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J/A+AS/109/447
  Eclipsing binaries EROS catalogue (Grison+, 1995)
Post annotation
img(gal)
1.J/A+AS/109/447/photomBe and Re photometry (87364 rows)
2.J/A+AS/109/447/table1(c)79 certain or probable eclipsing binary stars in the bar of the LMC (79 rows)
3.J/A+AS/109/447/table2Times of secondary minima for obviously eccentric systems (10 rows)

 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)Name (char) Name of star (meta.id;meta.main)
  (1)HJD d Heliocentric moment of mid observation (time.epoch)
  (1)Filt (char) Filter (Be or Re) (meta.code;instr.filter)
  (1)Mag mag EROS magnitude (phot.mag)
  (2+3)EROS   [1001/1079] EROS number starting at 10001 (eclipsing binaries) (meta.id;meta.main)
  (2)CCD  Number of the detector on which the star fell (meta.id;instr)
  (2)x arcsec Harvard (x,y) coordinates of the star, accurate to about 3 arcsec (Note 1)   (pos.proj)
  (2)y arcsec Harvard (x,y) coordinates of the star accurate to about 3 arcsec (Note 1)   (pos.proj)
  (2)RAJ2000 "h:m:s" (i) Right ascension J2000.0 (pos.eq.ra;meta.main)
  (2)DEJ2000 "d:m:s" (n)(i) Declination sign (pos.eq.dec;meta.main)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)To(p) d The heliocentric Julian date of the designated primary minimum and its uncertainty. Where one eclipse is clearly deeper, it has been taken as the primary minimum. For some stars neither minimum is clearly deeper and the eclipse designated as primary is mo (time.epoch)
  (2)e_To(p) d rms uncertainty on To(p) (stat.error)
  (2)P d Period of the system (time.period)
  (2)e_P d rms uncertainty on P (stat.error)
  (2)dTo(p)/dP   []? A partial derivative indicating how much To(p) is affected by errors in P, where this is significant. (src.orbital)
  (2)Be(max)  Approximate Be magnitudes at maximum light (phot.mag)
  (2)Re(max)   []? Approximate Re magnitude at maximum light (phot.mag)
  (2)Rem (char) Remarks: The section of the printed paper in which remarks are made about individual stars (meta.note)
  (3)To(s) d Heliocentric Julian date of the secondary minimum for clearly eccentric systems (time.epoch)
  (3)e_To(s) d rms uncertainty for To(s) (stat.error)
  (3)dTo(s)/dP   []? A partial derivative indicating how much To(s) is affected by errors in P, where this is significant. (src.orbital)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
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