| 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) | recno=1537 |
| Column | Value | Explain (UCD) | |
| 1537recno | 1537 | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) | |
| Ion | 23.00 | Ion code (G2) (Note 1) (meta.code;phys.atmol.ionStage) | |
| lambda | 6266 | 0.1nm | Line wavelength (em.wl;spect.line) |
| HD | 109358 | HD number (0 for Sun) (meta.id;meta.main) | |
| Teff | 5878.0 | 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 | 1.4 | 0.1pm | Equivalent width of the line (spect.line.eqWidth) |
| A(hfs) | 3.878 | Abundance obtained with hyperfine splitting (phys.abund) | |
| A(nohf) | 3.878 | Abundance obtained without hyperfine splitting (phys.abund) | |
| delta | 0.000 | hfs correction defined as A(hfs)-A(nohf) (phys.abund) | |
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