Conversion of standardized ReadMe file for
file /./ftp/cats/VII/283 into FORTRAN code for loading all data files into arrays.
Note that special values are assigned to unknown or unspecified
numbers (also called NULL numbers);
when necessary, the coordinate components making up the right ascension
and declination are converted into floating-point numbers
representing these angles in degrees.
program load_ReadMe
C=============================================================================
C F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2026-Oct-16
C=============================================================================
* This code was generated from the ReadMe file documenting a catalogue
* according to the "Standard for Documentation of Astronomical Catalogues"
* currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
* (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
* Please report problems or questions to
C=============================================================================
implicit none
* Unspecified or NULL values, generally corresponding to blank columns,
* are assigned one of the following special values:
* rNULL__ for unknown or NULL floating-point values
* iNULL__ for unknown or NULL integer values
real*4 rNULL__
integer*4 iNULL__
parameter (rNULL__=--2147483648.) ! NULL real number
parameter (iNULL__=(-2147483647-1)) ! NULL int number
integer idig ! testing NULL number
C=============================================================================
Cat. VII/283 The Million Quasars (Milliquas) catalog (6.3) (Flesch, 2019)
*================================================================================
*The Million Quasars (MILLIQUAS) catalogue, version 6.3.
* Flesch E.W.
* <Pub. Astron. Soc. Australia 32, 10 (2015)>
* =2015PASA...32...10F
* =2019yCat.7283....0F
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'catalog.dat' ! The Milliquas catalogue, V6.3 (16 June 2019)
integer*4 nr__
parameter (nr__=1986800) ! Number of records
character*192 ar__ ! Full-size record
C J2000 position composed of: RAdeg DEdeg
real*8 RAdeg (nr__) ! (deg) Right ascension J2000 (degrees)(1)
real*8 DEdeg (nr__) ! (deg) Declination J2000 (degrees)(1)
character*25 Name (nr__) ! ID from the literature, or J2000 (2)
character*4 Cl_Ass (nr__) ! [ABKQqNGL 2RX] Classification of object,
* and associations (3)
real*4 Rmag (nr__) ! (mag) ?=0 Red optical magnitude (4)
real*4 Bmag (nr__) ! (mag) ?=0 Blue optical magnitude (4)
character*3 Comment (nr__) ! Comment on optical object (5)
character*1 R (nr__) ! Red optical PSF class (6)
character*1 B (nr__) ! Blue optical PSF class (6)
real*4 z (nr__) ! ? Redshift from the literature or estimated (7)
character*6 rName (nr__) ! Citation for name (8)
character*6 rz (nr__) ! Citation for redshift (8)
integer*4 Qpct (nr__) ! (pct) ? Probability that this object is a QSO (9)
character*22 XName (nr__) ! X-ray ID, if any (10)
character*22 RName_1 (nr__) ! Radio ID, if any (10)
character*22 Lobe1 (nr__) ! Radio lobe ID or extra R/X ID, if any (10)
character*22 Lobe2 (nr__) ! Radio lobe ID or extra X-ray ID, if any (10)
*Note (1): These are to 7 decimals which suits Gaia-DR2 astrometry.
*Note (2): Nameless radio/X-ray associated objects here display the J2000
* position in HHMMSS.SS+DDMMSS.S for the convenience of the user. If needing
* a name for it, just preface the J2000 with "MQ", e.g., MQ J000001.5-251706.
*Note (3): Legend of class/type:
* Q = QSO, type-I broad-line core-dominated, 595972 of these.
* A = AGN, type-I Seyferts/host-dominated, 27032 of these.
* B = BL Lac object, 1724 of these.
* q = photometric quasar candidate from SDSS or WISE, 1266417 of these.
* ~1K are SDSS/LAMOST pipeline QSOs w/o subclass, with R/X associations.
* L = lensed quasar extra image, only 61 of these in this optical data.
* K = NLQSO, type-II narrow-line core-dominated, 5424 of these.
* N = NLAGN, type-II Seyferts/host-dominated, 30625 of these. Includes an
* unknown number of legacy NELGs/ELGs/LINERs for completeness.
* G = galaxy with double radio lobes (so calculated), 3581 of these.
* R = radio association displayed.
* X = X-ray association displayed.
* 2 = double radio lobes displayed (declared by data-driven algorithm).
*Note (4): Optical data is from the APM (http://www.ast.cam.ac.uk/~mike/apmcat),
* USNO-A & USNO-B
* (https://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/usno-b1.0),
* and the SDSS (http://sdss.org).
* APM/USNO-A magnitudes have been recalibrated from the original values as
* documented in QORG (2004,A&A,427,387), so such USNO-A magnitudes are often
* used in preference to USNO-B. APM galaxies < mag 17 are usually shown
* too bright due to PSF modelling. Integer magnitudes (e.g., 22.00) are
* estimates if both bands are integer or one band empty. Note: many SDSS
* magnitudes are "extinction-corrected" ~0.3 mag brighter than observed.
*Note (5): Legend as follows:
* p = optical magnitudes are POSS-I O (violet 4050A) and E (red 6400A).
* These are preferred because O is well-offset from E, and those plates
* were always taken on the same night, thus the red-blue color is
* correct even for variable objects.
* j = optical magnitudes are SERC J (Bj 4850A) and R (red 6400A) from the
* POSS-II or UKST surveys. Red-blue color is less reliable because the
* red & blue plates were taken in different epochs, i.e., years apart.
* b = blue magnitude is Vega 4400A (Johnson), red is 6400A (Cousins).
* g = blue magnitude is SDSS green 4900A, red is SDSS r 6200A.
* u = blue magnitude is SDSS ultraviolet 3850A.
* v = red magnitude is visual, i.e., white, 5500A midpoint.
* i = red magnitude is infrared 7500A.
* z = red magnitude is infrared z 8600A.
* r = red magnitude is r 6200A.
* (blank) = red alone is 6400A (Cousins), else they are r 6200A & g 4900A.
* G = Gaia-DR2 astrometry shown, precessed to J2000 by CDS. If 'G' is alone
* then the magnitudes are Gaia RP & BP, or Gaia G if red band only.
* + = variability nominally detected in both red/blue over multi-epoch data.
* m = proper motion nominally detected, from USNO-B.
* a = object is host-dominated with faint nuclear activity, such as an SDSS
* pipeline galaxy with an AGN subclass or AGN-classed elsewhere, see its
* citation. Milliquas class is 'A' if BROADLINE, else 'N'. (see note 2)
*Note (6): The APM, USNO-B, and SDSS provide PSF class, albeit using different
* criteria. These are shown here as follows:
* - = point source / stellar PSF (APM notation: -1, here truncated)
* 1 = fuzzy / galaxy shape (APM notation: 1 and some 2)
* n = no PSF available, whether borderline or too faint to tell, etc.
* x = not seen in this band (fainter than plate depth, or confused, etc.)
*Note (7): Spectroscopic/grism redshifts are required for objects classified as
* Q/A/K/N/L; photometric redshifts for objects classified as 'q' are rounded
* here to 0.1 z, except if pipeline redshifts are available from SDSS/LAMOST.
* The XDQSO catalog does not provide photometric redshifts, so those are
* provided either by NBCKDE or by this catalog using the four-color method
* detailed in Appendix 2 of my HMQ paper (2015PASA...32...10F,PASA,32,10).
* AllWISE photometric redshifts are similarly calculated using the four colors
* B-R, R-W1, W1-W2 and W2-W3, and are displayed where calculated as 50%+
* (usually 80%+) likely to be true within 0.5z of the displayed redshift value.
*Note (8): Legend (with counts of name and redshift) and references:
* (for numerical reference code, see refs.dat file):
* 2dF (327,233) : 2dF galaxy survey, Colless M. et al.,
* 2001MNRAS.328.1039C, Cat. VII/250
* 2MRS (10,34) : 2MASS, Huchra J.P. et al.,
* http://tdc-www.harvard.edu/2mrs
* 2QZ (27520,24161) : Croom S.M. et al., 2004MNRAS.349.1397C, Cat. VII/241
* 2SLAQ (10365,8709) : Croom S.M. et al., 2009, Cat. J/MNRAS/392/19
* 3FGL (16,16) : Fermi cleanups, Paiano S. et al., 2017ApJ...851..135P
* 3FGL2 (22,22) : Fermi cleanups II, Paiano S. et al.,
* 2019ApJ...871..162P
* 3XLSS (25,25) : The XXL Survey, Pierre M. et al., 2016A&A...592A...1P,
* Cat, IX/49
* 4LAC (366,199) : Fermi AGN v4 + LL, Fermi-LAT collab.,
* 2019,arXiv:1905.10771
* 6dF (300,277) : 6dF galaxy survey, Jones D.H. et al.,
* 2009MNRAS.399..683J, Cat. VII/259
* AAOz (1491,1498) : AAOmega XXL-South: Lidman C. et al.,
* 2016PASA...33....1L
* AGES (2046,2046) : AGES survey, Kochanek C.S. et al.,
* 2012, Cat. J/ApJS/200/8
* AGNELL (2,3) : DES lenses, Agnello A. et al., 2015MNRAS.454.1260A
* AGNELA (4,4) : SDSS J1433+6007 4-lens, Agnello A. et al.,
* 2018MNRAS.474.3391A
* AGNEL2 (13,13) : VST-Gaia QSO pairs, Agnello A. et al.,
* 2018MNRAS.475.2086A
* AKARI (1,1) : overlooked luminous quasar, Aoki K. et al.,
* 2011PASJ...63S.457A
* ALMA (4,4) : ALMA hi-z, Roberto Decarli R. et al.,
* 2018ApJ...854...97D
* ANGUIT (1,1) : COSMOS lens, Anguita T. et al., 2009A&A...507...35A
* ATel (5,5) : Astronomers Telegraph posts,
* http://www.astronomerstelegram.org
* ATLAS (229,269) : Mao M.Y. et al., 2012, Cat. J/MNRAS/426/3334
* BAHM (24,24) : dust-reddened QSOs, Banerji M. et al.,
* 2015MNRAS.447.3368B
* BASS (16,114) : Swift-BAT AGN, Koss M. et al., 2017, Cat. J/ApJ/850/74
* BERGHE (1,1) : Pan-STARRS lens, Berghea C.T. et al.,
* 2017ApJ...844...90B
* BGGFC (4,4) : COSMOS hi-z, Boutsia K. et al., 2018ApJ...869...20B
* BQLS (17,17) : BOSS QSO lenses & pairs, More A. et al.,
* 2016MNRAS.456.1595M
* BZCAT (5,4) : Blazars catalog, Massaro E. et al.,
* http://www.asdc.asi.it/bzcat
* C-COSM (180,180) : Chandra COSMOS IDs, Marchesi S. et al.,
* 2016ApJ...817...34M
* ChaMP (191,187) : Trichas M. et al., 2012ApJS..200...17T
* DABAST (1,1) : Diaz-Santos T. et al., 2018Sci...362.1034D
* Dart (26,25) : Heavily Obscured QSOs, Hviding R. et al.,
* 2018MNRAS.474.1955H
* DDC2 (14,14) : variable AGN, De Cicco D. et al., 2019,
* arXiv:1905.10374
* DEEP (143,139) : DEEP2, Newman J. et al., 2013ApJS..208....5N;
* deep.ps.uci.edu/DR4
* DES (1,1) : Dark Energy hi-z, Reed S.L. et al.,
* 2015MNRAS.454.3952R
* DESQQ (26,26) : STRIDES lenses, Anguita T. et al.,
* 2018MNRAS.480.5017A
* DESQQ2 (12,12) : STRIDES lenses, Treu T. et al., 2018MNRAS.481.1041T
* DPeake (683,656) : Double-peaked NELGs, Ge J.-Q. et al.,
* 2012, Cat. J/ApJS/201/31
* DR12 (18,23) : Alam S. et al., 2015ApJS..219...12A,
* http://sdss.org/dr12
* DR12Q (129,153) : SDSS-DR12Q, Paris I. et al., 2017A&A...597A..79P,
* Cat. VII/279
* DR14 (42582,45125) : Abolfathi B. et al., 2018ApJS..235...42A pipeline,
* data at
* https://data.sdss.org/sas/dr14/sdss/spectro/redux
* DR14Q (513025,525752) : SDSS-DR14Q, Paris I. et al., 2018A&A...613A..51P
* data at http://data.sdss.org/sas/dr14/eboss/qso/DR14Q
* DR7 (8,145) : SDSS DR7, Abazajian K.N. et al., 2009ApJS..182..543A,
* files at
* http://classic.sdss.org/dr7/products/spectra/getspectra.html
* DR7Q (2089,329) : SDSS Quasar DR7, Schneider D. et al.,
* 2010AJ....139.2360S, Cat. VII/26 data
* http://classic.sdss.org/dr7/products/value_added/qsocat_dr7.html
* DUHIZ (2,2) : DECaLS-UKIRT hi-z, Wang F. et al., 2017ApJ...839...27W
* Dusty (11,11) : Dusty Starbursts, Rodighiero G. et al.,
* 2019ApJ...877...38H
* DUz6 (18,18) : DESI & UKIRT hi-z, Wang F. et al.,
* 2018,arXiv:1810.11926
* eHAQ (82,81) : Extended High AV, Krogager J.-K., 2016ApJ...832...49K
* ELQ-PS (216,215) : ELQS on PS1, Schindler J.-T. et al., 2019,
* arXiv:1905.04069
* ELQS-N (38,38) : ELQS in NGC, Schindler J.-T. et al.,
* 2018ApJ...863..144S
* ELQS-S (126,126) : ELQS in SGC, Schindler J.-T. et al.,
* 2019ApJ...871..258S
* FISCBA (1,1) : HST lens, Fischer/Schade/Barrientos
* 1998ApJ...503L.127F
* GAIA2 (263,263) : Gaia DR2, Gaia Collaboration et al.,
* 2018A&A...616A...1G, Cat. I/345 data as presented by
* SIMBAD, http://simbad.u-strasbg.fr/simbad
* GEIER (1,1) : Geier S.J. et al., 2019,arXiv:1904.01686
* GLDD (1,1) : Lensed QSO data-driven, Ostrovski F. et al.,
* 2017MNRAS.465.4325O
* GLIKMA (29,29) : red WISE QSOs, Glikman E. et al., 2018ApJ...861...37G
* GLRED (1,1) : lensed red QSO, Glikman E. et al., 2018,
* arXiv:1807.05434
* GUTI (1,1) : not a ULX, Gutierrez C.M., 2013A&A...549A..81G
* H-DOGs (16,16) : Herschel DOGs, Riguccini L.A. et al.,
* 2019A&A...625A...9D
* HAQ (2,2) : High AV serendipitous, Heintz K.E. et al.,
* 2016AJ....152...13H
* HAQC (1,1) : High AV in COSMOS, Heintz K.E. et al.,
* 2016A&A...595A..13H
* HEINTZ (1,1) : dusty absorbed QSO, Heintz K.E. et al.,
* 2018A&A...615A..43H
* HIZ7.5 (1,1) : QSO z=7.5, Banados E. et al., 2018Natur.553..473B
* HSTvar (42,42) : variable AGN, Pouliasis E. et al., 2019,
* arXiv:1905.11995
* IGMCP (10,10) : IGM close pairs, Rorai A. et al., 2017Sci...356..418R
* IKEDA (1,1) : Ikeda H. et al., 2017ApJ...846...57I
* IMS (1,1) : IR medium-deep hi-z, Kim Y. et al.,
* 2015ApJ...813...35H
* IMS2 (10,11) : IR medium-deep hi-z, Kim Y. et al.,
* 2019ApJ...870...86K
* KOVACS (1,1) : bright QSO behind Milky Way, Kovacs T. et al.,
* 2019, RNAAS, 3, 3
* LAMDR4 (190,2249) : LAMOST-DR4, pipeline, http://dr4.lamost.org
* LAMQ1 (687,628) : LAMOST QUASAR DR1, Ai Y.L. et al.,
* 2016, Cat. J/AJ/151/24
* LAMQ3 (6773,6663) : LAMOST QUASAR DR3/DR2, Dong X.Y. et al.,
* 2018, Cat. J/AJ/155/189
* LAMQ5 (7998,7997) : LAMOST QUASAR DR5/DR4, Yao S. et al.,
* 2019ApJS..240....6Y
* LEMON (40,40) : 24 Gaia lenses, Lemon C. et al.,
* 2018MNRAS.479.5060L
* LEMON2 (30,30) : 22 Gaia lenses, Lemon/Auger/McMahon,
* 2019MNRAS.483.4242L
* LGGS (11,11) : M31/M33 area, Massey/Neugent/Levesque, 2019,
* arXiv:1904.07898
* LIDMAN (1,1) : SN Host Galaxy redshifts, Lidman C. et al.,
* 2013PASA...30....1L
* LIN (1,1) : DES lens, Lin H. et al., 2017ApJ...838...15L
* LIRAS (169,154) : LoCuSS IR AGNs, Xu, L. et al.,
* 2015, Cat. J/ApJS/219/18
* LOZAGN (32,11009) : Low-redshift AGN, Liu H.-Y. et al., 2019,
* arXiv:1906.05597
* LSSA (2,2) : 2 lenses, Lucey/Schechter/Smith/Anguita,
* 2018MNRAS.476..927L
* LUMIz5 (66,66) : Luminous hi-z, Yang J. et al., 2018,
* arXiv:1810.11927
* M31UV (1,1) : UV flare QSO on M31, Meusinger H. et al.,
* 2010A&A...512A...1M
* MALS-N (70,70) : MEERKAT QSOs, Krogager J.-K. et al.,
* 2018ApJS..235...10K
* MFJC (52,51) : McGreer I.D., Fan X., Jiang L. & Cai Z.,
* 2018, Cat. J/AJ/155/131
* MORX (49324,0) : Million Radio/X-ray Associations, Flesch E.,
* 2016PASA...33...52F, Cat. V/148
* MQ (6639,622652) : MILLIQUAS, original data in this catalog,
* Flesch E., 2019
* NBCKDE (40821,40930) : Richards G.T. et al., 2009, Cat. J/ApJS/180/67
* NBCKv3 (529572,563852): NBCKDE v3, Richards G.T. et al.,
* 2015, Cat. J/ApJS/219/39
* NED (3,3) : NASA/IPAC Extragalactic Database,
* https://ned.ipac.caltech.edu
* OGLE2 (2,2) : OGLE quasars, Kozlowski S. et al., 2018,
* arXiv:1810.08622
* OSTROV (1,1) : lensed, Ostrovski et al., 2019, in preparation
* OVRLAP (5,5) : SDSS overlap hi-z QSOs, Jiang L. et al.,
* 2015AJ....149..188J
* OzDES (664,638) : Dark Energy SN QSOs, Tie S.S. et al.,
* 2017AJ....153..107T
* P352-1 (1,1) : P352-15, Banados E. et al., 2018ApJ...861L..14B
* PETERS (12896,12914) : photo special, Peters C.M. et al.,
* 2015ApJ...811...95P
* PGC (13623,19) : Principal Galaxy Catalog, Paturel G. et al.,
* 2003A&A...412...45P, Cat. VII/237
* PHILLI (1,0) : MERLIN lens, Phillips P.M. et al.,
* 2000MNRAS.319L...7P
* PS1 (63,63) : PAN-STARRS1 hi-z, Banados E. et al.,
* 2016, Cat. J/ApJS/227/11
* PS1hiz (1,1) : Tang, Ji-Jia et al., 2017MNRAS.466.4568T
* PS1MAZ (6,6) : Mazzucchelli C. et al., 2017ApJ...849...91M
* PSO (3,3) : PAN-STARRS z-dropouts, Venemans B.P. et al.,
* 2015ApJ...801L..11V
* QLSV (20,19) : QUEST-La Silla, Sanchez-Saez P. et al.,
* 2019ApJS..242...10S
* QPQ10 (70,70) : Quasar pair DB, Findlay J.R. et al.,
* 2018ApJS..236...44F
* RBS (3,3) : Laporte N. et al., 2017ApJ...851...40L
* Redden (25,25) : Reddened QSOs, Temple M.J. et al., 2019MNRAS.487.2594R
* REQ4 (6,6) : Reionization-Era quasars, Yang J. et al.,
* 2019AJ....157..236Y
* RLQ (4,3) : Tuccillo D./Gonzalez-Serrano J.I./Benn C.R.,
* 2015, Cat. J/MNRAS/449/2818
* RSG (1,1) : Dorn-Wallenstein T.Z. & Levesque E.,
* 2017, IAUS, 329, 376
* S82X (72,77) : Stripe 82 AGN, LaMassa S.M. et al.,
* 2019ApJ...876...50L
* S82XRQ (8,8) : Red Quasars, LaMassa S.M. et al., 2017ApJ...847..100L
* SCULPT (2,3) : Sculptor X-ray, Arnason R. M. et al.,
* 2019MNRAS.485.2259A
* SDLENS (3,3) : SDSS Lenses, Williams P.R. et al.,
* 2018MNRAS.477L..70W
* SDSSHI (6,6) : SDSS hi-z, Jiang L. et al., 2016ApJ...833..222J
* SFM201 (1,1) : Schulze S. et al., 2012A&A...546A..20S
* SHELLQ (33,33) : Subaru hi-z, Matsuoka Y. et al., 2018PASJ...70S..35M
* SHELQS (30,30) : SHELLQS hi-z, Matsuoka Y. et al., 2018ApJS..237....5M
* SHELz7 (1,1) : SHELLQS z=7, Matsuoka Y. et al., 2019ApJ...872L...2M
* SMSSQ (2,2) : SkyMapper hi-z, Zefeng Li Z. et al., 2018,
* arXiv:1805.03429
* SPIN18 (1,1) : KiDS-SQuaD lens, Spiniello C. et al.,
* 2018MNRAS.480.1163S
* SPIN19 (2,2) : 2 lensed quasars, Spiniello C. et al.,
* 2019MNRAS.485.5086S
* SQLS (60,52) : SDSS DR7 QSO Lens Search, Inada N. et al.,
* Cat. J/AJ/143/119
* SQUAD (13,13) : UVES DB DR1, Murphy M.T. et al., 2019MNRAS.482.3458M
* SSLENS (3,3) : South sky lenses, Spiniello C. et al.,
* 2019MNRAS.483.3888S
* SUV (21,21) : SDSS-ULAS/VHS QSOs, Yang J. et al.,
* 2017AJ....153..184Y
* SXDF (39,39) : Subaru-XMMDF redshifts, Simpson C. et al.,
* 2012, Cat. J/MNRAS/421/3060
* SXDS (308,307) : Subaru-XMMDF spectra, Akiyama M. et al.,
* 2015PASJ...67...82A
* ULTRA (1,1) : Ultraluminous hi-z, Wu, X.-B. et al.,
* 2015Natur.518..512W
* UVQS (435,503) : UV QSOs, Monroe T.R. et al., 2016, Cat. J/AJ/152/25
* VAHIZ (2,2) : VST ATLAS hi-z, Carnall A.C. et al.,
* 2015MNRAS.451L..16C
* VAHIZ2 (1,1) : bright z>6 QSOs, Chehade B. et al.,
* 2018MNRAS.478.1649C
* VAHIZ3 (1,1) : VST-ATLAS lens, Schechter P.L. et al.,
* 2018, RNAAS, 2b, 21
* VAQL (11,11) : VST-ATLAS quasar systems,Schechter P.L. et al.,
* 2017AJ....153..219S
* VDES (8,8) : VISTA Dark Energy QSOs, Reed S.L. et al.,
* 2017MNRAS.468.4702R
* VDES2 (2,2) : more VHS-DES quasars, Reed S.L. et al.,
* 2019, arXiv:1901.07456
* VIKING (4,4) : VIKING IR, Venemans, G.A. et al., 2015MNRAS.453.2259V
* VIPERS (241,284) : VIPERS PDR-2, Scodeggio M. et al., 2018A&A...609A..84S
* VMC (34,34) : Magellanic IR QSOs, Ivanov V.D. et al.,
* 2016A&A...588A..93I
* WARSAW (3,3) : OGLE lens, Kostrzewa-Rutkowska Z. et al.,
* 2018MNRAS.476..663K
* WERTZ (1,1) : Gaia GraL lens, Wertz O. et al.,
* 2018, arXiv:1810.02624
* WGD (2,2) : DES/Gaia lenses; Agnello A. et al.,
* 2018MNRAS.479.4345A
* WISEA (447228,0) : AllWISE QSO candidates, Secrest N. et al.,
* 2015, Cat. J/ApJS/221/12
* WISEHI (72,70) : Hi-z QSOs from WISE, Wang F. et al.,
* 2016, Cat. J/ApJ/819/24
* WOLF1 (1,1) : most ultraluminous QSO, Wolf C. et al.,
* 2018PASA...35...24W
* XDQSO (235761,0) : SDSS-XDQSO, Bovy J. et al., 2011ApJ...729..141B
* XLSS (306,118) : Stalin C.S. et al., 2010, Cat. J/MNRAS/401/294
* XMM2 (12,12) : 2XMM-Newton cross-search, Combi J.A. et al.,
* 2011Ap&SS.331...53C, Cat. V/138
* XMMSMC (6,6) : SMC quasars, Maitral C. et al., 2019A&A...622A..29M
* XMSS (182,148) : Barcons X. et al., 2007, Cat. J/A+A/476/1191
* XWAS (490,449) : Esquej P. et al., 2013, Cat. J/A+A/557/A123
* YQLF (25,25) : deep CFHT QSOs, Yang J. et al.,
* 2018, Cat. J/AJ/155/110
* z6.51 (1,1) : lensed quasar z=6.51, Fan X. et al.,
* 2019ApJ...870L..11F
* z7.02 (1,1) : lensed quasar z=7.02, Wang F. et al.,
* 2018ApJ...869L...9W
*
* 4-digit numeric citations are indexed in the HMQ (2015,PASA,32,10)
* references list. The citation for the classification (e.g., that the
* object is a quasar) can be from either the name or redshift citation.
*Note (9): For a QSO candidate (type starting with q/R/X/2), this shows the
* percent chance that it is a QSO, based on photometric and/or radio/X-ray
* association analysis. Included candidates are those of 80%+ likelihood
* of being true quasars. For a known QSO (type=Q/A), Bl Lac type (type=B),
* type-II (type=K/N) or active galaxy (type=G), this shows the percent
* chance that the shown radio/X-ray detection(s) is truly associated to it.
*
* Candidates (objects without spectroscopic confirmation) originate from
* three types of sources:
*
* (1) Photometric quasars from the SDSS-based NBCKDE/NBCKDE-v3/XDQSO/Peters
* quasar candidate catalogs. Those catalogs give pQSOs (calculated QSO
* probabilities) for their objects which however are not reported here;
* instead, I have calibrated those pQSOs against SDSS-DR12Q classified
* objects to produce these QSO likelihoods -- see appendix 1 of my HMQ
* paper (Flesch 2015PASA...32...10F) for details of the calibration method.
*
* (2) WISE-sourced candidates (from Secrest et al. 2015ApJS..221...12S,
* Cat. J/ApJS/221/12) are presented by their authors with a bulk pQSO as
* an average figure, with no individual pQSOs given. These I have
* generated by matching WISE candidates to optical objects (within a two
* arcsecond radius) and then binning them into four-color (colors B-R,
* R-W1, W1-W2, and W2-W3) subsets which are then calibrated against
* SDSS-DR12Q classified objects to yield the pQSO for each four-color
* subset.
*
* (3) 56182 radio/X-ray associated optical objects are presented only here in
* Milliquas, with pQSO calculated as described in the QORG paper (Flesch
* & Hardcastle, 2004A&A...427..387F, Cat. J/A+A/427/387), with no redshift
* displayed. However, an additional 349 such objects show pipeline
* redshifts from SDSS-DR14.
*
* 71543 photometric quasars are also radio/X-ray associated, and the
* displayed probability figure combines the calibrated photometric QSO
* likelihood P1 and the radio/X-ray derived QSO likelihood P2 as
* P = 1/(1+((1-P1)*(1-P2))/(P1*P2)). Over all objects, using the probability
* as expected yield, the 1945385 type-I Milliquas objects will yield 1890994
* actual type-I quasars/AGN.
*Note (10): Four columns of Radio/X-ray detections are presented:
* * 1st column: best X-ray detection (i.e. highest probability association).
* * 2nd column: best core Radio detection.
* * 3rd column: a radio lobe if the description (see note 2) shows a "2",
* otherwise this is an additional radio or X-ray detection.
* * 4th column: a radio lobe if the description (see note 2) shows a "2",
* otherwise this is an additional X-ray detection.
*
* Legend of Radio/X-ray detection prefixes and catalog home pages:
*
* FIRST: VLA FIRST survey, 13Jun05 version, http://sundog.stsci.edu
* NVSS: NRAO VLA sky survey, http://www.cv.nrao.edu/nvss
* SUMSS: Sydney U. Molonglo, http://www.physics.usyd.edu.au/sifa/Main/SUMSS
* MGPS: Molonglo galactic plane survey, same attribution as SUMSS
* ROSAT catalogs home page: www.mpe.mpg.de/xray/wave/rosat/catalogue , for:
* - 1RXH: ROSAT HRI (high resolution imager)
* - 2RXP/2RXF: ROSAT PSPC (position sensitive proportional counter)
* - 1RXS: ROSAT RASS (all-sky survey, both bright & faint)
* 2RXS: 2nd RASS source catalog, Boller Th. et al., 2016,A&A,588,103
* 1WGA: White, Giommi & Angelini, wgacat.gsfc.nasa.gov/wgacat/wgacat.html
* CXO: Chandra Source Catalog v1.1, http://cxc.cfa.harvard.edu/csc
* CXOG: Chandra ACIS source catalog, Wang S. et al., 2016,ApJS,224,40
* CXOX: XAssist Chandra source list, http://xassist.pha.jhu.edu/
* 2XMM/2XMMi: XMM-Newton DR3, http://xmm.esac.esa.int/xsa/versions.shtml
* 3XMM: XMM-Newton DR8, http://www.cosmos.esa.int/web/xmm-newton/xsa
* XMMSL: XMM-Newton Slew Survey Release 2.0, same attribution as 3XMM
* XMMX: XAssist XMM-Newton source list, http://xassist.pha.jhu.edu/
* 1SXPS: Swift X-ray Point Source catalog, http://www.swift.ac.uk/1SXPS
*
* Optical field solutions are calculated from the raw source positions of all
* these catalogs as described in my MORX paper 2016PASA...33...52F.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'refs.dat' ! References (for numerical references)
integer*4 nr__1
parameter (nr__1=2171) ! Number of records
character*162 ar__1 ! Full-size record
integer*4 Ref (nr__1) ! Reference number
integer*4 N1 (nr__1) ! ? Number of this reference for Name
integer*4 N2 (nr__1) ! ? Number of this reference for redshift
character*19 Bibcode (nr__1) ! BibCode
character*31 Aut (nr__1) ! Author's name
character*90 Com (nr__1) ! Comments
C=============================================================================
C Loading file 'catalog.dat' ! The Milliquas catalogue, V6.3 (16 June 2019)
C Format for file interpretation
1 format(
+ F11.7,1X,F11.7,2X,A25,1X,A4,1X,F5.2,1X,F5.2,1X,A3,1X,A1,1X,A1,
+ 1X,F6.3,1X,A6,1X,A6,1X,I3,1X,A22,1X,A22,1X,A22,1X,A22)
C Effective file loading
open(unit=1,status='old',file=
+'catalog.dat')
write(6,*) '....Loading file: catalog.dat'
do i__=1,1986800
read(1,'(A192)')ar__
read(ar__,1)
+ RAdeg(i__),DEdeg(i__),Name(i__),Cl_Ass(i__),Rmag(i__),
+ Bmag(i__),Comment(i__),R(i__),B(i__),z(i__),rName(i__),
+ rz(i__),Qpct(i__),XName(i__),RName_1(i__),Lobe1(i__),
+ Lobe2(i__)
if(ar__(77:82) .EQ. '') z(i__) = rNULL__
if(ar__(98:100) .EQ. '') Qpct(i__) = iNULL__
c ..............Just test output...........
write(6,1)
+ RAdeg(i__),DEdeg(i__),Name(i__),Cl_Ass(i__),Rmag(i__),
+ Bmag(i__),Comment(i__),R(i__),B(i__),z(i__),rName(i__),
+ rz(i__),Qpct(i__),XName(i__),RName_1(i__),Lobe1(i__),
+ Lobe2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'refs.dat' ! References (for numerical references)
C Format for file interpretation
2 format(I4,1X,I6,1X,I6,2X,A19,1X,A31,1X,A90)
C Effective file loading
open(unit=1,status='old',file=
+'refs.dat')
write(6,*) '....Loading file: refs.dat'
do i__=1,2171
read(1,'(A162)')ar__1
read(ar__1,2)
+ Ref(i__),N1(i__),N2(i__),Bibcode(i__),Aut(i__),Com(i__)
if(ar__1(6:11) .EQ. '') N1(i__) = iNULL__
if(ar__1(13:18) .EQ. '') N2(i__) = iNULL__
c ..............Just test output...........
write(6,2)
+ Ref(i__),N1(i__),N2(i__),Bibcode(i__),Aut(i__),Com(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end