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J/AJ/134/926
  Chemical composition of V2314 Oph (Kim+, 2007)
Post annotation
  
1.J/AJ/134/926/table2Iron lines in the spectrum of V2314 Oph (168 rows)
2.J/AJ/134/926/table4Lines of other elements in the spectrum of V2314 Oph (111 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)
   (ALL)Wave 0.1nm Wavelength in Angstroms (em.wl)
  (1)Ion (char) Iron species (phys.atmol.element)
  (1)EW 0.1pm Equivalent width in milli-Angstroms (spect.line.eqWidth)
   (ALL)log(gf) [-] Log of the oscillator strength (phys.atmol.oscStrength)
   (ALL)Elow eV Energy of the low level (phys.energy;phys.atmol.level)
   (ALL)logN [-] Log of the iron number abundance (logH=12) (phys.abund)
  (2)Ion  Ion identification code (e.g. FeI = 26.00) (phys.atmol.element)
  (2)DlogN [-] Log of abundance difference from solar (Note 2)   (phys.abund)
  (2)logNSun [-] (n) Log of solar element abundance (Note 2)   (phys.abund)
  (2)bld   [0,1] Level of synthetic spectrum line blending in V2314 Oph (Note 3)   (meta.note)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)bldSun  (n) [0,1] Level of synthetic spectrum line blending in Sun (Note 3)   (meta.note)
  (2)Depth   [0,1] Synthetic spectrum line depth in V2314 Oph (phys.absorption.opticalDepth;spect.line)
  (2)DepthSun  (n) [0,1] Synthetic spectrum line depth in Sun (phot.flux.density;arith.ratio)
  (2)dlog(gf) [-] Change of log of the abundance for atmosphere model with log(gf) shifted by -0.2dex (stat.fit.param)
  (2)dTeff [-] Change of log of the abundance for atmosphere model with Teff shifted by +100K (stat.fit.param)

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