J/AJ/139/1338       UV-selected stars in Tau and Upper Sco   (Findeisen+, 2010)
Ultraviolet-selected field and pre-main-sequence stars toward Taurus and
upper Scorpius.
    Findeisen K., Hillenbrand L.
   <Astron. J., 139, 1338-1359 (2010)>
   =2010AJ....139.1338F 2010AJ....139.1338F
ADC_Keywords: Associations, stellar ; Stars, pre-main sequence ;
              Photometry, ultraviolet ; Photometry, infrared
Keywords: Galaxy: stellar content - stars: activity - stars: pre-main sequence -
          ultraviolet: stars
Abstract:
    We have carried out a Galaxy Evolution Explorer (GALEX) Cycle 1 guest
    investigator program covering 56deg2 near the Taurus T association
    and 12deg2 along the northern edge of the Upper Scorpius OB
    association. We combined photometry in the GALEX far-ultraviolet and
    near-ultraviolet bands with data from the Two Micron All Sky Survey to
    identify candidate young (≲100Myr old) stars as those with an
    ultraviolet excess relative to older main-sequence stars. Follow-up
    spectroscopy of a partial sample of these candidates suggests five new
    members of Taurus, with 8-20 expected from additional observations,
    and five new members of Upper Scorpius, with three to six expected
    from additional observations.
File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table6.dat    188      567   Sources with a 3σ or greater UV excess
                             in at least one band
table8.dat    147       64   UV excess stars observed at Palomar
table11.dat    66        9  *Spectroscopic candidate members of Taurus and
                             Upper Scorpius
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Note on table11.dat: These are the emission-line stars with spectral type and
   CMD location consistent with Taurus or Upper Scorpius membership. We also
   present proper motions and errors calculated by A. Kraus (2009, private
   communication) from published positions along with a qualitative indication
   of whether the proper motion is consistent with membership in the Taurus or
   Upper Scorpius association, respectively.
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See also:
    II/246 :  2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)
Byte-by-byte Description of file: table6.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 16  A16   ---     2MASS     2MASS identification (HHMMSSss+DDMMSSs, J2000)
  18- 27  F10.6 deg     RAdeg     Right Ascension in decimal degrees (J2000)
  29- 38  F10.6 deg     DEdeg     Declination in decimal degrees (J2000)
  40- 57  A18   ---     GALEX     GALEX tile identification
  59- 64  F6.3  mag     FUV       ? GALEX FUV band AB magnitude
  66- 70  F5.3  mag   e_FUV       ? The 1σ uncertainty in FUV
  72- 77  F6.3  mag     NUV       ? GALEX NUV band AB magnitude
  79- 83  F5.3  mag   e_NUV       ? The 1σ uncertainty in NUV
  85- 90  F6.3  mag     Jmag      2MASS J band Vega magnitude
  92- 96  F5.3  mag   e_Jmag      The 1σ uncertainty in Jmag
  98-103  F6.3  mag     Hmag      2MASS H band Vega magnitude
 105-109  F5.3  mag   e_Hmag      The 1σ uncertainty in Hmag
 111-116  F6.3  mag     Ksmag     2MASS Ks band Vega magnitude
 118-122  F5.3  mag   e_Ksmag     The 1σ uncertainty in Ksmag
 124-126  A3    ---     Qual      JHK band photometry quality
 128-131  F4.1  mag     DFUV      ? GALEX FUV band excess magnitude
 133-135  F3.1  mag   e_DFUV      ? The 1σ uncertainty in DFUV  
 137-140  F4.1  ---     RFUV      ? FUV excess to σ ratio
 142-145  F4.1  mag     DNUV      ? GALEX NUV band excess magnitude
 147-149  F3.1  mag   e_DNUV      ? The 1σ uncertainty in DNUV
 151-154  F4.1  ---     RNUV      ? NUV excess to σ ratio
 156-184  A29   ---     OName     Other identifier (1)
 186-188  A3    ---     Mmb       [Yes No] Previously known member? (1)
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Note (1): If we know of an association between the GALEX source and a known
  object, and if the literature confirms or rules out membership in
  Taurus or Upper Scorpius, we list the information in the last two
  columns. Our list of associations is not complete.
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Byte-by-byte Description of file: table8.dat
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   Bytes Format Units  Label   Explanations
--------------------------------------------------------------------------------
   1-  4  A4    ---    Zone    [Tau USco] Tau for Taurus, USco for Upper Sco
   6- 21  A16   ---    2MASS   2MASS identification (HHMMSSss+DDMMSSs, J2000)
  23- 43  A21   ---    OName   Previous Literature designation (1)
  45- 46  A2    ---    Mmb     Membership (M=member, nM=non-member)
                                 from previous Literature (1)
  48- 52  F5.2  mag    FUV     ? GALEX FUV band AB magnitude
  54- 58  F5.2  mag    NUV     ? GALEX NUV band AB magnitude
  60- 64  F5.2  mag    Jmag    2MASS J band Vega magnitude
  66- 70  F5.2  mag    Ksmag   2MASS Ks band Vega magnitude
  72- 75  F4.1  mag    DFUV    ? GALEX FUV band excess magnitude
  77- 80  F4.1  ---    DFUVs   ? GALEX FUV band excess magnitude in σ unit
  82- 85  F4.1  mag    DNUV    ? GALEX NUV band excess magnitude
  87- 90  F4.1  ---    DNUVs   ? GALEX NUV band excess magnitude in σ unit
  92-107  A16   ---    SpType  MK spectral type
 108-114  F7.3  0.1nm  WCaIIk  ? CaII-K equivalent width
     115  A1    ---- n_WCaIIk  [a] Note for no-measurement (2)
 116-122  F7.3  0.1nm  WCaIIh  ? CaII-H equivalent width
     123  A1    ---- n_WCaIIh  [abc] Note for no-measurement (2)
 124-130  F7.4  0.1nm  WHb     ? Hβ equivalent width
     131  A1    ---- n_WHb     [abd] Note for no-measurement (2)
 132-138  F7.4  0.1nm  WHa     ? Hα equivalent width
     139  A1    ---- n_WHa     [ab] Note for no-measurement (2)
     141  A1    ---  l_WLi     Limit flag on WLi
 142-147  F6.4  0.1nm  WLi     ? Lithium equivalent width
--------------------------------------------------------------------------------
Note (1): If we know of an association between the GALEX source and a known
   object, and if the literature confirms or rules out membership in Taurus or
   Upper Scorpius, we list the information.
Note (2): Notes give reason why we could not measure emission equivalent width
    as follows :
    a = Core emission line in an absorption line
    b = Self-absorbed profile
    c = Inverse P Cygni profile
    d = Core emission line in an absorption line and self-absorbed profile
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Byte-by-byte Description of file: table11.dat
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   Bytes Format Units     Label    Explanations
--------------------------------------------------------------------------------
   1-  4  A4    ---       Zone     [Tau USco] Tau for Taurus, USco for Upper Sco
   6- 21  A16   ---       2MASS    2MASS name
  23- 34  A12   ---       SpType   MK spectral type
  37- 45  A9    ---       Ind      Youth indicators
  48- 52  F5.1  mas/yr    pmRA     Proper motion along RA
  54- 58  F5.1  mas/yr    pmDE     Proper motion along DE
  60- 62  F3.1  mas/yr  e_pm       rms uncertainty on proper motions
  64- 66  A3    ---       Mmb      [Yes No] Proper-motion member?
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History:
    From electronic version of the journal
(End)                  Greg Schwarz [AAS], Patricia Vannier [CDS]    21-May-2012