J/AJ/135/850    Properties of eclipsing binaries found in TrES    (Devor+, 2008)
Identification, classifications, and absolute properties of 773 eclipsing
binaries found in the trans-atlantic exoplanet survey.
    Devor J., Charbonneau D., O'Donovan F.T., Mandushev G., Torres G.
   <Astron. J., 135, 850-877 (2008)>
   =2008AJ....135..850D 2008AJ....135..850D
ADC_Keywords: Binaries, eclipsing ; Models ; Proper motions ; Magnitudes
Keywords: binaries: eclipsing - catalogs - methods: data analysis -
          stars: statistics - techniques: photometric
Abstract:
    In recent years, we have witnessed an explosion of photometric
    time-series data, collected for the purpose of finding a small 
    number of rare sources, such as transiting extrasolar planets and
    gravitational microlenses. Once combed, these data are often set
    aside, and are not further searched for the many other variable
    sources that they undoubtedly contain. To this end, we describe a
    pipeline that is designed to systematically analyze such data, while
    requiring minimal user interaction. We ran our pipeline on a subset of
    the Trans-Atlantic Exoplanet Survey dataset, and used it to identify
    and model 773 eclipsing binary systems. For each system we conducted a
    joint analysis of its light curve, colors, and theoretical isochrones.
    This analysis provided us with estimates of the binary's absolute
    physical properties, including the masses and ages of their stellar
    components, as well as their physical separations and distances. We
    identified three types of eclipsing binaries that are of particular
    interest and merit further observations. The first category includes
    11 low-mass candidates, which may assist current efforts to explain
    the discrepancies between the observation and the models of stars at
    the bottom of the main sequence. The other two categories include 34
    binaries with eccentric orbits, and 20 binaries with abnormal light
    curves. Finally, this uniform catalog enabled us to identify a number
    of relations that provide further constraints on binary population
    models and tidal circularization theory.
Description:
    The data that we analyzed originate from ten fields of the
    Trans-atlantic Exoplanet Survey (TrES; Alonso et al.,
    2004ApJ...613L.153A 2004ApJ...613L.153A). TrES employs a network of three automated
    telescopes to survey 6°x6° fields-of-view. To avoid potential
    systematic noise, we use the data from only one telescope, Sleuth,
    located at the Palomar Observatory in Southern California.
File Summary:
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 FileName   Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe         80        .   This file
table1.dat     88       10   Observational parameters of the TrES fields
table7.dat    334      876   Eclipsing Binary catalog (773 stars)
table9.dat    457       88   EBs that appear in either the VSX or the SIMBAD
                             astronomical databases 
phot/*          .      773   Individual r-band normalized light curve
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See also:
  B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2010)
  B/vsx  : AAVSO International Variable Star Index VSX (Watson+, 2006-2010)
   V/115 : Semi-detached eclipsing binaries (Surkova+, 2004)
   V/118 : Catalog of eclipsing binaries parameters (Perevozkina+, 1999)
   V/119 : Catalogue of field contact binary stars (Pribulla+, 2003)
   V/120 : Catalog of early-type contact binaries (Bondarenko+, 1996)
   V/124 : Approximate elements of eclipsing binaries (Svechnikov+, 1990)
   V/121 : Catalog of DMS-type eclipsing binaries (Svechnikov+, 1999)
   J/A+A/337/403 : Low-mass stars evolutionary models (Baraffe+ 1998)
   http://www.cfa.harvard.edu/~jdevor/Catalog.html : online author's catalog
Byte-by-byte Description of file: table1.dat
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   Bytes Format Units   Label     Explanations
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   1-  4  A4    ---     Field     Field designation
   6- 20  A15   ---     Const     Constellation name
  22- 23  I2    h       RAh       Hour of right ascension (J2000) (1)
  25- 26  I2    min     RAm       Minute of right ascension (J2000)
  28- 34  F7.4  s       RAs       Second of right ascension (J2000)
      36  A1    ---     DE-       Declination sign (J2000) (1)
  37- 38  I2    deg     DEd       Degree of declination (J2000)
  40- 41  I2    arcmin  DEm       Arcminute of declination (J2000)
  43- 48  F6.3  arcsec  DEs       Arcsecond of declination (J2000)
  50- 55  F6.2  deg     GLON      Galactic longitude coordinate l
  57- 63  F7.2  deg     GLAT      Galactic latitude coordinate b
  65- 73  F9.1  d       T.start   Starting epoch (HJD)
  75- 83  F9.1  d       T.end     Ending epoch (HJD)
  85- 88  F4.1  d       Dur       Duration
--------------------------------------------------------------------------------
Note (1): ICRS 2000.0 coordinates of the guide star, which is located at
     the center of the field of view.
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Byte-by-byte Description of file: table7.dat
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   Bytes Format Units      Label  Explanations
--------------------------------------------------------------------------------
   1- 13  A13   ---        Cat    Eclipsing category (G1)
  15- 26  A12   ---     [DCO2008] Binary designation (2)
      27  A1    ---   f_[DCO2008] [*] Flag on T-Cas0-00524 (3)
  28- 29  I2    h          RAh    Hour of Right Ascension (J2000)
  31- 32  I2    min        RAm    Minute of Right Ascension (J2000)
  34- 39  F6.3  s          RAs    Second of Right Ascension (J2000)
      40  A1    ---        DE-    Declination sign (J2000)
  41- 42  I2    deg        DEd    Degree of Declination (J2000)
  44- 45  I2    arcmin     DEm    Arcminute of Declination (J2000)
  47- 51  F5.2  arcsec     DEs    Arcsecond of Declination (J2000)
  53- 63  F11.8 d          Per    Orbital period
  65- 74  F10.8 d        e_Per    Uncertainty in Per
  76- 83  F8.4 [solMass]   M1     ?=-99 Primary (more massive) component mass
  85- 92  F8.4 [solMass] e_M1     ? Uncertainty in M1
      93  A1    ---      f_M1     Flag on e_M1 (4)
  94-101  F8.4 [solMass]   M2     ?=-99 Secondary (less massive) component mass
 103-110  F8.4 [solMass] e_M2     ? Uncertainty in M2
     111  A1    ---      f_M2     Flag on e_M2 (4)
 112-119  F8.4  Gyr        Age    ?=-99 System age (assumed to be coeval)
 121-128  F8.4  Gyr      e_Age    ? Uncertainty in Age
     129  A1    ---      f_Age    Flag on e_Age (4)
 130-136  F7.3  ---        Score  ?=-99 Weighted reduced χ2 of MECI model
                                  (5)
 138-144  A7    ---        Iso    Isochrone table used (6)
 146-150  F5.1  ---        W      ?=-99 Relative weight of LC fit (5)
 152-158  A7    ---      r_pm     Proper motion measurement database (7)
 160-166  F7.1  mas/yr     pmRA   Right Ascension component of proper motion
 168-173  F6.1  mas/yr     pmDE   Declination component of proper motion
 175-178  F4.2  arcsec     epos   Distance between this work and proper
                                  motion database
 180-185  F6.3  mag        Bmag   ?=90 USNO-B B-band magnitude (8)
 187-192  F6.3  mag        Rmag   USNO-B R-band magnitude (8)
 194-199  F6.4  ---        3rd    Fraction of third-light flux blended (9)
 201-206  F6.3  mag        Jmag   2MASS J-band magnitude converted to ESO J-band
 208-213  F6.3  mag        Hmag   2MASS H-band magnitude converted to ESO H-band
 215-220  F6.3  mag        Kmag   2MASS Ks-band magnitude converted to ESO
                                  K-band
 222-228  F7.3  mag        JMAG   ?=-99 Absolute ESO J-band magnitude from
                                  isochrone table
 230-236  F7.3  mag        HMAG   ?=-99 Absolute ESO H-band magnitude from
                                  isochrone table
 238-244  F7.3  mag        KMAG   ?=-99 Absolute ESO K-band magnitude from
                                  isochrone table
 246-253  F8.3  pc         Dist   ?=-99 Distance from extinction-correct
                                  distance modulus
 255-261  F7.3  mag        AV     ?=-99 Galactic ISM V-band absorption
 263-271  F9.5  ---        sini   ?=-99 The sine of the orbital inclination
 273-280  F8.4  ---        ecosw  ?=-99 Robust lower eccentricity limit (10)
 282-289  F8.4  ---        e      ?=-99 Orbital eccentricity
 291-298  F8.4  ---      e_e      ? Uncertainty in e (-1 = assumed value)
     299  A1    ---      f_e      Fit at parameter bound on e_e (4)
 300-306  F7.3  mag        Dm1    ?=-99 R-band primary (deeper) eclipse depth
 308-316  F9.3  d          T0-1   ?=-99 Heliocentric Julian Date at center of
                                  primary eclipse
 318-324  F7.3  mag        Dm2    ?=-99 R-band secondary (shallower) eclipse
                                  depth
 326-334  F9.3  d          T0-2   ?=-99 Heliocentric Julian Date at center of
                                  secondary eclipse
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Note (2): Composed of the TrES field (see Table 1) and index.
          <[DCO2008] T-CCCN-NNNNN> in Simbad.
Note (3): Coordinates of T-Cas0-00524 have been corrected according to the
     online author's catalog erratum but as it was matched up with a wrong
     2MASS source, its listed colors and MECI analysis results are wrong.
     This target is a known Algol-type eclipsing binary, identified as 
     "V364 Cas" in the GCVS and Simbad.
Note (4): Flag as follows:
   -1 = one of the other parameters is at the upper/lower bound.
   -2 = the best fit is at the parameter lower bound.
   -3 = the best fit is at the parameter upper bound.
Note (5): MECI = Method for Eclipsing Component Identification, see Devor &
     Charbonneau (2006ApJ...653..647D 2006ApJ...653..647D) for futher details.
Note (6): References as follows:
        Y2 = Kim et al. (2002ApJS..143..499K 2002ApJS..143..499K);
   Baraffe = Baraffe et al. (1998, Cat. J/A+A/337/403);
       N/A = Not applicable.
Note (7): PM references as follows:
      UCAC = Zacharias et al. (2004, Cat I/289 superseded by UCAC3, Cat. I/315);
    USNO-B = Monet et al. (2003, Cat. I/284);
   Salim03 = Salim & Gould (2003, Revised NLTT, Cat. J/ApJ/582/1011).
Note (8): Average of both magnitude measurements, if available.
Note (9): i.e. the R-band flux within 30", excluding the target, divided by
          the total flux within 30".
Note (10): As in equation (1): ecosω~π/2xΔt/P 
     where P is the period.
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Byte-by-byte Description of file: table9.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 10  A10   ---     Cat       Eclipsing category (G1)
  12- 23  A12   ---     [DCO2008] Binary designation (T- FFFF-NNNNN)
  25- 26  I2    h       RAh       Hour of right ascension (J2000)
  28- 29  I2    min     RAm       Minute of right ascension (J2000)
  31- 36  F6.3  s       RAs       Second of right ascension (J2000)
      38  A1    ---     DE-       Declination sign (J2000)
  39- 40  I2    deg     DEd       Degree of declination (J2000)
  42- 43  I2    arcmin  DEm       Arcminute of declination (J2000)
  45- 49  F5.2  arcsec  DEs       Arcsecond of declination (J2000)
  51- 55  A5    ---     SpType    Spectral type
  57- 85  A29   ---     Otype     Object type
  87-457  A371  ---     Xid       VSX (International Variable Star Index) or
                                  SIMBAD identifiers
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Byte-by-byte Description of file: phot/*
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   Bytes Format Units   Label     Explanations
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   1- 16 F16.10 d       HJD       Heliocentric Julian Date minus 2400000
  18- 26  F9.6  ---     rmag      Normalized r-band magnitude
  28- 35  F8.6  ---   e_rmag      Magnitude uncertainty
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Global Notes:
Note (G1): The last step (10th) of the pipeline is to classify the resulting
     systems using both automatic and manual criteria. Seven groups are
     described as follows:
  Eccentric     = EBs with unequally-spaced eclipses
  Circular      = EBs with equally-spaced but distinct eclipses
  Ambig-unequal = Ambiguous-unequal: EBs with undetected secondary eclipses
  Ambig-equal   = Ambiguous-equal: EB with equally-spaced and indistinguishable
                  eclipses
  Inverted      = detached EBs that are not successfully modeled by MECI
  Roche-filled  = Roche-lobe-filling: non-detached EBs that are filling at least
                  one Roche-lobe
  Abnormal      = EBs with atypical out-of-eclipse distortions
History:
    From electronic version of the journal
(End)                 Greg Schwarz [AAS], Emmanuelle Perret [CDS]    24-Jun-2010