| I/355/paramp | Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) 1D astrophysical parameters produced by the Apsis processing chain developed in Gaia DPAC CU8 (1590932717 sources) (astrophysical_parameters) (original column names in green) (1590932717 rows) | -c=332.14208706103 +00.51190773843, eq=ICRS, rs=2 |
| Column | Value | Explain (UCD) | |
| _r | 0.000 | arcsec | Distance from center (332.14208706103+00.51190773843)[ICRS], at Epoch=J2016.0 (pos.angDistance) |
| _RAJ2000 | 22 08 34.1008946472 | "h:m:s" | Right ascension (FK5, Equinox=J2000.0) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.ra) |
| _DEJ2000 | +00 30 42.867858348 | "d:m:s" | Declination (FK5, Equinox=J2000.0) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.dec) |
| _RAB1950 | 22 06 00.5308808024 | "h:m:s" | Right ascension (FK4, Equinox=B1950.0) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.ra) |
| _DEB1950 | +00 15 59.623329213 | "d:m:s" | Declination (FK4, Equinox=B1950.0) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.eq.dec) |
| _Glon | 061.3893673477558 | deg | Galactic longitude at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.galactic.lon) |
| _Glat | -42.1020725691759 | deg | Galactic latitude at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services) (pos.galactic.lat) |
| source_id | 2681935329476252800 | (i) Source Identifier (source_id) (meta.id;meta.main) | |
| ra | 332.14208706103 | deg | (i) Right ascension (ICRS) at Ep=2016.0 (ra) (pos.eq.ra;meta.main) |
| dec | +00.51190773843 | deg | (i) Declination (ICRS) at Ep=2016.0 (dec) (pos.eq.dec;meta.main) |
| classprob_dsc_combmod_quasar | 0.00000000 | Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum) (classprob_dsc_combmod_quasar) (stat.probability) | |
| classprob_dsc_combmod_galaxy | 0.01902157 | Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_combmod_galaxy) (stat.probability) | |
| classprob_dsc_combmod_star | 0.98068929 | Probability from DSC-Combmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum) (classprob_dsc_combmod_star) (stat.probability) | |
| classprob_dsc_combmod_whitedwarf | 0.00028909 | Probability from DSC-Combmod of being a white dwarf (data used: BP/RP spectrum) (classprob_dsc_combmod_whitedwarf) (stat.probability) | |
| classprob_dsc_combmod_binarystar | 0.00000000 | Probability from DSC-Combmod of being a binary star (data used: BP/RP spectrum) (classprob_dsc_combmod_binarystar) (stat.probability) | |
| classprob_dsc_specmod_quasar | 0.00000000 | Probability from DSC-Specmod of being a quasar (data used: BP/RP spectrum) (classprob_dsc_specmod_quasar) (stat.probability) | |
| classprob_dsc_specmod_galaxy | 0.01902157 | Probability from DSC-Specmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_specmod_galaxy) (stat.probability) | |
| classprob_dsc_specmod_star | 0.98068929 | Probability from DSC-Specmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum) (classprob_dsc_specmod_star) (stat.probability) | |
| classprob_dsc_specmod_whitedwarf | 0.00028909 | Probability from DSC-Specmod of being a white dwarf (data used: BP/RP spectrum) (classprob_dsc_specmod_whitedwarf) (stat.probability) | |
| classprob_dsc_specmod_binarystar | 0.00000000 | Probability from DSC-Specmod of being a binary star (data used: BP/RP spectrum) (classprob_dsc_specmod_binarystar) (stat.probability) | |
| classprob_dsc_allosmod_quasar | Probability from DSC-Allosmod of being a quasar (data used: photometry) (classprob_dsc_allosmod_quasar) (stat.probability) | ||
| classprob_dsc_allosmod_galaxy | Probability from DSC-Allosmod of being a galaxy (data used: photometry) (classprob_dsc_allosmod_galaxy) (stat.probability) | ||
| classprob_dsc_allosmod_star | Probability from DSC-Allosmod of being a star (data used: photometry) (classprob_dsc_allosmod_star) (stat.probability) | ||
| teff_gspphot | K | Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot) (phys.temperature.effective) | |
| teff_gspphot_lower | K | Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_lower) (stat.value;phys.temperature.effective;stat.min) | |
| teff_gspphot_upper | K | Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_upper) (stat.value;phys.temperature.effective;stat.max) | |
| logg_gspphot | [cm/s2] | Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot) (phys.gravity) | |
| logg_gspphot_lower | [cm/s2] | Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_lower) (phys.gravity;stat.min) | |
| logg_gspphot_upper | [cm/s2] | Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_upper) (phys.gravity;stat.max) | |
| mh_gspphot | [-] | Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot) (phys.abund.Fe) | |
| mh_gspphot_lower | [-] | Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_lower) (phys.abund.Fe;stat.min) | |
| mh_gspphot_upper | [-] | Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_upper) (phys.abund.Fe;stat.max) | |
| distance_gspphot | pc | Distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot) (pos.distance) | |
| distance_gspphot_lower | pc | Lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_lower) (pos.distance;stat.min) | |
| distance_gspphot_upper | pc | Upper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_upper) (pos.distance;stat.max) | |
| azero_gspphot | mag | Monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot) (phys.absorption;em.opt.V) | |
| azero_gspphot_lower | mag | Lower confidence level (16%) of monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_lower) (phys.absorption;em.opt.V;stat.min) | |
| azero_gspphot_upper | mag | Upper confidence level (84%) of monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_upper) (phys.absorption;em.opt.V;stat.max) | |
| ag_gspphot | mag | Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot) (phys.absorption) | |
| ag_gspphot_lower | mag | Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_lower) (phys.absorption;em.opt;stat.min) | |
| ag_gspphot_upper | mag | Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_upper) (phys.absorption;em.opt;stat.max) | |
| abp_gspphot | mag | Extinction in GBP band from GSP-Phot Aeneas best library using BP/RP spectra (abp_gspphot) (phys.absorption;em.opt.B) | |
| abp_gspphot_lower | mag | Lower confidence level (16%) of extinction in GBP band from GSP-Phot Aeneas best library using BP/RP spectra (abp_gspphot_lower) (phys.absorption;em.opt.B;stat.min) | |
| abp_gspphot_upper | mag | Upper confidence level (84%) of extinction in GBP band from GSP-Phot Aeneas best library using BP/RP spectra (abp_gspphot_upper) (phys.absorption;em.opt.B;stat.max) | |
| arp_gspphot | mag | Extinction in GRP band from GSP-Phot Aeneas best library using BP/RP spectra (arp_gspphot) (phys.absorption;em.opt.R) | |
| arp_gspphot_lower | mag | Lower confidence level (16%) of extinction in GRP band from GSP-Phot Aeneas best library using BP/RP spectra (arp_gspphot_lower) (phys.absorption;em.opt.R;stat.min) | |
| arp_gspphot_upper | mag | Upper confidence level (84%) of extinction in GRP band from GSP-Phot Aeneas best library using BP/RP spectra (arp_gspphot_upper) (phys.absorption;em.opt.R;stat.max) | |
| ebpminrp_gspphot | mag | Reddening E(GBP-GRP) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot) (stat.value;phot.color.excess;em.opt) | |
| ebpminrp_gspphot_lower | mag | Lower confidence level (16%) of reddening E(GBP-GRP) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_lower) (phot.color.excess;em.opt;stat.min) | |
| ebpminrp_gspphot_upper | mag | Upper confidence level (84%) of reddening E(GBP-GRP) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_upper) (phot.color.excess;em.opt;stat.max) | |
| mg_gspphot | mag | Absolute magnitude MG from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot) (phys.magAbs;em.opt) | |
| mg_gspphot_lower | mag | Lower confidence level (16%) of absolute magnitude MG from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot_lower) (phys.magAbs;em.opt;stat.min) | |
| mg_gspphot_upper | mag | Upper confidence level (84%) of absolute magnitude MG from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot_upper) (phys.magAbs;em.opt;stat.max) | |
| radius_gspphot | solRad | Radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot) (phys.size.radius) | |
| radius_gspphot_lower | solRad | Lower confidence level (16%) of radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot_lower) (phys.size.radius;stat.min) | |
| radius_gspphot_upper | solRad | Upper confidence level (84%) of radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot_upper) (phys.size.radius;stat.max) | |
| logposterior_gspphot | Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC best library (logposterior_gspphot) (stat.fit.goodness) | ||
| mcmcaccept_gspphot | MCMC acceptance rate of GSP-Phot Aeneas MCMC best library (mcmcaccept_gspphot) (stat.value) | ||
| libname_gspphot | Name of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this table (libname_gspphot) (meta.record) | ||
| teff_gspspec | K | Effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec) (phys.temperature.effective;stat.median) | |
| teff_gspspec_lower | K | 16th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec_lower) (phys.temperature.effective;stat.min) | |
| teff_gspspec_upper | K | 84th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec_upper) (phys.temperature.effective;stat.max) | |
| logg_gspspec | [cm/s2] | Logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (logg_gspspec) (phys.gravity;stat.median) | |
| logg_gspspec_lower | [cm/s2] | 16th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (logg_gspspec_lower) (phys.gravity;stat.min) | |
| logg_gspspec_upper | [cm/s2] | 84th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (logg_gspspec_upper) (phys.gravity;stat.max) | |
| mh_gspspec | [-] | Global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mh_gspspec) (phys.abund.Fe;stat.median) | |
| mh_gspspec_lower | [-] | 16th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mh_gspspec_lower) (phys.abund.Fe;stat.min) | |
| mh_gspspec_upper | [-] | 84th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mh_gspspec_upper) (phys.abund.Fe;stat.max) | |
| alphafe_gspspec | [-] | Abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (alphafe_gspspec) (phys.abund;stat.median) | |
| alphafe_gspspec_lower | [-] | 16th percentile of the abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (alphafe_gspspec_lower) (phys.abund;stat.min) | |
| alphafe_gspspec_upper | [-] | 84th percentile of the abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (alphafe_gspspec_upper) (phys.abund;stat.max) | |
| fem_gspspec | [-] | Abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (fem_gspspec) (phys.abund.Fe;stat.median) | |
| fem_gspspec_lower | [-] | 16th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (fem_gspspec_lower) (phys.abund.Fe;stat.min) | |
| fem_gspspec_upper | [-] | 84th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (fem_gspspec_upper) (phys.abund.Fe;stat.max) | |
| fem_gspspec_nlines | [0/8] Number of lines used for [Fe/M] abundance estimation (fem_gspspec_nlines) (meta.number) | ||
| fem_gspspec_linescatter | [-] | Uncertainty estimation of [Fe/M] abundance using N lines of the element (fem_gspspec_linescatter) (stat.error;phys.abund.Z) | |
| sife_gspspec | [-] | Abundance of Silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sife_gspspec) (phys.abund.Z;stat.median) | |
| sife_gspspec_lower | [-] | 16th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sife_gspspec_lower) (phys.abund.Z;stat.min) | |
| sife_gspspec_upper | [-] | 84th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sife_gspspec_upper) (phys.abund.Z;stat.max) | |
| sife_gspspec_nlines | [0/3] Number of lines used for [Si/Fe] abundance estimation (sife_gspspec_nlines) (meta.number) | ||
| sife_gspspec_linescatter | [-] | Uncertainty estimation of [Si/Fe] abundance using N lines of the element (sife_gspspec_linescatter) (phys.abund.Z;stat.median) | |
| cafe_gspspec | [-] | Abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cafe_gspspec) (phys.abund.Z;stat.median) | |
| cafe_gspspec_lower | [-] | 16th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cafe_gspspec_lower) (phys.abund.Z;stat.min) | |
| cafe_gspspec_upper | [-] | 84th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cafe_gspspec_upper) (phys.abund.Z;stat.max) | |
| cafe_gspspec_nlines | [0/7] Number of lines used for [Ca/Fe] abundance estimation (cafe_gspspec_nlines) (meta.number) | ||
| cafe_gspspec_linescatter | [-] | Uncertainty estimation of [Ca/Fe] abundance using N lines of the element (cafe_gspspec_linescatter) (stat.error;phys.abund.Z) | |
| tife_gspspec | [-] | Abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (tife_gspspec) (phys.abund.Z;stat.median) | |
| tife_gspspec_lower | [-] | 16th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (tife_gspspec_lower) (phys.abund.Z;stat.min) | |
| tife_gspspec_upper | [-] | 84th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (tife_gspspec_upper) (phys.abund.Z;stat.max) | |
| tife_gspspec_nlines | [0/3] Number of lines used for [Ti/Fe] abundance estimation (tife_gspspec_nlines) (meta.number) | ||
| tife_gspspec_linescatter | [-] | Uncertainty estimation of [Ti/Fe] abundance using N lines of the element (tife_gspspec_linescatter) (stat.error;phys.abund.Z) | |
| mgfe_gspspec | [-] | Abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mgfe_gspspec) (phys.abund.Z;stat.median) | |
| mgfe_gspspec_lower | [-] | 16th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mgfe_gspspec_lower) (phys.abund.Z;stat.min) | |
| mgfe_gspspec_upper | [-] | 84th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mgfe_gspspec_upper) (phys.abund.Z;stat.max) | |
| ndfe_gspspec | [-] | Abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (ndfe_gspspec) (phys.abund.Z;stat.median) | |
| ndfe_gspspec_lower | [-] | 16th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (ndfe_gspspec_lower) (phys.abund.Z;stat.min) | |
| ndfe_gspspec_upper | [-] | 84th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (ndfe_gspspec_upper) (phys.abund.Z;stat.max) | |
| feiim_gspspec | [-] | Abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (feiim_gspspec) (phys.abund.Fe;stat.median) | |
| feiim_gspspec_lower | [-] | 16th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (feiim_gspspec_lower) (phys.abund.Fe;stat.min) | |
| feiim_gspspec_upper | [-] | 84th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (feiim_gspspec_upper) (phys.abund.Fe;stat.max) | |
| sfe_gspspec | [-] | Abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sfe_gspspec) (phys.abund.Z;stat.median) | |
| sfe_gspspec_lower | [-] | 16th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sfe_gspspec_lower) (phys.abund.Z;stat.min) | |
| sfe_gspspec_upper | [-] | 84th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sfe_gspspec_upper) (phys.abund.Z;stat.max) | |
| sfe_gspspec_nlines | [0/2] Number of lines used for [S/Fe] abundance estimation (sfe_gspspec_nlines) (meta.number) | ||
| sfe_gspspec_linescatter | [-] | Uncertainty estimation of [S/Fe] abundance using N lines of the element (sfe_gspspec_linescatter) (stat.error;phys.abund.Z) | |
| zrfe_gspspec | [-] | Abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (zrfe_gspspec) (phys.abund.Z;stat.median) | |
| zrfe_gspspec_lower | [-] | 16th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (zrfe_gspspec_lower) (phys.abund.Z;stat.min) | |
| zrfe_gspspec_upper | [-] | 84th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (zrfe_gspspec_upper) (phys.abund.Z;stat.max) | |
| nfe_gspspec | [-] | Abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nfe_gspspec) (phys.abund.Z;stat.median) | |
| nfe_gspspec_lower | [-] | 16th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nfe_gspspec_lower) (phys.abund.Z;stat.min) | |
| nfe_gspspec_upper | [-] | 84th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nfe_gspspec_upper) (phys.abund.Z;stat.max) | |
| nfe_gspspec_nlines | [0/2] Number of lines used for [N/Fe] abundance estimation (nfe_gspspec_nlines) (meta.number) | ||
| nfe_gspspec_linescatter | [-] | Uncertainty estimation of [N/Fe] abundance using N lines of the element (nfe_gspspec_linescatter) (stat.error;phys.abund.Z) | |
| crfe_gspspec | [-] | Abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (crfe_gspspec) (phys.abund.Z;stat.median) | |
| crfe_gspspec_lower | [-] | 16th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (crfe_gspspec_lower) (phys.abund.Z;stat.min) | |
| crfe_gspspec_upper | [-] | 84th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (crfe_gspspec_upper) (phys.abund.Z;stat.max) | |
| crfe_gspspec_nlines | [0/2] Number of lines used for [Cr/Fe] abundance estimation (crfe_gspspec_nlines) (meta.record) | ||
| crfe_gspspec_linescatter | [-] | Uncertainty estimation of [Cr/Fe] abundance using N lines of the element (crfe_gspspec_linescatter) (stat.error;phys.abund.Z) | |
| cefe_gspspec | [-] | Abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cefe_gspspec) (phys.abund.Z;stat.median) | |
| cefe_gspspec_lower | [-] | 16th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cefe_gspspec_lower) (phys.abund.Z;stat.min) | |
| cefe_gspspec_upper | [-] | 84th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cefe_gspspec_upper) (phys.abund.Z;stat.max) | |
| nife_gspspec | [-] | Abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nife_gspspec) (phys.abund.Z;stat.median) | |
| nife_gspspec_lower | [-] | 16th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nife_gspspec_lower) (phys.abund.Z;stat.min) | |
| nife_gspspec_upper | [-] | 84th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nife_gspspec_upper) (phys.abund.Z;stat.max) | |
| cn0ew_gspspec | nm | Equivalent width of cyoanogen line (cn0ew_gspspec) (spect.line.eqWidth) | |
| cn0ew_gspspec_uncertainty | nm | Uncertainty of equivalent width of cyanogen absorption line (cn0ew_gspspec_uncertainty) (stat.error;spect.line.eqWidth) | |
| cn0_gspspec_centralline | nm | Central wavelength of cyanogen line (cn0_gspspec_centralline) (em.wl.central) | |
| cn0_gspspec_width | nm | Width of cyoanogen line (cn0_gspspec_width) (spect.line.eqWidth) | |
| dib_gspspec_lambda | nm | DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra (dib_gspspec_lambda) (em.wl.central) | |
| dib_gspspec_lambda_uncertainty | nm | Uncertainty on DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra (dib_gspspec_lambda_uncertainty) (stat.error;em.wl.central) | |
| dibew_gspspec | 0.1nm | Equivalent width of the DIB from GSP-Spec MatisseGauguin using RVS spectra (dibew_gspspec) (stat.value;spect.line.eqWidth) | |
| dibew_gspspec_uncertainty | 0.1nm | Global uncertainty on DIB equivalent width value using DIB algorithm (dibew_gspspec_uncertainty) (stat.value;spect.line.eqWidth) | |
| dibewnoise_gspspec_uncertainty | 0.1nm | Uncertainty on DIB equivalent width value occuring from noise part (dibewnoise_gspspec_uncertainty) (stat.value;spect.line.eqWidth) | |
| dibp0_gspspec | Depth (p_0 parameter) of the DIB derived from a Gaussian model fit (dibp0_gspspec) (stat.fit.param) | ||
| dibp2_gspspec | 0.1nm | Width (p_2 parameter) of the DIB derived from a Gaussian model fit (dibp2_gspspec) (stat.fit.param) | |
| dibp2_gspspec_uncertainty | 0.1nm | Uncertainty on the dibp2Gspspec parameter (dibp2_gspspec_uncertainty) (stat.fit.param) | |
| dibqf_gspspec | [-2/5] Quality flag of the DIB computation (dibqf_gspspec) (meta.code.qual) | ||
| flags_gspspec | Catalogue flags for GSP-Spec MatisseGauguin (flags_gspspec) (Note 1) (meta.code.status) | ||
| logchisq_gspspec | Logarithm of the goodness-of-fit for the GSP-Spec MatisseGauguin parameters (logchisq_gspspec) (stat.fit.chi2) | ||
| ew_espels_halpha | nm | Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha) (spect.line.eqWidth) | |
| ew_espels_halpha_uncertainty | nm | Uncertainty of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_uncertainty) (stat.error;spect.line.eqWidth) | |
| ew_espels_halpha_flag | [0/9] Quality flag of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_flag) (meta.code.qual) | ||
| ew_espels_halpha_model | nm | Halpha pseudo-equivalent width from ESP-ELS measured on the synthetic spectrum (ew_espels_halpha_model) (spect.line.eqWidth) | |
| classlabel_espels | Adopted ELS class label from ESP-ELS (classlabel_espels) (meta.code.class) | ||
| classlabel_espels_flag | Quality flag of the adopted ELS class label from ESP-ELS (classlabel_espels_flag) (meta.code.class) | ||
| classprob_espels_wcstar | Probability from ESP-ELS of being a Wolf-Rayet star of type WC (classprob_espels_wcstar) (stat.probability) | ||
| classprob_espels_wnstar | Probability from ESP-ELS of being a Wolf-Rayet star of type WN (classprob_espels_wnstar) (stat.probability) | ||
| classprob_espels_bestar | Probability from ESP-ELS of being a Be Star (classprob_espels_bestar) (stat.probability) | ||
| classprob_espels_ttauristar | Probability from ESP-ELS of being a T Tauri Star (classprob_espels_ttauristar) (stat.probability) | ||
| classprob_espels_herbigstar | Probability from ESP-ELS of being a Herbig Ae/Be Star (classprob_espels_herbigstar) (stat.probability) | ||
| classprob_espels_dmestar | Probability from ESP-ELS of being an active M dwarf Star (classprob_espels_dmestar) (stat.probability) | ||
| classprob_espels_pne | Probability from ESP-ELS of being a planetary nebula (classprob_espels_pne) (stat.probability) | ||
| azero_esphs | mag | Monochromatic interstellar extinction (azero_esphs) (phys.absorption;em.opt.V) | |
| azero_esphs_uncertainty | mag | Uncertainty at a 68% confidence level on A0 from ESP-HS (azero_esphs_uncertainty) (stat.error;phys.absorption;em.opt.V) | |
| ag_esphs | mag | Intersterstellar extinction in G band from ESP-HS (ag_esphs) (phys.absorption;em.opt) | |
| ag_esphs_uncertainty | mag | Uncertainty on AG from ESP-HS (ag_esphs_uncertainty) (stat.error;phys.absorption;em.opt) | |
| ebpminrp_esphs | mag | Reddening E(GBP-GRP) from ESP-HS (ebpminrp_esphs) (phot.color.excess;em.opt) | |
| ebpminrp_esphs_uncertainty | mag | Uncertainty on E(GBP-GRP) from ESP-HS (ebpminrp_esphs_uncertainty) (stat.error;phot.color.excess;em.opt) | |
| teff_esphs | K | Effective temperature from ESP-HS (teff_esphs) (phys.temperature.effective) | |
| teff_esphs_uncertainty | K | Uncertainty at a 68% confidence level on the effective temperature from ESP-HS (teff_esphs_uncertainty) (stat.error;phys.temperature.effective) | |
| logg_esphs | [cm/s2] | Surface gravity from ESP-HS (logg_esphs) (phys.gravity) | |
| logg_esphs_uncertainty | [cm/s2] | Uncertainty at a 68% confidence level on the surface gravity from ESP-HS (logg_esphs_uncertainty) (stat.error;phys.gravity) | |
| vsini_esphs | km/s | Projected rotational velocity from ESP-HS (vsini_esphs) (phys.veloc.rotat) | |
| vsini_esphs_uncertainty | km/s | Uncertainty on the projected rotational velocity from ESP-HS (vsini_esphs_uncertainty) (stat.error;phys.veloc.rotat) | |
| flags_esphs | Quality flag of the ESP-HS parametrisation (flags_esphs) (Note 2) (meta.code.qual) | ||
| spectraltype_esphs | Spectral type from ESP-ELS (spectraltype_esphs) (src.spType) | ||
| activityindex_espcs | nm | Chromospheric activity index from ESP-CS (activityindex_espcs) (spect.index) | |
| activityindex_espcs_uncertainty | nm | Uncertainty in the chromospheric activity index from ESP-CS (activityindex_espcs_uncertainty) (stat.error;spect.index) | |
| activityindex_espcs_input | [12M] Source of input stellar parameters for the computation of the activity index by ESP-CS (activityindex_espcs_input) (meta.code) | ||
| teff_espucd | K | Effective temperature estimate from ESP-UCD based on the RP spectrum (teff_espucd) (phys.temperature.effective) | |
| teff_espucd_uncertainty | K | Uncertainty of the effective temperature estimate produced by ESP-UCD (teff_espucd_uncertainty) (stat.error;phys.temperature.effective) | |
| flags_espucd | [0/21] Quality flags of the ESP-UCD parameter estimates (flags_espucd) (Note 3) (meta.code.status) | ||
| radius_flame | Rsun | Radius of the star from FLAME using teff_gspphot and lum_flame (radius_flame) (phys.size.radius) | |
| radius_flame_lower | Rsun | Lower confidence level (16%) of radiusFlame (radius_flame_lower) (phys.size.radius;stat.min) | |
| radius_flame_upper | Rsun | Upper confidence level (84%) of radiusFlame (radius_flame_upper) (phys.size.radius;stat.max) | |
| lum_flame | Lsun | Luminosity of the star from FLAME using G band magnitude, extinction (ag_gspphot), parallax or distance, and a bolometric correction bc_flame (lum_flame) (phys.luminosity) | |
| lum_flame_lower | Lsun | Lower confidence level (16%) of lumFlame (lum_flame_lower) (phys.luminosity;stat.min) | |
| lum_flame_upper | Lsun | Upper confidence level (84%) of lumFlame (lum_flame_upper) (phys.luminosity;stat.max) | |
| mass_flame | Msun | Mass of the star from FLAME using stellar models, lum_flame, and teff_gspphot (mass_flame) (phys.mass) | |
| mass_flame_lower | Msun | Lower confidence level (16%) of mass of the star from FLAME (mass_flame_lower) (phys.mass;stat.min) | |
| mass_flame_upper | Msun | Upper confidence level (84%) of mass of the star from FLAME (mass_flame_upper) (phys.mass;stat.max) | |
| age_flame | Gyr | Age of the star from FLAME using stellar models (age_flame) (time.age) | |
| age_flame_lower | Gyr | Lower confidence level (84%) of age of the star from FLAME (age_flame_lower) (time.age;stat.min) | |
| age_flame_upper | Gyr | Upper confidence level (84%) of age of the star from FLAME (age_flame_upper) (time.age;stat.max) | |
| flags_flame | [0/22] Flags indicating quality and processing information from FLAME (flags_flame) (Note 4) (meta.code.qual) | ||
| evolstage_flame | Evolutionary stage of the star from FLAME using stellar models (evolstage_flame) (src.class) | ||
| gravredshift_flame | km/s | Gravitational redshift from FLAME using radiusFlame and loggGspphot (gravredshift_flame) (src.redshift) | |
| gravredshift_flame_lower | km/s | Lower confidence level (16%) of gravitational redshift from FLAME (gravredshift_flame_lower) (src.redshift;stat.min) | |
| gravredshift_flame_upper | km/s | Upper confidence level (84%) of gravitational redshift from FLAME (gravredshift_flame_upper) (src.redshift;stat.max) | |
| bc_flame | mag | Bolometric correction used to derive lumFlame (bc_flame) (phot.mag.bc) | |
| mh_msc | [-] | Metallicity of the source treated as a binary system from MSC using BP/RP spectra and parallax (mh_msc) (phys.abund) | |
| mh_msc_upper | [-] | Upper confidence level (84%) of the metallicity from MSC using BP/RP spectra and parallax (mh_msc_upper) (phys.abund;stat.max) | |
| mh_msc_lower | [-] | Lower confidence level (16%) of the metallicity from MSC using BP/RP spectra and parallax (mh_msc_lower) (phys.abund;stat.min) | |
| azero_msc | mag | Monochromatic extinction A0 at 541.4nm of the source treated as a binary system from MSC using BP/RP spectra and parallax (azero_msc) (phys.absorption;em.opt.V) | |
| azero_msc_upper | mag | Upper confidence level (84%) of monochromatic extinction A0 at 547.7nm from MSC using BP/RP spectra and parallax (azero_msc_upper) (phys.absorption;em.opt.V;stat.max) | |
| azero_msc_lower | mag | Lower confidence level (16%) of monochromatic extinction A0 at 547.7nm from MSC using BP/RP spectra and parallax (azero_msc_lower) (phys.absorption;em.opt.V;stat.min) | |
| distance_msc | pc | Distance from MSC using BP/RP spectra and parallax (distance_msc) (pos.distance) | |
| distance_msc_upper | pc | Upper confidence level (84%) of distance from MSC using BP/RP spectra and parallax (distance_msc_upper) (pos.distance;stat.max) | |
| distance_msc_lower | pc | Lower confidence level (16%) of distance from MSC using BP/RP spectra and parallax (distance_msc_lower) (pos.distance;stat.min) | |
| teff_msc1 | K | Effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1) (phys.temperature.effective) | |
| teff_msc1_upper | K | Upper confidence level (84%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_upper) (phys.temperature.effective;stat.max) | |
| teff_msc1_lower | K | Lower confidence level (16%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_lower) (phys.temperature.effective;stat.min) | |
| teff_msc2 | K | Effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2) (phys.temperature.effective) | |
| teff_msc2_upper | K | Upper confidence level (84%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_upper) (phys.temperature.effective;stat.max) | |
| teff_msc2_lower | K | Lower confidence level (16%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_lower) (phys.temperature.effective;stat.min) | |
| logg_msc1 | [cm/s2] | Surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1) (phys.gravity) | |
| logg_msc1_upper | [cm/s2] | Upper confidence level (84%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1_upper) (phys.gravity;stat.max) | |
| logg_msc1_lower | [cm/s2] | Lower confidence level (16%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1_lower) (phys.gravity;stat.min) | |
| logg_msc2 | [cm/s2] | Surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2) (phys.gravity) | |
| logg_msc2_upper | [cm/s2] | Upper confidence level (84%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2_upper) (phys.gravity;stat.max) | |
| logg_msc2_lower | [cm/s2] | Lower confidence level (16%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2_lower) (phys.gravity;stat.min) | |
| ag_msc | mag | Extinction in G band from MSC using BP/RP spectra and parallax (ag_msc) (phys.absorption) | |
| ag_msc_upper | mag | Upper confidence level (84%) of extinction in G band from MSC using BP/RP spectra and parallax (ag_msc_upper) (phys.absorption;stat.max) | |
| ag_msc_lower | mag | Lower confidence level (16%) of extinction in G band from MSC using BP/RP spectra and parallax (ag_msc_lower) (phys.absorption;stat.min) | |
| logposterior_msc | Goodness-of-fit score (normalised log-posterior) of MSC MCMC (logposterior_msc) (stat.fit.goodness) | ||
| mcmcaccept_msc | Mean MCMC acceptance rate of MSC MCMC (mcmcaccept_msc) (stat.fit.param) | ||
| mcmcdrift_msc | Mean drift of the MSC MCMC chain in units of parameter standard deviation (mcmcdrift_msc) (stat.fit.param) | ||
| flags_msc | [0/1] Flag indicating quality information from MSC (flags_msc) (Note 5) (meta.code.qual) | ||
| neuron_oa_id | Identifier of the OA SOM map neuron that represents the source (neuron_oa_id) (stat.fit.param) | ||
| neuron_oa_dist | Distance between the source XP spectra and the OA neuron XP prototype that represents the source (neuron_oa_dist) (stat.fit.param) | ||
| neuron_oa_dist_percentile_rank | [0/95] Percentile rank according to the distance distribution of the OA neuron that represents the source (neuron_oa_dist_percentile_rank) (stat.fit.param) | ||
| flags_oa | Flags indicating quality and processing information from OA (flags_oa) (Note 6) (meta.code.qual) | ||
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