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J/PASJ/59/335/dif Properties of 160 F-K disk dwarfs/subgiants (Takeda+, 2007)
Results 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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ColumnValue  Explain   (UCD)
1081recno 1081  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)

Ion23.00  Ion code (G2) (Note 1)   (meta.code;phys.atmol.ionStage)
lambda5657 0.1nm Line wavelength (em.wl;spect.line)
HD109358  HD number (0 for Sun) (;meta.main)
Teff5878.0 K Effective temperature (phys.temperature.effective)
logg 4.390 [m/s2] Logarithmic surface gravity (phys.gravity)
vt 1.14 km/s Microturbulent velocity (phys.veloc)
[Fe/H]-0.215  Fe abundance relative to the Sun (phys.abund.Fe)
EW 3.0 0.1pm Equivalent width of the line (spect.line.eqWidth)
A(hfs) 3.757  Abundance obtained with hyperfine splitting (phys.abund)
A(nohf) 3.758  Abundance obtained without hyperfine splitting (phys.abund)
delta-0.001  hfs correction defined as A(hfs)-A(nohf) (phys.abund)
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