VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

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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=017.19247207502 +86.25704383383, eq=ICRS, rs=2
Post annotation about this record
ColumnValue  Explain   (UCD)
_r0.000 arcsec Distance from center (017.19247207502+86.25704383383)[ICRS], at Epoch=J2016.0 (pos.angDistance)
_RAJ200001 08 46.1932980048 "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+86 15 25.357801788 "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)
_RAB195001 01 35.8406892502 "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+85 59 23.933284255 "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)
_Glon123.2398241686440 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+23.3956614332985 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 574112955678493824  (i) Source Identifier (source_id) (meta.id;meta.main)
ra017.19247207502 deg (i) Right ascension (ICRS) at Ep=2016.0 (ra) (pos.eq.ra;meta.main)
dec+86.25704383383 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 0.00000000   Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_combmod_galaxy) (stat.probability)
classprob_dsc_combmod_star 0.99995494   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 0.00000000   Probability from DSC-Combmod of being a white dwarf (data used: BP/RP spectrum) (classprob_dsc_combmod_whitedwarf) (stat.probability)
classprob_dsc_combmod_binarystar 0.00004504   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 0.00000000   Probability from DSC-Specmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_specmod_galaxy) (stat.probability)
classprob_dsc_specmod_star 0.99550790   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 0.00000771   Probability from DSC-Specmod of being a white dwarf (data used: BP/RP spectrum) (classprob_dsc_specmod_whitedwarf) (stat.probability)
classprob_dsc_specmod_binarystar 0.00448446   Probability from DSC-Specmod of being a binary star (data used: BP/RP spectrum) (classprob_dsc_specmod_binarystar) (stat.probability)
classprob_dsc_allosmod_quasar 0.00000000   Probability from DSC-Allosmod of being a quasar (data used: photometry) (classprob_dsc_allosmod_quasar) (stat.probability)
classprob_dsc_allosmod_galaxy 0.00000000   Probability from DSC-Allosmod of being a galaxy (data used: photometry) (classprob_dsc_allosmod_galaxy) (stat.probability)
classprob_dsc_allosmod_star 1.00000000   Probability from DSC-Allosmod of being a star (data used: photometry) (classprob_dsc_allosmod_star) (stat.probability)
teff_gspphot 4707.5229 K Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot) (phys.temperature.effective)
teff_gspphot_lower 4703.7798 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 4709.4229 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 2.2063 [cm/s2] Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot) (phys.gravity)
logg_gspphot_lower 2.1957 [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 2.2182 [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 0.2232 [-] Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot) (phys.abund.Fe)
mh_gspphot_lower 0.2164 [-] 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 0.2304 [-] 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 97.7160 pc Distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot) (pos.distance)
distance_gspphot_lower 96.1338 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 98.5335 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 0.2920 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 0.2882 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 0.2943 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 0.2252 mag Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot) (phys.absorption)
ag_gspphot_lower 0.2221 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 0.2269 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 0.2891 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 0.2853 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 0.2914 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 0.1727 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 0.1704 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 0.1740 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 0.1164 mag Upper confidence level (84%) of 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 0.1148 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 0.1174 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-1.2695 mag Absolute magnitude MG from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot) (phys.magAbs;em.opt)
mg_gspphot_lower-1.2836 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-1.2340 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 25.0103 solRad Radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot) (phys.size.radius)
radius_gspphot_lower 24.5725 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 25.2860 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-6.897952e+03   Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC best library (logposterior_gspphot) (stat.fit.goodness)
mcmcaccept_gspphot 0.308307201   MCMC acceptance rate of GSP-Phot Aeneas MCMC best library (mcmcaccept_gspphot) (stat.value)
libname_gspphotMARCS  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 4455.0 K Effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec) (phys.temperature.effective;stat.median)
teff_gspspec_lower 4450.0 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 4458.0 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 1.56 [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 1.55 [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 1.57 [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 0.00 [-] 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 0.00 [-] 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 0.01 [-] 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-0.08 [-] 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-0.09 [-] 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-0.08 [-] 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-0.15 [-] 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-0.19 [-] 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-0.12 [-] 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_nlines8   [0/8] Number of lines used for [Fe/M] abundance estimation (fem_gspspec_nlines) (meta.number)
fem_gspspec_linescatter 0.14 [-] Uncertainty estimation of [Fe/M] abundance using N lines of the element (fem_gspspec_linescatter) (stat.error;phys.abund.Z)
sife_gspspec-0.06 [-] 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-0.11 [-] 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-0.01 [-] 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_nlines3   [0/3] Number of lines used for [Si/Fe] abundance estimation (sife_gspspec_nlines) (meta.number)
sife_gspspec_linescatter 0.02 [-] Uncertainty estimation of [Si/Fe] abundance using N lines of the element (sife_gspspec_linescatter) (phys.abund.Z;stat.median)
cafe_gspspec-0.09 [-] 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-0.09 [-] 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-0.09 [-] 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_nlines7   [0/7] Number of lines used for [Ca/Fe] abundance estimation (cafe_gspspec_nlines) (meta.number)
cafe_gspspec_linescatter 0.01 [-] Uncertainty estimation of [Ca/Fe] abundance using N lines of the element (cafe_gspspec_linescatter) (stat.error;phys.abund.Z)
tife_gspspec-0.10 [-] 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-0.14 [-] 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-0.05 [-] 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_nlines2   [0/3] Number of lines used for [Ti/Fe] abundance estimation (tife_gspspec_nlines) (meta.number)
tife_gspspec_linescatter 0.07 [-] Uncertainty estimation of [Ti/Fe] abundance using N lines of the element (tife_gspspec_linescatter) (stat.error;phys.abund.Z)
mgfe_gspspec 0.15 [-] 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 0.11 [-] 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 0.18 [-] 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-0.11 [-] 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-0.12 [-] 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-0.09 [-] 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_nlines2   [0/2] Number of lines used for [N/Fe] abundance estimation (nfe_gspspec_nlines) (meta.number)
nfe_gspspec_linescatter 0.01 [-] Uncertainty estimation of [N/Fe] abundance using N lines of the element (nfe_gspspec_linescatter) (stat.error;phys.abund.Z)
crfe_gspspec 0.12 [-] 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 0.02 [-] 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 0.20 [-] 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_nlines1   [0/2] Number of lines used for [Cr/Fe] abundance estimation (crfe_gspspec_nlines) (meta.record)
crfe_gspspec_linescatter 0.00 [-] Uncertainty estimation of [Cr/Fe] abundance using N lines of the element (crfe_gspspec_linescatter) (stat.error;phys.abund.Z)
cefe_gspspec-0.02 [-] 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-0.18 [-] 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 0.14 [-] 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-0.06 [-] 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-0.10 [-] 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-0.02 [-] 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 0.02 nm Equivalent width of cyoanogen line (cn0ew_gspspec) (spect.line.eqWidth)
cn0ew_gspspec_uncertainty 0.02 nm Uncertainty of equivalent width of cyanogen absorption line (cn0ew_gspspec_uncertainty) (stat.error;spect.line.eqWidth)
cn0_gspspec_centralline862.87 nm Central wavelength of cyanogen line (cn0_gspspec_centralline) (em.wl.central)
cn0_gspspec_width 0.24 nm Width of cyoanogen line (cn0_gspspec_width) (spect.line.eqWidth)
dib_gspspec_lambda861.75781 nm DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra (dib_gspspec_lambda) (em.wl.central)
dib_gspspec_lambda_uncertainty 0.00198 nm Uncertainty on DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra (dib_gspspec_lambda_uncertainty) (stat.error;em.wl.central)
dibew_gspspec 1.7999999e-02 0.1nm Equivalent width of the DIB from GSP-Spec MatisseGauguin using RVS spectra (dibew_gspspec) (stat.value;spect.line.eqWidth)
dibew_gspspec_uncertainty 2.5000000e-02 0.1nm Global uncertainty on DIB equivalent width value using DIB algorithm (dibew_gspspec_uncertainty) (stat.value;spect.line.eqWidth)
dibewnoise_gspspec_uncertainty 6e-04 0.1nm Uncertainty on DIB equivalent width value occuring from noise part (dibewnoise_gspspec_uncertainty) (stat.value;spect.line.eqWidth)
dibp0_gspspec-2.720000e-02   Depth (p_0 parameter) of the DIB derived from a Gaussian model fit (dibp0_gspspec) (stat.fit.param)
dibp2_gspspec 0.2661 0.1nm Width (p_2 parameter) of the DIB derived from a Gaussian model fit (dibp2_gspspec) (stat.fit.param)
dibp2_gspspec_uncertainty 0.0171 0.1nm Uncertainty on the dibp2Gspspec parameter (dibp2_gspspec_uncertainty) (stat.fit.param)
dibqf_gspspec 5   [-2/5] Quality flag of the DIB computation (dibqf_gspspec) (meta.code.qual)
flags_gspspec00000000000000010009900000000990099229905   Catalogue flags for GSP-Spec MatisseGauguin (flags_gspspec) (Note 1)   (meta.code.status)
logchisq_gspspec-4.09442997   Logarithm of the goodness-of-fit for the GSP-Spec MatisseGauguin parameters (logchisq_gspspec) (stat.fit.chi2)
ew_espels_halpha -0.12030 nm Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha) (spect.line.eqWidth)
ew_espels_halpha_uncertainty 0.02835 nm Uncertainty of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_uncertainty) (stat.error;spect.line.eqWidth)
ew_espels_halpha_flag1   [0/9] Quality flag of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_flag) (meta.code.qual)
ew_espels_halpha_model 0.044750 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 92   Quality flag of the ESP-HS parametrisation (flags_esphs) (Note 2)   (meta.code.qual)
spectraltype_esphsK  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 23.7733 Rsun Radius of the star from FLAME using teff_gspphot and lum_flame (radius_flame) (phys.size.radius)
radius_flame_lower 23.2411 Rsun Lower confidence level (16%) of radiusFlame (radius_flame_lower) (phys.size.radius;stat.min)
radius_flame_upper 24.3133 Rsun Upper confidence level (84%) of radiusFlame (radius_flame_upper) (phys.size.radius;stat.max)
lum_flame 2.499e+02 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 2.448e+02 Lsun Lower confidence level (16%) of lumFlame (lum_flame_lower) (phys.luminosity;stat.min)
lum_flame_upper 2.552e+02 Lsun Upper confidence level (84%) of lumFlame (lum_flame_upper) (phys.luminosity;stat.max)
mass_flame 3.801 Msun Mass of the star from FLAME using stellar models, lum_flame, and teff_gspphot (mass_flame) (phys.mass)
mass_flame_lower 3.761 Msun Lower confidence level (16%) of mass of the star from FLAME (mass_flame_lower) (phys.mass;stat.min)
mass_flame_upper 3.841 Msun Upper confidence level (84%) of mass of the star from FLAME (mass_flame_upper) (phys.mass;stat.max)
age_flame 0.202 Gyr Age of the star from FLAME using stellar models (age_flame) (time.age)
age_flame_lower 0.200 Gyr Lower confidence level (84%) of age of the star from FLAME (age_flame_lower) (time.age;stat.min)
age_flame_upper 0.221 Gyr Upper confidence level (84%) of age of the star from FLAME (age_flame_upper) (time.age;stat.max)
flags_flame10   [0/22] Flags indicating quality and processing information from FLAME (flags_flame) (Note 4)   (meta.code.qual)
evolstage_flame 659   Evolutionary stage of the star from FLAME using stellar models (evolstage_flame) (src.class)
gravredshift_flame 0.09381264 km/s Gravitational redshift from FLAME using radiusFlame and loggGspphot (gravredshift_flame) (src.redshift)
gravredshift_flame_lower 0.09290801 km/s Lower confidence level (16%) of gravitational redshift from FLAME (gravredshift_flame_lower) (src.redshift;stat.min)
gravredshift_flame_upper 0.09449151 km/s Upper confidence level (84%) of gravitational redshift from FLAME (gravredshift_flame_upper) (src.redshift;stat.max)
bc_flame-0.0817268 mag Bolometric correction used to derive lumFlame (bc_flame) (phot.mag.bc)
mh_msc 0.499242 [-] Metallicity of the source treated as a binary system from MSC using BP/RP spectra and parallax (mh_msc) (phys.abund)
mh_msc_upper 0.500000 [-] 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 0.483402 [-] Lower confidence level (16%) of the metallicity from MSC using BP/RP spectra and parallax (mh_msc_lower) (phys.abund;stat.min)
azero_msc 0.352583 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 1.777911 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 0.000000 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 10.128 pc Distance from MSC using BP/RP spectra and parallax (distance_msc) (pos.distance)
distance_msc_upper 10.987 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 10.000 pc Lower confidence level (16%) of distance from MSC using BP/RP spectra and parallax (distance_msc_lower) (pos.distance;stat.min)
teff_msc14598.9883 K Effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1) (phys.temperature.effective)
teff_msc1_upper4609.4375 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_lower4572.8115 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_msc24136.0947 K Effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2) (phys.temperature.effective)
teff_msc2_upper4312.6719 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_lower3952.6523 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 4.4580 [cm/s2] Surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1) (phys.gravity)
logg_msc1_upper 4.7502 [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 3.9482 [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 4.5406 [cm/s2] Surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2) (phys.gravity)
logg_msc2_upper 5.2000 [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 4.4829 [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 0.264381 mag Extinction in G band from MSC using BP/RP spectra and parallax (ag_msc) (phys.absorption)
ag_msc_upper 1.297357 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 0.000000 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-3.6200262e+05   Goodness-of-fit score (normalised log-posterior) of MSC MCMC (logposterior_msc) (stat.fit.goodness)
mcmcaccept_msc 0.244534612   Mean MCMC acceptance rate of MSC MCMC (mcmcaccept_msc) (stat.fit.param)
mcmcdrift_msc 3.529283e-01   Mean drift of the MSC MCMC chain in units of parameter standard deviation (mcmcdrift_msc) (stat.fit.param)
flags_msc1   [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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