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=292.05541201126 +00.12039241991, eq=ICRS, rs=2
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ColumnValue  Explain   (UCD)
_r0.000 arcsec Distance from center (292.05541201126+00.12039241991)[ICRS], at Epoch=J2016.0 (pos.angDistance)
_RAJ200019 28 13.2988827031 "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 07 13.412711663 "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)
_RAB195019 25 39.5813210115 "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 01 02.341985476 "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)
_Glon037.2617759069191 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-08.1214298827534 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_id4263427122083992960  (i) Source Identifier (source_id) (meta.id;meta.main)
ra292.05541201126 deg (i) Right ascension (ICRS) at Ep=2016.0 (ra) (pos.eq.ra;meta.main)
dec+00.12039241991 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 0.99999560   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 0.00000440   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 0.99956006   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 0.00000000   Probability from DSC-Specmod of being a white dwarf (data used: BP/RP spectrum) (classprob_dsc_specmod_whitedwarf) (stat.probability)
classprob_dsc_specmod_binarystar 0.00043991   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 5047.7773 K Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot) (phys.temperature.effective)
teff_gspphot_lower 5022.4824 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 5072.7905 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 3.7100 [cm/s2] Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot) (phys.gravity)
logg_gspphot_lower 3.6651 [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 3.7406 [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-0.1603 [-] Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot) (phys.abund.Fe)
mh_gspphot_lower-0.1633 [-] 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-0.1578 [-] 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 1948.5518 pc Distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot) (pos.distance)
distance_gspphot_lower 1885.6309 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 2044.5452 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 1.1994 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 1.1778 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 1.2227 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 0.9209 mag Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot) (phys.absorption)
ag_gspphot_lower 0.9035 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 0.9396 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 1.1957 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 1.1733 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 1.2196 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 0.7053 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 0.6924 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 0.7191 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 0.4903 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 0.4808 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 0.5005 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 3.5944 mag Absolute magnitude MG from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot) (phys.magAbs;em.opt)
mg_gspphot_lower 3.5026 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 3.6570 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 2.2241 solRad Radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot) (phys.size.radius)
radius_gspphot_lower 2.1469 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 2.3420 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-4.753603e+02   Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC best library (logposterior_gspphot) (stat.fit.goodness)
mcmcaccept_gspphot 0.517116000   MCMC acceptance rate of GSP-Phot Aeneas MCMC best library (mcmcaccept_gspphot) (stat.value)
libname_gspphotPHOENIX  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 0.25502 nm Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha) (spect.line.eqWidth)
ew_espels_halpha_uncertainty 0.07818 nm Uncertainty of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_uncertainty) (stat.error;spect.line.eqWidth)
ew_espels_halpha_flag0   [0/9] Quality flag of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_flag) (meta.code.qual)
ew_espels_halpha_model 0.054605 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 93   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 2.1626 Rsun Radius of the star from FLAME using teff_gspphot and lum_flame (radius_flame) (phys.size.radius)
radius_flame_lower 2.0990 Rsun Lower confidence level (16%) of radiusFlame (radius_flame_lower) (phys.size.radius;stat.min)
radius_flame_upper 2.2493 Rsun Upper confidence level (84%) of radiusFlame (radius_flame_upper) (phys.size.radius;stat.max)
lum_flame 2.757e+00 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 2.638e+00 Lsun Lower confidence level (16%) of lumFlame (lum_flame_lower) (phys.luminosity;stat.min)
lum_flame_upper 2.949e+00 Lsun Upper confidence level (84%) of lumFlame (lum_flame_upper) (phys.luminosity;stat.max)
mass_flame 1.049 Msun Mass of the star from FLAME using stellar models, lum_flame, and teff_gspphot (mass_flame) (phys.mass)
mass_flame_lower 1.004 Msun Lower confidence level (16%) of mass of the star from FLAME (mass_flame_lower) (phys.mass;stat.min)
mass_flame_upper 1.091 Msun Upper confidence level (84%) of mass of the star from FLAME (mass_flame_upper) (phys.mass;stat.max)
age_flame 9.635 Gyr Age of the star from FLAME using stellar models (age_flame) (time.age)
age_flame_lower 8.691 Gyr Lower confidence level (84%) of age of the star from FLAME (age_flame_lower) (time.age;stat.min)
age_flame_upper10.843 Gyr Upper confidence level (84%) of age of the star from FLAME (age_flame_upper) (time.age;stat.max)
flags_flame11   [0/22] Flags indicating quality and processing information from FLAME (flags_flame) (Note 4)   (meta.code.qual)
evolstage_flame 495   Evolutionary stage of the star from FLAME using stellar models (evolstage_flame) (src.class)
gravredshift_flame 0.25684533 km/s Gravitational redshift from FLAME using radiusFlame and loggGspphot (gravredshift_flame) (src.redshift)
gravredshift_flame_lower 0.24579136 km/s Lower confidence level (16%) of gravitational redshift from FLAME (gravredshift_flame_lower) (src.redshift;stat.min)
gravredshift_flame_upper 0.26366124 km/s Upper confidence level (84%) of gravitational redshift from FLAME (gravredshift_flame_upper) (src.redshift;stat.max)
bc_flame-0.0102779 mag Bolometric correction used to derive lumFlame (bc_flame) (phot.mag.bc)
mh_msc 0.114097 [-] Metallicity of the source treated as a binary system from MSC using BP/RP spectra and parallax (mh_msc) (phys.abund)
mh_msc_upper 0.327065 [-] 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-0.017433 [-] Lower confidence level (16%) of the metallicity from MSC using BP/RP spectra and parallax (mh_msc_lower) (phys.abund;stat.min)
azero_msc 0.298866 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 0.378191 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 0.237074 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 802.964 pc Distance from MSC using BP/RP spectra and parallax (distance_msc) (pos.distance)
distance_msc_upper 860.570 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 697.831 pc Lower confidence level (16%) of distance from MSC using BP/RP spectra and parallax (distance_msc_lower) (pos.distance;stat.min)
teff_msc14549.3936 K Effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1) (phys.temperature.effective)
teff_msc1_upper4960.1553 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_lower4460.7900 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_msc23903.5460 K Effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2) (phys.temperature.effective)
teff_msc2_upper4013.3750 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_lower3843.2870 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 4.5153 [cm/s2] Surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1) (phys.gravity)
logg_msc1_upper 5.2000 [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 4.1549 [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 4.7994 [cm/s2] Surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2) (phys.gravity)
logg_msc2_upper 4.8519 [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 4.7563 [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 0.223367 mag Extinction in G band from MSC using BP/RP spectra and parallax (ag_msc) (phys.absorption)
ag_msc_upper 0.281758 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 0.176095 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 4.7493866e+01   Goodness-of-fit score (normalised log-posterior) of MSC MCMC (logposterior_msc) (stat.fit.goodness)
mcmcaccept_msc 0.233317420   Mean MCMC acceptance rate of MSC MCMC (mcmcaccept_msc) (stat.fit.param)
mcmcdrift_msc 7.402903e-02   Mean drift of the MSC MCMC chain in units of parameter standard deviation (mcmcdrift_msc) (stat.fit.param)
flags_msc0   [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)
  


The following problems were encountered in this VizieR run:
****catClient fails: (XmatchCatError) [Errno 111] Connection refused
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.errorfile=/tmp/VR1684591.err (2022-09-26T15:04:52)
-5
-ref=VIZ62fa0eb62bf4cb
-ref=VIZ62fa0eb62bf4cb
-out.add=.
-source=I/355/paramp
-c=292.05541201126 +00.12039241991,eq=ICRS,rs=2
-out.orig=o
elapse time 1

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