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  Properties of 160 F-K disk dwarfs/subgiants (Takeda+, 2007)
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1.J/PASJ/59/335/difResults of abundance corrections caused by inclusion of the hyper-fine splitting (hfs) effect for the relevant line (from tablee4) (2824 rows)

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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Ion  Ion code (G2) (Note 1)   (meta.code;phys.atmol.ionStage)
  lambda 0.1nm Line wavelength (em.wl;spect.line)
  HD  HD number (0 for Sun) (;meta.main)
  Teff K Effective temperature (phys.temperature.effective)
  logg [m/s2] Logarithmic surface gravity (phys.gravity)
  vt km/s Microturbulent velocity (phys.veloc)
  [Fe/H]  Fe abundance relative to the Sun (phys.abund.Fe)
  EW 0.1pm Equivalent width of the line (spect.line.eqWidth)
  A(hfs)  Abundance obtained with hyperfine splitting (phys.abund)
  A(nohf)  Abundance obtained without hyperfine splitting (phys.abund)
  delta  hfs correction defined as A(hfs)-A(nohf) (phys.abund)

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