Astrophysical Parameters (gaiadr3.astrophysical_parameters)

The table has 1590932717 rows, 226 columns.

Description

This is the main table containing the 1D astrophysical parameters produced by the Apsis processing chain developed in Gaia DPAC CU8 (see Chapter cu8par). Additional parameters can be found in table AstrophysicalParametersSupp.

Attribution

If you have used Gaia data in your research, please use the following acknowledgement:

This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.

More information can be found on the credit and citation instructions page.

Columns

Name Type UCD Unit Description
solution_id long meta.version

Solution Identifier

source_id long meta.id
meta.main
meta.ref

Source Identifier

classprob_dsc_combmod_quasar float stat.probability

Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)

classprob_dsc_combmod_galaxy float stat.probability

Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)

classprob_dsc_combmod_star float stat.probability

Probability from DSC-Combmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum, photometry, astrometry)

classprob_dsc_combmod_whitedwarf float stat.probability

Probability from DSC-Combmod of being a white dwarf (data used: BP/RP spectrum, photometry, astrometry)

classprob_dsc_combmod_binarystar float stat.probability

Probability from DSC-Combmod of being a binary star (data used: BP/RP spectrum, photometry, astrometry)

classprob_dsc_specmod_quasar float stat.probability

Probability from DSC-Specmod of being a quasar (data used: BP/RP spectrum)

classprob_dsc_specmod_galaxy float stat.probability

Probability from DSC-Specmod of being a galaxy (data used: BP/RP spectrum)

classprob_dsc_specmod_star float stat.probability

Probability from DSC-Specmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum)

classprob_dsc_specmod_whitedwarf float stat.probability

Probability from DSC-Specmod of being a white dwarf (data used: BP/RP spectrum)

classprob_dsc_specmod_binarystar float stat.probability

Probability from DSC-Specmod of being a binary star (data used: BP/RP spectrum)

classprob_dsc_allosmod_quasar float stat.probability

Probability from DSC-Allosmod of being a quasar (data used: photometry, astrometry)

classprob_dsc_allosmod_galaxy float stat.probability

Probability from DSC-Allosmod of being a galaxy (data used: photometry, astrometry)

classprob_dsc_allosmod_star float stat.probability

Probability from DSC-Allosmod of being a star (data used: photometry, astrometry)

teff_gspphot float phys.temperature.effective K

Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra

teff_gspphot_lower float stat.value
phys.temperature.effective
K

Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra

teff_gspphot_upper float stat.value
phys.temperature.effective
K

Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra

logg_gspphot float phys.gravity log(cm.s**-2)

Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra

logg_gspphot_lower float stat.value
phys.gravity
log(cm.s**-2)

Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra

logg_gspphot_upper float stat.value
phys.gravity
log(cm.s**-2)

Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra

mh_gspphot float phys.abund.Fe "dex"

Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra

mh_gspphot_lower float stat.value
phys.abund.Fe
"dex"

Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra

mh_gspphot_upper float stat.value
phys.abund.Fe
"dex"

Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra

distance_gspphot float pos.distance pc

Distance from GSP-Phot Aeneas best library using BP/RP spectra

distance_gspphot_lower float stat.value
pos.distance
pc

Lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra

distance_gspphot_upper float stat.value
pos.distance
pc

Upper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectra

azero_gspphot float phys.absorption
em.opt.V
mag

Monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra

azero_gspphot_lower float stat.value
phys.absorption
em.opt.V
mag

Lower confidence level (16%) of monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra

azero_gspphot_upper float stat.value
phys.absorption
em.opt.V
mag

Upper confidence level (84%) of monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra

ag_gspphot float phys.absorption
em.opt
mag

Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra

ag_gspphot_lower float stat.value
phys.absorption
em.opt
mag

Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra

ag_gspphot_upper float stat.value
phys.absorption
em.opt
mag

Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra

abp_gspphot float phys.absorption
em.opt.B
mag

Extinction in GBP band from GSP-Phot Aeneas best library using BP/RP spectra

abp_gspphot_lower float stat.value
phys.absorption
em.opt.B
mag

Lower confidence level (16%) of extinction in GBP band from GSP-Phot Aeneas best library using BP/RP spectra

abp_gspphot_upper float stat.value
phys.absorption
em.opt.B
mag

Upper confidence level (84%) of extinction in GBP band from GSP-Phot Aeneas best library using BP/RP spectra

arp_gspphot float phys.absorption
em.opt.R
mag

Extinction in GRP band from GSP-Phot Aeneas best library using BP/RP spectra

arp_gspphot_lower float stat.value
phys.absorption
em.opt.R
mag

Lower confidence level (16%) of extinction in GRP band from GSP-Phot Aeneas best library using BP/RP spectra

arp_gspphot_upper float stat.value
phys.absorption
em.opt.R
mag

Upper confidence level (84%) of extinction in GRP band from GSP-Phot Aeneas best library using BP/RP spectra

ebpminrp_gspphot float phot.color.excess
em.opt
mag

Reddening E(GBP - GRP) from GSP-Phot Aeneas best library using BP/RP spectra

ebpminrp_gspphot_lower float stat.value
phot.color.excess
em.opt
mag

Lower confidence level (16%) of reddening E(GBP - GRP) from GSP-Phot Aeneas best library using BP/RP spectra

ebpminrp_gspphot_upper float stat.value
phot.color.excess
em.opt
mag

Upper confidence level (84%) of reddening E(GBP - GRP) from GSP-Phot Aeneas best library using BP/RP spectra

mg_gspphot float phys.magAbs
em.opt
mag

Absolute magnitude MG from GSP-Phot Aeneas best library using BP/RP spectra

mg_gspphot_lower float stat.value
phys.magAbs
em.opt
mag

Lower confidence level (16%) of absolute magnitude MG from GSP-Phot Aeneas best library using BP/RP spectra

mg_gspphot_upper float stat.value
phys.magAbs
em.opt
mag

Upper confidence level (84%) of absolute magnitude MG from GSP-Phot Aeneas best library using BP/RP spectra

radius_gspphot float phys.size.radius solRad

Radius from GSP-Phot Aeneas best library using BP/RP spectra

radius_gspphot_lower float stat.value
phys.size.radius
solRad

Lower confidence level (16%) of radius from GSP-Phot Aeneas best library using BP/RP spectra

radius_gspphot_upper float stat.value
phys.size.radius
solRad

Upper confidence level (84%) of radius from GSP-Phot Aeneas best library using BP/RP spectra

logposterior_gspphot float stat.fit.goodness

Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC best library

mcmcaccept_gspphot float stat.value

MCMC acceptance rate of GSP-Phot Aeneas MCMC best library

libname_gspphot char meta.record

Name of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this table

teff_gspspec float phys.temperature.effective
stat.median
K

Effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

teff_gspspec_lower float stat.value
phys.temperature.effective
K

16th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

teff_gspspec_upper float stat.value
phys.temperature.effective
K

84th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

logg_gspspec float phys.gravity
stat.median
log(cm.s**-2)

Logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

logg_gspspec_lower float stat.value
phys.gravity
log(cm.s**-2)

16th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

logg_gspspec_upper float stat.value
phys.gravity
log(cm.s**-2)

84th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

mh_gspspec float phys.abund.Fe
stat.median
"dex"

Global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

mh_gspspec_lower float stat.value
phys.abund.Fe
"dex"

16th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

mh_gspspec_upper float stat.value
phys.abund.Fe
"dex"

84th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

alphafe_gspspec float phys.abund
stat.median
"dex"

Abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

alphafe_gspspec_lower float stat.value
phys.abund
"dex"

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_upper float stat.value
phys.abund
"dex"

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

fem_gspspec float phys.abund.Fe
stat.median
"dex"

Abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in femGspspecNlines

fem_gspspec_lower float stat.value
phys.abund.Fe
"dex"

16th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

fem_gspspec_upper float stat.value
phys.abund.Fe
"dex"

84th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

fem_gspspec_nlines integer meta.number

Number of lines used for [Fe/M] abundance estimation

fem_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [Fe/M] abundance using N lines of the element, given in femGspspecNlines

sife_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in sifeGspspecNlines

sife_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

sife_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

sife_gspspec_nlines integer meta.number

Number of lines used for [Si/Fe] abundance estimation

sife_gspspec_linescatter float phys.abund.Z
stat.median
"dex"

Uncertainty estimation of [Si/Fe] abundance using N lines of the element, given in sifeGspspecNlines

cafe_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in cafeGspspecNlines

cafe_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

cafe_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

cafe_gspspec_nlines integer meta.number

Number of lines used for [Ca/Fe] abundance estimation

cafe_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [Ca/Fe] abundance using N lines of the element, given in cafeGspspecNlines

tife_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in tifeGspspecNlines

tife_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

tife_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

tife_gspspec_nlines integer meta.number

Number of lines used for [Ti/Fe] abundance estimation

tife_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [Ti/Fe] abundance using N lines of the element, given in tifeGspspecNlines

mgfe_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in mgfeGspspecNlines

mgfe_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

mgfe_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

mgfe_gspspec_nlines integer meta.number

Number of lines used for [Mg/Fe] abundance estimation

mgfe_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [Mg/Fe] abundance using N lines of the element, given in mgfeGspspecNlines

ndfe_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in ndfeGspspecNlines

ndfe_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

ndfe_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

ndfe_gspspec_nlines integer meta.number

Number of lines used for [Nd/Fe] abundance estimation

ndfe_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [Nd/Fe] abundance using N lines of the element, given in ndfeGspspecNlines

feiim_gspspec float phys.abund.Fe
stat.median
"dex"

Abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in feiimGspspecNlines

feiim_gspspec_lower float stat.value
phys.abund.Fe
"dex"

16th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

feiim_gspspec_upper float stat.value
phys.abund.Fe
"dex"

84th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

feiim_gspspec_nlines integer meta.number

Number of lines used for [FeII/M] abundance estimation

feiim_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [FeII/M] abundance using N lines of the element, given in feiimGspspecNlines

sfe_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in sfeGspspecNlines

sfe_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

sfe_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

sfe_gspspec_nlines integer meta.number

Number of lines used for [S/Fe] abundance estimation

sfe_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [S/Fe] abundance using N lines of the element, given in sfeGspspecNlines

zrfe_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in zrfeGspspecNlines

zrfe_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

zrfe_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

zrfe_gspspec_nlines integer meta.number

Number of lines used for [Zr/Fe] abundance estimation

zrfe_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [Zr/Fe] abundance using N lines of the element, given in zrfeGspspecNlines

nfe_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in nfeGspspecNlines

nfe_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

nfe_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

nfe_gspspec_nlines integer meta.number

Number of lines used for [N/Fe] abundance estimation

nfe_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [N/Fe] abundance using N lines of the element, given in nfeGspspecNlines

crfe_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in crfeGspspecNlines

crfe_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

crfe_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

crfe_gspspec_nlines integer meta.record

Number of lines used for [Cr/Fe] abundance estimation

crfe_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [Cr/Fe] abundance using N lines of the element, given in crfeGspspecNlines

cefe_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in cefeGspspecNlines

cefe_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

cefe_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

cefe_gspspec_nlines integer meta.number

Number of lines used for [Ce/Fe] abundance estimation

cefe_gspspec_linescatter float stat.error
phys.abund.Z
"dex"

Uncertainty estimation of [Ce/Fe] abundance using N lines of the element, given in cefeGspspecNlines

nife_gspspec float phys.abund.Z
stat.median
"dex"

Abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in nifeGspspecNlines

nife_gspspec_lower float stat.value
phys.abund.Z
"dex"

16th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

nife_gspspec_upper float stat.value
phys.abund.Z
"dex"

84th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations

nife_gspspec_nlines integer meta.number

Number of lines used for [Ni/Fe] abundance estimation

nife_gspspec_linescatter float stat.value
phys.abund.Z
"dex"

Uncertainty estimation of [Ni/Fe] abundance using N lines of the element, given in nifeGspspecNlines

cn0ew_gspspec float spect.line.eqWidth nm

Equivalent witdh of cyanogen absorption line, derived from RVS spectra

cn0ew_gspspec_uncertainty float stat.error
spect.line.eqWidth
nm

Uncertainty of equivalent witdh of cyanogen absorption line, derived from RVS spectra

cn0_gspspec_centralline float spect.line.eqWidth nm

Central wavelength of cyanogen line, derived from RVS spectra using DIB algorithm

cn0_gspspec_width float stat.error
spect.line.eqWidth
nm

Width of cyoanogen line, derived from RVS spectra using DIB algorithm

dib_gspspec_lambda float em.wl.central nm

DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra

dib_gspspec_lambda_uncertainty float stat.error
em.wl.central
nm

Uncertainty on DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra

dibew_gspspec float spect.line.eqWidth angstrom

Equivalent width of the DIB from GSP-Spec MatisseGauguin using RVS spectra

dibew_gspspec_uncertainty float stat.value
spect.line.eqWidth
angstrom

Global uncertainty on DIB equivalent width value using DIB algorithm

dibewnoise_gspspec_uncertainty float stat.value
spect.line.eqWidth
angstrom

Uncertainty on DIB equivalent width value occuring from noise part

dibp0_gspspec float

Depth (p0 parameter) of the DIB derived from a Gaussian model fit

dibp2_gspspec float stat.fit.param angstrom

Width (p2 parameter) of the DIB derived from a Gaussian model fit

dibp2_gspspec_uncertainty float stat.fit.param angstrom

Uncertainty on the dibp2Gspspec parameter

dibqf_gspspec integer meta.code.qual

Quality flag of the DIB computation

flags_gspspec char meta.code.status

Catalogue flags for GSP-Spec MatisseGauguin

logchisq_gspspec float stat.fit.chi2

Logarithm of the goodness-of-fit for the GSP-Spec MatisseGauguin parameters

ew_espels_halpha float spect.line.eqWidth nm

Halpha pseudo-equivalent width from ESP-ELS

ew_espels_halpha_uncertainty float stat.error
spect.line.eqWidth
nm

Uncertainty of the Halpha pseudo-equivalent width from ESP-ELS

ew_espels_halpha_flag char meta.code.qual

Quality flag of the Halpha pseudo-equivalent width from ESP-ELS

ew_espels_halpha_model float spect.line.eqWidth nm

Halpha pseudo-equivalent width from ESP-ELS measured on the synthetic spectrum

classlabel_espels char meta.code.class

Adopted ELS class label from ESP-ELS

classlabel_espels_flag char meta.code.class

Quality flag of the adopted ELS class label from ESP-ELS

classprob_espels_wcstar float stat.probability

Probability from ESP-ELS of being a Wolf-Rayet star of type WC

classprob_espels_wnstar float stat.probability

Probability from ESP-ELS of being a Wolf-Rayet star of type WN

classprob_espels_bestar float stat.probability

Probability from ESP-ELS of being a Be Star

classprob_espels_ttauristar float stat.probability

Probability from ESP-ELS of being a T Tauri Star

classprob_espels_herbigstar float stat.probability

Probability from ESP-ELS of being a Herbig Ae/Be Star

classprob_espels_dmestar float stat.probability

Probability from ESP-ELS of being an active M dwarf Star

classprob_espels_pne float stat.probability

Probability from ESP-ELS of being a planetary nebula

azero_esphs float phys.absorption
em.opt.V
mag

Monochromatic interstellar extinction, A0, from ESP-HS

azero_esphs_uncertainty float stat.error
phys.absorption
em.opt.V
mag

Uncertainty at a 68% confidence level on A0 from ESP-HS

ag_esphs float phys.absorption
em.opt
mag

Intersterstellar extinction in G band from ESP-HS

ag_esphs_uncertainty float stat.error
phys.absorption
em.opt
mag

Uncertainty on AG from ESP-HS

ebpminrp_esphs float phot.color.excess
em.opt
mag

Reddening E(GBP - GRP) from ESP-HS

ebpminrp_esphs_uncertainty float stat.error
phot.color.excess
em.opt
mag

Uncertainty on E(GBP - GRP) from ESP-HS

teff_esphs float phys.temperature.effective K

Effective temperature from ESP-HS

teff_esphs_uncertainty float stat.error
phys.temperature.effective
K

Uncertainty at a 68% confidence level on the effective temperature from ESP-HS

logg_esphs float phys.gravity log(cm.s**-2)

Surface gravity from ESP-HS

logg_esphs_uncertainty float stat.error
phys.gravity
log(cm.s**-2)

Uncertainty at a 68% confidence level on the surface gravity from ESP-HS

vsini_esphs float phys.veloc.rotat km.s**-1

Projected rotational velocity from ESP-HS

vsini_esphs_uncertainty float stat.error
phys.veloc.rotat
km.s**-1

Uncertainty on the projected rotational velocity from ESP-HS

flags_esphs char meta.code.qual

Quality flag of the ESP-HS parametrisation

spectraltype_esphs char src.spType

Spectral type from ESP-ELS

activityindex_espcs float spect.index nm

Chromospheric activity index from ESP-CS, measured on the calcium triplet using RVS spectra

activityindex_espcs_uncertainty float stat.error
spect.index
nm

Uncertainty in the chromospheric activity index from ESP-CS

activityindex_espcs_input char

Source of input stellar parameters for the computation of the activity index by ESP-CS

teff_espucd float phys.temperature.effective K

Effective temperature estimate from ESP-UCD based on the RP spectrum

teff_espucd_uncertainty float stat.error
phys.temperature.effective
K

Uncertainty of the effective temperature estimate produced by ESP-UCD

flags_espucd char meta.code.status

Quality flags of the ESP-UCD parameter estimates

radius_flame float phys.size.radius solRad

Radius of the star from FLAME using teffGspphot and lumFlame

radius_flame_lower float stat.value
phys.size.radius
solRad

Lower confidence level (16%) of radiusFlame

radius_flame_upper float stat.value
phys.size.radius
solRad

Upper confidence level (84%) of radiusFlame

lum_flame float phys.luminosity solLum

Luminosity of the star from FLAME using G band magnitude, extinction (agGspphot), parallax or distance, and a bolometric correction bcFlame

lum_flame_lower float stat.value
phys.luminosity
solLum

Lower confidence level (16%) of lumFlame

lum_flame_upper float stat.value
phys.luminosity
solLum

Upper confidence level (84%) of lumFlame

mass_flame float phys.mass solMass

Mass of the star from FLAME using stellar models, lumFlame, and teffGspphot

mass_flame_lower float stat.value
phys.mass
solMass

Lower confidence level (16%) of massFlame

mass_flame_upper float stat.value
phys.mass
solMass

Upper confidence level (84%) of massFlame

age_flame float time.age Gyr

Age of the star from FLAME using stellar models, see massFlame for details

age_flame_lower float stat.value
time.age
Gyr

Lower confidence level (16%) of ageFlame

age_flame_upper float stat.value
time.age
Gyr

Upper confidence level (84%) of ageFlame

flags_flame char meta.code.qual

Flags indicating quality and processing information from FLAME

evolstage_flame integer src.class

Evolutionary stage of the star from FLAME using stellar models, see massFlame for details

gravredshift_flame float src.redshift km.s**-1

Gravitational redshift from FLAME using radiusFlame and loggGspphot

gravredshift_flame_lower float stat.value
src.redshift
km.s**-1

Lower confidence level (16%) of gravredshiftFlame

gravredshift_flame_upper float stat.value
src.redshift
km.s**-1

Upper confidence level (84%) of gravredshiftFlame

bc_flame float phot.mag.bc mag

Bolometric correction used to derive lumFlame

mh_msc float phys.abund "dex"

Metallicity of the source treated as a binary system from MSC using BP/RP spectra and parallax

mh_msc_upper float stat.value
phys.abund
"dex"

Upper confidence level (84%) of the metallicity from MSC using BP/RP spectra and parallax

mh_msc_lower float stat.value
phys.abund
"dex"

Lower confidence level (16%) of the metallicity from MSC using BP/RP spectra and parallax

azero_msc float phys.absorption
em.opt.V
mag

Monochromatic extinction A0 at 547.7nm of the source treated as a binary system from MSC using BP/RP spectra and parallax

azero_msc_upper float stat.value
phys.absorption
em.opt.V
mag

Upper confidence level (84%) of monochromatic extinction A0 at 547.7nm from MSC using BP/RP spectra and parallax

azero_msc_lower float stat.value
phys.absorption
em.opt.V
mag

Lower confidence level (16%) of monochromatic extinction A0 at 547.7nm from MSC using BP/RP spectra and parallax

distance_msc float pos.distance pc

Distance from MSC using BP/RP spectra and parallax

distance_msc_upper float stat.value
pos.distance
pc

Upper confidence level (84%) of distance from MSC using BP/RP spectra and parallax

distance_msc_lower float stat.value
pos.distance
pc

Lower confidence level (16%) of distance from MSC using BP/RP spectra and parallax

teff_msc1 float phys.temperature.effective K

Effective temperature of the primary from MSC using BP/RP spectra and parallax

teff_msc1_upper float stat.value
phys.temperature.effective
K

Upper confidence level (84%) of effective temperature of the primary from MSC using BP/RP spectra and parallax

teff_msc1_lower float stat.value
phys.temperature.effective
K

Lower confidence level (16%) of effective temperature of the primary from MSC using BP/RP spectra and parallax

teff_msc2 float phys.temperature.effective K

Effective temperature of the secondary from MSC using BP/RP spectra and parallax

teff_msc2_upper float stat.value
phys.temperature.effective
K

Upper confidence level (84%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax

teff_msc2_lower float stat.value
phys.temperature.effective
K

Lower confidence level (16%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax

logg_msc1 float phys.gravity log(cm.s**-2)

Surface gravity of the primary from MSC using BP/RP spectra and parallax

logg_msc1_upper float stat.value
phys.gravity
log(cm.s**-2)

Upper confidence level (84%) of surface gravity of the primary from MSC using BP/RP spectra and parallax

logg_msc1_lower float stat.value
phys.gravity
log(cm.s**-2)

Lower confidence level (16%) of surface gravity of the primary from MSC using BP/RP spectra and parallax

logg_msc2 float phys.gravity log(cm.s**-2)

Surface gravity of the secondary from MSC using BP/RP spectra and parallax

logg_msc2_upper float stat.value
phys.gravity
log(cm.s**-2)

Upper confidence level (84%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax

logg_msc2_lower float stat.value
phys.gravity
log(cm.s**-2)

Lower confidence level (16%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax

ag_msc float phys.absorption
em.opt
mag

Extinction in G band of the source treated as a binary system from MSC using BP/RP spectra and parallax

ag_msc_upper float stat.value
phys.absorption
mag

Upper confidence level (84%) of extinction in G band from MSC using BP/RP spectra and parallax

ag_msc_lower float stat.value
phys.absorption
mag

Lower confidence level (16%) of extinction in G band from MSC using BP/RP spectra and parallax

logposterior_msc float stat.fit.goodness

Goodness-of-fit score (normalised log-posterior) of MSC MCMC

mcmcaccept_msc float stat.fit.param

Mean MCMC acceptance rate of MSC MCMC

mcmcdrift_msc float stat.fit.param

Mean drift of the MSC MCMC chain in units of parameter standard deviation

flags_msc char meta.code.qual

Flag indicating quality information from MSC

neuron_oa_id long stat.fit.param

Identifier of the OA SOM map neuron that represents the source

neuron_oa_dist float stat.fit.param

Distance between the source XP spectra and the OA neuron XP prototype that represents the source

neuron_oa_dist_percentile_rank integer stat.fit.param

Percentile rank according to the distance distribution of the OA neuron that represents the source

flags_oa char meta.code.qual

Flags indicating quality and processing information from OA