| Show | Sort | Column | Constraint | Explain (UCD) |
| | | recno | | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) (RECORD) |
| | | Object | (char) | Object name used in this study (meta.id;meta.main) (ID_MAIN) |
| | | Species | (char) | Name of the species (phys.atmol.element) (AT_SPECIES) |
| | | lambda | 0.1nm | Wavelength (em.wl) (SPECT_WAVELENGTH_MISC) |
| | | chi | eV | Excitation potential (phys.atmol.excitation) (AT_ENERGY_EXCIT) |
| | | loggf | | log gf value (phys.absorption.coeff) (AT_OSC_STRENGTH) |
| | | EW | 0.1pm | Equivalent width (in mÅ) (spect.line.eqWidth) (SPECT_EQ-WIDTH) |
| | | e_EW | 0.1pm | Uncertainty in equivalent width (in mÅ) (stat.error;spect.line.eqWidth) (ERROR) |
| | | A | | Abundance from this line (phys.abund) (PHYS_ABUND_MISC) |
| | | eATeff | | Uncertainty in abundance due to effective temperature (stat.error) (ERROR) |
| | | eAlogg | | Uncertainty in abundance due to surface gravity (stat.error) (ERROR) |
| | | eAvt | | Uncertainty in abundance due to microturbulent velocity (stat.error) (ERROR) |
| | | eA[Fe/H] | | Uncertainty in abundance due to metallicity (stat.error) (ERROR) |
| | | eAEW | | Uncertainty in abundance due to equivalent widths of this star and the reference star (stat.error) (ERROR) |
| | | sX | | Uncertainty floor (stat.error) (ERROR) |
| | | Weight | | Weight used to obtain the best estimate for the abundance of the species (phys.atmol.weight;meta.modelled) (WEIGHT) |
ALL cols | | | |