J/A+A/564/A79     Proper motions of open clusters from UCAC4      (Dias+, 2014)

Proper motions of the optically visible open clusters based on the UCAC4 catalog. Dias W.S., Monteiro H., Caetano T.C., Lepine J.R.D., Assafin M., Oliveira A.F. <Astron. Astrophys. 564, A79 (2014)> =2014A&A...564A..79D 2014A&A...564A..79D
ADC_Keywords: Clusters, open ; Proper motions ; Radial velocities Keywords: open clusters and associations: general Abstract: We present a catalog of mean proper motions and membership probabilities of individual stars for optically visible open clusters, which have been determined using data from the UCAC4 catalog in a homogeneous way. The mean proper motion of the cluster and the membership probabilities of the stars in the region of each cluster were determined by applying the statistical method in a modified fashion. In this study, we applied a global optimization procedure to fit the observed distribution of proper motions with two overlapping normal bivariate frequency functions, which also take the individual proper motion errors into account. For 724 clusters, this is the first determination of proper motion, and for the whole sample, we present results with a much larger number of identified astrometric member stars. Furthermore, it was possible to estimate the mean radial velocity of 364 clusters (102 unpublished so far) with the stellar membership using published radial velocity catalogs. These results provide an increase of 30% and 19% in the sample of open clusters with a determined mean absolute proper motion and mean radial velocity, respectively. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 153 1805 List of the parameters provided by the statistical method for 1805 open clusters table3.dat 152 724 List of the parameters provided by the statistical method for 724 open clusters with previously unpublished proper motions in Table 2 table4.dat 36 102 Mean radial velocity for 102 open clusters pm/* . 1803 Proper motions and membership, by cluster, based on UCAC4 pm2/* . 2 Proper motions and membership, for IC 1805 and NGC 2437, based on PPMXL -------------------------------------------------------------------------------- See also: B/ocl : Optically visible open clusters and Candidates (Dias+ 2002-2013) III/254 : 2nd Cat. of Radial Velocities with Astrometric Data (Kharchenko+, 2007) III/265 : RAVE catalog A+B (also includes DR1 and DR2) (Siebert+, 2011) I/317 : The PPMXL Catalog (Roeser+ 2010) I/322 : UCAC4 Catalogue (Zacharias+, 2012) http://www.astro.iag.usp.br/ocdb : Open clusters and Galactic structure (Dias+, 2002) Byte-by-byte Description of file: table[23].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- n_Cluster [*] * indicates previously unpublished proper motions (table3) 3- 19 A17 --- Cluster Cluster name 21- 29 F9.5 deg RAdeg Right Ascension J2000 (degrees), at J2000.0 31- 39 F9.5 deg DEdeg Declination J2000 (degrees), at J2000.0 41- 46 F6.2 arcmin Rad Radius (centered in the coordinates of the cluster) used to extract the stars from the UCAC4 Catalogue 48- 53 I6 --- N [11/336543] Number of UCAC4 stars in the field 55- 60 I6 --- Nc [1/246150] Estimated number of cluster members 62- 67 F6.2 mas/yr pmRAc Mean proper motion of the cluster (µ_α.cos(δ), ICRS) 69- 73 F5.2 mas/yr e_pmRAc Error in pmRAc 75- 80 F6.2 mas/yr pmDEc Mean proper motion of the cluster (µδ, ICRS) 82- 86 F5.2 mas/yr e_pmDEc Error in pmDEc 88- 92 F5.2 --- rhoc [-1/1] Correlation coefficient ρc of the cluster stars 94- 98 I5 --- Nf [0/90393] Estimated number of field stars in the cluster 100-105 F6.2 mas/yr pmRAf Mean proper motion of the field stars in µα.cos(δ), ICRS 107-111 F5.2 mas/yr e_pmRAf Standard deviation of pmRAf 113-118 F6.2 mas/yr pmDEf Mean proper motion of the field stars in µδ, ICRS 120-124 F5.2 mas/yr e_pmDEf Standard deviation of pmDEf 126-130 F5.2 --- rhof [-1/1] Correlation coefficient ρf of the field stars 132-152 A21 --- FileName Name of the table in "pm" subdirectory with proper motions and membership 153 A1 --- n_FileName [2] 2 when a second file exists in subdirectory pm2, baased on PPMXL (I/317) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 17 A17 --- Cluster Cluster name 19- 25 F7.2 km/s RV Mean radial velocity of the cluster 27- 31 F5.2 km/s e_RV Error of the mean radial velocity of the cluster 33- 34 I2 --- o_RV Number of stars used for radial velocity 36 I1 --- r_RV Source for individual radial velocity (1) -------------------------------------------------------------------------------- Note (1): Sources as follows: 1 = CRVAD2 - 2nd Cat. of Radial Velocities with Astrometric Data (Kharchenko+, 2007, Cat. III/254) 2 = RAVE catalog - RAVE 3rd data release (Siebert+, 2011, Cat. III/265) -------------------------------------------------------------------------------- Byte-by-byte Description of file: pm/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 17 A17 --- Cluster Cluster name 19- 28 F10.6 arcmin R Distance from source 30- 39 A10 --- UCAC4 UCAC4 recommended identifier (ZZZ-NNNNNN) (1) 41- 51 F11.7 deg RAdeg Mean right ascension (ICRS), Ep=J2000 (2) 53- 55 I3 mas e_RAdeg Mean error of RAdeg at mean epoch 57- 67 F11.7 deg DEdeg Mean declination (ICRS), Ep=J2000 (2) 69- 71 I3 mas e_DEdeg Mean error of DEdeg at mean epoch 73- 76 I4 mas ePos Total mean error on position at Ep=J2000 (3) 78- 84 F7.2 yr EpRA Central epoch for mean RA 86- 92 F7.2 yr EpDE Central epoch for mean Declination 94- 99 F6.3 mag f.mag ? UCAC fit model magnitude (579-642nm) (4) 101-106 F6.3 mag a.mag ? UCAC aperture magnitude (579-642nm) (4) 108-111 F4.2 mag e_a.mag ? Mean error on f.mag and a.mag (5) 113 I1 --- of [0/9] UCAC4 object classification flag (6) 115-116 I2 --- db [0/36] UCAC4 double star flag (7) 118-120 I3 --- Na [0/71] Number of UCAC observations for the star 122-124 I3 --- Nu [0/70] Number of used UCAC observations (8) 126-128 I3 --- Nc [1/38] Number of catalog positions used for pm 130-137 F8.1 mas/yr pmRA ? Proper motion in RA(*cos(Dec)) (9) 139-142 F4.1 mas/yr e_pmRA ? Mean error on pmRA (9) 144-151 F8.1 mas/yr pmDE ? Proper motion in Dec (9) 153-156 F4.1 mas/yr e_pmDE ? Mean error on pmDE (9) -------------------------------------------------------------------------------- 158-166 I9 --- MPOS1 [1/182895114] Unique star ID number (10) 168-177 A10 --- UCAC2 UCAC2 (Cat. I/289) designation (ZZZ-NNNNNN) 179-190 A12 --- Tycho-2 Tycho-2 (Cat. I/259) designation (FFFF-NNNNN-N) -------------------------------------------------------------------------------- 192-201 I10 --- 2Mkey ? 2MASS (Cat. II/246) Unique source identifier 203-208 F6.3 mag Jmag ? 2MASS J magnitude (1.2um) 210-213 F4.2 mag e_Jmag ? Mean error (rounded to 0.01mag) 214 A1 --- --- [:] 215-216 I02 --- q_Jmag [0,58]? J-band quality-confusion flag (11) 218-223 F6.3 mag Hmag ? 2MASS H magnitude (1.6um) 225-228 F4.2 mag e_Hmag ? Mean error (rounded to 0.01mag) 229 A1 --- --- [:] 230-231 I02 --- q_Hmag [0,58]? H-band quality-confusion flag (11) 233-238 F6.3 mag Kmag ? 2MASS Ks magnitude (2.2um) 240-243 F4.2 mag e_Kmag ? Mean error (rounded to 0.01mag) 244 A1 --- --- [:] 245-246 I02 --- q_Kmag [0,58]? K-band quality-confusion flag (11) -------------------------------------------------------------------------------- 248-253 F6.3 mag Bmag ? B magnitude from APASS (12) 255-256 I02 cmag e_Bmag ? Estimated error on Bmag (12) 258 A1 --- f_Bmag [.-] Actual or S/N estimated error (12) 260-265 F6.3 mag Vmag ? V magnitude from APASS (12) 267-268 I02 cmag e_Vmag ? Estimated error on Vmag (12) 270 A1 --- f_Vmag [.-] Actual or S/N estimated error (12) 272-277 F6.3 mag gmag ? g magnitude from APASS (12) 279-280 I02 cmag e_gmag ? Estimated error on gmag (12) 282 A1 --- f_gmag [.-] Actual or S/N estimated error (12) 284-289 F6.3 mag rmag ? r magnitude from APASS (12) 291-292 I02 cmag e_rmag ? Estimated error on rmag (12) 294 A1 --- f_rmag [.-] Actual or S/N estimated error (12) 296-301 F6.3 mag imag ? i magnitude from APASS (12) 303-304 I02 cmag e_imag ? Estimated error on imag (12) 306 A1 --- f_imag [.-] Actual or S/N estimated error (12) -------------------------------------------------------------------------------- 308 I1 --- g [0,3] g-flag from SPM (13) 310 I1 --- c [0,7] c-flag from SPM (14) 312 I1 --- H [0/9] Hipparcos/Tycho flag (15) 314 I1 --- A [0/8] AC2000 flag (16) 316 I1 --- b [0/8] AGK2 Bonn match flag (16) 318 I1 --- h [0/8] AGK2 Hamburg match flag (16) 320 I1 --- Z [0/8] Zone astrographic match flag (16) 322 I1 --- B [0/8] Black Birch match flag (16) 324 I1 --- L [0/8] Lick Astrographic match flag (16) 326 I1 --- N [0/8] NPM Lick match flag (16) 328 I1 --- S [0/8] SPM Lick match flag (16) 330-331 I2 [6arcsec] LEDA LEDA I-band galaxy match (17) 333-334 I2 arcsec 2MX 2MASX K-band match (18) 339-341 I3 % P [0/100] Membership probability -------------------------------------------------------------------------------- Note (1): the UCAC4 number is the recommended identification of UCAC4 stars. It made as "ZZZ-NNNNNNN", where zzz is the zone number (between 1 and 900 from South pole to North pole, each zone being 0.2° wide), and nnnnnn the 6-digit running number in the zone. Note (2): Positions are on the International Celestial Reference System (ICRS) as represented by the Hipparcos / Tycho-2 catalogs. The epoch for the positions of all stars is J2000.0: the weighted mean catalog position was updated using the proper motions. The observational UCAC position is but one of several going into these values and is not given in the UCAC4; thus the original UCAC observation cannot be recovered from these data. Note (3): taking into account the propagation of the proper motion error between the mean epoch and J2000. Note (4): systematic errors are expected to be below 0.1mag. The aperture photometry (a.mag) is considered more robust, particularly for "odd" cases, while the model fit magnitude is expected to be more accurate for "well behaved" stars. Note (5): For many stars a photometric error based on the scatter from individual observations of that star on different CCD frames could be obtained. A model error was also attempted to be assigned, based on the S/N ratio. The error quoted here is the larger of the 2. If that error exceeds 0.9mag the error was set to 0.9mag Note (6): the object type flag is used to identify possible problems with a star and has the following meaning: 0 = good, clean star, no known problem 1 = near overexposed star 2 = possible streak object 3 = high proper motion (HPM) star 4 = actually use external HPM data instead of UCAC4 observed data (accuracy of positions varies between catalogs) 5 = poor proper motion solution, report only CCD epoch position 6 = substitute poor astrometric results by FK6/Hip/Tycho-2 data 7 = added supplement star (no CCD data) from FK6/Hip/Tycho-2 data, and 2 stars added from high proper motion surveys 8 = high proper motion solution in UCAC4, star not matched with PPMXL 9 = high proper motion solution in UCAC4, discrepant motion to PPMXL Note (7): The double star flag is used to indicate the type/quality of double star fit. It is a combination of 2 flags, dsf+dst: * dsf = double star flag, represents the overall classification: 0 = single star 10 = component #1 of "good" double star 20 = component #2 of "good" double star 30 = blended image * dst = double star type, derived from pixel data image profile fits (largest value of all images used for this star): 0 = no double star, not sufficient #pixels or elongation to even call double star fit subroutine 1 = elongated image but no more than 1 peak detected 2 = 2 separate peaks detected -> try double star fit 3 = secondary peak found on each side of primary 4 = case 1 after successful double fit (small separation, blended image) 5 = case 2 after successful double fit (most likely real double) 6 = case 3 after successful double fit (brighter secondary picked) Note (8): A zero for the number of used images indicates that all images have some "problem" (such as overexposure). In that case an unweighted mean over all available images (Na) is taken to derive the mean position, while normally a weighted mean was calculated based on the "good" images, excluding possible problem images (Nu≤Na). Note (9): For astrometric data copied from the FK6, Hipparcos and Tycho-2 catalogs a mean error in positions was adopted depending on input catalog and the brightness of the star rather than giving the individual star's error quoted in those catalogs. Note (10): This unique star identification number is between 200001 and 321640 for Hipparcos stars, and between 1 and 9430 for non-Hipparcos stars supplemented to the UCAC4 catalog (no CCD observation). For all other stars this unique star identification number is the internal mean-position-file (MPOS) number + 1million. Note, there are several thousand cases where different UCAC4 stars link to the same Hipparcos star number due to resolved binary stars with each component being a separate star entry in UCAC4. Note (11): For each 2MASS bandpass a combined flag was created (cc_flg + ph_qual) consisting of the contamination flag (0 to 50) and the photometric quality flag (0 to 8). 00 = cc_flg 2MASS '0', no artifacts or contamination 10 = cc_flg 2MASS 'p', source may be contaminated by a latent image 20 = cc_flg 2MASS 'c', photometric confusion 30 = cc_flg 2MASS 'd', diffraction spike confusion 40 = cc_flg 2MASS 's', electronic stripe 50 = cc_flg 2MASS 'b', bandmerge confusion 0 = no ph_qual flag 1 = ph_qual 2MASS 'X', no valid brightness estimate 2 = ph_qual 2MASS 'U', upper limit on magnitude 3 = ph_qual 2MASS 'F', no reliable estimate of the photometric error 4 = ph_qual 2MASS 'E', goodness-of-fit quality of profile-fit poor 5 = ph_qual 2MASS 'A', valid measurement, snr>10 AND cmsig<0.10857 6 = ph_qual 2MASS 'B', valid measurement, snr> 7 AND cmsig<0.15510 7 = ph_qual 2MASS 'C', valid measurement, snr> 5 AND cmsig<0.21714 8 = ph_qual 2MASS 'D', valid measurement, no snr OR cmsig req. For example the value 05 is decoded to be cc_flg=0, and ph_qual=5, meaning no artifacts or contamination and 2MASS qual flag = "A". Note (12): Data are from the AAVSO Photometric all-sky survey (APASS) DR6 plus single observation stars kindly provided by A.Henden. For bright stars the Bmag and Vmag columns contain the Hipparcos/Tycho Bt and Vt mags respectively, whenever there is no APASS B or V available and valid Bt or Vt mags were found. The errors flagged with "-" are formal errors estimated from the S/N, while the "normal" errors (flagged with ".") are from the official release data error estimates (at least 2 observations per star). Note (13): The g-flag from the Yale San Juan first epoch Southern Proper Motion data (YSJ1, SPM) has the following meaning: 0 = no info 1 = matched with 2MASS extended source list (2MASX 2 = LEDA galaxy 3 = known QSO Note (14): The c-flag from the Yale San Juan first epoch Southern Proper Motion data (YSJ1, SPM) indicates which input catalog has been used to identify stars for pipeline processing: 1 = Hipparcos (Cat. I/311) 2 = Tycho2 (Cat. I/259) 3 = UCAC2 (Cat. I/289) 4 = 2MASS psc (Cat. II/246) 5 = 2MASS xsc (extended sources, Cat. VII/233; largely galaxies) 6 = LEDA (confirmed galaxies, Paturel et al. 2005) 7 = QSO (Veron-Cetty & Veron 2006, Cat. VII/248) Note (15): The FK6-Hipparcos-Tycho-source-flag has the following meaning: 0 = not a Hipparcos or Tycho star 1 = Hipparcos 1997 version main catalog (Cat I/239) 2 = Hipparcos double star annex 3 = Tycho-2 (Cat. I/259) 4 = Tycho annex 1 5 = Tycho annex 2 6 = FK6 position and proper motion (instead of Hipparcos data) 7 = Hippparcos 2007 solution position and proper motion (Cat. I/311) 8 = FK6, only PM substitution (not in UCAC4 data) 9 = Hipparcos 2007, only proper motion substituted (Cat. I/311) Note (16): The catflg match flag is provided for major catalogs used in the computation of the proper motions. Each match is analyzed for multiple matches of entries of the 1st catalog to 2nd catalog entries, and the other way around. Matches are also classified by separation and difference in magnitude to arrive at a confidence level group. The flag has the following meaning: 0 = star not matched with this catalog 1 = unique-unique match, not involving a double star 2 = unique-unique match, but involving a flagged double star 3 = multiple match but unique in high confidence level group, no double 4 = as 3, but involving a flagged double star 5 = closest match, not involving a double, likely o.k. 6 = closest match, but involving a flagged double star 7 = maybe o.k. smallest separation match in both directions, no double 8 = as 7, but involving a flagged double star Note (17): value is either 0 (no match) or contains the log of the apparent total diameter (in 0.1arcmin) for I-band (object size) information copied from the LEDA catalog (galaxies). A size value of less than 1 has been rounded up to 1. Note (18): This flag is either 0 (no match) or contains the length of the semi-major axis of the fiducial ellipse at the K-band (object size) information copied from the 2MASS extended source catalog. -------------------------------------------------------------------------------- Byte-by-byte Description of file: pm2/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 17 A17 --- Cluster Cluster name 22- 28 F7.4 arcmin R Distance from source 30- 48 I19 --- PPMXL PPMXL recommended identifier (5) 51- 61 F11.7 deg RAdeg Mean right ascension (ICRS), Ep=J2000 63- 72 F10.6 deg DEdeg Mean declination (ICRS), Ep=J2000 73- 80 F8.3 mas/yr pmRA ? Proper motion in RA(*cos(Dec)) 81- 88 F8.3 mas/yr pmDE ? Proper motion in Dec 90- 96 F7.2 yr EpRA Central epoch for mean RA 98-104 F7.2 yr EpDE Central epoch for mean Declination 112-114 I3 mas e_RAdeg Mean error of RAdeg at mean epoch (6) 122-124 I3 mas e_DEdeg Mean error of DEdeg at mean epoch (6) 128-132 F5.2 mas/yr e_pmRA ? Mean error on pmRA 136-140 F5.2 mas/yr e_pmDE ? Mean error on pmDE 143-148 F6.3 mag Jmag ? 2MASS J magnitude (1.2um) 152-156 F5.3 mag e_Jmag ? Mean error (rounded to 0.01mag) 159-164 F6.3 mag Hmag ? 2MASS H magnitude (1.6um) 168-172 F5.3 mag e_Hmag ? Mean error (rounded to 0.01mag) 175-180 F6.3 mag Kmag ? 2MASS Ks magnitude (2.2um) 184-188 F5.3 mag e_Kmag ? Mean error (rounded to 0.01mag) -------------------------------------------------------------------------------- 191-196 F6.3 mag B1mag ? B magnitude from USNO-B, first epoch (1) 199-204 F6.3 mag B2mag ? B magnitude from USNO-B, second epoch (1) 207-212 F6.3 mag R1mag ? R magnitude from USNO-B, first epoch (1) 215-220 F6.3 mag R2mag ? R magnitude from USNO-B, second epoch (1) 223-228 F6.3 mag Imag ? I magnitude from USNO-B (1) 232-236 A5 --- Smags [0-8-] Surveys used for USNO-B magnitudes (2) 239-240 I2 --- No ?=- Number of observations used (4) 243-244 I2 --- Fl [0/15] Flags (3) 251-252 A2 --- 2M [2M] 256-260 A5 --- NOMAD [NOMAD] 264-266 I3 % P [0/100] Membership probability -------------------------------------------------------------------------------- Note (1): Magnitudes from USNO-B (Cat. I/284) should be used with care, photometric calibration may be severely off for some plates. For objects from PPMX (Cat I/312, bit#1 set in "fl"), these magnitudes have a special meaning: ------------------------------------------------------------ Column [PPMX] Content ------------------------------------------------------------ b1mag [Cmag] Catalogue magnitude from source b2mag [Bmag] Johnson B magnitude r1mag [Rmag] calculated Ru (UCAC) magnitude from source r2mag --- (always empty) imag [Vmag] Johnson V magnitude ------------------------------------------------------------ Note (2): Flags indicating the origin of the 5 USNO-B magnitudes, (except when bit#1 set in "fl", see Note(1) above): --------------------------------------------------- # Survey Emuls Wavelen. Zones Fld Dates (nm) Obs. --------------------------------------------------- 0 = POSS-I 103a-O 350-500 -30..+90 936 1949-1965 1 = POSS-I 103a-E 620-670 -30..+90 936 1949-1965 2 = POSS-II IIIa-J 385-540 +00..+87 897 1985-2000 3 = POSS-II IIIa-F 610-690 +00..+87 897 1985-1999 4 = SERC-J IIIa-J 385-540 -90..-05 606 1978-1990 5 = ESO-R IIIa-F 630-690 -90..-05 624 1974-1994 6 = AAO-R IIIa-F 590-690 -90..-20 606 1985-1998 7 = POSS-II* IV-N 730-900 +05..+87 800 1981-2002 8 = SERC-I IV-N 715-900 -90..+00 892 1978-2002 --------------------------------------------------- (*) Here #7 includes the SERC-I plates in the zones +05..+20 (numbered #9 in USNO-B1.0) --------------------------------------------------- Note (3): The flag is a bitwise or number (Σ2i) which each bit number (i) has the meaning: #0 (1) = if set, one of the coordinates had an excessively large chi square. #1 (2) = Row is from PPMX (Cat. I/312). These objects are mostly Tycho stars that were masked out of USNO-B. When this bit is set, the USNO magnitudes (b1mag through imag) have special meanings, see Note (1) above. #2 (4) = Row is from PPMX (Cat. I/312) and replaces a single row from USNO-B. This is done when the astrometry from PPMX was better (in terms of error estimates) than the astrometry of the corresponding PPMXL object. #3 (8) = Row replaces multiple USNO-B1.0 objects. When PPMX contains an object that has more than one counterpart in PPMXL, all such counterparts are discarded on the assumption that they should have been matched in USNO-B1.0 or result from erroneous matches. For these rows, bit#1 is always 1. Note (4): No may be blank (null) for stars coming from ARIHIP or Tycho-2 via PPMX (i.e. bit#1 is set in "fl") Note (5): the identifier is a 64-bit integer representing the "pixel" number of the USNO-B 1.0 object in Q3C (QuadTreeCube, Koposov and Glushkova 2006IAUJD..13E..43K 2006IAUJD..13E..43K [ADASS 2005]). Note (6): the mean errors at epoch J2000 are the convolution of the mean error at the mean epoch and the error due to the propagation of the error on the proper motion, i.e. σ(J2000) = sqrt[σ02 + ((2000-t0)*σ(pm))2] -------------------------------------------------------------------------------- Acknowledgements: This project is supported by FAPESP (grant number 2013/01115-6) Wilton Dias, wiltonsdias(at)yahoo.com.br History: * 07-May-2014: First on-line version * 30-Sep-2015: Cluster name added in pm/* and pm2/* files
(End) Patricia Vannier [CDS] 17-Apr-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line