J/MNRAS/443/432     Eclipsing binaries in LMC                (Muraveva+, 2014)
Eclipsing binary stars in the Large Magellanic Cloud:
results from the EROS-2, OGLE and VMC surveys.
    Muraveva T., Clementini G., Maceroni C., Evans C.J., Moretti M.I.,
    Cioni M.-R.L., Marquette J.B., Ripepi V., de Grijs R., Groenewegen M.A.T.,
    Piatti A.E., van Loon J.T.
   <Mon. Not. R. Astron. Soc., 443, 432-445 (2014)>
   =2014MNRAS.443..432M 2014MNRAS.443..432M
ADC_Keywords: Magellanic Clouds ; Binaries, eclipsing ; Photometry
Keywords: techniques: photometric - surveys - binaries: eclipsing -
          Magellanic Clouds
Abstract:
    We present a catalogue of 1768 eclipsing binary stars (EBs) detected
    in the Large Magellanic Cloud (LMC) by the second generation of the
    EROS survey (hereinafter EROS-2); 493 of them are new discoveries
    located in outer regions (out of the central bar) of the LMC. These
    sources were originally included in a list of candidate classical
    Cepheids (CCs) extracted from the EROS-2 catalogue on the basis of the
    period (0.89<PEROS<15.85d) versus luminosity
    [13.39≪BEROS><17.82mag] diagram. After visual inspection of the
    light curves we reclassified them as eclipsing binaries. They have
    blue colours (BEROS-REROS<0.2mag) hence we classed them as hot
    eclipsing binaries (HEBs) containing hot massive components: main
    sequence (MS) stars or blue giants. We present Ks-band light curves
    for 999 binaries from our sample that have a counterpart in the VISTA
    near-infrared ESO public survey of the Magellanic Clouds system (VMC).
    We provide spectral classifications of 13 HEBs with existing
    spectroscopy. We divided our sample into contact-like binaries and
    detached/semi-detached systems based on both visual inspection and the
    parameters of the Fourier decomposition of the light curves and
    analysed the period-luminosity (PL) relations of the contact-like
    systems using the REROS and Ks magnitudes at maximum light. The
    contact-like binaries in our sample do not follow PL relations. We
    analysed the sample of contact binaries from the OGLE III catalogue
    and confirmed that PLI and PLK sequences are defined only by
    eclipsing binaries containing a red giant component.
Description:
    The EROS-2 microlensing survey has monitored about 88deg2 of the
    LMC discovering a large number of CCs, RR Lyrae stars, binaries and
    long period variables (LPVs), both in the centre and in the outer
    regions of the galaxy. The survey was carried out with the Marly 1-m
    telescope at ESO, La Silla, from 1996 July to 2003 February.
    Observations were performed in two wide passbands, the so-called
    REROS band centred close to the IC standard band, and the BEROS
    band intermediate between the standard V and R bands.
File Summary:
--------------------------------------------------------------------------------
 FileName   Lrecl  Records  Explanations
--------------------------------------------------------------------------------
ReadMe         80        .  This file
tablea1.dat   107      493  Identification, main properties and Fourier
                            parameters of the light curves for the 493 new
                            Hot Eclipsing Binaries (HEB) in the LMC
tablea2.dat   107     1275  Identification, main properties and Fourier
                            parameters of the light curve for the 1275 HEBs in
                            the LMC which were already detected by other surveys
tablea3.dat    96       13  EROS-2 HEBs with existing optical spectroscopy
tablea6.dat    62      999  REROS and Ks magnitudes at maximum light of
                            EB stars in the LMC from the EROS-2 and VMC data
table4/*        .     1768  Individual EROS R and B time series photometry
table5/*        .      999  Individual Ks time series photometry
--------------------------------------------------------------------------------
See also:
   J/A+A/566/A43 : EPOCH Project. EROS-2 LMC periodic variables (Kim+, 2014)
Byte-by-byte Description of file: tablea1.dat tablea2.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 12  A12   ---     EROS2     EROS-2 identifier, lmNNNNaNNNNN (G1)
      13  A1    ---   n_Per       [*] * indicates star with period re-determined
                                      based on our study of the light curve
  16- 23  F8.5  deg     RAdeg     Right ascension (J2000)
  25- 33  F9.5  deg     DEdeg     Declination (J2000)
  35- 44  F10.7 d       Per       [0.8/21.1] Period P
  46- 50  F5.2  mag     <Rmag>    [13.5/18.1] Average EROS R magnitude
  52- 56  F5.2  mag     <Bmag>    [13.3/17.9] Average EROS B magnitude
  58- 66  F9.4  d       T0        Epoch of minimum (HJD-2450000)
  68- 72  F5.3  mag     a0        Fourier parameter a0 (1)
  74- 79  F6.3  mag     a1        Fourier parameter a1 (1)
  81- 86  F6.3  mag     a2        Fourier parameter a2 (1)
  88- 93  F6.3  mag     a3        Fourier parameter a3 (1)
  95-100  F6.3  mag     a4        Fourier parameter a4 (1)
 102-107  F6.3  mag     a5        Fourier parameter a5 (1)
--------------------------------------------------------------------------------
Note (1): model light curve with 6 terms (φ=2πt/P): 
    A = a0 + a1cos(φ) + a2cos(2φ) + a3cos(3φ) 
             + a4 a3cos(4φ) + a5sin(φ)
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Byte-by-byte Description of file: tablea3.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 12  A12   ---     EROS2     EROS-2 identifier, lmNNNNaNNNNN (G1)
  15- 22  F8.5  deg     RAdeg     Right ascension (J2000)
  24- 32  F9.5  deg     DEdeg     Declination (J2000)
  34- 41  F8.6  d       Per       [1.1/5.5] EROS-2 period
  43- 50  F8.6  d       Per3      [1.1/5.5]?=- OGLE III period from 
                                    Graczyk et al. (2011, Cat. J/AcA/61/103)
  52- 63  A12   ---     AName     Alternative name
  66- 85  A20   ---     SpType    MK spectral type
  87- 92  A6    ---     Note      Notes (1)
  94- 96  A3    ---     Ref       Reference (2)
--------------------------------------------------------------------------------
Note (1): SB1 and SB2 stand for single- and double-lined spectroscopic
          binaries, respectively.
Note (2): References as follows:
    E06 = Evans et al. 2006A&A...456..623E 2006A&A...456..623E, Cat. J/A+A/456/623
    W14 = Walborn et al. 2014A&A...564A..40W 2014A&A...564A..40W, Cat. J/A+A/564/A40
    E14 = Evans et al., 2015A&A...574A..13E 2015A&A...574A..13E, Cat. J/A+A/574/A13
--------------------------------------------------------------------------------
Byte-by-byte Description of file: tablea6.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 12  A12   ---     EROS2     EROS-2 identifier, lmNNNNaNNNNN (G1)
      13  A1    ---   n_EROS2     [*] * indicates star with period re-determined
                                      based on our study of the light curve
  15- 17  A3    ---     ---       [VMC]
  19- 38  A20   ---     VMC       VMC identifier (JHHMMSS.ss+DDMMSS.s) (1)
  40- 48  F9.6  d       Per       [0.9/21.1] Period
  50- 55  F6.3  mag     Ksmag     Maximum VISTA Ks magnitude
  57- 62  F6.3  mag     Rmag      Maximum EROS R magnitude
--------------------------------------------------------------------------------
Note (1): VMC catalogue (Vista Magellanic Clouds) available at VSA 
  (observations completed until 2013 April 1), Lewis, Irwin & Bunclark 
  (2010, ASP Conf. Ser. Vol 434, P. 91), Cross et al. 2012A&A...548A.119C 2012A&A...548A.119C).
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Byte-by-byte Description of file: table4/*
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   3- 12  F10.5 d       HJD       Heliocentric Julian date (HJD-2450000)
  15- 20  F6.3  mag     Rmag      ?=99.999 EROS R magnitude
  22- 27  F6.3  mag   e_Rmag      ?=9.999 rms uncertainty on Rmag
  30- 35  F6.3  mag     Bmag      ?=99.999 EROS B magnitude
  37- 42  F6.3  mag   e_Bmag      ?=9.999 rms uncertainty on Bmag
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table5/*
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
       1  A1    ---     ---       [5]
   2- 12  F11.6 d       HJD       Heliocentric Julian date (HJD-2450000)
  14- 20  F7.4  mag     Ksmag     ?=99.999 Ks magnitude
  22- 27  F6.4  mag   e_Ksmag     ?=9.999 rms uncertainty on Ksmag
--------------------------------------------------------------------------------
Global notes:
Note (G1):
   Sources identified as EROS2-star lmNNN-Na-NNNNN in Simbad.
--------------------------------------------------------------------------------
History:
    From electronic version of the journal
(End)                                      Patricia Vannier [CDS]    10-Mar-2015