| Show | Sort | Column | Constraint | Explain (UCD) |
| | | recno | | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) (RECORD) |
| | | Ion | | Ion identification code (e.g. FeI = 26.00) (phys.atmol.element) (AT_ELEMENT) |
| | | Wave | 0.1nm | Wavelength in Angstroms (em.wl) (SPECT_WAVELENGTH_MISC) |
| | | log(gf) | [-] | Log of the oscillator strength (phys.atmol.oscStrength) (AT_OSC_STRENGTH) |
| | | Elow | eV | Excitation energy (phys.atmol.excitation) (AT_ENERGY_EXCIT) |
| | | DlogN | [-] | Log of abundance difference from solar (Note 2)
(phys.abund) (PHYS_ABUND_MISC) |
| | | logN | [-] | Log of V2314 Oph element abundance (phys.abund) (PHYS_ABUND_MISC) |
| | | logNSun | [-] | (n) Log of solar element abundance (Note 2)
(phys.abund) (PHYS_ABUND_MISC) |
| | | bld | | [0,1] Level of synthetic spectrum line blending in V2314 Oph (Note 3)
(meta.note) (SPECT_PECUL) |
| | | bldSun | | (n) [0,1] Level of synthetic spectrum line blending in Sun (Note 3)
(meta.note) (SPECT_PECUL) |
| | | Depth | | [0,1] Synthetic spectrum line depth in V2314 Oph (phys.absorption.opticalDepth;spect.line) (SPECT_LINE_DEPTH_VALUE) |
| | | DepthSun | | (n) [0,1] Synthetic spectrum line depth in Sun (phot.flux.density;arith.ratio) (SPECT_LINE_DEPTH_VALUE) |
| | | dlog(gf) | [-] | Change of log of the abundance for atmosphere model with log(gf) shifted by -0.2dex (stat.fit.param) (FIT_PARAM_VALUE) |
| | | dTeff | [-] | Change of log of the abundance for atmosphere model with Teff shifted by +100K (stat.fit.param) (FIT_PARAM_VALUE) |
ALL cols | | | |