J/AcA/53/1    OGLE eclipsing binaries in LMC         (Wyrzykowski+, 2003)

The Optical Gravitational Lensing Experiment. Eclipsing binary stars in the Large Magellanic Cloud. Wyrzykowski L., Udalski A., Kubiak M., Szymanski M., Zebrun K., Soszynski I., Wozniak P.R., Pietrzynski G., Szewczyk O. <Acta Astron., 53, 1 (2003)> =2003AcA....53....1W 2003AcA....53....1W
ADC_Keywords: Magellanic Clouds ; Binaries, eclipsing ; Photometry Keywords: binaries: eclipsing, Magellanic Clouds, Catalogs Abstract: We present the catalog of 2580 eclipsing binary stars detected in 4.6 square degree area of the central parts of the Large Magellanic Cloud. The photometric data were collected during the second phase of the OGLE microlensing search from 1997 to 2000. The eclipsing objects were selected with the automatic search algorithm based on an artificial neural network. Basic statistics of eclipsing stars are presented. Also, the list of 36 candidates of detached eclipsing binaries for spectroscopic study and for precise LMC distance determination is provided. The full catalog is accessible from the OGLE Internet archive. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablee.dat 200 2681 List of 2580 detected eclipsing binary stars tableea.dat 200 39 *List of 39 well detached binary systems well suited for distance determination -------------------------------------------------------------------------------- Note on tableea.dat: Selection critera were: Idia<16mag, depth of the secondary eclipse >0.2mag. -------------------------------------------------------------------------------- See also: J/AcA/48/563 : OGLE SMC eclipsing binaries BVI photometry (Udalski+ 1998) J/AcA/49/223 : BVI photometry of OGLE LMC Cepheids (Udalski+, 1999) J/AcA/49/521 : OGLE LMC star clusters BVI photometry (Pietrzynski+, 1999) J/AcA/49/543 : OGLE LMC + SMC Cepheids VI photometry (Pietrzynski+, 1999) J/AcA/50/421 : OGLE-II DIA BUL_SC1 field (Wozniak, 2000) J/AcA/51/175 : OGLE-II DIA microlensing events (Wozniak+, 2001) Byte-by-byte Description of file: tablee.dat tableea.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- Seq Sequential number Catalog 6- 13 A8 --- Field Field designation 15- 18 A4 --- --- [OGLE] 19- 36 A18 --- Star Star identification (HHMMSS.ss+DDMMSS.s) 38- 39 I2 h RAh Right ascension (J2000) 40 A1 --- --- [:] 41- 42 I2 min RAm Right ascension (J2000) 43 A1 --- --- [:] 44- 48 F5.2 s RAs Right ascension (J2000) 50 A1 --- DE- Declination sign (J2000) 51- 52 I2 deg DEd Declination (J2000) 53 A1 --- --- [:] 54- 55 I2 arcmin DEm Declination (J2000) 56 A1 --- --- [:] 57- 60 F4.1 arcsec DEs Declination (J2000) 62- 69 F8.3 pix xpos x coordinate in the reference fts image 71- 78 F8.3 pix ypos y coordinate in the reference fts image 80- 89 F10.6 d Per Period 91-100 F10.5 d T0 Epoch (HJD-2450000) 102-106 F5.2 mag Idiamag DIA I-band magnitude at maximum 108-112 F5.2 mag Depth Depth of the primary eclipse (in DIA I band) 114-119 F6.2 --- Phase ?=-99.99 Phase of the secondary eclipse 121-126 F6.2 mag Depth2 ?=-99.99 Depth of the secondary eclipse (Idia magnitude) (1) 128-133 F6.2 mag Imag ?=-99.99 I magnitude at maximum (1)(2) 135-140 F6.2 mag Vmag ?=-99.99 V magnitude at maximum (1)(2) 142-147 F6.2 mag Bmag ?=-99.99 B magnitude at maximum (1)(2) 149-168 A20 --- Type Eclipsing binary type, 170-200 A31 ---- OStar Overlapping star (0 if none). -------------------------------------------------------------------------------- Note (1): From standard OGLE-II photometry Note (2): Magic number -99.99 for secondary eclipse parameters and for color columns means "no data". -------------------------------------------------------------------------------- History: Copied at ftp://sirius.astrouw.edu.pl/ogle/
(End) James Marcout, Patricia Bauer [CDS] 22-Sep-2003
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