J/AJ/146/43        WIYN open cluster study. LV. NGC 6819        (Platais+, 2013)

WIYN open cluster study. LV. Astrometry and membership in NGC 6819. Platais I., Gosnell N.M., Meibom S., Kozhurina-Platais V., Bellini A., Veillet C., Burkhead M.S. <Astron. J., 146, 43 (2013)> =2013AJ....146...43P 2013AJ....146...43P
ADC_Keywords: Clusters, open ; Proper motions ; Photometry, CCD ; X-ray sources ; Cross identifications Keywords: astrometry - open clusters and associations: individual: NGC 6819 Abstract: We present proper motions and astrometric membership analysis for 15750 stars around the intermediate-age open cluster NGC 6819. The accuracy of relative proper motions for well-measured stars ranges from ∼0.2mas/yr within 10' of the cluster center to 1.1mas/yr outside this radius. In the proper motion vector-point diagram, the separation between the cluster members and field stars is convincing down to V∼18 and within 10' from the cluster center. The formal sum of membership probabilities indicates a total of ∼2500 cluster members down to V∼22. We confirm the cluster membership of several variable stars, including some eclipsing binaries. The estimated absolute proper motion of NGC 6819 is µxabs=-2.6±0.5 and µyabs=-4.2±0.5mas/yr. A cross-identification between the proper motion catalog and a list of X-ray sources in the field of NGC 6819 resulted in a number of new likely optical counterparts, including a candidate CV. For the first time we show that there is significant differential reddening toward NGC 6819. Description: As part of the WIYN Open Cluster Study (WOCS; Mathieu, 2000ASPC..198..517M 2000ASPC..198..517M), we initiated a proper motion study of NGC 6819 based upon the new measurements of archival long-focus photographic plates in combination with recent CCD observations. A total of 30 scanned photographic plates are available for NGC 6819. However, only 23 of them are adequate for the purpose of astrometry. The plates are taken with the McDonald 82inch, the Yale 1m, the Hale 5m, the Mt. Wilson 60inch, and the CFHT 3.6m (Table1). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 51 5 Photographic plates and a set of CCD frames used in this study table4.dat 99 15750 Catalog of positions and proper motions in NGC 6819 table5.dat 82 51 Proposed optical counterparts of X-Ray sources in NGC 6819 -------------------------------------------------------------------------------- See also: J/ApJ/729/L10 : KIC stars properties in NGC 6791 and NGC 6819 (Basu+, 2011) J/AJ/138/159 : NGC 6819 stellar radial-velocity and photometry (Hole+, 2009) J/MNRAS/358/795 : Variable stars in NGC 6819 field (Street+, 2005) J/AJ/126/2922 : Astrometry & membership in NGC 188 (Platais+, 2003; Pap XVII) J/AJ/124/601 : Absolute positions and proper motions in NGC 188 (Platais+, 2002; Paper VIII) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 A18 --- Tel Telescope 20- 27 A8 --- Plate Number of plates in blue (B) and visual (V) bandpasses 29- 32 I4 yr Epoch Mean epoch (or beginning of Epoch) 33- 35 A3 --- Epoch2 Most recent epoch (1919-33) 37- 38 I2 mag Vlim [17/23] Approximate limiting V magnitude 40- 43 F4.1 arcsec/mm Scale Plate scale 45- 51 A7 arcmin FOV Size of the field-of-view -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- Star [441/999643] Star number in the master catalog <[PGM2013] NNNNNN> in Simbad 8- 17 F10.6 deg RAdeg Right ascension (Eq=J2000, Ep=2009.875) 19- 27 F9.6 deg DEdeg Declination (Eq=J2000, Ep=2009.875) 29- 34 F6.3 mag gmag Sloan g' magnitude 36- 41 F6.3 mag g-r Sloan g'-r' color index 43- 48 F6.2 mas/yr pmRA Relative proper motion in X (RA direction) 50- 55 F6.2 mas/yr pmDE Relative proper motion in Y (Dec direction) 57- 61 F5.2 mas/yr e_pmRA Standard error in pmRA 63- 67 F5.2 mas/yr e_pmDE Standard error in pmDE 69- 72 F4.2 mas/yr epm Estimated error of proper motion in X and Y (2) 74- 75 I2 % Mb [0/99] Cluster membership probability 77- 83 F7.3 arcmin oRA Tangential coordinate along RA direction (3) 85- 91 F7.3 arcmin oDE Tangential coordinate along Dec direction (3) 93 I1 --- Nt [0/6] Number of plates for McDonald 82inch (4) 94- 95 I2 --- Nu [0/13] Number of plates for Yale 1m (4) 96 I1 --- Nv [0/2] Number of plates for Hale 5m (4) 97 I1 --- Nz [0/2] Number of plates for Mt. Wilson 60inch (4) 99 I1 --- Nd [0/1] Number of deleted datasets -------------------------------------------------------------------------------- Note (2): This error is estimated from an average standard error at a given g'-magnitude and should be used only as a guide to the reliability of calculated proper motions and their errors. Note (3): With zeropint at the J2000 center of NGC 6819 (RA=295.32283°, DE=+40.19639°). Note (4): For each datasets and used for proper motion calculation. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [XMMUJ ] 7- 21 A15 arcsec XMMUJ X-ray source name (HHMMSS.s+DDMMSS; J2000) 23- 28 I6 --- Star [388118/938065] Optical counterpart number in the master catalog 30- 35 F6.3 mag gmag Sloan g' magnitude 37- 42 F6.3 mag g-r Sloan g'-r' color index 44- 46 F3.1 arcsec Xerr X-ray source estimated positional error from Gosnell et al. (2012ApJ...745...57G 2012ApJ...745...57G) 48- 51 F4.2 arcsec Dist [0/4] Counterpart/X-ray source total distance 53- 57 F5.2 mas/yr pmRA ? Relative proper motion in X (RA direction) 59- 63 F5.2 mas/yr pmDE ? Relative proper motion in Y (Dec direction) 65- 66 I2 % Mb [0/99]? Cluster membership probability (from proper motion) 68 A1 --- --- [X] 69- 70 I2 --- X [1/11]? ID number in Gosnell et al. 2012 (2) 72- 75 A4 --- --- [WOCS ] 77- 82 I6 --- WOCS ? WIYN Open Cluster Study (WOCS) number (3) -------------------------------------------------------------------------------- Note (2): X-ray source ID in Gosnell et al. (2012ApJ...745...57G 2012ApJ...745...57G): X1 is a quiescent low-mass X-ray binary candidate, X2 a cataclysmic variable candidate, X6 a RS CVn abd X9 an active binary. Note (3): From Hole et al. (2009, cat. J/AJ/138/159) and K. Milliman et al. 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(End) Greg Schwarz [AAS], Sylvain Guehenneux [CDS] 26-Jun-2014
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