J/AcA/66/421        Eclipsing binaries in the Magellanic System  (Pawlak+, 2016)
The OGLE collection of variable stars.
Eclipsing binaries in the Magellanic System.
    Pawlak M., Soszynski I., Udalski A., Szymanski M.K., Wyrzykowski L.,
    Ulaczyk K., Poleski R., Pietrukowicz P., Kozlowski S., Skowron D.M.,
    Skowron J., Mroz P., Hamanowicz A.
   <Acta Astron., 66, 421-432 (2016)>
   =2016AcA....66..421P 2016AcA....66..421P    (SIMBAD/NED BibCode)
ADC_Keywords: Magellanic Clouds ; Binaries, eclipsing ; Photometry
Keywords: binaries: eclipsing - stars: variables: general - Magellanic Clouds
Abstract:
    We present the collection of eclipsing binaries in the Large and Small
    Magellanic Clouds, based on the OGLE survey. It contains 48605
    systems, 40204 belonging to the LMC and 8401 to the SMC. Out of the
    total number of presented here binaries, 16374 are the new
    discoveries. We present the time-series photometry obtained for the
    selected objects during the fourth phase of the OGLE project. The
    catalog has been created using a two step machine learning procedure
    based on the Random Forest algorithm.
Description:
    All the data used in this work were collected during the fourth phase
    of the OGLE project, between March 2010 and July 2015, using the 1.3-m
    Warsaw telescope located at Las Campanas Observatory (operated by the
    Carnegie Institution for Science) in Chile. The telescope is equipped
    with a 32-chip mosaic camera, with a total field of view of 1.4 square
    degrees. The whole area of the Magellanic Clouds region covered by 475
    OGLE-IV fields is about 650 square degrees. Observations were carried
    out in the I- and V-band filters, with about 90%taken in the I-band.
    The I-band magnitude range covered by OGLE-IV is from 13mag to
    21.5mag. The number of collected epochs varies between 100 and 700.
    The photometry was obtained with the Differential Image Analysis
    method (Alard and Lupton, 1998ApJ...503..325A 1998ApJ...503..325A, Wozniak,
    2000AcA....50..421W 2000AcA....50..421W, Cat. J/AcA/50/421). For technical details of the
    OGLE-IV instrumental setup and date reduction system we refer the
    reader to Udalski et al. (2015AcA....65....1U 2015AcA....65....1U). The procedure of the
    correction of photometric uncertainties is presented in Skowron et al.
    (2016AcA....66....1S 2016AcA....66....1S)
File Summary:
--------------------------------------------------------------------------------
 FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe            80        .   This file
ident.dat        118    48605   Identification of stars (8401 SMC and 40204 LMC)
ecl.dat           70    48605   Parameters of stars
remarks.dat       80       21   Remarks
--------------------------------------------------------------------------------
See also:
 J/MNRAS/443/432 : Eclipsing binaries in LMC (Muraveva+, 2014)
 J/ApJ/824/74    : OGLE LC classification of MC Cepheids (Garcia-Varela+, 2016)
Byte-by-byte Description of file: ident.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 18  A18   ---     Star      Star's ID
                                   (OGLE-SMC-ECL-NNNN or OGLE-LMC-ECL-NNNNN)
  21- 23  A3    ---     Type      [C NC ELL] Subtype of binary star (1)
  26- 27  I2    h       RAh       Right ascension (J2000.0)
  29- 30  I2    min     RAm       Right ascension (J2000.0)
  32- 36  F5.2  s       RAs       Right ascension (J2000.0)
      38  A1    ---     DE-       Declination sign (J2000.0)
  39- 40  I2    deg     DEd       Declination (J2000.0)
  42- 43  I2    arcmin  DEm       Declination (J2000.0)
  45- 48  F4.1  arcsec  DEs       Declination (J2000.0)
  51- 66  A16   ---     OGLEIV    OGLE-IV ID
  68- 82  A15   ---     OGLEIII   OGLE-III ID
  84- 98  A15   ---     OGLEII    OGLE-II ID
 100-118  A19   ---     OName     Other designation (from GCVS)
-------------------------------------------------------------------------------
Note (1): Subtypes as follows:
           C = contact
          NC = detached or semi-detached
         ELL = ellipsoidal
--------------------------------------------------------------------------------
Byte-by-byte Description of file: ecl.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 18  A18   ---     Star      Star's ID
                                   (OGLE-SMC-ECL-NNNN or OGLE-LMC-ECL-NNNNN)
  21- 26  F6.3  mag     <Imag>    Intensity mean I-band magnitude
  28- 33  F6.3  mag     <Vmag>    ?=- Intensity mean V-band magnitude
  35- 46  F12.7 d       Per       Period
  49- 57  F9.4  d       T0        Epoch of primary eclipse (HJD-2450000)
  60- 64  F5.3  mag     Depth     ?=- Depth of primary eclipse
  66- 70  F5.3  mag     Depth2    ?=- Depth of secondary eclipse
--------------------------------------------------------------------------------
Byte-by-byte Description of file: remarks.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 18  A18   ---     Star      Star's ID
                                   (OGLE-SMC-ECL-NNNNN or OGLE-LMC-ECL-NNNNN)
  20- 80  A61   ---     Rem       Remarks
--------------------------------------------------------------------------------
History:
    Copied at ftp://ftp.astrouw.edu.pl/ogle/ogle4/OCVS/lmc/ecl/
     and ftp://ftp.astrouw.edu.pl/ogle/ogle4/OCVS/smc/ecl/
(End)                                      Patricia Vannier [CDS]    22-Oct-2018