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J/AcA/61/199   OGLE3 Magellanic Clouds High proper motion stars (Poleski+, 2011)

The Optical Gravitational Lensing Experiment. High proper motion stars in the OGLE-III data for Magellanic Clouds fields. Poleski R., Soszynski I., Udalski A., Szymanski M.K., Kubiak M., Pietrzynski G., Wyrzykowski L., Ulaczyk K. <Acta Astron., 61, 199-216 (2011)> =2011AcA....61..199P
ADC_Keywords: Magellanic Clouds ; Proper motions Keywords: astrometry - catalogs - stars: kinematics and dynamics - binaries: visual - white dwarfs Abstract: We present the results of a search for High Proper Motion (HPM) stars, i.e., the ones with pm>100mas/yr, in the direction to the Magellanic Clouds. This sky area was not examined in detail as the high stellar density hampers efforts in performing high-quality astrometry. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file ident.dat 128 551 Main catalog file cpm.dat 68 27 Common proper motion binaries otherid.dat 31 280 Identification of stars in other catalogs remarks.dat 80 11 Remarks
See also: J/AcA/52/143 : OGLE high proper motion stars towards MC (Soszynski+, 2002) J/MNRAS/327/601 : OGLE2 High proper motion stars (Eyer+, 2001) J/MNRAS/348/1439 : OGLE2 Galactic center proper motions (Sumi+, 2004) J/MNRAS/385/905 : OGLE2 high pm stars towards Galac. Centre (Rattenbury+ 2008) Byte-by-byte Description of file: ident.dat
Bytes Format Units Label Explanations
1- 15 A15 --- Star Star's ID (G1) 17- 18 I2 h RAh Right ascension, equinox J2000.0 (hours) 20- 21 I2 min RAm Right ascension, equinox J2000.0 (minutes) 23- 27 F5.2 s RAs Right ascension, equinox J2000.0 (seconds) 29 A1 --- DE- Declination, equinox J2000.0 (sign) 30- 31 I2 deg DEd Declination, equinox J2000.0 (degrees) 33- 34 I2 arcmin DEm Declination, equinox J2000.0 (arc minutes) 36- 39 F4.1 arcsec DEs Declination, equinox J2000.0 (arc seconds) 41- 47 F7.2 mas/yr pmRA Proper motion in RA (pmRA*cos(DE)) 49- 52 F4.2 mas/yr e_pmRA Statistical uncertainty of proper motion in RA 54- 57 F4.2 mas/yr spmRA Systematical uncertainty of proper motion in RA 59- 65 F7.2 mas/yr pmDE Proper motion in DE 67- 70 F4.2 mas/yr e_pmDE Statistical uncertainty of proper motion in DE 72- 75 F4.2 mas/yr spmDE Systematical uncertainty of proper motion in DE 77- 82 F6.2 mas/yr pm Total proper motion 84- 88 F5.2 mas plx ?=0.000 Parallax (1) 90- 93 F4.2 mas e_plx ?=0.000 Uncertainty of parallax 95-100 F6.3 mag Imag I-band brightness (1) 102-106 F5.3 mag e_Imag Uncertainty of I-band brightness 108-113 F6.3 mag V-I ?=9.999 V-I color index 115-119 F5.3 mag e_V-I ?=9.999 Uncertainty of V-I color index 121-128 A8 --- Lum Luminosity class (subdwarf, WD, WD_cand. or empty)
Note (1): Parallax and its uncertainty equal to "0.00" indicate that it was not possible to measure it. Similarly V-I color of "9.999" indicates V-band brightness is unknown.
Byte-by-byte Description of file: cpm.dat
Bytes Format Units Label Explanations
1- 14 A14 --- Name1 First name (G1) 16- 29 A14 --- Name2 Second name (G1) 31- 35 F5.1 arcsec Dist Angular distance 37- 39 I3 mas/yr pm Total proper motion 41- 68 A28 --- Note Note
Byte-by-byte Description of file: otherid.dat
Bytes Format Units Label Explanations
1- 15 A15 --- Star Star's ID (G1) 17- 31 A15 --- OName Other name (1)
Note (1): SPM4 (0580401860), OGLE-II (LMC_SC8 211845) and MACHO (78.5860.31)
Byte-by-byte Description of file: remarks.dat
Bytes Format Units Label Explanations
1- 15 A15 --- Star Star's ID (G1) 17- 80 A64 --- Remark Remark
Global notes: Note (G1): OGLE-III field and database number, SMC FFF.N.NNNNN or LMC FFF.N.NNNNN (Udalski et al., 2008AcA....58...89U)
Acknowledgements: Copied at ftp://sirius.astrouw.edu.pl/ogle/ogle3/pm/hpm_mcs/
(End) Patricia Vannier [CDS] 29-Oct-2011
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

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