J/AcA/62/133   Optical counterparts of X-ray sources in OGLE    (Udalski+, 2012)
The Optical Gravitational Lensing Experiment.
Optical counterparts to the X-ray sources in the Galactic Bulge.
    Udalski A., Kowalczyk K., Soszynski I., Poleski R., Szymanski M.K.,
    Kubiak M., Pietrzynski G., Kozlowski S., Pietrukowicz P., Ulaczyk K.,
    Skowron J., Wyrzykowski L.
   <Acta Astron., 62, 133-151 (2012)>
   =2012AcA....62..133U 2012AcA....62..133U
ADC_Keywords: X-ray sources ; Photometry
Keywords: X-ray: stars - X-ray: binaries - stars: activity -
          binaries: symbiotic - novae, cataclysmic variables - galaxies: Seyfert
Abstract:
    We present a sample of 209 variable objects - very likely optical
    counterparts to the X-ray sources detected in the direction of the
    Galactic center by the Galactic Bulge Survey (GBS) carried out with
    the Chandra satellite. The variable sources were found in the
    databases of the OGLE long term survey monitoring regularly the
    Galactic bulge since 1992. The counterpart candidates were searched
    based on the X-ray source position in the radius of 3.9 arcsec.
File Summary:
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 FileName   Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe         80        .   This file
table1.dat    119      212   Optical counterparts to the X-ray sources detected
                              by the Galactic Bulge Survey revealing optical
                              variability
table2.dat     71       19   Possible bright non-variable optical counterparts
                              to the X-ray sources detected by the
                              Galactic Bulge Survey
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See also:
        II/213   : OGLE Galactic Bulge periodic variables (Udalski+ 1996)
 J/A+A/439/559   : OGLE eclipsing binaries (bulge+lmc+smc) (Groenewegen+, 2005)
 J/A+A/478/659   : OGLE Be stars in Galactic Bulge (Sabogal+, 2008)
 J/AcA/50/1      : OGLE microlensing events in Galactic Bulge (Udalski+, 2000)
 J/AcA/52/217    : OGLE II. VI photometry of Galactic Bulge (Udalski+, 2002)
 J/ApJ/636/240   : OGLE II microlensing parameters (Sumi+, 2006)
 J/AcA/61/83     : OGLE-III photometric maps of Galactic Bulge (Szymanski+ 2011)
 J/MNRAS/356/331 : QSO-candidates in OGLE-II Galactic bulge fields (Sumi+, 2005
 ftp://ftp.astrouw.edu.pl/ogle/ogle4/XRAY-GBS : OGLE-IV Xray-GBS Home Page
Byte-by-byte Description of file: table[12].dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  3  A3    ---     DB        [II IV] OGLE datase number
   5-  7  A3    ---     ---       [GBS]
   9- 12  I4    ---     GBS       GBS (Galactic Bulge Survey) number
  14- 22  A9    ----    Field     OGLE field
                                   (in OGLE database, OGLE-IV or OGLE-II)
  24- 29  I6    ---     OGLE      OGLE identification number
  31- 32  I2    h       RAh       Right ascension (J2000)
  34- 35  I2    min     RAm       Right ascension (J2000)
  37- 41  F5.2  s       RAs       Right ascension (J2000)
      43  A1    ---     DE-       Declination sign (J2000)
  44- 45  I2    deg     DEd       Declination (J2000)
  47- 48  I2    arcmin  DEm       Declination (J2000)
  50- 53  F4.1  arcsec  DEs       Declination (J2000)
  55- 58  F4.2  arcsec  Dist      Distance from X-ray source
  60- 65  F6.3  mag     Imag      I magnitude
  67- 71  F5.3  mag     V-I       ?=9.999 V-I colour index
  73- 82  F10.6 d       Per       ?=- Period
  84- 88  A5    ---     Class     Classification (1)
  90-119  A30   ---     FileName  Name of the light curve file at
                                  ftp://ftp.astrouw.edu.pl/ogle/ogle4/XRAY-GBS/
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Note (1): Classifications found as follows:
    CV    = cataclysmic variable
    E     = eclipsing system
    E?    = possible eclipsing system
    I     = irregular variable
    MIRA  = Mira variable
    OSARG = OGLE Small Amplitude Red Giant
    P     = periodic
    RRLYR = RR Lyr star
    SP    = (rotating) spotted star (RS CVn)
    SRV   = semi-regular variable
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History:
    Copied at ftp://ftp.astrouw.edu.pl/ogle/ogle4/XRAY-GBS/
(End)                                      Patricia Vannier [CDS]    28-Dec-2012