample ", "columns": [{"name": "GRB", "desc": "GRB name (YYMMDDA) "}, {"name": "m_GRB", "desc": "[0/4] Components within time sequence (1) "}, {"name": "Comp", "desc": "Component (2) "}, {"name": "Epoch", "desc": "The time intervals for each component in the observer frame"}, {"name": "Model", "desc": "Model of the light-curve fits for each component"}, {"name": "g-r", "desc": "[-0.2/1.4]? g-r color index "}, {"name": "e_g-r", "desc": "[0.01/0.5]? g-r uncertainty "}, {"name": "r-i", "desc": "[-1.1/0.5]? r-i color index "}, {"name": "e_r-i", "desc": "[0.01/2.3]? r-i uncertainty "}, {"name": "i-z", "desc": "[-0.8/0.6]? i-z color index "}, {"name": "e_i-z", "desc": "[0.01/1.9]? i-z uncertainty "}, {"name": "J-H", "desc": "[-0.4/0.7]? J-H color index "}, {"name": "e_J-H", "desc": "[0.02/2]? J-H uncertainty "}, {"name": "H-Ks", "desc": "[-0.04/0.9]? H-Ks color index "}, {"name": "e_H-Ks", "desc": "[0.02/0.8]? H-Ks uncertainty "}]}, {"name": "table3.dat", "desc": "Color indices of the Silver sample ", "columns": [{"name": "GRB", "desc": "GRB name (YYMMDDA) "}, {"name": "m_GRB", "desc": "[0/3] Components within time sequence (1) "}, {"name": "Comp", "desc": "Component (2) "}, {"name": "Epoch", "desc": "The time intervals for each component in the observer frame"}, {"name": "Model", "desc": "Model of the light-curve fits for each component"}, {"name": "W2-M2", "desc": "[-0.6/1.5]? UVW2-UVM2 color index "}, {"name": "e_W2-M2", "desc": "[0.1/1.2]? W2-M2 uncertainty "}, {"name": "M2-W1", "desc": "[-1.1/0.6]? UVM2-UVW1 color index "}, {"name": "e_M2-W1", "desc": "[0.1/3]? M2-W1 uncertainty "}, {"name": "W1-U", "desc": "[0.1/2]? UVW1-U color index "}, {"name": "e_W1-U", "desc": "[0.1/3]? W1-U uncertainty "}, {"name": "U-B", "desc": "[-1.6/2.4]? U-B color index "}, {"name": "e_U-B", "desc": "[0.07/1.1]? U-B uncertainty "}, {"name": "B-V", "desc": "[-0.8/1.5]? B-V color index "}, {"name": "e_B-V", "desc": "[0.06/0.6]? B-V uncertainty "}, {"name": "V-R", "desc": "[-0.7/1.4]? V-R color index "}, {"name": "e_V-R", "desc": "[0.08/0.5]? V-R uncertainty "}, {"name": "R-I", "desc": "[-0.6/1.4]? R-I color index "}, {"name": "e_R-I", "desc": "[0.08/0.8]? R-I uncertainty "}, {"name": "I-J", "desc": "[-0.9/3.1]? I-J color index "}, {"name": "e_I-J", "desc": "[0.05/0.5]? I-J uncertainty "}, {"name": "J-H", "desc": "[-0.4/0.7]? J-H color index "}, {"name": "e_J-H", "desc": "[0.09/0.3]? J-H uncertainty "}, {"name": "H-K", "desc": "[-0.4/1.6]? H-K color index "}, {"name": "e_H-K", "desc": "[0.09/0.4]? H-K uncertainty "}]}, {"name": "table7.dat", "desc": "Color indices and their relation spectral indices for the Golden samples", "columns": [{"name": "GRB", "desc": "Gamma-ray burst identifier (YYMMDDA) "}, {"name": "Time(g-r)", "desc": "[0.1/29200]? The (g-r) color time window (1) "}, {"name": "g-r", "desc": "[-0.3/1.7]? The (g-r) color index "}, {"name": "e_g-r", "desc": "[0.01/0.8]? Uncertainty in g-r "}, {"name": "beta(g-r)", "desc": "[-0.7/5.6]? Spectral index of (g-r) color "}, {"name": "e_beta(g-r)", "desc": "[0.02/2.6]? Uncertainty in beta(g-r) "}, {"name": "Time(r-i)", "desc": "[0.1/29200]? The (r-i) color time window (1) "}, {"name": "r-i", "desc": "[-1.1/1.3]? The (r-i) color index "}, {"name": "e_r-i", "desc": "[0.01/2.3]? Uncertainty in r-i "}, {"name": "beta(r-i)", "desc": "[-5/6.2]? Spectral index of (r-i) color "}, {"name": "e_beta(r-i)", "desc": "[0.03/11]? Uncertainty in beta(r-i) "}, {"name": "Time(i-z)", "desc": "[0.1/29200]? The (i-z) color time window (1) "}, {"name": "i-z", "desc": "[-0.8/1.3]? The (i-z) color index "}, {"name": "e_i-z", "desc": "[0.01/2]? Uncertainty in i-z "}, {"name": "beta(i-z)", "desc": "[-4.3/7]? Spectral index of (i-z) color "}, {"name": "e_beta(i-z)", "desc": "[0.03/9.6]? Uncertainty in beta(i-z) "}, {"name": "Time(J-H)", "desc": "[0.1/2400]? The (J-H) color time window (1) "}, {"name": "J-H", "desc": "[-0.7/1.4]? The (J-H) color index "}, {"name": "e_J-H", "desc": "[0.03/3]? Uncertainty in J-H "}, {"name": "beta(J-H)", "desc": "[-2.3/4.5]? Spectral index of (J-H) color "}, {"name": "e_beta(J-H)", "desc": "[0.1/9.8]? Uncertainty in beta(J-H) "}, {"name": "Time(H-Ks)", "desc": "[0.1/1880]? The (H-K_s_) color time window (1) "}, {"name": "H-Ks", "desc": "[-0.5/2]? The (H-K_s_) color index "}, {"name": "e_H-Ks", "desc": "[0.04/1.1]? Uncertainty in H-Ks "}, {"name": "beta(H-Ks)", "desc": "[-1.4/5.7]? Spectral index of (H-Ks) color "}, {"name": "e_beta(H-Ks)", "desc": "[0.1/3.2]? Uncertainty in beta(H-Ks) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_236_31"}} {"id": "J/ApJS/236/31", "title_cds": "H2O & class I CH3OH masers toward red MSX sources", "title_create": "Kim+, 2018", "year": "2018", "author": "Kim C.-H., Kim K.-T., Park Y.-S.", "title_pub": "Simultaneous survey of water and class I methanol masers toward red MSX sources.", "first_author": "Kim C.-H.", "ref_biblio": [""], "bibcode": ["2018ApJS..236...31K"], "see_also": ["V/114 : MSX6C Infrared Point Source Catalog (Egan+ 2003)", "J/other/PPMtO/14.185 : Purple Mountain H_2_O maser atlas (Han+ 1995)", "J/AZh/72/22 : A 95 GHz Survey of Methanol Masers (Valtts+, 1995)", "J/A+AS/127/181 : H2O maser sources new detections (Han+ 1998)", "J/A+A/368/845 : Arcetri updated cat. of H2O masers (Valdettaro+, 2001)", "J/ApJ/581/325 : NGC 2071 water masers (Seth+, 2002)", "J/A+A/417/615 : Maser and outflows in UC HII region (Codella+, 2004)", "J/ApJS/155/149 : CH_3_OH 7_0_-6_1_ A^+^ maser sources (Kurtz+, 2004)", "J/A+A/428/1019 : Rest frequencies of methanol maser lines (Mueller+, 2004)", "J/MNRAS/359/1498 : Class I and class II methanol masers (Ellingsen+, 2005)", "J/A+A/434/613 : Water maser survey of methanol masers (Szymczak+, 2005)", "J/ApJ/641/389 : Millimetric observations of IRDC cores (Rathborne+, 2006)", "J/ApJ/651/L125 : H2O masers associated with IR dark cloud cores (Wang+, 2006)", "J/PASJ/59/1185 : Water maser in galactic IRAS sources (Sunada+, 2007)", "J/AZh/84/579 : Catalog of Class I methanol masers (Val'tts+, 2007)", "J/A+A/487/993 : MAMBO Mapping of c2d Clouds and Cores (Kauffmann+, 2008)", "J/other/PASA/26.454 : Precise positions of methanol masers (Caswell, 2009)", "J/ApJ/702/1615 : CH_3_OH maser survey of EGOs (Cyganowski+, 2009)", "J/A+A/501/539 : RMS survey. 6cm observations of YSOs (Urquhart+, 2009)", "J/ApJ/706/83 : Embedded YSO candidates in W51 (Kang+, 2009)", "J/MNRAS/416/178 : 1.2-mm dust clumps with luminous water masers (Breen+, 2011)", "J/ApJS/196/9 : Methanol maser survey toward GLIMPSE EGOs (Chen+, 2011)", "J/MNRAS/418/1689 : Red MSX water maser and ammonia emissions (Urquhart+, 2011)", "J/AZh/89/611 : Class I methanol maser catalog (Bayandina+, 2012)", "J/ApJS/200/5 : 95GHz class I methanol maser survey (Chen+, 2012)", "J/ApJS/206/9 : New EGOs from Spitzer GLIMPSE II survey. I. (Chen+, 2013)", "J/A+A/552/A40 : MSX high-contrast IRDCs with NH_3_ (Chira+, 2013)", "J/A+A/549/A45 : ATLASGAL Compact Source Catalog: 33030km/s) features in 27 H_2_O maser sources. The 95GHz", "maser emission is detected only in 44GHz maser sources. The two", "transitions show strong correlations in the peak velocity, peak flux", "density, and isotropic maser luminosity, indicating that they are", "likely generated in the same sites by the same mechanisms. The 44GHz", "masers have much narrower distributions than 22GHz masers in the", "relative peak velocity and velocity range, while 6.7GHz class II", "CH_3_OH masers have distributions intermediate between the two. The", "maser luminosity significantly correlates with the parental clump", "mass, while it correlates well with the bolometric luminosity of the", "central protostar only when data of the low-mass regime from the", "literature are added. Comparison with the results of previous maser", "surveys toward massive star-forming regions suggests that the", "detection rates of 22 and 44GHz masers tend to increase as the central", "objects evolve. This is contrary to the trends found in low- and", "intermediate-mass star-forming regions. Thus, the occurrence of both", "masers might depend on the surrounding environments as well as on the", "evolution of the central object."], "description": ["We surveyed 299 Red MSX Source (RMS; see Lumsden+, 2002MNRAS.336..621L", "2013, J/ApJS/208/11 and Urquhart+, 2014, J/MNRAS/437/1791) high-mass", "protostellar object (HMPO) candidates in three maser transitions:", "H_2_O 616-523 (22.235080GHz), CH_3_OH 70-61 A+ (44.069430GHz), and", "80-71 A+ (95.169463GHz). The observations were undertaken using the", "Korean VLBI Network (KVN) 21m telescopes from 2011 April to 2014 May.", "The FWHMs of the telescopes were about 130\" at 22GHz, 65\" at 44GHz,", "and 32\" at 95GHz. The pointing accuracy was better than 5\".", "We also surveyed 10 sources in our sample in the ^13^CO J=1-0 and", "HCO^+^ J=1-0 lines in 2013 June. The 13CO line observations were", "conducted with the Taeduk Radio Astronomy Observatory (TRAO) 14m", "telescope, while the HCO^+^ line observations were made with the KVN", "telescope at the Tamna station."], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/aab88f"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Summary of target sources ", "columns": [{"name": "ID", "desc": "[4/4954] Red MSX source identifier "}, {"name": "f_ID", "desc": "Flag on ID (1) "}, {"name": "MSX", "desc": "MSX identifier (GLLL.llll+BB.bbbbA) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Dist", "desc": "Distance "}, {"name": "Lbol", "desc": "[132/310000]? Bolometric luminosity "}, {"name": "Vsys", "desc": "[-88.6/113.6]? RMS archive systemic velocity "}, {"name": "Det22?", "desc": "Detection at 22 GHz? (2) "}, {"name": "f_Det22?", "desc": "Flag(s) on Det22? (3) "}, {"name": "Det44?", "desc": "Detection at 44 GHz? (2) "}, {"name": "f_Det44?", "desc": "Flag(s) on Det22? (3) "}, {"name": "Det95?", "desc": "Detection at 95 GHz? (2) "}, {"name": "f_Det95?", "desc": "Flag on Det22? (3) "}, {"name": "MMB", "desc": "MMB coverage? (y)es "}]}, {"name": "table4.dat", "desc": "Detected maser line parameters ", "columns": [{"name": "ID", "desc": "[4/4941] Red MSX source identifier "}, {"name": "Freq", "desc": "[6.7/95] Frequency of maser detection "}, {"name": "Date", "desc": "Date of the observation "}, {"name": "YS", "desc": "Station code (1) "}, {"name": "Vp", "desc": "[-96.4/125.8]? Velocity peak "}, {"name": "Sp", "desc": "[0.8/4552.1]? Peak flux density in Freq "}, {"name": "IntSnudv", "desc": "[0.2/14832.7] Integrated flux density "}, {"name": "Vmin", "desc": "[-109.5/122.4]? Minimum velocity of maser line "}, {"name": "Vmax", "desc": "[-91.8/150.8]? Maximum velocity of maser line "}, {"name": "Vrange", "desc": "[0.2/230.7]? Velocity range of maser line "}, {"name": "Lmaser", "desc": "[9.3e-09/0.01] Isotropic maser luminosity "}, {"name": "Notes", "desc": "Additional notes (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_239_14"}} {"id": "J/ApJS/239/14", "title_cds": "", "title_create": "Johns+, 2018", "year": "2018", "author": "Johns D., Marti C., Huff M., McCann J., Wittenmyer R.A., Horner J., Wright D.J.", "title_pub": "Revised exoplanet radii and habitability using Gaia Data Release 2.", "first_author": "Johns D.", "ref_biblio": [""], "bibcode": ["2018ApJS..239...14J"], "see_also": ["I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "J/A+A/375/L27 : HD 80606b, planet on an very elongated orbit (Naef+ 2001)", "J/A+A/491/889 : CoRoT-Exo-3b observations (Deleuil+, 2008)", "J/A+A/480/L33 : Radial velocities of HD 4113 and HD 156846 (Tamuz+, 2008)", "J/A+A/507/487 : GJ 581 radial velocity curve (Mayor+, 2009)", "J/A+A/523/A15 : HARPS XXIII: RV data for the 8 targets (Naef+, 2010)", "J/ApJ/761/123 : KELT-1 photometry and spectroscopy follow-up (Siverd+, 2012)", "J/ApJ/761/123 : KELT-1 photometry and spectroscopy follow-up (Siverd+, 2012)", "J/AJ/145/5 : Follow-up photometry of HATS-1 (Penev+, 2013)", "J/A+A/562/L3 : WASP-103b radial velocities and light curves (Gillon+, 2014)", "J/ApJS/210/20 : Small Kepler planets radial velocities (Marcy+, 2014)", "J/MNRAS/452/2127 : Fundamental param. of Kepler stars (Silva Aguirre+, 2015)", "J/AJ/152/105 : Kepler-80 transit timing observations (MacDonald+, 2016)", "J/AJ/153/211 : Differential photometry of F-subgiant HAT-P-67 (Zhou+, 2017)", "J/A+A/613/A25 : Radial velocity for Ross 128 (Bonfils+, 2018)"], "keyword_cds": "", "keyword_pub": "astrobiology ; planets and satellites: fundamental parameters ; planets and satellites: general ; catalogs ; surveys ; planets and satellites: fundamental parameters", "abstract": ["Accurate stellar properties are crucial for determining exoplanet", "characteristics. Gaia DR2 presents revised distances, luminosities,", "and radii for 1.6 billion stars. Here, we report the calculation of", "revised radii and densities for 320 non-Kepler exoplanets using this", "data and present updated calculations of the incident flux received by", "690 known exoplanets. This allows us to reassess the likelihood that", "those planets orbit in the habitable zone of their host stars. As a", "result of this analysis, three planets can be added to the catalog of", "potentially habitable worlds: HIP 67537b, HD 148156b, and HD 106720b.", "In addition, the changed parameterization of BD +49 898 means that its", "planet, BD +49 898b, now receives an incident flux that places it", "outside the optimistic habitable zone region, as defined by Kopparapu", "et al. We find that use of the new Gaia data results in a mean", "increase in the calculated exoplanet radius of 3.76%. Previously,", "CoRoT-3 b had been reported as having the highest density of all known", "exoplanets. Here, we use updated information to revise the calculated", "density of CoRoT-3 b from 26.4 to 16.1+/-3.98g/cm^3^. We also report", "the densest exoplanet in our data set, KELT-1 b, with a density of", "22.1_-9.16_^+5.62^g/cm^3^. Overall, our results highlight the", "importance of ensuring the parameterizations of known exoplanets are", "revisited whenever significant improvements are made to the precision", "of the stellar parameters upon which they are based."], "doi_pub": ["10.3847/1538-4365/aae5fb"], "orcid_pub": ["0000-0001-6311-8629"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Host star properties; all parameters are taken from Gaia DR2", "columns": [{"name": "Host", "desc": "Host name "}, {"name": "Lum", "desc": "[0.04/1244.2]? Host luminosity, solar units "}, {"name": "E_Lum", "desc": "[0/97.2]? Upper uncertainty in Lum "}, {"name": "e_Lum", "desc": "[-97.2/0]? Lower uncertainty in Lum "}, {"name": "Rad", "desc": "[0.5/78.2]? Host radius, solar units "}, {"name": "E_Rad", "desc": "[0.003/8.5]? Upper uncertainty in Rad "}, {"name": "e_Rad", "desc": "[-13.2/-0.003]? Lower uncertainty in Rad "}, {"name": "Teff", "desc": "[3382/9435] Host effective temperature "}]}, {"name": "table3.dat", "desc": "Revised properties of exoplanets ", "columns": [{"name": "Planet", "desc": "Planet Name "}, {"name": "Rad", "desc": "[0.1/2.9]? Planet Radius "}, {"name": "E_Rad", "desc": "[0.01/1.8]? Upper uncertainty in Rad "}, {"name": "e_Rad", "desc": "[-1.8/-0.01]? Lower uncertainty in Rad "}, {"name": "Mass", "desc": "[0.01/55.6]? Planet Mass (1) "}, {"name": "E_Mass", "desc": "[0/78.6]? Upper uncertainty in Mass "}, {"name": "e_Mass", "desc": "[-78.6/0]? Lower uncertainty in Mass "}, {"name": "rho", "desc": "[0.04/26]? Planet Density "}, {"name": "E_rho", "desc": "[0.01/27.1]? Upper uncertainty in rho "}, {"name": "e_rho", "desc": "[-27/-0.01]? Lower uncertainty in rho "}, {"name": "a", "desc": "[0.01/773]? Semi-major axis (1) "}, {"name": "E_a", "desc": "[0/30]? Upper uncertainty in a "}, {"name": "e_a", "desc": "[-30/0]? Lower uncertainty in a "}, {"name": "Sinc", "desc": "[0/19317]? Planet Incident Flux "}, {"name": "E_Sinc", "desc": "[0/3395]? Upper uncertainty in Sinc "}, {"name": "e_Sinc", "desc": "[-3388/0]? Lower uncertainty in Sinc "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_239_29"}} {"id": "J/ApJS/239/29", "title_cds": "Short Title", "title_create": "Peralta+, 2018", "year": "2018", "author": "Peralta J., Muto K., Hueso R., Horinouchi T., Sanchez-lavega A., Murakami S.-Y., Machado P., Young E.F., Lee Y.J., Kouyama T., Sagawa H., Mcgouldrick K., Satoh T., Imamura T., Limaye S.S., Sato T.M., Ogohara K., Nakamura M., Luz D.", "title_pub": "Nightside winds at the lower clouds of Venus with Akatsuki/IR2: longitudinal, local time, and decadal variations from comparison with previous measurements.", "first_author": "Peralta J.", "ref_biblio": [""], "bibcode": ["2018ApJS..239...29P"], "keyword_cds": "", "keyword_pub": "planets and satellites: atmospheres planets and satellites: terrestrial planets", "mission": "", "abstract": ["We present measurements of the wind speeds at the nightside lower clouds of Venus from observations by JAXA's mission Akatsuki during 2016, complemented by new wind measurements from ground-based observations acquired with the TNG/Near Infrared Camera Spectrometer (NICS) in 2012 and IRTF/SpeX in 2015 and 2017. The zonal and meridional components of the winds were measured via cloud tracking on a total of 466 Akatsuki images of Venus acquired by the camera IR2 using the 2.26 {mu}m filter, with spatial resolutions ranging from 10 to 80 km per pixel and covering 2016 March 22 to October 31. More than 149,000 wind vectors were obtained using an automatic template-matching technique, and 2947 wind vectors were inferred using a manual procedure. The meridional profiles for both components of the winds are found to be consistent with results from the Venus Express mission during 2006-2008, although stronger wind variability is found for the zonal component at equatorial latitudes where Akatsuki observations have better viewing geometry than Venus Express. The zonal winds at low latitudes also suggest a zonal variability that could be associated with solar tides or vertically propagating orographic waves. Finally, the combination of our wind measurements from TNG/NICS, IRTF/SpeX, and Akatsuki images with previously published data from 1978 to 2017 suggests variations of up to 30 m s^-1^ in the winds at the nightside lower clouds of Venus."], "object": [], "curator": "Emmanuelle Perret [CDS]", "doi_pub": ["10.3847/1538-4365/aae844"], "orcid_pub": ["0000-0002-6823-1695"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_239_33"}} {"id": "J/ApJS/239/33", "title_cds": "Radio-loud AGNs sample from literature", "title_create": "Yuan+, 2018", "year": "2018", "author": "Yuan Z., Wang J., Worrall D.M., Zhang B.-B., Mao J.", "title_pub": "Determining the core radio luminosity function of radio AGNs via copula.", "first_author": "Yuan Z.", "ref_biblio": [""], "bibcode": ["2018ApJS..239...33Y"], "see_also": ["VIII/36 : The Second Bologna Survey (Colla+ 1970-1974)", "VIII/2 : Molonglo Reference Catalog of Radio Sources (Large+ 1981)", "VIII/37 : The Third Bologna Survey (B3) (Ficarra+ 1985)", "VIII/22 : 6C Survey of Radio Sources - III. (Hales+ 1990)", "VIII/16 : Molonglo Reference Catalogue of Radio Sources (Large+ 1991)", "VIII/17 : The North 20cm Survey (White+ 1992)", "VIII/42 : Texas Survey of radio sources at 365MHz (Douglas+ 1996)", "VIII/38 : The Parkes-MIT-NRAO 4.85GHz (PMN) Surveys (Griffith+ 1993-1996)", "VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)", "J/MNRAS/268/602 : Compact radio cores in radio galaxies. (Jones+, 1994)", "J/A+A/298/375 : Jet-disk symbiosis II (Falcke+ 1995)", "J/ApJ/448/521 : Radio powers in radio galaxies (Zirbel+, 1995)", "J/A+AS/132/31 : Kinematical models for double radio sources (Nilsson 1998)", "J/ApJS/124/285 : VLA Images of Extragalactic Objects (Reid+, 1999)", "J/A+A/381/757 : List of extra-galactic radio jets (Liu+, 2002)", "J/MNRAS/371/898 : Extragalactic radio sources selected at 20GHz (Sadler+, 2006)", "J/AJ/138/1874 : MOJAVE. VI. Kinematic analysis of blazar jets (Lister+, 2009)", "J/MNRAS/402/2403 : Australia Telescope 20GHz Survey Cat. AT20G (Murphy+, 2010)", "J/MNRAS/416/1900 : CENSORS + other 1.4GHz sources (Rigby+, 2011)", "J/ApJ/744/84 : Combined sample of radio-loud AGNs at 408MHz (Yuan+, 2012)", "J/MNRAS/429/2080 : Lockman Hole 10C radio spectral indices (Whittam+ 2013)", "J/ApJ/780/73 : Redshifts of BL Lac objects from Fermi (Ajello+, 2014)", "J/MNRAS/445/955 : Radio-AGN feedback for 0.5"], "bibcode": ["2019ApJS..240...34M"], "see_also": ["II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)", "VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)", "J/MNRAS/362/9 : Radio-loud AGN in SDSS (Best+, 2005)", "J/AJ/133/2097 : FIRST \"Winged\" & X-shaped radio source cand. (Cheung, 2007)", "J/MNRAS/390/819 : Combined NVSS-FIRST Galaxies (CoNFIG) sample (Gendre+, 2008)", "J/MNRAS/404/1719 : CoNFIG sample. II (Gendre+, 2010)", "J/ApJ/723/1119 : Optical properties of radio galaxies at z<0.3 (Lin+, 2010)", "J/ApJS/194/31 : Morphology for groups in the FIRST database (Proctor, 2011)", "J/AJ/141/88 : Galaxy cluster environments of radio sources (Wing+, 2011)", "J/MNRAS/421/1569 : Properties of 18286 SDSS radio galaxies (Best+, 2012)", "J/ApJS/230/20 : Machine learning technique to classify CoNFIG gal.", "J/A+A/601/A81 : FIRST catalog of FR II radio galaxies (Capetti+, 2017)", "J/A+A/598/A49 : FRICAT FIRST catalog of FRI radio galaxies (Capetti+, 2017)", "J/A+A/608/A39 : X-ATLAS X-ray sources photom. redshifts (Mountrichas+, 2017)", "J/A+A/609/A1 : FR0CAT. a FIRST catalog of FR0 radio galaxies (Baldi+, 2018)", "http://sundog.stsci.edu/ : The VLA FIRST survey home page"], "keyword_cds": "Active gal. nuclei; Morphology; Radio sources; Galaxy catalogs", "keyword_pub": "catalogs ; galaxies: statistics ; methods: data analysis ; radio continuum: galaxies ; techniques: miscellaneous", "abstract": ["We present a morphological classification of 14245 radio active", "galactic nuclei (AGNs) into six types, i.e., typical Fanaroff-Riley", "Class I/II (FRI/II), FRI/II-like bent-tailed, X-shaped radio galaxy,", "and ringlike radio galaxy, by designing a convolutional neural network", "based autoencoder, namely MCRGNet, and applying it to a labeled radio", "galaxy (LRG) sample containing 1442 AGNs and an unlabeled radio galaxy", "(unLRG) sample containing 14245 unlabeled AGNs selected from the", "Best-Heckman sample (2012, J/MNRAS/421/1569). We train MCRGNet and", "implement the classification task by a three-step strategy, i.e.,", "pre-training, fine-tuning, and classification, which combines both", "unsupervised and supervised learnings. A four-layer dichotomous tree", "is designed to classify the radio AGNs, which leads to a significantly", "better performance than the direct six-type classification. On the LRG", "sample, our MCRGNet achieves a total precision of ~93% and an averaged", "sensitivity of ~87%, which are better than those obtained in previous", "works. On the unLRG sample, whose labels have been human-inspected,", "the neural network achieves a total precision of ~80%. Also, using", "Sloan Digital Sky Survey Data Release 7 to calculate the r-band", "absolute magnitude (Mopt) and using the flux densities to calculate", "the radio luminosity (Lradio), we find that the distributions of the", "unLRG sources on the Lradio-Mopt plane do not show an apparent", "redshift evolution and could confirm with a sufficiently large sample", "that there could not exist an abrupt separation between FRIs and FRIIs", "as reported in some previous works."], "description": ["All the images of the radio AGNs included in both the unlabeled sample", "(unlabeled radio galaxy sample or unLRG sample) and the labeled sample", "(LRG sample) are drawn from the Very Large Array (VLA) FIRST survey", "archive at http://sundog.stsci.edu/"], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/aaf9a2"], "orcid_pub": ["0000-0003-1263-9453"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table3.dat", "desc": "1442 labeled radio galaxies (LRGs) in the LRG sample ", "columns": [{"name": "Name", "desc": "Source name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "RAh", "desc": "Right ascension in decimal hours (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "z", "desc": "[0.006/3.9]? Spectroscopic redshift "}, {"name": "S1.4", "desc": "[6/14903]? NVSS 1.4GHz integrated flux density "}, {"name": "r_Name", "desc": "Original catalog of the source (1) "}, {"name": "BH12", "desc": "[0/1] Flag of source in the BH12 (Best & Heckman, 2012, J/MNRAS/421/1569) samples"}, {"name": "Type-Lit", "desc": "Morphology type labeled in literature (G1) "}, {"name": "Type-CNN", "desc": "Morphology type labeled by MCRGNet (G1) "}, {"name": "BT-Type", "desc": "Subtype label for BT sample (G2) "}, {"name": "Prob", "desc": "[0.77/1] Probability of classification by MCRGNet"}]}, {"name": "table4.dat", "desc": "14245 unlabeled radio AGNs (unLRG) in the unLRG sample", "columns": [{"name": "Name", "desc": "Source name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "RAh", "desc": "Right ascension in decimal hours (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "z", "desc": "[0.015/0.7] Spectroscopic redshift "}, {"name": "S1.4", "desc": "[5/22721] NVSS 1.4GHz integrated flux density "}, {"name": "rMag", "desc": "[-26.2/-10.4]? SDSS r band absolute magnitude "}, {"name": "Type-CNN", "desc": "Morphology type labeled by MCRGNet (G1) "}, {"name": "BT-CNN", "desc": "Subtype label for BT sample by the MCRGNet "}, {"name": "Type-MAN", "desc": "Morphology type labeled by human inspection (G1) "}, {"name": "BT-MAN", "desc": "Subtype label for BT sample by human inspection (G2)"}, {"name": "Prob", "desc": "[0.76/1] Probability of classification by MCRGNet "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_240_5"}} {"id": "J/ApJS/240/5", "title_cds": "SHELA. II. DECam and IRAC multiwavelength catalog", "title_create": "Wold+, 2019", "year": "2019", "author": "Wold I.G.B., Kawinwanichakij L., Stevans M.L., Finkelstein S.L., Papovich C., Devarakonda Y., Ciardullo R., Feldmeier J., Florez J., Gawiser E., Gronwall C., Jogee S., Marshall J.L., Sherman S., Shipley H.V., Somerville R.S., Valdes F., Zeimann G.R.", "title_pub": "The Spitzer-HETDEX Exploratory Large Area survey. II. The Dark Energy Camera and Spitzer/IRAC multiwavelength catalog.", "first_author": "Wold I.G.B.", "ref_biblio": [""], "bibcode": ["2019ApJS..240....5W"], "see_also": ["J/ApJS/162/1 : MUSYC: optical source catalog (Gawiser+, 2006)", "J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013)"], "keyword_cds": "Galaxies, photometry; Photometry, ugriz; Photometry, infrared ; Redshifts; Surveys", "keyword_pub": "catalogs; cosmology: observations; galaxies: photometry; surveys", "abstract": ["We present the ugriz-band Dark Energy Camera (DECam) plus 3.6 and", "4.5{mu}m IRAC catalogs for the Spitzer/HETDEX Exploratory Large-Area", "(SHELA) survey. SHELA covers ~24deg^2^ of the Sloan Digital Sky Survey", "(SDSS) \"Stripe 82\" region, with seven bandpasses spanning a wavelength", "range of 0.35 to 4.5{mu}m. SHELA falls within the footprint of the", "Hobby-Eberly Telescope Dark Energy Experiment (HETDEX), which will", "provide spectroscopic redshifts for ~200000 Ly{alpha} emitters at", "1.9=0.33 SDSS spectroscopic redshifts with a", "1{sigma} scatter in {Delta}z/(1+z) of 0.04."], "description": ["We observed with the Blanco 4m telescope at CTIO using the 3deg^2^", "DECam imager and the u-, g-, r-, i-, and z-band filters. Data were", "obtained over 5 nights in the 2013B semester (PI: Papovich; NOAO PID:", "2013B-0438). As shown in Figure 1, we observed six slightly", "overlapping pointings covering a total area of 17.5deg^2^."], "alias": ["SHELA"], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/aaee85"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table6.dat", "desc": "Spitzer/HETDEX Exploratory Large-Area (SHELA) Dark Energy Camera (DECam) catalog", "columns": [{"name": "ID", "desc": "Unique object ID number (B3_ to B6_ tiles plus 000001 to 684409 numbers)"}, {"name": "RAdeg", "desc": "[14/24.6] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-1.4/1.4] Declination (J2000) "}, {"name": "amaj", "desc": "[0.1/3048] Semimajor axis (1) "}, {"name": "ell", "desc": "[0/1] Ellipticity (1) "}, {"name": "PA", "desc": "[-90/90] Postion angle (1) "}, {"name": "rKron", "desc": "[0/877] Sextractor Kron radius, AUTO photometry (1)"}, {"name": "r0.5", "desc": "[0/15905] PSF half-light radius "}, {"name": "FuPSF", "desc": "[-4/993] DECam u-band PSF fitting flux (2)"}, {"name": "e_FuPSF", "desc": "[0.001/46] Uncertainty in FuPSF (5) "}, {"name": "Fu", "desc": "[-132/46824] DECam u-band AUTO aperture flux (3)"}, {"name": "e_Fu", "desc": "[0.001/2942] Uncertainty in Fu (5) "}, {"name": "uflagI", "desc": "[0/153] DECam u-band internal flag (4) "}, {"name": "uflagE", "desc": "[0/1] DECam u-band external flag (4) "}, {"name": "FgPSF", "desc": "[-4/34050] DECam g-band PSF fitting flux (2)"}, {"name": "e_FgPSF", "desc": "[0.001/1570] Uncertainty in FgPSF (5) "}, {"name": "Fg", "desc": "[-21/521598] DECam g-band AUTO aperture flux (3)"}, {"name": "e_Fg", "desc": "[0.001/24346] Uncertainty in Fg (5) "}, {"name": "gflagI", "desc": "[0/153] DECam g-band internal flag (4) "}, {"name": "gflagE", "desc": "[0/1] DECam g-band external flag (4) "}, {"name": "FrPSF", "desc": "[-6/19361] DECam r-band PSF fitting flux (2)"}, {"name": "e_FrPSF", "desc": "[0.001/892] Uncertainty in FrPSF (5) "}, {"name": "Fr", "desc": "[-54/366386] DECam r-band AUTO aperture flux (3)"}, {"name": "e_Fr", "desc": "[0.001/29114] Uncertainty in Fr (5) "}, {"name": "rflagI", "desc": "[0/157] DECam r-band internal flag (4) "}, {"name": "rflagE", "desc": "[0/1] DECam r-band external flag (4) "}, {"name": "FiPSF", "desc": "[-7/16418] DECam i-band PSF fitting flux (2)"}, {"name": "e_FiPSF", "desc": "[0.001/758] Uncertainty in FiPSF (5) "}, {"name": "Fi", "desc": "[-1135/743848] DECam i-band AUTO aperture flux (3)"}, {"name": "e_Fi", "desc": "[0.001/220928] Uncertainty in Fi (5) "}, {"name": "iflagI", "desc": "[0/157] DECam i-band internal flag (4) "}, {"name": "iflagE", "desc": "[0/1] DECam i-band external flag (4) "}, {"name": "FzPSF", "desc": "[-5/47832] DECam z-band PSF fitting flux (2)"}, {"name": "e_FzPSF", "desc": "[0.001/2216] Uncertainty in FzPSF (5) "}, {"name": "Fz", "desc": "[-322/568888] DECam z-band AUTO aperture flux (3)"}, {"name": "e_Fz", "desc": "[0.001/161580] Uncertainty in Fz (5) "}, {"name": "zflagI", "desc": "[0/157] DECam z-band internal flag (4) "}, {"name": "zflagE", "desc": "[0/1] DECam z-band external flag (4) "}, {"name": "---", "desc": "[VICS82] "}, {"name": "VICS82", "desc": "JK object ID number (JHHMMSS.ss+DDMMSS.s), Geach+ (2017ApJS..231....7G) => a faire."}, {"name": "FJ", "desc": "[0.01/948492]?=-99 J band AUTO aperture flux (6)"}, {"name": "e_FJ", "desc": "[0/4153]?=-99 Uncertainty in FJ (6) "}, {"name": "FK", "desc": "[0/921168]?=-99 K band AUTO aperture flux (6)"}, {"name": "e_FK", "desc": "[0/37964]?=-99 Uncertainty in FK (6) "}, {"name": "F3.6um", "desc": "[-5e+6/2.1e+6]?=-99 IRAC 3.6um Tractor total flux"}, {"name": "e_F3.6um", "desc": "[0.01/5e+12]?=-99 Uncertainty in F3.6um "}, {"name": "Mod3.6", "desc": "[0/4] IRAC Tractor model profile, 3.6um (7)"}, {"name": "logP3.6", "desc": "[-7e+10/0] IRAC Tractor log-probability, 3.6um"}, {"name": "Tflag3.6um", "desc": "[0/2] Tractor flag, 3.6um observation (8) "}, {"name": "F4.5um", "desc": "[-1e+6/1.3e+6]?=-99 IRAC 4.5um Tractor total flux"}, {"name": "e_F4.5um", "desc": "[0.01/3e+12]?=-99 Uncertainty in F4.5um "}, {"name": "Mod4.5um", "desc": "[0/4] IRAC Tractor model profile, 4.5um (7)"}, {"name": "logP4.5um", "desc": "[-3e+10/0] IRAC Tractor log-probability, 4.5um"}, {"name": "Tflag4.5um", "desc": "[0/2] Tractor flag, 4.5um observation (8) "}, {"name": "zspec", "desc": "[0/1.7]?=-99 SDSS spectroscopic redshift "}, {"name": "zpeak", "desc": "[0.01/10.5]?=-99 EAZY peak photometric redshift"}, {"name": "za", "desc": "[0.01/11]?=-99 EAZY {chi}^2^ minimum photometric redshift"}, {"name": "chi2a", "desc": "[0/2664]?=-99 EAZY {chi}^2 minimum value "}, {"name": "Nfilt", "desc": "[5/9]?=-99 EAZY number of filters "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_240_6"}} {"id": "J/ApJS/240/6", "title_cds": "", "title_create": "Yao+, 2019", "year": "2019", "author": "Yao Su, Wu X.-B., Ai Y.L., Yang J., Yang Q., Dong X., Joshi R., Wang F., Feng X., Fu Y., Hou W., Luo A.-L., Kong X., Liu Y., Zhao Y.-H., Zhang Y.-X., Yuan H.-L., Shen S.", "title_pub": "The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: The Fourth and Fifth Data Releases.", "first_author": "Yao Su", "bibcode": [""], "bibcode": ["1974ApJS...28....1J"], "keyword_cds": "Stars, M-type", "keyword_pub": "late-type stars ; luminosities ; spectral classification", "description": ["Spectral types are given for 426 M dwarf stars on a uniform system", "based on the TiO bands. Most of the stars where discovered by their", "large proper motions except for the McCormick (Vyssotkey) stars. The", "observations were made with the Mount Wilson telescopes at dispersions", "of 100{AA}/mm or higher."], "curator": "Brian Skiff [Lowell Obs.], Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190307"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_30_491"}} {"id": "J/ApJS/30/491", "title_cds": "Hen-3 list of southern emission-line stars", "title_create": "Henize+, 1976", "year": "1976", "author": "Henize K.G.", "title_pub": "Observations of southern emission-line stars.", "first_author": "Henize K.G.", "ref_biblio": [""], "bibcode": ["1976ApJS...30..491H"], "keyword_cds": "Stars, emission ; Spectral types", "keyword_pub": "clusters: associations ; stars: Be \u2014 stars: stellar statistics", "abstract": ["A catalog is presented of 1929 stars showing emission at H{alpha} on", "plates taken with the Mount Wilson 10inch (25cm) camera at the", "Lamont-Hussey Observatory in 1949\u20141951. The survey covers the entire", "southern sky south of declination -25{deg} to a red limiting magnitude", "of about 11.0. A region of the northern Milky Way approximately 600", "square degrees in area is also included in order to allow comparison", "with northern surveys. Emission-line stars of all spectral classes are", "listed including 16 M stars, 25 S stars, and 37 carbon stars, as well", "as 40 con\ufb01rmed or suspected T Tauri stars. This survey has resulted", "in the discovery of two new T associations, one in Lupus and one in", "Chamaeleon.", "Variations in the intensity of the continuous spectrum have been", "observed in 53 stars, of which 32 are newly discovered variable stars.", "Variations in Ha intensity only are observed in an addi- tional 32", "stars.", "Of the 1232 stars having spectral classi\ufb01cations (mostly HD types),", "the peak frequency (17%) occurs at spectral class B8. However,", "frequency of emission per 100 stars of a given spectral class", "increases gradually from 0.2 for A0\u2014A4 stars to a maximum of 18.5 at", "B2.", "The sky distribution of the emission-line stars shows signi\ufb01cant", "concentrations in the region of the small Sagittarius cloud and in the", "Carina region. The emission-line stars in the Carina region appear to", "be predominantly B8\u2014B9 stars. The B8\u2014B9 stars form a relatively", "compact group centered at a distance of 1200 pc and are probably a", "part of the concentration of B8\u2014A0 stars seen in the Carina", "direction."], "description": ["Accurate positions of this list were dervied by Brian Skiff", "(Lowell Obs.)"], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190369"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_35_111"}} {"id": "J/ApJS/35/111", "title_cds": "MK classification of OB stars", "title_create": "Garrison+, 1977", "year": "1977", "author": "Garrison R.F., Hiltner W.A., Schild R.E.", "title_pub": "MK spectral classifications for southern OB stars.", "first_author": "Garrison R.F.", "ref_biblio": [""], "bibcode": ["1977ApJS...35..111G"], "keyword_cds": "MK spectral classification", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190468"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_4_73"}} {"id": "J/ApJS/4/73", "title_cds": "The LF2 survey in infra-red", "title_create": "Westerlund, 1959", "year": "1959", "author": "Westerlund B.", "title_pub": "An infrared survey of a region in Cygnus.", "first_author": "Westerlund B.", "ref_biblio": [""], "bibcode": ["1959ApJS....4...73W"], "see_also": ["II/221 : The LF Survey (McCuskey+ 1949-1959)"], "keyword_cds": "", "description": ["Spectral classes on the Case infrared system and infrared photographic", "magnitudes are given in the LF2 region (see Cat. II/221). The data are", "complete down to 12.25mag for the early M stars, and 12.75mag for the", "late M and Carbon stars. The search for M and S stars was carried out", "also in 3 other regions of the same galactic longitude (32.5deg), and", "the search for Carbon stars was extended to all observations covering", "a surface of 50 sq.deg."], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190045"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_43_379"}} {"id": "J/ApJS/43/379", "title_cds": "MK Types of S and SC stars", "title_create": "Keenan+ 1980", "year": "1980", "author": "Keenan P.C., Boeshaar P.C.", "title_pub": "Spectral types of S and SC stars on the revised MK system.", "first_author": "Keenan P.C.", "ref_biblio": [""], "bibcode": ["1980ApJS...43..379K"], "see_also": ["http://www.astronomy.ohio-state.edu/MKCool/ : The Revised Catalog of"], "keyword_cds": "Stars, S ; MK spectral classification", "keyword_pub": "", "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190673"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_58_439"}} {"id": "J/ApJS/58/439", "title_cds": "Observations of double stars. XII.", "title_create": "Heintz, 1985", "year": "1985", "author": "Heintz W.D.", "title_pub": "Micrometer observations of double stars and new pairs. XII.", "first_author": "Heintz W.D.", "ref_biblio": [""], "bibcode": ["1985ApJS...58..439H"], "see_also": ["J/ApJS/74/275 : Observations of double stars. XIV. (Heintz 1990)", "J/ApJS/83/351 : Observations of double stars. XV. (Heintz, 1992)", "J/ApJS/99/693 : Observations of double stars. XVI. (Heintz 1995)", "J/ApJS/105/475 : Observations of double stars. XVII. (Heintz 1996)", "J/ApJS/117/587 : Observations of double stars. XVIII. (Heintz 1998)"], "keyword_cds": "Stars, double and multiple", "keyword_pub": "stars: visual multiples", "abstract": ["Measures of 2235 pairs, including 103 new doubles, obtained at", "Swarthmore and at Cerro Tololo in the time 1982.4 to 1984.8 are", "listed."], "doi_pub": ["10.1086/191048"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Observations with the 61cm refractor ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "RAh", "desc": "? Right ascension (1900.0) "}, {"name": "RAdm", "desc": "? Right ascension (1900.0) (deci-minutes) "}, {"name": "DE-", "desc": "Declination sign (1900.0) "}, {"name": "DEd", "desc": "? Declination (1900.0) "}, {"name": "DEm", "desc": "? Declination (1900.0) "}, {"name": "Date-1980", "desc": "Observing date (minus 1980) "}, {"name": "PA", "desc": "? Position angle "}, {"name": "n_PA", "desc": "[r:?] r: round "}, {"name": "Sep", "desc": "? Separation "}, {"name": "u_Sep", "desc": "Uncertainnty flag on Sep "}, {"name": "Nnights", "desc": "Number of nights "}, {"name": "m_Name", "desc": "[ABCD -] Components for multiple systems "}, {"name": "m1/dm", "desc": "? Magnitude of brightest component or difference of magnitude (1)"}, {"name": "n_m2", "desc": "[-] '-' when m1 = magnitude of the primary "}, {"name": "m2", "desc": "? Magnitude of second brightest component "}, {"name": "Rem", "desc": "Remarks "}]}, {"name": "table2.dat", "desc": "Observations with the 100 and 91cm reflectors ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "RAh", "desc": "? Right ascension (1900.0) "}, {"name": "RAdm", "desc": "? Right ascension (1900.0) (deci-minutes) "}, {"name": "DE-", "desc": "Declination sign (1900.0) "}, {"name": "DEd", "desc": "? Declination (1900.0) "}, {"name": "DEm", "desc": "? Declination (1900.0) "}, {"name": "Date-1980", "desc": "Observing date (minus 1980) "}, {"name": "PA", "desc": "? Position angle "}, {"name": "n_PA", "desc": "[r:?] r: round "}, {"name": "Sep", "desc": "? Separation "}, {"name": "u_Sep", "desc": "Uncertainnty flag on Sep "}, {"name": "Nnights", "desc": "Number of nights "}, {"name": "m_Name", "desc": "[ABCD -] Components for multiple systems "}, {"name": "m1/dm", "desc": "? Magnitude of brightest component or difference of magnitude (1)"}, {"name": "n_m2", "desc": "[-] '-' when m1 = magnitude of the primary "}, {"name": "m2", "desc": "? Magnitude of second brightest component "}, {"name": "Rem", "desc": "Remarks "}]}, {"name": "table3a.dat", "desc": "Stars of table3 ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "m_Name", "desc": "[ABC] Multiplicity index on name "}, {"name": "IDS", "desc": "IDS designation "}, {"name": "m1", "desc": "? Magnitude of the primary "}, {"name": "---", "desc": "[-] "}, {"name": "m2", "desc": "? Magnitude of the secondary "}, {"name": "n_m2", "desc": "[v] v: variable "}, {"name": "Rem", "desc": "Remarks "}]}, {"name": "table3b.dat", "desc": "Measures of astrometric plates ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "m_Name", "desc": "[ABC] Multiplicity index on name "}, {"name": "Obs-1900", "desc": "Observation date (minus 1900) "}, {"name": "PA", "desc": "Position angle "}, {"name": "Sep", "desc": "Separation "}, {"name": "Nnights", "desc": "? Number of nights "}, {"name": "Nexp", "desc": "Number of exposures "}]}, {"name": "table4.dat", "desc": "New pairs ", "columns": [{"name": "Hei", "desc": "Hei number "}, {"name": "RAh", "desc": "Right ascension (2000.0) "}, {"name": "RA1dm", "desc": "Rigth ascension (1900.0) "}, {"name": "RAdm", "desc": "Rigth ascension (2000.0) "}, {"name": "DE-", "desc": "[NS] Declination sign (2000.0) "}, {"name": "DEd", "desc": "Declination (2000.0) "}, {"name": "DE1m", "desc": "Declination (1900.0) "}, {"name": "DEm", "desc": "[0/90] Declination (2000.0) "}, {"name": "BD/CPD", "desc": "BD (Cat. ) or CPD (Cat. ) designation"}, {"name": "Com", "desc": "Comment "}]}, {"name": "notes.dat", "desc": "Notes ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_60_507"}} {"id": "J/ApJS/60/507", "title_cds": "GRI photometry of NGC 6822", "title_create": "Hoessel+, 1986", "year": "1986", "author": "Hoessel J.G., Anderson N.", "title_pub": "Photometry of resolved galaxies. V. NGC 6822.", "first_author": "Hoessel J.G.", "ref_biblio": [""], "bibcode": ["1986ApJS...60..507H"], "see_also": ["J/ApJ/501/153 : VRB photometry of red supergiants (Massey 1998)", "J/AJ/110/2715 : UBV photometry in NGC 6822, M31 and M33 (Massey+ 1995)"], "keyword_cds": "Galaxies, photometry ; Photometry, CCD", "keyword_pub": "galaxies: individual - galaxies: Local Group - galaxies: photometry - galaxies: stellar content - luminosity function", "abstract": ["Three-color CCD frames of the local group irregular galaxy NGC 6822", "have been reduced to GRI photometry for 3475 stars using RICHFLD", "point-spread function fitting techniques. The data are compared with", "earlier work on this galaxy, particularly with Kayser (1966, Ph.D.", "Thesis, California Institute of Technology) on a star-by-star basis.", "While the general agreement between the results of photographic and", "electronic techniques is good, some differences in detail exist, which", "are attributed to a small nonlinearity in the photographic results and", "zero-point offsets of ~0.1mag. Color-magnitude diagrams are", "constructed from the data and compared with both theoretical stellar", "model tracks and the expected foreground star contamination. A", "luminosity function for the blue stars (G-R<0) is derived; comparison", "of this luminosity function with those of 10 other irregular galaxies", "indicates that NGC 6822 has a typical young star population. The", "stellar birthrate and initial mass function are estimated for this", "galaxy. The slope at the bright end of the mass function looks similar", "to recent results for the Galaxy, the Magellanic Clouds, and the", "irregular galaxy Sextans A. NGC 6822 appears to be presently forming", "stars at a slower rate for its mass than Sextans A or the Magellanic", "Clouds.", "For a description of the GRI photometric system, see e.g.", " and "], "object": ["19 44 57.8 -14 48 11 NGC 6822 = IC 4895"], "doi_pub": ["10.1086/191095"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Photometry of stars in CCD field 1 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table2.dat", "desc": "Photometry of stars in CCD field 2 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table3.dat", "desc": "Photometry of stars in CCD field 3 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table4.dat", "desc": "Photometry of stars in CCD field 4 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table5.dat", "desc": "Photometry of stars in CCD field 5 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table6.dat", "desc": "Photometry of stars in CCD field 6 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table7.dat", "desc": "Photometry of stars in CCD field 7 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table8.dat", "desc": "Photometry of stars in CCD field 8 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table9.dat", "desc": "Photometry of stars in CCD field 9 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_62_751"}} {"id": "J/ApJS/62/751", "title_cds": "A catalog of Markarian galaxies", "title_create": "Mazzarella+, 1986", "year": "1986", "author": "Mazzarella J.M., Balzano V.A.", "title_pub": "A catalog of Markarian galaxies.", "first_author": "Mazzarella J.M.", "ref_biblio": [""], "bibcode": ["1986ApJS...62..751M\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191155"], "orcid_pub": ["0000-0002-8204-8619"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_69_1"}} {"id": "J/ApJS/69/1", "title_cds": "First addition to the new optical catalog of QSO", "title_create": "Hewitt+, 1989", "year": "1989", "author": "Hewitt A., Burbidge G.", "title_pub": "The first addition to the new optical catalog of quasi-stellar objects.", "first_author": "Hewitt A.", "ref_biblio": [""], "bibcode": ["1989ApJS...69....1H\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricio Ortiz [CDS]", "doi_pub": ["10.1086/191307"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_70_637"}} {"id": "J/ApJS/70/637", "title_cds": "Southern Milky Way carbon stars", "title_create": "Aaronson+, 1989", "year": "1989", "author": "Aaronson M., Blanco V.M., Cook K.H., Schechter P.L.", "title_pub": "Southern Milky Way carbon stars: new candidates, JHK photometry and radial velocities.", "first_author": "Aaronson M.", "ref_biblio": [""], "bibcode": ["1989ApJS...70..637A"], "keyword_cds": "Stars, carbon;", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191350"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_72_715"}} {"id": "J/ApJS/72/715", "title_cds": "Cluster Radial Velocity Samples", "title_create": "Teague+, 1990", "year": "1990", "author": "Teague P.F., Carter D., Gray P.M.", "title_pub": "The dynamics and structure of rich clusters of galaxies. I. Velocity data.", "first_author": "Teague P.F.", "ref_biblio": [""], "bibcode": ["1990ApJS...72..715T"], "keyword_cds": "Clusters, galaxy ; X-ray sources ; Redshifts", "keyword_pub": "galaxies: clustering - galaxies: redshifts", "abstract": ["An extensive spectroscopic study of 10 rich southern X-ray clusters of", "galaxies is presented. Between 40 and 200 redshifts have been obtained", "in the field of each of the clusters, which cover a wide range of", "morphological types and richnesses. Applying rigorous statistical", "analyses to the total data base of 1000 precise radial velocities", "provides the necessary information to undertake a thorough dynamical", "investigation of these individual clusters and of cluster systems in", "general."], "doi_pub": ["10.1086/191430"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table4.dat", "desc": "Cluster radial velocity samples ", "columns": [{"name": "TCG", "desc": "Galaxy identification number (ANNNN NNNA) (1) "}, {"name": "RA1h", "desc": "Right ascension (B1950) "}, {"name": "RA1m", "desc": "Right ascension (B1950) "}, {"name": "RA1s", "desc": "Right ascension (B1950) "}, {"name": "DE1-", "desc": "Declination sign (B1950) "}, {"name": "DE1d", "desc": "Declination (B1950) "}, {"name": "DE1m", "desc": "Declination (B1950) "}, {"name": "DE1s", "desc": "Declination (B1950) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Dist", "desc": "Projected radial distance of galaxy from cluster centre"}, {"name": "HRV", "desc": "Heliocentric radial velocity "}, {"name": "u_HRV", "desc": "Uncertainty flag on HRV "}, {"name": "e_HRV", "desc": "Error in radial velocity "}, {"name": "R(TD)", "desc": "? Tonry & Davis (1979AJ.....84.1511T) R-value "}, {"name": "Com", "desc": "Comments (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_73_841"}} {"id": "J/ApJS/73/841", "title_cds": "Carbon stars in the Northern Milky Way", "title_create": "Aaronson+, 1990", "year": "1990", "author": "Aaronson M., Blanco V.M., Cook K.H., Olszewski E.W., Schechter P.L.", "title_pub": "Northern Milky Way carbon star: new candidates, JHK photometry and radial velocities.", "first_author": "Aaronson M.", "ref_biblio": [""], "bibcode": ["1990ApJS...73..841A"], "keyword_cds": "Stars, carbon", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191491"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_82_1"}} {"id": "J/ApJS/82/1", "title_cds": "Optical identification of Texas Survey radio sources", "title_create": "Bozyan, 1992", "year": "1992", "author": "Bozyan E.P.", "title_pub": "Optical identification, radio galaxy environment and statistical properties for a homogeneous sample of 3196 radio sources from the Texas survey.", "first_author": "Bozyan E.P.", "ref_biblio": [""], "bibcode": ["1992ApJS...82....1B"], "see_also": ["VII/54 : Extragalactic Radio Source Identifications (Veron-Cetty+ 1983)", "VIII/42 : Texas Survey of Radio Sources at 365 MHz (Douglas+ 1996)"], "keyword_cds": "Radio sources ; Galaxies, radio ; QSOs ; Clusters, galaxy ; Surveys", "keyword_pub": "Galaxies: clustering - Quasars: general - Radio continuum: galaxies", "description": ["National Geographic Society Palomar Sky Survey E and O glass copy", "plates were searched for optical counterparts to a homogeneous sample", "of 3196 sources from the 365MHz Texas Survey in the region", "+31{deg}20{deg}. The search resulted in 860", "optical identifications coincident with the radio centroid within the", "4 arcsecond search radius. There were also 728 possible", "identifications at the plate limit and 1608 empty fields with no", "optical counterpart to the plate limit. Radio source data and optical", "identification data are tabulated for the entire sample. For the", "positive identifications, the optical data includes magnitudes", "estimated from the plates to 0.5mag and classifications of the", "appearance as stellar or diffuse."], "doi_pub": ["10.1086/191709"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table456.dat", "desc": "Optical identifications ", "columns": [{"name": "Name", "desc": "Texas Survey radio source name in IAU format "}, {"name": "Mflg", "desc": "Goodness of structure model fit (1) "}, {"name": "Eflg", "desc": "Influence of environment on fit (1) "}, {"name": "Lflg", "desc": "Probability the position is lobe-shifted (1) "}, {"name": "RAh", "desc": "Right Ascension (1950) "}, {"name": "RAm", "desc": "Right Ascension (1950) "}, {"name": "RAs", "desc": "Right Ascension (1950) "}, {"name": "e_RAs", "desc": "Right Ascension error "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "DEs", "desc": "Declination (1950) "}, {"name": "e_DEs", "desc": "Declination error "}, {"name": "S365MHz", "desc": "365 MHz flux density "}, {"name": "e_S365MHz", "desc": "Flux density error "}, {"name": "Sp+Index", "desc": "? 335-385 MHz spectral index, S{prop.to}nu^(-Sp+Index)^"}, {"name": "e_Sp+Index", "desc": "? Error in spectral index "}, {"name": "Chi2", "desc": "? Chi-squared per dof flux residual over 4 observing cycles"}, {"name": "Vflg", "desc": "[*]? * means source may be variable "}, {"name": "Sep", "desc": "? Component separation in double model "}, {"name": "e_Sep", "desc": "? Error in component separation "}, {"name": "Struct", "desc": "Structure model type, P: point source, D: double, AD: asymmetric double"}, {"name": "q", "desc": "? Flux asymmetry parameter for AD model (2) "}, {"name": "Xi", "desc": "[-180,180]? Position angle of double "}, {"name": "e_Xi", "desc": "? Error in position angle (99=unknown) "}, {"name": "KA2", "desc": "? Second most likely RA lobe "}, {"name": "KD2", "desc": "? Second most likely Dec lobe "}, {"name": "IDE", "desc": "Identification on E plate (3) "}, {"name": "AppE", "desc": "[SD]? Appearance on E plate S: stellar, D: diffuse"}, {"name": "IDO", "desc": "Identification on O plate (3) "}, {"name": "AppO", "desc": "[SD]? Appearance on O plate: S: stellar, D: diffuse"}, {"name": "Color", "desc": "[BRN]? B: blue, R: red, N: neutral "}, {"name": "QualE", "desc": "? Qualifications for E identification (4) "}, {"name": "QualO", "desc": "? Qualifications for O identification (4) "}, {"name": "Comment", "desc": "? Additional identifications, close optical companions, or other comments"}, {"name": "Known", "desc": "? Previous ID, or ID within 2 arcmin of center of Abell or Zwicky cluster (5)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_83_203"}} {"id": "J/ApJS/83/203", "title_cds": "Catalog of faint A, F and G stars at SGP", "title_create": "Lu+, 1992", "year": "1992", "author": "Lu P.K., Miller J., Platt D.", "title_pub": "A catalog of faint A, F, and G stars at the South Galactic Pole.", "first_author": "Lu P.K.", "ref_biblio": [""], "bibcode": ["1992ApJS...83..203L"], "see_also": ["II/119 : Stellar Distribution near the South Galactic Pole (Bok+ 1964)", "III/74 : Faint blue stars in the region near SGP (Haro+ 1962)", "II/120 : Phot and Spectrophot Investigation, SGP (Eriksson 1978)", "I/129 : Parallaxes and Proper Motions near SGP (Murray+ 1986)", "J/AJ/112/772 : VI photometry in South Galactic Pole (Caldwell+ 1996)", "J/AJ/109/2229 : South Galactic Pole stars photometry (Eggen 1995)"], "keyword_cds": "Stars, faint ; Galactic pole, south ; MK spectral classification ; Photometry", "keyword_pub": "catalogs - stars: fundamental parameters", "abstract": ["A catalog of identifications and positions for 3155 A, F, and G stars", "at the south Galactic pole is presented. The new thin-prism spectra", "survey yields a set of uniformly selected A, F, and early G stars to", "a limiting magnitude of 16.0. The positions are based on PDS scans of", "a 6.3{deg}x6.3{deg} UK Schmidt direct film centered on the SGP.", "Objective-prism plates covering approximately 100{deg}^2^ centered on", "the SGP were obtained using the Michigan Curtis Schmidt telescope at", "CTIO with a dispersion of 1360{AA}/mm. Approximately 30% of the", "catalog stars now have 2D-Frutti MK spectral types and uvby,H{beta}", "photometry. Of 822 spectra classified with luminosities, 76 stars (9%)", "have classes III and IV-III; 21 (3%) stars are class IV, 669 stars", "(81%) are of luminosity classes V and V-IV, and 56 stars (7%) are", "classified as Vw for weak-lined or intermediate Population II objects.", "The mean spectral distribution for dwarf stars peaks at F9.3 V and", "declines sharply at G4. The mean color index for 1104 stars is", "=0.359+/-0.080, a value typical of F9 V. Correlations between", "spectral types and photometry (b-y) index are also presented. Detailed", "analyses of radial velocity determinations using cross-correlation", "techniques and direct CCD and ASCAP photometry will be reported in a", "subsequent paper. The purpose of publishing the catalog at this stage", "is to invite other investigators to collaborate in collecting the", "photometric and spectroscopic data."], "alias": ["[LMP92]"], "type": ["OC"], "doi_pub": ["10.1086/191735"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Catalog of faint F and G stars at the South Galactic Pole", "columns": [{"name": "SAx", "desc": "Frame number (pixel number in RA) "}, {"name": "SAy", "desc": "Frame number (pixel number in DE) "}, {"name": "Star", "desc": "Number of the star in the Frame SAxSAy (1) "}, {"name": "m_Star", "desc": "[AB] Multiplicity index on Star "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "[0/60] Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "[0/60] Declination (J2000) "}, {"name": "u_SpT", "desc": "[:] Uncertainty flag on SpT "}, {"name": "n_SpT", "desc": "[*] *: Multiple observations exist "}, {"name": "SpT", "desc": "Spectral type "}, {"name": "Vmag", "desc": "V or photographic magnitude "}, {"name": "b-y", "desc": "? b-y colour index "}, {"name": "n_b-y", "desc": "[*] *: Multiple observations exist "}, {"name": "2DF", "desc": "? 2D-Frutti frame number "}, {"name": "Note", "desc": "[ac*] FLAGS NOT EXPLANED "}, {"name": "CCD", "desc": "? CCD frame number "}, {"name": "HD", "desc": "? HD, Bok or CGG number (see \"n_HD\" column) "}, {"name": "n_HD", "desc": "[cb] b = Bok and Basinski, 1964, Cat. ) number; c = Corbally+Garrison SGP number"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_83_273"}} {"id": "J/ApJS/83/273", "title_cds": "High Galactic latitude stars photometry", "title_create": "Penprase+, 1992", "year": "1992", "author": "Penprase B.E.", "title_pub": "Photometric and spectroscopic analysis of high galactic latitude molecular clouds. I. Distances and extinctions of stars toward 25 selected regions.", "first_author": "Penprase B.E.", "ref_biblio": [""], "bibcode": ["1992ApJS...83..273P"], "see_also": ["III/31 : Michigan catalogue for the HD stars, vol. 1 (Houk+, 1975)"], "keyword_cds": "Molecular clouds ; Photometry, UBV ; Photometry, H-beta ; Photometry, uvby, beta ; Reddening", "keyword_pub": "ISM: clouds - ISM: molecules - stars: fundamental parameters", "abstract": ["New photoelectric photometry in the UBV, uvby, and H{beta} systems is", "presented for 320 stars at high Galactic latitudes, selected for their", "proximity to the densest portions of a variety of high Galactic", "latitude atomic and molecular clouds. Low-resolution digital spectra", "are used to classify 115 of the stars, using both stellar line", "strengths and statistical tests against a library of standard stars of", "all spectral types. Several new techniques are developed for automatic", "digital spectral classification, and for dereddening Stromgren", "uvby{beta} and Johnson UBV, H{beta} photometry. An empirical determination", "of the errors in the derived dereddened colors, and techniques for", "converting between the two photometric systems are presented, based on", "the analysis of a statistically significant sample of 1480 stars with", "complete data sets in both photometric systems and with an accurate MK", "spectral type. For several stars, spectroscopic and photometric", "observations are combined to derive distances and reddenings toward", "selected high-latitude clouds. New constraints on the distances to", "several clouds are presented: for MBM 41, 200 < d < 300pc;", "for MBM 3-4, 90 < d < 180pc; for MBM 27-31, 130 < d < 220pc;", "for MBM 15, 110 < d < 160pc; and for MBM 57, 150 < d < 210pc. Additional", "distance constraints have been obtained for over 25 cloud complexes,", "and several highly reddened sightlines have been identified which", "should offer opportunities for spectroscopic analysis of the molecular", "clouds."], "doi_pub": ["10.1086/191738"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table3.dat", "desc": "The stars observed with UBV,H{beta} photometry ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "SAO", "desc": "? SAO (Cat. ) number) "}, {"name": "RAh", "desc": "Right ascension (B1950) "}, {"name": "RAm", "desc": "Right ascension (B1950) "}, {"name": "RAs", "desc": "Right ascension (B1950) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) "}, {"name": "DEm", "desc": "Declination (B1950) "}, {"name": "DEs", "desc": "Declination (B1950) "}, {"name": "SpType", "desc": "Spectral type (from HD catalogue) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "LRS", "desc": "[yes no] Low-resolution digital spectroscopy "}, {"name": "ubvybeta", "desc": "[yes no] uvby{beta} photometry "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "U-B", "desc": "U-B colour index "}, {"name": "o_Vmag", "desc": "Number of observations in UBV "}, {"name": "e_Vmag", "desc": "rms uncertainty on UBV observations "}, {"name": "Hbeta", "desc": "H{beta} colour index "}, {"name": "o_Hbeta", "desc": "Number of observations in Hbeta "}, {"name": "e_Hbeta", "desc": "rms uncertainty on Hbeta "}, {"name": "Region", "desc": "Associated interstellar cloud (G1) "}]}, {"name": "table4.dat", "desc": "The stars observed with ubvy,{beta} photometry ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "SAO", "desc": "? SAO (Cat. ) number) "}, {"name": "RAh", "desc": "Right ascension (B1950) "}, {"name": "RAm", "desc": "Right ascension (B1950) "}, {"name": "RAs", "desc": "Right ascension (B1950) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) "}, {"name": "DEm", "desc": "Declination (B1950) "}, {"name": "DEs", "desc": "Declination (B1950) "}, {"name": "SpType", "desc": "Spectral type (HD) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "LRS", "desc": "[yes no] Low-resolution spectroscopy "}, {"name": "UBVbeta", "desc": "[yes no] UBV,H{beta} photometry "}, {"name": "vmag", "desc": "v magnitude "}, {"name": "b-y", "desc": "b-y colour index "}, {"name": "m1", "desc": "m1 colour index "}, {"name": "c1", "desc": "c1 colour index "}, {"name": "o_vmag", "desc": "Number of observations in uvby "}, {"name": "e_vmag", "desc": "rms uncertainty on uvby observations "}, {"name": "Hbeta", "desc": "H{beta} colour index "}, {"name": "o_Hbeta", "desc": "Number of observations in Hbeta "}, {"name": "e_Hbeta", "desc": "rms uncertainty on Hbeta "}, {"name": "Region", "desc": "Associated interstellar cloud (G1) "}]}, {"name": "table6.dat", "desc": "Photometric estimates of E(B-V) and distance ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "SAO", "desc": "? SAO (Cat. ) number) "}, {"name": "Sys", "desc": "Photometric system used for the classification "}, {"name": "Hbeta", "desc": "H{beta} colour index "}, {"name": "Index", "desc": "Q (UBV) or [m1] (uvby) reddening-free index (1) "}, {"name": "sigma1", "desc": "Number of standard deviations for the star from the average relation in the H{beta},Q or H{beta},[m1] plane in the direction of H{beta}"}, {"name": "sigma2", "desc": "Number of standard deviations for the star from the average relation in the H{beta},Q or H{beta},[m1] plane in the direction of Q or [m1]"}, {"name": "(B-V)0", "desc": "? Dereddened B-V colour index "}, {"name": "VMAG", "desc": "? Absolute V magnitude "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "E(B-V)", "desc": "? Colour excess "}, {"name": "e_E(B-V)", "desc": "? rms uncertainty on E(B-V) "}, {"name": "Dist", "desc": "? Distance "}, {"name": "e_Dist", "desc": "? rms uncertainty on Dist "}, {"name": "Region", "desc": "Nearest interstellar cloud to the star (G1) "}]}, {"name": "table7b.dat", "desc": "Comparison of Michigan Spectral Catalog (MSC, ) spectral types with Digital Spectral Classification", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "SAO", "desc": "SAO (Cat. ) number) "}, {"name": "SpTypeM", "desc": "MSC spectral type "}, {"name": "(B-V)0M", "desc": "MSC dereddened B-V colour index "}, {"name": "(U-B)0M", "desc": "MSC dereddened U-B colour index "}, {"name": "VMAGM", "desc": "MSC absolute V magnitude "}, {"name": "SpType", "desc": "This work spectral type "}, {"name": "(B-V)0", "desc": "This work dereddened B-V colour index "}, {"name": "(U-B)0", "desc": "This work dereddened U-B colour index "}, {"name": "VMAG", "desc": "This work absolute V magnitude "}]}, {"name": "table8.dat", "desc": "Spectroscopic classification and estimates of E(B-V) and distance", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "n_HD", "desc": "[#] Note on E(B-V) and distance determination (1) "}, {"name": "SAO", "desc": "? SAO (Cat. ) number) "}, {"name": "RAh", "desc": "Right ascension (B1950) "}, {"name": "RAm", "desc": "Right ascension (B1950) "}, {"name": "RAs", "desc": "Right ascension (B1950) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) "}, {"name": "DEm", "desc": "Declination (B1950) "}, {"name": "DEs", "desc": "Declination (B1950) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "Sys", "desc": "Photometric system used for the classification "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "(B-V)0", "desc": "Dereddened B-V colour index "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "E(B-V)", "desc": "Colour excess (1) "}, {"name": "e_E(B-V)", "desc": "rms uncertainty on E(B-V) "}, {"name": "Dist", "desc": "Distance (1) "}, {"name": "e_Dist", "desc": "rms uncertainty on Dist "}, {"name": "Region", "desc": "Nearest interstellar cloud to the star (G1) "}]}, {"name": "table9.dat", "desc": "Summary of cloud distance and extinction estimates ", "columns": [{"name": "Cloud", "desc": "Cloud name "}, {"name": "Nobs", "desc": "Number of observations "}, {"name": "Dinf", "desc": "? Lower limit for distance "}, {"name": "---", "desc": "[<] "}, {"name": "---", "desc": "[d] "}, {"name": "---", "desc": "[<] "}, {"name": "Dsup", "desc": "? Upper limit for distance "}, {"name": "Av", "desc": "? Estimates of Av extinction, computed used an average value of R_V_=3.05"}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_87_197"}} {"id": "J/ApJS/87/197", "title_cds": "Carina OB2 association", "title_create": "Garcia+, 1993", "year": "1993", "author": "Garcia B.", "title_pub": "A study of Carina OB2 assciation. I. Observational data.", "first_author": "Garcia B.", "ref_biblio": [""], "bibcode": ["1993ApJS...87..197G"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191802"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_91_1"}} {"id": "J/ApJS/91/1", "title_cds": "Lyman-Alpha forest near 34 QSOs", "title_create": "Bechtold 1994", "year": "1994", "author": "Bechtold J.", "title_pub": "The Lyman-Alpha forest near 34 quasi-stellar objects with z > 2.6.", "first_author": "Bechtold J.", "ref_biblio": [""], "bibcode": ["1994ApJS...91....1B"], "see_also": ["http://lithops.as.arizona.edu/~jill/QuasarSpectra/MMT/ :"], "keyword_cds": "Spectra", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191937"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_94_551"}} {"id": "J/ApJS/94/551", "title_cds": "The first EGRET catalog", "title_create": "Fichtel+ 1994", "year": "1994", "author": "Fichtel C.E., Bertsch D.L., Chiang J., Dingus B.L., Esposito J.A., Fierro J.M., Hartman R.C., Hunter S.D., Kanbach G., Kniffen D.A., Kwok P.W., Lin Y.C., Mattox J.R., Mayer-Hasselwander H.A., McDonald L., Michelson P.F., von Montigny C., Nolan P.L., Pinkau K., Radecke H.-D., Rothermel H., Sreekumar P., Sommer M., Schneid E.J., Thompson D.J., Willis T.", "title_pub": "The first energetic gamma-ray experiment telescope (EGRET) source catalog", "first_author": "Fichtel C.E.", "ref_biblio": [""], "bibcode": ["1994ApJS...94..551F\t(SIMBAD/NED"], "keyword_cds": "Gamma rays", "keyword_pub": "gamma rays: observations", "mission": "EGRET", "description": ["In this catalog the results related to high-energy gamma-ray sources", "obtained from the Energetic Gamma Ray Experiment Telescope (EGRET) on", "the Compton Gamma Ray Observatory are summarized for the period from", "1991 April 22 to 1992 November 17, called phase I. This phase of the", "Compton Observatory mission was devoted to an all-sky survey. Tables", "are included for the following EGRET results; solar flares with", "detected gamma radiation; pulsars; sources with |b|<10deg; gamma-ray", "bursts; normal galaxies; clusters of galaxies; positive detections of", "radio-loud quasars and BL Lac objects; marginal detections of", "radio-loud quasars and BL Lac objects; upper limits for radio-loud", "quasars and BL Lac objects; uppet limits for Seyfert galaxies and", "selected radio-quiet quasars, and other sources with |b|>+10deg in the", "Galactic Plane. There is also a table relating the dates of the", "observations to the Compton Observatory viewing period numbers to", "assist in referencing the observations."], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/192082"], "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_99_223"}} {"id": "J/ApJS/99/223", "title_cds": "IUE UV Observations of SN 1987A", "title_create": "Pun+ 1995", "year": "1995", "author": "Pun C.S.J., Kirshner R.P., Sonneborn G., Challis P., Nassiopoulos G., Arquilla R., Michael C.D., Shrader C., Teays T., Cassatella A., Gilmozzi R., Talavera A., Wamsteker W., Fransson C., Panagia N.", "title_pub": "Ultraviolet Observations of SN 1987A with the IUE Satellite", "first_author": "Pun C.S.J.", "ref_biblio": [""], "bibcode": ["1995ApJS...99..223P"], "keyword_cds": "Supernovae ; Spectra, ultraviolet", "keyword_pub": "ultraviolet: stars - stars: individual (SN 1987A)", "abstract": ["Ultraviolet (lambda: 1150-3300A) observations of SN 1987A with the", "IUE satellite provide a unique data set. Observations started the day", "after discovery, 1987 February 24 (day 1.6), and a total of 751", "spectra were obtained through 1992 June 9 (day 1567). The data have", "been processed to generate a complete catalog of SN 1987A ultraviolet", "spectra. The data reduction procedure includes careful line-by-line", "extraction, removing hits and hot pixels, and, most importantly, a", "scrupulous subtraction of the contribution from stars near SN 1987A", "within the IUE aperture. In addition to processing the data, we have", "also extracted light curves, and combined them with the ground-based", "optical data and HST observations (day 1278 to 2431) to extend the", "study in both wavelength and time. The data-processing procedures of", "our IUE study produce results that are consistent with the HST data", "where they overlap, but not with the IUE study by Sanz Fernandez de", "Cordoba (1993A&A...276..103S) because of its incorrect background", "subtraction. The IUE data are consistent with the ground-based", "Walraven VBLUW photometry, while we found that flux scale of the", "Soviet ASTRON satellite spectroscopic data is low by ~15%. The UV flux", "plummeted during the earliest days of observations because of the drop", "in the photospheric temperature and the increase in opacity. However,", "after reaching a minimum of 0.04% on day 44, the UV flux increased by", "175 times in its contribution to 7% of the total UVOIR bolometric", "luminosity at day 800. A revised set of bolometric data has been", "constructed which includes the contribution of UV from day 1 to day", "1352. Studies of the UV colors show that the supernova started to get", "bluer in UV around the time when dust started to form in the ejecta.", "Our results are consistent with the possibility that the dust", "condensed may be metal-rich."], "description": ["The data for this paper were supplied in five UNIX tar files", "containing the FITS images for (1) the IUE LWP background, (2) LWP", "data, (3) SWP background, (4) SWP data, and (5) optical observations.", "Tables 2(a), 2(b), 3(a), and 3(b) containing the journal of IUE", "observations were also included. The FITS files contained in the tar", "files had names such as 'lwp.18792.bgd.fits'. These names are not", "compatible with the ISO 9660 CD-ROM file system standard. The files", "were renamed first by placing each of the files from the five tar", "files into their own subdirectory, e.g. 'lwpbgd', and renaming the", "files to ISO 9660-style names, e.g. 'l18792.fit'. The tables", "containing the journals of observations include the new file names so", "that the user can correlate the FITS files to the proper observations.", "The author-supplied README file has been included to provide further", "explanations of the data."], "doi_pub": ["10.1086/192185"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "readme.dat", "desc": "Author-supplied description of data files ", "columns": []}, {"name": "table2a.dat", "desc": "Journal of observations: swpbgd FITS files ", "columns": [{"name": "File", "desc": "Name of FITS file in swpbgd directory "}, {"name": "CAM", "desc": "IUE camera, always SWP "}, {"name": "IMG", "desc": "IUE image number "}, {"name": "Date", "desc": "Date of observation "}, {"name": "Day", "desc": "Day number of SN 1987A "}, {"name": "Exp", "desc": "Exposure time. Trailing 's' for sec, 'm' for min"}]}, {"name": "table2b.dat", "desc": "Journal of observations: lwpbgd FITS files ", "columns": [{"name": "File", "desc": "Name of FITS file in lwpbgd directory "}, {"name": "CAM", "desc": "IUE camera, always LWP "}, {"name": "IMG", "desc": "IUE image number "}, {"name": "Date", "desc": "Date of observation "}, {"name": "Day", "desc": "Day number of SN 1987A "}, {"name": "Exp", "desc": "Exposure time. Trailing 's' for sec, 'm' for min"}]}, {"name": "table3a.dat", "desc": "Journal of observations: swpdata FITS files ", "columns": [{"name": "File", "desc": "*Name of FITS file in swpdata directory "}, {"name": "CAM", "desc": "IUE camera, always SWP "}, {"name": "IMG", "desc": "IUE image number "}, {"name": "n_IMG", "desc": "[*] "}, {"name": "Date", "desc": "Date of observation "}, {"name": "Day", "desc": "[]? Day number of SN 1987A "}, {"name": "Exp", "desc": "Exposure time. Trailing 's' for sec, 'm' for min"}]}, {"name": "table3b.dat", "desc": "Journal of observations: lwpdata FITS files ", "columns": [{"name": "File", "desc": "*Name of FITS file in lwpdata directory "}, {"name": "CAM", "desc": "IUE camera, always LWP "}, {"name": "IMG", "desc": "*IUE image number "}, {"name": "n_IMG", "desc": "[*] "}, {"name": "Date", "desc": "Date of observation "}, {"name": "Day", "desc": "[]? Day number of SN 1987A "}, {"name": "Exp", "desc": "Exposure time. Trailing 's' for sec, 'm' for min"}]}, {"name": "swpbgd/*", "desc": "Short wavelength spectra (1150 - 1975 A) averaged for background subtraction", "columns": []}, {"name": "lwpbgd/*", "desc": "Long wavelength spectra (1975 - 3300 A) averaged for background subtraction", "columns": []}, {"name": "swpdat/*", "desc": "IUE SWP camera (1150 - 1975 A) observations of SN 1987A", "columns": []}, {"name": "lwpdat/*", "desc": "IUE LWP camera (1975 - 3300 A) observations of SN 1987A", "columns": []}, {"name": "optfit/*", "desc": "Combined IUE and CTIO spectra of SN 1987A ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_99_693"}} {"id": "J/ApJS/99/693", "title_cds": "Observations of double stars. XVI.", "title_create": "Heintz 1995", "year": "1995", "author": "Heintz W.D.", "title_pub": "Observations of double stars and new pairs. XVI. Results in 1992-1994.", "first_author": "Heintz W.D.", "ref_biblio": [""], "bibcode": ["1995ApJS...99..693H"], "see_also": ["J/AJ/108/2338 : Photographic astrometry. VIII. (Heintz 1994)", "J/ApJS/74/275 : Observations of double stars. XIV. (Heintz 1990)", "J/ApJS/83/351 : Observations of double stars. XV. (Heintz 1992)", "J/ApJS/105/475 : Observations of double stars. XVII. (Heintz 1996)", "J/ApJS/117/587 : Observations of double stars. XVIII. (Heintz 1998)"], "keyword_cds": "Stars, double and multiple", "keyword_pub": "binaries: visual", "abstract": ["Visual and photographic measures listed for 730 pairs were obtained in", "the time 1992.2-1994.9. Tables and notes include corrections to", "catalog positions and some revised orbits."], "doi_pub": ["10.1086/192202"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1", "desc": "New pairs ", "columns": [{"name": "Hei", "desc": "Heintz number "}, {"name": "RAh1", "desc": "Right ascension (1900) "}, {"name": "RAdm1", "desc": "Right ascension (1900) "}, {"name": "DE-1", "desc": "Declination sign "}, {"name": "DEd1", "desc": "Declination (1900) "}, {"name": "DEm1", "desc": "Declination (1900) "}, {"name": "RAh2", "desc": "Right ascension (2000) "}, {"name": "RAdm2", "desc": "Right ascension (2000) "}, {"name": "DE-2", "desc": "Declination sign "}, {"name": "DEd2", "desc": "Declination (2000) "}, {"name": "DEm2", "desc": "Declination (2000) "}, {"name": "BD", "desc": "BD (Cat. ) number "}, {"name": "Com", "desc": "Comment "}]}, {"name": "table2", "desc": "Micrometer observations ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "RAh", "desc": "Right ascension (2000) "}, {"name": "RAdm", "desc": "Right ascension (2000) (deci-minutes) "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (2000) "}, {"name": "DEm", "desc": "Declination (2000) "}, {"name": "Ep-1990", "desc": "Epoch of observation 1990+ "}, {"name": "PA", "desc": "? Position angle "}, {"name": "n_PA", "desc": "[rs:] r: round; s: single; : uncertain value "}, {"name": "Sep", "desc": "? Separation between the components "}, {"name": "u_Sep", "desc": "Uncertainty flag on Sep "}, {"name": "Nobs", "desc": "? Number of nights "}, {"name": "Comp", "desc": "[ABCa -] Components for multiple systems "}, {"name": "m1", "desc": "? Magnitude of brightest component "}, {"name": "m2", "desc": "? Magnitude of second brightest component "}]}, {"name": "table3", "desc": "Measures on astronomic plates ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "m1", "desc": "? Magnitude of brightest component "}, {"name": "m2", "desc": "? Magnitude of second brightest component "}, {"name": "RAh", "desc": "Right ascension (2000) "}, {"name": "RAdm", "desc": "Right ascension (2000) (deci-minutes) "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (2000) "}, {"name": "DEm", "desc": "Declination (2000) "}, {"name": "Ep-1900", "desc": "Epoch of observation 1900+ "}, {"name": "PA", "desc": "Position angle "}, {"name": "Sep", "desc": "Separation between the components "}, {"name": "Nobs", "desc": "? Number of nights "}, {"name": "Nexp", "desc": "Measured exposures "}]}, {"name": "table4", "desc": "Orbits ", "columns": [{"name": "RAh", "desc": "Right ascension (2000) "}, {"name": "RAdm", "desc": "Right ascension (2000) "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "DEclination (2000) "}, {"name": "DEm", "desc": "DEclination (2000) "}, {"name": "ADS", "desc": "? ADS number "}, {"name": "Name", "desc": "Star name "}, {"name": "mag1", "desc": "Visual magnitude of the primary "}, {"name": "mmag2", "desc": "Visual magnitude of the secondary "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Per", "desc": "Period "}, {"name": "n", "desc": "Yearly motion "}, {"name": "T", "desc": "Time of the perihelion passage "}, {"name": "a", "desc": "Semi-major axis "}, {"name": "e", "desc": "Eccentricity "}, {"name": "i", "desc": "Inclination angle "}, {"name": "omega", "desc": "Longitude of the perihelion "}, {"name": "OMEGA", "desc": "Longitude of the ascensing node "}, {"name": "plx", "desc": "? Dynamical parallax "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_244_18"}} {"id": "J/ApJS/244/18", "title_cds": "Kepler Smear Campaign: LCs & sp of very bright stars", "title_create": "Pope+, 2019", "year": "2019", "author": "Pope B.J.S., Davies G.R., Hawkins K., White T.R., Stokholm A., Bieryla A., Latham D.W., Lucey M., Aerts C., Aigrain S., Antoci V., Bedding T.R., Bowman D.M., Caldwell D.A., Chontos A., Esquerdo G.A., Huber D., Jofre P., Murphy S.J., van Reeth T., Silva Aguirre V., Yu J.", "title_pub": "The Kepler Smear Campaign: light curves for 102 very bright stars.", "first_author": "Pope B.J.S.", "ref_biblio": [""], "bibcode": ["2019ApJS..244...18P"], "see_also": ["I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)", "V/133 : Kepler Input Catalog (Kepler, 2009)", "I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/A+A/275/101 : Chemical evolution of the gal. disk I. (Edvardsson+ 1993)", "J/MNRAS/389/869 : Multiplicity among bright stellar systems (Eggleton+, 2008)", "J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)", "J/A+A/545/A32 : Chemical abundances of 1111 FGK stars (Adibekyan+, 2012)", "J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)", "J/PASP/124/1279 : Q3 Kepler's combined photometry (Christiansen+, 2012)", "J/A+A/540/A143 : Oscillations of red giants with Kepler (Mosser+, 2012)", "J/MNRAS/431/2240 : Activity in A-type stars from Kepler (Balona, 2013)", "J/ApJ/767/127 : Asteroseismic solutions for 77 Kepler stars (Huber+, 2013)", "J/MNRAS/441/3543 : Possible planets around A stars (Balona, 2014)", "J/A+A/562/A71 : Abundances of solar neighbourhood dwarfs (Bensby+, 2014)", "J/A+A/566/A98 : The Gaia Benchmark Stars - Library (Blanco-Cuaresma+, 2014)", "J/AJ/148/54 : The Hypatia Catalog ((Hinkel+, 2014)", "J/A+A/564/A133 : Gaia FGK benchmark stars: metallicity (Jofre+, 2014)", "J/A+A/571/A47 : Extensive linelist of CH in stellar atm. (Masseron+, 2014)", "J/A+A/572/L5 : Red giant evolution states from seismology (Mosser+, 2014)", "J/ApJS/215/19 : APOKASC catalog of Kepler red giants (Pinsonneault+, 2014)", "J/A+A/577/A9 : Sc, V, Mn, and Co in Milky Way stars (Battistini+, 2015)", "J/A+A/575/A26 : Properties of the Pop. II star HD 140283 (Creevey+, 2015)", "J/A+A/582/A81 : Gaia FGK benchmark stars: abundances (Jofre+, 2015)", "J/MNRAS/452/2127 : Fundamental param. of Kepler stars (Silva Aguirre+, 2015)", "J/AJ/151/101 : Kepler Mission. VIII. False positives (Abdul-Masih+, 2016)", "J/A+A/586/A49 : r- & s- process elements in MW disk (Battistini+, 2016)", "J/MNRAS/460/1970 : Kepler {delta}Sct stars amplitude modulation (Bowman+, 2016)", "J/ApJ/829/23 : Stellar flares from Q0-Q17 Kepler LCs (Davenport, 2016)", "J/A+A/592/A70 : Gaia FGK stars: low-metallicities cand. (Hawkins+, 2016)", "J/A+A/594/A43 : APOGEE/Kepler sample stars abundances (Hawkins+, 2016)", "J/MNRAS/467/1830 : Starspots on A stars (Balona, 2017)", "J/ApJ/844/102 : KIC star plx from asteroseismology vs Gaia (Huber+, 2017)", "J/ApJ/835/172 : Kepler asteroseismic LEGACY sample. I. (Lund+, 2017)", "J/MNRAS/471/770 : Parameters & IR excesses of Gaia DR1 stars (McDonald+, 2017)", "J/ApJS/233/23 : APOKASC cat. of KIC dwarfs and subgiants (Serenelli+, 2017)", "J/ApJ/835/173 : Kepler asteroseism. LEGACY sample II. (Silva Aguirre+, 2017)", "J/MNRAS/474/4322 : Orbital parameters of 341 new binaries (Murphy+, 2018)", "J/A+A/609/A116 : Low extinction TGAS HR Catalogue (Ruiz-Dern+, 2018)", "http://gaia-kepler.fun/ : Gaia and Kepler/K2 cross-matched catalogs webpage", "http://archive.stsci.edu/kepler/data_search/search.php : Kepler data on MAST"], "keyword_cds": "Asteroseismology; Stars, giant; Stars, variable; Radial velocities Abundances; Photometry; Spectra, optical; Rotational velocities Stars, masses", "keyword_pub": "asteroseismology ; stars: early-type ; stars: rotation ; stars: variables: general ; techniques: photometric", "abstract": ["We present the first data release of the Kepler Smear Campaign, using", "collateral \"smear\" data obtained in the Kepler four-year mission to", "reconstruct light curves of 102 stars too bright to have been", "otherwise targeted. We describe the pipeline developed to extract and", "calibrate these light curves and show that we attain photometric", "precision comparable to stars analyzed by the standard pipeline in the", "nominal Kepler mission. In this paper, aside from publishing the light", "curves of these stars, we focus on 66 red giants for which we detect", "solar-like oscillations, characterizing 33 of these in detail with", "spectroscopic chemical abundances and asteroseismic masses as", "benchmark stars. We also classify the whole sample, finding nearly all", "to be variable, with classical pulsations and binary effects."], "description": ["We selected all stars on silicon in Kepler with Kp<9 that were", "targeted for fewer than eight quarters. The full sample of stars is", "listed in Table 1.", "The Kepler spacecraft rotates between quarters, so that it cycles", "through four orientation \"seasons\" each rotated from the last by 90{deg}.", "When generating light curves of the Kepler smear stars, we followed", "the methods described by Pope+ (2016MNRAS.455L..36P), with some", "improvements. See section 2.2 for further explanations.", "We have obtained high-resolution spectroscopy with the Tillinghast", "Reflector Echelle Spectrograph (TRES) for 63 stars, mainly giants, in", "order to constrain stellar parameters and elemental abundances.", "Operating with a spectral resolving power of R=44000, we have obtained", "spectra with a mean S/N of ~100 per resolution element."], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/ab2c04"], "orcid_pub": ["0000-0003-2595-9114"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Input catalog ", "columns": [{"name": "Name", "desc": "Identifier "}, {"name": "m_Name", "desc": "Component identifier for HD 189636 "}, {"name": "SpType", "desc": "SIMBAD spectral type if available "}, {"name": "[Fe/H]", "desc": "[-0.6/1.4]? Metallicity "}, {"name": "theta", "desc": "[0.226/3.429]? Estimated angular size for interferometric scheduling"}, {"name": "Obs", "desc": "Observing comment "}, {"name": "Sea", "desc": "[1/4] Season observed "}, {"name": "Teff", "desc": "[3676/9887]? Effective temperature "}, {"name": "log(g)", "desc": "[1.4/4.4]? log surface gravity "}, {"name": "E(B-V)", "desc": "[0.01/0.09]? The (B-V) color excess "}, {"name": "gmag", "desc": "[5.3/10.5] Apparent SDSS g band magnitude "}, {"name": "rmag", "desc": "[5/9] Apparent SDSS r band magnitude "}, {"name": "Jmag", "desc": "[1.8/8.3] Apparent 2MASS J band magnitude "}, {"name": "kpmag", "desc": "[5/8.7] Apparent Kepler magnitude "}, {"name": "Edge", "desc": "[0/458]? Distance from edge of Kepler chip "}, {"name": "Note", "desc": "Additional notes "}, {"name": "IF?", "desc": "Interferometry available? "}, {"name": "TRES?", "desc": "TRES data available? "}, {"name": "RAdeg", "desc": "[281.2/300.5] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[37/51.4] Declination (J2000) "}, {"name": "KIC", "desc": "[1572070/12456737] Kepler identifier "}, {"name": "Class", "desc": "Variability classification (1) "}, {"name": "rEst", "desc": "[41/1867]? Estimated radius from KIC "}, {"name": "b_rEst", "desc": "[41/1746]? Lower boundary on rEst "}, {"name": "B_rEst", "desc": "[41/2005]? Upper boundary on rEst "}, {"name": "RAIdeg", "desc": "Input Right Ascension (J2000) "}, {"name": "DEIdeg", "desc": "Input Declination (J2000) "}, {"name": "Sep", "desc": "[3e-7/0.0007] Distance "}, {"name": "---", "desc": "[Gaia DR2] "}, {"name": "Gaia", "desc": "Gaia DR2 designation "}, {"name": "RAGdeg", "desc": "Gaia DR2 Right Ascension (J2000) "}, {"name": "DEGdeg", "desc": "Gaia DR2 Declination (J2000) "}, {"name": "GLON", "desc": "[68.8/84] Galactic longitude "}, {"name": "GLAT", "desc": "[5.9/20] Galactic latitude "}, {"name": "ELON", "desc": "[290/323.7] Ecliptic longitude "}, {"name": "ELAT", "desc": "[57.9/72] Ecliptic latitude "}, {"name": "plx", "desc": "[0.5/24.3]? Gaia parallax "}, {"name": "pmRA", "desc": "[-94.7/84.4]? Proper motion along RA "}, {"name": "pmDE", "desc": "[-104.8/120.3]? Proper motion along DE "}, {"name": "Gmag", "desc": "[4.8/8.7] Mean Gaia DR2 magnitude "}, {"name": "bpmag", "desc": "[5/9.3] Mean Gaia DR2 blue passband magnitude"}, {"name": "rpmag", "desc": "[4/8.2] Mean Gaia DR2 red passband magnitude"}, {"name": "e_RAGdeg", "desc": "[0.01/1] Uncertainty in RAGdeg "}, {"name": "e_DEGdeg", "desc": "[0.02/1] Uncertainty in DEGdeg "}, {"name": "e_plx", "desc": "[0.01/0.4]? Uncertainty in plx "}, {"name": "e_pmRA", "desc": "[0.03/0.7]? Uncertainty in pmRA "}, {"name": "e_pmDE", "desc": "[0.03/0.7]? Uncertainty in pmDE "}, {"name": "E_Gmag", "desc": "[0/1.3]? Upper percentile uncertainty in Gmag"}, {"name": "e_Gmag", "desc": "[0.07/2.5]? Lower percentile uncertainty in Gmag"}, {"name": "FileName", "desc": "Name of the FITS file in subdirectory Sp; column added by CDS"}, {"name": "m_FileName", "desc": "? Number indicating the number of spectra available in the subdirectory Sp for this star; column added by CDS"}]}, {"name": "table2.dat", "desc": "Global asteroseismic parameters for the red giant sample as discussed in Section 2.3", "columns": [{"name": "Name", "desc": "Object identifier "}, {"name": "Delnu", "desc": "[0.37/5.94] Mean large spacing {Delta}{nu} "}, {"name": "e_Delnu", "desc": "[0.004/0.06] Uncertainty in Delnu "}, {"name": "numax", "desc": "[1.5/70] Asteroseismic frequency at maximum amplitude {nu}_max_"}, {"name": "e_numax", "desc": "[0.03/1.1] Uncertainty in numax "}, {"name": "eps", "desc": "[0.6/1.1] Asteroseismic parameter {epsilon} "}, {"name": "e_eps", "desc": "[0.01/0.4] Uncertainty in epsilon "}]}, {"name": "table3.dat", "desc": "Fundamental stellar parameters for the red giant sample as determined jointly by asteroseismology and spectroscopy", "columns": [{"name": "Name", "desc": "Object identifier "}, {"name": "BJD", "desc": "Barycentric Julian Date; TDB "}, {"name": "RVel", "desc": "[-80.4/31] Radial velocity "}, {"name": "e_RVel", "desc": "[0.01/0.2] Uncertainty in RVel "}, {"name": "Teff", "desc": "[3556/5090] Effective temperature "}, {"name": "e_Teff", "desc": "[50] Uncertainty in Teff "}, {"name": "log(g)a", "desc": "[1/2.8] log surface gravity from asteroseismology"}, {"name": "e_log(g)a", "desc": "[0.1] Uncertainty in log(g)a "}, {"name": "[M/H]", "desc": "[-1.7/0.2] Metallicity "}, {"name": "e_[M/H]", "desc": "[0.08] Uncertainty in [M/H] "}, {"name": "Vsin(i)", "desc": "[3.5/11] Projected rotational velocity "}, {"name": "e_Vsin(i)", "desc": "[0.5] Uncertainty in Vsin(i) "}, {"name": "CCF", "desc": "[0.9/1.1] Unknown "}, {"name": "SNRe", "desc": "[31.7/187.2] Unknown "}, {"name": "nAps", "desc": "[3] Unknown (always = 3) "}, {"name": "Exp", "desc": "[45/360] Exposure time "}, {"name": "Spec", "desc": "Spectrograph used; always \"tres\" "}, {"name": "Res", "desc": "Spectrograph resolution "}, {"name": "Version", "desc": "Method used in reduction (always \"SPC2.9\"); the Stellar Parameter Classification code (SPC; Buchhave+ 2012, J/other/Nat/486.375)"}, {"name": "numax", "desc": "[1.5/69.8] Asteroseismic parameter {nu}_max_ (1)"}, {"name": "e_numax", "desc": "[0.03/1.1] Uncertainty in numax "}, {"name": "log(g)", "desc": "[1/2.8] log surface gravity "}, {"name": "e_log(g)", "desc": "[0.003/0.02] Uncertainty in log(g) "}, {"name": "Mass", "desc": "[0.7/3.4] Mass "}, {"name": "E_Mass", "desc": "[0.02/0.3] Upper uncertainty in Mass "}, {"name": "e_Mass", "desc": "[0.007/0.2] Lower uncertainty in Mass "}, {"name": "Rad", "desc": "[9.6/48.6] Radius "}, {"name": "E_Rad", "desc": "[0.02/2] Upper uncertainty in Rad "}, {"name": "e_Rad", "desc": "[0.03/2] Lower uncertainty in Rad "}, {"name": "log(g)s", "desc": "[1/2.8] log surface gravity from spectroscopy "}, {"name": "E_log(g)s", "desc": "[0.001/0.02] Upper uncertainty in log(g)s "}, {"name": "e_log(g)s", "desc": "[0.001/0.02] Lower uncertainty in log(g)s "}, {"name": "logAge", "desc": "[0.2/16] log age "}, {"name": "E_logAge", "desc": "[0.02/3.6] Upper uncertainty in logAge "}, {"name": "e_logAge", "desc": "[0/4] Lower uncertainty in logAge "}]}, {"name": "table4.dat", "desc": "Chemical abundances relative to iron for stars in the red giant sample as determined by BACCHUS, differential line-by-line comparison to Arcturus, as described in Section 2.4", "columns": [{"name": "Name", "desc": "Object identifier "}, {"name": "[O/Fe]", "desc": "?=-9.999 log O/Fe abundance ratio (always blank) (1)"}, {"name": "e_[O/Fe]", "desc": "?=-9.999 Uncertainty in [O/Fe] (always blank) (1)"}, {"name": "[Mg/Fe]", "desc": "[0.03/0.4]?=-9.999 log Mg/Fe abundance ratio (1) "}, {"name": "e_[Mg/Fe]", "desc": "[0.007/0.2]?=-9.999 Uncertainty in [Mg/Fe] (1) "}, {"name": "[Ca/Fe]", "desc": "[-0.3/0.1]?=-9.999 log Ca/Fe abundance ratio (1) "}, {"name": "e_[Ca/Fe]", "desc": "[0.001/0.07]?=-9.999 Uncertainty in [Ca/Fe] (1) "}, {"name": "[Si/Fe]", "desc": "[-0.0041/0.4]?=-9.999 log Si/Fe abundance ratio (1)"}, {"name": "e_[Si/Fe]", "desc": "[0.008/0.3]?=-9.999 Uncertainty in [Si/Fe] (1) "}, {"name": "[Ti/Fe]", "desc": "[-0.3/0.4]?=-9.999 log Ti/Fe abundance ratio (1) "}, {"name": "e_[Ti/Fe]", "desc": "[0.006/0.1]?=-9.999 Uncertainty in [Ti/Fe] (1) "}, {"name": "[Al/Fe]", "desc": "[0.04/0.3]?=-9.999 log Al/Fe abundance ratio (1) "}, {"name": "e_[Al/Fe]", "desc": "[0.0003/0.1]?=-9.999 Uncertainty in [Al/Fe] (1) "}, {"name": "[Ni/Fe]", "desc": "[-0.3/0.3]?=-9.999 log Ni/Fe abundance ratio (1) "}, {"name": "e_[Ni/Fe]", "desc": "[0.01/0.3]?=-9.999 Uncertainty in [Ni/Fe] (1) "}, {"name": "[Na/Fe]", "desc": "?=-9.999 log Na/Fe abundance ratio (always blank) (1)"}, {"name": "e_[Na/Fe]", "desc": "?=-9.999 Uncertainty in [Na/Fe] (always blank) (1)"}, {"name": "[Mn/Fe]", "desc": "[-0.2/0.3]?=-9.999 log Mn/Fe abundance ratio (1) "}, {"name": "e_[Mn/Fe]", "desc": "[0.02/0.1]?=-9.999 Uncertainty in [Mn/Fe] (1) "}, {"name": "[Cr/Fe]", "desc": "[-0.4/0.2]?=-9.999 log Cr/Fe abundance ratio (1) "}, {"name": "e_[Cr/Fe]", "desc": "[0.0003/0.2]?=-9.999 Uncertainty in [Cr/Fe] (1) "}, {"name": "[Co/Fe]", "desc": "[-0.3/0.2]?=-9.999 log Co/Fe abundance ratio (1) "}, {"name": "e_[Co/Fe]", "desc": "[0.007/0.2]?=-9.999 Uncertainty in [Co/Fe] (1) "}, {"name": "[V/Fe]", "desc": "[-0.2/0.4]?=-9.999 log V/Fe abundance ratio (1) "}, {"name": "e_[V/Fe]", "desc": "[0.002/0.1]?=-9.999 Uncertainty in [V/Fe] (1) "}, {"name": "[Cu/Fe]", "desc": "[-0.8/0.08]?=-9.999 log Cu/Fe abundance ratio (1) "}, {"name": "e_[Cu/Fe]", "desc": "[0.0007/0.2]?=-9.999 Uncertainty in [Cu/Fe] (1) "}]}, {"name": "table5.dat", "desc": "Chemical abundances relative to iron of neutron capture elements for stars in the red giant sample as determined by BACCHUS, without differential line-by-line comparison to Arcturus, as described in Section 2.4", "columns": [{"name": "Name", "desc": "Object identifier "}, {"name": "[Mg/Fe]", "desc": "[0.02/0.5]?=-9.999 log Mg/Fe abundance ratio (1) "}, {"name": "e_[Mg/Fe]", "desc": "[0.01/0.2]?=-9.999 Uncertainty in [Mg/Fe] (1) "}, {"name": "[Si/Fe]", "desc": "[-0.1/0.4]?=-9.999 log Si/Fe abundance ratio (1) "}, {"name": "e_[Si/Fe]", "desc": "[0.01/0.2]?=-9.999 Uncertainty in [Si/Fe] (1) "}, {"name": "[Ca/Fe]", "desc": "[-0.2/0.2]?=-9.999 log Ca/Fe abundance ratio (1) "}, {"name": "e_[Ca/Fe]", "desc": "[0/0.09]?=-9.999 Uncertainty in [Ca/Fe] (1) "}, {"name": "[Ti/Fe]", "desc": "[-0.2/0.2]?=-9.999 log Ti/Fe abundance ratio (1) "}, {"name": "e_[Ti/Fe]", "desc": "[0.001/0.2]?=-9.999 Uncertainty in [Ti/Fe] (1) "}, {"name": "[Mn/Fe]", "desc": "[-0.7/-0.05]?=-9.999 log Mn/Fe abundance ratio (1)"}, {"name": "e_[Mn/Fe]", "desc": "[0.002/0.2]?=-9.999 Uncertainty in [Mn/Fe] (1) "}, {"name": "[Co/Fe]", "desc": "[-0.3/0.2]?=-9.999 log Co/Fe abundance ratio (1) "}, {"name": "e_[Co/Fe]", "desc": "[0.01/0.2]?=-9.999 Uncertainty in [Co/Fe] (1) "}, {"name": "[O/Fe]", "desc": "[0.2/0.4]?=-9.999 log O/Fe abundance ratio (1) "}, {"name": "e_[O/Fe]", "desc": "[0.02/0.1]?=-9.999 Uncertainty in [O/Fe] (1) "}, {"name": "[Li/Fe]", "desc": "[-0.7/0.03]?=-9.999 log Li/Fe abundance ratio (1) "}, {"name": "e_[Li/Fe]", "desc": "[0.1]?=-9.999 Uncertainty in [Li/Fe] (1) "}, {"name": "[Cr/Fe]", "desc": "[-0.5/0.03]?=-9.999 log Cr/Fe abundance ratio (1) "}, {"name": "e_[Cr/Fe]", "desc": "[0.006/0.3]?=-9.999 Uncertainty in [Cr/Fe] (1) "}, {"name": "[Cu/Fe]", "desc": "[-0.4/0.4]?=-9.999 log Cu/Fe abundance ratio (1) "}, {"name": "e_[Cu/Fe]", "desc": "[0.02/0.3]?=-9.999 Uncertainty in [Cu/Fe] (1) "}, {"name": "[La/Fe]", "desc": "[-0.4/0.3]?=-9.999 log La/Fe abundance ratio (1) "}, {"name": "e_[La/Fe]", "desc": "[0.006/0.3]?=-9.999 Uncertainty in [La/Fe] (1) "}, {"name": "[Al/Fe]", "desc": "[0.1/0.4]?=-9.999 log Al/Fe abundance ratio (1) "}, {"name": "e_[Al/Fe]", "desc": "[0.004/0.2]?=-9.999 Uncertainty in [Al/Fe] (1) "}, {"name": "[Na/Fe]", "desc": "[-0.5/0.4]?=-9.999 log Na/Fe abundance ratio (1) "}, {"name": "e_[Na/Fe]", "desc": "[0.001/0.2]?=-9.999 Uncertainty in [Na/Fe] (1) "}, {"name": "[Ni/Fe]", "desc": "[-0.08/0.3]?=-9.999 log Ni/Fe abundance ratio (1) "}, {"name": "e_[Ni/Fe]", "desc": "[0.02/0.3]?=-9.999 Uncertainty in [Ni/Fe] (1) "}, {"name": "[Ba/Fe]", "desc": "[-0.05/0.6]?=-9.999 log Ba/Fe abundance ratio (1) "}, {"name": "e_[Ba/Fe]", "desc": "[0.1]?=-9.999 Uncertainty in [Ba/Fe] (1) "}, {"name": "[Sr/Fe]", "desc": "[-0.5/0.3]?=-9.999 log Sr/Fe abundance ratio (1) "}, {"name": "e_[Sr/Fe]", "desc": "[0.01/0.3]?=-9.999 Uncertainty in [Sr/Fe] (1) "}, {"name": "[Y/Fe]", "desc": "[-0.5/-0.05]?=-9.999 log Y/Fe abundance ratio (1) "}, {"name": "e_[Y/Fe]", "desc": "[0.006/0.3]?=-9.999 Uncertainty in [Y/Fe] (1) "}, {"name": "[Eu/Fe]", "desc": "[-0.09/0.3]?=-9.999 log Eu/Fe abundance ratio (1) "}, {"name": "e_[Eu/Fe]", "desc": "[0.1]?=-9.999 Uncertainty in [Eu/Fe] (1) "}, {"name": "[V/Fe]", "desc": "[-0.3/0.3]?=-9.999 log V/Fe abundance ratio (1) "}, {"name": "e_[V/Fe]", "desc": "[0.01/0.2]?=-9.999 Uncertainty in [V/Fe] (1) "}, {"name": "[Sc/Fe]", "desc": "[-0.05/0.2]?=-9.999 log Sc/Fe abundance ratio (1) "}, {"name": "e_[Sc/Fe]", "desc": "[0.03/0.2]?=-9.999 Uncertainty in [Sc/Fe] (1) "}, {"name": "[Zr/Fe]", "desc": "[-0.5/0.4]?=-9.999 log Zr/Fe abundance ratio (1) "}, {"name": "e_[Zr/Fe]", "desc": "[0.02/0.3]?=-9.999 Uncertainty in [Zr/Fe] (1) "}, {"name": "[Nd/Fe]", "desc": "[-0.7/0.2]?=-9.999 log Nd/Fe abundance ratio (1) "}, {"name": "e_[Nd/Fe]", "desc": "[0.02/0.3]?=-9.999 Uncertainty in [Nd/Fe] (1) "}]}, {"name": "lcs/*", "desc": "Individual light curves from the Kepler Smear Campaign in CSV format", "columns": []}, {"name": "sp/*", "desc": "Raw data of all spectra in FITS format ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_247_50"}} {"id": "J/ApJS/247/50", "title_cds": "Late-type contact binaries in CSS DR1", "title_create": "Sun+, 2020", "year": "2020", "author": "Sun W., Chen X., Deng L., de Grijs R.", "title_pub": "Physical parameters of late-type contact binaries in the northern Catalina Sky Survey.", "first_author": "Sun W.", "ref_biblio": [""], "bibcode": ["2020ApJS..247...50S"], "see_also": ["I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "V/119 : Catalogue of field contact binary stars (Pribulla+, 2003)", "V/146 : LAMOST DR1 catalogs (Luo+, 2015)", "J/AJ/106/2096 : Limb-darkening coefficients in binaries (Van Hamme 1993)", "J/A+A/311/523 : Photometry of W UMa (Maceroni+, 1996)", "J/A+A/426/1001 : Catalog of contact binary stars (Csizmadia+, 2004)", "J/ApJ/629/1055 : Evolution of close binary systems (Yakut+, 2005)", "J/MNRAS/373/1483 : W UMa type and CAB stars dynamical evolution (Eker+, 2006)", "J/AJ/131/621 : Catalog of 1022 bright contact binary stars (Gettel+, 2006)", "J/A+A/528/A90 : SuperWASP short period eclipsing binaries (Norton+, 2011)", "J/ApJ/763/32 : Galactic halo RRab stars from CSS (Drake+, 2013)", "J/AJ/146/101 : LINEAR. III. Periodic variables (Palaversa+, 2013)", "J/ApJS/208/9 : Intrinsic colors & temperatures of PMS stars (Pecaut+, 2013)", "J/MNRAS/430/2029 : Initial masses of W UMa contact binaries (Yildiz+, 2013)", "J/ApJS/213/9 : Catalina Surveys periodic variable stars (Drake+, 2014)", "J/AJ/148/81 : APASS BVgri photometry of RAVE stars. I. (Munari+, 2014)", "J/MNRAS/446/2251 : Southern Catalina Survey type-ab RR Lyrae (Torrealba+, 2015)", "J/AJ/152/129 : VR photometry for 914 stars in NGC 188 (Chen+, 2016)", "J/MNRAS/465/4678 : 9380 contact binaries from CRTS VSC (Marsh+, 2017)", "J/ApJ/859/140 : Multi-band magnitudes for W UMa EB* candidates (Chen+, 2018)", "J/ApJS/237/28 : WISE catalog of periodic variable stars (Chen+, 2018)", "J/AJ/156/241 : A first cat. of var. stars measured by ATLAS (Heinze+, 2018)"], "keyword_cds": "Binaries, eclipsing; Stars, masses ; Effective temperatures ; Stars, diameters; Optical", "keyword_pub": "Astronomy data analysis ; contact binary stars ; fundamental parameters of stars", "abstract": ["We present the physical parameters of 2335 late-type contact binary", "(CB) systems extracted from the Catalina Sky Survey (CSS). Our sample", "was selected from the CSS Data Release 1 by strictly limiting the", "prevailing temperature uncertainties and light-curve fitting", "residuals, allowing us to almost eliminate any possible contaminants.", "We developed an automatic Wilson-Devinney-type code to derive the", "relative properties of CBs based on their light-curve morphology. By", "adopting the distances derived from CB (orbital) period-luminosity", "relations (PLRs), combined with the well-defined mass-luminosity", "relation for the systems' primary stars and assuming solar", "metallicity, we calculated the objects' masses, radii, and", "luminosities. Our sample of fully eclipsing CBs contains 1530 W-, 710", "A-, and 95 B-type CBs. A comparison with literature data and with the", "results from different surveys confirms the accuracy and coherence of", "our measurements. The period distributions of the various CB subtypes", "are different, hinting at a possible evolutionary sequence. W-type CBs", "are clearly located in a strip in the total mass versus mass-ratio", "plane, while A-type CBs may exhibit a slightly different dependence.", "There are no significant differences among the PLRs of A- and W-type", "CBs, but the PLR zero-points are affected by their mass ratios and", "fill-out factors. Determination of zero-point differences for", "different types of CBs may help us improve the accuracy of the", "resulting PLRs. We demonstrate that automated approaches to deriving", "CB properties could be a powerful tool for application to the much", "larger CB samples expected to result from future surveys."], "description": ["We used contact binary (CB) data from the Catalina Sky Survey (CSS)", "Data Release 1 (CSDR1; Drake+ 2014, J/ApJS/213/9). The survey used", "three telescopes to cover the sky between declinations DEC=-75{deg}", "and +70{deg} at Galactic latitudes |b|>15{deg}."], "type": ["CCC"], "doi_pub": ["10.3847/1538-4365/ab7894"], "orcid_pub": ["0000-0002-3279-0233"], "data": "f-v", "date_creation": "20-Jul-2020", "xmatch": "J/ApJS/247/50/table1", "last_update": "07-Sep-2021", "catid": "22470050", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Total-eclipsing contact binary (CB) catalog ", "columns": [{"name": "---", "desc": "[CSS_] "}, {"name": "CRTS", "desc": "Catalina Sky Survey (CSS) identifier (JHHMMSS.s+DDMMSS)"}, {"name": "RAdeg", "desc": "Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-19.7/70.1] Declination (J2000) "}, {"name": "Period", "desc": "[0.196/0.56] Orbital period "}, {"name": "Teff1", "desc": "[3436/15530] Primary effective temperature (1) "}, {"name": "Teff2", "desc": "[3520/11079] Secondary effective temperature (1)"}, {"name": "e_Teff1", "desc": "[8/4226]? Uncertainty in Teff1 (1) "}, {"name": "e_Teff2", "desc": "[13/3290]? Uncertainty in Teff2 (1) "}, {"name": "inc", "desc": "[70/90] Inclination angle "}, {"name": "e_inc", "desc": "[0.1/22.2] Uncertainty in inc "}, {"name": "Omega", "desc": "[1.8/15] Surface potential ({Omega}={Omega}_1_={Omega}_2_)"}, {"name": "e_Omega", "desc": "[0/0.8] Uncertainty in Omega "}, {"name": "q", "desc": "[0.07/0.8] Mass ratio; M2/M1 "}, {"name": "e_q", "desc": "[0.09] Uncertainty in q "}, {"name": "f", "desc": "[-1/1] Fill-out factor (2) "}, {"name": "e_f", "desc": "[0.01/4.1] Uncertainty in f "}, {"name": "LFrac", "desc": "[0.4/1] Primary to total V band luminosity ratio"}, {"name": "e_LFrac", "desc": "[0/0.4] Uncertainty in LFrac "}, {"name": "OT", "desc": "CB classification (1530 W-, 710 A-, and 95 B-type CBs)"}, {"name": "M1", "desc": "[0.8/2.5] Primary mass "}, {"name": "M2", "desc": "[0.08/1.4] Secondary mass "}, {"name": "e_M1", "desc": "[0.02/0.1] Uncertainty in M1 "}, {"name": "e_M2", "desc": "[0.07/0.3] Uncertainty in M2 "}, {"name": "r1", "desc": "[0.7/2.2] Primary radius "}, {"name": "r2", "desc": "[0.3/1.5] Secondary radius "}, {"name": "e_r1", "desc": "[0.02/0.07] Uncertainty in r1 "}, {"name": "e_r2", "desc": "[0.01/0.03] Uncertainty in r2 "}, {"name": "L1", "desc": "[0.3/26.8] Primary luminosity "}, {"name": "L2", "desc": "[0.05/9.2] Secondary luminosity "}, {"name": "e_L1", "desc": "[0.08/6.4] Uncertainty in L1 "}, {"name": "e_L2", "desc": "[0.02/4.6] Uncertainty in L2 "}, {"name": "a", "desc": "[1.5/4.2] Semi-major axis "}, {"name": "e_a", "desc": "[0.03/0.1] Uncertainty in a "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_249_7"}} {"id": "J/ApJS/249/7", "title_cds": "Stellar ages & masses of main-sequence and giant stars", "title_create": "Bu+, 2020", "year": "2020", "author": "Bu Y., Kumar Y.B., Xie J., Pan J., Zhao G., Wu Y.", "title_pub": "Estimation of stellar ages and masses using Gaussian process regression.", "first_author": "Bu Y.", "ref_biblio": [""], "bibcode": ["2020ApJS..249....7B"], "see_also": ["V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)", "J/AcA/41/167 : UBV photometry in Berkeley 32 (Kaluzny+, 1991)", "J/A+A/348/897 : Ages of main-sequence stars (Lachaume+, 1999)", "J/A+AS/141/371 : Low-mass stars evolutionary tracks (Girardi+, 2000)", "J/ApJ/562/528 : Teff and log(g) of low-metallicity stars (Snider+, 2001)", "J/AJ/127/1513 : Lick indices on M67 members (Schiavon+, 2004)", "J/A+A/530/A115 : Rotating massive MS stars evolutionary models (Brott+, 2011)", "J/A+A/537/A146 : Stellar models with rotation. 0.8"], "bibcode": ["2020ApJS..250...32L"], "see_also": ["II/363 : The band-merged unWISE Catalog (Schlafly+, 2019)", "VIII/51 : the FIRST Survey, version 1998Feb (White+ 1998)", "VIII/90 : The FIRST Survey Catalog, Version 12Feb16 (Becker+ 2012)", "J/MNRAS/356/568 : Deep Chandra survey of the Groth Strip (Nandra+, 2005)", "J/A+A/497/635 : XMM-Newton wide-field survey in COSMOS (Cappelluti+, 2009)", "J/ApJ/692/758 : BAL QSOs in SDSS-DR5 (Gibson+, 2009)", "J/ApJS/180/102 : AEGIS-X: Chandra deep survey (Laird+, 2009)", "J/A+A/493/339 : XMM-Newton serendipitous Survey. V. (Watson+, 2009)", "J/ApJS/202/6 : XDEEP2 survey catalog (Goulding+, 2012)", "J/ApJS/199/34 : Clusters of galaxies in SDSS-III (Wen+, 2012)", "J/ApJ/766/60 : GALEX Time Domain Survey I. UV variables (Gezari+, 2013)", "J/ApJS/220/10 : AEGIS-X Deep survey of EGS (AEGIS-XD) (Nandra+, 2015)", "J/A+A/577/A121 : The XMM-ATLAS catalogues (Ranalli+, 2015)", "J/ApJS/216/4 : SDSS-RM project: technical overview (Shen+, 2015)", "J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016)", "J/A+A/594/A116 : HI4PI spectra and column density maps (HI4PI team+, 2016)", "J/ApJ/817/172 : X-ray Observations of Stripe 82 (LaMassa+, 2016)", "J/ApJS/228/2 : Chandra Deep Field-South survey: 7Ms sources (Luo+, 2017)", "J/MNRAS/473/4937 : AllWISE ctp to ROSAT/2RXS & XMMSLEW2 cat. (Salvato+, 2018)", "http://www.mpe.mpg.de/XraySurveys/XMM-RM/ : XMM-RM project home page", "http://www.legacysurvey.org/ : Legacy Survey home page"], "keyword_cds": "X-ray sources; Cross identifications; Photometry, ugriz", "keyword_pub": "Astronomy data analysis ; Supermassive black holes ; Active galactic nuclei ; X-ray active galactic nuclei ; Quasars ; X-ray point sources", "abstract": ["The XMM-RM project was designed to provide X-ray coverage of the Sloan", "Digital Sky Survey Reverberation Mapping (SDSS-RM) field. Forty-one", "XMM-Newton exposures, placed surrounding the Chandra AEGIS field, were", "taken, covering an area of 6.13deg^2^ and reaching a nominal exposure", "depth of ~15ks. We present an X-ray catalog of 3553 sources detected", "in these data, using a PSF-fitting algorithm and a sample selection", "threshold that produces a ~5% fraction of spurious sources. In", "addition to the PSF-fitting likelihood, we calculate a second source", "reliability measure based on Poisson theory using source and", "background counts within an aperture. Using the Poissonian likelihood,", "we select a subsample with a high purity and find that it has number", "count profiles similar to previous X-ray surveys. The Bayesian method", "\"NWAY\" was employed to identify counterparts of the X-ray sources from", "the optical Legacy and the IR unWISE catalogs, using a two-dimensional", "unWISE magnitude-color prior created from optical/IR counterparts of", "Chandra X-ray sources. A significant number of the optical/IR", "counterparts correspond to sources with low detection likelihoods,", "proving the value of retaining the low-likelihood detections in the", "catalog. A total of 932 of the XMM-RM sources are covered by SDSS", "spectroscopic observations, where 89% of them are classified as active", "galactic nuclei, and 71% of these active galactic nuclei are in the", "SDSS-RM quasar catalog. Among the SDSS-RM quasars, 80% are detectable", "at the depth of the XMM observations."], "description": ["The XMM-Newton observations cover a total sky area of ~6.13deg^2^", "within the 7deg^2^ Sloan Digital Sky Survey Reverberation Mapping (RM)", "field. The main data set is formed by 41 XMM observations with", "individual exposure times of ~15ks, with 13 pointings obtained in AO15", "(PI P. Green) and 28 in AO16 (PI A. Merloni). All observations were", "taken in full-frame mode of the EPIC-PN/MOS cameras.", "In addition to these XMM-RM dedicated observations, we also reanalyze", "seven archival XMM observations in the RM field (see Figure 1),", "including five Groth-Westphal Strip observations (PI R. Griffiths) and", "two object-targeted observations (0503960101, PI M. Agueros;", "0723860101, PI D. Lin).", "We identify multiband counterparts of the XMM-RM sources from the", "optical Legacy (Dey+ 2019AJ....157..168D) and the infrared unWISE", "(Schlafly+ 2019, II/363) catalogs. The Legacy catalog presents g-, r-,", "and z-band magnitudes for each source. The unWISE catalog provides the", "W1 (3.4um) and W2 (4.6um) magnitudes, although some sources are", "detected in only one of the two bands. Considering that the typical", "XMM positional uncertainty (~2\", half-pixel size) is much larger than", "that of the optical/IR positions, we first combine the Legacy and", "unWISE catalogs and then match the XMM sources to the combined", "catalog. See Section 5 for further details.", "In order to efficiently identify optical/IR counterparts of the XMM-RM", "sources using the Bayesian method NWAY (Salvato+ 2018, J/MNRAS/473/4937),", "we create optical/IR color and magnitude priors on the basis of the", "Chandra catalogs of C-COSMOS (Marchesi+ 2016ApJ...830..100M) and", "Stripe 82 (LaMassa+ 2016, J/ApJ/817/172). See Section 5.2."], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "maincat.dat", "desc": "XMM-RM main X-ray source catalog ", "columns": [{"name": "RACdeg", "desc": "[211.3/216.3] Combined Legacy-unWISE catalog right ascension (J2000) (UWLS_RA) (1)"}, {"name": "DECdeg", "desc": "[51.6/54.6] Combined Legacy-unWISE catalog declination (J2000) (UWLS_DEC) (1)"}, {"name": "eCPos", "desc": "[0.3/8] Error on position (UWLS_POSERR) (1) "}, {"name": "Distbf", "desc": "[-124.5/11.4] Log of ratio between prior and posterior from distance matching"}]}, {"name": "xid.dat", "desc": "Optical-IR counterpart catalog ", "columns": [{"name": "ID", "desc": "[1/3560] Identifier (ID) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) (RA) "}, {"name": "DEdeg", "desc": "Declination (J2000) (DEC) "}, {"name": "ePos", "desc": "[0.08/16] Positional uncertainty from PSF fitting (RADEC_ERR)"}, {"name": "eSys", "desc": "[0.28/1.6] Additional systematic positional uncertainty (SYSERRCC) (1)"}, {"name": "Band", "desc": "[FHS] The detection band that has the highest detection likelihood and in which"}]}, {"name": "phot.dat", "desc": "X-ray photometry of the SDSS-RM catalog ", "columns": [{"name": "RMID", "desc": "SDSS-RM catalog ID (RMID) (G2) "}, {"name": "RAdeg", "desc": "Right ascension in decimal degrees (J2000) (RA)"}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) (DEC) "}, {"name": "CRlimF", "desc": "2{sigma} count rate upper limit in full band (0.5-10keV) on the background-subtracted"}]}, {"name": "table1.dat", "desc": "XMM-RM observations ", "columns": [{"name": "obsID", "desc": "[127921001/804272801] XMM observation ID "}, {"name": "RAdeg", "desc": "[211.7/216] Aim point right ascension (J2000) "}, {"name": "DEdeg", "desc": "[51.8/54.4] Aim point declination (J2000) "}, {"name": "Date", "desc": "Date of observation (UT) "}, {"name": "ModePN", "desc": "Observation mode and filter for PN camera (1) "}, {"name": "ExpPN", "desc": "[2.8/45]? Cleaned exposure time (\"ONTIME\") after removal of background flares for PN"}, {"name": "RatioPN", "desc": "[18/99]? Clean to raw exposure time ratio for PN"}, {"name": "ModeMOS", "desc": "Observation mode and filter for MOS camera (1) "}, {"name": "ExpMOS", "desc": "[4.1/53.1] Cleaned exposure time (\"ONTIME\") after removal of background flares for MOS"}, {"name": "RatioMOS", "desc": "[34/100] Clean to raw exposure time ratio for MOS"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_253_7"}} {"id": "J/ApJS/253/7", "title_cds": "IR parallaxes of brown dwarfs within 20pc", "title_create": "Kirkpatrick+, 2021", "year": "2021", "author": "Kirkpatrick J.D., Gelino C.R., Faherty J.K., Meisner A.M., Caselden D., Schneider A.C., Marocco F., Cayago A.J., Smart R.L., Eisenhardt P.R., Kuchner M.J., Wright E.L., Cushing M.C., Allers K.N., Bardalez Gagliuffi D.C., Burgasser A.J., Gagne J., Logsdon S.E., Martin E.C., Ingalls J.G., Lowrance P.J., Abrahams E.S., Aganze C., Gerasimov R., Gonzales E.C., Hsu C.-C., Kamraj N., Kiman R., Rees J., Theissen C., Ammar K., Andersen N.S., Beaulieu P., Colin G., Elachi C.A., Goodman S.J., Gramaize L., Hamlet L.K., Hong J., Jonkeren A., Khalil M., Martin D.W., Pendrill W., Pumphrey B., Rothermich A., Sainio A., Stenner A., Tanner C., Thevenot M., Voloshin N.V., Walla J., Wedracki Z.", "title_pub": "The field substellar mass function based on the full-sky 20pc census of 525 L, T, and Y dwarfs.", "first_author": "Kirkpatrick J.D.", "ref_biblio": [""], "bibcode": ["2021ApJS..253....7K"], "see_also": ["II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)", "II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/ApJ/476/311 : 2MASS M-dwarf discoveries (Kirkpatrick+ 1997)", "J/ApJ/564/421 : Spectra of T dwarfs. I. (Burgasser+, 2002)", "J/AJ/123/3409 : SDSS M, L, and T dwarfs (Hawley+, 2002)", "J/AJ/126/1526 : IR photometry of ultracool dwarfs (Bouy+, 2003)", "J/AJ/126/2487 : T dwarfs in the southern hemisphere (Burgasser+, 2003)", "J/AJ/126/2421 : 2MASS-Selected sample of ultracool dwarfs (Cruz+, 2003)", "J/AJ/125/3302 : HST binary very low mass stars & brown dwarfs (Gizis+, 2003)", "J/AJ/127/2856 : Brown dwarfs in the 2MASS Survey (Burgasser+, 2004)", "J/AJ/127/3553 : JHK phot. & spectroscopy for L and T dwarfs (Knapp+, 2004)", "J/A+A/435/363 : Southern Infrared Proper Motion Survey (Deacon+, 2005)", "J/other/ARA+A/43.195 : L and T dwarf stars (Kirkpatrick, 2005)", "J/A+A/440/1061 : Southern red high proper motion objects (Lodieu+, 2005)", "J/ApJS/159/141 : Spectroscopic properties of cool stars. I. (Valenti+, 2005)", "J/ApJ/637/1067 : NIR spectral classification of T dwarfs (Burgasser+, 2006)", "J/AJ/131/2722 : New L and T dwarfs from the SDSS (Chiu+, 2006)", "J/PASP/118/659 : RI photometry of 2MASS late M and L dwarfs (Liebert+, 2006)", "J/ApJ/651/502 : Spitzer IRAC phot. of M, L, and T dwarfs (Patten+, 2006)", "J/AJ/132/891 : Binaries among nearby L dwarfs (Reid+, 2006)", "J/AJ/133/439 : Luminosity function of M7-L8 ultracool dwarfs (Cruz+, 2007)", "J/AJ/134/1162 : 11 new T dwarfs in 2MASS (Looper+, 2007)", "J/AJ/133/2258 : Activity and kinematics of ultracool dwarfs (Schmidt+, 2007)", "J/MNRAS/390/1517 : Proper motions of field L and T dwarfs (Casewell+, 2008)", "J/ApJ/689/1295 : Lithium test implications for BDs (Kirkpatrick+, 2008)", "J/ApJ/676/1281 : L and T dwarfs in 2MASS/SDSS (Metchev+, 2008)", "J/MNRAS/383/831 : New DENIS nearby L and late-M dwarfs (Phan-Bao+, 2008)", "J/AJ/136/1290 : Ultracool dwarfs from the 2MASS (Reid+, 2008)", "J/AJ/135/785 : SDSS-DR5 low-mass star spectroscopic sample (West+, 2008)", "J/AJ/137/1 : PMs and astrometry of late-type dwarfs (Faherty+, 2009)", "J/ApJ/710/1142 : SpeX spectroscopy of low mass bin. I. (Burgasser+, 2010)", "J/A+A/510/A99 : Epsilon Indi Ba and Bb IR spectra (King+, 2010)", "J/ApJS/190/100 : NIR proper motion survey using 2MASS (Kirkpatrick+, 2010)", "J/AJ/139/1808 : Colors and kinematics of SDSS L dwarfs (Schmidt+, 2010)", "J/AJ/142/77 : New T dwarfs identified in Pan-STARRS 1 (Deacon+, 2011)", "J/ApJS/197/19 : First brown dwarfs discovered by WISE (Kirkpatrick+, 2011)", "J/ApJS/201/19 : Hawaii Infrared Parallax Program. I. (Dupuy+, 2012)", "J/ApJ/752/56 : BDKP. III. Plx for 70 ultracool dwarfs (Faherty+, 2012)", "J/MNRAS/427/3280 : Ultra-cool dwarfs at low Galactic latitudes (Folkes+, 2012)", "J/ApJ/753/156 : T/Y brown dwarfs with WISE photometry (Kirkpatrick+, 2012)", "J/ApJ/748/93 : K-band spectra for 133 nearby M dwarfs (Rojas-Ayala+, 2012)", "J/MNRAS/433/457 : 76 T dwarfs from the UKIDSS LAS (Burningham+, 2013)", "J/MNRAS/430/1171 : Sub-stellar birth rate from UKIDSS (Day-Jones+, 2013)", "J/ApJS/205/6 : T dwarf population revealed by WISE (Mace+, 2013)", "J/ApJS/208/9 : Intrinsic colors & temperatures of PMS stars (Pecaut+, 2013)", "J/PASP/125/809 : New nearby M, L, and T dwarfs (Thompson+, 2013)", "J/ApJ/794/143 : New SpeX Observations of M7-L6 Dwarfs (Bardalez+, 2014)", "J/ApJ/792/119 : Companions to nearby stars from Pan-STARRS 1 (Deacon+, 2014)", "J/AJ/147/94 : Solar neighborhood. XXXII. L and M dwarfs (Dieterich+, 2014)", "J/ApJ/783/121 : BANYAN II. Nearby young assoc. cand. members (Gagne+, 2014)", "J/ApJ/783/122 : AllWISE motion survey (Kirkpatrick+, 2014)", "J/ApJ/781/4 : Photometry of high PM objects from WISE (Luhman, 2014)", "J/ApJ/787/126 : WISE reduced proper motions & spectral types (Luhman+, 2014)", "J/ApJ/792/30 : NEOWISE magnitudes for near-Earth objects (Mainzer+, 2014)", "J/AJ/147/34 : SpeX library of L-type dwarfs (Schneider+, 2014)", "J/MNRAS/443/2327 : New proper motion objects from UKIDSS GPS (Smith+, 2014)", "J/MNRAS/454/593 : Young moving groups in solar neighbourhood (Bell+, 2015)", "J/ApJ/814/118 : L/T transition dwarfs with PS1 & WISE. II. (Best+, 2015)", "J/ApJ/810/158 : M,L,T dwarfs fundamental param. and SEDs (Filippazzo+, 2015)", "J/ApJS/219/33 : BANYAN. VII. Candidate YMG members from BASS (Gagne+, 2015)", "J/MNRAS/449/3651 : L and T dwarfs from UKIDSS LAS (Marocco+, 2015)", "J/AJ/149/5 : Solar neighborhood. XXXV. M dwarfs (Winters+, 2015)", "J/ApJS/225/10 : Kinematic analysis of M7-L8 dwarfs (Faherty+, 2016)", "J/ApJS/224/36 : The AllWISE motion survey (AllWISE2) (Kirkpatrick+, 2016)", "J/ApJ/833/96 : Hawaii infrared plx prog. II. Ultracool dwarfs (Liu+, 2016)", "J/ApJ/817/112 : NEOWISE/AllWISE high PM objects (Schneider+, 2016)", "J/AJ/152/24 : Trigonometric plx of 134 low-mass stars (Weinberger+, 2016)", "J/AJ/154/151 : Solar neighborhood .XXXX. New young stars (Bartlett+, 2017)", "J/AJ/154/147 : Astrometry & phot. for late-type subdwarfs (Dahn+, 2017)", "J/MNRAS/468/3499 : Partially resolved binaries in PS1 data (Deacon+, 2017)", "J/ApJS/231/15 : Astrometric monitoring of ultracool binaries (Dupuy+, 2017)", "J/MNRAS/465/4723 : Log of SALT-RSS observations (Koen+, 2017)", "J/ApJ/842/118 : BDs with spectral type later than T6 (Leggett+, 2017)", "J/AJ/153/95 : Catalog of Suspected Nearby Young Stars (Riedel+, 2017)", "J/AJ/154/69 : ACRONYM II. {beta} Pictoris Moving Group (Shkolnik+, 2017)", "J/MNRAS/469/401 : Known LT dwarfs in the Gaia DR1 (Smart+, 2017)", "J/ApJ/856/23 : BANYAN. XI. The BANYAN {Sigma} algorithm (Gagne+, 2018)", "J/ApJ/854/145 : Opt. phot. & NIR spectroscopy of Wolf 1130 (Mace+, 2018)", "J/ApJ/867/109 : Spitzer observations of Y and T dwarfs (Martin+, 2018)", "J/A+A/619/L8 : Ultra-cool dwarfs candidates in Gaia DR2 (Reyle, 2018)", "J/AJ/158/182 : Discoveries from NEOWISE proper motion survey (Greco+, 2019)", "J/ApJS/240/19 : Parallaxes of late-T and Y dwarfs (Kirkpatrick+, 2019)", "J/AJ/157/101 : HST/WFC3 NIR spectral library (Manjavacas+, 2019)", "J/A+A/629/A139 : Closest stars to the Sun within 50pc catalog (Torres+, 2019)", "J/AJ/159/257 : Hawaii IR plx program. IV. L0-T8 with UKIRT (Best+, 2020)", "J/A+A/642/A179 : beta Pictoris moving group RVs (Miret-Roig+, 2020)"], "keyword_cds": "Parallaxes, trigonometric; Infrared sources; Stars, brown dwarf; Spectral types; Stars, L-type; Stars, T-type; Stars, Y-type", "keyword_pub": "Stellar mass functions ; Trigonometric parallax ; Brown dwarfs ; Solar neighborhood ; Absolute magnitude ; Stellar effective temperatures ; L dwarfs ; T dwarfs ; Y dwarfs ; Stellar classification ; Binary stars ; Two-color diagrams", "abstract": ["We present final Spitzer trigonometric parallaxes for 361 L, T, and Y", "dwarfs. We combine these with prior studies to build a list of 525", "known L, T, and Y dwarfs within 20pc of the Sun, 38 of which are", "presented here for the first time. Using published photometry and", "spectroscopy as well as our own follow-up, we present an array of", "color-magnitude and color-color diagrams to further characterize", "census members, and we provide polynomial fits to the bulk trends.", "Using these characterizations, we assign each object a Teff value and", "judge sample completeness over bins of Teff and spectral type. Except", "for types >=T8 and Teff<600K, our census is statistically complete to", "the 20pc limit. We compare our measured space densities to simulated", "density distributions and find that the best fit is a power law", "(dN/dM{propto}M^-{alpha}^) with {alpha}=0.6+/-0.1. We find that the", "evolutionary models of Saumon & Marley correctly predict the observed", "magnitude of the space density spike seen at 1200K=Y0.5 and with Teff<400K. We conclude that such frigid objects must", "exist in substantial numbers, despite the fact that few have so far", "been identified, and we discuss possible reasons why they have largely", "eluded detection."], "description": ["In Kirkpatrick+ (2019, J/ApJS/240/19), we used the Infrared Array", "Camera (IRAC) to measure preliminary trigonometric parallaxes a", "selection of objects having spectral types of T6 and later. These", "results were based on data from Spitzer programs 70062, 80109, 90007,", "11059, and the first year's data from 13012 (all with Kirkpatrick as", "PI). This left a gap in the L and T dwarf sequence between T6 and the", "latest type for which Gaia has complete coverage (~L5). The aim of", "Spitzer program 14000 (Kirkpatrick, PI) was to astrometrically monitor", "those objects in the gap that lacked published parallaxes of high", "quality but were believed to fall within 23pc. An extension to provide", "additional data points for these objects at the end of the Spitzer", "mission was further approved as program 14326 (Kirkpatrick, PI). See", "Section 3 and Table 2 for the full list of Spitzer program IDs", "(spanning 2004 Nov 01 to 2019 May 30)."], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "New L, T, and Y dwarf candidates ", "columns": [{"name": "---", "desc": "[CWISE] "}, {"name": "CWISE", "desc": "CWISE position-based identifier (JHHMMSS.ss+DDMMSS.s)"}, {"name": "f_CWISE", "desc": "b: background (1) "}, {"name": "Note", "desc": "Note (2) "}, {"name": "Disc", "desc": "Discoverer code (3) "}]}, {"name": "table2.dat", "desc": "Objects on the IRAC ch2 Spitzer Parallax Programs ", "columns": [{"name": "SName", "desc": "Short name used "}, {"name": "PName", "desc": "Short name position code for object "}, {"name": "m_PName", "desc": "Component for object "}, {"name": "FirstObs.Y", "desc": "[2004/2019] First observation date, year "}, {"name": "FirstObs.M", "desc": "First observation date, month "}, {"name": "FirstObs.D", "desc": "First observation date, day in month "}, {"name": "LastObs.Y", "desc": "[2018/2020] Last observation date, year "}, {"name": "LastObs.M", "desc": "Last observation date, month "}, {"name": "LastObs.D", "desc": "Last observation date, day in month "}, {"name": "Baseline", "desc": "[0.5/15] Baseline in years (1) "}, {"name": "Epochs", "desc": "Spitzer IRAC program # (# epochs in program) "}]}, {"name": "table4.dat", "desc": "Astrometry on the Gaia DR2 Reference Frame ", "columns": [{"name": "PName", "desc": "Short name position code for object (HHMM+DDMM) "}, {"name": "RAdeg", "desc": "[1.3/359.4] Right Ascension (ICRS) at Epoch "}, {"name": "DEdeg", "desc": "[-82.2/84.8] Declination (ICRS) at Epoch "}, {"name": "e_RAdeg", "desc": "[0.01/2.5] Positional uncertainty in RA "}, {"name": "e_DEdeg", "desc": "[0.01/2.5] Positional uncertainty in DE "}, {"name": "Src", "desc": "Source (1) "}, {"name": "Epoch", "desc": "[53310.5/58874.8] Epoch, Modified Julian Date (JD-2400000.5)"}, {"name": "X", "desc": "[-150232823/153255842] Solar System position, X, of observation in km (2)"}, {"name": "Y", "desc": "[-152281985/148013402] Solar System position, Y, of observation in km (2)"}, {"name": "Z", "desc": "[-62689519/62070770] Solar System position, Z, of observation in km (2)"}]}, {"name": "table5.dat", "desc": "Parallax and motion fits for objects with high-quality parallaxes", "columns": [{"name": "FName", "desc": "Full name, position-based identifier "}, {"name": "RAdeg", "desc": "Right Ascension (ICRS) at t0 "}, {"name": "e_RAdeg", "desc": "[1.6/175] Positional uncertainty in RA "}, {"name": "DEdeg", "desc": "[-82.2/84.8] Declination (ICRS) at t0 "}, {"name": "e_DEdeg", "desc": "[1.6/141] Positional uncertainty in DE "}, {"name": "t0", "desc": "[57064.5/58254.2] Mean Epoch, Modified Julian Date (JD-2400000.5)"}, {"name": "plx", "desc": "[-12.4/439]? Absolute parallax "}, {"name": "e_plx", "desc": "[1.7/73]? Uncertainty in plx "}, {"name": "pmRA", "desc": "[-8123.7/1289.1] Absolute proper motion in RA "}, {"name": "e_pmRA", "desc": "[0.4/59] Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-3107.5/1311.5] Absolute proper motion in DE "}, {"name": "e_pmDE", "desc": "[0.6/45] Uncertainty in pmDE "}, {"name": "chisq", "desc": "[9.9/4401] {chi}^2 of fit "}, {"name": "dof", "desc": "[17/133] Degrees of freedom "}, {"name": "chisq/dof", "desc": "[0.2/77.2] Reduced {chi}^2 of fit "}, {"name": "NSp", "desc": "[2/39] Number of Spitzer astrometric epochs "}, {"name": "NW1", "desc": "[0/29] Number of unWISE W1 astrometric epochs "}, {"name": "NW2", "desc": "[0/29] Number of unWISE W2 astrometric epochs "}, {"name": "NGDR2", "desc": "[3/344] Number of Gaia DR2 five-parameter re-registration stars"}]}, {"name": "table6.dat", "desc": "Parallax and motion fits for objects with low-quality parallaxes", "columns": [{"name": "FName", "desc": "Full name, position-based identifier "}, {"name": "RAdeg", "desc": "Right Ascension (ICRS) at t0 "}, {"name": "e_RAdeg", "desc": "[1.6/175] Positional uncertainty in RA "}, {"name": "DEdeg", "desc": "[-82.2/84.8] Declination (ICRS) at t0 "}, {"name": "e_DEdeg", "desc": "[1.6/141] Positional uncertainty in DE "}, {"name": "t0", "desc": "[57064.5/58254.2] Mean Epoch, Modified Julian Date (JD-2400000.5)"}, {"name": "plx", "desc": "[-12.4/439]? Absolute parallax "}, {"name": "e_plx", "desc": "[1.7/73]? Uncertainty in plx "}, {"name": "pmRA", "desc": "[-8123.7/1289.1] Absolute proper motion in RA "}, {"name": "e_pmRA", "desc": "[0.4/59] Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-3107.5/1311.5] Absolute proper motion in DE "}, {"name": "e_pmDE", "desc": "[0.6/45] Uncertainty in pmDE "}, {"name": "chisq", "desc": "[9.9/4401] {chi}^2 of fit "}, {"name": "dof", "desc": "[17/133] Degrees of freedom "}, {"name": "chisq/dof", "desc": "[0.2/77.2] Reduced {chi}^2 of fit "}, {"name": "NSp", "desc": "[2/39] Number of Spitzer astrometric epochs "}, {"name": "NW1", "desc": "[0/29] Number of unWISE W1 astrometric epochs "}, {"name": "NW2", "desc": "[0/29] Number of unWISE W2 astrometric epochs "}, {"name": "NGDR2", "desc": "[3/344] Number of Gaia DR2 five-parameter re-registration stars"}]}, {"name": "table7.dat", "desc": "Astrometry for objects with poor-quality (or unmeasurable) parallaxes that need improvement", "columns": [{"name": "FName", "desc": "Full name, position-based identifier "}, {"name": "RAdeg", "desc": "Right Ascension (ICRS) at t0 "}, {"name": "e_RAdeg", "desc": "[1.6/175] Positional uncertainty in RA "}, {"name": "DEdeg", "desc": "[-82.2/84.8] Declination (ICRS) at t0 "}, {"name": "e_DEdeg", "desc": "[1.6/141] Positional uncertainty in DE "}, {"name": "t0", "desc": "[57064.5/58254.2] Mean Epoch, Modified Julian Date (JD-2400000.5)"}, {"name": "plx", "desc": "[-12.4/439]? Absolute parallax "}, {"name": "e_plx", "desc": "[1.7/73]? Uncertainty in plx "}, {"name": "pmRA", "desc": "[-8123.7/1289.1] Absolute proper motion in RA "}, {"name": "e_pmRA", "desc": "[0.4/59] Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-3107.5/1311.5] Absolute proper motion in DE "}, {"name": "e_pmDE", "desc": "[0.6/45] Uncertainty in pmDE "}, {"name": "chisq", "desc": "[9.9/4401] {chi}^2 of fit "}, {"name": "dof", "desc": "[17/133] Degrees of freedom "}, {"name": "chisq/dof", "desc": "[0.2/77.2] Reduced {chi}^2 of fit "}, {"name": "NSp", "desc": "[2/39] Number of Spitzer astrometric epochs "}, {"name": "NW1", "desc": "[0/29] Number of unWISE W1 astrometric epochs "}, {"name": "NW2", "desc": "[0/29] Number of unWISE W2 astrometric epochs "}, {"name": "NGDR2", "desc": "[3/344] Number of Gaia DR2 five-parameter re-registration stars"}]}, {"name": "table8.dat", "desc": "Ancillary Spitzer photometry ", "columns": [{"name": "SName", "desc": "Short name used "}, {"name": "PName", "desc": "Short name position code for object "}, {"name": "OName", "desc": "Othe name "}, {"name": "AOR", "desc": "[10374912/67453440]? Spitzer Astronomical Observation Request"}, {"name": "Bands", "desc": "List of Spitzer/IRAC bands used "}, {"name": "Prog", "desc": "[35/90152] Spitzer program "}, {"name": "IRAC", "desc": "IRAC state (1) "}, {"name": "PI", "desc": "Spitzer program PI "}]}, {"name": "table9.dat", "desc": "Spectroscopic follow-up ", "columns": [{"name": "SName", "desc": "Short name used "}, {"name": "PName", "desc": "Short name position code for object "}, {"name": "Instr", "desc": "Instrument used "}, {"name": "Obs.Y", "desc": "[2016/2020] Observation date, UT, year "}, {"name": "Obs.M", "desc": "Observation date, UT, month "}, {"name": "Obs.D", "desc": "Observation date, UT, day in month "}, {"name": "SpT", "desc": "Spectral type(s) "}, {"name": "f_SpT", "desc": "Spectral type wavelength regime (1) "}]}, {"name": "table10.dat", "desc": "Other objects considered for the 20-pc census ", "columns": [{"name": "SName", "desc": "Short name used "}, {"name": "PName", "desc": "Short name position code for object "}, {"name": "SpTIR", "desc": "Spectral type, bkg=background (1) "}, {"name": "r_SpTIR", "desc": "Reference for SpT (2) "}, {"name": "plx", "desc": "[-12.4/116.4]? Absolute parallax, this work "}, {"name": "e_plx", "desc": "[3.4/72.3]? Uncertainty in plx "}, {"name": "plx-lit", "desc": "[9.9/62.4]? Published parallax "}, {"name": "e_plx-lit", "desc": "[0.2/19]? Uncertainty in plx-lit "}, {"name": "r_plx-lit", "desc": "Reference(s) for plx-lit (3) "}, {"name": "Dest-JW2", "desc": "[12.4/42.3]? Distance estimate based on J+W2 magnitudes"}, {"name": "Dest-HSpT", "desc": "[6.6/40.7]? Distance estimate based on H and Spectral type"}, {"name": "Dest-IRAC", "desc": "[8.2/41.3]? Distance estimate based on IRAC ch1+ch2 magnitudes"}, {"name": "Dest-WISE", "desc": "[10.3/26.5]? Distance estimate based on WISE W1+W2 magnitudes"}, {"name": "l_Dist", "desc": "Limit flag on Dist "}, {"name": "Dist", "desc": "[7.5/108]? Final distance estimate "}, {"name": "f_Dist", "desc": "Flag on Dest, bkg=background, ?=uncertain "}, {"name": "20pc", "desc": "Included in 20pc census? "}, {"name": "Remarks", "desc": "Remarks (4) "}]}, {"name": "table11.dat", "desc": "The full-sky 20-pc census of L, T, and Y dwarfs (known as of 2020 Oct)", "columns": [{"name": "FName", "desc": "Full name, position-based identifier "}, {"name": "f_FName", "desc": "Cross identification flags for Table A1 (1) "}, {"name": "r_FName", "desc": "Discovery Reference(s) (see refs.dat file) "}, {"name": "SpTO", "desc": "Optical spectral type "}, {"name": "f_SpTO", "desc": "Flag on SpTO (2) "}, {"name": "r_SpTO", "desc": "Reference(s) for SpTO (see refs.dat file) "}, {"name": "SpTIR", "desc": "Near-IR spectral type "}, {"name": "r_SpTIR", "desc": "Reference(s) for SpTIR (see refs.dat file) "}, {"name": "u_plx", "desc": "[:u ] :=uncertainty flag on plx: values are estimates only ;"}]}, {"name": "table12.dat", "desc": "Potentially young L, T, and Y dwarfs within 20pc of the Sun", "columns": [{"name": "SName", "desc": "Short name used "}, {"name": "PName", "desc": "Short name position code for object "}, {"name": "m_PName", "desc": "Component of PName "}, {"name": "OName", "desc": "Other name "}, {"name": "SpTO", "desc": "Optical spectral type "}, {"name": "SpTIR", "desc": "Near-IR spectral type "}, {"name": "PBan", "desc": "[0/99.8]? Banyan {Sigma} probability "}, {"name": "ABanyan", "desc": "Banyan {Sigma} association (2) "}, {"name": "Plac", "desc": "[0/56]? LACEwING probability "}, {"name": "ALACEwING", "desc": "LACEwING association (2) "}, {"name": "lowg", "desc": "Low gravity object? "}, {"name": "Assoc", "desc": "Association member? "}, {"name": "f_Assoc", "desc": "Flag on Association (3) "}, {"name": "Youth", "desc": "Youth Reference (4) "}, {"name": "Mass", "desc": "[10/25]? Mass in Jupiter mass units (5) "}, {"name": "e_Mass", "desc": "[1/6.2]? Uncertainty in Mass (5) "}, {"name": "B_Mass", "desc": "[12/12]? Upper mass bound (5) "}, {"name": "r_Mass", "desc": "Reference for Mass (4) "}]}, {"name": "table14.dat", "desc": "Late-M, L, T, and Y dwarfs with Teff measurements ", "columns": [{"name": "Name", "desc": "Object name, either short name or full name (1) "}, {"name": "SpTIR", "desc": "[-4/24] Numeric near-IR based spectral type (2) "}, {"name": "plx", "desc": "[21.9/439] Absolute parallax "}, {"name": "e_plx", "desc": "[0.02/6.5] Uncertainty in plx "}, {"name": "Teff", "desc": "[250/2871] Effective surface temperature "}, {"name": "e_Teff", "desc": "[23/320] Uncertainty in Teff "}, {"name": "Hmag", "desc": "[6.4/25.3]? H band magnitude "}, {"name": "e_Hmag", "desc": "[0.01/0.4]? Uncertainty in Hmag "}, {"name": "r_SpTIR", "desc": "Reference for SpT (3) "}, {"name": "r_plx", "desc": "Reference for plx (3) "}, {"name": "r_Teff", "desc": "Reference Teff (3) "}, {"name": "r_Hmag", "desc": "Reference Hmag (3) "}]}, {"name": "table16.dat", "desc": "Masses for L, T, and Y members of the 20-pc census ", "columns": [{"name": "SName", "desc": "Short name used (1) "}, {"name": "SpTIR", "desc": "Spectral type "}, {"name": "Teff", "desc": "[581/2274]? Effective surface temperature "}, {"name": "e_Teff", "desc": "[10/198]? Uncertainty in Teff "}, {"name": "Mass", "desc": "[10.0/87.0] Mass, Jupiter units (2) "}, {"name": "e_Mass", "desc": "[0.7/6.14]? Lower or symmetric error on Mass (2) "}, {"name": "E_Mass", "desc": "[1.1/2.9]? Upper uncertainty on Mass (2) "}, {"name": "B_Mass", "desc": "[12.0/12.0]? Upper bound on Mass (2) "}, {"name": "Method", "desc": "Method (3) "}, {"name": "r_Mass", "desc": "Mass references (4) "}]}, {"name": "tablea1.dat", "desc": "Amassed spectroscopic, astrometric, and photometric data for objects listed in Tables 5, 6, 7, 8, 9, 10, and 11", "columns": [{"name": "T", "desc": "Table listing (1) "}, {"name": "SName", "desc": "Short name used in other tables (2) "}, {"name": "SpTO", "desc": "[-2/19]?=-9 Optical spectral type (3) "}, {"name": "SpTIR", "desc": "[-1/22]?=-9 Near-IR spectral type (3) "}, {"name": "SpAd", "desc": "[-9/24] Adopted spectral type (3) "}, {"name": "OI", "desc": "Source of the spectral type "}, {"name": "plx", "desc": "[-12.4/501.6]?=-33333 best measured trigonometric parallax (4) "}, {"name": "plxe", "desc": "[0.019/72.3]?=3333 Uncertainty in plxe (4) "}, {"name": "mura", "desc": "?=-22222. best measured proper motion, in RA (4) "}, {"name": "mre", "desc": "?=222. Uncertainty in mura (4) "}, {"name": "mudec", "desc": "?=-11111. best measured proper motion, in DE (4) "}, {"name": "mde", "desc": "?=111. Uncertainty in mudec (4) "}, {"name": "AS", "desc": "Source of the astrometry (4) "}, {"name": "JMKO", "desc": "?=98888. J-band photometry on the MKO system (5) "}, {"name": "JMKe", "desc": "?=988. Uncertainty in JMKO (5) "}, {"name": "J2MASS", "desc": "?=97777. J-band photometry one the 2MASS system (5) "}, {"name": "J2Me", "desc": "?=977. Uncertainty in J2MASS (5) "}, {"name": "Hmag", "desc": "?=96666. H-band photometry on either the MKO or 2MASS system (5) "}, {"name": "Herr", "desc": "?=966. Uncertainty in Hmag (5) "}, {"name": "KMKO", "desc": "?=95555. K-band photometry on the MKO system (5) "}, {"name": "KMKe", "desc": "?=955. Uncertainty in KMKO (5) "}, {"name": "Ks2MASS", "desc": "?=94444. Ks-band photometry on the 2MASS system (5) "}, {"name": "Ks2e", "desc": "?=944. Uncertainty in Ks2MASS (5) "}, {"name": "PhotS", "desc": "Source of the near-IR photometry (5) "}, {"name": "RA_C2", "desc": "CatWISE2020 Right Ascension, decimal degrees (J2000) (6) "}, {"name": "Dec_C2", "desc": "CatWISE2020 Declination, decimal degrees (J2000) (6) "}, {"name": "pmra_C2", "desc": "?=844444. CatWISE2020 measured proper motion in RA (7) "}, {"name": "pmraerr_C2", "desc": "?=84444. Uncertainty in pmra_C2 (7) "}, {"name": "pmdec_C2", "desc": "?=855555. CatWISE2020 measured proper motion in DE (7) "}, {"name": "pmdcerr_C2", "desc": "?=85555. Uncertainty in pmdec_C2 (7) "}, {"name": "W1mag_C2", "desc": "?=86666. CatWISE2020 moving-object PSF-fit W1 band photometry (7 "}, {"name": "W1err_C2", "desc": "?=8666. Uncertainty in W1mag_C2 (7) "}, {"name": "W2mag_C2", "desc": "?=87777. CatWISE2020 moving-object PSF-fit W2 band photometry (7 "}, {"name": "W2err_C2", "desc": "?=8777. Uncertainty in W2mag_C2 (7) "}, {"name": "par_C2", "desc": "?=8999. CatWISE2020 par_pm parallax estimate (7) "}, {"name": "par_err_C2", "desc": "?=899. Uncertainty in par_C2 (7) "}, {"name": "C2S", "desc": "Source of the CatWISE2020 data (7) "}, {"name": "W1mag", "desc": "?=88888. WISE stationary-object PSF-fit W1 band photometry (8) "}, {"name": "W1err", "desc": "?=8888. Uncertainty in W1mag (8) "}, {"name": "W2mag", "desc": "?=77777. WISE stationary-object PSF-fit W2 band photometry (8) "}, {"name": "W2err", "desc": "?=7777. Uncertainty in W2mag (8) "}, {"name": "W3mag", "desc": "?=66666. WISE stationary-object PSF-fit W3 band photometry (8) "}, {"name": "W3err", "desc": "?=6666. Uncertainty in W3mag (8) "}, {"name": "WS", "desc": "Source of the stationary-object photometry (8) "}, {"name": "ch1mag", "desc": "?=55555. Spitzer channel 1 photometry (9) "}, {"name": "ch1err", "desc": "?=5555. Uncertainty in ch1mag (9) "}, {"name": "ch2mag", "desc": "?=44444. Spitzer channel 2 photometry (9) "}, {"name": "ch2err", "desc": "?=4444. Uncertainty in ch2mag (9) "}, {"name": "SS", "desc": "Source of Spitzer photometry (9) "}, {"name": "N", "desc": "Note (10) "}, {"name": "FName", "desc": "Full discovery designation of the system (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_253_39"}} {"id": "J/ApJS/253/39", "title_cds": "The H{alpha} Dots survey. IV. KPNO obs.", "title_create": "Watkins+, 2021", "year": "2021", "author": "Watkins J.D., Salzer J.J., Van Sistine A., Hayslip A., Hoar E., Rampalli R.", "title_pub": "The H{alpha} Dots survey. IV. A fourth list of faint emission-line objects.", "first_author": "Watkins J.D.", "ref_biblio": [""], "bibcode": ["2021ApJS..253...39W"], "see_also": ["J/AJ/109/2376 : Case blue/emission-line galaxies (Salzer+ 1995)", "J/AJ/123/1292 : KISS III. [O III]-selected survey list (Salzer+, 2002)", "J/AJ/142/170 : ALFALFA survey: {alpha}.40 HI source catalog (Haynes+, 2011)", "J/AJ/143/145 : Emission-line objects from ALFALFA Ha survey (Kellar+, 2012)", "J/ApJ/861/49 : ALFALFA extragalactic HI source catalog (Haynes+, 2018)", "J/AJ/160/242 : The H{alpha} dots survey. II. 119 new dots (Salzer+, 2020)"], "keyword_cds": "Galaxies, optical; Photometry, H-alpha; Photometry, RI; Surveys", "keyword_pub": "Emission line galaxies; Seyfert galaxies; Blue compact dwarf galaxies; Dwarf galaxies; Quasars; Starburst galaxies; Star formation", "abstract": ["We present the fourth catalog of serendipitously discovered compact", "extragalactic emission-line sources-H{alpha} Dots. A total of", "454 newly discovered objects are included in the current survey list.", "These objects have been detected in searches of moderately deep", "narrowband images acquired for the ALFALFA H{alpha} project. The", "catalog of H{alpha} Dots presented in the current paper was derived", "from searches carried out using ALFALFA H{alpha} images obtained with", "the KPNO 2.1m telescope. This results in a substantially deeper sample", "of Dots compared to our previous lists, which were all discovered in", "images taken with the WIYN 0.9m telescope. The median R-band magnitude", "of the current catalog is 21.59, more than 1.6mag fainter than the", "median for the 0.9m sample (a factor of 4.4x fainter). Likewise, the", "median emission-line flux of the detected sources is a factor of", "4.3x fainter. The line flux completeness limit of the current sample", "is ~3x10^-16^erg/s/cm^2^. We present accurate coordinates, apparent", "magnitudes, and narrowband line fluxes for each object in the sample.", "Unlike our previous lists of H{alpha} Dots, the current sample does", "not include follow-up spectroscopy."], "description": ["The current study analyzes all 10 observing runs (spanning 2010", "September to 2014 March) of ALFALFA H{alpha} project (AHA;", "Van Sistine+ 2016ApJ...824...25V) data obtained with the KPNO 2.1m", "telescope.", "Once the list of H{alpha} Dots discovered in the AHA 2.1m images was", "finalized (see Section 2), the entire catalog was crossed-matched with", "objects in the SDSS Data Release 14 (Abolfathi+ 2018ApJS..235...42A);", "see Section 3.", "The final catalog of H{alpha} Dots detected using the KPNO 2.1m AHA", "images contains 454 newly discovered emission-line galaxies (ELGs).", "This list of objects was arrived at after searching 611 AHA fields.", "The total sky coverage of these images represents 15.494deg^2^,", "resulting in a surface density of new H{alpha} Dots of 29.30deg^-2^."], "alias": ["[KSW2012]"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Fourth list of H{alpha} dots ", "columns": [{"name": "Dot", "desc": "[1001/1454] H{alpha} dot candidate number (1) "}, {"name": "RAdeg", "desc": "[0.2/358.6] SDSS right ascension (J2000) (2) "}, {"name": "DEdeg", "desc": "[4.27/29.05] SDSS declination (J2000) (2) "}, {"name": "Run", "desc": "Observing Run number "}, {"name": "Filt", "desc": "[2/4] Narrowband filter used for the observation of that field (3)"}, {"name": "Dmag", "desc": "[-2.95/-0.4] Magnitude difference ({Delta}m) between narrowband and continuum R-band (4)"}, {"name": "Ratio", "desc": "[4.5/201.5] Ratio of the absolute value of Dmag to the error in Dmag (5)"}, {"name": "Rmag", "desc": "[17/25.4] Measured R-band magnitude from continuum images"}, {"name": "e_Rmag", "desc": "[0.02/2.3] Uncertainty in Rmag "}, {"name": "NBFlux", "desc": "[0.001/1.83] Narrowband Line Flux, in 10^-14^erg/s/cm^2^ units (6)"}, {"name": "e_NBFlux", "desc": "[0.001/0.07] Uncertainty in NBFlux (6) "}, {"name": "rmag", "desc": "[17.2/23.6]? SDSS r-band magnitude "}, {"name": "e_rmag", "desc": "[0.01/0.5]? Uncertainty in rmag "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_256_25"}} {"id": "J/ApJS/256/25", "title_cds": "Nobeyama mapping survey of SCUBA-2 cores", "title_create": "Tatematsu+, 2021", "year": "2021", "author": "Tatematsu K., Kim G., Liu T., Evans II N.J., Yi H.-W., Lee J.-E., Wu Y., Hirano N., Liu S.-Y., Dutta S., Sahu D., Sanhueza P., Kim K.-T., Juvela M., Toth L.V., Feher O., He J., Ge J., Feng S., Choi M., Kang M., Thompson M.A., Fuller G.A., Li Di, Ristorcelli I., Wang Ke, Di Francesco J., Eden D., Ohashi S., Kandori R., Vastel C., Hirota T., Sakai T., Lu X., Nguyen Lu'o'ng Q., Shinnaga H., Kim J., the JCMT Large Program \"SCOPE\" col.", "title_pub": "Molecular cloud cores with high deuterium fractions: Nobeyama mapping survey.", "first_author": "Tatematsu K.", "ref_biblio": [""], "bibcode": ["2021ApJS..256...25T"], "see_also": ["II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "J/AJ/144/192 : Spitzer survey of Orion A & B. I. YSO catalog (Megeath+, 2012)", "J/ApJ/767/36 : APEX observations of HOPS protostars (Stutz+, 2013)", "J/A+A/579/A80 : Star-forming regions deuteration (Gerner+, 2015)", "J/A+A/594/A28 : Planck Catalogue of Galactic cold clumps (PGCC) (Planck+, 2016)", "J/ApJ/834/142 : Gould's Belt Distances Survey. II. OMC (Kounkel+, 2017)", "J/ApJ/846/144 : Virial analysis of the dense cores in Orion A (Kirk+, 2017)", "J/ApJS/236/51 : PGCCs in lambda Orionis complex. II. Cores at 850um (Yi+, 2018)", "J/AJ/156/18 : APOGEE:Binary companions of evolved stars (Price-Whelan+, 2018)", "J/A+A/644/A29 : 14N/15N ratio in YSOs (Redaelli+, 2020)", "J/ApJS/249/33 : Nobeyama molecular line survey of SCUBA-2 cores (Kim+, 2020)", "J/ApJS/251/20 : ALMA survey of Orion PGCCs (ALMASOP). II. 1.3mm (Dutta+, 2020)", "J/ApJS/254/14 : Planck Cold Clumps in lambda Orionis complex. III. (Yi+, 2021)"], "keyword_cds": "Molecular data; Interstellar medium; Radio lines; YSOs; Velocity dispersion; Star Forming Region; Molecular clouds; Millimetric/submm sources", "keyword_pub": "Interstellar clouds", "abstract": ["We present the results of on-the-fly mapping observations of 44 fields", "containing 107 SCUBA-2 cores in the emission lines of molecules", "N_2_H^+^, HC_3_N, and CCS at 82-94GHz using the Nobeyama 45m", "telescope. This study aimed at investigating the physical properties", "of cores that show high deuterium fractions and might be close to the", "onset of star formation. We found that the distributions of the N2H+", "and HC3N line emissions are approximately similar to the distribution", "of the 850{mu}m dust continuum emission, whereas the CCS line emission", "is often undetected or is distributed in a clumpy structure", "surrounding the peak position of the 850{mu}m dust continuum emission.", "Occasionally (12%), we observe CCS emission, which is an early-type", "gas tracer toward the young stellar object, probably due to local high", "excitation. Evolution toward star formation does not immediately", "affect the nonthermal velocity dispersion."], "description": ["We conducted mapping observations of 44 fields of 3'x3' or larger", "areas covering 107 SCUBA-2 cores in the N_2_H^+^ J=1->0 (93.17GHz),", "HC_3_N J=9->8 (81.88GHz), CCS J_N_=8_7_->7_6_ (CCS-H; 93.87GHz), and", "CCS J_N_=7_6_->6_5_ (CCS-L; 81.50GHz) lines using the 45m radio", "telescope of the Nobeyama Radio Observatory (LP177001; P.I.=K.Tatematsu).", "Observations were performed in the on-the-fly (OTF) mapping mode from", "2017 December to 2019 May.", "We also included the SCUBA-2 data (Yi+ 2018, J/ApJS/236/51) and our", "previous single-pointing data toward the SCUBA-2 position", "(Kim+ 2020, J/ApJS/249/33) in the analysis."], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/ac0978"], "orcid_pub": ["0000-0002-8149-8546"], "data": "f-v", "date_creation": "31-Mar-2022", "xmatch": "J/ApJS/256/25/cores", "last_update": "13-Jun-2022", "catid": "22560025", "date_update": "24-Oct-2022", "tables": [{"name": "table4.dat", "desc": "Physical properties of N_2_H^+^ core for SCUBA-2 cores in the Orion region", "columns": [{"name": "Name", "desc": "SCUBA-2 core name "}, {"name": "DelV", "desc": "[0.35/1.42] N_2_H^+^ FWHM line width toward the SCUBA-2 position (Kim+ 2020, J/ApJS/249/33) (1)"}, {"name": "e_DelV", "desc": "[0.01/0.16] DelV uncertainty "}, {"name": "SigNt", "desc": "[0.13/0.6] Nonthermal velocity dispersion (1) "}, {"name": "e_SigNt", "desc": "[0.01/0.06] Signt uncertainty "}, {"name": "SigTot", "desc": "[0.25/0.65] Total velocity dispersion (1) "}, {"name": "e_SigTot", "desc": "[0.01/0.11] Sigtot uncertainty "}, {"name": "Rdust", "desc": "[0.005/0.12] HWHM dust continuum radius (Yi+ 2018, J/ApJS/236/51) (2)"}, {"name": "Mdust", "desc": "[0.07/12.25] Mass from the dust continuum (Yi+ 2018, J/ApJS/236/51) (2)"}, {"name": "e_Mdust", "desc": "[0.02/3.18] Mdust uncertainty "}, {"name": "Mvir", "desc": "[1.2/17.1] Virial mass (2) "}, {"name": "e_Mvir", "desc": "[0.2/3] Mvir uncertainty "}, {"name": "aVir", "desc": "[0.1/18] Virial parameter (2) "}, {"name": "e_aVir", "desc": "[0.03/14.5] AVir uncertainty "}, {"name": "Tkin", "desc": "[10.8/19.7] Kinetic temperature (1) "}, {"name": "Fil", "desc": "Association with the filament? "}]}, {"name": "table6.dat", "desc": "Deuterium fraction and CEF2.0 ", "columns": [{"name": "Name", "desc": "SCUBA-2 core name "}, {"name": "Vlsr", "desc": "[-19.3/105] Local Standard of Rest velocity "}, {"name": "l_N2D/N2H", "desc": "Limit flag on N2D/N2H "}, {"name": "N2D/N2H", "desc": "[0.04/0.63]? N_2_D^+^ to N_2_H^+^ column density ratio"}, {"name": "e_N2D/N2H", "desc": "[0.01/0.13]? N2D/N2H uncertainty "}, {"name": "l_DNC/HNC", "desc": "Limit flag on DNC/HNC "}, {"name": "DNC/HNC", "desc": "[0.4/14.6]? DNC to HN^13^C column density ratio "}, {"name": "e_DNC/HNC", "desc": "[0.3/10.3]? DNC/HNC uncertainty "}, {"name": "YSO", "desc": "YSO association? "}, {"name": "CEF2", "desc": "[-67/-18]? CEF2.0 value (1) "}, {"name": "e_CEF2", "desc": "[3/36]? CEF2 uncertainty "}]}, {"name": "tablea1.dat", "desc": "Mapped fields and SCUBA-2 cores ", "columns": [{"name": "Field", "desc": "Field name of the mapped region "}, {"name": "RAMh", "desc": "Map center hour of right ascension (J2000) "}, {"name": "RAMm", "desc": "Map center minute of right ascension (J2000) "}, {"name": "RAMs", "desc": "Map center second of right ascension (J2000) "}, {"name": "DEM-", "desc": "Map center sign of declination (J2000) "}, {"name": "DEMd", "desc": "Map center degree of declination (J2000) "}, {"name": "DEMm", "desc": "Map center arcminute of declination (J2000) "}, {"name": "DEMs", "desc": "Map center arcsecond of declination (J2000) "}, {"name": "Size", "desc": "Map size "}, {"name": "Dist", "desc": "[0.11/9.21]? Distance "}, {"name": "Reg", "desc": "Region (1) "}, {"name": "Name", "desc": "SCUBA-2 core name "}, {"name": "RAh", "desc": "SCUBA-2 core hour of right ascension (J2000) "}, {"name": "RAm", "desc": "SCUBA-2 core minute of right ascension (J2000) "}, {"name": "RAs", "desc": "SCUBA-2 core second of right ascension (J2000) "}, {"name": "DE-", "desc": "SCUBA-2 core sign of declination (J2000) "}, {"name": "DEd", "desc": "SCUBA-2 core degree of declination (J2000) "}, {"name": "DEm", "desc": "SCUBA-2 core arcminute of declination (J2000) "}, {"name": "DEs", "desc": "SCUBA-2 core arcsecond of declination (J2000) "}]}, {"name": "tablea2.dat", "desc": "Basic information of YSOs associated with SCUBA-2 Cores", "columns": [{"name": "Name", "desc": "SCUBA-2 core name "}, {"name": "Class", "desc": "Core classification (1) "}, {"name": "YSO", "desc": "YSO name "}, {"name": "RAYh", "desc": "? YSO hour of right ascension (J2000) "}, {"name": "RAYm", "desc": "? YSO minute of right ascension (J2000) "}, {"name": "RAYs", "desc": "? YSO second of right ascension (J2000) "}, {"name": "DEY-", "desc": "? YSO sign of declination (J2000) "}, {"name": "DEYd", "desc": "? YSO degree of declination (J2000) "}, {"name": "DEYm", "desc": "? YSO arcminute of declination (J2000) "}, {"name": "DEYs", "desc": "? YSO arcsecond of declination (J2000) "}, {"name": "Tbol", "desc": "[15/158]? Bolometric temperature "}, {"name": "e_Tbol", "desc": "[5/25]? Tbol uncertainty "}, {"name": "Lbol", "desc": "[0.1/180]? Bolometric luminosity "}, {"name": "e_Lbol", "desc": "[0.1/70]? Lbol uncertainty "}, {"name": "Sep", "desc": "[0/31.6]? Separation, {theta}_core_-YSO "}]}, {"name": "tablea3.dat", "desc": "Parameters for integrated-intensity maps for the N_2_H^+^, HC_3_N, CCS-H, and CCS-L lines", "columns": [{"name": "Field", "desc": "Field name of the mapped area "}, {"name": "b_VN2H", "desc": "[-22.2/102.4] Lower limit of the velocity integration range for the integrated-intensity map of N_2_H^+^ line"}, {"name": "B_VN2H", "desc": "[-16.3/109] Upper limit of the velocity integration range for the integrated-intensity map of N_2_H^+^ line"}, {"name": "b_Vel", "desc": "[-20.4/103.7] Lower limit of velocity range for the integrated-intensity map of HC_3_N, CCS-H, and CCS-L lines"}, {"name": "B_Vel", "desc": "[-17.8/109] Upper limit of velocity range for the integrated-intensity map of HC_3_N, CCS-H, and CCS-L lines"}, {"name": "e_IN2Hpk", "desc": "[0.05/0.16] RMS value of the N_2_H^+^ integrated intensity"}, {"name": "IN2Hpk", "desc": "[1.15/17.38] Peak value of the N_2_H^+^ integrated intensity"}, {"name": "e_IHC3Npk", "desc": "[0.03/0.24] RMS value of the HC_3_N integrated intensity"}, {"name": "IHC3Npk", "desc": "[0.16/6.5] Peak value of the HC_3_N integrated intensity"}, {"name": "e_ICCSHpk", "desc": "[0.03/0.2] RMS value of the CCS-H integrated intensity"}, {"name": "ICCSHpk", "desc": "[0.13/0.75] Peak value of the CCS-H integrated intensity"}, {"name": "e_ICCSLpk", "desc": "[0.03/0.16] RMS value of the CCS-L integrated intensity"}, {"name": "ICCSLpk", "desc": "[0.12/0.86] Peak value of the CCS-L integrated intensity"}]}, {"name": "tablea4.dat", "desc": "Line emission distribution in the Orion region for N_2_H^+^ and HC_3_N", "columns": [{"name": "Name", "desc": "SCUBA-2 core name "}, {"name": "RAh", "desc": "? Hour of right ascension (J2000) (1) "}, {"name": "RAm", "desc": "? Minute of right ascension (J2000) (1) "}, {"name": "RAs", "desc": "? Second of right ascension (J2000) (1) "}, {"name": "DE-", "desc": "? Sign of declination (J2000) (1) "}, {"name": "DEd", "desc": "? Degree of declination (J2000) (1) "}, {"name": "DEm", "desc": "? Arcminute of declination (J2000) (1) "}, {"name": "DEs", "desc": "? Arcsecond of declination (J2000) (1) "}, {"name": "SepN2H", "desc": "[0.001/0.14]? Separation between the SCUBA-2 core and the N2H+ core"}, {"name": "RadN2H", "desc": "[0.029/0.14]? Deconvolved radius of the N_2_H^+^ core"}, {"name": "RAHh", "desc": "? Hour of right ascension (J2000) (2) "}, {"name": "RAHm", "desc": "? Minute of right ascension (J2000) (2) "}, {"name": "RAHs", "desc": "? Second of right ascension (J2000) (2) "}, {"name": "DEH-", "desc": "? Sign of declination (J2000) (2) "}, {"name": "DEHd", "desc": "? Degree of declination (J2000) (2) "}, {"name": "DEHm", "desc": "? Arcminute of declination (J2000) (2) "}, {"name": "DEHs", "desc": "? Arcsecond of declination (J2000) (2) "}, {"name": "SepHC3N", "desc": "[0.001/0.16]? Separation between SCUBA-2 core and HC_3_N core"}, {"name": "RadHC3N", "desc": "[0.025/0.14]? Deconvolved radius of the HC_3_N core"}]}, {"name": "tablea5.dat", "desc": "Line emission distribution in the Orion region for CCS-H and CCS-L", "columns": [{"name": "Name", "desc": "SCUBA-2 core name "}, {"name": "RACh", "desc": "? Hour of right ascension (J2000) (3) "}, {"name": "RACm", "desc": "? Minute of right ascension (J2000) (3) "}, {"name": "RACs", "desc": "? Second of right ascension (J2000) (3) "}, {"name": "DEC-", "desc": "? Sign of declination (J2000) (3) "}, {"name": "DECd", "desc": "? Degree of declination (J2000) (3) "}, {"name": "DECm", "desc": "? Arcminute of declination (J2000) (3) "}, {"name": "DECs", "desc": "? Arcsecond of declination (J2000) (3) "}, {"name": "SepCCSH", "desc": "[0.0001/0.06]? Separation between the SCUBA-2 core and the CCS-H core"}, {"name": "RadCCSH", "desc": "[0.038/0.11]? Deconvolved radius of the CCS-H core"}, {"name": "RALh", "desc": "? Hour of right ascension (J2000) (4) "}, {"name": "RALm", "desc": "? Minute of right ascension (J2000) (4) "}, {"name": "RALs", "desc": "? Second of right ascension (J2000) (4) "}, {"name": "DEL-", "desc": "? Sign of declination (J2000) (4) "}, {"name": "DELd", "desc": "? Degree of declination (J2000) (4) "}, {"name": "DELm", "desc": "? Arcminute of declination (J2000) (4) "}, {"name": "DELs", "desc": "? Arcsecond of declination (J2000) (4) "}, {"name": "SepCCSL", "desc": "[0.006/0.16]? Separation between the SCUBA-2 core and the CCS-L core"}, {"name": "RadCCSL", "desc": "[0.021/0.16]? Deconvolved radius of the CCS-L core"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_258_11"}} {"id": "J/ApJS/258/11", "title_cds": "The COSMOS2020 catalog", "title_create": "Weaver+, 2022", "year": "2022", "author": "Weaver J.R., Kauffmann O.B., Ilbert O., Mccracken H.J., Moneti A., Toft S., Brammer G., Shuntov M., Davidzon I., Hsieh B.C., Laigle C., Anastasiou A., Jespersen C.K., Vinther J., Capak P., Casey C.M., Mcpartland C.J.R., Milvang-Jensen B., Mobasher B., Sanders D.B., Zalesky L., Arnouts S., Aussel H., Dunlop J.S., Faisst A., Franx M., Furtak L.J., Fynbo J.P.U., Gould K.M.L., Greve T.R., Gwyn S., Kartaltepe J.S., Kashino D., Koekemoer A.M., Kokorev V., Le Fevre O., Lilly S., Masters D., Magdis G., Mehta V., Peng Y., Riechers D.A., Salvato M., Sawicki M., Scarlata C., Scoville N., Shirley R., Silverman J.D., Sneppen A., Smolcic V., Steinhardt C., Stern D., Tanaka M., Taniguchi Y., Teplitz H.I., Vaccari M., Wang W.-H., Zamorani G.", "title_pub": "COSMOS2020: a panchromatic view of the Universe to z~10 from two complementary catalogs.", "first_author": "Weaver J.R.", "ref_biblio": [""], "bibcode": ["2022ApJS..258...11W"], "see_also": ["J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)", "II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)", "J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016)", "J/ApJ/817/34 : C-COSMOS Legacy sources multiwavelength catalog"], "keyword_cds": "Galaxy catalogs ; Photometry, infrared ; Photometry, ugriz ; Photometry, ultraviolet ; Radio sources ; X-ray sources ; Cross identifications ; Redshifts ; Stars, masses", "keyword_pub": "catalogs - surveys - galaxy evolution - high-redshift galaxies - photometry - observational astronomy - astronomical methods", "abstract": ["The Cosmic Evolution Survey (COSMOS) has become a cornerstone of", "extragalactic astronomy. Since the last public catalog in 2015, a", "wealth of new imaging and spectroscopic data have been collected in", "the COSMOS field. This paper describes the collection, processing, and", "analysis of these new imaging data to produce a new reference", "photometric redshift catalog. Source detection and multiwavelength", "photometry are performed for 1.7 million sources across the 2 deg^2^", "of the COSMOS field, ~966000 of which are measured with all", "available broadband data using both traditional aperture photometric", "methods and a new profile-fitting photometric extraction tool, THE", "FARMER, which we have developed. A detailed comparison of the two", "resulting photometric catalogs is presented. Photometric redshifts are", "computed for all sources in each catalog utilizing two independent", "photometric redshift codes. Finally, a comparison is made between the", "performance of the photometric methodologies and of the redshift codes", "to demonstrate an exceptional degree of self-consistency in the", "resulting photometric redshifts. The i<21 sources have subpercent", "photometric redshift accuracy and even the faintest sources at 255% in PDF (lp_zp_2)"}, {"name": "lpchi22", "desc": "?=- LePhare reduced chi2 for the second photo-z solution (lp_chi2_2)"}, {"name": "lpNbFilt", "desc": "?=- LePhare number of filters used in the fit (lp_NbFilt)"}, {"name": "lpzq", "desc": "?=- LePhare photo-z for the AGN library (lp_zq)"}, {"name": "lpchiq", "desc": "?=- LePhare reduced chi2 for photo-z for the AGN library (lp_chiq)"}, {"name": "lpmodq", "desc": "?=- LePhare best fit template number in the AGN library (lp_modq)"}, {"name": "lpmods", "desc": "?=- LePhare best fit template number in the star library (lp_mods)"}, {"name": "lpchis", "desc": "?=- LePhare reduced chi2 for the best fit with the star library (lp_chis)"}, {"name": "lpmask", "desc": "?=- LePhare mask flag (0: in UVISTA and in clean part of HSC and SUPCAM) (lp_mask)"}, {"name": "lpmodel", "desc": "?=- LePhare BC03 best fit template number (lp_model)"}, {"name": "lpage", "desc": "?=- LePhare BC03 age of best fit template at zPDF (lp_age)"}, {"name": "lpdust", "desc": "?=- LePhare BC03 colour excess E(B-V) of best fit template at zPDF (lp_dust)"}, {"name": "lpAtt", "desc": "?=- LePhare BC03 best-fit dust law number at zPDF (lp_Attenuation)"}, {"name": "lpFUVMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in GALEX FUV band at zPDF (lp_MFUV)"}, {"name": "lpNUVMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in GALEX NUV band at zPDF (lp_MNUV)"}, {"name": "lpUMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in CFHT u* band at zPDF (lp_MU)"}, {"name": "lpGMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC g band at zPDF (lp_MG)"}, {"name": "lpRMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC r band at zPDF (lp_MR)"}, {"name": "lpIMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC i band at zPDF (lp_MI)"}, {"name": "lpZMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC z band at zPDF (lp_MZ)"}, {"name": "lpYMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in VISTA Y band at zPDF (lp_MY)"}, {"name": "lpJMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in VISTA J band at zPDF (lp_MJ)"}, {"name": "lpHMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in VISTA H band at zPDF (lp_MH)"}, {"name": "lpKMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in VISTA Ks band at zPDF (lp_MK)"}, {"name": "loglpMassmed", "desc": "?=- LePhare BC03 log stellar mass at zPDF (lp_mass_med)"}, {"name": "b_loglpMassmed", "desc": "?=- LePhare BC03 log stellar mass at zPDF, lower limit, 68% conf. level (lp_mass_med_min68)"}, {"name": "B_loglpMassmed", "desc": "?=- LePhare BC03 log stellar mass at zPDF, upper limit, 68% conf. level (lp_mass_med_max68)"}, {"name": "loglpMassbest", "desc": "?=- LePhare BC03 log stellar mass at zMinChi2 (lp_mass_best)"}, {"name": "loglpSFRmed", "desc": "?=- LePhare BC03 log SFR at zPDF (lp_SFR_med)"}, {"name": "b_loglpSFRmed", "desc": "?=- LePhare BC03 log SFR at zPDF, lower limit, 68% confidence level (lp_SFR_med_min68)"}, {"name": "B_loglpSFRmed", "desc": "?=- LePhare BC03 log SFR at zPDF, upper limit, 68% confidence level (lp_SFR_med_max68)"}, {"name": "loglpSFRbest", "desc": "?=- LePhare BC03 log SFR at zMinChi2 (lp_SFR_best)"}, {"name": "loglpsSFRmed", "desc": "?=- LePhare BC03 log sSFR at zPDF (lp_sSFR_med)"}, {"name": "b_loglpsSFRmed", "desc": "?=- LePhare BC03 log sSFR at zPDF, lower limit, 68% confidence level (lp_sSFR_med_min68)"}, {"name": "B_loglpsSFRmed", "desc": "?=- LePhare BC03 log sSFR at zPDF, upper limit, 68% confidence level (lp_sSFR_med_max68)"}, {"name": "loglpsSFRbest", "desc": "?=- LePhare BC03 log sSFR at zMinChi2 (lp_sSFR_best)"}, {"name": "EZzphot", "desc": "?=- EAZY maximum a-posteriori photo-z (ez_z_phot)"}, {"name": "EZzphotchi2", "desc": "?=- EAZY chi2 at ez_z_phot, with z-prior (ez_z_phot_chi2)"}, {"name": "EZzphotrisk", "desc": "?=- EAZY risk parameter (Tanaka et al, 2018PASJ...70S...9T) at ez_z_phot, R (ez_z_phot) (ez_z_phot_risk)"}, {"name": "EZzminrisk", "desc": "?=- EAZY photo-z where risk parameter R (z) is minimised (ez_z_min_risk)"}, {"name": "EZminrisk", "desc": "?=- EAZY risk parameter at ez_z_min_risk, R (ez_z_min_risk) (ez_min_risk)"}, {"name": "EZzrawchi2", "desc": "?=- EAZY photo-z where chi2 is minimised, without priors (ez_z_raw_chi2)"}, {"name": "EZrawchi2", "desc": "?=- EAZY chi2 at ez_z_raw_chi2 (ez_raw_chi2)"}, {"name": "EZzp025", "desc": "?=- EAZY 2.5% percentile of photo-z (ez_z025)"}, {"name": "EZzp160", "desc": "?=- EAZY 16.0% percentile of photo-z (ez_z160)"}, {"name": "EZzp500", "desc": "?=- EAZY 50.0% percentile of photo-z (ez_z500)"}, {"name": "EZzp840", "desc": "?=- EAZY 84.0% percentile of photo-z (ez_z840)"}, {"name": "EZzp975", "desc": "?=- EAZY 97.5% percentile of photo-z (ez_z975)"}, {"name": "EZnusefilt", "desc": "?=- EAZY no. of filters used for photo-z (only filters w/o missing data) (ez_nusefilt)"}, {"name": "EZlcmin", "desc": "?=- EAZY minimum effective wavelength of valid filters (ez_lc_min)"}, {"name": "EZlcmax", "desc": "?=- EAZY minimum effective wavelength of valid filters (ez_lc_max)"}, {"name": "EZstarminchi2", "desc": "?=- EAZY chi2 best stellar template fit (BT-SETTL models) as, 8% sys unc (ez_star_min_chi2)"}, {"name": "EZstarTeff", "desc": "?=- EAZY effective temperature of the stellar template (ez_star_teff)"}, {"name": "EZrestU", "desc": "?=- EAZY rest-frame U-band flux density (ez_restU)"}, {"name": "e_EZrestU", "desc": "?=- EAZY rest-frame U-band flux density uncertainty (ez_restU_err)"}, {"name": "EZrestB", "desc": "?=- EAZY rest-frame B-band flux density (ez_restB)"}, {"name": "e_EZrestB", "desc": "?=- EAZY rest-frame B-band flux density uncertainty (ez_restB_err)"}, {"name": "EZrestV", "desc": "?=- EAZY rest-frame V-band flux density (ez_restV)"}, {"name": "e_EZrestV", "desc": "?=- EAZY rest-frame V-band flux density uncertainty (ez_restV_err)"}, {"name": "EZrestJ", "desc": "?=- EAZY rest-frame J-band flux density (ez_restJ)"}, {"name": "e_EZrestJ", "desc": "?=- EAZY rest-frame J-band flux density uncertainty (ez_restJ_err)"}, {"name": "EZdL", "desc": "?=- EAZY luminosity distance at ez_z_phot (ez_dL)"}, {"name": "logEZMass", "desc": "?=- EAZY log stellar mass (ez_mass)"}, {"name": "logEZSFR", "desc": "?=- EAZY log SFR (ez_sfr) "}, {"name": "logEZsSFR", "desc": "?=- EAZY log sSFR (ez_ssfr) "}, {"name": "logEZLV", "desc": "?=- EAZY log V-band luminosity (ez_Lv)"}, {"name": "EZLIR", "desc": "?=- EAZY total 8-1000um luminosity (ez_LIR)"}, {"name": "EZEnerAbs", "desc": "?=- EAZY implied absorbed energy associated with Av (ez_energy_abs)"}, {"name": "EZLU", "desc": "?=- EAZY luminosity in rest-frame U band (ez_Lu)"}, {"name": "EZLJ", "desc": "?=- EAZY luminosity in rest-frame J band (ez_Lj)"}, {"name": "EZL1400", "desc": "?=- EAZY luminosity in tophat filter at 1400{AA} (200{AA} wide) rest-frame (ez_L1400)"}, {"name": "EZL2800", "desc": "?=- EAZY luminosity in tophat filter at 2800{AA} (200{AA} wide) rest-frame (ez_L2800)"}, {"name": "EZLHa", "desc": "?=- EAZY Halpha line luminosity (reddened) (ez_LHa)"}, {"name": "EZLOIII", "desc": "?=- EAZY [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII)"}, {"name": "EZLHb", "desc": "?=- EAZY Hbeta line luminosity (reddened) (ez_LHb)"}, {"name": "EZLOII", "desc": "?=- EAZY [OII] 3726+3729 line luminosity (reddened) (ez_LOII)"}, {"name": "EZMLV", "desc": "?=- EAZY mass-to-light ratio in V band (ez_MLv)"}, {"name": "EZAv", "desc": "?=- EAZY extinction in V band (ez_Av)"}, {"name": "EZlwAgeV", "desc": "?=- EAZY light-weighted age in the V band (ez_lwAgeV)"}, {"name": "logEZmassp025", "desc": "?=- EAZY 2.5% percentile of log stellar mass (ez_mass_p025)"}, {"name": "logEZmassp160", "desc": "?=- EAZY 16.0% percentile of log stellar mass (ez_mass_p160)"}, {"name": "logEZmassp500", "desc": "?=- EAZY 50.0% percentile of log stellar mass (ez_mass_p500)"}, {"name": "logEZmassp840", "desc": "?=- EAZY 84.0% percentile of log stellar mass (ez_mass_p840)"}, {"name": "logEZmassp975", "desc": "?=- EAZY 97.5% percentile of log stellar mass (ez_mass_p975)"}, {"name": "logEZsfrp025", "desc": "?=- EAZY 2.5% percentile of log SFR (ez_sfr_p025)"}, {"name": "logEZsfrp160", "desc": "?=- EAZY 16.0% percentile of log SFR (ez_sfr_p160)"}, {"name": "logEZsfrp500", "desc": "?=- EAZY 50.0% percentile of log SFR (ez_sfr_p500)"}, {"name": "logEZsfrp840", "desc": "?=- EAZY 84.0% percentile of log SFR (ez_sfr_p840)"}, {"name": "logEZsfrp975", "desc": "?=- EAZY 97.5% percentile of log SFR (ez_sfr_p975)"}, {"name": "logEZLVp025", "desc": "?=- EAZY 2.5% percentile of log V-band luminosity (ez_Lv_p025)"}, {"name": "logEZLVp160", "desc": "?=- EAZY 16.0% percentile of log V-band luminosity (ez_Lv_p160)"}, {"name": "logEZLVp500", "desc": "?=- EAZY 50.0% percentile of log V-band luminosity (ez_Lv_p500)"}, {"name": "logEZLVp840", "desc": "?=- EAZY 84.0% percentile of log V-band luminosity (ez_Lv_p840)"}, {"name": "logEZLVp975", "desc": "?=- EAZY 97.5% percentile of log V-band luminosity (ez_Lv_p975)"}, {"name": "EZLIRp025", "desc": "?=- EAZY 2.5% percentile of total 8-1000 um luminosity (ez_LIR_p025)"}, {"name": "EZLIRp160", "desc": "?=- EAZY 16.0% percentile of total 8-1000 um luminosity (ez_LIR_p160)"}, {"name": "EZLIRp500", "desc": "?=- EAZY 50.0% percentile of total 8-1000 um luminosity (ez_LIR_p500)"}, {"name": "EZLIRp840", "desc": "?=- EAZY 84.0% percentile of total 8-1000 um luminosity (ez_LIR_p840)"}, {"name": "EZLIRp975", "desc": "?=- EAZY 97.5% percentile of total 8-1000 um luminosity (ez_LIR_p975)"}, {"name": "EZEnerAbsp025", "desc": "?=- EAZY 2.5% percentile of implied absorbed energy associated with Av (ez_energy_abs_p025)"}, {"name": "EZEnerAbsp160", "desc": "?=- EAZY 16.0% percentile of implied absorbed energy associated with Av (ez_energy_abs_p160)"}, {"name": "EZEnerAbsp500", "desc": "?=- EAZY 50.0% percentile of implied absorbed energy associated with Av (ez_energy_abs_p500)"}, {"name": "EZEnerAbsp840", "desc": "?=- EAZY 84.0% percentile of implied absorbed energy associated with Av (ez_energy_abs_p840)"}, {"name": "EZEnerAbsp975", "desc": "?=- EAZY 97.5% percentile of implied absorbed energy associated with Av (ez_energy_abs_p975)"}, {"name": "EZLUp025", "desc": "?=- EAZY 2.5% percentile of luminosity in rest-frame U band (ez_Lu_p025)"}, {"name": "EZLUp160", "desc": "?=- EAZY 16.0% percentile of luminosity in rest-frame U band (ez_Lu_p160)"}, {"name": "EZLUp500", "desc": "?=- EAZY 50.0% percentile of luminosity in rest-frame U band (ez_Lu_p500)"}, {"name": "EZLUp840", "desc": "?=- EAZY 84.0% percentile of luminosity in rest-frame U band (ez_Lu_p840)"}, {"name": "EZLUp975", "desc": "?=- EAZY 97.5% percentile of luminosity in rest-frame U band (ez_Lu_p975)"}, {"name": "EZLJp025", "desc": "?=- EAZY 2.5% percentile of luminosity in rest-frame J band (ez_Lj_p025)"}, {"name": "EZLjp160", "desc": "?=- EAZY 16.0% percentile of luminosity in rest-frame J band (ez_Lj_p160)"}, {"name": "EZLjp500", "desc": "?=- EAZY 50.0% percentile of luminosity in rest-frame J band (ez_Lj_p500)"}, {"name": "EZLJp840", "desc": "?=- EAZY 84.0% percentile of luminosity in rest-frame J band (ez_Lj_p840)"}, {"name": "EZLJp975", "desc": "?=- EAZY 97.5% percentile of luminosity in rest-frame J band (ez_Lj_p975)"}, {"name": "EZL1400p025", "desc": "?=- EAZY 2.5% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p025)"}, {"name": "EZL1400p160", "desc": "?=- EAZY 16.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p160)"}, {"name": "EZL1400p500", "desc": "?=- EAZY 50.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p500)"}, {"name": "EZL1400p840", "desc": "?=- EAZY 84.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p840)"}, {"name": "EZL1400p975", "desc": "?=- EAZY 97.5% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p975)"}, {"name": "EZL2800p025", "desc": "?=- EAZY 2.5% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p025)"}, {"name": "EZL2800p160", "desc": "?=- EAZY 16.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p160)"}, {"name": "EZL2800p500", "desc": "?=- EAZY 50.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p500)"}, {"name": "EZL2800p840", "desc": "?=- EAZY 84.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p840)"}, {"name": "EZL2800p975", "desc": "?=- EAZY 97.5% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p975)"}, {"name": "EZLHap025", "desc": "?=- EAZY 2.5% percentile of Halpha line luminosity (reddened) (ez_LHa_p025)"}, {"name": "EZLHap160", "desc": "?=- EAZY 16.0% percentile of Halpha line luminosity (reddened) (ez_LHa_p160)"}, {"name": "EZLHap500", "desc": "?=- EAZY 50.0% percentile of Halpha line luminosity (reddened) (ez_LHa_p500)"}, {"name": "EZLHap840", "desc": "?=- EAZY 84.0% percentile of Halpha line luminosity (reddened) (ez_LHa_p840)"}, {"name": "EZLHap975", "desc": "?=- EAZY 97.5% percentile of Halpha line luminosity (reddened) (ez_LHa_p975)"}, {"name": "EZLOIIIp025", "desc": "?=- EAZY 2.5% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p025)"}, {"name": "EZLOIIIp160", "desc": "?=- EAZY 16.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p160)"}, {"name": "EZLOIIIp500", "desc": "?=- EAZY 50.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p500)"}, {"name": "EZLOIIIp840", "desc": "?=- EAZY 84.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p840)"}, {"name": "EZLOIIIp975", "desc": "?=- EAZY 97.5% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p975)"}, {"name": "EZLHbp025", "desc": "?=- EAZY 2.5% percentile of Hbeta line luminosity (reddened) (ez_LHb_p025)"}, {"name": "EZLHbp160", "desc": "?=- EAZY 16.0% percentile of Hbeta line luminosity (reddened) (ez_LHb_p160)"}, {"name": "EZLHbp500", "desc": "?=- EAZY 50.0% percentile of Hbeta line luminosity (reddened) (ez_LHb_p500)"}, {"name": "EZLHbp840", "desc": "?=- EAZY 84.0% percentile of Hbeta line luminosity (reddened) (ez_LHb_p840)"}, {"name": "EZLHbp975", "desc": "?=- EAZY 97.5% percentile of Hbeta line luminosity (reddened) (ez_LHb_p975)"}, {"name": "EZLOIIp025", "desc": "?=- EAZY 2.5% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p025)"}, {"name": "EZLOIIp160", "desc": "?=- EAZY 16.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p160)"}, {"name": "EZLOIIp500", "desc": "?=- EAZY 50.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p500)"}, {"name": "EZLOIIp840", "desc": "?=- EAZY 84.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p840)"}, {"name": "EZLOIIp975", "desc": "?=- EAZY 97.5% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p975)"}, {"name": "logEZsSFRp025", "desc": "?=- EAZY 2.5% percentile of log sSFR (ez_ssfr_p025)"}, {"name": "logEZsSFRp160", "desc": "?=- EAZY 16.0% percentile of log sSFR (ez_ssfr_p160)"}, {"name": "logEZsSFRp500", "desc": "?=- EAZY 50.0% percentile of log sSFR (ez_ssfr_p500)"}, {"name": "logEZsSFRp840", "desc": "?=- EAZY 84.0% percentile of log sSFR (ez_ssfr_p840)"}, {"name": "logEZsSFRp975", "desc": "?=- EAZY 97.5% percentile of log sSFR (ez_ssfr_p975)"}, {"name": "EZAVp025", "desc": "?=- EAZY 2.5% percentile of extinction in V band (ez_Av_p025)"}, {"name": "EZAVp160", "desc": "?=- EAZY 16.0% percentile of extinction in V band (ez_Av_p160)"}, {"name": "EZAVp500", "desc": "?=- EAZY 50.0% percentile of extinction in V band (ez_Av_p500)"}, {"name": "EZAVp840", "desc": "?=- EAZY 84.0% percentile of extinction in V band (ez_Av_p840)"}, {"name": "EZAVp975", "desc": "?=- EAZY 97.5% percentile of extinction in V band (ez_Av_p975)"}]}, {"name": "farmer.dat", "desc": "COSMOS2020 Photometric catalogue \"Farmer\" created using The Farmer / The Tractor (COSMOS2020_FARMER_R1_v2.1_p3.fits)", "columns": [{"name": "Farmer", "desc": "?=- Farmer catalogue ID (ID) "}, {"name": "RAmdeg", "desc": "Right ascension (J2000) of model, or of SEP when model is not avail. (ALPHA_J2000)"}, {"name": "DEmdeg", "desc": "Declination (J2000) of model, or of SEP when model is not available (DELTA_J2000)"}, {"name": "Xmodel", "desc": "?=- Object model position along X, with the scale being 0.15\"/pix (X_MODEL)"}, {"name": "Ymodel", "desc": "?=- Object model position along Y, with the scale being 0.15\"/pix (Y_MODEL)"}, {"name": "e_Xmodel", "desc": "?=- Uncertainty on object model position along X (ERRX_MODEL)"}, {"name": "e_Ymodel", "desc": "?=- Uncertainty on object model position along Y (ERRY_MODEL)"}, {"name": "RAdeg", "desc": "Right ascension (J2000) of object as determined by SEP at detection (ALPHA_DETECTION)"}, {"name": "DEdeg", "desc": "Declination (J2000) of object as determined by SEP at detection (DELTA_DETECTION)"}, {"name": "FarmerID", "desc": "Farmer internal source identifier ({brick}_{source}) (FARMER_ID)"}, {"name": "Group", "desc": "?=- Farmer group identifier; unique within a brick (GROUP_ID)"}, {"name": "NGroup", "desc": "?=- Farmer group occupation number (N_GROUP)"}, {"name": "FModel", "desc": "[0/2]?=- Flag (0: OK, 1: failed to converge, 2: drifted >0.6\" from detection) (MODEL_FLAG)"}, {"name": "SolModel", "desc": "The Tractor model type selected by The Farmer (SOLUTION_MODEL)"}, {"name": "FHSC", "desc": "?=- Flag indicating quality of HSC imaging (0: clean, 1: masked) (FLAG_HSC)"}, {"name": "FSUPCAM", "desc": "?=- Flag indicating quality of Suprime-Cam imaging (0: clean, 1: masked) (FLAG_SUPCAM)"}, {"name": "FUDEEP", "desc": "?=- Flag for the UltraVISTA ultra-deep regions (0: ultra-deep, 1 :deep) (FLAG_UDEEP)"}, {"name": "FUVISTA", "desc": "?=- Flag for the UltraVISTA region (0: inside, 1: outside) (FLAG_UVISTA)"}, {"name": "FCOMBINED", "desc": "?=- Comb. FLAG_UVISTA, FLAG_HSC, FLAG_SUPCAM (0: clean and inside UVISTA) (FLAG_COMBINED)"}, {"name": "E(B-V)", "desc": "Galactic reddening E(B-V) (EBV_MW) (1)"}, {"name": "FCFHTu", "desc": "?=- CFHT_u flux density (CFHT_u_FLUX)"}, {"name": "e_FCFHTu", "desc": "?=- CFHT_u flux density error (CFHT_u_FLUXERR)"}, {"name": "CFHTumag", "desc": "?=- CFHT_u AB magnitude (CFHT_u_MAG)"}, {"name": "e_CFHTumag", "desc": "?=- CFHT_u AB magnitude error (CFHT_u_MAGERR)"}, {"name": "CFHTuchi2", "desc": "?=- CFHT_u reduced Chi2 goodness of fit stat for source prof model (CFHT_u_CHISQ)"}, {"name": "CFHTuDrift", "desc": "?=- CFHT_u distance travelled from RA,Dec model centroid (CFHT_u_DRIFT)"}, {"name": "CFHTuValid", "desc": "[0/1] CFHT_u flag=0 if FLUX/MAG or its error is not trustworthy (CFHT_u_VALID)"}, {"name": "FCFHTustar", "desc": "?=- CFHT_ustar flux density (CFHT_ustar_FLUX)"}, {"name": "e_FCFHTustar", "desc": "?=- CFHT_ustar flux density error (CFHT_ustar_FLUXERR)"}, {"name": "CFHTustarmag", "desc": "?=- CFHT_ustar AB magnitude (CFHT_ustar_MAG)"}, {"name": "e_CFHTustarmag", "desc": "?=- CFHT_ustar AB magnitude error (CFHT_ustar_MAGERR)"}, {"name": "CFHTustarchi2", "desc": "?=- CFHT_ustar reduced Chi2 goodness of fit stat for source prof model (CFHT_ustar_CHISQ)"}, {"name": "CFHTustarDrift", "desc": "?=- CFHT_ustar distance travelled from RA,Dec model centroid (CFHT_ustar_DRIFT)"}, {"name": "CFHTustarValid", "desc": "[0/1] CFHT_ustar flag=0 if FLUX/MAG or its error is not trustworthy (CFHT_ustar_VALID)"}, {"name": "FHSCg", "desc": "?=- HSC_g flux density (HSC_g_FLUX)"}, {"name": "e_FHSCg", "desc": "?=- HSC_g flux density error (HSC_g_FLUXERR)"}, {"name": "HSCgmag", "desc": "?=- HSC_g AB magnitude (HSC_g_MAG) "}, {"name": "e_HSCgmag", "desc": "?=- HSC_g AB magnitude error (HSC_g_MAGERR)"}, {"name": "HSCgchi2", "desc": "?=- HSC_g reduced Chi2 goodness of fit stat for source prof model (HSC_g_CHISQ)"}, {"name": "HSCgDrift", "desc": "?=- HSC_g distance travelled from RA,Dec model centroid (HSC_g_DRIFT)"}, {"name": "HSCgValid", "desc": "[0,1] HSC_g flag=0 if FLUX/MAG or its error is not trustworthy (HSC_g_VALID)"}, {"name": "FHSCr", "desc": "?=- HSC_r flux density (HSC_r_FLUX)"}, {"name": "e_FHSCr", "desc": "?=- HSC_r flux density error (HSC_r_FLUXERR)"}, {"name": "HSCrmag", "desc": "?=- HSC_r AB magnitude (HSC_r_MAG) "}, {"name": "e_HSCrmag", "desc": "?=- HSC_r AB magnitude error (HSC_r_MAGERR)"}, {"name": "HSCrchi2", "desc": "?=- HSC_r reduced Chi2 goodness of fit stat for source prof model (HSC_r_CHISQ)"}, {"name": "HSCrDrift", "desc": "?=- HSC_r distance travelled from RA,Dec model centroid (HSC_r_DRIFT)"}, {"name": "HSCrValid", "desc": "[0/1] HSC_r flag=0 if FLUX/MAG or its error is not trustworthy (HSC_r_VALID)"}, {"name": "FHSCi", "desc": "?=- HSC_i flux density (HSC_i_FLUX)"}, {"name": "e_FHSCi", "desc": "?=- HSC_i flux density error (HSC_i_FLUXERR)"}, {"name": "HSCimag", "desc": "?=- HSC_i AB magnitude (HSC_i_MAG) "}, {"name": "e_HSCimag", "desc": "?=- HSC_i AB magnitude error (HSC_i_MAGERR)"}, {"name": "HSCichi2", "desc": "?=- HSC_i reduced Chi2 goodness of fit stat for source prof model (HSC_i_CHISQ)"}, {"name": "HSCiDrift", "desc": "?=- HSC_i distance travelled from RA,Dec model centroid (HSC_i_DRIFT)"}, {"name": "HSCiValid", "desc": "[0/1] HSC_i flag=0 if FLUX/MAG or its error is not trustworthy (HSC_i_VALID)"}, {"name": "FHSCz", "desc": "?=- HSC_i flux density (HSC_z_FLUX)"}, {"name": "e_FHSCz", "desc": "?=- HSC_z flux density error (HSC_z_FLUXERR)"}, {"name": "HSCzmag", "desc": "?=- HSC_z AB magnitude (HSC_z_MAG) "}, {"name": "e_HSCzmag", "desc": "?=- HSC_z AB magnitude error (HSC_z_MAGERR)"}, {"name": "HSCzchi2", "desc": "?=- HSC_z reduced Chi2 goodness of fit stat for source prof model (HSC_z_CHISQ)"}, {"name": "HSCzDrift", "desc": "?=- HSC_z distance travelled from RA,Dec model centroid (HSC_z_DRIFT)"}, {"name": "HSCzValid", "desc": "[0/1] HSC_z flag=0 if FLUX/MAG or its error is not trustworthy (HSC_z_VALID)"}, {"name": "FHSCy", "desc": "?=- HSC_y flux density (HSC_y_FLUX)"}, {"name": "e_FHSCy", "desc": "?=- HSC_y flux density error (HSC_y_FLUXERR)"}, {"name": "HSCymag", "desc": "?=- HSC_y AB magnitude (HSC_y_MAG) "}, {"name": "e_HSCymag", "desc": "?=- HSC_y AB magnitude error (HSC_y_MAGERR)"}, {"name": "HSCychi2", "desc": "?=- HSC_y reduced Chi2 goodness of fit stat for source prof model (HSC_y_CHISQ)"}, {"name": "HSCyDrift", "desc": "?=- HSC_y distance travelled from RA,Dec model centroid (HSC_y_DRIFT)"}, {"name": "HSCyValid", "desc": "[0/1] HSC_y flag=0 if FLUX/MAG or its error is not trustworthy (HSC_y_VALID)"}, {"name": "FUVISTAY", "desc": "?=- UVISTA_Y flux density (UVISTA_Y_FLUX)"}, {"name": "e_FUVISTAY", "desc": "?=- UVISTA_Y flux density error (UVISTA_Y_FLUXERR)"}, {"name": "UVISTAYmag", "desc": "?=- UVISTA_Y AB magnitude (UVISTA_Y_MAG)"}, {"name": "e_UVISTAYmag", "desc": "?=- UVISTA_Y AB magnitude error (UVISTA_Y_MAGERR)"}, {"name": "UVISTAYchi2", "desc": "?=- UVISTA_Y reduced Chi2 goodness of fit stat for source prof model (UVISTA_Y_CHISQ)"}, {"name": "UVISTAYDrift", "desc": "?=- UVISTA_Y distance travelled from RA,Dec model centroid (UVISTA_Y_DRIFT)"}, {"name": "UVISTAYValid", "desc": "[0/1] UVISTA_Y flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA_Y_VALID)"}, {"name": "FUVISTAJ", "desc": "?=- UVISTA_J flux density (UVISTA_J_FLUX)"}, {"name": "e_FUVISTAJ", "desc": "?=- UVISTA_J flux density error (UVISTA_J_FLUXERR)"}, {"name": "UVISTAJmag", "desc": "?=- UVISTA_J AB magnitude (UVISTA_J_MAG)"}, {"name": "e_UVISTAJmag", "desc": "?=- UVISTA_J AB magnitude error (UVISTA_J_MAGERR)"}, {"name": "UVISTAJchi2", "desc": "?=- UVISTA_J reduced Chi2 goodness of fit stat for source prof model (UVISTA_J_CHISQ)"}, {"name": "UVISTAJDrift", "desc": "?=- UVISTA_J distance travelled from RA,Dec model centroid (UVISTA_J_DRIFT)"}, {"name": "UVISTAJValid", "desc": "[0/1] UVISTA_J flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA_J_VALID)"}, {"name": "FUVISTAH", "desc": "?=- UVISTA_H flux density (UVISTA_H_FLUX)"}, {"name": "e_FUVISTAH", "desc": "?=- UVISTA_H flux density error (UVISTA_H_FLUXERR)"}, {"name": "UVISTAHmag", "desc": "?=- UVISTA_H AB magnitude (UVISTA_H_MAG)"}, {"name": "e_UVISTAHmag", "desc": "?=- UVISTA_H AB magnitude error (UVISTA_H_MAGERR)"}, {"name": "UVISTAHchi2", "desc": "?=- UVISTA_H reduced Chi2 goodness of fit stat for source prof model (UVISTA_H_CHISQ)"}, {"name": "UVISTAHDrift", "desc": "?=- UVISTA_H distance travelled from RA,Dec model centroid (UVISTA_H_DRIFT)"}, {"name": "UVISTAHValid", "desc": "[0/1] UVISTA_H flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA_H_VALID)"}, {"name": "FUVISTAKs", "desc": "?=- UVISTA_Ks flux density (UVISTA_Ks_FLUX)"}, {"name": "e_FUVISTAKs", "desc": "?=- UVISTA_Ks flux density error (UVISTA_Ks_FLUXERR)"}, {"name": "UVISTAKsmag", "desc": "?=- UVISTA_Ks AB magnitude (UVISTA_Ks_MAG)"}, {"name": "e_UVISTAKsmag", "desc": "?=- UVISTA_Ks AB magnitude error (UVISTA_Ks_MAGERR)"}, {"name": "UVISTAKschi2", "desc": "?=- UVISTA_Ks reduced Chi2 goodness of fit stat for source prof model (UVISTA_Ks_CHISQ)"}, {"name": "UVISTAKsDrift", "desc": "?=- UVISTA_Ks distance travelled from RA,Dec model centroid (UVISTA_Ks_DRIFT)"}, {"name": "UVISTAKsValid", "desc": "[0/1] UVISTA_Ks flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA_Ks_VALID)"}, {"name": "FUVISTANB118", "desc": "?=- UVISTA_NB118 flux density (UVISTA_NB118_FLUX)"}, {"name": "e_FUVISTANB118", "desc": "?=- UVISTA_NB118 flux density error (UVISTA_NB118_FLUXERR)"}, {"name": "UVISTANB118mag", "desc": "?=- UVISTA_NB118 AB magnitude (UVISTA_NB118_MAG)"}, {"name": "e_UVISTANB118mag", "desc": "?=- UVISTA_NB118 AB magnitude error (UVISTA_NB118_MAGERR)"}, {"name": "UVISTANB118chi2", "desc": "?=- UVISTA_NB118 reduced Chi2 goodness of fit stat for source prof model (UVISTA_NB118_CHISQ)"}, {"name": "UVISTANB118Drift", "desc": "?=- UVISTA_NB118 distance travelled from RA,Dec model centroid (UVISTA_NB118_DRIFT)"}, {"name": "UVISTANB118Valid", "desc": "[0/1] UVISTA_NB118 flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA_NB118_VALID)"}, {"name": "FSCIB427", "desc": "?=- SC_IB427 flux density (SC_IB427_FLUX)"}, {"name": "e_FSCIB427", "desc": "?=- SC_IB427 flux density error (SC_IB427_FLUXERR)"}, {"name": "SCIB427mag", "desc": "?=- SC_IB427 AB magnitude (SC_IB427_MAG)"}, {"name": "e_SCIB427mag", "desc": "?=- SC_IB427 AB magnitude error (SC_IB427_MAGERR)"}, {"name": "SCIB427chi2", "desc": "?=- SC_IB427 reduced Chi2 goodness of fit stat for source prof model (SC_IB427_CHISQ)"}, {"name": "SCIB427Drift", "desc": "?=- SC_IB427 distance travelled from RA,Dec model centroid (SC_IB427_DRIFT)"}, {"name": "SCIB427Valid", "desc": "[0/1] SC_IB427 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IB427_VALID)"}, {"name": "FSCIB464", "desc": "?=- SC_IB464 flux density (SC_IB464_FLUX)"}, {"name": "e_FSCIB464", "desc": "?=- SC_IB464 flux density error (SC_IB464_FLUXERR)"}, {"name": "SCIB464mag", "desc": "?=- SC_IB464 AB magnitude (SC_IB464_MAG)"}, {"name": "e_SCIB464mag", "desc": "?=- SC_IB464 AB magnitude error (SC_IB464_MAGERR)"}, {"name": "SCIB464chi2", "desc": "?=- SC_IB464 reduced Chi2 goodness of fit stat for source prof model (SC_IB464_CHISQ)"}, {"name": "SCIB464Drift", "desc": "?=- SC_IB464 distance travelled from RA,Dec model centroid (SC_IB464_DRIFT)"}, {"name": "SCIB464Valid", "desc": "[0/1] SC_IB464 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IB464_VALID)"}, {"name": "FSCIA484", "desc": "?=- SC_IA484 flux density (SC_IA484_FLUX)"}, {"name": "e_FSCIA484", "desc": "?=- SC_IA484 flux density error (SC_IA484_FLUXERR)"}, {"name": "SCIA484mag", "desc": "?=- SC_IA484 AB magnitude (SC_IA484_MAG)"}, {"name": "e_SCIA484mag", "desc": "?=- SC_IA484 AB magnitude error (SC_IA484_MAGERR)"}, {"name": "SCIA484chi2", "desc": "?=- SC_IA484 reduced Chi2 goodness of fit stat for source prof model (SC_IA484_CHISQ)"}, {"name": "SCIA484Drift", "desc": "?=- SC_IA484 distance travelled from RA,Dec model centroid (SC_IA484_DRIFT)"}, {"name": "SCIA484Valid", "desc": "[0/1] SC_IA484 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IA484_VALID)"}, {"name": "FSCIB505", "desc": "?=- SC_IB505 flux density (SC_IB505_FLUX)"}, {"name": "e_FSCIB505", "desc": "?=- SC_IB505 flux density error (SC_IB505_FLUXERR)"}, {"name": "SCIB505mag", "desc": "?=- SC_IB505 AB magnitude (SC_IB505_MAG)"}, {"name": "e_SCIB505mag", "desc": "?=- SC_IB505 AB magnitude error (SC_IB505_MAGERR)"}, {"name": "SCIB505chi2", "desc": "?=- SC_IB505 reduced Chi2 goodness of fit stat for source prof model (SC_IB505_CHISQ)"}, {"name": "SCIB505Drift", "desc": "?=- SC_IB505 distance travelled from RA,Dec model centroid (SC_IB505_DRIFT)"}, {"name": "SCIB505Valid", "desc": "[0/1] SC_IB505 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IB505_VALID)"}, {"name": "FSCIA527", "desc": "?=- SC_IA527 flux density (SC_IA527_FLUX)"}, {"name": "e_FSCIA527", "desc": "?=- SC_IA527 flux density error (SC_IA527_FLUXERR)"}, {"name": "SCIA527mag", "desc": "?=- SC_IA527 AB magnitude (SC_IA527_MAG)"}, {"name": "e_SCIA527mag", "desc": "?=- SC_IA527 AB magnitude error (SC_IA527_MAGERR)"}, {"name": "SCIA527chi2", "desc": "?=- SC_IA527 reduced Chi2 goodness of fit stat for source prof model (SC_IA527_CHISQ)"}, {"name": "SCIA527Drift", "desc": "?=- SC_IA527 distance travelled from RA,Dec model centroid (SC_IA527_DRIFT)"}, {"name": "SCIA527Valid", "desc": "[0/1] SC_IA527 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IA527_VALID)"}, {"name": "FSCIB574", "desc": "?=- SC_IB574 flux density (SC_IB574_FLUX)"}, {"name": "e_FSCIB574", "desc": "?=- SC_IB574 flux density error (SC_IB574_FLUXERR)"}, {"name": "SCIB574mag", "desc": "?=- SC_IB574 AB magnitude (SC_IB574_MAG)"}, {"name": "e_SCIB574mag", "desc": "?=- SC_IB574 AB magnitude error (SC_IB574_MAGERR)"}, {"name": "SCIB574chi2", "desc": "?=- SC_IB574 reduced Chi2 goodness of fit stat for source prof model (SC_IB574_CHISQ)"}, {"name": "SCIB574Drift", "desc": "?=- SC_IB574 distance travelled from RA,Dec model centroid (SC_IB574_DRIFT)"}, {"name": "SCIB574Valid", "desc": "[0/1] SC_IB574 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IB574_VALID)"}, {"name": "FSCIA624", "desc": "?=- SC_IA624 flux density (SC_IA624_FLUX)"}, {"name": "e_FSCIA624", "desc": "?=- SC_IA624 flux density error (SC_IA624_FLUXERR)"}, {"name": "SCIA624mag", "desc": "?=- SC_IA624 AB magnitude (SC_IA624_MAG)"}, {"name": "e_SCIA624mag", "desc": "?=- SC_IA624 AB magnitude error (SC_IA624_MAGERR)"}, {"name": "SCIA624chi2", "desc": "?=- SC_IA624 reduced Chi2 goodness of fit stat for source prof model (SC_IA624_CHISQ)"}, {"name": "SCIA624Drift", "desc": "?=- SC_IA624 distance travelled from RA,Dec model centroid (SC_IA624_DRIFT)"}, {"name": "SCIA624Valid", "desc": "[0/1] SC_IA624 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IA624_VALID)"}, {"name": "FSCIA679", "desc": "?=- SC_IA679 flux density (SC_IA679_FLUX)"}, {"name": "e_FSCIA679", "desc": "?=- SC_IA679 flux density error (SC_IA679_FLUXERR)"}, {"name": "SCIA679mag", "desc": "?=- SC_IA679 AB magnitude (SC_IA679_MAG)"}, {"name": "e_SCIA679mag", "desc": "?=- SC_IA679 AB magnitude error (SC_IA679_MAGERR)"}, {"name": "SCIA679chi2", "desc": "?=- SC_IA679 reduced Chi2 goodness of fit stat for source prof model (SC_IA679_CHISQ)"}, {"name": "SCIA679Drift", "desc": "?=- SC_IA679 distance travelled from RA,Dec model centroid (SC_IA679_DRIFT)"}, {"name": "SCIA679Valid", "desc": "[0/1] SC_IA679 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IA679_VALID)"}, {"name": "FSCIB709", "desc": "?=- SC_IB709 flux density (SC_IB709_FLUX)"}, {"name": "e_FSCIB709", "desc": "?=- SC_IB709 flux density error (SC_IB709_FLUXERR)"}, {"name": "SCIB709mag", "desc": "?=- SC_IB709 AB magnitude (SC_IB709_MAG)"}, {"name": "e_SCIB709mag", "desc": "?=- SC_IB709 AB magnitude error (SC_IB709_MAGERR)"}, {"name": "SCIB709chi2", "desc": "?=- SC_IB709 reduced Chi2 goodness of fit stat for source prof model (SC_IB709_CHISQ)"}, {"name": "SCIB709Drift", "desc": "?=- SC_IB709 distance travelled from RA,Dec model centroid (SC_IB709_DRIFT)"}, {"name": "SCIB709Valid", "desc": "[0/1] SC_IB709_VALID flag=0 if FLUX/MAG or its error is not trustworthy (SC_IB709_VALID)"}, {"name": "FSCIA738", "desc": "?=- SC_IA738 flux density (SC_IA738_FLUX)"}, {"name": "e_FSCIA738", "desc": "?=- SC_IA738 flux density error (SC_IA738_FLUXERR)"}, {"name": "SCIA738mag", "desc": "?=- SC_IA738 AB magnitude (SC_IA738_MAG)"}, {"name": "e_SCIA738mag", "desc": "?=- SC_IA738 AB magnitude error (SC_IA738_MAGERR)"}, {"name": "SCIA738chi2", "desc": "?=- SC_IA738 reduced Chi2 goodness of fit stat for source prof model (SC_IA738_CHISQ)"}, {"name": "SCIA738Drift", "desc": "?=- SC_IA738 distance travelled from RA,Dec model centroid (SC_IA738_DRIFT)"}, {"name": "SCIA738Valid", "desc": "[0/1] SC_IA738 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IA738_VALID)"}, {"name": "FSCIA767", "desc": "?=- SC_IA767 flux density (SC_IA767_FLUX)"}, {"name": "e_FSCIA767", "desc": "?=- SC_IA767 flux density error (SC_IA767_FLUXERR)"}, {"name": "SCIA767mag", "desc": "?=- SC_IA767 AB magnitude (SC_IA767_MAG)"}, {"name": "e_SCIA767mag", "desc": "?=- SC_IA767 AB magnitude error (SC_IA767_MAGERR)"}, {"name": "SCIA767chi2", "desc": "?=- SC_IA767 reduced Chi2 goodness of fit stat for source prof model (SC_IA767_CHISQ)"}, {"name": "SCIA767Drift", "desc": "?=- SC_IA767 distance travelled from RA,Dec model centroid (SC_IA767_DRIFT)"}, {"name": "SCIA767Valid", "desc": "[0/1] SC_IA767 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IA767_VALID)"}, {"name": "FSCIB827", "desc": "?=- SC_IB827 flux density (SC_IB827_FLUX)"}, {"name": "e_FSCIB827", "desc": "?=- SC_IB827 flux density error (SC_IB827_FLUXERR)"}, {"name": "SCIB827mag", "desc": "?=- SC_IB827 AB magnitude (SC_IB827_MAG)"}, {"name": "e_SCIB827mag", "desc": "?=- SC_IB827 AB magnitude error (SC_IB827_MAGERR)"}, {"name": "SCIB827chi2", "desc": "?=- SC_IB827 reduced Chi2 goodness of fit stat for source prof model (SC_IB827_CHISQ)"}, {"name": "SCIB827Drift", "desc": "?=- SC_IB827 distance travelled from RA,Dec model centroid (SC_IB827_DRIFT)"}, {"name": "SCIB827Valid", "desc": "[0/1] SC_IB827 flag=0 if FLUX/MAG or its error is not trustworthy (SC_IB827_VALID)"}, {"name": "FSCNB711", "desc": "?=- SC_NB711 flux density (SC_NB711_FLUX)"}, {"name": "e_FSCNB711", "desc": "?=- SC_NB711 flux density error (SC_NB711_FLUXERR)"}, {"name": "SCNB711mag", "desc": "?=- SC_NB711 AB magnitude (SC_NB711_MAG)"}, {"name": "e_SCNB711mag", "desc": "?=- SC_NB711 AB magnitude error (SC_NB711_MAGERR)"}, {"name": "SCNB711chi2", "desc": "?=- SC_NB711 reduced Chi2 goodness of fit stat for source prof model (SC_NB711_CHISQ)"}, {"name": "SCNB711Drift", "desc": "?=- SC_NB711 distance travelled from RA,Dec model centroid (SC_NB711_DRIFT)"}, {"name": "SCNB711Valid", "desc": "[0/1] SC_NB711 flag=0 if FLUX/MAG or its error is not trustworthy (SC_NB711_VALID)"}, {"name": "FSCNB816", "desc": "?=- SC_NB816 flux density (SC_NB816_FLUX)"}, {"name": "e_FSCNB816", "desc": "?=- SC_NB816 flux density error (SC_NB816_FLUXERR)"}, {"name": "SCNB816mag", "desc": "?=- SC_NB816 AB magnitude (SC_NB816_MAG)"}, {"name": "e_SCNB816mag", "desc": "?=- SC_NB816 AB magnitude error (SC_NB816_MAGERR)"}, {"name": "SCNB816chi2", "desc": "?=- SC_NB816 reduced Chi2 goodness of fit stat for source prof model (SC_NB816_CHISQ)"}, {"name": "SCNB816Drift", "desc": "?=- SC_NB816 distance travelled from RA,Dec model centroid (SC_NB816_DRIFT)"}, {"name": "SCNB816Valid", "desc": "[0/1] SC_NB816 flag=0 if FLUX/MAG or its error is not trustworthy (SC_NB816_VALID)"}, {"name": "FIRACCH1", "desc": "?=- IRAC_CH1 flux density (IRAC_CH1_FLUX)"}, {"name": "e_FIRACCH1", "desc": "?=- IRAC_CH1 flux density error (IRAC_CH1_FLUXERR)"}, {"name": "IRACCH1mag", "desc": "?=- IRAC_CH1 AB magnitude (IRAC_CH1_MAG)"}, {"name": "e_IRACCH1mag", "desc": "?=- IRAC_CH1 AB magnitude error (IRAC_CH1_MAGERR)"}, {"name": "IRACCH1chi2", "desc": "?=- IRAC_CH1 reduced Chi2 goodness of fit stat for source prof model (IRAC_CH1_CHISQ)"}, {"name": "IRACCH1Drift", "desc": "?=- IRAC_CH1 distance travelled from RA,Dec model centroid (IRAC_CH1_DRIFT)"}, {"name": "IRACCH1Valid", "desc": "[0/1] IRAC_CH1 flag=0 if FLUX/MAG or its error is not trustworthy (IRAC_CH1_VALID)"}, {"name": "FIRACCH2", "desc": "?=- IRAC_CH2 flux density (IRAC_CH2_FLUX)"}, {"name": "e_FIRACCH2", "desc": "?=- IRAC_CH2 flux density error (IRAC_CH2_FLUXERR)"}, {"name": "IRACCH2mag", "desc": "?=- IRAC_CH2 AB magnitude (IRAC_CH2_MAG)"}, {"name": "e_IRACCH2mag", "desc": "?=- IRAC_CH2 AB magnitude error (IRAC_CH2_MAGERR)"}, {"name": "IRACCH2chi2", "desc": "?=- IRAC_CH2 reduced Chi2 goodness of fit stat for source prof model (IRAC_CH2_CHISQ)"}, {"name": "IRACCH2Drift", "desc": "?=- IRAC_CH2 distance travelled from RA,Dec model centroid (IRAC_CH2_DRIFT)"}, {"name": "IRACCH2Valid", "desc": "[0/1] IRAC_CH2 flag=0 if FLUX/MAG or its error is not trustworthy (IRAC_CH2_VALID)"}, {"name": "FIRACCH3", "desc": "?=- IRAC_CH3 flux density (IRAC_CH3_FLUX)"}, {"name": "e_FIRACCH3", "desc": "?=- IRAC_CH3 flux density error (IRAC_CH3_FLUXERR)"}, {"name": "IRACCH3mag", "desc": "?=- IRAC_CH3 AB magnitude (IRAC_CH3_MAG)"}, {"name": "e_IRACCH3mag", "desc": "?=- IRAC_CH3 AB magnitude error (IRAC_CH3_MAGERR)"}, {"name": "IRACCH3chi2", "desc": "?=- IRAC_CH3 reduced Chi2 goodness of fit stat for source prof model (IRAC_CH3_CHISQ)"}, {"name": "IRACCH3Drift", "desc": "?=- IRAC_CH3 distance travelled from RA,Dec model centroid (IRAC_CH3_DRIFT)"}, {"name": "IRACCH3Valid", "desc": "[0/1] IRAC_CH3 flag=0 if FLUX/MAG or its error is not trustworthy (IRAC_CH3_VALID)"}, {"name": "FIRACCH4", "desc": "?=- IRAC_CH4 flux density (IRAC_CH4_FLUX)"}, {"name": "e_FIRACCH4", "desc": "?=- IRAC_CH4 flux density error (IRAC_CH4_FLUXERR)"}, {"name": "IRACCH4mag", "desc": "?=- IRAC_CH4 AB magnitude (IRAC_CH4_MAG)"}, {"name": "e_IRACCH4mag", "desc": "?=- IRAC_CH4 AB magnitude error (IRAC_CH4_MAGERR)"}, {"name": "IRACCH4chi2", "desc": "?=- IRAC_CH4 reduced Chi2 goodness of fit stat for source prof model (IRAC_CH4_CHISQ)"}, {"name": "IRACCH4Drift", "desc": "?=- IRAC_CH4 distance travelled from RA,Dec model centroid (IRAC_CH4_DRIFT)"}, {"name": "IRACCH4Valid", "desc": "[0/1] IRAC_CH4 flag=0 if FLUX/MAG or its error is not trustworthy (IRAC_CH4_VALID)"}, {"name": "GALEX", "desc": "?=- ID in GALEX cat. (Zamojski et al., 2007ApJS..172..468Z, Capak et al., 2007, Cat. II/284), crossm. with 0.6\" rad. (ID_GALEX)"}, {"name": "FGALEXNUV", "desc": "?=- GALEX_NUV flux density (GALEX_NUV_FLUX)"}, {"name": "e_FGALEXNUV", "desc": "?=- GALEX_NUV flux density error (GALEX_NUV_FLUXERR)"}, {"name": "GALEXNUVmag", "desc": "?=- GALEX_NUV AB magnitude (GALEX_NUV_MAG)"}, {"name": "e_GALEXNUVmag", "desc": "?=- GALEX_NUV AB magnitude error (GALEX_NUV_MAGERR)"}, {"name": "FGALEXFUV", "desc": "?=- GALEX_FUV flux density (GALEX_FUV_FLUX)"}, {"name": "e_FGALEXFUV", "desc": "?=- GALEX_FUV flux density error (GALEX_FUV_FLUXERR)"}, {"name": "GALEXFUVmag", "desc": "?=- GALEX_FUV AB magnitude (GALEX_FUV_MAG)"}, {"name": "e_GALEXFUVmag", "desc": "?=- GALEX_FUV AB magnitude error (GALEX_FUV_MAGERR)"}, {"name": "COSMOS2015", "desc": "?=- ID in COSMOS2015 cat. (Laigle et al., 2016, Cat. J/ApJS/224/24) crossmatched with 0.6\" radius (ID_COSMOS2015)"}, {"name": "FSPLASHCH1", "desc": "?=- SPLASH_CH1 flux density (SPLASH_CH1_FLUX)"}, {"name": "e_FSPLASHCH1", "desc": "?=- SPLASH_CH1 flux density error (SPLASH_CH1_FLUXERR)"}, {"name": "SPLASHCH1mag", "desc": "?=- SPLASH_CH1 AB magnitude (SPLASH_CH1_MAG)"}, {"name": "e_SPLASHCH1mag", "desc": "?=- SPLASH_CH1 AB magnitude error (SPLASH_CH1_MAGERR)"}, {"name": "FSPLASHCH2", "desc": "?=- SPLASH_CH2 flux density (SPLASH_CH2_FLUX)"}, {"name": "e_FSPLASHCH2", "desc": "?=- SPLASH_CH2 flux density error (SPLASH_CH2_FLUXERR)"}, {"name": "SPLASHCH2mag", "desc": "?=- SPLASH_CH2 AB magnitude (SPLASH_CH2_MAG)"}, {"name": "e_SPLASHCH2mag", "desc": "?=- SPLASH_CH2 AB magnitude error (SPLASH_CH2_MAGERR)"}, {"name": "FSPLASHCH3", "desc": "?=- SPLASH_CH3 flux density (SPLASH_CH3_FLUX)"}, {"name": "e_FSPLASHCH3", "desc": "?=- SPLASH_CH3 flux density error (SPLASH_CH3_FLUXERR)"}, {"name": "SPLASHCH3mag", "desc": "?=- SPLASH_CH3 AB magnitude (SPLASH_CH3_MAG)"}, {"name": "e_SPLASHCH3mag", "desc": "?=- SPLASH_CH3 AB magnitude error (SPLASH_CH3_MAGERR)"}, {"name": "FSPLASHCH4", "desc": "?=- SPLASH_CH4 flux density (SPLASH_CH4_FLUX)"}, {"name": "e_FSPLASHCH4", "desc": "?=- SPLASH_CH4 flux density error (SPLASH_CH4_FLUXERR)"}, {"name": "SPLASHCH4mag", "desc": "?=- SPLASH_CH4 AB magnitude (SPLASH_CH4_MAG)"}, {"name": "e_SPLASHCH4mag", "desc": "?=- SPLASH_CH4 AB magnitude error (SPLASH_CH4_MAGERR)"}, {"name": "ACS", "desc": "?=- ID in HST ACS F814W cat. (Leauthaud et al., 2007ApJS..172..219L), crossm. with 0.6\" radius (ID_ACS)"}, {"name": "ACSF814Wmag", "desc": "?=- ACS_F814W AB magnitude (ACS_F814W_MAG)"}, {"name": "e_ACSF814Wmag", "desc": "?=- ACS_F814W AB magnitude error (ACS_F814W_MAGERR)"}, {"name": "FACSF814W", "desc": "?=- ACS_F814W flux density (ACS_F814W_FLUX)"}, {"name": "e_FACSF814W", "desc": "?=- ACS_F814W flux density error (ACS_F814W_FLUXERR)"}, {"name": "ACSAWorld", "desc": "?=- ACS F814W semi-major axis length (ACS_A_WORLD)"}, {"name": "ACSBWorld", "desc": "?=- ACS F814W semi-minor axis length (ACS_B_WORLD)"}, {"name": "ACSthetaWorld", "desc": "?=- ACS F814W angle; to get PA measured from N through E, add/subtr. 90 (ACS_THETA_WORLD)"}, {"name": "ACSFWHMWorld", "desc": "?=- ACS F814W FWHM assuming a gaussian core (ACS_FWHM_WORLD)"}, {"name": "ACSmu", "desc": "?=- ACS F814W peak surface brightness above background (ACS_MU_MAX)"}, {"name": "ACSmuClass", "desc": "[1/3]? ACS F814W star/galaxy classifier: 1=galaxy, 2=star, 3=fake detection (ACS_MU_CLASS)"}, {"name": "CHANDRA", "desc": "ID in Chandra cat. (Civano et al., 2016, Cat. J/ApJ/819/62, Marchesi et al., 2016, Cat. J/ApJ/817/34), crossm. w. 0.6\" rad (ID_CHANDRA)"}, {"name": "Classic", "desc": "?=- ID in the Classic catalogue, crossmatched with 0.6\" radius (ID_CLASSIC)"}, {"name": "lpzBEST", "desc": "?=- LePhare photo-z (=lp_zPDF if galaxy, NaN if X-ray source or masked) (lp_zBEST)"}, {"name": "lptype", "desc": "[0/2]?=- LePhare type (0: galaxy, 1: star, 2: Xray sour., -: failure in fit) (lp_type)"}, {"name": "lpzPDF", "desc": "?=- LePhare photo-z using the galaxy templ., median of likelihood distr. (lp_zPDF)"}, {"name": "lpzPDFl68", "desc": "?=- LePhare photo-z lower limit, 68% confidence level (galaxy templates) (lp_zPDF_l68)"}, {"name": "lpzPDFu68", "desc": "?=- LePhare photo-z upper limit, 68% confidence level (galaxy templates) (lp_zPDF_u68)"}, {"name": "lpzMinChi2", "desc": "?=- LePhare photo-z using the galaxy templates, minimum chi2 (lp_zMinChi2)"}, {"name": "lpchi2best", "desc": "?=- LePhare reduced chi2 for lp_zMinChi2 (NaN if less than 3 filters) (lp_chi2_best)"}, {"name": "lpzp2", "desc": "?=- LePhare 2nd photo-z solution if a 2nd peak detected w. P>5% in PDF (lp_zp_2)"}, {"name": "lpchi22", "desc": "?=- LePhare reduced chi2 for the second photo-z solution (lp_chi2_2)"}, {"name": "lpNbFilt", "desc": "?=- LePhare number of filters used in the fi (lp_NbFilt)"}, {"name": "lpzq", "desc": "?=- LePhare photo-z for the AGN library (lp_zq)"}, {"name": "lpchiq", "desc": "?=- LePhare reduced chi2 for photo-z for the AGN library (lp_chiq)"}, {"name": "lpmodq", "desc": "?=- LePhare best fit template number in the AGN library (lp_modq)"}, {"name": "lpmods", "desc": "?=- LePhare best fit template number in the star library (lp_mods)"}, {"name": "lpchis", "desc": "?=- LePhare reduced chi2 for the best fit with the star library (lp_chis)"}, {"name": "lpmask", "desc": "?=- LePhare mask flag (0: in UVISTA and in clean part of HSC and SUPCAM) (lp_mask)"}, {"name": "lpmodel", "desc": "?=- LePhare BC03 best fit template number (lp_model)"}, {"name": "lpage", "desc": "?=- LePhare BC03 age of best fit template at zPDF (lp_age)"}, {"name": "lpdust", "desc": "?=- LePhare BC03 colour excess E(B-V) of best fit template at zPDF (lp_dust)"}, {"name": "lpAtt", "desc": "?=- LePhare BC03 best-fit dust law number at zPDF (lp_Attenuation)"}, {"name": "lpFUVMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in GALEX FUV band at zPDF (lp_MFUV)"}, {"name": "lpNUVMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in GALEX NUV band at zPDF (lp_MNUV)"}, {"name": "lpUMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in CFHT u* band at zPD (lp_MU)"}, {"name": "lpGMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC g band at zPDF (lp_MG)"}, {"name": "lpRMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC r band at zPDF (lp_MR)"}, {"name": "lpIMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC i band at zPDF (lp_MI)"}, {"name": "lpZMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC z band at zPDF (lp_MZ)"}, {"name": "lpYMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC Y band at zPDF (lp_MY)"}, {"name": "lpJMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC J band at zPDF (lp_MJ)"}, {"name": "lpHMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC H band at zPDF (lp_MH)"}, {"name": "lpKMAG", "desc": "?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC Ks band at zPDF (lp_MK)"}, {"name": "loglpMassmed", "desc": "?=- LePhare BC03 log stellar mass at zPDF (lp_mass_med)"}, {"name": "b_loglpMassmed", "desc": "?=- LePhare BC03 log stellar mass at zPDF, lower limit, 68% conf. level (lp_mass_med_min68)"}, {"name": "B_loglpMassmed", "desc": "?=- LePhare BC03 log stellar mass at zPDF, upper limit, 68% conf. level (lp_mass_med_max68)"}, {"name": "loglpMassbest", "desc": "?=- LePhare BC03 log stellar mass at zMinChi2 (lp_mass_best)"}, {"name": "loglpSFRmed", "desc": "?=- LePhare BC03 log stellar mass at zPDF (lp_SFR_med)"}, {"name": "b_loglpSFRmed", "desc": "?=- LePhare BC03 log SFR at zPDF, lower limit, 68% confidence level (lp_SFR_med_min68)"}, {"name": "B_loglpSFRmed", "desc": "?=- LePhare BC03 log SFR at zPDF, upper limit, 68% confidence level (lp_SFR_med_max68)"}, {"name": "loglpSFRbest", "desc": "?=- LePhare BC03 log SFR at zMinChi2 (lp_SFR_best)"}, {"name": "loglpsSFRmed", "desc": "?=- LePhare BC03 log sSFR at zPDF (lp_sSFR_med)"}, {"name": "b_loglpsSFRmed", "desc": "?=- LePhare BC03 log sSFR at zPDF, lower limit, 68% confidence level (lp_sSFR_med_min68)"}, {"name": "B_loglpsSFRmed", "desc": "?=- LePhare BC03 log sSFR at zPDF, upper limit, 68% confidence level (lp_sSFR_med_max68)"}, {"name": "loglpsSFRbest", "desc": "?=- LePhare BC03 log sSFR at zMinChi2 (lp_sSFR_best)"}, {"name": "EZzphot", "desc": "?=- EAZY maximum a-posteriori photo-z (ez_z_phot)"}, {"name": "EZzphotchi2", "desc": "?=- EAZY chi2 at ez_z_phot, with z-prior (ez_z_phot_chi2)"}, {"name": "EZzphotrisk", "desc": "?=- EAZY risk parameter (Tanaka, 2018PASJ...70S...9T) at ez_z_phot, R(ez_z_phot) (ez_z_phot_risk)"}, {"name": "EZzminrisk", "desc": "?=- EAZY photo-z where risk parameter R(z) is minimised (ez_z_min_risk)"}, {"name": "EZminrisk", "desc": "?=- EAZY risk parameter at ez_z_min_risk, R(ez_z_min_risk) (ez_min_risk)"}, {"name": "EZzrawchi2", "desc": "?=- EAZY photo-z where chi2 is minimised, without priors (ez_z_raw_chi2)"}, {"name": "EZrawchi2", "desc": "?=- EAZY chi2 at ez_z_raw_chi2 (ez_raw_chi2)"}, {"name": "EZzp025", "desc": "?=- EAZY 2.5% percentile of photo-z (ez_z025)"}, {"name": "EZzp160", "desc": "?=- EAZY 16.0% percentile of photo-z (ez_z160)"}, {"name": "EZzp500", "desc": "?=- EAZY 50.0% percentile of photo-z (ez_z500)"}, {"name": "EZzp840", "desc": "?=- EAZY 84.0% percentile of photo-z (ez_z840)"}, {"name": "EZzp975", "desc": "?=- EAZY 97.5% percentile of photo-z (ez_z975)"}, {"name": "EZnusefilt", "desc": "?=- EAZY no. of filters used for photo-z (only filters w/o missing data) (ez_nusefilt)"}, {"name": "EZlcmin", "desc": "?=- EAZY minimum effective wavelength of valid filters (ez_lc_min)"}, {"name": "EZlcmax", "desc": "?=- EAZY maximum effective wavelength of valid filters (ez_lc_max)"}, {"name": "EZstarminchi2", "desc": "?=- EAZY chi2 best stellar template fit (BT-SETTL models) as, 8% sys unc (ez_star_min_chi2)"}, {"name": "EZstarTeff", "desc": "?=- EAZY effective temperature of the stellar template (ez_star_teff)"}, {"name": "EZrestU", "desc": "?=- EAZY rest-frame U-band flux density (ez_restU)"}, {"name": "e_EZrestU", "desc": "?=- EAZY rest-frame U-band flux density uncertainty (ez_restU_err)"}, {"name": "EZrestB", "desc": "?=- EAZY rest-frame B-band flux density (ez_restB)"}, {"name": "e_EZrestB", "desc": "?=- EAZY rest-frame B-band flux density uncertainty (ez_restB_err)"}, {"name": "EZrestV", "desc": "?=- EAZY rest-frame V-band flux density (ez_restV)"}, {"name": "e_EZrestV", "desc": "?=- EAZY rest-frame V-band flux density uncertainty (ez_restV_err)"}, {"name": "EZrestJ", "desc": "?=- EAZY rest-frame J-band flux density (ez_restJ)"}, {"name": "e_EZrestJ", "desc": "?=- EAZY rest-frame J-band flux density uncertainty (ez_restJ_err)"}, {"name": "EZdL", "desc": "?=- EAZY luminosity distance at ez_z_phot (ez_dL)"}, {"name": "logEZMass", "desc": "?=- EAZY log stellar mass (ez_mass)"}, {"name": "logEZSFR", "desc": "?=- EAZY log SFR (ez_sfr) "}, {"name": "logEZsSFR", "desc": "?=- EAZY log sSFR (ez_ssfr) "}, {"name": "logEZLV", "desc": "?=- EAZY log V-band luminosity (ez_Lv)"}, {"name": "EZLIR", "desc": "?=- EAZY total 8-1000um luminosity (ez_LIR)"}, {"name": "EZEnerAbs", "desc": "?=- EAZY implied absorbed energy associated with Av (ez_energy_abs)"}, {"name": "EZLU", "desc": "?=- EAZY luminosity in rest-frame U band (ez_Lu)"}, {"name": "EZLJ", "desc": "?=- EAZY luminosity in rest-frame J band (ez_Lj)"}, {"name": "EZL1400", "desc": "?=- EAZY luminosity in tophat filter at 1400{AA} (200{AA} wide) rest-frame (ez_L1400)"}, {"name": "EZL2800", "desc": "?=- EAZY luminosity in tophat filter at 2800{AA} (200{AA} wide) rest-frame (ez_L2800)"}, {"name": "EZLHa", "desc": "?=- EAZY Halpha line luminosity (reddened) (ez_LHa)"}, {"name": "EZLOIII", "desc": "?=- EAZY [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII)"}, {"name": "EZLHb", "desc": "?=- EAZY Hbeta line luminosity (reddened) (ez_LHb)"}, {"name": "EZLOII", "desc": "?=- EAZY [OII] 3726+3729 line luminosity (reddened) (ez_LOII)"}, {"name": "EZM/LV", "desc": "?=- EAZY mass-to-light ratio in V band (ez_MLv)"}, {"name": "EZAV", "desc": "?=- EAZY extinction in V band (ez_Av)"}, {"name": "EZlwAgev", "desc": "?=- EAZY light-weighted age in the V band (ez_lwAgeV)"}, {"name": "logEZMassp025", "desc": "?=- EAZY 2.5% percentile of log stellar mass (ez_mass_p025)"}, {"name": "logEZMassp160", "desc": "?=- EAZY 16.0% percentile of log stellar mass (ez_mass_p160)"}, {"name": "logEZMassp500", "desc": "?=- EAZY 50.0% percentile of log stellar mass (ez_mass_p500)"}, {"name": "logEZMassp840", "desc": "?=- EAZY 84.0% percentile of log stellar mass (ez_mass_p840)"}, {"name": "logEZMassp975", "desc": "?=- EAZY 97.5% percentile of log stellar mass (ez_mass_p975)"}, {"name": "logEZSFRp025", "desc": "?=- EAZY 2.5% percentile of log SFR (ez_sfr_p025)"}, {"name": "logEZSFRp160", "desc": "?=- EAZY 16.0% percentile of log SFR (ez_sfr_p160)"}, {"name": "logEZSFRp500", "desc": "?=- EAZY 50.0% percentile of log SFR (ez_sfr_p500)"}, {"name": "logEZSFRp840", "desc": "?=- EAZY 84.0% percentile of log SFR (ez_sfr_p840)"}, {"name": "logEZSFRp975", "desc": "?=- EAZY 95.5% percentile of log SFR (ez_sfr_p975)"}, {"name": "logEZLVp025", "desc": "?=- EAZY 2.5% percentile of log V-band luminosity (ez_Lv_p025)"}, {"name": "logEZLVp160", "desc": "?=- EAZY 16.0% percentile of log V-band luminosity (ez_Lv_p160)"}, {"name": "logEZLVp500", "desc": "?=- EAZY 50.0% percentile of log V-band luminosity (ez_Lv_p500)"}, {"name": "logEZLVp840", "desc": "?=- EAZY 84.0% percentile of log V-band luminosity (ez_Lv_p840)"}, {"name": "logEZLVp975", "desc": "?=- EAZY 97.5% percentile of log V-band luminosity (ez_Lv_p975)"}, {"name": "EZLIRp025", "desc": "?=- EAZY 2.5% percentile of total 8-1000um luminosity (ez_LIR_p025)"}, {"name": "EZLIRp160", "desc": "?=- EAZY 16.0% percentile of total 8-1000um luminosity (ez_LIR_p160)"}, {"name": "EZLIRp500", "desc": "?=- EAZY 50.0% percentile of total 8-1000um luminosity (ez_LIR_p500)"}, {"name": "EZLIRp840", "desc": "?=- EAZY 84.0% percentile of total 8-1000um luminosity (ez_LIR_p840)"}, {"name": "EZLIRp975", "desc": "?=- EAZY 97.5% percentile of total 8-1000um luminosity (ez_LIR_p975)"}, {"name": "EZEnerAbsp025", "desc": "?=- EAZY 2.5% percentile of implied absorbed energy associated with Av (ez_energy_abs_p025)"}, {"name": "EZEnerAbsp160", "desc": "?=- EAZY 16.0% percentile of implied absorbed energy associated with Av (ez_energy_abs_p160)"}, {"name": "EZEnerAbsp500", "desc": "?=- EAZY 50.0% percentile of implied absorbed energy associated with Av (ez_energy_abs_p500)"}, {"name": "EZEnerAbsp840", "desc": "?=- EAZY 84.0% percentile of implied absorbed energy associated with Av (ez_energy_abs_p840)"}, {"name": "EZEnerAbsp975", "desc": "?=- EAZY 97.5% percentile of implied absorbed energy associated with Av (ez_energy_abs_p975)"}, {"name": "EZLUp025", "desc": "?=- EAZY 2.5% percentile of luminosity in rest-frame U band (ez_Lu_p025)"}, {"name": "EZLUp160", "desc": "?=- EAZY 16.0% percentile of luminosity in rest-frame U band (ez_Lu_p160)"}, {"name": "EZLUp500", "desc": "?=- EAZY 50.0% percentile of luminosity in rest-frame U band (ez_Lu_p500)"}, {"name": "EZLUp840", "desc": "?=- EAZY 84.0% percentile of luminosity in rest-frame U band (ez_Lu_p840)"}, {"name": "EZLUp975", "desc": "?=- EAZY 97.5% percentile of luminosity in rest-frame U band (ez_Lu_p975)"}, {"name": "EZLJp025", "desc": "?=- EAZY 2.5% percentile of luminosity in rest-frame J band (ez_Lj_p025)"}, {"name": "EZLJp160", "desc": "?=- EAZY 16.0% percentile of luminosity in rest-frame J band (ez_Lj_p160)"}, {"name": "EZLJp500", "desc": "?=- EAZY 50.0% percentile of luminosity in rest-frame J band (ez_Lj_p500)"}, {"name": "EZLJp840", "desc": "?=- EAZY 84.0% percentile of luminosity in rest-frame J band (ez_Lj_p840)"}, {"name": "EZLJp975", "desc": "?=- EAZY 97.5% percentile of luminosity in rest-frame J band (ez_Lj_p975)"}, {"name": "EZL1400p025", "desc": "?=- EAZY 2.5% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p025)"}, {"name": "EZL1400p160", "desc": "?=- EAZY 16.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p160)"}, {"name": "EZL1400p500", "desc": "?=- EAZY 50.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p500)"}, {"name": "EZL1400p840", "desc": "?=- EAZY 84.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p840)"}, {"name": "EZL1400p975", "desc": "?=- EAZY 97.5% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez_L1400_p975)"}, {"name": "EZL2800p025", "desc": "?=- EAZY 2.5% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p025)"}, {"name": "EZL2800p160", "desc": "?=- EAZY 16.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p160)"}, {"name": "EZL2800p500", "desc": "?=- EAZY 50.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p500)"}, {"name": "EZL2800p840", "desc": "?=- EAZY 84.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p840)"}, {"name": "EZL2800p975", "desc": "?=- EAZY 97.5% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez_L2800_p975)"}, {"name": "EZLHap025", "desc": "?=- EAZY 2.5% percentile of Halpha line luminosity (reddened) (ez_LHa_p025)"}, {"name": "EZLHap160", "desc": "?=- EAZY 16.0% percentile of Halpha line luminosity (reddened) (ez_LHa_p160)"}, {"name": "EZLHap500", "desc": "?=- EAZY 50.0% percentile of Halpha line luminosity (reddened) (ez_LHa_p500)"}, {"name": "EZLHap840", "desc": "?=- EAZY 84.0% percentile of Halpha line luminosity (reddened) (ez_LHa_p840)"}, {"name": "EZLHap975", "desc": "?=- EAZY 97.5% percentile of Halpha line luminosity (reddened) (ez_LHa_p975)"}, {"name": "EZLOIIIp025", "desc": "?=- EAZY 2.5% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p025)"}, {"name": "EZLOIIIp160", "desc": "?=- EAZY 16.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p160)"}, {"name": "EZLOIIIp500", "desc": "?=- EAZY 50.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p500)"}, {"name": "EZLOIIIp840", "desc": "?=- EAZY 84.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p840)"}, {"name": "EZLOIIIp975", "desc": "?=- EAZY 97.5% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez_LOIII_p975)"}, {"name": "EZLHbp025", "desc": "?=- EAZY 2.5% percentile of Hbeta line luminosity (reddened) (ez_LHb_p025)"}, {"name": "EZLHbp160", "desc": "?=- EAZY 16.0% percentile of Hbeta line luminosity (reddened) (ez_LHb_p160)"}, {"name": "EZLHbp500", "desc": "?=- EAZY 50.0% percentile of Hbeta line luminosity (reddened) (ez_LHb_p500)"}, {"name": "EZLHbp840", "desc": "?=- EAZY 84.0% percentile of Hbeta line luminosity (reddened) (ez_LHb_p840)"}, {"name": "EZLHbp975", "desc": "?=- EAZY 97.5% percentile of Hbeta line luminosity (reddened) (ez_LHb_p975)"}, {"name": "EZLOIIp025", "desc": "?=- EAZY 2.5% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p025)"}, {"name": "EZLOIIp160", "desc": "?=- EAZY 16.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p160)"}, {"name": "EZLOIIp500", "desc": "?=- EAZY 50.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p500)"}, {"name": "EZLOIIp840", "desc": "?=- EAZY 84.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p840)"}, {"name": "EZLOIIp975", "desc": "?=- EAZY 97.5% percentile of [OII] 3726+3729 line luminosity (reddened) (ez_LOII_p975)"}, {"name": "logEZsSFRp025", "desc": "?=- EAZY 2.5% percentile of log sSFR (ez_ssfr_p025)"}, {"name": "logEZsSFRp160", "desc": "?=- EAZY 16.0% percentile of log sSFR (ez_ssfr_p160)"}, {"name": "logEZsSFRp500", "desc": "?=- EAZY 50.0% percentile of log sSFR (ez_ssfr_p500)"}, {"name": "logEZsSFRp840", "desc": "?=- EAZY 84.0% percentile of log sSFR (ez_ssfr_p840)"}, {"name": "logEZsSFRp975", "desc": "?=- EAZY 97.5% percentile of log sSFR (ez_ssfr_p975)"}, {"name": "EZAVp025", "desc": "?=- EAZY 2.5% percentile of extinction in V band (ez_Av_p025)"}, {"name": "EZAVp160", "desc": "?=- EAZY 16.0% percentile of extinction in V band (ez_Av_p160)"}, {"name": "EZAVp500", "desc": "?=- EAZY 50.0% percentile of extinction in V band (ez_Av_p500)"}, {"name": "EZAVp840", "desc": "?=- EAZY 84.0% percentile of extinction in V band (ez_Av_p840)"}, {"name": "EZAVp975", "desc": "?=- EAZY 97.5% percentile of extinction in V band (ez_Av_p975)"}]}, {"name": "list.dat", "desc": "Fits image and catalogs ", "columns": [{"name": "RAdeg", "desc": "? Right Ascension of center (J2000) "}, {"name": "DEdeg", "desc": "? Declination of center (J2000) "}, {"name": "scale", "desc": "? Scale of the image "}, {"name": "Nx", "desc": "? Number of pixels along X-axis "}, {"name": "Ny", "desc": "? Number of pixels along Y-axis "}, {"name": "size", "desc": "? Size of FITS file "}, {"name": "FileName", "desc": "Name of FITS file, in subdirectory fits "}, {"name": "Title", "desc": "Title of the FITS file "}]}, {"name": "fits/*", "desc": "CHI-MEAN detection image used to prepare COSMOS2020 and original fits catalogs", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_259_18"}} {"id": "J/ApJS/259/18", "title_cds": "SHELLQs. XVI. New quasars at 5.8"], "bibcode": ["2022ApJS..259...18M"], "see_also": ["J/ApJ/633/630 : Low-mass stars found in CFHTLS (Willott+, 2005)", "J/MNRAS/435/3306 : Candidate type II QSOs in SDSS III (Alexandroff+, 2013)", "J/ApJS/227/11 : PS1 z>5.6 quasars follow-up (Banados+, 2016)", "J/PASJ/70/S10 : GOLDRUSH I. UV magnitudes (Ono+, 2018)", "J/MNRAS/477/2817 : Luminous Ly{alpha} emitters at z~2-3 (Sobral+, 2018)", "J/A+A/643/A149 : J-PLUS Ly{alpha}-emitting candidates (Spinoso+, 2020)"], "keyword_cds": "QSOs; Redshifts; Photometry, ugriz; Spectra, optical; Equivalent widths; Stars, brown dwarf; Spectral types", "keyword_pub": "Reionization; Quasars; Supermassive black holes; High-redshift galaxies", "abstract": ["We present the spectroscopic discovery of 69 quasars at 5.80.1", "in the HSC-SSP third public data release (PDR3). The sample reported", "here also includes three quasars with P_Q_^B^<0.1 at z~6.6, which we", "selected in an effort to completely cover the reddest point sources", "with simple color cuts. The number of high-z quasars discovered in", "SHELLQs has now grown to 162, including 23 type II quasar candidates.", "This paper also presents identification of seven galaxies at", "5.65.6. This demonstrates that the", "algorithm has very high efficiency, even though we are probing an", "unprecedentedly low luminosity population down to M_1450_~-21mag."], "description": ["The Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP) candidates", "were fed into follow-up spectroscopy programs at the 8.2m Subaru", "Telescope and the 10.4m Gran Telescopio Canarias (GTC).", "We use the Faint Object Camera and Spectrograph (FOCAS) on Subaru to", "observe the wavelength range 0.75-1.0um with the VPH900 grism and 1.0\"", "slits, giving a spectral resolution of R~1200 (Program ID: S18B-011I).", "Similarly, the Optical System for Imaging and", "low-intermediate-Resolution Integrated Spectroscopy (OSIRIS) on GTC is", "used with the R2500I grism and 1.0\" long slit, yielding spectra over", "0.75-1.0um with R~1500 (Program IDs: GTC5-20A, GTC10-20B, GTC42-21B)."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Journal of discovery spectroscopy ", "columns": [{"name": "Class", "desc": "Object type (1) "}, {"name": "Name", "desc": "Object name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "l_imag", "desc": "5{sigma} upper limit flag on imag "}, {"name": "imag", "desc": "[23.41/27.71]? Subaru/HSC i-band AB magnitude (2) "}, {"name": "e_imag", "desc": "[0.02/0.9]? Uncertainty on the imag "}, {"name": "l_zmag", "desc": "5{sigma} upper limit flag on zmag "}, {"name": "zmag", "desc": "[20.91/26] Subaru/HSC z-band AB magnitude (2) "}, {"name": "e_zmag", "desc": "[0.01/0.7]? Uncertainty on the zmag "}, {"name": "ymag", "desc": "[20.65/25.79] Subaru/HSC y band AB magnitude (2) "}, {"name": "e_ymag", "desc": "[0.01/0.7] Uncertainty on the ymag "}, {"name": "Prob", "desc": "[0/1] Bayesian quasar probability, P_Q_^B^ "}, {"name": "Exp", "desc": "[5/120] Total exposure time for the object "}, {"name": "Date", "desc": "Date of observation (UT) "}, {"name": "Date2", "desc": "Other date(s) of observation (UT) "}, {"name": "Inst", "desc": "Instrument (F=Subaru/FOCAS or O=GTC/OSIRIS) "}]}, {"name": "table2.dat", "desc": "Objects detected in the near-IR bands ", "columns": [{"name": "Class", "desc": "Object type (QSOs or cool dwarfs) "}, {"name": "Name", "desc": "Object name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "Jmag", "desc": "[20.4/22.36]? J-band AB magnitude "}, {"name": "e_Jmag", "desc": "[0.07/0.35]? Uncertainty on the Jmag "}, {"name": "Hmag", "desc": "[19.27/21.64]? H-band AB magnitude "}, {"name": "e_Hmag", "desc": "[0.04/0.28]? Uncertainty on the Hmag "}, {"name": "Kmag", "desc": "[18.72/21.92]? K band AB magnitude "}, {"name": "e_Kmag", "desc": "[0.03/0.43]? Uncertainty on the Kmag "}, {"name": "Cam", "desc": "Camera (1) "}]}, {"name": "table3.dat", "desc": "Spectroscopic properties ", "columns": [{"name": "Class", "desc": "Object type (QSOs, Gal or OIII emitter) "}, {"name": "Name", "desc": "Object name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "z", "desc": "[0.95/6.94] Spectroscopic redshift (1) "}, {"name": "1450Mag", "desc": "[-25.95/-21.53] Absolute magnitude at 1450{AA} "}, {"name": "e_1450Mag", "desc": "[0.02/0.8] 1450Mag uncertainty "}, {"name": "Line", "desc": "Emission line "}, {"name": "l_EW", "desc": "3{sigma} upper limit flag on EW (2) "}, {"name": "EW", "desc": "[4/696]? Rest-frame equivalent width; in Angstrom units"}, {"name": "e_EW", "desc": "[1/240]? EW uncertainty "}, {"name": "l_FWHM", "desc": "3{sigma} upper limit flag on FWHM (2) "}, {"name": "FWHM", "desc": "[220/16000]? Line Full Width at Half Maximum "}, {"name": "e_FWHM", "desc": "[20/7700]? FWHM uncertainty "}, {"name": "logLline", "desc": "[40.87/45.17]? log of line luminosity in erg/s "}, {"name": "e_logLline", "desc": "[0.01/0.08]? logLline uncertainty "}]}, {"name": "table4.dat", "desc": "*Spectral classes of the Galactic dwarfs ", "columns": [{"name": "Name", "desc": "Object name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "SpT", "desc": "Approximate spectral type "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_260_1"}} {"id": "J/ApJS/260/1", "title_cds": "The Low-redshift Lyman Continuum Survey (LzLCS). I.", "title_create": "Flury+, 2022", "year": "2022", "author": "Flury S.R., Jaskot A.E., Ferguson H.C., Worseck G., Makan K., Chisholm J., Saldana-Lopez A., Schaerer D., McCandliss S., Wang B., Ford N.M., Heckman T., Ji Z., Giavalisco M., Amorin R., Atek H., Blaizot J., Borthakur S., Carr C., Castellano M., Cristiani S., De Barros S., Dickinson M., Finkelstein S.L., Fleming B., Fontanot F., Garel T., Grazian A., Hayes M., Henry A., Mauerhofer V., Micheva G., Oey M.S., Ostlin G., Papovich C., Pentericci L., Ravindranath S., Rosdahl J., Rutkowski M., Santini P., Scarlata C., Teplitz H., Thuan T., Trebitsch M., Vanzella E., Verhamme A., Xu X.", "title_pub": "The Low-redshift Lyman Continuum Survey. I. New, diverse local Lyman continuum emitters.", "first_author": "Flury S.R.", "ref_biblio": [""], "bibcode": ["2022ApJS..260....1F"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "VI/64 : Recombination line intensities for hydrogenic ions (Storey+ 1995)", "V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)", "VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)", "J/ApJ/803/34 : z~4-10 galaxies from HST legacy fields (Bouwens+, 2015)", "J/ApJ/810/71 : UV mag of cand. galaxies at 3~"], "bibcode": ["2022ApJS..261....4O"], "see_also": ["VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009)", "V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)", "J/ApJS/121/473 : A diagnostic diagram for Seyfert 2 Galaxies (Bassani+, 1999)", "J/A+A/378/30 : ROSAT-BSC galaxy identifications (Zimmermann+, 2001)", "J/ApJ/633/L77 : SWIFT/BAT detections of AGN (Markwardt+, 2005)", "J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)", "J/ApJ/681/113 : Swift BAT survey of AGNs (Tueller+, 2008)", "J/MNRAS/398/1165 : AGN in nearby galaxies (Goulding+, 2009)", "J/A+A/495/691 : Multifreq. catalogue of blazars, Roma-BZCAT (Massaro+, 2009)", "J/ApJ/705/L76 : AGNs with double-peaked [OIII] lines (Wang+, 2009)", "J/ApJ/708/427 : Type 2 AGNs with double-peaked [OIII] lines (Liu+, 2010)", "J/ApJS/186/378 : Hard X-ray survey from Swift-BAT 2004-2006 (Tueller+, 2010)", "J/MNRAS/421/1043 : Emission-line galaxies from SDSS DR7 (Shirazi+, 2012)", "J/ApJS/207/19 : Hard X-ray survey from Swift-BAT (Baumgartner+, 2013)", "J/A+A/565/A117 : X-Shooter Spectral Library (XSL). DR1 (Chen+, 2014)", "J/A+A/561/A67 : Spectra of 75 Swift/BAT optical counterparts (Parisi, 2014)", "J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)", "J/ApJS/219/1 : Catalog of Type-1 AGNs from SDSS-DR7 (Oh+, 2015)", "J/ApJ/815/L13 : AGNs from the 70-month Swift/BAT cat. (Ricci+, 2015)", "J/ApJ/815/129 : X-ray AGNs with Subaru/FMOS NIR observations (Suh+, 2015)", "J/A+A/588/A103 : 2nd ROSAT all-sky survey (2RXS) source cat. (Boller+, 2016)", "J/MNRAS/463/24 : AGNs with double-peaked narrow emission lines (Lyu+, 2016)", "J/ApJ/850/74 : Swift/BAT AGN Spectroscopic Survey. I. (Koss+, 2017)", "J/ApJ/836/99 : NuSTAR serendipitous survey: 40-month cat. (Lansbury+, 2017)", "J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray (Ricci+, 2017)", "J/ApJS/235/4 : 105-month Swift-BAT all-sky hard X-ray survey (Oh+, 2018)", "J/ApJ/881/154 : BAT AGN spectroscopic survey. XVI. Blazars (Paliya+, 2019)", "J/ApJS/261/2 : BASS. XXII. Swift/BAT AGN Sp. Survey DR2 cat. (Koss+, 2022)", "http://swift.gsfc.nasa.gov/results/bs70mon/ : Swift-BAT 70-months", "http://www.bass-survey.com/ : The BAT AGN Spectroscopic Survey home page"], "keyword_cds": "Active gal. nuclei; Spectra, optical; Galaxies, Seyfert; QSOs", "keyword_pub": "Supermassive black holes ; Active galactic nuclei ; X-ray active galactic nuclei ; AGN host galaxies ; Quasars", "abstract": ["We present the second catalog and data release of optical spectral", "line measurements and active galactic nucleus (AGN) demographics of", "the BAT AGN Spectroscopic Survey, which focuses on the Swift-BAT hard", "X-ray detected AGNs. We use spectra from dedicated campaigns and", "publicly available archives to investigate spectral properties of most", "of the AGNs listed in the 70 month Swift-BAT all-sky catalog;", "specifically, 743 of the 746 unbeamed and unlensed AGNs (99.6%). We", "find a good correspondence between the optical emission line widths", "and the hydrogen column density distributions using the X-ray spectra,", "with a clear dichotomy of AGN types for N_H_=10^22^cm^-2^. Based on", "optical emission-line diagnostics, we show that 48%-75% of BAT AGNs", "are classified as Seyfert, depending on the choice of emission lines", "used in the diagnostics. The fraction of objects with upper limits on", "line emission varies from 6% to 20%. Roughly 4% of the BAT AGNs have", "lines too weak to be placed on the most commonly used diagnostic", "diagram, [OIII]{lambda}5007/H{beta} versus [NII]{lambda}6584/H{alpha},", "despite the high signal-to-noise ratio of their spectra. This value", "increases to 35% in the [OIII]{lambda}5007/[OII]{lambda}3727 diagram,", "owing to difficulties in line detection. Compared to optically", "selected narrow-line AGNs in the Sloan Digital Sky Survey, the BAT", "narrow-line AGNs have a higher rate of reddening/extinction, with", "H{alpha}/H{beta}>5 (~36%), indicating that hard X-ray selection more", "effectively detects obscured AGNs from the underlying AGN population.", "Finally, we present a subpopulation of AGNs that feature complex broad", "lines (34%, 250/743) or double-peaked narrow emission lines (2%,", "17/743)."], "description": ["Following BASS DR1 (Paper I.; Koss+ 2017, J/ApJ/850/74), we limit our", "sample of interest to nonbeamed and nonlensed AGNs by crossmatching", "the 858 BAT AGNs from BASS DR2 (Papers XXI & XXII;", "Koss+ 2022ApJS..261....1K and J/ApJS/262/2) with the Roma Blazar", "Catalog (BZCAT; Massaro+ 2009, J/A+A/495/691) and the follow-up work", "by Paliya+ (2019, J/ApJ/881/154).", "In this study, we present 743 optical spectra from the DR2 cat. (see", "Koss+ 2022, J/ApJS/262/2).", "The largest number of optical spectra was obtained from the", "spectroscopic programs using the Palomar Double Spectrograph (DBSP),", "which is attached to the Hale 200 inch telescope (N=271, 36.4% of our", "AGNs). These spectra were obtained as part of a dedicated Yale program", "on BAT AGN (led by C. M. Urry and M. Powell) or from observations of", "NuSTAR programs (led by F. Harrison and D. Stern). Most of the", "observations were performed between 2012 October and 2020 November.", "Another large portion of the spectra (N=169, 22.7%) was obtained", "using the X-Shooter spectrograph, mounted on the European Southern", "Observatory's Very Large Telescope (ESO-VLT). The service-mode", "X-Shooter observations took place between 2016 December and 2019", "October, under the ESO run IDs 98.A-0635, 99.A-0403, 100.B-0672,", "101.A-0765, 102.A-0433, 103.A-0521, and 104.A-0353 (led by K. Oh and", "B. Trakhtenbrot). We also included available archival X-shooter spectra.", "We also utilized observations (led by C. Ricci) with the Boller and", "Chivens (B and C) spectrograph mounted on the 2.5m Irenee du Pont", "telescope at the Las Campanas Observatory for 41 sources in 2016 March", "and September.", "Additionally, we used observations from the Goodman spectrograph", "on the Southern Astrophysical Research (SOAR) telescope for 32 sources", "between 2017 and 2020 (led by C. Ricci).", "Finally, five spectra were obtained with the low-resolution imaging", "spectrometer (LRIS) on the Keck telescope (led by D. Stern and", "F. Harrison).", "The largest number of archival optical spectra (118 sources, 15.9%;", "see Figure 1) is from SDSS Data Release 15 (Aguado+ 2019ApJS..240...23A).", "The second largest portion of the spectra (N=36, 4.8%) is drawn from", "the 6dF Galaxy Survey (6dFGS; Jones et al. 2009, VII/259)."], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/ac5b68"], "orcid_pub": ["0000-0002-5037-951X"], "data": "f-v", "date_creation": "03-Oct-2022", "xmatch": "J/ApJS/261/4/lines", "last_update": "04-Oct-2022", "catid": "22610004", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Optical spectra ", "columns": [{"name": "ID", "desc": "[1/1210] Swift-BAT 70-month hard X-ray survey identification number (G1)"}, {"name": "m_ID", "desc": "[AB] Component ID on BAT number "}, {"name": "---", "desc": "[SWIFT] "}, {"name": "SWIFT", "desc": "Swift/BAT position-based identifier (JHHMM.m+DDMMA)"}, {"name": "CName", "desc": "Counterpart source name "}, {"name": "RAdeg", "desc": "Right Ascension (J2000) (1) "}, {"name": "DEdeg", "desc": "[-86.64/86] Declination (J2000) (1) "}, {"name": "Tel", "desc": "Source of optical spectrum "}, {"name": "z[OIII]", "desc": "[-0.0001/0.6] Input redshift used from [OIII]{lambda}5007 (2)"}, {"name": "Date", "desc": "Date taken optical spectra "}, {"name": "Exp", "desc": "Exposure time (3) "}, {"name": "Type", "desc": "? AGN classification (4) "}]}, {"name": "table4.dat", "desc": "Emission line classification ", "columns": [{"name": "ID", "desc": "[1/1210] Swift-BAT 70-month hard X-ray survey identification number (G1)"}, {"name": "m_ID", "desc": "[AB] Component ID on BAT number "}, {"name": "CName", "desc": "Counterpart source name "}, {"name": "[NII]/Ha", "desc": "The [NII]{lambda}6584/H{alpha} diagnostic classification (5)"}, {"name": "[SII]/Ha", "desc": "The [SII]{lambda}6717, {lambda}6731/H{alpha} diagnostic classification (5)"}, {"name": "[OI]/Ha", "desc": "The [OI]{lambda}6300/H{alpha} diagnostic classification (5)"}, {"name": "HeII", "desc": "The HeII{lambda}4686 diagnostic classification (5)"}, {"name": "[OIII]/[OII]", "desc": "The [OIII]{lambda}5007/[OII]{lambda}3727 diagnostic classification (5)"}]}, {"name": "table5.dat", "desc": "Double-peaked narrow emission-line BAT AGNs ", "columns": [{"name": "ID", "desc": "[37/1186] Swift-BAT 70-month hard X-ray survey ID (G1)"}, {"name": "dV", "desc": "[114/347] Average velocity offset (1)"}, {"name": "lambda-Hb-b", "desc": "[-6/0]? Emission line center, H{beta}, Angstroms, blue component"}, {"name": "lambda-Hb-r", "desc": "[-0.6/5]? Emission line center, H{beta}, Angstroms, red component"}, {"name": "l_Flux-Hb-b", "desc": "Limit flag on Flux-Hb-b "}, {"name": "Flux-Hb-b", "desc": "[19/1126]? Emission line flux, H{beta, rblueed component}, 10-17 erg/s/cm2"}, {"name": "e_Flux-Hb-b", "desc": "[3/34]? Uncertainty in Flux-Hb-b "}, {"name": "l_Flux-Hb-r", "desc": "Limit flag on Flux-Hb-r "}, {"name": "Flux-Hb-r", "desc": "[19/858]? Emission line flux, H{beta}, red component, 10-17 erg/s/cm2"}, {"name": "e_Flux-Hb-r", "desc": "[4/36]? Uncertainty in Flux-Hb-r "}, {"name": "lambda-OIII-b", "desc": "[-6/0.5]? Emission line center, H{beta}, Angstroms, blue component"}, {"name": "lambda-OIII-r", "desc": "[-0.6/3.8]? Emission line center, H{beta}, Angstroms, red component"}, {"name": "Flux-OIII-b", "desc": "[169/6922]? Emission line flux, [OIII], blue component, 10-17 erg/s/cm2"}, {"name": "e_Flux-OIII-b", "desc": "[9/241]? Uncertainty in Flux-OIII-b "}, {"name": "Flux-OIII-r", "desc": "[208/3319]? Emission line flux, [OIII], red component, 10-17 erg/s/cm2"}, {"name": "e_Flux-OIII-r", "desc": "[6/189]? Uncertainty in Flux-OIII-r "}, {"name": "FWHM-F", "desc": "[30/246]? FWHM, forbidden lines, [N II]{lambda}6584"}, {"name": "lambda-Ha-b", "desc": "[-7/1.5]? Emission line center, H{alpha}, Angstroms, blue component"}, {"name": "lambda-Ha-r", "desc": "[-0.6/5.5]? Emission line center, H{alpha}, Angstroms, red component"}, {"name": "Flux-Ha-b", "desc": "[50/5828]? Emission line flux, H{alpha}, blue component, 10-17 erg/s/cm2"}, {"name": "e_Flux-Ha-b", "desc": "[11/98]? Uncertainty in Flux-Ha-b "}, {"name": "Flux-Ha-r", "desc": "[85/7194]? Emission line flux, H{alpha}, red component, 10-17 erg/s/cm2"}, {"name": "e_Flux-Ha-r", "desc": "[12/283]? Uncertainty in Flux-Ha-r "}, {"name": "lambda-NII-b", "desc": "[-7/1.7]? Emission line center, [NII], Angstroms, blue component"}, {"name": "lambda-NII-r", "desc": "[-0.6/5]? Emission line center, [NII], Angstroms, red component"}, {"name": "Flux-NII-b", "desc": "[63/4979]? Emission line flux, [NII], blue component, 10-17 erg/s/cm2"}, {"name": "e_Flux-NII-b", "desc": "[8/126]? Uncertainty in Flux-NII-b "}, {"name": "Flux-NII-r", "desc": "[65/3752]? Emission line flux, [NII], red component, 10-17 erg/s/cm2"}, {"name": "e_Flux-NII-r", "desc": "[8/111]? Uncertainty in Flux-NII-r "}, {"name": "FWHM-B", "desc": "[37/282]? FWHM, Balmer lines measured from H{alpha}"}]}, {"name": "table6.dat", "desc": "Wing components ", "columns": [{"name": "ID", "desc": "[1/1203] Swift-BAT 70-month hard X-ray survey identification number (G1)"}, {"name": "m_ID", "desc": "[AB] Component ID on BAT number "}, {"name": "lambda-Hb", "desc": "[4855.4/4874.7]? Emission line center, H{beta} Angstroms"}, {"name": "FWHM-Hb", "desc": "[94/864]? Full width at half max, km/s, H{beta}"}, {"name": "l_Flux-Hb", "desc": "Limit flag on Flux-Hb "}, {"name": "Flux-Hb", "desc": "[43.1/45604.1]? Emission line flux, H{beta}, 10-17 erg/s/cm2"}, {"name": "e_Flux-Hb", "desc": "[0.2/50.2]? Uncertainty in Flux-Hb "}, {"name": "lambda-OIII", "desc": "[4994.7/5021.8]? Emission line center, [OIII] Angstroms"}, {"name": "FWHM-OIII", "desc": "[94/1696]? Full width at half max, km/s, [OIII]"}, {"name": "l_Flux-OIII", "desc": "Limit flag on Flux-OIII "}, {"name": "Flux-OIII", "desc": "[31.9/438096]? Emission line flux, [OIII], 10-17 erg/s/cm2"}, {"name": "e_Flux-OIII", "desc": "[0/736]? Uncertainty in Flux-OIII "}, {"name": "lambda-Ha", "desc": "[6556.3/6573.7]? Emission line center, H{alpha} Angstroms"}, {"name": "FWHM-Ha", "desc": "[94/1177]? Full width at half max, km/s, H{alpha}"}, {"name": "Flux-Ha", "desc": "[210/125945]? Emission line flux, H{alpha}, 10-17 erg/s/cm2"}, {"name": "e_Flux-Ha", "desc": "[0.4/224]? Uncertainty in Flux-Ha "}, {"name": "lambda-NII", "desc": "[6576.8/6591.3]? Emission line center, [NII] Angstroms"}, {"name": "FWHM-NII", "desc": "[117/851]? Full width at half max, km/s, [NII]"}, {"name": "l_Flux-NII", "desc": "Limit flag on Flux-NII "}, {"name": "Flux-NII", "desc": "[39.5/87686]? Emission line flux, [NII], 10-17 erg/s/cm2"}, {"name": "e_Flux-NII", "desc": "[0.2/244]? Uncertainty in Flux-NII "}]}, {"name": "table7.dat", "desc": "Emission-line Measurements from HeII{lambda}3203 to H{gamma}{lambda}4340", "columns": [{"name": "ID", "desc": "[1/1210] Swift-BAT 70-month hard X-ray survey identification number (G1)"}, {"name": "m_ID", "desc": "[AB] Component on sequential number "}, {"name": "l_FHeII3203", "desc": "Limit flag for FHeII3203, 3{sigma} upper limit (G2)"}, {"name": "FHeII3203", "desc": "[12.6/7168]? Emission line flux, HeII{lambda}3203 (G2)"}, {"name": "e_FHeII3203", "desc": "[0/32]? Uncertainty for FHeII3203 (G2) "}, {"name": "l_FNeV3345", "desc": "Limit flag for FNeV3345, 3{sigma} upper limit (G2)"}, {"name": "FNeV3345", "desc": "[10.6/8794]? Emission line flux, [NeV]{lambda}3345 (G2)"}, {"name": "e_FNeV3345", "desc": "[0/70]? Uncertainty for FNeV3345 (G2) "}, {"name": "l_FNeV3425", "desc": "Limit flag for FNeV3425, 3{sigma} upper limit (G2)"}, {"name": "FNeV3425", "desc": "[26/30623]? Emission line flux, [NeV]{lambda}3425 (G2)"}, {"name": "e_FNeV3425", "desc": "[0/590]? Uncertainty for FNeV3425 (G2) "}, {"name": "l_FOII3727", "desc": "Limit flag for FOII3727, 3{sigma} upper limit (G2)"}, {"name": "FOII3727", "desc": "[33/101595]? Emission line flux, [OII]{lambda}3727 (G2)"}, {"name": "e_FOII3727", "desc": "[0/6636]? Uncertainty for FOII3727 (G2) "}, {"name": "l_FNeIII3868", "desc": "Limit flag for FNeIII3868, 3{sigma} upper limit (G2)"}, {"name": "FNeIII3868", "desc": "[19.6/104594]? Emission line flux, [NeIII]{lambda}3868 (G2)"}, {"name": "e_FNeIII3868", "desc": "[0/2017]? Uncertainty for FNeIII3868 (G2)"}, {"name": "l_FNeIII3967", "desc": "Limit flag for FNeIII3967, 3{sigma} upper limit (G2)"}, {"name": "FNeIII3967", "desc": "[7.5/32397]? Emission line flux, [NeIII]{lambda}3967 (G2)"}, {"name": "e_FNeIII3967", "desc": "[0/2242]? Uncertainty for FNeIII3967 (G2)"}, {"name": "l_FHz", "desc": "Limit flag for FHz, 3{sigma} upper limit (G2)"}, {"name": "FHz", "desc": "[3.9/18723]? Emission line flux, H{zeta}{lambda}3889 (G2)"}, {"name": "e_FHz", "desc": "[0/13]? Uncertainty for FHz (G2) "}, {"name": "l_FHeps", "desc": "Limit flag for FHeps, 3{sigma} upper limit (G2)"}, {"name": "FHeps", "desc": "[6.5/21609]? Emission line flux, H{epsilon}{lambda}3970 (G2)"}, {"name": "e_FHeps", "desc": "[0/19]? Uncertainty for FHeps (G2) "}, {"name": "l_FHd", "desc": "Limit flag for FHd, 3{sigma} upper limit (G2)"}, {"name": "FHd", "desc": "[5.6/19747]? Emission line flux, H{delta}{lambda}4101 (G2)"}, {"name": "e_FHd", "desc": "[0/31]? Uncertainty for FHd (G2) "}, {"name": "l_FHg", "desc": "Limit flag for FHg, 3{sigma} upper limit (G2)"}, {"name": "FHg", "desc": "[4/147007]? Emission line flux, H{gamma}{lambda}4340 (G2)"}, {"name": "e_FHg", "desc": "[0/1375]? Uncertainty for FHg (G2) "}, {"name": "FWHM-N2", "desc": "[22/4968]? FWHM, forbidden lines, [NII]{lambda}6584 (G2)"}, {"name": "e_FWHM-N2", "desc": "[0/42]? Uncertainty in FWHM-N2 (G2) "}, {"name": "Flag7", "desc": "Flag for emission line measurements from HeII{lambda}3203 to"}]}, {"name": "table8.dat", "desc": "Emission-line Measurements - from [OIII]{lambda}4363 to HeI{lambda}5875", "columns": [{"name": "ID", "desc": "[1/1210] Swift-BAT 70-month hard X-ray survey ID (G1)"}, {"name": "m_ID", "desc": "[AB] Component on sequential number "}, {"name": "l_FOIII4363", "desc": "Limit flag for FOIII4363, 3{sigma} upper limit (G2)"}, {"name": "FOIII4363", "desc": "[0/187391]? Emission line flux, [OIII]{lambda}4363 (G2)"}, {"name": "e_FOIII4363", "desc": "[0/287]? Uncertainty for FOIII4363 (G2) "}, {"name": "l_FHeII4685", "desc": "Limit flag for FHeII4685, 3{sigma} upper limit (G2)"}, {"name": "FHeII4685", "desc": "[9.6/436892]? Emission line flux, HeII{lambda}4685 (G2)"}, {"name": "e_FHeII4685", "desc": "[0/1082]? Uncertainty for FHeII4685 (G2) "}, {"name": "l_FArIV4711", "desc": "Limit flag for FArIV4711, 3{sigma} upper limit (G2)"}, {"name": "FArIV4711", "desc": "[5.3/202343]? Emission line flux, [ArIV]{lambda}4711 (G2)"}, {"name": "e_FArIV4711", "desc": "[0/605]? Uncertainty for FArIV4711 (G2) "}, {"name": "l_FArIV4740", "desc": "Limit flag for FArIV4740, 3{sigma} upper limit (G2)"}, {"name": "FArIV4740", "desc": "[6.3/39998]? Emission line flux, [ArIV]{lambda}4740 (G2)"}, {"name": "e_FArIV4740", "desc": "[0/561]? Uncertainty for FArIV4740 (G2) "}, {"name": "l_FHb", "desc": "Limit flag for FHb, 3{sigma} upper limit (G2)"}, {"name": "FHb", "desc": "[7/980571]? Emission line flux, H{beta}{lambda}4861 (G2)"}, {"name": "e_FHb", "desc": "[0/2933]? Uncertainty for FHb (G2) "}, {"name": "l_FOIII4958", "desc": "Limit flag for FOIII4958, 3{sigma} upper limit (G2)"}, {"name": "FOIII4958", "desc": "[15.8/1401943]? Emission line flux, [OIII]{lambda}4958 (G2)"}, {"name": "e_FOIII4958", "desc": "[0/5497]? Uncertainty for FOIII4958 (G2) "}, {"name": "l_FOIII5007", "desc": "Limit flag for FOIII5007, 3{sigma} upper limit (G2)"}, {"name": "FOIII5007", "desc": "[27.7/4005550]? Emission line flux, [OIII]{lambda}5007 (G2)"}, {"name": "e_FOIII5007", "desc": "[0/15704]? Uncertainty for FOIII5007 (G2)"}, {"name": "l_FNI5197", "desc": "Limit flag for FNI5197, 3{sigma} upper limit (G2)"}, {"name": "FNI5197", "desc": "[5.8/223242]? Emission line flux, [NI]{lambda}5197 (G2)"}, {"name": "e_FNI5197", "desc": "[0/487]? Uncertainty for FNI5197 (G2) "}, {"name": "l_FNI5200", "desc": "Limit flag for FNI5200, 3{sigma} upper limit (G2)"}, {"name": "FNI5200", "desc": "[6.6/12041]? Emission line flux, [NI{lambda}5200 (G2)"}, {"name": "e_FNI5200", "desc": "[0/20929]? Uncertainty for FNI5200 (G2) "}, {"name": "l_FHeI5875", "desc": "Limit flag for FHeI5875, 3{sigma} upper limit (G2)"}, {"name": "FHeI5875", "desc": "[11.6/146759]? Emission line flux, HeI{lambda}5875 (G2)"}, {"name": "e_FHeI5875", "desc": "[0/59423]? Uncertainty for FHeI5875 (G2) "}, {"name": "FWHMHa", "desc": "[16/1292]? FWHM, Balmer lines measured from H{alpha} (G2)"}, {"name": "e_FWHMHa", "desc": "[0/35]? Uncertainty in FWHMHa (G2) "}, {"name": "Flag8", "desc": "Flag for emission line measurements from [OIII]{lambda}4363 to"}]}, {"name": "table9.dat", "desc": "Emission-line Measurements - from [OI]{lambda}6300 to [OII]{lambda}7330", "columns": [{"name": "ID", "desc": "[1/1210] Swift-BAT 70-month hard X-ray survey ID (G1)"}, {"name": "m_ID", "desc": "[AB] Component on sequential number "}, {"name": "l_FOI6300", "desc": "Limit flag for FOI6300, 3{sigma} upper limit (G2)"}, {"name": "FOI6300", "desc": "[13.8/57614]? Emission line flux, [OI]{lambda}6300 (G2)"}, {"name": "e_FOI6300", "desc": "[0/1926]? Uncertainty for FOI6300 (G2) "}, {"name": "l_FOI6363", "desc": "Limit flag for FOI6363, 3{sigma} upper limit (G2)"}, {"name": "FOI6363", "desc": "[4.7/21523]? Emission line flux, [OI]{lambda}6363 (G2)"}, {"name": "e_FOI6363", "desc": "[0/642]? Uncertainty for FOI6363 (G2) "}, {"name": "l_FNII654", "desc": "Limit flag for FNII654, 3{sigma} upper limit (G2)"}, {"name": "FNII654", "desc": "[17.5/197348]? Emission line flux, [NII]{lambda}6548 (G2)"}, {"name": "e_FNII654", "desc": "[0/1797]? Uncertainty for FNII654 (G2) "}, {"name": "l_FHa", "desc": "Limit flag for FHa, 3{sigma} upper limit (G2)"}, {"name": "FHa", "desc": "[14.4/2801632]? Emission line flux, H{alpha}{lambda}6562 (G2)"}, {"name": "e_FHa", "desc": "[0/8380]? Uncertainty for FHa (G2) "}, {"name": "l_FNII6583", "desc": "Limit flag for FNII6583, 3{sigma} upper limit (G2)"}, {"name": "FNII6583", "desc": "[29.4/414516]? Emission line flux, [NII]{lambda}6583 (G2)"}, {"name": "e_FNII6583", "desc": "[0/5283]? Uncertainty for FNII6583 (G2) "}, {"name": "l_FSII6716", "desc": "Limit flag for FSII6716, 3{sigma} upper limit (G2)"}, {"name": "FSII6716", "desc": "[19.5/92443]? Emission line flux, [SII]{lambda}6716 (G2)"}, {"name": "e_FSII6716", "desc": "[0/983]? Uncertainty for FSII6716 (G2) "}, {"name": "l_FSII6730", "desc": "Limit flag for FSII6730, 3{sigma} upper limit (G2)"}, {"name": "FSII6730", "desc": "[20.6/94253]? Emission line flux, [SII]{lambda}6730 (G2)"}, {"name": "e_FSII6730", "desc": "[0/1328]? Uncertainty for FSII6730 (G2) "}, {"name": "l_FArIII7135", "desc": "Limit flag for FArIII7135, 3{sigma} upper limit (G2)"}, {"name": "FArIII7135", "desc": "[4.4/20080]? Emission line flux, [ArIII]{lambda}7135 (G2)"}, {"name": "e_FArIII7135", "desc": "[0/616]? Uncertainty for FArIII7135 (G2)"}, {"name": "l_FOII7310", "desc": "Limit flag for FOII7310, 3{sigma} upper limit (G2)"}, {"name": "FOII7310", "desc": "[6/13775]? Emission line flux, [OII]{lambda}7310 (G2)"}, {"name": "e_FOII7310", "desc": "[0/31]? Uncertainty for FOII7310 (G2) "}, {"name": "l_FOII7330", "desc": "Limit flag for FOII7330, 3{sigma} upper limit (G2)"}, {"name": "FOII7330", "desc": "[6/11969]? Emission line flux, [OII]{lambda}7330 (G2)"}, {"name": "e_FOII7330", "desc": "[0/21]? Uncertainty for FOII7330 (G2) "}, {"name": "Flag9", "desc": "Flag for emission line measurements from [OI]{lambda}6300"}]}, {"name": "table10.dat", "desc": "Emission-line Measurements - from [SXII]{lambda}7611 to Pa13{lambda}8665", "columns": [{"name": "ID", "desc": "[1/1210] Swift-BAT 70-month hard X-ray survey ID (G1)"}, {"name": "m_ID", "desc": "[AB] Component on sequential number "}, {"name": "l_FSXII7611", "desc": "Limit flag for FSXII7611, 3{sigma} upper limit (G2)"}, {"name": "FSXII7611", "desc": "[8.7/340]? Emission line flux, [SXII]{lambda}7611 (G2)"}, {"name": "e_FSXII7611", "desc": "[0.1/5]? Uncertainty for FSXII7611 (G2) "}, {"name": "l_FArIII7751", "desc": "Limit flag for FArIII7751, 3{sigma} upper limit (G2)"}, {"name": "FArIII7751", "desc": "[4.6/9294]? Emission line flux, [ArIII]{lambda}7751 (G2)"}, {"name": "e_FArIII7751", "desc": "[0/15]? Uncertainty for FArIII7751 (G2) "}, {"name": "l_FHeI7816", "desc": "Limit flag for FHeI7816, 3{sigma} upper limit (G2)"}, {"name": "FHeI7816", "desc": "[6.8/410]? Emission line flux, HeI{lambda}7816 (G2)"}, {"name": "e_FHeI7816", "desc": "[0.1/18]? Uncertainty for FHeI7816 (G2) "}, {"name": "l_FArI7868", "desc": "Limit flag for FArI7868, 3{sigma} upper limit (G2)"}, {"name": "FArI7868", "desc": "[6.4/891]? Emission line flux, [ArI]{lambda}7868 (G2)"}, {"name": "e_FArI7868", "desc": "[0.1/24]? Uncertainty for FArI7868 (G2) "}, {"name": "l_FFeXI7891", "desc": "Limit flag for FFeXI7891, 3{sigma} upper limit (G2)"}, {"name": "FFeXI7891", "desc": "[6.1/894]? Emission line flux, [FeXI]{lambda}7891 (G2)"}, {"name": "e_FFeXI7891", "desc": "[0/28]? Uncertainty for FFeXI7891 (G2) "}, {"name": "l_FHeII8236", "desc": "Limit flag for FHeII8236, 3{sigma} upper limit (G2)"}, {"name": "FHeII8236", "desc": "[6.7/1914]? Emission line flux, HeII{lambda}8236 (G2)"}, {"name": "e_FHeII8236", "desc": "[0/23]? Uncertainty for FHeII8236 (G2) "}, {"name": "l_FOI8446", "desc": "Limit flag for FOI8446, 3{sigma} upper limit (G2)"}, {"name": "FOI8446", "desc": "[6.9/9317]? Emission line flux, [OI]{lambda}8446 (G2)"}, {"name": "e_FOI8446", "desc": "[0/22]? Uncertainty for FOI8446 (G2) "}, {"name": "l_FPa16", "desc": "Limit flag for FPa16, 3{sigma} upper limit (G2)"}, {"name": "FPa16", "desc": "[6.9/7582]? Emission line flux, Pa16 {lambda}8502 (G2)"}, {"name": "e_FPa16", "desc": "[0/22]? Uncertainty for FPa16 (G2) "}, {"name": "l_FPa15", "desc": "Limit flag for FPa15, 3{sigma} upper limit (G2)"}, {"name": "FPa15", "desc": "[10.5/5262]? Emission line flux, Pa15 {lambda}8545 (G2)"}, {"name": "e_FPa15", "desc": "[0/18]? Uncertainty for FPa15 (G2) "}, {"name": "l_FPa14", "desc": "Limit flag for FPa14, 3{sigma} upper limit (G2)"}, {"name": "FPa14", "desc": "[7/4909]? Emission line flux, Pa14 {lambda}8598 (G2)"}, {"name": "e_FPa14", "desc": "[0.1/19]? Uncertainty for FPa14 (G2) "}, {"name": "l_FPa13", "desc": "Limit flag for FPa13, 3{sigma} upper limit (G2)"}, {"name": "FPa13", "desc": "[7/3226]? Emission line flux, Pa13 {lambda}8665 (G2)"}, {"name": "e_FPa13", "desc": "[0/21]? Uncertainty for FPa13 (G2) "}]}, {"name": "table11.dat", "desc": "Emission-line measurements - from Pa12{lambda}8750 to [SVIII]{lambda}9913", "columns": [{"name": "ID", "desc": "[1/1210] Swift-BAT 70-month hard X-ray survey identifier (G1)"}, {"name": "m_ID", "desc": "[AB] Component on sequential number "}, {"name": "l_FPa12", "desc": "Limit flag for FPa12, 3{sigma} upper limit (G2)"}, {"name": "FPa12", "desc": "[10.8/5291]? Emission line flux, Pa12 {lambda}8750 (G2)"}, {"name": "e_FPa12", "desc": "[0.1/11]? Uncertainty for FPa12 (G2) "}, {"name": "l_FSIII8829", "desc": "Limit flag for FSIII8829, 3{sigma} upper limit (G2)"}, {"name": "FSIII8829", "desc": "[10.9/12598]? Emission line flux, [SIII]{lambda}8829 (G2)"}, {"name": "e_FSIII8829", "desc": "[0/17]? Uncertainty for FSIII8829 (G2) "}, {"name": "l_FPa11", "desc": "Limit flag for FPa11, 3{sigma} upper limit (G2)"}, {"name": "FPa11", "desc": "[7/16497]? Emission line flux, Pa11 {lambda}8862 (G2)"}, {"name": "e_FPa11", "desc": "[0.1/24]? Uncertainty for FPa11 (G2) "}, {"name": "l_FFeIII8891", "desc": "Limit flag for FFeIII8891, 3{sigma} upper limit (G2)"}, {"name": "FFeIII8891", "desc": "[11/17669]? Emission line flux, [FeIII]{lambda}8891 (G2)"}, {"name": "e_FFeIII8891", "desc": "[0.1/17]? Uncertainty for FFeIII8891 (G2)"}, {"name": "l_FPa10", "desc": "Limit flag for FPa10, 3{sigma} upper limit (G2)"}, {"name": "FPa10", "desc": "[10.9/17885]? Emission line flux, Pa10 {lambda}9014 (G2)"}, {"name": "e_FPa10", "desc": "[0.1/19]? Uncertainty for FPa10 (G2) "}, {"name": "l_FSIII9068", "desc": "Limit flag for FSIII9068, 3{sigma} upper limit (G2)"}, {"name": "FSIII9068", "desc": "[23.5/38973]? Emission line flux, [SIII]{lambda}9068 (G2)"}, {"name": "e_FSIII9068", "desc": "[0.1/58]? Uncertainty for FSIII9068 (G2)"}, {"name": "l_FPa9", "desc": "Limit flag for FPa9, 3{sigma} upper limit (G2)"}, {"name": "FPa9", "desc": "[13.4/7513]? Emission line flux, Pa9 {lambda}9229 (G2)"}, {"name": "e_FPa9", "desc": "[0.1/43]? Uncertainty for FPa9 (G2) "}, {"name": "l_FSIII9531", "desc": "Limit flag for FSIII9531, 3{sigma} upper limit (G2)"}, {"name": "FSIII9531", "desc": "[22/103562]? Emission line flux, [SIII]{lambda}9531 (G2)"}, {"name": "e_FSIII9531", "desc": "[0.1/131]? Uncertainty for FSIII9531 (G2)"}, {"name": "l_FPaeps", "desc": "Limit flag for FPaeps, 3{sigma} upper limit (G2)"}, {"name": "FPaeps", "desc": "[8.6/14104]? Emission line flux, Pa{epsilon} {lambda}9545 (G2)"}, {"name": "e_FPaeps", "desc": "[0.1/33]? Uncertainty for FPaeps (G2) "}, {"name": "l_FCI9824", "desc": "Limit flag for FCI9824, 3{sigma} upper limit (G2)"}, {"name": "FCI9824", "desc": "[28/261]? Emission line flux, [CI]{lambda}9824 (G2)"}, {"name": "e_FCI9824", "desc": "[4/37]? Uncertainty for FCI9824 (G2) "}, {"name": "l_FCI9850", "desc": "Limit flag for FCI9850, 3{sigma} upper limit (G2)"}, {"name": "FCI9850", "desc": "[28/733]? Emission line flux, [CI]{lambda}9850 (G2)"}, {"name": "e_FCI9850", "desc": "[4/112]? Uncertainty for FCI9850 (G2) "}, {"name": "l_FSVIII9913", "desc": "Limit flag for FSIV9913, 3{sigma} upper limit (G2)"}, {"name": "FSVIII9913", "desc": "[31/723]? Emission line flux, [SVIII]{lambda}9913 (G2)"}, {"name": "e_FSVIII9913", "desc": "[4/23]? Uncertainty for FSIV9913 (G2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_261_23"}} {"id": "J/ApJS/261/23", "title_cds": "Type 1 & Type 2 AGNs velocity dispersions from SDSS", "title_create": "Zhang, 2022", "year": "2022", "author": "Zhang X.", "title_pub": "Are there larger stellar velocity dispersions in low-redshift type 1 AGNs than in type 2 AGNs?", "first_author": "Zhang X.", "ref_biblio": [""], "bibcode": ["2022ApJS..261...23Z"], "see_also": ["III/218 : ELODIE archive (Prugniel+, 2001)", "V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)", "VII/289 : SDSS quasar catalog, 16th data release (DR16Q) (Lyke+, 2020)", "J/ApJ/613/682 : AGN masses & broad-line region sizes (Peterson+, 2004)", "J/ApJS/152/251 : Indo-US library of coude feed stellar sp. (Valdes+, 2004)", "J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006)", "J/ApJ/716/993 : LAMP: reverberation mapping of H and He lines (Bentz+, 2010)", "J/ApJS/189/15 : FeII emission in a sample of AGN spectra (Kovacevic+, 2010)", "J/ApJS/194/42 : SDSS-DR3 MgII-based black hole masses (Rafiee+, 2011)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/ApJS/201/29 : Velocity dispersions in active galaxies (Harris+, 2012)", "J/ApJS/199/3 : The quasars MMT-BOSS pilot survey (Ross+, 2012)", "J/MNRAS/438/557 : BLR-less AGNs in Stripe82 (Zhang, 2014)", "J/ApJS/217/26 : Lick AGN monitoring 2011: light curves (Barth+, 2015)", "J/ApJ/809/20 : M_BH_-{sigma} relation for active galaxies (Bennert+, 2015)", "J/ApJS/219/1 : Catalog of Type-1 AGNs from SDSS-DR7 (Oh+, 2015)", "J/MNRAS/446/2330 : Overmassive black holes (Savorgnan+, 2015)", "J/ApJS/216/4 : SDSS-RM project: technical overview (Shen+, 2015)", "J/ApJ/805/96 : SDSS-RM project: velocity dispersions of QSOs (Shen+, 2015)", "J/ApJ/851/21 : SDSS RM project first year of observations (Grier+, 2017)", "J/ApJS/229/39 : Narrow line Seyfert 1 gal. from SDSS-DR12 (Rakshit+, 2017)", "J/ApJ/878/11 : Type 1 vs 2 X-ray-selected COSMOS AGNs & env. (Zou+, 2019)", "J/ApJS/256/40 : HST imaging survey of low-z Swift-BAT AGNs (Kim+, 2021)"], "keyword_cds": "Active gal. nuclei; Velocity dispersion; Redshifts; Spectra, optical", "keyword_pub": "Active galaxies ; Active galactic nuclei ; Supermassive black holes ; Emission line galaxies", "abstract": ["The main objective of this article is to check the Unified Model (UM)", "for the expected similar stellar velocity dispersions between Type 1", "and Type 2 active galactic nuclei (AGNs) and then to provide further", "clues on black hole (BH) mass properties. Unlike previous comparisons", "of BH masses estimated from M_BH_-{sigma} relations for Type 2 AGNs", "and from virial BH masses for Type 1 AGNs, reliable stellar velocity", "dispersions {sigma} measured from absorption features around 4000{AA}", "are directly compared between the thus far largest samples of", "6260 low-redshift (z<0.3) Type 1 AGNs and almost all Type 2 AGNs in", "SDSS-DR12. Although half of Type 1 AGNs do not have a measured {sigma}", "due to unapparent absorption features overwhelmed by AGN activities,", "both properties of the mean spectra of Type 1 AGNs with and without a", "measured {sigma} and a positive dependence of {sigma} on the [OIII]", "luminosity can lead to a statistically larger {sigma} for all Type 1", "AGNs compared to the 6260 Type 1 AGNs with measured stellar velocity", "dispersions. Then, direct {sigma} comparisons can lead to a", "statistically larger {sigma} in Type 1 AGNs, with a confidence level", "higher than 10{sigma}, after considering the necessary effects of", "different redshifts and different central AGN activities. Although", "Type 1 AGNs have a {sigma} of only about (9+/-3)% larger than Type 2", "AGNs, the difference cannot be well explained at the current stage.", "Unless there is strong evidence to support different M_BH_-{sigma}", "relations or to support quite different evolutionary histories between", "Type 1 and Type 2 AGNs, the statistically larger {sigma} in Type 1", "AGNs provides a strong challenge to the UM of AGNs."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Parameters of the 1445 Type-1 AGN in the subsample ", "columns": [{"name": "mpf", "desc": "SDSS identifier (1) "}, {"name": "z", "desc": "[0.018/0.3] Redshift "}, {"name": "vdisp", "desc": "[54/399] Stellar velocity dispersion (2) "}, {"name": "e_vdisp", "desc": "[3/59] Uncertainty in vdisp "}, {"name": "logLOIII", "desc": "[38.9/42.3] Log of [OIII] line luminosity in erg/s units"}, {"name": "logOIII/Hb", "desc": "[-0.14/1.3] Flux ratio of [OIII] to narrow Hbeta"}, {"name": "logNII/Ha", "desc": "[-1.81/0.33] Flux ratio of [NII] to narrow Halpha"}]}, {"name": "table2.dat", "desc": "Parameters of the 1445 Type-2 AGN in the subsample ", "columns": [{"name": "mpf", "desc": "SDSS identifier (1) "}, {"name": "z", "desc": "[0.018/0.3] Redshift "}, {"name": "vdisp", "desc": "[54/399] Stellar velocity dispersion (2) "}, {"name": "e_vdisp", "desc": "[3/59] Uncertainty in vdisp "}, {"name": "logLOIII", "desc": "[38.9/42.3] Log of [OIII] line luminosity in erg/s units"}, {"name": "logOIII/Hb", "desc": "[-0.14/1.3] Flux ratio of [OIII] to narrow Hbeta"}, {"name": "logNII/Ha", "desc": "[-1.81/0.33] Flux ratio of [NII] to narrow Halpha"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_261_24"}} {"id": "J/ApJS/261/24", "title_cds": "AGNs in the HETDEX survey. I. First AGN catalog", "title_create": "Liu+, 2022", "year": "2022", "author": "Liu C., Gebhardt K., Cooper E.M., Davis D., Schneider D.P., Ciardullo R., Farrow D.J., Finkelstein S.L., Gronwall C., Guo Y., Hill G.J., House L., Jeong D., Jogee S., Kollatschny W., Krumpe M., Landriau M., Chavez Ortiz O.A., Zhang Y., The HETDEX Collaboration", "title_pub": "The active galactic nuclei in the Hobby-Eberly Telescope Dark Energy Experiment survey (HETDEX). I. Sample selection.", "first_author": "Liu C.", "ref_biblio": [""], "bibcode": ["2022ApJS..261...24L"], "see_also": ["B/cfht : Log of CFHT Exposures (CADC, 1979-)", "II/261 : GOODS initial results (Giavalisco+, 2004)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "VII/286 : SDSS quasar catalog, fourteenth data release (Paris+, 2018)", "V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)", "VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)", "J/AJ/126/539 : The Chandra Deep Fields North and South (Alexander+, 2003)", "J/A+A/457/79 : VIMOS VLT Deep Survey: faint type-1 AGNs (Gavignaud+, 2006)", "J/MNRAS/374/664 : Stellar atmospheric param. in MILES library (Cenarro+, 2007)", "J/ApJ/681/1163 : Late-type galaxies in Chandra deep fields (Lehmer+, 2008)", "J/ApJ/702/767 : CIV and FeK{alpha} Baldwin effects in AGNs (Wu+, 2009)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/ApJS/195/10 : The CDF-S survey: 4Ms source catalogs (Xue+, 2011)", "J/ApJS/199/3 : The quasars MMT-BOSS pilot survey (Ross+, 2012)", "J/A+A/559/A14 : VIMOS VLT Deep Survey final data release (Le Fevre+, 2013)", "J/ApJ/817/172 : X-ray Observations of Stripe 82 (LaMassa+, 2016)", "J/ApJS/224/15 : Improved 2Ms and 250ks Chandra catalogs (Xue+, 2016)", "J/ApJ/850/66 : Stripe 82X survey multiwavelength catalog (Ananna+, 2017)", "J/ApJS/228/2 : Chandra Deep Field-South survey: 7Ms sources (Luo+, 2017)", "J/ApJ/876/50 : X-ray & MIR AGNs in Stripe 82 with eBOSS sp. (LaMassa+, 2019)", "J/ApJS/249/17 : SDSS QSO DR14 spectral properties (Rakshit+, 2020)", "J/A+A/643/A149 : J-PLUS Ly{alpha}-emitting candidates (Spinoso+, 2020)"], "keyword_cds": "Active gal. nuclei; Spectra, optical; Surveys; Redshifts; Equivalent widths; Photometry", "keyword_pub": "Active galactic nuclei", "abstract": ["We present the first active galactic nuclei (AGN) catalog of the", "Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX) observed", "between 2017 January and 2020 June. HETDEX is an ongoing spectroscopic", "survey (3500-5500{AA}) with no target preselection based on", "magnitudes, colors or morphologies, enabling us to select AGN based", "solely on their spectral features. Both luminous quasars and", "low-luminosity Seyferts are found in our catalog. AGN candidates are", "selected with at least two significant AGN emission lines, such as the", "Ly{alpha} and CIV{lambda}1549 line pair, or with a single broad", "emission line with FWHM>1000km/s. Each source is further confirmed by", "visual inspections. This catalog contains 5322 AGN, covering an", "effective sky coverage of 30.61deg^2^. A total of 3733 of these AGN", "have secure redshifts, and we provide redshift estimates for the", "remaining 1589 single broad-line AGN with no crossmatched spectral", "redshifts from the Sloan Digital Sky Survey Data Release 14 of QSOs.", "The redshift range of the AGN catalog is 0.2522.5, and 2.6% reaching the", "detection limit at r~26mag of the deepest imaging surveys we searched.", "We also provide a composite spectrum of the AGN sample covering", "700-4400{AA}."], "description": ["The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX;", "Gebhardt+ 2021ApJ...923..217G) is a spectroscopic survey without", "target preselection on the 10m Hobby-Eberly Telescope (HET).", "It uses the Visible Integral-field Replicable Unit Spectrograph", "(VIRUS) to record spectra for all targets within its field of view.", "The survey began with 16 active IFUs on 2017 January 1. By 2020 June", "26, there were 71 IFUs actively working on the telescope, and as of", "2021 September 1, the full-array 78 IFUs were actively producing data.", "As of 2020 June 26, the end date of this catalog, the effective sky", "coverage of HETDEX was 30.61deg^2^."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "catalog.dat", "desc": "The HETDEX AGN catalog ", "columns": [{"name": "Seq", "desc": "[1/5378] Running sequence number (agnid)"}, {"name": "RAdeg", "desc": "Right ascension of the AGN, center of flux-weighted fof (J2000) (ra)"}, {"name": "DEdeg", "desc": "Declination of the AGN, center of flux-weighted fof (J2000) (dec)"}, {"name": "z", "desc": "[0.18/4.2] Measured redshift "}, {"name": "e_z", "desc": "[1e-05/0.013] z uncertainty (z_er) "}, {"name": "f_z", "desc": "Flag on z (1=confirmed z; 3733 occurrences) (zflag)"}, {"name": "Field", "desc": "Field in the HETDEX survey (1) "}, {"name": "Nrep", "desc": "[0/12] Number of repeat observations (nshots)"}, {"name": "Det-ID", "desc": "[2100002267/2190088018] ID in the HETDEX catalog closest to friend-of-friend (fof) center (detectid_best)"}, {"name": "RABdeg", "desc": "Right ascension of Det-ID (J2000) (ra_best)"}, {"name": "DEBdeg", "desc": "Declination of Det-ID (J2000) (dec_best)"}, {"name": "roff", "desc": "[0/3.3] Offset between RABdeg, DEBdeg with fof center (roff)"}, {"name": "Nmm", "desc": "[1/48] Number of member Det-IDs (see Sections 3.1 and 3.2) (nmem)"}, {"name": "alpha", "desc": "[-4.5/3.7]?=-99 {alpha}_{Lambda}_ of the power-law-fitted continuum"}, {"name": "e_alpha", "desc": "[0/0.9]?=-99 alpha uncertainty (alpha_er)"}, {"name": "fpl0", "desc": "[-4.15e+10/3.91e+15] Power-law continuum = fpl0*{lambda}^{alpha}{lambda}^"}, {"name": "e_fpl0", "desc": "[0/2.2e+14]?=-99 fpl0 uncertainty (fpl0_er)"}, {"name": "Slope", "desc": "[-0.4/0.07] Slope of the linear-fitted continuum"}, {"name": "e_Slope", "desc": "[6e-6/0.004] Slope uncertainty (slope_er)"}, {"name": "Int", "desc": "[-52/708] Intercept of the linear-fitted continuum (intercept)"}, {"name": "e_Int", "desc": "[0.017/5] Int uncertainty (intercept_er)"}, {"name": "L1350", "desc": "[-21/1449] Monochromatic luminosity at rest-frame 1350{AA} in 10^44erg/s"}, {"name": "e_L1350", "desc": "[0/8] L1350 uncertainty (L1350_er) "}, {"name": "L1450", "desc": "[-27/1354] Monochromatic luminosity at rest-frame 1450{AA} in 10^44erg/s"}, {"name": "e_L1450", "desc": "[0/10] L1450 uncertainty (L1450_er) "}, {"name": "L3000", "desc": "[-1092/17235] Monochromatic luminosity at rest-frame 3000{AA} in 10^44erg/s"}, {"name": "e_L3000", "desc": "[0/532] L3000 uncertainty (L3000_er) "}, {"name": "L5100", "desc": "[-6293/208695] Monochromatic luminosity at rest-frame 5100{AA} in 10^44erg/s"}, {"name": "e_L5100", "desc": "[0/7747] L5100 uncertainty (L5100_er)"}, {"name": "FWHMLyA", "desc": "[0/22033]?=- Rest-frame FWHM of the LyA emission (fwhm_LyA)"}, {"name": "e_FWHMLyA", "desc": "[2/1455]?=- FWHMLyA uncertainty (fwhm_LyA_er)"}, {"name": "EWLyA", "desc": "[0/14820]?=- Rest-frame EW of the LyA emission in {AA} (ew_LyA)"}, {"name": "e_EWLyA", "desc": "[0/2143]?=- EWLyA uncertainty (ew_LyA_er)"}, {"name": "FLyA", "desc": "[0/18171]?=- Rest-frame flux of the LyA emission in 10^-17^erg/s/cm^2^ (flux_LyA)"}, {"name": "e_FLyA", "desc": "[0/504]?=- FLyA uncertainty (flux_LyA_er)"}, {"name": "cLyA", "desc": "[-0.6/302]?=- Rest-frame continuum at the LyA emission in 10^-17erg/cm^2^/s/{AA} (cont_LyA)"}, {"name": "e_cLyA", "desc": "[0.008/1.1]?=- cLyA uncertainty (cont_LyA_er)"}, {"name": "SNRLyA", "desc": "[0/234]?=- S/N of the LyA region (snr_LyA)"}, {"name": "e_SNRLyA", "desc": "[0/8]?=- SNRLyA uncertainty (snr_LyA_er)"}, {"name": "Chi2LyA", "desc": "[0.05/229]?=- Chi2 of the LyA region (chi2_LyA)"}, {"name": "e_Chi2LyA", "desc": "[0.016/1483]?=- Chi2LyA uncertainty (chi2_LyA_er)"}, {"name": "FWHMNV", "desc": "[0/20448]?=- Rest-frame FWHM of the NV emission (flux_WHMNV)"}, {"name": "e_FWHMNV", "desc": "[2/1501]?=- FWHMNV uncertainty (flux_WHMNV_er)"}, {"name": "EWNV", "desc": "[0/18299]?=- Rest-frame EW of the NV emission in {AA} (EWNV)"}, {"name": "e_EWNV", "desc": "[0/2235]?=- EWNV uncertainty (EWNV_er)"}, {"name": "FNV", "desc": "[0/12574]?=- Rest-frame flux of the NV emission in 10^-17^erg/s/cm^2^ (flux_NV)"}, {"name": "e_FNV", "desc": "[0/417]?=- FNV uncertainty (flux_NV_er)"}, {"name": "cNV", "desc": "[-0.6/290]?=- Rest-frame continuum at the NV emission in 10^-17erg/cm^2^/s/{AA} (cont_NV)"}, {"name": "e_cNV", "desc": "[0.008/1]?=- cNV uncertainty (cont_NV_er)"}, {"name": "FWHMSiO", "desc": "[0/21429]?=- Rest-frame FWHM of the SiO emission (fwhm_SiO)"}, {"name": "e_FWHMSiO", "desc": "[0.6/1500]?=- FWHMSiO uncertainty (fwhm_SiO_er)"}, {"name": "EWSiO", "desc": "[0/3.1e+15]?=- Rest-frame EW of the SiO emission in {AA} (ew_SiO)"}, {"name": "e_EWSiO", "desc": "[0/2.4e+15]?=- EWSiO uncertainty (ew_SiO_er)"}, {"name": "FSiO", "desc": "[0/2118]?=- Rest-frame flux of the SiO emission in 10^-17^erg/s/cm^2^ (flux_SiO)"}, {"name": "e_FSiO", "desc": "[0/176]?=- FSiO uncertainty (flux_SiO_er)"}, {"name": "cSiO", "desc": "[-1.6/229]?=- Rest-frame continuum at the SiO emission in 10^-17erg/cm^2^/s/{AA} (cont_SiO)"}, {"name": "e_cSiO", "desc": "[0.007/1.5]?=- cSiO uncertainty (cont_SiO_er)"}, {"name": "SNRSiO", "desc": "[0/63]?=- S/N of the SiO region (snr_SiO)"}, {"name": "e_SNRSiO", "desc": "[0/3]?=- SNRSiO uncertainty (snr_SiO_er)"}, {"name": "Chi2SiO", "desc": "[0.02/253]?=- Chi2 of the SiO region (chi2_SiO)"}, {"name": "e_Chi2SiO", "desc": "[0.016/0.6]?=- Chi2SiO uncertainty (chi2_SiO_er)"}, {"name": "FWHMCIV", "desc": "[0/19355]?=- Rest-frame FWHM of the CIV emission (fwhm_CIV)"}, {"name": "e_FWHMCIV", "desc": "[0/1296]?=- FWHMCIV uncertainty (fwhm_CIV_er)"}, {"name": "EWCIV", "desc": "[0/5.9e+15]?=- Rest-frame EW of the CIV emission in {AA} (ew_CIV)"}, {"name": "e_EWCIV", "desc": "[0/4.6e+15]?=- EWCIV uncertainty (ew_CIV_er)"}, {"name": "FCIV", "desc": "[0/9371]?=- Rest-frame flux of the CIV emission in 10^-17^erg/s/cm^2^ (flux_CIV)"}, {"name": "e_FCIV", "desc": "[0/144]?=- FCIV uncertainty (flux_CIV_er)"}, {"name": "cCIV", "desc": "[-1.2/188]?=- Rest-frame continuum at the CIV emission in 10^-17erg/cm^2^/s/{AA} (cont_CIV)"}, {"name": "e_cCIV", "desc": "[0.006/1.1]?=- cCIV uncertainty (cont_CIV_er)"}, {"name": "SNRCIV", "desc": "[0/163]?=- S/N of the CIV region (snr_CIV)"}, {"name": "e_SNRCIV", "desc": "[0/3]?=- SNRCIV uncertainty (snr_CIV_er)"}, {"name": "Chi2CIV", "desc": "[0.03/1135]?=- Chi2 of the CIV region (chi2_CIV)"}, {"name": "e_Chi2CIV", "desc": "[0.017/2]?=- Chi2CIV uncertainty (chi2_CIV_er)"}, {"name": "FWHMHeII", "desc": "[0/18282]?=- Rest-frame FWHM of the HeII emission (fwhm_HeII)"}, {"name": "e_FWHMHeII", "desc": "[0/1259]?=- FWHMHeII uncertainty (fwhm_HeII_er)"}, {"name": "EWHeII", "desc": "[0/4.5e+15]?=- Rest-frame EW of the HeII emission in {AA} (ew_HeII)"}, {"name": "e_EWHeII", "desc": "[0/4.4e+15]?=- EWHeII uncertainty (ew_HeII_er)"}, {"name": "FHeII", "desc": "[0/3409]?=- Rest-frame flux of the HeII emission in 10^-17^erg/s/cm^2^ (flux_HeII)"}, {"name": "e_FHeII", "desc": "[0/143]?=- FHeII uncertainty (flux_HeII_er)"}, {"name": "cHeII", "desc": "[-1.7/168]?=- Rest-frame continuum at the HeII emission in 10^-17erg/cm^2^/s/{AA} (cont_HeII)"}, {"name": "e_cHeII", "desc": "[0.005/1]?=- cHeII uncertainty (cont_HeII_er)"}, {"name": "SNRHeII", "desc": "[0/70]?=- S/N of the HeII region (snr_HeII)"}, {"name": "e_SNRHeII", "desc": "[0/2]?=- SNRHeII uncertainty (snr_HeII_er)"}, {"name": "Chi2HeII", "desc": "[0.05/13]?=- Chi2 of the HeII region (chi2_HeII)"}, {"name": "e_Chi2HeII", "desc": "[0.017/0.6]?=- Chi2HeII uncertainty (chi2_HeII_er)"}, {"name": "FWHMCIII", "desc": "[0/15659]?=- Rest-frame FWHM of the CIII emission (fwhm_CIII)"}, {"name": "e_FWHMCIII", "desc": "[0.6/1052]?=- FWHMCIII uncertainty (fwhm_CIII_er)"}, {"name": "EWCIII", "desc": "[0/1.3e+15]?=- Rest-frame EW of the CIII emission in {AA} (ew_CIII)"}, {"name": "e_EWCIII", "desc": "[0/4.5e+14]?=- EWCIII uncertainty (ew_CIII_er)"}, {"name": "FCIII", "desc": "[0/5637]?=- Rest-frame flux of the CIII emission in 10^-17^erg/s/cm^2^ (flux_CIII)"}, {"name": "e_FCIII", "desc": "[0.004/350]?=- FCIII uncertainty (flux_CIII_er)"}, {"name": "cCIII", "desc": "[-0.1/207]?=- Rest-frame continuum at the CIII emission in 10^-17erg/cm^2^/s/{AA} (cont_CIII)"}, {"name": "e_cCIII", "desc": "[0.003/2.3]?=- cCIII uncertainty (cont_CIII_er)"}, {"name": "SNRCIII", "desc": "[0/95]?=- S/N of the CIII region (snr_CIII)"}, {"name": "e_SNRCIII", "desc": "[0/2.4]?=- SNRCIII uncertainty (snr_CIII_er)"}, {"name": "Chi2CIII", "desc": "[0.05/11]?=- Chi2 of the CIII region (chi2_CIII)"}, {"name": "e_Chi2CIII", "desc": "[0.018/0.3]?=- Chi2CIII uncertainty (chi2_CIII_er)"}, {"name": "FWHMMgII", "desc": "[38/10688]?=- Rest-frame FWHM of the MgII emission (fwhm_MgII)"}, {"name": "e_FWHMMgII", "desc": "[6/526]?=- FWHMMgII uncertainty (fwhm_MgII_er)"}, {"name": "EWMgII", "desc": "[0.04/1.2e+15]?=- Rest-frame EW of the MgII emission in {AA} (ew_MgII)"}, {"name": "e_EWMgII", "desc": "[0.004/2.2e+14]?=- EWMgII uncertainty (ew_MgII_er)"}, {"name": "FMgII", "desc": "[3.4/10427]?=- Rest-frame flux of the MgII emission in 10^-17^erg/s/cm^2^ (flux_MgII)"}, {"name": "e_FMgII", "desc": "[0.28/619]?=- FMgII uncertainty (flux_MgII_er)"}, {"name": "cMgII", "desc": "[0/226]?=- Rest-frame continuum at the MgII emission in 10^-17erg/cm^2^/s/{AA} (cont_MgII)"}, {"name": "e_cMgII", "desc": "[0.002/4.2]?=- cMgII uncertainty (cont_MgII_er)"}, {"name": "SNRMgII", "desc": "[0.4/293]?=- S/N of the MgII region (snr_MgII)"}, {"name": "e_SNRMgII", "desc": "[0.04/17]?=- SNRMgII uncertainty (snr_MgII_er)"}, {"name": "Chi2MgII", "desc": "[0.2/23]?=- Chi2 of the MgII region (chi2_MgII)"}, {"name": "e_Chi2MgII", "desc": "[0.02/0.6]?=- Chi2MgII uncertainty (chi2_MgII_er)"}, {"name": "FWHMOII", "desc": "[0/7932]?=- Rest-frame FWHM of the OII emission (fwhm_OII)"}, {"name": "e_FWHMOII", "desc": "[0.6/320]?=- FWHMOII uncertainty (fwhm_OII_er)"}, {"name": "EWOII", "desc": "[-8.5/183]?=- Rest-frame EW of the OII emission in {AA} (ew_OII)"}, {"name": "e_EWOII", "desc": "[0/7.7e+12]?=- EWOII uncertainty (ew_OII_er)"}, {"name": "FOII", "desc": "[0/451]?=- Rest-frame flux of the OII emission in 10^-17^erg/s/cm^2^ (flux_OII)"}, {"name": "e_FOII", "desc": "[0.001/13]?=- FOII uncertainty (flux_OII_er)"}, {"name": "cOII", "desc": "[0.3/120]?=- Rest-frame continuum at the OII emission in 10^-17erg/cm^2^/s/{AA} (cont_OII)"}, {"name": "e_cOII", "desc": "[0.002/0.2]?=- cOII uncertainty (cont_OII_er)"}, {"name": "SNROII", "desc": "[0/95]?=- S/N of the OII region (snr_OII)"}, {"name": "e_SNROII", "desc": "[0/0.4]?=- SNROII uncertainty (snr_OII_er)"}, {"name": "Chi2OII", "desc": "[0.3/46]?=- Chi2 of the OII region (chi2_OII)"}, {"name": "e_Chi2OII", "desc": "[0.03/0.3]?=- Chi2OII uncertainty (chi2_OII_er)"}, {"name": "FWHMOVI", "desc": "[0/28982]?=- Rest-frame FWHM of the OVI emission (fwhm_OVI)"}, {"name": "e_FWHMOVI", "desc": "[0/2023]?=- FWHMOVI uncertainty (fwhm_OVI_er)"}, {"name": "EWOVI", "desc": "[-47/1.8e+13]?=- Rest-frame EW of the OVI emission in {AA} (ew_OVI)"}, {"name": "e_EWOVI", "desc": "[0/9.7e+14]?=- EWOVI uncertainty (ew_OVI_er)"}, {"name": "FOVI", "desc": "[0/1877]?=- Rest-frame flux of the OVI emission in 10^-17^erg/s/cm^2^ (flux_OVI)"}, {"name": "e_FOVI", "desc": "[0/120]?=- FOVI uncertainty (flux_OVI_er)"}, {"name": "cOVI", "desc": "[-1.6/413]?=- Rest-frame continuum at the OVI emission in 10^-17erg/cm^2^/s/{AA} (cont_OVI)"}, {"name": "e_cOVI", "desc": "[0.007/2.6]?=- cOVI uncertainty (cont_OVI_er)"}, {"name": "SNROVI", "desc": "[0/96]?=- S/N of the OVI region (snr_OVI)"}, {"name": "e_SNROVI", "desc": "[0/4]?=- SNROVI uncertainty (snr_OVI_er)"}, {"name": "Chi2OVI", "desc": "[0.1/378]?=- Chi2 of the OVI region (chi2_OVI)"}, {"name": "e_Chi2OVI", "desc": "[0/16]?=- Chi2OVI uncertainty (chi2_OVI_er)"}, {"name": "fiberid", "desc": "fiberid in HETDEX fiber design (2) "}, {"name": "rmag", "desc": "[16.67/34.3]?=- r-band aperture magnitude (r_aper)"}, {"name": "e_rmag", "desc": "[0.0001/72.1]?=- rmag uncertainty (r_aper_er)"}, {"name": "rrad", "desc": "[0.29/3.3]?=- r-band best aperture radius (r_radius)"}, {"name": "rdepth", "desc": "[24/27.3]?=- r-band 5{sigma} depth (r_depth)"}, {"name": "r_rmag", "desc": "Survey of rmag (r_cat) (3) "}, {"name": "gmag", "desc": "[15.5/31.5]?=- g-band aperture magnitude (g_aper)"}, {"name": "e_gmag", "desc": "[0.0001/74]?=- gmag uncertainty (g_aper_er)"}, {"name": "grad", "desc": "[0.35/4.7]?=- g-band best aperture radius (g_radius)"}, {"name": "gdepth", "desc": "[24/27.3]?=- g-band 5{sigma} depth (g_depth)"}, {"name": "r_gmag", "desc": "Survey of gmag (g_cat) (3) "}, {"name": "umag", "desc": "[16.74/33.5]?=- u-band aperture magnitude (u_aper)"}, {"name": "e_umag", "desc": "[0.0002/70]?=- umag uncertainty (u_aper_er)"}, {"name": "urad", "desc": "[0.36/3]?=- u-band best aperture radius (u_radius)"}, {"name": "udepth", "desc": "[25.7/27.3]?=- u-band 5{sigma} depth (u_depth)"}, {"name": "r_umag", "desc": "Survey of umag (u_cat) (3) "}, {"name": "Sepdr14q", "desc": "[0.0027/13704] Smallest separation to dr14q (rsep_dr14q)"}, {"name": "IDdr14q", "desc": "ID of the closest AGN in dr14q (plate-mjd-fiber) (id_dr14q)"}, {"name": "zdr14q", "desc": "[0.15/5.1] Spectral redshift of IDdr14q (z_dr14q)"}, {"name": "Sepdr16", "desc": "[0.0027/11936] Smallest separation to dr16 (rsep_dr16)"}, {"name": "Platedr16", "desc": "Plate of the closest AGN in dr16 (plate_dr16)"}, {"name": "Fiberdr16", "desc": "Fiber of the closest AGN in dr16 (fiber_dr16)"}, {"name": "MJDdr16", "desc": "[51783/58251] MJD of the closest AGN in dr16 (mjd_dr16)"}, {"name": "zdr16", "desc": "[-0.0042/7.03] Spectral redshift of ID-DR16 (z_dr16)"}, {"name": "Flag", "desc": "AGN selection flag (sflag) (4) "}, {"name": "Apcor", "desc": "[0.084/0.99] Aperture correction at the wavelength of the strongest emission of detectid_best_"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_261_26"}} {"id": "J/ApJS/261/26", "title_cds": "Exoplanet host stars from LAMOST, TESS, Kepler & K2", "title_create": "Su+, 2022", "year": "2022", "author": "Su T., Zhang L.-Y., Long L., Han X.L., Misra P., Meng G., Pi Q., Yang Z., Yang J.", "title_pub": "Magnetic activity and physical parameters of exoplanet host stars based on LAMOST DR7, TESS, Kepler, and K2 surveys.", "first_author": "Su T.", "ref_biblio": [""], "bibcode": ["2022ApJS..261...26S"], "see_also": ["II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)", "V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)", "V/146 : LAMOST DR1 catalogs (Luo+, 2015)", "IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "V/156 : LAMOST DR7 catalogs (Luo+, 2019)", "J/AJ/106/2096 : Limb-darkening coefficients in binaries (Van Hamme 1993)", "J/AJ/135/785 : SDSS-DR5 low-mass star spectroscopic sample (West+, 2008)", "J/A+A/505/901 : OGLE-TR-10 u', g' and i'-band photometry (Bentley+, 2009)", "J/ApJ/707/167 : Transiting planetary system WASP-18 (Southworth+, 2009)", "J/AJ/140/1402 : M dwarf flares from SDSS spectra (Hilton+, 2010)", "J/AJ/141/50 : White-light flares on Kepler cool stars (Walkowicz+, 2011)", "J/ApJ/743/48 : Stars with rot. periods & X-ray luminosities (Wright+, 2011)", "J/other/Nat/485.478 : Superflares on solar-type stars (Maehara+, 2012)", "J/ApJS/209/5 : Superflares of Kepler stars. I. (Shibayama+, 2013)", "J/A+A/557/A119 : Eclipsing binary system LL Aquarii (Southworth, 2013)", "J/ApJ/795/161 : Activity & rotation in Praesepe & the Hyades (Douglas+, 2014)", "J/ApJS/211/2 : Revised properties of Q1-16 Kepler targets (Huber+, 2014)", "J/A+A/594/A39 : LAMOST-Kepler param. and activity indicators (Frasca+, 2016)", "J/ApJS/224/37 : White-light flares on close binaries from Kepler (Gao+, 2016)", "J/ApJ/829/34 : Kepler heartbeat star radial velocities (Shporer+, 2016)", "J/ApJ/849/36 : Flaring activity of M dwarfs in Kepler field (Yang+, 2017)", "J/ApJS/239/2 : Simulated exoplanets from TESS targets (Barclay+, 2018)", "J/MNRAS/476/908 : Chromospheric activity in 4 open clusters (Fang+, 2018)", "J/AJ/156/220 : V, R and I LCs of 4 new low-mass M-type EBs (Long+, 2018)", "J/ApJ/881/9 : EvryFlare. I. Cool stars's flares (Howard+, 2019)", "J/ApJS/243/28 : M-type star magnetic activities (Lu+, 2019)", "J/ApJS/241/29 : Flare catalog through LC data of Kepler DR25 (Yang+, 2019)", "J/AJ/159/60 : Flares from 1228 stars in TESS sectors 1 & 2 (Gunther+, 2020)", "J/ApJ/890/46 : Superflares on solar-type stars from TESS 1st yr (Tu+, 2020)", "J/ApJS/247/9 : FGK stars magnetic activity in LAMOST-Kepler (Zhang+, 2020)", "J/ApJS/247/28 : K2 star param. from Gaia & LAMOST (Hardegree-Ullman+, 2020)", "J/ApJS/253/19 : Halpha and other EWs of LAMOST M-type stars (Zhang+, 2021)", "J/AJ/162/100 : PAST. II. LAMOST-Gaia-Kepler star catalog (Chen+, 2021)", "J/MNRAS/514/4781 : Active stars in the LAMOST-K2 field (Xiang+, 2022)", "http://exoplanetarchive.ipac.caltech.edu/ : NASA Exoplanet archive"], "keyword_cds": "Stars, flare; Exoplanets; Spectra, optical; Radial velocities; Spectral types; Equivalent widths; Abundances, [Fe/H]; Stars, diameters", "keyword_pub": "Stellar chromospheres ; Stellar flares ; Exoplanet catalogs", "abstract": ["Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)", "low- and medium-resolution spectroscopic surveys are important for", "determination of the orbital parameters and chromospheric activity of", "extrasolar planet systems. We crossmatched the exoplanet catalog", "confirmed before 2021 March 11 with the LAMOST DR7 survey to study", "their properties. There are 1026 targets with exoplanets observed in", "the LAMOST DR7 low-resolution spectroscopic survey and 158 targets in", "the medium-resolution spectroscopic survey. We have calculated the", "equivalent width of the H{alpha} line and determined their stellar", "activity. The H{alpha} and flare intensities are almost constant for", "the Rossby number Ro<=0.12 in the saturated regime and decrease with", "increasing Ro in the unsaturated regime. In addition, we searched the", "flare events of all stars with exoplanets in the Transiting Exoplanet", "Survey Satellite (TESS), Kepler, and K2 surveys. Among the 733", "extrasolar planetary systems observed by TESS, we found 481 flares", "from 57 stars. For Kepler data, we obtained the light curve of 1699", "stars and found 1886 flares from 417 stars. For K2 data, we obtained", "the light curves of 347 stars and found 467 flares from 89 stars.", "There were light curves of 361 objects with obvious eclipse observed", "from the TESS survey. We have fitted their light curves with a high", "signal-to-noise ratio using the JKTEBOP program, and we reobtained the", "orbital parameters, such as inclination, radius, and period. In the", "end, we made a judgment on the habitability of exoplanets of stars", "with flares."], "description": ["Based on the release of the Large Sky Area Multi-Object Fiber", "Spectroscopic Telescope (LAMOST) DR7 (2019 June 8), LAMOST has", "released 10,608,416 low-resolution (R~1800) spectra and 3,889,383", "medium-resolution (R~7500) spectra. We crossmatched the LAMOST", "spectral survey with the exoplanet catalog published before", "2021-March-11. A total of 1928 spectra from 1026 stars meeting the", "requirements were found in the LAMOST low-resolution spectral survey,", "and 282 spectra from 121 stars were found in the LAMOST", "medium-resolution survey. We selected the spectra with signal-to-noise", "ratio (S/N)>10 as our sample. Finally, 1669 low-resolution spectra of", "940 stars and 282 medium-resolution spectra of 121 stars were obtained.", "The Transiting Exoplanet Survey Satellite (TESS) is a space telescope", "that was launched from the Cape Canaveral Air Force Base in the United", "States on 2018 April 18. By crossmatching the exoplanet catalog with", "the first 31 sections of TESS, we obtained 1575 light curves of 733", "targets of stars with exoplanets.", "The Kepler mission started on 2009 May 2 and ended on 2013 May 11. The", "K2 mission started on 2014 February 4 and ended on 2018 September 26.", "In this work, we primarily use the data provided by Kepler and K2 in", "order to search for the flares and calculate the flare energy. We", "found 1886 flares from the light curves of 1699 stars from the Kepler", "mission. Based on 347 extrasolar planet targets of K2, we found 467", "flares from 89 stars and calculated the energies of the flares."], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Low-resolution spectral parameters of exoplanet host stars in LAMOST DR7", "columns": [{"name": "LAMOST", "desc": "LAMOST identifier (JHHMMSS.ss+DDMMSS.s) "}, {"name": "MJD", "desc": "[55940.13/58604.89] Modified Julian Date "}, {"name": "Exp", "desc": "[600/5400] Exposure time "}, {"name": "SN", "desc": "[10/949] Signal-to-Noise ratio "}, {"name": "SpT", "desc": "Spectral type "}, {"name": "RVel", "desc": "[-165/171]? Radial velocity "}, {"name": "e_RVel", "desc": "[0.3/33]? Uncertainty in RVel "}, {"name": "EWHa", "desc": "[-3.7/6.2] H{alpha} equivalent width; in Angstrom units"}, {"name": "SNHa", "desc": "[8.8/272] Signal-to-Noise of EWHa "}, {"name": "HHa", "desc": "[1/53] Height of EWHa; in Angstrom units "}, {"name": "Fe/H", "desc": "[-1.33/0.45]? LAMOST Metallicity "}, {"name": "e_Fe/H", "desc": "[0.003/0.5]? Uncertainty in Fe/H "}, {"name": "log(g)", "desc": "[2.53/4.85]? LAMOST log surface gravity "}, {"name": "e_log(g)", "desc": "[0.002/0.9]? Uncertainty in log(g) "}, {"name": "Teff", "desc": "[3871/7853]? LAMOST Effective temperature "}, {"name": "e_Teff", "desc": "[3/514]? Uncertainty in Teff "}, {"name": "RHa", "desc": "[-8.3e-6/0.0007]? Chromospheric activity level, R'_H{alpha}_ (G1)"}]}, {"name": "table3.dat", "desc": "Medium-resolution spectral parameters of exoplanet host stars in LAMOST DR7", "columns": [{"name": "LAMOST", "desc": "LAMOST identifier (JHHMMSS.ss+DDMMSS.s) "}, {"name": "SN", "desc": "[10/999] Signal-to-Noise "}, {"name": "RVel", "desc": "[-79/118]? Radial velocity "}, {"name": "e_RVel", "desc": "[0.27/6]? Uncertainty in RVel "}, {"name": "EW", "desc": "[-2/18] H{alpha} equivalent width "}, {"name": "e_EW", "desc": "[0.016/0.5] Uncertainty in EW "}, {"name": "Teff", "desc": "[4079/6987]? LAMOST Effective temperature "}, {"name": "log(g)", "desc": "[2/4.82]? LAMOST log surface gravity "}, {"name": "e_log(g)", "desc": "[0.027/0.9]? Uncertainty in log(g) "}, {"name": "Fe/H", "desc": "[-1.83/0.25]? LAMOST Metallicity "}, {"name": "e_Fe/H", "desc": "[0.017/0.9]? Uncertainty in Fe/H "}, {"name": "RHa", "desc": "[-1.2e-5/0.0007]? Chromospheric activity level, R'_H{alpha}_ (G1)"}]}, {"name": "table4.dat", "desc": "Flare parameters of exoplant system of TESS ", "columns": [{"name": "---", "desc": "[TIC] "}, {"name": "TIC", "desc": "TESS identifier "}, {"name": "Peak", "desc": "[1325.46/2110.18] Peak Heliocentric Julian Date of flare"}, {"name": "Start", "desc": "[1325.44/2110.16] Flare Heliocentric Julian start date"}, {"name": "End", "desc": "[1325.47/2110.21] Flare Heliocentric Julian start date"}, {"name": "Dur", "desc": "[0.016/0.3] Flare duration "}, {"name": "Amp", "desc": "[0.0003/1.5] Flare amplitude "}, {"name": "Teff", "desc": "[2620/6513]? Effective temperature "}, {"name": "Rad", "desc": "[0.12/91.5]? Stellar radius "}, {"name": "Energy", "desc": "? Flare energy; in erg units "}]}, {"name": "table5.dat", "desc": "Flare parameters of Kepler ", "columns": [{"name": "---", "desc": "[KIC] "}, {"name": "KIC", "desc": "Kepler identifier "}, {"name": "Peak", "desc": "[124/1589.5] Peak Heliocentric Julian Date of flare"}, {"name": "Start", "desc": "[124/1589.4] Flare Heliocentric Julian start date "}, {"name": "End", "desc": "[124/1589.5] Flare Heliocentric Julian start date "}, {"name": "Dur", "desc": "[0.005/1.17] Flare duration "}, {"name": "Amp", "desc": "[0.0002/0.6] Flare amplitude "}, {"name": "Teff", "desc": "[3068/27730] Effective temperature "}, {"name": "Rad", "desc": "[0.14/9.4] Stellar radius "}, {"name": "Energy", "desc": "[1.3e+31/1.9e+36] Flare energy; in erg units "}]}, {"name": "table6.dat", "desc": "Flare parameters of K2 ", "columns": [{"name": "---", "desc": "[EPIC] "}, {"name": "EPIC", "desc": "K2 identifier "}, {"name": "Peak", "desc": "[1983.8/3468.5] Peak Heliocentric Julian Date of flare"}, {"name": "Start", "desc": "[1983.7/3468.5] Flare Heliocentric Julian start date"}, {"name": "End", "desc": "[1983.98/3468.52] Flare Heliocentric Julian start date"}, {"name": "Dur", "desc": "[0.012/0.7] Flare duration "}, {"name": "Amp", "desc": "[0.0005/24.21] Flare amplitude "}, {"name": "Teff", "desc": "[2321/9746] Effective temperature "}, {"name": "Rad", "desc": "[0.1/78.7] Stellar radius "}, {"name": "Energy", "desc": "[2.48e+31/1.4e+39] Flare energy; in erg units "}]}, {"name": "table7.dat", "desc": "The revised parameters for exoplanet systems ", "columns": [{"name": "TIC", "desc": "[8767448/468987719] TESS identifier "}, {"name": "Planet", "desc": "Exoplanet identifier "}, {"name": "Ratio", "desc": "[0.01/0.38] Ratio of (R*+Rp)/orbital semi-major axis"}, {"name": "e_Ratio", "desc": "[0.0013/0.05] Uncertainty in Ratio "}, {"name": "Rp/R*", "desc": "[0.036/0.31] Planet to star radii ratio "}, {"name": "e_Rp/R*", "desc": "[0.00088/0.2] Uncertainty in Rp/R* "}, {"name": "Inc", "desc": "[78.9/89.8] Orbital inclination "}, {"name": "e_Inc", "desc": "[0.2/9] Uncertainty in Inc "}, {"name": "Per", "desc": "[0.78/17.01] Orbital period "}, {"name": "e_Per", "desc": "[1e-5/0.008] Uncertainty in Per "}, {"name": "Rp", "desc": "[5.39/24.1]? Exoplanet radius "}, {"name": "e_Rp", "desc": "[0.015/0.7]? Uncertainty in Rp "}, {"name": "t0", "desc": "[1325.37/2112.63] Minima time "}, {"name": "e_t0", "desc": "[0.00017/0.006] Uncertainty in t0 "}]}, {"name": "table8.dat", "desc": "Habitable exoplanet parameters ", "columns": [{"name": "ID", "desc": "Object identifier (EPIC, KIC or TIC numbers) "}, {"name": "Planet", "desc": "Exoplanet identifier "}, {"name": "Start", "desc": "[120.5/3418.6] Observation start time "}, {"name": "End", "desc": "[130.25/3469.5] Observation end time "}, {"name": "Dur", "desc": "[4.2/97.7] Observation duration "}, {"name": "Sum", "desc": "[17.69/1417] Total observation time on ID "}, {"name": "Rp", "desc": "[0.006/3500] Exoplanet radius "}, {"name": "Num", "desc": "[1/163] Number of flares observed "}, {"name": "ESum", "desc": "[1.5e+32/1.4e+39] Sum of all flare energy; in erg units"}, {"name": "S", "desc": "[9.3e-5/7350000] Flare energy flux density received by the planet of stars with multiple flares"}, {"name": "EFlux", "desc": "[449/60000000000000] Flare energy flux received by the planet of stars with single flare"}, {"name": "L?", "desc": "Livability judgement; (Y)es or (N)o "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_261_31"}} {"id": "J/ApJS/261/31", "title_cds": "COS Legacy Archive Sp. Survey (CLASSY) treasury", "title_create": "Berg+, 2022", "year": "2022", "author": "Berg D.A., James B.L., King T., McDonald M., Chen Z., Chisholm J., Heckman T., Martin C.L., Stark D.P., Aloisi A., Amorin R.O., Arellano-Cordova K.Z., Bayliss M., Bordoloi R., Brinchmann J., Charlot S., Chevallard J., Clark I., Erb D.K., Feltre A., Gronke M., Hayes M., Henry A., Hernandez S., Jaskot A., Jones T., Kewley L.J., Kumari N., Leitherer C., Llerena M., Maseda M., Mingozzi M., Nanayakkara T., Ouchi M., Plat A., Pogge R.W., Ravindranath S., Rigby J.R., Sanders R., Scarlata C., Senchyna P., Skillman E.D., Steidel C.C., Strom A.L., Sugahara Y., Wilkins S.M., Wofford A., Xu X., The CLASSY Team", "title_pub": "The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury atlas.", "first_author": "Berg D.A.", "ref_biblio": [""], "bibcode": ["2022ApJS..261...31B"], "see_also": ["II/311 : WISE All-Sky Data Release (Cutri+ 2012)", "V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)", "II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)", "II/335 : Revised catalog of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)", "V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)", "II/371 : The Dark Energy Survey (DES): Data Release 2 (Abott+, 2021)", "J/ApJS/178/247 : H{alpha} and [NII] survey in local 11 Mpc (Kennicutt+, 2008)", "J/ApJ/706/599 : H{alpha} and UV SFR in the local volume (Lee+, 2009)", "J/ApJS/190/233 : Spectroscopy & abundances of SINGS galaxies (Moustakas+, 2010)", "J/A+A/561/A64 : Mrk 996 optical spectroscopy (Telles+, 2014)", "J/ApJ/806/16 : CHemical Abundances of Spirals. I. NGC628 (Berg+, 2015)", "J/ApJS/219/8 : SFR for WISE + SDSS spectroscopic galaxies (Chang+, 2015)", "J/ApJ/814/L6 : CIII] emission in near & far star-forming gal. (Rigby+, 2015)", "J/A+A/608/A139 : 237 Lyman-alpha spectra of MUSE-Wide survey (Gronke, 2017)", "J/A+A/615/A78 : Spectral models for binary products (Goetberg+, 2018)", "J/AJ/155/104 : MEGaSaURA. I. The sample and the spectra (Rigby+, 2018)", "J/ApJ/869/123 : Keck Lyman continuum sp. survey (KLCS) (Steidel+, 2018)", "J/ApJ/893/96 : CHAOS IV: NGC3184 LBT obs. & 3 other gal. abund. (Berg+, 2020)", "J/A+A/654/A80 : MUSE Catalog of UV emission line measurement (Schmidt+, 2021)", "http://archive.stsci.edu/hlsp/classy : CLASSY home page"], "keyword_cds": "Spectra, ultraviolet; Spectra, optical; Galaxies, nearby; Redshifts; Abundances; Reddening", "keyword_pub": "Galaxies ; Ultraviolet surveys ; Emission line galaxies ; Interstellar line absorption ; Lyman-alpha galaxies ; High-redshift galaxies", "abstract": ["Far-ultraviolet (FUV; ~1200-2000{AA}) spectra are fundamental to our", "understanding of star-forming galaxies, providing a unique window on", "massive stellar populations, chemical evolution, feedback processes,", "and reionization. The launch of the James Webb Space Telescope will", "soon usher in a new era, pushing the UV spectroscopic frontier to", "higher redshifts than ever before; however, its success hinges on a", "comprehensive understanding of the massive star populations and gas", "conditions that power the observed UV spectral features. This requires", "a level of detail that is only possible with a combination of ample", "wavelength coverage, signal-to-noise, spectral-resolution, and sample", "diversity that has not yet been achieved by any FUV spectral database.", "We present the Cosmic Origins Spectrograph Legacy Spectroscopic Survey", "(CLASSY) treasury and its first high-level science product, the CLASSY", "atlas. CLASSY builds on the Hubble Space Telescope (HST) archive to", "construct the first high-quality (S/N_1500{AA}_>~5/resel),", "high-resolution (R~15000) FUV spectral database of 45 nearby", "(0.002~2", "galaxies. This unique set of properties makes the CLASSY atlas the", "benchmark training set for star-forming galaxies across cosmic time."], "description": ["The COS Legacy Archive Spectroscopy Survey (CLASSY) combines", "135 orbits of new HST data with 177 orbits of archival HST data, for a", "total of 312 orbits, to complete the first atlas of high-quality", "rest-FUV COS spectra of 45 local star-forming galaxies.", "In order to complete the FUV spectral coverage of the CLASSY sample,", "the archival observations were supplemented with 76 new HST/COS", "spectroscopic data sets of 42 galaxies, compiled over 135 orbits in", "Cycle 27 as part of PID 15840. These data consist of 27 G130M data", "sets, 5 G160M data sets, 29 G185M data sets, and 8 G225M data sets.", "Details of all individual data sets are provided in Table 2.", "High-quality optical spectra have been compiled for the entire CLASSY", "sample to ensure uniform determinations of galaxy properties.", "Initially, much of the sample was selected from the SDSS, and so", "archival SDSS spectra exist for 38 of the CLASSY galaxies. The", "exceptions are J0036-3333, J0127-0619, J0144+0453, J0337-0502,", "J0405-3648, J0934+5514, and J1444+4237. Instead, we use VLT/VIMOS", "integral field unit (IFU) from James+ (2009MNRAS.398....2J) for", "J0127-0619, MMT Blue Channel Spectrograph spectra from", "Senchyna+ (2019MNRAS.488.3492S) for J0144+0453 and J1444+4237,", "Keck/KCWI IFU spectra from Rickards Vaught+ (2021ApJ...911L..17R) for", "J0337-0502, and VLT/MUSE IFU spectra for the remaining four galaxies.", "To ensure robust direct T_e_ measurements for J0808+3948, J0944+3442,", "and J1545+0858, very high-S/N optical spectral were obtained using the", "Multi-Object Double Spectrographs (MODS) on the Large Binocular", "Telescope (LBT).", "We gathered additional optical spectra from archival VLT/MUSE IFU", "spectra and Keck/ESI spectra from R. L. Sanders et al. (2022, in", "preparation), and spectra that were prioritized over the SDSS spectra", "due to their superior S/N and spectral resolution.", "The details of the ancillary optical spectra adopted for the CLASSY", "sample are listed in Table 4.", "The SDSS provides optical imaging in ugriz for 42 galaxies in the", "CLASSY sample. For the other three, J0036-3333 and J0405-3648 have", "grizY images from the DES (Abbott+ 2021, II/371), and J0337-0502 is", "observed by the Pan-STARRS1 (Chambers+ 2016, II/349). For the UV, 43", "galaxies (all but J0337-0502 and J1157+3220) have imaging in the NUV", "and FUV available from GALEX (Martin+ 2005ApJ...619L...1M ; see II/335).", "Additionally, Wide-field Infrared Survey Explorer (WISE) W1 and W2", "near-infrared (NIR) data are also available for the entire CLASSY", "sample.", "See Appendix C."], "alias": ["CLASSY"], "type": ["OC"], "data": "a", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "CLASSY New+Archival HST/COS observations ", "columns": [{"name": "Seq", "desc": "[1/45] Internal target index number "}, {"name": "Name", "desc": "Galaxy identifier (JHHMM+DDMM) "}, {"name": "z", "desc": "[0.0016/0.182] Spectroscopic redshift "}, {"name": "PID", "desc": "[11523/15840]? HST Program ID (1) "}, {"name": "ImData", "desc": "Acquisition image dataset name "}, {"name": "ImExpT", "desc": "[0.6/510]? Acquisition image exposure time "}, {"name": "f_ImExpT", "desc": "NA = Not applicable "}, {"name": "ImMir", "desc": "[AB] Acquisition image mirror "}, {"name": "PA", "desc": "[1/355]? Position angle of aperture "}, {"name": "ImGFWHM", "desc": "[0.1/1.42]? GFWHM along spatial axis of acquisition image"}, {"name": "f_ImGFWHM", "desc": "NA = Not applicable "}, {"name": "SpData", "desc": "Spectrum dataset name "}, {"name": "Grating", "desc": "Spectrum grating "}, {"name": "clambda", "desc": "[1105/2339]? Spectrum central wavelength; in Angstrom units"}, {"name": "LP", "desc": "[1/4]? Spectrum lifetime position "}, {"name": "f_LP", "desc": "NA = Not applicable "}, {"name": "SpExpT", "desc": "[356/13852]? Spectrum exposure time "}, {"name": "lambdaSt", "desc": "[966.6/1889.3]? Starting rest wavelength (3) "}, {"name": "lambdaEnd", "desc": "[1221.7/2414.6]? Ending rest wavelength (3) "}]}, {"name": "table3.dat", "desc": "Nominal and measured spectral resolution of CLASSY coadded spectra", "columns": [{"name": "Name", "desc": "Galaxy identifier (JHHMM+DDMM) "}, {"name": "lambda", "desc": "Rest-frame wavelength; Angstroms "}, {"name": "VHR", "desc": "[11.6/14.3] Nominal resolution of the VHR spectrum in units of km/s per resolution element (1)"}, {"name": "HR", "desc": "[14.2/17.4] Nominal resolution of the HR spectrum in units of km/s per resolution element (1)"}, {"name": "MR", "desc": "[38.8/47.6] Nominal resolution of the MR spectrum in units of km/s per resolution element (1)"}, {"name": "LR", "desc": "[96.5/119.6] Nominal resolution of the LR spectrum in units of km/s per resolution element (1)"}, {"name": "Res", "desc": "[20/128] Resolution of measured absorption feature (2)"}]}, {"name": "table4.dat", "desc": "Ancillary optical spectra for the CLASSY galaxy sample", "columns": [{"name": "Name", "desc": "Galaxy identifier (JHHMM+DDMM) "}, {"name": "Inst", "desc": "Telescope/spectrograph of optical spectrum "}, {"name": "Ap", "desc": "Aperture size (1) "}, {"name": "ExpTime", "desc": "Cumulative exposure time "}, {"name": "Reference", "desc": "Reference for the observations "}, {"name": "FileName", "desc": "Name of the FITS file in subdirectory \"fits\"; column added by CDS"}]}, {"name": "table5.dat", "desc": "CLASSY galaxy spectroscopy-derived properties ", "columns": [{"name": "Seq", "desc": "[1/45] Internal target index number "}, {"name": "Name", "desc": "Galaxy identifier (JHHMM+DDMM) "}, {"name": "AName", "desc": "Alternate name(s) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "z", "desc": "[0.0016/0.182] Spectroscopic redshift "}, {"name": "F1500", "desc": "[0.69/16.6] Continuum flux at 1500{AA} from the CLASSY coadded spectra; in units of 10^-15^erg/s/cm^2^/{AA}"}, {"name": "Z", "desc": "[6.98/8.8] Direct method oxygen abundance (12+log (O/H))"}, {"name": "e_Z", "desc": "[0.01/11.4] Uncertainty in Z "}, {"name": "r_Z", "desc": "Ion temperature used to determine Z "}, {"name": "ne", "desc": "[10/910] Gas-hase electron density "}, {"name": "e_ne", "desc": "[10/160] Uncertainty in ne "}, {"name": "O32", "desc": "[0.5/38] The [OIII]5007{AA}/[OII]3727{AA} flux ratio"}, {"name": "e_O32", "desc": "[0.1/3] Uncertainty in O32 "}, {"name": "E(B-V)", "desc": "[0.039/0.5] Reddening value from Balmer decrement"}, {"name": "e_E(B-V)", "desc": "[0.004/0.07] Uncertainty in E (B-V) "}]}, {"name": "table6.dat", "desc": "CLASSY galaxy photometry-derived properties ", "columns": [{"name": "Seq", "desc": "[1/45] Internal target index number "}, {"name": "Name", "desc": "Target identifier (JHHMM+DDMM) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "z", "desc": "[0.0016/0.182] Spectroscopic redshift "}, {"name": "Dist", "desc": "[8/880] Luminosity distance (1) "}, {"name": "r50", "desc": "[0.7/7.3] Optical half light radius (2) "}, {"name": "MAper", "desc": "[4.9/10] COS aperture log stellar mass (3) "}, {"name": "E_MAper", "desc": "[0.12/0.6] Upper uncertainty in MAper "}, {"name": "e_MAper", "desc": "[0.09/0.5] Lower uncertainty in MAper "}, {"name": "MTot", "desc": "[6.2/10.1] Total log stellar mass for entire galaxy (3)"}, {"name": "E_MTot", "desc": "[0.15/0.51] Upper uncertainty in MTot "}, {"name": "e_MTot", "desc": "[0.1/0.42] Lower uncertainty in MTot "}, {"name": "SFRAper", "desc": "[-3.1/1.5] Within COS aperture log star formation rate (3)"}, {"name": "E_SFRAper", "desc": "[0.07/0.3] Upper uncertainty in SFRAper "}, {"name": "e_SFRAper", "desc": "[0.08/0.5] Lower uncertainty in SFRAper "}, {"name": "SFRTot", "desc": "[-2.1/1.6] Total log star formation rate for entire galaxy (3)"}, {"name": "E_SFRTot", "desc": "[0.07/0.7] Upper uncertainty in SFRTot "}, {"name": "e_SFRTot", "desc": "[0.07/0.65] Lower uncertainty in SFRTot "}]}, {"name": "fits/*", "desc": "Individual CLASSY HLSP galaxy spectrum in FITS format", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_261_32"}} {"id": "J/ApJS/261/32", "title_cds": "Finding GPQs. II. Spectroscopic data of 204 QSOs", "title_create": "Fu+, 2022", "year": "2022", "author": "Fu Y., Wu X.-B., Jiang L., Zhang Y., Huo Z.-Y., Ai Y.L., Yang Q., Ma Q., Feng X., Joshi R., Hon W.J., Wolf C., Li J.-T., Jin J.-J., Yao Su, Pang Y., Wang J.-G., Lu K.-X., Wang C.-J., Zheng J., Xu L., Yu X.-G., Lun B.-L., Zuo P.", "title_pub": "Finding quasars behind the Galactic plane. II. Spectroscopic identifications of 204 quasars at |b|<20{deg}.", "first_author": "Fu Y.", "ref_biblio": [""], "bibcode": ["2022ApJS..261...32F"], "see_also": ["VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)", "VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "I/323 : International Celestial Reference Frame 2, ICRF2 (Ma+, 2009)", "II/328 : AllWISE Data Release (Cutri+ 2013)", "V/146 : LAMOST DR1 catalogs (Luo+, 2015)", "II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)", "VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)", "J/AJ/131/2766 : Quasar luminosity function from SDSS-DR3 (Richards+, 2006)", "J/ApJS/165/1 : BAL QSOs from SDSS DR3 (Trump+, 2006)", "J/ApJ/701/508 : 5000 AGNs behind the Magellanic clouds (Kozlowski+, 2009)", "J/ApJS/180/67 : Phot. selection of quasars from SDSS. II. (Richards+, 2009)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/A+A/542/A110 : Neutral gas in the Milky Way halo (Ben Bekhti+, 2012)", "J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012)", "J/AJ/145/159 : LAMOST. II. ugriz photometry of 526 new quasars (Huo+, 2013)", "J/other/RAA/15.1438 : LAMOST new QSOs in M31 and M33 vicinity (Huo+, 2015)", "J/ApJ/825/126 : SEAMBHs. V. The third year (Du+, 2016)", "J/ApJS/241/34 : The SDSS Reverberation Mapping (SDSS-RM) project (Shen+, 2019)", "J/ApJS/249/17 : SDSS QSO DR14 spectral properties (Rakshit+, 2020)", "J/ApJS/254/6 : Finding QSOs behind the Galactic Plane. I. (Fu+, 2021)"], "keyword_cds": "QSOs; Galactic plane; Redshifts; Spectra, optical; Photometry, VRI; Black holes; Equivalent widths; Line Profiles", "keyword_pub": "Active galactic nuclei ; Catalogs ; Supermassive black holes ; Galactic and extragalactic astronomy ; Quasars ; Spectroscopy", "abstract": ["Quasars behind the Galactic plane (GPQs) are important astrometric", "references and valuable probes of Galactic gas, yet the search for", "GPQs is difficult due to severe extinction and source crowding in the", "Galactic plane. In this paper, we present a sample of 204", "spectroscopically confirmed GPQs at |b|<20{deg}, 191 of which are", "new discoveries. This GPQ sample covers a wide redshift range from", "0.069 to 4.487. For the subset of 230 observed GPQ candidates, the", "lower limit of the purity of quasars is 85.2%, and the lower limit of", "the fraction of stellar contaminants is 6.1%. Using a multicomponent", "spectral fitting, we measure the emission line and continuum flux of", "the GPQs, and estimate their single-epoch virial black hole masses.", "Due to selection effects raised from Galactic extinction and target", "magnitude, these GPQs have higher black hole masses and continuum", "luminosities in comparison to the SDSS DR7 quasar sample. The", "spectral-fitting results and black hole mass estimates are compiled", "into a main spectral catalog, and an extended spectral catalog of", "GPQs. The successful identifications prove the reliability of both our", "GPQ selection methods and the GPQ candidate catalog, shedding light on", "the astrometric and astrophysical programs that make use of a large", "sample of GPQs in the future."], "description": ["Spectroscopic observations for quasar behind the Galactic plane (GPQ)", "candidates have been carried out with five telescopes in China, USA,", "and Australia since 2018. A total of 243 GPQ candidates have been", "observed until 2021 May, 230 of which are selected from the GPQ", "candidate catalog in Paper I (Fu+ 2021, J/ApJS/254/6).", "The Xinglong 2.16m Telescope (XLT) is an equatorial mount reflector at", "Xinglong Observatory, National Astronomical Observatories, Chinese", "Academy of Sciences. Since 2018, we have been using the Beijing Faint", "Object Spectrograph and Camera on XLT to identify GPQ candidates with", "low-resolution spectroscopy (R=265 at 5007{AA}).", "The Lijiang 2.4m Telescope (LJT) is an altitude-azimuth mount", "reflector operated by Lijiang Observatory, Yunnan Observatories,", "Chinese Academy of Sciences. The instrument we use is the Yunnan Faint", "Object Spectrograph and Camera on LJT (R~250 at 6030{AA}).", "The 200 inch (5.3m) Hale Telescope (P200) is operated by Palomar", "Observatory. The Double Spectrograph (DBSP) has been used for the", "observations (R~900 at central wavelengths of blue (2500-5700{AA}) and", "red (4800-10700{AA}) channels).", "The 2.3m telescope (ANU23) at Siding Spring Observatory is operated by", "the Australian National University. For all observations, we use the", "Wide-Field Spectrograph (R~3000, ~3300-9000{AA}).", "The McGraw-Hill 1.3m Telescope (MDM13) is operated by the MDM", "Observatory, which is located adjacent to the Kitt Peak National", "Observatory. We use the Boller and Chivens CCD Spectrograph", "(resolution of ~4.4{AA}/pixel).", "Throughout this paper we adopt a flat {Lambda}CDM cosmology with", "{Omega}_{Lambda}_=0.7 and h=0.7."], "alias": ["GPQ GPQC"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "tablea1.dat", "desc": "Main spectral catalog of the 204 identified quasars behind the Galactic plane (GPQs)", "columns": [{"name": "Name", "desc": "Designation (JHHMMSS.ss+DDMMSS.s based on PS1) (G1)"}, {"name": "GLON", "desc": "[6.8/355] Galactic longitude "}, {"name": "GLAT", "desc": "[-19.9/19.9] Galactic latitude "}, {"name": "imag", "desc": "[15.51/19.91] Mean PSF AB magnitude from PS1 i-filter detections"}, {"name": "z", "desc": "[0.068/4.5] Redshift from visual inspection "}, {"name": "logL1350", "desc": "[46.16/48.01]?=-999 Log, continuum luminosity at rest-frame 1350{AA}, in erg/s units (G3)"}, {"name": "e_logL1350", "desc": "[0.002/0.04]?=-999 Measurement error in logL1350 (G3)"}, {"name": "logL3000", "desc": "[44.8/48.41]?=-999 Log, continuum luminosity at rest-frame 3000{AA}, erg/s"}, {"name": "e_logL3000", "desc": "[0.001/0.06]?=-999 Measurement error in logL3000"}, {"name": "logL5100", "desc": "[42.88/46]?=-999 Log, continuum luminosity at rest-frame 5100{AA}, erg/s"}, {"name": "e_logL5100", "desc": "[0.002/0.04]?=-999 Measurement error in logL5100"}, {"name": "logBHHb", "desc": "[7.3/9.4]?=-999 Log, single-epoch virial BH mass based on H{beta}"}, {"name": "e_logBHHb", "desc": "[0.012/0.5]?=-999 Uncertainty in logBH-HB "}, {"name": "logBHMgII", "desc": "[8.13/10.62]?=-999 Log, single-epoch virial BH mass based on MgII"}, {"name": "e_logBHMgII", "desc": "[0.0009/0.64]?=-999 Uncertainty in logBHMgII"}, {"name": "logBHCIV", "desc": "[9.1/10.52]?=-999 Log, single-epoch virial BH mass based on CIV (G3)"}, {"name": "e_logBHCIV", "desc": "[0.025/0.34]?=-999 Uncertainty in logBHCIV (G3)"}, {"name": "Tel", "desc": "Telescope used to acquire the spectrum (G4) "}]}, {"name": "tablea2.dat", "desc": "Extended spectral catalog of the 204 identified GPQs ", "columns": [{"name": "Name", "desc": "Designation (JHHMMSS.ss+DDMMSS.s based on PS1) (G1)"}, {"name": "RAdeg", "desc": "PS1 Right Ascension (J2000) (G2) "}, {"name": "DEdeg", "desc": "PS1 Declination (J2000) (G2) "}, {"name": "GLON", "desc": "[6.8/355] Galactic longitude "}, {"name": "GLAT", "desc": "[-20/20] Galactic latitude "}, {"name": "imag", "desc": "[15.51/19.91] Mean PSF AB magnitude from PS1 i-filter detections"}, {"name": "EBV", "desc": "[0.029/0.7] Line-of-sight E(B-V) given by the Planck (2014A&A...571A..11P) dust map"}, {"name": "z", "desc": "[0.068/4.5] Redshift from visual inspection"}, {"name": "iMAG2", "desc": "[-31/-21] SDSS i-band absolute magnitude M_i(z=2), K-corrected to z=2"}, {"name": "MJD", "desc": "[58252.77/59345.88] Modified Julian Date of spectroscopic observation (JD-2400000.5)"}, {"name": "Tel", "desc": "Telescope used to acquire the spectrum (G4)"}, {"name": "SNRSp", "desc": "[1.4/41] Median S/N per pixel of the spectrum"}, {"name": "logL1350", "desc": "[46/48.1]?=-999 Log, continuum luminosity at rest-frame 1350{AA}, in erg/s units (G3)"}, {"name": "e_logL1350", "desc": "[0.002/0.04]?=-999 Measurement error in logL1350 (G3)"}, {"name": "logL3000", "desc": "[44.8/48.41]?=-999 Log, continuum luminosity at rest-frame 3000{AA}, erg/s"}, {"name": "e_logL3000", "desc": "[0.001/0.06]?=-999 Measurement error in logL3000"}, {"name": "logL5100", "desc": "[42.88/46]?=-999 Log, continuum luminosity at rest-frame 5100{AA}, erg/s"}, {"name": "e_logL5100", "desc": "[0.002/0.04]?=-999 Measurement error in logL5100"}, {"name": "logBHHb", "desc": "[7.33/9.4]?=-999 Log, single-epoch virial BH mass based on H{beta}"}, {"name": "e_logBHHb", "desc": "[0.012/0.5]?=-999 Uncertainty in logBHHb"}, {"name": "logBHMgII", "desc": "[8.13/10.62]?=-999 Log, single-epoch virial BH mass based on MgII"}, {"name": "e_logBHMgII", "desc": "[0.0009/0.7]?=-999 Uncertainty in logBHMgII"}, {"name": "logBHCIV", "desc": "[9.1/10.52]?=-999 Log, single-epoch virial BH mass based on CIV (G3)"}, {"name": "e_logBHCIV", "desc": "[0.02/0.4]?=-999 Uncertainty in logBHCIV (G3)"}, {"name": "FenormUV", "desc": "[0.07/239]?=-999 Normalization factor of the ultraviolet FeII template"}, {"name": "FeShiftUV", "desc": "[-0.01/0.01]?=-999 Wavelength shift of the ultraviolet FeII template"}, {"name": "FeFWHMUV", "desc": "[1200/10000]?=-999 Gaussian FWHM applied to convolve the ultraviolet FeII"}, {"name": "FenormOp", "desc": "[0.38/755]?=-999 Normalization factor of the optical FeII template"}, {"name": "FeShiftOp", "desc": "[-0.01/0.01]?=-999 Wavelength shift of the optical FeII template"}, {"name": "FeFWHMOp", "desc": "[1200/10000]?=-999 Gaussian FWHM applied to convolve the optical FeII template"}, {"name": "PLnorm", "desc": "[0.06/10397]?=-999 Normalization factor of the power-law model, in 10^-17^erg/s/cm2/{AA}"}, {"name": "PLalpha", "desc": "[-5/3]?=-999 Wavelength power-law index"}, {"name": "PolyA", "desc": "[-4.2/4.8]?=-999 Efficient of the three-order polynomial model (b1)"}, {"name": "PolyB", "desc": "[-0.007/0.004]?=-999 Efficient of the three-order polynomial model (b2)"}, {"name": "PolyC", "desc": "[-3.4e-7/3.3e-6]?=-999 Efficient of the three-order polynomial model (b3)"}, {"name": "NpixCIV", "desc": "[134/946]?=-999 Number of good pixels for the rest-frame 1500-1700{AA}"}, {"name": "StCIV", "desc": "[1/5]?=-999 Line-fitting status of CIV"}, {"name": "SNCIV", "desc": "[1.6/33.4]?=-999 Median S/N per pixel for the rest-frame 1500-1700{AA}"}, {"name": "FWHMCIV", "desc": "[3135/13615]?=-999 FWHM of the whole CIV"}, {"name": "e_FWHMCIV", "desc": "[148/3100]?=-999 Measurement error in FWHMCIV"}, {"name": "EWCIV", "desc": "[10/91]?=-999 Rest-frame equivalent width of the whole CIV"}, {"name": "e_EWCIV", "desc": "[0.4/12]?=-999 Measurement error in EWCIV"}, {"name": "FCIV", "desc": "[259/789498]?=-999 FLUX of the whole CIV, 10-^17^erg/s/cm2"}, {"name": "e_FCIV", "desc": "[17/47653]?=-999 Measurement error in FCIV"}, {"name": "NpixCIII", "desc": "[56/1159]?=-999 Number of good pixels for the rest-frame 1700-1970{AA}"}, {"name": "StCIII", "desc": "[1/2]?=-999 Line-fitting status of CIII"}, {"name": "SNCIII", "desc": "[0.29/35]?=-999 Median S/N per pixel for the rest-frame 1700-1970{AA}"}, {"name": "FWHMCIII", "desc": "[2826/14449]?=-999 FWHM of the whole CIII"}, {"name": "e_FWHMCIII", "desc": "[48/4223]?=-999 Measurement error in FWHMCIII"}, {"name": "EWCIII", "desc": "[2/71]?=-999 Rest-frame equivalent width of the whole CIII"}, {"name": "e_EWCIII", "desc": "[0.36/8.6]?=-999 Measurement error in EWCIII"}, {"name": "FCIII", "desc": "[148/254655]?=-999 FLUX of the whole CIII, 10^-17^erg/s/cm2"}, {"name": "e_FCIII", "desc": "[26/16181]?=-999 Measurement error in FCIII"}, {"name": "NpixMgII", "desc": "[47/730]?=-999 Number of good pixels for the rest-frame 2700-2900{AA}"}, {"name": "StMgII", "desc": "[1/5]?=-999 Line-fitting status of MgII"}, {"name": "SNMedMgII", "desc": "[0.5/42]?=-999 Median S/N per pixel for the rest-frame 2700-2900{AA}"}, {"name": "FWHMbMgII", "desc": "[1622/10609]?=-999 FWHM of the whole broad MgII"}, {"name": "e_FWHMbMgII", "desc": "[12/2826]?=-999 Measurement error in FWHMbMgII"}, {"name": "EWbMgII", "desc": "[8/107]?=-999 Rest-frame equivalent width of the whole broad MgII"}, {"name": "e_EWbMgII", "desc": "[0.4/5.4]?=-999 Measurement error in EWbMgII"}, {"name": "FbMgII", "desc": "[306/403613]?=-999 Flux of the whole broad MgII, 10^-17^erg/s/cm2"}, {"name": "e_FbMgII", "desc": "[21/38994]?=-999 Measurement error in FbMgII"}, {"name": "FWHMnMgII", "desc": "[351/1206]?=-999 FWHM of Narrow MgII"}, {"name": "e_FWHMnMgII", "desc": "[0.007/407]?=-999 Measurement error in FWHMnMgII"}, {"name": "EWnMgII", "desc": "[0.0016/9.42]?=-999 Rest-frame equivalent width of Narrow MgII"}, {"name": "e_EWnMgII", "desc": "[0.08/4]?=-999 Measurement error in EWnMgII"}, {"name": "FnMgII", "desc": "[0.39/5375]?=-999 Flux of Narrow MgII, 10^-17^erg/s/cm2"}, {"name": "e_FnMgII", "desc": "[5/8513]?=-999 Measurement error in FnMgII"}, {"name": "NpixHb", "desc": "[140/1065]?=-999 Number of good pixels for the rest-frame 4640-5100{AA}"}, {"name": "StHb", "desc": "[1/5]?=-999 Line-fitting status of 4640-5100{AA}"}, {"name": "SNMedHb", "desc": "[3.7/43.2]?=-999 Median S/N per pixel for the res t-frame 4640-5100{AA}"}, {"name": "FWHMbHb", "desc": "[2826/15493]?=-999 FWHM of broad Hbeta"}, {"name": "e_FWHMbHb", "desc": "[33/3623]?=-999 Measurement error in FWHMbHb"}, {"name": "EWbHb", "desc": "[6/361]?=-999 Rest-frame equivalent width of broad Hbeta"}, {"name": "e_EWbHb", "desc": "[1/39]?=-999 Measurement error in EWbHb"}, {"name": "FbHb", "desc": "[100/135788]?=-999 Flux of broad Hbeta, 10-17erg/s/cm2"}, {"name": "e_FbHb", "desc": "[43/25315]?=-999 Measurement error in FbHb"}, {"name": "FWHMnHb", "desc": "[168/1204]?=-999 FWHM of narrow Hbeta"}, {"name": "e_FWHMnHb", "desc": "[14/371]?=-999 Measurement error in FWHMnHb"}, {"name": "EWnHb", "desc": "[0.28/37]?=-999 Rest-frame equivalent width of narrow Hbeta"}, {"name": "e_EWnHb", "desc": "[0.19/9]?=-999 Measurement error in EWnHb"}, {"name": "FnHb", "desc": "[4/7991]?=-999 Flux of narrow Hbeta, 10-17erg/s/cm2"}, {"name": "e_FnHb", "desc": "[11.9/2879]?=-999 Measurement error in FnHb"}, {"name": "FWHMOIII4959", "desc": "[258.9/2284]?=-999 FWHM of [OIII]MgII4959"}, {"name": "e_FWHMOIII4959", "desc": "[0.78/767]?=-999 Measurement error in FWHMOIII4959"}, {"name": "EWOIII4959", "desc": "[0.6/42]?=-999 Rest-frame equivalent width of [OIII]MgII4959"}, {"name": "e_EWOIII4959", "desc": "[0.2/8]?=-999 Measurement error in EWOIII4959"}, {"name": "FOIII4959", "desc": "[14.8/3551]?=-999 Flux of [OIII]MgII4959, 10^-17^erg/s/cm2"}, {"name": "e_FOIII4959", "desc": "[11/2439]?=-999 Measurement error in FOIII4959"}, {"name": "FWHMOIII5007", "desc": "[336/1954]?=-999 FWHM of [OIII]MgII5007"}, {"name": "e_FWHMOIII5007", "desc": "[0.7/694]?=-999 Measurement error in FWHMOIII5007"}, {"name": "EWOIII5007", "desc": "[1/21152]?=-999 Rest-frame equivalent width of [OIII]MgII5007"}, {"name": "e_EWOIII5007", "desc": "[0.2/23816586]?=-999 Measurement error in EWOIII5007"}, {"name": "FOIII5007", "desc": "[10/371363]?=-999 Flux of [OIII]MgII5007, 10-17erg/s/cm2"}, {"name": "e_FOIII5007", "desc": "[10/415655263]?=-999 Measurement error in FOIII5007"}, {"name": "NpixHa", "desc": "[138/421]?=-999 Number of good pixels for the rest-frame 6400-6800{AA}"}, {"name": "StHa", "desc": "[1/5]?=-999 Line-fitting status of H{alpha}"}, {"name": "SNMedHa", "desc": "[7.5/36]?=-999 Median S/N per pixel for the rest-frame 6400-6800{AA}"}, {"name": "FWHMbHa", "desc": "[2820/10166]?=-999 FWHM of broad H{alpha}"}, {"name": "e_FWHMbHa", "desc": "[231/984]?=-999 Measurement error in FWHMbHa"}, {"name": "EWbHa", "desc": "[16.8/2578644]?=-999 Rest-frame equivalent width of broad H{alpha}"}, {"name": "e_EWbHa", "desc": "[9/557576]?=-999 Measurement error in EWbHa"}, {"name": "FbHa", "desc": "[82/57519]?=-999 Flux of broad H{alpha}, 10-17erg/s/cm2"}, {"name": "e_FbHa", "desc": "[33.9/11765]?=-999 Measurement error in FbHa"}, {"name": "FWHMnHa", "desc": "[353/1205]?=-999 FWHM of narrow H{alpha}"}, {"name": "e_FWHMnHa", "desc": "[0.14/349]?=-999 Measurement error in FWHMnHa"}, {"name": "EWnHa", "desc": "[0.59/51230]?=-999 Rest-frame equivalent width of narrow H{alpha}"}, {"name": "e_EWnHa", "desc": "[4.8/481024]?=-999 Measurement error in EWnHa"}, {"name": "FnHa", "desc": "[22/47532]?=-999 Flux of narrow H{alpha}, 10-17erg/s/cm2"}, {"name": "e_FnHa", "desc": "[11/6961]?=-999 Measurement error in FnHa"}, {"name": "FWHMNII6549", "desc": "[353/1205]?=-999 FWHM of [NII]6549"}, {"name": "e_FWHMNII6549", "desc": "[0.4/348]?=-999 Measurement error in FWHMNII6549"}, {"name": "EWNII6549", "desc": "[2.7/1816]?=-999 Rest-frame equivalent width of [NII]6549"}, {"name": "e_EWNII6549", "desc": "[2.8/3583]?=-999 Measurement error in EWNII6549"}, {"name": "FNII6549", "desc": "[40/11937]?=-999 Flux of [NII]6549, 10-17erg/s/cm2"}, {"name": "e_FNII6549", "desc": "[8/4359]?=-999 Measurement error in FNII6549"}, {"name": "FWHMNII6585", "desc": "[453/1205]?=-999 FWHM of [NII]6585"}, {"name": "e_FWHMNII6585", "desc": "[0.14/304]?=-999 Measurement error in FWHMNII6585"}, {"name": "EWNII6585", "desc": "[1.8/1038]?=-999 Rest-frame equivalent width of [NII]6585"}, {"name": "e_EWNII6585", "desc": "[4/570]?=-999 Measurement error in EWNII6585"}, {"name": "FNII6585", "desc": "[187/15319]?=-999 Flux of [NII]6585, 10^-17^erg/s/cm2"}, {"name": "e_FNII6585", "desc": "[12/3455]?=-999 Measurement error in FNII6585"}, {"name": "FWHMSII6718", "desc": "[353/1204]?=-999 FWHM of [SII] "}, {"name": "e_FWHMSII6718", "desc": "[0.15/364]?=-999 Measurement error in FWHMSII6718"}, {"name": "EWSII6718", "desc": "[0.4/166]?=-999 Rest-frame equivalent width of [SII]MgII6718"}, {"name": "e_EWSII6718", "desc": "[1/57]?=-999 Measurement error in EWSII6718"}, {"name": "FSII6718", "desc": "[12/1282]?=-999 Flux of [SII]MgII6718, 10^-17^erg/s/cm2"}, {"name": "e_FSII6718", "desc": "[5/440]?=-999 Measurement error in FSII6718"}, {"name": "FWHMSII6732", "desc": "[453/1205]?=-999 FWHM of [SII]MgII6732"}, {"name": "e_FWHMSII6732", "desc": "[0.14/330]?=-999 Measurement error in FWHMSII6732"}, {"name": "EWSII6732", "desc": "[0.29/55]?=-999 Rest-frame equivalent width of [SII]MgII6732"}, {"name": "e_EWSII6732", "desc": "[0.7/25]?=-999 Measurement error in EWSII6732"}, {"name": "FSII6732", "desc": "[33/516]?=-999 Flux of [SII]MgII6732, 10^-17^erg/s/cm2"}, {"name": "e_FSII6732", "desc": "[5/283]?=-999 Measurement error in FSII6732"}]}, {"name": "tablec1.dat", "desc": "List of the stellar and galaxy contaminants ", "columns": [{"name": "Name", "desc": "Designation (JHHMMSS.ss+DDMMSS.s) (G1) "}, {"name": "RAdeg", "desc": "[2.3/300] PS1 right ascension (J2000) (G2) "}, {"name": "DEdeg", "desc": "[4.4/62.1] PS1 declination (J2000) (G2) "}, {"name": "GLON", "desc": "[80.3/212.5] Galactic longitude "}, {"name": "GLAT", "desc": "[-3.9/17] Galactic latitude "}, {"name": "imag", "desc": "[15.12/19.65] Mean PSF AB magnitude from PS1 i-filter detections"}, {"name": "Class", "desc": "Class (\"star\" or \"galaxy\") "}, {"name": "z", "desc": "[0.04/0.11]?=0 Redshift from visual inspection "}, {"name": "MJD", "desc": "[58252.85/59229.3] Modified Julian Date of spectroscopic observation (JD-2400000.5)"}, {"name": "Tel", "desc": "Telescope "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_261_33"}} {"id": "J/ApJS/261/33", "title_cds": "Phot. metallicity prediction of RR Lyrae stars", "title_create": "Dekany+, 2022", "year": "2022", "author": "Dekany I., Grebel E.K.", "title_pub": "Photometric metallicity prediction of fundamental-mode RR Lyrae stars in the Gaia optical and Ks infrared wave bands by deep learning.", "first_author": "Dekany I.", "ref_biblio": [""], "bibcode": ["2022ApJS..261...33D"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/AJ/108/1016 : Kinematics of local RR lyrae stars. I. (Layden, 1994)", "J/AJ/110/2319 : Abundances in RR Lyr variables (Clementini+ 1995)", "J/A+A/312/111 : [Fe/H] from RR Lyrae light curves (Jurcsik+, 1996)", "J/ApJS/197/29 : Chemical compositions of 11 RR Lyrae (For+, 2011)", "J/ApJ/782/59 : Abundances of 8 RR Lyrae subclass C stars (Govea+, 2014)", "J/MNRAS/447/2404 : Equivalent width of 21 RR Lyrae stars (Pancino+, 2015)", "J/MNRAS/466/2602 : Blazhko effect in Galactic RR Lyrae (Prudil+, 2017)", "J/ApJ/848/68 : Abund. & RVs of stable and Blazhko RRc stars (Sneden+, 2017)", "J/ApJ/857/54 : JHKs photometry of VVV RR Lyrae stars (Dekany+, 2018)", "J/MNRAS/478/4590 : Light curves of RR Lyrae variables in M31 (Tanakul+, 2018)", "J/A+A/622/A60 : Gaia DR2 misclassified RR Lyrae list (Clementini+, 2019)", "J/ApJ/898/46 : NIR LCs of RRab stars from the VVV survey (Dekany+, 2020)", "J/ApJ/908/20 : Field RR Lyrae as galactic probes. II. (Crestani+, 2021)", "http://ogledb.astrouw.edu.pl/~ogle/OCVS/ : OCVS home page"], "keyword_cds": "Stars, variable; Abundances, [Fe/H]; Photometry, UBVRI; Surveys; Models", "keyword_pub": "RR Lyrae variable stars ; Metallicity ; Light curves ; Neural networks", "abstract": ["RR Lyrae stars are useful chemical tracers thanks to the empirical", "relationship between their heavy-element abundance and the shape of", "their light curves. However, the consistent and accurate calibration", "of this relation across multiple photometric wave bands has been", "lacking. We have devised a new method for the metallicity estimation", "of fundamental-mode RR Lyrae stars in the Gaia optical G and", "near-infrared VISTA Ks wave bands by deep learning. First, an existing", "metallicity prediction method is applied to large photometric data", "sets, which are then used to train long short-term memory recurrent", "neural networks for the regression of the [Fe/H] to the light curves", "in other wave bands. This approach allows an unbiased transfer of our", "accurate, spectroscopically calibrated I-band formula to additional", "bands at the expense of minimal additional noise. We achieve a low", "mean absolute error of 0.1 dex and high R2 regression performance of", "0.84 and 0.93 for the Ks and G bands, respectively, measured by", "cross-validation. The resulting predictive models are deployed on the", "Gaia DR2 and VVV inner bulge RR Lyrae catalogs. We estimate mean", "metallicities of -1.35dex for the inner bulge and -1.7dex for the", "halo, which are significantly less than the values obtained by earlier", "photometric prediction methods. Using our results, we establish a", "public catalog of photometric metallicities of over 60,000 Galactic", "RR Lyrae stars and provide an all-sky map of the resulting RR Lyrae", "metallicity distribution. The software code used for training and", "deploying our recurrent neural networks is made publicly available in", "the open-source domain."], "type": ["MC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "*I-band photometric parameters and metallicities of RRab stars in the bulge and disk areas of the OGLE Collection of Variable Stars (OCVS)", "columns": [{"name": "Field", "desc": "Field identifier (1) "}, {"name": "ID", "desc": "[1/68197] Object identifier within the Field (1) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "[Fe/H]", "desc": "[-8.7/3.2] Metallicity estimate "}, {"name": "Imag", "desc": "[10.78/21.3] Mean I band magnitude "}, {"name": "Nep", "desc": "[16/15016] Number of epochs in the light curve "}, {"name": "Per", "desc": "[0.27/1] Period "}, {"name": "Atot", "desc": "[0.016/1.2] Total (peak-to-valley) amplitude "}, {"name": "A1", "desc": "[0.006/0.5] The A_1_ Fourier parameter "}, {"name": "A2", "desc": "[0.001/0.3] The A_2_ Fourier parameter "}, {"name": "A3", "desc": "[0/0.2] The A_3_ Fourier parameter "}, {"name": "phi21", "desc": "[5.16/10.5] The {phi}_21_ Fourier parameter "}, {"name": "phi31", "desc": "[2.7/9.1] The {phi}_31_ Fourier parameter "}, {"name": "Cphi", "desc": "[0.8/1] Phase coverage (1-maximum phase lag) "}, {"name": "S/N", "desc": "[50/8796] Signal-to-Noise "}]}, {"name": "table4.dat", "desc": "G-band photometric metallicity estimates and basic light-curve attributes of Gaia DR2 RRab stars", "columns": [{"name": "Gaia", "desc": "Gaia DR2 source identifier "}, {"name": "[Fe/H]", "desc": "[-3.1/-0.06] Mean Metallicity prediction from a model ensemble"}, {"name": "e_[Fe/H]", "desc": "[0.01/0.8] Standard deviation of [Fe/H] "}, {"name": "Gmag", "desc": "[9.4/21] Mean Gaia DR2 G band magnitude "}, {"name": "Nep", "desc": "[21/247] Number of epochs in the light curve "}, {"name": "Per", "desc": "[0.3/0.98] Period "}, {"name": "Atot", "desc": "[0.12/1.4] Total (peak-to-valley) amplitude "}, {"name": "Cphi", "desc": "[0.85/1] Phase coverage (1-maximum phase lag) "}, {"name": "S/N", "desc": "[30/5443] Signal-to-Noise "}]}, {"name": "table5.dat", "desc": "K_S_-band photometric metallicity estimates and basic light-curve attributes of the VVV bulge RRab stars discovered by Dekany & Grebel (2020, J/ApJ/898/46)", "columns": [{"name": "[DG2020]", "desc": "[7/13250] Dekany & Grebel 2020, J/ApJ/898/46 identifier"}, {"name": "RAh", "desc": "[17/18] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "[Fe/H]", "desc": "[-2.6/-0.06] Metallicity estimate from a model ensemble"}, {"name": "e_[Fe/H]", "desc": "[0.008/0.5] Standard deviation of [Fe/H] "}, {"name": "Ksmag", "desc": "[12/16.3] Mean K_S_ band magnitude "}, {"name": "Nep", "desc": "[33/469] Number of epochs in the light curve "}, {"name": "Per", "desc": "[0.29/0.98] Period "}, {"name": "Atot", "desc": "[0.058/0.7] Total (peak-to-valley) amplitude "}, {"name": "Cphi", "desc": "[0.8/0.99] Phase coverage (1-maximum phase lag) "}, {"name": "S/N", "desc": "[30.4/272] Signal-to-Noise "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_261_34"}} {"id": "J/ApJS/261/34", "title_cds": "Bulge-disk decomposition of H-KPAIR sample", "title_create": "He+, 2022", "year": "2022", "author": "He C., Xu C.K., Domingue D., Cao C., Huang J.-S.", "title_pub": "Close major-merger pairs at z=0: bulge-to-total ratio and star formation enhancement.", "first_author": "He C.", "ref_biblio": [""], "bibcode": ["2022ApJS..261...34H"], "see_also": ["VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "J/ApJS/142/1 : DEEP Groth Strip Survey. II. (Simard+, 2002)", "J/ApJ/713/330 : Spitzer observations of major-merger galaxies (Xu+, 2010)", "J/MNRAS/415/32 : COLD GASS survey (Saintonge+, 2011)", "J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies (Simard+, 2011)", "J/MNRAS/446/3943 : galaxies 2D phot. decompositions in SDSS-DR7 (Meert+, 2015)", "J/ApJS/222/16 : Major-merger pairs of z<0.1 gal. with Herschel (Cao+, 2016)", "J/ApJ/829/78 : Dust properties of major-merger gal. pairs (Domingue+, 2016)", "J/MNRAS/455/2440 : Gal. 2D phot. decompositions in r, g & i (Meert+, 2016)", "J/A+A/627/A107 : CO obs. of major merger pairs at z=0 (Lisenfeld+, 2019)"], "keyword_cds": "Galaxies, IR; Models; Morphology; Photometry; Optical; Redsfhits", "keyword_pub": "Galaxy evolution ; Galaxy interactions ; Galaxy structure ; Star formation", "abstract": ["We present a study of the bulge-to-total ratio (B/T) of a", "Ks-band-selected sample of 88 close major-merger pairs of galaxies", "(H-KPAIR), based on two-dimensional decompositions of SDSS r-band", "images with GALFIT. We investigate the dependence of the", "interaction-induced specific star formation rate enhancement", "(sSFR_enh_) on the B/T ratio, and the effects of this dependence on", "the differences between star-forming galaxies (SFGs) in spiral+spiral", "(S+S) and spiral+elliptical (S+E) pairs. Of all the 132 spiral", "galaxies in H-KPAIR, the 44 in S+E pairs show higher B/T than those in", "the 44 S+S pairs, with means of B/T=0.35+/-0.05 and B/T=0.26+/-0.03,", "respectively. There is a strong negative dependence of sSFRenh on the", "B/T ratio, and only paired SFGs with B/T<0.3 show significant", "(>5{sigma}) enhancement. Paired SFGs in S+S pairs show a similar", "trend, and many disky SFGs (B/T<0.1) in S+S pairs have strong sSFR", "enhancements (sSFR_enh_>0.7dex). For SFGs in S+E pairs, the sSFR has", "no clear B/T dependence, nor any significant enhancement in any B/T", "bin. Disky SFGs in S+S pairs show significant (>4{sigma}) enhancement", "in molecular gas content (M_H2_/M_star_), while SFGs in S+E pairs have", "no such enhancement in any B/T bin. No significant enhancement of the", "total gas content (M_gas_/M_star_) is found in any B/T bin for paired", "galaxies. The star formation efficiency of either the total gas", "(SFE_gas_=SFR/M_gas_) or molecular gas (SFE_H2_=SFR/M_H2_) does not", "depend on the B/T ratio. The only significant (>4{sigma}) SFE", "enhancement found for paired SFGs is the SFEgas for disky SFGs in S+S", "pairs."], "alias": ["H-KPAIR"], "type": ["MC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table1.dat", "desc": "GALFIT results of 2MASX Ks-band-selected close major-merger galaxy pair sample (H-KPAIR)", "columns": [{"name": "GIDp", "desc": "Galaxy name (JHHMMSSss+DDMMSSs) from Cao+ 2016, J/ApJS/222/16"}, {"name": "z", "desc": "[0.0065/0.091] Redshift (after the correction for Virgocentric flow)"}, {"name": "Morph", "desc": "Galaxy morphology (1) "}, {"name": "mISO", "desc": "[11.85/16.55] Magnitude from SExtractor 25mag/arcsec^2^ isophot or polygon aperture"}, {"name": "mGAL", "desc": "[11.47/16.69] Model magnitude from GALFIT (2) "}, {"name": "B/T", "desc": "[0/1] Bulge-to-total ratio "}, {"name": "mB", "desc": "[12.57/22.31] Bulge magnitude "}, {"name": "nB", "desc": "[1/8] bulge Sersic index "}, {"name": "re", "desc": "[0/34.4] Bulge effective radius (3) "}, {"name": "b/aB", "desc": "[0.02/0.98] Bulge axis ratio "}, {"name": "PAB", "desc": "[-89.8/89.8] Bulge position angle (4) "}, {"name": "mD", "desc": "[11.9/]?=99 Disk magnitude "}, {"name": "rs", "desc": "[0/38.5]? Disk scale length (3) "}, {"name": "b/aD", "desc": "[0.05/1]? Disk axis ratio "}, {"name": "PAD", "desc": "[-89.8/88.5]? Disk position angle "}, {"name": "Chi2", "desc": "[1/1.9]? Reduced chi-square "}, {"name": "Flag", "desc": "[0/9] binary flag in decimal number (5) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_261_36"}} {"id": "J/ApJS/261/36", "title_cds": "LAMOST DR7 stellar param. from RRNet model", "title_create": "Xiong+, 2022", "year": "2022", "author": "Xiong S., Li X., Liao C.", "title_pub": "A model RRNet for spectral information exploitation and LAMOST Medium-Resolution Spectrum parameter estimation.", "first_author": "Xiong S.", "ref_biblio": [""], "bibcode": ["2022ApJS..261...36X"], "see_also": ["V/146 : LAMOST DR1 catalogs (Luo+, 2015)", "V/156 : LAMOST DR7 catalogs (Luo+, 2019)", "J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009)", "J/other/RAA/11.924 : Atmospheric parameters for 771 stars (Wu+, 2011)", "J/AJ/151/144 : ASPCAP weights for the APOGEE elements (Garcia+, 2016)", "J/AJ/156/126 : Stellar parameters from BACCHUS analysis (Jonsson+, 2018)", "J/ApJS/245/34 : Abundances for 6 million stars from LAMOST DR5 (Xiang+, 2019)", "J/ApJ/891/23 : Stellar abundances from LAMOST MRS (SPCAnet) (Wang+, 2020)", "J/A+A/640/A127 : Open cluster properties with Gaia and LAMOST (Zhong+, 2020)", "J/MNRAS/506/150 : The GALAH+ Survey DR3 (Buder+, 2021)", "http://www.lamost.org/dr7/ : LAMOST DR7 home page", "http://github.com/Chan-0312/RRNet : RRNet code and trained models"], "keyword_cds": "Models; Spectra, optical; Abundances", "keyword_pub": "Astronomy data analysis ; Spectroscopy ; Stellar atmospheres ; Stellar abundances", "abstract": ["This work proposes a residual recurrent neural network (RRNet) for", "synthetically extracting spectral information and estimating stellar", "atmospheric parameters together with 15 chemical element abundances", "for medium-resolution spectra from the Large Sky Area Multi-Object", "Fiber Spectroscopic Telescope (LAMOST). The RRNet consists of two", "fundamental modules: a residual module and a recurrent module. The", "residual module extracts spectral features based on the longitudinally", "driving power from parameters, while the recurrent module recovers", "spectral information and restrains the negative influences from noises", "based on Cross-band Belief Enhancement. RRNet is trained by the", "spectra from common stars between LAMOST DR7 and the APOGEE-Payne", "catalog. The 17 stellar parameters and their uncertainties for 2.37", "million medium-resolution spectra from LAMOST DR7 are predicted. For", "spectra with a signal-to-noise ratio >=10, the precision of", "estimations (Teff and logg) are 88K and 0.13dex, respectively,", "elements C, Mg, Al, Si, Ca, Fe, and Ni are 0.05-0.08dex, and N, O, S,", "K, Ti, Cr, and Mn are 0.09-0.14dex, while that of Cu is 0.19dex.", "Compared with StarNet and SPCANet, RRNet shows higher accuracy and", "robustness. In comparison to Apache Point Observatory Galactic", "Evolution Experiment and Galactic Archaeology with HERMES surveys,", "RRNet manifests good consistency within a reasonable range of bias."], "type": ["MC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "rrnetcat.dat", "desc": "The LAMOST-RRNet catalog ", "columns": [{"name": "obsID", "desc": "[588902003/747816250] Identification of LAMOST spectrum"}, {"name": "FileName", "desc": "Name of the FITS file LAMOST spectrum "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "[-9.15/79.1] Declination (J2000) "}, {"name": "Nameb", "desc": "Spectrum extension name of blue part "}, {"name": "Namer", "desc": "Spectrum extension name of red part "}, {"name": "SNRb", "desc": "[10/999] Signal-to-noise ratio of blue part "}, {"name": "SNRr", "desc": "[10/999] Signal-to-noise ratio of red part "}, {"name": "Teff", "desc": "[3779/6597] Effective temperature "}, {"name": "e_Teff", "desc": "[33/484] Teff uncertainty "}, {"name": "logg", "desc": "[0.95/4.8] Log of surface gravity "}, {"name": "e_logg", "desc": "[0.08/0.8] logg uncertainty "}, {"name": "CH", "desc": "[-2.38/0.34] [C/H] abundance "}, {"name": "e_CH", "desc": "[0.029/0.5] CH uncertainty "}, {"name": "[N/H]", "desc": "[-1.94/0.9] [N/H] abundance "}, {"name": "e_[N/H]", "desc": "[0.038/0.52] [N/H] uncertainty "}, {"name": "OH", "desc": "[-1.44/0.44] [O/H] abundance "}, {"name": "e_OH", "desc": "[0.028/0.5] OH uncertainty "}, {"name": "MgH", "desc": "[-1.9/0.6] [Mg/H] abundance "}, {"name": "e_MgH", "desc": "[0.02/0.4] MgH uncertainty "}, {"name": "AlH", "desc": "[-2.7/0.8] [Al/H] abundance "}, {"name": "e_AlH", "desc": "[0.027/0.6] AlH uncertainty "}, {"name": "SiH", "desc": "[-1.81/0.61] [Si/H] abundance "}, {"name": "e_SiH", "desc": "[0.019/0.31] SiH uncertainty "}, {"name": "SH", "desc": "[-1.91/0.5] [S/H] abundance "}, {"name": "e_SH", "desc": "[0.039/0.42] SH uncertainty "}, {"name": "KH", "desc": "[-2.1/0.5] [K/H] abundance "}, {"name": "e_KH", "desc": "[0.04/0.61] KH uncertainty "}, {"name": "CaH", "desc": "[-1.97/0.52] [Ca/H] abundance "}, {"name": "e_CaH", "desc": "[0.02/0.4] CaH uncertainty "}, {"name": "TiH", "desc": "[-1.75/0.6] [Ti/H] abundance "}, {"name": "e_TiH", "desc": "[0.026/0.6] TiH uncertainty "}, {"name": "CrH", "desc": "[-2.25/0.64] [Cr/H] abundance "}, {"name": "e_CrH", "desc": "[0.028/0.5] CrH uncertainty "}, {"name": "MnH", "desc": "[-2.1/0.5] [Mn/H] abundance "}, {"name": "e_MnH", "desc": "[0.029/0.6] MnH uncertainty "}, {"name": "[Fe/H]", "desc": "[-1.88/0.61] [Fe/H] abundance "}, {"name": "e_[Fe/H]", "desc": "[0.025/0.4] [Fe/H] uncertainty "}, {"name": "NiH", "desc": "[-2.55/0.72] [Ni/H] abundance "}, {"name": "e_NiH", "desc": "[0.02/0.5] NiH uncertainty "}, {"name": "CuH", "desc": "[-2.6/0.6] [Cu/H] abundance "}, {"name": "e_CuH", "desc": "[0.05/0.7] CuH uncertainty "}, {"name": "Flag", "desc": "[0/1] Recommended flag: 1=good "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_ApJS_261_37"}} {"id": "J/ApJS/261/37", "title_cds": "^13^CO emission in the MWISP ^12^CO molecular clouds", "title_create": "Yuan+, 2022", "year": "2022", "author": "Yuan L., Yang J., Du F., Su Y., Liu X., Zhang S., Sun Y., Zhou X., Yan Q.-Z., Ma Y.", "title_pub": "Molecular gas structures traced by ^13^CO emission in the 18190 ^12^CO molecular clouds from the MWISP survey.", "first_author": "Yuan L.", "ref_biblio": [""], "bibcode": ["2022ApJS..261...37Y"], "see_also": ["J/A+A/592/A54 : Combined ArTeMiS+SPIRE 350um image of NGC6334 (Andre+, 2016)", "J/A+A/600/A141 : Orion A integral shaped filament image (Kainulainen+, 2017)", "J/ApJ/858/90 : Radial profiles of 5 nearby galaxies (Gallagher+, 2018)", "J/A+A/631/A72 : SABOCA 350um view of ATLASGAL massive clumps (Lin+, 2019)", "J/A+A/638/A44 : Infrared dark cloud G28.3 HI and CI maps (Beuther+, 2020)", "J/A+A/646/A170 : Serpens filament ^13^CO, C18O and C17O datacubes (Gong+, 2021)", "J/A+A/645/A27 : Orion B in 18 molecular tracers maps (Gratier+, 2021)", "J/ApJS/257/51 : Morphologies of MWISP ^12^CO mol. clouds (Yuan+, 2021)", "J/A+A/660/A56 : NGC 6334 maps and CO velocity cubes (Arzoumanian+, 2022)", "J/A+A/663/A56 : SEDIGISM: Molecular Cloud morphology I. (Neralwar+, 2022)"], "keyword_cds": "Molecular clouds; Carbon monoxide; Interstellar medium; Surveys", "keyword_pub": "Interstellar medium ; Interstellar molecules ; Molecular clouds", "abstract": ["After morphological classification of 18190 ^12^CO molecular clouds,", "we further investigate the properties of their internal molecular gas", "structures traced by the ^13^CO (J=1-0) line emissions. Using three", "different methods to extract the ^13^CO gas structures within each", "^12^CO cloud, we find that ~15% of the ^12^CO clouds (2851) have", "^13^CO gas structures and these ^12^CO clouds contribute about 93% of", "the total integrated flux of ^12^CO emission. In each of the", "2851 ^12^CO clouds with ^13^CO gas structures, the ^13^CO emission", "area generally does not exceed 70% of the ^12^CO emission area, and", "the ^13^CO integrated flux does not exceed 20% of the ^12^CO", "integrated flux. We reveal a strong correlation between the", "velocity-integrated intensities of ^12^CO lines and those of ^13^CO", "lines in both ^12^CO and ^13^CO emission regions. This indicates the", "H2 column densities of molecular clouds are crucial for the ^13^CO", "line emission. After linking the ^13^CO structure detection rates of", "the 18190 ^12^CO molecular clouds to their morphologies, i.e.,", "nonfilaments and filaments, we find that the ^13^CO gas structures are", "primarily detected in ^12^CO clouds with filamentary morphologies.", "Moreover, these filaments tend to harbor more than one ^13^CO", "structure. That demonstrates filaments not only have larger spatial", "scales, but also have more molecular gas structures traced by ^13^CO", "lines, i.e., local gas density enhancements. Our results favor the", "turbulent compression scenario for filament formation, in which", "dynamical compression of turbulent flows induces local density", "enhancements. The nonfilaments tend to be in the low-pressure and", "quiescent turbulent environments of the diffuse interstellar medium."], "description": ["The ^13^CO data is from the MWISP survey, which is an ongoing northern", "Galactic plane CO survey. This survey is conducted by the 13.7m", "telescope at Delingha, China.", "As described in Yan+ (2021, J/ApJS/257/51), a total of 18190 available", "molecular clouds have been identified from the ^12^CO data cube. In", "Paper I, we completed the morphological classification for these", "^12^CO molecular clouds, which are mainly classified into filaments", "and nonfilaments. In this work, we aim to analyze the properties of", "high column density gas traced by the ^13^CO line emission in these", "molecular cloud samples."], "alias": ["MWISP"], "type": ["OC"], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "table2.dat", "desc": "A catalog of ^12^CO/^13^CO line emission parameters ", "columns": [{"name": "ID", "desc": "[674/627890] Identifier number "}, {"name": "Name", "desc": "Name (GLLL.lll+BB.bbb-VLSR) "}, {"name": "GLON", "desc": "[104.79/150.2] Galactic longitude, ^12^CO intensity-weighted average center (1)"}, {"name": "GLAT", "desc": "[-5.11/5.3] Galactic latitude, ^12^CO intensity-weighted average center (1)"}, {"name": "VLSR", "desc": "[-93.6/9] ^12^CO intensity-weighted average central (LSR) velocity (2)"}, {"name": "Area12CO", "desc": "[2/60746] Angular area, ^12^CO (1-0) "}, {"name": "Vspan12CO", "desc": "[0.8/43.5] Velocity span of ^12^CO(1-0) (3)"}, {"name": "Tpk12CO", "desc": "[2.4/51] Peak value of ^12^CO (1-0) "}, {"name": "Flux12CO", "desc": "[3/390097] Integrated flux of ^12^CO(1-0) line emission (4)"}, {"name": "Area13CO", "desc": "[1.2/13881] Angular area, ^13^CO(1-0)"}, {"name": "Vspan13CO", "desc": "[0.5/37.4] Velocity span of ^13^CO(1-0) (3)"}, {"name": "Tpk13CO", "desc": "[0.6/16] Peak value of ^13^CO (1-0) "}, {"name": "Flux13CO", "desc": "[0.3/39385] Integrated flux of ^13^CO(1-0) line emission (4)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_BaltA_16_349"}} {"id": "J/BaltA/16/349", "title_cds": "Vilnius photometry in Collinder 428 area", "title_create": "Laugalys+, 2007", "year": "2007", "author": "Laugalys V., Straizys V., Vrba F.J., Cernis K., Kazlauskas A., Boyle R.P., Davis P.A.G.", "title_pub": "CCD photometry and classification of stars in the North America and Pelican Nebulae region. IV. The region of a supposed cluster Collinder 428.", "first_author": "Laugalys V.", "ref_biblio": [""], "bibcode": ["2007BaltA..16..349L"], "keyword_cds": "", "keyword_pub": "stars: fundamental parameters, classification - ISM: dust, extinction, clouds - ISM: individual: LDN 935 - open clusters: individual (Collinder 428, NGC6997)", "mission": "", "abstract": ["Magnitudes and color indices of 860 stars down to V=16.7mag in the", "seven-color Vilnius photometric system were obtained in the area of", "the suspected open cluster Collinder 428 in the North America Nebula.", "Spectral types, interstellar color excesses, extinctions and distances", "of stars were determined for 290 stars from the photometric data. The", "plot of extinction vs. distance gives the front edge of the dust cloud", "at 540 pc. We conclude that Collinder 428 is not a real star cluster."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "08-Oct-2016"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_BaltA_17_161"}} {"id": "J/BaltA/17/161", "title_cds": "NGC 7023 photometry", "title_create": "Zdanavicius+, 2008", "year": "2008", "author": "Zdanavicius K., Zdanavicius J., Straizys V., Kotovas A.", "title_pub": "Photometry and classification of stars around the reflection nebula NGC 7023 in Cepheus. I. A catalog of magnitudes, indices and spectral types of 1240 stars.", "first_author": "Zdanavicius K.", "ref_biblio": [""], "bibcode": ["2008BaltA..17..161Z"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Alexandra Bauer, Patricia Vannier [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_BaltA_24_157"}} {"id": "J/BaltA/24/157", "title_cds": "Visual binaries", "title_create": "Isaeva+, 2015", "year": "2015", "author": "Isaeva A.A., Kovaleva D.A., Malkov O.Y.", "title_pub": "Visual binaries: cross-matching and compiling of a comprehensive list.", "first_author": "Isaeva A.A.", "ref_biblio": [""], "bibcode": ["2015BaltA..24..157I"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1515/astro-2017-0215"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_121_337"}} {"id": "J/MNRAS/121/337", "title_cds": "Radcliffe Catalog of stars in Magellanic Clouds", "title_create": "Feast+ 1960", "year": "1960", "author": "Feast M.W., Thackeray A.D., Wesselink A.J.", "title_pub": "The brightest stars in the Magellanic Clouds.", "first_author": "Feast M.W.", "ref_biblio": [""], "bibcode": ["1960MNRAS.121..337F"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["RMC"], "type": ["OC"], "doi_pub": ["10.1093/mnras/121.4.337"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_130_45"}} {"id": "J/MNRAS/130/45", "title_cds": "Infrared survey of the region of SA 193", "title_create": "Westerlund+, 1965", "year": "1965", "author": "Westerlund B.E.", "title_pub": "An infrared survey of the region of SA 193.", "first_author": "Westerlund B.E.", "ref_biblio": [""], "bibcode": ["1965MNRAS.130...45W"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1093/mnras/130.1.45"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_202_761"}} {"id": "J/MNRAS/202/761", "title_cds": "Southern close visual double stars", "title_create": "Hurly+, 1983", "year": "1983", "author": "Hurly P.R., Warner B.", "title_pub": "Area scanner observations of close visual double stars. II. Results for 153 southern stars.", "first_author": "Hurly P.R.", "ref_biblio": [""], "bibcode": ["1983MNRAS.202..761H"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1093/mnras/202.3.761"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_267_431"}} {"id": "J/MNRAS/267/431", "title_cds": "Photographic study of A3558", "title_create": "Metcalfe+, 1994", "year": "1994", "author": "Metcalfe N., Godwin J.G., Peach J.V.", "title_pub": "Multicolour photometry of the Shapley 8 cluster of galaxies.", "first_author": "Metcalfe N.", "ref_biblio": [""], "bibcode": ["1994MNRAS.267..431M"], "see_also": ["VII/42 : GMP catalogue: galaxies in the Coma cluster (Godwin+ 1983)", "J/MNRAS/239/459 : The clusters of galaxies A2197 and A2199 (Dixon+ 1989)", "J/ApJ/485/447 : Evidence of substructure in A3558 (Dantas+ 1997)", "J/MNRAS/296/599 : A3558 complex redshifts (Bardelli+, 1998)", "J/A+A/419/71 : 1.4GHz obs. and optical ident. in A3558 (Giacintucci+, 2004)", "J/AJ/130/2541 : Core of the Shapley supercluster at 1.4GHz (Miller+, 2005)", "http://users.ox.ac.uk/~jgodwin/clusters.htm"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1093/mnras/267.2.431"], "orcid_pub": ["0000-0001-9034-4402"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_284_477"}} {"id": "J/MNRAS/284/477", "title_cds": "The old open cluster NGC 6253", "title_create": "Bragaglia+, 1997", "year": "1997", "author": "Bragaglia A., Tessicini G., Tosi M., Marconi G., Munari U.", "title_pub": "UBVRI CCD photometry of the old open cluster NGC 6253.", "first_author": "Bragaglia A.", "ref_biblio": [""], "bibcode": ["1997MNRAS.284..477B"], "see_also": ["J/AJ/125/1383 : Stromgren photometry of NGC 6253 (Anthony-Twarog+, 2003)", "J/A+A/465/185 : Element abundances of 7 stars of NGC 6253 (Sestito+, 2007)", "J/A+A/505/1129 : BVRIJHK and proper motions in NGC 6253 (Montalto+, 2009)", "J/A+A/509/A17 : R light curves of NGC 6253 variables (De Marchi+, 2010)", "J/MNRAS/327/23 : CCD UBVRI photometry of 7 open star clusters (Sagar+, 2001)", "J/A+A/535/A39 : Radial velocity survey toward NGC 6253 (Montalto+, 2011)", "J/AJ/139/2034 : NGC 6253 stars equivalent widths (Anthony-Twarog+, 2010)"], "keyword_cds": "Clusters, open ; Photometry, CCD", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1093/mnras/284.2.477"], "orcid_pub": ["0000-0002-0338-7883"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_301_1019"}} {"id": "J/MNRAS/301/1019", "title_cds": "Seyfert galaxies/radio-quiet QSO correlation", "title_create": "Roy+, 1998", "year": "1998", "author": "Roy A.L., Norris R.P., Kesteven M.J., Troup E.R., Reynolds J.E.", "title_pub": "Seyfert galaxies and the radio-far-infrared correlation.", "first_author": "Roy A.L.", "ref_biblio": [""], "bibcode": ["1998MNRAS.301.1019R\t(SIMBAD/NED"], "keyword_cds": "Galaxies, Seyfert ; Redshifts ; Radio sources", "keyword_pub": "galaxies: active - galaxies: nuclei - galaxies: Seyfert - galaxies: starburst - infrared: galaxies - radio continuum: galaxies", "abstract": ["We have observed a sample of 149 Seyfert galaxies and radio-quiet", "quasars at 13 cm with both a 275-km radio interferometer and the 6-km", "compact array of the Australia Telescope. The high-resolution", "observations searched for the presence of compact,", "high-brightness-temperature radio emission from the active nucleus.", "The low-resolution observations measured the total radio emission from", "the galaxy disc and Seyfert core and lobes. From these we draw the", "following conclusions. (i) Seyfert galaxies that lack compact radio", "cores display a correlation between radio and far-infrared (FIR)", "emission similar to the correlation displayed by normal spirals,", "albeit with greater scatter. The correlation is found to be intrinsic", "and is not an artefact of the richness effect. (ii) A very different", "radio-FIR correlation is displayed by those Seyferts that harbour", "compact radio cores. These tend to be more radio-loud than either", "normal spirals or the Seyferts that lack compact cores. The compact", "core emission thus seems to be responsible for the generally poor", "radio-FIR correlation displayed by Seyfert galaxies. (iii) The", "radio-FIR correlation is not significantly improved by subtracting off", "the 0.1arcsec (20 to 200pc) compact radio emission from the total", "radio emission. This suggests that the emission from the active", "galactic nucleus has significant structure on scales larger than", "0.1arcsec. Perhaps these structures are the `linear' radio features", "that have been seen previously in Seyfert nuclei."], "doi_pub": ["10.1046/j.1365-8711.1998.02060.x"], "orcid_pub": ["0000-0002-1931-0135"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": " ", "columns": [{"name": "Name", "desc": "IRAS or IRAS-like name (B1950) "}, {"name": "NoteFlag", "desc": "[*] Note flag (1) "}, {"name": "Alias", "desc": "Name "}, {"name": "z", "desc": "Redshift (2) "}, {"name": "Class", "desc": "Seyfert classification (3) "}, {"name": "Smpl", "desc": "Sample in which the galaxy appears (4) "}, {"name": "l_S2.4GHz", "desc": "Limit flag on S2.4GHz "}, {"name": "S2.4GHz", "desc": "? Total flux density at 2.4GHz "}, {"name": "r_S2.4GHz", "desc": "Reference for S2.4GHz "}, {"name": "l_S2.3c", "desc": "Limit flag on S2.3c "}, {"name": "S2.3c", "desc": "? Core flux density at 2.3GHz "}, {"name": "n_S2.3c", "desc": "[*] Note on S2.3c "}, {"name": "l_HI", "desc": "Limit flag on HI "}, {"name": "HI", "desc": "? HI flux "}, {"name": "l_lgLFIR", "desc": "Limit flag on lgLFIR "}, {"name": "lgLFIR", "desc": "? FIR luminosity "}, {"name": "l_lgL2.4GHz", "desc": "Limit flag on lgL2.4GHz "}, {"name": "lgL2.4GHz", "desc": "? Total 2.4GHz luminosity "}, {"name": "l_lgMHI", "desc": "Limit flag on lgMHI "}, {"name": "lgMHI", "desc": "? HI mass "}, {"name": "lgD25", "desc": "? Major isophotal diameter "}, {"name": "lgLB", "desc": "? Total face-on magnitude corrected for "}, {"name": "internal", "desc": "extinction and "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_310_585"}} {"id": "J/MNRAS/310/585", "title_cds": "Scorpius OB2 parallaxes", "title_create": "de Bruijne+, 1999", "year": "1999", "author": "de Bruijne J.H.J.", "title_pub": "Structure and colour-magnitude diagrams of Scorpius OB2 based on kinematic modelling of Hipparcos data.", "first_author": "de Bruijne J.H.J.", "ref_biblio": [""], "bibcode": ["1999MNRAS.310..585D"], "see_also": ["I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)", "J/AJ/117/354 : OB associations from Hipparcos (de Zeeuw+, 1999)"], "keyword_cds": "Associations, stellar ; Parallaxes, trigonometric ; Photometry, UBV", "keyword_pub": "astrometry - stars: distances - stars: kinematics - open clusters and associations: general - open clusters and associations: individual: Hyades - open clusters and associations: individual: Scorpius OB2", "description": ["ll stars in a `moving group' share the same space motion. The", "presence of such a coherent structure in velocity space can be", "used to derive (improved) estimates of the stellar parallaxes", "from the observed positions and proper motions. A Lund Observatory", "group (Dravins et al., 1999A&A...348.1040D) describes an elegant", "and sophisticated maximum likelihood procedure to do so using", "Hipparcos data.", "We implement the Lund procedure, and test it extensively", "using Monte Carlo simulations.", "We present an application to the nearby association Scorpius", "OB2, which consists of the three subgroups Upper Scorpius", "(mean distance 145 pc), Upper Centaurus Lupus (140 pc), and", "Lower Centaurus Crux (118 pc). Membership of these groups has recently", "been established by de Zeeuw et al. using", "Hipparcos data."], "doi_pub": ["10.1046/j.1365-8711.1999.02953.x"], "orcid_pub": ["0000-0001-6459-8599"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "tablea1.dat", "desc": "*Upper Scorpius Z99 members ", "columns": [{"name": "HIP", "desc": "Hipparcos (Cat. ) number "}, {"name": "plx", "desc": "Hipparcos (Cat. ) trigonometric parallax "}, {"name": "e_plx", "desc": "rms uncertainty on plx "}, {"name": "plxs", "desc": "Secular parallax (g_lim_=Y) ??? "}, {"name": "plx9", "desc": "? Secular parallax (g_lim_=9) "}, {"name": "e_plxs", "desc": "Secular parallax error (equations 16 and 17; s_v_=1km/s)"}, {"name": "gi", "desc": "Goodness-of-fit parameter (g_lim_=Y) ??? (1) "}, {"name": "gi9", "desc": "Goodness-of-fit parameter (g_lim_=9) (1) "}, {"name": "Vmag", "desc": "Hipparcos (Cat. ) V magnitude "}, {"name": "B-V", "desc": "Hipparcos (Cat. ) B-V colour index "}, {"name": "Ext", "desc": "? Visual extinction A_V_R_V_xE(B-V) "}, {"name": "E(B-V)", "desc": "? Colour excess "}, {"name": "Mult.", "desc": "? Multiplicity label (multiple star if M=1) "}, {"name": "Label", "desc": "Peculiarity label (2) "}, {"name": "Note", "desc": "[*] *: individual note "}, {"name": "SpType", "desc": "Hipporcos (Cat. ) spectral type "}]}, {"name": "tablea2.dat", "desc": "Upper Centaurus Lupus Z99 members ", "columns": [{"name": "HIP", "desc": "Hipparcos (Cat. ) number "}, {"name": "plx", "desc": "Hipparcos (Cat. ) trigonometric parallax "}, {"name": "e_plx", "desc": "rms uncertainty on plx "}, {"name": "plxs", "desc": "Secular parallax (g_lim_=Y) ??? "}, {"name": "plx9", "desc": "? Secular parallax (g_lim_=9) "}, {"name": "e_plxs", "desc": "Secular parallax error (equations 16 and 17; s_v_=1km/s)"}, {"name": "gi", "desc": "Goodness-of-fit parameter (g_lim_=Y) ??? (1) "}, {"name": "gi9", "desc": "Goodness-of-fit parameter (g_lim_=9) (1) "}, {"name": "Vmag", "desc": "Hipparcos (Cat. ) V magnitude "}, {"name": "B-V", "desc": "Hipparcos (Cat. ) B-V colour index "}, {"name": "Ext", "desc": "? Visual extinction A_V_R_V_xE(B-V) "}, {"name": "E(B-V)", "desc": "? Colour excess "}, {"name": "Mult.", "desc": "? Multiplicity label (multiple star if M=1) "}, {"name": "Label", "desc": "Peculiarity label (2) "}, {"name": "Note", "desc": "[*] *: individual note "}, {"name": "SpType", "desc": "Hipporcos (Cat. ) spectral type "}]}, {"name": "tablea3.dat", "desc": "Lower Centaurus Crux Z99 members ", "columns": [{"name": "HIP", "desc": "Hipparcos (Cat. ) number "}, {"name": "plx", "desc": "Hipparcos (Cat. ) trigonometric parallax "}, {"name": "e_plx", "desc": "rms uncertainty on plx "}, {"name": "plxs", "desc": "Secular parallax (g_lim_=Y) ??? "}, {"name": "plx9", "desc": "? Secular parallax (g_lim_=9) "}, {"name": "e_plxs", "desc": "Secular parallax error (equations 16 and 17; s_v_=1km/s)"}, {"name": "gi", "desc": "Goodness-of-fit parameter (g_lim_=Y) ??? (1) "}, {"name": "gi9", "desc": "Goodness-of-fit parameter (g_lim_=9) (1) "}, {"name": "Vmag", "desc": "Hipparcos (Cat. ) V magnitude "}, {"name": "B-V", "desc": "Hipparcos (Cat. ) B-V colour index "}, {"name": "Ext", "desc": "? Visual extinction A_V_R_V_xE(B-V) "}, {"name": "E(B-V)", "desc": "? Colour excess "}, {"name": "Mult.", "desc": "? Multiplicity label (multiple star if M=1) "}, {"name": "Label", "desc": "Peculiarity label (2) "}, {"name": "Note", "desc": "[*] *: individual note "}, {"name": "SpType", "desc": "Hipporcos (Cat. ) spectral type "}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "HIP", "desc": "Hipparcous number "}, {"name": "Note", "desc": "Text of the note (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_357_945"}} {"id": "J/MNRAS/357/945", "title_cds": "Evolutionary stellar pop. synthesis", "title_create": "Gonzalez-Delgado+, 2005", "year": "2005", "author": "Gonzalez-Delgado R.M., Cervino M., Martins L.P., Leitherer C., Hauschildt P.H.", "title_pub": "Evolutionary stellar population synthesis at high spectral resolution: optical wavelengths.", "first_author": "Gonzalez-Delgado R.M.", "ref_biblio": [""], "bibcode": ["2005MNRAS.357..945G"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["We present the single stellar population (SSP) synthesis results of", "our new synthetic stellar atmosphere models library with a spectral", "sampling of 0.3{AA}, covering the wavelength range from 3000 to 7000{AA}", "for a wide range of metallicities (twice solar, solar, half solar and", "1/10 solar). The stellar library is composed of 1650 spectra computed", "with the latest improvements in stellar atmospheres. In particular, it", "incorporates non-local thermodynamic equilibrium (LTE) line-blanketed", "models for hot (Teff>=27500K), and LTE line-blanketed models", "(Phoenix) for cool (3000<=Teff<=4500K) stars. Because of the high", "spectral resolution of this library, evolutionary synthesis models can", "be used to predict the strength of numerous weak absorption lines and", "the evolution of the profiles of the strongest lines over a wide range", "of ages. The SSP results have been calculated for ages from 1Myr to", "17Gyr using the stellar evolutionary tracks provided by the Geneva", "and Padova groups. For young stellar populations, our results have a", "very detailed coverage of high-temperature stars with similar results", "for the Padova and Geneva isochrones. For intermediate and old stellar", "populations, our results, once degraded to a lower resolution, are", "similar to the ones obtained by other groups (limitations imposed by", "the stellar evolutionary physics notwidthstanding). The limitations", "and advantages of our models for the analysis of integrated", "populations are described.", "The full set of the stellar library and the evolutionary models are", "available for retrieval at the websites http://www.iaa.csic.es/~rosa", "and http://www.iaa.csic.es/~mcs/sed@ ."], "description": ["The library contains 415, 409, 416 and 411 spectra for Z= 0.002, 0.010,", "0.020 (solar) and 0.040, respectively."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2005.08692.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_358_1290"}} {"id": "J/MNRAS/358/1290", "title_cds": "NGC 663 and 654 stellar contents", "title_create": "Pandey+, 2005", "year": "2005", "author": "Pandey A.K., Upadhyay K., Ogura K., Sagar R., Mohan V., Mito H., Bhatt H.C., Bhatt B.C.", "title_pub": "Stellar contents of two young open clusters: NGC 663 and 654.", "first_author": "Pandey A.K.", "ref_biblio": [""], "bibcode": ["2005MNRAS.358.1290P"], "keyword_cds": "", "keyword_pub": "stars: formation - stars: luminosity function, mass function - dust, extinction - galaxies: star clusters", "mission": "", "abstract": ["UBVRI CCD photometry in a wide field around two young open clusters,", "NGC 663 and 654, has been carried out. H{alpha} and polarimetric", "observations for the cluster NGC 654 have also been obtained. We use", "the photometric data to construct colour-colour and colour-magnitude", "diagrams, from which we can investigate the reddening, age, mass and", "evolutionary states of the stellar contents of the these clusters."], "description": ["For NGC 663, the CCD UBVIC data were acquired in 1999 November using", "the 2048x2048pixel^2^ CCD camera mounted on the 105-cm Schmidt", "telescope of the Kiso Observatory.", "For NGC 654, the CCD BVIC and H observations were carried out in 1993", "October-November and in 1998 December, respectively, using the", "1024x1024pixel^2^ CCD camera mounted on the f/13 Cassegrain focus of", "the 104-cm Sampurnanand telescope of the State Observatory, Naini Tal."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2005.08784.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_361_607"}} {"id": "J/MNRAS/361/607", "title_cds": "K_s_-selected galaxies", "title_create": "Caputi+, 2005", "year": "2005", "author": "Caputi K.I., Dunlop J.S., Mclure R.J., Roche N.D.", "title_pub": "The evolution of K_s_-selected galaxies in the GOODS/CDFS deep ISAAC field.", "first_author": "Caputi K.I.", "ref_biblio": [""], "bibcode": ["2005MNRAS.361..607C"], "keyword_cds": "", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: high-redshift - galaxies: luminosity function, mass function", "mission": "", "abstract": ["We present estimated redshifts and derived properties of a sample of", "1663 galaxies with Ks<=22 (Vega), selected from 50.4-arcmin^2^ of the", "Great Observatories Origins Deep Survey/Chandra Deep Field South", "(GOODS/CDFS) field with deep Infrared Spectrometer and Array Camera", "(ISAAC) imaging, and make an extensive comparison of their properties", "with those of the extremely red galaxies (ERGs) selected in the same", "field. We study in detail the evolution of Ks-selected galaxies up to", "redshifts z~4, and clarify the role of ERGs within the total Ks-band", "galaxy population. We compute the total Ks-band luminosity function", "(LF) and compare its evolution with the ERG LF."], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2005.09222.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_362_689"}} {"id": "J/MNRAS/362/689", "title_cds": "AAO/UKST SuperCOSMOS H{alpha} survey", "title_create": "Parker+, 2005", "year": "2005", "author": "Parker Q.A., Phillipps S., Pierce M.J., Hartley M., Hambly N.C., Read M.A., Macgillivray H.T., Tritton S.B., Cass C.P., Cannon R.D., Cohen M., Drew J.E., Frew D.J., Hopewell E., Mader S., Malin D.F., Masheder M.R.W., Morgan D.H., Morris R.A.H., Russeil D., Russell K.S., Walker R.N.F.", "title_pub": "The AAO/UKST SuperCOSMOS H{alpha} survey.", "first_author": "Parker Q.A.", "ref_biblio": [""], "bibcode": ["2005MNRAS.362..689P"], "keyword_cds": "", "keyword_pub": "astronomical data bases: miscellaneous - catalogues - surveys - stars: emission line - photometry", "abstract": ["The UK Schmidt Telescope (UKST) of the Anglo-Australian Observatory", "completed a narrow-band H{alpha} plus [N II] 6548, 6584{AA} survey of", "the Southern Galactic Plane and Magellanic Clouds in late 2003. The", "survey, which was the last UKST wide-field photographic survey and the", "only one undertaken in a narrow-band, is now an online digital data", "product of the Wide-Field Astronomy Unit of the Royal Observatory", "Edinburgh (ROE). The survey utilized a high specification, monolithic", "H{alpha} interference bandpass filter of exceptional quality. In", "conjunction with the fine-grained Tech-Pan film as a detector it has", "produced a survey with a powerful combination of area coverage (4000", "square degrees), resolution (~1 arcsec) and sensitivity (5 Rayleighs),", "reaching a depth for continuum point sources of R=~20.5. The main", "survey consists of 233 individual fields on a grid of centres", "separated by 4{deg} at declinations below +2{deg} and covers a swathe", "approximately 20{deg} wide about the Southern Galactic Plane. The", "original survey films were scanned by the SuperCOSMOS measuring", "machine at the Royal Observatory, Edinburgh, to provide the online", "digital atlas called the SuperCOSMOS H{alpha} Survey (SHS). We present", "the background of the survey, the key survey characteristics, details", "and examples of the data product, calibration process, comparison with", "other surveys and a brief description of its potential for scientific", "exploitation."], "doi_pub": ["10.1111/j.1365-2966.2005.09350.x"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "fields.dat", "desc": "H-alpha (HA) and matching Short-red (SR) fields currently available online", "columns": [{"name": "Field", "desc": "Field number "}, {"name": "RAh", "desc": "Centre Right ascnesion (B1950) "}, {"name": "RAm", "desc": "Centre Right ascnesion (B1950) "}, {"name": "DE-", "desc": "Centre Declination sign (B1950) "}, {"name": "DEd", "desc": "Centre Declination (B1950) "}, {"name": "HaFITS", "desc": "Halpha.FITS file name (HANNNN.fits.gz) "}, {"name": "HablFITS", "desc": "Halpha-block.FITS file name (halNNNNblock.fits.gz) "}, {"name": "HaGIF", "desc": "Halpha.GIF file name (HANNNN.gif) "}, {"name": "HablGIF", "desc": "Halpha-block.GIF file name (halNNNNblock.gif) "}, {"name": "SRFITS", "desc": "Short-red FITS file name (SRNNNN.fits.gz) "}, {"name": "SRblFITS", "desc": "Short-red-block FITS file (harNNNNblock.fits.gz) "}, {"name": "SRGIF", "desc": "Short-red.GIF file name (SRNNNN.gif) "}, {"name": "SRblGIF", "desc": "Short-red-block.GIF file name (harNNNNblock.gif) "}]}, {"name": "table3.dat", "desc": "Content of the fits files ", "columns": []}, {"name": "HAL0067block.fits", "desc": "Example of file : Field 0067 ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_380_1064"}} {"id": "J/MNRAS/380/1064", "title_cds": "New spectroscopic orbits of Am stars", "title_create": "Carquillat+, 2007", "year": "2007", "author": "Carquillat J.-M., Prieur J.-L.", "title_pub": "Contribution to the search for binaries among Am stars. VIII. New spectroscopic orbits of eight systems and statistical study of a sample of 91 Am stars.", "first_author": "Carquillat J.-M.", "ref_biblio": [""], "bibcode": ["2007MNRAS.380.1064C"], "keyword_cds": "", "keyword_pub": "binaries: spectroscopic - stars: fundamental parameters - stars: luminosity function, mass function", "mission": "", "abstract": ["This paper is the last of a series devoted to the study of Am stars,", "with the monitoring of radial velocities of a sample of 91 objects", "during more than 20yr. The purpose was to determine which stars were", "members of spectroscopic binaries (SBs) and study in detail those", "systems in order to obtain observational constraints on the origin of", "the Am phenomenon.", "We then present some statistical properties of the orbital parameters", "of the SBs whose primary is an Am star, on an extended sample obtained", "by adding 29 Am SB orbits published by other authors."], "description": ["Most of the observations concerning the eight objects were performed", "at OHP, but additional observations were also carried out by R.F.", "Griffin who kindly observed some stars of our programme with his own", "CORAVEL in Cambridge."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2007.12143.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_397_405"}} {"id": "J/MNRAS/397/405", "title_cds": "Variable stars in h Per", "title_create": "Saunders+, 2009", "year": "2009", "author": "Saunders E.S., Naylor T., Mayne N., Littlefair S.P.", "title_pub": "Pre-main-sequence variability across the radiative-convective gap.", "first_author": "Saunders E.S.", "ref_biblio": [""], "bibcode": ["2009MNRAS.397..405S"], "keyword_cds": "", "keyword_pub": "stars: fundamental parameters ; Hertzsprung\u2013Russell (HR) diagram ; stars: magnetic fields ; stars: pre-main-sequence ; stars: spots ; stars: variables: other", "abstract": ["We use I-band imaging to perform a variability survey of the 13Myr old", "cluster h Per. We find a significant fraction of the cluster members", "to be variable. Most importantly, we find that variable members lie", "almost entirely on the convective side of the gap in the cluster", "sequence between fully convective stars and those which have a", "radiative core. This result is consistent with a scenario in which the", "magnetic field changes topology when the star changes from being fully", "convective to one containing a radiative core. When the star is", "convective, the magnetic field appears dominated by large-scale", "structures, resulting in global-size spots that drive the observed", "variability. For those stars with radiative cores, we observe a marked", "absence of variability due to spots, which suggests a switch to a", "magnetic field dominated by smaller-scale structures, resulting in", "many smaller spots and thus less apparent variability. This implies", "that wide field variability surveys may only be sensitive to fully", "convective stars. On the one hand, this reduces the chances of picking", "out young groups (since the convective stars are the lower mass and", "therefore fainter objects), but conversely the absolute magnitude of", "the head of the convective sequence provides a straightforward measure", "of age for those groups which are discovered."], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1111/j.1365-2966.2009.14936.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_399_o.683"}} {"id": "J/MNRAS/399/683", "title_cds": "6dF galaxy survey final redshift release (6dFGS)", "title_create": "Jones+, 2009", "year": "2009", "author": "Jones D.H., Read M.A., Saunders W., Colless M., Jarrett T., Parker Q.A., Fairall A.P., Mauch T., Sadler E.M., Watson F.G., Burton D., Campbell L.A., Cass P., Croom S.M., Dawe J., Fiegert K., Frankcombe L., Hartley M., Huchra J., James D., Kirby E., Lahav O., Lucey J., Mamon G.A., Moore L., Peterson B.A., Prior S., Proust D., Russell K., Safouris V., Wakamatsu K.-I., Westra E., Williams M.", "title_pub": "The 6dF galaxy survey: final redshift release (DR3) and southern large-scale structures.", "first_author": "Jones D.H.", "ref_biblio": [""], "bibcode": ["2009MNRAS.399..683J"], "see_also": ["VII/193 : The CfA Redshift Catalogue, Version June 1995 (Huchra+ 1995)", "VII/250 : The 2dF Galaxy Redshift Survey (2dFGRS) (2dFGRS Team, 1998-2003)", "http://www.sdss.org : SDSS Home Page"], "keyword_cds": "Surveys ; Galaxy catalogs ; Redshifts ; Magnitudes", "keyword_pub": "surveys - galaxies: distances and redshifts - cosmology: observations - large-scale structure of Universe", "abstract": ["We report the final redshift release of the 6dF Galaxy Survey (6dFGS),", "a combined redshift and peculiar velocity survey over the southern sky", "(|b|>10{deg}). Its 136304 spectra have yielded 110256 new", "extragalactic redshifts and a new catalogue of 125071 galaxies making", "near-complete samples with (K, H, J, rF, bJ)<=(12.65, 12.95, 13.75,", "15.60, 16.75). The median redshift of the survey is 0.053. Survey", "data, including images, spectra, photometry and redshifts, are", "available through an online data base. We describe changes to the", "information in the data base since earlier interim data releases.", "Future releases will include velocity dispersions, distances and", "peculiar velocities for the brightest early-type galaxies, comprising", "about 10 per cent of the sample. Here we provide redshift maps of the", "southern local Universe with z<=0.1 , showing nearby large-scale", "structures in hitherto unseen detail. A number of regions known", "previously to have a paucity of galaxies are confirmed as", "significantly underdense regions. The URL of the 6dFGS data base is", "http://www-wfau.roe.ac.uk/6dFGS ."], "description": ["Basic data for the galaxies in the 6dFGS with redshifts, using the", "best 6dFGS redshifts (Q=3 or 4) plus available redshifts from SDSS,", "2dFGRS and ZCAT (124646 entries in all)."], "date_update": "02-May-2010", "tables": [{"name": "catalog.dat", "desc": "The 6dF Galaxy Survey Redshift Catalogue Data Release 3 (Heath Jones, Anglo-Australian Observatory, 28 February 2009)", "columns": [{"name": "6dFGS", "desc": "Galaxy survey target ID (gHHMMSDDMMSS) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Nmeas", "desc": "Number of 6dFGS measurements (of any redshift Q value)"}, {"name": "Ncz", "desc": "Number of measurements used in final cz (Q=3 or 4 only)"}, {"name": "bJmag", "desc": "Recalibrated b_J magnitude (BMAG in 6dFGS database)"}, {"name": "PROGID", "desc": "Programme ID number (PROGID in database) "}, {"name": "rFmag", "desc": "Recalibrated r_F magnitude (RMAG in database) "}, {"name": "S/G", "desc": "[0/4] SuperCOSMOS star/galaxy classifier (1) "}, {"name": "Flag", "desc": "Sum of comparison flags (comparison threshold =330km/s) (2)"}, {"name": "cz", "desc": "Best available combined recession velocity cz "}, {"name": "e_cz", "desc": "Combined uncertainty in cz (3) "}, {"name": "r_cz", "desc": "Code identifying source of redshift (4) "}, {"name": "q_cz", "desc": "Best redshift quality value available for this source (5)"}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "AV", "desc": "Galactic extinction in V magnitudes (from Schlegel et al., 1998ApJ...500..525S)"}, {"name": "W", "desc": "Original weight source had for first round of fibre allocation"}, {"name": "Target", "desc": "TARGETID number from the 6dFGS database "}, {"name": "Temp", "desc": "Template code(s) (6) "}, {"name": "FileName", "desc": "Name of redshift field file containing the redshift (7)"}, {"name": "SPECID", "desc": "SPECID values of redshifts contributing to the final combined redshift"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_400_1690"}} {"id": "J/MNRAS/400/1690", "title_cds": "Ages and metallicities for quiescent galaxies", "title_create": "Smith+, 2009", "year": "2009", "author": "Smith R.J., Lucey J.R., Hudson M.J.", "title_pub": "Ages and metallicities for quiescent galaxies in the Shapley supercluster: driving parameters of the stellar populations.", "first_author": "Smith R.J.", "ref_biblio": [""], "bibcode": ["2009MNRAS.400.1690S"], "see_also": ["J/MNRAS/381/1035 : Spectroscopy in Shapley supercluster (Smith+, 2007)"], "keyword_cds": "Galaxies, spectra ; Models ; Velocity dispersion ; Abundances", "keyword_pub": "galaxies: elliptical and lenticular, cD - galaxies: evolution", "abstract": ["We use high signal-to-noise spectroscopy for a sample of 232 quiescent", "galaxies in the Shapley supercluster, to investigate how their stellar", "populations depend on velocity dispersion (sigma) luminosity and", "stellar mass. The sample spans a large range in velocity dispersion", "(30-300km/s) and in luminosity (M_R_ from -18.7 to -23.2). Estimates", "of age, total metallicity (Z/H) and alpha-element abundance ratio", "(alpha/Fe) were derived from absorption-line analysis, using", "single-burst models of Thomas and collaborators. Using the Rose CaII", "index, we conclude that recent star formation (frosting) events are", "not responsible for the intermediate ages observed in some of the", "galaxies."], "description": ["Paper I (Smith et al., 2007, Cat. ) provides a full", "description of the observations and data processing."], "type": ["MC"], "doi_pub": ["10.1111/j.1365-2966.2009.15580.x"], "orcid_pub": ["0000-0001-5998-2297"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Model inversion results ", "columns": [{"name": "---", "desc": "[NFP] "}, {"name": "NFP", "desc": "Galaxy name (JHHMMSS.s+DDMMSS) "}, {"name": "logLR", "desc": "R-band luminosity "}, {"name": "logsigma", "desc": "?=- Velocitiy dispersion "}, {"name": "e_logsigma", "desc": "?=- rms uncertainty on logsigma "}, {"name": "logAge", "desc": "Age "}, {"name": "e_logAge", "desc": "rms uncertainty on logAge "}, {"name": "[Z/H]", "desc": "Metallicity "}, {"name": "e_[Z/H]", "desc": "rms uncertainty on [Z/H] "}, {"name": "[alpha/H]", "desc": "alpha-element enhancement (1) "}, {"name": "e_[alpha/H]", "desc": "rms uncertainty on [alpha/H] "}, {"name": "C(Age,Z)", "desc": "Error correlation coefficient (2) "}, {"name": "C(Age,alpha)", "desc": "Error correlation coefficient (2) "}, {"name": "C(Z,alpha)", "desc": "Error correlation coefficient (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_400_589"}} {"id": "J/MNRAS/400/589", "title_cds": "Ionization of emission-line gas", "title_create": "Holt+, 2009", "year": "2009", "author": "Holt J., Tadhunter C.N., Morganti R.", "title_pub": "The ionization of the emission-line gas in young radio galaxies.", "first_author": "Holt J.", "ref_biblio": [""], "bibcode": ["2009MNRAS.400..589H"], "keyword_cds": "", "keyword_pub": "ISM: jets and outflows - galaxies: active - galaxies: ISM - galaxies: kinematics and dynamics", "abstract": ["This paper is the second in a series in which we present", "intermediate-resolution, wide-wavelength coverage spectra for a", "complete sample of 14 compact radio sources, taken with the aim of", "investigating the impact of the nuclear activity on the circumnuclear", "interstellar medium (ISM) in the early stages of radio source", "evolution. In the first paper (Holt, Tadhunter & Morganti,", "2008MNRAS.387..639H), we presented the kinematic results from the", "nuclear emission-line modelling and reported fast outflows in the", "circumnuclear gas. In this paper, we use the line fluxes to", "investigate the physical conditions and dominant ionization mechanisms", "of the emission-line gas. We find evidence for large electron", "densities and high reddening in the nuclear regions, particularly in", "the broader, blueshifted components."], "description": ["Our complete sample comprises 14 compact radio sources derived from", "the northern 3C and 4C samples and southern 2Jy sample and includes", "eight CSS, three GPS, two compact core sources and one compact", "flat-spectrum source. The sample has intermediate redshifts (z<0.7)", "and a radio power range of 26"], "bibcode": ["2010MNRAS.406..952S"], "see_also": ["http://www.astro.wisc.edu/glimpse/Carina_Nebula/ : Spitzer Imaging of", "II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008)"], "keyword_cds": "", "keyword_pub": "HII regions ; ISM: individual (NGC 3372) ; stars: formation ; stars: luminosity function, mass function ; stars: pre-main-sequence", "mission": "Spitzer", "abstract": ["We report the first results of imaging the Carina Nebula (NGC 3372)", "with the Infrared Array Camera (IRAC) onboard the Spitzer Space", "Telescope, providing a photometry catalog of over 44,000 point sources", "as well as a catalog of over 900 candidate young stellar objects", "(YSOs) based on fits to their spectral energy distributions (SEDs).", "We discuss several aspects of the extended emission, including the", "structure of dozens of dust pillars that result when a clumpy", "molecular cloud is shredded by feedback from massive stars. There", "are surprisingly few of the \"extended green objects\" (EGOs) that are", "normally taken as signposts of outflow activity in Spitzer data, and", "not one of the dozens of Herbig-Haro jets detected optically are seen", "as EGOs. EGOs are apparently poor tracers of outflow activity in", "strongly irradiated environments, due to the effects of massive star", "feedback. A population of \"extended red objects\" tends to be found", "around late O-type and early B-type stars, some with clear bow-shock", "morphology. These are dusty shocks where stellar winds collide with", "photoevaporative flows off nearby clouds. Finally, the relative", "distributions of O-type stars, small star clusters, and sub-clusters", "of YSOs as compared to the dust pillars shows that while smplying that", "while some YSOs are located within dust pillars, many more stars and", "YSOs reside just outside pillar heads. We suggest that pillars are", "transient phenomena, part of a continuous outwardly propagating wave", "of star formation driven by feedback from massive stars. As the", "pillars are destroyed, they leave newly formed stars in their wake,", "and these are then subsumed into the young OB association. The YSOs", "are found predominantly in the cavity between pillars and massive", "stars, arguing that their formation was in fact triggered. Altogether,", "the current generation of YSOs shows no strong deviation from a normal", "initial mass function (IMF). The number of YSOs is consistent with a", "roughly constant star-formation rate over the past ~3Myr, implying", "that propagating star formation in pillars constitutes an important", "mechanism to construct unbound OB associations. These accelerated", "pillars may give birth to massive O-type stars that, after several", "Myr, could appear to have formed in isolation."], "curator": "Francois Ochsenbein [CDS]", "alias": ["SSTCARA SSTCARC"], "type": ["OC"], "doi_pub": ["10.1111/j.1365-2966.2010.16792.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_407_870"}} {"id": "J/MNRAS/407/870", "title_cds": "Super star clusters in Haro 11", "title_create": "Adamo+, 2010", "year": "2010", "author": "Adamo A., Ostlin G., Zackrisson E., Hayes M., Cumming R.J., Micheva G.", "title_pub": "Super star clusters in Haro 11: properties of a very young starburst and evidence for a near-infrared flux excess.", "first_author": "Adamo A.", "ref_biblio": [""], "bibcode": ["2010MNRAS.407..870A"], "keyword_cds": "", "keyword_pub": "galaxies: irregular - galaxies: starburst - galaxies: star clusters: individual: Haro 11", "abstract": ["We have used multiband imaging to investigate the nature of an extreme", "starburst environment in the nearby Lyman break galaxy analogue", "Haro 11 (ESO 350\u2212IG038) by means of its stellar cluster population.", "The central starburst region has been observed in eight different", "high-resolution Hubble Space Telescope (HST) wavebands, sampling the", "stellar and gas components from UV to near-infrared. Photometric", "imaging of the galaxy was also carried out at 2.16um by NaCo AO", "instrument at the ESO Very Large Telescope. We constructed integrated", "spectral energy distributions (SEDs) for about 200 star clusters", "located in the active star-forming regions and compared them with", "single stellar population models (suitable for physical properties of", "very young cluster population) in order to derive ages, masses and", "extinctions of the star clusters."], "description": ["We have used archival\u2002HST/ACS imaging of Haro 11, with observations", "from the FUV to the optical (~8000{AA}) wavebands. We have", "supplemented these data with new\u2002HST/WFPC2 broad-band imaging in V", "(F606W), I (F814W) and H[NIC3/F160W; NICMOS near-IR (NIR)]. To sample", "further into the IR we have used the NaCo adaptive optics (AO) imager", "in the Ks band."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2010.16983.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_417_1402"}} {"id": "J/MNRAS/417/1402", "title_cds": "Groups and clusters in 2SLAQ catalogue", "title_create": "Farrens+, 2011", "year": "2011", "author": "Farrens S., Abdalla F.B., Cypriano E.S., Sabiu C., Blake C.", "title_pub": "Friends-of-friends groups and clusters in the 2SLAQ catalogue.", "first_author": "Farrens S.", "ref_biblio": [""], "bibcode": ["2011MNRAS.417.1402F"], "keyword_cds": "", "keyword_pub": "galaxies: clusters: general - galaxies: distances and redshifts", "abstract": ["We present a catalogue of galaxy groups and clusters selected using a", "friends-of-friends (FoF) algorithm with a dynamic linking length from", "the 2dF-SDSS LRG and QSO (2SLAQ) luminous red galaxy survey. The", "linking parameters for the code are chosen through an analysis of", "simulated 2SLAQ haloes. The resulting catalogue includes 313 clusters", "containing 1152 galaxies."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2011.19356.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_417_3047"}} {"id": "J/MNRAS/417/3047", "title_cds": "Infrared two-colour diagrams for AGB stars", "title_create": "Suh+, 2011", "year": "2011", "author": "Suh K.-W., Kwon Y.-J.", "title_pub": "Infrared two-colour diagrams for AGB stars using AKARI, MSX, IRAS and near-infrared data.", "first_author": "Suh K.-W.", "ref_biblio": [""], "bibcode": ["2011MNRAS.417.3047S"], "keyword_cds": "Stars, giant ; Infrared sources", "keyword_pub": "radiative transfer - catalogues - stars: AGB and post-AGB - circumstellar matter - dust, extinction - infrared: stars", "abstract": ["Using a revised version of the catalogue of asymptotic giant branch", "(AGB) stars by Suh & Kwon, we present various infrared two-colour", "diagrams (2CDs) for 3003 O-rich, 1168 C-rich, 362 S-type and 35", "silicate carbon stars in our Galaxy. For each object in the new", "catalogue, we cross-identify the AKARI, Midcourse Space Experiment", "(MSX) and Two-Micron All-Sky Survey (2MASS) counterparts by finding", "the nearest object from the position information in the Infrared", "Astronomical Satellite (IRAS) Point Source Catalog (PSC)."], "description": ["For the sample of AGB stars, we use a revised version of the catalogue", "by Suh & Kwon (2009, JKAS, 42, 81). They presented a catalogue of AGB", "stars in our Galaxy from the sources listed in the IRAS PSC, compiling", "the lists of previous works with verifying processes; their catalogue", "was composed of 2193 O-rich stars, 1167 C-rich stars, 287 S stars and", "36 silicate carbon stars.", "ONLY the list of IRAS sources"], "type": ["CCC"], "doi_pub": ["10.1111/j.1365-2966.2011.19462.x"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "c-agb.dat", "desc": "C-rich AGB stars ", "columns": [{"name": "IRAS", "desc": "IRAS PSC name (HHMM+DDMMA) "}]}, {"name": "o-agb.dat", "desc": "O-rich AGB stars ", "columns": [{"name": "IRAS", "desc": "IRAS PSC name (HHMM+DDMMA) "}]}, {"name": "s.dat", "desc": "S stars ", "columns": [{"name": "IRAS", "desc": "IRAS PSC name (HHMM+DDMMA) "}]}, {"name": "sc.dat", "desc": "Silicate carbon stars ", "columns": [{"name": "IRAS", "desc": "IRAS PSC name (HHMM+DDMMA) "}]}, {"name": "alumina.dat", "desc": "Optical constants for amorphous alumina (Al2O3) dust (Density = 3.2g/cc)", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "n", "desc": "Refractive index "}, {"name": "k", "desc": "Extinction coefficient "}]}, {"name": "amc.dat", "desc": "Optical constants for amorphous carbon (Density = 2.0g/cc)", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "n", "desc": "Refractive index "}, {"name": "k", "desc": "Extinction coefficient "}]}, {"name": "silc.dat", "desc": "Optical constants for warm silicate (Density = 3.3g/cc)", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "n", "desc": "Refractive index "}, {"name": "k", "desc": "Extinction coefficient "}]}, {"name": "silw.dat", "desc": "Optical constants for cold silicate (Density = 3.3g/cc)", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "n", "desc": "Refractive index "}, {"name": "k", "desc": "Extinction coefficient "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_418_1452"}} {"id": "J/MNRAS/418/1452", "title_cds": "NIR Atlas of S0-Sa galaxies (NIRS0S)", "title_create": "Laurikainen+, 2011", "year": "2011", "author": "Laurikainen E., Salo H., Buta R., Knapen J.H.", "title_pub": "Near-infrared atlas of S0-Sa galaxies (NIRS0S).", "first_author": "Laurikainen E.", "ref_biblio": [""], "bibcode": ["2011MNRAS.418.1452L"], "keyword_cds": "", "keyword_pub": "galaxies: elliptical and lenticular, cD - galaxies: evolution - galaxies: structure", "abstract": ["We present an atlas of Ks-band images of 206 early-type galaxies,", "including 160 S0-S0/a galaxies, 12 ellipticals and 33 Sa galaxies", "(+1 later type). The majority of the atlas galaxies belong to a", "magnitude-limited (m_B_<=12.5mag) sample of 185 Near-InfraRed S0", "Survey galaxies. To ensure that misclassified S0s are not omitted,", "25 ellipticals from the Third Reference Catalogue of Bright Galaxies", "classified as S0s in the Carnegie Atlas were included in the sample.", "The observations were carried out using 3-4m class telescopes with", "subarcsecond pixel resolution (~0.25arcsec), and were obtained in good", "seeing conditions (full width at half-maximum ~1arcsec). The images", "are 2-3mag deeper than Two-Micron All-Sky Survey images, allowing the", "detection of faint outer discs in S0s. Both visual and photometric", "classifications are made, largely following the classification", "criteria of de Vaucouleurs. Special attention is paid to the", "classification of lenses, which are coded in a more systematic manner", "than in any of the previous studies. A new lens type, called a", "\"barlens\", is introduced, possibly forming part of the bar itself.", "Also, boxy/peanut/x-shaped structures are identified in many barred", "galaxies, even though the galaxies are not seen edge-on, indicating", "that vertical thickening is not enough to explain these structures.", "Photometric classification includes detection of exponential outer", "discs or other structures not directly visible in the images, but", "becoming clear in unsharp masking or residual images in", "decompositions. In our photometric classification, nuclear bars are", "assigned for 15 galaxies, which are overshadowed by bulges in visual", "classification. The mean Hubble stage in the near-infrared is found to", "be similar to that in the optical. We give dimensions of structure", "components, and radial profiles of the position angles and", "ellipticities, and show deviations from perfect elliptical isophotes.", "Shells and ripples, generally assumed to be manifestations of recent", "mergers, are detected only in six galaxies. However, multiple lenses", "appear in as much as 25 per cent of the atlas galaxies, which is a", "challenge to the hierarchical evolutionary picture of galaxies. Such", "models need to explain how the lenses were formed and then survived in", "multiple merger events that galaxies may have suffered during their", "lifetimes."], "object": [], "curator": "Patricia Vannier [CDS]", "alias": ["NIRS0S"], "doi_pub": ["10.1111/j.1365-2966.2011.19283.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_424_1930"}} {"id": "J/MNRAS/424/1930", "title_cds": "O and N abundances of HII regions in spiral gal.", "title_create": "Gusev+, 2012", "year": "2012", "author": "Gusev A.S., Pilyugin L.S., Sakhibov F., Dodonov S.N., Ezhkova O.V., Khramtsova M.S.", "title_pub": "Oxygen and nitrogen abundances of HII regions in six spiral galaxies.", "first_author": "Gusev A.S.", "ref_biblio": [""], "bibcode": ["2012MNRAS.424.1930G"], "see_also": ["J/A+AS/123/305 : Yields of intermediate mass stars (van den Hoek+ 1997)", "J/ApJ/510/104 : Ionizing Stars of Extragalactic H II Regions (Bresolin+ 1999)"], "keyword_cds": "Galaxies, nearby ; H II regions ; Abundances", "keyword_pub": "techniques: spectroscopic - ISM: abundances - HII regions - galaxies: abundances", "abstract": ["Spectroscopic observations of 63 HII regions in six spiral", "galaxies (NGC628, NGC783, NGC2336, NGC6217, NGC7331 and NGC7678) were", "carried out with the 6-m telescope (BTA) of Russian Special", "Astrophysical Observatory with the Spectral Camera attached to the", "focal reducer SCORPIO in multislit mode with a dispersion of", "2.1{AA}/pixel and a spectral resolution of 10{AA}. These", "observations were used to estimate the oxygen and nitrogen abundances", "and the electron temperatures in HII regions through the recent", "variant of the strong-line method (NS calibration). The parameters of", "the radial distribution (the extrapolated central intercept value and", "the gradient) of the oxygen and nitrogen abundances in the discs of", "spiral galaxies NGC628, NGC783, NGC2336, NGC7331 and NGC7678 have been", "determined. The abundances in NGC783, NGC2336, NGC6217 and NGC7678 are", "measured for the first time. Galaxies from our sample follow well the", "general trend in the luminosity-central metallicity diagram for", "spiral and irregular galaxies."], "description": ["We selected galaxies with known UBVRI photometry of HII regions, as", "obtained by our team in previous works: NGC 628 (Bruevich et al.,", "2007ARep...51..222B), NGC 783 (Gusev, 2006ARep...50..167G,", "2006ARep...50..182G), NGC 2336 (Gusev & Park, 2003A&A...410..117G),", "NGC 6217 (Artamonov et al., 1999ARep...43..377A), NGC 7331", "(unpublished) and NGC 7678 (Artamonov, Bruevich & Gusev,", "1997ARep...41..577A)."], "type": ["OC"], "doi_pub": ["10.1111/j.1365-2966.2012.21322.x"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "The galaxy sample ", "columns": [{"name": "Gal", "desc": "Galaxy name "}, {"name": "MType", "desc": "Morphological type "}, {"name": "Bt", "desc": "BT magnitude "}, {"name": "RAh", "desc": "Right ascension of the galaxy centre (J2000) "}, {"name": "RAm", "desc": "Right ascension of the galaxy centre (J2000) "}, {"name": "RAs", "desc": "Right ascension of the galaxy centre (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Incl", "desc": "Inclination "}, {"name": "PA", "desc": "Position angle "}, {"name": "HVR", "desc": "Heliocentric radial velocity "}, {"name": "Rc25", "desc": "Isophotal radius (25mag/arcsec^2^ in the B band) corrected for Galactic extinction and absorption due to the inclination of a galaxy (arcmin)"}, {"name": "Rc25k", "desc": "Isophotal radius (25mag/arcsec^2^ in the B band) corrected for Galactic extinction and absorption due to the inclination of a galaxy (kpc)"}, {"name": "d", "desc": "Distance "}, {"name": "BMAG", "desc": "Absolute B magnitude "}]}, {"name": "table3.dat", "desc": "Offsets, galactocentric distances, radial velocities of H II regions", "columns": [{"name": "Gal", "desc": "Galaxy name "}, {"name": "HII", "desc": "HII region number, within the galaxy "}, {"name": "n_HII", "desc": "[ab] Multiplicity index on HII "}, {"name": "Pos", "desc": "Slit position "}, {"name": "Name", "desc": "?=- HII region number from other works (1) "}, {"name": "RO", "desc": "? HII region number from Rosales-Ortega et al. (2011MNRAS.415.2439R)"}, {"name": "vZ", "desc": "? HII region number from van Zee et al. (1998, cat. J/A+AS/123/305)"}, {"name": "oDE", "desc": "Offsets from the Galactic Centre, positive to the north (N-S)"}, {"name": "oRA", "desc": "Offsets from the Galactic Centre, positive to the west (E-W)"}, {"name": "rd", "desc": "Deprojected galactocentric distance "}, {"name": "RV", "desc": "Radial velocity of H II region "}]}, {"name": "table4.dat", "desc": "The reddening-corrected fluxes of the main emission lines of H II regions", "columns": [{"name": "Gal", "desc": "Galaxy "}, {"name": "HII", "desc": "HII region number within the galaxy "}, {"name": "m_HII", "desc": "Multiplicty index on HII "}, {"name": "[OII]", "desc": "?=- [OII] 3727+3729 intensity normalized to H{beta} (1)"}, {"name": "e_[OII]", "desc": "?=- rms uncertainty on [OII] "}, {"name": "[OIII]", "desc": "?=- [OIII] 5007 intensity normalized to H{beta} (1)"}, {"name": "e_[OIII]", "desc": "?=- rms uncertainty on [OIII] "}, {"name": "[NII]", "desc": "?=- [NII] 6584 intensity normalized to H{beta} (1)"}, {"name": "e_[NII]", "desc": "?=- rms uncertainty on [NII] "}, {"name": "[SII]", "desc": "?=- [NII] 6717+6731 intensity normalized to H{beta} (1)"}, {"name": "e_[SII]", "desc": "?=- rms uncertainty on [NII] "}, {"name": "FHb", "desc": "H{beta} 4861 flux "}, {"name": "e_FHb", "desc": "rms uncertainty on FHb "}, {"name": "c(Hb)", "desc": "logarithmic extinction coefficient c(H{beta}) "}, {"name": "e_c(Hb)", "desc": "rms uncertainty on c(Hb) "}]}, {"name": "table5.dat", "desc": "Oxygen and nitrogen abundances and electron temperatures t2 in H II regions derived using the NS calibrations", "columns": [{"name": "Gal", "desc": "Galaxy "}, {"name": "HII", "desc": "HII region number, within the galaxy "}, {"name": "n_HII", "desc": "[ab] Multiplicity index on HII "}, {"name": "RG", "desc": "Galacto-centric radius in units of isophotal radius R25"}, {"name": "12+log(O/H)NS", "desc": "Abundance 12+log(O/H) using the NS calibration"}, {"name": "12+log(N/H)NS", "desc": "Abundance 12+log(N/H) using the NS calibration"}, {"name": "tNSB", "desc": "Electron temperatures t2 "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_428_2085"}} {"id": "J/MNRAS/428/2085", "title_cds": "Chandra X-ray measurements of galactic coronae", "title_create": "Li+, 2013", "year": "2013", "author": "Li J.-T., Wang Q.D.", "title_pub": "Chandra survey of nearby highly inclined disc galaxies. I. X-ray measurements of galactic coronae.", "first_author": "Li J.-T.", "ref_biblio": [""], "bibcode": ["2013MNRAS.428.2085L"], "keyword_cds": "", "keyword_pub": "galaxies: general - galaxies: haloes - X-rays: galaxies", "abstract": ["We present a systematical analysis of the Chandra observations of 53", "nearby highly inclined (i>~60{deg}) disc galaxies to study the coronae", "around them. This sample covers a broad range of galaxy properties:", "e.g. about three orders of magnitude in the star formation rate and", "more than two orders of magnitude in the stellar mass. The Chandra", "observations of the diffuse soft X-ray emission from 20 of these", "galaxies are presented for the first time. The data are reduced in a", "uniform manner, including the excision/subtraction of both resolved", "and unresolved stellar contributions. Various coronal properties, such", "as the scale height and luminosity, are characterized for all the", "sample galaxies. For galaxies with high enough counting statistics, we", "also examine the thermal and chemical states of the coronal gas. We", "note on galaxies with distinct multiwavelength characteristics which", "may affect the coronal properties. The uniformly processed images,", "spectra and brightness profiles, as well as the inferred hot gas", "parameters, form a large X-ray data base for studying the coronae", "around nearby disc galaxies. We also discuss various complications", "which may cause biases to this data base and their possible", "corrections or effects, such as the uncertainty in the thermal and", "chemical states of hot gas, the different galactic disc inclination", "angles, the presence of active galactic nuclei and the contribution of", "the emission from charge exchange at interfaces between hot and cool", "gases. Results from a detailed correlation analysis are presented in a", "companion paper to gain a more comprehensive statistical understanding", "of the origin of galactic coronae."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/sts183"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_428_476"}} {"id": "J/MNRAS/428/476", "title_cds": "Group members in the Leo cloud", "title_create": "Marino+, 2013", "year": "2013", "author": "Marino A., Plana H., Rampazzo R., Bianchi L., Rosado M., Bettoni D., Galletta G., Mazzei P., Buson L., Ambrocio-Cruz P., Gabbasov R.F.", "title_pub": "Galaxy evolution in nearby loose groups. II. Photometric and kinematic characterization of USGC U268 and USGC U376 group members in the Leo cloud.", "first_author": "Marino A.", "ref_biblio": [""], "bibcode": ["2013MNRAS.428..476M"], "see_also": ["VII/237 : HYPERLEDA. I. Catalog of galaxies (Paturel+, 2003)"], "keyword_cds": "Clusters, galaxy ; Galaxies, photometry ; Radial velocities", "keyword_pub": "galaxies: evolution - galaxies: groups: individual: USGC U268 - galaxies: groups: individual: USGC U376 - galaxies: kinematics and dynamics - galaxies: photometry - ultraviolet: galaxies", "abstract": ["This paper is the second of a series of papers in which we are", "exploring the coevolution of galaxies and groups in the local", "Universe, by adopting a multiwavelength approach. Here, we present the", "photometric and kinematic characterization of two groups, USGC U268", "and USGC U376 (U268 and U376 hereafter), which are located in", "different regions of the Leo cloud. We revisit the group membership,", "using results from recent redshift surveys, and we investigate their", "substructures. U268, which is composed of 10 catalogued members and 11", "new added members, has a small fraction (~24 per cent) of", "early-type galaxies (ETGs). U376 has 16 catalogued members plus eight", "new added members, with ~38 per cent of ETGs."], "description": ["The group sample has been selected from the catalogue of Ramella et", "al. (2002, Cat. J/AJ/123/2976). The cross-matching of the member", "galaxies of the catalogue with the GALEX and SDSS (York et al.", "2000AJ....120.1579Y) archives has led to a sample of 13 nearby groups", "that have almost all of the members covered by both surveys. Here, we", "focus on two of the above groups, U268 and U376."], "type": ["OC"], "data": "", "date_update": "16-Mar-2021", "tables": [{"name": "table1.dat", "desc": "*Characteristics of the galaxy members ", "columns": [{"name": "Group", "desc": "Group name "}, {"name": "Galaxy", "desc": "Galaxy name "}, {"name": "n_Galaxy", "desc": "[f,g ] Note on Galaxy (1) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "n_Pos", "desc": "[a] Note on Position (1) "}, {"name": "MType", "desc": "Morphologycal type "}, {"name": "n_MType", "desc": "[ab] Note on MType (1) "}, {"name": "T", "desc": "? RC3 T type "}, {"name": "E(B-V)", "desc": "? Redenning (Taken from NED) "}, {"name": "Incl", "desc": "? Inclination "}, {"name": "logD25", "desc": "? Major axis diameter "}, {"name": "logr25", "desc": "? Axial ratio "}, {"name": "PA", "desc": "? Position angle "}, {"name": "n_PA", "desc": "[de] Note on PA (1) "}, {"name": "HV", "desc": "Mean heliocentric systemic velocity "}, {"name": "e_HV", "desc": "rms uncertainty on HV "}, {"name": "n_HV", "desc": "[c] Note on HV (1) "}, {"name": "BTmag", "desc": "? B total magnitude (AB mag) "}, {"name": "e_BTmag", "desc": "? rms uncertainty on BTmag "}]}, {"name": "table6.dat", "desc": "UV and optical photometry ", "columns": [{"name": "Group", "desc": "Group name "}, {"name": "Galaxy", "desc": "Galaxy name "}, {"name": "MType", "desc": "This paper morphological type "}, {"name": "FUV", "desc": "?=- FUV magnitude (AB mag) "}, {"name": "e_FUV", "desc": "? rms uncertainty on FUV "}, {"name": "NUV", "desc": "?=- NUV magnitude (AB mag) "}, {"name": "e_NUV", "desc": "? rms uncertainty on NUV "}, {"name": "umag", "desc": "?=- SDSS u magnitude (AB mag) "}, {"name": "e_umag", "desc": "? rms uncertainty on umag "}, {"name": "gmag", "desc": "?=- SDSS g magnitude (AB mag) "}, {"name": "e_gmag", "desc": "? rms uncertainty on gmag "}, {"name": "rmag", "desc": "?=- SDSS r magnitude (AB mag) "}, {"name": "e_rmag", "desc": "? rms uncertainty on rmag "}, {"name": "imag", "desc": "?=- SDSS i magnitude (AB mag) "}, {"name": "e_imag", "desc": "? rms uncertainty on imag "}, {"name": "zmag", "desc": "?=- SDSS z magnitude (AB mag) "}, {"name": "e_zmag", "desc": "? rms uncertainty on zmag "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_429_3047"}} {"id": "J/MNRAS/429/3047", "title_cds": "Observational parameters of SMGs programme", "title_create": "Bothwell+, 2013", "year": "2013", "author": "Bothwell M.S., Smail I., Chapman S.C., Genzel R., Ivison R.J., Tacconi L.J., Alaghband-zadeh S., Bertoldi F., Blain A.W., Casey C.M., Cox P., Greve T.R., Lutz D., Neri R., Omont A., Swinbank A.M.", "title_pub": "A survey of molecular gas in luminous sub-millimetre galaxies.", "first_author": "Bothwell M.S.", "ref_biblio": [""], "bibcode": ["2013MNRAS.429.3047B"], "keyword_cds": "", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: ISM - cosmology: observations", "abstract": ["We present the results from a survey of ^12^CO emission in 40 luminous", "sub-millimetre galaxies (SMGs), with 850-{mu}m fluxes of", "S_850{mu}m_=4-20mJy, conducted with the Plateau de Bure", "Interferometer. We detect ^12^CO emission in 32 SMGs at z~1.2-4.1,", "including 16 SMGs not previously published. Using multiple ^12^CO line", "(J_up_=2-7) observations, we derive a median spectral line energy", "distribution for luminous SMGs. We report the discovery of a", "fundamental relationship between ^12^CO FWHM and ^12^CO line", "luminosity in high-redshift starbursts, which we interpret as a", "natural consequence of the baryon-dominated dynamics within the", "regions probed by our observations. We use far-infrared luminosities", "to assess the star formation efficiency in our SMGs, finding that the", "slope of the L_'CO_-L_FIR_ relation is close to linear. We", "derive molecular gas masses, finding a mean gas mass of", "(5.3+/-1.0)x10^10^M_{sun}_. Combining these with dynamical masses, we", "determine the redshift evolution of the gas content of SMGs, finding", "that they do not appear to be significantly more gas rich than less", "vigorously star-forming galaxies at high redshifts. Finally, we", "collate X-ray observations, and study the interdependence of gas and", "dynamical properties of SMGs with their AGN activity and supermassive", "black hole masses (M_BH_), finding that SMGs lie significantly", "below the local M_BH_-{sigma} relation."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/sts562"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_429_L55"}} {"id": "J/MNRAS/429/L55", "title_cds": "Short Title", "title_create": "Banerji+, 2013", "year": "2013", "author": "Banerji M., Mcmahon R.G., Hewett P.C., Gonzalez-solares E., Koposov S.E.", "title_pub": "Hyperluminous reddened broad-line quasars at z ~ 2 from the VISTA Hemisphere Survey and WISE All-Sky Survey.", "first_author": "Banerji M.", "ref_biblio": [""], "bibcode": ["2013MNRAS.429L..55B"], "keyword_cds": "", "keyword_pub": "galaxies: active - quasars: emission lines - quasars: general", "abstract": ["We present the first sample of spectroscopically confirmed heavily", "reddened broad-line quasars selected using the new near-infrared VISTA", "Hemisphere Survey and Wide-field Infrared Survey Explorer} (WISE)", "all-sky survey. Observations of four candidates with (J-K)>2.5 and", "K<=16.5 over ~180deg^2^ lead to confirmation that two are highly", "dust-reddened broad-line Type 1 quasars at z~2. The typical dust", "extinctions are A_V_~ 2-2.5mag. We measure black hole masses of", "~10^9^M{sun} and extinction-corrected bolometric luminosities of", "~10^47^erg/s, making them some of the brightest Type 1 quasars", "currently known. Despite this, these quasars lie well below the", "detection limits of wide-field optical surveys like the Sloan Digital", "Sky Survey (SDSS) with i_AB_>22. We also present WISE photometry at", "3-22{mu}m, for our full sample of spectroscopically confirmed reddened", "quasars including those selected from the UKIDSS Large Area Survey. We", "demonstrate that the rest-frame infrared spectral energy distributions", "of these reddened quasars are similar to ultraviolet-luminous Type 1", "quasars with significant hot dust emission and starburst quasar hosts", "like Mrk 231. The average 12{mu}m flux density of our reddened quasars", "is similar to that of the recently discovered hyperluminous infrared", "galaxy (HyLIRG) WISE 1814+3412 (z=2.452) at similar redshifts, with", "two of our reddened quasars also having comparable 22{mu}m flux", "densities to this extreme HyLIRG. These optically faint, heavily", "reddened broad-line quasars are therefore among the most", "mid-infrared-luminous galaxies at z~2, now being discovered using", "WISE."], "description": ["VHS is a NIR photometric survey being conducted using the VISTA", "telescope in Chile that aims to survey 18000deg^2^ of the Southern", "celestial hemisphere to a depth 30 times fainter than the 2MASS survey", "in at least two wavebands (J and K). In the South Galactic Cap,", "4500deg^2^ will be imaged deeper, including the H band, and will have", "supplemental deep grizY imaging provided by the Dark Energy Survey.", "The remainder of the high galactic latitude sky will be imaged at YJHK", "and combined with optical photometry from the VST-ATLAS survey. In", "this work, we use \u223c180deg^2^ data from the VHS VST-ATLAS overlap", "region at 205{deg}"], "bibcode": ["2013MNRAS.431.1039H"], "keyword_cds": "Atomic physics", "keyword_pub": "atomic data - atomic processes - line: profiles", "abstract": ["Stark-broadening parameters have been calculated for 114 spectral", "lines of triply charged lead ion (Pbiv) using semiclassical", "perturbation approach in the impact approximation. The provided widths", "and shifts have been obtained for a set of temperatures from 20000 to", "300000K and an electron density of 10^17^cm^-3^. The studied lines", "correspond to transitions between the configurations", "5d^10^nl-5d^10^n'l' and 5d^9^6s^2^-5d^10^nl. Energy levels and", "oscillator strengths needed for this calculation have been calculated", "using a Hartree-Fock relativistic (HFR) approach. Comparison has also", "been made with available theoretical and experimental results. In", "addition, the regularity in the 5d^10^6s^2^S_1/2_-5d^10^np^2^P^o^_1/2_", "spectral series has been studied."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stt228"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_431_3510"}} {"id": "J/MNRAS/431/3510", "title_cds": "GX 339-4 X-ray binary", "title_create": "Salvesen+, 2013", "year": "2013", "author": "Salvesen G., Miller J.M., Reis R.C., Begelman M.C.", "title_pub": "Spectral hardening as a viable alternative to disc truncation in black hole state transitions.", "first_author": "Salvesen G.", "ref_biblio": [""], "bibcode": ["2013MNRAS.431.3510S"], "keyword_cds": "", "keyword_pub": "accretion, accretion discs - black hole physics - X-rays: binaries - X-rays: individual: GX 339-4", "abstract": ["Constraining the accretion flow geometry of black hole binaries in", "outburst is complicated by the inability of simplified multicolour", "disc models to distinguish between changes in the inner disc radius", "and alterations to the emergent spectrum, parametrized by the", "phenomenological colour-correction factor, f_col_. We analyse Rossi", "X-ray Timing Explorer observations of the low-mass Galactic black hole", "X-ray binary, GX 339-4, taken over seven epochs when the source was", "experiencing a state transition. The accretion disc component is", "isolated using a pipeline resulting in robust detections for disc", "luminosities, 10^-3^<~L_disc_/L_Edd_<~0.5. Assuming that the inner", "disc remains situated at the innermost stable circular orbit over the", "course of a state transition, we measure the relative degree of change", "in f_col_ required to explain the spectral evolution of the disc", "component. A variable f_col_ that increases by a factor of ~2.0-3.5 as", "the source transitions from the high/soft state to the low/hard state", "can adequately explain the observed disc spectral evolution. For the", "observations dominated by a disc component, the familiar scaling", "between the disc luminosity and effective temperature,", "L_disc_{prop.to}T_eff_^4^, is observed; however, significant", "deviations from this relation appear when GX 339-4 is in the hard", "intermediate and low/hard states. Allowing for an evolving f_col_", "between spectral states, the L_disc_-T_eff_^4^ law is recovered over", "the full range of disc luminosities, although this depends heavily on", "the physically conceivable range of f_col_. We demonstrate that", "physically reasonable changes in f_col_ provide a viable description", "for multiple state transitions of a black hole binary without invoking", "radial motion of the inner accretion disc."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stt436"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_432_2824"}} {"id": "J/MNRAS/432/2824", "title_cds": "UK IR telescope M33 monitoring project. III.", "title_create": "Javadi+, 2013", "year": "2013", "author": "Javadi A., van Loon J.T., Khosroshahi H., Mirtorabi M.T.", "title_pub": "The UK infrared telescope M33 monitoring project. III. Feedback from dusty stellar winds in the central square kiloparsec.", "first_author": "Javadi A.", "ref_biblio": [""], "bibcode": ["2013MNRAS.432.2824J"], "keyword_cds": "", "keyword_pub": "stars: AGB and post-AGB - stars: carbon - stars: mass-loss - supergiants - galaxies: individual: M33 - galaxies: structure", "abstract": ["We have conducted a near-infrared monitoring campaign at the UK", "Infrared Telescope, of the Local Group spiral galaxy M33 (Triangulum).", "The main aim was to identify stars in the very final stage of their", "evolution, and for which the luminosity is more directly related to", "the birth mass than the more numerous less evolved giant stars that", "continue to increase in luminosity. In this third paper of the series,", "we measure the dust production and rates of mass-loss by the pulsating", "asymptotic giant branch (AGB) stars and red supergiants. To this aim,", "we combined our time-averaged near-IR photometry with the multi-epoch", "mid-IR photometry obtained with the Spitzer Space Telescope. The", "mass-loss rates are seen to increase with increasing strength of", "pulsation and with increasing bolometric luminosity. Low-mass stars", "lose most of their mass through stellar winds, but even super-AGB", "stars and red supergiants lose ~ 40percent of their mass via a dusty", "stellar wind. More than three-quarters of the dust return is", "oxygenous. We construct a 2D map of the mass-return rate, showing a", "radial decline but also local enhancements due to agglomerations of", "massive stars. We estimate a total mass-loss rate of", "0.004-0.005M_{sun}_/yr/kpc^2^, increasing to ~0.006M_{sun}_/yr/kpc^2^", "when accounting for eruptive mass-loss (e.g., supernovae); comparing", "this to the current star formation rate of ~0.03M_{sun}_/yr/kpc^2^ we", "conclude that star formation in the central region of M33 can only be", "sustained if gas is accreted from further out in the disc or from", "circumgalactic regions."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stt640"], "data": "", "date_update": "11-May-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_432_3097"}} {"id": "J/MNRAS/432/3097", "title_cds": "Halpha/FUV ratios in star-forming regions", "title_create": "Hermanowicz+, 2013", "year": "2013", "author": "Hermanowicz M.T., Kennicutt R.C., Eldridge J.J.", "title_pub": "H{alpha} to FUV ratios in resolved star-forming region populations of nearby spiral galaxies.", "first_author": "Hermanowicz M.T.", "ref_biblio": [""], "bibcode": ["2013MNRAS.432.3097H"], "keyword_cds": "", "keyword_pub": "stars: formation - stars: luminosity function, mass function - HII regions - galaxies: spiral - galaxies: star formation", "abstract": ["We present a new study of H{alpha}/FUV flux ratios of star-forming", "regions within a sample of nearby spiral galaxies. We search for", "evidence of the existence of a cluster-mass-dependent truncation in", "the underlying stellar initial mass function (IMF). We use an", "automated approach to identification of extended objects based on the", "SExtractor algorithm to catalogue resolved Hii regions within a set of", "nearby spiral galaxies. Corrections due to dust attenuation effects", "are applied to avoid artificially boosted H{alpha}/FUV values. We use", "thebpass stellar population synthesis code to create a benchmark", "population of star-forming regions to act as a reference for our", "observations. Based on those models, we identify a zone of parameter", "space populated by regions that cannot be obtained with a", "cluster-mass-dependent truncation in the stellar IMF imposed. We find", "that the investigated galaxies display small subpopulations of", "star-forming regions falling within our zone of interest, which", "appears to be inconsistent with imposing an IMF truncation at maximum", "stellar mass dependent on the total cluster mass. The presence of", "those regions is expected in models using both stochastic and sorted", "sampling of the full extent of the stellar IMF. This result persists", "after taking dust attenuation effects into account. We highlight the", "significance of stochastic effects in environments with low star", "formation activity and in studies describing systems associated with", "small physical scales."], "object": [], "curator": "Patricia Vannier [CDS]", "alias": ["[HKE2013]"], "doi_pub": ["10.1093/mnras/stt665"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_437_195"}} {"id": "J/MNRAS/437/195", "title_cds": "Super and massive AGB stars nucleosynthesis", "title_create": "Doherty+, 2014", "year": "2014", "author": "Doherty C.L., Gil-pons P., Lau H.H.B., Lattanzio J.C., Siess L.", "title_pub": "Super and massive AGB stars. II. Nucleosynthesis and yields. Z = 0.02, 0.008 and 0.004.", "first_author": "Doherty C.L.", "ref_biblio": [""], "bibcode": ["2014MNRAS.437..195D"], "see_also": ["J/A+A/512/A10 : Evolution of massive AGB stars. III. (Siess, 2010)"], "keyword_cds": "Models, evolutionary ; Stars, giant", "keyword_pub": "nuclear reactions - nucleosynthesis, abundances - stars: AGB and post-AGB - ISM: abundances", "abstract": ["We have computed detailed evolution and nucleosynthesis models for", "super and massive asymptotic giant branch (AGB) stars over the mass", "range 6.5-9.0M_{sun}_ in divisions of 0.5M_{sun}_ with metallicities", "Z=0.02, 0.008 and 0.004. These calculations, in which we find third", "dredge-up and hot bottom burning, fill the gap between existing low-", "and intermediate-mass AGB star models and high-mass star models that", "become supernovae. For the considered metallicities, the composition", "of the yields is largely dominated by the thermodynamic conditions at", "the base of the convective envelope rather than by the pollution", "arising from third dredge-up. We investigate the effects of various", "uncertainties, related to the mass-loss rate, mixing length parameter,", "and the treatment of evolution after the envelope instability that", "develops near the end of the (super)AGB phase. Varying these", "parameters alters the yields mainly because of their impact on the", "amount of third dredge-up enrichment, and to a lesser extent on the", "hot bottom burning conditions. Our models produce significant amounts", "of ^4^He, ^7^Li (depending on the mass-loss formulation) ^13^C, ^14^N,", "^17^O, ^23^Na, ^25^Mg, as well the radioactive isotope ^26^Al in", "agreement with previous investigation. In addition, our results show", "enrichment of ^22^Ne, ^26^Mg and ^60^Fe, as well as a substantial", "increase in our proxy neutron capture species representing all species", "heavier than iron. These stars may provide important contributions to", "the Galaxy's inventory of the heavier Mg isotopes, ^14^N, ^7^Li and", "^27^Al."], "doi_pub": ["10.1093/mnras/stt1877"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "tableb1.dat", "desc": "VW93 model ", "columns": [{"name": "M", "desc": "Initial mass "}, {"name": "---", "desc": "[M] "}, {"name": "---", "desc": "[Z=] "}, {"name": "Z", "desc": "Initial metallicity "}, {"name": "Mod", "desc": "Model "}, {"name": "Species", "desc": "Species "}, {"name": "Yield", "desc": "Yield "}, {"name": "MassExp", "desc": " "}, {"name": "ProdFact", "desc": " "}, {"name": "E-Yield", "desc": " "}, {"name": "E-MassExp", "desc": " "}, {"name": "E-ProdFact", "desc": " "}]}, {"name": "tableb2.dat", "desc": "VW-M model ", "columns": [{"name": "M", "desc": "Initial mass "}, {"name": "---", "desc": "[M] "}, {"name": "---", "desc": "[Z=] "}, {"name": "Z", "desc": "Initial metallicity "}, {"name": "Mod", "desc": "Model "}, {"name": "Species", "desc": "Species "}, {"name": "Yield", "desc": "Yield "}, {"name": "MassExp", "desc": " "}, {"name": "ProdFact", "desc": " "}, {"name": "E-Yield", "desc": " "}, {"name": "E-MassExp", "desc": " "}, {"name": "E-ProdFact", "desc": " "}]}, {"name": "tableb3.dat", "desc": "Test cases for 8.5M ", "columns": [{"name": "M", "desc": "Initial mass "}, {"name": "---", "desc": "[M] "}, {"name": "---", "desc": "[Z=] "}, {"name": "Z", "desc": "Initial metallicity "}, {"name": "Mod", "desc": "Model "}, {"name": "Species", "desc": "Species "}, {"name": "Yield", "desc": "Yield "}, {"name": "MassExp", "desc": " "}, {"name": "ProdFact", "desc": " "}, {"name": "E-Yield", "desc": " "}, {"name": "E-MassExp", "desc": " "}, {"name": "E-ProdFact", "desc": " "}]}, {"name": "tableb4.dat", "desc": "Initial Compositions (Mass Fractions) ", "columns": [{"name": "Species", "desc": "Species "}, {"name": "IC20", "desc": "Initial composition for Z=0.02 "}, {"name": "IC8", "desc": "Initial composition for Z=0.008 "}, {"name": "IC4", "desc": "Initial composition for Z=0.004 "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_438_2753"}} {"id": "J/MNRAS/438/2753", "title_cds": "Galactic disc evolution", "title_create": "Mitschang+, 2014", "year": "2014", "author": "Mitschang A.W., De Silva G., Zucker D.B., Anguiano B., Bensby T., Feltzing S.", "title_pub": "Quantitative chemical tagging, stellar ages and the chemo-dynamical evolution of the Galactic disc.", "first_author": "Mitschang A.W.", "ref_biblio": [""], "bibcode": ["2014MNRAS.438.2753M"], "keyword_cds": "", "keyword_pub": "techniques: miscellaneous - stars: abundances - Galaxy: disc - Galaxy: evolution - open clusters and associations: general", "abstract": ["The early science results from the new generation of high-resolution", "stellar spectroscopic surveys, such as Galactic Archaeology with", "HERMES (GALAH) and the Gaia European Southern Observatory survey", "(Gaia-ESO), will represent major milestones in the quest to", "chemically tag the Galaxy. Yet this technique to reconstruct dispersed", "coeval stellar groups has remained largely untested until recently. We", "build on previous work that developed an empirical chemical tagging", "probability function, which describes the likelihood that two field", "stars are conatal, that is, they were formed in the same cluster", "environment. In this work, we perform the first ever blind chemical", "tagging experiment, i.e. tagging stars with no known or otherwise", "discernible associations, on a sample of 714 disc field stars with a", "number of high-quality high-resolution homogeneous metal abundance", "measurements. We present evidence that chemical tagging of field stars", "does identify coeval groups of stars, yet these groups may not", "represent distinct formation sites, e.g. as in dissolved open", "clusters, as previously thought. Our results point to several", "important conclusions, among them that group finding will be limited", "strictly to chemical abundance space, e.g. stellar ages, kinematics,", "colours, temperature and surface gravity do not enhance the", "detectability of groups. We also demonstrate that in addition to its", "role in probing the chemical enrichment and kinematic history of the", "Galactic disc, chemical tagging represents a powerful new stellar age", "determination technique."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stt2320"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_440_1880"}} {"id": "J/MNRAS/440/1880", "title_cds": "Eigenvectors for galaxy SED classification", "title_create": "Wild+, 2014", "year": "2014", "author": "Wild V., Almaini O., Cirasuolo M., Dunlop J., Mclure R., Bowler R., Ferreira J., Bradshaw E., Chuter R., Hartley W.", "title_pub": "A new method for classifying galaxy SEDs from multiwavelength photometry.", "first_author": "Wild V.", "ref_biblio": [""], "bibcode": ["2014MNRAS.440.1880W"], "keyword_cds": "Galaxies, photometry ; Models", "keyword_pub": "methods: statistical - galaxies: fundamental parameters - galaxies: luminosity function, mass function - galaxies: photometry - galaxies: statistics - galaxies: stellar content", "abstract": ["We present a new method to classify the broad-band", "optical-near-infrared spectral energy distributions (SEDs) of galaxies", "using three shape parameters (super-colours) based on a principal", "component analysis of model SEDs. As well as providing a compact", "representation of the wide variety of SED shapes, the method allows", "for easy visualization of information loss and biases caused by the", "incomplete sampling of the rest-frame SED as a function of redshift.", "We apply the method to galaxies in the United Kingdom Infrared", "Telescope Infrared Deep Sky Survey Ultra Deep Survey with 0.9~10 percent of their mass", "in a recent unsustained starburst event; and metal-poor quiescent", "dwarf galaxies. We find that quiescent galaxies account for 45 percent", "of galaxies with logM*/M_{sun}_>11, declining steadily to 13", "percent at logM*/M_{sun}_=10. The properties and mass function", "of the post-starburst galaxies are consistent with a scenario in which", "gas-rich mergers contribute to the growth of the low- and", "intermediate-mass range of the red sequence."], "description": ["Eigenvector used for the analysis."], "type": ["MC"], "doi_pub": ["10.1093/mnras/stu212"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "udsz.dat", "desc": "Eigenbasis information ", "columns": [{"name": "Filt", "desc": "Filter name (1) "}, {"name": "z", "desc": "Redshift of galaxy that would use this element "}, {"name": "lambda", "desc": "Effective wavelength of this filter at this redshift"}, {"name": "Flux", "desc": "Eigenbasis mean array in normalised f_lambda_ "}, {"name": "E1", "desc": "First eigenvector in normalised f_lambda__ "}, {"name": "E2", "desc": "Second eigenvector in normalised f_lambda_ "}, {"name": "E3", "desc": "Third eigenvector in normalised f_lambda_ "}]}, {"name": "vwsc_mnras_example.pro", "desc": "Program for calculating the first 3 super-colours for galaxies with 0.9"], "bibcode": ["2015MNRAS.446.4205B"], "keyword_cds": "", "keyword_pub": "stars: activity - binaries: eclipsing - stars: flare - starspots", "abstract": ["We review the results of the 1988 multiwavelength campaign on the", "late-type eclipsing binary YY Geminorum. Observations include:", "broad-band optical and near-infrared photometry, simultaneous optical", "and ultraviolet ({\\it IUE}) spectroscopy, X-ray ({\\it Ginga}) and", "radio (VLA) data. From models fitted to the optical light curves,", "fundamental physical parameters have been determined together with", "evidence for transient maculations (spots) located near quadrature", "longitudes and intermediate latitudes. Eclipses were observed at", "optical, ultraviolet and radio wavelengths. Significant drops in 6 cm", "radio emission near the phases of both primary and secondary eclipse", "indicate relatively compact radio emitting volumes that may lie", "between the binary components. {\\it IUE} observations during secondary", "eclipse are indicative of a uniform chromosphere saturated with Mg ii", "emission and an extended volume of Ly{alpha} emission. Profile fitting", "of high-dispersion H{alpha} spectra confirms the chromospheric", "saturation and indicates significant H{alpha} opacity to heights of a", "few percent of the photospheric radius. There is evidence for an", "enhanced H{alpha} emission region visible near phase 0.25-0.35 which", "may be associated with a large spot on the primary and with two small", "optical flares which were also observed at other wavelengths: one in", "microwave radiation and the other in X-rays. For both flares, {\\it", "L}X/{\\it L}opt is consistent with energy release in closed magnetic", "structures."], "object": ["07 34 37.58 +31 52 11.0 YY Geminorum = * alf Gem C"], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1093/mnras/stu2398"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_446_599"}} {"id": "J/MNRAS/446/599", "title_cds": "Seyfert and LINER galaxies", "title_create": "Singh+, 2015", "year": "2015", "author": "Singh V., Ishwara-Chandra C.H., Wadadekar Y., Beelen A., Kharb P.", "title_pub": "Kiloparsec-scale radio emission in Seyfert and LINER galaxies.", "first_author": "Singh V.", "ref_biblio": [""], "bibcode": ["2015MNRAS.446..599S"], "see_also": ["VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)", "VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)", "VIII/92 : The FIRST Survey Catalog, Version 2014Dec17 (Helfand+ 2015)"], "keyword_cds": "Galaxies, Seyfert ; Galaxies, radio", "keyword_pub": "galaxies: active - galaxies: Seyfert - radio continuum: galaxies", "abstract": ["Seyfert and LINER galaxies are known to exhibit compact radio emission", "on ~10-100pc scales, but larger Kiloparsec-Scale Radio structures", "(KSRs) often remain undetected in sub-arcsec high-resolution", "observations. We investigate the prevalence and nature of KSRs in", "Seyfert and LINER galaxies using the 1.4GHz VLA FIRST and NVSS", "observations. Our sample consists of 2651 sources detected in FIRST", "and of these 1737 sources also have NVSS counterparts. Considering the", "ratio of total to peak flux density ({theta}=(S_int_/S_peak_)^1/2^) as", "a parameter to infer the presence of extended radio emission we show", "that >=30% of FIRST-detected sources possess extended radio structures", "on scales larger than 1.0kpc. The use of low-resolution NVSS", "observations help us to recover faint extended KSRs that are resolved", "out in FIRST observations and results in >=42.5% KSR sources in", "FIRST-NVSS sub-sample. This fraction is only a lower limit owing to", "the combination of projection, resolution and sensitivity effects. Our", "study demonstrates that KSRs may be more common than previously", "thought and are found across all redshifts, luminosities and radio", "loudness. The extranuclear radio luminosity of KSR sources is found to", "be positively correlated with the core radio luminosity as well as the", "[OIII] {lambda}5007{AA} line luminosity and this can be interpreted as", "KSRs being powered by AGN rather than star formation. The", "distributions of the FIR-to-radio ratios and mid-IR colours of KSR", "sources are also consistent with their AGN origin. However,", "contribution from star formation cannot be ruled out particularly in", "sources with low radio luminosities."], "description": ["Our sample of Seyfert and LINER galaxies is derived from the 13th", "edition AGN catalogue of Veron-Cetty & Veron (2010A&A...518A..10V,", "Cat. VII/258) which is the most updated complete survey of the", "literature and lists all the quasars, BL Lacs, active galaxies known", "to the catalogue authors prior to 2009 July 1."], "doi_pub": ["10.1093/mnras/stu2124"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "tablea1.dat", "desc": "First 10 entries of our cross-matched catalogue of VV10 and FIRST and NVSS for our sample of Seyfert and LINER galaxies", "columns": [{"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sing (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "z", "desc": "Redshfit (from VV10) "}, {"name": "Type", "desc": "Seyfert type (from VV10) (1) "}, {"name": "Vmag", "desc": "V mangitude (from VV10) "}, {"name": "SpF", "desc": "FIRST 1.4GHz peak flux density "}, {"name": "SintF", "desc": "FIRST integrated 1.4GH flux density "}, {"name": "SizeF1", "desc": "FIRST fitted source size "}, {"name": "---", "desc": "[x] "}, {"name": "SizeF2", "desc": "FIRST fitted source size "}, {"name": "PAF", "desc": "Position angle of FIRST source "}, {"name": "RF", "desc": "Offset of FIRST counterpart from optical position "}, {"name": "SintN", "desc": "NVSS total flux density "}, {"name": "SizeN1", "desc": "NVSS fitted source size "}, {"name": "---", "desc": "[x] "}, {"name": "SizeN2", "desc": "NVSS fitted source size "}, {"name": "PAN", "desc": "Position angle of NVSS source "}, {"name": "RN", "desc": "Offset of NVSS position from optical position "}, {"name": "thetaF", "desc": "{theta}_FIRST_=(SintF/SpF)^1/2^ "}, {"name": "thetaN-F", "desc": "{theta}_NVSS-FIRST_=(SintN/SintF)^1/2^ "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_448_1945"}} {"id": "J/MNRAS/448/1945", "title_cds": "Short Title", "title_create": "Helminiak+, 2015", "year": "2015", "author": "Helminiak K.G., Graczyk D., Konacki M., Pilecki B., Ratajczak M., Pietrzynski G., Sybilski P., Villanova S., Gieren W., Pojmanski G., Konorski P., Suchomska K., Reichart D.E., Ivarsen K.M., Haislip J.B., Lacluyze A.P.", "title_pub": "Orbital and physical parameters of eclipsing binaries from the ASAS catalogue - VIII. The totally eclipsing double-giant system HD 187669.", "first_author": "Helminiak K.G.", "ref_biblio": [""], "bibcode": ["2015MNRAS.448.1945H"], "keyword_cds": "", "keyword_pub": "binaries: eclipsing - binaries: spectroscopic - stars: evolution - stars: fundamental parameters - stars: individual: HD 187669 - stars: late-type", "abstract": ["We present the first full orbital and physical analysis of HD 187669,", "recognized by the All-Sky Automated Survey (ASAS) as the eclipsing", "binary ASAS J195222-3233.7. We combined multi-band photometry from the", "ASAS and SuperWASP public archives and 0.41-m PROMPT robotic", "telescopes with our high-precision radial velocities from the HARPS", "spectrograph. Two different approaches were used for the analysis: (1)", "fitting to all data simultaneously with the WD code and (2) analysing", "each light curve (with jktebop) and radial velocities separately and", "combining the partial results at the end. This system also shows a", "total primary (deeper) eclipse, lasting for about 6 d. A spectrum", "obtained during this eclipse was used to perform atmospheric analysis", "with the moog and sme codes to constrain the physical parameters of", "the secondary. We found that ASAS J195222-3233.7 is a double-lined", "spectroscopic binary composed of two evolved, late-type giants, with", "masses of {\\it M}1 = 1.504+/-0.004 and {\\it M}2 = 1.505+/-0.004", "M_{sun}_, and radii of {\\it R}1 = 11.33+/-0.28 and {\\it R}2 =", "22.62+/-0.50 R_{sun}_. It is slightly less metal abundant than the", "Sun, and has a {\\it P} = 88.39 d orbit. Its properties are well", "reproduced by a 2.38-Gyr isochrone, and thanks to the metallicity", "estimation from the totality spectrum and high precision of the", "masses, it was possible to constrain the age down to 0.1Gyr. It is the", "first so evolved Galactic eclipsing binary measured with such good", "accuracy, and as such it is a unique benchmark for studying the late", "stages of stellar evolution."], "object": ["19 52 22.08 -32 33 39.7 HD 187669 = ASAS J195222-3233.7"], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1093/mnras/stu2680"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_448_3132"}} {"id": "J/MNRAS/448/3132", "title_cds": "Planetary nebula central stars binary fraction", "title_create": "Douchin+, 2015", "year": "2015", "author": "Douchin D., De Marco O., Frew D.J., Jacoby G.H., Jasniewicz G., Fitzgerald M., Passy J.-C., Harmer D., Hillwig T., Moe M.", "title_pub": "The binary fraction of planetary nebula central stars. II. A larger sample and improved technique for the infrared excess search.", "first_author": "Douchin D.", "ref_biblio": [""], "bibcode": ["2015MNRAS.448.3132D"], "see_also": ["J/MNRAS/428/2118 : Binarity in planetary nebula central stars (De Marco+ 2013)"], "keyword_cds": "", "keyword_pub": "techniques: photometric - surveys; binaries: general - stars: evolution - stars: statistics - planetary nebulae: general", "abstract": ["There is no conclusive explanation of why ~80% of planetary nebulae", "(PNe) are non-spherical. In the Binary Hypothesis, a binary", "interaction is a preferred channel to form a non-spherical PN. A", "fundamental step to corroborate or disprove the Binary Hypothesis is", "to estimate the binary fraction of central stars of PNe (CSPNe) and", "compare it with a prediction based on the binary fraction of the", "progenitor, main-sequence population. In this paper, the second in a", "series, we search for spatially unresolved I- and J-band flux excess", "in an extended sample of 34 CSPN by a refined measurement technique", "with a better quantification of the uncertainties. The detection rate", "of I- (J-)band flux excess is 32+/-16% (50+/-24%). This result is very", "close to what was obtained in with a smaller sample. We account", "conservatively for unobserved cool companions down to brown dwarf", "luminosities, increasing these fractions to 40+/-20% (62+/-30%). This", "step is very sensitive to the adopted brightness limit of our survey.", "Accounting for visual companions increases the binary fraction to", "46+/-23% (71+/-34%). These figures are lower than in. The error bars", "are better quantified, but still unacceptably large. Taken at face", "value, the current CSPN binary fraction is in line with the", "main-sequence progenitor population binary fraction. However,", "including white dwarfs companions could increase this fraction by as", "much as 13 (21) per cent points."], "description": ["Our Johnso-\u2013Cousins U, B, V and I images were taken during a seven", "night observing run at the National Optical Astronomical Observatory", "(NOAO) 2.1-m telescope at Kitt Peak between 2011 March 11 and 17."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stu2700"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_448_3382"}} {"id": "J/MNRAS/448/3382", "title_cds": "Short Title", "title_create": "Tanga+, 2015", "year": "2015", "author": "Tanga P., Carry B., Colas F., Delbo M., Matter A., Hanus J., Ali Lagoa V., Andrei A.H., Assafin M., Audejean M., Behrend R., Camargo J.I.B., Carbognani A., Cedres Reyes M., Conjat M., Cornero N., Coward D., Crippa R., De Ferra Fantin E., Devogele M., Dubos G., Frappa E., Gillon M., Hamanowa H., Jehin E., Klotz A., Kryszczynska A., Lecacheux J., Leroy A., Manfroid J., Manzini F., Maquet L., Morelle E., Mottola S., Polinska M., Roy R., Todd M., Vachier F., Vera Hernandez C., Wiggins P.", "title_pub": "The non-convex shape of (234) Barbara, the first Barbarian.", "first_author": "Tanga P.", "ref_biblio": [""], "bibcode": ["2015MNRAS.448.3382T"], "keyword_cds": "", "keyword_pub": "Techniques: photometric - Techniques: polarimetry - occultations - Minor planets - asteroids: individual: 234 Barbara", "abstract": ["Asteroid (234) Barbara is the prototype of a category of asteroids", "that has been shown to be extremely rich in refractory inclusions, the", "oldest material ever found in the Solar system. It exhibits several", "peculiar features, most notably its polarimetric behaviour. In recent", "years other objects sharing the same property (collectively known as", "`Barbarians') have been discovered. Interferometric observations in", "the mid-infrared with the ESO VLTI (Very Large Telescope", "Interferometer) suggested that (234) Barbara might have a bi-lobated", "shape or even a large companion satellite. We use a large set of 57", "optical light curves acquired between 1979 and 2014, together with the", "timings of two stellar occultations in 2009, to determine the rotation", "period, spin-vector coordinates, and 3-D shape of (234) Barbara, using", "two different shape reconstruction algorithms. By using the light", "curves combined to the results obtained from stellar occultations, we", "are able to show that the shape of (234) Barbara exhibits large", "concave areas. Possible links of the shape to the polarimetric", "properties and the object evolution are discussed. We also show that", "VLTI data can be modelled without the presence of a satellite."], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1093/mnras/stv229"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_448_3442"}} {"id": "J/MNRAS/448/3442", "title_cds": "Galaxy Zoo", "title_create": "Galloway+, 2015", "year": "2015", "author": "Galloway M.A., Willett K.W., Fortson L.F., Cardamone C.N., Schawinski K., Cheung E., Lintott C.J., Masters K.L., Melvin T., Simmons B.D.", "title_pub": "Galaxy Zoo: the effect of bar-driven fuelling on the presence of an active galactic nucleus in disc galaxies.", "first_author": "Galloway M.A.", "ref_biblio": [""], "bibcode": ["2015MNRAS.448.3442G"], "keyword_cds": "", "keyword_pub": "galaxies: active - galaxies: Seyfert - galaxies: spiral", "abstract": ["We study the influence of the presence of a strong bar in disc", "galaxies which host an active galactic nucleus (AGN). Using data from", "the Sloan Digital Sky Survey and morphological classifications from", "the Galaxy Zoo 2 project, we create a volume-limited sample of 19756", "disc galaxies at 0.01"], "bibcode": ["2015MNRAS.452.3776G"], "keyword_cds": "", "keyword_pub": "galaxies: active - infrared: galaxies", "abstract": ["We examine the relationship between star formation and active galactic", "nuclei (AGN) activity by constructing matched samples of local", "(0"], "bibcode": ["2015MNRAS.452..884N"], "keyword_cds": "", "keyword_pub": "stars: emission-line, Be - stars: Wolf-Rayet - X-rays: binaries - X-rays: stars", "abstract": ["The nature of the low- to intermediate-luminosity (LX~10^32-34^erg/s)", "source population revealed in hard band (2-10keV) X-ray surveys of the", "Galactic plane is poorly understood. To overcome such problem, we", "cross-correlated the XMM-Newton 3XMM-DR4 survey with the infrared Two", "Micron All Sky Survey and Galactic Legacy Infrared Mid-Plane Survey", "Extraordinaire catalogues. We identified reliable X-ray-infrared", "associations for 690 sources. We selected 173 sources having hard", "X-ray spectra, typical of hard X-ray high-mass stars (kT>5keV), and", "517 sources having soft X-ray spectra, typical of active coronae.", "About 18 per cent of the soft sources are classified in the", "literature: ~91 percent as stars, with a minor fraction of Wolf-Rayet", "(WR) stars. Roughly 15 per cent of the hard sources are classified in", "the literature: ~68 percent as high-mass X-ray stars single or in", "binary systems (WR, Be and high-mass X-ray binaries - HMXBs), with a", "small fraction of G and B stars. We carried out infrared spectroscopic", "pilot observations at the William Herschel Telescope for five hard", "X-ray sources. Three of them are high-mass stars with spectral types", "WN7-8h, Ofpe/WN9 and Be, and LX~10^32^-10^33^erg/s. One source is a", "colliding-wind binary, while another source is a colliding-wind binary", "or a supergiant fast X-ray transient in quiescence. The Be star is a", "likely {gamma}-Cas system. The nature of the other two X-ray sources", "is uncertain. The distribution of hard X-ray sources in the parameter", "space made of X-ray hardness ratio, infrared colours and", "X-ray-to-infrared flux ratio suggests that many of the unidentified", "sources are new {gamma}-Cas analogues, WRs and low LX HMXBs. However,", "the nature of the X-ray population with Ks>=11 and average", "X-ray-to-infrared flux ratio remains unconstrained."], "description": ["We cross-matched the 3XMM-DR4 catalogue with the 2MASS and GLIMPSE", "catalogues using the method developed by Pineau et al.", "(2011A&A...527A.126P, Cat. J/A+A/527/A126)."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stv1020"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_453_172"}} {"id": "J/MNRAS/453/172", "title_cds": "Short Title", "title_create": "Ponti+, 2015", "year": "2015", "author": "Ponti G., Morris M.R., Terrier R., Haberl F., Sturm R., Clavel M., Soldi S., Goldwurm A., Predehl P., Nandra K., Belanger G., Warwick R.S., Tatischeff V.", "title_pub": "The XMM-Newton view of the central degrees of the Milky Way.", "first_author": "Ponti G.", "ref_biblio": [""], "bibcode": ["2015MNRAS.453..172P"], "keyword_cds": "", "keyword_pub": "plasmas - methods: data analysis - ISM: bubbles - ISM: kinematics and dynamics - ISM: supernova remnants - Galaxy: centre", "abstract": ["The deepest XMM-Newton mosaic map of the central 1.5{deg} of the", "Galaxy is presented, including a total of about 1.5Ms of EPIC-pn", "cleaned exposures in the central 15arcsec and about 200ks outside.", "This compendium presents broad-band X-ray continuum maps, soft X-ray", "intensity maps, a decomposition into spectral components and a", "comparison of the X-ray maps with emission at other wavelengths. Newly", "discovered extended features, such as supernova remnants (SNRs),", "superbubbles and X-ray filaments are reported. We provide an atlas of", "extended features within +/-1{deg} of Sgr A*. We discover the", "presence of a coherent X-ray-emitting region peaking around G0.1-0.1", "and surrounded by the ring of cold, mid-IR-emitting material known", "from previous work as the 'Radio Arc Bubble' and with the addition of", "the X-ray data now appears to be a candidate superbubble. Sgr A's", "bipolar lobes show sharp edges, suggesting that they could be the", "remnant, collimated by the circumnuclear disc, of an SN explosion that", "created the recently discovered magnetar, SGR J1745-2900. Soft X-ray", "features, most probably from SNRs, are observed to fill holes in the", "dust distribution, and to indicate a direct interaction between SN", "explosions and Galactic centre (GC) molecular clouds. We also discover", "warm plasma at high Galactic latitude, showing a sharp edge to its", "distribution that correlates with the location of known radio/mid-IR", "features such as the 'GC Lobe'. These features might be associated", "with an inhomogeneous hot 'atmosphere' over the GC, perhaps fed by", "continuous or episodic outflows of mass and energy from the GC region."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stv1331"], "orcid_pub": ["0000-0003-0293-3608"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_453_3685"}} {"id": "J/MNRAS/453/3685", "title_cds": "Shapley Supercluster Survey", "title_create": "Mercurio+, 2015", "year": "2015", "author": "Mercurio A., Merluzzi P., Busarello G., Grado A., Limatola L., Haines C.P., Brescia M., Cavuoti S., Dopita M., Dall'ora M., Capaccioli M., Napolitano N., Pimbblet K.A.", "title_pub": "Shapley Supercluster Survey: construction of the photometric catalogues and i-band data release.", "first_author": "Mercurio A.", "ref_biblio": [""], "bibcode": ["2015MNRAS.453.3685M"], "keyword_cds": "", "keyword_pub": "methods: data analysis; methods: observational; catalogues virtual observatory tools; galaxies: clusters: general galaxies: photometry", "mission": "", "abstract": ["The Shapley Supercluster Survey is a multi-wavelength survey covering an area of ~ 23 deg2 ( ~ 260 Mpc2 at {\\it z} = 0.048) around the supercluster core, including nine Abell and two poor clusters, having redshifts in the range 0.045-0.050. The survey aims to investigate the role of the cluster-scale mass assembly on the evolution of galaxies, mapping the effects of the environment from the cores of the clusters to their outskirts and along the filaments. The optical ({\\it ugri}) imaging acquired with OmegaCAM on the VLT Survey Telescope is essential to achieve the project goals providing accurate multi-band photometry for the galaxy population down to {\\it m}* + 6. We describe the methodology adopted to construct the optical catalogues and to separate extended and point-like sources. The catalogues reach average 5{sigma} limiting magnitudes within a 3 arcsec diameter aperture of {\\it ugri} = [24.4,24.6,24.1,23.3] and are 93 percent complete down to {\\it ugri} = [23.8,23.8,23.5,22.0] mag, corresponding to", "~ {\\it m}*{\\it r} + 8.5. The data are highly uniform in terms of observing conditions and all acquired with seeing less than 1.1 arcsec full width at half-maximum. The median seeing in {\\it r} band is 0.6 arcsec, corresponding to 0.56 kpc \\begin{tex}$h^{-1}_{70}$\\end{tex} at {\\it z} = 0.048. While the observations in the {\\it u}, {\\it g} and {\\it r} bands are still ongoing, the {\\it i}-band observations have been completed, and we present the {\\it i}-band catalogue over the whole survey area. The latter is released and it will be regularly updated, through the use of the Virtual Observatory tools. This includes 734 319 sources down to {\\it i} = 22.0 mag and it is the first optical homogeneous catalogue at such a depth, covering the central region of the Shapley supercluster."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stv1905"], "orcid_pub": ["0000-0001-9261-7849"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_458_1267"}} {"id": "J/MNRAS/458/1267", "title_cds": "Short Title", "title_create": "Verbiest+, 2016", "year": "2016", "author": "Verbiest J.P.W., Lentati L., Hobbs G., Van Haasteren R., Demorest P.B., Janssen G.H., Wang J.-B., Desvignes G., Caballero R.N., Keith M.J., Champion D.J., Arzoumanian Z., Babak S., Bassa C.G., Bhat N.D.R., Brazier A., Brem P., Burgay M., Burke-spolaor S., Chamberlin S.J., Chatterjee S., Christy B., Cognard I., Cordes J.M., Dai S., Dolch T., Ellis J.A., Ferdman R.D., Fonseca E., Gair J.R., Garver-daniels N.E., Gentile P., Gonzalez M.E., Graikou E., Guillemot L., Hessels J.W.T., Jones G., Karuppusamy R., Kerr M., Kramer M., Lam M.T., Lasky P.D., Lassus A., Lazarus P., Lazio T.J.W., Lee K.J., Levin L., Liu K., Lynch R.S., Lyne A.G., Mckee J., Mclaughlin M.A., Mcwilliams S.T., Madison D.R., Manchester R.N., Mingarelli C.M.F., Nice D.J., Oslowski S., Palliyaguru N.T., Pennucci T.T., Perera B.B.P., Perrodin D., Possenti A., Petiteau A., Ransom S.M., Reardon D., Rosado P.A., Sanidas S.A., Sesana A., Shaifullah G., Shannon R.M., Siemens X., Simon J., Smits R., Spiewak R., Stairs I.H., Stappers B.W., Stinebring D.R., Stovall K., Swiggum J.K., Taylor S.R., Theureau G., Tiburzi C., Toomey L., Vallisneri M., Van Straten W., Vecchio A., Wang Y., Wen L., You X.P., Zhu W.W., Zhu X.-J.", "title_pub": "The International Pulsar Timing Array: First data release.", "first_author": "Verbiest J.P.W.", "ref_biblio": [""], "bibcode": ["2016MNRAS.458.1267V"], "keyword_cds": "", "keyword_pub": "methods: data analysis - pulsars: general", "abstract": ["The highly stable spin of neutron stars can be exploited for a variety", "of (astro)physical investigations. In particular, arrays of pulsars", "with rotational periods of the order of milliseconds can be used to", "detect correlated signals such as those caused by gravitational waves.", "Three such 'pulsar timing arrays' (PTAs) have been set up around", "the world over the past decades and collectively form the", "'International' PTA (IPTA). In this paper, we describe the first", "joint analysis of the data from the three regional PTAs, i.e. of the", "first IPTA data set. We describe the available PTA data, the approach", "presently followed for its combination and suggest improvements for", "future PTA research. Particular attention is paid to subtle details", "(such as underestimation of measurement uncertainty and long-period", "noise) that have often been ignored but which become important in this", "unprecedentedly large and inhomogeneous data set. We identify and", "describe in detail several factors that complicate IPTA research and", "provide recommendations for future pulsar timing efforts. The first", "IPTA data release presented here (and available online) is used to", "demonstrate the IPTA's potential of improving upon gravitational-wave", "limits placed by individual PTAs by a factor of ~2 and provides a", "2{sigma} limit on the dimensionless amplitude of a stochastic", "gravitational-wave background of 1.7x10^-15^ at a frequency of", "1yr^-1^. This is 1.7 times less constraining than the limit placed by", "Shannon et al. (2010ApJ...725.1607S), due mostly to the more recent,", "high-quality data they used."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw347"], "orcid_pub": ["0000-0002-4088-896X"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_458_425"}} {"id": "J/MNRAS/458/425", "title_cds": "Short Title", "title_create": "van Vledder+, 2016", "year": "2016", "author": "van Vledder I., Van Der Vlugt D., Holwerda B.W., Kenworthy M.A., Bouwens R.J., Trenti M.", "title_pub": "The size and shape of the Milky Way disc and halo from M-type brown dwarfs in the BoRG survey.", "first_author": "van Vledder I.", "ref_biblio": [""], "bibcode": ["2016MNRAS.458..425V"], "keyword_cds": "", "keyword_pub": "techniques: photometric- stars: low-mass - stars: luminosity function, mass function - Galaxy: disc - Galaxy: halo - Galaxy: stellar content", "abstract": ["We have identified 274 M-type brown dwarfs in the Hubble Space", "Telescope's Wide Field Camera 3 pure parallel fields from the", "Brightest of Reionizing Galaxies (BoRG) survey for high-redshift", "galaxies. These are near-infrared observations with multiple lines of", "sight out of our Milky Way. Using these observed M-type brown dwarfs,", "we fitted a Galactic disc and halo model with a Markov chain Monte", "Carlo analysis. This model worked best with the scalelength of the", "disc fixed at h=2.6kpc. For the scaleheight of the disc, we found", "z0=0.29^+0.02^_0.019_kpc and for the central number density,", "{rho}0=0.29^+0.20^_-0.13_pc^\u22123^. For the halo, we derived a", "flattening parameter {kappa}=0.45+/-0.04 and a power-law index", "p=2.4+/-0.07. We found the fraction of M-type brown dwarfs in the", "local density that belong to the halo to be", "f_h_=0.0075^+0.0025^_-0.0019_. We found no correlation between subtype", "of M-dwarf and any model parameters. The total number of M-type brown", "dwarfs in the disc and halo was determined to be", "58.2^+9.81^_-6.70_x10^9^. We found an upper limit for the fraction of", "M-type brown dwarfs in the halo of 7^+5^_-4_ per cent. The upper limit", "for the total Galactic disc mass in M-dwarfs is", "4.34^+0.73^_-0.5_M_{sun}_, assuming all M-type brown dwarfs have a", "mass of 80M_J_."], "description": ["The brown dwarfs used in this research were found with the Brightest", "of Reionizing Galaxies (BoRG) survey. Observations were made with the", "WFC3 aboard the HST during a pure-parallel programme. The WFC3 was", "taking exposures whilst the HST was pointing for primary spectroscopic", "observations on e.g. quasars"], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw258"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_460_1846"}} {"id": "J/MNRAS/460/1846", "title_cds": "NGC 6273 intrinsic abundance spread", "title_create": "Yong+, 2016", "year": "2016", "author": "Yong D., Da Costa G.S., Norris J.E.", "title_pub": "Confirming the intrinsic abundance spread in the globular cluster NGC 6273 (M19) with calcium triplet spectroscopy.", "first_author": "Yong D.", "ref_biblio": [""], "bibcode": ["2016MNRAS.460.1846Y"], "see_also": ["II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "J/MNRAS/438/3507 : NGC 5824 calcium triplet equivalent widths (Da Costa+, 2014)"], "keyword_cds": "Clusters, globular ; Photometry, infrared ; Abundances ;", "keyword_pub": "stars: abundances - stars: Population II - globular clusters: general - globular clusters: individual: NGC 6273", "abstract": ["We present metallicities for red giant stars in the globular cluster", "NGC 6273 based on intermediate resolution GMOS-S spectra of the", "calcium triplet region. For the 42 radial velocity members with", "reliable calcium triplet line strength measurements, we obtain", "metallicities, [Fe/H], using calibrations established from standard", "globular clusters. We confirm the presence of an intrinsic abundance", "dispersion identified by Johnson et al. The total range in [Fe/H] is", "~1.0dex and after taking into account the measurement errors, the", "intrinsic abundance dispersion is {sigma}_int_[Fe/H]=0.17dex. Among", "the Galactic globular clusters, the abundance dispersion in NGC 6273", "is only exceeded by {omega} Cen, which is regarded as the remnant of a", "disrupted dwarf galaxy, and M54, which is the nuclear star cluster of", "the Sagittarius dwarf galaxy. If these three globular clusters share", "the same formation mechanism, then NGC 6273 may also be the remnant", "nucleus of a disrupted dwarf galaxy."], "description": ["Programme stars (see Table 1) were selected from JK colour-magnitude", "diagrams (CMD) using 2MASS photometry (Skrutskie et al., 2006, Cat.", "VII/233). All targets occupy plausible locations in the J-K versus K", "CMD. Specifically, we required 0.68<=J-K<=1.2 and 8.572<=K<=13.0.", "Furthermore, all program stars were required to have 'AAA' 2MASS", "photometric quality flags and to lie within 3 arcmin of the cluster", "centre.", "Observations of the program stars were obtained using the GMOS-S", "multi-object spectrograph at the Gemini-S telescope in queue mode", "(GS-2012A-Q-58). All observations were taken on 2012 May 05 and the", "set-up was identical to that of Da Costa et al. (2014, Cat.", "J/MNRAS/438/3507). We used the R831 grating and the RG610 filter with", "central wavelengths of 8550 and 8600{AA} (wavelength coverage was", "typically from ~7500 to ~9000{AA})."], "type": ["OC"], "doi_pub": ["10.1093/mnras/stw1091"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Program stars ", "columns": [{"name": "2MASS", "desc": "2MASS name (HHMMSSss+DDMMSSs) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Mask", "desc": "[1/6] Mask number "}, {"name": "Jmag", "desc": "2MASS J magnitude "}, {"name": "Hmag", "desc": "2MASS H magnitude "}, {"name": "Kmag", "desc": "2MASS K magnitude "}]}, {"name": "table2.dat", "desc": "Radial velocities, equivalent widths and metallicities", "columns": [{"name": "2MASS", "desc": "2MASS name (HHMMSSss+DDMMSSs) "}, {"name": "Mask", "desc": "[1/6] Mask number "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "EW8542a", "desc": "?=- Equivalent width at 8542{AA} measured from central wavelength at 8550{AA}"}, {"name": "EW8542b", "desc": "?=- Equivalent width at 8542{AA} measured from central wavelength at 8600{AA}"}, {"name": "EW8662a", "desc": "?=- Equivalent width at 8662{AA} measured from central wavelength at 8550{AA}"}, {"name": "EW8662b", "desc": "?=- Equivalent width at 8662{AA} measured from central wavelength at 8600{AA}"}, {"name": "SW", "desc": "Sum of the equivalent widths, {Sigma}W "}, {"name": "e_SW", "desc": "rms uncertainty on SW "}, {"name": "W'", "desc": "?=- Reduced equivalent width "}, {"name": "[Fe/H]", "desc": "?=- Metallicity "}, {"name": "e_[Fe/H]", "desc": "?=- rms uncertainty on [Fe/H] "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_460_2611"}} {"id": "J/MNRAS/460/2611", "title_cds": "APOGEE K and M dwarfs", "title_create": "Schmidt+, 2016", "year": "2016", "author": "Schmidt S.J., Wagoner E.L., Johnson J.A., Davenport J.R.A., Stassun K.G., Souto D., Ge J.", "title_pub": "Examining the relationships between colour, Teff, and [M/H] for APOGEE K and M dwarfs.", "first_author": "Schmidt S.J.", "ref_biblio": [""], "bibcode": ["2016MNRAS.460.2611S"], "keyword_cds": "", "keyword_pub": "surveys - stars: abundances - stars: fundamental parameters - stars: late-type - stars: low-mass", "abstract": ["We present the effective temperatures (Teff), metallicities, and", "colours in Sloan Digital Sky Survey (SDSS), Two Micron All Sky Survey,", "and Wide-field Infrared Survey Explorer filters, of a sample of 3834", "late-K and early-M dwarfs selected from the SDSS Apache Point", "Observatory Galactic Evolution Experiment (APOGEE) spectroscopic", "survey ASPCAP (APOGEE Stellar Parameters and Chemical Abundances", "Pipeline) catalogue. We confirm that ASPCAP Teff values between", "3550"], "bibcode": ["2016MNRAS.460.3232C"], "keyword_cds": "", "keyword_pub": "radiation mechanisms: general - shock waves - gamma-ray burst: general - supernovae: general - galaxies: abundances - galaxies: high-redshift", "abstract": ["We compare the physical parameters and the relative abundances", "calculated throughout supernova (SN) and {gamma}-ray burst (GRB) host", "galaxies using a detailed modelling of the spectra. The coupled effect", "of shocks and radiation from the starburst within the host galaxy is", "considered. We have found the following. (i) Shock velocities are", "lower in long-period GRBs (LGRBs) than in SN host galaxies. (ii) O/H", "relative abundances in SN hosts are scattered within a range", "8.0<12+log(O/H)<8.85 but they are close to solar in LGRB hosts. LGRB", "galaxies hosting Wolf-Rayet stars have He/H=0.13 in a few objects.", "(iii) The starburst temperatures within a few SN hosts are relatively", "high (T*>10^5^K). The values of T* in LGRB hosts are ~3-8x10^4^K. (iv)", "The H{alpha} absolute flux calculated from the emitting clouds of a", "few SN hosts at 0.1"], "bibcode": ["2016MNRAS.462.1563M"], "keyword_cds": "Stars, nearby ; Abundances", "keyword_pub": "stars: abundances - planetary systems", "abstract": ["We conducted an analysis of the distribution of elements from lithium", "to europium in 200 dwarfs in the solar neighbourhood (~20pc)", "with temperatures in the range 4800-6200K and metallicities [Fe/H]", "higher than -0.5dex. Determinations of atmospheric parameters and the", "chemical compositions of the dwarfs were taken from our previous", "studies. We found that the lithium abundances in the planet-hosting", "solar-analogue stars of our sample were lower than those in the stars", "without planetary systems. Our results reveal no significant", "differences exceeding the determination errors for the abundances of", "investigated elements, except for aluminium and barium, which are more", "and less abundant in the planet-hosting stars, respectively. We did", "not find confident dependences of the lithium, aluminium and barium", "abundances on the ages of our target stars (which is probably because", "of the small number of stars). Furthermore, we found no correlation", "between the abundance differences in [El/Fe] and the condensation", "temperature (T_cond_) for stars in the 16 Cyg binary system, unlike", "the case for 51 Peg (HD 217014), for which a slight excess of volatile", "elements and a deficit of refractories were obtained relative to those", "of solar twins. We found that one of the components of 16 Cyg exhibits", "a slightly higher average abundance than its counterpart", "(<[El/H](A-B)>=0.08+/-0.02dex); however, no significant abundance", "trend versus T_cond_ was observed. Owing to the relatively large", "errors, we cannot provide further constraints for this system."], "description": ["Our sample consists of 200 dwarfs with temperatures in the range", "4800-6200K and metallicities from -0.4dex, corresponding to the", "range of stellar parameters of 14 stars that host planets", "(Exoplanets.eu data base; Schneider et al., 2011A&A...532A..79S) from", "our data base."], "type": ["OC"], "doi_pub": ["10.1093/mnras/stw1658"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "tablea1.dat", "desc": "Comparison of atmospheric parameters for each hosting planet stars in our sample with the data of other authors", "columns": [{"name": "HD", "desc": "HD number "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "surface gravity "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "r_[Fe/H]", "desc": "Reference for [Fe/H] "}]}, {"name": "tablea2.dat", "desc": "Abundance of hosting planet stars ", "columns": [{"name": "HD", "desc": "HD number "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "Li", "desc": "?=- Lithium abundance "}, {"name": "Liup", "desc": "?=- Upper limit on Lithium abundance "}, {"name": "[O/Fe]", "desc": "?=- Abundance [O/Fe] "}, {"name": "[Na/Fe]", "desc": "?=- Abundance [Na/Fe] "}, {"name": "[Al/Fe]", "desc": "?=- Abundance [Al/Fe] "}, {"name": "[Mg/Fe]", "desc": "?=- Abundance [Mg/Fe] "}, {"name": "[S/Fe]", "desc": "?=- Abundance [S/Fe] "}, {"name": "[Si/Fe]", "desc": "Abundance [Si/Fe] "}, {"name": "[Ca/Fe]", "desc": "Abundance [Ca/Fe] "}, {"name": "[Mn/Fe]", "desc": "?=- Abundance [Mn/Fe] "}, {"name": "[Ni/Fe]", "desc": "Abundance [Ni/Fe] "}, {"name": "[Zn/Fe]", "desc": "Abundance [Zn/Fe] "}, {"name": "[Y/Fe]", "desc": "Abundance [Y/Fe] "}, {"name": "[Zr/Fe]", "desc": "?=- Abundance [Zr/Fe] "}, {"name": "[Ba/Fe]", "desc": "Abundance [Ba/Fe] "}, {"name": "[La/Fe]", "desc": "Abundance [La/Fe] "}, {"name": "[Ce/Fe]", "desc": "Abundance [Ce/Fe] "}, {"name": "[Nd/Fe]", "desc": "?=- Abundance [Nd/Fe] "}, {"name": "[Sm/Fe]", "desc": "Abundance [Sm/Fe] "}, {"name": "[Eu/Fe]", "desc": "?=- Abundance [Eu/Fe] "}]}, {"name": "tablea3.dat", "desc": "Abundance of stars without planets (Li-Eu) ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "n_Name", "desc": "[*] * for solar-analogue stars "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "[Fe/H]", "desc": "?=- Metallicity "}, {"name": "Li", "desc": "?=- Lithium abundance "}, {"name": "Liup", "desc": "?=- Upper limit Lithium abundance "}, {"name": "[O/Fe]", "desc": "?=- Abundance [O/Fe] "}, {"name": "[Na/Fe]", "desc": "?=- Abundance [Na/Fe] "}, {"name": "[Al/Fe]", "desc": "?=- Abundance [Al/Fe] "}, {"name": "[Mg/Fe]", "desc": "?=- Abundance [Mg/Fe] "}, {"name": "[S/Fe]", "desc": "?=- Abundance [S/Fe] "}, {"name": "[Si/Fe]", "desc": "?=- Abundance [Si/Fe] "}, {"name": "[Ca/Fe]", "desc": "?=- Abundance [Ca/Fe] "}, {"name": "[Mn/Fe]", "desc": "?=- Abundance [Mn/Fe] "}, {"name": "[Ni/Fe]", "desc": "?=- Abundance [Ni/Fe] "}, {"name": "[Zn/Fe]", "desc": "?=- Abundance [Zn/Fe] "}, {"name": "[Y/Fe]", "desc": "?=- Abundance [Y/Fe] "}, {"name": "[Zr/Fe]", "desc": "?=- Abundance [Zr/Fe] "}, {"name": "[Ba/Fe]", "desc": "?=- Abundance [Ba/Fe] "}, {"name": "[La/Fe]", "desc": "?=- Abundance [La/Fe] "}, {"name": "[Ce/Fe]", "desc": "?=- Abundance [Ce/Fe] "}, {"name": "[Nd/Fe]", "desc": "?=- Abundance [Nd/Fe] "}, {"name": "[Sm/Fe]", "desc": "?=- Abundance [Sm/Fe] "}, {"name": "[Eu/Fe]", "desc": "?=- Abundance [Eu/Fe] "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_463_1213"}} {"id": "J/MNRAS/463/1213", "title_cds": "s-process enhanced barium stars", "title_create": "Mahanta+, 2016", "year": "2016", "author": "Mahanta U., Karinkuzhi D., Goswami A., Duorah K.", "title_pub": "Abundance analysis of s-process enhanced barium stars.", "first_author": "Mahanta U.", "ref_biblio": [""], "bibcode": ["2016MNRAS.463.1213M"], "keyword_cds": "Stars, peculiar ; Equivalent widths", "keyword_pub": "stars: abundances - stars: chemically peculiar stars: individual: HD 49641 - stars: individual: HD 58368 - stars: individual: HD 119650 - stars: individual: HD 191010", "abstract": ["Detailed chemical composition studies of stars with enhanced", "abundances of neutron-capture elements can provide observational", "constraints for neutron-capture nucleosynthesis studies and clues for", "understanding their contribution to the Galactic chemical enrichment.", "We present abundance results from high-resolution spectral analyses of", "a sample of four chemically peculiar stars characterized by s-process", "enhancement. High-resolution spectra (R~42000) of these objects", "spanning a wavelength range from 4000 to 6800{AA} are taken from the", "ELODIE archive. We have estimated the stellar atmospheric parameters,", "the effective temperature T_eff_, the surface gravity log g and", "metallicity [Fe/H] from local thermodynamic equilibrium analysis using", "model atmospheres. We report estimates of elemental abundances for", "several neutron-capture elements, Sr, Y, Zr, Ba, La, Ce, Pr, Nd, Sm,", "Eu and Dy. While HD 49641 and HD 58368 show [Ba/Fe]>= 1.16, the other", "two objects HD 119650 and HD 191010 are found to be mild barium stars", "with [Ba/Fe]~0.4. The derived abundances of the elements are", "interpreted on the basis of existing theories for understanding their", "origin and evolution."], "description": ["Elemental abundances are presented for four peculiar stars listed in", "the barium star catalogue of Lu (1991AJ....101.2229L, Cat. V/81). All", "the objects are found to be low-velocity objects (Vr<45km/s)."], "object": ["06 49 29.45 +03 41 30.2 HD 49641 = HIP 32713", "07 25 38.97 +07 33 39.0 HD 58368 = HIP 36042", "13 44 27.12 +00 42 07.0 HD 119650 = HIP 67050", "20 06 45.84 +25 41 06.8 HD 191010 = HIP 99067"], "type": ["OC"], "doi_pub": ["10.1093/mnras/stw1995"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table4.dat", "desc": "Equivalent widths of Fe lines used for deriving atmospheric parameters", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "Ion", "desc": "Ion "}, {"name": "Elow", "desc": "Lower value of energy potential "}, {"name": "loggf", "desc": "Oscillator strength "}, {"name": "EW1", "desc": "?=- HD 49641 equivalent width "}, {"name": "e_EW1", "desc": "? rms uncertainty on EW1 "}, {"name": "f_EW1", "desc": "[h] h for hfs-syn "}, {"name": "EW2", "desc": "?=- HD 58368 equivalent width "}, {"name": "e_EW2", "desc": "? rms uncertainty on EW3 "}, {"name": "f_EW2", "desc": "[h] h for hfs-syn "}, {"name": "EW3", "desc": "?=- HD 119650 equivalent width "}, {"name": "e_EW3", "desc": "? rms uncertainty on EW3 "}, {"name": "f_EW3", "desc": "[h] h for hfs-syn "}, {"name": "EW4", "desc": "?=- HD 191010 equivalent width "}, {"name": "e_EW4", "desc": "? rms uncertainty on EW4 "}, {"name": "f_EW4", "desc": "[h] h for hfs-syn "}, {"name": "Ref", "desc": "[1/19] Reference (1) "}]}, {"name": "table8.dat", "desc": "Equivalent widths of lines used for calculation of elemental abundances", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "Ion", "desc": "Ion "}, {"name": "Elow", "desc": "Lower value of energy potential "}, {"name": "loggf", "desc": "Oscillator strength "}, {"name": "EW1", "desc": "?=- HD 49641 equivalent width "}, {"name": "e_EW1", "desc": "? rms uncertainty on EW1 "}, {"name": "f_EW1", "desc": "[h] h for hfs-syn "}, {"name": "EW2", "desc": "?=- HD 58368 equivalent width "}, {"name": "e_EW2", "desc": "? rms uncertainty on EW3 "}, {"name": "f_EW2", "desc": "[h] h for hfs-syn "}, {"name": "EW3", "desc": "?=- HD 119650 equivalent width "}, {"name": "e_EW3", "desc": "? rms uncertainty on EW3 "}, {"name": "f_EW3", "desc": "[h] h for hfs-syn "}, {"name": "EW4", "desc": "?=- HD 191010 equivalent width "}, {"name": "e_EW4", "desc": "? rms uncertainty on EW4 "}, {"name": "f_EW4", "desc": "[h] h for hfs-syn "}, {"name": "Ref", "desc": "[1/19] Reference (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_463_2494"}} {"id": "J/MNRAS/463/2494", "title_cds": "Short Title", "title_create": "Fang+, 2016", "year": "2016", "author": "Fang X.-S., Zhao G., Zhao J.-K., Chen Y.-Q., Bharat Kumar Y.", "title_pub": "Stellar activity with LAMOST. I. Spot configuration in Pleiades.", "first_author": "Fang X.-S.", "ref_biblio": [""], "bibcode": ["2016MNRAS.463.2494F"], "keyword_cds": "", "keyword_pub": "stars: activity - stars: late-type - stars: rotation - starspots", "abstract": ["We use the spectra of Pleiades and field stars from the LAMOST DR2", "archive to study how spottedness and activity vary as a function of", "mass at young ages. We obtained the standard TiO band strength by", "measuring TiO bands near 7050{AA} from LAMOST spectra (R~=1800) for a", "large sample of field GKM dwarfs with solar metallicity. Analysis", "shows that active dwarfs, including those of late G and early K types,", "have extra TiO absorption compared to their inactive counterparts,", "indicating the presence of cool spots on their surface. Active late K", "and M dwarfs show deeper TiO2 and shallower TiO4 compared to inactive", "stars at a given TiO5, which could be partly explained through cool", "spots. We estimated the cool-spot fractional coverage for 304 Pleiades", "candidates by modelling their TiO2 (and TiO5) band strength with", "respect to the standard value. The results show that the surfaces of a", "large fraction of K- and M-type members have very large spot coverage", "(~50 per cent). We analysed the correlation between spot", "coverage, rotation and the amplitude of light variation, and found", "spot coverage on slow rotators (R_o_>0.1) increases with decreasing", "Rossby number R_o_. Interestingly, we detected a saturation-like", "feature for spot coverage in fast rotators with a saturation level of", "40-50 per cent. In addition, the spot distribution in hotter fast", "rotators is more symmetrical compared to slow rotators. More", "interestingly, we detected a large spot coverage in many M-type", "members with no or little light variation. In the bigger picture,", "these results provide important constraints for the stellar dynamos of", "these cool active stars."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw1923"], "orcid_pub": ["0000-0003-3240-1688"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_463_2640"}} {"id": "J/MNRAS/463/2640", "title_cds": "SDSS-DR12 QSOs MgII absorption systems", "title_create": "Raghunathan+, 2016", "year": "2016", "author": "Raghunathan S., Clowes R.G., Campusano L.E., Sochting I.K., Graham M.J., Williger G.M.", "title_pub": "Intervening Mg II absorption systems from the SDSS DR12 quasar spectra.", "first_author": "Raghunathan S.", "ref_biblio": [""], "bibcode": ["2016MNRAS.463.2640R"], "see_also": ["J/MNRAS/452/4153 : SDSS DR12 QSOs [OIII] doublet (Albareti+, 2015)"], "keyword_cds": "Surveys ; QSOs ; Spectroscopy ; Equivalent widths", "keyword_pub": "catalogues - quasars: absorption lines - large-scale structure of Universe", "abstract": ["We present the catalogue of the MgII absorption systems detected at a", "high significance level using an automated search algorithm in the", "spectra of quasars from the 12th data release of the Sloan Digital Sky", "Survey. A total of 266,433 background quasars were searched for the", "presence of absorption systems in their spectra. The continuum", "modelling for the quasar spectra was performed using a mean filter. A", "pseudo-continuum derived using a median filter was used to trace the", "emission lines. The absorption system catalogue contains 39,694 Mg II", "systems detected at a 6.0, 3.0{sigma} level respectively for the two", "lines of the doublet. The catalogue was constrained to an absorption", "line redshift of 0.35<=z_2796_<=2.3. The rest-frame equivalent", "width of the {lambda}2796 line ranges between 0.2<=W_r_<=6.2{AA}.", "Using Gaussian noise-only simulations, we estimate a false positive", "rate of 7.7 per cent in the catalogue. We measured the number density", "dN^2796^/dz of MgII absorbers and find evidence for steeper", "evolution of the systems with W_r_>=1.2{AA} at low redshifts", "(z_2796_<=1.0), consistent with other earlier studies. A suite of", "null tests over the redshift range 0.5<=z_2796_<=1.5 was used to", "study the presence of systematics and selection effects like the", "dependence of the number density evolution of the absorption systems", "on the properties of the background quasar spectra. The null tests do", "not indicate the presence of any selection effects in the absorption", "catalogue if the quasars with spectral signal-to-noise level less than", "5.0 are removed. The resultant catalogue contains 36,981 absorption", "systems. The Mg II absorption catalogue is publicly available and can", "be downloaded from the link http://srini.ph.unimelb.edu.au/mgii.php."], "description": ["We describe the MgII absorption catalogue detected using an automated", "search algorithm from the spectra of the SDSS DR12Q. The detection", "threshold was SNR >= 6.0, 3.0 respectively for the two lines of the", "doublet. The continuum fitting is performed using a mean filter", "algorithm which was modified with a pseudo-continuum using a median", "filter to trace the emission lines. The catalogue contains 39694", "systems distributed in the EW range 0.2<=Wr<=6.2{AA} constrained to", "the redshift range 0.35<=z<=2.3."], "type": ["OC"], "doi_pub": ["10.1093/mnras/stw2095"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "MgII absorption catalogue ", "columns": [{"name": "SDSS", "desc": "SDSS DR12 name (HHMMSS.SS+DDMMSS.s) "}, {"name": "P-M-F", "desc": "SDSS DR12 plate-mjd-fibre "}, {"name": "RAdeg", "desc": "Rigth ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "zQSO", "desc": "QSO redshift "}, {"name": "imag", "desc": "QSO PSF i-band magnitude "}, {"name": "zabs", "desc": "Absorption redshift "}, {"name": "e_zabs", "desc": "rms uncertainty on zabs "}, {"name": "EW2796", "desc": "Rest-frame MgII 2796{AA} equivalent width "}, {"name": "e_EW2796", "desc": "rms uncertainty on EW2796 "}, {"name": "EW2803", "desc": "Rest-frame MgII 1803{AA} equivalent width "}, {"name": "e_EW2803", "desc": "rms uncertainty on EW1803 "}, {"name": "Flag", "desc": "[0/1] Flag showing if the detection could be a CIV line"}, {"name": "SNRcon", "desc": "Continuum signal-to-noise ratio "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_464_274"}} {"id": "J/MNRAS/464/274", "title_cds": "New variable stars", "title_create": "Sokolovsky+, 2017", "year": "2017", "author": "Sokolovsky K.V., Gavras P., Karampelas A., Antipin S.V., Bellas-velidis I., Benni P., Bonanos A.Z., Burdanov A.Y., Derlopa S., Hatzidimitriou D., Khokhryakova A.D., Kolesnikova D.M., Korotkiy S.A., Lapukhin E.G., Moretti M.I., Popov A.A., Pouliasis E., Samus N.N., Spetsieri Z., Veselkov S.A., Volkov K.V., Yang M., Zubareva A.M.", "title_pub": "Comparative performance of selected variability detection techniques in photometric time series data.", "first_author": "Sokolovsky K.V.", "ref_biblio": [""], "bibcode": ["2017MNRAS.464..274S"], "keyword_cds": "Stars, variable ; Photometry", "keyword_pub": "methods: data analysis - methods: statistical - stars: variables: general", "abstract": ["Photometric measurements are prone to systematic errors presenting a", "challenge to low-amplitude variability detection. In search for a", "general-purpose variability detection technique able to recover a", "broad range of variability types including currently unknown ones, we", "test 18 statistical characteristics quantifying scatter and/or", "correlation between brightness measurements. We compare their", "performance in identifying variable objects in seven time series data", "sets obtained with telescopes ranging in size from a telephoto lens to", "1 m-class and probing variability on time-scales from minutes to", "decades. The test data sets together include light curves of 127 539", "objects, among them 1251 variable stars of various types and represent", "a range of observing conditions often found in ground-based", "variability surveys. The real data are complemented by simulations. We", "propose a combination of two indices that together recover a broad", "range of variability types from photometric data characterized by a", "wide variety of sampling patterns, photometric accuracies and", "percentages of outlier measurements. The first index is the", "interquartile range (IQR) of magnitude measurements, sensitive to", "variability irrespective of a time-scale and resistant to outliers. It", "can be complemented by the ratio of the light-curve variance to the", "mean square successive difference, 1/{eta}, which is efficient in", "detecting variability on time-scales longer than the typical time", "interval between observations. Variable objects have larger 1/{eta}", "and/or IQR values than non-variable objects of similar brightness.", "Another approach to variability detection is to combine many", "variability indices using principal component analysis. We present 124", "previously unknown variable stars found in the test data."], "description": ["We compare 18 variability indices quantifying the overall scatter", "and/or degree of correlations between consecutive measurements in a", "light curve. The ability of these indices to distinguish variable", "stars from non-variable ones is tested on seven data sets collected", "with various ground-based telescopes and on simulated data", "incorporating actual light curves of non-variable objects as realistic", "models of photometric noise. We apply the PCA in search for an optimal", "combination of multiple variability indices.", "We were able to identify 124 new variable stars during the test.", "The information about the new variables is summarized in Table 4."], "type": ["CCC"], "doi_pub": ["10.1093/mnras/stw2262"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table4.dat", "desc": "New variable stars found in the test data ", "columns": [{"name": "Name", "desc": "Name "}, {"name": "OName", "desc": "Other name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "mag1", "desc": "Lower value of magnitude interval "}, {"name": "---", "desc": "[-] "}, {"name": "mag2", "desc": "Upper value of magnitude interval "}, {"name": "u_mag2", "desc": "Uncertainty flag on magnitude interval "}, {"name": "Band", "desc": "[VI] Band for magnitude interval "}, {"name": "Type", "desc": "Variable type "}, {"name": "Per", "desc": "? Period "}, {"name": "u_Per", "desc": "Uncertainty flag on Per "}, {"name": "n_Per", "desc": "Note on Per "}, {"name": "n_Epoch", "desc": "[min max] Minimum of maximum for Epoch "}, {"name": "Epoch", "desc": "? Epoch "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_464_3920"}} {"id": "J/MNRAS/464/3920", "title_cds": "GALEX/WISE early-type galaxies sample", "title_create": "Simonian+, 2017", "year": "2017", "author": "Simonian G.V., Martini P.", "title_pub": "Circumstellar dust, PAHs and stellar populations in early-type galaxies: insights from GALEX and WISE.", "first_author": "Simonian G.V.", "ref_biblio": [""], "bibcode": ["2017MNRAS.464.3920S"], "see_also": ["J/MNRAS/413/813 : ATLAS3D project. I. (Cappellari+, 2011)"], "keyword_cds": "Galaxy catalogs ; Photometry, ultraviolet ; Photometry, infrared ; Morphology", "keyword_pub": "galaxies: elliptical and lenticular, cD - galaxies: stellar content - infrared: galaxies - ultraviolet: galaxies", "abstract": ["A majority of early-type galaxies contain interstellar dust, yet the", "origin of this dust, and why the dust sometimes exhibits unusual", "polycyclic aromatic hydrocarbon (PAH) ratios, remains a mystery. If", "the dust is internally produced, it likely originates from the large", "number of asymptotic giant branch stars associated with the old", "stellar population. We present GALEX and WISE elliptical aperture", "photometry of ~310 early-type galaxies with Spitzer mid-infrared", "spectroscopy and/or ancillary data from ATLAS3D, to characterize their", "circumstellar dust and the shape of the radiation field that", "illuminates the interstellar PAHs. We find that circumstellar dust is", "ubiquitous in early-type galaxies, which indicates some tension", "between stellar population age estimates and models for circumstellar", "dust production in very old stellar populations. We also use dynamical", "masses from ATLAS3D to show that WISE W1 (3.4um) mass-to-light", "ratios are consistent with the initial mass function variation found", "by previous work. While the stellar population differences in", "early-type galaxies correspond to a range of radiation field shapes", "incident upon the diffuse dust, the ratio of the ionization-sensitive", "7.7um/11.3um PAH feature does not correlate with the shape of", "the radiation field, nor to variations with the size-sensitive", "11.3um/17um ratio. The 7.7um/11.3um PAH ratio does tend to be smaller", "in galaxies with proportionally greater H2 emission, which is evidence", "that processing of primarily smaller grains by shocks is responsible", "for the unusual ratios, rather than substantial differences in the", "overall PAH size or ionization distribution."], "description": ["We use MIR and UV photometry to study circumstellar and interstellar", "dust in early-type galaxies (ETGs). Our sample is drawn from two", "recent, comprehensive studies of ETGs: the characterizations of", "interstellar dust in ETGs with Spitzer-IRS spectra (Rampazzo et al.,", "2013MNRAS.432..374R), and the stellar population and dynamical study", "from the ATLAS3D survey (Cappellari et al., 2011, Cat.", "J/MNRAS/413/813."], "type": ["CCC"], "doi_pub": ["10.1093/mnras/stw2623"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Aperture photometry parameters for galaxies in the ATLAS3D (J/MNRAS/413/813) and Rampazzo et al. (2013MNRAS.432..374R) samples", "columns": [{"name": "Name", "desc": "Galaxy name "}, {"name": "MType", "desc": "Morphological type "}, {"name": "Dist", "desc": "Distance "}, {"name": "Sample", "desc": "Originating Sample "}, {"name": "aW1", "desc": "WISE W1 aperture semimajor axis "}, {"name": "aW4", "desc": "WISE W4 aperture semimajor axis "}, {"name": "b/aW1", "desc": "WISE W1 axis ratio "}, {"name": "b/aW4", "desc": "WISE W4 axis ratio "}, {"name": "PA", "desc": "[] Position Angle "}, {"name": "WISEDR", "desc": "WISE data release catalog "}, {"name": "GALEXNUV", "desc": "GALEX NUV tilename "}, {"name": "GALEXFUV", "desc": "GALEX NUV tilename "}]}, {"name": "table2.dat", "desc": "Galaxy magnitudes for the ATLAS3D (J/MNRAS/413/813) and Rampazzo et al. (2013MNRAS.432..374R) samples", "columns": [{"name": "Name", "desc": "Galaxy Name "}, {"name": "l_FUV", "desc": "Limit flag on FUV "}, {"name": "FUV", "desc": "?=- FUV magnitude (1) "}, {"name": "e_FUV", "desc": "?=- rms uncertainty on FUV magnitude "}, {"name": "NUV", "desc": "?=- NUV magnitude (1) "}, {"name": "e_NUV", "desc": "?=- rms uncertainty on NUV magnitude "}, {"name": "W1mag", "desc": "?=- W1 magnitude (1) "}, {"name": "e_W1mag", "desc": "?=- rms uncertainty on W1 magnitude "}, {"name": "W2mag", "desc": "?=- W2 magnitude (1) "}, {"name": "e_W2mag", "desc": "?=- rms uncertainty on W2 magnitude "}, {"name": "W3mag", "desc": "?=- W3 magnitude (1) "}, {"name": "e_W3mag", "desc": "?=- rms uncertainty on W3 magnitude "}, {"name": "l_W4mag", "desc": "Limit flag on W4mag "}, {"name": "W4mag", "desc": "?=- W4 magnitude (1) "}, {"name": "e_W4mag", "desc": "?=- rms uncertainty on W4 magnitude "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_464_4176"}} {"id": "J/MNRAS/464/4176", "title_cds": "Short Title", "title_create": "Willett+, 2017", "year": "2017", "author": "Willett K.W., Galloway M.A., Bamford S.P., Lintott C.J., Masters K.L., Scarlata C., Simmons B.D., Beck M., Cardamone C.N., Cheung E., Edmondson E.M., Fortson L.F., Griffith R.L., Haussler B., Han A., Hart R., Melvin T., Parrish M., Schawinski K., Smethurst R.J., Smith A.M.", "title_pub": "Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging.", "first_author": "Willett K.W.", "ref_biblio": [""], "bibcode": ["2017MNRAS.464.4176W"], "keyword_cds": "", "keyword_pub": "methods: data analysis - catalogues - galaxies: evolution - galaxies: high-redshift - galaxies: structure", "abstract": ["We present the data release paper for the Galaxy Zoo: Hubble (GZH)", "project. This is the third phase in a large effort to measure", "reliable, detailed morphologies of galaxies by using crowdsourced", "visual classifications of colour-composite images. Images in GZH were", "selected from various publicly released Hubble Space Telescope legacy", "programmes conducted with the Advanced Camera for Surveys, with", "filters that probe the rest-frame optical emission from galaxies out", "to z~1. The bulk of the sample is selected to have m_I814W_<23.5,", "but goes as faint as m_I814W_<26.8 for deep images combined over five", "epochs. The median redshift of the combined samples is =0.9+/-0.6,", "with a tail extending out to z~=4. The GZH morphological data include", "measurements of both bulge- and disc-dominated galaxies, details on", "spiral disc structure that relate to the Hubble type, bar", "identification, and numerous measurements of clump identification and", "geometry. This paper also describes a new method for calibrating", "morphologies for galaxies of different luminosities and at different", "redshifts by using artificially redshifted galaxy images as a", "baseline. The GZH catalogue contains both raw and calibrated", "morphological vote fractions for 119\u2009849 galaxies, providing the", "largest data set to date suitable for large-scale studies of galaxy", "evolution out to z~1."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw2568"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_465_1181"}} {"id": "J/MNRAS/465/1181", "title_cds": "Short Title", "title_create": "Liakos+, 2017", "year": "2017", "author": "Liakos A., Niarchos P.", "title_pub": "Catalogue and properties of {delta} Scuti stars in binaries.", "first_author": "Liakos A.", "ref_biblio": [""], "bibcode": ["2017MNRAS.465.1181L"], "keyword_cds": "", "keyword_pub": "binaries: close - binaries: eclipsing - stars: fundamental parameters - stars: variables: delta Scuti", "abstract": ["The catalogue contains 199 confirmed cases of binary systems", "containing at least one pulsating component of delta Sct type. The", "sample is divided into subgroups in order to describe the properties", "and characteristics of the delta Sct-type stars in binaries according", "to their Roche geometry. Demographics describing quantitatively our", "knowledge for these systems as well as the distributions of their", "pulsating components in the mass\u2013radius, colour\u2013magnitude, and", "evolutionary status\u2013temperature diagrams are presented and", "discussed. It is shown that a threshold of ~13d of the orbital", "period regarding the influence of binarity on the pulsations is", "established. Finally, the correlations between the pulsation periods", "and the orbital periods, evolutionary status, and companion's gravity", "influence are updated based on the largest sample to date."], "description": ["The catalogue consists of five lists given in Tables 1-5 of this", "paper. It contains all of the currently known binaries with a delta", "Sct component, ambiguous ones, and others that were incorrectly", "reported as being of this type. This catalogue is online", "(https://alexiosliakos.weebly.com/catalogue.html) and is frequently", "updated."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw2756"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_467_412"}} {"id": "J/MNRAS/467/412", "title_cds": "Simulated globular clusters with Gaia", "title_create": "Pancino+, 2017", "year": "2017", "author": "Pancino E., Bellazzini M., Giuffrida G., Marinoni S.", "title_pub": "Globular clusters with Gaia.", "first_author": "Pancino E.", "ref_biblio": [""], "bibcode": ["2017MNRAS.467..412P"], "see_also": ["I/337 : Gaia DR1 (Gaia Collaboration, 2016)"], "keyword_cds": "Models ; Globular clusters", "keyword_pub": "astrometry - parallaxes - globular clusters: general", "abstract": ["The treatment of crowded fields in Gaia data will only be a reality in", "a few years from now. In particular, for globular clusters, only the", "end-of-mission data (public in 2022-2023) will have the necessary full", "crowding treatment and will reach sufficient quality for the faintest", "stars. As a consequence, the work on the deblending and", "decontamination pipelines is still ongoing. We describe the present", "status of the pipelines for different Gaia instruments, and we model", "the end-of-mission crowding errors on the basis of available", "information. We then apply the nominal post-launch Gaia performances,", "appropriately worsened by the estimated crowding errors, to a set of", "18 simulated globular clusters with different concentration, distance", "and field contamination. We conclude that there will be 10^3^-10^4^", "stars with astrometric performances virtually untouched by crowding", "(contaminated by <1mmag) in the majority of clusters. The most", "limiting factor will be field crowding, not cluster crowding: the most", "contaminated clusters will only contain 10-100 clean stars. We also", "conclude that (i) the systemic proper motions and parallaxes will be", "determined to 1 per cent or better up to ~=15kpc, and the", "nearby clusters will have radial velocities to a few km/s; (ii)", "internal kinematics will be of unprecedented quality, cluster masses", "will be determined to ~=10 per cent up to 15kpc and beyond, and", "it will be possible to identify differences of a few km/s or less", "in the kinematics (if any) of cluster sub-populations up to 10kpc and", "beyond; (iii) the brightest stars (V~=17mag) will have", "space-quality, wide-field photometry (mmag errors), and all Gaia", "photometry will have 1-3 per cent errors on the absolute photometric", "calibration."], "description": ["We used all the available information on the presently available Gaia", "deblending pipelines, along with their results on simulated data, to", "model the behaviour of Gaia in crowded areas. We computed additional", "crowding errors that were combined with the post-launch science", "performances of Gaia and applied to a set of simulated GCs with", "different concentration (c=1.0 and 2.5), distance (5, 10 and 15kpc),", "and field population (halo, disc and bulge)."], "doi_pub": ["10.1093/mnras/stx079"], "orcid_pub": ["0000-0003-0788-5879"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "Simulated cluster properties and crowding evaluation results", "columns": [{"name": "Cluster", "desc": "[1/18] Cluster number "}, {"name": "c", "desc": "GC concentration parameter, c=log(rt/rc) "}, {"name": "Dist", "desc": "GC projected distance "}, {"name": "Bckg", "desc": "Type of simulated background "}, {"name": "ntot", "desc": "Total number of simulated stars (GC and background) above Gaia detection limit"}, {"name": "nGC", "desc": "Number of GC members "}, {"name": "nclassic", "desc": "Number of classic blends "}, {"name": "nblends", "desc": "Number of Gaia blends "}, {"name": "ncontam", "desc": "Number of contaminated stars "}, {"name": "nclean", "desc": "Number of clean stars (1) "}, {"name": "Des", "desc": "Quick GC designation used in the paper "}, {"name": "Examp", "desc": "Some examples of GCs with similar distance, concentration and background field"}]}, {"name": "catalog.dat", "desc": "Final simulated stars (partial !!!!!) ", "columns": [{"name": "Cluster", "desc": "[1/16] Cluster number "}, {"name": "Star", "desc": "Star ID "}, {"name": "RAdeg", "desc": "Position along the RA direction (1) "}, {"name": "DEdeg", "desc": "Position along the Dec direction (1) "}, {"name": "e_pos", "desc": "Error on RA and DE "}, {"name": "pmRA", "desc": "Proper motion along RA "}, {"name": "pmDE", "desc": "Proper motion along DE "}, {"name": "e_pm", "desc": "Error on proper motion "}, {"name": "plx", "desc": "Parallax "}, {"name": "e_plx", "desc": "Parallax error "}, {"name": "Gmag", "desc": "G-band integrated magnitude "}, {"name": "e_Gmag", "desc": "G magnitude error "}, {"name": "GBPmag", "desc": "GBP integrated magnitude "}, {"name": "e_GBPmag", "desc": "GBP magnitude error "}, {"name": "GRPmag", "desc": "GRP integrated magnitude "}, {"name": "e_GRPmag", "desc": "GRP magnitude error "}, {"name": "Memb", "desc": "[0/1] True membership (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_467_3361"}} {"id": "J/MNRAS/467/3361", "title_cds": "", "title_create": "Wiegand+, 2017", "year": "2017", "author": "Wiegand A., Eisenstein D.J.", "title_pub": "The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: higher order correlations revealed by germ-grain Minkowski functionals.", "first_author": "Wiegand A.", "ref_biblio": [""], "bibcode": ["2017MNRAS.467.3361W"], "keyword_cds": "", "keyword_pub": "methods: data analysis - methods: statistical - cosmology: observations - large-scale structure of Universe", "abstract": ["We probe the higher order clustering of the galaxies in the final data", "release (DR12) of the Sloan Digital Sky Survey Baryon Oscillation", "Spectroscopic Survey (BOSS), using the method of germ-grain Minkowski", "functionals (MFs). Our sample consists of 410615 BOSS galaxies from", "the northern Galactic cap in the redshift range 0.450-0.595. We show", "the MFs to be sensitive to contributions up to the six-point", "correlation function for this data set. We ensure with a custom", "angular mask that the results are more independent of boundary effects", "than in previous analyses of this type. We extract the higher order", "part of the MFs and quantify the difference to the case without higher", "order correlations. The resulting {chi}^2^ value of over 10000 for a", "modest number of degrees of freedom, O(200), indicates a 100{sigma}", "deviation and demonstrates that we have a highly significant signal of", "the non-Gaussian contributions to the galaxy distribution. This", "statistical power can be useful in testing models with differing", "higher order correlations. Comparing the galaxy data to the quick", "particle mesh and MultiDark(MD)-Patchy mocks, we find that the latter", "better describes the observed structure. From an order-by-order", "decomposition, we expect that, for example, already a reduction of the", "amplitude of the MD-Patchy mock power spectrum by 5 per cent would", "remove the remaining tension."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stx292"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_469_1065"}} {"id": "J/MNRAS/469/1065", "title_cds": "SPIDERS catalogs", "title_create": "Dwelly+, 2017", "year": "2017", "author": "Dwelly T., Salvato M., Merloni A., Brusa M., Buchner J., Anderson S.F., Boller T., Brandt W.N., Budavari T., Clerc N., Coffey D., Del Moro A., Georgakakis A., Green P.J., Jin C., Menzel M.-L., Myers A.D., Nandra K., Nichol R.C., Ridl J., Schwope A.D., Simm T.", "title_pub": "SPIDERS: selection of spectroscopic targets using AGN candidates detected in all-sky X-ray surveys.", "first_author": "Dwelly T.", "ref_biblio": [""], "bibcode": ["2017MNRAS.469.1065D"], "keyword_cds": "", "keyword_pub": "surveys - galaxies: active - quasars: general - galaxies: Seyfert - cosmology: observations - X-rays: galaxies", "abstract": ["SPIDERS (SPectroscopic IDentification of eROSITA Sources) is a Sloan", "Digital Sky Survey IV (SDSS-IV) survey running in parallel to the", "Extended Baryon Oscillation Spectroscopic Survey (eBOSS) cosmology", "project. SPIDERS will obtain optical spectroscopy for large numbers of", "X-ray-selected active galactic nuclei (AGN) and galaxy cluster members", "detected in wide-area eROSITA, XMM-Newton and ROSAT surveys. We", "describe the methods used to choose spectroscopic targets for two", "sub-programmes of SPIDERS X-ray selected AGN candidates detected in", "the ROSAT All Sky and the XMM-Newton Slew surveys. We have exploited a", "Bayesian cross-matching algorithm, guided by priors based on mid-IR", "colour-magnitude information from the Wide-field Infrared Survey", "Explorer survey, to select the most probable optical counterpart to", "each X-ray detection. We empirically demonstrate the high fidelity of", "our counterpart selection method using a reference sample of bright", "well-localized X-ray sources collated from XMM-Newton, Chandra and", "Swift-XRT serendipitous catalogues, and also by examining blank-sky", "locations. We describe the down-selection steps which resulted in the", "final set of SPIDERS-AGN targets put forward for spectroscopy within", "the eBOSS/TDSS/SPIDERS survey, and present catalogues of these", "targets. We also present catalogues of ~12000 ROSAT and ~1500", "XMM-Newton Slew survey sources that have existing optical spectroscopy", "from SDSS-DR12, including the results of our visual inspections. On", "completion of the SPIDERS programme, we expect to have collected", "homogeneous spectroscopic redshift information over a footprint of", "~7500 deg^2^ for >85 per cent of the ROSAT and XMM-Newton Slew survey", "sources having optical counterparts in the magnitude range 17"], "bibcode": ["2017MNRAS.469..800M"], "keyword_cds": "", "keyword_pub": "Hertzsprung-Russell and colour-magnitude diagrams stars: low-mass: Population II; globular clusters: general globular clusters: individual: \\object{\u03c9 Centauri, M4, NGC2808}{}", "mission": "", "abstract": ["As part of a large investigation with Hubble Space Telescope to study the faintest stars within the globular cluster {omega} Centauri, in this work we present early results on the multiplicity of its main sequence (MS) stars, based on deep optical and near-infrared observations. By using appropriate colour-magnitude diagrams, we have identified, for the first time, the two main stellar Populations I and II along the entire MS, from the turn-off towards the hydrogen-burning limit. We have compared the observations with suitable synthetic spectra of MS stars and conclude that the two main sequences (MSs) are consistent with stellar populations with different metallicity, helium and light-element abundance. Specifically, MS-I corresponds to a metal-poor stellar population ([Fe/H]~ -1.7) with Y~ 0.25 and [O/Fe]~ 0.30. The MS-II hosts helium-rich (Y~ 0.37-0.40) stars with metallicity ranging from [Fe/H]~ -1.7 to -1.4. Below the MS knee (m_F160W_ ~ 19.5), our photometry reveals that each of the two main MSs hosts stellar subpopulations with different oxygen abundances, with very O-poor stars ([O/Fe] ~ -0.5) populating the MS-II. Such a complexity has never been observed in previous studies of M-dwarfs in globular clusters. A few months before the launch of the James Webb Space Telescope, these results demonstrate the power of optical and near-infrared photometry in the study of multiple stellar populations in globular clusters."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "30-Mar-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_471_404"}} {"id": "J/MNRAS/471/404", "title_cds": "Short Title", "title_create": "Kielty+, 2017", "year": "2017", "author": "Kielty C.L., Venn K.A., Loewen N.B., Shetrone M.D., Placco V.M., Jahandar F., Meszaros S., Martell S.L.", "title_pub": "Carbon-enhanced metal-poor stars in the SDSS-APOGEE data base.", "first_author": "Kielty C.L.", "ref_biblio": [""], "bibcode": ["2017MNRAS.471..404K"], "keyword_cds": "", "keyword_pub": "surveys; stars: abundances; stars: carbon; stars: chemically peculiar Galaxy: halo; infrared: stars", "mission": "", "abstract": ["We identify six new carbon-enhanced metal-poor (CEMP) stars ([C/Fe]>+0.7 and [Fe/H] < -1.8) and another seven likely candidates within the APOGEE data base following Data Release 12. These stars have chemical compositions typical of metal-poor halo stars, e.g. mean [{alpha}/Fe] = +0.24 {\\pm} 0.24, based on the APOGEE Stellar Parameters and Chemical Abundances Pipeline results. A lack of heavy-element spectral lines impedes further sub-classification of these CEMP stars, however, based on radial velocity (RV) scatter, we predict most are not CEMP-s stars which are typically found in binary systems. Only one object, 2M15312547+4220551, may be in a binary since it exhibits a scatter in its RV of 1.7 {\\pm} 0.6 km s^-1^ based on three visits over a 25.98 d baseline. Optical observations are now necessary to confirm the stellar parameters and low metallicities of these stars, to determine the heavy-element abundance ratios and improve the precision in the derived abundances, and to examine their CEMP sub-classifications."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "15-May-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_471_3494"}} {"id": "J/MNRAS/471/3494", "title_cds": "Short Title", "title_create": "Zhu+, 2017", "year": "2017", "author": "Zhu H., Tian W., Li A., Zhang M.", "title_pub": "The gas-to-extinction ratio and the gas distribution in the Galaxy.", "first_author": "Zhu H.", "ref_biblio": [""], "bibcode": ["2017MNRAS.471.3494Z"], "keyword_cds": "", "keyword_pub": "galaxies: active - galaxies: individual: NGC 6240 - galaxies: starburst; X-rays: galaxies", "abstract": ["We investigate the relation between the optical extinction (A_V_) and", "the hydrogen column density (N_H_) determined from X-ray observations", "of a large sample of Galactic sightlines towards 35 supernova", "remnants, 6 planetary nebulae and 70 X-ray binaries for which N_H_ was", "determined in the literature with solar abundances. We derive an", "average ratio of =(2.08+/-0.02)x10^21^Hcm^-2^mag^-1^ for", "the whole Galaxy. We find no correlation between and the", "number density of hydrogen, the distance away from the Galactic Centre", "and the distance above or below the Galactic plane. The ", "ratio is generally invariant across the Galaxy, with", "=(2.04+/-0.05)x10^21^Hcm^-2^mag^-1^ for the first and", "fourth Galactic quadrants and", "=(2.09+/-0.03)x10^21^Hcm^-2^mag^-1^ for the second and", "third Galactic quadrants. We also explore the distribution of hydrogen", "in the Galaxy by enlarging our sample with additional 74 supernova", "remnants for which both N_H_ and distances are known. We find that,", "between the Galactic radius of 2 and 10 kpc, the vertical distribution", "of hydrogen can be roughly described by a Gaussian function with a", "scaleheight of h=75.5+/-12.4pc and a mid-plane density of", "n_H_(0)=1.11+/-0.15cm^-3^, corresponding to a total gas surface", "density of {sum}_gas_~7.0 M_{sun}_/pc^2^. We also compile N_H_ from 19", "supernova remnants and 29 X-ray binaries for which N_H_ was determined", "with subsolar abundances. We obtain", "=(2.47+/-0.04)x10^21^Hcm^-2^mag^-1^ which exceeds that", "derived with solar abundances by ~20 per cent. We suggest that in", "future studies one may simply scale N_H_ derived from subsolar", "abundances"], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "28-May-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_471_4087"}} {"id": "J/MNRAS/471/4087", "title_cds": "Gaia 1 HERMES and AAOmega spectroscopy", "title_create": "Simpson+, 2017", "year": "2017", "author": "Simpson J.D., De Silva G.M., Martell S.L., Zucker D.B., Ferguson A.M.N., Bernard E.J., Irwin M., Penarrubia J., Tolstoy E.", "title_pub": "Siriusly, a newly identified intermediate-age Milky Way stellar cluster: a spectroscopic study of Gaia 1.", "first_author": "Simpson J.D.", "ref_biblio": [""], "bibcode": ["2017MNRAS.471.4087S"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)"], "keyword_cds": "Milky Way ; Associations, stellar ; Radial velocities", "keyword_pub": "catalogues - Galaxy: general - Galaxy: structure", "abstract": ["We confirm the reality of the recently discovered Milky Way stellar", "cluster Gaia 1 using spectra acquired with the HERMES and AAOmega", "spectrographs of the Anglo-Australian Telescope. This cluster had been", "previously undiscovered due to its close angular proximity to Sirius,", "the brightest star in the sky at visual wavelengths. Our observations", "identified 41 cluster members, and yielded an overall metallicity of", "[Fe/H]=-0.13+/-0.13 and barycentric radial velocity of", "v_r_=58.30+/-0.22km/s. These kinematics provide a dynamical mass", "estimate of 12.9^+4.6^_-3.9_x10^3^M_{sun}_. Isochrone fits to Gaia,", "2MASS, and Pan-STARRS1 photometry indicate that Gaia 1 is an", "intermediate age (~3Gyr) stellar cluster. Combining the spatial", "and kinematic data we calculate Gaia 1 has a circular orbit with a", "radius of about 12kpc, but with a large out of plane motion:", "z_max_=1.1^+0.4^_-0.3_kpc."], "description": ["Gaia 1 was observed with two of the spectrographs of the 3.9-m", "Anglo-Australian Telescope over three nights: on the night of 2017", "February 15 with the four-armed high-resolution HERMES spectrograph,", "and on the nights of 2017 February 24 and 26 with the two-armed", "AAOmega spectrograph."], "object": ["06 45 53 -16 45 00 Gaia 1 = [KBT2017] Gaia 1"], "type": ["OC"], "data": "", "date_update": "10-Feb-2021", "tables": [{"name": "tablea1.dat", "desc": "The line list used for the HERMES stellar parameter determination", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "El", "desc": "Element "}, {"name": "EP", "desc": "Energy potential "}, {"name": "loggf", "desc": "Osccilator strength "}]}, {"name": "tableb1.dat", "desc": "Parameters for members of Gaia 1 observed with HERMES", "columns": [{"name": "GaiaDR1", "desc": "Gaia DR1 source_id "}, {"name": "PS1", "desc": "PS1 objID "}, {"name": "r", "desc": "Radius "}, {"name": "SNR1", "desc": "Signa-to-noise 1 (blue: 4715-4900{AA}) "}, {"name": "SNR2", "desc": "Signa-to-noise 2 (green: 5649-5873{AA}) "}, {"name": "SNR3", "desc": "Signa-to-noise 3 (red: 6478-6737{AA}) "}, {"name": "SNR4", "desc": "Signa-to-noise 4 (near-infrared: 7585-7887{AA}) "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "e_RV", "desc": "Radial velocity error "}, {"name": "Teff", "desc": "? Effective temperature "}, {"name": "loggsp", "desc": "? Spectroscopic gravity surface "}, {"name": "loggph", "desc": "? Photometric gravity surface "}, {"name": "[Fe/H]", "desc": "? Metallicity "}, {"name": "e_[Fe/H]", "desc": "? Metallicity error "}]}, {"name": "tableb2.dat", "desc": "Parameters for members of Gaia 1 observed with AAOmega", "columns": [{"name": "GaiaDR1", "desc": "Gaia DR1 source_id "}, {"name": "PS1", "desc": "PS1 objID "}, {"name": "r", "desc": "Radius "}, {"name": "SNR", "desc": "Signal-to-noise ratio "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "e_RV", "desc": "Radial velocity error "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "e_[Fe/H]", "desc": "Metallicity error "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_472_4051"}} {"id": "J/MNRAS/472/4051", "title_cds": "Short Title", "title_create": "Calderone+, 2017", "year": "2017", "author": "Calderone G., Nicastro L., Ghisellini G., Dotti M., Sbarrato T., Shankar F., Colpi M.", "title_pub": "QSFIT: automatic analysis of optical AGN spectra.", "first_author": "Calderone G.", "ref_biblio": [""], "bibcode": ["2017MNRAS.472.4051C"], "keyword_cds": "", "keyword_pub": "methods: data analysis - catalogues; galaxies: active quasars: emission lines", "mission": "", "abstract": ["We present QSFIT (Quasar Spectral Fitting package), a new software package to automatically perform the analysis of active galactic nuclei (AGNs) optical spectra. The software provides luminosity estimates for the AGN continuum, the Balmer continuum, both optical and ultraviolet iron blended complex, host galaxy and emission lines, as well as width, velocity offset and equivalent width of 20 emission lines. Improving on a number of previous studies on AGN spectral analysis, QSFIT fits all the components simultaneously, using an AGN continuum model which extends over the entire available spectrum, and is thus a probe of the actual AGN continuum whose estimates are scarcely influenced by localized features (e.g. emission lines) in the spectrum. We used QSFIT to analyse 71 251 optical spectra of Type 1 AGN at z < 2 (obtained by the Sloan Digital Sky Survey, SDSS) and to produce a publicly available catalogue of AGN spectral properties. Such catalogueallowed us (for the first time) to estimate the AGN continuum slope and the Balmer continuum luminosity on a very large sample, and to show that there is no evident correlation between these quantities the redshift. All data in the catalogue, the plots with best-fitting model and residuals, and the IDL code we used to perform the analysis, are available on a dedicated website. The whole fitting process is customizable for specific needs, and can be extended to analysespectra from other data sources. The ultimate purpose of QSFIT is to allow astronomers to run standardized recipes to analyse the AGN data, in a simple, replicable and shareable way."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "26-Jun-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_473_2020"}} {"id": "J/MNRAS/473/2020", "title_cds": "Short Title", "title_create": "Lodieu+, 2018", "year": "2018", "author": "Lodieu N., Zapatero Osorio M.R., Bejar V.J.S., Pena Ramirez K.", "title_pub": "The optical + infrared l dwarf spectral sequence of young planetary-mass objects in the upper scorpius association.", "first_author": "Lodieu N.", "ref_biblio": [""], "bibcode": ["2018MNRAS.473.2020L"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "21-Nov-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_473_2853"}} {"id": "J/MNRAS/473/2853", "title_cds": "Short Title", "title_create": "Rosslowe+, 2018", "year": "2018", "author": "Rosslowe C.K., Crowther P.A.", "title_pub": "A deep near-infrared spectroscopic survey of the Scutum-Crux arm for Wolf-Rayet stars.", "first_author": "Rosslowe C.K.", "ref_biblio": [""], "bibcode": ["2018MNRAS.473.2853R"], "keyword_cds": "", "keyword_pub": "stars: emission-line, Be - stars: evolution - stars: Wolf\u2013Rayet \u2013 Galaxy: stellar content - infrared: stars", "abstract": ["We present a New Technology Telescope/Son-of-Isaac spectroscopic", "survey of infrared selected Wolf\u2013Rayet (WR) candidates in the", "Scutum-Crux spiral arm (298{deg}<=l<=340{deg}, |b|<=0.5{deg}). We", "obtained near-IR spectra of 127 candidates, revealing 17 WR stars \u2013", "a ~13 per cent success rate \u2013 of which 16 are newly identified here.", "The majority of the new WR stars are classified as narrow-lined", "WN5\u20137 stars, with two broad-lined WN4\u20136 stars and three WC6\u20138", "stars. The new stars, with distances estimated from previous absolute", "magnitude calibrations, have no obvious association with the", "Scutum-Crux arm. Refined near-infrared (YHJK) classification criteria", "based on over a hundred Galactic and Magellanic Cloud WR stars,", "providing diagnostics for hydrogen in WN stars, plus the", "identification of WO stars and intermediate WN/C stars. Finally, we", "find that only a quarter of WR stars in the survey region are", "associated with star clusters and/or HII regions, with similar", "statistics found for luminous blue variables (LBVs) in the Milky Way.", "The relative isolation of evolved massive stars is discussed, together", "with the significance of the co-location of LBVs and WR stars in young", "star clusters."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "21-Nov-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_473_5393"}} {"id": "J/MNRAS/473/5393", "title_cds": "Wide binaries in Tycho-Gaia", "title_create": "Andrews+, 2018", "year": "2018", "author": "Andrews J.J., Chaname J., Agueros M.A.", "title_pub": "Wide binaries in Tycho-Gaia. II: metallicities, abundances and prospects for chemical tagging.", "first_author": "Andrews J.J.", "ref_biblio": [""], "bibcode": ["2018MNRAS.473.5393A"], "see_also": ["I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "III/279 : RAVE 5th data release (Kunder+, 2017)", "V/153 : LAMOST DR4 catalogs (Luo+, 2018)"], "keyword_cds": "Milky Way ; Stars, double and multiple ; Abundances ; Effective temperatures", "keyword_pub": "stars: abundances - binaries: visual - Galaxy: structure", "abstract": ["From our recent catalogue based on the first Gaia data release (TGAS),", "we select wide binaries in which both stars have been observed by the", "Radial Velocity Experiment (RAVE) or the Large Sky Area Multi-Object", "Fiber Spectroscopic Telescope (LAMOST). Using RAVE and LAMOST", "metallicities and RAVE Mg, Al, Si, Ti and Fe abundances, we find that", "the differences in the metallicities and elemental abundances of", "components of wide binaries are consistent with being due to", "observational uncertainties, in agreement with previous results for", "smaller and more restricted samples. The metallicity and elemental", "abundance consistency between wide binary components presented in this", "work confirms their common origin and bolsters the status of wide", "binaries as 'mini-open clusters'. Furthermore, this is evident that", "wide binaries are effectively co-eval and co-chemical, supporting", "their use for, e.g. constraining age-activity-rotation relations,", "the initial-final mass relation for white dwarfs and M-dwarf", "metallicity indicators. Additionally, we demonstrate that the common", "proper motion, common parallax pairs in TGAS with the most extreme", "separations (s>~0.1pc) typically have inconsistent metallicities,", "radial velocities or both and are therefore likely to be predominantly", "comprised of random alignments of unassociated stars with similar", "astrometry, in agreement with our previous results. Finally, we", "propose that wide binaries form an ideal data set with which we can", "test chemical tagging as a method to identify stars of common origin,", "particularly because the stars in wide binaries span a wide range of", "metallicities, much wider than that spanned by nearby open clusters."], "description": ["From our catalogue of 7108 wide binaries identified in TGAS in Paper I", "(Andrews et al., 2017MNRAS.472..675A, Cat. J/MNRAS/472/675, we select", "the subset of pairs in which the posterior probability is above", "99 per cent when using a power-law prior on the distribution of", "orbital separations (for details, see Paper I).", "We first cross-match these pairs with the RAVE DR5 catalogue (Kunder", "et al., 2017AJ....153...75K, Cat. III/279) and obtain 115 wide", "binaries in which both components are detected by RAVE (table1).", "We also cross-match with the LAMOST DR3 catalogue to identify", "additional 85 wide binaries with measured RVs, although only 62 of", "these have measured metallicities with uncertainties less than 0.2dex", "(table 2)."], "type": ["OC"], "doi_pub": ["10.1093/mnras/stx2685"], "orcid_pub": ["0000-0001-5261-3923"], "data": "", "date_creation": "10-Feb-2021", "date_update": "09-Mar-2021", "tables": [{"name": "table1.dat", "desc": "Wide binaries in which RAVE has observed both stars in the pair and data pass the quality cuts", "columns": [{"name": "SourceID1", "desc": "Primary Gaia DR1 designation "}, {"name": "RV1", "desc": "Primary radial velocity "}, {"name": "e_RV1", "desc": "Primary radial velocity error "}, {"name": "[M/H]1", "desc": "Primary metallicity "}, {"name": "e_[M/H]1", "desc": "Primary metallicity error "}, {"name": "Teff1", "desc": "Primary effective temperature "}, {"name": "logg1", "desc": "Primary surface gravity "}, {"name": "SourceID2", "desc": "Secondary Gaia DR1 designation "}, {"name": "RV2", "desc": "Secondary radial velocity "}, {"name": "e_RV2", "desc": "Secondary radial velocity error "}, {"name": "[M/H]2", "desc": "Secondary metallicity "}, {"name": "e_[M/H]2", "desc": "Secondary metallicity error "}, {"name": "Teff2", "desc": "Secondary effective temperature "}, {"name": "logg2", "desc": "Secondary surface gravity "}]}, {"name": "table2.dat", "desc": "Wide binaries in which LAMOST has observed both stars in the pair and data pass the quality cuts", "columns": [{"name": "SourceID1", "desc": "Primary Gaia DR1 designation "}, {"name": "RV1", "desc": "Primary radial velocity "}, {"name": "e_RV1", "desc": "Primary radial velocity error "}, {"name": "[Fe/H]1", "desc": "Primary metallicity "}, {"name": "l_e_[Fe/H]1", "desc": "Limit flag on e_[Fe/H]1 "}, {"name": "e_[Fe/H]1", "desc": "Primary metallicity error "}, {"name": "Teff1", "desc": "Primary effective temperature "}, {"name": "logg1", "desc": "Primary surface gravity "}, {"name": "SourceID2", "desc": "Secondary Gaia DR1 designation "}, {"name": "RV2", "desc": "Secondary radial velocity "}, {"name": "e_RV2", "desc": "Secondary radial velocity error "}, {"name": "[Fe/H]2", "desc": "Secondary metallicity "}, {"name": "e_[Fe/H]2", "desc": "Secondary metallicity error "}, {"name": "Teff2", "desc": "Secondary effective temperature "}, {"name": "logg2", "desc": "Secondary surface gravity "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_474_3344"}} {"id": "J/MNRAS/474/3344", "title_cds": "Short Title", "title_create": "Britavskiy+, 2018", "year": "2018", "author": "Britavskiy N., Pancino E., Tsymbal V., Romano D., Fossati L.", "title_pub": "A new method of measuring centre-of-mass velocities of radially pulsating stars from high-resolution spectroscopy.", "first_author": "Britavskiy N.", "ref_biblio": [""], "bibcode": ["2018MNRAS.474.3344B"], "keyword_cds": "", "keyword_pub": "methods: data analysis - techniques: radial velocities - stars: oscillations - stars: variables: Cepheids - stars: variables: RR Lyrae", "abstract": ["We present a radial velocity analysis of 20 solar neighbourhood RR", "Lyrae and three Population II Cepheid variables. We obtained", "high-resolution, moderate-to-high signal-to-noise ratio spectra for", "most stars; these spectra covered different pulsation phases for each", "star. To estimate the gamma (centre-of-mass) velocities of the", "programme stars, we use two independent methods. The first,", "\u2018classic\u2019 method is based on RR Lyrae radial velocity curve", "templates. The second method is based on the analysis of", "absorption-line profile asymmetry to determine both pulsational and", "gamma velocities. This second method is based on the least-squares", "deconvolution (LSD) technique applied to analyse the line asymmetry", "that occurs in the spectra. We obtain measurements of the pulsation", "component of the radial velocity with an accuracy of +/-3.5km/s.", "The gamma velocity was determined with an accuracy of +/-10km/s,", "even for those stars having a small number of spectra. The main", "advantage of this method is the possibility of obtaining an estimation", "of gamma velocity even from one spectroscopic observation with", "uncertain pulsation phase. A detailed investigation of LSD profile", "asymmetry shows that the projection factor p varies as a function of", "the pulsation phase - this is a key parameter, which converts", "observed spectral line radial velocity variations into photospheric", "pulsation velocities. As a by-product of our study, we present 41", "densely spaced synthetic grids of LSD profile bisectors based on", "atmospheric models of RR Lyr covering all pulsation phases."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "26-Feb-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_475_4504"}} {"id": "J/MNRAS/475/4504", "title_cds": "Short Title", "title_create": "Barker+, 2018", "year": "2018", "author": "Barker H., Zijlstra A., De Marco O., Frew D.J., Drew J.E., Corradi R.L.M., Eisloffel J., Parker Q.A.", "title_pub": "The binary fraction of planetary nebula central stars. III. The promise of VPHAS+.", "first_author": "Barker H.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.4504B"], "keyword_cds": "", "keyword_pub": "planetary nebulae, central stars, photometry", "abstract": ["The majority of planetary nebulae (PNe) are not spherical, and current", "single-star models cannot adequately explain all the morphologies we", "observe. This has led to the Binary Hypothesis, which states that PNe", "are preferentially formed by binary systems. This hypothesis can be", "corroborated or disproved by comparing the estimated binary fraction", "of all PNe central stars (CS) to that of the supposed progenitor", "population. One way to quantify the rate of CS binarity is to detect", "near infrared excess indicative of a low-mass main-sequence companion.", "In this paper, a sample of known PNe within data release 2 of the", "ongoing VPHAS+ is investigated. We give details of the method used to", "calibrate VPHAS+ photometry, and present the expected colours of CS", "and main-sequence stars within the survey. Objects were scrutinized to", "remove PN mimics from our sample and identify true CS. Within our", "final sample of seven CS, six had previously either not been", "identified or confirmed. We detected an i-band excess indicative of a", "low-mass companion star in three CS, including one known binary,", "leading us to conclude that VPHAS+ provides the precise photometry", "required for the IR excess method presented here, and will likely", "improve as the survey completes and the calibration process finalized.", "Given the promising results from this trial sample, the entire VPHAS+", "catalogue should be used to study PNe and extend the IR excess-tested", "CS sample."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stx3240"], "orcid_pub": ["0000-0002-2326-2885"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_475_716"}} {"id": "J/MNRAS/475/716", "title_cds": "Short Title", "title_create": "Green+, 2018", "year": "2018", "author": "Green A.W., Croom S.M., Scott N., Cortese L., Medling A.M., D'eugenio F., Bryant J.J., Bland-Hawthorn J., Allen J.T., Sharp R., Ho I.-T., Groves B., Drinkwater M.J., Mannering E., Harischandra L., Van De Sande J., Thomas A.D., O'Toole S., Mcdermid R.M., Vuong M., Sealey K., Bauer A.E., Brough S., Catinella B., Cecil G., Colless M., Couch W.J., Driver S.P., Federrath C., Foster C., Goodwin M., Hampton E.J., Hopkins A.M., Jones D.H., Konstantopoulos I.S., Lawrence J.S., Leon-Saval S.G., Liske J., Lopez-sanchez A.R., Lorente N.P.F., Mould J., Obreschkow D., Owers M.S., Richards S.N., Robotham A.S.G., Schaefer A.L., Sweet S.M., Taranu D.S., Tescari E., Tonini C., Zafar T.", "title_pub": "The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products.", "first_author": "Green A.W.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475..716G"], "keyword_cds": "", "keyword_pub": "surveys - galaxies: general", "abstract": ["We present the first major release of data from the SAMI Galaxy", "Survey. This data release focuses on the emission-line physics of", "galaxies. Data Release One includes data for 772 galaxies, about 20", "per cent of the full survey. Galaxies included have the redshift range", "0.004"], "bibcode": ["2018MNRAS.475.1306G"], "keyword_cds": "", "keyword_pub": "galaxies: active - galaxies: statistics - radio continuum: galaxies", "abstract": ["We present high sensitivity ({sigma}_P_~=0.6mJy) polarimetric", "observations in seven bands, from 2.1 to 38GHz, of a complete sample", "of 104 compact extragalactic radio sources brighter than 200mJy at", "20GHz. Polarization measurements in six bands, in the range 5.5-38GHz,", "for 53 of these objects were reported by Galluzzi et al. We have added", "new measurements in the same six bands for another 51 sources and", "measurements at 2.1GHz for the full sample of 104 sources. Also, the", "previous measurements at 18, 24, 33, and 38GHz were re-calibrated", "using the updated model for the flux density absolute calibrator,", "PKS1934-638, not available for the earlier analysis. The observations,", "carried out with the Australia Telescope Compact Array, achieved a 90", "per cent detection rate (at 5{sigma}) in polarization. 89 of our", "sources have a counterpart in the 72-231MHz GLEAM (GaLactic and", "Extragalactic All-sky Murchison Widefield Array) survey, providing an", "unparalleled spectral coverage of 2.7 decades of frequency for these", "sources. While the total intensity data from 5.5 to 38GHz could be", "interpreted in terms of single component emission, a joint analysis of", "more extended total intensity spectra presented here, and of the", "polarization spectra, reveals that over 90 per cent of our sources", "show clear indications of at least two emission components. We", "interpret this as an evidence of recurrent activity. Our high", "sensitivity polarimetry has allowed a 5{sigma} detection of the weak", "circular polarization for ~38 per cent of the data set, and a deeper", "estimate of 20GHz polarization source counts than has been possible so", "far."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "01-Apr-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_475_4768"}} {"id": "J/MNRAS/475/4768", "title_cds": "Short Title", "title_create": "Tucker+, 2018", "year": "2018", "author": "Tucker M.A., Fleming S.W., Pelisoli I., Romero A., Bell K.J., Kepler S.O., Caton D.B., Debes J., Montgomery M.H., Thompson S.E., Koester D., Million C., Shiao B.", "title_pub": "White dwarf variability with gPhoton: pulsators.", "first_author": "Tucker M.A.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.4768T"], "keyword_cds": "", "keyword_pub": "techniques: photometric - stars: oscillations - white dwarfs - ultraviolet: stars", "abstract": ["We present results from a search for short time-scale white dwarf", "variability using gPhoton, a time-tagged data base of GALEX photon", "events and associated software package. We conducted a survey of 320", "white dwarf stars in the McCook-Sion catalogue, inspecting each for", "photometric variability with particular emphasis on variability over", "time-scales less than ~30 min. From that survey, we present the", "discovery of a new pulsating white dwarf: WD 2246-069. A CaII K line", "is found in archival ESO spectra and an IR excess is seen in WISE W1", "and W2 bands. Its independent modes are identified in follow-up", "optical photometry and used to model its interior structure.", "Additionally, we detect UV pulsations in four previously known", "pulsating ZZ Ceti-type (DAVs). Included in this group is the", "simultaneous fitting of the pulsations of WD 1401-147 in optical,", "near-ultraviolet and far-ultraviolet bands using nearly concurrent", "Whole Earth Telescope and GALEX data, providing observational insight", "into the wavelength dependence of white dwarf pulsation amplitudes."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "08-Apr-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_476_307"}} {"id": "J/MNRAS/476/307", "title_cds": "Short Title", "title_create": "Moreno-Raya+, 2018", "year": "2018", "author": "Moreno-Raya M.E., Galbany L., Lopez-Sanchez A.R., Molla M., Gonzalez-Gaitan S., Vilchez J.M., Carnero A.", "title_pub": "Elemental gas-phase abundances of intermediate redshift type Ia supernova star-forming host galaxies.", "first_author": "Moreno-Raya M.E.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476..307M"], "keyword_cds": "", "keyword_pub": "methods: data analysis - techniques: spectroscopic - supernovae: general - ISM: abundances - HII regions - galaxies: abundances", "abstract": ["The maximum luminosity of type Ia supernovae (SNe Ia) depends on the", "oxygen abundance of the regions of the host galaxies, where they", "explode. This metallicity dependence reduces the dispersion in the", "Hubble diagram (HD) when included with the traditional two-parameter", "calibration of SN Ia light-curve parameters and absolute magnitude. In", "this work, we use empirical calibrations to carefully estimate the", "oxygen abundance of galaxies hosting SNe Ia from the SDSS-II/SN (Sloan", "Digital Sky Survey-II Supernova) survey at intermediate redshift by", "measuring their emission-line intensities. We also derive electronic", "temperature with the direct method for a small fraction of objects for", "consistency. We find a trend of decreasing oxygen abundance with", "increasing redshift for the most massive galaxies. Moreover, we study", "the dependence of the HD residuals (HR) with galaxy oxygen abundance", "obtaining a correlation in line with those found in other works. In", "particular, the HR versus oxygen abundance shows a slope of", "-0.186+/-0.123mag/dex (1.52{sigma}) in good agreement with theoretical", "expectations. This implies smaller distance modulii after corrections", "for SNe Ia in metal-rich galaxies. Based on our previous results on", "local SNe Ia, we propose this dependence to be due to the lower", "luminosity of the SNe Ia produced in more metal-rich environments."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "13-Apr-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_476_528"}} {"id": "J/MNRAS/476/528", "title_cds": "Short Title", "title_create": "El-badry+, 2018", "year": "2018", "author": "El-badry K., Ting Y.-S., Rix H.-W., Quataert E., Weisz D.R., Cargile P., Conroy C., Hogg D.W., Bergemann M., Liu C.", "title_pub": "Discovery and characterization of 3000+ main-sequence binaries from APOGEE spectra.", "first_author": "El-badry K.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476..528E"], "keyword_cds": "", "keyword_pub": "methods: data analysis - binaries: spectroscopic - Galaxy: stellar content", "abstract": ["We develop a data-driven spectral model for identifying and", "characterizing spatially unresolved multiple-star systems and apply it", "to APOGEE DR13 spectra of main-sequence stars. Binaries and triples", "are identified as targets whose spectra can be significantly better", "fit by a superposition of two or three model spectra, drawn from the", "same isochrone, than any single-star model. From an initial sample of", "~20000 main-sequence targets, we identify ~2500 binaries in", "which both the primary and secondary stars contribute detectably to", "the spectrum, simultaneously fitting for the velocities and stellar", "parameters of both components. We additionally identify and fit", "~200 triple systems, as well as ~700 velocity-variable systems in", "which the secondary does not contribute detectably to the spectrum.", "Our model simplifies the process of simultaneously fitting single- or", "multi-epoch spectra with composite models and does not depend on a", "velocity offset between the two components of a binary, making it", "sensitive to traditionally undetectable systems with periods of", "hundreds or thousands of years. In agreement with conventional", "expectations, almost all the spectrally identified binaries with", "measured parallaxes fall above the main sequence in the", "colour-magnitude diagram. We find excellent agreement between", "spectrally and dynamically inferred mass ratios for the ~600", "binaries in which a dynamical mass ratio can be measured from", "multi-epoch radial velocities. We obtain full orbital solutions for 64", "systems, including 14 close binaries within hierarchical triples. We", "make available catalogues of stellar parameters, abundances, mass", "ratios, and orbital parameters."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "13-Apr-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_477_3343"}} {"id": "J/MNRAS/477/3343", "title_cds": "Short Title", "title_create": "Sitnova+, 2018", "year": "2018", "author": "Sitnova T.M., Mashonkina L.I., Ryabchikova T.A.", "title_pub": "A NLTE line formation for neutral and singly ionized calcium in model atmospheres of B-F stars.", "first_author": "Sitnova T.M.", "ref_biblio": [""], "bibcode": ["2018MNRAS.477.3343S"], "keyword_cds": "", "keyword_pub": "line: formation - stars: abundances - stars: atmospheres", "abstract": ["We present non-local thermodynamic equilibrium (NLTE) line formation", "calculations for CaI and CaII in B-F stars. The sign and the", "magnitude of NLTE abundance corrections depend on line and stellar", "parameters. We determine calcium abundances for nine stars with", "reliable stellar parameters. For all stars, where the lines of both", "species could be measured, the NLTE abundances are found to be", "consistent within the error bars. We obtain consistent NLTE abundances", "from CaII lines in the visible and near infra-red (IR, 8912-27,", "9890{AA}) spectrum range, in contrast with LTE, where the discrepancy", "between the two groups of lines ranges from -0.5 to 0.6 dex for", "different stars. Our NLTE method reproduces the CaII 8912-27, 9890{AA}", "lines observed in emission in the late B-type star HD 160762 with the", "classical plane-parallel and LTE model atmosphere. NLTE abundance", "corrections for lines of CaI and CaII were calculated in a grid of", "model atmospheres with 7000<=T_eff_<=13000K, 3.2<=logg<=5.0,", "-0.5<=[Fe/H]<=0.5, {xi}_t_=2.0km/s. Our NLTE results can be applied", "for calcium NLTE abundance determination from Gaia spectra, given that", "accurate continuum normalization and proper treatment of the hydrogen", "Paschen lines are provided. The NLTE method can be useful to refine", "calcium underabundances in Am stars and to provide accurate", "observational constraints on the models of diffusion."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "10-Jun-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_478_L116"}} {"id": "J/MNRAS/478/L116", "title_cds": "Short Title", "title_create": "Mernier+, 2018", "year": "2018", "author": "Mernier F., De Plaa J., Werner N., Kaastra J.S., Raassen A.J.J., Gu L., Mao J., Urdampilleta I., Truong N., Simionescu A.", "title_pub": "Mass-invariance of the iron enrichment in the hot haloes of massive ellipticals, groups, and clusters of galaxies.", "first_author": "Mernier F.", "ref_biblio": [""], "bibcode": ["2018MNRAS.478L.116M"], "keyword_cds": "", "keyword_pub": "galaxies: clusters: intracluster medium - X-rays: galaxies: clusters - X-rays: galaxies", "abstract": ["X-ray measurements find systematically lower Fe abundances in the", "X-ray emitting haloes pervading groups (kT<=1.7keV) than in", "clusters of galaxies. These results have been difficult to reconcile", "with theoretical predictions. However, models using incomplete atomic", "data or the assumption of isothermal plasmas may have biased the", "best-fitting Fe abundance in groups and giant elliptical galaxies low.", "In this work, we take advantage of a major update of the atomic code", "in the spectral fitting package SPEX to re-evaluate the Fe abundance", "in 43 clusters, groups, and elliptical galaxies (the CHEERS sample) in", "a self-consistent analysis and within a common radius of 0.1r_500_.", "For the first time, we report a remarkably similar average Fe", "enrichment in all these systems. Unlike previous results, this", "strongly suggests that metals are synthesized and transported in these", "haloes with the same average efficiency across two orders of magnitude", "in total mass. We show that the previous metallicity measurements in", "low-temperature systems were biased low due to incomplete atomic data", "in the spectral fitting codes. The reasons for such a code-related Fe", "bias, also implying previously unconsidered biases in the emission", "measure and temperature structure, are discussed."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "25-Jun-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_478_4669"}} {"id": "J/MNRAS/478/4669", "title_cds": "Short Title", "title_create": "Themessl+, 2018", "year": "2018", "author": "Themessl N., Hekker S., Southworth J., Beck P.G., Pavlovski K., Tkachenko A., Angelou G.C., Ball W.H., Barban C., Corsaro E., Elsworth Y., Handberg R., Kallinger T.", "title_pub": "Oscillating red giants in eclipsing binary systems: empirical reference value for asteroseismic scaling relation.", "first_author": "Themessl N.", "ref_biblio": [""], "bibcode": ["2018MNRAS.478.4669T"], "keyword_cds": "", "keyword_pub": "asteroseismology - binaries: eclipsing - stars: individual: KIC 8410637, KIC 5640750, KIC 9540226 - stars: interiors - stars: oscillations", "abstract": ["The internal structures and properties of oscillating red-giant stars", "can be accurately inferred through their global oscillation modes", "(asteroseismology). Based on 1460 d of Kepler observations we perform", "a thorough asteroseismic study to probe the stellar parameters and", "evolutionary stages of three red giants in eclipsing binary systems.", "We present the first detailed analysis of individual oscillation modes", "of the red-giant components of KIC 8410637, KIC 5640750, and", "KIC 9540226. We obtain estimates of their asteroseismic masses, radii,", "mean densities, and logarithmic surface gravities by using the", "asteroseismic scaling relations as well as grid-based modelling. As", "these red giants are in double-lined eclipsing binaries, it is", "possible to derive their independent dynamical masses and radii from", "the orbital solution and compare it with the seismically inferred", "values. For KIC 5640750 we compute the first spectroscopic orbit based", "on both components of this system. We use high-resolution", "spectroscopic data and light curves of the three systems to determine", "up-to-date values of the dynamical stellar parameters. With our", "comprehensive set of stellar parameters we explore consistencies", "between binary analysis and asteroseismic methods, and test the", "reliability of the well-known scaling relations. For the three red", "giants under study, we find agreement between dynamical and", "asteroseismic stellar parameters in cases where the asteroseismic", "methods account for metallicity, temperature, and mass dependence as", "well as surface effects. We are able to attain agreement from the", "scaling laws in all three systems if we use", "{Delta}{nu}_ref,emp_=130.8+/-0.9uHz instead of the usual solar", "reference value."], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "04-Oct-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_478_5547"}} {"id": "J/MNRAS/478/5547", "title_cds": "Short Title", "title_create": "Alger+, 2018", "year": "2018", "author": "Alger M.J., Banfield J.K., Ong C.S., Rudnick L., Wong O.I., Wolf C., Andernach H., Norris R.P., Shabala S.S.", "title_pub": "Radio Galaxy Zoo: machine learning for radio source host galaxy cross-identification.", "first_author": "Alger M.J.", "ref_biblio": [""], "bibcode": ["2018MNRAS.478.5547A"], "keyword_cds": "", "keyword_pub": "methods: statistical - techniques: miscellaneous - galaxies: active - infrared: galaxies - radio continuum: galaxies", "abstract": ["We consider the problem of determining the host galaxies of radio", "sources by cross-identification. This has traditionally been done", "manually, which will be intractable for wide-area radio surveys like", "the Evolutionary Map of the Universe. Automated cross-identification", "will be critical for these future surveys, and machine learning may", "provide the tools to develop such methods. We apply a standard", "approach from computer vision to cross-identification, introducing one", "possible way of automating this problem, and explore the pros and cons", "of this approach. We apply our method to the 1.4GHz Australian", "Telescope Large Area Survey (ATLAS) observations of the Chandra Deep", "Field South (CDFS) and the ESO Large Area ISO Survey South 1 fields by", "cross-identifying them with the Spitzer Wide-area Infrared", "Extragalactic survey. We train our method with two sets of data:", "expert cross-identifications of CDFS from the initial ATLAS data", "release and crowdsourced cross-identifications of CDFS from Radio", "Galaxy Zoo. We found that a simple strategy of cross-identifying a", "radio component with the nearest galaxy performs comparably to our", "more complex methods, though our estimated best-case performance is", "near 100 per cent. ATLAS contains 87 complex radio sources that have", "been cross-identified by experts, so there are not enough complex", "examples to learn how to cross-identify them accurately. Much larger", "data sets are therefore required for training methods like ours. We", "also show that training our method on Radio Galaxy Zoo", "cross-identifications gives comparable results to training on expert", "cross-identifications, demonstrating the value of crowdsourced", "training data."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "20-Jan-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_480_768"}} {"id": "J/MNRAS/480/768", "title_cds": "Short Title", "title_create": "Davies+, 2018", "year": "2018", "author": "Davies L.J.M., Robotham A.S.G., Driver S.P., Lagos C.D.P., Cortese L., Mannering E., Foster C., Lidman C., Hashemizadeh A., Koushan S., O'toole S., Baldry I.K., Bilicki M., Bland-hawthorn J., Bremer M.N., Brown M.J.I., Bryant J.J., Catinella B., Croom S.M., Grootes M.W., Holwerda B.W., Jarvis M.J., Maddox N., Meyer M., Moffett A.J., Phillipps S., Taylor E.N., Windhorst R.A., Wolf C.", "title_pub": "Deep Extragalactic VIsible Legacy Survey (DEVILS): motivation,design, and target catalogue.", "first_author": "Davies L.J.M.", "ref_biblio": [""], "bibcode": ["2018MNRAS.480..768D"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "13-May-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_480_1218"}} {"id": "J/MNRAS/480/1218", "title_cds": "Short Title", "title_create": "Wan+, 2018", "year": "2018", "author": "Wan Z., Kafle P.R., Lewis G.F., Mackey D., Sharma S., Ibata R.A.", "title_pub": "Galactic cartography with SkyMapper - I. Population substructure and the stellar number density of the inner halo.", "first_author": "Wan Z.", "ref_biblio": [""], "bibcode": ["2018MNRAS.480.1218W"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "16-May-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_480_1384"}} {"id": "J/MNRAS/480/1384", "title_cds": "K-enhanced and possibly Mg-depleted stars", "title_create": "Kemp+, 2018", "year": "2018", "author": "Kemp A.J., Casey A.R., Miles M.T., Norfolk B.J., Lattanzio J.C., Karakas A.I., Schlaufman K.C., Ho A.Y.Q., Tout C.A., Ness M., Ji A.P.", "title_pub": "On the discovery of K-enhanced and possibly Mg-depleted stars throughout the Milky Way.", "first_author": "Kemp A.J.", "ref_biblio": [""], "bibcode": ["2018MNRAS.480.1384K"], "keyword_cds": "Abundances ; Clusters, globular ; Stars, peculiar ; Spectroscopy", "keyword_pub": "methods: data analysis, catalogues - stars: chemically peculiar - Galaxy: abundances - Galaxy: evolution - globular clusters: individual: evolution", "abstract": ["Stars with unusual elemental abundances offer clues about rare", "astrophysical events or nucleosynthetic pathways. Stars with", "significantly depleted magnesium and enhanced potassium ([Mg/Fe]<-0.5;", "[K/Fe]>1) have to date only been found in the massive globular cluster", "NGC 2419 and, to a lesser extent, NGC 2808. The origin of this", "abundance signature remains unknown, as does the reason for its", "apparent exclusivity to these two globular clusters. Here we present", "112 field stars, identified from 454 180 LAMOST giants, that show", "significantly enhanced [K/Fe] and possibly depleted [Mg/Fe] abundance", "ratios. Our sample spans a wide range of metallicities", "(-1.5<[Fe/H]<0.3), yet none show abundance ratios of [K/Fe] or [Mg/Fe]", "that are as extreme as those observed in NGC 2419. If confirmed, the", "identified sample of stars represents evidence that the", "nucleosynthetic process producing the anomalous abundances ratios of", "[K/Fe] and [Mg/Fe] probably occurs at a wide range of metallicities.", "This would suggest that pollution scenarios that are limited to early", "epochs (such as Population III supernovae) are an unlikely", "explanation, although they cannot be ruled out entirely. This sample", "is expected to help guide modelling attempts to explain the origin of", "the Mg-K abundance signature."], "description": ["We used a set of 454 180 giant stars from the second LAMOST data", "release (Luo et al. 2015RAA....15...15L). The spectra were placed at", "rest-frame on a common wavelength sampling from 3905{AA} to 9000{AA}", "and normalized by Ho et al. (2017ApJ...836....5H). The Cannon (Ness et", "al. 2016ApJ...823..114N; Ho et al. 2017ApJ...836....5H) was used to", "estimate effective temperature Teff, surface gravity", "log_10_(gcm^-1^s^-2^), metallicity [Fe/H], and mean{alpha}-element", "abundance relative to iron [{alpha}/Fe] using 9,952 stars in common", "between LAMOST and the APOGEE (Alam et al. 2015ApJS..219...12A)", "survey. We fit a Gaussian profile of amplitude A to the flux residuals", "for all three absorption lines in the Mg triplet (5167{AA}, 5172{AA},", "5184{AA}) as well as the K doublet (7665{AA}, 7699{AA}) for all 454", "180 giants. We identified candidates by requiring that they match at", "least one of three quality filters. These filters identified 384", "unique stars. We visually inspected every candidate (multiple times)", "and excluded stars that showed any evidence of being a false positive.", "The distilled catalogue contains 112 candidate stars with spectra", "consistent with enhancements in K and depletions in Mg."], "type": ["OC"], "data": "", "date_update": "30-May-2022", "tables": [{"name": "tablea2.dat", "desc": "Atomic line abundances measured from Magellan/MIKE follow-up spectra of three Mg/K candidates", "columns": [{"name": "LAMOST", "desc": "LAMOST ID (JHHMMSS.ss+DDMMSS.s) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "S/N", "desc": "Signal to noise ratio "}, {"name": "RV", "desc": "Radial velocity of the star "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "[alpha/Fe]", "desc": "Mean {alpha}-element abundance relative to iron"}, {"name": "Chi2", "desc": "Chi-squared "}, {"name": "[K/Fe]", "desc": "K abundance relative to iron "}, {"name": "e_[K/Fe]", "desc": "Error on [K/Fe] "}, {"name": "[Na/Fe]", "desc": "Na abundance relative to iron "}, {"name": "e_[Na/Fe]", "desc": "Error on [Na/Fe] "}, {"name": "[Mg/Fe]", "desc": "Mg abundance relative to iron "}, {"name": "e_[Mg/Fe]", "desc": "Error on [Mg/Fe] "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_480_2343"}} {"id": "J/MNRAS/480/2343", "title_cds": "Short Title", "title_create": "Choksi+, 2018", "year": "2018", "author": "Choksi N., Gnedin O.Y., Li H.", "title_pub": "Formation of globular cluster systems: from dwarf galaxies to giants.", "first_author": "Choksi N.", "ref_biblio": [""], "bibcode": ["2018MNRAS.480.2343C"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "19-May-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_480_3871"}} {"id": "J/MNRAS/480/3871", "title_cds": "Short Title", "title_create": "Coughlin+, 2018", "year": "2018", "author": "Coughlin M.W., Dietrich T., Doctor Z., Kasen D., Coughlin S., Jerkstrand A., Leloudas G., Mcbrien O., Metzger B.D., O'shaughnessy R., Smartt S.J.", "title_pub": "Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations.", "first_author": "Coughlin M.W.", "ref_biblio": [""], "bibcode": ["2018MNRAS.480.3871C"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "25-May-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_482_L139"}} {"id": "J/MNRAS/482/L139", "title_cds": "Short Title", "title_create": "El-badry+, 2019", "year": "2019", "author": "El-badry K., Rix H.-W.", "title_pub": "The wide binary fraction of solar-type stars: emergence of metallicity dependence at a < 200 au.", "first_author": "El-badry K.", "ref_biblio": [""], "bibcode": ["2019MNRAS.482L.139E"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "17-Jun-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_482_5302"}} {"id": "J/MNRAS/482/5302", "title_cds": "GALAH co-orbiting stars and chemical tagging", "title_create": "Simpson+, 2019", "year": "2019", "author": "Simpson J.D., Martell S.L., Da Costa G., Casey A.R., Freeman K.C., Horner J., Ting Y.-S., Nataf D.M., Lewis G.F., Ness M.K., Zucker D.B., Cottrell P.L., Cotar K., Asplund M., Bland-Hawthorn J., Buder S., D'Orazi V., De Silva G.M., Duong L., Kos J., Lin J., Lind K., Schlesinger K.J., Sharma S., Zwitter T., Kafle P.R., Nordlander T.", "title_pub": "The GALAH survey: co-orbiting stars and chemical tagging.", "first_author": "Simpson J.D.", "ref_biblio": [""], "bibcode": ["2019MNRAS.482.5302S"], "see_also": ["J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018)", "J/AJ/153/257 : Comoving stars in Gaia DR1 (Oh+, 2017)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)"], "keyword_cds": "Abundances ; Galactic plane ; Magnitudes ; Stars, fundamental", "keyword_pub": "stars: abundances, stars: formation, galaxy: disc", "abstract": ["We present a study using the second data release of the GALAH survey", "of stellar parameters and elemental abundances of 15 pairs of stars", "identified by Oh et al. They identified these pairs as potentially", "co-moving pairs using proper motions and parallaxes from Gaia DR1. We", "find that 11 very wide (>1pc) pairs of stars do in fact have similar", "Galactic orbits, while a further four claimed co-moving pairs are not", "truly co-orbiting. Eight of the 11 co-orbiting pairs have reliable", "stellar parameters and abundances, and we find that three of those are", "quite similar in their abundance patterns, while five have significant", "[Fe/H] differences. For the latter, this indicates that they could be", "co-orbiting because of the general dynamical coldness of the thin", "disc, or perhaps resonances induced by the Galaxy, rather than a", "shared formation site. Stars such as these, wide binaries, debris of", "past star formation episodes, and coincidental co-orbiters, are", "crucial for exploring the limits of chemical tagging in the Milky Way."], "description": ["We make use of an internally released catalogue of a similar size and", "composition to the GALAH survey's second data release (GALAH DR2;", "Buder et al. 2018MNRAS.478.4513B, Cat. J/MNRAS/478/4513) that", "maximized the overlap between GALAH and Oh et al.", "(2017AJ....153..257O, Cat. J/AJ/153/257) (hereafter O17). It is based", "upon spectra obtained between 2014 January and 2018 January using the", "3.9-m Anglo-Australian Telescope with the HERMES spectrograph (Sheinis", "et al. 2015JATIS...1c5002S) and the Two-Degree Field (2dF) top-end", "(Lewis et al. 2002MNRAS.333..279L). The 2dF allows for the concurrent", "acquisition of up to ~360 science targets per exposure. HERMES", "simultaneously acquires spectra using four independent cameras with", "non-contiguous wavelength coverage totalling ~1000{AA} at a spectral", "resolving power of R~28000.", "Overall, the GALAH release used in this work contains a total of", "365516 stars with up to 23 elemental abundances per star. For a", "minority of stars, the label results from the cannon are not reliable:", "The label result could be too far from the training set, the {chi}^2^", "between the observed spectrum and the spectrum calculated by the", "cannon could be too large, or the spectra could have been classified", "by t-SNE (for details on the application of t-SNE to GALAH spectra see", "Traven et al. 2017ApJS..228...24T, Cat. J/ApJS/228/24) as having", "problems. In addition, the individual elemental abundance can be", "flagged for similar reasons.", "O17 identified 10606 stars to be in non-exclusive co-moving pairs or", "groups.3 Unfortunately, only 117 of these stars are found in the GALAH", "catalogue, and only 15 pairs had both stars observed (i.e. 30 stars).", "Table 1 lists the O17 group ID, the GALAH sobject_id, stellar", "parameters, photometry, and orbital parameters for the 15 pairs."], "data": "", "date_update": "04-Jul-2022", "tables": [{"name": "table1.dat", "desc": "The stellar parameters and orbital characteristics of the 15 pairs", "columns": [{"name": "Name", "desc": "GALAH Name (GALAH NNNNNNNNNNNNNNN) "}, {"name": "GName", "desc": "Group Name ([OPH2017] NNNN) "}, {"name": "e", "desc": "Eccentricity "}, {"name": "e_e", "desc": "Error on e "}, {"name": "zmax", "desc": "Maximum distance above Galactic plane "}, {"name": "e_zmax", "desc": "Error on zmax "}, {"name": "Rperi", "desc": "Perigalactic distance of the Galactic orbit "}, {"name": "e_Rperi", "desc": "Error on Rperi "}, {"name": "Rapo", "desc": "Apogalactic distance of the Galactic orbit "}, {"name": "e_Rapo", "desc": "Error on Rapo "}, {"name": "GaiaDR2", "desc": "Gaia DR2 identifier "}, {"name": "Gmag", "desc": "Gaia DR2 G-band magnitude "}, {"name": "BP-RP", "desc": "Gaia DR2 BP-RP color index "}, {"name": "RVsynt", "desc": "Barycentric radial velocity from cross-correlation against synthetic spectra"}, {"name": "e_RVsynt", "desc": "Error on RVsynt "}, {"name": "flagcannon", "desc": "Flags for spectrum information in a bitmask format (1)"}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "e_Teff", "desc": "Error on Teff "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "e_logg", "desc": "Error on logg "}, {"name": "[Fe/H]", "desc": "Iron abundance "}, {"name": "e_[Fe/H]", "desc": "Error on [Fe/H] "}, {"name": "vmic", "desc": "Microturbulence velocity "}, {"name": "e_vmic", "desc": "Error on vmic "}, {"name": "vsini", "desc": "Line of sight rotational velocity "}, {"name": "e_vsini", "desc": "Error on vsini "}, {"name": "[alpha/Fe]", "desc": "? {alpha} enhancement, determined as an error-weighted combination of Mg, Si, Ca, Ti abundances"}, {"name": "e_[alpha/Fe]", "desc": "? Error on [alpha/Fe] "}, {"name": "[Li/Fe]", "desc": "Lithium to iron abundance ratio "}, {"name": "e_[Li/Fe]", "desc": "Error on [Li/Fe] "}, {"name": "f_[Li/Fe]", "desc": "Flag on [Li/Fe] (2) "}, {"name": "[C/Fe]", "desc": "Carbon to iron abundance ratio "}, {"name": "e_[C/Fe]", "desc": "Error on [C/Fe] "}, {"name": "f_[C/Fe]", "desc": "Flag on [C/Fe] (2) "}, {"name": "[O/Fe]", "desc": "Oxygen to iron abundance ratio "}, {"name": "e_[O/Fe]", "desc": "Error on [O/Fe] "}, {"name": "f_[O/Fe]", "desc": "Flag on [O/Fe] (2) "}, {"name": "[Na/Fe]", "desc": "Sodium to iron abundance ratio "}, {"name": "e_[Na/Fe]", "desc": "Error on [Na/Fe] "}, {"name": "f_[Na/Fe]", "desc": "Flag on [Na/Fe] (2) "}, {"name": "[Mg/Fe]", "desc": "? Magnesium to iron abundance ratio "}, {"name": "e_[Mg/Fe]", "desc": "? Error on [Mg/Fe] "}, {"name": "f_[Mg/Fe]", "desc": "Flag on [Mg/Fe] (2) "}, {"name": "[Al/Fe]", "desc": "Aluminum to iron abundance ratio "}, {"name": "e_[Al/Fe]", "desc": "Error on [Al/Fe] "}, {"name": "f_[Al/Fe]", "desc": "Flag on [Al/Fe] (2) "}, {"name": "[Si/Fe]", "desc": "? Silicon to iron abundance ratio "}, {"name": "e_[Si/Fe]", "desc": "? Error on [Si/Fe] "}, {"name": "f_[Si/Fe]", "desc": "Flag on [Si/Fe] (2) "}, {"name": "[K/Fe]", "desc": "Potassium to iron abundance ratio "}, {"name": "e_[K/Fe]", "desc": "Error on [K_Fe] "}, {"name": "f_[K/Fe]", "desc": "Flag on [K_Fe] (2) "}, {"name": "[Ca/Fe]", "desc": "Calcuim to iron abundance ratio "}, {"name": "e_[Ca/Fe]", "desc": "Error on [Ca/Fe] "}, {"name": "f_[Ca/Fe]", "desc": "Flag on [Ca/Fe] (2) "}, {"name": "[Sc/Fe]", "desc": "Scandium to iron abundance ratio "}, {"name": "e_[Sc/Fe]", "desc": "Error on [Sc/Fe] "}, {"name": "f_[Sc/Fe]", "desc": "Flag on [Sc/Fe] (2) "}, {"name": "[Ti/Fe]", "desc": "? Titanium to iron abundance ratio "}, {"name": "e_[Ti/Fe]", "desc": "? Error on [Ti/Fe] "}, {"name": "f_[Ti/Fe]", "desc": "Flag on [Ti/Fe] (2) "}, {"name": "[V/Fe]", "desc": "Vanadium to iron abundance ratio "}, {"name": "e_[V/Fe]", "desc": "Error on [V/Fe] "}, {"name": "f_[V/Fe]", "desc": "Flag on [V/Fe] (2) "}, {"name": "[Cr/Fe]", "desc": "Chromium to iron abundance ratio "}, {"name": "e_[Cr/Fe]", "desc": "Error on [Cr/Fe] "}, {"name": "f_[Cr/Fe]", "desc": "Flag on [Cr/Fe] (2) "}, {"name": "[Mn/Fe]", "desc": "Manganese to iron abundance ratio "}, {"name": "e_[Mn/Fe]", "desc": "Error on [Mn/Fe] "}, {"name": "f_[Mn/Fe]", "desc": "Flag on [Mn/Fe] (2) "}, {"name": "[Co/Fe]", "desc": "Cobalt to iron abundance ratio "}, {"name": "e_[Co/Fe]", "desc": "Error on [Co/Fe] "}, {"name": "f_[Co/Fe]", "desc": "Flag on [Co/Fe] (2) "}, {"name": "[Ni/Fe]", "desc": "Nickel to iron abundance ratio "}, {"name": "e_[Ni/Fe]", "desc": "Error on [Ni/Fe] "}, {"name": "f_[Ni/Fe]", "desc": "Flag on [Ni/Fe] (2) "}, {"name": "[Cu/Fe]", "desc": "Copper to iron abundance ratio "}, {"name": "e_[Cu/Fe]", "desc": "Error on [Cu/Fe] "}, {"name": "f_[Cu/Fe]", "desc": "Flag on [Cu/Fe] (2) "}, {"name": "[Zn/Fe]", "desc": "Zinc to iron abundance ratio "}, {"name": "e_[Zn/Fe]", "desc": "Error on [Zn/Fe] "}, {"name": "f_[Zn/Fe]", "desc": "Flag on [Zn/Fe] (2) "}, {"name": "[Y/Fe]", "desc": "Yttrium to iron abundance ratio "}, {"name": "e_[Y/Fe]", "desc": "Error on [Y/Fe] "}, {"name": "f_[Y/Fe]", "desc": "Flag on [Y/Fe] (2) "}, {"name": "[Ba/Fe]", "desc": "Barium to iron abundance ratio "}, {"name": "e_[Ba/Fe]", "desc": "Error on [Ba/Fe] "}, {"name": "f_[Ba/Fe]", "desc": "Flag on [Ba/Fe] (2) "}, {"name": "[La/Fe]", "desc": "Lanthanum to iron abundance ratio "}, {"name": "e_[La/Fe]", "desc": "Error on [La/Fe] "}, {"name": "f_[La/Fe]", "desc": "Flag on [La/Fe] (2) "}, {"name": "[Eu/Fe]", "desc": "Europium to iron abundance ratio "}, {"name": "e_[Eu/Fe]", "desc": "Error on [Eu/Fe] "}, {"name": "f_[Eu/Fe]", "desc": "Flag on [Eu/Fe] (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_961"}} {"id": "J/MNRAS/485/961", "title_cds": "Short Title", "title_create": "Jayasinghe+, 2019", "year": "2019", "author": "Jayasinghe T., Stanek K.Z., Kochanek C.S., Shappee B.J., Holoien T.W.-S., Thompson T.A., Prieto J.L., Dong S., Pawlak M., Pejcha O., Shields J.V., Pojmanski G., Otero S., Hurst N., Britt C.A., Will D.", "title_pub": "The ASAS-SN catalogue of variable stars III: variables in the southern TESS continuous viewing zone.", "first_author": "Jayasinghe T.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485..961J"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "14-Sep-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_1085"}} {"id": "J/MNRAS/485/1085", "title_cds": "Classification of emission-line galaxies", "title_create": "Stampoulis+, 2019", "year": "2019", "author": "Stampoulis V., van Dyk D.A., Kashyap V.L., Zezas A.", "title_pub": "Multidimensional data-driven classification of emission-line galaxies.", "first_author": "Stampoulis V.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.1085S"], "keyword_cds": "Clusters, galaxy ; Galaxy catalogs", "keyword_pub": "galaxies: active - galaxies: clusters - galaxies: emission lines", "abstract": ["We propose a new soft clustering scheme for classifying galaxies in", "different activity classes using simultaneously four emission-line", "ratios: log([NII]/H{alpha}), log([SII]/H{alpha}), log([OI]/H{alpha}),", "and log([OIII]/H{beta}). We fit 20 multivariate Gaussian distributions", "to the four-dimensional distribution of these lines obtained from the", "Sloan Digital Sky Survey in order to capture local structures and", "subsequently group the multivariate Gaussian distributions to", "represent the complex multidimensional structure of the joint", "distribution of galaxy spectra in the four-dimensional line ratio", "space. The main advantages of this method are the use of all four", "optical-line ratios simultaneously and the adoption of a clustering", "scheme. This maximizes the use of the available information, avoids", "contradicting classifications, and treats each class as a distribution", "resulting in soft classification boundaries and providing the", "probability for an object to belong to each class. We also introduce", "linear multidimensional decision surfaces using support vector", "machines based on the classification of our soft clustering scheme.", "This linear multidimensional hard clustering technique shows high", "classification accuracy with respect to our soft clustering scheme."], "description": ["The SDSS provides an excellent resource of spectra of the central", "regions (~5.5kpc for z<0.1) of galaxies covering all different", "activity types (e.g. Kauffmann et al. 2003MNRAS.346.1055K). For the", "definition of our multidimensional activity diagnostics we use the", "'galspec' data base of spectral-line measurements from the Max-Plank", "Institute for Astronomy and Johns Hopkins University group. We used", "the version of the catalogue made publicly available through the SDSS", "Data Release 8 (Aihara et al. 2011ApJS..193...29A,", "2011ApJS..195...26A; Eisenstein et al. 2011AJ....142...72E), which", "contains 1843200 objects.", "Since the same catalogue has been used for the definition of the", "two-dimensional and multidimensional diagnostics of Kauffmann et al.", "(2003MNRAS.346.1055K) and Vogt et al. (2014ApJ...793..127V),", "respectively, it is the best benchmark for testing the SoDDA. Before", "proceeding with our analysis, we applied the corrections on the", "line-measurement errors reported in Juneau et al.", "(2014ApJ...788...88J), and we corrected the flux of the H{beta} line", "following Groves, Brinchmann & Walcher (2012MNRAS.419.1402G).", "The final sample consists of 130799 galaxies, and it provides a direct", "comparison with the reference diagnostics of Kauffmann et al.", "(2003MNRAS.346.1055K) and Kewley et al. (2006MNRAS.372..961K), which", "have used very similar selection criteria."], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "14-Sep-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_1477"}} {"id": "J/MNRAS/485/1477", "title_cds": "Sample of face-on bulgeless galaxies", "title_create": "Karachentsev+, 2019", "year": "2019", "author": "Karachentsev I.D., Karachentseva V.E.", "title_pub": "A reference sample of face-on bulgeless galaxies.", "first_author": "Karachentsev I.D.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.1477K"], "keyword_cds": "Galaxies ; Magnitudes ; Radial velocities", "keyword_pub": "galaxies: bulges - galaxies: nuclei - galaxies: spiral", "abstract": ["We present a list of 220 face-on, almost bulgeless galaxies assumed to", "be counterparts to the objects from the Reference Flat Galaxy", "Catalogue (RFGC). We selected the Sc-, Scd-, and Sd-type galaxies", "according to their apparent axial ratio log(r_25_)<0.05 and major", "standard angular diameter log(d_25_)>0.90 as defined in HyperLEDA. The", "sample objects are restricted by the radial velocity V_LG_<10000km/s", "and a declination of above -30deg. The morphological composition of", "our sample is quite similar to that of RFGC. We notice the following", "common properties of face-on bulgeless galaxies. About half of them", "have bar-like structures occurring in the whole range of the absolute", "magnitudes of galaxies: from -17 to -22mag. An essential part of our", "sample (27-50 per cent) exhibit distorted spiral patterns. The", "galaxies do not show significant asymmetry in numbers of the 'S'- and", "'Z'-like spin orientation. The mean (pseudo-)bulge-to-total mass ratio", "for the sample is estimated as 0.11. Due to a negligible internal", "extinction, low-light background, and small projection effect, the", "face-on Sc-Sd discs are suitable objects to recognize their central", "nuclei as moderate-mass BH candidates. About 40-60 per cent of the", "galaxies have distinct unresolved nuclei, and their presence steeply", "depends on the luminosity of the host galaxy."], "description": ["Based on the data from Pan-STARRS1 (Chambers et al.", "2016arXiv161205560C), SDSS (Abazajian et al. 2009ApJS..182..543A),", "2MASS (Jarrett et al. 2000AJ....119.2498J), and HyperLEDA (Makarov et", "al. 2014A&A...570A..13M), we compiled a sample of face-on bulgeless", "galaxies. The sample includes 220 Sc-Scd-Sd galaxies distributed over", "the whole sky with the declinations >-30{deg}. The galaxies have the", "angular diameters d_25_>0.8arcmin, the typical inclination angle to", "the line of sight i~23{deg}, and the median radial velocity ~5000km/s.", "Table 1 presents the list of these Sc-Scd-Sd galaxies viewed at a", "slight angle. The list includes seven bright nearby galaxies: IC 342", "(3.28Mpc), NGC 5068 (5.15Mpc), M 101 (6.95Mpc), NGC 6946 (7.73Mpc),", "NGC 3344 (9.82Mpc), NGC 628 (10.19Mpc), and NGC 3184 (11.12Mpc), the", "distances to which are measured with an accuracy of ~5 per cent from", "the tip of the red giant branch, cepheids, or supernovae."], "data": "", "date_update": "15-Sep-2022", "tables": [{"name": "table1.dat", "desc": "Basic properties of the face-on bulgeless galaxies", "columns": [{"name": "Name", "desc": "Galaxy name in HyperLEDA "}, {"name": "Bmag", "desc": "Apparent integrated B magnitude from HyperLEDA with some refinements from"}, {"name": "and", "desc": " "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_1528"}} {"id": "J/MNRAS/485/1528", "title_cds": "Morphological study of galaxies in ZwCl0024+1652", "title_create": "Amado+, 2019", "year": "2019", "author": "Amado Z.B., Povic M., Sanchez-Portal M., Tessema S.B., Bongiovanni A., Cepa J., Cervino M., Gonzalez-Serrano J.I., Nadolny J., Perez Garcia A.M., Perez-Martinez R., Pintos-Castro I.", "title_pub": "A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z~0.4.", "first_author": "Amado Z.B.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.1528A"], "see_also": ["J/ApJ/591/53 : I photometry of Cl 0024+16 (Treu+, 2003)", "J/ApJ/634/977 : Redshifts in Cl 0024+16 members (Moran+, 2005)", "J/ApJ/671/1503 : Cl 0024+16 and MS 0451-03 spectrophotometry (Moran+, 2007)", "J/A+A/578/A30 : Emission-line galaxies in ZwCl0024.0+1652"], "keyword_cds": "Clusters, galaxy ; Galaxies ; Morphology ; Abundances", "keyword_pub": "ZwCl0024+1652 - galaxy cluster - galaxies - Morphology - Early-Type - Late-Type - Galsvm - Morphological fraction", "abstract": ["The well-known cluster of galaxies ZwCl0024+1652 at z~0.4 lacks an", "in-depth morphological classification of its central region. While", "previous studies provide a visual classification of a patched area, we", "used the public code called galaxy Support Vector Machine (GALSVM) and", "HST/ACS data as well as the WFP2 master catalogue to automatically", "classify all cluster members up to 1Mpc. GALVSM analyses galaxy", "morphologies through support vector machine (SVM). From the 231", "cluster galaxies, we classified 97 as early types (ETs) and 83 as late", "types (LTs). The remaining 51 stayed unclassified (or undecided). By", "cross-matching our results with the existing visual classification, we", "found an agreement of 81 per cent. In addition to previous Zwcl0024", "morphological classifications, 121 of our galaxies were classified for", "the first time in this work. In addition, we tested the location of", "classified galaxies on the standard morphological diagrams,", "colour-colour and colour-magnitude diagrams. Out of all cluster", "members, ~20 per cent are emission-line galaxies, taking into account", "previous GLACE results. We have verified that the ET fraction is", "slightly higher near the cluster core and decreases with the", "clustercentric distance, while the opposite trend has been observed", "for LT galaxies. We found a higher fraction of ETs (54 per cent) than", "LTs (46 per cent) throughout the analysed central region, as expected.", "In addition, we analysed the correlation between the five", "morphological parameters (Abraham concentration, Bershady-Concelice", "concentration, asymmetry, Gini, and M20 moment of light) and the", "clustercentric distance, without finding a clear trend. Finally, as a", "result of our work, the morphological catalogue of 231 galaxies", "containing all the measured parameters and the final classification is", "available in the electronic form of this paper."], "description": ["We used the public HST reduced scientific image of ZwCl0024+16521 from", "the observation made on 2004 November 16 with the ACS Wide Field", "Camera (WFC) using the F775W filter. The ACS/WFC has a pixel scale of", "0.05arcsec/pixel and field of view of 202x202arcsec^2^. The cluster is", "centred at RA=6.64433deg and Dec.=17.16211deg, and the used image", "covers the central part of the cluster of~1Mpc.", "To extract redshift information and to identify cluster members, we", "used the public ZwCl0024+1652 master catalogue", "(http://www.astro.caltech.edu/~smm/clusters/) described in Treu et al.", "(2003ApJ...591...53T, Cat. J/ApJ/591/53) and Moran et al.", "(2005ApJ...634..977M, J/ApJ/634/977). The catalogue consists of 73318", "sources, with photometric and/or spectroscopically confirmed redshifts", "available, and covering the area of 0.5x0.5deg^2^ up to the", "clustercentric distance of about 5Mpc. All observations were carried", "out with the Canada-France-Hawaii Telescope (CFHT) and its CFH12K wide", "field camera, and/or the HST Wide Field and Planetary Camera (WFP2),", "as described in Treu et al. (2003ApJ...591...53T, Cat. J/ApJ/591/53).", "Besides redshifts, this catalogue includes the visual morphological", "classification of sources brighter than I=22.5 (Moran et al.", "2005ApJ...634..977M, Cat. J/ApJ/634/977). We cross-matched this", "catalogue with our SExtractor catalogue (3515 sources) using a maximum", "radius of 2arcsec. This radius was selected after testing different", "ones from 1 to 5arcsec and finding it to be the best compromise", "between being the counterparts and having multiple matches. We", "obtained a total of 255 counterparts (hereafter cluster sample) with", "available redshifts."], "data": "", "date_update": "15-Sep-2022", "tables": [{"name": "tablea1.dat", "desc": "Morphological catalogue of galaxies in the ZwCl0024+1652 cluster", "columns": [{"name": "ID", "desc": "Galaxy index "}, {"name": "HST", "desc": "? HST identification number of the galaxy "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "ELLIP", "desc": "Ellipticity of the galaxy measured by SExtractor"}, {"name": "MUMEAN", "desc": "Surface brightness of the galaxy measured by SExtractor"}, {"name": "ASYM", "desc": "Asymmetry index measured by GALSVM (1) "}, {"name": "CABR", "desc": "Abraham concentration index measured by GALSVM (2)"}, {"name": "GINI", "desc": "GINI coefficient measured by GALSVM (3) "}, {"name": "M20", "desc": "M20 moment of light index measured by GALSVM (4)"}, {"name": "CCON", "desc": "Bershady-Concelice concentration index measured by GALSVM (5)"}, {"name": "F775Wmag", "desc": "MAG_AUTO (F775W) measured by SExtractor "}, {"name": "e_F775Wmag", "desc": "Error on F775Wmag "}, {"name": "z", "desc": "Redshift (6) "}, {"name": "r_z", "desc": "References for z (7) "}, {"name": "Dist", "desc": "Distance of the galaxy from the centre of the cluster (clustercentric distance)"}, {"name": "Prob", "desc": "Final probability of a galaxy to be early-type taking the uncertainity into account"}, {"name": "Class", "desc": "Final morphological class based on the probability value (Prob) (8)"}, {"name": "MType", "desc": "Visual morphology as given in Moran et al. (2007ApJ...671.1503M, Cat. J/ApJ/671/1503)"}, {"name": "ELGType", "desc": "Emission line galaxy (ELG) type adapted from Sanchez-Portal et al. (2015A&A...578A..30S,"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_2010"}} {"id": "J/MNRAS/485/2010", "title_cds": "Kinematics of the Tucana Dwarf Galaxy", "title_create": "Gregory+, 2019", "year": "2019", "author": "Gregory A.L., Collins M.L.M., Read J.I., Irwin M.J., Ibata R.A., Martin N.F., McConnachie A.W., Weisz D.R.", "title_pub": "Kinematics of the Tucana Dwarf Galaxy: an unusually dense dwarf in the Local Group.", "first_author": "Gregory A.L.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.2010G"], "keyword_cds": "Galaxies, optical ; Galaxies, photometry ; Galaxies, spectra", "keyword_pub": "galaxies: dwarf - galaxies: evolution - galaxies: haloes - galaxies: kinematics and dynamics - Local Group", "abstract": ["We present new FLAMES+GIRAFFE spectroscopy of 36 member stars in the", "isolated Local Group dwarf spheroidal galaxy Tucana. We measure a", "systemic velocity for the system of v_Tuc_=216.7^+2.9^_-2.8_km/s, and", "a velocity dispersion of {sigma}_v,Tuc_=14.4^+2.8^_-2.3_km/s. We also", "detect a rotation gradient of dv_r_/d{Chi}=7.6^+4.2^_-4.3_km/s/kpc,", "which reduces the systemic velocity to v_Tuc_=215.2^+2.8^_-2.7_km/s", "and the velocity dispersion to {sigma}_v,Tuc_=13.3^+2.7^_-2.3_km/s. We", "perform Jeans modelling of the density profile of Tucana, using the", "line-of-sight velocities of the member stars. We find that it favours", "a high central density consistent with 'pristine' subhaloes in", "{Lambda} cold dark matter, and a massive dark matter halo", "(~10^10^M_{sun}_) consistent with expectations from abundance", "matching. Tucana appears to be significantly more centrally dense than", "other isolated Local Group dwarfs, making it an ideal laboratory for", "testing dark matter models."], "description": ["Photometric data for Tucana was obtained using the Magellan/Megacam", "instrument on the Clay telescope at Las Campanas observatory on 2012", "November 14 as part of the Solo (Solitary Local Dwarfs) observing", "campaign (Higgs et al. 2016MNRAS.458.1678H). Magellan/Megacam is a 9x4", "array of pixel CCDs with a pixel scale 0.08arcsec/pixel. Two pointings", "were targeted, with three exposures were stacked in both the g and i", "bands for each field. Each g-band exposure was 150s for a total", "integration time of 450s. In the i band, the exposures were 300s each", "for a total integration time of 900s. Seeing ranged from 0.68 to", "0.90arcsec in the g band and 0.55 to 0.72 in the i band. The", "photometry was reduced using the Cambridge Astronomical Survey Unit", "(CASU), following the process described in Richardson et al.", "(2011ApJ...732...76R) and Higgs et al. (2016MNRAS.458.1678H).", "To obtain accurate spectroscopy of the faint stellar population of", "Tucana, the 8.2m VLT in Paranal, Chile was used. Observations were", "taken using the FLAMES+GIRAFFE spectrograph over six nights through", "2015 June, August, and September. GIRAFFE is a fibre-fed spectrograph", "for the visible range 3700-9000{AA}.", "The FLAMES+GIRAFFE spectrograph is a higher resolution instrument than", "FORS2 (which was used in Fraternali et al. (2009A&A...499..121F)", "(F09)), with a resolving power of R=6500 as opposed to R=3200. F09", "observe 23 stars to an S/N suitable for determining velocities, with", "20 of these identified as members. We observe a much larger number of", "stars out to a wider radius than F09, generating a larger catalogue of", "Tucana members and reducing the uncertainties in the results."], "data": "", "date_update": "12-Oct-2022", "tables": [{"name": "table2.dat", "desc": "Details of all successfully reduced targets observed with FLAMES+GIRAFFE", "columns": [{"name": "ID", "desc": "Object identifier "}, {"name": "HV", "desc": "Line-of-sight heliocentric velocity "}, {"name": "e_HV", "desc": "Error on HV "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "gmag", "desc": "g-band magnitude from Magellan/MegaCam imaging "}, {"name": "imag", "desc": "i-band magnitude from Magellan/MegaCam imaging "}, {"name": "SNR", "desc": "Signal to noise ratio "}, {"name": "Member", "desc": "Determination of Tucana membership "}, {"name": "OName", "desc": "? ID of counterpart in Fraternali et al. (2009A&A...499..121F) (F09) data set"}, {"name": "HVF09", "desc": "? Velocity of F09 counterpart (Fraternali et al. 2009A&A...499..121F)"}, {"name": "e_HVF09", "desc": "? Error on HVF09 "}]}, {"name": "table3.dat", "desc": "Details of the 36 identified members of Tucana observed with FLAMES+GIRAFFE", "columns": [{"name": "ID", "desc": "Object identifier "}, {"name": "HV", "desc": "Line-of-sight heliocentric velocity "}, {"name": "e_HV", "desc": "Error on HV "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Sep", "desc": "On-sky separation of the object from the central coordinates of Tucana (22 41 49.6,"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_2167"}} {"id": "J/MNRAS/485/2167", "title_cds": "M-type stars in LAMOST DR5 unclassified spectra", "title_create": "Guo+, 2019", "year": "2019", "author": "Guo Y.-X., Luo A.-L., Zhang S., Du B., Wang Y.-F., Chen J.-J., Zuo F., Kong X., Hou Y.-H.", "title_pub": "Recognition of M-type stars in the unclassified spectra of LAMOST DR5 using a hash-learning method.", "first_author": "Guo Y.-X.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.2167G"], "keyword_cds": "Spectroscopy ; Stars, M-type ; Stars, late-type", "keyword_pub": "techniques: spectroscopic - stars: late-type - stars: low-mass", "abstract": ["Our study aims to recognize M-type stars which are classified as", "'UNKNOWN' due to poor quality in the Large sky Area Multi-Object fiber", "Spectroscopic Telescope (LAMOST) DR5 V1. A binary nonlinear hashing", "algorithm based on Multi-Layer Pseudo-Inverse Learning (ML-PIL) is", "proposed to effectively learn spectral features for M-type-star", "detection, which can overcome the bad fitting problem of template", "matching, particularly for low S/N spectra. The key steps and the", "performance of the search scheme are presented. A positive data set is", "obtained by clustering the existing M-type spectra to train the ML-PIL", "networks. By employing this new method, we find 11410 M-type spectra", "out of 642178 'UNKNOWN' spectra, and provide a supplemental catalogue.", "Both the supplemental objects and released M-type stars in DR5 V1 are", "composed of a whole M-type sample, which will be released in the", "official DR5 to the public in June 2019. All the M-type stars in the", "data set are classified as giants and dwarfs by two suggested", "separators: (1) a colour diagram of H versus J-K from 2MASS, (2) line", "indices CaOH versus CaH1, and the separation is validated with the", "Hertzsprung-Russell diagram (HRD) derived from Gaia DR2. The magnetic", "activities and kinematics of M dwarfs are also provided with the", "equivalent width (EW) of the H{alpha} emission line and the", "astrometric data from Gaia DR2 respectively."], "description": ["LAMOST is a 4-m reflecting Schmidt telescope with a large field of", "view (FoV) of 5 degrees in diameter. It has 4000 fibres mounted on its", "focal plane and 16 spectrographs with 32 CCD cameras, so that it can", "simultaneously observe up to 4000 objects (Cui et al.", "2012RAA....12.1197C). The raw CCD data are reduced and analyzed by the", "LAMOST data pipelines, which consist of a 2D pipeline and a 1D", "pipeline. The primary functions of the 2D pipeline include bias", "calibration, flat-field correction, spectral extraction, sky", "subtraction, wavelength calibration, flux calibration, and", "sub-exposures combination. The calibrated spectra from the 2D pipeline", "are then fed to the 1D pipeline which performs spectral classification", "and parameter determination based on template matching and chi-square", "criteria (Luo et al. 2015RAA....15.1095L, Cat. V/146).", "By July 2017, LAMOST had completed its five-year regular survey. The", "LAMOST DR5 V1 includes 9017844 spectra of stars, galaxies, quasars,", "and unrecognized objects. These spectra cover the wavelength range", "from 3690 to 9100{AA} with a resolution of R~1800 at the wavelength", "5500{AA}.", "Among the 9 million spectra in LAMOST DR5 V1, 642178 unrecognized", "spectra were labelled 'UNKNOWN'. During the classification process of", "the 1D pipeline, a spectrum is classified as 'UNKNOWN' if the", "confidence of the classification result is lower than a given", "threshold value. In this study we build a multilayer Pseudo-Inverse", "Learning (ML-PIL) to fulfil the hash-learning process, so as to search", "M-type stars in the 'UNKNOWN' spectra of LAMOST DR5 V1."], "data": "", "date_update": "19-Sep-2022", "tables": [{"name": "catalog.dat", "desc": "Supplemental catalogue of 11410 recognized M-type stars", "columns": [{"name": "ID", "desc": "LAMOST object ID (JHHMMSS.ss+DDMMSS.s) "}, {"name": "ObsDate", "desc": "LAMOST Target observation date "}, {"name": "MJD", "desc": "Modified Julian Day "}, {"name": "PlanId", "desc": "LAMOST Plan Name "}, {"name": "specId", "desc": "LAMOST unique spectra ID "}, {"name": "FiberId", "desc": "LAMOST Fiber ID "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "SNR", "desc": "Signal to noise ratio of r filter "}, {"name": "subClass", "desc": "Stellar Sub-Class "}, {"name": "HRV", "desc": "Heliocentric radial velocity "}, {"name": "EWHa", "desc": "? Equivalent width of H{alpha} line "}, {"name": "e_EWHa", "desc": "? Error on EWHa "}, {"name": "TiO5", "desc": "? Spectral index of TiO5 "}, {"name": "CaH2", "desc": "? Spectral index of CaH2 "}, {"name": "CaH3", "desc": "? Spectral index of CaH3 "}, {"name": "TiO1", "desc": "? Spectral index of TiO1 "}, {"name": "TiO2", "desc": "? Spectral index of TiO2 "}, {"name": "TiO3", "desc": "? Spectral index of TiO3 "}, {"name": "TiO4", "desc": "? Spectral index of TiO4 "}, {"name": "CaH1", "desc": "? Spectral index of CaH1 "}, {"name": "CaOH", "desc": "? Spectral index of CaOH "}, {"name": "e_TiO5", "desc": "? Error on TiO5 "}, {"name": "e_CaH2", "desc": "? Error on CaH2 "}, {"name": "e_CaH3", "desc": "? Error on CaH3 "}, {"name": "e_TiO1", "desc": "? Error on TiO1 "}, {"name": "e_TiO2", "desc": "? Error on TiO2 "}, {"name": "e_TiO3", "desc": "? Error on TiO3 "}, {"name": "e_TiO4", "desc": "? Error on TiO4 "}, {"name": "e_CaH1", "desc": "? Error on CaH1 "}, {"name": "e_CaOH", "desc": "? Error on CaOH "}, {"name": "na", "desc": "? Line index of Na line "}, {"name": "zeta", "desc": "? Metal-sensitive parameter (Yi et al. 2014AJ....147...33Y;"}, {"name": "al.", "desc": "2015RAA....15.1182G, "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_2343"}} {"id": "J/MNRAS/485/2343", "title_cds": "Short Title", "title_create": "Papadogiannakis+, 2019", "year": "2019", "author": "Papadogiannakis S., Dhawan S., Morosin R., Goobar A.", "title_pub": "Characterizing the secondary maximum in the r-band for Type Ia supernovae: diagnostic for the ejecta mass.", "first_author": "Papadogiannakis S.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.2343P"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "19-Sep-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_2380"}} {"id": "J/MNRAS/485/2380", "title_cds": "Gaia-derived luminosities of Kepler A/F stars", "title_create": "Murphy+, 2019", "year": "2019", "author": "Murphy S.J., Hey D., Van Reeth T., Bedding T.R.", "title_pub": "Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the {delta} Scuti instability strip.", "first_author": "Murphy S.J.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.2380M"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)"], "keyword_cds": "Asteroseismology ; Parallaxes, trigonometric ; Stars, variable", "keyword_pub": "asteroseismology - parallaxes - Hertzsprung-Russell and colour-magnitude diagrams - stars: oscillations - stars: variables: {delta}Scuti", "abstract": ["We study the fraction of stars in and around the {delta}Scuti", "instability strip that are pulsating, using Gaia DR2 parallaxes to", "derive precise luminosities. We classify a sample of over 15000 Kepler", "A and F stars into {delta}Sct and non-{delta}Sct stars, paying close", "attention to variability that could have other origins. We find that", "18 per cent of the {delta}Sct stars have their dominant frequency", "above the Kepler long-cadence Nyquist frequency (periods<1h), and 30", "per cent have some super-Nyquist variability. We analyse the pulsator", "fraction as a function of effective temperature and luminosity,", "finding that many stars in the {delta}Sct instability strip do not", "pulsate. The pulsator fraction peaks at just over 70 per cent in the", "middle of the instability strip. The results are insensitive to the", "amplitude threshold used to identify the pulsators. We define a new", "empirical instability strip based on the observed pulsator fraction", "that is systematically hotter than theoretical strips currently in", "use. The stellar temperatures, luminosities, and pulsation", "classifications are provided in an online catalogue."], "description": ["We selected Kepler targets with temperatures between 6500 and 10000K,", "according to the 'input' temperatures in Mathur et al.", "(2017ApJS..229...30M, Cat. J/ApJS/229/30). This range covers the", "{delta}Sct instability strip and the region around it where {delta}Sct", "pulsators are observed.", "We made no selection based on logg or [Fe/H] values, which we also", "gathered from the input values of Mathur et al. (2017ApJS..229...30M,", "Cat. J/ApJS/229/30). We made no cut on Kepler magnitude, but we did", "cut stars with a luminosity 0.4dex (i.e. 1mag) fainter than the", "zero-age main-sequence (ZAMS) because we focus here on stars on the", "main-sequence and immediate post-main-sequence. We did not include", "stars for which there are no Kepler light curves available. The total", "sample size in our Teff range and after filtering by luminosity is", "15229.", "In DR2, stars with Gaia temperatures above 8000K had no available", "extinction values in the Gaia G band, A_G_, and thus no luminosities.", "It also appears that extinctions were not used in calculating the", "luminosities of stars where A_G_ was available (Andrae et al.", "2018A&A...616A...8A), hence the Gaia luminosities as provided in the", "DR2 catalogue are unreliable for our targets. We therefore calculated", "luminosities for all targets, taking from Gaia DR2 only stellar", "parallaxes, {pi}, and their uncertainties (Gaia Collaboration", "2018A&A...616A...1G, Cat. I/345). Most of our targets have precise", "parallaxes, with only 249 having fractional uncertainties above 0.2."], "data": "", "date_update": "21-Sep-2022", "tables": [{"name": "table1.dat", "desc": "Stellar data ", "columns": [{"name": "KIC", "desc": "KIC name (NNNNNNNN) "}, {"name": "GaiaDR2", "desc": "Gaia DR2 source name "}, {"name": "gmag", "desc": "g-band SDSS magnitude "}, {"name": "plx", "desc": "Parallax "}, {"name": "e_plx", "desc": "Error on plx "}, {"name": "Ag", "desc": "Computed extinctions in the g-band "}, {"name": "e_Ag", "desc": "Error on Ag "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "e_Teff", "desc": "Error on Teff "}, {"name": "[Fe/H]", "desc": "Iron to hydrogen abundance ratio "}, {"name": "e_[Fe/H]", "desc": "Error on [Fe/H] "}, {"name": "logg", "desc": "? Surface gravity "}, {"name": "e_logg", "desc": "? Error on logg "}, {"name": "Rad", "desc": "Star radius "}, {"name": "e_Rad", "desc": "Error on Rad "}, {"name": "Mstar", "desc": "Star mass "}, {"name": "e_Mstar", "desc": "Error on Mstar "}, {"name": "q_Mstar", "desc": "Quality flag on Mstar (1) "}, {"name": "logLbol", "desc": "Star luminosity (2) "}, {"name": "E_logLbol", "desc": "Upper error on logLbol "}, {"name": "e_logLbol", "desc": "Lower error on logLbol "}, {"name": "dSct", "desc": "Indicates if the star is a {delta}Sct (3) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_2562"}} {"id": "J/MNRAS/485/2562", "title_cds": "Eclipse timing variation of eclipsing binaries", "title_create": "Hajdu+, 2019", "year": "2019", "author": "Hajdu T., Borkovits T., Forgacs-dajka E., Sztakovics J., Marschalko G., Kutrovatz G.", "title_pub": "Eclipse timing variation analysis of OGLE-IV eclipsing binaries towards the Galactic Bulge - I. Hierarchical triple system candidates.", "first_author": "Hajdu T.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.2562H"], "see_also": ["J/AcA/66/405 : Galactic bulge eclipsing & ellipsoidal binaries"], "keyword_cds": "Stars, double and multiple ; Binaries, eclipsing", "keyword_pub": "methods: numerical - binaries: close - binaries: eclipsing", "abstract": ["We report a study of the eclipse timing variation (ETV) of short", "period (P1=<6d) eclipsing binaries (EBs) monitored during the", "photometric survey optical gravitational lensing experiment-IV. From", "the 425193 EBs, we selected approximately 80000 binaries that we found", "suitable for further examination. Among them, we identified 992", "potential hierarchical triple (or multiple) system candidates", "exhibiting light-travel time effect (LTTE). Besides, we obtained the", "orbital parameters of these systems and carried out statistical", "analyses on the properties of these candidates. We found that (i)", "there is a significant lack of triple systems where the outer period", "is less than 500d, (ii) the distribution of the outer eccentricities", "has a maximum around e_2_~0.3, and (iii) the outer mass ratio", "calculated from an estimated minimum mass of the third component is", "lower than q_2_~0.5 for the majority of the sample. We also present", "some systems that deserve special attention: (i) There are four", "candidates that show double periodic ETV, which we explain by the", "presence of a fourth companion; (ii) For two systems, the", "perturbations of the third component are also found to be significant", "therefore we give a combined dynamical and LTTE ETV solution; and", "(iii) For one system, the third component is found to be probably in", "the substellar mass domain."], "description": ["The OGLE-IV survey (Soszynski et al. 2016AcA....66..405S, Cat.", "J/AcA/66/405) provided around 425193 light curves of EBs that were", "observed in I and V bands. Since the I band light curves typically", "contain much more points than V band ones, we relied only on the", "former photometric band data for our analysis. Observations of the", "currently running project OGLE-IV are made at Las Campanas", "Observatory, Chile with the 1.3m Warsaw Telescope, which is currently", "equipped with a mosaic CCD camera.", "Our main goal was to find hierarchical triple stellar candidates whose", "outer period (P2) is shorter than, or comparable to, the length of the", "observations. Unfortunately, most of the data trains do not contain", "enough data points (more than the half of the cases contain less than", "1000 points) for a detailed examination. Therefore, we investigated", "only those systems whose light curves contain more than 4000 points.", "Applying this criterion, we reduced our sample from the original", "425193 EBs to ~80000 systems.", "Owing to the long-term observations, we were able to find 992 third", "body candidates. For the more reliable results, we selected 258", "systems where the period and the eccentricity were estimated with", "lower uncertainties (see Table 1).", "For four of them (OGLE-BLG-ECL-136469, OGLE-BLG-ECL-153291,", "OGLE-BLG-ECL-165849, and OGLE-BLG-ECL-259162), we came to the", "conclusion that their ETVs can be well modelled with a double LTTE", "solution rather than a simple hierarchical stellar system solution", "(see Table 4). However, since our model neglects dynamic effects, the", "resulting parameters are only indicative.", "We also found two systems with significant dynamical amplitudes", "(OGLE-BLG-ECL-143356 and OGLE-BLG-ECL-169255), described in Table 3."], "data": "", "date_update": "22-Sep-2022", "tables": [{"name": "table1.dat", "desc": "LTTE solutions for the 258 most certain hierarchical triple star candidates of the OGLE-IV sample", "columns": [{"name": "ID", "desc": "OGLE-BLG-ECL identifier (NNNNNN) "}, {"name": "T0", "desc": "Epoch (HJD-2450000d) "}, {"name": "P1", "desc": "Inner period "}, {"name": "P2", "desc": "Outer period "}, {"name": "e_P2", "desc": "Error on P2 "}, {"name": "asini2", "desc": "Projected semi-major axis of the light-time orbit"}, {"name": "e_asini2", "desc": "Error on asini2 "}, {"name": "e2", "desc": "Eccentricity "}, {"name": "e_e2", "desc": "Error on e2 "}, {"name": "omega2", "desc": "Argument of the periastron "}, {"name": "e_omega2", "desc": "Error on omega2 "}, {"name": "tau2", "desc": "Periastron passage time of the third companion "}, {"name": "e_tau2", "desc": "Error on tau2 "}, {"name": "fmC", "desc": "Mass function "}, {"name": "e_fmC", "desc": "Error on fmC "}, {"name": "DeltaP1", "desc": "? Parabolic term (1) "}, {"name": "e_DeltaP1", "desc": "? Error on DeltaP1 (1) "}]}, {"name": "table2.dat", "desc": "LTTE solutions for the remaining, less certain hierarchical triple star candidates of the OGLE-IV sample", "columns": [{"name": "ID", "desc": "OGLE-BLG-ECL identifier (NNNNNN) "}, {"name": "T0", "desc": "Epoch (HJD-2450000d) "}, {"name": "P1", "desc": "Inner period "}, {"name": "P2", "desc": "Outer period "}, {"name": "e_P2", "desc": "Error on P2 "}, {"name": "asini2", "desc": "Projected semi-major axis of the light-time orbit"}, {"name": "e_asini2", "desc": "Error on asini2 "}, {"name": "e2", "desc": "Eccentricity "}, {"name": "e_e2", "desc": "Error on e2 "}, {"name": "omega2", "desc": "Argument of the periastron "}, {"name": "e_omega2", "desc": "Error on omega2 "}, {"name": "tau2", "desc": "Periastron passage time of the third companion "}, {"name": "e_tau2", "desc": "Error on tau2 "}, {"name": "fmC", "desc": "Mass function "}, {"name": "e_fmC", "desc": "Error on fmC "}, {"name": "DeltaP1", "desc": "? Parabolic term (1) "}, {"name": "e_DeltaP1", "desc": "? Error on DeltaP1 (1) "}]}, {"name": "table3.dat", "desc": "Orbital elements from combined dynamical and LTTE solutions", "columns": [{"name": "ID", "desc": "OGLE-BLG-ECL identifier (NNNNNN) "}, {"name": "T0", "desc": "Epoch (HJD-2450000d) "}, {"name": "P1", "desc": "Inner period "}, {"name": "P2", "desc": "Outer period "}, {"name": "e_P2", "desc": "Error on P2 "}, {"name": "asini2", "desc": "Projected semi-major axis of the light-time orbit"}, {"name": "e_asini2", "desc": "Error on asini2 "}, {"name": "e2", "desc": "Eccentricity "}, {"name": "e_e2", "desc": "Error on e2 "}, {"name": "omega2", "desc": "Argument of the periastron "}, {"name": "e_omega2", "desc": "Error on omega2 "}, {"name": "tau2", "desc": "Periastron passage time of the third companion"}, {"name": "e_tau2", "desc": "Error on tau2 "}, {"name": "ALTTE", "desc": "Light-travel time effect (LTTE) amplitude "}, {"name": "e_ALTTE", "desc": "Error on ALTTE "}, {"name": "Adyn", "desc": "Amplitude-like quantity of the dynamical eclipse timing variation (ETV) component"}, {"name": "Adyn/ALTTE", "desc": "Adyn to ALTTE ratio "}, {"name": "fmC", "desc": "Mass function "}, {"name": "e_fmC", "desc": "Error on fmC "}, {"name": "mC/mABC", "desc": "mC to mABC ratio "}, {"name": "e_mC/mABC", "desc": "Error on mC/mABC "}, {"name": "mAB", "desc": "Total mass of the inner binary "}, {"name": "e_mAB", "desc": "Error on mAB "}, {"name": "mC", "desc": "Mass of the third component "}, {"name": "e_mC", "desc": "Error on mC "}]}, {"name": "table4.dat", "desc": "Results of double LTTE solution fit ", "columns": [{"name": "ID", "desc": "OGLE-BLG-ECL identifier (NNNNNN) "}, {"name": "T0", "desc": "Epoch (HJD-2450000d) "}, {"name": "P1", "desc": "Inner period "}, {"name": "P2", "desc": "Outer period of the first light-travel time effect (LTTE)"}, {"name": "e_P2", "desc": "Error on P2 "}, {"name": "asini2", "desc": "Projected semi-major axis of the light-time or bit associated to the first LTTE"}, {"name": "e_asini2", "desc": "Error on asini2 "}, {"name": "e2", "desc": "Eccentricity associated to the first LTTE "}, {"name": "e_e2", "desc": "Error on e2 "}, {"name": "omega2", "desc": "Argument of the periastron associated to the first LTTE"}, {"name": "e_omega2", "desc": "Error on omega2 "}, {"name": "tau2", "desc": "Periastron passage time of the third companion associated to the first LTTE"}, {"name": "e_tau2", "desc": "Error on tau2 "}, {"name": "fmC", "desc": "Mass function associated to the first LTTE "}, {"name": "e_fmC", "desc": "Error on fmC "}, {"name": "P3", "desc": "Outer period of the second light-travel time effect (LTTE)"}, {"name": "e_P3", "desc": "Error on P3 "}, {"name": "asini3", "desc": "Projected semi-major axis of the light-time or bit associated to the first LTTE"}, {"name": "e_asini3", "desc": "Error on asini3 "}, {"name": "e3", "desc": "Eccentricity associated to the first LTTE "}, {"name": "e_e3", "desc": "Error on e3 "}, {"name": "omega3", "desc": "Argument of the periastron associated to the first LTTE"}, {"name": "e_omega3", "desc": "Error on omega3 "}, {"name": "tau3", "desc": "Periastron passage time of the third companion associated to the first LTTE"}, {"name": "e_tau3", "desc": "Error on tau3 "}, {"name": "fmD", "desc": "Mass function associated to the first LTTE "}, {"name": "e_fmD", "desc": "Error on fmD "}]}, {"name": "table5.dat", "desc": "The seven systems where the third component has higher mass than the EB", "columns": [{"name": "ID", "desc": "OGLE-BLG-ECL identifier (NNNNNN) "}, {"name": "P1", "desc": "Inner period "}, {"name": "P2", "desc": "Outer period "}, {"name": "e_P2", "desc": "Error on P2 "}, {"name": "fmC", "desc": "Mass function "}, {"name": "e_fmC", "desc": "Error on fmC "}, {"name": "mC", "desc": "Mass of the third component "}, {"name": "e_mC", "desc": "Error on mC "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_2710"}} {"id": "J/MNRAS/485/2710", "title_cds": "Radio jets associated with galactic outflows", "title_create": "Jarvis+, 2019", "year": "2019", "author": "Jarvis M.E., Harrison C.M., Thomson A.P., Circosta C., Mainieri V., Alexander D.M., Edge A.C., Lansbury G.B., Molyneux S.J., Mullaney J.R.", "title_pub": "Prevalence of radio jets associated with galactic outflows and feedback from quasars.", "first_author": "Jarvis M.E.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.2710J"], "see_also": ["VIII/92 : The FIRST Survey Catalog, Version 2014Dec17 (Helfand+ 2015)"], "keyword_cds": "Galaxies, radio ; Active gal. nuclei ; QSOs ; Radio sources", "keyword_pub": "galaxy: evolution - galaxies: active - galaxies: jets - quasars: general", "abstract": ["We present 1-7GHz high-resolution radio imaging (VLA and e-MERLIN) and", "spatially resolved ionized gas kinematics for 10 z<0.2 type 2", "'obscured' quasars (log[L_AGN_/erg.s^-1^]>~45) with moderate radio", "luminosities (log[L1.4GHz/W.Hz^-1^]=23.3-24.4). These targets were", "selected to have known ionized outflows based on broad [OIII]", "emission-line components (full width at half-maximum~800-1800km/s).", "Although 'radio-quiet' and not 'radio AGN' by many traditional", "criteria, we show that for nine of the targets, star formation likely", "accounts for ~<10 per cent of the radio emission. We find that ~80-90", "per cent of these nine targets exhibit extended radio structures on", "1-25kpc scales. The quasars' radio morphologies, spectral indices, and", "position on the radio size-luminosity relationship reveals that these", "sources are consistent with being low power compact radio galaxies.", "Therefore, we favour radio jets as dominating the radio emission in", "the majority of these quasars. The radio jets we observe are", "associated with morphologically and kinematically distinct features in", "the ionized gas, such as increased turbulence and outflowing bubbles,", "revealing jet-gas interaction on galactic scales. Importantly, such", "conclusions could not have been drawn from current low-resolution", "radio surveys such as FIRST. Our observations support a scenario where", "compact radio jets, with modest radio luminosities, are a crucial", "feedback mechanism for massive galaxies during a quasar phase."], "description": ["In this work, we focus on 10 type 2 ('obscured') z<0.2AGN, which have", "quasar-like luminosities (i.e. L[OIII]>10^42^erg/s; Reyes et al.", "2008AJ....136.2373R, Cat. J/AJ/136/2373). These were originally", "selected by Harrison et al. (2014MNRAS.441.3306H) from our parent", "sample of 24264 z<0.4 spectroscopically identified AGN presented in", "Mullaney et al. (2013MNRAS.433..622M).", "We observed with VLA under two proposals: programme 13B-127, with", "observations carried out on 2013 December 1-2014 May 13 and programme", "16A-182 with observations carried out on 2016 May 30-2017 January 20.", "For 13B-127, we observed nine targets, from our primary sample of 10,", "in four configuration-frequency combinations: (1) A-array in L band", "(1-2GHz; ~1.3arcsec resolution); (2) A-array in C band (4-8GHz;", "~0.3arcsec resolution); (3) B-array in L band (1-2GHz; ~4.3arcsec", "resolution), and (4) B-array in C band (4-8GHz; ~1.0arcsec", "resolution). The final target in our primary sample (J1338+1503) was", "observed by VLA during our 16A-182 project. Due to incomplete", "observations, this was only observed in one configuration-frequency", "combination: B-array in the C band (i.e. 4-8GHz; ~1.0arcsec", "resolution).We also gathered archival data from the UV to FIR to", "derive the stellar masses.", "The positions, redshifts, [OIII] properties, and radio properties", "(from the FIRST Survey; Becker, White & Helfand 1995ApJ...450..559B,", "Cat. VIII/92) of the 10 targets studied in this paper are presented in", "Table 1. We use SED fitting from the UV to FIR to isolate the FIR", "luminosity associated with star formation (LIR, SF) in addition to", "getting stellar masses and AGN bolometric luminosities (LAGN) (see", "Table 2). The final flux densities (or 5{sigma} upper limits) and", "their 1{sigma} uncertainties at 1.5, 5.2, and 7.2GHz are presented in", "Table 4."], "data": "", "date_update": "12-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Target list and basic properties ", "columns": [{"name": "Name", "desc": "Object name "}, {"name": "RAh", "desc": "Right ascension (J2000) (1) "}, {"name": "RAm", "desc": "Right ascension (J2000) (1) "}, {"name": "RAs", "desc": "Right ascension (J2000) (1) "}, {"name": "DE-", "desc": "Declination sign (J2000) (1) "}, {"name": "DEd", "desc": "Declination (J2000) (1) "}, {"name": "DEm", "desc": "Declination (J2000) (1) "}, {"name": "DEs", "desc": "Declination (J2000) (1) "}, {"name": "z", "desc": "Systemic redshifts from the GMOS data "}, {"name": "logLOIII", "desc": "Total observed [OIII] {lambda}5007 luminosity from Mullaney et al."}]}, {"name": "table2.dat", "desc": "Galaxy and AGN parameters derived from SED fitting for the primary sample", "columns": [{"name": "Name", "desc": "Object name "}, {"name": "f_Name", "desc": "Flag on name (1) "}, {"name": "logLAGN", "desc": "Bolometric AGN luminosity "}, {"name": "logMsun", "desc": "? Stellar mass "}, {"name": "E_logMsun", "desc": "? Upper error on logMsun "}, {"name": "e_logMsun", "desc": "? Lower error on logMsun "}, {"name": "f_logMsun", "desc": "Flag on logMsun (2) "}, {"name": "logLIR", "desc": "Infrared luminosity from star formation in the range 8-1000{mu}m"}, {"name": "E_logLIR", "desc": "Upper error on logLIR "}, {"name": "e_logLIR", "desc": "Lower error on logLIR "}, {"name": "SFR", "desc": "Star formation rate "}, {"name": "e_SFR", "desc": "Error on SFR "}, {"name": "S1.4", "desc": "1.4GHz flux predicted from star formation following the radio-LIR relation"}]}, {"name": "table4.dat", "desc": "Radio properties of the morphological structures extracted from resolution matched e-MERLIN and VLA images", "columns": [{"name": "Name", "desc": "Object name "}, {"name": "SFIRST", "desc": "Flux density from the FIRST survey "}, {"name": "e_SFIRST", "desc": "Error on SFIRST "}, {"name": "Struc", "desc": "Name of structure "}, {"name": "f_Struc", "desc": "Flag on structure (1) "}, {"name": "Interp", "desc": "Interpretation of structure or largest linear size observed at that resolution in kpc"}, {"name": "f_Interp", "desc": "Flag on Interp (2) "}, {"name": "l_S1.5", "desc": "Limit flag on S1.5 "}, {"name": "S1.5", "desc": "? Flux density in at 1.5GHz (3) "}, {"name": "e_S1.5", "desc": "? Error on S1.5 (4) "}, {"name": "l_S5.2", "desc": "Limit flag on S5.2 "}, {"name": "S5.2", "desc": "Flux density in at 5.2GHz (3) "}, {"name": "e_S5.2", "desc": "? Error on S5.2 (4) "}, {"name": "l_S7.2", "desc": "Limit flag on S7.2 "}, {"name": "S7.2", "desc": "Flux density in at 7.2GHz (3) "}, {"name": "e_S7.2", "desc": "? Error on S7.2 (4) "}, {"name": "alpha", "desc": "? Spectral index (5) "}, {"name": "e_alpha", "desc": "? Error on alpha "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_2825"}} {"id": "J/MNRAS/485/2825", "title_cds": "Filaments hosting Planck Galactic cold clumps", "title_create": "Alina+, 2019", "year": "2019", "author": "Alina D., Ristorcelli I., Montier L., Abdikamalov E., Juvela M., Ferriere K., Bernard J.-P., Micelotta E.R.", "title_pub": "Statistical analysis of the interplay between interstellar magnetic fields and filaments hosting Planck Galactic cold clumps.", "first_author": "Alina D.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.2825A"], "keyword_cds": "Polarization ; Interstellar medium ; Extinction", "keyword_pub": "polarization - methods: statistical - (ISM:) dust, extinction", "abstract": ["We present a statistical study of the relative orientation in the", "plane of the sky between interstellar magnetic fields and filaments", "hosting cold clumps. For the first time, we consider both the density", "of the environment and the density contrast between the filaments and", "their environment. Moreover, we geometrically distinguish between the", "clumps and the remaining portions of the filaments. We infer the", "magnetic field orientations in the filaments and in their environment", "from the Stokes parameters, assuming optically thin conditions. Thus,", "we analyse the relative orientations between filaments, embedded", "clumps, internal and background magnetic fields, depending on their", "environment and evolutionary stages. We recover the previously", "observed trend for filaments in low column density environments to be", "aligned parallel to the background magnetic field; however, we find", "that this trend is significant only for low-contrast filaments,", "whereas high-contrast filaments tend to be randomly orientated with", "respect to the background magnetic field. Filaments in high column", "density environments do not globally show any preferential", "orientation, although low-contrast filaments alone tend to have", "perpendicular relative orientation with respect to the background", "magnetic field. For a subsample of nearby filaments, for which volume", "densities can be derived, we find a clear transition in the relative", "orientation with increasing density, at n_H_~10^3^cm^-3^, changing", "from mostly parallel to mostly perpendicular in the off-clump portions", "of filaments and from even to bimodal in clumps. Our results confirm a", "strong interplay between interstellar magnetic fields and filaments", "during their formation and evolution."], "description": ["In our analysis, we use the Planck 353GHz full mission data, which is", "a part of the Planck Product 2015 release.", "The Planck all-sky Galactic cold clump catalogue (Planck Collaboration", "XXVIII 2016A&A...594A..28P, Cat. J/A+A/594/A28) contains 13188 sources", "detected using a dedicated method (Montier et al. 2010A&A...522A..83M;", "Planck Collaboration XXIII 2011A&A...536A..23P). The method consists", "of a colour-based detection of the excess emission in the cold", "residual maps after subtraction of the warm component traced by IRAS", "100{mu}m observations. Clumps were fitted using elliptical Gaussian", "functions, and the catalogue contains the resulting semimajor and", "semiminor axes and the position angles of the ellipses. With the", "exception of some sources in the Large Magellanic Cloud and in the", "Small Magellanic Cloud, the catalogue excludes extragalactic sources", "(Planck Collaboration XXVIII 2016A&A...594A..28P, Cat. J/A+A/594/A28)", "and contains nearby cores, clumps, and distant molecular clouds. This", "makes the catalogue particularly useful in studies related to the", "early stages of star formation.", "Several methods exist to detect filamentary structures (Sousbie", "2011MNRAS.414..350S; Soler et al. 2013ApJ...774..128S; Planck", "Collaboration XI 2014A&A...571A..11P). Among those, we opted for the", "SupRHT method, which is an improved version of the Rolling Hough", "Transform proposed by Clark, Peek & Putman (2014ApJ...789...82C).", "After applying some selection criteria, we detected 137 linear", "filaments."], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "23-Sep-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_3457"}} {"id": "J/MNRAS/485/3457", "title_cds": "Rotational modulation in TESS B stars", "title_create": "Balona+, 2019", "year": "2019", "author": "Balona L.A., Handler G., Chowdhury S., Ozuyar D., Engelbrecht C.A., Mirouh G.M., Wade G.A., David-Uraz A., Cantiello M.", "title_pub": "Rotational modulation in TESS B stars.", "first_author": "Balona L.A.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.3457B"], "see_also": ["J/AJ/156/102 : The TESS Input Catalog and Candidate Target List", "V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)", "IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)"], "keyword_cds": "Stars, early-type ; Stars, B-type ; Stars, variable ; Rotational velocities ; Effective temperatures", "keyword_pub": "stars: early-type - stars: oscillations - stars: rotation", "abstract": ["Light curves and periodograms of 160 B stars observed by the", "Transiting Exoplanet Survey Satellite (TESS) space mission and 29", "main-sequence B stars from Kepler and K2 were used to classify the", "variability type. There are 114 main-sequence B stars in the TESS", "sample, of which 45 are classified as possible rotational variables.", "This confirms previous findings that a large fraction (about 40 per", "cent) of A and B stars may exhibit rotational modulation. Gaia DR2", "parallaxes were used to estimate luminosities, from which the radii", "and equatorial rotational velocities can be deduced. It is shown that", "observed values of the projected rotational velocities are lower than", "the estimated equatorial velocities for nearly all the stars, as they", "should be if rotation is the cause of the light variation. We conclude", "that a large fraction of main-sequence B stars appear to contain", "surface features which cannot likely be attributed to abundance", "patches."], "description": ["TESS observes the sky in sectors measuring 24{deg}x96{deg} that extend", "from near the ecliptic equator to beyond the ecliptic pole. Each", "sector is observed for two orbits of the satellite around the Earth,", "or about 27d.", "The data analysed in this paper are from the light curves of the first", "release (Sectors 1 and 2). Most of the stars discussed here are at", "mid-latitudes and have been observed for a time span of about 55d. A", "description of how these data products were generated is found in", "Jenkins et al. (2016SPIE.9913E..3EJ).", "The TESS input catalogue (Stassun et al. 2018AJ....156..102S, Cat.", "J/AJ/156/102) lists stellar parameters for stars observed by TESS. The", "effective temperatures, Teff, for stars without spectroscopic", "determinations were obtained from near-infrared photometry, which is", "not reliable for B stars, particularly since reddening is important in", "many cases. The stars observed by TESS were matched with the SIMBAD", "astronomical data base (Wenger et al. 2000A&AS..143....9W) and only", "those known to be B stars were selected, giving a total of 160 stars", "with spectral types earlier than A0 (see Table 1).", "In addition to the TESS stars, we have examined the light curves of", "Kepler (Kepler Mission Team, 2009yCat.5133....0K, Cat. V/133) and K2", "(Huber et al. 2017yCat.4034....0H, Cat. IV/34) data for possible", "rotational modulation. The Kepler data have a time span of nearly 4yr", "which results in a very low periodogram noise level. The K2 data have", "a time span of around 80d. Table 3 lists the measurements and stellar", "parameters obtained for Kepler and K2 light curves."], "data": "", "date_update": "23-Sep-2022", "tables": [{"name": "table1.dat", "desc": "List of B stars observed by TESS ", "columns": [{"name": "Name", "desc": "TIC star name (NNNNNNNNN) "}, {"name": "OName", "desc": "Other name "}, {"name": "VarType", "desc": "Assigned variability type (GCVS type in parenthesis from Samus et al."}]}, {"name": "table3.dat", "desc": "Additional rotational variables identified from the light curves of the Kepler and K2 missions", "columns": [{"name": "Name", "desc": "Star name from KIC/EPIC "}, {"name": "OName", "desc": "Other name "}, {"name": "VarType", "desc": "Assigned variability type (GCVS type in parenthesis from Samus et al. 2017ARep...61...80S, Cat. B/gcvs)"}, {"name": "Vmag", "desc": "Apparent V magnitude "}, {"name": "nurot", "desc": "Presumed rotational frequency (in cycles/d) "}, {"name": "Arot", "desc": "Amplitude of the periodogram peak "}, {"name": "S/N", "desc": "Signal to noise ratio of the periodogram peak "}, {"name": "NH", "desc": "Number of visible harmonics "}, {"name": "ve", "desc": "Derived equatorial rotational velocity (G1) "}, {"name": "vsini", "desc": "Projected rotational velocity from the literature"}, {"name": "Teff", "desc": "Adopted effective temperature "}, {"name": "r_Teff", "desc": "Reference for Teff (G2) "}, {"name": "logLstar", "desc": "Stellar luminosity obtained from the Gaia parallax (Gaia Collaboration 2018A&A...616A...1G, Cat. I/345)"}, {"name": "SpType", "desc": "Spectral type ((Be) indicates classical Be star)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_3623"}} {"id": "J/MNRAS/485/3623", "title_cds": "Red giants abundance analysis in open clusters", "title_create": "Reddy+, 2019", "year": "2019", "author": "Reddy A.B.S., Lambert D.L.", "title_pub": "Comprehensive abundance analysis of red giants in the open clusters Stock 2, NGC 2168, 6475, 6991, and 7762.", "first_author": "Reddy A.B.S.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.3623R"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)"], "keyword_cds": "Abundances ; Clusters, open ; Spectra, optical ; Effective temperatures ; Positional data", "keyword_pub": "stars: abundances - Galaxy: abundances - Galaxy: disc - Galaxy: kinematics and dynamics - open clusters and associations: general - open clusters and associations: individual: Stock 2, NGC 2168, NGC 6475, NGC 6991 and NGC 7762", "abstract": ["We have analysed high-dispersion Echelle spectra (R=60000) of red", "giant members of five open clusters to derive abundances for many", "elements from Na to Eu. The [Fe/H] values are -0.06+/-0.03 for Stock", "2, -0.11+/-0.03 for NGC 2168, -0.01+/-0.03 for NGC 6475, 0.00+/-0.03", "for NGC 6991, and -0.07+/-0.03 for NGC 7662. Sodium is enriched in the", "giants relative to the abundance expected of main-sequence stars of", "the same metallicity. This enrichment of [Na/Fe] by about +0.25", "attributed to the first dredge-up is discussed in the light of", "theoretical predictions and recently published abundance", "determinations. Abundance ratios [El/Fe] for other elements are with", "very few exceptions equal to those of field giants and dwarfs, i.e.", "[El/Fe]~0.00 for [Fe/H]~0.0. An exception is the overabundance of La,", "Ce, Nd, and Sm in NGC 6991 but this is consistent with our previous", "demonstration that the abundances of these s-process products vary by", "about +/-0.2 among clusters of the same [Fe/H], a variation found also", "among field giants and dwarfs."], "description": ["Selection of red giants for subsequent spectroscopic observations was", "made by identifying stars having common proper motions at the putative", "red giant clump in the cluster colour-magnitude diagram (CMD). The", "CMDs were created from the available BV and Gaia DR2 photometric", "magnitudes.", "High-resolution and high signal-to-noise (S/N) ratio optical spectra", "of 18 giant stars in six OCs, namely Stock 2 (3 giants), NGC 2168 (3", "giants), NGC 6475 (3 giants), NGC 6991 (4 giants), and NGC 7762 (3", "giants) were observed in 2016 September, October, and November with", "the Robert G. Tull coude cross-dispersed Echelle spectrograph (Tull et", "al. 1995PASP..107..251T) at the 2.7-m Harlan J. Smith Telescope of the", "McDonald Observatory. On all occasions we employed the camera with a", "2048x2048 24{mu}m pixel CCD detector and 52.67 grooves/mm Echelle", "grating with exposures centred at 5060{AA} in order 69. We secured two", "to four exposures of cluster giants in our target list (Table 1) with", "each exposure limited to 20-30min to minimize the influence of cosmic", "rays and to acquire a global S/N of above 100."], "data": "", "date_update": "27-Sep-2022", "tables": [{"name": "table1.dat", "desc": "The journal of the observations for the cluster members", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "Star", "desc": "Star ID "}, {"name": "f_Star", "desc": "? Flag on Star (1) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Vmag", "desc": "? V magnitude "}, {"name": "B-V", "desc": "? B-V colour index "}, {"name": "V-Ks", "desc": "? V-Ks colour index "}, {"name": "J-Ks", "desc": "? J-Ks colour index "}, {"name": "RV", "desc": "Radial heliocentric velocity "}, {"name": "e_RV", "desc": "Error on RV "}, {"name": "S/N", "desc": "Signal to noise ratio "}, {"name": "Date", "desc": "Observation date "}, {"name": "Exp", "desc": "Exposure time "}]}, {"name": "table2.dat", "desc": "Photometric and spectroscopic atmospheric parameters for open cluster members analysed in this study", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "Star", "desc": "Star ID "}, {"name": "f_Star", "desc": "? Flag on Star (1) "}, {"name": "TeffBV", "desc": "? Effective temperature deduced from B-V (2) "}, {"name": "TeffVK", "desc": "? Effective temperature deduced from V-K (2) "}, {"name": "TeffJK", "desc": "? Effective temperature deduced from J-K (2) "}, {"name": "loggph", "desc": "? Photometric estimate of surface gravity (3) "}, {"name": "Teffsp", "desc": "? Spectroscopic effective temperature "}, {"name": "loggsp", "desc": "? Spectroscopic surface gravity "}, {"name": "vturbsp", "desc": "? Microturbulence velocity "}, {"name": "logLph", "desc": "? log of photometric stellar luminosity "}, {"name": "logLsp", "desc": "? log of spectroscopic stellar luminosity "}]}, {"name": "table3.dat", "desc": "Elemental abundance ratios [El/Fe] for elements from Na to Eu for Stock 2, NGC 2168, 6475, 6991, and 7762 from this study", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "[NaI/Fe]", "desc": "NaI to iron abundance ratio "}, {"name": "e_[NaI/Fe]", "desc": "Error on [NaI/Fe] "}, {"name": "[MgI/Fe]", "desc": "MgI to iron abundance ratio "}, {"name": "e_[MgI/Fe]", "desc": "Error on [MgI/Fe] "}, {"name": "[AlI/Fe]", "desc": "AlI to iron abundance ratio "}, {"name": "e_[AlI/Fe]", "desc": "Error on [AlI/Fe] "}, {"name": "[SiI/Fe]", "desc": "SiI to iron abundance ratio "}, {"name": "e_[SiI/Fe]", "desc": "Error on [SiI/Fe] "}, {"name": "[CaI/Fe]", "desc": "CaI to iron abundance ratio "}, {"name": "e_[CaI/Fe]", "desc": "Error on [CaI/Fe] "}, {"name": "[ScI/Fe]", "desc": "? ScI to iron abundance ratio "}, {"name": "e_[ScI/Fe]", "desc": "? Error on [ScI/Fe] "}, {"name": "[ScII/Fe]", "desc": "ScII to iron abundance ratio "}, {"name": "e_[ScII/Fe]", "desc": "Error on [ScII/Fe] "}, {"name": "[ScII/Fe]s", "desc": "ScII to iron abundance ratio calculated by synthesis"}, {"name": "e_[ScII/Fe]s", "desc": "Error on [ScII/Fe]s "}, {"name": "[TiI/Fe]", "desc": "TiI to iron abundance ratio "}, {"name": "e_[TiI/Fe]", "desc": "Error on [TiI/Fe] "}, {"name": "[TiII/Fe]", "desc": "TiII to iron abundance ratio "}, {"name": "e_[TiII/Fe]", "desc": "Error on [TiII/Fe] "}, {"name": "[VI/Fe]", "desc": "VI to iron abundance ratio "}, {"name": "e_[VI/Fe]", "desc": "Error on [VI/Fe] "}, {"name": "[CrI/Fe]", "desc": "CrI to iron abundance ratio "}, {"name": "e_[CrI/Fe]", "desc": "Error on [CrI/Fe] "}, {"name": "[CrII/Fe]", "desc": "CrII to iron abundance ratio "}, {"name": "e_[CrII/Fe]", "desc": "Error on [CrII/Fe] "}, {"name": "[MnI/Fe]", "desc": "MnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[MnI/Fe]", "desc": "Error on [MnI/Fe] "}, {"name": "[FeI/H]", "desc": "FeI to hydrogen abundance ratio "}, {"name": "e_[FeI/H]", "desc": "Error on [FeI/H] "}, {"name": "[FeII/H]", "desc": "FeII to hydrogen abundance ratio "}, {"name": "e_[FeII/H]", "desc": "Error on [FeII/H] "}, {"name": "[CoI/Fe]", "desc": "CoI to iron abundance ratio "}, {"name": "e_[CoI/Fe]", "desc": "Error on [CoI/Fe] "}, {"name": "[NiI/Fe]", "desc": "NiI to iron abundance ratio "}, {"name": "e_[NiI/Fe]", "desc": "Error on [NiI/Fe] "}, {"name": "[CuI/Fe]", "desc": "CuI to iron abundance ratio calculated by synthesis"}, {"name": "e_[CuI/Fe]", "desc": "Error on [CuI/Fe] "}, {"name": "[ZnI/Fe]", "desc": "ZnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[ZnI/Fe]", "desc": "Error on [ZnI/Fe] "}, {"name": "[YII/Fe]", "desc": "YII to iron abundance ratio "}, {"name": "e_[YII/Fe]", "desc": "Error on [YII/Fe] "}, {"name": "[ZrI/Fe]", "desc": "ZrI to iron abundance ratio "}, {"name": "e_[ZrI/Fe]", "desc": "Error on [ZrI/Fe] "}, {"name": "[ZrII/Fe]", "desc": "ZrII to iron abundance ratio "}, {"name": "e_[ZrII/Fe]", "desc": "Error on [ZrII/Fe] "}, {"name": "[BaII/Fe]", "desc": "BaII to iron abundance ratio calculated by synthesis"}, {"name": "e_[BaII/Fe]", "desc": "Error on [BaII/Fe] "}, {"name": "[LaII/Fe]", "desc": "LaII to iron abundance ratio "}, {"name": "e_[LaII/Fe]", "desc": "Error on [LaII/Fe] "}, {"name": "[CeII/Fe]", "desc": "CeII to iron abundance ratio "}, {"name": "e_[CeII/Fe]", "desc": "Error on [CeII/Fe] "}, {"name": "[NdII/Fe]", "desc": "NdII to iron abundance ratio "}, {"name": "e_[NdII/Fe]", "desc": "Error on [NdII/Fe] "}, {"name": "[SmII/Fe]", "desc": "SmII to iron abundance ratio "}, {"name": "e_[SmII/Fe]", "desc": "Error on [SmII/Fe] "}, {"name": "[EuII/Fe]", "desc": "EuII to iron abundance ratio calculated by synthesis"}, {"name": "e_[EuII/Fe]", "desc": "Error on [EuII/Fe] "}]}, {"name": "table4.dat", "desc": "Cluster fundamental parameters derived in this study using the BV and Gaia-based CMDs", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "[Fe/H]", "desc": "Iron to hydrogen abundance ratio "}, {"name": "E(B-V)", "desc": "Reddening "}, {"name": "DMV", "desc": "Distance modulus V-Mv "}, {"name": "AgeBV", "desc": "Age using (V,B-V) colour-magnitude diagram "}, {"name": "dBV", "desc": "Distance using (V,B-V) colour-magnitude diagram"}, {"name": "E(BP-RP)", "desc": "Reddening using Gaia DR2 BP and RP magnitudes (1)"}, {"name": "DMG", "desc": "Distance modulus using Gaia DR2 photometry (1) "}, {"name": "dG", "desc": "Distance using colour-magnitude diagrams based on Gaia DR2 photometry (1)"}, {"name": "AgeG", "desc": "Age using colour-magnitude diagrams based on Gaia DR2 photometry (1)"}]}, {"name": "table5.dat", "desc": "Cluster fundamental parameters derived by taking the mean of Gaia astrometric parameters of cluster members", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "d", "desc": "Mean distance of all cluster members "}, {"name": "E_d", "desc": "Upper error on d "}, {"name": "e_d", "desc": "Lower error on d "}, {"name": "plx", "desc": "Mean parallax of all cluster members "}, {"name": "e_plx", "desc": "Error on plx "}, {"name": "pmRA", "desc": "Mean proper motion in right ascension of all cluster members"}, {"name": "e_pmRA", "desc": "Error on pmRA "}, {"name": "pmDE", "desc": "Mean proper motion in declination of all cluster members"}, {"name": "e_pmDE", "desc": "Error on pmDE "}, {"name": "dRG", "desc": "Mean distance of the red giants analysed in this paper"}, {"name": "E_dRG", "desc": "Upper error on dRG "}, {"name": "e_dRG", "desc": "Lower error on dRG "}, {"name": "plxRG", "desc": "Mean parallax of the red giants analysed in this paper"}, {"name": "e_plxRG", "desc": "Error on plxRG "}, {"name": "pmRARG", "desc": "Mean proper motion in right ascension of the red giants analysed in this paper"}, {"name": "e_pmRARG", "desc": "Error on pmRARG "}, {"name": "pmDERG", "desc": "Mean proper motion in declination of the red giants analysed in this paper"}, {"name": "e_pmDERG", "desc": "Error on pmDERG "}]}, {"name": "table6.dat", "desc": "The chemical abundances of red giants (ID: 43, 1011, 1082) in the star cluster Stock 2", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "Star", "desc": "Star ID (Avg stands for the average of the entire cluster)"}, {"name": "[NaI/Fe]", "desc": "NaI to iron abundance ratio "}, {"name": "e_[NaI/Fe]", "desc": "Error on [NaI/Fe] "}, {"name": "o_[NaI/Fe]", "desc": "? Number of lines used to calculate [NaI/Fe] "}, {"name": "[MgI/Fe]", "desc": "MgI to iron abundance ratio "}, {"name": "e_[MgI/Fe]", "desc": "Error on [MgI/Fe] "}, {"name": "o_[MgI/Fe]", "desc": "? Number of lines used to calculate [MgI/Fe] "}, {"name": "[AlI/Fe]", "desc": "AlI to iron abundance ratio "}, {"name": "e_[AlI/Fe]", "desc": "Error on [AlI/Fe] "}, {"name": "o_[AlI/Fe]", "desc": "? Number of lines used to calculate [AlI/Fe] "}, {"name": "[SiI/Fe]", "desc": "SiI to iron abundance ratio "}, {"name": "e_[SiI/Fe]", "desc": "Error on [SiI/Fe] "}, {"name": "o_[SiI/Fe]", "desc": "? Number of lines used to calculate [SiI/Fe] "}, {"name": "[CaI/Fe]", "desc": "CaI to iron abundance ratio "}, {"name": "e_[CaI/Fe]", "desc": "Error on [CaI/Fe] "}, {"name": "o_[CaI/Fe]", "desc": "? Number of lines used to calculate [CaI/Fe] "}, {"name": "[ScI/Fe]", "desc": "? ScI to iron abundance ratio "}, {"name": "e_[ScI/Fe]", "desc": "? Error on [ScI/Fe] "}, {"name": "o_[ScI/Fe]", "desc": "? Number of lines used to calculate [ScI/Fe] "}, {"name": "[ScII/Fe]", "desc": "ScII to iron abundance ratio "}, {"name": "e_[ScII/Fe]", "desc": "Error on [ScII/Fe] "}, {"name": "o_[ScII/Fe]", "desc": "? Number of lines used to calculate [ScII/Fe] "}, {"name": "[ScII/Fe]s", "desc": "ScII to iron abundance ratio calculated by synthesis"}, {"name": "e_[ScII/Fe]s", "desc": "Error on [ScII/Fe]s "}, {"name": "o_[ScII/Fe]s", "desc": "? Number of lines used to calculate [ScII/Fe]s"}, {"name": "[TiI/Fe]", "desc": "TiI to iron abundance ratio "}, {"name": "e_[TiI/Fe]", "desc": "Error on [TiI/Fe] "}, {"name": "o_[TiI/Fe]", "desc": "? Number of lines used to calculate [TiI/Fe] "}, {"name": "[TiII/Fe]", "desc": "TiII to iron abundance ratio "}, {"name": "e_[TiII/Fe]", "desc": "Error on [TiII/Fe] "}, {"name": "o_[TiII/Fe]", "desc": "? Number of lines used to calculate [TiII/Fe] "}, {"name": "[VI/Fe]", "desc": "VI to iron abundance ratio "}, {"name": "e_[VI/Fe]", "desc": "Error on [VI/Fe] "}, {"name": "o_[VI/Fe]", "desc": "? Number of lines used to calculate [VI/Fe] "}, {"name": "[CrI/Fe]", "desc": "CrI to iron abundance ratio "}, {"name": "e_[CrI/Fe]", "desc": "Error on [CrI/Fe] "}, {"name": "o_[CrI/Fe]", "desc": "? Number of lines used to calculate [CrI/Fe] "}, {"name": "[CrII/Fe]", "desc": "CrII to iron abundance ratio "}, {"name": "e_[CrII/Fe]", "desc": "Error on [CrII/Fe] "}, {"name": "o_[CrII/Fe]", "desc": "? Number of lines used to calculate [CrII/Fe] "}, {"name": "[MnI/Fe]", "desc": "MnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[MnI/Fe]", "desc": "Error on [MnI/Fe] "}, {"name": "o_[MnI/Fe]", "desc": "? Number of lines used to calculate [MnI/Fe] "}, {"name": "[FeI/H]", "desc": "FeI to hydrogen abundance ratio "}, {"name": "e_[FeI/H]", "desc": "Error on [FeI/H] "}, {"name": "o_[FeI/H]", "desc": "? Number of lines used to calculate [FeI/H] "}, {"name": "[FeII/H]", "desc": "FeII to hydrogen abundance ratio "}, {"name": "e_[FeII/H]", "desc": "Error on [FeII/H] "}, {"name": "o_[FeII/H]", "desc": "? Number of lines used to calculate [FeII/H] "}, {"name": "[CoI/Fe]", "desc": "CoI to iron abundance ratio "}, {"name": "e_[CoI/Fe]", "desc": "Error on [CoI/Fe] "}, {"name": "o_[CoI/Fe]", "desc": "? Number of lines used to calculate [CoI/Fe] "}, {"name": "[NiI/Fe]", "desc": "NiI to iron abundance ratio "}, {"name": "e_[NiI/Fe]", "desc": "Error on [NiI/Fe] "}, {"name": "o_[NiI/Fe]", "desc": "? Number of lines used to calculate [NiI/Fe] "}, {"name": "[CuI/Fe]", "desc": "CuI to iron abundance ratio calculated by synthesis"}, {"name": "e_[CuI/Fe]", "desc": "Error on [CuI/Fe] "}, {"name": "o_[CuI/Fe]", "desc": "? Number of lines used to calculate [CuI/Fe] "}, {"name": "[ZnI/Fe]", "desc": "ZnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[ZnI/Fe]", "desc": "Error on [ZnI/Fe] "}, {"name": "o_[ZnI/Fe]", "desc": "? Number of lines used to calculate [ZnI/Fe] "}, {"name": "[YII/Fe]", "desc": "YII to iron abundance ratio "}, {"name": "e_[YII/Fe]", "desc": "Error on [YII/Fe] "}, {"name": "o_[YII/Fe]", "desc": "? Number of lines used to calculate [YII/Fe] "}, {"name": "[ZrI/Fe]", "desc": "ZrI to iron abundance ratio "}, {"name": "e_[ZrI/Fe]", "desc": "Error on [ZrI/Fe] "}, {"name": "o_[ZrI/Fe]", "desc": "? Number of lines used to calculate [ZrI/Fe] "}, {"name": "[ZrII/Fe]", "desc": "ZrII to iron abundance ratio "}, {"name": "e_[ZrII/Fe]", "desc": "Error on [ZrII/Fe] "}, {"name": "o_[ZrII/Fe]", "desc": "? Number of lines used to calculate [ZrII/Fe] "}, {"name": "[BaII/Fe]", "desc": "BaII to iron abundance ratio calculated by synthesis"}, {"name": "e_[BaII/Fe]", "desc": "Error on [BaII/Fe] "}, {"name": "o_[BaII/Fe]", "desc": "? Number of lines used to calculate [BaII/Fe] "}, {"name": "[LaII/Fe]", "desc": "LaII to iron abundance ratio "}, {"name": "e_[LaII/Fe]", "desc": "Error on [LaII/Fe] "}, {"name": "o_[LaII/Fe]", "desc": "? Number of lines used to calculate [LaII/Fe] "}, {"name": "[CeII/Fe]", "desc": "CeII to iron abundance ratio "}, {"name": "e_[CeII/Fe]", "desc": "Error on [CeII/Fe] "}, {"name": "o_[CeII/Fe]", "desc": "? Number of lines used to calculate [CeII/Fe] "}, {"name": "[NdII/Fe]", "desc": "NdII to iron abundance ratio "}, {"name": "e_[NdII/Fe]", "desc": "Error on [NdII/Fe] "}, {"name": "o_[NdII/Fe]", "desc": "? Number of lines used to calculate [NdII/Fe] "}, {"name": "[SmII/Fe]", "desc": "SmII to iron abundance ratio "}, {"name": "e_[SmII/Fe]", "desc": "Error on [SmII/Fe] "}, {"name": "o_[SmII/Fe]", "desc": "? Number of lines used to calculate [SmII/Fe] "}, {"name": "[EuII/Fe]", "desc": "EuII to iron abundance ratio calculated by synthesis"}, {"name": "e_[EuII/Fe]", "desc": "Error on [EuII/Fe] "}, {"name": "o_[EuII/Fe]", "desc": "? Number of lines used to calculate [EuII/Fe] "}]}, {"name": "table7.dat", "desc": "The chemical abundances of stars (IDs: 81, 310, and 662) in NGC 2168 and stars (IDs: 134 and HD 162496) in NGC 6475", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "Star", "desc": "Star ID (Avg stands for the average of the entire cluster)"}, {"name": "[NaI/Fe]", "desc": "NaI to iron abundance ratio "}, {"name": "e_[NaI/Fe]", "desc": "Error on [NaI/Fe] "}, {"name": "o_[NaI/Fe]", "desc": "? Number of lines used to calculate [NaI/Fe] "}, {"name": "[MgI/Fe]", "desc": "MgI to iron abundance ratio "}, {"name": "e_[MgI/Fe]", "desc": "Error on [MgI/Fe] "}, {"name": "o_[MgI/Fe]", "desc": "? Number of lines used to calculate [MgI/Fe] "}, {"name": "[AlI/Fe]", "desc": "AlI to iron abundance ratio "}, {"name": "e_[AlI/Fe]", "desc": "Error on [AlI/Fe] "}, {"name": "o_[AlI/Fe]", "desc": "? Number of lines used to calculate [AlI/Fe] "}, {"name": "[SiI/Fe]", "desc": "SiI to iron abundance ratio "}, {"name": "e_[SiI/Fe]", "desc": "Error on [SiI/Fe] "}, {"name": "o_[SiI/Fe]", "desc": "? Number of lines used to calculate [SiI/Fe] "}, {"name": "[CaI/Fe]", "desc": "CaI to iron abundance ratio "}, {"name": "e_[CaI/Fe]", "desc": "Error on [CaI/Fe] "}, {"name": "o_[CaI/Fe]", "desc": "? Number of lines used to calculate [CaI/Fe] "}, {"name": "[ScI/Fe]", "desc": "? ScI to iron abundance ratio "}, {"name": "e_[ScI/Fe]", "desc": "? Error on [ScI/Fe] "}, {"name": "o_[ScI/Fe]", "desc": "? Number of lines used to calculate [ScI/Fe] "}, {"name": "[ScII/Fe]", "desc": "ScII to iron abundance ratio "}, {"name": "e_[ScII/Fe]", "desc": "Error on [ScII/Fe] "}, {"name": "o_[ScII/Fe]", "desc": "? Number of lines used to calculate [ScII/Fe] "}, {"name": "[ScII/Fe]s", "desc": "ScII to iron abundance ratio calculated by synthesis"}, {"name": "e_[ScII/Fe]s", "desc": "Error on [ScII/Fe]s "}, {"name": "o_[ScII/Fe]s", "desc": "? Number of lines used to calculate [ScII/Fe]s"}, {"name": "[TiI/Fe]", "desc": "TiI to iron abundance ratio "}, {"name": "e_[TiI/Fe]", "desc": "Error on [TiI/Fe] "}, {"name": "o_[TiI/Fe]", "desc": "? Number of lines used to calculate [TiI/Fe] "}, {"name": "[TiII/Fe]", "desc": "TiII to iron abundance ratio "}, {"name": "e_[TiII/Fe]", "desc": "Error on [TiII/Fe] "}, {"name": "o_[TiII/Fe]", "desc": "? Number of lines used to calculate [TiII/Fe] "}, {"name": "[VI/Fe]", "desc": "VI to iron abundance ratio "}, {"name": "e_[VI/Fe]", "desc": "Error on [VI/Fe] "}, {"name": "o_[VI/Fe]", "desc": "? Number of lines used to calculate [VI/Fe] "}, {"name": "[CrI/Fe]", "desc": "CrI to iron abundance ratio "}, {"name": "e_[CrI/Fe]", "desc": "Error on [CrI/Fe] "}, {"name": "o_[CrI/Fe]", "desc": "? Number of lines used to calculate [CrI/Fe] "}, {"name": "[CrII/Fe]", "desc": "CrII to iron abundance ratio "}, {"name": "e_[CrII/Fe]", "desc": "Error on [CrII/Fe] "}, {"name": "o_[CrII/Fe]", "desc": "? Number of lines used to calculate [CrII/Fe] "}, {"name": "[MnI/Fe]", "desc": "MnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[MnI/Fe]", "desc": "Error on [MnI/Fe] "}, {"name": "o_[MnI/Fe]", "desc": "? Number of lines used to calculate [MnI/Fe] "}, {"name": "[FeI/H]", "desc": "FeI to hydrogen abundance ratio "}, {"name": "e_[FeI/H]", "desc": "Error on [FeI/H] "}, {"name": "o_[FeI/H]", "desc": "? Number of lines used to calculate [FeI/H] "}, {"name": "[FeII/H]", "desc": "FeII to hydrogen abundance ratio "}, {"name": "e_[FeII/H]", "desc": "Error on [FeII/H] "}, {"name": "o_[FeII/H]", "desc": "? Number of lines used to calculate [FeII/H] "}, {"name": "[CoI/Fe]", "desc": "CoI to iron abundance ratio "}, {"name": "e_[CoI/Fe]", "desc": "Error on [CoI/Fe] "}, {"name": "o_[CoI/Fe]", "desc": "? Number of lines used to calculate [CoI/Fe] "}, {"name": "[NiI/Fe]", "desc": "NiI to iron abundance ratio "}, {"name": "e_[NiI/Fe]", "desc": "Error on [NiI/Fe] "}, {"name": "o_[NiI/Fe]", "desc": "? Number of lines used to calculate [NiI/Fe] "}, {"name": "[CuI/Fe]", "desc": "CuI to iron abundance ratio calculated by synthesis"}, {"name": "e_[CuI/Fe]", "desc": "Error on [CuI/Fe] "}, {"name": "o_[CuI/Fe]", "desc": "? Number of lines used to calculate [CuI/Fe] "}, {"name": "[ZnI/Fe]", "desc": "ZnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[ZnI/Fe]", "desc": "Error on [ZnI/Fe] "}, {"name": "o_[ZnI/Fe]", "desc": "? Number of lines used to calculate [ZnI/Fe] "}, {"name": "[YII/Fe]", "desc": "YII to iron abundance ratio "}, {"name": "e_[YII/Fe]", "desc": "Error on [YII/Fe] "}, {"name": "o_[YII/Fe]", "desc": "? Number of lines used to calculate [YII/Fe] "}, {"name": "[ZrI/Fe]", "desc": "ZrI to iron abundance ratio "}, {"name": "e_[ZrI/Fe]", "desc": "Error on [ZrI/Fe] "}, {"name": "o_[ZrI/Fe]", "desc": "? Number of lines used to calculate [ZrI/Fe] "}, {"name": "[ZrII/Fe]", "desc": "ZrII to iron abundance ratio "}, {"name": "e_[ZrII/Fe]", "desc": "Error on [ZrII/Fe] "}, {"name": "o_[ZrII/Fe]", "desc": "? Number of lines used to calculate [ZrII/Fe] "}, {"name": "[BaII/Fe]", "desc": "BaII to iron abundance ratio calculated by synthesis"}, {"name": "e_[BaII/Fe]", "desc": "Error on [BaII/Fe] "}, {"name": "o_[BaII/Fe]", "desc": "? Number of lines used to calculate [BaII/Fe] "}, {"name": "f_[BaII/Fe]", "desc": "Flag on [BaII/Fe] (1) "}, {"name": "[LaII/Fe]", "desc": "LaII to iron abundance ratio "}, {"name": "e_[LaII/Fe]", "desc": "Error on [LaII/Fe] "}, {"name": "o_[LaII/Fe]", "desc": "? Number of lines used to calculate [LaII/Fe] "}, {"name": "[CeII/Fe]", "desc": "CeII to iron abundance ratio "}, {"name": "e_[CeII/Fe]", "desc": "Error on [CeII/Fe] "}, {"name": "o_[CeII/Fe]", "desc": "? Number of lines used to calculate [CeII/Fe] "}, {"name": "[NdII/Fe]", "desc": "NdII to iron abundance ratio "}, {"name": "e_[NdII/Fe]", "desc": "Error on [NdII/Fe] "}, {"name": "o_[NdII/Fe]", "desc": "? Number of lines used to calculate [NdII/Fe] "}, {"name": "[SmII/Fe]", "desc": "SmII to iron abundance ratio "}, {"name": "e_[SmII/Fe]", "desc": "Error on [SmII/Fe] "}, {"name": "o_[SmII/Fe]", "desc": "? Number of lines used to calculate [SmII/Fe] "}, {"name": "[EuII/Fe]", "desc": "EuII to iron abundance ratio calculated by synthesis"}, {"name": "e_[EuII/Fe]", "desc": "Error on [EuII/Fe] "}, {"name": "o_[EuII/Fe]", "desc": "? Number of lines used to calculate [EuII/Fe] "}]}, {"name": "table8.dat", "desc": "The chemical abundances of stars (IDs: 22, 67, 100, and 131) in NGC 6991", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "Star", "desc": "Star ID (Avg stands for the average of the entire cluster)"}, {"name": "[NaI/Fe]", "desc": "NaI to iron abundance ratio "}, {"name": "e_[NaI/Fe]", "desc": "Error on [NaI/Fe] "}, {"name": "o_[NaI/Fe]", "desc": "? Number of lines used to calculate [NaI/Fe] "}, {"name": "[MgI/Fe]", "desc": "MgI to iron abundance ratio "}, {"name": "e_[MgI/Fe]", "desc": "Error on [MgI/Fe] "}, {"name": "o_[MgI/Fe]", "desc": "? Number of lines used to calculate [MgI/Fe] "}, {"name": "[AlI/Fe]", "desc": "AlI to iron abundance ratio "}, {"name": "e_[AlI/Fe]", "desc": "Error on [AlI/Fe] "}, {"name": "o_[AlI/Fe]", "desc": "? Number of lines used to calculate [AlI/Fe] "}, {"name": "[SiI/Fe]", "desc": "SiI to iron abundance ratio "}, {"name": "e_[SiI/Fe]", "desc": "Error on [SiI/Fe] "}, {"name": "o_[SiI/Fe]", "desc": "? Number of lines used to calculate [SiI/Fe] "}, {"name": "[CaI/Fe]", "desc": "CaI to iron abundance ratio "}, {"name": "e_[CaI/Fe]", "desc": "Error on [CaI/Fe] "}, {"name": "o_[CaI/Fe]", "desc": "? Number of lines used to calculate [CaI/Fe] "}, {"name": "[ScI/Fe]", "desc": "? ScI to iron abundance ratio "}, {"name": "e_[ScI/Fe]", "desc": "? Error on [ScI/Fe] "}, {"name": "o_[ScI/Fe]", "desc": "? Number of lines used to calculate [ScI/Fe] "}, {"name": "[ScII/Fe]", "desc": "ScII to iron abundance ratio "}, {"name": "e_[ScII/Fe]", "desc": "Error on [ScII/Fe] "}, {"name": "o_[ScII/Fe]", "desc": "? Number of lines used to calculate [ScII/Fe] "}, {"name": "[ScII/Fe]s", "desc": "ScII to iron abundance ratio calculated by synthesis"}, {"name": "e_[ScII/Fe]s", "desc": "Error on [ScII/Fe]s "}, {"name": "o_[ScII/Fe]s", "desc": "? Number of lines used to calculate [ScII/Fe]s"}, {"name": "[TiI/Fe]", "desc": "TiI to iron abundance ratio "}, {"name": "e_[TiI/Fe]", "desc": "Error on [TiI/Fe] "}, {"name": "o_[TiI/Fe]", "desc": "? Number of lines used to calculate [TiI/Fe] "}, {"name": "[TiII/Fe]", "desc": "TiII to iron abundance ratio "}, {"name": "e_[TiII/Fe]", "desc": "Error on [TiII/Fe] "}, {"name": "o_[TiII/Fe]", "desc": "? Number of lines used to calculate [TiII/Fe] "}, {"name": "[VI/Fe]", "desc": "VI to iron abundance ratio "}, {"name": "e_[VI/Fe]", "desc": "Error on [VI/Fe] "}, {"name": "o_[VI/Fe]", "desc": "? Number of lines used to calculate [VI/Fe] "}, {"name": "[CrI/Fe]", "desc": "CrI to iron abundance ratio "}, {"name": "e_[CrI/Fe]", "desc": "Error on [CrI/Fe] "}, {"name": "o_[CrI/Fe]", "desc": "? Number of lines used to calculate [CrI/Fe] "}, {"name": "[CrII/Fe]", "desc": "CrII to iron abundance ratio "}, {"name": "e_[CrII/Fe]", "desc": "Error on [CrII/Fe] "}, {"name": "o_[CrII/Fe]", "desc": "? Number of lines used to calculate [CrII/Fe] "}, {"name": "[MnI/Fe]", "desc": "MnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[MnI/Fe]", "desc": "Error on [MnI/Fe] "}, {"name": "o_[MnI/Fe]", "desc": "? Number of lines used to calculate [MnI/Fe] "}, {"name": "[FeI/H]", "desc": "FeI to hydrogen abundance ratio "}, {"name": "e_[FeI/H]", "desc": "Error on [FeI/H] "}, {"name": "o_[FeI/H]", "desc": "? Number of lines used to calculate [FeI/H] "}, {"name": "[FeII/H]", "desc": "FeII to hydrogen abundance ratio "}, {"name": "e_[FeII/H]", "desc": "Error on [FeII/H] "}, {"name": "o_[FeII/H]", "desc": "? Number of lines used to calculate [FeII/H] "}, {"name": "[CoI/Fe]", "desc": "CoI to iron abundance ratio "}, {"name": "e_[CoI/Fe]", "desc": "Error on [CoI/Fe] "}, {"name": "o_[CoI/Fe]", "desc": "? Number of lines used to calculate [CoI/Fe] "}, {"name": "[NiI/Fe]", "desc": "NiI to iron abundance ratio "}, {"name": "e_[NiI/Fe]", "desc": "Error on [NiI/Fe] "}, {"name": "o_[NiI/Fe]", "desc": "? Number of lines used to calculate [NiI/Fe] "}, {"name": "[CuI/Fe]", "desc": "CuI to iron abundance ratio calculated by synthesis"}, {"name": "e_[CuI/Fe]", "desc": "Error on [CuI/Fe] "}, {"name": "o_[CuI/Fe]", "desc": "? Number of lines used to calculate [CuI/Fe] "}, {"name": "[ZnI/Fe]", "desc": "ZnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[ZnI/Fe]", "desc": "Error on [ZnI/Fe] "}, {"name": "o_[ZnI/Fe]", "desc": "? Number of lines used to calculate [ZnI/Fe] "}, {"name": "[YII/Fe]", "desc": "YII to iron abundance ratio "}, {"name": "e_[YII/Fe]", "desc": "Error on [YII/Fe] "}, {"name": "o_[YII/Fe]", "desc": "? Number of lines used to calculate [YII/Fe] "}, {"name": "[ZrI/Fe]", "desc": "ZrI to iron abundance ratio "}, {"name": "e_[ZrI/Fe]", "desc": "Error on [ZrI/Fe] "}, {"name": "o_[ZrI/Fe]", "desc": "? Number of lines used to calculate [ZrI/Fe] "}, {"name": "[ZrII/Fe]", "desc": "ZrII to iron abundance ratio "}, {"name": "e_[ZrII/Fe]", "desc": "Error on [ZrII/Fe] "}, {"name": "o_[ZrII/Fe]", "desc": "? Number of lines used to calculate [ZrII/Fe] "}, {"name": "[BaII/Fe]", "desc": "BaII to iron abundance ratio calculated by synthesis"}, {"name": "e_[BaII/Fe]", "desc": "Error on [BaII/Fe] "}, {"name": "o_[BaII/Fe]", "desc": "? Number of lines used to calculate [BaII/Fe] "}, {"name": "[LaII/Fe]", "desc": "LaII to iron abundance ratio "}, {"name": "e_[LaII/Fe]", "desc": "Error on [LaII/Fe] "}, {"name": "o_[LaII/Fe]", "desc": "? Number of lines used to calculate [LaII/Fe] "}, {"name": "[CeII/Fe]", "desc": "CeII to iron abundance ratio "}, {"name": "e_[CeII/Fe]", "desc": "Error on [CeII/Fe] "}, {"name": "o_[CeII/Fe]", "desc": "? Number of lines used to calculate [CeII/Fe] "}, {"name": "[NdII/Fe]", "desc": "NdII to iron abundance ratio "}, {"name": "e_[NdII/Fe]", "desc": "Error on [NdII/Fe] "}, {"name": "o_[NdII/Fe]", "desc": "? Number of lines used to calculate [NdII/Fe] "}, {"name": "[SmII/Fe]", "desc": "SmII to iron abundance ratio "}, {"name": "e_[SmII/Fe]", "desc": "Error on [SmII/Fe] "}, {"name": "o_[SmII/Fe]", "desc": "? Number of lines used to calculate [SmII/Fe] "}, {"name": "[EuII/Fe]", "desc": "? EuII to iron abundance ratio calculated by synthesis"}, {"name": "e_[EuII/Fe]", "desc": "? Error on [EuII/Fe] "}, {"name": "o_[EuII/Fe]", "desc": "? Number of lines used to calculate [EuII/Fe] "}]}, {"name": "table9.dat", "desc": "The chemical abundances of stars (IDs: 35, 91, and 110) in NGC 7762", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "Star", "desc": "Star ID (Avg stands for the average of the entire cluster)"}, {"name": "[NaI/Fe]", "desc": "NaI to iron abundance ratio "}, {"name": "e_[NaI/Fe]", "desc": "Error on [NaI/Fe] "}, {"name": "o_[NaI/Fe]", "desc": "? Number of lines used to calculate [NaI/Fe] "}, {"name": "[MgI/Fe]", "desc": "MgI to iron abundance ratio "}, {"name": "e_[MgI/Fe]", "desc": "Error on [MgI/Fe] "}, {"name": "o_[MgI/Fe]", "desc": "? Number of lines used to calculate [MgI/Fe] "}, {"name": "[AlI/Fe]", "desc": "AlI to iron abundance ratio "}, {"name": "e_[AlI/Fe]", "desc": "Error on [AlI/Fe] "}, {"name": "o_[AlI/Fe]", "desc": "? Number of lines used to calculate [AlI/Fe] "}, {"name": "[SiI/Fe]", "desc": "SiI to iron abundance ratio "}, {"name": "e_[SiI/Fe]", "desc": "Error on [SiI/Fe] "}, {"name": "o_[SiI/Fe]", "desc": "? Number of lines used to calculate [SiI/Fe] "}, {"name": "[CaI/Fe]", "desc": "CaI to iron abundance ratio "}, {"name": "e_[CaI/Fe]", "desc": "Error on [CaI/Fe] "}, {"name": "o_[CaI/Fe]", "desc": "? Number of lines used to calculate [CaI/Fe] "}, {"name": "[ScII/Fe]", "desc": "ScII to iron abundance ratioo "}, {"name": "e_[ScII/Fe]", "desc": "Error on [ScII/Fe]] "}, {"name": "o_[ScII/Fe]", "desc": "? Number of lines used to calculate [ScII/Fe] "}, {"name": "[ScII/Fe]s", "desc": "ScII to iron abundance ratio calculated by synthesis"}, {"name": "e_[ScII/Fe]s", "desc": "Error on [ScII/Fe]s "}, {"name": "o_[ScII/Fe]s", "desc": "? Number of lines used to calculate [ScII/Fe]s"}, {"name": "[TiI/Fe]", "desc": "TiI to iron abundance ratio "}, {"name": "e_[TiI/Fe]", "desc": "Error on [TiI/Fe] "}, {"name": "o_[TiI/Fe]", "desc": "? Number of lines used to calculate [TiI/Fe] "}, {"name": "[TiII/Fe]", "desc": "TiII to iron abundance ratio "}, {"name": "e_[TiII/Fe]", "desc": "Error on [TiII/Fe] "}, {"name": "o_[TiII/Fe]", "desc": "? Number of lines used to calculate [TiII/Fe] "}, {"name": "[VI/Fe]", "desc": "VI to iron abundance ratio "}, {"name": "e_[VI/Fe]", "desc": "Error on [VI/Fe] "}, {"name": "o_[VI/Fe]", "desc": "? Number of lines used to calculate [VI/Fe] "}, {"name": "[CrI/Fe]", "desc": "CrI to iron abundance ratio "}, {"name": "e_[CrI/Fe]", "desc": "Error on [CrI/Fe] "}, {"name": "o_[CrI/Fe]", "desc": "? Number of lines used to calculate [CrI/Fe] "}, {"name": "[CrII/Fe]", "desc": "CrII to iron abundance ratio "}, {"name": "e_[CrII/Fe]", "desc": "Error on [CrII/Fe] "}, {"name": "o_[CrII/Fe]", "desc": "? Number of lines used to calculate [CrII/Fe] "}, {"name": "[MnI/Fe]", "desc": "MnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[MnI/Fe]", "desc": "Error on [MnI/Fe] "}, {"name": "o_[MnI/Fe]", "desc": "? Number of lines used to calculate [MnI/Fe] "}, {"name": "[FeI/H]", "desc": "FeI to hydrogen abundance ratio "}, {"name": "e_[FeI/H]", "desc": "Error on [FeI/H] "}, {"name": "o_[FeI/H]", "desc": "? Number of lines used to calculate [FeI/H] "}, {"name": "[FeII/H]", "desc": "FeII to hydrogen abundance ratio "}, {"name": "e_[FeII/H]", "desc": "Error on [FeII/H] "}, {"name": "o_[FeII/H]", "desc": "? Number of lines used to calculate [FeII/H] "}, {"name": "[CoI/Fe]", "desc": "CoI to iron abundance ratio "}, {"name": "e_[CoI/Fe]", "desc": "Error on [CoI/Fe] "}, {"name": "o_[CoI/Fe]", "desc": "? Number of lines used to calculate [CoI/Fe] "}, {"name": "[NiI/Fe]", "desc": "NiI to iron abundance ratio "}, {"name": "e_[NiI/Fe]", "desc": "Error on [NiI/Fe] "}, {"name": "o_[NiI/Fe]", "desc": "? Number of lines used to calculate [NiI/Fe] "}, {"name": "[CuI/Fe]", "desc": "CuI to iron abundance ratio calculated by synthesis"}, {"name": "e_[CuI/Fe]", "desc": "Error on [CuI/Fe] "}, {"name": "o_[CuI/Fe]", "desc": "? Number of lines used to calculate [CuI/Fe] "}, {"name": "[ZnI/Fe]", "desc": "ZnI to iron abundance ratio calculated by synthesis"}, {"name": "e_[ZnI/Fe]", "desc": "Error on [ZnI/Fe] "}, {"name": "o_[ZnI/Fe]", "desc": "? Number of lines used to calculate [ZnI/Fe] "}, {"name": "[YII/Fe]", "desc": "YII to iron abundance ratio "}, {"name": "e_[YII/Fe]", "desc": "Error on [YII/Fe] "}, {"name": "o_[YII/Fe]", "desc": "? Number of lines used to calculate [YII/Fe] "}, {"name": "[ZrI/Fe]", "desc": "ZrI to iron abundance ratio "}, {"name": "e_[ZrI/Fe]", "desc": "Error on [ZrI/Fe] "}, {"name": "o_[ZrI/Fe]", "desc": "? Number of lines used to calculate [ZrI/Fe] "}, {"name": "[ZrII/Fe]", "desc": "ZrII to iron abundance ratio "}, {"name": "e_[ZrII/Fe]", "desc": "Error on [ZrII/Fe] "}, {"name": "o_[ZrII/Fe]", "desc": "? Number of lines used to calculate [ZrII/Fe] "}, {"name": "[BaII/Fe]", "desc": "BaII to iron abundance ratio calculated by synthesis"}, {"name": "e_[BaII/Fe]", "desc": "Error on [BaII/Fe] "}, {"name": "o_[BaII/Fe]", "desc": "? Number of lines used to calculate [BaII/Fe] "}, {"name": "[LaII/Fe]", "desc": "LaII to iron abundance ratio "}, {"name": "e_[LaII/Fe]", "desc": "Error on [LaII/Fe] "}, {"name": "o_[LaII/Fe]", "desc": "? Number of lines used to calculate [LaII/Fe] "}, {"name": "[CeII/Fe]", "desc": "CeII to iron abundance ratio "}, {"name": "e_[CeII/Fe]", "desc": "Error on [CeII/Fe] "}, {"name": "o_[CeII/Fe]", "desc": "? Number of lines used to calculate [CeII/Fe] "}, {"name": "[NdII/Fe]", "desc": "NdII to iron abundance ratio "}, {"name": "e_[NdII/Fe]", "desc": "Error on [NdII/Fe] "}, {"name": "o_[NdII/Fe]", "desc": "? Number of lines used to calculate [NdII/Fe] "}, {"name": "[SmII/Fe]", "desc": "SmII to iron abundance ratio "}, {"name": "e_[SmII/Fe]", "desc": "Error on [SmII/Fe] "}, {"name": "o_[SmII/Fe]", "desc": "? Number of lines used to calculate [SmII/Fe] "}, {"name": "[EuII/Fe]", "desc": "EuII to iron abundance ratio calculated by synthesis"}, {"name": "e_[EuII/Fe]", "desc": "Error on [EuII/Fe] "}, {"name": "o_[EuII/Fe]", "desc": "? Number of lines used to calculate [EuII/Fe] "}]}, {"name": "table10.dat", "desc": "Mean LTE and non-LTE abundances of Na and Al in OCs analysed in this paper and in Reddy et al. (2012MNRAS.419.1350R, Cat. J/MNRAS/419/1350, 2013MNRAS.431.3338R, Cat. J/MNRAS/431/3338, 2015MNRAS.450.4301R, Cat. J/MNRAS/450/4301, 2016MNRAS.463.4366R)", "columns": [{"name": "Cluster", "desc": "Cluster name "}, {"name": "[Fe/H]", "desc": "Iron to hydrogen abundance ratio "}, {"name": "e_[Fe/H]", "desc": "Error on [Fe/H] "}, {"name": "[Na/Fe]LTE", "desc": "Mean LTE Na to Fe abundance ratio "}, {"name": "e_[Na/Fe]LTE", "desc": "Error on [Na/Fe]LTE "}, {"name": "[Na/Fe]", "desc": "Mean non-LTE Na to Fe abundance ratio (1) "}, {"name": "e_[Na/Fe]", "desc": "Error on [Na/Fe] "}, {"name": "[Al/Fe]LTE", "desc": "Mean LTE Al to Fe abundance ratio "}, {"name": "e_[Al/Fe]LTE", "desc": "Error on [Al/Fe]LTE "}, {"name": "[Al/Fe]", "desc": "Mean non-LTE Al to Fe abundance ratio (2) "}, {"name": "e_[Al/Fe]", "desc": "Error on [Al/Fe] "}, {"name": "Mturnoff", "desc": "Cluster's turn-off mass "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_3738"}} {"id": "J/MNRAS/485/3738", "title_cds": "3D structure in the A370 MUSE Mosaic", "title_create": "Lagattuta+, 2019", "year": "2019", "author": "Lagattuta D.J., Richard J., Bauer F.E., Clement B., Mahler G., Soucail G., Carton D., Kneib J.-P., Laporte N., Martinez J., Patricio V., Payne A.V., Pello R., Schmidt K.B., de la Vieuville G.", "title_pub": "Probing 3D structure with a large MUSE mosaic: extending the mass model of Frontier Field Abell 370.", "first_author": "Lagattuta D.J.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.3738L"], "keyword_cds": "Clusters, galaxy ; Gravitational lensing ; Redshifts ; Photometry, HST ; Models", "keyword_pub": "gravitational lensing: strong - techniques: imaging spectroscopy - galaxies: clusters: individual: Abell 370 - galaxies: high-redshift - dark matter - large-scale structure of Universe", "abstract": ["We present an updated strong-lensing analysis of the massive cluster", "Abell 370 (A370), continuing the work first presented in L17. In this", "new analysis, we take advantage of the deeper imaging data from the", "Hubble Space Telescope Frontier Fields programme, as well as a large", "spectroscopic mosaic obtained with the Multi-Unit Spectroscopic", "Explorer (MUSE). Thanks to the extended coverage of this mosaic, we", "probe the full 3D distribution of galaxies in the field, giving us a", "unique picture of the extended structure of the cluster and its", "surroundings. Our final catalogue contains 584 redshifts, representing", "the largest spectroscopic catalogue of A370 to date. Constructing the", "model, we measure a total mass distribution that is quantitatively", "similar to our previous work - though to ensure a low rms error in the", "model fit, we invoke a significantly large external shear term. Using", "the redshift catalogue, we search for other bound groups of galaxies,", "which may give rise to a more physical interpretation of this shear.", "We identify three structures in narrow redshift ranges along the line", "of sight, highlighting possible infalling substructures into the main", "cluster halo. We also discover additional substructure candidates in", "low-resolution imaging at larger projected radii. More spectroscopic", "coverage of these regions (pushing close to the A370 virial radius)", "and more extended, high-resolution imaging will be required to", "investigate this possibility, further advancing the analysis of these", "interesting developments."], "description": ["These catalogs contain observational and model-dependent data for", "objects within and along the line of sight of the Abell 370 galaxy", "cluster. MUSE data are acquired in Wide-field, non-AO mode (WFM-NOAO)", "using both Guaranteed Time Observations (GTO) and General Observer", "(GO) time. The Frontier Fields images used to measure photometry and", "astrometry are publicly available at", "[https://archive.stsci.edu/prepds/frontier/]. All magnitudes are", "presented in the AB system. Lens model parameters are generated with", "the LENSTOOL software package (Kneib et al. 1996ApJ...471..643K; Jullo", "et al. 2007NJPh....9..447J; Jullo & Kneib 2009MNRAS.395.1319J)", "available at the following location:", "[https://projets.lam.fr/projects/lenstool/wiki]. The potentials used", "to construct the lens models are based on the dual Pseudo-Isothermal", "Ellipsoid density profile presented in Eliasdottir et al.", "2007arXiv0710.5636E."], "data": "", "date_update": "28-Sep-2022", "tables": [{"name": "table1.dat", "desc": "Multiply imaged systems ", "columns": [{"name": "mID", "desc": "Multiple Image ID "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "zspec", "desc": "? Spectroscopic redshift (1) "}, {"name": "zmod", "desc": "? Lens model predicted redshift (2) "}, {"name": "e_zmod", "desc": "? Error on zmod "}, {"name": "Class", "desc": "Multiple Image constraint class (3) "}, {"name": "Note", "desc": "?=- Notes on specific Multiple Images (4) "}]}, {"name": "tablea1a.dat", "desc": "Lens Models (goodness-of-fit statistics) ", "columns": [{"name": "Model", "desc": "Lens model name "}, {"name": "n", "desc": "Total number of model constraints "}, {"name": "k", "desc": "Total number of model parameters "}, {"name": "rms", "desc": "Best-fit model rms error "}, {"name": "chi2", "desc": "Best-fit model chi-squared per degree of freedom"}, {"name": "logL", "desc": "Best-fit model log(likelihood) value "}, {"name": "logE", "desc": "Best-fit model log(evidence) value "}, {"name": "BIC", "desc": "Best-fit model Bayesian Information Criteria "}]}, {"name": "tablea1b.dat", "desc": "Lens Models (best-fit model parameters) ", "columns": [{"name": "Model", "desc": "Lens model name "}, {"name": "Comp", "desc": "Model component name "}, {"name": "dRA", "desc": "? Relative right ascension (1) "}, {"name": "f_dRA", "desc": "Flag on dRA (2) "}, {"name": "E_dRA", "desc": "? Upper error on dRA "}, {"name": "e_dRA", "desc": "? Lower error on dRA "}, {"name": "dDE", "desc": "? Relative declination (1) "}, {"name": "f_dDE", "desc": "Flag on dDE (2) "}, {"name": "E_dDE", "desc": "? Upper error on dDE "}, {"name": "e_dDE", "desc": "? Lower error on dDE "}, {"name": "ell", "desc": "? Ellipticity (or shear magnitude) (3) "}, {"name": "f_ell", "desc": "Flag on ell (2) "}, {"name": "E_ell", "desc": "? Upper error on ell "}, {"name": "e_ell", "desc": "? Lower error on ell "}, {"name": "PA", "desc": "[]? Position angle (East of North) "}, {"name": "f_PA", "desc": "Flag on PA (2) "}, {"name": "E_PA", "desc": "? Upper error on PA "}, {"name": "e_PA", "desc": "? Lower error on PA "}, {"name": "rCore", "desc": "? Core radius of dPIE potential "}, {"name": "f_rCore", "desc": "Flag on rCore (2) "}, {"name": "E_rCore", "desc": "? Upper error on rCore "}, {"name": "e_rCore", "desc": "? Lower error on rCore "}, {"name": "rCut", "desc": "? Cut radius of dPIE potential "}, {"name": "f_rCut", "desc": "Flag on rCut (2) "}, {"name": "E_rCut", "desc": "? Upper error on rCut "}, {"name": "e_rCut", "desc": "? Lower error on rCut "}, {"name": "sig0", "desc": "? Central velocity dispersion of potential "}, {"name": "E_sig0", "desc": "? Upper error on sig0 "}, {"name": "e_sig0", "desc": "? Lower error on sig0 "}]}, {"name": "tablec1.dat", "desc": "Master MUSE Redshift Catalog ", "columns": [{"name": "ID", "desc": "Object ID (1) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "z", "desc": "MUSE redshift "}, {"name": "Type", "desc": "Spectroscopic type flag (2) "}, {"name": "Conf", "desc": "Spectroscopic confidence flag (3) "}, {"name": "F435Wmag", "desc": "?=99.0 AB Magnitude (apparent) in F435W filter (4)"}, {"name": "e_F435Wmag", "desc": "?=99.0 Mean error on F435Wmag "}, {"name": "F606Wmag", "desc": "?=99.0 AB Magnitude (apparent) in F606W filter (4)"}, {"name": "e_F606Wmag", "desc": "?=99.0 Mean error on F606Wmag "}, {"name": "F814Wmag", "desc": "?=99.0 AB Magnitude (apparent) in F814W filter (4)"}, {"name": "e_F814Wmag", "desc": "?=99.0 Mean error on F814Wmag "}, {"name": "F105Wmag", "desc": "?=99.0 AB Magnitude (apparent) in F105W filter (4)"}, {"name": "e_F105Wmag", "desc": "?=99.0 Mean error on F105Wmag "}, {"name": "F125Wmag", "desc": "?=99.0 AB Magnitude (apparent) in F125W filter (4)"}, {"name": "e_F125Wmag", "desc": "?=99.0 Mean error on F125Wmag "}, {"name": "F140Wmag", "desc": "?=99.0 AB Magnitude (apparent) in F140W filter (4)"}, {"name": "e_F140Wmag", "desc": "?=99.0 Mean error on F140Wmag "}, {"name": "F160Wmag", "desc": "?=99.0 AB Magnitude (apparent) in F160W filter (4)"}, {"name": "e_F160Wmag", "desc": "?=99.0 Mean error on F160Wmag "}, {"name": "mu", "desc": "Lensing magnification (5) "}, {"name": "e_mu", "desc": "Mean error on mu "}, {"name": "mID", "desc": "? Multiply-Imaged object ID (6) "}, {"name": "lines", "desc": "Summary of features seen in MUSE spectrum "}]}, {"name": "tabled1.dat", "desc": "MUSE-GLASS Redshift Comparisons ", "columns": [{"name": "IDMUSE", "desc": "Object ID in MUSE catalog "}, {"name": "zMUSE", "desc": "MUSE redshift "}, {"name": "cMUSE", "desc": "MUSE spectroscopic confidence flag "}, {"name": "cMUSEnew", "desc": "? Updated MUSE spectroscopic confidence flag "}, {"name": "IDGLASS", "desc": "Object ID in GLASS catalog "}, {"name": "zGLASS", "desc": "GLASS redshift (1) "}, {"name": "zGLASSnew", "desc": "? Updated GLASS redshift "}, {"name": "cGLASS", "desc": "GLASS spectroscopic confidence flag "}, {"name": "cGLASSnew", "desc": "? Updated GLASS spectroscopic confidence flag "}, {"name": "Comments", "desc": "Summary of the comparison between MUSE and GLASS data"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_3834"}} {"id": "J/MNRAS/485/3834", "title_cds": "Short Title", "title_create": "De+, 2019", "year": "2019", "author": "De Ruiter I., Van Den Eijnden J., Ingram A., Uttley P.", "title_pub": "A systematic study of the phase difference between QPO harmonics in black hole X-ray binaries.", "first_author": "De Ruiter I.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.3834D"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "28-Sep-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_3999"}} {"id": "J/MNRAS/485/3999", "title_cds": "Magnetic dipole moments on rocky exoplanets", "title_create": "McIntyre+, 2019", "year": "2019", "author": "McIntyre S.R.N., Lineweaver C.H., Ireland M.J.", "title_pub": "Planetary magnetism as a parameter in exoplanet habitability.", "first_author": "McIntyre S.R.N.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.3999M"], "see_also": ["J/AJ/156/264 : California-Kepler Survey. VII. Planet radius gap", "J/ApJ/834/17 : Mass & radius of planets, moons, low mass stars"], "keyword_cds": "Exoplanets ; Magnetic fields ; Models", "keyword_pub": "planets and satellites: general - planets and satellites: magnetic fields - planets and satellites: terrestrial planets", "abstract": ["Evidence from the Solar system suggests that, unlike Venus and Mars,", "the presence of a strong magnetic dipole moment on Earth has helped", "maintain liquid water on its surface. Therefore, planetary magnetism", "could have a significant effect on the long-term maintenance of", "atmosphere and liquid water on rocky exoplanets. We use Olson &", "Christensen's (2006E&PSL.250..561O) model to estimate magnetic dipole", "moments of rocky exoplanets with radii R_p_=<1.23R_{oplus}_. Even when", "modelling maximum magnetic dipole moments, only Kepler-186 f has a", "magnetic dipole moment larger than the Earth's, while approximately", "half of rocky exoplanets detected in the circumstellar habitable zone", "have a negligible magnetic dipole moment. This suggests that planetary", "magnetism is an important factor when prioritizing observations of", "potentially habitable planets."], "description": ["Before applying our magnetic moment model, we compile a data base of", "rocky exoplanets using the NASA composite exoplanet data base (Akeson", "et al. 2013PASP..125..989A), in conjunction with the higher precision", "radii of Kepler planets given in Fulton & Petigura", "(2018AJ....156..264F, Cat. J/AJ/156/264) (Table A1). Unknown masses or", "radii and their associated uncertainties are estimated using Chen &", "Kipping (2017ApJ...834...17C, Cat. J/ApJ/834/17) M-R relationship for", "terrestrial planets: R_p_~M_p_^0.279+/-0.009^.", "Following the Chen & Kipping (2017ApJ...834...17C, Cat. J/ApJ/834/17)", "definition of the boundary between terrestrial and Jovian planets, we", "restrict our sample to exoplanets with radii R_p_=<1.23R_{oplus}_,", "which corresponds to ~2M_{oplus}_. These constraints restrict our", "sample to 496 rocky exoplanets (490 tidally locked), nine of which are", "located in the circumstellar habitable zone (CHZ) - where the CHZ is", "the insolation between recent Venus and ancient Mars as defined by the", "Kopparapu et al. (2013ApJ...765..131K) optimistic habitable zone.", "Eight of the nine rocky exoplanets from our CHZ subset are tidally", "locked.", "For each exoplanet we perform 10000 Monte Carlo simulations. These", "simulations allow us to determine the median and 68 per cent", "confidence intervals on M_max_ (maximum magnetic dipole momement)", "values."], "data": "", "date_update": "29-Sep-2022", "tables": [{"name": "tablea1.dat", "desc": "Rocky exoplanets sample (in order of decreasing dipole moment)", "columns": [{"name": "Name", "desc": "Planet name "}, {"name": "f_Name", "desc": "Flag on Name (1) "}, {"name": "Mass", "desc": "Planet mass "}, {"name": "e_Mass", "desc": "Error on Mass "}, {"name": "Rad", "desc": "Planet radius "}, {"name": "e_Rad", "desc": "Error on Rad "}, {"name": "Period", "desc": "Orbital period "}, {"name": "e_Period", "desc": "Error on Period "}, {"name": "Age", "desc": "Stellar age "}, {"name": "Mmax", "desc": "Maximum magnetic dipole moment "}, {"name": "e_Mmax", "desc": "Error on Mmax "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_4311"}} {"id": "J/MNRAS/485/4311", "title_cds": "Light element discontinuities in NGC 6402", "title_create": "Johnson+, 2019", "year": "2019", "author": "Johnson C.I., Caldwell N., Rich R.M., Mateo M., Bailey J.I.", "title_pub": "Light element discontinuities suggest an early termination of star formation in the globular cluster NGC 6402 (M14).", "first_author": "Johnson C.I.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.4311J"], "see_also": ["VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)"], "keyword_cds": "Clusters, globular ; Stars, giant ; Spectra, optical ; Abundances ; Magnitudes ; Effective temperatures ; Radial velocities", "keyword_pub": "galaxies: star clusters: individual: NGC 6402 (M14)", "abstract": ["NGC 6402 is among the most massive globular clusters in the Galaxy,", "but little is known about its detailed chemical composition.", "Therefore, we obtained radial velocities and/or chemical abundances of", "11 elements for 41 red giant branch stars using high resolution", "spectra obtained with the Magellan-M2FS instrument. We find NGC 6402", "to be only moderately metal-poor with <[Fe/H]>=-1.13dex ({sigma}=0.05", "dex) and to have a mean heliocentric radial velocity of -61.1km/s", "({sigma}=8.5km/s). In general, NGC 6402 exhibits mean composition", "properties that are similar to other inner Galaxy clusters, such as", "[{alpha}/Fe]~+0.3dex, [Cr,Ni/Fe]~0.0dex, and <[La/Eu]>=-0.08dex.", "Similarly, we find large star-to-star abundance variations for O, Na,", "Mg, Al, and Si that are indicative of gas that experienced high", "temperature proton-capture burning. Interestingly, we not only detect", "three distinct populations but also find large gaps in the [O/Fe],", "[Na/Fe], and [Al/Fe] distributions that may provide the first direct", "evidence of delayed formation for intermediate composition stars. A", "qualitative enrichment model is discussed where clusters form stars", "through an early (~<5-10Myr) phase, which results in first generation", "and 'extreme' composition stars, and a delayed phase (>~40Myr), which", "results in the dilution of processed and pristine gas and the", "formation of intermediate composition stars. For NGC 6402, the missing", "intermediate composition stars suggest the delayed phase terminated", "prematurely, and as a result the cluster may uniquely preserve details", "of the chemical enrichment process."], "description": ["The spectra for this project were obtained using the Michigan-Magellan", "Fiber System (M2FS; Mateo et al. 2012SPIE.8446E..4YM) and MSpec", "spectrograph on the Magellan-Clay 6.5m telescope at Las Campanas", "Observatory. The total wavelength coverage of all six orders ranged", "from ~6140-6720{AA}. The spectra were obtained under clear but", "moderately humid conditions with reasonable seeing (~1.2arcsec) on", "2017 September 11, 12, and 15. The integration time totalled 18000s", "(5h) and was distributed over ten 1800s exposures. Signal-to-noise", "ratios (S/N) for individual exposures were approximately 25-50 per", "reduced pixel.", "Targets and coordinates were obtained using the Two Micron All Sky", "Survey (2MASS; Skrutskie et al. 2006AJ....131.1163S, Cat. VII/233),", "and membership probabilities were estimated using a fiducial sequence", "derived from 2MASS CMDs that only included stars within 1arcmin of the", "cluster core. The brightest RGB-tip stars were not included in order", "to avoid targets with effective temperatures (T_eff_) lower than", "~4100K."], "data": "", "date_update": "29-Sep-2022", "tables": [{"name": "table1.dat", "desc": "Abundance ratios and population designations for all member stars", "columns": [{"name": "Name", "desc": "Star name (2MHHMMSSSS+DDMMSSS) "}, {"name": "f_Name", "desc": "Flag on Name (1) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Jmag", "desc": "J-band magnitude from 2MASS "}, {"name": "Hmag", "desc": "H-band magnitude from 2MASS "}, {"name": "Ksmag", "desc": "Ks-band magnitude from 2MASS "}, {"name": "RV", "desc": "Heliocentric radial velocity "}, {"name": "e_RV", "desc": "Error on RV "}, {"name": "Teff", "desc": "? Effective temperature "}, {"name": "logg", "desc": "? Surface gravity "}, {"name": "[Fe/H]", "desc": "? Iron to hydrogen abundance ratio "}, {"name": "vt", "desc": "? Microturbulence velocity "}]}, {"name": "table23.dat", "desc": "Abundance ratios and population designations for all member stars", "columns": [{"name": "Name", "desc": "Star name (2MHHMMSSSS+DDMMSSS) "}, {"name": "Pop", "desc": "Population designation (G1) "}, {"name": "[FeI/H]", "desc": "? FeI to hydrogen abundance ratio "}, {"name": "[FeII/H]", "desc": "? FeII to hydrogen abundance ratio "}, {"name": "[OI/Fe]", "desc": "? OI to iron abundance ratio "}, {"name": "[NaI/Fe]", "desc": "? NaI to iron abundance ratio "}, {"name": "[MgI/Fe]", "desc": "? MgI to iron abundance ratio "}, {"name": "[AlI/Fe]", "desc": "? AlI to iron abundance ratio "}, {"name": "[SiI/Fe]", "desc": "? SiI to iron abundance ratio "}, {"name": "[CaI/Fe]", "desc": "? CaI to iron abundance ratio "}, {"name": "[CrI/Fe]", "desc": "? CrI to iron abundance ratio "}, {"name": "[NiI/Fe]", "desc": "? NiI to iron abundance ratio "}, {"name": "[LaII/Fe]", "desc": "? LaII to iron abundance ratio "}, {"name": "[EuII/Fe]", "desc": "? EuII to iron abundance ratio "}, {"name": "e_[FeI/H]", "desc": "? Error on [FeI/H] "}, {"name": "e_[FeII/H]", "desc": "? Error on [FeII/H] "}, {"name": "e_[OI/Fe]", "desc": "? Error on [OI/Fe] "}, {"name": "e_[NaI/Fe]", "desc": "? Error on [NaI/Fe] "}, {"name": "e_[MgI/Fe]", "desc": "? Error on [MgI/Fe] "}, {"name": "e_[AlI/Fe]", "desc": "? Error on [AlI/Fe] "}, {"name": "e_[SiI/Fe]", "desc": "? Error on [SiI/Fe] "}, {"name": "e_[CaI/Fe]", "desc": "? Error on [CaI/Fe] "}, {"name": "e_[CrI/Fe]", "desc": "? Error on [CrI/Fe] "}, {"name": "e_[NiI/Fe]", "desc": "? Error on [NiI/Fe] "}, {"name": "e_[LaII/Fe]", "desc": "? Error on [LaII/Fe] "}, {"name": "e_[EuII/Fe]", "desc": "? Error on [EuII/Fe] "}]}, {"name": "table4a.dat", "desc": "Mean abundance ratios for the P1, P2, and E populations", "columns": [{"name": "Pop", "desc": "Population designation (G1) "}, {"name": "[Fe/H]", "desc": "Mean Fe to hydrogen abundance ratio "}, {"name": "[O/Fe]", "desc": "Mean O to iron abundance ratio "}, {"name": "[Na/Fe]", "desc": "Mean Na to iron abundance ratio "}, {"name": "[Mg/Fe]", "desc": "Mean Mg to iron abundance ratio "}, {"name": "[Al/Fe]", "desc": "Mean Al to iron abundance ratio "}, {"name": "[Si/Fe]", "desc": "Mean Si to iron abundance ratio "}, {"name": "[Ca/Fe]", "desc": "Mean Ca to iron abundance ratio "}, {"name": "[Cr/Fe]", "desc": "Mean Cr to iron abundance ratio "}, {"name": "[Ni/Fe]", "desc": "Mean Ni to iron abundance ratio "}, {"name": "[La/Fe]", "desc": "Mean La to iron abundance ratio "}, {"name": "[Eu/Fe]", "desc": "Mean Eu to iron abundance ratio "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_4375"}} {"id": "J/MNRAS/485/4375", "title_cds": "Chronochemokinematic analysis of UMaG", "title_create": "Dopcke+, 2019", "year": "2019", "author": "Dopcke G., Porto de Mello G.F., Sneden C.", "title_pub": "The Ursa Major Moving Group: a chronochemokinematic analysis.", "first_author": "Dopcke G.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.4375D"], "keyword_cds": "Abundances ; Effective temperatures ; Spectra, optical ; Stars, ages ; Space velocities ; Photometry, UBVRI ; Photometry, uvby", "keyword_pub": "techniques: spectroscopic, stars: abundances", "abstract": ["Stars in kinematic groups are believed to share the same age,", "metallicity, and velocity vectors, and are disrupted by events such as", "encounters with massive objects, leaving a residue of stars sharing", "the same kinematic properties, thus bridging an important evolutionary", "gap between clusters and field stars. We determine the most likely", "metallicity for the unevolved stars of the group, collectively, by", "assuming that these stars all conform to a single zero-age main", "sequence line and requiring that residual T_eff_ and luminosity values", "be minimized: the [Fe/H] value that best describes the observed HR", "diagram of the group lies in the range +0.05<[Fe/H]<+0.10. In this", "work, we report the detailed spectroscopic analysis of 23 stars in the", "Ursa Major Group (UMaG), together with seven young field stars that", "function as a control sample, based on high S/N, R~60000 optical", "spectra. We present abundances for C, Na, Al, Si, Ca, Sc, Ti, V, Cr,", "Mn, Co, Fe, Ni, Cu, Zn, Sr, Y, Zr, Ba, La, Ce, Nd, Sm, Gd, and Eu. We", "also found that there is a clear kinematic nucleus in the UVW space,", "but from the spectroscopic analysis only a fraction of these stars", "could be considered chemically and chronologically homogeneous. The", "results suggest that the UMaG has physical existence in a", "chronochemokinematic sense, but is not chemically peculiar: high Ba", "abundance seems to be a common feature of young stars. From the", "initial sample, only 14 (61 per cent) stars were finally considered", "members of the UMaG, resulting in an average metallicity and standard", "deviation of [Fe/H]=0.01 and 0.07, respectively, consistent with", "previous works. We finally conclude that even though the UMaG stars", "share a common kinematics, age, and metallicity, they do not have the", "same chemical abundance pattern, pointing to a dynamical origin of the", "Group."], "description": ["Our sample consists of 23 UMaG stars that had membership assignment in", "the literature, and seven young stars for comparison. Such young stars", "have chromospheric activity logR'_HK_>-4.44 (Noyes et al.", "1984ApJ...279..763N). This implies that the stars are young, not older", "than the Hyades (635Myr; Cummings et al. 2017AJ....153..128C). We also", "obtained a spectrum of Ganymede, under the same conditions as the", "stellar spectra, to use it as a solar proxy.", "The stellar spectra we analysed here were obtained between 1999 27th", "February and 1st March, at the McDonald Observatory, using a 2.7m", "telescope, and the Tull coude Echelle spectrograph (Tull et al.", "1995PASP..107..251T). The spectra have R=60000 and S/N>150 for all", "spectra, and >300 in most cases, with wavelength coverage from 4500 to", "6800{AA}.", "The Paschen slope in the type K, G, and F stars, studied here, is", "sensitive to T_eff_ changes, so we used the colours (B-V) Johnson,", "(B_T_-V_T_) Tycho, and (b-y) Stromgren, which are good indicators of", "this slope."], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "05-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_4423"}} {"id": "J/MNRAS/485/4423", "title_cds": "The Gaia ultracool dwarf sample", "title_create": "Smart+, 2019", "year": "2019", "author": "Smart R.L., Marocco F., Sarro L.M., Barrado D., Beamin J.C., Caballero J.A., Jones H.R.A.", "title_pub": "The Gaia ultracool dwarf sample - II. Structure at the end of the main sequence.", "first_author": "Smart R.L.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.4423S"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)", "II/328 : AllWISE Data Release (Cutri+ 2013)"], "keyword_cds": "Stars, double and multiple ; Stars, brown dwarf ; Stars, late-type", "keyword_pub": "binaries: visual - brown dwarfs - stars: late-type - Hertzsprung-Russell and colour-magnitude diagrams - solar neighbourhood", "abstract": ["We identify and investigate known late M, L, and T dwarfs in the Gaia", "second data release. This sample is being used as a training set in", "the Gaia data processing chain of the ultracool dwarfs work package.", "We find 695 objects in the optical spectral range M8-T6 with accurate", "Gaia coordinates, proper motions, and parallaxes which we combine with", "published spectral types and photometry from large area optical and", "infrared sky surveys. We find that 100 objects are in 47 multiple", "systems, of which 27 systems are published and 20 are new. These will", "be useful benchmark systems and we discuss the requirements to produce", "a complete catalogue of multiple systems with an ultracool dwarf", "component. We examine the magnitudes in the Gaia passbands and find", "that the GBP magnitudes are unreliable and should not be used for", "these objects. We examine progressively redder colour-magnitude", "diagrams and see a notable increase in the main-sequence scatter and a", "bivariate main sequence for old and young objects. We provide an", "absolute magnitude-spectral subtype calibration for G and G_RP_", "passbands along with linear fits over the range M8-L8 for other", "passbands."], "description": ["The initial list of known ulta cool dwarfs (UCDs) was the input", "catalogue from Paper 1 (Smart et al. 2017MNRAS.469..401S, Cat.", "J/MNRAS/469/401) of 1885 objects with M, L, T, or Y spectral", "classification. To this we added the photometrically identified LT", "dwarfs from Skrzypek, Warren & Faherty (2016A&A...589A..49S, Cat.", "J/A+A/589/A49) and a few other recent discoveries (e.g. Marocco et al.", "2017MNRAS.470.4885M; Scholz & Bell 2018RNAAS...2...33S; Smith et al.", "2018MNRAS.474.1826S, Cat. II/364). The current list contains 3093 UCDs", "ranging from M8 to Y2 dwarfs. The M dwarfs were retained to facilitate", "differentiation of the spectral types in the magnitude and colour", "space, as some objects are classed as M in optical spectra and L in", "infrared spectra and vice versa. Since this input catalogue is", "dominated by L and T dwarfs we refer to it as the LT catalogue", "(hereafter LTC).", "For all objects we have collected photometry from the Two Micron All", "Sky Survey (2MASS; Skrutskie et al. 2006AJ....131.1163S, Cat.", "VII/233), the Panoramic Survey Telescope and Rapid Response System", "release 1 (PS1; Chambers et al. 2016arXiv161205560C, Cat. II/349), and", "the Wide-field Infrared Survey Explorer extension (AllWISE; Wright et", "al. 2010AJ....140.1868W), providing up to 11 homogeneous magnitudes in", "passbands ranging from Gunn g to WISE W3. The WISE W4 band was not", "included as the number of objects with reliable magnitudes were very", "low.", "We started by searching for any objects in the Gaia DR2 release that", "had a parallax larger than 10mas and was within 20arcsec of the LTC", "entry at the Gaia DR2 epoch. We choose 20arcsec as not all entries", "have published proper motions, the epoch difference can be up to 20yr,", "and typical proper motions are 500-1000mas/yr. This resulted in 753", "entries from Gaia DR2. For each entry we then propagated the Gaia DR2", "position to the epoch of the LTC positions in the input catalogue", "using the Gaia DR2 proper motions."], "data": "", "date_update": "07-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Input catalogue entries with multiple Gaia DR2 matches within 20 arcsec", "columns": [{"name": "ID", "desc": "Short name (1) "}, {"name": "Name", "desc": "Discovery name "}, {"name": "Offset", "desc": "Offset on the sky of the LTC position (generally 2MASS coordinates)"}, {"name": "Gmag", "desc": "Gaia DR2 G-band magnitude (G1) "}, {"name": "G-Gest", "desc": "G-Gest difference where Gest is the average magnitude for all objects in the LTC"}, {"name": "plx", "desc": "Gaia DR2 parallax (G1) "}, {"name": "e_plx", "desc": "Error on plx (G1) "}, {"name": "pmtot", "desc": "Total proper motion "}, {"name": "PApm", "desc": "Position angle of the proper motion "}]}, {"name": "table2.dat", "desc": "Intrinsically bright (M_G_<14.0mag) objects matched to LT objects sorted by absolute magnitude (top) and matches with offset >5.0 arcsec sorted by separation (bottom)", "columns": [{"name": "ID", "desc": "Short name "}, {"name": "Name", "desc": "Discovery name "}, {"name": "GaiaDR2", "desc": "Gaia DR2 Source identifier (G1) "}, {"name": "Offset", "desc": "Offset on the sky of the LTC position (generally 2MASS coordinates)"}, {"name": "Gmag", "desc": "Gaia DR2 G-band magnitude (G1) "}, {"name": "Gestmag", "desc": "Gest is the average magnitude for all objects in the LTC"}, {"name": "GMag", "desc": "Absolute magnitude in the G band "}]}, {"name": "table3.dat", "desc": "Data for Ultra-Cool Dwarfs in Gaia DR2 ", "columns": [{"name": "ID", "desc": "Short name "}, {"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2015.5 (G1) "}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2015.5 (G1) "}, {"name": "Name", "desc": "Discovery name "}, {"name": "r_Name", "desc": "Reference for Name "}, {"name": "GaiaDR2", "desc": "Gaia DR2 Source identifier (G1) "}, {"name": "Distcat", "desc": "Distance DR2 to catalogue position "}, {"name": "VBURMG", "desc": "?=- Multiple code VB/UR/MG "}, {"name": "r_VBURMG", "desc": "?=- Reference for VBURMG "}, {"name": "SpTop", "desc": "?=- Optical Spectral type "}, {"name": "r_SpTop", "desc": "?=- Reference for SPTop "}, {"name": "SpTnir", "desc": "?=- Near infrared Spectral type "}, {"name": "r_SpTnir", "desc": "?=- Reference for SpTnir "}, {"name": "SpTph", "desc": "?=- Photometric Spectral type "}, {"name": "r_SpTph", "desc": "?=- Reference for SpTph "}, {"name": "plxlit", "desc": "? Published parallax "}, {"name": "e_plxlit", "desc": "? Error on plxlit "}, {"name": "r_plxlit", "desc": "Reference for plxlit "}, {"name": "Jmag", "desc": "? 2MASS J-band magnitude "}, {"name": "e_Jmag", "desc": "? Error on Jmag "}, {"name": "Hmag", "desc": "? 2MASS H-band magnitude "}, {"name": "e_Hmag", "desc": "? Error on Hmag "}, {"name": "Kmag", "desc": "? 2MASS K-band magnitude "}, {"name": "e_Kmag", "desc": "? Error on Kmag "}, {"name": "W1mag", "desc": "? AllWISE W1-band magnitude "}, {"name": "e_W1mag", "desc": "? Error on W1mag "}, {"name": "W2mag", "desc": "? AllWISE W2-band magnitude "}, {"name": "e_W2mag", "desc": "? Error on W2mag "}, {"name": "W3mag", "desc": "? AllWISE W3-band magnitude "}, {"name": "e_W3mag", "desc": "? Error on W3mag "}, {"name": "GmagPS", "desc": "? Pan-STARRS G-band magnitude "}, {"name": "e_GmagPS", "desc": "? Error on GmagPS "}, {"name": "RmagPS", "desc": "? Pan-STARRS R-band magnitude "}, {"name": "e_RmagPS", "desc": "? Error on RmagPS "}, {"name": "imagPS", "desc": "? Pan-STARRS i-band magnitude "}, {"name": "e_imagPS", "desc": "? Error on imagPS "}, {"name": "ZmagPS", "desc": "? Pan-STARRS Z-band magnitude "}, {"name": "e_ZmagPS", "desc": "? Error on ZmagPS "}, {"name": "YmagPS", "desc": "? Pan-STARRS Y-band magnitude "}, {"name": "e_YmagPS", "desc": "? Error on YmagPS "}, {"name": "Gmag", "desc": "Gaia DR2 G-band magnitude (G1) "}, {"name": "e_Gmag", "desc": "Error on Gmag (1) "}, {"name": "FG", "desc": "Gaia DR2 G-band flux (G1) "}, {"name": "e_FG", "desc": "Error on FG (G1) "}, {"name": "BPmag", "desc": "? Gaia DR2 BP-band magnitude (G1) "}, {"name": "e_BPmag", "desc": "? Error on BPmag (1) "}, {"name": "FBP", "desc": "? Gaia DR2 BP-band flux (G1) "}, {"name": "e_FBP", "desc": "? Error on FBP (G1) "}, {"name": "RPmag", "desc": "? Gaia DR2 RP-band magnitude (G1) "}, {"name": "e_RPmag", "desc": "? Error on RPmag (1) "}, {"name": "FRP", "desc": "? Gaia DR2 RP-band flux (G1) "}, {"name": "e_FRP", "desc": "? Error on FRP (G1) "}, {"name": "GaiaGest", "desc": "Estimated DR2 G from spectral type "}, {"name": "plx", "desc": "Gaia DR2 parallax (G1) "}, {"name": "e_plx", "desc": "Error on plx (G1) "}, {"name": "pmRA", "desc": "Gaia DR2 proper motion in right ascension (G1)"}, {"name": "e_pmRA", "desc": "Error on pmRA (G1) "}, {"name": "pmDE", "desc": "Gaia DR2 proper motion in declination (G1) "}, {"name": "e_pmDE", "desc": "Error on pmDE (G1) "}]}, {"name": "table4.dat", "desc": "Objects with published parallax estimates differing by more than 2.5{sigma} with the Gaia DR2 parallax", "columns": [{"name": "ID", "desc": "Short name "}, {"name": "plx", "desc": "Gaia DR2 parallax "}, {"name": "e_plx", "desc": "Error on plx "}, {"name": "plxlit", "desc": "Published parallax "}, {"name": "e_plxlit", "desc": "Error on plxlit "}, {"name": "r_plxlit", "desc": "Reference for plxlit (1) "}]}, {"name": "table5.dat", "desc": "New candidate binary systems containing LT dwarfs, identified in Gaia DR2", "columns": [{"name": "Name", "desc": "Discovery name "}, {"name": "rho", "desc": "? Separation on the sky of the two components "}, {"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2015.5 (G1) "}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2015.5 (G1) "}, {"name": "SpType", "desc": "?=- Spectral type "}, {"name": "Gmag", "desc": "Gaia DR2 G-band magnitude (G1) "}, {"name": "plx", "desc": "Gaia DR2 parallax (G1) "}, {"name": "e_plx", "desc": "Error on plx (G1) "}, {"name": "pmtot", "desc": "Total proper motion "}, {"name": "PApm", "desc": "Position angle of the proper motion "}]}, {"name": "table6.dat", "desc": "J1711+5430 and NLTT 44368 Gaia DR2 parameters ", "columns": [{"name": "ID", "desc": "Short name "}, {"name": "plx", "desc": "Gaia DR2 parallax (G1) "}, {"name": "e_plx", "desc": "Error on plx (G1) "}, {"name": "pmRA", "desc": "Proper motion in right ascension from Gaia DR2 (G1)"}, {"name": "e_pmRA", "desc": "Error on pmRA (G1) "}, {"name": "pmDE", "desc": "Proper motion in declination from Gaia DR2 (G1) "}, {"name": "e_pmDE", "desc": "Error on pmDE (G1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_4726"}} {"id": "J/MNRAS/485/4726", "title_cds": "An all-sky view of the Orphan Stream", "title_create": "Koposov+, 2019", "year": "2019", "author": "Koposov S.E., Belokurov V., Li T.S., Mateu C., Erkal D., Grillmair C.J., Hendel D., Price-Whelan A.M., Laporte C.F.P., Hawkins K., Sohn S.T., del Pino A., Evans N.W., Slater C.T., Kallivayalil N., Navarro J.F., (the Oats: Orphan Aspen Treasury Collaboration)", "title_pub": "Piercing the Milky Way: an all-sky view of the Orphan Stream.", "first_author": "Koposov S.E.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.4726K"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)"], "keyword_cds": "Stars, variable ; Stars, halo ; Positional data ; Stars, distances ; Proper motions", "keyword_pub": "Galaxy: halo - Galaxy: kinematics and dynamics - Galaxy: structure - galaxies: dwarf - galaxies: structure", "abstract": ["We use astrometry, broad-band photometry, and variability information", "from the Data Release 2 of ESA's Gaia mission (GDR2) to identify", "members of the Orphan Stream (OS) across the whole sky. The stream is", "traced above and below the celestial equator and in both Galactic", "hemispheres, thus increasing its visible length to ~210{deg}", "equivalent to ~150kpc in physical extent. Taking advantage of the", "large number of RR Lyrae stars in the OS, we extract accurate", "distances and proper motions across the entire stretch of the tidal", "debris studied. As delineated by the GDR2 RR Lyrae, the stream", "exhibits two prominent twists in its shape on the sky which are", "accompanied by changes in the tangential motion. We complement the RR", "Lyrae maps with those created using GDR2 Red Giants and the DECam", "Legacy Survey Main Sequence Turn-Off stars. The behaviour of the OS", "track on the sky is consistent across all three tracers employed. We", "detect a strong non-zero motion in the across-stream direction for a", "substantial portion of the stream. Such a misalignment between the", "debris track and the streaming velocity cannot be reproduced in a", "static gravitational potential and signals an interaction with a", "massive perturber."], "description": ["We select a high-purity all-sky sample of RRL candidate stars from two", "separate source catalogues released as part of the Gaia DR2 (Gaia", "Collaboration et al. 2018A&A...616A...1G, Cat. I/345). More precisely,", "tables vari classifier result and vari rrlyrae (see Clementini et al.", "2019A&A...622A..60C, Cat. J/A+A/622/A60; Holl et al.", "2018A&A...618A..30H) are joined, removing the duplicates, and the", "stellar astrometry and photometry are obtained from the main gaia", "source catalogue.", "To select the likely Orphan Stream (OS) members, we translate the", "stellar celestial coordinates in equatorial system ({alpha},{delta})", "into a new coordinate system ({Phi}_1_,{Phi}_2_) aligned with the", "stream (see e.g. Koposov et al. 2010ApJ...712..260K). More", "specifically, based on the OS detections reported in Belokurov et al.", "(2007ApJ...658..337B), Grillmair (2006ApJ...645L..37G), and Newberg et", "al. (2010ApJ...711...32N), we use a great circle with a pole at", "({alpha}_OS_,{delta}_OS_)=(72{deg},-14{deg}). The origin of this", "stream's coordinate system is chosen to be at", "({alpha}_0_,{delta}_0_)=(191.10487{deg},-62.86084{deg}), near the", "position where the equator of this coordinate system (and the OS)", "crosses the Galactic plane. We provide the rotation matrix to this", "coordinate system in Appendix B. Finally, {Phi}_1_ increases in the", "direction of the stream's motion, i.e. from the Galactic South to the", "Galactic North."], "data": "", "date_update": "07-Oct-2022", "tables": [{"name": "table1.dat", "desc": "The subset of the likely Orphan RRL selected based on their distance, proper motion, and position on the sky", "columns": [{"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2015.5 (1) "}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2015.5 (1) "}, {"name": "EBV", "desc": "Colour excess E(B-V) "}, {"name": "pmRA", "desc": "Proper motion in right ascension (1) "}, {"name": "e_pmRA", "desc": "Error on pmRA (1) "}, {"name": "pmDE", "desc": "Proper motion in declination (1) "}, {"name": "e_pmDE", "desc": "Error on pmDE (1) "}, {"name": "pmRApmDEcor", "desc": "Correlation between proper motion in right ascension and in declination (1)"}, {"name": "Gmag", "desc": "Gaia DR2 G-band magnitude (1) "}, {"name": "BP-RP", "desc": "Gaia DR2 BP-RP colour index (1) "}, {"name": "E(BR/RP)", "desc": "Gaia DR2 BP/RP excess factor (1) "}, {"name": "Dist", "desc": "Heliocentric distance "}]}, {"name": "table5.dat", "desc": "Adopted light-curve periods and Bailey types for the likely Orphan RRL members", "columns": [{"name": "GaiaDR2", "desc": "Gaia DR2 source identifier "}, {"name": "Period", "desc": "? Light-curve period "}, {"name": "Type", "desc": "Bailey type "}, {"name": "r_Type", "desc": "References for Type (1) "}, {"name": "Note", "desc": "Reference legend (Gaia, PS1 or ThisWork) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_4906"}} {"id": "J/MNRAS/485/4906", "title_cds": "GC number density profiles using Gaia DR2", "title_create": "de Boer+, 2019", "year": "2019", "author": "de Boer T.J.L., Gieles M., Balbinot E., Henault-Brunet V., Sollima A., Watkins L.L., Claydon I.", "title_pub": "Globular cluster number density profiles using Gaia DR2.", "first_author": "de Boer T.J.L.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.4906D"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)"], "keyword_cds": "Models ; Clusters, globular", "keyword_pub": "methods: numerical - stars: kinematics and dynamics - globular clusters: general - galaxies: star clusters", "abstract": ["Using data from Gaia DR2, we study the radial number density profiles", "of the Galactic globular cluster sample. Proper motions are used for", "accurate membership selection, especially crucial in the cluster", "outskirts. Due to the severe crowding in the centres, the Gaia data", "are supplemented by literature data from HST and surface brightness", "measurements, where available. This results in 81 clusters with a", "complete density profile covering the full tidal radius (and beyond)", "for each cluster. We model the density profiles using a set of", "single-mass models ranging from King and Wilson models to generalized", "lowered isothermal LIMEPY models and the recently introduced SPES", "models, which allow for the inclusion of potential escapers. We find", "that both King and Wilson models are too simple to fully reproduce the", "density profiles, with King (Wilson) models on average underestimating", "(overestimating) the radial extent of the clusters. The truncation", "radii derived from the LIMEPY models are similar to estimates for the", "Jacobi radii based on the cluster masses and their orbits. We show", "clear correlations between structural and environmental parameters, as", "a function of Galactocentric radius and integrated luminosity.", "Notably, the recovered fraction of potential escapers correlates with", "cluster pericentre radius, luminosity, and cluster concentration. The", "ratio of half mass over Jacobi radius also correlates with both", "truncation parameter and PE fraction, showing the effect of Roche lobe", "filling."], "description": ["To study the density profiles of Globular Clusters (GCs) we will use", "data from the Gaia mission (Gaia Collaboration et al.", "2018A&A...616A...1G, Cat. I/345), which contains exquisite data for", "about 1.6 billion sources covering the full sky.", "We use the extensive catalogue of GCs from Harris", "(1996AJ....112.1487H, Cat. VII/202) for our input list of targets. To", "avoid regions of excessive crowding where Gaia measurements become", "less reliable, we limit our sample to |b|>5deg, leaving 113 GCs. Each", "of these targets is queried in the Gaia data archive", "(https://gea.esac.esa.int/archive/) using a cone search out to a", "radius of 2.5 times the Jacobi radius (r_J_) determined by Balbinot &", "Gieles (2018MNRAS.474.2479B, Cat. J/MNRAS/474/2479).", "A crucial step in the study of GC density profiles is a reliable", "membership selection. In this work, we first employ a fixed parallax", "cut to remove nearby stars, followed by a selection in", "colour-magnitude space and proper motion space. Following these", "selections, we use the Gaia proper motions to compute the membership", "probability of each star. The proper motion cloud is fit using a", "Gaussian mixture model consisting of one Gaussian for the cluster", "distribution and another for the MW foreground distribution.", "We have fit the combined density profiles using a variety of", "single-mass models, including often-used King (1966AJ.....71...64K)", "and Wilson (1975AJ.....80..175W) models, as well as the recently", "introduced LIMEPY models (https://github.com/mgieles/limepy). Finally,", "we also utilize the recently developed SPES models, which include a", "prescription for the presence of PE stars, essential for reproducing", "the outskirts of GCs."], "data": "", "date_update": "07-Oct-2022", "tables": [{"name": "tableb1.dat", "desc": "Best-fitting parameters of LIMEPY and SPES models fit to 81 GCs", "columns": [{"name": "Name", "desc": "Globular cluster name "}, {"name": "WKing", "desc": "Dimensionless central potential from the King model fit"}, {"name": "e_WKing", "desc": "Error on WKing "}, {"name": "rtKing", "desc": "Tidal radius from the King model fit "}, {"name": "e_rtKing", "desc": "Error on rtKing "}, {"name": "WWil", "desc": "Dimensionless central potential from the Wilson model fit"}, {"name": "e_WWil", "desc": "Error on WWil "}, {"name": "rtWil", "desc": "Tidal radius from the Wilson model fit "}, {"name": "e_rtWil", "desc": "Error on rtWil "}, {"name": "WLime", "desc": "Dimensionless central potential from the Limepy model fit"}, {"name": "e_WLime", "desc": "Error on WLime "}, {"name": "gLime", "desc": "Truncation parameter from the Limepy model fit"}, {"name": "e_gLime", "desc": "Error on gLime "}, {"name": "rhLime", "desc": "Half-mass radius from the Limepy model fit "}, {"name": "e_rhLime", "desc": "Error on rhLime "}, {"name": "rtLime", "desc": "Tidal radius from the Limepy model fit "}, {"name": "e_rtLime", "desc": "Error on rtLime "}, {"name": "WSPES", "desc": "Dimensionless central potential from the SPES model fit"}, {"name": "e_WSPES", "desc": "Error on WSPES "}, {"name": "etaSPES", "desc": "{eta} parameter from the spherical potential escapers (SPES) stitched models fit (1)"}, {"name": "e_etaSPES", "desc": "Error on etaSPES "}, {"name": "log1B", "desc": "Logarithm of 1-B, with parameter B coming from the SPES model fit (2)"}, {"name": "e_log1B", "desc": "Error on log1B "}, {"name": "rhSPES", "desc": "Half-mass radius from the SPES model fit "}, {"name": "e_rhSPES", "desc": "Error on rhSPES "}, {"name": "rtSPES", "desc": "Tidal radius from the SPES model fit "}, {"name": "e_rtSPES", "desc": "Error on rtSPES "}, {"name": "logfPE", "desc": "Logarithm of the fraction of potential escapers (PEs) recovered in the SPES best"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_5153"}} {"id": "J/MNRAS/485/5153", "title_cds": "Spectroscopy of extremely metal-poor stars", "title_create": "Marino+, 2019", "year": "2019", "author": "Marino A.F., Da Costa G.S., Casey A.R., Asplund M., Bessell M.S., Frebel A., Keller S.C., Lind K., Mackey A.D., Murphy S.J., Nordlander T., Norris J.E., Schmidt B.P., Yong D.", "title_pub": "Keck HIRES spectroscopy of SkyMapper commissioning survey candidate extremely metal-poor stars.", "first_author": "Marino A.F.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.5153M"], "see_also": ["J/ApJ/807/171 : SkyMapper Survey metal-poor star spectroscopy", "II/358 : SkyMapper Southern Sky Survey. DR1.1 (Wolf+, 2018)"], "keyword_cds": "Abundances ; Stars, population II ; Stars, metal-deficient ; Spectroscopy", "keyword_pub": "stars: abundances - stars: Population II - Galaxy: halo - Galaxy: stellar content", "abstract": ["We present results from the analysis of high-resolution spectra", "obtained with the Keck HIRES spectrograph for a sample of 17 candidate", "extremely metal-poor (EMP) stars originally selected from", "commissioning data obtained with the SkyMapper telescope. Fourteen of", "the stars have not been observed previously at high dispersion. Three", "have [Fe/H]=<-3.0, while the remainder, with two more metal-rich", "exceptions, have -3.0=<[Fe/H]=<-2.0dex. Apart from Fe, we also derive", "abundances for the elements C, N, Na, Mg, Al, Si, Ca, Sc, Ti, Cr, Mn,", "Co, Ni, and Zn, and for n-capture elements Sr, Ba, and Eu. None of the", "current sample of stars is found to be carbon-rich. In general, our", "chemical abundances follow previous trends found in the literature,", "although we note that two of the most metal-poor stars show very low", "[Ba/Fe] (~-1.7) coupled with low [Sr/Ba] (~-0.3). Such stars are", "relatively rare in the Galactic halo. One further star, and possibly", "two others, meet the criteria for classification as a r-I star. This", "study, together with that of Jacobson et al. (2015ApJ...807..171J,", "Cat. J/ApJ/807/171), completes the outcomes of the SkyMapper", "commissioning data survey for EMP stars."], "description": ["The candidates observed with the HIRES spectrograph (Vogt et al.", "1994SPIE.2198..362V) at the Keck-I telescope were those in the", "commissioning survey EMP candidate sample that had not been previously", "observed at high dispersion (cf. Jacobson et al. 2015ApJ...807..171J,", "Cat. J/ApJ/807/171), which were accessible from the Keck Observatory", "on the scheduled date and which had low-resolution spectroscopic", "abundance estimates [Fe/H]_2.3m_=<-2.5dex, as determined from the 2.3m", "spectra. In all, HIRES spectra were obtained for 15 candidate EMP", "stars on the ANU-allocated night of 2013 September 21 (UT), together", "with spectra of two stars that had also been observed at Magellan with", "the MIKE spectrograph in the Jacobson et al. (2015ApJ...807..171J,", "Cat. J/ApJ/807/171) study. One further star, SMSS J221334.13-072604.1,", "was subsequently found to be included in the sample analysed by Aoki", "et al. (2013AJ....145...13A, Cat. J/AJ/145/13) under the designation", "SDSS J2213-0726.", "Observing conditions were good with the seeing slowly rising from 0.6", "to 1arcsec by the end of the night. The spectrograph was configured", "with the HIRESb cross-disperser and the C1 decker that has a slit", "width of 0.86arcsec yielding a resolution R~50000. Detector binning", "was 2(spatial)x1(spectral) and the low-gain setting (~2e^-^/DN) was", "used for the three CCDs in the detector mosaic. Details of the", "observations are given in Table 1. The table lists the SkyMapper", "survey designations, the positions, and the SkyMapper g, (g-i)_0_ and", "m_i_ photometry taken from the SkyMapper DR1.1 data release (Wolf et", "al. 2018PASA...35...10W, Cat. II/358), which supersede the original", "commissioning-era photometry."], "data": "", "date_update": "10-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Details of the target stars and the Keck HIRES observations", "columns": [{"name": "Name", "desc": "SkyMapper identifier (SMSS JHHMMSS.ss+DDMMSS.s) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "gmag", "desc": "SkyMapper g-band magnitude "}, {"name": "g-i", "desc": "g-i colour index "}, {"name": "mi", "desc": "Metallicity index (1) "}, {"name": "Texp", "desc": "Integration time "}, {"name": "S/N450", "desc": "Signal to noise ratio per pixel at 450nm "}, {"name": "S/N600", "desc": "Signal to noise ratio per pixel at 600nm "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "Notes", "desc": "? Previous observations (2) "}]}, {"name": "table2.dat", "desc": "Adopted atmospheric parameters ", "columns": [{"name": "Name", "desc": "SkyMapper identifier (SMSS JHHMMSS.ss+DDMMSS.s)"}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "[Fe/H]LTE", "desc": "LTE Iron to hydrogen abundance ratio "}, {"name": "[Fe/H]nLTE", "desc": "Iron to hydrogen abundance ratio obtained by applying non-LTE corrections to FeI lines"}, {"name": "vt", "desc": "Microturbulence velocity "}]}, {"name": "table3.dat", "desc": "Atomic data and EWs for program stars ", "columns": [{"name": "Name", "desc": "SkyMapper identifier (SMSS JHHMMSS.ss+DDMMSS.s) "}, {"name": "wvl", "desc": "Wavelenghts of the spectral lines used in the abundance analysis"}, {"name": "Species", "desc": "Chemical species analysed "}, {"name": "EP", "desc": "Excitational potentials "}, {"name": "loggf", "desc": "Total oscillator strengths employed "}, {"name": "EW", "desc": "Measured equivalent widths "}]}, {"name": "table4.dat", "desc": "Chemical abundance ratios for the light elements C, N, Na, and Al", "columns": [{"name": "Name", "desc": "SkyMapper identifier (SMSS JHHMMSS.ss+DDMMSS.s)"}, {"name": "[C/Fe]", "desc": "C to iron abundance ratio "}, {"name": "e_[C/Fe]", "desc": "Error on [C/Fe] "}, {"name": "o_[C/Fe]", "desc": "Number of spectral features analysed for [C/Fe]"}, {"name": "[C/Fe]evol", "desc": "Evolutionary corrected [C/Fe] abundance (1) "}, {"name": "[N/Fe]", "desc": "? N to iron abundance ratio "}, {"name": "e_[N/Fe]", "desc": "? Error on [N/Fe] "}, {"name": "o_[N/Fe]", "desc": "? Number of spectral features analysed for [N/Fe]"}, {"name": "[Na/Fe]LTE", "desc": "LTE [Na/Fe] abundance "}, {"name": "e_[Na/Fe]LTE", "desc": "Error on [Na/Fe]LTE "}, {"name": "[Na/Fe]nLTE", "desc": "non-LTE [Na/Fe] abundance "}, {"name": "e_[Na/Fe]nLTE", "desc": "Error on [Na/Fe]nLTE "}, {"name": "o_[Na/Fe]LTE", "desc": "Number of spectral features analysed for [Na/Fe]LTE"}, {"name": "[Al/Fe]", "desc": "? Al to iron abundance ratio "}, {"name": "e_[Al/Fe]", "desc": "? Error on [Al/Fe] "}, {"name": "o_[Al/Fe]", "desc": "? Number of spectral features analysed for [Al/Fe]"}]}, {"name": "table5.dat", "desc": "Chemical abundances for {alpha} elements, Mg, Si, Ca, and Ti", "columns": [{"name": "Name", "desc": "SkyMapper identifier (SMSS JHHMMSS.ss+DDMMSS.s) "}, {"name": "[Mg/Fe]", "desc": "Mg to iron abundance ratio "}, {"name": "e_[Mg/Fe]", "desc": "Error on [Mg/Fe] "}, {"name": "o_[Mg/Fe]", "desc": "Number of spectral features analysed for [Mg/Fe]"}, {"name": "[Si/Fe]", "desc": "Si to iron abundance ratio "}, {"name": "e_[Si/Fe]", "desc": "? Error on [Si/Fe] "}, {"name": "o_[Si/Fe]", "desc": "Number of spectral features analysed for [Si/Fe]"}, {"name": "[Ca/Fe]", "desc": "? Ca to iron abundance ratio "}, {"name": "e_[Ca/Fe]", "desc": "? Error on [Ca/Fe] "}, {"name": "o_[Ca/Fe]", "desc": "? Number of spectral features analysed for [Ca/Fe]"}, {"name": "[TiI/Fe]", "desc": "? TiI to iron abundance ratio "}, {"name": "e_[TiI/Fe]", "desc": "? Error on [TiI/Fe] "}, {"name": "o_[TiI/Fe]", "desc": "? Number of spectral features analysed for [TiI/Fe]"}, {"name": "[TiII/Fe]", "desc": "TiII to iron abundance ratio "}, {"name": "f_[TiII/Fe]", "desc": "? Flag on [TiII/Fe] (1) "}, {"name": "e_[TiII/Fe]", "desc": "Error on [TiII/Fe] "}, {"name": "o_[TiII/Fe]", "desc": "Number of spectral features analysed for [TiII/Fe]"}]}, {"name": "table6.dat", "desc": "Chemical abundances for FeI and FeII, and Fe-peak elements Sc (ScII), Cr, Mn, Co, Ni, and Zn", "columns": [{"name": "Name", "desc": "SkyMapper identifier (SMSS JHHMMSS.ss+DDMMSS.s)"}, {"name": "[FeI/H]", "desc": "FeI to hydrogen abundance ratio "}, {"name": "e_[FeI/H]", "desc": "Error on [FeI/H] "}, {"name": "o_[FeI/H]", "desc": "Number of spectral features analysed for [FeI/H]"}, {"name": "[FeII/H]", "desc": "? FeII to iron abundance ratio "}, {"name": "e_[FeII/H]", "desc": "? Error on [FeII/H] "}, {"name": "o_[FeII/H]", "desc": "? Number of spectral features analysed for [FeII/H]"}, {"name": "[Sc/Fe]", "desc": "? Sc to iron abundance ratio "}, {"name": "e_[Sc/Fe]", "desc": "? Error on [Sc/Fe] "}, {"name": "o_[Sc/Fe]", "desc": "? Number of spectral features analysed for [Sc/Fe]"}, {"name": "[CrI/Fe]", "desc": "? CrI to iron abundance ratio "}, {"name": "e_[CrI/Fe]", "desc": "? Error on [CrI/Fe] "}, {"name": "o_[CrI/Fe]", "desc": "? Number of spectral features analysed for [CrI/Fe]"}, {"name": "[CrII/Fe]", "desc": "? CrII to iron abundance ratio "}, {"name": "o_[CrII/Fe]", "desc": "? Number of spectral features analysed for [CrII/Fe]"}, {"name": "[Mn/Fe]", "desc": "Mn to iron abundance ratio "}, {"name": "e_[Mn/Fe]", "desc": "Error on [Mn/Fe] "}, {"name": "o_[Mn/Fe]", "desc": "Number of spectral features analysed for [Mn/Fe]"}, {"name": "[Co/Fe]", "desc": "? Co to iron abundance ratio "}, {"name": "e_[Co/Fe]", "desc": "? Error on [Co/Fe] "}, {"name": "o_[Co/Fe]", "desc": "? Number of spectral features analysed for [Co/Fe]"}, {"name": "[Ni/Fe]", "desc": "? Ni to iron abundance ratio "}, {"name": "e_[Ni/Fe]", "desc": "? Error on [Ni/Fe] "}, {"name": "o_[Ni/Fe]", "desc": "? Number of spectral features analysed for [Ni/Fe]"}, {"name": "[Zn/Fe]", "desc": "? Zn to iron abundance ratio "}, {"name": "e_[Zn/Fe]", "desc": "? Error on [Zn/Fe] "}, {"name": "o_[Zn/Fe]", "desc": "? Number of spectral features analysed for [Zn/Fe]"}]}, {"name": "table7.dat", "desc": "Chemical abundances for the n-capture elements, Sr, Ba, and Eu", "columns": [{"name": "Name", "desc": "SkyMapper identifier (SMSS JHHMMSS.ss+DDMMSS.s)"}, {"name": "[Sr/Fe]", "desc": "Sr to iron abundance ratio "}, {"name": "e_[Sr/Fe]", "desc": "Error on [Sr/Fe] "}, {"name": "o_[Sr/Fe]", "desc": "Number of spectral features analysed for [Sr/Fe]"}, {"name": "l_[Ba/Fe]", "desc": "Limit flag on [Ba/Fe] "}, {"name": "[Ba/Fe]", "desc": "Ba to iron abundance ratio "}, {"name": "e_[Ba/Fe]", "desc": "Error on [Ba/Fe] "}, {"name": "o_[Ba/Fe]", "desc": "Number of spectral features analysed for [Ba/Fe]"}, {"name": "l_[Eu/Fe]", "desc": "Limit flag on [Eu/Fe] "}, {"name": "[Eu/Fe]", "desc": "Eu to iron abundance ratio "}, {"name": "e_[Eu/Fe]", "desc": "? Error on [Eu/Fe] "}, {"name": "o_[Eu/Fe]", "desc": "? Number of spectral features analysed for [Eu/Fe]"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_5345"}} {"id": "J/MNRAS/485/5345", "title_cds": "Finding black holes with black boxes", "title_create": "Askar+, 2019", "year": "2019", "author": "Askar A., Askar A., Pasquato M., Giersz M.", "title_pub": "Finding black holes with black boxes - using machine learning to identify globular clusters with black hole subsystems.", "first_author": "Askar A.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.5345A"], "see_also": ["VII/202 : Globular Clusters in the Milky Way (Harris, 1997)", "J/MNRAS/478/1520 : Milky Way globular clusters data (Baumgardt+, 2018)"], "keyword_cds": "Black holes ; Clusters, globular ; Models", "keyword_pub": "methods: data analysis - methods: numerical - methods: statistical - stars: black holes - globular clusters: general", "abstract": ["Machine learning is a powerful technique, becoming increasingly", "popular in astrophysics. In this paper, we apply machine learning to", "more than a thousand globular cluster (GC) models simulated with the", "MOCCA-Survey Database I project in order to correlate present-day", "observable properties with the presence of a subsystem of stellar mass", "black holes (BHs). The machine learning model is then applied to", "available observed parameters for Galactic GCs to identify which of", "them that are most likely to be hosting a sizeable number of BHs and", "reveal insights into what properties lead to the formation of BH", "subsystems. With our machine learning model, we were able to shortlist", "18 Galactic GCs that are most likely to contain a BH subsystem. We", "show that the clusters shortlisted by the machine learning classifier", "include those in which BH candidates have been observed (M22, M10, and", "NGC 3201) and that our results line up well with independent", "simulations and previous studies that manually compared simulated GC", "models with observed properties of Galactic GCs. These results can be", "useful for observers searching for elusive stellar mass BH candidates", "in GCs and further our understanding of the role BHs play in GC", "evolution. In addition, we have released an online tool that allows", "one to get predictions from our model after they input observable", "properties."], "description": ["For the purpose of this study, we used results from numerical", "simulations of GC models that were carried out using the MOCCA code", "(Hypki & Giersz 2013MNRAS.429.1221H; Giersz et al.", "2013MNRAS.429.1221H) as part of the MOCCA-Survey Database I (Askar et", "al. 2017MNRAS.464L..36A) project. MOCCA is a code for simulating star", "clusters based on Henon's implementation of the Monte Carlo method", "(Henon 1971Ap&SS..14..151H; Stodolkiewicz 1982AcA....32...63S,", "1986AcA....36...19S) to follow the long-term dynamical evolution of", "spherically symmetric stellar clusters.", "In this work, we applied machine learning in a new and novel way to", "astrophysics: predicting real world properties based on simulations.", "An empirical comparison was performed between multiple classifiers", "with the guiding metric primarily being a low false positive rate", "(F-score). We successfully trained a fairly accurate gradient boosted", "decision tree classifier on simulation data and then applied the", "learned model on to real world data. K-fold testing with our", "simulation data showed that the model had an accuracy of 95 per cent", "and a false positive rate of less than 1 per cent. Moreover, applying", "the classifier on an independent set of simulations (N-body versus", "Monte Carlo) yielded accurate results as well, a classifier trained on", "MOCCA Monte Carlo simulations was able to accurately predict the", "presence of BHS in N-body (Wang et al. 2016MNRAS.458.1450W) simulated", "clusters using just the observational properties.", "Applied on to real world data, our results are also fairly", "encouraging. We ran our model on two different catalogues of Milky Way", "GCs in order to get predictions based on independent data sets. We", "managed to successfully identify several clusters which have been", "ascertained to contain BHs by previous observational studies."], "data": "", "date_update": "11-Oct-2022", "tables": [{"name": "tablea1.dat", "desc": "Predictions for the presence of BHSs with data from the Harris (1996AJ....112.1487H, Cat. VII/202) catalogue", "columns": [{"name": "Name", "desc": "Cluster name "}, {"name": "R50", "desc": "Half-light radius "}, {"name": "CSB", "desc": "Central surface brightness "}, {"name": "CVD", "desc": "? Central velocity dispersion "}, {"name": "f_CVD", "desc": "Flag on CVD (1) "}, {"name": "TVL", "desc": "Total V-band luminosity "}, {"name": "HMRT", "desc": "Half-mass relaxation time "}, {"name": "Rad", "desc": "Core radius "}, {"name": "BHSpred", "desc": "[False/True ] Predictions for the presence of Black Hole Subsystems (BHS) from the"}]}, {"name": "tablea2.dat", "desc": "Predictions for the presence of BHSs with data from Baumgardt & Hilker (2018MNRAS.478.1520B, Cat. J/MNRAS/478/1520) catalogue for Milky Way GC parameters", "columns": [{"name": "Name", "desc": "Cluster name "}, {"name": "R50", "desc": "Half-light radius "}, {"name": "CSB", "desc": "Central surface brightness "}, {"name": "CVD", "desc": "Central velocity dispersion "}, {"name": "TVL", "desc": "Total V-band luminosity "}, {"name": "HMRT", "desc": "Half-mass relaxation time "}, {"name": "Rad", "desc": "Core radius "}, {"name": "BHSpred", "desc": "[False/True ] Predictions for the presence of Black Hole Subsystems (BHS) from the"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_5573"}} {"id": "J/MNRAS/485/5573", "title_cds": "Gaia-DR2 100pc white dwarf population", "title_create": "Torres+, 2019", "year": "2019", "author": "Torres S., Cantero C., Rebassa-Mansergas A., Skorobogatov G., Jimenez-Esteban F.M., Solano E.", "title_pub": "Random Forest identification of the thin disc, thick disc, and halo Gaia-DR2 white dwarf population.", "first_author": "Torres S.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.5573T"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)"], "keyword_cds": "Stars, white dwarf ; Populations, stellar ; Milky Way ; Models", "keyword_pub": "stars: luminosity function - mass function - white dwarfs - Galaxy: stellar content", "abstract": ["Gaia-DR2 has provided an unprecedented number of white dwarf", "candidates of our Galaxy. In particular, it is estimated that Gaia-DR2", "has observed nearly 400000 of these objects and close to 18000 up to", "100pc from the Sun. This large quantity of data requires a thorough", "analysis in order to uncover their main Galactic population", "properties, in particular the thin and thick disc and halo components.", "Taking advantage of recent developments in artificial intelligence", "techniques, we make use of a detailed Random Forest algorithm to", "analyse an 8D space (equatorial coordinates, parallax, proper motion", "components, and photometric magnitudes) of accurate data provided by", "Gaia-DR2 within 100pc from the Sun. With the aid of a thorough and", "robust population synthesis code, we simulated the different", "components of the Galactic white dwarf population to optimize the", "information extracted from the algorithm for disentangling the", "different population components. The algorithm is first tested in a", "known simulated sample achieving an accuracy of 85.3 per cent. Our", "methodology is thoroughly compared to standard methods based on", "kinematic criteria demonstrating that our algorithm substantially", "improves previous approaches. Once trained, the algorithm is then", "applied to the Gaia-DR2 100pc white dwarf sample, identifying 12227", "thin disc, 1410 thick disc, and 95 halo white dwarf candidates, which", "represent a proportion of 74:25:1, respectively. Hence, the numerical", "spatial densities are (3.6+/-0.4)x10^-3^pc^-3^,", "(1.2+/-0.4)x10^-3^pc^-3^, and (4.8+/-0.4)x10^-5^pc^-3^ for the thin", "disc, thick disc, and halo components, respectively. The populations", "thus obtained represent the most complete and volume-limited samples", "to date of the different components of the Galactic white dwarf", "population."], "description": ["We have identified 12227 thin disc, 1410 thick disc, and 95 halo white", "dwarf candidates belonging to the Gaia 100pc sample (Jimenez-Esteban", "et al. 2018MNRAS.480.4505J, Cat. J/MNRAS/480/4505) by means of an", "accurate Random Forest algorithm (Breiman 2001MachL..45....5B). The", "unprecedented wealth of valuable information provided to the", "scientific community by the Gaia-DR2 (Gaia Collaboration", "2018A&A...616A...1G, Cat. I/345) and, in particular, the quantity and", "quality of their data related to the white dwarf population requires", "the application of novel artificial intelligence matching learning", "algorithms in order to extract the maximum information. To this aim we", "used a supervised Random Forest algorithm to disentangle the different", "white dwarf Galactic populations given its flexibility and low number", "of input parameters. The algorithm has been applied to an 8D space", "that includes astrometric as well as photometric values for each", "object. With the aid of a thorough population synthesis model, we", "accurately reproduce the characteristics of a standard three-component", "Galactic model. The synthetic population is used for the training of", "the classification algorithm as well as a testbed for assessing its", "accuracy."], "data": "", "date_update": "11-Oct-2022", "tables": [{"name": "table3.dat", "desc": "Halo white dwarf candidates within 100 pc identified by our Random Forest algorithm", "columns": [{"name": "GaiaDR2", "desc": "Gaia DR2 source identifier "}, {"name": "Name", "desc": "Star name in equatorial coordinate format "}, {"name": "pmRA", "desc": "Gaia DR2 proper motion in right ascension (pmRA*cosDE)"}, {"name": "pmDE", "desc": "Gaia DR2 proper motion in declination "}, {"name": "Dist", "desc": "Distance "}, {"name": "Gmag", "desc": "Gaia DR2 g-bang magnitude "}, {"name": "GMag", "desc": "Absolute G-band magnitude "}, {"name": "BP-RP", "desc": "Gaia DR2 BP-RP colour index "}, {"name": "Vtan", "desc": "Tangential velocity "}, {"name": "Ref", "desc": "?=- References where the source has already been identified as a halo member (1)"}]}, {"name": "g100pcwd.dat", "desc": "Gaia 100 pc White Dwarf sample ", "columns": [{"name": "---", "desc": "[Gaia DR2] "}, {"name": "GaiaDR2", "desc": "Gaia DR2 source identifier "}, {"name": "Name", "desc": "Star name in equatorial coordinate format "}, {"name": "RN", "desc": "Random number "}, {"name": "RAdeg", "desc": "Right ascension (ICRS) at Ep=2015.5 "}, {"name": "DEdeg", "desc": "Declination (ICRS) at Ep=2015.5 "}, {"name": "plx", "desc": "Parallax "}, {"name": "pmRA", "desc": "Gaia DR2 proper motion in right ascension (pmRA*cosDE)"}, {"name": "pmDE", "desc": "Gaia DR2 proper motion in declination "}, {"name": "Gmag", "desc": "Gaia DR2 g-band magnitude "}, {"name": "BPmag", "desc": "Gaia DR2 BP-band magnitude "}, {"name": "RPmag", "desc": "Gaia DR2 RP-band magnitude "}, {"name": "BP-RP", "desc": "Gaia DR2 BP-RP colour index "}, {"name": "BP-G", "desc": "Gaia DR2 BP-G colour index "}, {"name": "G-RP", "desc": "Gaia DR2 G-RP colour index "}, {"name": "GMag", "desc": "Absolute G-band magnitude "}, {"name": "U", "desc": "U component of space velocity "}, {"name": "V", "desc": "V component of space velocity "}, {"name": "W", "desc": "W component of space velocity "}, {"name": "Pop", "desc": "Galactic component classification (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_5616"}} {"id": "J/MNRAS/485/5616", "title_cds": "Red giant solar-like oscillations in Kepler data", "title_create": "Hon+, 2019", "year": "2019", "author": "Hon M., Stello D., Garcia R.A., Mathur S., Sharma S., Colman I.L., Bugnet L.", "title_pub": "A search for red giant solar-like oscillations in all Kepler data.", "first_author": "Hon M.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.5616H"], "see_also": ["J/ApJ/866/99 : Revised radii of KIC stars & planets using Gaia DR2", "J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)"], "keyword_cds": "Stars, giant ; Asteroseismology ; Stars, diameters", "keyword_pub": "asteroseismology - methods: data analysis - techniques: image processing - stars: oscillations - stars: statistics", "abstract": ["The recently published Kepler mission Data Release 25 (DR25) reported", "on ~197000 targets observed during the mission. Despite this, no wide", "search for red giants showing solar-like oscillations have been made", "across all stars observed in Kepler's long-cadence mode. In this work,", "we perform this task using custom apertures on the Kepler pixel files", "and detect oscillations in 21914 stars, representing the largest", "sample of solar-like oscillating stars to date. We measure their", "frequency at maximum power, {nu}_max_, down to {nu}_max_~=4{mu}Hz and", "obtain log(g) estimates with a typical uncertainty below 0.05dex,", "which is superior to typical measurements from spectroscopy.", "Additionally, the {nu}_max_ distribution of our detections show good", "agreement with results from a simulated model of the Milky Way, with a", "ratio of observed to predicted stars of 0.992 for stars with", "10<{nu}_max_<270{mu}Hz. Among our red giant detections, we find 909 to", "be dwarf/subgiant stars whose flux signal is polluted by a", "neighbouring giant as a result of using larger photometric apertures", "than those used by the NASA Kepler science processing pipeline. We", "further find that only 293 of the polluting giants are known Kepler", "targets. The remainder comprises over 600 newly identified oscillating", "red giants, with many expected to belong to the Galactic halo,", "serendipitously falling within the Kepler pixel files of targeted", "stars."], "description": ["From all 196581 Kepler stars observed in long cadence, we detected", "21914 stars showing solar-like oscillations with our deep learning", "classifier, yielding the current largest list of stars showing", "solar-like oscillations that will provide many more targets of", "interest for various asteroseismic and Galactic archaeology analyses.", "We also predict {nu}_max_ for each detection, which will provide", "useful prior values for more precise measurements using asteroseismic", "model-fitting pipelines. In addition, our {nu}_max_ values provide", "log(g) estimates, for which ~88 per cent are good to within 0.05dex,", "which is still superior to typical spectroscopic log(g)", "determinations.", "From our list of 21914 detections, we identified 21005 Kepler targets", "with Gaia-derived radii representative of red giants. Even though we", "do not account for giants with R>~40R_{sun}_, our number of detections", "is within estimates of the total number of red giants (~21000) as", "reported by Berger et al. (2018ApJ...866...99B, Cat. J/ApJ/866/99)", "(B18) because we also detect giant oscillations in stars with", "R~<10R_{sun}_ that they classified as subgiants. We also found 1671", "stars with R=<40R_{sun}_ that are predicted as non-detections but have", "been classified as red giants by Berger et al. (2018ApJ...866...99B,", "Cat. J/ApJ/866/99)."], "data": "", "date_update": "12-Oct-2022", "tables": [{"name": "table1.dat", "desc": "Kepler long-cadence stars showing red giant solar-like oscillations", "columns": [{"name": "Name", "desc": "KIC object identifier (NNNNNNNN) (G1) "}, {"name": "p", "desc": "?=-99 Detection probability (1) "}, {"name": "e_p", "desc": "?=-99 Error on p (1) "}, {"name": "numax", "desc": "Frequency at maximum power of the star "}, {"name": "e_numax", "desc": "Error on numax "}, {"name": "logg", "desc": "?=-99 Surface gravity (2) "}, {"name": "e_logg", "desc": "?=-99 Error on logg (2) "}, {"name": "f_Name", "desc": "Flag on name (3) "}]}, {"name": "table2.dat", "desc": "A list of blended targets, each assigned with the identity of its polluting star", "columns": [{"name": "Name", "desc": "KIC object identifier (NNNNNNNN) (G1) "}, {"name": "Poll", "desc": "?=-99 Polluting star ID "}, {"name": "f_Poll", "desc": "Flag on Poll (1) "}]}, {"name": "tablea1.dat", "desc": "A list of Kepler targets with radii, R, smaller than 40R_{sun}_ that are predicted to not show giant oscillations but are classified as red giants by Berger et al. (2018ApJ...866...99B, Cat. J/ApJ/866/99)", "columns": [{"name": "Name", "desc": "KIC object identifier (NNNNNNNN) (G1) "}, {"name": "Radius", "desc": "Star radius adopted from the Berger et al. (2018ApJ...866...99B, Cat. J/ApJ/866/99)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_485_5790"}} {"id": "J/MNRAS/485/5790", "title_cds": "Short Title", "title_create": "Turner+, 2019", "year": "2019", "author": "Turner O.D., Anderson D.R., Barkaoui K., Bouchy F., Benkhaldoun Z., Brown D.J.A., Burdanov A., Collier Cameron A., Ducrot E., Gillon M., Hellier C., Jehin E., Lendl M., Maxted P.F.L., Nielsen L.D., Pepe F., Pollacco D., Pozuelos F.J., Queloz D., Segransan D., Smalley B., Triaud A.H.M.J., Udry S., West R.G.", "title_pub": "Three hot-Jupiters on the upper edge of the mass-radius distribution: WASP-177, WASP-181, and WASP-183.", "first_author": "Turner O.D.", "ref_biblio": [""], "bibcode": ["2019MNRAS.485.5790T"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "12-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_486_21"}} {"id": "J/MNRAS/486/21", "title_cds": "Quasar Sightline and Galaxy Evolution Survey I", "title_create": "Bielby+, 2019", "year": "2019", "author": "Bielby R.M., Stott J.P., Cullen F., Tripp T.M., Burchett J.N., Fumagalli M., Morris S.L., Tejos N., Crain R.A., Bower R.G., Prochaska J.X.", "title_pub": "Quasar Sightline and Galaxy Evolution (QSAGE) survey - I. The galaxy environment of O VI absorbers up to z = 1.4 around PKS 0232-04.", "first_author": "Bielby R.M.", "ref_biblio": [""], "bibcode": ["2019MNRAS.486...21B"], "keyword_cds": "Galaxies, optical ; Galaxies, IR ; Intergalactic medium ; QSOs ; Redshifts", "keyword_pub": "galaxies: distances and redshifts - intergalactic medium - quasars: absorption lines", "abstract": ["We present the first results from a study of OVI absorption around", "galaxies at z<1.44 using data from a near-infrared grism spectroscopic", "Hubble Space Telescope Large Programme, the Quasar Sightline and", "Galaxy Evolution (QSAGE) survey. QSAGE is the first grism galaxy", "survey to focus on the circumgalactic medium at z~1, providing a blind", "survey of the galaxy population. The galaxy sample is H{alpha} flux", "limited (f(H{alpha})>2x10^-17^erg.s^-1^cm^-2^) at 0.68~0.2-0.8M_{sun}_yr^-1^. In this first of 12 fields,", "we combine the galaxy data with high-resolution STIS and COS", "spectroscopy of the background quasar to study OVI in the", "circumgalactic medium. At z~1, we find OVI absorption systems up to", "b~350kpc (~4R_vir_) from the nearest detected galaxy. Further, we find", "~50 per cent of >~1M_{sun}_yr^-1^ star-forming galaxies within 2R_vir_", "show no associated OVI absorption to a limit of at least", "N(OVI)=10^13.9^cm^-2^. That we detect OVI at such large distances from", "galaxies and that a significant fraction of star-forming galaxies show", "no detectable OVI absorption disfavours outflows from ongoing star", "formation as the primary medium traced by these absorbers. Instead, by", "combining our own low- and high-redshift data with existing samples,", "we find tentative evidence for many strong (N(OVI)>10^14^cm^-2^) OVI", "absorption systems to be associated with M_*_~10^9.5-10^M_{sun}_ mass", "galaxies (M_halo_~10^11.5-12^M_{sun}_ dark matter haloes), and infer", "that they may be tracing predominantly collisionally ionized gas", "within the haloes of such galaxies."], "description": ["The Quasar Sightline and Galaxy Evolution (QSAGE) survey targets 12", "z>~1.2 quasars with the aim of mapping and characterizing the galaxy", "populations in their foregrounds (HST Large Programme 14594; PIs: R.", "Bielby, J. P. Stott). The full survey consists of 96 orbits with the", "WFC3 in imaging and grism mode (i.e. 8 h per quasar sightline). In", "this paper we focus on the first field to be fully analysed, centred", "on the z=1.44 quasar PKS 0232-04, chosen due to the extensive data", "available to complement the WFC3 grism and STIS sightline data:", "Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) optical imaging", "(Cuillandre et al. 2012SPIE.8448E..0MC), MUSE IFU data (MUSE Program", "(096.A-0222, PI: Schaye)) and HST/COS sightline spectroscopy (CASBaH,", "HST Programs 11741 and 13846, PI: T. Tripp).", "Table 4 provides names, coordinates, and measured and derived", "properties for galaxies found as part of the QSAGE survey in close", "proximity to the quasar sightline of PKS 0232-04 (aka PHL 1377)."], "data": "", "date_update": "13-Oct-2022", "tables": [{"name": "table4.dat", "desc": "Properties of proximate galaxies to the quasar sightline", "columns": [{"name": "Name", "desc": "Galaxy name (QSAGE JHHMMSS.ss+DDMMSS.s) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "F140Wmag", "desc": "HST/WFC3 F140W filter AB magnitude "}, {"name": "e_F140Wmag", "desc": "Error on F140Wmag "}, {"name": "z", "desc": "Redshift "}, {"name": "b", "desc": "Impact parameter to QSO sightline "}, {"name": "logMass", "desc": "Logarithm of galaxy stellar mass "}, {"name": "e_logMass", "desc": "Lower error on logMass "}, {"name": "E_logMass", "desc": "Upper error on logMass "}, {"name": "logMhalo", "desc": "Logarithm of halo mass "}, {"name": "e_logMhalo", "desc": "Lower error on logMhalo "}, {"name": "E_logMhalo", "desc": "Upper error on logMhalo "}, {"name": "Rvir", "desc": "Virial radius "}, {"name": "e_Rvir", "desc": "Lower error on Rvir "}, {"name": "E_Rvir", "desc": "Upper error on Rvir "}, {"name": "logSFR", "desc": "Star formation rate "}, {"name": "e_logSFR", "desc": "Lower error on logSFR "}, {"name": "E_logSFR", "desc": "Upper error on logSFR "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_486_175"}} {"id": "J/MNRAS/486/175", "title_cds": "HiZELS star-forming galaxies at z=0.8-3.3", "title_create": "Gillman+, 2019", "year": "2019", "author": "Gillman S., Swinbank A.M., Tiley A.L., Harrison C.M., Smail I., Dudzeviciute U., Sharples R.M., Best P.N., Bower R.G., Cochrane R., Fisher D., Geach J.E., Glazebrook K., Ibar E., Molina J., Obreschkow D., Schaller M., Sobral D., Sweet S., Trayford J.W., Theuns T.", "title_pub": "The dynamics and distribution of angular momentum in HiZELS star-forming galaxies at z=0.8-3.3.", "first_author": "Gillman S.", "ref_biblio": [""], "bibcode": ["2019MNRAS.486..175G"], "keyword_cds": "Galaxies, spectra ; Redshifts ; Rotational velocities ; Morphology", "keyword_pub": "galaxies: evolution - galaxies: high redshift - galaxies: kinematics and dynamics", "abstract": ["We present adaptive optics assisted integral field spectroscopy of 34", "star-forming galaxies at z=0.8-3.3 selected from the HiZELS", "narrow-band survey. We measure the kinematics of the ionized", "interstellar medium on ~1kpc scales, and show that the galaxies are", "turbulent, with a median ratio of rotational to dispersion support of", "V/{sigma}=0.82+/-0.13. We combine the dynamics with high-resolution", "rest-frame optical imaging and extract emission-line rotation curves.", "We show that high-redshift star-forming galaxies follow a similar", "power-law trend in specific angular momentum with stellar mass to that", "of local late-type galaxies. We exploit the high resolution of our", "data and examine the radial distribution of angular momentum within", "each galaxy by constructing total angular momentum profiles. Although", "the stellar mass of a typical star-forming galaxy is expected to grow", "by a factor ~8 in the ~5Gyr between z~3.3 and z~0.8, we show that the", "internal distribution of angular momentum becomes less centrally", "concentrated in this period; that is, the angular momentum grows", "outwards. To interpret our observations, we exploit the EAGLE", "simulation and trace the angular momentum evolution of star-forming", "galaxies from z~3 to z~0, identifying a similar trend of decreasing", "angular momentum concentration. This change is attributed to a", "combination of gas accretion in the outer disc, and feedback that", "preferentially arises from the central regions of the galaxy. We", "discuss how the combination of the growing bulge and angular momentum", "stabilizes the disc and gives rise to the Hubble sequence."], "description": ["The majority of the observations (31 targets; 90 per cent of the", "sample) were obtained from follow-up spectroscopic observations of the", "High Redshift Emission Line Survey (HiZELS; Geach et al.", "2008MNRAS.388.1473G; Best et al. 2013ASSP...37..235B), which targets", "H{alpha}-emitting galaxies in five narrow ({Delta}z=0.03) redshift", "slices: z=0.40, 0.84, 1.47, 2.23, and 3.33 (Sobral et al.", "2013MNRAS.428.1128S, Cat. J/MNRAS/428/1128). This panoramic survey", "provides a luminosity-limited sample of H{alpha} and [OIII] emitters", "spanning z=0.4-3.3. The other 3 galaxies were taken from the KMOS", "Galaxy Evolution Survey (KGES; Tiley et al. 2021MNRAS.506..323T), a", "sample of ~300 star-forming galaxies at z~1.5.", "Exploiting the wide survey area, the targets from the HiZELS survey", "were selected to lie within 25.0arcsec of a natural guide star to", "allow for adaptive optics capabilities. The sample spans the full", "range of the rest-frame (U-V) and rest-frame (V-J) colour space as", "well as the stellar mass and star formation rate plane of the HiZELS", "parent sample (Table A1). The data were collected from 2012 August to", "2017 December from a series of observing runs on the SINFONI (VLT),", "NIFS (Gemini North Observatory), and OSIRIS (Keck) integral field", "spectrographs (see Table B1 for details). Finally, a summary of the", "morphological properties for our sample is shown in Table C1."], "data": "", "date_update": "13-Oct-2022", "tables": [{"name": "tablea1.dat", "desc": "Integrated galaxy properties ", "columns": [{"name": "Name", "desc": "Galaxy name (SHIZELS-NN) "}, {"name": "r_OName", "desc": "? References for OName (1) "}, {"name": "OName", "desc": "Previously published name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "z", "desc": "Spectroscopic redshift (2) "}, {"name": "Hmag", "desc": "? H-band AB magnitude (3) "}, {"name": "logMass", "desc": "Logarithm of galaxy stellar mass (3) "}, {"name": "SFR", "desc": "Star formation rate (3) "}, {"name": "e_SFR", "desc": "Error on SFR "}]}, {"name": "tableb1.dat", "desc": "Integrated field observations ", "columns": [{"name": "Name", "desc": "Galaxy name (SHIZELS-NN) "}, {"name": "z", "desc": "Spectroscopic H{alpha} or [OIII] redshift derived from spectrum"}, {"name": "EGF", "desc": "Extra-galactic Field "}, {"name": "Band", "desc": "Wavelength band used for spectroscopic observation"}, {"name": "IFU", "desc": "Integral Field Spectrograph used for spectroscopic observation"}, {"name": "f_IFU", "desc": "Flag on IFU (1) "}, {"name": "texp", "desc": "Total on source integration time of integral field observations"}, {"name": "PSF", "desc": "Integral field PSF size as measured from standard star observations"}, {"name": "Broadband", "desc": "Ancillary photometric data available for each target"}]}, {"name": "tablec1.dat", "desc": "Morpho-kinematic properties ", "columns": [{"name": "Name", "desc": "Galaxy name (SHIZELS-NN) "}, {"name": "Rh", "desc": "Half-light radius "}, {"name": "e_Rh", "desc": "Error on Rh "}, {"name": "n", "desc": "Sersic index "}, {"name": "e_n", "desc": "Error on n "}, {"name": "b/a", "desc": "Semiminor to semimajor axis ratio "}, {"name": "e_b/a", "desc": "Error on b/a "}, {"name": "thetai", "desc": "Inclination (1) "}, {"name": "e_thetai", "desc": "Error on thetai "}, {"name": "PAvel", "desc": "Kinematic position angle "}, {"name": "e_PAvel", "desc": "Error on PAvel "}, {"name": "Vrot", "desc": "Beam-smearing-corrected rotation velocity at r=2Rh"}, {"name": "e_Vrot", "desc": "Error on Vrot "}, {"name": "Vcirc/Vrot", "desc": "Circular velocity to rotational velocity ratio at r=2Rh"}, {"name": "sig", "desc": "Velocity dispersion "}, {"name": "e_sig", "desc": "Error on sig "}, {"name": "Vrot/sig", "desc": "Rotational velocity to velocity dispersion ratio"}, {"name": "e_Vrot/sig", "desc": "Error on Vrot/sig "}, {"name": "Quality", "desc": "Qualify flag based on kinematic criteria (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_486_251"}} {"id": "J/MNRAS/486/251", "title_cds": "Short Title", "title_create": "Deacon+, 2019", "year": "2019", "author": "Deacon N.R., Henning T., Kossakowski D.E.", "title_pub": "Data-driven stellar parameters for southern TESS FGK targets.", "first_author": "Deacon N.R.", "ref_biblio": [""], "bibcode": ["2019MNRAS.486..251D"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "13-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_486_378"}} {"id": "J/MNRAS/486/378", "title_cds": "BHB stars reveal halo's metal-rich progenitor", "title_create": "Lancaster+, 2019", "year": "2019", "author": "Lancaster L., Koposov S.E., Belokurov V., Evans N.W., Deason A.J.", "title_pub": "The halo's ancient metal-rich progenitor revealed with BHB stars.", "first_author": "Lancaster L.", "ref_biblio": [""], "bibcode": ["2019MNRAS.486..378L"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "V/139 : The SDSS Photometric Catalog, Release 8", "J/ApJ/738/79 : SDSS-DR8 BHB stars in the Milky Way's halo (Xue+, 2011)"], "keyword_cds": "Milky Way ; Stars, halo ; Stars, blue ; Stars, horizontal branch ; Proper motions ; Radial velocities ; Stars, distances ; Photometry, SDSS", "keyword_pub": "Galaxy: formation - Galaxy: halo - Galaxy: kinematics and dynamics", "abstract": ["Using the data from the Sloan Digital Sky Survey and the Gaia", "satellite, we assemble a pure sample of ~3000 blue horizontal branch", "(BHB) stars with 7D information, including positions, velocities, and", "metallicities. We demonstrate that, as traced with BHBs, the Milky", "Way's stellar halo is largely unmixed and cannot be well represented", "with a conventional Gaussian velocity distribution. A single-component", "model fails because the inner portions of the halo are swamped with", "metal-rich tidal debris from an ancient, head-on collision, known as", "the 'Gaia Sausage'. Motivated by the data, we build a flexible mixture", "model that allows us to track the evolution of the halo make-up across", "a wide range of radii. It is built from two components, one", "representing the radially anisotropic Sausage stars with their lobed", "velocity distribution, and the other representing a more metal-poor", "and more isotropic component built up from minor mergers. We show that", "inside 25kpc the 'Sausage' contributes at least 50 per cent of the", "Galactic halo. The fraction of 'Sausage' stars diminishes sharply", "beyond 30kpc, which is the long-established break radius of the", "classical stellar halo."], "description": ["We aim to measure the evolution of the velocity ellipsoid of the Milky", "Way's stellar halo as a function of Galactocentric radius. To do this,", "we need 3D kinematic information for a large sample of stars in the", "stellar halo. We supplement the proper motion measurements of the Gaia", "satellite (Gaia Collaboration 2018A&A...616A...1G, Cat. I/345) with", "spectroscopic radial velocity and photometric distance relations for a", "large sample of BHB stars.", "Our initial sample consists of a catalogue of 4985 BHB stars compiled", "by Xue et al. (2011ApJ...738...79X, Cat. J/ApJ/738/79). These stars", "were selected using spectroscopic and photometric information from the", "SEGUE-1, SEGUE-2, and older SDSS surveys and the data was publicly", "released as part of SDSS DR8 (Aihara et al. 2011ApJS..193...29A, Cat.", "V/139).", "We provide a new catalogue of the BHB stars that we use in this study", "with all of the information that we have derived here. We give a file", "that use all of our selections to remove BS contaminants and stars", "with poor spectroscopic or astrometric data (table bhball, 3680", "sources), as well as a file that additionally removes the Sagittarius", "stream (table bhbfilt, 3064 sources)."], "data": "", "date_update": "14-Oct-2022", "tables": [{"name": "bhball.dat", "desc": "Blue Horizontal Branch stars in the Stellar Halo of the Milky Way", "columns": [{"name": "RAdeg", "desc": "Right ascension (ICRS) Ep=2015.5 (1) "}, {"name": "e_RAdeg", "desc": "Error on RAdeg (1) "}, {"name": "DEdeg", "desc": "Declination (ICRS) Ep=2015.5 (1) "}, {"name": "e_DEdeg", "desc": "Error on DEdeg (1) "}, {"name": "pmRA", "desc": "Proper motion in right ascension (pmRA*cosDE) (1)"}, {"name": "e_pmRA", "desc": "Error on pmRA "}, {"name": "pmDE", "desc": "Proper motion in declination (1) "}, {"name": "e_pmDE", "desc": "Error on pmDE "}, {"name": "pmRApmDEcor", "desc": "Correlation between pmRA and pmDE (1) "}, {"name": "RV", "desc": "Heliocentric radial velocity (2) "}, {"name": "e_RV", "desc": "Error on RV (2) "}, {"name": "logDist", "desc": "Logarithm of the heliocentric distance to the star (4)"}, {"name": "e_logDist", "desc": "Error on logDist (4) "}, {"name": "[Fe/H]", "desc": "Iron to hydrogen abundance ratio relative to solar (3)"}, {"name": "e_[Fe/H]", "desc": "Error on [Fe/H] (3) "}, {"name": "umag", "desc": "SDSS PSF magnitude in u-band (3) "}, {"name": "e_umag", "desc": "Error on umag (3) "}, {"name": "gmag", "desc": "SDSS PSF magnitude in g-band (3) "}, {"name": "e_gmag", "desc": "Error on gmag (3) "}, {"name": "rmag", "desc": "SDSS PSF magnitude in r-band (3) "}, {"name": "e_rmag", "desc": "Error on rmag (3) "}, {"name": "Au", "desc": "Dust extinction in the u-band (3) "}, {"name": "Ag", "desc": "Dust extinction in the g-band (3) "}, {"name": "Ar", "desc": "Dust extinction in the r-band (3) "}, {"name": "bHg", "desc": "Line width of the H{gamma} line of the star (2)"}, {"name": "cHg", "desc": "Line shape of the H{gamma} line of the star (2)"}, {"name": "epsi", "desc": "Astrometric excess noise from Gaia DR2 (1)"}, {"name": "sepsi", "desc": "Astrometric excess noise significance (1)"}, {"name": "plx", "desc": "Parallax (1) "}, {"name": "e_plx", "desc": "Error on plx (1) "}, {"name": "pmRAplxcor", "desc": "Correlation between pmRA and plx (1) "}, {"name": "pmDEplxcor", "desc": "Correlation between pmDE and plx (1) "}, {"name": "Rgal", "desc": "Galactocentric radial distance (4) "}, {"name": "varRgal", "desc": "Variance in the measurement of Rgal (4) "}, {"name": "Vlon", "desc": "Galactocentric longitudinal velocity (4) "}, {"name": "varVlon", "desc": "Variance in the measurement of Vlon (4) "}, {"name": "Vlat", "desc": "Galactocentric latitudinal velocity (4) "}, {"name": "varVlat", "desc": "Variance in the measurement of Vlat (4) "}, {"name": "RVgal", "desc": "Galactocentric radial velocity (4) "}, {"name": "RVgalvar", "desc": "Variance in the measurement of RVgal (4) "}, {"name": "RgalVloncov", "desc": "Covariance between Rgal and Vlon (4) "}, {"name": "RgalVlatcov", "desc": "Covariance between Rgal and Vlat (4) "}, {"name": "RgalRVgalcov", "desc": "Covariance between Rgal and RVgal (4) "}, {"name": "VlonVlatcov", "desc": "Covariance between Vlon and Vlat (4) "}, {"name": "VlonRVgalcov", "desc": "Covariance between Vlon and RVgal (4) "}, {"name": "VlatRVgalcov", "desc": "Covariance between Vlat and RVgal (4) "}, {"name": "VRA", "desc": "Physical space velocity in the direction of increasing right ascension (4)"}, {"name": "VRAvar", "desc": "Variance in the measurement of VRA (4) "}, {"name": "VDE", "desc": "Physical space velocity in the direction of increasing declination (4)"}, {"name": "vDEvar", "desc": "Variance in the measurement of VDE (4) "}, {"name": "VRAVDEcov", "desc": "Covariance between VRA and VDE (4) "}]}, {"name": "bhbfilt.dat", "desc": "Blue Horizontal Branch stars in the Stellar Halo of the Milky Way (Sagittarius stream removed)", "columns": [{"name": "RAdeg", "desc": "Right ascension (ICRS) Ep=2015.5 (1) "}, {"name": "e_RAdeg", "desc": "Error on RAdeg (1) "}, {"name": "DEdeg", "desc": "Declination (ICRS) Ep=2015.5 (1) "}, {"name": "e_DEdeg", "desc": "Error on DEdeg (1) "}, {"name": "pmRA", "desc": "Proper motion in right ascension (pmRA*cosDE) (1)"}, {"name": "e_pmRA", "desc": "Error on pmRA "}, {"name": "pmDE", "desc": "Proper motion in declination (1) "}, {"name": "e_pmDE", "desc": "Error on pmDE "}, {"name": "pmRApmDEcor", "desc": "Correlation between pmRA and pmDE (1) "}, {"name": "RV", "desc": "Heliocentric radial velocity (2) "}, {"name": "e_RV", "desc": "Error on RV (2) "}, {"name": "logDist", "desc": "Logarithm of the heliocentric distance to the star (4)"}, {"name": "e_logDist", "desc": "Error on logDist (4) "}, {"name": "[Fe/H]", "desc": "Iron to hydrogen abundance ratio relative to solar (3)"}, {"name": "e_[Fe/H]", "desc": "Error on [Fe/H] (3) "}, {"name": "umag", "desc": "SDSS PSF magnitude in u-band (3) "}, {"name": "e_umag", "desc": "Error on umag (3) "}, {"name": "gmag", "desc": "SDSS PSF magnitude in g-band (3) "}, {"name": "e_gmag", "desc": "Error on gmag (3) "}, {"name": "rmag", "desc": "SDSS PSF magnitude in r-band (3) "}, {"name": "e_rmag", "desc": "Error on rmag (3) "}, {"name": "Au", "desc": "Dust extinction in the u-band (3) "}, {"name": "Ag", "desc": "Dust extinction in the g-band (3) "}, {"name": "Ar", "desc": "Dust extinction in the r-band (3) "}, {"name": "bHg", "desc": "Line width of the H{gamma} line of the star (2)"}, {"name": "cHg", "desc": "Line shape of the H{gamma} line of the star (2)"}, {"name": "epsi", "desc": "Astrometric excess noise from Gaia DR2 (1)"}, {"name": "sepsi", "desc": "Astrometric excess noise significance (1)"}, {"name": "plx", "desc": "Parallax (1) "}, {"name": "e_plx", "desc": "Error on plx (1) "}, {"name": "pmRAplxcor", "desc": "Correlation between pmRA and plx (1) "}, {"name": "pmDEplxcor", "desc": "Correlation between pmDE and plx (1) "}, {"name": "Rgal", "desc": "Galactocentric radial distance (4) "}, {"name": "varRgal", "desc": "Variance in the measurement of Rgal (4) "}, {"name": "Vlon", "desc": "Galactocentric longitudinal velocity (4) "}, {"name": "varVlon", "desc": "Variance in the measurement of Vlon (4) "}, {"name": "Vlat", "desc": "Galactocentric latitudinal velocity (4) "}, {"name": "varVlat", "desc": "Variance in the measurement of Vlat (4) "}, {"name": "RVgal", "desc": "Galactocentric radial velocity (4) "}, {"name": "RVgalvar", "desc": "Variance in the measurement of RVgal (4) "}, {"name": "RgalVloncov", "desc": "Covariance between Rgal and Vlon (4) "}, {"name": "RgalVlatcov", "desc": "Covariance between Rgal and Vlat (4) "}, {"name": "RgalRVgalcov", "desc": "Covariance between Rgal and RVgal (4) "}, {"name": "VlonVlatcov", "desc": "Covariance between Vlon and Vlat (4) "}, {"name": "VlonRVgalcov", "desc": "Covariance between Vlon and RVgal (4) "}, {"name": "VlatRVgalcov", "desc": "Covariance between Vlat and RVgal (4) "}, {"name": "VRA", "desc": "Physical space velocity in the direction of increasing right ascension (4)"}, {"name": "VRAvar", "desc": "Variance in the measurement of VRA (4) "}, {"name": "VDE", "desc": "Physical space velocity in the direction of increasing declination (4)"}, {"name": "vDEvar", "desc": "Variance in the measurement of VDE (4) "}, {"name": "VRAVDEcov", "desc": "Covariance between VRA and VDE (4) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_486_390"}} {"id": "J/MNRAS/486/390", "title_cds": "Morphology of 16908 SDSS Stripe 82 galaxies", "title_create": "Bottrell+, 2019", "year": "2019", "author": "Bottrell C., Simard L., Mendel J.T., Ellison S.L.", "title_pub": "Bulge plus disc and Sersic decomposition catalogues for 16 908 galaxies in the SDSS Stripe 82 co-adds: a detailed study of the ugriz structural measurements.", "first_author": "Bottrell C.", "ref_biblio": [""], "bibcode": ["2019MNRAS.486..390B"], "see_also": ["II/294 : The SDSS Photometric Catalog, Release 7", "J/ApJ/794/120 : Sloan Digital Sky Survey coadd. Stripe 82 (Annis+, 2014)", "J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies (Simard+, 2011)", "J/ApJS/142/1 : DEEP Groth Strip Survey. II. (Simard+, 2002)"], "keyword_cds": "Galaxy catalogs ; Galaxies, optical ; Morphology ; Photometry, SDSS", "keyword_pub": "catalogues - surveys - galaxies: general - galaxies: photometry - galaxies: fundamental parameters - galaxies: structure", "abstract": ["Quantitative characterization of galaxy morphology is vital in", "enabling comparison of observations to predictions from galaxy", "formation theory. However, without significant overlap between the", "observational footprints of deep and shallow galaxy surveys, the", "extent to which structural measurements for large galaxy samples are", "robust to image quality (e.g. depth and spatial resolution) cannot be", "established. Deep images from the Sloan Digital Sky Survey (SDSS)", "Stripe 82 co-adds provide a unique solution to this problem - offering", "1.6-1.8mag improvement in depth with respect to SDSS Legacy images.", "Having similar spatial resolution to Legacy, the co-adds make it", "possible to examine the sensitivity of parametric morphologies to", "depth alone. Using the gim2d surface-brightness decomposition", "software, we provide public morphology catalogues for 16908 galaxies", "in the Stripe 82 ugriz co-adds. Our methods and selection are", "completely consistent with the Simard et al. (2011ApJS..196...11S,", "Cat. J/ApJS/196/11) and Mendel et al. (2014ApJS..210....3M, Cat.", "J/ApJS/210/3) photometric decompositions. We rigorously compare", "measurements in the deep and shallow images. We find no systematics in", "total magnitudes and sizes except for faint galaxies in the u band and", "the brightest galaxies in each band. However, characterization of", "bulge-to-total fractions is significantly improved in the deep images.", "Furthermore, statistics used to determine whether single-Sersic or", "two-component (e.g. bulge+disc) models are required become more", "bimodal in the deep images. Lastly, we show that asymmetries are", "enhanced in the deep images and that the enhancement is positively", "correlated with the asymmetries measured in Legacy images."], "description": ["SDSS Legacy imaging was performed with the dedicated 2.5-m wide-field", "telescope at Apache Point Observatory (APO) in New Mexico (Abazajian", "et al. 2009ApJS..182..543A, Cat. II/294). A total of around", "45000deg^2^ of science quality images across five broad bands (ugriz)", "were produced during operation and calibrated to the AB magnitude", "system (Oke & Gunn 1983ApJ...266..713O). DR7 imaging is complimented", "by a 640-fibre-fed pair of multi-object double spectrographs with", "coverage from 3800 to 9200{AA} at a resolution of", "{lambda}/{Delta}{lambda}~2000.", "The SDSS Stripe 82 (Annis et al. 2014ApJ...794..120A, Cat.", "J/ApJ/794/120) resides at 1.25{deg}<{delta}<+1.25{deg},", "-50{deg}<{alpha}<+60{deg} along the celestial equator in the Southern", "Galactic Cap. Repeated imaging runs of Stripe 82 were carried out to", "enable stacking of images and reach fainter magnitudes.", "We select galaxies from the SDSS DR7 spectroscopic galaxy catalogue", "that are previously analysed by Simard et al. (2011ApJS..196...11S,", "Cat. J/ApJS/196/11) (S11) and which reside in Stripe 82. This provides", "a sample of 16908 galaxies for which decompositions in the deeper", "images can be directly compared with the more shallow reference", "decompositions from S11. We avoid misclassified non-galaxy sources in", "our galaxy sample by selecting targets determined to be galaxies from", "SDSS fibre spectroscopy. Consequently, we have spectroscopic redshifts", "for all galaxies in our sample.", "Using images constructed from multiple exposures of 275deg^2^ in the", "SDSS Stripe 82, which permit an additional 1.6-1.8mag of depth with", "respect to single-exposure SDSS Legacy images, we have performed", "free-n_b_ and n_b_=4bulge+exp.disc (fn and n4) as well as", "single-component Sersic ps decompositions on 16908 galaxies -", "obtaining parametric morphologies in the u, g, r, i, z bands.", "Twelve tables are released in total - one for each unique combination", "of model and Xr-band pairing."], "data": "", "date_update": "21-Oct-2022", "tables": [{"name": "s82grfn.dat", "desc": "Stripe 82 galaxy morphology catalogue for the fn model and a gr-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band "}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length "}, {"name": "radd", "desc": "Disc scale length "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle "}, {"name": "PAd", "desc": "Disc position angle "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle "}, {"name": "e_dxg", "desc": "(16-50)% range of dxg "}, {"name": "dxg", "desc": "Model centroid offset from PHOTO x on the g-band"}, {"name": "E_dxg", "desc": "(50-84)% range of dxg "}, {"name": "e_dyg", "desc": "(16-50)% range of dyg "}, {"name": "dyg", "desc": "Model centroid offset from PHOTO y on the g-band"}, {"name": "E_dyg", "desc": "(50-84)% range of dyg "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82grn4.dat", "desc": "Stripe 82 galaxy morphology catalogue for the n4 model and a gr-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band "}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length "}, {"name": "radd", "desc": "Disc scale length "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle "}, {"name": "PAd", "desc": "Disc position angle "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle "}, {"name": "e_dxg", "desc": "(16-50)% range of dxg "}, {"name": "dxg", "desc": "Model centroid offset from PHOTO x on the g-band"}, {"name": "E_dxg", "desc": "(50-84)% range of dxg "}, {"name": "e_dyg", "desc": "(16-50)% range of dyg "}, {"name": "dyg", "desc": "Model centroid offset from PHOTO y on the g-band"}, {"name": "E_dyg", "desc": "(50-84)% range of dyg "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82grps.dat", "desc": "Stripe 82 galaxy morphology catalogue for the ps model and a gr-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr (G9) "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band (G9)"}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr (G9) "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length (G9)"}, {"name": "radd", "desc": "Disc scale length (G9) "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length (G9)"}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination (G9) "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) (G9) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination (G9) "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle (G9)"}, {"name": "PAd", "desc": "Disc position angle (G9) "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle (G9)"}, {"name": "e_dxg", "desc": "(16-50)% range of dxg "}, {"name": "dxg", "desc": "Model centroid offset from PHOTO x on the g-band"}, {"name": "E_dxg", "desc": "(50-84)% range of dxg "}, {"name": "e_dyg", "desc": "(16-50)% range of dyg "}, {"name": "dyg", "desc": "Model centroid offset from PHOTO y on the g-band"}, {"name": "E_dyg", "desc": "(50-84)% range of dyg "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82irfn.dat", "desc": "Stripe 82 galaxy morphology catalogue for the fn model and a ir-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band"}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band "}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length "}, {"name": "radd", "desc": "Disc scale length "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle "}, {"name": "PAd", "desc": "Disc position angle "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle "}, {"name": "e_dxi", "desc": "(16-50)% range of dxi "}, {"name": "dxi", "desc": "Model centroid offset from PHOTO x on the i-band"}, {"name": "E_dxi", "desc": "(50-84)% range of dxi "}, {"name": "e_dyi", "desc": "(16-50)% range of dyi "}, {"name": "dyi", "desc": "Model centroid offset from PHOTO y on the i-band"}, {"name": "E_dyi", "desc": "(50-84)% range of dyi "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82irn4.dat", "desc": "Stripe 82 galaxy morphology catalogue for the n4 model and a ir-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band "}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length "}, {"name": "radd", "desc": "Disc scale length "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle "}, {"name": "PAd", "desc": "Disc position angle "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle "}, {"name": "e_dxi", "desc": "(16-50)% range of dxi "}, {"name": "dxi", "desc": "Model centroid offset from PHOTO x on the i-band"}, {"name": "E_dxi", "desc": "(50-84)% range of dxi "}, {"name": "e_dyi", "desc": "(16-50)% range of dyi "}, {"name": "dyi", "desc": "Model centroid offset from PHOTO y on the i-band"}, {"name": "E_dyi", "desc": "(50-84)% range of dyi "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82irps.dat", "desc": "Stripe 82 galaxy morphology catalogue for the ps model and a ir-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr (G9) "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band (G9)"}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr (G9) "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius "}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius "}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length (G9) "}, {"name": "radd", "desc": "Disc scale length (G9) "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length (G9) "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination (G9) "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) (G9) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination (G9) "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle (G9)"}, {"name": "PAd", "desc": "Disc position angle (G9) "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle (G9)"}, {"name": "e_dxi", "desc": "(16-50)% range of dxi "}, {"name": "dxi", "desc": "Model centroid offset from PHOTO x on the i-band"}, {"name": "E_dxi", "desc": "(50-84)% range of dxi "}, {"name": "e_dyi", "desc": "(16-50)% range of dyi "}, {"name": "dyi", "desc": "Model centroid offset from PHOTO y on the i-band"}, {"name": "E_dyi", "desc": "(50-84)% range of dyi "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1) "}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82urfn.dat", "desc": "Stripe 82 galaxy morphology catalogue for the fn model and a ur-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band "}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length "}, {"name": "radd", "desc": "Disc scale length "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle "}, {"name": "PAd", "desc": "Disc position angle "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle "}, {"name": "e_dxu", "desc": "(16-50)% range of dxu "}, {"name": "dxu", "desc": "Model centroid offset from PHOTO x on the u-band"}, {"name": "E_dxu", "desc": "(50-84)% range of dxu "}, {"name": "e_dyu", "desc": "(16-50)% range of dyu "}, {"name": "dyu", "desc": "Model centroid offset from PHOTO y on the u-band"}, {"name": "E_dyu", "desc": "(50-84)% range of dyu "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82urn4.dat", "desc": "Stripe 82 galaxy morphology catalogue for the n4 model and a ur-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band "}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length "}, {"name": "radd", "desc": "Disc scale length "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle "}, {"name": "PAd", "desc": "Disc position angle "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle "}, {"name": "e_dxu", "desc": "(16-50)% range of dxu "}, {"name": "dxu", "desc": "Model centroid offset from PHOTO x on the u-band"}, {"name": "E_dxu", "desc": "(50-84)% range of dxu "}, {"name": "e_dyu", "desc": "(16-50)% range of dyu "}, {"name": "dyu", "desc": "Model centroid offset from PHOTO y on the u-band"}, {"name": "E_dyu", "desc": "(50-84)% range of dyu "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82urps.dat", "desc": "Stripe 82 galaxy morphology catalogue for the ps model and a ur-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr (G9) "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band (G9)"}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr (G9) "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length (G9)"}, {"name": "radd", "desc": "Disc scale length (G9) "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length (G9)"}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination (G9) "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) (G9) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination (G9) "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle (G9)"}, {"name": "PAd", "desc": "Disc position angle (G9) "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle (G9)"}, {"name": "e_dxu", "desc": "(16-50)% range of dxu "}, {"name": "dxu", "desc": "Model centroid offset from PHOTO x on the u-band"}, {"name": "E_dxu", "desc": "(50-84)% range of dxu "}, {"name": "e_dyu", "desc": "(16-50)% range of dyu "}, {"name": "dyu", "desc": "Model centroid offset from PHOTO y on the u-band"}, {"name": "E_dyu", "desc": "(50-84)% range of dyu "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82zrfn.dat", "desc": "Stripe 82 galaxy morphology catalogue for the fn model and a zr-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "? (50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band "}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length "}, {"name": "radd", "desc": "Disc scale length "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle "}, {"name": "PAd", "desc": "Disc position angle "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle "}, {"name": "e_dxz", "desc": "(16-50)% range of dxz "}, {"name": "dxz", "desc": "Model centroid offset from PHOTO x on the z-band"}, {"name": "E_dxz", "desc": "(50-84)% range of dxz "}, {"name": "e_dyz", "desc": "(16-50)% range of dyz "}, {"name": "dyz", "desc": "Model centroid offset from PHOTO y on the z-band"}, {"name": "E_dyz", "desc": "(50-84)% range of dyz "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82zrn4.dat", "desc": "Stripe 82 galaxy morphology catalogue for the n4 model and a zr-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude"}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band "}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius"}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius"}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length "}, {"name": "radd", "desc": "Disc scale length "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle "}, {"name": "PAd", "desc": "Disc position angle "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle "}, {"name": "e_dxz", "desc": "(16-50)% range of dxz "}, {"name": "dxz", "desc": "Model centroid offset from PHOTO x on the z-band"}, {"name": "E_dxz", "desc": "(50-84)% range of dxz "}, {"name": "e_dyz", "desc": "(16-50)% range of dyz "}, {"name": "dyz", "desc": "Model centroid offset from PHOTO y on the z-band"}, {"name": "E_dyz", "desc": "(50-84)% range of dyz "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1)"}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}, {"name": "s82zrps.dat", "desc": "Stripe 82 galaxy morphology catalogue for the ps model and a zr-band decomposition", "columns": [{"name": "S82ID", "desc": "Stripe 82 object identifier "}, {"name": "SDSSID", "desc": "SDSS DR7 object identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "run", "desc": "Stripe 82 run: South-106, North-206 "}, {"name": "rerun", "desc": "Processing/calibration identifier "}, {"name": "camcol", "desc": "CCD camera column "}, {"name": "field", "desc": "Stripe 82 field "}, {"name": "fieldID", "desc": "Object ID within given field "}, {"name": "rPmag", "desc": "SDSS Petrosian apparent r-band magnitude "}, {"name": "Ar", "desc": "Galactic extinction (r-band) "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "Nx", "desc": "Size of science cut-out x "}, {"name": "Ny", "desc": "Size of science cut-out y "}, {"name": "prcHost", "desc": "Processing host (decomposition) "}, {"name": "prcStart", "desc": "Processing start-time "}, {"name": "prcEnd", "desc": "Processing end-time "}, {"name": "e_Fr", "desc": "(16-50)% range of Fr "}, {"name": "Fr", "desc": "Galaxy total flux on the r-band "}, {"name": "E_Fr", "desc": "(50-84)% range of Fr "}, {"name": "e_rmag", "desc": "(16-50)% range of rmag "}, {"name": "rmag", "desc": "Galaxy apparent magnitude on the r-band "}, {"name": "E_rmag", "desc": "(50-84)% range of rmag "}, {"name": "e_B/Tr", "desc": "(16-50)% range of B/Tr (G9) "}, {"name": "B/Tr", "desc": "Bulge-to-total fraction on the r-band (G9)"}, {"name": "E_B/Tr", "desc": "(50-84)% range of B/Tr (G9) "}, {"name": "e_radb", "desc": "(16-50)% range of bulge effective radius "}, {"name": "radb", "desc": "Bulge effective radius "}, {"name": "E_radb", "desc": "(50-84)% range of bulge effective radius "}, {"name": "e_be", "desc": "(16-50)% range of bulge ellipticity "}, {"name": "be", "desc": "Bulge ellipticity "}, {"name": "E_be", "desc": "(50-84)% range of bulge ellipticity "}, {"name": "e_PAb", "desc": "(16-50)% range of bulge position angle "}, {"name": "PAb", "desc": "Bulge position angle "}, {"name": "E_PAb", "desc": "(50-84)% range of bulge position angle "}, {"name": "e_radd", "desc": "(16-50)% range of disc scale length (G9) "}, {"name": "radd", "desc": "Disc scale length (G9) "}, {"name": "E_radd", "desc": "(50-84)% range of disc scale length (G9) "}, {"name": "e_inc", "desc": "(16-50)% range of disc inclination (G9) "}, {"name": "inc", "desc": "Disc inclination, b/a=cos(inc) (G9) "}, {"name": "E_inc", "desc": "(50-84)% range of disc inclination (G9) "}, {"name": "e_PAd", "desc": "(16-50)% range of disc position angle (G9)"}, {"name": "PAd", "desc": "Disc position angle (G9) "}, {"name": "E_PAd", "desc": "(50-84)% range of disc position angle (G9)"}, {"name": "e_dxz", "desc": "(16-50)% range of dxz "}, {"name": "dxz", "desc": "Model centroid offset from PHOTO x on the z-band"}, {"name": "E_dxz", "desc": "(50-84)% range of dxz "}, {"name": "e_dyz", "desc": "(16-50)% range of dyz "}, {"name": "dyz", "desc": "Model centroid offset from PHOTO y on the z-band"}, {"name": "E_dyz", "desc": "(50-84)% range of dyz "}, {"name": "e_bkr", "desc": "(16-50)% range of bkr "}, {"name": "bkr", "desc": "(GIM2D-SExtractor) residual background on the r-band"}, {"name": "E_bkr", "desc": "(50-84)% range of bkr "}, {"name": "e_n", "desc": "(16-50)% range of sersic index "}, {"name": "n", "desc": "Sersic index "}, {"name": "E_n", "desc": "(50-84)% range of sersic index "}, {"name": "hlrr", "desc": "Galaxy half-light radius on the r-band "}, {"name": "chi2r", "desc": "Reduced chi-squared statistic on the r-band"}, {"name": "c1r", "desc": "? Concentration parameter within 1 hlrr on the r-band (G1)"}, {"name": "c2r", "desc": "? Concentration parameter within 2 hlrr on the r-band (G1)"}, {"name": "c3r", "desc": "? Concentration parameter within 3 hlrr on the r-band (G1)"}, {"name": "c4r", "desc": "? Concentration parameter within 4 hlrr on the r-band (G1)"}, {"name": "asymr", "desc": "? Asymmetry parameter on the r-band (G1) "}, {"name": "e_asymr", "desc": "? Error on asymr "}, {"name": "Az21r", "desc": "? Simard et al. (2002ApJS..142....1S, Cat. J/ApJS/142/1) Az parameter for"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_486_1034"}} {"id": "J/MNRAS/486/1034", "title_cds": "O stars of the Galactic starburst NGC 3603", "title_create": "Drew+, 2019", "year": "2019", "author": "Drew J.E., Monguio M., Wright N.J.", "title_pub": "The O star hinterland of the Galactic starburst, NGC 3603.", "first_author": "Drew J.E.", "ref_biblio": [""], "bibcode": ["2019MNRAS.486.1034D"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/MNRAS/465/1807 : Deep OB star population in Carina (Mohr-Smith+, 2017)"], "keyword_cds": "Stars, O ; Stars, early-type ; Clusters, open ; Positional data ; Proper motions ; Effective temperatures ; Optical", "keyword_pub": "proper motions - stars: early-type - stars: massive - open clusters and associations: individual: NGC 3603", "abstract": ["The very bright and compact massive young cluster, NGC 3603, has been", "cited as an example of a starburst in the Milky Way and compared with", "the much-studied R136/30 Doradus region in the Large Magellanic Cloud.", "Here we build on the discovery by Mohr-Smith et al. of a large number", "of reddened O stars around this cluster. We construct a list of 288", "candidate O stars with proper motions (PMs), in a region of sky", "spanning 1.5x1.5deg^2^ centred on NGC 3603, by cross-matching the", "Mohr-Smith et al. catalogue with Gaia DR2. This provides the basis for", "a first comprehensive examination of the PMs of these massive stars in", "the halo of NGC 3603, relative to the much better studied central", "region. We identify up to 11 likely O star ejections - 8 of which", "would have been ejected between 0.60 and 0.95Myr ago (supporting the", "age of ~1Myr that has been attributed to the bright cluster centre).", "Seven candidate ejections are arranged in a partial ring to the south", "of the cluster core spanning radii of 9-18arcmin (18-36pc if the", "cluster is 7kpc away). We also show that the cluster has a halo of a", "further ~100 O stars extending to a radius of at least 5arcmin, adding", "to the picture of NGC 3603 as a scaled down version of the R136/30 Dor", "region."], "description": ["We adopt as the central reference position in the core of NGC 3603 the", "Galactic coordinates, l=291.617{deg},b=-0.523{deg}. The selection box", "on the sky around this position is a square occupying 1.5x1.5deg^2^,", "with sides oriented along the directions of constant Galactic", "longitude and latitude. Within this region, the MS-II data base", "(Mohr-Smith et al. 2017MNRAS.465.1807M, Cat. J/MNRAS/465/1807)", "provides a list of 1663 blue-selected OB candidate stars. Of these we", "retain as a long list those objects for which the reported quality of", "fits to their optical-NIR SEDs is {chi}^2^<25. MS-II recommended a", "tighter {chi}^2^ limit than this for the selection of 'good OB stars':", "it is relaxed here so as not to exclude detected objects close to the", "centre of NGC 3603 that are known already to be early-type", "emission-line stars. This reduces the list to 1537 objects.", "After selecting the stars with log(Teff)>4.44 and Kmag<13.0, we", "cross-matched this sample with Gaia DR2 (Gaia Collaboration", "2018A&A...616A...1G, Cat. I/345). Then, after applying some quality", "filters based on the Gaia DR2 documentation, we obtained a sample of", "288 candidate O stars of which 15 are already in the literature. Table", "B1 lists the names, positions, and other important quantities of our", "sample."], "data": "", "date_update": "24-Oct-2022", "tables": [{"name": "tableb1.dat", "desc": "Complete sample of 288 candidate O stars obtained by cross-matching MS-II and Gaia DR2", "columns": [{"name": "Name", "desc": "MS-II object identifier (NNNNN) (1) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "logTeff", "desc": "Logarith of the effective temperature (1) "}, {"name": "A0", "desc": "Monochromatic extinction at 5495{AA} (1) "}, {"name": "GaiaDR2", "desc": "Gaia DR2 source identifier "}, {"name": "plx", "desc": "Parallax "}, {"name": "Gmag", "desc": "Gaia DR2 G-band magnitude "}, {"name": "Radius", "desc": "Angular distance from the adopted cluster centre, at (l=291.617{deg},b=-0.523{deg})"}, {"name": "rpmGLON", "desc": "Relative proper motion in galactic longitude relative to the core-region mean"}, {"name": "rpmGLAT", "desc": "Relative proper motion in galactic latitude relative to the core-region mean"}, {"name": "rpm", "desc": "Total relative proper motion magnitude "}, {"name": "IP", "desc": "Trajectory impact parameter "}, {"name": "e_IP", "desc": "Error on IP "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_MNRAS_486_3266"}} {"id": "J/MNRAS/486/3266", "title_cds": "Short Title", "title_create": "Purandardas+, 2019", "year": "2019", "author": "Purandardas M., Goswami A., Goswami P.P., Shejeelammal J., Masseron T.", "title_pub": "Chemical analysis of CH stars - III. Atmospheric parameters and elemental abundances.", "first_author": "Purandardas M.", "ref_biblio": [""], "bibcode": ["2019MNRAS.486.3266P"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Ana Fiallos [CDS]", "data": "", "date_update": "24-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASJ_55_771"}} {"id": "J/PASJ/55/771", "title_cds": "Hdelta-strong galaxies in SDSS", "title_create": "Goto+, 2003", "year": "2003", "author": "Goto T., Nichol R.C., Okamura S., Sekiguchi M., Miller C.J., Bernardi M., Hopkins A., Tremonti C., Connolly A., Castander F.J., Brinkmann J., Fukugita M., Harvanek M., Ivezic Z., Kleinman S.J., Krzesinski J., Long D., Loveday J., Neilsen E.H., Newman P.R., Nitta A., Snedden S.A., Subbarao M.", "title_pub": "Hdelta-strong galaxies in the Sloan Digital Sky Survey : I. The Catalog.", "first_author": "Goto T.", "ref_biblio": [""], "bibcode": ["2003PASJ...55..771G"], "keyword_cds": "", "keyword_pub": "galaxies: evolution - galaxies: interaction - galaxies: peculiar - galaxies: starburst", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/pasj/55.4.771"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASJ_59_245"}} {"id": "J/PASJ/59/245", "title_cds": "High-Resolution and S/N Spectrum Atlas of Vega", "title_create": "Takeda+, 2006", "year": "2006", "author": "Takeda Y., Kawanomoto S., and Ohishi N.", "title_pub": "High-Resolution and High-S/N Spectrum Atlas of Vega", "first_author": "Takeda Y.", "ref_biblio": [""], "bibcode": ["2007PASJ...59..245T"], "see_also": ["J/ApJ/380/223 : Metallic line profiles of the AO V star VEGA", "J/A&A/420/183 : S4N: A spectroscopic survey of stars in the solar", "J/PASP/116/693 : The ELODIE Archive (Moultaka+ 2004)", "J/other/PBeiO/33.34 : The high resolution spectrum of Vega.I. Spectral", "J/other/PBeiO/33.58 : The high resolution spectrum of Vega.II. Spectral", "J/PASJ/57/13 : High-Dispersion Spectra Collection of Nearby F--K Stars", "at Okayama Astrophysical Observatory: A Basis for"], "keyword_cds": "Abundances ; Atlases ; Spectroscopy ; Stars, early-type ; Stars, A-type ; Line Profiles", "keyword_pub": "atlases - line: profiles - stars: early-type - stars: individual({alpha}Lyr, {alpha}Leo) - techniques: spectroscopic", "abstract": ["We present a digital spectral atlas of Vega covering from", "violet to near-IR region (~3900-8800A), which has so high", "resolution (R~100000) and high signal-to-noise ratio", "(typically ~1000-2000 on the average) as to allow a detailed", "line-profile analysis. In addition, theoretically simulated", "spectra and lists of lines predicted to have appreciable", "strengths are also provided, which may be useful for identifying", "or searching lines on the atlas. Besides, the spectra of", "Regulus (a representative rapid rotator) obtained at the same", "night are appended as a reference of telluric lines."], "description": ["The data contained in the five directories (\"fitsfiles\",", "\"finalspectra\", \"synthespec\", \"lineprediction\", and \"appendix\")", "constitute the electronic data table of our paper \"High-Resolution", "and High-S/N Spectrum Atlas of Vega\" published in PASJ, Vol. 59,", "pp245-261 (2007)."], "object": ["18 36 56.3 +38 47 01 {alpha} Lyr = HD 172167", "10 08 22.3 +11 58 02 {alpha} Leo = HD 87901"], "doi_pub": ["10.1093/pasj/59.1.245"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "obslog_vega.dat", "desc": "basic data of our Vega observations ", "columns": [{"name": "frameNo", "desc": "[1-9hb] serial number of each spectral frame "}, {"name": "region", "desc": "[bgri] wavelength region indicator "}, {"name": "date", "desc": "date of observation "}, {"name": "UT", "desc": "observation time (in UT) at mid-exposure "}, {"name": "secz", "desc": "air mass at the time of observation "}, {"name": "texp", "desc": "exposure time (in second) "}, {"name": "count", "desc": "mean spectrum count "}]}, {"name": "fitsfiles/*", "desc": "FITS files of spectrum of Vega ", "columns": []}, {"name": "obslog_regu.dat", "desc": "basic data of our Regulus observations ", "columns": [{"name": "frameNo", "desc": "[1-9hb] serial number of each spectral frame "}, {"name": "region", "desc": "[bgri] wavelength region indicator "}, {"name": "date", "desc": "date of observation "}, {"name": "UT", "desc": "observation time (in UT) at mid-exposure "}, {"name": "secz", "desc": "air mass at the time of observation "}, {"name": "texp", "desc": "exposure time (in second) "}, {"name": "count", "desc": "mean spectrum count "}]}, {"name": "appendix/*", "desc": "FITS files of spectrum of Regulus ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASJ_60_1267"}} {"id": "J/PASJ/60/1267", "title_cds": "Old open clusters photometric data", "title_create": "Hasegawa+, 2008", "year": "2008", "author": "Hasegawa T., Sakamoto T., Malasan H.L.", "title_pub": "New photometric data of old open clusters. II. A dataset for 36 clusters.", "first_author": "Hasegawa T.", "ref_biblio": [""], "bibcode": ["2008PASJ...60.1267H"], "see_also": ["J/PASJ/56/295 : BVIc photometry of old open clusters (Hasegawa+, 2004)"], "keyword_cds": "Clusters, open ; Photometry, UBVRI", "keyword_pub": "Galaxy: evolution - Galaxy: open clusters and associations: general - Galaxy: open clusters and associations: HR diagram - Galaxy: structure", "abstract": ["We present new photometric data on 36 old open clusters using the", "65-cm telescope at Gunma Astronomical Observatory. This dataset is a", "continuation of photometric data of old open clusters (Hasegawa et al.", "2004, Cat. ) collected mainly in the antigalactic", "center region. By constructing a color-magnitude diagram, we inspected", "the main sequence and (if richly populated) red-clump stars to", "evaluate the cluster parameters, that is, the age, distance, and", "reddening, by applying an isochrone provided by the Padova group. Now,", "49 old clusters have consistently measured parameters (36 clusters in", "this study and 13 from Hasegawa et al. 2004, Cat. ).", "The clusters are exclusively older than the Hyades cluster, and the", "age is distributed in the range 0.6-5.0Gyr."], "description": ["Optical observations were conducted using the 65-cm telescope (F/12.0,", "f=7800mm) at Gunma Astronomical Observatory. Data were collected", "between 2000 December 4 and 2006 December 22, mostly in 2004 and 2006."], "type": ["OC"], "doi_pub": ["10.1093/pasj/60.6.1267"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "List of open clusters observed in this study ", "columns": [{"name": "Name", "desc": "Cluster name "}, {"name": "RAh", "desc": "Revised central right ascension (J2000.0) "}, {"name": "RAm", "desc": "Revised central right ascension (J2000.0) "}, {"name": "RAs", "desc": "Revised central right ascension (J2000.0) "}, {"name": "DE-", "desc": "Revised central declination sign (J2000.0) "}, {"name": "DEd", "desc": "Revised central declination (J2000.0) "}, {"name": "DEm", "desc": "Revised central declination (J2000.0) "}, {"name": "GLON", "desc": "Revised central Galactic longitude "}, {"name": "GLAT", "desc": "Revised central Galactic latitude "}, {"name": "Morph", "desc": "Morphological parameters given in COCD; contrast (1,2), richness (m,p), and detachment (I-IIII) (1)"}]}, {"name": "table2.dat", "desc": "Log of optical photometric observations using the 65-cm telescope", "columns": [{"name": "Name", "desc": "Cluster name "}, {"name": "Cam", "desc": "Adopted camera system "}, {"name": "FWHM", "desc": "Typical seeing size at I-band "}, {"name": "TexpB", "desc": "Total exposure time in B band "}, {"name": "TexpV", "desc": "Total exposure time in V band "}, {"name": "TexpI", "desc": "Total exposure time in I band "}, {"name": "Bmaglim", "desc": "Limiting B magnitude "}, {"name": "Vmaglim", "desc": "Limiting V magnitude "}, {"name": "Imaglim", "desc": "Limiting I magnitude "}]}, {"name": "table4.dat", "desc": "Parameters of the open clusters, as determined in this study", "columns": [{"name": "Name", "desc": "Cluster name "}, {"name": "Age", "desc": "Age (Isochrone fitting) "}, {"name": "Z", "desc": "Assumed metallicity Z (Isochrone fitting) "}, {"name": "E(V-I)", "desc": "V-I colour excess (Isochrone fitting) "}, {"name": "(m-M)0", "desc": "Deredenned distance modulus (Isochrone fitting) "}, {"name": "rGC", "desc": "Galactocentric distance (Isochrone fitting) (1) "}, {"name": "z", "desc": "Distance from the galactic plane (Isochrone fitting)"}, {"name": "l_E(V-I)D", "desc": "[~] Limit flag on E(V-I)D "}, {"name": "E(V-I)D", "desc": "V-I color excess quoted from the DIRBE/ISSA "}, {"name": "dE(V-I)D", "desc": "Differential reddening, which is the peak-to-peak difference of the DIRBE/ISSA color excess in the 10' box area"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASJ_65_8"}} {"id": "J/PASJ/65/8", "title_cds": "Catalog of SDSS quasar absorption redshift", "title_create": "Qin+, 2013", "year": "2013", "author": "Qin Y.-P., Chen Z.-F., Lu L.-Z., Huang W.-R., Li M.-S., Li G.-Q., Wang M.P., Zhong Y.-Q., Wen S.-Q., Liao R.-H., Ye F.", "title_pub": "Catalog of SDSS quasar absorption redshifts measured from MgII absorption lines. I. For sources with z_em_ <= 0.8.", "first_author": "Qin Y.-P.", "ref_biblio": [""], "bibcode": ["2013PASJ...65....8Q"], "keyword_cds": "", "keyword_pub": "line: identification - quasars: absorption lines - quasars: general", "abstract": ["We are going to analyze the whole Sloan Digital Sky Survey (SDSS)", "quasar spectra by visually identifying Mg II absorption line systems", "one by one. In this paper, we limit our analysis to quasars with $", "z_em_<=0.8, which leaves 8006 quasars in total. Based on this, we are", "able to present the first catalog of these redshifts (in the interval", "of 0.36=0.3{AA}, and about 71% (2957/4158) of the absorbers", "have W__r{lambda}2803>=0.3{AA}, showing that the main portion of our", "catalog is likely to be occupied by strong absorbers."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/pasj/65.1.8"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASJ_71_62"}} {"id": "J/PASJ/71/62", "title_cds": "Short Title", "title_create": "Gao, 2019", "year": "2019", "author": "Gao X.-H.", "title_pub": "Membership and fundamental parameters of the intermediate-age open clusters NGC 2281 and NGC 2539 based on Gaia-DR2.", "first_author": "Gao X.-H.", "ref_biblio": [""], "bibcode": ["2019PASJ...71...62G"], "keyword_cds": "", "keyword_pub": "", "abstract": ["This paper presents an investigation on the two intermediate-age open", "clusters NGC 2281 and NGC 2539 based on Gaia Data Release 2", "(Gaia-DR2). A combined machine-learning method is used to identify", "likely cluster members of the two clusters, taking into account the", "astrometric and photometric data of Gaia-DR2. It is found that NGC", "2281 and NGC 2539 each have more than 600 likely cluster members,", "which are highly suitable for further investigation of the fundamental", "parameters of the two clusters. Robust estimates of the distances,", "proper motions, and radial velocities for the two clusters are", "obtained via a Monte Carlo simulation technique. NGC 2281 is found to", "have a distance of 522+/-12pc, a proper motion of", "(, =(\u22122.94+/-0.014, -8.344+/-0.014)mas/yr,", "and a radial velocity of +20.0+/-0.7km/s. The distance, proper motion,", "and radial velocity of NGC 2539 are determined to be 1271+/-70pc,", "()=(-2.33+/-\u00b10.007, -0.583+/-0.006)mas/yr, and", "+29.6+/-0.4km/s, respectively. We find that NGC 2281 has a core radius", "of 8.89'+/-0.27' (1.3pc) and a limiting radius of 79.26'+/-2.86'", "(12.0pc). The core and limiting radius of NGC 2539 are determined to", "be 5.62'+/-0.28' (2.1pc) and 33.65'+/-1.96 (12.4pc), respectively. In", "addition, we find strong evidence for the existence of mass", "segregation in the two clusters."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/pasj/psz039"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_102_865"}} {"id": "J/PASP/102/865", "title_cds": "Stars in the field of NGC 2353.", "title_create": "Fitzgerald+, 1990", "year": "1990", "author": "Fitzgerald M.P., Harris G.L.H., Reed B.C.", "title_pub": "The moderately young open cluster NGC 2353.", "first_author": "Fitzgerald M.P.", "ref_biblio": [""], "bibcode": ["1990PASP..102..865F"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/132711"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_108_o.277"}} {"id": "J/PASP/108/277", "title_cds": "Night-Sky High-Res Spectral Atlas of OH and O2", "title_create": "Osterbrock+ 1996", "year": "1996", "author": "Osterbrock D.E., Fulbright J.P., Martel A.R., Keane M.J, Trager S.C. and Basri G.", "title_pub": "Night-Sky High-Resolution Spectral Atlas of OH and O2 Emission Lines for Echelle Spectrograph Wavelength Calibration", "first_author": "Osterbrock D.E.", "ref_biblio": [""], "bibcode": ["1995PASP..108..277O"], "see_also": ["http://ucowww.ucsc.edu/~jfulb/OH.html : the original data distribution"], "keyword_cds": "Atomic and molecular data", "keyword_pub": "OH; O2", "description": ["This catalog provides a list of atmospheric OH and O2 lines that are", "useful for wavelength calibration of high resolution spectra.", "Tables of observed OH lines supplemented by calculated values from the", "literature, observed and calculated wavelengths for molecular oxygen", "(O2), atomic lines of O I and Na I and postscript files for all", "spectral regions with identifications from all the figures of the paper", "are given."], "date_update": "31-Jan-2000", "tables": [{"name": "table2.dat", "desc": "Observed OH Lines Not Listed in Abrams et al. (1994) ", "columns": [{"name": "trans", "desc": "OH transition nu'-nu\" "}, {"name": "ID", "desc": "OH line Identification "}, {"name": "lambda", "desc": "wavelength observed OH line "}]}, {"name": "table3.dat", "desc": "Calculated Wavelengths for O2 (0-1) ", "columns": [{"name": "ID1", "desc": "O2 line identification "}, {"name": "lambda1", "desc": "? calculated wavelength "}, {"name": "ID2", "desc": "O2 line identification "}, {"name": "lambda2", "desc": "? calculated wavelength "}]}, {"name": "table4.dat", "desc": "Atomic Lines ", "columns": [{"name": "ID", "desc": "Ion identification "}, {"name": "lambda", "desc": "wavelength of atomic night-sky lines "}]}, {"name": "tablea.dat", "desc": "Supplemental Table of OH Wavelengths (Abrams et al.) ", "columns": [{"name": "trans", "desc": "OH transition nu'-nu\" "}, {"name": "ID", "desc": "OH identification "}, {"name": "lambda", "desc": "wavelength from Abrams et al. (1994) "}]}, {"name": "figures.tar", "desc": "Postscript files for all figures ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_109_289"}} {"id": "J/PASP/109/289", "title_cds": "Emission lines in PNe", "title_create": "Kaler+ 1997", "year": "1997", "author": "Kaler J.B., Shaw R.A., Browning L.", "title_pub": "Title of the paper", "first_author": "Kaler J.B.", "ref_biblio": [""], "bibcode": ["1997PASP..109..289K\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/133887"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_110_1342"}} {"id": "J/PASP/110/1342", "title_cds": "Unusual objects in the SDSS", "title_create": "Krisciunas+ 1998", "year": "1998", "author": "Authors", "title_pub": "Title of the paper", "first_author": "Authors", "ref_biblio": [""], "bibcode": ["1998PASP..110.1342K\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/316264"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_111_221"}} {"id": "J/PASP/111/221", "title_cds": "Detection of O VII in PNe from IUE spectra", "title_create": "Feibelman, 1999", "year": "1999", "author": "Authors", "title_pub": "Title of the paper", "first_author": "Authors", "ref_biblio": [""], "bibcode": ["1999PASP..111..221F\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/316317"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_112_1008"}} {"id": "J/PASP/112/1008", "title_cds": "Near-infrared galaxy morphology atlas", "title_create": "Jarrett+, 2000", "year": "2000", "author": "Jarrett T.H.", "title_pub": "Near-infrared galaxy morphology atlas.", "first_author": "Jarrett T.H.", "ref_biblio": [""], "bibcode": ["2000PASP..112.1008J\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "James Marcout, Patricia Bauer [CDS]", "doi_pub": ["10.1086/316603"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_122_516"}} {"id": "J/PASP/122/516", "title_cds": "Hogg 12 and NGC 3590", "title_create": "Piatti+, 2010", "year": "2010", "author": "Piatti A.E., Claria J.J., Ahumada A.V.", "title_pub": "Hogg 12 and NGC 3590: a new open cluster binary system candidate.", "first_author": "Piatti A.E.", "ref_biblio": [""], "bibcode": ["2010PASP..122..516P"], "keyword_cds": "", "abstract": ["We have obtained CCD UBVI_KC_ photometry down to V~22.0 for the open", "clusters Hogg 12 and NGC 3590 and the fields surrounding them. Based", "on photometric and morphological criteria, as well as on the stellar", "density in the region, our evidence is sufficient to confirm that Hogg", "12 is a genuine open cluster. NGC 3590 was used as a control cluster.", "The color-magnitude diagrams of Hogg 12, cleaned from field star", "contamination, reveal that this is a solar metal content cluster,", "affected by E(B-V)=0.40+/-0.05, located at a heliocentric", "distance d=2.0+/-0.5kpc, and of an age similar to that of NGC 3590", "(t=30Myr). Both clusters are surprisingly small objects whose radii", "are barely ~1pc, andthey are separated in the sky by scarcely 3.6pc.", "These facts, added to their similar ages, reddenings, and", "metallicities, allow us to consider them a new open cluster binary", "system candidate. Of the 180 open cluster binary systems estimated to", "exist in the Galaxy, of which 27 are actually well known, Hogg 12 and", "NGC 3590 appear to be one of the two closest pairs."], "description": ["We obtained CCD images for Hogg 12 on the nights of 2000 27 December", "and 29 December with the UBVIKC filters and a 2048x2048pixel", "Tektronix CCD attached to the 0.9m telescope (scale 0.4\"/pixel)", "at Cerro Tololo Inter-American Observatory (CTIO) Chile."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/652501"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_81_804"}} {"id": "J/PASP/81/804", "title_cds": "Four southern photoelectric sequences", "title_create": "Fitzgerald+, 1969", "year": "1969", "author": "Fitzgerald M.P., Wilson W., Stegman J.E.", "title_pub": "Four southern photoelectric sequences.", "first_author": "Fitzgerald M.P.", "ref_biblio": [""], "bibcode": ["1969PASP...81..804F"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_86_829"}} {"id": "J/PASP/86/829", "title_cds": "Transmission grating spectra", "title_create": "Miller+ 1974", "year": "1974", "author": "Miller E.W., Graham J.A.", "title_pub": "Transmission grating spectra: a new search technique for faint blue stars.", "first_author": "Miller E.W.", "ref_biblio": [""], "bibcode": ["1974PASP...86..829M"], "keyword_cds": "Stars, blue", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/129681"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PASP_96_707"}} {"id": "J/PASP/96/707", "title_cds": "Hyades lower main sequence", "title_create": "Duncan+, 1984", "year": "1984", "author": "Duncan D.K., Baliunas S.L., Noyes R.W., Vaughan A.H., Frazer J., Lanning H.H.", "title_pub": "Chromospheric emission and rotation of the Hyades lower main sequence.", "first_author": "Duncan D.K.", "ref_biblio": [""], "bibcode": ["1984PASP...96..707D"], "keyword_cds": "Clusters, open ; Stars, emission ; Spectroscopy", "keyword_pub": "Stellar rotation - emission lines - late-type stars", "abstract": ["The identity of chromospheric CaII H- and K-line emission has been", "monitored for two seasons in a large sample of Hyades F and G dwarfs.", "Mean emission levels vary smoothly with spectral type, suggesting that", "the rotation rate at a given spectral type varies relatively little,", "and that the rotation rate decreases smoothly as a function of mass.", "In this case the mechanism which controls pre-main-sequence angular", "momentum loss in late-type stars must be self-regulating to a high", "degree."], "object": [], "doi_pub": ["10.1086/131409"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "stars.dat", "desc": " ", "columns": [{"name": "VB", "desc": "van Bueren number (1952BAN....11..385V) "}, {"name": "logRhk", "desc": " "}, {"name": "logR'hk", "desc": "Chromospheric activity index "}, {"name": "logP", "desc": "Period "}, {"name": "SimbadName", "desc": "Designation of the star in SIMBAD "}, {"name": "RAdeg", "desc": "Right ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "TYC1", "desc": "Tycho-2 designation (Cat. I/259) "}, {"name": "TYC2", "desc": "Tycho-2 designation (Cat. I/259) "}, {"name": "TYC3", "desc": "Tycho-2 designation (Cat. I/259) "}, {"name": "HIP", "desc": "? Hipparcos number (Cat. I/239/hip_main) "}, {"name": "HD", "desc": "Henry Draper number (III/135) "}, {"name": "ASCC", "desc": "ASCC number (Kharchenko et al., Cat. I/280) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_PAZh_26_843"}} {"id": "J/PAZh/26/843", "title_cds": "Catalog of high- and low-mass X-ray binaries", "title_create": "Guseinov+, 2000", "year": "2000", "author": "Guseinov O.H., Sayagac A.T., Allakhverdiev A., Caliskan H., Ozdemir S., Yerli S.K., Ankay A.", "title_pub": "A preliminary version of a catalog of high-low-mass X-ray binaries", "first_author": "Guseinov O.H.", "ref_biblio": [""], "bibcode": ["2000PAZh...26..843G", "2000AstL...26..725G"], "see_also": ["V/106 : High- and low mass X-ray binaries catalogue (Liu+ 2000)"], "keyword_cds": "Binaries, X-ray ; Photometry, UBV ; Cross identifications", "keyword_pub": "catalogs, X-ray binaries, neutron stars, X-rays", "abstract": ["The aim of this catalogue is to provide basic information on X-ray", "sources and their counterparts. The catalogue contains positions,", "information about distances and counterparts, spectral, photometric", "and timing properties of the X-ray sources in X-ray and optical bands", "as well as references. The list of references, comments and the", "catalogue as a whole will be periodically updated to include the most", "up to date information on all X-ray binaries and guide users to the", "recent literature on individual sources. In some cases, there is some", "doubt about the nature of the X-ray source, which has been noted. The", "sources are ordered according to their right ascension.", "The first comprehensive catalogue of X-ray binaries was presented by", "van Paradijs (1995, Cat. ). Our catalogue includes, as X-ray", "binaries, the point X-ray sources powered by accretion onto neutron", "stars and blackholes. The weak sources powered by stellar coronae,", "Wolf-Rayet stars, and cataclysmic variables are not included. Among", "those X-ray binaries presented in the catalogue there are 78 HMXBs (35", "and 5 of which are pulsars and possible pulsars, respectively) and 138", "LMXBs (only 9 of which are pulsars), 89 transient and possible", "transient sources, and 25 possible blackholes (6 HMXBs+19 LMXBs).", "There are also 43 bursters (all of which are Galactic LMXBs) and 21", "QPOs. The present catalogue extends the work by van Paradijs,", "tabulates further information on the compact objects and their", "companions as well as attempting a more comprehensive guide to the", "literature. Where different authors obtained different values for", "system parameters, we have quoted all parameter values together with", "the references to guide the reader to the relevant literature for the", "derivation of the parameters."], "description": ["The catalogue mainly consists of 2 parts, 'hmxb' and 'lmxb', each of", "which has 4 files:", "1) The main catalogue is consisted of 'hmxbcat.dat' and 'lmxbcat.dat'.", "The most recent and/or the most reliable data are given in these files.", "2) All of the cross catalogue names of the sources and the names of", "the optical counterparts are given in 'hmxbnam.dat' and 'lmxbnam.dat'.", "3) The intensity values, energy bands, dates of observations, names of", "satellites for these observations, and the references of all of these", "data are given in 'hmxbobs.dat' and 'lmxbobs.dat'.", "4) All of the data other than the most recent and/or the most reliable", "ones are presented in 'hmxbrem.dat' and 'lmxbrem.dat'. The values given", "in intervals are also presented in these two files (e.g. A distance value", "of 4-5kpc of a source is given in 'hmxbrem.dat' or'lmxbrem.dat' (not in", "'hmxbcat.dat' or 'lmxbcat.dat') even if it is the most recent and/or the", "most reliable distance value of that source)."], "type": ["CCC"], "data": "", "date_update": "07-Sep-2011", "tables": [{"name": "lmxbcat.dat", "desc": "Low-Mass X-ray Binaries catalogue ", "columns": [{"name": "Name", "desc": "*Object name "}, {"name": "Location", "desc": "*[GOLS] Object's location "}, {"name": "Supersoft", "desc": "[S] Supersoft flag "}, {"name": "Type", "desc": "*Object's type "}, {"name": "RAh", "desc": "? Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "? Right Ascension 2000 (minutes) "}, {"name": "RAs", "desc": "? Right Ascension 2000 (seconds) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "? Declination 2000 (degrees) "}, {"name": "DEm", "desc": "? Declination 2000 (minutes) "}, {"name": "DEs", "desc": "? Declination 2000 (seconds) "}, {"name": "RA1950h", "desc": "? Right Ascension 1950 (hours) "}, {"name": "RA1950m", "desc": "? Right Ascension 1950 (minutes) "}, {"name": "RA1950s", "desc": "? Right Ascension 1950 (seconds) "}, {"name": "DE1950-", "desc": "Declination 1950 (sign) "}, {"name": "DE1950d", "desc": "? Declination 1950 (degrees) "}, {"name": "DE1950m", "desc": "? Declination 1950 (minutes) "}, {"name": "DE1950s", "desc": "? Declination 1950 (seconds) "}, {"name": "GLON", "desc": "? Galactic Longtitude "}, {"name": "GLAT", "desc": "? Galactic Latitude "}, {"name": "l_Porb", "desc": "[~<>= ] Limit flag on Porb "}, {"name": "Porb", "desc": "? Orbital Period "}, {"name": "u_Porb", "desc": "[:] Uncertainity flag on Porb "}, {"name": "n_Porb", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Ppulse", "desc": "[~<>= ] Limit flag on Ppulse "}, {"name": "Ppulse", "desc": "? Pulse Period "}, {"name": "u_Ppulse", "desc": "[:] Uncertainity flag on Ppulse "}, {"name": "n_Ppulse", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "n_Period", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Energy", "desc": "[~<>= ] Limit flag on Energy "}, {"name": "Energy", "desc": "? Energy, kT "}, {"name": "u_Energy", "desc": "[:] Uncertainity flag on Energy "}, {"name": "n_Energy", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Sp+Index", "desc": "[~<>= ] Limit flag on Sp+Index "}, {"name": "Sp+Index", "desc": "? Spectral Index "}, {"name": "u_Sp+Index", "desc": "[:] Uncertainity flag on Sp+Index "}, {"name": "n_Sp+Index", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "n_Fieldmag", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Dist", "desc": "[~<>= ] Limit flag on Dist "}, {"name": "Dist", "desc": "? Distance "}, {"name": "u_Dist", "desc": "[:] Uncertainity flag on Dist "}, {"name": "n_Dist", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_logNH", "desc": "[~<>= ] Limit flag on logNH "}, {"name": "logNH", "desc": "? log NH "}, {"name": "u_logNH", "desc": "[:] Uncertainity flag on logNH "}, {"name": "n_logNH", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_AV", "desc": "[~<>= ] Limit flag on AV "}, {"name": "AV", "desc": "? Total optical absorption "}, {"name": "u_AV", "desc": "[:] Uncertainity flag on AV "}, {"name": "n_AV", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_LX", "desc": "[~<>= ] Limit flag on LX "}, {"name": "LX", "desc": "? X-ray luminosity "}, {"name": "u_LX", "desc": "[:] Uncertainity flag on LX "}, {"name": "n_LX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_LX/Lopt", "desc": "[~<>= ] Limit flag on LX/Lopt "}, {"name": "LX/Lopt", "desc": "? Ratio of X-ray to optical luminosity "}, {"name": "u_LX/Lopt", "desc": "[:] Uncertainity flag on LX/Lop "}, {"name": "n_LX/Lopt", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "SpType", "desc": "*Spectral Type (Spectral type part 1) "}, {"name": "SpClass", "desc": "*Spectral Class (Spectal type part 2) "}, {"name": "SpType3", "desc": "*[dnefp ] Spectral Type (part 3) "}, {"name": "u_SpType", "desc": "*[:] Uncertainity flag on SpType "}, {"name": "l_Vmag1", "desc": "[~<>= ] Limit flag on Vmag1 "}, {"name": "Vmag1", "desc": "? V magnitude (1st component) "}, {"name": "Vmag2", "desc": "? V magnitude (2nd component) "}, {"name": "u_Vmag1", "desc": "[:] Uncertainity flag on Vmag1 "}, {"name": "n_Vmag1", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_B-V", "desc": "[~<>= ] Limit flag on B-V "}, {"name": "B-V", "desc": "? B-V magnitude "}, {"name": "u_B-V", "desc": "[:] Uncertainity flag on B-V "}, {"name": "n_B-V", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_U-B", "desc": "[~<>= ] Limit flag on U-B "}, {"name": "U-B", "desc": "? U-B magnitude "}, {"name": "u_U-B", "desc": "[:] Uncertainity flag on U-B "}, {"name": "n_U-B", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_E(B-V)", "desc": "[~<>= ] Limit flag on E(B-V) "}, {"name": "E(B-V)", "desc": "? E(B-V) colour excess "}, {"name": "u_E(B-V)", "desc": "[:] Uncertainity flag on E(B-V) "}, {"name": "n_E(B-V)", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassX", "desc": "[~<>= ] Limit flag on MassX "}, {"name": "MassX", "desc": "? Mass of compact object "}, {"name": "u_MassX", "desc": "[:] Uncertainity flag on MassX "}, {"name": "n_MassX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassO", "desc": "[~<>= ] Limit flag on MassO "}, {"name": "MassO", "desc": "? Mass of companion "}, {"name": "u_MassO", "desc": "[:] Uncertainity flag on MassO "}, {"name": "n_MassO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassFX", "desc": "[~<>= ] Limit flag on Mass FX "}, {"name": "MassFX", "desc": "? Mass function of compact object "}, {"name": "u_MassFX", "desc": "[:] Uncertainity flag on Mass FX "}, {"name": "n_MassFX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassFO", "desc": "[~<>= ] Limit flag on Mass FO "}, {"name": "MassFO", "desc": "? Mass function of companion "}, {"name": "u_MassFO", "desc": "[:] Uncertainity flag on Mass FO "}, {"name": "n_MassFO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_eOpt", "desc": "[~<>= ] Limit flag on eOpt "}, {"name": "eOpt", "desc": "? Eccentricity of the orbit "}, {"name": "u_eOpt", "desc": "[:] Uncertainity flag on eOpt "}, {"name": "n_eOpt", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelKX", "desc": "[~<>= ] Limit flag on VelKX "}, {"name": "VelKX", "desc": "? Semi-amplitude velocity of compact "}, {"name": "u_VelKX", "desc": "[:] Uncertainity flag on VelKX "}, {"name": "n_VelKX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelKO", "desc": "[~<>= ] Limit flag on VelKO "}, {"name": "VelKO", "desc": "? Semi-amplitude velocity of companion "}, {"name": "u_VelKO", "desc": "[:] Uncertainity flag on VelKO "}, {"name": "n_VelKO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelVG", "desc": "[~<>= ] Limit flag on VelVG "}, {"name": "VelVG", "desc": "? Center-of-mass velocity "}, {"name": "u_VelVG", "desc": "[:] Uncertainity flag on VelVG "}, {"name": "n_VelVG", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_a1sini", "desc": "[~<>= ] Limit flag on a1sini "}, {"name": "a1sini", "desc": "? A sin(I) for compact object "}, {"name": "u_a1sini", "desc": "[:] Uncertainity flag on a1sini "}, {"name": "n_a1sini", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_a2sini", "desc": "[~<>= ] Limit flag on a2sini "}, {"name": "a2sini", "desc": "? A sin(I) for companion "}, {"name": "u_a2sini", "desc": "[:] Uncertainity flag on a2sini "}, {"name": "n_a2sini", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Incl", "desc": "[~<>= ] Limit flag on Incl "}, {"name": "Incl", "desc": "? Inclination of orbit "}, {"name": "u_Incl", "desc": "[:] Uncertainity flag on Incl "}, {"name": "n_Incl", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "---", "desc": "[|] "}]}, {"name": "hmxbcat.dat", "desc": "High-Mass X-ray Binaries catalogue ", "columns": [{"name": "Name", "desc": "*Object name "}, {"name": "Location", "desc": "*[GOLS] Object's location "}, {"name": "Supersoft", "desc": "[S] Supersoft flag "}, {"name": "Type", "desc": "*Object's type "}, {"name": "RAh", "desc": "? Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "? Right Ascension 2000 (minutes) "}, {"name": "RAs", "desc": "? Right Ascension 2000 (seconds) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "? Declination 2000 (degrees) "}, {"name": "DEm", "desc": "? Declination 2000 (minutes) "}, {"name": "DEs", "desc": "? Declination 2000 (seconds) "}, {"name": "RA1950h", "desc": "? Right Ascension 1950 (hours) "}, {"name": "RA1950m", "desc": "? Right Ascension 1950 (minutes) "}, {"name": "RA1950s", "desc": "? Right Ascension 1950 (seconds) "}, {"name": "DE1950-", "desc": "Declination 1950 (sign) "}, {"name": "DE1950d", "desc": "? Declination 1950 (degrees) "}, {"name": "DE1950m", "desc": "? Declination 1950 (minutes) "}, {"name": "DE1950s", "desc": "? Declination 1950 (seconds) "}, {"name": "GLON", "desc": "? Galactic Longtitude "}, {"name": "GLAT", "desc": "? Galactic Latitude "}, {"name": "l_Porb", "desc": "[~<>= ] Limit flag on Porb "}, {"name": "Porb", "desc": "? Orbital Period "}, {"name": "u_Porb", "desc": "[:] Uncertainity flag on Porb "}, {"name": "n_Porb", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Ppulse", "desc": "[~<>= ] Limit flag on Ppulse "}, {"name": "Ppulse", "desc": "? Pulse Period "}, {"name": "u_Ppulse", "desc": "[:] Uncertainity flag on Ppulse "}, {"name": "n_Ppulse", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "n_Period", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Energy", "desc": "[~<>= ] Limit flag on Energy "}, {"name": "Energy", "desc": "? Energy, kT "}, {"name": "u_Energy", "desc": "[:] Uncertainity flag on Energy "}, {"name": "n_Energy", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Sp+Index", "desc": "[~<>= ] Limit flag on Sp+Index "}, {"name": "Sp+Index", "desc": "? Spectral Index "}, {"name": "u_Sp+Index", "desc": "[:] Uncertainity flag on Sp+Index "}, {"name": "n_Sp+Index", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "n_Fieldmag", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Dist", "desc": "[~<>= ] Limit flag on Dist "}, {"name": "Dist", "desc": "? Distance "}, {"name": "u_Dist", "desc": "[:] Uncertainity flag on Dist "}, {"name": "n_Dist", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_logNH", "desc": "[~<>= ] Limit flag on logNH "}, {"name": "logNH", "desc": "? log NH "}, {"name": "u_logNH", "desc": "[:] Uncertainity flag on logNH "}, {"name": "n_logNH", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_AV", "desc": "[~<>= ] Limit flag on AV "}, {"name": "AV", "desc": "? Total optical absorption "}, {"name": "u_AV", "desc": "[:] Uncertainity flag on AV "}, {"name": "n_AV", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_LX", "desc": "[~<>= ] Limit flag on LX "}, {"name": "LX", "desc": "? X-ray luminosity "}, {"name": "u_LX", "desc": "[:] Uncertainity flag on LX "}, {"name": "n_LX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_LX/Lopt", "desc": "[~<>= ] Limit flag on LX/Lopt "}, {"name": "LX/Lopt", "desc": "? Ratio of X-ray to optical luminosity "}, {"name": "u_LX/Lopt", "desc": "[:] Uncertainity flag on LX/Lop "}, {"name": "n_LX/Lopt", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "SpType", "desc": "*Spectral Type (Spectral type part 1) "}, {"name": "SpClass", "desc": "*Spectral Class (Spectal type part 2) "}, {"name": "SpType3", "desc": "*[dnefp ] Spectral Type (part 3) "}, {"name": "u_SpType", "desc": "*[:] Uncertainity flag on SpType "}, {"name": "l_Vmag1", "desc": "[~<>= ] Limit flag on Vmag1 "}, {"name": "Vmag1", "desc": "? V magnitude (1st component) "}, {"name": "Vmag2", "desc": "? V magnitude (2nd component) "}, {"name": "u_Vmag1", "desc": "[:] Uncertainity flag on Vmag1 "}, {"name": "n_Vmag1", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_B-V", "desc": "[~<>= ] Limit flag on B-V "}, {"name": "B-V", "desc": "? B-V magnitude "}, {"name": "u_B-V", "desc": "[:] Uncertainity flag on B-V "}, {"name": "n_B-V", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_U-B", "desc": "[~<>= ] Limit flag on U-B "}, {"name": "U-B", "desc": "? U-B magnitude "}, {"name": "u_U-B", "desc": "[:] Uncertainity flag on U-B "}, {"name": "n_U-B", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_E(B-V)", "desc": "[~<>= ] Limit flag on E(B-V) "}, {"name": "E(B-V)", "desc": "? E(B-V) colour excess "}, {"name": "u_E(B-V)", "desc": "[:] Uncertainity flag on E(B-V) "}, {"name": "n_E(B-V)", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassX", "desc": "[~<>= ] Limit flag on MassX "}, {"name": "MassX", "desc": "? Mass of compact object "}, {"name": "u_MassX", "desc": "[:] Uncertainity flag on MassX "}, {"name": "n_MassX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassO", "desc": "[~<>= ] Limit flag on MassO "}, {"name": "MassO", "desc": "? Mass of companion "}, {"name": "u_MassO", "desc": "[:] Uncertainity flag on MassO "}, {"name": "n_MassO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassFX", "desc": "[~<>= ] Limit flag on Mass FX "}, {"name": "MassFX", "desc": "? Mass function of compact object "}, {"name": "u_MassFX", "desc": "[:] Uncertainity flag on Mass FX "}, {"name": "n_MassFX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassFO", "desc": "[~<>= ] Limit flag on Mass FO "}, {"name": "MassFO", "desc": "? Mass function of companion "}, {"name": "u_MassFO", "desc": "[:] Uncertainity flag on Mass FO "}, {"name": "n_MassFO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_eOpt", "desc": "[~<>= ] Limit flag on eOpt "}, {"name": "eOpt", "desc": "? Eccentricity of the orbit "}, {"name": "u_eOpt", "desc": "[:] Uncertainity flag on eOpt "}, {"name": "n_eOpt", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelKX", "desc": "[~<>= ] Limit flag on VelKX "}, {"name": "VelKX", "desc": "? Semi-amplitude velocity of compact "}, {"name": "u_VelKX", "desc": "[:] Uncertainity flag on VelKX "}, {"name": "n_VelKX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelKO", "desc": "[~<>= ] Limit flag on VelKO "}, {"name": "VelKO", "desc": "? Semi-amplitude velocity of companion "}, {"name": "u_VelKO", "desc": "[:] Uncertainity flag on VelKO "}, {"name": "n_VelKO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelVG", "desc": "[~<>= ] Limit flag on VelVG "}, {"name": "VelVG", "desc": "? Center-of-mass velocity "}, {"name": "u_VelVG", "desc": "[:] Uncertainity flag on VelVG "}, {"name": "n_VelVG", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_a1sini", "desc": "[~<>= ] Limit flag on a1sini "}, {"name": "a1sini", "desc": "? A sin(I) for compact object "}, {"name": "u_a1sini", "desc": "[:] Uncertainity flag on a1sini "}, {"name": "n_a1sini", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_a2sini", "desc": "[~<>= ] Limit flag on a2sini "}, {"name": "a2sini", "desc": "? A sin(I) for companion "}, {"name": "u_a2sini", "desc": "[:] Uncertainity flag on a2sini "}, {"name": "n_a2sini", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Incl", "desc": "[~<>= ] Limit flag on Incl "}, {"name": "Incl", "desc": "? Inclination of orbit "}, {"name": "u_Incl", "desc": "[:] Uncertainity flag on Incl "}, {"name": "n_Incl", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "---", "desc": "[|] "}]}, {"name": "lmxbobs.dat", "desc": "LMXB observations ", "columns": [{"name": "Seq", "desc": "[001/139]+= Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "OBSS.D", "desc": "? Start Day of observation date "}, {"name": "OBSS.M", "desc": "? Start Month of observation date "}, {"name": "OBSS.Y", "desc": "? Start Year of observation date "}, {"name": "OBSE.D", "desc": "? End Day of observation date "}, {"name": "OBSE.M", "desc": "? End Month of observation date "}, {"name": "OBSE.Y", "desc": "? End Year of observation date "}, {"name": "SAT", "desc": "*Satellite abbreviation "}, {"name": "EnergyS", "desc": "? Start of energy range "}, {"name": "EnergyE", "desc": "? End of energy range "}, {"name": "l_Flux1", "desc": "[<>~] Limit flag "}, {"name": "Flux1", "desc": "? Flux in {mu}Jy "}, {"name": "---", "desc": "[-] "}, {"name": "Flux1u", "desc": "? Upper limit of Flux1 when interval "}, {"name": "l_Flux2S", "desc": "[<>~ =] Limit flag "}, {"name": "Flux2S", "desc": "? Start of flux range in mW/m^2^ "}, {"name": "Flux2E", "desc": "? End of flux range in mW/m^2^ "}, {"name": "l_Flux3", "desc": "[<> ~ ] Limit flag on Flux3 "}, {"name": "Flux3", "desc": "? Flux (in count/s if x_Flux3=\" \") "}, {"name": "---", "desc": "[-] "}, {"name": "Flux3u", "desc": "? Upper limit of Flux3 when interval "}, {"name": "x_Flux3", "desc": "*[pmc] Units of Flux3 if not ct/s "}, {"name": "---", "desc": "[|] "}]}, {"name": "hmxbobs.dat", "desc": "HMXB observations ", "columns": [{"name": "Seq", "desc": "[001/139]+= Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "OBSS.D", "desc": "? Start Day of observation date "}, {"name": "OBSS.M", "desc": "? Start Month of observation date "}, {"name": "OBSS.Y", "desc": "? Start Year of observation date "}, {"name": "OBSE.D", "desc": "? End Day of observation date "}, {"name": "OBSE.M", "desc": "? End Month of observation date "}, {"name": "OBSE.Y", "desc": "? End Year of observation date "}, {"name": "SAT", "desc": "*Satellite abbreviation "}, {"name": "EnergyS", "desc": "? Start of energy range "}, {"name": "EnergyE", "desc": "? End of energy range "}, {"name": "l_Flux1", "desc": "[<>~] Limit flag "}, {"name": "Flux1", "desc": "? Flux in {mu}Jy "}, {"name": "---", "desc": "[-] "}, {"name": "Flux1u", "desc": "? Upper limit of Flux1 when interval "}, {"name": "l_Flux2S", "desc": "[<>~ =] Limit flag "}, {"name": "Flux2S", "desc": "? Start of flux range in mW/m^2^ "}, {"name": "Flux2E", "desc": "? End of flux range in mW/m^2^ "}, {"name": "l_Flux3", "desc": "[<> ~ ] Limit flag on Flux3 "}, {"name": "Flux3", "desc": "? Flux (in count/s if x_Flux3=\" \") "}, {"name": "---", "desc": "[-] "}, {"name": "Flux3u", "desc": "? Upper limit of Flux3 when interval "}, {"name": "x_Flux3", "desc": "*[pmc] Units of Flux3 if not ct/s "}, {"name": "---", "desc": "[|] "}]}, {"name": "hmxbname.dat", "desc": "HMXB cross-identifications ", "columns": [{"name": "Seq", "desc": "[1/139]? Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "n_Name", "desc": "[?E] Flag on name, not explicited in the paper "}, {"name": "Opt", "desc": "Optical name "}, {"name": "HD", "desc": "HD or HDE name "}, {"name": "SAO", "desc": "SAO name "}, {"name": "BD", "desc": "BD number "}, {"name": "Other", "desc": "Other name "}, {"name": "Xname", "desc": "X name "}, {"name": "3A", "desc": "3A name "}, {"name": "AX", "desc": "AX name "}, {"name": "1E", "desc": "1E/2E name "}, {"name": "EXO", "desc": "EXO name "}, {"name": "1H", "desc": "H/1H name "}, {"name": "RX", "desc": "RX/1RXS name "}, {"name": "2S", "desc": "2S nam,e "}, {"name": "SAX", "desc": "SAX name "}, {"name": "4U", "desc": "2U/3U/4U name "}, {"name": "1XRS", "desc": "1XRS name "}, {"name": "Names", "desc": "Other names "}, {"name": "---", "desc": "[|] "}]}, {"name": "lmxbname.dat", "desc": "LMXB cross-identifications ", "columns": [{"name": "Seq", "desc": "[1/139]? Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "n_Name", "desc": "[?E] Flag on name, not explicited in the paper "}, {"name": "Opt", "desc": "Optical name "}, {"name": "HD", "desc": "HD or HDE name "}, {"name": "SAO", "desc": "SAO name "}, {"name": "BD", "desc": "BD number "}, {"name": "Other", "desc": "Other name "}, {"name": "Xname", "desc": "X name "}, {"name": "3A", "desc": "3A name "}, {"name": "AX", "desc": "AX name "}, {"name": "1E", "desc": "1E/2E name "}, {"name": "EXO", "desc": "EXO name "}, {"name": "1H", "desc": "H/1H name "}, {"name": "RX", "desc": "RX/1RXS name "}, {"name": "2S", "desc": "2S nam,e "}, {"name": "SAX", "desc": "SAX name "}, {"name": "4U", "desc": "2U/3U/4U name "}, {"name": "1XRS", "desc": "1XRS name "}, {"name": "Names", "desc": "Other names "}, {"name": "---", "desc": "[|] "}]}, {"name": "lmxbrem.dat", "desc": "Other data for LMXB ", "columns": [{"name": "Seq", "desc": "[001/139]+= Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "Data", "desc": "Data "}, {"name": "f_Data", "desc": "[prvd] "}, {"name": "Value", "desc": "Value(s) of Data "}]}, {"name": "hmxbrem.dat", "desc": "Other data for HMXB ", "columns": [{"name": "Seq", "desc": "[001/139]+= Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "Data", "desc": "Data "}, {"name": "f_Data", "desc": "[prvd] "}, {"name": "Value", "desc": "Value(s) of Data "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_A&A_543_o.A100"}} {"id": "J/A+A/543/A100", "title_cds": "GaiaSimu Universe Model Snapshot", "title_create": "Robin+, 2012", "year": "2012", "author": "Robin A.C., Luri X., Reyle C., Isasi Y., Grux E., Blanco-Cuaresma S., Arenou F., Babusiaux C., Belcheva M., Drimmel R., Jordi C., Krone-Martins A., Masana E., Mauduit J.C., Mignard F., Mowlavi N., Rocca-Volmerange B., Sartoretti P., Slezak E., Sozzetti A.", "title_pub": "Gaia Universe model snapshot. A statistical analysis of the expected contents of the Gaia catalogue.", "first_author": "Robin A.C.", "ref_biblio": [""], "bibcode": ["2012A&A...543A.100R"], "keyword_cds": "Positional data ; Surveys ; Models", "keyword_pub": "methods: data analysis - Galaxy: stellar content - catalogs - Galaxy: structure - galaxies: statistics - stars: statistics", "mission": "GAIA", "abstract": ["This study has been developed in the framework of the computational", "simulations that are executed for the preparation of the ESA Gaia", "astrometric mission.", "We focus on describing the objects and characteristics that Gaia will", "potentially observe without taking into consideration instrumental", "effects (detection efficiency, observing errors).", "The theoretical Universe model prepared for the Gaia simulation has", "been statistically analysed at a given time. Ingredients of the model", "are described, with the greatest emplasis on the stellar content, the", "double and multiple stars, and variability.", "**************************************************************************", "* *", "* The simulated catalogue will be soon available *", "* *", "**************************************************************************"], "curator": "Patricia Vannier [CDS]", "date_update": "10-Oct-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_A&A_548_o.A66"}} {"id": "J/A+A/548/A66", "title_cds": "SDSS Quasar Catalog, DR9Q", "title_create": "Paris+, 2012", "year": "2012", "author": "Paris I., Petitjean P., Aubourg E., Bailey S., Ross N.P., Myers A.D., Strauss M.A., Anderson S.F., Arnau E., Bautista J., Bizyaev D., Bolton A.S., Bovy J., Brandt W.N., Brewington H., Brownstein J.R., Busca N., Capellupo D., Carithers W., Croft R.A.C., Dawson K., Delubac T., Ebelke G., Eisenstein D.J., Engelke P., Fan X., Filiz Ak N., Finley H., Font-Ribera A., Ge J., Gibson R.R., Hall P.B., Hamann F., Hennawi J.F., Ho S., Hogg D.W., Ivezic Z., Jiang L., Kimball A.E., Kirky D., Kirkpatrick J.A., Lee K-G., Le Goff J.-M., Lundgren B., MacLeod C.L., Malanushenko E., Malanushenko V., Maraston C., McGreer I.D., McMahon R.G., Miralda-Escude J., Muna D., Noterdaeme P., Oravetz D., Palanque-Delabrouille N., Pan K., Perez-Fournon I., Pieri M.M., Richards G.T., Rollinde E., Sheldon E.S., Schlegel D.J., Schneider D.P., Slosar A., Shelden A., Shen Y., Simmons A., Snedden S., Suzuki N., Tinker J., Viel M., Weaver B.A., Weinberg D.W., White M., Wood-Vasey W.M., Yeche C.", "title_pub": "The Sloan Digital Sky Survey Quasar Catalog: ninth data release.", "first_author": "Paris I.", "ref_biblio": [""], "bibcode": ["2012A&A...548A..66P"], "see_also": ["VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)", "J/A+A/547/L1 : SDSS-III DR9 DLA catalogue (Noterdaeme+, 2012)", "http://www.sdss.org : SDSS Home Page"], "keyword_cds": "Surveys ; QSOs ; Active gal. nuclei", "keyword_pub": "catalogs - surveys - quasars: general", "abstract": ["We present the Data Release 9 Quasar (DR9Q) catalog from the Baryon", "Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky", "Survey III. The catalog includes all BOSS objects that were targeted", "as quasar candidates during the survey, are spectroscopically confirmed", "as quasars via visual inspection. This catalog contains 87,822 quasars", "(78,086 are new discoveries) detected over 3,275{deg}^2^ with robust", "identification and redshift measured by a combination of principal", "component eigenspectra newly derived from a training set of 8,632", "spectra from SDSS-DR7. The number of quasars with z>2.15 (61,931) is", "2.8 times larger than the number of z>2.15 quasars previously known.", "Redshifts and FWHMs are provided for the strongest emission lines", "(CIV, CIII], MgII). The catalog identifies 7,533 broad absorption line", "quasars and gives their characteristics. For each object the catalog", "presents five-band (u,g,r,i,z) CCD-based photometry with typical", "accuracy of 0.03mag, and information on the morphology and selection", "method. The catalog also contains X-ray, ultraviolet, near-infrared,", "and radio emission properties of the quasars, when available, from", "other large-area surveys. We also provide a supplemental list of an", "additional 949 quasars that have been identified, among galaxy targets", "of the BOSS or among quasar targets after DR9 was frozen."], "description": ["The SDSS-DR9 Quasar Catalog presents photometric and spectroscopic", "properties of 87,822 quasars observed by the SDSS-III/BOSS survey. We", "provide the catalog in the form of a fits file but also an ascii file.", "We also provide a supplemental list containing 949 quasars with", "exactly the same format as the main catalog."], "date_update": "10-Oct-2022", "tables": [{"name": "dr9q.dat", "desc": "Main DR9 Quasar catalog ", "columns": [{"name": "SDSS", "desc": "SDSS-DR9 designation (HHMMSS.ss+DDMMSS.s) "}, {"name": "RAdeg", "desc": "Right ascension (J2000.0) "}, {"name": "DEdeg", "desc": "Declination (J2000.0) "}, {"name": "THINGID", "desc": "[26159535/512342668] Unique identifier "}, {"name": "Plate", "desc": "SDSS Plate number "}, {"name": "MJD", "desc": "SDSS Spectroscopic MJD "}, {"name": "Fiber", "desc": "SDSS Fiber number "}, {"name": "z.v", "desc": "Visual inspection redshift "}, {"name": "z.b", "desc": "BOSS pipeline redshift "}, {"name": "e_z.b", "desc": "?=-1 Error on pipeline redshift "}, {"name": "f_z.b", "desc": "[0/196] zwarning flag (G2) "}, {"name": "z.p", "desc": "?=-1 PCA redshift (G3) "}, {"name": "e_z.p", "desc": "?=-1 Error on PCA redshift (G3) "}, {"name": "qCont", "desc": "[0/1]?=-1 Quality of PCA continuum (G3) "}, {"name": "zCIV", "desc": "?=-1 CIV redshift "}, {"name": "zCIII", "desc": "?=-1 CIII] complex redshift "}, {"name": "zMgII", "desc": "?=-1 MgII redshift "}, {"name": "Morph", "desc": "[0/1] Morphology flag (0=point, 1=extended) "}, {"name": "Btarg1", "desc": "?=0 Main (BOSS) survey primary target selection flags (G4)"}, {"name": "Atarg1", "desc": "?=0 Ancillary target selection flag 1 (G4) "}, {"name": "Atarg2", "desc": "?=0 Ancillary target selection flag 2 (G4) "}, {"name": "f7", "desc": "[0/1] 1=quasar in SDSS-DR7 (Cat. VII/260) "}, {"name": "Plate7", "desc": "?=-1 SDSS DR7 Plate number "}, {"name": "MJD7", "desc": "?=-1 SDSS DR7 spectroscopic MJD "}, {"name": "Fiber7", "desc": "?=-1 SDSS DR7 Fiber number "}, {"name": "US", "desc": "[0/2]?=-1 Uniform sample flag (G6) "}, {"name": "iMAG", "desc": "?=-9999. Absolute Magnitude Mi[z=2] (G5) "}, {"name": "D(g-i)", "desc": "?=-9999. Diff. color {Delta}(g-i) (G7) "}, {"name": "alpha", "desc": "Spectral index {alpha}_{nu}_ "}, {"name": "SNRsp", "desc": "Median S/N ratio (whole spectrum) "}, {"name": "SNR1700", "desc": "?=-1 Median SNR (1650-175nm rest) "}, {"name": "SNR3000", "desc": "?=-1 Median SNR (2950-305nm rest) "}, {"name": "SNR5150", "desc": "?=-1 Median SNR (5100-525nm rest) "}, {"name": "FW(CIV)", "desc": "?=-1 FWHM of CIV emission "}, {"name": "HW(CIV)b", "desc": "?=-1 Blue HWHM of CIV emission "}, {"name": "HW(CIV)r", "desc": "?=-1 Red HWHM of CIV emission "}, {"name": "A(CIV)", "desc": "?=-1 Amplitude of CIV emission "}, {"name": "W(CIV)", "desc": "?=-1 Rest equivalent width of CIV emission "}, {"name": "e_W(CIV)", "desc": "?=-1 Error on rest EW of CIV emission "}, {"name": "FW(CIII)", "desc": "?=-1 FWHM of CIII] complex "}, {"name": "HW(CIII)b", "desc": "?=-1 Blue HWHM of CIII] complex "}, {"name": "HW(CIII)r", "desc": "?=-1 Red HWHM of CIII] complex "}, {"name": "A(CIII)", "desc": "?=-1 Amplitude of CIII] complex "}, {"name": "W(CIII)", "desc": "?=-1 Rest equivalent width of CIII] complex "}, {"name": "e_W(CIII)", "desc": "?=-1 Error on rest EW of CIII] complex "}, {"name": "FW(MgII)", "desc": "?=-1 FWHM of MgII emission "}, {"name": "HW(MgII)b", "desc": "?=-1 Blue HWHM of MgII emission "}, {"name": "HW(MgII)r", "desc": "?=-1 Red HWHM of MgII emission "}, {"name": "A(MgII)", "desc": "?=-1 Amplitude of MgII emission "}, {"name": "W(MgII)", "desc": "?=-1 Rest equivalent width of MgII emission "}, {"name": "e_W(MgII)", "desc": "?=-1 Error on rest EW of MgII emission "}, {"name": "BAL-VI", "desc": "[0/1] BAL flag from visual inspection "}, {"name": "BI(CIVt)", "desc": "?=-1 Balnicity index (BI) of CIV trough "}, {"name": "e_BI(CIVt)", "desc": "?=-1 Error on BI of CIV trough "}, {"name": "AI(CIVt)", "desc": "?=-1 AI index of CIV trough "}, {"name": "e_AI(CIVt)", "desc": "?=-1 Error on AI of CIV trough "}, {"name": "DI(CIVt)", "desc": "?=-1 Detection index (DI) of CIV trough "}, {"name": "e_DI(CIVt)", "desc": "?=-1 Error on the DI of CIV trough "}, {"name": "Chi2CIVt", "desc": "Chi2 of the CIV troughs "}, {"name": "N2t", "desc": "[0/5] Number of CIV troughs > 1999km/s "}, {"name": "Vmin2t", "desc": "?=0 Min velocity of CIV troughs (NCIV2) "}, {"name": "Vmax2t", "desc": "?=0 Max velocity of CIV troughs (NCIV2) "}, {"name": "N.45t", "desc": "[0/13] Number of CIV troughs > 449km/s "}, {"name": "Vmin.45t", "desc": "Min velocity of CIV troughs (NCIV4.5) "}, {"name": "Vmax.45t", "desc": "Max velocity of CIV troughs (NCIV4.5) "}, {"name": "W(SiIVt)", "desc": "?=0 Rest equivalent width of SiIV trough "}, {"name": "W(CIVt)", "desc": "?=0 Rest equivalent width of CIV trough "}, {"name": "W(AlIIIt)", "desc": "?=0 Rest equivalent width of AlIII trough "}, {"name": "Run", "desc": "Imaging Run Number "}, {"name": "Ph-MJD", "desc": "Photometric MJD "}, {"name": "Rerun", "desc": "Photometric Processing Rerun number "}, {"name": "Colcam", "desc": "[1/6] camera column number "}, {"name": "Field", "desc": "Field number "}, {"name": "objID", "desc": "?=-9999. Object Identification number "}, {"name": "Fu", "desc": "?=-9999. u-band flux (in nanomaggies) (G1) "}, {"name": "e_Fu", "desc": "?=-9999. Error on Fu (in nanomaggies) (G1) "}, {"name": "Fg", "desc": "?=-9999. g-band flux (in nanomaggies) (G1) "}, {"name": "e_Fg", "desc": "?=-9999. Error on Fg (in nanomaggies) (G1) "}, {"name": "Fr", "desc": "?=-9999. r-band flux (in nanomaggies) (G1) "}, {"name": "e_Fr", "desc": "?=-9999. Error on Fr (in nanomaggies) (G1) "}, {"name": "Fi", "desc": "?=-9999. i-band flux (in nanomaggies) (G1) "}, {"name": "e_Fi", "desc": "?=-9999. Error on Fi (in nanomaggies) (G1) "}, {"name": "Fz", "desc": "?=-9999. z-band flux (in nanomaggies) (G1) "}, {"name": "e_Fz", "desc": "?=-9999. Error on Fz (in nanomaggies) (G1) "}, {"name": "Fut", "desc": "?=-9999 TARGET flux in the u-band (in nanomaggies) (G1)"}, {"name": "Fgt", "desc": "?=-9999 TARGET flux in the g-band (in nanomaggies) (G1)"}, {"name": "Frt", "desc": "?=-9999 TARGET flux in the r-band (in nanomaggies) (G1)"}, {"name": "Fit", "desc": "?=-9999 TARGET flux in the i-band (in nanomaggies) (G1)"}, {"name": "Fzt", "desc": "?=-9999 TARGET flux in the z-band (in nanomaggies) (G1)"}, {"name": "Extu", "desc": "u-band Galactic extinction "}, {"name": "logNHI", "desc": "?=-9 log of Galactic HI column density "}, {"name": "logXcr", "desc": "?=-9 log RASS full band count rate "}, {"name": "SNR(X)", "desc": "?=-9 SNR of RASS count rate "}, {"name": "sepX", "desc": "[0] SDSS-RASS separation "}, {"name": "FNUV", "desc": "NUV flux (GALEX) (in nanomaggies) (G1) "}, {"name": "e_FNUV", "desc": "?=0 Error on NUV flux (in nanomaggies)(G1) "}, {"name": "FFUV", "desc": "FUV flux (GALEX) (in nanomaggies) (G1) "}, {"name": "e_FFUV", "desc": "?=0 Error on FUV flux (in nanomaggies)(G1) "}, {"name": "Jmag", "desc": "?=0 J-band magnitude (Vega, 2MASS) "}, {"name": "e_Jmag", "desc": "?=-1 Error on J-band magnitude "}, {"name": "SNR(J)", "desc": "?=-1 J-band SNR "}, {"name": "f_Jmag", "desc": "[0/6] J-band photometry flag "}, {"name": "Hmag", "desc": "?=0 H-band magnitude (Vega, 2MASS) "}, {"name": "e_Hmag", "desc": "?=-1 Error on H-band magnitude "}, {"name": "SNR(H)", "desc": "?=-1 H-band SNR "}, {"name": "f_Hmag", "desc": "[0/6] H-band photometry flag "}, {"name": "Kmag", "desc": "?=0 K-band magnitude (Vega, 2MASS) "}, {"name": "e_Kmag", "desc": "?=-1 Error on K-band magnitude "}, {"name": "SNR(K)", "desc": "?=-1 K-band SNR "}, {"name": "f_Kmag", "desc": "[0/6] K-band photometry flag "}, {"name": "sep2", "desc": "?=0 SDSS-2MASS separation "}, {"name": "W1mag", "desc": "?=0 W1 magnitude (Vega, WISE=Cat. II/311) "}, {"name": "e_W1mag", "desc": "?=0 Error on W1 magnitude "}, {"name": "W1SNR", "desc": "?=0 SNR in W1 band "}, {"name": "W1chi2", "desc": "?=0 Chi2 in W1 band "}, {"name": "W2mag", "desc": "?=0 W2 magnitude (Vega, WISE=Cat. II/311) "}, {"name": "e_W2mag", "desc": "?=0 Error on W2 magnitude "}, {"name": "W2SNR", "desc": "?=0 SNR in W2 band "}, {"name": "W2chi2", "desc": "?=0 Chi2 in W2 band "}, {"name": "W3mag", "desc": "?=0 W3 magnitude (Vega, WISE=Cat. II/311) "}, {"name": "e_W3mag", "desc": "?=0 Error on W3 magnitude "}, {"name": "W3SNR", "desc": "?=0 SNR in W3 band "}, {"name": "W3chi2", "desc": "?=0 Chi2 in W3 band "}, {"name": "W4mag", "desc": "?=0 W4 magnitude (Vega, WISE=Cat. II/311) "}, {"name": "e_W4mag", "desc": "?=0 Error on W4 magnitude "}, {"name": "W4SNR", "desc": "?=0 SNR in W4 band "}, {"name": "W4chi2", "desc": "?=0 Chi2 in W4 band "}, {"name": "sepW", "desc": "?=0 SDSS-WISE separation "}, {"name": "F1p", "desc": "?=0 FIRST (Cat. VIII/90) peak flux density at 20cm"}, {"name": "SNR(1)", "desc": "?=0 SNR of the FIRST flux density "}, {"name": "sep1", "desc": "?=0 SDSS-FIRST separation "}]}, {"name": "dr9q.fits", "desc": "Main DR9 Quasar catalog, FITS format ", "columns": []}, {"name": "dr9qsup.dat", "desc": "Supplemental list ", "columns": [{"name": "SDSS", "desc": "SDSS-DR9 designation (HHMMSS.ss+DDMMSS.s) (1) "}, {"name": "RAdeg", "desc": "? Right ascension (J2000.0) (1) "}, {"name": "DEdeg", "desc": "? Declination (J2000.0) (1) "}, {"name": "THINGID", "desc": "?=-1 Unique identifier (1) "}, {"name": "Plate", "desc": "SDSS Plate number "}, {"name": "MJD", "desc": "SDSS Spectroscopic MJD "}, {"name": "Fiber", "desc": "SDSS Fiber number "}, {"name": "z.v", "desc": "Visual inspection redshift "}, {"name": "z.b", "desc": "BOSS pipeline redshift "}, {"name": "e_z.b", "desc": "?=-1 Error on pipeline redshift "}, {"name": "f_z.b", "desc": "[0/134] zwarning flag (G2) "}, {"name": "z.p", "desc": "?=-1 PCA redshift (G3) "}, {"name": "e_z.p", "desc": "?=-1 Error on PCA redshift (G3) "}, {"name": "qCont", "desc": "?=-1 Quality of PCA continuum (G3) "}, {"name": "zCIV", "desc": "?=-1 CIV redshift "}, {"name": "zCIII", "desc": "?=-1 CIII] complex redshift "}, {"name": "zMgII", "desc": "?=-1 MgII redshift "}, {"name": "Morph", "desc": "[0/1] Morphology flag (0=point, 1=extended) "}, {"name": "Btarg1", "desc": "?=1 Main (BOSS) survey primary target selection flags (G4)"}, {"name": "Atarg1", "desc": "?=1 Ancillary target selection flag 1 (G4) "}, {"name": "Atarg2", "desc": "?=1 Ancillary target selection flag 2 (G4) "}, {"name": "alpha", "desc": "Spectral index {alpha}_{nu}_ "}, {"name": "SNRsp", "desc": "Median SNR (whole spectrum) "}, {"name": "SNR1700", "desc": "?=-1 Median SNR (1650-175nm rest) "}, {"name": "SNR3000", "desc": "?=-1 Median SNR (2950-305nm rest) "}, {"name": "SNR5150", "desc": "?=-1 Median SNR (5100-525nm rest) "}, {"name": "FW(CIV)", "desc": "?=-1 FWHM of CIV emission "}, {"name": "HW(CIV)b", "desc": "?=-1 Blue HWHM of CIV emission "}, {"name": "HW(CIV)r", "desc": "?=-1 Red HWHM of CIV emission "}, {"name": "A(CIV)", "desc": "?=-1 Amplitude of CIV emission "}, {"name": "W(CIV)", "desc": "?=-1 Rest equivalent width of CIV emission "}, {"name": "e_W(CIV)", "desc": "?=-1 Error on rest EW of CIV emission "}, {"name": "FW(CIII)", "desc": "?=-1 FWHM of CIII] complex "}, {"name": "HW(CIII)b", "desc": "?=-1 Blue HWHM of CIII] complex "}, {"name": "HW(CIII)r", "desc": "?=-1 Red HWHM of CIII] complex "}, {"name": "A(CIII)", "desc": "?=-1 Amplitude of CIII] complex "}, {"name": "W(CIII)", "desc": "?=-1 Rest equivalent width of CIII] complex "}, {"name": "e_W(CIII)", "desc": "?=-1 Error on rest EW of CIII] complex "}, {"name": "FW(MGII)", "desc": "?=-1 FWHM of MgII emission "}, {"name": "HW(MGII)b", "desc": "?=-1 Blue HWHM of MgII emission "}, {"name": "HW(MGII)r", "desc": "?=-1 Red HWHM of MgII emission "}, {"name": "A(MGII)", "desc": "?=-1 Amplitude of MgII emission "}, {"name": "W(MGII)", "desc": "?=-1 Rest equivalent width of MgII emission "}, {"name": "e_W(MGII)", "desc": "?=-1 Error on rest EW of MgII emission "}, {"name": "BAL-VI", "desc": "[0/1] BAL flag from visual inspection "}, {"name": "BI(CIVt)", "desc": "?=-1 Balnicity index (BI) of CIV trough "}, {"name": "e_BI(CIVt)", "desc": "?=-1 Error on BI of CIV trough "}, {"name": "AI(CIVt)", "desc": "?=-1 AI index of CIV trough "}, {"name": "e_AI(CIVt)", "desc": "?=-1 Error on AI of CIV trough "}, {"name": "DI(CIVt)", "desc": "?=-1 Detection index (DI) of CIV trough "}, {"name": "e_DI(CIVt)", "desc": "?=-1 Error on the DI of CIV trough "}, {"name": "Chi2CIVt", "desc": "?=-1 Chi2 of the CIV troughs "}, {"name": "N2t", "desc": "?=-1 Number of CIV troughs > 1999km/s "}, {"name": "Vmin2t", "desc": "?=0 Min velocity of CIV troughs (NCIV2) "}, {"name": "Vmax2t", "desc": "?=0 Max velocity of CIV troughs (NCIV2) "}, {"name": "N.45t", "desc": "?=-1 Number of CIV troughs > 449km/s "}, {"name": "Vmin.45t", "desc": "Min velocity of CIV troughs (NCIV4.5) "}, {"name": "Vmax.45t", "desc": "Max velocity of CIV troughs (NCIV4.5) "}, {"name": "Run", "desc": "?=0 Imaging Run Number "}, {"name": "Ph-MJD", "desc": "?=0 Photometric MJD "}, {"name": "Rerun", "desc": "? Photometric Processing Rerun number "}, {"name": "Colcam", "desc": "?=0 camera column number "}, {"name": "Field", "desc": "?=0 Field number "}, {"name": "OBJID", "desc": "? Object Identification number "}, {"name": "Fu", "desc": "?=-999. u-band flux (in nanomaggies) (G1) "}, {"name": "e_Fu", "desc": "?=-9. Error on Fu (in nanomaggies) (G1) "}, {"name": "Fg", "desc": "?=-999. g-band flux (in nanomaggies) (G1) "}, {"name": "e_Fg", "desc": "?=-9. Error on Fg (in nanomaggies) (G1) "}, {"name": "Fr", "desc": "?=-999. r-band flux (in nanomaggies) (G1) "}, {"name": "e_Fr", "desc": "?=-9. Error on Fr (in nanomaggies) (G1) "}, {"name": "Fi", "desc": "?=-999. i-band flux (in nanomaggies) (G1) "}, {"name": "e_Fi", "desc": "?=-9. Error on Fi (in nanomaggies) (G1) "}, {"name": "Fz", "desc": "?=-999. z-band flux (in nanomaggies) (G1) "}, {"name": "e_Fz", "desc": "?=-9. Error on Fz (in nanomaggies) (G1) "}, {"name": "Extu", "desc": "u-band Galactic extinction "}]}, {"name": "dr9q_sup.fits", "desc": "Supplemental list, FITS format ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_Ap+SS_163.275"}} {"id": "J/other/ApSS/163.275", "title_cds": "UV & Geneva photometry around HD 173009", "title_create": "Reichen+, 1990", "year": "1990", "author": "Reichen M., Lanz T., Golay M., Huguenin D.", "title_pub": "A detailed study of a 6{deg} diameter field in Scutum. I. Data presentation and overall description of the interstellar matter distribution.", "first_author": "Reichen M.", "ref_biblio": [""], "bibcode": ["1990Ap&SS.163..275R"], "see_also": ["II/59 : Catalogue of stellar UV fluxes (TD1) (Thompson+ 1978)"], "keyword_cds": "Surveys ; Photometry, ultraviolet ; Photometry, Geneva ; MK spectral classification", "abstract": ["A 6{deg} diameter field centered on the star {epsilon} Scutum has been", "selected from the SCAP-2000 balloon-borne UV survey for its high", "apparent stellar density contrast and relatively good transparency on", "a small projected portion of the galactic plane. In view of a detailed", "study of the absorption and interstellar matter distribution in this", "field, a large collection of data has been made and is presented here.", "Ultraviolet magnitudes at 2000{AA} have been obtained from the", "reduction of three SCAP frames. In addition, 322 stars among the 487", "stars detected on the UV frames have been measured in the Geneva", "photometric system. For a small number of photometrically distant", "objects, medium resolution spectra have been obtained in order to", "determine spectral types and confirm the distances determination. An", "overall description of the distribution of interstellar material in", "the ultraviolet is made using star counting methods, and is confronted", "to similar studies in the visible range. A discussion of the", "variations of the extinction law in different parts of the field is", "made. A new distance determination of the Sct OB2 association is", "proposed, as well as a list of additional probable members of the", "association. A certain number of distant hot stars seem to indicate", "the presence of an unknown OB association at the edge of the Scutum", "spiral arm, at a distance of over 3 kpc from the Sun."], "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Calibration stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (see Table2) "}, {"name": "Name", "desc": "HD, BD or CSI identification "}, {"name": "SpType", "desc": "Spectral type (see table 2) "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude from the Geneva system"}, {"name": "UVmag", "desc": "UV magnitude at 2000{AA} deduced from calibration"}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag "}, {"name": "n_UVmag", "desc": "[abcd ] Note on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965{AA} passband of the TD1 catalogue (Thompson et al., 1978, Cat. ). (2)"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "n_UVmagTD1", "desc": "[)] ) indicates that the UV magnitude UVmagboxes was preferred for the calibration"}, {"name": "UVmagboxes", "desc": "UV magnitude deduced by the method of the so-called \"photometric boxes\" (see text.) (3)"}, {"name": "e_UVmagboxes", "desc": "rms uncertainty on UVmagboxes "}, {"name": "n_UVmagboxes", "desc": "[)] ) indicates that the UV magnitude UVmagTD1 was preferred for the calibration"}, {"name": "N", "desc": "Number of stars in the photometric box "}, {"name": "Rem", "desc": "Remarks related to the UV_TD1_ magnitudes (G2) "}]}, {"name": "table2.dat", "desc": "All stars measured on SCAP frames 11.65/14.48/14.49 ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (1) "}, {"name": "n_SCAP", "desc": "[* o] \"*\" star measured in the Geneva system (see Table 3) \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[+*] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (see Table 3) "}, {"name": "Vmag", "desc": "? Visual magnitude (3) "}, {"name": "UVmag", "desc": "UV magnitude at 2000A from the SCAP frames "}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag (4) "}, {"name": "n_UVmag", "desc": "[abcd ] Notes on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965A passband of the TD1 catalogue (Thompson et al., 1978, )"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "UV-V", "desc": "? (UVmag-Vmag) color index "}, {"name": "(UV-V)0", "desc": "? Intrinsic (UV-V)_0_ color index taken from Carnochan (1982) following the MK, photometric or other spectra type"}, {"name": "E(UV-V)", "desc": "? UV color excess (from (UV-V) and (UV-V)0) "}, {"name": "Rem", "desc": "Various remarks and comments (G2) "}]}, {"name": "table3.dat", "desc": "All stars with Geneva photometry ", "columns": [{"name": "SCAP", "desc": "SCAP identification (see Table 2) "}, {"name": "n_SCAP", "desc": "[o] \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[*+] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "GLONd", "desc": "Galactic longitude "}, {"name": "GLONm", "desc": "Galactic longitude "}, {"name": "GLATd", "desc": "Galactic latitude "}, {"name": "GLATm", "desc": "Galactic latitude "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (1) "}, {"name": "[U-B]", "desc": "Geneva [U-B] colour index "}, {"name": "[B-V]", "desc": "Geneva [B-V] colour index "}, {"name": "[B1-B]", "desc": "Geneva [B1-B] colour index "}, {"name": "[B2-B]", "desc": "Geneva [B2-B] colour index "}, {"name": "[V1-B]", "desc": "Geneva [V1-B] colour index "}, {"name": "[G-B]", "desc": "Geneva [G-B] colour index "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude "}, {"name": "E[B-V]", "desc": "? Color excess deduced from the X,Y,Z parameters (Cramer, 1982A&A...112..330C) unless stated otherwise in the remarks"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters (Cramer and Maeder, 1979A&A....78..305C) unless stated otherwise in the remarks"}, {"name": "r", "desc": "? Decuced heliocentric distance "}, {"name": "Rem", "desc": "Various remarks (2) "}]}, {"name": "table4.dat", "desc": "Spectroscopic standard stars ", "columns": [{"name": "HD", "desc": "HD identification "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "? Visible absorption derived from E[B-V]. "}, {"name": "n_AV", "desc": "[)] ): values deduced from Johnson's U-B/B-V diagram"}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypeH", "desc": "Spectral type given by Houk and Cowley (1975, ) or Houk (1978, , 1982, )"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHg", "desc": "Equivalent width of the H{gamma} line derived from our spectroscopic observations"}, {"name": "VMAGHg", "desc": "Absolute magnitude derived from EW_H{gamma}_ using calibrations by Millward and Walker (1985ApJS...57...63M) or Hill et al. (1986PASP...98.1186H)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}]}, {"name": "table5.dat", "desc": "Spectroscopy of Scutum field stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "Visible absorption derived from E[B-V] "}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHa", "desc": "Equivalent width of the H{alpha} line derived from our spectroscopic observations"}, {"name": "u_EWHa", "desc": "[)] Uncertainty flag on EWHa "}, {"name": "VMAGHa", "desc": "? Absolute magnitude derived from EW_H{alpha}_ (See notes to Table 4)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}, {"name": "Rem", "desc": "Individual remarks (1) "}]}, {"name": "notes2.dat", "desc": "Individual notes to table2.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "notes3.dat", "desc": "Individual notes to table3.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_MNRAS_486L_46"}} {"id": "J/MNRAS/486L/46", "title_cds": "GRB E_p_-E_iso_ correlation circularity problem", "title_create": "Amati+, 2019", "year": "2019", "author": "Amati L., D'Agostino R., Luongo O., Muccino M., Tantalo M.", "title_pub": "Addressing the circularity problem in the E_p_-E_iso_ correlation of gamma-ray bursts.", "first_author": "Amati L.", "ref_biblio": [""], "bibcode": ["2019MNRAS.486L..46A"], "keyword_cds": "GRB ; Gamma rays ; Redshifts", "keyword_pub": "cosmology: observations - dark energy - gamma-rays: general", "abstract": ["We here propose a new model-independent technique to overcome the", "circularity problem affecting the use of gamma-ray bursts (GRBs) as", "distance indicators through the use of E_p_-E_iso_ correlation. We", "calibrate the E_p_-E_iso_ correlation and find the GRB distance moduli", "that can be used to constrain dark energy models. We use observational", "Hubble data to approximate the cosmic evolution through Bezier", "parametric curve obtained through the linear combination of Bernstein", "basis polynomials. In doing so, we build up a new data set consisting", "of 193 GRB distance moduli. We combine this sample with the supernova", "JLA data set to test the standard {Lambda}CDM model and its wCDM", "extension. We place observational constraints on the cosmological", "parameters through Markov Chain Monte Carlo numerical technique.", "Moreover, we compare the theoretical scenarios by performing the", "Akaike and Deviance Information statistical Criteria. For the", "{Lambda}CDM model we find {Omega}_m_=0.397^+0.040^_-0.039_ at the", "2{sigma} level, while for the wCDM model we obtain", "{Omega}_m_=0.34^+0.13^_-0.15_ and w=-0.86^+0.36^_-0.38_ at the", "2{sigma} level. Our analysis suggests that {Lambda}CDM model is", "statistically favoured over the wCDM scenario. No evidence for", "extension of the {Lambda}CDM model is found."], "description": ["In this work, we faced out the circularity problem in using GRBs as", "distance indicators. To do so, we employed the E_p_-E_iso_ correlation", "(Amati et al. 2008MNRAS.391..577A) and we proposed a new technique to", "build d_L_ in a model-independent way, using the most recent values of", "observational Hubble Data (OHD) (see Capozziello et al.", "2018MNRAS.476.3924C). In particular, we considered the OHD data points", "and we approximated the Hubble function by means of a Bezier", "parametric curve obtained from the linear combinations of Bernstein's", "polynomials. Assuming vanishing spatial curvature as suggested by", "Planck's results, we were able to calibrate the Amati relation in a", "model-independent way. We thus obtained a new sample of distance", "moduli for 193 different GRBs (see Table A1)."], "date_update": "12-Oct-2022", "tables": [{"name": "tablea1.dat", "desc": "List of the full sample of GRBs used in this work and their redshift z and calibrated {mu}_GRB_", "columns": [{"name": "Name", "desc": "Gamma-Ray Burst name (GRB YYMMDDA) "}, {"name": "z", "desc": "Redshift "}, {"name": "muGRB", "desc": "GRB distance moduli {mu}_GRB_ (1) "}, {"name": "e_muGBR", "desc": "Error on muGRB "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_Natur_585.363"}} {"id": "J/other/Nat/585.363", "title_cds": "WD 1856+534 transit curves", "title_create": "Vanderburg+, 2020", "year": "2020", "author": "Vanderburg A., Rappaport S.A., Xu S., Crossfield I.J.M., Becker J.C., Gary B., Murgas F., Blouin S., Kaye T.G., Palle E., Melis C., Morris B.M., Kreidberg L., Gorjian V., Morley C.V., Mann A.W., Parviainen H., Pearce L.A., Newton E.R., Carrillo A., Zuckerman B., Nelson L., Zeimann G., Brown W.R., Tronsgaard R., Klein B., Ricker G.R., Vanderspek R.K., Latham D.W., Seager S., Winn J.N., Jenkins J.M., Adams F.C., Benneke B., Berardo D., Buchhave L.A., Caldwell D.A., Christiansen J.L., Collins K.A., Colon K.D., Daylan T., Doty J., Doyle A.E., Dragomir D., Dressing C., Dufour P., Fukui A., Glidden A., Guerrero N.M., Guo X., Heng K., Henriksen A.I., Huang C.X., Kaltenegger L., Kane S.R., Lewis J.A., Lissauer J.J., Morales F., Narita N., Pepper J., Rose M.E., Smith J.C., Stassun K.G., Yu L.", "title_pub": "A giant planet candidate transiting a white dwarf.", "first_author": "Vanderburg A.", "ref_biblio": [""], "bibcode": ["2020Natur.585..363V"], "keyword_cds": "Stars, white dwarf ; Spectra, optical ; Photometry, SDSS", "abstract": ["Astronomers have discovered thousands of planets outside the Solar", "System, most of which orbit stars that will eventually evolve into red", "giants and then into white dwarfs. During the red giant phase, any", "close-orbiting planets will be engulfed by the star, but more distant", "planets can survive this phase and remain in orbit around the white", "dwarf. Some white dwarfs show evidence for rocky material floating in", "their atmospheres5, in warm debris disks or orbiting very closely,", "which has been interpreted as the debris of rocky planets that were", "scattered inwards and tidally disrupted. Recently, the discovery of", "a gaseous debris disk with a composition similar to that of ice giant", "planets14 demonstrated that massive planets might also find their way", "into tight orbits around white dwarfs, but it is unclear whether these", "planets can survive the journey. So far, no intact planets have been", "detected in close orbits around white dwarfs. Here we report the", "observation of a giant planet candidate transiting the white dwarf", "WD 1856+534 (TIC 267574918) every 1.4days. We observed and modelled", "the periodic dimming of the white dwarf caused by the planet candidate", "passing in front of the star in its orbit. The planet candidate is", "roughly the same size as Jupiter and is no more than 14 times as", "massive (with 95 per cent confidence). Other cases of white dwarfs", "with close brown dwarf or stellar companions are explained as the", "consequence of common-envelope evolution, wherein the original orbit", "is enveloped during the red giant phase and shrinks owing to friction.", "In this case, however, the long orbital period (compared with other", "white dwarfs with close brown dwarf or stellar companions) and low", "mass of the planet candidate make common-envelope evolution less", "likely. Instead, our findings for the WD 1856+534 system indicate that", "giant planets can be scattered into tight orbits without being tidally", "disrupted, motivating the search for smaller transiting planets around", "white dwarfs."], "description": ["We show spectra from four observatories, using the Low Resolution", "Spectrograph 2 on the Hobby-Eberly Telescope (HET/LRS2), the Gemini", "Near InfraRed Spectrograph on the Gemini North Telescope", "(Gemini/GNIRS), the Kast Double Spectrograph on the Shane Telescope at", "Lick Observatory (Lick/Kast) and the Blue Channel spectrograph at MMT", "Observatory. The data have been scaled to remove offsets in their", "absolute flux calibrations. The optical spectra show a pure continuum,", "confirming the DC spectral classification, whereas the near-infrared", "spectrum from Gemini North shows only spurious features, owing to", "imperfect correction of the telluric absorption and sky emission from", "Earth's atmosphere.", "We show the light curves from TESS; data from several private", "telescopes in Arizona (operated by B.G. and T.G.K.) with odd and", "even-numbered transits shown separately; simultaneous light curves in", "four colours from MuSCAT2; a light curve from the GTC, and a light", "curve from Spitzer. The individual two-minute-cadence TESS flux", "measurements are shown as grey points, and the rose-coloured points", "are averages of the brightness in roughly 30s in orbital phase. The", "TESS data have been corrected for dilution from nearby stars so that", "the transit depth matches that of the GTC data."], "object": ["18 57 39.34 +53 30 33.3 WD 1856+534 = TOI 1690"], "date_update": "17-Nov-2020", "tables": [{"name": "fig2.dat", "desc": "Spectroscopic observation of WD 1856+534 ", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "RelFlux", "desc": "? Relative Flux "}, {"name": "Inst", "desc": "Observatory/Spectrograph (1) "}]}, {"name": "fig2ext.dat", "desc": "All transit observation of WD 1856+534 ", "columns": [{"name": "Time", "desc": "Observation date (TDB) "}, {"name": "Relmag", "desc": "Relative Brightness "}, {"name": "Inst", "desc": "Observatory/Filter (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_Ap_32.252"}} {"id": "J/other/Ap/32.252", "title_cds": "Second Byurakan Spectral Sky Survey. VII.", "title_create": "Stepanyan+, 1990", "year": "1990", "author": "Stepanyan D.A., Lipovetskii V.A., Erastova L.K.", "title_pub": "Second Byurakan Spectral Sky Survey. VII. Results fo R region centered on alpha=12h00m, delta=+59d00.", "first_author": "Stepanyan D.A.", "ref_biblio": [""], "bibcode": ["1990Ap.....32..252S"], "keyword_cds": "", "abstract": ["The paper gives the seventh list of objects of the Second Byurakan", "Spectral Sky Survey situated in an area measuring 4{deg}x4{deg} with", "coordinates of its center RA=12:00, DE=+59:00. The observations", "were made with the 40\"-52\" Schmidt telescope of the Byurakan", "Astrophysical Observatory with a set of three objective prisms. The", "list contains data on 94 peculiar objects and galaxies and 12 blue", "stars. This part of the survey has revealed II QSOs, two galaxies", "exhibiting Seyfert features, 20 BSOs, 29 galaxies with appreciable", "ultraviolet continuum, and 34 emission galaxies without significant", "ultraviolet radiation. The surface density of QSOs and Seyferts in the", "investigated area is about unity, while for emission galaxies it is of", "the order of four per square degree down to the 19th magnitude."], "object": [], "curator": "Alexandra Bauer, Patricia Vannier [CDS]", "doi_pub": ["10.1007/BF01005507"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_Ap_43.413"}} {"id": "J/other/Ap/43.413", "title_cds": "Ellipticity of nearby elliptical galaxies", "title_create": "Andreasyan+, 2000", "year": "2000", "author": "Andreasyan R.R., Sol H.", "title_pub": "Ellipticity of nearby elliptical galaxies identified with extended extragalactic radio sources.", "first_author": "Andreasyan R.R.", "ref_biblio": [""], "bibcode": ["2000Ap.....43..413A"], "keyword_cds": "Radio sources ; Galaxies, radio ; Morphology", "abstract": ["The dependence of the ellipticity of nearby optical galaxies", "associated with extragalactic radio sources on the type of radio", "galaxy is considered. It is shown that elliptical galaxies identified", "with radio galaxies of the FRI type and with radio sources having a", "radio image with a small elongation have a smaller ellipticity, on the", "average, than those associated with radio galaxies of the FRII type", "and with radio sources with greater elongation. As one possible", "explanation for this phenomenon, one can assume that the optical", "galaxies associated with radio galaxies of type FRI and with radio", "sources of small elongation are oriented in space so that they are", "observed edge-on relatively rarely."], "doi_pub": ["10.1023/A:1010962807367"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Parameters of the radio sources ", "columns": [{"name": "Name", "desc": "Radio source designation (based on B1950 position) "}, {"name": "E", "desc": "Ellipticity "}, {"name": "l_K", "desc": "Limit flag on K "}, {"name": "K", "desc": "? Ratio of the major to the minor axes "}, {"name": "FR", "desc": "Fanaroff & Riley (1974MNRAS.167p..31F) FR type "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_ApSS_163.275"}} {"id": "J/other/ApSS/163.275", "title_cds": "UV & Geneva photometry around HD 173009", "title_create": "Reichen+, 1990", "year": "1990", "author": "Reichen M., Lanz T., Golay M., Huguenin D.", "title_pub": "A detailed study of a 6{deg} diameter field in Scutum. I. Data presentation and overall description of the interstellar matter distribution.", "first_author": "Reichen M.", "ref_biblio": [""], "bibcode": ["1990Ap&SS.163..275R"], "see_also": ["II/59 : Catalogue of stellar UV fluxes (TD1) (Thompson+ 1978)"], "keyword_cds": "Surveys ; Photometry, ultraviolet ; Photometry, Geneva ; MK spectral classification", "abstract": ["A 6{deg} diameter field centered on the star {epsilon} Scutum has been", "selected from the SCAP-2000 balloon-borne UV survey for its high", "apparent stellar density contrast and relatively good transparency on", "a small projected portion of the galactic plane. In view of a detailed", "study of the absorption and interstellar matter distribution in this", "field, a large collection of data has been made and is presented here.", "Ultraviolet magnitudes at 2000{AA} have been obtained from the", "reduction of three SCAP frames. In addition, 322 stars among the 487", "stars detected on the UV frames have been measured in the Geneva", "photometric system. For a small number of photometrically distant", "objects, medium resolution spectra have been obtained in order to", "determine spectral types and confirm the distances determination. An", "overall description of the distribution of interstellar material in", "the ultraviolet is made using star counting methods, and is confronted", "to similar studies in the visible range. A discussion of the", "variations of the extinction law in different parts of the field is", "made. A new distance determination of the Sct OB2 association is", "proposed, as well as a list of additional probable members of the", "association. A certain number of distant hot stars seem to indicate", "the presence of an unknown OB association at the edge of the Scutum", "spiral arm, at a distance of over 3 kpc from the Sun."], "doi_pub": ["10.1007/BF00655749"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Calibration stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (see Table2) "}, {"name": "Name", "desc": "HD, BD or CSI identification "}, {"name": "SpType", "desc": "Spectral type (see table 2) "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude from the Geneva system"}, {"name": "UVmag", "desc": "UV magnitude at 2000{AA} deduced from calibration"}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag "}, {"name": "n_UVmag", "desc": "[abcd ] Note on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965{AA} passband of the TD1 catalogue (Thompson et al., 1978, Cat. ). (2)"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "n_UVmagTD1", "desc": "[)] ) indicates that the UV magnitude UVmagboxes was preferred for the calibration"}, {"name": "UVmagboxes", "desc": "UV magnitude deduced by the method of the so-called \"photometric boxes\" (see text.) (3)"}, {"name": "e_UVmagboxes", "desc": "rms uncertainty on UVmagboxes "}, {"name": "n_UVmagboxes", "desc": "[)] ) indicates that the UV magnitude UVmagTD1 was preferred for the calibration"}, {"name": "N", "desc": "Number of stars in the photometric box "}, {"name": "Rem", "desc": "Remarks related to the UV_TD1_ magnitudes (G2) "}]}, {"name": "table2.dat", "desc": "All stars measured on SCAP frames 11.65/14.48/14.49 ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (1) "}, {"name": "n_SCAP", "desc": "[* o] \"*\" star measured in the Geneva system (see Table 3) \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[+*] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (see Table 3) "}, {"name": "Vmag", "desc": "? Visual magnitude (3) "}, {"name": "UVmag", "desc": "UV magnitude at 2000A from the SCAP frames "}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag (4) "}, {"name": "n_UVmag", "desc": "[abcd ] Notes on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965A passband of the TD1 catalogue (Thompson et al., 1978, )"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "UV-V", "desc": "? (UVmag-Vmag) color index "}, {"name": "(UV-V)0", "desc": "? Intrinsic (UV-V)_0_ color index taken from Carnochan (1982) following the MK, photometric or other spectra type"}, {"name": "E(UV-V)", "desc": "? UV color excess (from (UV-V) and (UV-V)0) "}, {"name": "Rem", "desc": "Various remarks and comments (G2) "}]}, {"name": "table3.dat", "desc": "All stars with Geneva photometry ", "columns": [{"name": "SCAP", "desc": "SCAP identification (see Table 2) "}, {"name": "n_SCAP", "desc": "[o] \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[*+] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "GLONd", "desc": "Galactic longitude "}, {"name": "GLONm", "desc": "Galactic longitude "}, {"name": "GLATd", "desc": "Galactic latitude "}, {"name": "GLATm", "desc": "Galactic latitude "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (1) "}, {"name": "[U-B]", "desc": "Geneva [U-B] colour index "}, {"name": "[B-V]", "desc": "Geneva [B-V] colour index "}, {"name": "[B1-B]", "desc": "Geneva [B1-B] colour index "}, {"name": "[B2-B]", "desc": "Geneva [B2-B] colour index "}, {"name": "[V1-B]", "desc": "Geneva [V1-B] colour index "}, {"name": "[G-B]", "desc": "Geneva [G-B] colour index "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude "}, {"name": "E[B-V]", "desc": "? Color excess deduced from the X,Y,Z parameters (Cramer, 1982A&A...112..330C) unless stated otherwise in the remarks"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters (Cramer and Maeder, 1979A&A....78..305C) unless stated otherwise in the remarks"}, {"name": "r", "desc": "? Decuced heliocentric distance "}, {"name": "Rem", "desc": "Various remarks (2) "}]}, {"name": "table4.dat", "desc": "Spectroscopic standard stars ", "columns": [{"name": "HD", "desc": "HD identification "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "? Visible absorption derived from E[B-V]. "}, {"name": "n_AV", "desc": "[)] ): values deduced from Johnson's U-B/B-V diagram"}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypeH", "desc": "Spectral type given by Houk and Cowley (1975, ) or Houk (1978, , 1982, )"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHg", "desc": "Equivalent width of the H{gamma} line derived from our spectroscopic observations"}, {"name": "VMAGHg", "desc": "Absolute magnitude derived from EW_H{gamma}_ using calibrations by Millward and Walker (1985ApJS...57...63M) or Hill et al. (1986PASP...98.1186H)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}]}, {"name": "table5.dat", "desc": "Spectroscopy of Scutum field stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "Visible absorption derived from E[B-V] "}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHa", "desc": "Equivalent width of the H{alpha} line derived from our spectroscopic observations"}, {"name": "u_EWHa", "desc": "[)] Uncertainty flag on EWHa "}, {"name": "VMAGHa", "desc": "? Absolute magnitude derived from EW_H{alpha}_ (See notes to Table 4)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}, {"name": "Rem", "desc": "Individual remarks (1) "}]}, {"name": "notes2.dat", "desc": "Individual notes to table2.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "notes3.dat", "desc": "Individual notes to table3.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AstBu_64.123_o64.123"}} {"id": "J/other/AstBu/64.123", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. I: Construction of the sample.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..123K"], "see_also": ["J/other/AstBu/64.276 : Paper II. Photometry (Khabibullina+, 2009)", "J/other/AstBu/64.357 : Paper III. Sizes & flux densities (Khabibullina+, 2009)", "ftp://cats.sao.ru/pub/CATS/RGLIST : CATS Home Page"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio", "keyword_pub": "elliptical galaxies - quasars - active or peculiar galaxies, objects, and systems - radio galaxies - statistical and correlative studies of properties - radio sources - observational cosmology", "abstract": ["The procedure of the construction of a sample of distant (z>0.3)", "radio galaxies using NED, SDSS, and CATS databases for further", "application in statistical tests is described. The sample is assumed", "to be cleaned from objects with quasar properties. Primary statistical", "analysis of the list is performed and the regression dependence of the", "spectral index on redshift is found."], "date_update": "09-Dec-2009", "tables": [{"name": "table1.dat", "desc": "Spectral indexes and redshifts for 2442 galaxies ", "columns": [{"name": "Name", "desc": "Name of the source catalog or source name (1) "}, {"name": "n_Name", "desc": "Note on source (2) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "alf1", "desc": "? Spectral index for frequency 325MHz (3) "}, {"name": "alf2", "desc": "? Spectral index for frequency 1400MHz (3) "}, {"name": "alf3", "desc": "? Spectral index for frequency 4850MHz (3) "}, {"name": "z", "desc": "Spectroscopic redshift "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AstBu_64.123_o64.276"}} {"id": "J/other/AstBu/64.276", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. II: Photometric data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..276K"], "see_also": ["J/other/AstBu/64.123 : Paper I. Sample (Khabibullina+, 2009)", "J/other/AstBu/64.357 : Paper III. 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We report the", "photometric parameters for the objects of the list, and perform its", "preliminary statistical analysis including the construction of the", "Hubble diagrams."], "date_update": "12-Nov-2009", "tables": [{"name": "table2.dat", "desc": "Magnitudes for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "Name", "desc": "Name of galaxies "}, {"name": "Band1", "desc": "Band name (1) "}, {"name": "l_mag1", "desc": "[=>] Limit flag on Band1 "}, {"name": "mag1", "desc": "? Magnitude in mag1 "}, {"name": "e_mag1", "desc": "? rms uncertainty on mag1 "}, {"name": "u_mag1", "desc": "[)] Uncertainty flag on mag1 "}, {"name": "Band2", "desc": "Band name (1) "}, {"name": "l_mag2", "desc": "[=>] Limit flag on mag2 "}, {"name": "mag2", "desc": "? Magnitude in Band2 "}, {"name": "e_mag2", "desc": "? rms uncertainty on mag2 "}, {"name": "u_mag2", "desc": "[)] Uncertainty flag on mag2 "}, {"name": "Band3", "desc": "Band name (1) "}, {"name": "l_mag3", "desc": "[=>] Limit flag on mag3 "}, {"name": "mag3", "desc": "? Magnitude in Band3 "}, {"name": "e_mag3", "desc": "? rms uncertainty on mag3 "}, {"name": "Band4", "desc": "Band name (1) "}, {"name": "l_mag4", "desc": "[=><] Limit flag on mag4 "}, {"name": "mag4", "desc": "? Magnitude in Band4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "Band5", "desc": "Band name (1) "}, {"name": "l_mag5", "desc": "[=>] Limit flag on mag5 "}, {"name": "mag5", "desc": "? Magnitude in Band5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "Band6", "desc": "Band name (1) "}, {"name": "l_mag6", "desc": "[=>] Limit flag on mag6 "}, {"name": "mag6", "desc": "? Magnitude in Band6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "Band7", "desc": "Band name (1) "}, {"name": "l_mag7", "desc": "[=>] Limit flag on mag7 "}, {"name": "mag7", "desc": "? Magnitude in Band7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "Band8", "desc": "Band name (1) "}, {"name": "l_mag8", "desc": "[=>] Limit flag on mag8 "}, {"name": "mag8", "desc": "? Magnitude in Band8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "Band9", "desc": "Band name (1) "}, {"name": "l_mag9", "desc": "[=>] Limit flag on mag9 "}, {"name": "mag9", "desc": "? Magnitude in Band9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "Band10", "desc": "Band name (1) "}, {"name": "l_mag10", "desc": "[=>] Limit flag on mag10 "}, {"name": "mag10", "desc": "? Magnitude in Band10 "}, {"name": "Band11", "desc": "Band name (1) "}, {"name": "l_mag11", "desc": "[=>] Limit flag on mag11 "}, {"name": "mag11", "desc": "? Magnitude in Band11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AstBu_64.123_o64.357"}} {"id": "J/other/AstBu/64.357", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. III: Sizes and flux density according to the NVSS data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..357K"], "see_also": ["J/other/AstBu/64.123 : Spectral indexes and redshifts (I) (Khabibullina+, 2009)", "J/other/AstBu/64.276 : Magnitudes (II) (Khabibullina+, 2009)"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio ; Redshifts", "keyword_pub": "radio galaxies - spatial distribution of galaxies - radio sources - observational cosmology", "abstract": ["We describe the procedure of the construction of a sample of distant", "(z>0.3) radio galaxies using the NED, CATS and SDSS databases for", "further use in various statistical tests. We believe the sample to be", "free of objects with quasar properties. This paper is the third part", "of the description of the radio galaxies catalog that we plan to use", "for cosmological tests. We report the results of the sample of angular", "sizes for the NVSS survey list objects, and its preliminary", "statistical analysis. Three-parameter diagrams \"angular", "size-redshift-flux density\" and \"angular size-redshift-spectral", "index\", and their two-parameter projections are constructed. Three", "subsamples of radio galaxies are separated in the \"source size-flux", "density\" diagram."], "date_update": "12-Nov-2009", "tables": [{"name": "table3.dat", "desc": "Sizes and flux density for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "RAh", "desc": "? NVSS Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "? NVSS Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "? NVSS Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? NVSS Declination J2000 (degrees) "}, {"name": "DEm", "desc": "? NVSS Declination J2000 (minutes) "}, {"name": "DEs", "desc": "? NVSS Declination J2000 (seconds) "}, {"name": "l_MajAxis", "desc": "Limit flag on MajAxis "}, {"name": "MajAxis", "desc": "? Max diameter of source in arcsec (NVSS) "}, {"name": "l_MinAxis", "desc": "Limit flag on MinAxis "}, {"name": "MinAxis", "desc": "? Min diameter of source in arcsec (NVSS) "}, {"name": "Flux", "desc": "? 1.4GHz flux density of source (NVSS) "}, {"name": "z", "desc": "Redshift "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AstBu_64.276_o64.123"}} {"id": "J/other/AstBu/64.123", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. 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Primary statistical", "analysis of the list is performed and the regression dependence of the", "spectral index on redshift is found."], "date_update": "09-Dec-2009", "tables": [{"name": "table1.dat", "desc": "Spectral indexes and redshifts for 2442 galaxies ", "columns": [{"name": "Name", "desc": "Name of the source catalog or source name (1) "}, {"name": "n_Name", "desc": "Note on source (2) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "alf1", "desc": "? Spectral index for frequency 325MHz (3) "}, {"name": "alf2", "desc": "? Spectral index for frequency 1400MHz (3) "}, {"name": "alf3", "desc": "? Spectral index for frequency 4850MHz (3) "}, {"name": "z", "desc": "Spectroscopic redshift "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AstBu_64.276_o64.276"}} {"id": "J/other/AstBu/64.276", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. II: Photometric data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..276K"], "see_also": ["J/other/AstBu/64.123 : Paper I. Sample (Khabibullina+, 2009)", "J/other/AstBu/64.357 : Paper III. 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We report the", "photometric parameters for the objects of the list, and perform its", "preliminary statistical analysis including the construction of the", "Hubble diagrams."], "date_update": "12-Nov-2009", "tables": [{"name": "table2.dat", "desc": "Magnitudes for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "Name", "desc": "Name of galaxies "}, {"name": "Band1", "desc": "Band name (1) "}, {"name": "l_mag1", "desc": "[=>] Limit flag on Band1 "}, {"name": "mag1", "desc": "? Magnitude in mag1 "}, {"name": "e_mag1", "desc": "? rms uncertainty on mag1 "}, {"name": "u_mag1", "desc": "[)] Uncertainty flag on mag1 "}, {"name": "Band2", "desc": "Band name (1) "}, {"name": "l_mag2", "desc": "[=>] Limit flag on mag2 "}, {"name": "mag2", "desc": "? Magnitude in Band2 "}, {"name": "e_mag2", "desc": "? rms uncertainty on mag2 "}, {"name": "u_mag2", "desc": "[)] Uncertainty flag on mag2 "}, {"name": "Band3", "desc": "Band name (1) "}, {"name": "l_mag3", "desc": "[=>] Limit flag on mag3 "}, {"name": "mag3", "desc": "? Magnitude in Band3 "}, {"name": "e_mag3", "desc": "? rms uncertainty on mag3 "}, {"name": "Band4", "desc": "Band name (1) "}, {"name": "l_mag4", "desc": "[=><] Limit flag on mag4 "}, {"name": "mag4", "desc": "? Magnitude in Band4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "Band5", "desc": "Band name (1) "}, {"name": "l_mag5", "desc": "[=>] Limit flag on mag5 "}, {"name": "mag5", "desc": "? Magnitude in Band5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "Band6", "desc": "Band name (1) "}, {"name": "l_mag6", "desc": "[=>] Limit flag on mag6 "}, {"name": "mag6", "desc": "? 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We report the results of the sample of angular", "sizes for the NVSS survey list objects, and its preliminary", "statistical analysis. Three-parameter diagrams \"angular", "size-redshift-flux density\" and \"angular size-redshift-spectral", "index\", and their two-parameter projections are constructed. Three", "subsamples of radio galaxies are separated in the \"source size-flux", "density\" diagram."], "date_update": "12-Nov-2009", "tables": [{"name": "table3.dat", "desc": "Sizes and flux density for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "RAh", "desc": "? NVSS Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "? NVSS Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "? NVSS Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? NVSS Declination J2000 (degrees) "}, {"name": "DEm", "desc": "? NVSS Declination J2000 (minutes) "}, {"name": "DEs", "desc": "? NVSS Declination J2000 (seconds) "}, {"name": "l_MajAxis", "desc": "Limit flag on MajAxis "}, {"name": "MajAxis", "desc": "? Max diameter of source in arcsec (NVSS) "}, {"name": "l_MinAxis", "desc": "Limit flag on MinAxis "}, {"name": "MinAxis", "desc": "? Min diameter of source in arcsec (NVSS) "}, {"name": "Flux", "desc": "? 1.4GHz flux density of source (NVSS) "}, {"name": "z", "desc": "Redshift "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AstBu_64.357_o64.123"}} {"id": "J/other/AstBu/64.123", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. 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Primary statistical", "analysis of the list is performed and the regression dependence of the", "spectral index on redshift is found."], "date_update": "09-Dec-2009", "tables": [{"name": "table1.dat", "desc": "Spectral indexes and redshifts for 2442 galaxies ", "columns": [{"name": "Name", "desc": "Name of the source catalog or source name (1) "}, {"name": "n_Name", "desc": "Note on source (2) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "alf1", "desc": "? Spectral index for frequency 325MHz (3) "}, {"name": "alf2", "desc": "? Spectral index for frequency 1400MHz (3) "}, {"name": "alf3", "desc": "? Spectral index for frequency 4850MHz (3) "}, {"name": "z", "desc": "Spectroscopic redshift "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AstBu_64.357_o64.276"}} {"id": "J/other/AstBu/64.276", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. II: Photometric data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..276K"], "see_also": ["J/other/AstBu/64.123 : Paper I. Sample (Khabibullina+, 2009)", "J/other/AstBu/64.357 : Paper III. 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We report the", "photometric parameters for the objects of the list, and perform its", "preliminary statistical analysis including the construction of the", "Hubble diagrams."], "date_update": "12-Nov-2009", "tables": [{"name": "table2.dat", "desc": "Magnitudes for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "Name", "desc": "Name of galaxies "}, {"name": "Band1", "desc": "Band name (1) "}, {"name": "l_mag1", "desc": "[=>] Limit flag on Band1 "}, {"name": "mag1", "desc": "? Magnitude in mag1 "}, {"name": "e_mag1", "desc": "? rms uncertainty on mag1 "}, {"name": "u_mag1", "desc": "[)] Uncertainty flag on mag1 "}, {"name": "Band2", "desc": "Band name (1) "}, {"name": "l_mag2", "desc": "[=>] Limit flag on mag2 "}, {"name": "mag2", "desc": "? Magnitude in Band2 "}, {"name": "e_mag2", "desc": "? rms uncertainty on mag2 "}, {"name": "u_mag2", "desc": "[)] Uncertainty flag on mag2 "}, {"name": "Band3", "desc": "Band name (1) "}, {"name": "l_mag3", "desc": "[=>] Limit flag on mag3 "}, {"name": "mag3", "desc": "? Magnitude in Band3 "}, {"name": "e_mag3", "desc": "? rms uncertainty on mag3 "}, {"name": "Band4", "desc": "Band name (1) "}, {"name": "l_mag4", "desc": "[=><] Limit flag on mag4 "}, {"name": "mag4", "desc": "? Magnitude in Band4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "Band5", "desc": "Band name (1) "}, {"name": "l_mag5", "desc": "[=>] Limit flag on mag5 "}, {"name": "mag5", "desc": "? Magnitude in Band5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "Band6", "desc": "Band name (1) "}, {"name": "l_mag6", "desc": "[=>] Limit flag on mag6 "}, {"name": "mag6", "desc": "? Magnitude in Band6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "Band7", "desc": "Band name (1) "}, {"name": "l_mag7", "desc": "[=>] Limit flag on mag7 "}, {"name": "mag7", "desc": "? Magnitude in Band7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "Band8", "desc": "Band name (1) "}, {"name": "l_mag8", "desc": "[=>] Limit flag on mag8 "}, {"name": "mag8", "desc": "? Magnitude in Band8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "Band9", "desc": "Band name (1) "}, {"name": "l_mag9", "desc": "[=>] Limit flag on mag9 "}, {"name": "mag9", "desc": "? Magnitude in Band9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "Band10", "desc": "Band name (1) "}, {"name": "l_mag10", "desc": "[=>] Limit flag on mag10 "}, {"name": "mag10", "desc": "? Magnitude in Band10 "}, {"name": "Band11", "desc": "Band name (1) "}, {"name": "l_mag11", "desc": "[=>] Limit flag on mag11 "}, {"name": "mag11", "desc": "? Magnitude in Band11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AstBu_64.357_o64.357"}} {"id": "J/other/AstBu/64.357", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. III: Sizes and flux density according to the NVSS data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..357K"], "see_also": ["J/other/AstBu/64.123 : Spectral indexes and redshifts (I) (Khabibullina+, 2009)", "J/other/AstBu/64.276 : Magnitudes (II) (Khabibullina+, 2009)"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio ; Redshifts", "keyword_pub": "radio galaxies - spatial distribution of galaxies - radio sources - observational cosmology", "abstract": ["We describe the procedure of the construction of a sample of distant", "(z>0.3) radio galaxies using the NED, CATS and SDSS databases for", "further use in various statistical tests. We believe the sample to be", "free of objects with quasar properties. This paper is the third part", "of the description of the radio galaxies catalog that we plan to use", "for cosmological tests. We report the results of the sample of angular", "sizes for the NVSS survey list objects, and its preliminary", "statistical analysis. Three-parameter diagrams \"angular", "size-redshift-flux density\" and \"angular size-redshift-spectral", "index\", and their two-parameter projections are constructed. Three", "subsamples of radio galaxies are separated in the \"source size-flux", "density\" diagram."], "date_update": "12-Nov-2009", "tables": [{"name": "table3.dat", "desc": "Sizes and flux density for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "RAh", "desc": "? NVSS Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "? NVSS Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "? NVSS Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? NVSS Declination J2000 (degrees) "}, {"name": "DEm", "desc": "? NVSS Declination J2000 (minutes) "}, {"name": "DEs", "desc": "? NVSS Declination J2000 (seconds) "}, {"name": "l_MajAxis", "desc": "Limit flag on MajAxis "}, {"name": "MajAxis", "desc": "? Max diameter of source in arcsec (NVSS) "}, {"name": "l_MinAxis", "desc": "Limit flag on MinAxis "}, {"name": "MinAxis", "desc": "? Min diameter of source in arcsec (NVSS) "}, {"name": "Flux", "desc": "? 1.4GHz flux density of source (NVSS) "}, {"name": "z", "desc": "Redshift "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AuJPA_14.1"}} {"id": "J/other/AuJPA/14.1", "title_cds": "5000MHz galactic radio sources", "title_create": "Goss+, 1970", "year": "1970", "author": "Goss W.M., Shaver P.A.", "title_pub": "Galactic radio sources. I. High resolution 5000 MHz observations.", "first_author": "Goss W.M.", "ref_biblio": [""], "bibcode": ["1970AuJPA..14....1G"], "see_also": ["J/other/AuJPA/14.77 : Paper II, 408MHz galactic radio sources (Shaver+ 1970)", "J/other/AuJPA/14.133 : Paper III, galactic radio sources spectra (Shaver+ 1970)"], "keyword_cds": "Radio sources", "abstract": ["Contour maps of 63 regions in the galactic plane are presented. The", "half-power beamwidth was 4'arc at 5000 MHZ. Positions and composite", "flux densities are given for 206 sources."], "data": "", "date_update": "28-Jun-1999", "tables": [{"name": "table1.dat", "desc": "Flux Densities and Positions of Calactic Sources ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "RAh", "desc": "Right ascension (1950.0) "}, {"name": "RAm", "desc": "Right ascension (1950.0) "}, {"name": "RAs", "desc": "Right ascension (1950.0) "}, {"name": "DE-", "desc": "Declination sign (1950.0) "}, {"name": "DEd", "desc": "Declination (1950.0) "}, {"name": "DEm", "desc": "Declination (1950.0) "}, {"name": "Tb", "desc": "? Baselevel (in brightness temperature) above which the composite flux was measured"}, {"name": "n_Tb", "desc": "Note on Tb (1) "}, {"name": "F5GHz", "desc": "? Composite flux at 5000MHz "}, {"name": "n_F5GHz", "desc": "Note on Flux (1) "}, {"name": "FigNo", "desc": "? Number of figure "}, {"name": "Note", "desc": "[a-d] Notes (2) "}, {"name": "Names", "desc": "Other names "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_AuJPA_14.133"}} {"id": "J/other/AuJPA/14.133", "title_cds": "Galactic radio sources. III.", "title_create": "shaver+ 1970", "year": "1970", "author": "Shaver P.A., Goss W.M.", "title_pub": "Galactic radio sources. III. Spectra and physical characteristics", "first_author": "Shaver P.A.", "ref_biblio": [""], "bibcode": ["1970AuJPA..14..133S"], "see_also": ["J/other/AuJPA/14.1 : 5000MHz galactic radio sources (Goss+, 1970)", "J/other/AuJPA/14.77 : 408MHz galactic radio sources (Shaver+ 1970)"], "keyword_cds": "Radio sources", "abstract": ["Spectral indices for over 250 galactic radio sources have been", "determined from high resolution observations at 408 and 5000MHz. About", "14% of the sources have nonthermal spectra. A comparison with results", "from an H109{alpha} line survey shows that the line-to-continuum", "temperature ratios for thermal sources are greater than about 2.5%,", "and no recombination line above the detectable threshold has been", "found in a nonthermal source. A search for optical emission from the", "vicinity of the thermal and nonthermal radio sources resulted in", "positive identifications for one-third of them. In 16 cases the radio", "contours are shown superimposed on optical photographs.", "Electron temperatures have been determined directly from the 408MHz", "brightness distribution for 50 thermal sources and are found to be", "consistent with values obtained from H109{alpha} recombination line", "work, indicating that any departures from local thermodynamic", "equilibrium, and their effects on the recombination lines, are small.", "Physical properties of the thermal sources have been computed assuming", "a spherical HII region model. It is shown that HII regions have a", "strong tendency to cluster, and that the cluster sizes are comparable", "with those of open star clusters. No HII regions were found with", "turnover frequencies greater than 1400MHz, indicating that high", "density sources (N_e_>5x10^3^cm^-3^ over a region >0.1pc in extent)", "are very rare. The largest, least dense HII regions have shell", "structure which is consistent with current ideas about the dynamical", "effects of radiation pressure on the dust within HII regions. Fifteen", "new supernova remnants have been identified and distances and physical", "properties computed for them. For the well-resolved supernova remnants", "the shell thickness is a constant fraction of the diameter. It is", "shown that supernova remnants are frequently located in OB", "associations."], "data": "", "date_update": "08-Jul-1999", "tables": [{"name": "table1.dat", "desc": "Measured continuum data for all sources ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "Tb408MHz", "desc": "? Base-level (in brightness temperature) for 408MHz flux density"}, {"name": "Tp408MHz", "desc": "? Peak temperature for 408MHz flux density "}, {"name": "M1RA", "desc": "? Half-power width in right ascension at 408MHz "}, {"name": "M1DE", "desc": "? Half-power width in declination at 408MHz "}, {"name": "S408MHz", "desc": "? Flux density at 408MHz "}, {"name": "n_S408MHz", "desc": "[+] Note on S408MHz (1) "}, {"name": "Tb5GHz", "desc": "? Base-level (in brightness temperature) for 5GHz flux density"}, {"name": "Tp5GHz", "desc": "? Peak temperature for 5GHz flux density "}, {"name": "M2RA", "desc": "? Half-power width in right ascension at 5GHz "}, {"name": "M2DE", "desc": "? Half-power width in declination at 5GHz "}, {"name": "S5GHz", "desc": "? Flux density a 5GHz "}, {"name": "n_S5GHz", "desc": "[*] *: S5GHz is an upper limit "}, {"name": "C1/C2", "desc": "? Half-power width ratio (2) "}, {"name": "T2/T1", "desc": "? Peak temperature ratio (2) "}, {"name": "e_T2/T1", "desc": "? rms uncertainty on T2/T1 "}, {"name": "Source", "desc": "Nature of source (3) "}, {"name": "l_TL/TC", "desc": "Limit flag on TL/TC "}, {"name": "TL/TC", "desc": "? Line-to-continuum temperature ratio from the H109{alpha} recombination line and 5GHz continuum surveys"}, {"name": "Note", "desc": "[N] N: H109{alpha} line observations have been made in the northern survey"}]}, {"name": "table2.dat", "desc": "Flux Densities from Other References ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "n_[GS70]", "desc": "[abc] For same letter, the other values are for the group of sources"}, {"name": "Freq", "desc": "Frequency "}, {"name": "l_SFreq", "desc": "[~ <=] Limit flag on SFreq "}, {"name": "SFreq", "desc": "Flux density "}, {"name": "l_SI", "desc": "[<= ] Limit flag on SI "}, {"name": "SI", "desc": "? Spectral index (1) "}, {"name": "n_SI", "desc": "[n] n: value not significantly different from zero "}, {"name": "Ref", "desc": "[1/15] Reference (2) "}]}, {"name": "table3.dat", "desc": "Optical identifications ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "n_[GS70]", "desc": "[a-n] Group "}, {"name": "Fig", "desc": "Figure number "}, {"name": "OptID", "desc": "Optical identification, comments "}]}, {"name": "table4.dat", "desc": "Electron Temperatures ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "n_[GS70]", "desc": "[*] *: notes in file notes4.dat "}, {"name": "Tb", "desc": "Base-level of 408MHz maps "}, {"name": "T1b", "desc": "Observed 408MHz peak brightness temperature "}, {"name": "T'1", "desc": "Restored 408MHz peak brightness temperature "}, {"name": "T'2", "desc": "? Restored value of T2 "}, {"name": "l_tau1", "desc": "[<= ] Limit flag on tau1 "}, {"name": "tau1", "desc": "? 408MHz optical depth "}, {"name": "l_Tec", "desc": "[>= ] Limit flag on Tec "}, {"name": "Tec", "desc": "Continuum estimate of electron temperature "}, {"name": "Ter", "desc": "? H109{alpha} line estimate of electron temperature"}, {"name": "l_Tec/Ter", "desc": "[ >=] Limit flag on Tec/Ter "}, {"name": "Tec/Ter", "desc": "? Continuum to H109{alpha} line electron temperature ratio"}]}, {"name": "notes4.dat", "desc": "Individual notes to table4.dat ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "table5.dat", "desc": "Properties of HII Regions ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "W1", "desc": "? 408MHz corrected geometric mean half-power source width"}, {"name": "W2", "desc": "? 5GHz corrected geometric mean half-power source width"}, {"name": "EM", "desc": "? Emission measure "}, {"name": "Te", "desc": "? Electron temperature "}, {"name": "Distn", "desc": "? Near distance "}, {"name": "Diam", "desc": "? Linear diameter "}, {"name": "Ne", "desc": "? Electron density "}, {"name": "Mass", "desc": "? Mass "}, {"name": "U", "desc": "? Excitation parameter "}, {"name": "Disf", "desc": "? Far distance "}, {"name": "DiamC", "desc": "? Linear diameter computed for the spherical model"}, {"name": "NeC", "desc": "? Electron density computed for the spherical model"}, {"name": "MassC", "desc": "? Mass computed for the spherical model "}, {"name": "UC", "desc": "? Excitation parameter computed for the spherical model"}]}, {"name": "table6.dat", "desc": "Unresolved HII Regions ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "Freq", "desc": "? Turnover frequency "}, {"name": "W", "desc": "Computed width "}, {"name": "n_W", "desc": "[*+] Note (1) "}]}, {"name": "table7.dat", "desc": "References for distances of HII Regions ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "n_[GS70]", "desc": "[a-j] Group "}, {"name": "Dist", "desc": "Distance (1) "}, {"name": "Ref", "desc": "References (2) "}]}, {"name": "table8.dat", "desc": "Extragalactic sources ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "l_SI", "desc": "[<= ] Limit flag on SI "}, {"name": "SI", "desc": "Spectral index "}, {"name": "S408MHz", "desc": "408MHz flux density "}]}, {"name": "table9.dat", "desc": "Properties of Supernova Remnants ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "SI", "desc": "Spectral index "}, {"name": "Diam", "desc": "Angular diameter "}, {"name": "S1GHz", "desc": "1GHz flux density "}, {"name": "Dist", "desc": "Distance "}, {"name": "Z", "desc": "Displacement above of below the Galactic Plane "}, {"name": "2R", "desc": "Diameter "}, {"name": "P1GHz", "desc": "Power output at 1GHz "}, {"name": "Power", "desc": "Total power "}]}, {"name": "appen.dat", "desc": "Notes on individual sources ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_BAN_14.265"}} {"id": "J/other/BAN/14.265", "title_cds": "UBV photometry in 3 clusters", "title_create": "Koelbloed+, 1959", "year": "1959", "author": "Koelbloed D.", "title_pub": "Three-colour photometry of the three southern open clusters NGC 3532, 6475 (M7) and 6124.", "first_author": "Koelbloed D.", "ref_biblio": [""], "bibcode": ["1959BAN....14..265K"], "keyword_cds": "Clusters, open ; Photometry, UBV", "keyword_pub": "", "object": ["NGC 6475 (Koelbloed)"], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_BASI_40.65"}} {"id": "J/other/BASI/40.65", "title_cds": "Spatial orientation of galaxies in ZoA", "title_create": "Aryal+, 2012", "year": "2012", "author": "Aryal B., Yadav S.N., Saurer W.", "title_pub": "Spatial orientation of galaxies in the Zone of Avoidance.", "first_author": "Aryal B.", "ref_biblio": [""], "bibcode": ["2012BASI...40...65A"], "see_also": ["J/A+AS/110/269 : Galaxies in the \"zone of avoidance\". I. (Weinberger+, 1995)", "J/A+AS/117/1 : Galaxies in the \"zone of avoidance\". II. (Seeberger+, 1996)", "J/A+AS/117/369 : Galaxies in the \"zone of avoidance\". III. (Lercher+, 1996)", "J/A+AS/126/247 : Galaxies in the \"zone of avoidance\". IV. (Saurer+, 1997)", "J/A+AS/127/101 : Galaxies in the \"zone of avoidance\". V. (Seeberger+ 1998)"], "keyword_cds": "Galaxy catalogs ; Morphology", "keyword_pub": "catalogues - surveys - galaxies: evolution - galaxies: statistics", "abstract": ["We present spatial orientation of spin vectors of galaxies found in", "the region 20{deg}<=l<=80{deg}, -10{deg}<=b<=-5{deg} in the first", "Palomar Observatory Sky Survey. The inclination angle and intrinsic", "flatness of a galaxy are used to determine the spin vector and spin", "vector projections of the galaxy. We studied the preferred alignments", "of spin vectors of galaxies with respect to equatorial, Galactic and", "supergalactic coordinate systems."], "type": ["OC"], "data": "", "date_update": "10-Jul-2012", "tables": [{"name": "table.dat", "desc": "*Position angle (PA) and diameters of the galaxies ", "columns": [{"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "PA", "desc": "Position angle "}, {"name": "a", "desc": "Semi-major axis "}, {"name": "b", "desc": "Semi-minor axis "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_BSAO_49.53"}} {"id": "J/other/BSAO/49.53", "title_cds": "Catalogue of radio decametric sources", "title_create": "Verkhodanov+, 2000", "year": "2000", "author": "Verkhodanov O.V., Andernach H., Verkhodanova N.V.", "title_pub": "Radio identification of decametric sources. I. Catalogue", "first_author": "Verkhodanov O.V.", "ref_biblio": [""], "bibcode": ["2000BSAO...49...53V"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "James Marcout, Patricia Bauer [CDS]", "data": "", "date_update": "16-Jul-2002"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_ChJAA_2.501"}} {"id": "J/other/ChJAA/2.501", "title_cds": "Seyfert 1 galaxies", "title_create": "Zhou+, 2002", "year": "2002", "author": "Zhou H.-Y., Wang T.-G.", "title_pub": "Properties of broad band continuum of narrow line Seyfert 1 galaxies.", "first_author": "Zhou H.-Y.", "ref_biblio": [""], "bibcode": ["2002ChJAA...2..501Z"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1088/1009-9271/2/6/501"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_CoVVO_2.33"}} {"id": "J/other/CoVVO/2.33", "title_cds": "Southern M-type stars", "title_create": "Lu+, 1984", "year": "1984", "author": "Lu P.K., Macconnell D.J.", "title_pub": "A search for southern M-type stars.", "first_author": "Lu P.K.", "ref_biblio": [""], "bibcode": ["1984CoVVO...2...33L"], "keyword_cds": "Stars, late-type", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_JAD_20.5"}} {"id": "J/other/JAD/20.5", "title_cds": "Detectability of micro-variables in ASAS", "title_create": "David+, 2014", "year": "2014", "author": "David M., Hensberge H., Nitschelm C.", "title_pub": "Detectability of micro-variables in the ASAS database: the Scorpius - Centaurus Complex.", "first_author": "David M.", "ref_biblio": [""], "bibcode": ["2014JAD....20....5D\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "stars: variables: general - techniques: photometric - open clusters and associations: individual: Sco - Cen Complex - stars: individual: HD 46057, HD 146285, HD 116794, HD 119022", "abstract": ["We present a star-by-star discussion of the light variability of stars", "belonging to the Sco-Cen Complex, as detected in the ASAS\u2013V", "database by David et al. (2013A&A...557A..47D). Most of the variables", "(30) are young stars with irregular and/or cyclic patterns of", "variability, almost all with spectral types that indicate that they", "did not yet reach the zero-age main-sequence. The ZAMS starts at A3,", "F2 and F4 for the Upper-Scorpius, the Upper Centaurus-Lupus and the", "Lower Centaurus-Crux subgroups, respectively. A minority of stars (7),", "mainly of spectral type B or late-A, show strictly (multi-)periodic", "variability induced by rigid rotation of a spotted magnetic star, by", "slight deformation of the stellar shape in a binary, or by pulsation", "of stars situated in the instability domain of either SPB, {delta} Sct", "or {gamma} Dor stars. For some stars comments on yet unpublished", "high-resolution spectra are included."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "08-Oct-2016"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_JAD_9.1"}} {"id": "J/other/JAD/9.1", "title_cds": "Munster Red Sky Survey", "title_create": "Seitter+, 2015", "year": "2015", "author": "Seitter W.C., Duerbeck H.W.", "title_pub": "The Munster Red Sky Survey. Large=scale structures in the universe.", "first_author": "Seitter W.C.", "ref_biblio": ["<(various journals) JAD, 9.1 (2015)>"], "bibcode": ["2015other.JAD..9.1.\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "sky surveys: stars - sky surveys: galaxies - CCD photometry: galaxy clusters", "abstract": ["We present"], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "08-Oct-2016"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_JApA_33.227"}} {"id": "J/other/JApA/33.227", "title_cds": "Photoelectric radial velocities", "title_create": "Griffin, 2012", "year": "2012", "author": "Griffin R.F.", "title_pub": "Photoelectric radial velocities. Paper XIX: Additional spectroscopic binaries among the Redman K stars.", "first_author": "Griffin R.F.", "ref_biblio": [""], "bibcode": ["2012JApA...33..227G"], "keyword_cds": "", "keyword_pub": "stars: late-type - stars: radial velocities - spectroscopic binaries - orbits", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1007/s12036-012-9140-x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_Nat_585.363"}} {"id": "J/other/Nat/585.363", "title_cds": "WD 1856+534 transit curves", "title_create": "Vanderburg+, 2020", "year": "2020", "author": "Vanderburg A., Rappaport S.A., Xu S., Crossfield I.J.M., Becker J.C., Gary B., Murgas F., Blouin S., Kaye T.G., Palle E., Melis C., Morris B.M., Kreidberg L., Gorjian V., Morley C.V., Mann A.W., Parviainen H., Pearce L.A., Newton E.R., Carrillo A., Zuckerman B., Nelson L., Zeimann G., Brown W.R., Tronsgaard R., Klein B., Ricker G.R., Vanderspek R.K., Latham D.W., Seager S., Winn J.N., Jenkins J.M., Adams F.C., Benneke B., Berardo D., Buchhave L.A., Caldwell D.A., Christiansen J.L., Collins K.A., Colon K.D., Daylan T., Doty J., Doyle A.E., Dragomir D., Dressing C., Dufour P., Fukui A., Glidden A., Guerrero N.M., Guo X., Heng K., Henriksen A.I., Huang C.X., Kaltenegger L., Kane S.R., Lewis J.A., Lissauer J.J., Morales F., Narita N., Pepper J., Rose M.E., Smith J.C., Stassun K.G., Yu L.", "title_pub": "A giant planet candidate transiting a white dwarf.", "first_author": "Vanderburg A.", "ref_biblio": [""], "bibcode": ["2020Natur.585..363V"], "keyword_cds": "Stars, white dwarf ; Spectra, optical ; Photometry, SDSS", "abstract": ["Astronomers have discovered thousands of planets outside the Solar", "System, most of which orbit stars that will eventually evolve into red", "giants and then into white dwarfs. During the red giant phase, any", "close-orbiting planets will be engulfed by the star, but more distant", "planets can survive this phase and remain in orbit around the white", "dwarf. Some white dwarfs show evidence for rocky material floating in", "their atmospheres5, in warm debris disks or orbiting very closely,", "which has been interpreted as the debris of rocky planets that were", "scattered inwards and tidally disrupted. Recently, the discovery of", "a gaseous debris disk with a composition similar to that of ice giant", "planets14 demonstrated that massive planets might also find their way", "into tight orbits around white dwarfs, but it is unclear whether these", "planets can survive the journey. So far, no intact planets have been", "detected in close orbits around white dwarfs. Here we report the", "observation of a giant planet candidate transiting the white dwarf", "WD 1856+534 (TIC 267574918) every 1.4days. We observed and modelled", "the periodic dimming of the white dwarf caused by the planet candidate", "passing in front of the star in its orbit. The planet candidate is", "roughly the same size as Jupiter and is no more than 14 times as", "massive (with 95 per cent confidence). Other cases of white dwarfs", "with close brown dwarf or stellar companions are explained as the", "consequence of common-envelope evolution, wherein the original orbit", "is enveloped during the red giant phase and shrinks owing to friction.", "In this case, however, the long orbital period (compared with other", "white dwarfs with close brown dwarf or stellar companions) and low", "mass of the planet candidate make common-envelope evolution less", "likely. Instead, our findings for the WD 1856+534 system indicate that", "giant planets can be scattered into tight orbits without being tidally", "disrupted, motivating the search for smaller transiting planets around", "white dwarfs."], "description": ["We show spectra from four observatories, using the Low Resolution", "Spectrograph 2 on the Hobby-Eberly Telescope (HET/LRS2), the Gemini", "Near InfraRed Spectrograph on the Gemini North Telescope", "(Gemini/GNIRS), the Kast Double Spectrograph on the Shane Telescope at", "Lick Observatory (Lick/Kast) and the Blue Channel spectrograph at MMT", "Observatory. The data have been scaled to remove offsets in their", "absolute flux calibrations. The optical spectra show a pure continuum,", "confirming the DC spectral classification, whereas the near-infrared", "spectrum from Gemini North shows only spurious features, owing to", "imperfect correction of the telluric absorption and sky emission from", "Earth's atmosphere.", "We show the light curves from TESS; data from several private", "telescopes in Arizona (operated by B.G. and T.G.K.) with odd and", "even-numbered transits shown separately; simultaneous light curves in", "four colours from MuSCAT2; a light curve from the GTC, and a light", "curve from Spitzer. The individual two-minute-cadence TESS flux", "measurements are shown as grey points, and the rose-coloured points", "are averages of the brightness in roughly 30s in orbital phase. The", "TESS data have been corrected for dilution from nearby stars so that", "the transit depth matches that of the GTC data."], "object": ["18 57 39.34 +53 30 33.3 WD 1856+534 = TOI 1690"], "type": ["OC"], "data": "", "date_update": "17-Nov-2020", "tables": [{"name": "fig2.dat", "desc": "Spectroscopic observation of WD 1856+534 ", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "RelFlux", "desc": "? Relative Flux "}, {"name": "Inst", "desc": "Observatory/Spectrograph (1) "}]}, {"name": "fig2ext.dat", "desc": "All transit observation of WD 1856+534 ", "columns": [{"name": "Time", "desc": "Observation date (TDB) "}, {"name": "Relmag", "desc": "Relative Brightness "}, {"name": "Inst", "desc": "Observatory/Filter (1) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_NewA_27.102"}} {"id": "J/other/NewA/27.102", "title_cds": "HAT-P-16b photometric observations", "title_create": "Pearson+, 2014", "year": "2014", "author": "Pearson K.A., Turner J.D., Sagan T.G.", "title_pub": "Photometric observation of HAT-P-16b in the near-UV.", "first_author": "Pearson K.A.", "ref_biblio": [""], "bibcode": ["2014NewA...27..102P"], "keyword_cds": "", "keyword_pub": "planetary systems - techniques: photometric - planets and satellites: magnetic fields", "abstract": ["We present the first primary transit light curve of the hot Jupiter", "HAT-P-16b in the near-UV photometric band. We observed this object on", "December 29, 2012 in order to update the transit ephemeris, constrain", "its planetary parameters and search for magnetic field interference.", "Vidotto et al. (2011MNRAS.414.1573V) postulate that the magnetic field", "of HAT-P-16b can be constrained if its near-UV light curve shows an", "early ingress compared to its optical light curve, while its egress", "remains unchanged. However, we did not detect an early ingress in our", "night of observing when using a cadence of 60 seconds and an average", "photometric precision of 2.26 mmag. We find a near-UV planetary radius", "of Rp=1.274+/-0.057R_Jup_ which is consistent with its near-IR radius", "of Rp=1.289+/-0.066R_Jup_ (Buchhave et al., 2010, Cat.", "J/ApJ/720/1118). We developed an automated reduction pipeline and a", "modeling package to process our data. The data reduction package", "synthesizes a set of IRAF scripts to calibrate images and perform", "aperture photometry. The modeling package utilizes the", "Levenberg\u2013Marquardt minimization algorithm to find a least-squares", "best fit and a differential evolution Markov Chain Monte Carlo", "algorithm to find the best fit to the light curve. To constrain the", "red noise in both fitting models we use the residual permutation", "(rosary bead) method and time-averaging method."], "description": ["Our observation was conducted on December 29, 2012 at the Steward", "Observatory 1.55-m Kuiper Telescope on Mt. Bigelow, using the Mont4k", "CCD. The Mont4k CCD contains a 4096x4096 pixel sensor with a field", "of view (FOV) of 9.7arcminx9.7arcmin."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1016/j.newast.2013.08.002"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_NewA_34.27"}} {"id": "J/other/NewA/34.27", "title_cds": "Sh2-311 region deep optical survey", "title_create": "Yadav+, 2015", "year": "2015", "author": "Yadav R.K., Pandey A.K., Sharma S., Jose J., Ogura K., Kobayashi N., Samal M.R., Eswaraiah C., Chandola H.C.", "title_pub": "Deep optical survey of the stellar content of Sh2-311 region.", "first_author": "Yadav R.K.", "ref_biblio": [""], "bibcode": ["2015NewA...34...27Y"], "keyword_cds": "", "keyword_pub": "stars: clusters - star clusters: individual (Haffner 18, Haffner 19 and NGC 2467) - stars: pre-main sequence - stars: formation", "abstract": ["The stellar content in and around Sh2-311 region have been studied", "using the deep optical observations as well as near-infrared (NIR)", "data from 2MASS. The region contains three clusters, viz. NGC 2467,", "Haffner 18 and Haffner 19. We have made an attempt to distinguish the", "stellar content of these individual regions as well as to re-determine", "their fundamental parameters such as distance, reddening, age, onto", "the basis of a new and more extended optical and infrared photometric", "data set. NGC 2467 and Haffner 19 are found to be located in the", "Perseus arm at the distances of 5.0+/-0.4kpc and 5.7+/-0.4kpc,", "respectively, whereas Haffner 18 is located at the distance of", "11.2+/-1.0kpc. The clusters NGC 2467 and Haffner 19 might have formed", "from the same molecular cloud, whereas the cluster Haffner 18 is", "located in the outer galactic arm, i.e. the Norma\u2013Cygnus arm. We", "identify 8 class II young stellar objects (YSOs) using the NIR", "(J-H)/(H-K)(J-H)/(H-K) two colour diagram. We have estimated the age", "and mass of the YSOs identified in the present work and those by", "Snider et al. (2009) using the V/(V-I)V/(V-I) colour-magnitude", "diagram. The estimated ages and mass range of the majority of the YSOs", "are <~1Myr and ~0.4-3.5M_{sun}_, respectively, indicating that these", "sources could be T-Tauri stars or their siblings. Spatial distribution", "of the YSOs shows that some of the YSOs are distributed around the Hii", "region Sh2-311, suggesting a triggered star formation at its", "periphery."], "description": ["The data used in this work are a combination of archived optical UBVI", "images taken with the Wide Field Imager (WFI) camera at the 2.2-m MPG", "Telescope of the European Southern Observatory (ESO) and NIR data from", "the 2MASS Point Source catalogue (Cutri et al., 2003, Cat. II/246)", "available on the WEB. Low resolution spectroscopic observation of", "three stars were also taken using the 2.0-m Himalayan Chandra", "Telescope (HCT) of Indian Astronomical Observatory (IAO), Hanle.", "The archived optical observations of Sh2-311 region used in this study", "were taken using the WFI camera (PI: Rubio, M.) mounted at the", "Cassegrain focus of the ESO 2.2-m Telescope."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1016/j.newast.2014.05.004"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_NewA_52.96"}} {"id": "J/other/NewA/52.96", "title_cds": "Short Title", "title_create": "Cakirli+, 2017", "year": "2017", "author": "Cakirli O., Ibanoglu C., Sipahi E., Akan M.C.", "title_pub": "V850 Cyg: An eclipsing binary with a giant {gamma} Dor pulsator.", "first_author": "Cakirli O.", "ref_biblio": [""], "bibcode": ["2017NewA...52...96C"], "keyword_cds": "", "keyword_pub": "stars: fundamental parameters - stars: individual: V850 Cyg - binaries: eclipses", "abstract": ["We present new spectroscopic observations of the double-lined", "eclipsing binary V850 Cyg. The long-cadence photometric observations", "obtained by Kepler were analysed and combined with the analysis of", "radial velocities for deriving the absolute parameters of the", "components. Masses and radii were determined as", "Mp=1.601+/-0.076M_{sun}_ and Rp=4.239+/-0.076R_{sun}_,", "Ms=0.851+/-0.053M_{sun}_ and Rs=5.054+/-0.087R_{sun}_ for the", "components of V850 Cyg. We estimate an interstellar reddening of", "0.28+/-0.12mag and a distance of 1040+/-160pc for the system. The", "measured rotational velocity of the secondary appears to lower than", "that of synchronize rotation. However its spectral lines are too weak", "to be measured the rotational velocity with reasonable accuracy. We", "have extracted the synthetic light curve from the observations and", "excluded the data within the eclipses for the frequency analysis. We", "obtained at least nine frequencies in the {gamma} Dor regime. It seems", "that the primary component oscillates with a dominant period of about", "1.152549+/-0.000009-days. We also compare pulsational properties of", "the primary star of V850 Cyg with the {gamma} Dor type pulsating", "components in other binaries."], "description": ["V850 Cyg was observed in both long- and short-cadence by the Kepler", "satellite. Detailed descriptions of the characteristics of these", "observations can be found in Slawson (2011, Cat. J/AJ/142/160). The", "short-cadence observations comprise about 24,000 data points obtained", "in the Quarters 0, 1, 2a, 2b, 2c, 3a, 3b, 3c, 4a, 4b, 4c, 8, 12, and", "16, and the long-cadence data encompass 57,535 data points in the", "Quarters 0,... ,17 obtained over four years. The corrected flux", "measurements were used in our analysis. The times of the observational", "data are transformed to the heliocentric Julian dates and the flux", "measurements converted to Kepler magnitude scale."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1016/j.newast.2016.10.008"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_PASA_16.175"}} {"id": "J/other/PASA/16.175", "title_cds": "-73<=DE<=+27 X-ray sources catalog", "title_create": "Meliani, 1999", "year": "1999", "author": "Meliani M.T.", "title_pub": "A catalogue of X-ray sources in the sky region between {delta}=-73{deg} and {delta}=+27{deg}.", "first_author": "Meliani M.T.", "ref_biblio": [""], "bibcode": ["1999PASA...16..175M"], "keyword_cds": "X-ray sources ; Binaries, X-ray ; Pulsars ; Active gal. nuclei ; Cross identifications ; Photometry, UBV", "abstract": ["This catalogue lists coordinates, X-ray fluxes in different energy", "ranges, magnitudes and color indices, optical counterparts, orbital", "periods of binaries, pulsar periods and other characteristics of", "226 X-ray sources (HMXBs, LMXBs, pulsars and galaxies) between", "DE=-73{deg} and DE=+27{deg}."], "doi_pub": ["10.1071/AS99175"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "position.dat", "desc": "X-ray names and positions ", "columns": [{"name": "Bname", "desc": "Source B or J name "}, {"name": "Type", "desc": "Type of source (1) "}, {"name": "RAh", "desc": "Right ascension (2000) "}, {"name": "RAm", "desc": "Right ascension (2000) "}, {"name": "RAs", "desc": "? Right ascension (2000) "}, {"name": "DE-", "desc": "Declination sign (2000) "}, {"name": "DEd", "desc": "Declination (2000) "}, {"name": "DEm", "desc": "Declination (2000) "}, {"name": "DEs", "desc": "? Declination (2000) "}, {"name": "RA1h", "desc": "Right ascension (1950) "}, {"name": "RA1m", "desc": "Right ascension (1950) "}, {"name": "RA1s", "desc": "? Right ascension (1950) "}, {"name": "DE1-", "desc": "Declination sign (1950) "}, {"name": "DE1d", "desc": "Declination (1950) "}, {"name": "DE1m", "desc": "? Declination (1950) "}, {"name": "DE1s", "desc": "? Declination (1950) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "ObsType", "desc": "[oxir, ] Type of observation "}, {"name": "PosErr", "desc": "? Source position error "}, {"name": "x_PosErr", "desc": "Unit of PosErr (\", ' or {deg}) "}, {"name": "Names", "desc": "Other names "}]}, {"name": "optical.dat", "desc": "UBV photometry, optical counterpart ", "columns": [{"name": "Name", "desc": "Usual name "}, {"name": "l_Vmag", "desc": "[->] Limit flag on Vmag "}, {"name": "Vmag", "desc": "? V magnitude "}, {"name": "---", "desc": "[-] - when interval of magnitudes "}, {"name": "Vmag2", "desc": "? Lower V magnitude when interval "}, {"name": "u_Vmag", "desc": "[:v] \":\" : uncertainty flag on Vmag, v: var "}, {"name": "Band", "desc": "[BK] When Vmag contains B or K magnitude "}, {"name": "r_Vmag", "desc": "References for Vmag (1) "}, {"name": "n_Vmag", "desc": "[*] Note for B1608-522, B1657-415 (2) "}, {"name": "B-V", "desc": "? B-V colour index (3) "}, {"name": "---", "desc": "[-] - when interval of B-V colour index "}, {"name": "B-V2", "desc": "? Lower B-V colour index when interval "}, {"name": "u_B-V", "desc": "Uncertainty flag on B-V "}, {"name": "r_B-V", "desc": "Reference for B-V (1) "}, {"name": "U-B", "desc": "? U-B colour index "}, {"name": "r_U-B", "desc": "Reference for U-B (1) "}, {"name": "l_E(B-V)", "desc": "Limit flag on E(B-V) "}, {"name": "E(B-V)", "desc": "? Interstellar reddening "}, {"name": "---", "desc": "[-] - when interval on interstellar reddening "}, {"name": "E(B-V)2", "desc": "? Upper value of E(B-V) when interval "}, {"name": "u_E(B-V)", "desc": "Uncertainty flag on E(B-V) "}, {"name": "r_E(B-V)", "desc": "Reference for E(B-V) (1) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "OName", "desc": "Optical counterpart, if known, and associations "}]}, {"name": "xfluxes.dat", "desc": "X-ray fluxes and periods ", "columns": [{"name": "Bname", "desc": "Source B or J name "}, {"name": "n_F2-10", "desc": "[*] *: 0.1-2.4KeV flux in F2-10 "}, {"name": "l_F2-10", "desc": "[> <] Limit flag on F2-10 "}, {"name": "F2-10", "desc": "? X-ray flux in the range 2-10 keV (or 0.1-2.4keV if *)"}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F2-10u", "desc": "? Upper limit on F2-10 when interval "}, {"name": "r_F2-10", "desc": "References for F2-10 (1) "}, {"name": "n_F40-80", "desc": "[*] *: 10-40keV flux in F10-40 "}, {"name": "l_F40-80", "desc": "Limit flag on F40-80 "}, {"name": "F40-80", "desc": "? X-ray flux in the range 40-80KeV (or 10-40keV if *)"}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F40-80u", "desc": "? Upper limit on F40-80 when interval "}, {"name": "r_F40-80", "desc": "Reference for F40-80 (1) "}, {"name": "l_F80-120", "desc": "Limit flag on F80-120 "}, {"name": "F80-120", "desc": "? X-ray flux in the range 80-120keV "}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F80-120u", "desc": "? Upper limit on F80-120 for interval "}, {"name": "r_F80-120", "desc": "Reference on F80-120 (1) "}, {"name": "F100-200", "desc": "? X-ray flux in the range 100-200keV "}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F100-200u", "desc": "? Upper limit on F100-200 if interval "}, {"name": "l_F200-600", "desc": "Limit flag on F200-600 "}, {"name": "F200-600", "desc": "? X-ray flux in the range 200-600keV "}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F200-600u", "desc": "? Upper limit on F200-600 if interval "}, {"name": "l_F1000+", "desc": "Limit flag on F1000+ "}, {"name": "F1000+", "desc": "? X-ray flux in the range >1000keV "}, {"name": "---", "desc": "[-] - when interval "}, {"name": "F1000+u", "desc": "? Upper limit on F1000+ if interval "}, {"name": "r_F1000+", "desc": "Reference for F1000+ (1) "}, {"name": "l_Porb", "desc": "Limit flag on Porb "}, {"name": "Porb", "desc": "? Orbital period "}, {"name": "x_Porb", "desc": "Units of Porb (d, h) "}, {"name": "u_Porb", "desc": "[: ?] Uncertainty flag on Porb "}, {"name": "r_Porb", "desc": "Reference for Porb (1) "}, {"name": "n_Porb", "desc": "Second possible period or upper value if interval"}, {"name": "Ppul", "desc": "? Pulsar period "}, {"name": "x_Ppul", "desc": "Units of Pulsar period (s or ms) "}, {"name": "n_Ppul", "desc": "Reference or second possible value for Ppul (1)"}, {"name": "Char", "desc": "Characteristics (2) "}, {"name": "Cat.", "desc": "X-ray catalogues and experiments in which the source was listed and/or detected (3)"}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "Bname", "desc": "Name "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference number "}, {"name": "BibCode", "desc": "BibCode "}, {"name": "Authors", "desc": "Author's names "}, {"name": "Com", "desc": "Comments "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_PASAu_5.290"}} {"id": "J/other/PASAu/5.290", "title_cds": "MDS2 survey", "title_create": "Author+, ", "title_pub": "Title of the paper", "first_author": "Authors", "author": "Authors", "ref_biblio": ["<(various journals) PASAu, 5.290 (2000)>"], "bibcode": ["2000PASAu5.290.\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["MDS2"], "data": "", "date_update": "09-Aug-2006"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_POAN_2.59"}} {"id": "J/other/POAN/2.59", "title_cds": "Peculiar stars in 5 southern fields", "title_create": "Stock+, 1972", "year": "1972", "author": "Stock J., Wroblewski H.", "title_pub": "A southern objective prism survey.", "first_author": "Stock J.", "ref_biblio": [""], "bibcode": ["1972POAN....2...59S"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "12-Jul-2006"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_RAA_20.97"}} {"id": "J/other/RAA/20.97", "title_cds": "Short Title", "title_create": "Zhang+, 2020", "year": "2020", "author": "Zhang M., Chen B.-Q., Huo Z.-Y., Zhang H.-W., Xiang M.-S., Yuan H.-B., Huang Y., Wang C., Liu X.-W.", "title_pub": "A catalogue of H{alpha} emission-line point sources in the vicinity fields of M 31 and M 33 from the LAMOST survey.", "first_author": "Zhang M.", "ref_biblio": [""], "bibcode": ["2020RAA....20...97Z"], "keyword_cds": "", "keyword_pub": "galaxies: individual (M31,M33) - stars: emission-line - planetary nebulae: general - H II regions", "abstract": ["We present a catalogue of 3305H emission-line point sources observed", "with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope", "(LAMOST) in the vicinity fields of M31 and M33 during September 2011", "and January 2016. The catalogue contains 1487 emission-line stars, 532", "emission-line nebulae including 377 likely planetary nebulae (PNe), 83", "HII region candidates and 20 possible supernova remnants (SNRs) and", "1286 unknown objects. Among them, 24 PN candidates, 19 HII region", "candidates, 10 SNR candidates and one symbiotic star candidate are new", "discoveries. Radial velocities and fluxes estimated from the H line", "and those quantities of seven other major emission lines including", "H{beta}, [OIII] 4959, [OIII] 5007, [NII] 6548, [NII] 6583, [SII] 6717", "and [SII] 6731 lines of all the catalogued sources yielded from the", "LAMOST spectra are also presented in our catalogue. Our catalogue is", "an ideal starting point to study the chemistry properties and", "kinematics of M31 and M33."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "23-Aug-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_RAA_22.H5013"}} {"id": "J/other/RAA/22.H5013Short", "title_cds": "Title", "title_create": "Ali+, 2022", "year": "2022", "author": "Ali A., Algarni E., Mindil A., Alghamdi S.A.", "title_pub": "A New Statistical Distance Scale for Planetary Nebulae, Based on Gaia EDR3.", "first_author": "Ali A.", "ref_biblio": [""], "bibcode": ["2022RAA....22h5013A"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "date_update": "26-Sep-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_RAA_22.F5015"}} {"id": "J/other/RAA/22.F5015Short", "title_cds": "Title", "title_create": "Lu+, 2022", "year": "2022", "author": "Lu Y., Luo A.-L., Wang L.-L., Wang Y.-F., Li Y.-B., Han J.-S., Qin L., Tang Y.-K., Qiu B., Zhang S., Zhang J.-N., Zhao Y.-H.", "title_pub": "106 New Emission-line Galaxies and 29 New Galactic H II Regions are Identified with Spectra in the Unknown Data Set of LAMOST DR7.", "first_author": "Lu Y.", "ref_biblio": [""], "bibcode": ["2022RAA....22f5015L"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "date_update": "26-Sep-2022"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_RMxAA_22.43"}} {"id": "J/other/RMxAA/22.43", "title_cds": "IR stellar population in the Galaxy", "title_create": "Ruelas-Mayorga, 1991", "year": "1991", "author": "Ruelas-Mayorga R.A.", "title_pub": "Distribution and studies of the infrared stellar population in the Galaxy. II. The data base.", "first_author": "Ruelas-Mayorga R.A.", "ref_biblio": [""], "bibcode": ["1991RMxAA..22...43R"], "see_also": ["J/A+AS/93/61 : IR Stellar Population in Baade's window (Ruelas-Mayorga+ 1992)", "J/A+AS/97/587 : JHK photometry of Galactic center stars (Ruelas-Mayorga+ 1993)"], "keyword_cds": "Populations, stellar; Photometry, infrared ; Infrared sources", "keyword_pub": "Galaxy: stellar content - Galaxy: structure - Interstellar: dust", "abstract": ["In this paper we utilised the galactic model developed in", "Ruelas-Mayorga (1991RMxAA..22...27R) in order to predict the", "Cumulative Counts Function (CCF) (log. of the number of sources down", "to a given K-magnitude per unit of area) in 39 directions of the sky.", "We present stellar-counts observations for these directions and", "compare the observational results with the predictions of the model.", "We conclude that the global description of the distribution of the", "stellar population responsible for the 2.2{mu}m radiation in our galaxy", "is very well represented by the model's predictions. There are a few", "regions for which the global description is not satisfactory. We", "present evidence for some cases that this is due to anomalous stellar", "concentrations or to excess or deficiency of absorption."], "data": "", "date_update": "24-Oct-2000", "tables": [{"name": "tables.dat", "desc": "Infrared sources ", "columns": [{"name": "Table", "desc": "Table number (A2 to A30) "}, {"name": "---", "desc": "[l=] "}, {"name": "GLON", "desc": "Region field center galactic longitude "}, {"name": "---", "desc": "[b=] "}, {"name": "GLAT", "desc": "Region field center galactic latitude "}, {"name": "Scan", "desc": "Row number in the scan "}, {"name": "---", "desc": "[/] "}, {"name": "Source", "desc": "Source number along scan-line "}, {"name": "RAh", "desc": "Right ascension (1950.0) "}, {"name": "RAm", "desc": "Right ascension (1950.0) "}, {"name": "RAs", "desc": "[0/60] Right ascension (1950.0) "}, {"name": "DE-", "desc": "Declination sign (1950.0) "}, {"name": "DEd", "desc": "Declination (1950.0) "}, {"name": "DEm", "desc": "Declination (1950.0) "}, {"name": "DEs", "desc": "Declination (1950.0) "}, {"name": "Kmag", "desc": "? K magnitude "}, {"name": "n_Kmag", "desc": "[SAT ] SAT: saturated, for sources brighter than K~+8.5"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_RMxAA_6.83"}} {"id": "J/other/RMxAA/6.83", "title_cds": "Carbon stars", "title_create": "Fuenmayor, 1981", "year": "1981", "author": "Fuenmayor F.J.", "title_pub": "A deep near infrared objective prism survey for carbon stars toward the galactic center and anticenter.", "first_author": "Fuenmayor F.J.", "ref_biblio": [""], "bibcode": ["1981RMxAA...6...83F"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_Sci_368.1477"}} {"id": "J/other/Sci/368.1477", "title_cds": "Short Title", "title_create": "Author+, ", "title_pub": "A multiplanet system of super-Earths orbiting the brightest red dwarf star GJ 887.", "first_author": "Jeffers S.V.", "author": "Jeffers S.V., Dreizler S., Barnes J.R., Haswell C.A., Nelson R.P., Rodriguez E., Lopez-Gonzalez M.J., Morales N., Luque R., Zechmeister M., Vogt S.S., Jenkins J.S., Palle E., Berdinas Z.M., Coleman G.A.L., Diaz M.R., Ribas I., Jones H.R.A., Butler R.P., Tinney C.G., Bailey J., Carter B.D., O'Toole S., Wittenmyer R.A., Crane J.D., Feng F., Shectman S.A., Teske J., Reiners A., Amado P.J., Anglada-Escude G.", "ref_biblio": [""], "bibcode": ["2020Sci...368.1477J"], "keyword_cds": "", "abstract": ["The closet exoplanets to the Sun provide opportunities for detailed", "characterization of planets outside the Solar System. We report the", "discovery, using radial velocity measurements, of a compact", "multiplanet system of super-Earth exoplanets orbiting the nearby red", "dwarf star GJ 887. The two planets have orbital periods of 9.3 and", "21.8 days. Assuming an Earth-like albedo, the equilibrium temperature", "of the 21.8-day planet is ~350 kelvin. The planets are interior to,", "but close to the inner edge of, the liquid-water habitable zone. We", "also detect an unconfirmed signal with a period of ~50 days, which", "could correspond to a third super-Earth in a more temperate orbit. Our", "observations show that GJ 887 has photometric variability below 500", "parts per million, which is unusually quiet for a red dwarf."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "16-Nov-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_Sci_371.168"}} {"id": "J/other/Sci/371.168", "title_cds": "Short Title", "title_create": "Kaiser+, 2021", "year": "2021", "author": "Kaiser B.C., Clemens J.C., Blouin S., Dufour P., Hegedus R.J., Reding J.S., Bedard A.", "title_pub": "Lithium pollution of a white dwarf records the accretion of an extrasolar planetesimal.", "first_author": "Kaiser B.C.", "ref_biblio": [""], "bibcode": ["2021Sci...371..168K"], "keyword_cds": "", "abstract": ["Tidal disruption and subsequent accretion of planetesimals by white", "dwarfs can reveal the elemental abundances of rocky bodies in", "exoplanetary systems. Those abundances provide information on the", "composition of the nebula from which the systems formed, which is", "analogous to how meteorite abundances inform our understanding of the", "early Solar System. We report the detection of lithium, sodium,", "potassium, and calcium in the atmosphere of the white dwarf Gaia DR2", "4353607450860305024, which we ascribe to the accretion of a", "planetesimal. Using model atmospheres, we determine abundance ratios", "of these elements, and, with the exception of lithium, they are", "consistent with meteoritic values in the Solar System. We compare the", "measured lithium abundance with measurements in old stars and with", "expectations from Big Bang nucleosynthesis."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "15-Dec-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_Sci_371.713"}} {"id": "J/other/Sci/371.713", "title_cds": "Short Title", "title_create": "Lelli+, 2021", "year": "2021", "author": "Lelli F., Di Teodoro E., Fraternali F., Man A.W.S., Zhang Z.-Y., De Breuck C., Davis T.A., Maiolino R.", "title_pub": "A massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang.", "first_author": "Lelli F.", "ref_biblio": [""], "bibcode": ["2021Sci...371..713L"], "keyword_cds": "", "abstract": ["Cosmological models predict that galaxies forming in the early", "Universe experience a chaotic phase of gas accretion and star", "formation, followed by gas ejection due to feedback processes. Galaxy", "bulges may assemble later via mergers or internal evolution. Here we", "present submillimeter observations (with spatial resolution of 700", "parsecs) of ALESS 073.1, a starburst galaxy at redshift z~5 when", "the Universe was 1.2 billion years old. This galaxy\u2019s cold gas forms", "a regularly rotating disk with negligible noncircular motions. The", "galaxy rotation curve requires the presence of a central bulge in", "addition to a star-forming disk. We conclude that massive bulges and", "regularly rotating disks can form more rapidly in the early Universe", "than predicted by models of galaxy formation."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "15-Dec-2021"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_A+SP_163.275"}} {"id": "J/other/ApSS/163.275", "title_cds": "UV & Geneva photometry around HD 173009", "title_create": "Reichen+, 1990", "year": "1990", "author": "Reichen M., Lanz T., Golay M., Huguenin D.", "title_pub": "A detailed study of a 6{deg} diameter field in Scutum. I. Data presentation and overall description of the interstellar matter distribution.", "first_author": "Reichen M.", "ref_biblio": [""], "bibcode": ["1990Ap&SS.163..275R"], "see_also": ["II/59 : Catalogue of stellar UV fluxes (TD1) (Thompson+ 1978)"], "keyword_cds": "Surveys ; Photometry, ultraviolet ; Photometry, Geneva ; MK spectral classification", "abstract": ["A 6{deg} diameter field centered on the star {epsilon} Scutum has been", "selected from the SCAP-2000 balloon-borne UV survey for its high", "apparent stellar density contrast and relatively good transparency on", "a small projected portion of the galactic plane. In view of a detailed", "study of the absorption and interstellar matter distribution in this", "field, a large collection of data has been made and is presented here.", "Ultraviolet magnitudes at 2000{AA} have been obtained from the", "reduction of three SCAP frames. In addition, 322 stars among the 487", "stars detected on the UV frames have been measured in the Geneva", "photometric system. For a small number of photometrically distant", "objects, medium resolution spectra have been obtained in order to", "determine spectral types and confirm the distances determination. An", "overall description of the distribution of interstellar material in", "the ultraviolet is made using star counting methods, and is confronted", "to similar studies in the visible range. A discussion of the", "variations of the extinction law in different parts of the field is", "made. A new distance determination of the Sct OB2 association is", "proposed, as well as a list of additional probable members of the", "association. A certain number of distant hot stars seem to indicate", "the presence of an unknown OB association at the edge of the Scutum", "spiral arm, at a distance of over 3 kpc from the Sun."], "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Calibration stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (see Table2) "}, {"name": "Name", "desc": "HD, BD or CSI identification "}, {"name": "SpType", "desc": "Spectral type (see table 2) "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude from the Geneva system"}, {"name": "UVmag", "desc": "UV magnitude at 2000{AA} deduced from calibration"}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag "}, {"name": "n_UVmag", "desc": "[abcd ] Note on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965{AA} passband of the TD1 catalogue (Thompson et al., 1978, Cat. ). (2)"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "n_UVmagTD1", "desc": "[)] ) indicates that the UV magnitude UVmagboxes was preferred for the calibration"}, {"name": "UVmagboxes", "desc": "UV magnitude deduced by the method of the so-called \"photometric boxes\" (see text.) (3)"}, {"name": "e_UVmagboxes", "desc": "rms uncertainty on UVmagboxes "}, {"name": "n_UVmagboxes", "desc": "[)] ) indicates that the UV magnitude UVmagTD1 was preferred for the calibration"}, {"name": "N", "desc": "Number of stars in the photometric box "}, {"name": "Rem", "desc": "Remarks related to the UV_TD1_ magnitudes (G2) "}]}, {"name": "table2.dat", "desc": "All stars measured on SCAP frames 11.65/14.48/14.49 ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (1) "}, {"name": "n_SCAP", "desc": "[* o] \"*\" star measured in the Geneva system (see Table 3) \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[+*] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (see Table 3) "}, {"name": "Vmag", "desc": "? Visual magnitude (3) "}, {"name": "UVmag", "desc": "UV magnitude at 2000A from the SCAP frames "}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag (4) "}, {"name": "n_UVmag", "desc": "[abcd ] Notes on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965A passband of the TD1 catalogue (Thompson et al., 1978, )"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "UV-V", "desc": "? (UVmag-Vmag) color index "}, {"name": "(UV-V)0", "desc": "? Intrinsic (UV-V)_0_ color index taken from Carnochan (1982) following the MK, photometric or other spectra type"}, {"name": "E(UV-V)", "desc": "? UV color excess (from (UV-V) and (UV-V)0) "}, {"name": "Rem", "desc": "Various remarks and comments (G2) "}]}, {"name": "table3.dat", "desc": "All stars with Geneva photometry ", "columns": [{"name": "SCAP", "desc": "SCAP identification (see Table 2) "}, {"name": "n_SCAP", "desc": "[o] \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[*+] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "GLONd", "desc": "Galactic longitude "}, {"name": "GLONm", "desc": "Galactic longitude "}, {"name": "GLATd", "desc": "Galactic latitude "}, {"name": "GLATm", "desc": "Galactic latitude "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (1) "}, {"name": "[U-B]", "desc": "Geneva [U-B] colour index "}, {"name": "[B-V]", "desc": "Geneva [B-V] colour index "}, {"name": "[B1-B]", "desc": "Geneva [B1-B] colour index "}, {"name": "[B2-B]", "desc": "Geneva [B2-B] colour index "}, {"name": "[V1-B]", "desc": "Geneva [V1-B] colour index "}, {"name": "[G-B]", "desc": "Geneva [G-B] colour index "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude "}, {"name": "E[B-V]", "desc": "? Color excess deduced from the X,Y,Z parameters (Cramer, 1982A&A...112..330C) unless stated otherwise in the remarks"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters (Cramer and Maeder, 1979A&A....78..305C) unless stated otherwise in the remarks"}, {"name": "r", "desc": "? Decuced heliocentric distance "}, {"name": "Rem", "desc": "Various remarks (2) "}]}, {"name": "table4.dat", "desc": "Spectroscopic standard stars ", "columns": [{"name": "HD", "desc": "HD identification "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "? Visible absorption derived from E[B-V]. "}, {"name": "n_AV", "desc": "[)] ): values deduced from Johnson's U-B/B-V diagram"}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypeH", "desc": "Spectral type given by Houk and Cowley (1975, ) or Houk (1978, , 1982, )"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHg", "desc": "Equivalent width of the H{gamma} line derived from our spectroscopic observations"}, {"name": "VMAGHg", "desc": "Absolute magnitude derived from EW_H{gamma}_ using calibrations by Millward and Walker (1985ApJS...57...63M) or Hill et al. (1986PASP...98.1186H)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}]}, {"name": "table5.dat", "desc": "Spectroscopy of Scutum field stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "Visible absorption derived from E[B-V] "}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHa", "desc": "Equivalent width of the H{alpha} line derived from our spectroscopic observations"}, {"name": "u_EWHa", "desc": "[)] Uncertainty flag on EWHa "}, {"name": "VMAGHa", "desc": "? Absolute magnitude derived from EW_H{alpha}_ (See notes to Table 4)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}, {"name": "Rem", "desc": "Individual remarks (1) "}]}, {"name": "notes2.dat", "desc": "Individual notes to table2.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "notes3.dat", "desc": "Individual notes to table3.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"J_other_RNAAS_4.12"}} {"id": "J/other/RNAAS/4.12", "title_cds": "Galactic RSG+B binary systems", "title_create": "Pantaleoni Gonzalez+, 2020", "year": "2020", "author": "Pantaleoni Gonzalez M., Maiz Apellaniz J., Barba R.H., Negueruela I.", "title_pub": "A catalog of Galactic multiple systems with a red supergiant and a B star.", "first_author": "Pantaleoni Gonzalez M.", "ref_biblio": [""], "bibcode": ["2020RNAAS...4...12P"], "see_also": ["B/sb9 : SB9: 9th Cat. of Spectroscopic Binary Orbits (Pourbaix+ 2004-2014)", "B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)", "B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2020)", "B/mk : Catalogue of Stellar Spectral Classifications (Skiff, 2009- )", "III/117 : MK Classifications of Close Visual Binaries (Corbally, 1984)", "III/135 : Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989)", "III/150 : Perkins Revised MK Types for the Cooler Stars (Keenan+ 1989)", "III/274 : Galactic O-Star Spectroscopic Survey (GOSSS) (Sota+, 2014)", "J/ApJS/99/135 : A-type stars rotation and spectral peculiarities (Abt+ 1995)", "J/ApJS/119/83 : IUE sample of binaries with hot component (Parsons+, 1998)", "J/ApJS/143/513 : Spectral classification of close binaries (Ginestet+, 2002)", "J/MNRAS/427/3209 : Galactic and MC O-AGBs and RSGs stars (Jones+, 2012)", "J/A+A/571/A43 : Red supergiants in Galactic clusters (Messineo+, 2014)", "J/ApJS/224/4 : GOSSS III. Additional O-type systems (Maiz Apellaniz+, 2016)", "J/MNRAS/469/1330 : NGC 6067 stars (Alonso-Santiago+, 2017)", "J/MNRAS/475/2003 : Red supergiant population in Perseus arm (Dorda+, 2018)", "J/A+A/616/A124 : NGC 3105 UBVR photometry (Alonso-Santiago+, 2018)", "J/AJ/158/20 : K-M stars of class I cand. RSGs in Gaia (Messineo+, 2019)"], "keyword_cds": "Stars, double and multiple; Stars, giant; Stars, B-type; References", "keyword_pub": "Binary stars ; Catalogs ; Early-type stars ; Late-type stars ; Late-type supergiant stars ; Red supergiant stars ; B stars", "description": ["We have searched the literature and Simbad to find Galactic red", "supergiant (RSG)+B binary systems. More specifically, we define RSGs", "as objects with spectral type G, K, or M and luminosity classes II to", "Ia for consistency with Neugent+ (2019ApJ...875..124N), but we note", "that criterion includes some Cepheids, which can be of spectral type", "G-K0 in some phases. Results are listed in Table 1.", "We have found 108 Galactic RSG+B binary systems in the literature,", "with 61% of the sample already present in two references alone", "(Ginestet & Carquillat 2002, J/ApJS/143/513 and", "Samus'+ 2017ARep...61...80S). A significant number of the objects have", "two entries in the HD catalog, a likely consequence of the composite", "nature of the spectra. The total number in the sample has to be taken", "with care, as literature spectral classifications can include gross", "errors."], "type": ["GCC"], "data": "", "date_update": "09-Sep-2020", "tables": [{"name": "table1.dat", "desc": "Objects, spectral classifications, Galactic coordinates, V magnitudes, separations, references, and comments", "columns": [{"name": "Name", "desc": "Identifier "}, {"name": "AName", "desc": "Alternate name "}, {"name": "SpT-RSG", "desc": "Red supergiant spectral type "}, {"name": "LC-RSG", "desc": "Red supergiant luminosity class "}, {"name": "Q-RSG", "desc": "[ep ] Red supergiant qualifier "}, {"name": "SpT-B", "desc": "B star spectral type "}, {"name": "LC-B", "desc": "B star luminosity class "}, {"name": "Q-B", "desc": "B star qualifier "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "[-39.4/21] Galactic latitude "}, {"name": "Vmag", "desc": "[0.9/14.4]?=99.9 Apparent V band magnitude "}, {"name": "Sep", "desc": "[0/9.4]? Binary separation (1) "}, {"name": "Ref", "desc": "Reference code (see refs.dat file) "}, {"name": "Comm", "desc": "Additional comments "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference code "}, {"name": "BibCode", "desc": "Bibcode of the reference "}, {"name": "Auth", "desc": "Author's name(s) "}, {"name": "Comm", "desc": "Comment "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"V_100"}} {"id": "V/100", "title_cds": "Strasbourg-ESO Catalogue of Galactic Planetary Nebulae", "title_create": "Acker+ 1996", "year": "1996", "author": "Acker A., Ochsenbein F., Stenholm B., Tylenda R., Marcout J., Schohn C.", "title_pub": "Strasbourg-ESO Catalogue of Galactic Planetary Nebulae and First Supplement", "first_author": "Acker A.", "ref_biblio": [""], "bibcode": ["1992ESOPN...1....1A"], "see_also": ["J/A+A/307/215 : Spectrophotometry of PNe (Cuisinier+, 1996)"], "keyword_cds": "Planetary nebulae ; Spectroscopy", "description": ["This new edition of the \"Catalogue of Galactic Planetary Nebulae\" is a", "merging of the \"Strasbourg-ESO Catalogue of Galactic Planetary", "Nebulae\" published by ESO in 1992 and the \"First Supplement to the", "Strasbourg-ESO Catalogue of Galactic Planetary Nebulae\" prepared at", "Strasbourg for the Mexico meeting...", "Compared to the previous edition, 384 new objects discovered since", "1991/92 have been added: 242 have been added as \"true or probable\"", "PNe, and 142 which status is stilll unclear were classified among", "the \"possible\" planetary nebulae.", "Errors reported until ... were also corrected."], "alias": ["GPN", "PNG"], "data": "", "date_update": "31-Aug-2010", "tables": [{"name": "main.dat", "desc": "Discoverers, Designations, and Positions of True and Possible Planetary Nebulae (1)", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "*Designation of the Galactic Planetary Nebula (blank for Possible PNe from 1992)"}, {"name": "RAh", "desc": "Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension 2000 (minutes) "}, {"name": "RAs", "desc": "? Right Ascension 2000 (seconds) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "Declination 2000 (degrees) "}, {"name": "DEm", "desc": "Declination 2000 (minutes) "}, {"name": "DEs", "desc": "[0/60[? Declination 2000 (seconds) "}, {"name": "qualPos", "desc": "*[ad*] Accuracy on the 2000 Position: "}, {"name": "r_Pos", "desc": "Reference of position "}, {"name": "Name", "desc": "Main designation "}, {"name": "PK", "desc": "Designation in PK67 "}, {"name": "IRAS", "desc": "Designation in IRAS catalogue "}, {"name": "Disc", "desc": "*Discoverer name and publication year "}, {"name": "Idents", "desc": "Other names separated by commas "}]}, {"name": "diam.dat", "desc": "Diameters of PN (optical and radio) (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "l_oDiam", "desc": "Limit flag on oDiam "}, {"name": "oDiam", "desc": "? Optical diameter "}, {"name": "u_oDiam", "desc": "[:e] Uncertainty flag (:) on oDiam, or e for \"extended\" (without value)"}, {"name": "r_oDiam", "desc": "References for oDiam "}, {"name": "l_rDiam", "desc": "Limit flag on Radio diameter "}, {"name": "rDiam", "desc": "? Radio diameter "}, {"name": "u_rDiam", "desc": "Uncertainty flag (:) on oDiam "}, {"name": "r_rDiam", "desc": "Reference on Radio diameter "}]}, {"name": "dist.dat", "desc": "Distance estimations (2) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "Method", "desc": "*[EKSWXDCM] Method used for distance determination"}, {"name": "Dist1", "desc": "? Lower distance if l_Dist is '-' "}, {"name": "l_Dist", "desc": "[-<>] '-' if Dist1 is a lower limit; '<' or '>' apply to Dist."}, {"name": "Dist", "desc": "Distance in kiloparsecs. "}, {"name": "u_Dist", "desc": "[?:] Uncertainty flag on Dist "}, {"name": "r_Dist", "desc": "Reference of Dist determination. "}]}, {"name": "dista.dat", "desc": "Statistical distances (2) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "Method", "desc": "*[EKSWXDCM] Method used for distance determination"}, {"name": "Dist1", "desc": "? Lower distance if l_Dist is '-' "}, {"name": "l_Dist", "desc": "[-<>] '-' if Dist1 is a lower limit; '<' or '>' apply to Dist."}, {"name": "Dist", "desc": "Distance in kiloparsecs. "}, {"name": "u_Dist", "desc": "[?:] Uncertainty flag on Dist "}, {"name": "r_Dist", "desc": "Reference of Dist determination. "}]}, {"name": "hbeta.dat", "desc": "H-beta fluxes (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "log(Fbeta)", "desc": "[-15/-9] log of flux in H-beta "}, {"name": "e_log(Fbeta)", "desc": "? Mean error on log(Fbeta) "}, {"name": "r_log(Fbeta)", "desc": "References "}]}, {"name": "intens.dat", "desc": "Line intensities results (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "ObsLabel", "desc": "Observation name (includes the date) "}, {"name": "LineRef", "desc": "[ab] Line taken as reference (value=100): 'a'=H-alpha (6563), 'b'=H-beta (4861)"}, {"name": "I4363", "desc": "]0/15000]? Line intensity of [OIII] at 436.3nm "}, {"name": "u_I4363", "desc": "Uncertainty flag on I4363 "}, {"name": "I4686", "desc": "]0/15000]? Line intensity of HeII at 468.6nm "}, {"name": "u_I4686", "desc": "Uncertainty flag on I4686 "}, {"name": "n_I5007", "desc": "[*] '*' if the measurement refers to 495.9nm because 500.7nm line is saturated"}, {"name": "I5007", "desc": "]0/15000]? Line intensity of [OIII] at 500.7nm "}, {"name": "u_I5007", "desc": "Uncertainty flag on I5007 "}, {"name": "I5876", "desc": "]0/15000]? Line intensity of HeI "}, {"name": "u_I5876", "desc": "Uncertainty flag on I5876 at 587.6nm "}, {"name": "I6563", "desc": "]0/15000]? Line intensity of H-alpha at 656.3nm"}, {"name": "u_I6563", "desc": "Uncertainty flag on I6563 "}, {"name": "I6584", "desc": "[0/15000]? Line intensity of [NII] at 658.4nm "}, {"name": "u_I6584", "desc": "Uncertainty flag on I6584 "}, {"name": "n_I6717", "desc": "[B] 'B' if line is blended "}, {"name": "I6717", "desc": "]0/15000]? Line intensity of [SII] at 671.7nm "}, {"name": "u_I6717", "desc": "Uncertainty flag on I6717 "}, {"name": "n_I6731", "desc": "[B] 'B' if line is blended "}, {"name": "I6731", "desc": "]0/15000]? Line intensity of [SII] at 673.1nm "}, {"name": "u_I6731", "desc": "Uncertainty flag on I6731 "}, {"name": "r_Line", "desc": "Reference of the spectroscopic values "}]}, {"name": "iue.dat", "desc": "IUE observations log (2) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "IUEname", "desc": "Name as found in the IUE Merged Log "}, {"name": "1950Pos", "desc": "Position as found in the IUE Merged Log "}, {"name": "ObsDate", "desc": "Date and time (hours, minutes) of the Observation"}, {"name": "OType", "desc": "Object class as found in the IUE Merged Log "}, {"name": "Camera", "desc": "designation, LW=Long Wavelength, SW=Short Wavelength"}, {"name": "Image", "desc": "identification of the Observation "}]}, {"name": "iras.dat", "desc": "IRAS Point Source Catalogue fluxes (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "IRAS", "desc": "IRAS source name "}, {"name": "RAIRASh", "desc": "Hours RA, equinox 1950.0, epoch 1983.5 "}, {"name": "RAIRASm", "desc": "Minutes RA, equinox 1950.0, epoch 1983.5 "}, {"name": "RAIRASds", "desc": "Seconds RA, equinox 1950.0, epoch 1983.5 "}, {"name": "DEIRAS-", "desc": "Sign Dec, equinox 1950.0, epoch 1983.5 "}, {"name": "DEIRASd", "desc": "Degrees Dec, equinox 1950.0, epoch 1983.5 "}, {"name": "DEIRASm", "desc": "Minutes Dec, equinox 1950.0, epoch 1983.5 "}, {"name": "DEIRASs", "desc": "Seconds Dec, equinox 1950.0, epoch 1983.5 "}, {"name": "Major", "desc": "Uncertainty ellipse major axis "}, {"name": "Minor", "desc": "Uncertainty ellipse minor axis "}, {"name": "PosAng", "desc": "Uncertainty ellipse position angle (1) "}, {"name": "NHcon", "desc": "Number of times observed "}, {"name": "Fnu12", "desc": "Average non-color corrected flux density, 12um"}, {"name": "Fnu25", "desc": "Average non-color corrected flux density, 25um"}, {"name": "Fnu60", "desc": "Average non-color corrected flux density, 60um"}, {"name": "Fnu100", "desc": "Average non-color corrected flux density, 100um"}, {"name": "q_Fnu12", "desc": "[1/3] Flux density quality, 12um (1) "}, {"name": "q_Fnu25", "desc": "[1/3] Flux density quality, 25um (1) "}, {"name": "q_Fnu60", "desc": "[1/3] Flux density quality, 60um (1) "}, {"name": "q_Fnu100", "desc": "[1/3] Flux density quality, 100um (1) "}]}, {"name": "nir.dat", "desc": "Near infra-red observations (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "Jmag", "desc": "? Magnitude in J filter (1.25um) "}, {"name": "l_Hmag", "desc": "Limit flag on Hmag "}, {"name": "Hmag", "desc": "? Magnitude in H filter (1.65um) "}, {"name": "l_Kmag", "desc": "Limit flag on Kmag "}, {"name": "Kmag", "desc": "? Magnitude in K filter (2.22um) "}, {"name": "l_Lmag", "desc": "Limit flag on Lmag "}, {"name": "Lmag", "desc": "? Magnitude in L/L' filter (3.5/3.8um) "}, {"name": "n_Lmag", "desc": "['] the apostrophe indicates the L' filter "}, {"name": "l_Mmag", "desc": "Limit flag on Mmag "}, {"name": "Mmag", "desc": "? Magnitude in M (5.0um) "}, {"name": "Class", "desc": "*[NDSP,?+ ] Class based on the near-IR "}, {"name": "r_Phot", "desc": "References for JHKL "}, {"name": "r_Sp", "desc": "References describing the Spectrum "}]}, {"name": "radio.dat", "desc": "Radio observations (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "l_Rad2cm", "desc": "Limit flag on Rad2cm "}, {"name": "Rad2cm", "desc": "? Radio flux density at 2cm (14.7GHz) "}, {"name": "r_Rad2cm", "desc": "Reference of Rad2cm "}, {"name": "l_Rad6cm", "desc": "Limit flag on Rad6cm "}, {"name": "Rad6cm", "desc": "? Radio flux density at 6cm (5GHz) "}, {"name": "u_Rad6cm", "desc": "Uncertainty flag on Rad6cm "}, {"name": "r_Rad6cm", "desc": "Reference of Rad6cm "}]}, {"name": "vel.dat", "desc": "Radial and Expansion Velocities (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "RVel", "desc": "? Radial Velocity "}, {"name": "e_RVel", "desc": "? Mean error on RVel "}, {"name": "r_RVel", "desc": "Source of the Radial Velocity "}, {"name": "l_ExpVel", "desc": "Limit flag on ExpVel "}, {"name": "ExpVel", "desc": "? Expansion velocity [OIII] "}, {"name": "u_ExpVel", "desc": "[*] Note on ExpVel (1) "}, {"name": "r_ExpVel", "desc": "Source of ExpVel "}, {"name": "n_ExpVel", "desc": "[+-] Note on the elements (2) "}, {"name": "l_ExpVel2", "desc": "Limit flag on ExpVel2 "}, {"name": "ExpVel2", "desc": "? Expansion velocity [NII] "}, {"name": "u_ExpVel2", "desc": "[*] Note on ExpVel2 (1) "}, {"name": "r_ExpVel2", "desc": "Reference of ExpVel2 "}, {"name": "n_ExpVel2", "desc": "[+-] Note on the elements (2) "}]}, {"name": "cstar.dat", "desc": "Data concerning Central Stars of PN (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "AG82", "desc": "Name in ref. AG82 (Acker et al., Publ. Speciale CDS 3, 1982)"}, {"name": "Umag", "desc": "? Johnson's U filter mag. of central star "}, {"name": "l_Bmag", "desc": "Limit flag on Bmag "}, {"name": "Bmag", "desc": "? Johnson's B filter mag. of central star "}, {"name": "l_Vmag", "desc": "Limit flag on Vmag "}, {"name": "Vmag", "desc": "? Johnson's V filter mag. of central star "}, {"name": "Quality", "desc": "*[ABCDP] Accuracy of the photometry "}, {"name": "r_UBV", "desc": "References of Photometry "}, {"name": "Remarks", "desc": "Remarks on Photometry "}, {"name": "Sp", "desc": "Spectral type of central star "}, {"name": "r_Sp", "desc": "Reference of Spectral type "}, {"name": "Sp2", "desc": "Other spectral classification "}, {"name": "r_Sp2", "desc": "Reference of Sp2 "}, {"name": "Sp3", "desc": "Other spectral classification "}, {"name": "r_Sp3", "desc": "Reference of Sp3 "}, {"name": "Names", "desc": "Various designations of the Central Star separated by a semi-colon (;)"}]}, {"name": "notes.dat", "desc": "Notes and remarks about some nebulae (2) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "Text", "desc": "Text of the note "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference code (repeated on each line) "}, {"name": "Text", "desc": "Text if reference (authors and titles) "}]}, {"name": "pospn.dat", "desc": "Possible PN (table 2) ", "columns": [{"name": "Name", "desc": "Usual name "}, {"name": "n_PK", "desc": "[*] The '*' indicates that PK was not published in the PK67 reference"}, {"name": "PK", "desc": "Designation in PK67 (or later, see n_PK) "}, {"name": "RAh", "desc": "Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension 2000 (minutes) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "Declination 2000 (degrees) "}, {"name": "DEm", "desc": "Declination 2000 (minutes) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "Class", "desc": "*[UHPLNE?*2 ] Class of the object "}, {"name": "OtherNames", "desc": "separated by a comma (,) "}]}, {"name": "notpn.dat", "desc": "Objects rejected as PN (table 3) ", "columns": [{"name": "Name", "desc": "Usual name "}, {"name": "n_PK", "desc": "[*] The '*' indicates that PK was not published in the PK67 reference"}, {"name": "PK", "desc": "Designation in PK67 (or later, see n_PK) "}, {"name": "RAh", "desc": "[0/24[? Right Ascension 2000 (hours) (1) "}, {"name": "RAm", "desc": "[0/60[? Right Ascension 2000 (minutes) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "[0/90[? Declination 2000 (degrees) "}, {"name": "DEm", "desc": "[0/60[? Declination 2000 (minutes) "}, {"name": "GLON", "desc": "[0/360[? Galactic longitude "}, {"name": "GLAT", "desc": "[-90/90]? Galactic latitude "}, {"name": "Notes", "desc": "*Notes concerning the object "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"V_5"}} {"id": "V/5A", "title_cds": "Colours, Luminosities, and Motions Nearer K-M Giants", "title_create": "Eggen 1966", "year": "1966", "author": "Eggen O.J.", "title_pub": "Colours, Luminosities, and Motions of the Nearer Giants of Types K and M", "first_author": "Eggen O.J.", "ref_biblio": [""], "keyword_cds": "Colors - 235; Space velocities - 730; Stars, giant - 880; Stars, late-type - 895", "description": ["The data compilation Colours, Luminosities and Motions of the Nearer", "Giants of Types of K and M (Eggen 1966) contains all stars in the", "Yale Catalogue of Bright Stars (Hoffleit 1964) that have visual", "magnitudes brighter than 5.5 and that have been observed to have B-V", "redder than +0.8 mag, with the exception of a few K-type dwarfs. In", "addition to mostly K- and M-type giants, a few subgiants and", "supergiants are included. The data result from some 1600", "photoelectric observations of 600 stars with the 50.8-cm reflector", "of the Hale Observatories. Approximately one-third of the stars had", "been observed at the Cape Observatory (Cousins and Stoy 1963).", "Although spectral types are given in the published catalog, they", "were taken from a variety of sources, are very inhomogeneous, and", "are not included in this catalog."], "date_update": "20-Nov-1995", "tables": [{"name": "giantkm.dat", "desc": "Catalog Data ", "columns": [{"name": "HR", "desc": "HR number from the Yale Catalogue of Bright Stars (Hoffleit 1964)."}, {"name": "HR2", "desc": "A slash (/) and additional digit if a second HR star is included in the measurements."}, {"name": "flag1", "desc": "An asterisk (*) is present if there are remarks in the published catalog."}, {"name": "GCRV", "desc": "GCRV number in the General Catalogue of Stellar Radial Velocities (Wilson 1953)."}, {"name": "GCRV2", "desc": "A slash and additional digit if a GCRV star is included in the value given"}, {"name": "V", "desc": "? Photoelectric V(E) magnitude. The precision varies within the data field."}, {"name": "flag2", "desc": "A \"v\" if the magnitude is variable; a colon (:) for uncertainty. If the magnitude given is considered to be a maximum, a code M is given in byte 46."}, {"name": "B-V", "desc": "? B-V color. The precision varies. "}, {"name": "flag3", "desc": "uncertainty flag: colon (:) for uncertainty, \"V\" for variable."}, {"name": "U-B", "desc": "? U-B color. The precision varies. "}, {"name": "flag4", "desc": "U-B flag (see byte 32). A question mark (?) is present if the value is surrounded by parentheses in the published table."}, {"name": "ObsNum", "desc": "? Number of observations, n, for UBV data. "}, {"name": "UBVcode", "desc": "*Code for UBV measurements "}, {"name": "M(V)", "desc": "? Absolute visual magnitude, M(V), taken from various sources, as indicated by the codes in bytes 53-54. Precision varies."}, {"name": "flag5", "desc": "*Flag for M(V) "}, {"name": "Source", "desc": "*Source of M(V) "}, {"name": "U-", "desc": "Sign of U component "}, {"name": "U", "desc": "? U component of the space velocity relative to Sun."}, {"name": "u_U", "desc": "Colon if U uncertain. "}, {"name": "V-", "desc": "Sign of V component "}, {"name": "V", "desc": "? V component of the space velocity "}, {"name": "u_V", "desc": "Colon (:) if V uncertain. "}, {"name": "W-", "desc": "Sign of W component "}, {"name": "W", "desc": "? W component of the space velocity "}, {"name": "u_W", "desc": "Colon (:) if W uncertain. "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"V_155"}} {"id": "V/155", "title_cds": "GDR2AP. Gaia DR2, 2MASS, AllWISE astrophys. param.", "title_create": "Fouesneau+, 2022", "year": "2022", "author": "Fouesneau M., Andrae R., Dharmawardena T., Rybizki J., Bailer-Jones C.A.L., Demleitner M.", "title_pub": "Astrophysical Parameters from Gaia DR2, 2MASS and AllWISE.", "first_author": "Fouesneau M.", "ref_biblio": [""], "bibcode": ["2022A&A...662A.125F", "2022yCat.5155....0F"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "II/328 : AllWISE Data Release (Cutri+ 2013)", "http://dc.g-vo.org/tableinfo/gdr2ap.main : GRD2AP Home Page"], "keyword_cds": "Surveys ; Extinction ; Stars, distances ; Stars, masses ; Photometry ; Optical", "keyword_pub": "stars: distances - stars: fundamental parameters - methods: statistical - Galaxy: stellar content - ISM: dust extinction - catalogs", "abstract": ["Stellar physical and dynamical properties are essential knowledge to", "understanding the structure, formation, and evolution of our Galaxy.", "We produced an all-sky uniformly derived catalog of stellar", "astrophysical parameters (APs; age, mass, temperature, bolometric", "luminosity, distance, dust extinction) to give insight into the", "physical properties of Milky-Way stars.", "Exploiting the power of multi-wavelength and multi-survey observations", "from Gaia DR2 parallaxes and integrated photometry along with 2MASS", "and AllWISE photometry, we introduce an all-sky uniformly derived", "catalog of stellar astrophysical parameters, including dust extinction", "(A0) average grain size (R0) along the line of sight, for 123097070", "stars. In contrast with previous works, we do not use a Galactic model", "as prior in our analysis.", "We validate our results against other literature (e.g., benchmark", "stars, interferometry, Bayestar, StarHorse). The limited optical", "information in the Gaia photometric bands or the lack of ultraviolet", "or spectroscopic information renders the chemistry inference prior", "dominated. We demonstrate that Gaia parallaxes bring sufficient", "leverage to explore the detailed structures of the interstellar medium", "in our Milky Way.", "In Gaia DR3, we will obtain the dispersed optical light information to", "break through some limitations of this analysis, allowing us to infer", "stellar chemistry in particular. Gaia promises us data to construct", "the most detailed view of the chemo-dynamics of field star populations", "in our Galaxy.", "Our catalog is available from the German Astrophysical Virtual", "Observatory (GAVO) at http://dc.g-vo.org/tableinfo/ gdr2ap.main where", "one can query it via ADQL and TAP (and soon in the Gaia Archive)."], "description": ["We constructed a crossmatch catalog by considering the \"obvious\"", "all-sky non-Gaia data provided by DPAC2 that span a different", "wavelength range, i.e., 2MASS (Skrutskie et al., 2006, Cat. VII/233;", "Cutri et al., 2003, Cat. II/246) and AllWISE (Cutri & et al., 2014,", "Cat. II/328). For the latter, Wise provides us with four photometric", "bands spanning wavelengths from 1 to 30um. Because the interstellar", "dust emits at those wavelengths contaminating W3 and W4 photometry, we", "only included W1 and W2 in our analysis."], "alias": ["GDR2AP", "J/A+A/662/A125"], "type": ["CCC"], "records": ["123097070 stars"], "doi_pub": ["10.1051/0004-6361/202141828"], "orcid_pub": ["0000-0001-9256-5516"], "data": "f-v", "islargetable": true, "date_creation": "01-Feb-2022", "xmatch": "V/155/gdr2ap", "last_update": "16-Aug-2022", "catid": "5155", "date_update": "16-Aug-2022", "tables": [{"name": "gdr2ap.sam", "desc": "Sample records of GDR2AP ", "columns": [{"name": "GaiaDR2", "desc": "Unique source identifier (source_id)) (1)"}, {"name": "RAdeg", "desc": "Barycentric right ascension (ICRS) at Ep=2015.5 (RA_ICRS)"}, {"name": "DEdeg", "desc": "Barycentric declination (ICRS) at Ep=2015.5 (DE_ICRS)"}, {"name": "A0best", "desc": "multivariate maximum posterior estimate for the dust extinction A0 (A0_best)"}, {"name": "A0max", "desc": "Maximum of the A0 distribution (A0_max)"}, {"name": "A0min", "desc": "Minimum of the A0 distribution (A0_min)"}, {"name": "A0p16", "desc": "16th percentile of the A0 distribution (A0_p16)"}, {"name": "A0p25", "desc": "25th percentile of the A0 distribution (A0_p25)"}, {"name": "A0med", "desc": "median of the distribution of dust extinction A0 towards this source (A0_p50)"}, {"name": "A0p75", "desc": "75th percentile of the A0 distribution (A0_p75)"}, {"name": "A0p84", "desc": "84th percentile of the A0 distribution (A0_p84)"}, {"name": "R0best", "desc": "multivariate maximum posterior estimate for the average dust grain size extinction parameter (R0_best)"}, {"name": "R0max", "desc": "Maximum of the R0 distribution (R0_max)"}, {"name": "R0min", "desc": "Minimum of the R0 distribution (R0_min)"}, {"name": "R0p16", "desc": "16th percentile of the R0 distribution (R0_p16)"}, {"name": "R0p25", "desc": "25th percentile of the R0 distribution (R0_p25)"}, {"name": "R0med", "desc": "median of the distribution of average dust grain size extinction parameter (R0_p50)"}, {"name": "R0p75", "desc": "75th percentile of the R0 distribution (R0_p75)"}, {"name": "R0p84", "desc": "84th percentile of the R0 distribution (R0_p84)"}, {"name": "dmodbest", "desc": "multivariate maximum posterior estimate for the distance modulus (dmod_best)"}, {"name": "dmodmax", "desc": "Maximum of the dmod distribution (dmod_max)"}, {"name": "dmodmin", "desc": "Minimum of the dmod distribution (dmod_min)"}, {"name": "dmodp16", "desc": "16th percentile of the dmod distribution (dmod_p16)"}, {"name": "dmodp25", "desc": "25th percentile of the dmod distribution (dmod_p25)"}, {"name": "dmodmed", "desc": "median of the distribution of distance modulus (dmod_p50)"}, {"name": "dmodp75", "desc": "75th percentile of the dmod distribution (dmod_p75)"}, {"name": "dmodp84", "desc": "84th percentile of the dmod distribution (dmod_p84)"}, {"name": "lnlikebest", "desc": "multivariate maximum posterior estimate for the log likelihood of the solution (paper Eq. 1) (lnlike_best)"}, {"name": "lnlikemax", "desc": "Maximum of the lnlike distribution (lnlike_max)"}, {"name": "lnlikemin", "desc": "Minimum of the lnlike distribution (lnlike_min)"}, {"name": "lnlikep16", "desc": "16th percentile of the lnlike distribution (lnlike_p16)"}, {"name": "lnlikep25", "desc": "25th percentile of the lnlike distribution (lnlike_p25)"}, {"name": "lnlikemed", "desc": "median of the distribution of log likelihood of the solution (paper Eq. 1) (lnlike_p50)"}, {"name": "lnlikep75", "desc": "75th percentile of the lnlike distribution (lnlike_p75)"}, {"name": "lnlikep84", "desc": "84th percentile of the lnlike distribution (lnlike_p84)"}, {"name": "lnpbest", "desc": "multivariate maximum posterior estimate for the log posterior of the solution (paper Eq. 2) (lnp_best)"}, {"name": "lnpmax", "desc": "Maximum of the lnp distribution (lnp_max)"}, {"name": "lnpmin", "desc": "Minimum of the lnp distribution (lnp_min)"}, {"name": "lnpp16", "desc": "16th percentile of the lnp distribution (lnp_p16)"}, {"name": "lnpp25", "desc": "25th percentile of the lnp distribution (lnp_p25)"}, {"name": "lnpmed", "desc": "median of the distribution of log posterior of the solution (paper Eq. 2) (lnp_p50)"}, {"name": "lnpp75", "desc": "75th percentile of the lnp distribution (lnp_p75)"}, {"name": "lnpp84", "desc": "84th percentile of the lnp distribution (lnp_p84)"}, {"name": "log10jitterbest", "desc": "multivariate maximum posterior estimate for the log photometric likelihood jitter common to all bands (log10jitter_best)"}, {"name": "log10jittermax", "desc": "Maximum of the log10jitter distribution (log10jitter_max)"}, {"name": "log10jittermin", "desc": "Minimum of the log10jitter distribution (log10jitter_min)"}, {"name": "log10jitterp16", "desc": "16th percentile of the log10jitter distribution (log10jitter_p16)"}, {"name": "log10jitterp25", "desc": "25th percentile of the log10jitter distribution (log10jitter_p25)"}, {"name": "log10jittermed", "desc": "median of the distribution of log photometric likelihood jitter common to all bands (log10jitter_p50)"}, {"name": "log10jitterp75", "desc": "75th percentile of the log10jitter distribution (log10jitter_p75)"}, {"name": "log10jitterp84", "desc": "84th percentile of the log10jitter distribution (log10jitter_p84)"}, {"name": "logAbest", "desc": "multivariate maximum posterior estimate for the log10 of the age (logA_best)"}, {"name": "logAmax", "desc": "Maximum of the logA distribution (logA_max)"}, {"name": "logAmin", "desc": "Minimum of the logA distribution (logA_min)"}, {"name": "logAp16", "desc": "16th percentile of the logA distribution (logA_p16)"}, {"name": "logAp25", "desc": "25th percentile of the logA distribution (logA_p25)"}, {"name": "logAmed", "desc": "median of the distribution of log10 of the age (logA_p50)"}, {"name": "logAp75", "desc": "75th percentile of the logA distribution (logA_p75)"}, {"name": "logAp84", "desc": "84th percentile of the logA distribution (logA_p84)"}, {"name": "logLbest", "desc": "multivariate maximum posterior estimate for the log10 of the luminosity (logL_best)"}, {"name": "logLmax", "desc": "Maximum of the logL distribution (logL_max)"}, {"name": "logLmin", "desc": "Minimum of the logL distribution (logL_min)"}, {"name": "logLp16", "desc": "16th percentile of the logL distribution (logL_p16)"}, {"name": "logLp25", "desc": "25th percentile of the logL distribution (logL_p25)"}, {"name": "logLmed", "desc": "median of the distribution of log10 of the luminosity (logL_p50)"}, {"name": "logLp75", "desc": "75th percentile of the logL distribution (logL_p75)"}, {"name": "logLp84", "desc": "84th percentile of the logL distribution (logL_p84)"}, {"name": "logMbest", "desc": "multivariate maximum posterior estimate for the log10 of the mass (logM_best)"}, {"name": "logMmax", "desc": "Maximum of the logM distribution (logM_max)"}, {"name": "logMmin", "desc": "Minimum of the logM distribution (logM_min)"}, {"name": "logMp16", "desc": "16th percentile of the logM distribution (logM_p16)"}, {"name": "logMp25", "desc": "25th percentile of the logM distribution (logM_p25)"}, {"name": "logMmed", "desc": "median of the distribution of log10 of the mass (logM_p50)"}, {"name": "logMp75", "desc": "75th percentile of the logM distribution (logM_p75)"}, {"name": "logMp84", "desc": "84th percentile of the logM distribution (logM_p84)"}, {"name": "logTbest", "desc": "multivariate maximum posterior estimate for the log10 of the effective temperature (logT_best)"}, {"name": "logTmax", "desc": "Maximum of the logT distribution (logT_max)"}, {"name": "logTmin", "desc": "Minimum of the logT distribution (logT_min)"}, {"name": "logTp16", "desc": "16th percentile of the logT distribution (logT_p16)"}, {"name": "logTp25", "desc": "25th percentile of the logT distribution (logT_p25)"}, {"name": "logTmed", "desc": "median of the distribution of log10 of the effective temperature (logT_p50)"}, {"name": "logTp75", "desc": "75th percentile of the logT distribution (logT_p75)"}, {"name": "logTp84", "desc": "84th percentile of the logT distribution (logT_p84)"}, {"name": "loggbest", "desc": "multivariate maximum posterior estimate for the log10 of the surface gravity (logg_best)"}, {"name": "loggmax", "desc": "Maximum of the logg distribution (logg_max)"}, {"name": "loggmin", "desc": "Minimum of the logg distribution (logg_min)"}, {"name": "loggp16", "desc": "16th percentile of the logg distribution (logg_p16)"}, {"name": "loggp25", "desc": "25th percentile of the logg distribution (logg_p25)"}, {"name": "loggmed", "desc": "median of the distribution of log10 of the surface gravity (logg_p50)"}, {"name": "loggp75", "desc": "75th percentile of the logg distribution (logg_p75)"}, {"name": "loggp84", "desc": "84th percentile of the logg distribution (logg_p84)"}, {"name": "Plx", "desc": "Recalibrated parallax (parallax) (2) "}, {"name": "e_Plx", "desc": "Error in recalibrated parallax (parallax_sigma) (3)"}, {"name": "ABPbest", "desc": "multivariate maximum posterior estimate for the attenuation in the Gaia BP band towards this source (A_BP_best)"}, {"name": "ABPmax", "desc": "Maximum of the A_BP distribution (A_BP_max)"}, {"name": "ABPmin", "desc": "Minimum of the A_BP distribution (A_BP_min)"}, {"name": "ABPp16", "desc": "16th percentile of the A_BP distribution (A_BP_p16)"}, {"name": "ABPp25", "desc": "25th percentile of the A_BP distribution (A_BP_p25)"}, {"name": "ABPmed", "desc": "median of the distribution of attenuation in the Gaia BP band towards this source (A_BP_p50)"}, {"name": "ABPp75", "desc": "75th percentile of the A_BP distribution (A_BP_p75)"}, {"name": "ABPp84", "desc": "84th percentile of the A_BP distribution (A_BP_p84)"}, {"name": "AGbest", "desc": "multivariate maximum posterior estimate for the attenuation in the Gaia G band towards this source (A_G_best)"}, {"name": "AGmax", "desc": "Maximum of the A_G distribution (A_G_max)"}, {"name": "AGmin", "desc": "Minimum of the A_G distribution (A_G_min)"}, {"name": "AGp16", "desc": "16th percentile of the A_G distribution (A_G_p16)"}, {"name": "AGp25", "desc": "25th percentile of the A_G distribution (A_G_p25)"}, {"name": "AGmed", "desc": "median of the distribution of attenuation in the Gaia G band towards this source (A_G_p50)"}, {"name": "AGp75", "desc": "75th percentile of the A_G distribution (A_G_p75)"}, {"name": "AGp84", "desc": "84th percentile of the A_G distribution (A_G_p84)"}, {"name": "ARPbest", "desc": "multivariate maximum posterior estimate for the attenuation in the Gaia RP band towards this source (A_RP_best)"}, {"name": "ARPmax", "desc": "Maximum of the A_RP distribution (A_RP_max)"}, {"name": "ARPmin", "desc": "Minimum of the A_RP distribution (A_RP_min)"}, {"name": "ARPp16", "desc": "16th percentile of the A_RP distribution (A_RP_p16)"}, {"name": "ARPp25", "desc": "25th percentile of the A_RP distribution (A_RP_p25)"}, {"name": "ARPmed", "desc": "median of the distribution of attenuation in the Gaia RP band towards this source (A_RP_p50)"}, {"name": "ARPp75", "desc": "75th percentile of the A_RP distribution (A_RP_p75)"}, {"name": "ARPp84", "desc": "84th percentile of the A_RP distribution (A_RP_p84)"}, {"name": "BP", "desc": "Recalibrated Gaia BP magnitude (BP) (4)"}, {"name": "BPbest", "desc": "multivariate maximum posterior estimate for the Gaia BP magnitude (BP_best)"}, {"name": "BPmax", "desc": "Maximum of the BP distribution (BP_max)"}, {"name": "BPmin", "desc": "Minimum of the BP distribution (BP_min)"}, {"name": "BPp16", "desc": "16th percentile of the BP distribution (BP_p16)"}, {"name": "BPp25", "desc": "25th percentile of the BP distribution (BP_p25)"}, {"name": "BPmed", "desc": "median of the distribution of Gaia BP magnitude (BP_p50)"}, {"name": "BPp75", "desc": "75th percentile of the BP distribution (BP_p75)"}, {"name": "BPp84", "desc": "84th percentile of the BP distribution (BP_p84)"}, {"name": "e_BP", "desc": "Recalibrated error from original Gaia BP magnitude (BP_sigma) (5)"}, {"name": "G", "desc": "Recalibrated Gaia G magnitude (G) (6) "}, {"name": "Gbest", "desc": "multivariate maximum posterior estimate for the Gaia G magnitude (G_best)"}, {"name": "Gmax", "desc": "Maximum of the G distribution (G_max) "}, {"name": "Gmin", "desc": "Minimum of the G distribution (G_min) "}, {"name": "Gp16", "desc": "16th percentile of the G distribution (G_p16)"}, {"name": "Gp25", "desc": "25th percentile of the G distribution (G_p25)"}, {"name": "Gmed", "desc": "median of the distribution of Gaia G magnitude (G_p50)"}, {"name": "Gp75", "desc": "75th percentile of the G distribution (G_p75)"}, {"name": "Gp84", "desc": "84th percentile of the G distribution (G_p84)"}, {"name": "e_G", "desc": "Recalibrated error from original Gaia G magnitude (G_sigma) (5)"}, {"name": "H", "desc": "Recalibrated 2MASS H magnitude (H) "}, {"name": "Hbest", "desc": "multivariate maximum posterior estimate for the 2MASS H magnitude (H_best)"}, {"name": "Hmax", "desc": "Maximum of the H distribution (H_max) "}, {"name": "Hmin", "desc": "Minimum of the H distribution (H_min) "}, {"name": "Hp16", "desc": "16th percentile of the H distribution (H_p16)"}, {"name": "Hp25", "desc": "25th percentile of the H distribution (H_p25)"}, {"name": "Hmed", "desc": "median of the distribution of 2MASS H magnitude (H_p50)"}, {"name": "Hp75", "desc": "75th percentile of the H distribution (H_p75)"}, {"name": "Hp84", "desc": "84th percentile of the H distribution (H_p84)"}, {"name": "e_H", "desc": "Recalibrated error from original 2MASS H magnitude (H_sigma) (5)"}, {"name": "J", "desc": "Recalibrated 2MASS J magnitude (J) "}, {"name": "Jbest", "desc": "multivariate maximum posterior estimate for the 2MASS J magnitude (J_best)"}, {"name": "Jmax", "desc": "Maximum of the J distribution (J_max) "}, {"name": "Jmin", "desc": "Minimum of the J distribution (J_min) "}, {"name": "Jp16", "desc": "16th percentile of the J distribution (J_p16)"}, {"name": "Jp25", "desc": "25th percentile of the J distribution (J_p25)"}, {"name": "Jmed", "desc": "median of the distribution of 2MASS J magnitude (J_p50)"}, {"name": "Jp75", "desc": "75th percentile of the J distribution (J_p75)"}, {"name": "Jp84", "desc": "84th percentile of the J distribution (J_p84)"}, {"name": "e_J", "desc": "Recalibrated error from original 2MASS J magnitude (J_sigma) (5)"}, {"name": "Ks", "desc": "Recalibrated 2MASS Ks magnitude (Ks) "}, {"name": "Ksbest", "desc": "multivariate maximum posterior estimate for the 2MASS Ks magnitude (Ks_best)"}, {"name": "Ksmax", "desc": "Maximum of the Ks distribution (Ks_max)"}, {"name": "Ksmin", "desc": "Minimum of the Ks distribution (Ks_min)"}, {"name": "Ksp16", "desc": "16th percentile of the Ks distribution (Ks_p16)"}, {"name": "Ksp25", "desc": "25th percentile of the Ks distribution (Ks_p25)"}, {"name": "Ksmed", "desc": "median of the distribution of 2MASS Ks magnitude (Ks_p50)"}, {"name": "Ksp75", "desc": "75th percentile of the Ks distribution (Ks_p75)"}, {"name": "Ksp84", "desc": "84th percentile of the Ks distribution (Ks_p84)"}, {"name": "e_Ks", "desc": "Recalibrated error from original 2MASS Ks magnitude (Ks_sigma) (5)"}, {"name": "RP", "desc": "Recalibrated Gaia RP magnitude (RP) (4)"}, {"name": "RPbest", "desc": "multivariate maximum posterior estimate for the Gaia RP magnitude (RP_best)"}, {"name": "RPmax", "desc": "Maximum of the RP distribution (RP_max)"}, {"name": "RPmin", "desc": "Minimum of the RP distribution (RP_min)"}, {"name": "RPp16", "desc": "16th percentile of the RP distribution (RP_p16)"}, {"name": "RPp25", "desc": "25th percentile of the RP distribution (RP_p25)"}, {"name": "RPmed", "desc": "median of the distribution of Gaia RP magnitude (RP_p50)"}, {"name": "RPp75", "desc": "75th percentile of the RP distribution (RP_p75)"}, {"name": "RPp84", "desc": "84th percentile of the RP distribution (RP_p84)"}, {"name": "e_RP", "desc": "Recalibrated error from original (RP) Gaia RP magnitude (RP_sigma) (5)"}, {"name": "W1", "desc": "Recalibrated error from original (W1) WISE W1 magnitude (5)"}, {"name": "W1best", "desc": "multivariate maximum posterior estimate for the WISE W1 magnitude (W1_best)"}, {"name": "W1max", "desc": "Maximum of the W1 distribution (W1_max)"}, {"name": "W1min", "desc": "Minimum of the W1 distribution (W1_min)"}, {"name": "W1p16", "desc": "16th percentile of the W1 distribution (W1_p16)"}, {"name": "W1p25", "desc": "25th percentile of the W1 distribution (W1_p25)"}, {"name": "W1med", "desc": "median of the distribution of WISE W1 magnitude (W1_p50)"}, {"name": "W1p75", "desc": "75th percentile of the W1 distribution (W1_p75)"}, {"name": "W1p84", "desc": "84th percentile of the W1 distribution (W1_p84)"}, {"name": "e_W1", "desc": "Recalibrated error from original WISE W1 magnitude (W1_sigma) (5)"}, {"name": "W2", "desc": "Recalibrated WISE W2 magnitude (W2) "}, {"name": "W2best", "desc": "multivariate maximum posterior estimate for the WISE W2 magnitude (W2_best)"}, {"name": "W2max", "desc": "Maximum of the W2 distribution (W2_max)"}, {"name": "W2min", "desc": "Minimum of the W2 distribution (W2_min)"}, {"name": "W2p16", "desc": "16th percentile of the W2 distribution (W2_p16)"}, {"name": "W2p25", "desc": "25th percentile of the W2 distribution (W2_p25)"}, {"name": "W2med", "desc": "median of the distribution of WISE W2 magnitude (W2_p50)"}, {"name": "W2p75", "desc": "75th percentile of the W2 distribution (W2_p75)"}, {"name": "W2p84", "desc": "84th percentile of the W2 distribution (W2_p84)"}, {"name": "e_W2", "desc": "Recalibrated error from original WISE W2 magnitude (W2_sigma) (5)"}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VI_115"}} {"id": "VI/115", "title_cds": "Second Epoch Sky Survey Plate List", "title_create": "Read 2005", "year": "2005", "author": "Read M.", "title_pub": "Second Epoch Sky Survey Plate List", "first_author": "Read M.", "ref_biblio": [""], "see_also": ["VI/25 : POSS Plate Data (Palomar Obs. 1960)", "VI/30 : Plates of the ESO Sky Survey (Holmberg+ 1974-)", "VI/114 : second epoch Palomar Oschin Schmidt Sky Survey (POSS2)", "http://www.roe.ac.uk/ifa/wfau/ukstu/pltcat.html : ROE Plate Catalogue"], "keyword_cds": "Surveys; Plate data", "type": ["OC"], "records": ["606 fields"], "data": "", "date_update": "03-Feb-2006", "tables": [{"name": "ukstu.dat", "desc": "List plats for 606 fields ", "columns": [{"name": "FE", "desc": "[OR] Plate prefix, a one- or two-character code for the filter/emulsion combination"}, {"name": "Plate", "desc": "Plate number "}, {"name": "---", "desc": "[*] "}, {"name": "---", "desc": "[R] Color "}, {"name": "Tpl", "desc": "? Non-survey field code "}, {"name": "Field", "desc": "Field number "}, {"name": "RAh", "desc": "Right Ascension 1950 of plate centre (hours) "}, {"name": "RAm", "desc": "Right Ascension 1950 of plate centre (minutes) "}, {"name": "DE-", "desc": "Declination 1950 of plate centre (sign) "}, {"name": "DEd", "desc": "Declination 1950 of plate centre (deg) "}, {"name": "DEm", "desc": "Declination 1950 of plate centre (min) "}, {"name": "Obs.Y", "desc": "Observation date (year) "}, {"name": "Obs.M", "desc": "Observation date (month) "}, {"name": "Obs.D", "desc": "Observation date (day) "}, {"name": "---", "desc": "[:] "}, {"name": "LST", "desc": "Local Sideral Time of start of exposure "}, {"name": "Emuls", "desc": "Plate emulsion "}, {"name": "Filter", "desc": "Filter name "}, {"name": "Exp", "desc": "Exposure time "}, {"name": "Grade", "desc": "Image quality (2) "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VI_123"}} {"id": "VI/123", "title_cds": "Photometrical Catalogues and Standards, 1953-1968", "title_create": "Sharov+ 1970", "year": "1970", "author": "Sharov A.S., Jakimova N.N.", "title_pub": "A new, machine-readable version of the compilation \"Photometrical Catalogues and Standards\", updated and revised by M. Morel, 2006 Oct. 24", "first_author": "Sharov A.S.", "ref_biblio": [""], "bibcode": ["1970TrSht..40..106S"], "keyword_cds": "Photometry, sequences; Photometry, standards; Photometry, UBV; Photometry, UcBV; Photometry, UBVRI; Photometry, Eggen", "description": ["The Sharov & Jakimova compilation of published photometrical standards", "is presented as computer readable files. Two main tables (References", "and Catalogue) are presented, plus an Errors file. Russian", "script/terms are replaced by the English equivalents. The original", "coordinate system (1950) are replaced by J2000 positions. A number of", "errors or ambiguous entries have been amended. SIMBAD bibcodes are", "provided for papers cited by Sharov and Jakimova."], "records": ["734 stars"], "data": "", "date_update": "24-Oct-2006", "tables": [{"name": "catalog.dat", "desc": "List of photometric standards/sequences ", "columns": [{"name": "Object", "desc": "Name of object / field / sequence "}, {"name": "RAh", "desc": "Right Ascension (J2000), hours "}, {"name": "RAmin", "desc": "Right Ascension (J2000), minutes "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (J2000), degrees "}, {"name": "DEm", "desc": "Declination (J2000), minutes "}, {"name": "Ref.", "desc": "Ref. number assigned by Sharov & Jakimova "}, {"name": "System", "desc": "Photometric system "}, {"name": "Stars", "desc": "Number of stars in sequence "}, {"name": "Vmag1", "desc": "Bright limit of sequence "}, {"name": "Hyphen", "desc": "Range separator "}, {"name": "Vmag2", "desc": "Faint limit of sequence "}, {"name": "Notes", "desc": "Supplementary remarks "}]}, {"name": "refs.dat", "desc": "SIMBAD Bibcodes for all cited papers ", "columns": [{"name": "Ref.No.", "desc": "Number assigned by Sharov & Jakimova (Table 1). "}, {"name": "Bibcode", "desc": "SIMBAD / NED bibcode "}, {"name": "Reference", "desc": "Full reference from Sharov & Jakimova (Table 1). "}]}, {"name": "errors.dat", "desc": "Amendments included in file Catalog.txt ", "columns": [{"name": "Object", "desc": "Name of object / field / sequence "}, {"name": "RAh", "desc": "Right Ascension (J2000), hours "}, {"name": "RAmin", "desc": "Right Ascension (J2000), minutes "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (J2000), degrees "}, {"name": "DEm", "desc": "Declination (J2000), minutes "}, {"name": "Ref.", "desc": "Ref. number assigned by Sharov & Jakimova "}, {"name": "Problem", "desc": "Correction or amendment made "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VI_124"}} {"id": "VI/124", "title_cds": "Plate centers of the Direct observations of UKST", "title_create": "SuperCOSMOS, 2002", "year": "2002", "author": "SuperCOSMOS Sky Surveys", "title_pub": "Plate centers of the Direct observations of UKST", "first_author": "SuperCOSMOS Sky Surveys", "ref_biblio": [""], "keyword_cds": "Plate data ; Observatory log", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["UKST"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "24-Jun-2007"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VI_126"}} {"id": "VI/126", "title_cds": "Catalogue of Wide-Field Plate Archives", "title_create": "Tsvetkova+ 2008", "year": "2008", "author": "Tsvetkova K., Tsvetkov M.", "title_pub": "Catalogue of Wide-Field Plate Archives (V5.2, July 2008)", "first_author": "Tsvetkova K.", "ref_biblio": [""], "see_also": ["http://www.wfpa.bas.bg/ : Wide-Field Plate Database home page", "VI/90 : Wide-Field Plate Database (Tsvetkov+ 1997)"], "keyword_cds": "Observatory log ; Plate data", "keyword_pub": "Catalogues; Photographic plate archives; Plate data", "description": ["The Catalogue of Wide-Field Plate Archives (CWFPAs, version 5.2 from", "July 2008) contains the information for 440 plate archives stored in", "astronomical observatories and institutions all over the world. It is", "an integrated part of the Wide-Field Plate Database (WFPDB) aiming to", "store the valuable astronomical plate observations (more than", "2,200,000 wide-field plates or films) and quickly to offer the", "opportunity to see back in time records of interesting astronomical", "phenomena. The Catalogue provides information for the location", "(storage) of the plate archives - site and country; for the", "observatory, where the archive was made - name, site, country,", "Marsden's number, time zone, coordinates and altitude; for the archive", "instrument - original name, clear aperture, mirror diameter, focal", "length, scale, type, field size and years of operation; for the number", "of direct and objective prism plates; for the archive type, quality", "and the name of astronomer in charge for possible contacts. Search for", "plate archives can be made using the WFPDB instrument identifier", "(equal to archive identifier), which constitutes from the WFPDB", "observatory identifier, instrument aperture, and possible suffix to", "the instrument identifier in the cases when more instruments with the", "same aperture exist in the observatory."], "alias": ["CWFPA"], "type": ["BCC"], "records": ["records"], "data": "", "date_update": "06-Oct-2008", "tables": [{"name": "cwfpa.dat", "desc": "Catalogue of wide-field plate archives ", "columns": [{"name": "IDobs", "desc": "*WFPDB observatory identifier "}, {"name": "IDins", "desc": "*? Instrument aperture "}, {"name": "m_IDins", "desc": "*[A-Z ] Suffix to the instrument identifier "}, {"name": "ORI", "desc": "Original name of the instrument "}, {"name": "LOC.site", "desc": "Location of the plate archive, town (site) "}, {"name": "LOC.ctry", "desc": "Location of the plate archive, country "}, {"name": "OBS.name", "desc": "Observatory, name "}, {"name": "OBS.site", "desc": "Observatory, site "}, {"name": "OBS.ctry", "desc": "Observatory, country "}, {"name": "MNo", "desc": "? Marsden's number "}, {"name": "TZ", "desc": "? Time zone "}, {"name": "LON-", "desc": "? Observatory longitude, sign "}, {"name": "LONd", "desc": "? Observatory longitude, deg "}, {"name": "LONm", "desc": "? Observatory longitude, arcmin "}, {"name": "LAT-", "desc": "? Observatory latitude, sign "}, {"name": "LATd", "desc": "? Observatory latitude, deg "}, {"name": "LATm", "desc": "? Observatory latitude, arcmin "}, {"name": "ALT", "desc": "? Observatory altitude "}, {"name": "MULT", "desc": "? Multiplicity of telescope cameras "}, {"name": "---", "desc": "[x] Sign 'x' "}, {"name": "APR", "desc": "? Clear aperture of the telescope "}, {"name": "MD", "desc": "? Diameter of telescope mirror "}, {"name": "FL", "desc": "? Focal length of the telescope "}, {"name": "SCL", "desc": "? Plate scale "}, {"name": "ITYPE", "desc": "*Instrument type "}, {"name": "FIELD", "desc": "? Field angular dimension "}, {"name": "YEAR1", "desc": "? Year of beginning of telescope operation "}, {"name": "YEAR2", "desc": "? Year of end of telescope operation "}, {"name": "PF", "desc": "Indication F for film, PF for plate and film "}, {"name": "NPd", "desc": "? Number of direct plates "}, {"name": "NPUNd", "desc": "[: ] Uncertainty of the number of plates "}, {"name": "NOT", "desc": "? Notes to the number of plates "}, {"name": "CFORMd", "desc": "*Plate catalog form (direct plates) "}, {"name": "NPs", "desc": "? Number of objective prism plates "}, {"name": "CFORMs", "desc": "*Plate catalog form (obj. prism plates) "}, {"name": "QUAL", "desc": "*[ABD ] Code for plte archive quality "}, {"name": "ANAME", "desc": "Astronomer in charge "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VI_61"}} {"id": "VI/61", "title_cds": "O2 Absorption Cross Sections", "title_create": "Yoshino+ 1992", "year": "1992", "author": "Yoshino K., Esmond J.R., Cheung A.S.-C., Freeman D.E., Parkinson W.H", "title_pub": "High resolution absorption cross sections in the transmission window region of the Schumann-Runge bands and Herzberg continuum of O_2_", "first_author": "Yoshino K.", "ref_biblio": [""], "bibcode": ["1992P&SS...40..185Y"], "keyword_cds": "Atomic physics ; Spectra, ultraviolet", "abstract": ["The absorption cross sections of the Schumann-Runge bands in the", "window region between the rotational lines have been measured in the", "wavelength region 180-195 nm. The measurements have been done with", "many different pressures of oxygen, 2.5-760 torr, so that the", "pressure- dependent absorption can be separated from the main cross", "sections. The published cross sections [Yoshino et al., Planet. Space", "Sci. 31, 339 (1983)] in the window region are superseded by the", "present cross sections. The combined cross sections are available at", "wavenumber intervals of ~0.1 cm-1. The Herzberg continuum cross", "sections are derived after subtracting calculated contributions from", "the Schumann-Runge bands and are significantly smaller than any", "previous measurements."], "type": ["OC"], "records": ["94384 points"], "doi_pub": ["10.1016/0032-0633(92)90056-T"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "o2wb01x0.dat", "desc": "Data file (wave num 49362. - 50050.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb02x0.dat", "desc": "Data file (wave num 50050. - 50720.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb03x0.dat", "desc": "Data file (wave num 50720. - 51370.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb04x0.dat", "desc": "Data file (wave num 50370. - 51980.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb05x0.dat", "desc": "Data file (wave num 51980. - 52661.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb06x0.dat", "desc": "Data file (wave num 52661. - 53250.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb07x0.dat", "desc": "Data file (wave num 53250. - 53746.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb08x0.dat", "desc": "Data file (wave num 53746. - 54256.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb09x0.dat", "desc": "Data file (wave num 54260. - 54685.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb10x0.dat", "desc": "Data file (wave num 54685. - 55115.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb11x0.dat", "desc": "Data file (wave num 55115. - 55485.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb12x0.dat", "desc": "Data file (wave num 55485. - 55800.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VI_77"}} {"id": "VI/77", "title_cds": "Theoretical Stellar Fluxes", "title_create": "Kurucz+Buser, 1994", "year": "1994", "author": "Kurucz R.L., Buser R.B.", "title_pub": "A Library of Theoretical Stellar Fluxes for F- to K-type stars", "first_author": "Kurucz R.L.", "ref_biblio": ["2) abundance relative to Sun (logarithmic scale)"}, {"name": "Vturb", "desc": "[2] Microturbulence velocity "}, {"name": "l/H", "desc": "[0/1.25] Mixing-length-to-scale-height ratio "}]}, {"name": "fm50k2.dat", "desc": "Fluxes, [Fe/H]=-5.00 ", "columns": []}, {"name": "fm45k2.dat", "desc": "Fluxes, [Fe/H]=-4.50 ", "columns": []}, {"name": "fm40k2.dat", "desc": "Fluxes, [Fe/H]=-4.00 ", "columns": []}, {"name": "fm35k2.dat", "desc": "Fluxes, [Fe/H]=-3.50 ", "columns": []}, {"name": "fm30k2.dat", "desc": "Fluxes, [Fe/H]=-3.00 ", "columns": []}, {"name": "fm25k2.dat", "desc": "Fluxes, [Fe/H]=-2.50 ", "columns": []}, {"name": "fm20k2.dat", "desc": "Fluxes, [Fe/H]=-2.00 ", "columns": []}, {"name": "fm15k2.dat", "desc": "Fluxes, [Fe/H]=-1.50 ", "columns": []}, {"name": "fm10k2.dat", "desc": "Fluxes, [Fe/H]=-1.00 ", "columns": []}, {"name": "fm05k2.dat", "desc": "Fluxes, [Fe/H]=-0.50 ", "columns": []}, {"name": "fm03k2.dat", "desc": "Fluxes, [Fe/H]=-0.30 ", "columns": []}, {"name": "fm02k2.dat", "desc": "Fluxes, [Fe/H]=-0.20 ", "columns": []}, {"name": "fp00k2.dat", "desc": "Fluxes, [Fe/H]=+0.00 ", "columns": []}, {"name": "fm01k2.dat", "desc": "Fluxes, [Fe/H]=-0.10 ", "columns": []}, {"name": "fp01k2.dat", "desc": "Fluxes, [Fe/H]=+0.10 ", "columns": []}, {"name": "fp02k2.dat", "desc": "Fluxes, [Fe/H]=+0.20 ", "columns": []}, {"name": "fp03k2.dat", "desc": "Fluxes, [Fe/H]=+0.30 ", "columns": []}, {"name": "fp05k2.dat", "desc": "Fluxes, [Fe/H]=+0.50 ", "columns": []}, {"name": "fp10k2.dat", "desc": "Fluxes, [Fe/H]=+1.00 ", "columns": []}, {"name": "fsun.dat", "desc": "Fluxes, Sun ", "columns": []}, {"name": "fvega.dat", "desc": "Fluxes, Vega ", "columns": []}, {"name": "uvby.f", "desc": "FORTRAN program to compute uvby colors ", "columns": []}, {"name": "uvbyca.f", "desc": "FORTRAN program to compute uvbyca colors ", "columns": []}, {"name": "ubvm50.dat", "desc": "Theoretical UBV, [Fe/H]=-5.00 ", "columns": []}, {"name": "ubvm45.dat", "desc": "Theoretical UBV, [Fe/H]=-4.50 ", "columns": []}, {"name": "ubvm40.dat", "desc": "Theoretical UBV, [Fe/H]=-4.00 ", "columns": []}, {"name": "ubvm35.dat", "desc": "Theoretical UBV, [Fe/H]=-3.50 ", "columns": []}, {"name": "ubvm30.dat", "desc": "Theoretical UBV, [Fe/H]=-3.00 ", "columns": []}, {"name": "ubvm25.dat", "desc": "Theoretical UBV, [Fe/H]=-2.50 ", "columns": []}, {"name": "ubvm20.dat", "desc": "Theoretical UBV, [Fe/H]=-2.00 ", "columns": []}, {"name": "ubvm15.dat", "desc": "Theoretical UBV, [Fe/H]=-1.50 ", "columns": []}, {"name": "ubvm10.dat", "desc": "Theoretical UBV, [Fe/H]=-1.00 ", "columns": []}, {"name": "ubvm05.dat", "desc": "Theoretical UBV, [Fe/H]=-0.50 ", "columns": []}, {"name": "ubvm03.dat", "desc": "Theoretical UBV, [Fe/H]=-0.30 ", "columns": []}, {"name": "ubvm02.dat", "desc": "Theoretical UBV, [Fe/H]=-0.20 ", "columns": []}, {"name": "ubvm01.dat", "desc": "Theoretical UBV, [Fe/H]=-0.10 ", "columns": []}, {"name": "ubvp00.dat", "desc": "Theoretical UBV, [Fe/H]=+0.00 ", "columns": []}, {"name": "ubvp01.dat", "desc": "Theoretical UBV, [Fe/H]=+0.10 ", "columns": []}, {"name": "ubvp02.dat", "desc": "Theoretical UBV, [Fe/H]=+0.20 ", "columns": []}, {"name": "ubvp03.dat", "desc": "Theoretical UBV, [Fe/H]=+0.30 ", "columns": []}, {"name": "ubvp05.dat", "desc": "Theoretical UBV, [Fe/H]=+0.50 ", "columns": []}, {"name": "ubvp10.dat", "desc": "Theoretical UBV, [Fe/H]=+1.00 ", "columns": []}, {"name": "ubvsun.dat", "desc": "UBV, Sun ", "columns": []}, {"name": "ubvvega.dat", "desc": "UBV, Vega ", "columns": []}, {"name": "uvbym50.dat", "desc": "Theoretical uvby, [Fe/H]=-5.00 ", "columns": []}, {"name": "uvbym45.dat", "desc": "Theoretical uvby, [Fe/H]=-4.50 ", "columns": []}, {"name": "uvbym40.dat", "desc": "Theoretical uvby, [Fe/H]=-4.00 ", "columns": []}, {"name": "uvbym35.dat", "desc": "Theoretical uvby, [Fe/H]=-3.50 ", "columns": []}, {"name": "uvbym30.dat", "desc": "Theoretical uvby, [Fe/H]=-3.00 ", "columns": []}, {"name": "uvbym25.dat", "desc": "Theoretical uvby, [Fe/H]=-2.50 ", "columns": []}, {"name": "uvbym20.dat", "desc": "Theoretical uvby, [Fe/H]=-2.00 ", "columns": []}, {"name": "uvbym15.dat", "desc": "Theoretical uvby, [Fe/H]=-1.50 ", "columns": []}, {"name": "uvbym10.dat", "desc": "Theoretical uvby, [Fe/H]=-1.00 ", "columns": []}, {"name": "uvbym05.dat", "desc": "Theoretical uvby, [Fe/H]=-0.50 ", "columns": []}, {"name": "uvbym03.dat", "desc": "Theoretical uvby, [Fe/H]=-0.30 ", "columns": []}, {"name": "uvbym02.dat", "desc": "Theoretical uvby, [Fe/H]=-0.20 ", "columns": []}, {"name": "uvbym01.dat", "desc": "Theoretical uvby, [Fe/H]=-0.10 ", "columns": []}, {"name": "uvbyp00.dat", "desc": "Theoretical uvby, [Fe/H]=+0.00 ", "columns": []}, {"name": "uvbyp01.dat", "desc": "Theoretical uvby, [Fe/H]=+0.10 ", "columns": []}, {"name": "uvbyp02.dat", "desc": "Theoretical uvby, [Fe/H]=+0.20 ", "columns": []}, {"name": "uvbyp03.dat", "desc": "Theoretical uvby, [Fe/H]=+0.30 ", "columns": []}, {"name": "uvbyp05.dat", "desc": "Theoretical uvby, [Fe/H]=+0.50 ", "columns": []}, {"name": "uvbyp10.dat", "desc": "Theoretical uvby, [Fe/H]=+1.00 ", "columns": []}, {"name": "uvbysun.dat", "desc": "uvby, Sun ", "columns": []}, {"name": "uvbyvega.dat", "desc": "uvby, Vega ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VI_80A"}} {"id": "VI/80", "title_cds": "Opacities from the Opacity Project", "title_create": "Seaton+, 1995", "year": "1995", "author": "Seaton M.J., Yan Y., Mihalas D., Pradhan A.K.", "title_pub": "Opacities for stellar envelopes", "first_author": "Seaton M.J.", "ref_biblio": ["", " (OPF)"], "bibcode": ["1994MNRAS.266..805S", "1994MNRAS.265L..25S"], "keyword_pub": "Opacities", "description": ["1 CODES.", "*****", "1.1 Code rop.for", "************", "This code reads opacity files written in standard OP format.", "Its main purpose is to provide documentation on the contents of the", "files.", "This code, like the other codes provided, prompts for the name of", "the file (or files) to be read.", "The file names read in response to the prompt may have up to 128", "characters.", "1.2 Code opfit.for", "**************", "This code reads opacity files in standard OP format, and", "provides for interpolation of opacities to any required values", "of temperature and mass-density. The method used is described in OPF.", "The code prompts for the name of a file giving all required control", "parameters. As an example, the file opfit.dat is provided (users", "will need to change directory names and file names).", "The use of opfit.for is illustrated using opfit.dat.", "Most users will probably want to adapt opfit.for for use as a subroutine", "in other codes.", "Timings for DEC 7000 ALPHA: 0.3 sec for data read and initialisations;", "then 0.0007 sec for each temperature-density point.", "Users who like OPAL formats should note that opfit.for has a facility", "to produce files of OP data in OPAL-type formats.", "1.3 Code ixz.for", "************", "This code provides for interpolations to any required values of X and", "Z. See S95A. It prompts for the name of a file giving all required control", "parameters. An example of such a file if provided, ixz.dat (the user", "will need to change directory and file names).", "The output files have names s92INT.'nnn'. The user specifies the first", "value of nnn, and the number of files to be produced.", "2. DATA FILES", "**********", "2.1 Data files for solar metal-mix", "******************************", "Data for solar metal-mix s92 as defined in SYMP. These files are", "from version 2 runs of December 1994 (see S95A for details on Version 2).", "There are 213 files with names s92.'nnn', 'nnn'=201 to 413.", "Each file occupies 83762 bytes.", "The file s92.version2 gives values of X (hydrogen mass-faction) and", "Z (metals mass-fraction) for each value of 'nnn'. The user can get", "s92.version2, select the values of 'nnn' required, then get the", "required files s92.'nnn'. The user can see the file in ftp,", "displayed on the screen, by typing \"get s92.version2 -\".", "The files s92.'nnn' can be used with opfit.for to obtain opacities", "for any requires value of temperature and mass density.", "Files for other metal-mixtures will be added in due course.", "Send requests to mjs@star.ucl.ac.uk.", "2.2 Files for interpolation in X and Z", "**********************************", "The data files have names s92xz.'mmm', where 'mmm'=001 to 096.", "They differ from the standard OP files (such as s92.'nnn' ---", "section 2.1 above) in that they contain information", "giving derivatives of opacities with respect to X and Z.", "Each file s92xz.'mmm' occupies 148241 bytes.", "The interpolations to any required values of X and Z are made using", "ixz.for.", "Timings: on DEC 7000 ALPHA, 2.16 sec for each new-mixture file.", "For interpolations to some specified values of X and Z, one requires just", "4 files s92xz.'mmm'. Most users will not require the complete set", "of files s92xz.'mmm'. The file s92xz.index includes a table (starting", "on line 3) giving values, for each 'mmm' file, of x,y,z (abundances by", "number-factions) and X,Y,Z (abundances by mass-fractions). Users are", "advised to get the file s92.index, and select values of 'mmm' for", "files required, then get those files.", "The files produced by ixz.for are in standard OP format and can be", "used with opfit.for to obtain opacities for any required values of", "temperature and mass density.", "3 RECOMMENDED PROCEDURE FOR USE OF OPACITY FILES", "**********************************************", "(1) Get the file s92.version2.", "(2) If the values of X and Z you require are available in the", "files s92.'nnn' then get those files.", "(3) If not, get the file s92xz.index.", "(4) Select from s92xz.index the values of 'mmm' which cover the", "range of X and Z in which your are interested. Get those", "files and use ixz.for to generate files for your exact", "required values of X and Z.", "(5) Note that the exact abundance mixtures used are specified in each", "file (see rop.for). Also each run of opfit.for produces a", "table of abundances.", "(6) If you want a metal-mix different from that of s92, contact", "mjs@star.ucl.ac.uk.", "4 FUTURE DEVELOPMENTS", "*******************", "(1) Files will be added very shortly for calculation of radiative", "forces.", "(2) Facilities will be added later which will enable the user", "to make calculations giving files for any required mixtures."], "date_update": "04-Sep-1995", "tables": [{"name": "rop.for", "desc": "Code to read opacity files (s92.* files) ", "columns": []}, {"name": "opfit.for", "desc": "Code to read opacity files and interpolate to any temperature and mass-density.", "columns": []}, {"name": "ixz.for", "desc": "Code for interpolations to any X and Z values ", "columns": []}, {"name": "ixz.dat", "desc": "Example of input for ixz code ", "columns": []}, {"name": "opfit.dat", "desc": "Example of input for opfit code ", "columns": []}, {"name": "s92.version2", "desc": "Summary of solar metal-mix s92 data ", "columns": [{"name": "Version", "desc": "Version designation \"OP Version 2.0 S92\" "}, {"name": "Mix", "desc": "[201/413]+ Mixture number "}, {"name": "text", "desc": "\"X=\" "}, {"name": "X", "desc": "[0/1] Hydrogen mass-fraction "}, {"name": "text", "desc": "\", Z=\" "}, {"name": "Z", "desc": "[0/1] Metal (Z>=3) mass-fraction "}, {"name": "Date", "desc": "Computation date "}]}, {"name": "s92.*", "desc": "Solar metal-mix s92 as defined in SYMP in standard OP format (213 files)", "columns": []}, {"name": "s92xz.*", "desc": "Opacity derivatives with respect to X and Z (96 files)", "columns": []}, {"name": "s92xz.index", "desc": "Summary of s92xz.* files ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VI_93"}} {"id": "VI/93", "title_cds": "Archive of spectrogrammes of AGNs.", "title_create": "Denisyuk+, 1984", "year": "1984", "author": "Denisyuk E.K., Kondrat'eva L.N.", "title_pub": "Archive of spectrogrammes of the active galaxies nuclei.", "first_author": "Denisyuk E.K.", "ref_biblio": [""], "bibcode": ["1984Afz....20..525D"], "keyword_cds": "Active gal. nuclei; Spectroscopy", "description": ["The archive of the spectrogrammes of the active galaxy nucleis", "obtained in the Fessenkov Astrophysical Institute by Denisyuk E.K. and", "Kondrat'eva L.N. during 25 years has been presented. The spectral", "observations have been carried out using the slit spectrograph with", "three-cascades image-tube, attached to 70-cm reflector. The spectral", "region 370 - 850 nm is available. The optical system allows to choose", "the dispersion in the range: 12-200 0.1nm/mm. The spectral resolution", "is 0.8-13 A in dependence on the dispersion. It is the first part of", "the archive."], "records": ["81 AGNs"], "data": "", "date_update": "06-May-2020", "tables": [{"name": "objects.dat", "desc": "List of Objects ", "columns": [{"name": "RAh", "desc": "Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension 2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension 2000 (seconds) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "Declination 2000 (degrees) "}, {"name": "DEm", "desc": "Declination 2000 (minutes) "}, {"name": "DEs", "desc": "Declination 2000 (seconds) "}, {"name": "Name", "desc": "Principal Name of galaxies, as in table "}, {"name": "---", "desc": "[=] "}, {"name": "Other", "desc": "Other names of galaxies "}]}, {"name": "table", "desc": "The archive of the spectrograms ", "columns": [{"name": "Name", "desc": "*The name of the galaxy "}, {"name": "Date", "desc": "Observation date "}, {"name": "Disp", "desc": "Dispersion "}, {"name": "Grt", "desc": "Grating parameter "}, {"name": "Ord", "desc": "*Order of grating "}, {"name": "N", "desc": "Number of the spectrogrammes "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VI_94"}} {"id": "VI/94", "title_cds": "Archive of spectrogrammes of planetary nebulae", "title_create": "Kondrat'eva, 1994", "year": "1994", "author": "Kondrat'eva L.N.", "title_pub": "The archive of spectrogrammes of the planetary nebulae", "first_author": "Kondrat'eva L.N.", "ref_biblio": ["="], "bibcode": ["1994PAZh..20...644K"], "keyword_cds": "Planetary nebulae; Spectrophotometry", "description": ["The archive of the spectrogrammes of the planetary nebulae", "obtained in the Fessenkov Astrophysical Institute by Kondrat'eva", "L.N. during 25 years. The spectral observations have been carried", "out using the slit spectrograph with three-cascades image-tube,", "attached to 70-cm reflector. The spectral region is 3700 - 8500A.", "Dispersion is in the range: 12-200 A/mm. The spectral resolution", "is 0.8-13 A in dependence on the dispersion. The part of the", "spectrogrammes has been treated and the results have been", "published [1-7]."], "alias": [""], "records": ["165 PNe"], "data": "", "date_update": "12-Oct-2000", "tables": [{"name": "table", "desc": "The archive of the spectrogrammes ", "columns": [{"name": "name", "desc": "The name of the planetary nebula "}, {"name": "LLpb", "desc": "Lower limit of the passband "}, {"name": "ULpb", "desc": "Upper limit of the passband "}, {"name": "Date", "desc": "Date of observation "}, {"name": "n", "desc": "the number of the spectrograms "}]}, {"name": "objects", "desc": "Objects ", "columns": [{"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "? Declination J2000 (seconds) "}, {"name": "name", "desc": "The name of the planetary nebula "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VII_23"}} {"id": "VII/23", "title_cds": "Absorption Lines in QSO Spectra", "title_create": "Ellis+ 1978", "year": "1978", "author": "Ellis R.S., Phillipps S.", "title_pub": "A Catalogue of Absorption Lines in QSO Spectra", "first_author": "Ellis R.S.", "ref_biblio": [""], "bibcode": ["1978MNRAS.183..271E"], "keyword_cds": "QSOs ; Spectroscopy", "description": ["The catalog is a collection of spectral data for 128 quasi-stellar", "objects (QSO). The data have been assembled from the catalogs of de", "Veny et al. (1971), Smith-Haenni (1977), and Burbidge et al. (1977).", "To ensure every observation is recorded and to search for new or", "omitted results, the entire literature up to 1977 September was", "scanned. The catalog distributed by the ADC is an updated version of", "the original catalog published as microfiche in Ellis and Phillipps", "(1978). The catalog includes object names, positions and", "identifications, V, B-V, U-B, emission redshifts, observation", "references, analyses, and line lists.", "The lists of observed spectral lines come from many observers and", "instruments. References to observations and to analyses are included", "for each QSO, as are alternate names for the QSO, coordinates, and", "magnitude. Each observed line has a reference to the observer, and", "most have the possible line identifications and redshifts listed as", "well. See the original paper for a discussion of the purpose behind", "the compilation of the catalog, in particular, for a discussion of its", "use as a base of raw spectral data that is not tied to any particular", "redshift system."], "records": ["108 records"], "doi_pub": ["10.1093/mnras/183.2.271"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "id.dat", "desc": "Identification of each object ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "Ident", "desc": "*Object identifiers "}, {"name": "LineRec", "desc": "*Number of line data records "}]}, {"name": "coord.dat", "desc": "Coordinates ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "RAtag", "desc": "Right Ascension tag, \"RA=\" "}, {"name": "RAh", "desc": "RA hours (B1950) "}, {"name": "RAm", "desc": "RA minutes "}, {"name": "RAs", "desc": "RA seconds "}, {"name": "Dectag", "desc": "Declination tag, \"DEC=\" "}, {"name": "DE-", "desc": "Dec sign "}, {"name": "DEd", "desc": "Dec degrees (B1950) "}, {"name": "DEm", "desc": "Dec arc minutes "}, {"name": "DEs", "desc": "Dec arc seconds "}, {"name": "IDtag", "desc": "*ID reference tag "}, {"name": "IDref", "desc": "*ID reference "}]}, {"name": "mag.dat", "desc": "Magnitudes ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "Magtag", "desc": "Magnitude tag, \"V=\" "}, {"name": "Vmag", "desc": "*Visual magnitude "}, {"name": "Varflag", "desc": "*Variability flag "}, {"name": "B-Vtag", "desc": "B-V color tag, \"B-V=\" "}, {"name": "B-V", "desc": "*B-V color "}, {"name": "U-Btab", "desc": "U-B color tag, \"U-B=\" "}, {"name": "U-B", "desc": "*U-B color "}, {"name": "Ztag", "desc": "Emission redshift tag, \"ZEM=\" "}, {"name": "Z", "desc": "*Emission redshift "}, {"name": "q_Z", "desc": "*Redshift quality flag "}, {"name": "Lflag", "desc": "Left parenthesis "}, {"name": "Nline", "desc": "*? Number of emission lines "}, {"name": "Rflag", "desc": "Right parenthesis "}]}, {"name": "lines.dat", "desc": "line data ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "Lstflag", "desc": "*Last line flag "}, {"name": "ObsWave", "desc": "*? Observed wavelength "}, {"name": "Gsymbol", "desc": "*Group symbols "}, {"name": "RefNum", "desc": "*? Observer reference number "}, {"name": "S-EW", "desc": "*Strength or equivalent width "}, {"name": "Ion", "desc": "*Identified ion "}, {"name": "RestWave", "desc": "? Ion rest wavelength "}, {"name": "Z", "desc": "*? Actual redshift "}, {"name": "SysNum", "desc": "*System numbers "}]}, {"name": "note.dat", "desc": "notes ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "note", "desc": "General notes for each object "}]}, {"name": "obs.dat", "desc": "note of observations and analyses ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VII_230"}} {"id": "VII/230", "title_cds": "CfA Redshift Survey, Version Feb. 2000", "title_create": "Huchra+ 2000", "year": "2000", "author": "Huchra J.P., et al.", "title_pub": "The CfA Redshift Survey, Version Feb. 2000", "first_author": "Huchra J.P.", "ref_biblio": [""], "keyword_cds": "Redshifts", "description": ["The CfA Redshift Survey was started in 1977 by Marc Davis, John", "Huchra, Dave Latham and John Tonry. The First CfA Survey, completed in", "1982, (Huchra, Davis, Latham and Tonry, 1983, ApJS 52, 89) had as its", "goal the measurement of radial velocities for all galaxies brighter", "than 14.5 and at high galactic latitude in the merged catalogs of", "Zwicky and Nilson (the UGC). This survey produce the first large area", "and moderately deep maps of large scale structure in the nearby", "universe, as well as the first crude but truly quantitative", "measurements of the 3-D clustering properties of galaxies. The second", "CfA survey (CfA2) was started by John Huchra and Margaret Geller in", "the winter of 1984/5. Between 1985 and 1995, we and our students and", "co-workers measured relative distances via redshifts for about 18,000", "bright galaxies in the northern sky."], "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["zCat", "CfA"], "type": ["CCC"], "records": ["records"], "data": "", "date_update": "05-Oct-2002"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VII_268"}} {"id": "VII/268", "title_cds": "South-Equatorial Galaxy Catalogue", "title_create": "Corwin+ 2010", "year": "2010", "author": "Corwin H.G. Jr, Skiff B.A.", "title_pub": "South-Equatorial Galaxy Catalogue, Version 1.4.3", "first_author": "Corwin H.G. Jr", "ref_biblio": [""], "bibcode": ["2010yCat.7268....0C"], "see_also": ["VII/116 : Southern Galaxy Catalogue (SGC) (Corwin+ 1985)"], "keyword_cds": "Galaxies, optical ; Positional data ; Morphology ;", "description": ["This version (1.4.3) of the South-Equatorial Galaxy Catalogue (SEGC)", "contains accurate positions, diameters, position angles, and de", "Vaucouleurs revised Hubble-Sandage (VRHS) types for 3333 single or", "multiple galaxies in the south-equatorial declination zones between", "+03 and -21{deg}. The data were gleaned from POSS1 103a-O copy plates,", "then checked against the UKST IIIa-J portion of the DSS. The corrected", "position angles and VRHS types are published here in full for the", "first time. Notes on the individual objects are also available. SEGC", "provides a finding list for galaxies generally larger than about 1.8", "arcmin at the 25.0 B-mag.arcsec^-2^ in the south-equatorial zone."], "alias": ["SEGC-1.4.3", "SEGC"], "type": ["CCC"], "records": ["records"], "data": "", "date_update": "05-Oct-2012", "tables": [{"name": "segc143.dat", "desc": " ", "columns": [{"name": "RAh", "desc": "Right Ascension B1950 (hours) "}, {"name": "RAm", "desc": "Right Ascension B1950 (minutes) "}, {"name": "RAs", "desc": "Right Ascension B1950 (seconds) "}, {"name": "DE-", "desc": "Declination B1950 (sign) "}, {"name": "DEd", "desc": "Declination B1950 (degrees) "}, {"name": "DEm", "desc": "Declination B1950 (minutes) "}, {"name": "DEs", "desc": "[0/60] Declination B1950 (seconds) "}, {"name": "Np", "desc": "number of positions used "}, {"name": "Src.pos", "desc": "Position sources "}, {"name": "Names", "desc": "Names of this galaxy found in the literature "}, {"name": "NEDname", "desc": "NED-friendly name "}, {"name": "MType", "desc": "Morphological type on the deVaucouleurs revied Hubble-Sandage system "}, {"name": "n_logD", "desc": "[[] '[' if the diameter applies to more than 1 galaxy "}, {"name": "logD", "desc": "log of major diameter expressed in 0.1arcmin "}, {"name": "u_logD", "desc": "[:? ] Uncertainty flags on logD "}, {"name": "e_logD", "desc": "? standard deviation in logD when 2 or more values were averaged. "}, {"name": "logR", "desc": "Ratio max/min axis "}, {"name": "u_logR", "desc": "[:? ] Uncertainty flags on logR "}, {"name": "e_logR", "desc": "? standard deviation in logR "}, {"name": "---", "desc": "[]] "}, {"name": "Nd", "desc": "Number of diameters and axis rations used "}, {"name": "n_PA", "desc": "[[] '[' if the position angle applies to more than 1 galaxy "}, {"name": "PA", "desc": "?=--- Position angle of major axis "}, {"name": "u_PA", "desc": "[:? ] Uncertainty flags on PA "}, {"name": "---", "desc": "[]] "}, {"name": "e_PA", "desc": "? standard deviation in PA "}, {"name": "Na", "desc": "Number of position angles "}]}, {"name": "notes.dat", "desc": "Notes ", "columns": []}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VII_90A"}} {"id": "VII/90A", "title_cds": "Merged Catalogue of Galaxies", "title_create": "Kogoshvili 1983-1986", "year": "1986", "author": "Kogoshvili N.G.", "title_pub": "Merged Catalogue of Galaxies", "first_author": "Kogoshvili N.G.", "ref_biblio": ["", "", ""], "bibcode": ["1983BICDS..25...63K"], "keyword_cds": "Galaxy catalogs;", "description": ["The catalog has been compiled at Abastumani Astrophysical Observatory.", "It comprises, on the whole, nearly all galaxies in the region between", "+90 degrees and -33 degrees declination and brighter than mag 15.1 as", "well as some fainter ones. The Morphological Catalogue of Galaxies has", "been used as a main source of data for this catalog. The number of", "galaxies in the catalog is 31917. The catalog is kept up to date, and", "this version adds the data published from 1973-1983. The catalog", "includes designations, equatorial coordinates, magnitudes and colors,", "angular diameters, surface brightness, position angles, detailed", "structure descriptions, classifications on several different systems,", "rotation curve data, supernova dates and counts, HII regions, radio", "flux densities, multiple-system membership, and interaction details in", "the first file. The second file lists the full forms of the references", "cited by code numbers in the first file. Also included are brief", "descriptions of the content of second file lists the full forms of the", "references cited by code numbers in the first file. Also included are", "brief descriptions of the content of each reference."], "records": ["31917 galaxies"], "data": "", "date_update": "04-Nov-1999", "tables": [{"name": "adc.doc", "desc": "Documentation from ADC by Anne C. Raugh ", "columns": []}, {"name": "catalog", "desc": "The Merged Catalogue of Galaxies ", "columns": [{"name": "MCG", "desc": "Morphological Catalog of Galaxies (MCG) number "}, {"name": "Name", "desc": "NGC, IC, or Anonymous RC1 number "}, {"name": "Info", "desc": "[*] '*' if additional information is given (It is not clear what \"additional information\" this flag alludes to)"}, {"name": "RAh", "desc": "Hours RA, epoch 1950.0 "}, {"name": "RAm", "desc": "Minutes RA, epoch 1950.0 "}, {"name": "RAs", "desc": "Seconds RA, epoch 1950.0 "}, {"name": "DE-", "desc": "Degrees Dec, epoch 1950.0 "}, {"name": "DEd", "desc": "Degrees Dec, epoch 1950.0 "}, {"name": "DEm", "desc": "Minutes Dec, epoch 1950.0 "}, {"name": "Mag", "desc": "? Integrated magnitude "}, {"name": "q_Mag", "desc": "[0/3]? Magnitude accuracy code (1) "}, {"name": "r_Mag", "desc": "[1/253]? Magnitude reference code (2) "}, {"name": "n_Mag", "desc": "[Z] 'Z' if Mag is from 2 or more galaxies "}, {"name": "MagCnt", "desc": "? Number of galaxies contributing to Mag "}, {"name": "MajDiamIn", "desc": "? Major angular diameter, inner part "}, {"name": "MinDiamIn", "desc": "? Minor angular diameter, inner part "}, {"name": "SurfBrIn", "desc": "[1/6]? Surface brightness of inner part of galaxy as in MCG (3)"}, {"name": "MajDiamWh", "desc": "? Major angular diameter, whole galaxy "}, {"name": "MinDiamWh", "desc": "? Minor angular diameter, whole galaxy "}, {"name": "l_MajDiamWh", "desc": "[>] '>' if [Min,Maj]DiamWh are lower limits "}, {"name": "SurfBr1", "desc": "[1/6]? Surface brightness, first outer region (3)"}, {"name": "SurfBr2", "desc": "[1/6]? Surface Brightness, second outer region (3)"}, {"name": "Incl", "desc": "[1/5]? Estimated inclination to the line of sight as in MCG (4)"}, {"name": "MajDiamB", "desc": "? Major angular diameter from POSS blue print "}, {"name": "MinDiamB", "desc": "? Minor angular diameter from POSS blue print "}, {"name": "MajDiamR", "desc": "? Major angular diameter from POSS red print "}, {"name": "MinDiamR", "desc": "? Minor angular diameter from POSS red print "}, {"name": "POSS_Unc", "desc": "[1/3]? Code for uncertainty in POSS angular diameters (5)"}, {"name": "PosAng", "desc": "? Position angle from UGC (ref.10) "}, {"name": "u_PosAng", "desc": "[1/3]? Code for uncertainty in PosAng (6) "}, {"name": "GenApp", "desc": "[EPLF] General appearance code from MCG "}, {"name": "GenDet1", "desc": "Structural detail 1 (see adc.doc) "}, {"name": "GenDet2", "desc": "Structural detail 2 (see adc.doc) "}, {"name": "fGal/Sup", "desc": "Faint galaxy or superimposed star description (see adc.doc) (7)"}, {"name": "GalStar", "desc": "Structure of the faint galaxy, or inclination, or position of the star (byte 121='*') (see adc.doc)"}, {"name": "NucCnt", "desc": "? Number of nuclei seen in contact "}, {"name": "InnDet", "desc": "Inner region detail (see adc.doc) "}, {"name": "NucInn1", "desc": "Nuclear inner region detail 1 (see adc.doc) "}, {"name": "NucInn2", "desc": "Nuclear inner region detail 2 (see adc.doc) "}, {"name": "Out1Sep", "desc": "Outer region 1 separation symbol (see adc.doc) "}, {"name": "Out1Ndet", "desc": "Outer region 1 number of structural details "}, {"name": "Out1Gen", "desc": "Outer region 1 general description "}, {"name": "Out1Det", "desc": "Outer region 1 structural details "}, {"name": "Out1Unc", "desc": "Outer region 1 structure uncertainty flag "}, {"name": "Out2Sep", "desc": "Outer region 2 separation symbol (see adc.doc) "}, {"name": "Out2Ndet", "desc": "Outer region 2 number of structural details "}, {"name": "Out2Gen", "desc": "Outer region 2 general description "}, {"name": "Out2Det", "desc": "Outer region 2 structural details "}, {"name": "Out2Unc", "desc": "Outer region 2 structure uncertainty flag "}, {"name": "Out3Sep", "desc": "Outer region 3 separation symbol (see adc.doc) "}, {"name": "Out3Ndet", "desc": "Outer region 3 number of structural details "}, {"name": "Out3Gen", "desc": "Outer region 3 general description "}, {"name": "Out3Det", "desc": "Outer region 3 structural details "}, {"name": "Out3Unc", "desc": "Outer region 3 structure uncertainty flag "}, {"name": "Out4Sep", "desc": "Outer region 4 separation symbol (see adc.doc) "}, {"name": "Out4Ndet", "desc": "Outer region 4 number of structural details "}, {"name": "Out4Gen", "desc": "Outer region 4 general description "}, {"name": "Out4Det", "desc": "Outer region 4 structural details "}, {"name": "Out4Unc", "desc": "Outer region 4 structure uncertainty flag "}, {"name": "Out5Sep", "desc": "Outer region 5 separation symbol (see adc.doc) "}, {"name": "Out5Ndet", "desc": "Outer region 5 number of structural details "}, {"name": "Out5Gen", "desc": "Outer region 5 general description "}, {"name": "Out5Det", "desc": "Outer region 5 structural details "}, {"name": "Out5Unc", "desc": "Outer region 5 structure uncertainty flag "}, {"name": "r_Hubble", "desc": "[RPU] Source of revised Hubble class (8) "}, {"name": "HubbleRing", "desc": "Revised Hubble class, outer ring "}, {"name": "Hubble", "desc": "Revised Hubble classification "}, {"name": "HubblePec", "desc": "Revised Hubble class, peculiarities "}, {"name": "Morgan", "desc": "Morgan classification type "}, {"name": "MorganSpc", "desc": "Morgan classification spectral class "}, {"name": "MorganPec", "desc": "Morgan classification peculiarities "}, {"name": "Class", "desc": "Hubble or van den Bergh classification (9) "}, {"name": "r_Class", "desc": "[RU] Source of Hubble or van den Bergh class. "}, {"name": "RV", "desc": "? Heliocentric radial velocity "}, {"name": "r_RV", "desc": "[1/253]? Reference for RV "}, {"name": "RVo", "desc": "? Radial velocity corrected for solar motion "}, {"name": "r_RVo", "desc": "[1/253]? Reference for RVo "}, {"name": "RotVel", "desc": "? Rotational velocity "}, {"name": "R.H", "desc": "? Distance from center of the bending point in the rotational velocity curve; units are arcmin(Ref.11) or kpc(Ref.12)"}, {"name": "l_R.H", "desc": "'>' if R.H is a lower limit "}, {"name": "r_RotVel", "desc": "[1/253]? Reference for RotVel and R.H "}, {"name": "SN_Yr1", "desc": "? Year of first observed supernova "}, {"name": "SN_Yr2", "desc": "? Year of second observed supernova "}, {"name": "SN_Cnt", "desc": "? Number of observed supernovae (Ref.49) "}, {"name": "HII", "desc": "? Number of H II regions "}, {"name": "r_HII", "desc": "[1/253]? H II region reference code "}, {"name": "U-B", "desc": "? Integrated U-B "}, {"name": "r_U-B", "desc": "[1/253]? Integrated U-B reference code "}, {"name": "B-V", "desc": "? Integrated B-V "}, {"name": "r_B-V", "desc": "[1/253]? Integrated B-V reference code "}, {"name": "(U-B)(0)", "desc": "? Integrated face-on U-B, from RC1 or RC2 "}, {"name": "(B-V)(0)", "desc": "? Integrated face-on (B-V)o, from RC1 or RC2 "}, {"name": "Spectrum", "desc": "Integral spectrum "}, {"name": "Flux178", "desc": "? Flux density at 178 MHz "}, {"name": "r_Flux178", "desc": "[1/253]? Reference of Flux178 "}, {"name": "Flux780", "desc": "? Flux density at 780 MHz "}, {"name": "r_Flux780", "desc": "[1/253]? Reference of Flux780 "}, {"name": "Flux1400", "desc": "? Flux density at 1400 MHz (21cm) "}, {"name": "r_Flux1400", "desc": "[1/253]? Reference of Flux1400 "}, {"name": "Flux2700", "desc": "? Flux density at 2700 MHz (11cm) "}, {"name": "r_Flux2700", "desc": "[1/253]? Reference of Flux2700 "}, {"name": "Flux5000", "desc": "? Flux density at 5000 MHz (6cm) "}, {"name": "r_Flux5000", "desc": "[1/253]? Reference of Flux5000 "}, {"name": "CGCG", "desc": "? CGCG (Ref.2) number of nearby cluster "}, {"name": "inCCG", "desc": "[1] '1' if galaxy in CCG (Ref.55) "}, {"name": "inMKN", "desc": "[1] '1' if galaxy in Markarian's (ref.56) "}, {"name": "inIG", "desc": "[1] '1' if galaxy in Isolated Gal. (ref.58) "}, {"name": "inIPG", "desc": "[1] '1' if galaxy in Isolated Pairs (ref.57) "}, {"name": "ByuType", "desc": "Byurakan classification of nucleus "}, {"name": "EmLines", "desc": "[1] '1' if emission lines in spectrum (ref.54) "}, {"name": "CompCode", "desc": "[1/4]? Companion code (10) "}, {"name": "MultCode", "desc": "Multiple-galaxy membership code (see adc.doc) "}, {"name": "CompMCG", "desc": "? MCG number of companion galaxy "}, {"name": "Isolation", "desc": "? Degree of isolation (see adc.doc) "}, {"name": "InterCnt", "desc": "? Number of members observed to be interacting "}, {"name": "u_InterType", "desc": "[BQ] 'B' if interaction is evident, 'Q' if interaction is suspected (11)"}, {"name": "InterType", "desc": "? Interaction type (11) "}, {"name": "Distortion", "desc": "? Type of galaxy distortion (see adc.doc) "}, {"name": "Sep", "desc": "? Angular separation "}, {"name": "FCompCnt", "desc": "? Number of faint components "}, {"name": "FCompCode", "desc": "[1/4]? Code for type of faint component (12) "}, {"name": "FCompMCG", "desc": "? Faint component MCG number or magnitude (13) "}, {"name": "CompDist", "desc": "? Angular distance to the nearest companion "}]}, {"name": "refs", "desc": "References ", "columns": [{"name": "RefNum", "desc": "[1/253]? Reference code number, blank if a continuation of the previous record."}, {"name": "Text", "desc": "Text of reference "}, {"name": "Subject", "desc": "Subject matter of reference "}]}]} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VIII_93"}} {"id": "VIII/93", "title_cds": "The VLA Low-frequency Sky Survey at 74MHz", "title_create": "Cohen+ 2007-2013", "year": "2013", "author": "Cohen A.S., Lane W.M., Cotton W.D., Kassim N.E., Lazio T.J.W., Perley R.A., Condon J.J., Erickson W.C. < Astron. J. 134, 1245 (2007) >", "title_pub": "The VLA Low-frequency Sky Survey, Version 2013", "first_author": "Cohen A.S.", "ref_biblio": [""], "bibcode": ["2007AJ....134.1245C", "2013yCat.8093....0C"], "keyword_cds": "Radio continuum ; Radio sources ; Surveys", "keyword_pub": "Atmospheric Effects - Catalogs - Radio Continuum: General - Surveys", "abstract": ["The VLA Low-Frequency Sky Survey (VLSS) is a 74MHz (4m) continuum", "survey covering the entire sky north of -30{deg} declination. Using", "the VLA in B- and BnA-configurations, we will map the entire survey", "region at a resolution of 80\" and with an average rms noise of 0.1", "Jy/beam. For a detailed description of the survey and its scientific", "motivations, please see the original proposal to the NRAO skeptical", "review committee.", "The VLSS is being made as a service to the astronomical community,", "and the principal data products are being released to the public as", "soon as they are produced and verified. Details and access to the", "images can be found at http://lwa.nrl.navy.mil/VLSS/"], "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["VLSS", "4MASS"], "type": ["OC"], "records": ["records"], "doi_pub": ["10.1086/520719"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2022-10-24_11h48m08.558482","_type":"_doc","_id":"VIII_110"}} {"id": "VIII/110", "title_cds": "GLEAM-X Data Release 1", "title_create": "Hurley-Walker+, 2022", "year": "2022", "author": "Hurley-Walker N., Galvin T.J., Duchesne S.W., Zhang X., Morgan J., Hancock P.J., An T., Franzen T.M.O., Heald G., Ross K., Vernstrom T., Anderson G.E., Gaensler B.M., Johnston-Hollitt M., Kaplan D.L., Riseley C.J., Tingay S.J., Walker M.", "title_pub": "GaLactic and Extragalactic All-sky Murchison Widefield Array survey eXtended (GLEAM-X). I: Survey Description and Initial Data Release.", "first_author": "Hurley-Walker N.", "ref_biblio": [""], "bibcode": ["2022yCat.8110....0H"], "see_also": ["VIII/100 : GaLactic and Extragalactic All-sky MWA survey", "VIII/102 : GLEAM II. Galactic plane (Hurley-Walker+, 2019)", "VIII/105 : The GLEAM 4-Jy (G4Jy) Sample (White+, 2020)", "VIII/107 : GLEAM sources ionospheric position shifts", "VIII/109 : GLEAM III. South Galactic Pole (Franzen+, 2021)", "J/other/PASA/38.41 : GLEAM 200MHz local radio luminosity function"], "keyword_cds": "Surveys ; Galaxy catalogs ; Radio continuum ; Radio sources", "keyword_pub": "techniques: interferometric - galaxies: general - radio continuum: surveys", "abstract": ["We describe a new low-frequency wideband radio survey of the southern", "sky. Observations covering 72-231MHz and Declinations south of", "+30{deg} have been performed with the Murchison Widefield Array", "\"extended\" Phase II configuration over 2018-2020 and will be processed", "to form data products including continuum and polarisation images and", "mosaics, multi-frequency catalogues, transient search data, and", "ionospheric measurements. From a pilot field described in this work,", "we publish an initial data release covering 1,447 sq. deg over", "4h