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Fields Dictionary

Field	Variable	Type	Units	Description
_file_upper	_file_upper	integer		Upper bound for HEALpix index level 8 of source file for this row (used in determining source file name: "%s_%06d-%06d" % (table_name, source_id >> 43, _file_max))
source_id	source_id	long		Unique source identifier (unique within a particular Data Release)
random_index	random_index	long		Random index for use when selecting subsets
ref_epoch	ref_epoch	double	yr	Reference epoch
pos		float		Barycentric position
ra	ra	double	deg	Right ascension
ra_error	ra_error	float	mas	Standard error of right ascension
dec	dec	double	deg	Declination
dec_error	dec_error	float	mas	Standard error of declination
l	l	double	deg	Galactic longitude
b	b	double	deg	Galactic latitude
ecl_lon	ecl_lon	double	deg	Ecliptic longitude
ecl_lat	ecl_lat	double	deg	Ecliptic latitude
parallax	parallax	double	mas	Parallax
parallax_error	parallax_error	float	mas	Standard error of parallax
parallax_over_error	parallax_over_error	float		Parallax divided by its standard error
pm		double	mas/year	Proper motion
pm	pm	float	mas.yr**-1	Total proper motion
pmra	pmra	double	mas.yr**-1	Proper motion in right ascension direction
pmra_error	pmra_error	float	mas.yr**-1	Standard error of proper motion in right ascension direction
pmdec	pmdec	double	mas.yr**-1	Proper motion in declination direction
pmdec_error	pmdec_error	float	mas.yr**-1	Standard error of proper motion in declination direction
corr		float		astrometric correlation coefficients
ra_dec_corr	ra_dec_corr	float		Correlation between right ascension and declination
ra_parallax_corr	ra_parallax_corr	float		Correlation between right ascension and parallax
ra_pmra_corr	ra_pmra_corr	float		Correlation between right ascension and proper motion in right ascension
ra_pmdec_corr	ra_pmdec_corr	float		Correlation between right ascension and proper motion in declination
dec_parallax_corr	dec_parallax_corr	float		Correlation between declination and parallax
dec_pmra_corr	dec_pmra_corr	float		Correlation between declination and proper motion in right ascension
dec_pmdec_corr	dec_pmdec_corr	float		Correlation between declination and proper motion in declination
parallax_pmra_corr	parallax_pmra_corr	float		Correlation between parallax and proper motion in right ascension
parallax_pmdec_corr	parallax_pmdec_corr	float		Correlation between parallax and proper motion in declination
pmra_pmdec_corr	pmra_pmdec_corr	float		Correlation between proper motion in right ascension and proper motion in declination
astrometric solution metadata		float
astrometric_n_obs_al	astrometric_n_obs_al	short		Total number of observations in the along-scan (AL) direction
astrometric_n_obs_ac	astrometric_n_obs_ac	short		Total number of observations in the across-scan (AC) direction
astrometric_n_good_obs_al	astrometric_n_good_obs_al	short		Number of good observations in the along-scan (AL) direction
astrometric_n_bad_obs_al	astrometric_n_bad_obs_al	short		Number of bad observations in the along-scan (AL) direction
astrometric_gof_al	astrometric_gof_al	float		Goodness of fit statistic of model wrt along-scan observations
astrometric_chi2_al	astrometric_chi2_al	float		AL chi-square value
astrometric_excess_noise	astrometric_excess_noise	float	mas	Excess noise of the source
astrometric_excess_noise_sig	astrometric_excess_noise_sig	float		Significance of excess noise
astrometric_params_solved	astrometric_params_solved	byte		Which parameters have been solved for?
astrometric_primary_flag	astrometric_primary_flag	boolean		Primary or secondary
nu_eff_used_in_astrometry	nu_eff_used_in_astrometry	float	um**-1	Effective wavenumber of the source used in the astrometric solution
pseudocolour	pseudocolour	float	um**-1	Astrometrically estimated pseudocolour of the source
pseudocolour_error	pseudocolour_error	float	um**-1	Standard error of the pseudocolour of the source
ra_pseudocolour_corr	ra_pseudocolour_corr	float		Correlation between right ascension and pseudocolour
dec_pseudocolour_corr	dec_pseudocolour_corr	float		Correlation between declination and pseudocolour
parallax_pseudocolour_corr	parallax_pseudocolour_corr	float		Correlation between parallax and pseudocolour
pmra_pseudocolour_corr	pmra_pseudocolour_corr	float		Correlation between proper motion in right asension and pseudocolour
pmdec_pseudocolour_corr	pmdec_pseudocolour_corr	float		Correlation between proper motion in declination and pseudocolour
astrometric_matched_transits	astrometric_matched_transits	short		Matched FOV transits used in the AGIS solution
visibility_periods_used	visibility_periods_used	short		Number of visibility periods used in Astrometric solution
astrometric_sigma5d_max	astrometric_sigma5d_max	float	mas	The longest semi-major axis of the 5-d error ellipsoid
matched_transits	matched_transits	short		The number of transits matched to this source
new_matched_transits	new_matched_transits	short		The number of transits newly incorporated into an existing source in the current cycle
matched_transits_removed	matched_transits_removed	short		The number of transits removed from an existing source in the current cycle
ipd_gof_harmonic_amplitude	ipd_gof_harmonic_amplitude	float		Amplitude of the IPD GoF versus position angle of scan
ipd_gof_harmonic_phase	ipd_gof_harmonic_phase	float	deg	Phase of the IPD GoF versus position angle of scan
ipd_frac_multi_peak	ipd_frac_multi_peak	byte		Percent of successful-IPD windows with more than one peak
ipd_frac_odd_win	ipd_frac_odd_win	byte		Percent of transits with truncated windows or multiple gate
ruwe	ruwe	float		Renormalised unit weight error
scan_direction_strength_k1	scan_direction_strength_k1	float		Degree of concentration of scan directions across the source
scan_direction_strength_k2	scan_direction_strength_k2	float		Degree of concentration of scan directions across the source
scan_direction_strength_k3	scan_direction_strength_k3	float		Degree of concentration of scan directions across the source
scan_direction_strength_k4	scan_direction_strength_k4	float		Degree of concentration of scan directions across the source
scan_direction_mean_k1	scan_direction_mean_k1	float	deg	Mean position angle of scan directions across the source
scan_direction_mean_k2	scan_direction_mean_k2	float	deg	Mean position angle of scan directions across the source
scan_direction_mean_k3	scan_direction_mean_k3	float	deg	Mean position angle of scan directions across the source
scan_direction_mean_k4	scan_direction_mean_k4	float	deg	Mean position angle of scan directions across the source
duplicated_source	duplicated_source	boolean		Source with multiple source identifiers
phot_g		float		G-band photometry
phot_g_n_obs	phot_g_n_obs	short		Number of observations contributing to G photometry
phot_g_mean_flux	phot_g_mean_flux	double	'electron'.s**-1	G-band mean flux
phot_g_mean_flux_error	phot_g_mean_flux_error	float	'electron'.s**-1	Error on G-band mean flux
phot_g_mean_flux_over_error	phot_g_mean_flux_over_error	float		G-band mean flux divided by its error
phot_g_mean_mag	phot_g_mean_mag	float	mag	G-band mean magnitude
phot_bp		float		BP photometry
phot_bp_n_obs	phot_bp_n_obs	short		Number of observations contributing to BP photometry
phot_bp_mean_flux	phot_bp_mean_flux	double	'electron'.s**-1	Integrated BP mean flux
phot_bp_mean_flux_error	phot_bp_mean_flux_error	float	'electron'.s**-1	Error on the integrated BP mean flux
phot_bp_mean_flux_over_error	phot_bp_mean_flux_over_error	float		Integrated BP mean flux divided by its error
phot_bp_mean_mag	phot_bp_mean_mag	float	mag	Integrated BP mean magnitude
phot_bp_n_contaminated_transits	phot_bp_n_contaminated_transits	short		Number of BP contaminated transits
phot_bp_n_blended_transits	phot_bp_n_blended_transits	short		Number of BP blended transits
phot_rp		float		RP photometry
phot_rp_n_obs	phot_rp_n_obs	short		Number of observations contributing to RP photometry
phot_rp_mean_flux	phot_rp_mean_flux	double	'electron'.s**-1	Integrated RP mean flux
phot_rp_mean_flux_error	phot_rp_mean_flux_error	float	'electron'.s**-1	Error on the integrated RP mean flux
phot_rp_mean_flux_over_error	phot_rp_mean_flux_over_error	float		Integrated RP mean flux divided by its error
phot_rp_mean_mag	phot_rp_mean_mag	float	mag	Integrated RP mean magnitude
phot_bp_rp_excess_factor	phot_bp_rp_excess_factor	float		BP/RP excess factor
phot_rp_n_contaminated_transits	phot_rp_n_contaminated_transits	short		Number of RP contaminated transits
phot_rp_n_blended_transits	phot_rp_n_blended_transits	short		Number of RP blended transits
phot_proc_mode	phot_proc_mode	byte		Photometry processing mode
bp_rp	bp_rp	float	mag	BP - RP colour
bp_g	bp_g	float	mag	BP - G colour
g_rp	g_rp	float	mag	G - RP colour
rv		float		Radial velocity
radial_velocity	radial_velocity	float	km.s**-1	Radial velocity
radial_velocity_error	radial_velocity_error	float	km.s**-1	Radial velocity error
rv_method_used	rv_method_used	byte		Method used to obtain the radial velocity
rv_nb_transits	rv_nb_transits	short		Number of transits used to compute the radial velocity
rv_nb_deblended_transits	rv_nb_deblended_transits	short		Number of valid transits that have undergone deblending
rv_visibility_periods_used	rv_visibility_periods_used	short		Number of visibility periods used to estimate the radial velocity
rv_expected_sig_to_noise	rv_expected_sig_to_noise	float		Expected signal to noise ratio in the combination of the spectra used to obtain the radial velocity
rv_renormalised_gof	rv_renormalised_gof	float		Radial velocity renormalised goodness of fit
rv_chisq_pvalue	rv_chisq_pvalue	float		P-value for constancy based on a chi-squared criterion
rv_time_duration	rv_time_duration	float	d	Time coverage of the radial velocity time series
rv_amplitude_robust	rv_amplitude_robust	float	km.s**-1	Total amplitude in the radial velocity time series after outlier removal
rv_template_teff	rv_template_teff	float	K	Teff of the template used to compute the radial velocity
rv_template_logg	rv_template_logg	float	log(cm.s**-2)	Logg of the template used to compute the radial velocity
rv_template_fe_h	rv_template_fe_h	float	'dex'	[Fe/H] of the template used to compute the radial velocityy
rv_atm_param_origin	rv_atm_param_origin	short		Origin of the atmospheric parameters associated to the template
vbroad	vbroad	float	km.s**-1	Spectral line broadening parameter
vbroad_error	vbroad_error	float	km.s**-1	Uncertainty on the spectral line broadening
vbroad_nb_transits	vbroad_nb_transits	short		Number of transits used to compute vbroad
grvs_mag	grvs_mag	float	mag	Integrated Grvs magnitude
grvs_mag_error	grvs_mag_error	float	mag	Grvs magnitude uncertainty
grvs_mag_nb_transits	grvs_mag_nb_transits	short		Number of transits used to compute Grvs
rvs_spec_sig_to_noise	rvs_spec_sig_to_noise	float		Signal to noise ratio in the mean RVS spectrum
phot_variable_flag	phot_variable_flag	byte		Photometric variability flag
metadata_flags		float		Flags that indicate presence of more specialized data for a given source
in_qso_candidates	in_qso_candidates	boolean		Flag indicating the availability of additional information in the QsoCandidates table
in_galaxy_candidates	in_galaxy_candidates	boolean		Flag indicating the availability of additional information in the GalaxyCandidates table
non_single_star	non_single_star	short		Flag indicating the availability of additional information in the various Non-Single Star tables
has_xp_continuous	has_xp_continuous	boolean		Flag indicating the availability of mean BP/RP spectrum in continuous representation for this source
has_xp_sampled	has_xp_sampled	boolean		Flag indicating the availability of mean BP/RP spectrum in sampled form for this source
has_rvs	has_rvs	boolean		Flag indicating the availability of mean RVS spectrum for this source
has_epoch_photometry	has_epoch_photometry	boolean		Flag indicating the availability of epoch photometry for this source
has_epoch_rv	has_epoch_rv	boolean		Flag indicating the availability of epoch radial velocity for this source
has_mcmc_gspphot	has_mcmc_gspphot	boolean		Flag indicating the availability of GSP-Phot MCMC samples for this source
has_mcmc_msc	has_mcmc_msc	boolean		Flag indicating the availability of MSC MCMC samples for this source
in_andromeda_survey	in_andromeda_survey	boolean		Flag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS)
astrophysical_parameters		float		This is the main table containing the 1D astrophysical parameters produced by the Apsis processing chain developed in Gaia DPAC CU8. Additional parameters can be found in table AstrophysicalParametersSupp.
_index	astrophysical_parameters__index	integer		Offset of this row in the source file for this table (see _file_max)
classprob		float		Class probabilities for source classification
classprob_dsc_combmod_quasar	astrophysical_parameters_classprob_dsc_combmod_quasar	float		Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)
classprob_dsc_combmod_galaxy	astrophysical_parameters_classprob_dsc_combmod_galaxy	float		Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)
classprob_dsc_combmod_star	astrophysical_parameters_classprob_dsc_combmod_star	float		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	astrophysical_parameters_classprob_dsc_combmod_whitedwarf	float		Probability from DSC-Combmod of being a white dwarf (data used: BP/RP spectrum, photometry, astrometry)
classprob_dsc_combmod_binarystar	astrophysical_parameters_classprob_dsc_combmod_binarystar	float		Probability from DSC-Combmod of being a binary star (data used: BP/RP spectrum, photometry, astrometry)
classprob_dsc_specmod_quasar	astrophysical_parameters_classprob_dsc_specmod_quasar	float		Probability from DSC-Specmod of being a quasar (data used: BP/RP spectrum)
classprob_dsc_specmod_galaxy	astrophysical_parameters_classprob_dsc_specmod_galaxy	float		Probability from DSC-Specmod of being a galaxy (data used: BP/RP spectrum)
classprob_dsc_specmod_star	astrophysical_parameters_classprob_dsc_specmod_star	float		Probability from DSC-Specmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum)
classprob_dsc_specmod_whitedwarf	astrophysical_parameters_classprob_dsc_specmod_whitedwarf	float		Probability from DSC-Specmod of being a white dwarf (data used: BP/RP spectrum)
classprob_dsc_specmod_binarystar	astrophysical_parameters_classprob_dsc_specmod_binarystar	float		Probability from DSC-Specmod of being a binary star (data used: BP/RP spectrum)
classprob_dsc_allosmod_quasar	astrophysical_parameters_classprob_dsc_allosmod_quasar	float		Probability from DSC-Allosmod of being a quasar (data used: photometry, astrometry)
classprob_dsc_allosmod_galaxy	astrophysical_parameters_classprob_dsc_allosmod_galaxy	float		Probability from DSC-Allosmod of being a galaxy (data used: photometry, astrometry)
classprob_dsc_allosmod_star	astrophysical_parameters_classprob_dsc_allosmod_star	float		Probability from DSC-Allosmod of being a star (data used: photometry, astrometry)
teff		float	K	stellar effective temperature
teff_gspphot	astrophysical_parameters_teff_gspphot	float	K	Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra
teff_gspphot_lower	astrophysical_parameters_teff_gspphot_lower	float	K	Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra
teff_gspphot_upper	astrophysical_parameters_teff_gspphot_upper	float	K	Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra
teff_gspspec	astrophysical_parameters_teff_gspspec	float	K	Effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
teff_gspspec_lower	astrophysical_parameters_teff_gspspec_lower	float	K	16th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
teff_gspspec_upper	astrophysical_parameters_teff_gspspec_upper	float	K	84th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
logg		float	log(cm.s**-2)	stellar surface gravity
logg_gspphot	astrophysical_parameters_logg_gspphot	float	log(cm.s**-2)	Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra
logg_gspphot_lower	astrophysical_parameters_logg_gspphot_lower	float	log(cm.s**-2)	Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra
logg_gspphot_upper	astrophysical_parameters_logg_gspphot_upper	float	log(cm.s**-2)	Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra
logg_gspspec	astrophysical_parameters_logg_gspspec	float	log(cm.s**-2)	Logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
logg_gspspec_lower	astrophysical_parameters_logg_gspspec_lower	float	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	astrophysical_parameters_logg_gspspec_upper	float	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		float	dex	stellar metallicity
mh_gspphot	astrophysical_parameters_mh_gspphot	float	dex	Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra
mh_gspphot_lower	astrophysical_parameters_mh_gspphot_lower	float	dex	Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra
mh_gspphot_upper	astrophysical_parameters_mh_gspphot_upper	float	dex	Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra
mh_gspspec	astrophysical_parameters_mh_gspspec	float	'dex'	Global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
mh_gspspec_lower	astrophysical_parameters_mh_gspspec_lower	float	'dex'	16th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
mh_gspspec_upper	astrophysical_parameters_mh_gspspec_upper	float	'dex'	84th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
distance		float	pc	distance to star
distance_gspphot	astrophysical_parameters_distance_gspphot	float	pc	Distance from GSP-Phot Aeneas best library using BP/RP spectra
distance_gspphot_lower	astrophysical_parameters_distance_gspphot_lower	float	pc	Lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra
distance_gspphot_upper	astrophysical_parameters_distance_gspphot_upper	float	pc	Upper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectra
azero		float	mag	monochromatic extinction
azero_gspphot	astrophysical_parameters_azero_gspphot	float	mag	Monochromatic extinction \(A_0\) at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra
azero_gspphot_lower	astrophysical_parameters_azero_gspphot_lower	float	mag	Lower confidence level (16%) of monochromatic extinction \(A_0\) at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra
azero_gspphot_upper	astrophysical_parameters_azero_gspphot_upper	float	mag	Upper confidence level (84%) of monochromatic extinction \(A_0\) at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra
ag		float	mag	extinction in G band
ag_gspphot	astrophysical_parameters_ag_gspphot	float	mag	Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra
ag_gspphot_lower	astrophysical_parameters_ag_gspphot_lower	float	mag	Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra
ag_gspphot_upper	astrophysical_parameters_ag_gspphot_upper	float	mag	Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra
abp		float	mag	extinction in Bp
abp_gspphot	astrophysical_parameters_abp_gspphot	float	mag	Extinction in \(G_{\rm BP}\) band from GSP-Phot Aeneas best library using BP/RP spectra
abp_gspphot_lower	astrophysical_parameters_abp_gspphot_lower	float	mag	Lower confidence level (16%) of extinction in \(G_{\rm BP}\) band from GSP-Phot Aeneas best library using BP/RP spectra
abp_gspphot_upper	astrophysical_parameters_abp_gspphot_upper	float	mag	Upper confidence level (84%) of extinction in \(G_{\rm BP}\) band from GSP-Phot Aeneas best library using BP/RP spectra
arp		float	mag	extinction in Rp
arp_gspphot	astrophysical_parameters_arp_gspphot	float	mag	Extinction in \(G_{\rm RP}\) band from GSP-Phot Aeneas best library using BP/RP spectra
arp_gspphot_lower	astrophysical_parameters_arp_gspphot_lower	float	mag	Lower confidence level (16%) of extinction in \(G_{\rm RP}\) band from GSP-Phot Aeneas best library using BP/RP spectra
arp_gspphot_upper	astrophysical_parameters_arp_gspphot_upper	float	mag	Upper confidence level (84%) of extinction in \(G_{\rm RP}\) band from GSP-Phot Aeneas best library using BP/RP spectra
ebpminrp		float	mag	reddening
ebpminrp_gspphot	astrophysical_parameters_ebpminrp_gspphot	float	mag	Reddening \(E(G_{\rm BP} - G_{\rm RP})\) from GSP-Phot Aeneas best library using BP/RP spectra
ebpminrp_gspphot_lower	astrophysical_parameters_ebpminrp_gspphot_lower	float	mag	Lower confidence level (16%) of reddening \(E(G_{\rm BP} - G_{\rm RP})\) from GSP-Phot Aeneas best library using BP/RP spectra
ebpminrp_gspphot_upper	astrophysical_parameters_ebpminrp_gspphot_upper	float	mag	Upper confidence level (84%) of reddening \(E(G_{\rm BP} - G_{\rm RP})\) from GSP-Phot Aeneas best library using BP/RP spectra
mg		float	mag	Absolute magnitude
mg_gspphot	astrophysical_parameters_mg_gspphot	float	mag	Absolute magnitude \(M_{\rm G}\) from GSP-Phot Aeneas best library using BP/RP spectra
mg_gspphot_lower	astrophysical_parameters_mg_gspphot_lower	float	mag	Lower confidence level (16%) of absolute magnitude \(M_{\rm G}\) from GSP-Phot Aeneas best library using BP/RP spectra
mg_gspphot_upper	astrophysical_parameters_mg_gspphot_upper	float	mag	Upper confidence level (84%) of absolute magnitude \(M_{\rm G}\) from GSP-Phot Aeneas best library using BP/RP spectra
radius		float	solRad	Stellar radius
radius_gspphot	astrophysical_parameters_radius_gspphot	float	solRad	Radius from GSP-Phot Aeneas best library using BP/RP spectra
radius_gspphot_lower	astrophysical_parameters_radius_gspphot_lower	float	solRad	Lower confidence level (16%) of radius from GSP-Phot Aeneas best library using BP/RP spectra
radius_gspphot_upper	astrophysical_parameters_radius_gspphot_upper	float	solRad	Upper confidence level (84%) of radius from GSP-Phot Aeneas best library using BP/RP spectra
gspphot_metadata		float		Metadata related to the gspphot processing
logposterior_gspphot	astrophysical_parameters_logposterior_gspphot	float		Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC best library
mcmcaccept_gspphot	astrophysical_parameters_mcmcaccept_gspphot	float		MCMC acceptance rate of GSP-Phot Aeneas MCMC best library
libname_gspphot	astrophysical_parameters_libname_gspphot	byte		Name of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this table
alphafe		float	dex	Abundance of alpha-elements [alpha/Fe]
alphafe_gspspec	astrophysical_parameters_alphafe_gspspec	float	'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	astrophysical_parameters_alphafe_gspspec_lower	float	'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	astrophysical_parameters_alphafe_gspspec_upper	float	'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		float	dex	Abundance of neutral iron
fem_gspspec	astrophysical_parameters_fem_gspspec	float	'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	astrophysical_parameters_fem_gspspec_lower	float	'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	astrophysical_parameters_fem_gspspec_upper	float	'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	astrophysical_parameters_fem_gspspec_nlines	integer	dex	Number of lines used for [Fe/M] abundance estimation
fem_gspspec_linescatter	astrophysical_parameters_fem_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Fe/M] abundance using N lines of the element, given in femGspspecNlines
sife		float	dex	Abundance of Silicon
sife_gspspec	astrophysical_parameters_sife_gspspec	float	'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	astrophysical_parameters_sife_gspspec_lower	float	'dex'	16th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
sife_gspspec_upper	astrophysical_parameters_sife_gspspec_upper	float	'dex'	84th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
sife_gspspec_nlines	astrophysical_parameters_sife_gspspec_nlines	integer	dex	Number of lines used for [Si/Fe] abundance estimation
sife_gspspec_linescatter	astrophysical_parameters_sife_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Si/Fe] abundance using N lines of the element, given in sifeGspspecNlines
cafe		float	dex	Abundance of Calcium
cafe_gspspec	astrophysical_parameters_cafe_gspspec	float	'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	astrophysical_parameters_cafe_gspspec_lower	float	'dex'	16th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
cafe_gspspec_upper	astrophysical_parameters_cafe_gspspec_upper	float	'dex'	84th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
cafe_gspspec_nlines	astrophysical_parameters_cafe_gspspec_nlines	integer	dex	Number of lines used for [Ca/Fe] abundance estimation
cafe_gspspec_linescatter	astrophysical_parameters_cafe_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Ca/Fe] abundance using N lines of the element, given in cafeGspspecNlines
tife		float	dex	Abundance of Titanium
tife_gspspec	astrophysical_parameters_tife_gspspec	float	'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	astrophysical_parameters_tife_gspspec_lower	float	'dex'	16th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
tife_gspspec_upper	astrophysical_parameters_tife_gspspec_upper	float	'dex'	84th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
tife_gspspec_nlines	astrophysical_parameters_tife_gspspec_nlines	integer	dex	Number of lines used for [Ti/Fe] abundance estimation
tife_gspspec_linescatter	astrophysical_parameters_tife_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Ti/Fe] abundance using N lines of the element, given in tifeGspspecNlines
mgfe		float	dex	Abundance of Magnesium
mgfe_gspspec	astrophysical_parameters_mgfe_gspspec	float	'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	astrophysical_parameters_mgfe_gspspec_lower	float	'dex'	16th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
mgfe_gspspec_upper	astrophysical_parameters_mgfe_gspspec_upper	float	'dex'	84th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
mgfe_gspspec_nlines	astrophysical_parameters_mgfe_gspspec_nlines	integer	dex	Number of lines used for [Mg/Fe] abundance estimation
mgfe_gspspec_linescatter	astrophysical_parameters_mgfe_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Mg/Fe] abundance using N lines of the element, given in mgfeGspspecNlines
ndfe		float	dex	Abundance of Neodymium
ndfe_gspspec	astrophysical_parameters_ndfe_gspspec	float	'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	astrophysical_parameters_ndfe_gspspec_lower	float	'dex'	16th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
ndfe_gspspec_upper	astrophysical_parameters_ndfe_gspspec_upper	float	'dex'	84th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
ndfe_gspspec_nlines	astrophysical_parameters_ndfe_gspspec_nlines	integer	dex	Number of lines used for [Nd/Fe] abundance estimation
ndfe_gspspec_linescatter	astrophysical_parameters_ndfe_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Nd/Fe] abundance using N lines of the element, given in ndfeGspspecNlines
feiim		float	dex	Abundance of ionised Iron
feiim_gspspec	astrophysical_parameters_feiim_gspspec	float	'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	astrophysical_parameters_feiim_gspspec_lower	float	'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	astrophysical_parameters_feiim_gspspec_upper	float	'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	astrophysical_parameters_feiim_gspspec_nlines	integer	dex	Number of lines used for [FeII/M] abundance estimation
feiim_gspspec_linescatter	astrophysical_parameters_feiim_gspspec_linescatter	float	'dex'	Uncertainty estimation of [FeII/M] abundance using N lines of the element, given in feiimGspspecNlines
sfe		float	dex	Abundance of Sulphur
sfe_gspspec	astrophysical_parameters_sfe_gspspec	float	'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	astrophysical_parameters_sfe_gspspec_lower	float	'dex'	16th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
sfe_gspspec_upper	astrophysical_parameters_sfe_gspspec_upper	float	'dex'	84th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
sfe_gspspec_nlines	astrophysical_parameters_sfe_gspspec_nlines	integer	dex	Number of lines used for [S/Fe] abundance estimation
sfe_gspspec_linescatter	astrophysical_parameters_sfe_gspspec_linescatter	float	'dex'	Uncertainty estimation of [S/Fe] abundance using N lines of the element, given in sfeGspspecNlines
zrfe		float	dex	Abundance of Zirconium
zrfe_gspspec	astrophysical_parameters_zrfe_gspspec	float	'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	astrophysical_parameters_zrfe_gspspec_lower	float	'dex'	16th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
zrfe_gspspec_upper	astrophysical_parameters_zrfe_gspspec_upper	float	'dex'	84th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
zrfe_gspspec_nlines	astrophysical_parameters_zrfe_gspspec_nlines	integer	dex	Number of lines used for [Zr/Fe] abundance estimation
zrfe_gspspec_linescatter	astrophysical_parameters_zrfe_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Zr/Fe] abundance using N lines of the element, given in zrfeGspspecNlines
nfe		float	dex	Abundance of Nitrogen
nfe_gspspec	astrophysical_parameters_nfe_gspspec	float	'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	astrophysical_parameters_nfe_gspspec_lower	float	'dex'	16th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
nfe_gspspec_upper	astrophysical_parameters_nfe_gspspec_upper	float	'dex'	84th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
nfe_gspspec_nlines	astrophysical_parameters_nfe_gspspec_nlines	integer	dex	Number of lines used for [N/Fe] abundance estimation
nfe_gspspec_linescatter	astrophysical_parameters_nfe_gspspec_linescatter	float	'dex'	Uncertainty estimation of [N/Fe] abundance using N lines of the element, given in nfeGspspecNlines
crfe		float	dex	Abundance of Chromium
crfe_gspspec	astrophysical_parameters_crfe_gspspec	float	'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	astrophysical_parameters_crfe_gspspec_lower	float	'dex'	16th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
crfe_gspspec_upper	astrophysical_parameters_crfe_gspspec_upper	float	'dex'	84th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
crfe_gspspec_nlines	astrophysical_parameters_crfe_gspspec_nlines	integer	dex	Number of lines used for [Cr/Fe] abundance estimation
crfe_gspspec_linescatter	astrophysical_parameters_crfe_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Cr/Fe] abundance using N lines of the element, given in crfeGspspecNlines
cefe		float	dex	Abundance of Cerium
cefe_gspspec	astrophysical_parameters_cefe_gspspec	float	'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	astrophysical_parameters_cefe_gspspec_lower	float	'dex'	16th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
cefe_gspspec_upper	astrophysical_parameters_cefe_gspspec_upper	float	'dex'	84th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
cefe_gspspec_nlines	astrophysical_parameters_cefe_gspspec_nlines	integer	dex	Number of lines used for [Ce/Fe] abundance estimation
cefe_gspspec_linescatter	astrophysical_parameters_cefe_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Ce/Fe] abundance using N lines of the element, given in cefeGspspecNlines
nife		float	dex	Abundance of Nickel
nife_gspspec	astrophysical_parameters_nife_gspspec	float	'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	astrophysical_parameters_nife_gspspec_lower	float	'dex'	16th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
nife_gspspec_upper	astrophysical_parameters_nife_gspspec_upper	float	'dex'	84th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations
nife_gspspec_nlines	astrophysical_parameters_nife_gspspec_nlines	integer	dex	Number of lines used for [Ni/Fe] abundance estimation
nife_gspspec_linescatter	astrophysical_parameters_nife_gspspec_linescatter	float	'dex'	Uncertainty estimation of [Ni/Fe] abundance using N lines of the element, given in nifeGspspecNlines
cn0ew		float	dex	Equivalent witdh of cyanogen absorption line
cn0ew_gspspec	astrophysical_parameters_cn0ew_gspspec	float	nm	Equivalent witdh of cyanogen absorption line, derived from RVS spectra
cn0ew_gspspec_uncertainty	astrophysical_parameters_cn0ew_gspspec_uncertainty	float	nm	Uncertainty of equivalent witdh of cyanogen absorption line, derived from RVS spectra
cn0_gspspec_centralline	astrophysical_parameters_cn0_gspspec_centralline	float	nm	Central wavelength of cyanogen line, derived from RVS spectra using DIB algorithm
cn0_gspspec_width	astrophysical_parameters_cn0_gspspec_width	float	nm	Width of cyoanogen line, derived from RVS spectra using DIB algorithm
dib		float		Diffuse interstellar band (DIB)
dib_gspspec_lambda	astrophysical_parameters_dib_gspspec_lambda	float	nm	DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra
dib_gspspec_lambda_uncertainty	astrophysical_parameters_dib_gspspec_lambda_uncertainty	float	nm	Uncertainty on DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra
dibew_gspspec	astrophysical_parameters_dibew_gspspec	float	angstrom	Equivalent width of the DIB from GSP-Spec MatisseGauguin using RVS spectra
dibew_gspspec_uncertainty	astrophysical_parameters_dibew_gspspec_uncertainty	float	angstrom	Global uncertainty on DIB equivalent width value using DIB algorithm
dibewnoise_gspspec_uncertainty	astrophysical_parameters_dibewnoise_gspspec_uncertainty	float	angstrom	Uncertainty on DIB equivalent width value occuring from noise part
dibp0_gspspec	astrophysical_parameters_dibp0_gspspec	float		Depth (\(p_0\) parameter) of the DIB derived from a Gaussian model fit
dibp2_gspspec	astrophysical_parameters_dibp2_gspspec	float	angstrom	Width (\(p_2\) parameter) of the DIB derived from a Gaussian model fit
dibp2_gspspec_uncertainty	astrophysical_parameters_dibp2_gspspec_uncertainty	float	angstrom	Uncertainty on the dibp2Gspspec parameter
dibqf_gspspec	astrophysical_parameters_dibqf_gspspec	integer		Quality flag of the DIB computation
gspspec_metadata		float		Metadata related to the gspspec processing
logchisq_gspspec	astrophysical_parameters_logchisq_gspspec	float		Logarithm of the goodness-of-fit for the GSP-Spec MatisseGauguin parameters
espels		float		Data from the ESP-ELS (emission line stars) processing
ew_espels_halpha	astrophysical_parameters_ew_espels_halpha	float	nm	Halpha pseudo-equivalent width from ESP-ELS
ew_espels_halpha_uncertainty	astrophysical_parameters_ew_espels_halpha_uncertainty	float	nm	Uncertainty of the Halpha pseudo-equivalent width from ESP-ELS
ew_espels_halpha_flag	astrophysical_parameters_ew_espels_halpha_flag	byte		Quality flag of the Halpha pseudo-equivalent width from ESP-ELS
ew_espels_halpha_model	astrophysical_parameters_ew_espels_halpha_model	float	nm	Halpha pseudo-equivalent width from ESP-ELS measured on the synthetic spectrum
classlabel_espels	astrophysical_parameters_classlabel_espels	byte		Adopted ELS class label from ESP-ELS
classlabel_espels_flag	astrophysical_parameters_classlabel_espels_flag	byte		Quality flag of the adopted ELS class label from ESP-ELS
classprob_espels_wcstar	astrophysical_parameters_classprob_espels_wcstar	float		Probability from ESP-ELS of being a Wolf-Rayet star of type WC
classprob_espels_wnstar	astrophysical_parameters_classprob_espels_wnstar	float		Probability from ESP-ELS of being a Wolf-Rayet star of type WN
classprob_espels_bestar	astrophysical_parameters_classprob_espels_bestar	float		Probability from ESP-ELS of being a Be Star
classprob_espels_ttauristar	astrophysical_parameters_classprob_espels_ttauristar	float		Probability from ESP-ELS of being a T Tauri Star
classprob_espels_herbigstar	astrophysical_parameters_classprob_espels_herbigstar	float		Probability from ESP-ELS of being a Herbig Ae/Be Star
classprob_espels_dmestar	astrophysical_parameters_classprob_espels_dmestar	float		Probability from ESP-ELS of being an active M dwarf Star
classprob_espels_pne	astrophysical_parameters_classprob_espels_pne	float		Probability from ESP-ELS of being a planetary nebula
esphs		float		Data from the ESP-HS (hot stars) processing
azero_esphs	astrophysical_parameters_azero_esphs	float	mag	Monochromatic interstellar extinction, A\(_\mathrm{0}\), from ESP-HS
azero_esphs_uncertainty	astrophysical_parameters_azero_esphs_uncertainty	float	mag	Uncertainty at a 68% confidence level on A\(_\mathrm{0}\) from ESP-HS
ag_esphs	astrophysical_parameters_ag_esphs	float	mag	Intersterstellar extinction in G band from ESP-HS
ag_esphs_uncertainty	astrophysical_parameters_ag_esphs_uncertainty	float	mag	Uncertainty on \(A_{\rm G}\) from ESP-HS
ebpminrp_esphs	astrophysical_parameters_ebpminrp_esphs	float	mag	Reddening \(E(G_{\rm BP} - G_{\rm RP})\) from ESP-HS
ebpminrp_esphs_uncertainty	astrophysical_parameters_ebpminrp_esphs_uncertainty	float	mag	Uncertainty on \(E(G_{\rm BP} - G_{\rm RP})\) from ESP-HS
teff_esphs	astrophysical_parameters_teff_esphs	float	K	Effective temperature from ESP-HS
teff_esphs_uncertainty	astrophysical_parameters_teff_esphs_uncertainty	float	K	Uncertainty at a 68% confidence level on the effective temperature from ESP-HS
logg_esphs	astrophysical_parameters_logg_esphs	float	log(cm.s**-2)	Surface gravity from ESP-HS
logg_esphs_uncertainty	astrophysical_parameters_logg_esphs_uncertainty	float	log(cm.s**-2)	Uncertainty at a 68% confidence level on the surface gravity from ESP-HS
vsini_esphs	astrophysical_parameters_vsini_esphs	float	km.s**-1	Projected rotational velocity from ESP-HS
vsini_esphs_uncertainty	astrophysical_parameters_vsini_esphs_uncertainty	float	km.s**-1	Uncertainty on the projected rotational velocity from ESP-HS
spectraltype_esphs	astrophysical_parameters_spectraltype_esphs	byte		Spectral type from ESP-ELS
espcs		float		Data from the ESP-CS (cool stars) processing
activityindex_espcs	astrophysical_parameters_activityindex_espcs	float	nm	Chromospheric activity index from ESP-CS, measured on the calcium triplet using RVS spectra
activityindex_espcs_uncertainty	astrophysical_parameters_activityindex_espcs_uncertainty	float	nm	Uncertainty in the chromospheric activity index from ESP-CS
activityindex_espcs_input	astrophysical_parameters_activityindex_espcs_input	byte		Source of input stellar parameters for the computation of the activity index by ESP-CS
espucd		float		Data from the ESP-UCD (ultra cool dwarfs) processing
teff_espucd	astrophysical_parameters_teff_espucd	float	K	Effective temperature estimate from ESP-UCD based on the RP spectrum
teff_espucd_uncertainty	astrophysical_parameters_teff_espucd_uncertainty	float	K	Uncertainty of the effective temperature estimate produced by ESP-UCD
flags_espucd	astrophysical_parameters_flags_espucd	byte		Quality flags of the ESP-UCD parameter estimates
flame		float		Stellar parameters from the Final Luminosity Age Mass Estimator (FLAME)
radius_flame	astrophysical_parameters_radius_flame	float	solRad	Radius of the star from FLAME using teffGspphot and lumFlame
radius_flame_lower	astrophysical_parameters_radius_flame_lower	float	solRad	Lower confidence level (16%) of radiusFlame
radius_flame_upper	astrophysical_parameters_radius_flame_upper	float	solRad	Upper confidence level (84%) of radiusFlame
lum_flame	astrophysical_parameters_lum_flame	float	solLum	Luminosity of the star from FLAME using G band magnitude, extinction (agGspphot), parallax or distance, and a bolometric correction bcFlame
lum_flame_lower	astrophysical_parameters_lum_flame_lower	float	solLum	Lower confidence level (16%) of lumFlame
lum_flame_upper	astrophysical_parameters_lum_flame_upper	float	solLum	Upper confidence level (84%) of lumFlame
mass_flame	astrophysical_parameters_mass_flame	float	solMass	Mass of the star from FLAME using stellar models, lumFlame, and teffGspphot
mass_flame_lower	astrophysical_parameters_mass_flame_lower	float	solMass	Lower confidence level (16%) of massFlame
mass_flame_upper	astrophysical_parameters_mass_flame_upper	float	solMass	Upper confidence level (84%) of massFlame
age_flame	astrophysical_parameters_age_flame	float	Gyr	Age of the star from FLAME using stellar models, see massFlame for details
age_flame_lower	astrophysical_parameters_age_flame_lower	float	Gyr	Lower confidence level (16%) of ageFlame
age_flame_upper	astrophysical_parameters_age_flame_upper	float	Gyr	Upper confidence level (84%) of ageFlame
flags_flame	astrophysical_parameters_flags_flame	byte		Flags indicating quality and processing information from FLAME
evolstage_flame	astrophysical_parameters_evolstage_flame	integer		Evolutionary stage of the star from FLAME using stellar models, see massFlame for details
gravredshift_flame	astrophysical_parameters_gravredshift_flame	float	km.s**-1	Gravitational redshift from FLAME using radiusFlame and loggGspphot
gravredshift_flame_lower	astrophysical_parameters_gravredshift_flame_lower	float	km.s**-1	Lower confidence level (16%) of gravredshiftFlame
gravredshift_flame_upper	astrophysical_parameters_gravredshift_flame_upper	float	km.s**-1	Upper confidence level (84%) of gravredshiftFlame
bc_flame	astrophysical_parameters_bc_flame	float	mag	Bolometric correction used to derive lumFlame
msc		float		Stellar parameters from the Multiple Star Classifier (MSC)
mh_msc	astrophysical_parameters_mh_msc	float	'dex'	Metallicity of the source treated as a binary system from MSC using BP/RP spectra and parallax
mh_msc_upper	astrophysical_parameters_mh_msc_upper	float	'dex'	Upper confidence level (84%) of the metallicity from MSC using BP/RP spectra and parallax
mh_msc_lower	astrophysical_parameters_mh_msc_lower	float	'dex'	Lower confidence level (16%) of the metallicity from MSC using BP/RP spectra and parallax
azero_msc	astrophysical_parameters_azero_msc	float	mag	Monochromatic extinction \(A_0\) at 547.7nm of the source treated as a binary system from MSC using BP/RP spectra and parallax
azero_msc_upper	astrophysical_parameters_azero_msc_upper	float	mag	Upper confidence level (84%) of monochromatic extinction \(A_0\) at 547.7nm from MSC using BP/RP spectra and parallax
azero_msc_lower	astrophysical_parameters_azero_msc_lower	float	mag	Lower confidence level (16%) of monochromatic extinction \(A_0\) at 547.7nm from MSC using BP/RP spectra and parallax
distance_msc	astrophysical_parameters_distance_msc	float	pc	Distance from MSC using BP/RP spectra and parallax
distance_msc_upper	astrophysical_parameters_distance_msc_upper	float	pc	Upper confidence level (84%) of distance from MSC using BP/RP spectra and parallax
distance_msc_lower	astrophysical_parameters_distance_msc_lower	float	pc	Lower confidence level (16%) of distance from MSC using BP/RP spectra and parallax
teff_msc1	astrophysical_parameters_teff_msc1	float	K	Effective temperature of the primary from MSC using BP/RP spectra and parallax
teff_msc1_upper	astrophysical_parameters_teff_msc1_upper	float	K	Upper confidence level (84%) of effective temperature of the primary from MSC using BP/RP spectra and parallax
teff_msc1_lower	astrophysical_parameters_teff_msc1_lower	float	K	Lower confidence level (16%) of effective temperature of the primary from MSC using BP/RP spectra and parallax
teff_msc2	astrophysical_parameters_teff_msc2	float	K	Effective temperature of the secondary from MSC using BP/RP spectra and parallax
teff_msc2_upper	astrophysical_parameters_teff_msc2_upper	float	K	Upper confidence level (84%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax
teff_msc2_lower	astrophysical_parameters_teff_msc2_lower	float	K	Lower confidence level (16%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax
logg_msc1	astrophysical_parameters_logg_msc1	float	log(cm.s**-2)	Surface gravity of the primary from MSC using BP/RP spectra and parallax
logg_msc1_upper	astrophysical_parameters_logg_msc1_upper	float	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	astrophysical_parameters_logg_msc1_lower	float	log(cm.s**-2)	Lower confidence level (16%) of surface gravity of the primary from MSC using BP/RP spectra and parallax
logg_msc2	astrophysical_parameters_logg_msc2	float	log(cm.s**-2)	Surface gravity of the secondary from MSC using BP/RP spectra and parallax
logg_msc2_upper	astrophysical_parameters_logg_msc2_upper	float	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	astrophysical_parameters_logg_msc2_lower	float	log(cm.s**-2)	Lower confidence level (16%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax
ag_msc	astrophysical_parameters_ag_msc	float	mag	Extinction in G band of the source treated as a binary system from MSC using BP/RP spectra and parallax
ag_msc_upper	astrophysical_parameters_ag_msc_upper	float	mag	Upper confidence level (84%) of extinction in G band from MSC using BP/RP spectra and parallax
ag_msc_lower	astrophysical_parameters_ag_msc_lower	float	mag	Lower confidence level (16%) of extinction in G band from MSC using BP/RP spectra and parallax
logposterior_msc	astrophysical_parameters_logposterior_msc	float		Goodness-of-fit score (normalised log-posterior) of MSC MCMC
mcmcaccept_msc	astrophysical_parameters_mcmcaccept_msc	float		Mean MCMC acceptance rate of MSC MCMC
mcmcdrift_msc	astrophysical_parameters_mcmcdrift_msc	float		Mean drift of the MSC MCMC chain in units of parameter standard deviation
flags_msc	astrophysical_parameters_flags_msc	boolean		Flag indicating quality information from MSC
oa		float		ID and information for Outlier Analysis (OA) cross-match
neuron_oa_id	astrophysical_parameters_neuron_oa_id	long		Identifier of the OA SOM map neuron that represents the source
neuron_oa_dist	astrophysical_parameters_neuron_oa_dist	float		Distance between the source XP spectra and the OA neuron XP prototype that represents the source
neuron_oa_dist_percentile_rank	astrophysical_parameters_neuron_oa_dist_percentile_rank	integer		Percentile rank according to the distance distribution of the OA neuron that represents the source
flags_oa	astrophysical_parameters_flags_oa	short		Flags indicating quality and processing information from OA
astrophysical_parameters_supp		float		This table contains additional parameters from the Apsis processing chain, compared to the main table AstrophysicalParameters, from modules that produce more than one result for a parameter. It contains (1) the individual library results from GSP-Phot, (2) FLAME results from processing GSP-Spec parameters given in the AstrophysicalParameters table, and (3) results from the GSP-Spec ANN algorithm.
_index	astrophysical_parameters_supp__index	integer		Offset of this row in the source file for this table (see _file_max)
epoch_photometry		float		Epoch photometry. Each row in this table contains the light curve for a given object in bands G, BP and RP as stored in the DataLink Massive data base. This table makes extensive use of array types. It can be obtained selecting the RAW data structure option. A flat table (sparse cube), which one photometric point per source per row can be obtained using INDIVIDUAL or COMBINED. Note this table is not available through the main archive TAP interface, but via the Massive Data service, indexed by the VO Datalink protocol.
_index	epoch_photometry__index	integer		Offset of this row in the source file for this table (see _file_max)
galaxy_candidates		float		This table contains parameters derived from various modules dedicated to the classification and characterisation of sources considered as galaxy candidates. This table has been constructed with the intention to be complete rather than pure and, as such, it will contain a large fraction of non-genuine extragalactic sources. Purer samples can be drawn using dedicated flags or queries.
_index	galaxy_candidates__index	integer		Offset of this row in the source file for this table (see _file_max)
nss_acceleration_astro		float		This table contains non-single-star astrometric models for sources having a non-linear proper motion which is compatible with an acceleration solution. Several possible models are hosted within the same table and they are indicated by the field nssSolutionType. The description of this latter lists all possible solution types considered for this release. Only a selection of parameters hosted in this table are provided here, depending on the solution. The details of those is given in the description of field bitIndex, which can also be used to extract the relevant elements of the correlation vector corrVec.
_index	nss_acceleration_astro__index	integer		Offset of this row in the source file for this table
nss_solution_type	nss_acceleration_astro_nss_solution_type	byte		NSS model adopted
accel_ra	nss_acceleration_astro_accel_ra	double	mas.yr**-2	Acceleration in RA
accel_ra_error	nss_acceleration_astro_accel_ra_error	float	mas.yr**-2	Standard error of Acceleration in RA
accel_dec	nss_acceleration_astro_accel_dec	double	mas.yr**-2	Acceleration in DEC
accel_dec_error	nss_acceleration_astro_accel_dec_error	float	mas.yr**-2	Standard error of Acceleration in DEC
deriv_accel_ra	nss_acceleration_astro_deriv_accel_ra	double	mas.yr**-3	Time derivative of the accel. in RA
deriv_accel_ra_error	nss_acceleration_astro_deriv_accel_ra_error	float	mas.yr**-3	Standard error of Time derivative of the acceleration in RA
deriv_accel_dec	nss_acceleration_astro_deriv_accel_dec	double	mas.yr**-3	Time derivative of the accel. in DEC
deriv_accel_dec_error	nss_acceleration_astro_deriv_accel_dec_error	float	mas.yr**-3	Standard error of Time derivative of the acceleration in DEC
astrometric_n_obs_al	nss_acceleration_astro_astrometric_n_obs_al	integer		Total astrometric CCD observations in AL considered
astrometric_n_good_obs_al	nss_acceleration_astro_astrometric_n_good_obs_al	integer		Total astrometric CCD observations in AL actually used
bit_index	nss_acceleration_astro_bit_index	long		Boolean mask for the fields above in the corrVec matrix
corr_vec	nss_acceleration_astro_corr_vec	array float		Vector form of the upper triangle of the correlation matrix
obj_func	nss_acceleration_astro_obj_func	float		Value of the objective function at the solution
goodness_of_fit	nss_acceleration_astro_goodness_of_fit	float		Goodness of fit in the Hipparcos sense
significance	nss_acceleration_astro_significance	float		The significance of the solution (i.e. how worth keeping a model is)
flags	nss_acceleration_astro_flags	long		Quality flag for the achieved NSS solution
nss_non_linear_spectro		float		This table contains non-single-star orbital models for spectroscopic binaries compatible with a trend. Several possible models are hosted within the same table and they are indicated by the field nssSolutionType. The description of this latter lists all possible solution types considered for this release. Only a selection of parameters hosted in this table are provided here, depending on the solution. The details of those is given in the description of field bitIndex, which can also be used to extract the relevant elements of the correlation vector corrVec.
_index	nss_non_linear_spectro__index	integer		Offset of this row in the source file for this table
nss_solution_type	nss_non_linear_spectro_nss_solution_type	byte		NSS model adopted
mean_velocity	nss_non_linear_spectro_mean_velocity	double	km.s**-1	Mean velocity
mean_velocity_error	nss_non_linear_spectro_mean_velocity_error	float	km.s**-1	Standard error of Mean velocity
first_deriv_velocity	nss_non_linear_spectro_first_deriv_velocity	double	Km.s-1.d-1	First order derivative of the velocity
first_deriv_velocity_error	nss_non_linear_spectro_first_deriv_velocity_error	float	Km.s-1.d-1	Standard error of First order derivative of the velocity
second_deriv_velocity	nss_non_linear_spectro_second_deriv_velocity	double	Km.s-1.d-2	Second order derivative of the velocity
second_deriv_velocity_error	nss_non_linear_spectro_second_deriv_velocity_error	float	Km.s-1.d-2	Standard error of Second order derivative of the velocity
rv_n_obs_primary	nss_non_linear_spectro_rv_n_obs_primary	integer		Total number of radial velocities considered for the primary
rv_n_good_obs_primary	nss_non_linear_spectro_rv_n_good_obs_primary	integer		Total number of radial velocities actually used for the primary
bit_index	nss_non_linear_spectro_bit_index	long		Boolean mask for the fields above in the corrVec matrix
corr_vec	nss_non_linear_spectro_corr_vec	array float		Vector form of the upper triangle of the correlation matrix
obj_func	nss_non_linear_spectro_obj_func	float		Value of the objective function at the solution
goodness_of_fit	nss_non_linear_spectro_goodness_of_fit	float		Goodness of fit in the Hipparcos sense
flags	nss_non_linear_spectro_flags	long		Quality flag for the achieved NSS solution
nss_two_body_orbit		float		This table contains non-single-star orbital models for sources compatible with an orbital two-body solution. This covers astrometric binaries, spectroscopic binaries, eclipsing binaries and certain combinations thereof. Several possible models are hosted within the same table and they are indicated by the field nssSolutionType. The description of this latter lists all possible solution types considered for this release. Only a selection of parameters hosted in this table are provided here, depending on the solution. The details of those is given in the description of field bitIndex, which can also be used to extract the relevant elements of the correlation vector corrVec. Warning: as a source may receive independent astrometric, spectroscopic or photometric orbits, a query using a given sourceId may return several solutions. This has to be accounted for when doing a crossmatch by sourceId.
_index	nss_two_body_orbit__index	array integer		Offset of rows for this source_id in the source file for this table
nss_vim_fl		float		This table contains non-single-star models for sources compatible with an Variability Induced Mover (VIM) solution. Several possible models are in principle hosted within the same table and they are indicated by the field nssSolutionType. The description of this latter lists all possible solution types considered for this release. Only a selection of parameters hosted in this table are provided here, depending on the solution. The details of those is given in the description of field bitIndex, which can also be used to extract the relevant elements of the correlation vector corrVec. For DR3, only VIMF solutions are provided here.
_index	nss_vim_fl__index	integer		Offset of this row in the source file for this table
nss_solution_type	nss_vim_fl_nss_solution_type	byte		NSS model adopted
ref_flux_g	nss_vim_fl_ref_flux_g	float	'electron'.s**-1	Reference flux in the G band
vim_d_ra	nss_vim_fl_vim_d_ra	double	mas	VIM coordinate in RA
vim_d_ra_error	nss_vim_fl_vim_d_ra_error	float	mas	Standard error of VIM coordinate in RA
vim_d_dec	nss_vim_fl_vim_d_dec	double	mas	VIM coordinate in DEC
vim_d_dec_error	nss_vim_fl_vim_d_dec_error	float	mas	Standard error of VIM coordinate in DEC
astrometric_n_obs_al	nss_vim_fl_astrometric_n_obs_al	integer		Total astrometric CCD observations in AL considered
astrometric_n_good_obs_al	nss_vim_fl_astrometric_n_good_obs_al	integer		Total astrometric CCD observations in AL actually used
bit_index	nss_vim_fl_bit_index	long		Boolean mask for the fields above in the corrVec matrix
corr_vec	nss_vim_fl_corr_vec	array float		Vector form of the upper triangle of the correlation matrix
obj_func	nss_vim_fl_obj_func	float		Value of the objective function at the solution
goodness_of_fit	nss_vim_fl_goodness_of_fit	float		Goodness of fit in the Hipparcos sense
efficiency	nss_vim_fl_efficiency	float		Efficiency of the solution
significance	nss_vim_fl_significance	float		The significance of the solution (i.e. how worth keeping a model is)
flags	nss_vim_fl_flags	long		Quality flag for the achieved NSS solution
qso_candidates		float		This table contains parameters derived from various modules dedicated to the classification and characterisation of sources considered as QSO candidates. Together with those, the QSOs used to define the Gaia-CRF3 are also listed in this table. This table has been constructed with the intention to be complete rather than pure and, as such, it will contain a large fraction of non-genuine extragalactic sources. Purer samples can be drawn using dedicated flags or queries.
_index	qso_candidates__index	integer		Offset of this row in the source file for this table (see _file_max)
astrometric_selection_flag	qso_candidates_astrometric_selection_flag	boolean		Flag indicating if the source is part of the astrometric selection
gaia_crf_source	qso_candidates_gaia_crf_source	boolean		Flag indicative of whether the source was used define the Gaia-CRF3
vari_best_class_name	qso_candidates_vari_best_class_name	byte		Name of best class, see table VariClassifierClassDefinition for details of the class
vari_best_class_score	qso_candidates_vari_best_class_score	float		Score of the best class
fractional_variability_g	qso_candidates_fractional_variability_g	float		Fractional variability in the G band
structure_function_index	qso_candidates_structure_function_index	float		Index of the first-order structure function in the G band
structure_function_index_scatter	qso_candidates_structure_function_index_scatter	double		Standard deviation of the index of the structure function
qso_variability	qso_candidates_qso_variability	float		Quasar variability metric in the G band
non_qso_variability	qso_candidates_non_qso_variability	float		Non-quasar variability metric in the G band
vari_agn_membership_score	qso_candidates_vari_agn_membership_score	double		Membership score (0=lowest,1=highest) of source to be of AGN type
classprob_dsc_combmod_quasar	qso_candidates_classprob_dsc_combmod_quasar	float		Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)
classprob_dsc_combmod_galaxy	qso_candidates_classprob_dsc_combmod_galaxy	float		Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)
classlabel_dsc	qso_candidates_classlabel_dsc	byte		Class assigned by DSC based on the probability from its Combmod classifier
classlabel_dsc_joint	qso_candidates_classlabel_dsc_joint	byte		Class assigned by DSC based on the probability from its Specmod and Allosmod classifiers
classlabel_oa	qso_candidates_classlabel_oa	byte		Class assigned by OA the neuron that represents the source
redshift_qsoc	qso_candidates_redshift_qsoc	float		Redshift from QSOC
redshift_qsoc_lower	qso_candidates_redshift_qsoc_lower	float		Redshift lower confidence level from QSOC
redshift_qsoc_upper	qso_candidates_redshift_qsoc_upper	float		Redshift upper confidence level from QSOC
ccfratio_qsoc	qso_candidates_ccfratio_qsoc	float		Value of the cross-correlation function used to derive the redshift from QSOC, relative to the maximum value
zscore_qsoc	qso_candidates_zscore_qsoc	float		Redshift zscore from QSOC
flags_qsoc	qso_candidates_flags_qsoc	long		Processing flags for the analysis based on BP/RP Spectra from QSOC
n_transits	qso_candidates_n_transits	integer		Number of transits used for the morphological analysis
intensity_quasar	qso_candidates_intensity_quasar	double	'electron'.s**-1	Fitted intensity of the quasar at its center
intensity_quasar_error	qso_candidates_intensity_quasar_error	double	'electron'.s**-1	Error on the fitted intensity of the quasar at its center
intensity_hostgalaxy	qso_candidates_intensity_hostgalaxy	double	'electron'.s**-1	Fitted intensity of the host galaxy at the effective radius
intensity_hostgalaxy_error	qso_candidates_intensity_hostgalaxy_error	double	'electron'.s**-1	Error on the fitted intensity of the host galaxy at effective radius
radius_hostgalaxy	qso_candidates_radius_hostgalaxy	double	mas	Fitted effective radius of the host galaxy
radius_hostgalaxy_error	qso_candidates_radius_hostgalaxy_error	double	mas	Error on the fitted effective radius of the host galaxy
sersic_index	qso_candidates_sersic_index	float		Fitted sersic Index
sersic_index_error	qso_candidates_sersic_index_error	float		Error on the fitted sersic Index
ellipticity_hostgalaxy	qso_candidates_ellipticity_hostgalaxy	double		Fitted ellipticity of the host galaxy
ellipticity_hostgalaxy_error	qso_candidates_ellipticity_hostgalaxy_error	double		Error on the fitted ellipticity of the host galaxy
posangle_hostgalaxy	qso_candidates_posangle_hostgalaxy	double	deg	Fitted position angle of the host galaxy
posangle_hostgalaxy_error	qso_candidates_posangle_hostgalaxy_error	double	deg	Error on the fitted position angle of the host galaxy
host_galaxy_detected	qso_candidates_host_galaxy_detected	boolean		Flag indicating whether a host galaxy has been detected
l2_norm	qso_candidates_l2_norm	double		L2 norm for the fitted Sersic profile
morph_params_corr_vec	qso_candidates_morph_params_corr_vec	array double		Vector form of the upper triangle of the correlation matrix for the fitted morphological parameters
host_galaxy_flag	qso_candidates_host_galaxy_flag	byte		Flag indicative of processing or scientific quality for the morphological parameters fitting
source_selection_flags	qso_candidates_source_selection_flags	integer		Bit indicative of whether the input data from a given module met the source list eligibility criteria for the source of interest
rvs_mean_spectrum		float		This is the RVS mean sampled spectrum table. The spectra are in the rest frame, they are normalised and their wavelength grid ranges from 846 to 870 nm in steps of 0.01 nm (2401 elements).
_index	rvs_mean_spectrum__index	integer		Offset of this row in the source file for this table (see _file_max)
ra	rvs_mean_spectrum_ra	double	deg	Right Ascension
dec	rvs_mean_spectrum_dec	double	deg	Declination
flux	rvs_mean_spectrum_flux	array float		array of fluxes
flux_error	rvs_mean_spectrum_flux_error	array float		array of uncertainties in flux
combined_transits	rvs_mean_spectrum_combined_transits	short		number of combined transits
combined_ccds	rvs_mean_spectrum_combined_ccds	short		number of combined CCD spectra
deblended_ccds	rvs_mean_spectrum_deblended_ccds	short		number of deblended CCD spectra
vari_agn		float		This table provides information on AGN properties.
_index	vari_agn__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_cepheid		float		This table describes the Cepheid stars.
_index	vari_cepheid__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_classifier_result		float		Table with variability classification results of all classifiers, which are identified by the classifierName column. In DR3, multiple classifiers (depending on class) are combined into a single classifier with classifierName=`nTransits:5+', which is described in VariClassifierDefinition and identifies the classes defined in VariClassifierClassDefinition.
_index	vari_classifier_result__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_compact_companion		float		This table describes the compact companion candidates.
_index	vari_compact_companion__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_eclipsing_binary		float		This table describes the properties of the eclipsing binaries resulting from the variability analysis.
_index	vari_eclipsing_binary__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_long_period_variable		float		This table describes the Long Period Variable stars. Some entries can be NaN when absent.
_index	vari_long_period_variable__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_microlensing		float		This table describes the microlensing events.
_index	vari_microlensing__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_ms_oscillator		float		This table describes the main-sequence oscillators.
_index	vari_ms_oscillator__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_planetary_transit		float		This table describes the Planetary Transit candidate events.
_index	vari_planetary_transit__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_rad_vel_statistics		float		Statistical parameters of radial velocity time series, using only transits not rejected, see rejectedByVariability column in VariEpochRadialVelocity. Note that NaN will be reported when the parameter value is missing or cannot be calculated.
_index	vari_rad_vel_statistics__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_rotation_modulation		float		This table describes the solar-like stars with rotational modulation.
_index	vari_rotation_modulation__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_rrlyrae		float		This table describes the RR Lyrae stars.
_index	vari_rrlyrae__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_short_timescale		float		This table describes the short-timescale sources.
_index	vari_short_timescale__index	integer		Offset of this row in the source file for this table (see _file_max)
vari_summary		float		Summary table that provides the information on where a sourceId can be found in the different Variability tables and statistical parameters of time series, using only transits not rejected. Note that NULL is reported when the statistical parameter value is missing or cannot be calculated.
_index	vari_summary__index	integer		Offset of this row in the source file for this table (see _file_max)
xp_continuous_mean_spectrum		float		Table hosting the mean BP and RP spectra based on the continuous representation in basis functions.
_index	xp_continuous_mean_spectrum__index	integer		Offset of this row in the source file for this table (see _file_max)
bp_basis_function_id	xp_continuous_mean_spectrum_bp_basis_function_id	short		Identifier defining the set of basis functions for the BP spectrum representation
bp_degrees_of_freedom	xp_continuous_mean_spectrum_bp_degrees_of_freedom	short		Degrees of freedom for the BP spectrum representation
bp_n_parameters	xp_continuous_mean_spectrum_bp_n_parameters	byte		Number of parameters for the BP spectrum representation
bp_n_measurements	xp_continuous_mean_spectrum_bp_n_measurements	short		Number of measurements used for the BP spectrum generation
bp_n_rejected_measurements	xp_continuous_mean_spectrum_bp_n_rejected_measurements	short		Number of rejected measurements in the BP spectrum generation
bp_standard_deviation	xp_continuous_mean_spectrum_bp_standard_deviation	float		Standard deviation for the BP spectrum representation
bp_chi_squared	xp_continuous_mean_spectrum_bp_chi_squared	float		Chi squared for the BP spectrum representation
bp_coefficients	xp_continuous_mean_spectrum_bp_coefficients	array double		Basis function coefficients for the BP spectrum representation
bp_coefficient_errors	xp_continuous_mean_spectrum_bp_coefficient_errors	array float		Basis function coefficient errors for the BP spectrum representation
bp_n_relevant_bases	xp_continuous_mean_spectrum_bp_n_relevant_bases	short		Number of bases that are relevant for the representation of this mean BP spectrum
bp_relative_shrinking	xp_continuous_mean_spectrum_bp_relative_shrinking	float		Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean BP spectrum
rp_basis_function_id	xp_continuous_mean_spectrum_rp_basis_function_id	short		Identifier defining the set of basis functions for the BP spectrum representation
rp_degrees_of_freedom	xp_continuous_mean_spectrum_rp_degrees_of_freedom	short		Degrees of freedom for the RP spectrum representation
rp_n_parameters	xp_continuous_mean_spectrum_rp_n_parameters	byte		Number of parameters for the RP spectrum representation
rp_n_measurements	xp_continuous_mean_spectrum_rp_n_measurements	short		Number of measurements used for the RP spectrum generation
rp_n_rejected_measurements	xp_continuous_mean_spectrum_rp_n_rejected_measurements	short		Number of rejected measurements in the RP spectrum generation
rp_standard_deviation	xp_continuous_mean_spectrum_rp_standard_deviation	float		Standard deviation for the RP spectrum representation
rp_chi_squared	xp_continuous_mean_spectrum_rp_chi_squared	float		Chi squared for the RP spectrum representation
rp_coefficients	xp_continuous_mean_spectrum_rp_coefficients	array double		Basis function coefficients for the RP spectrum representation
rp_coefficient_errors	xp_continuous_mean_spectrum_rp_coefficient_errors	array float		Basis function coefficient errors for the RP spectrum representation
rp_n_relevant_bases	xp_continuous_mean_spectrum_rp_n_relevant_bases	short		Number of bases that are relevant for the representation of this mean RP spectrum
rp_relative_shrinking	xp_continuous_mean_spectrum_rp_relative_shrinking	float		Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean RP spectrum
xp_sampled_mean_spectrum		float		This is the BP/RP externally calibrated sampled mean spectrum. All mean spectra are sampled to the same set of absolute wavelength positions, which can be found in the field wavelength of table XpMerge.
_index	xp_sampled_mean_spectrum__index	integer		Offset of this row in the source file for this table (see _file_max)
ra	xp_sampled_mean_spectrum_ra	double	deg	Right Ascension
dec	xp_sampled_mean_spectrum_dec	double	deg	Declination
flux	xp_sampled_mean_spectrum_flux	array float	W.m-2.nm-1	mean BP + RP combined spectrum flux
flux_error	xp_sampled_mean_spectrum_flux_error	array float	W.m-2.nm-1	mean BP + RP combined spectrum flux error
xp_summary		float		This tables contains auxiliary information about the mean BP/RP spectrum of a given source. It should be used in order to refine queries on spectra and build dedicated samples before interrogating the DataLink protocol to download the results of those queries.
_index	xp_summary__index	integer		Offset of this row in the source file for this table (see _file_max)
bp_n_relevant_bases	xp_summary_bp_n_relevant_bases	short		Number of bases that are relevant for the representation of this mean BP spectrum
bp_relative_shrinking	xp_summary_bp_relative_shrinking	float		Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean BP spectrum
bp_n_measurements	xp_summary_bp_n_measurements	short		Number of measurements used for the BP spectrum generation
bp_n_rejected_measurements	xp_summary_bp_n_rejected_measurements	short		Number of rejected measurements in the BP spectrum generation
bp_standard_deviation	xp_summary_bp_standard_deviation	float	'electron'.s-1.pixel-1	Standard deviation for the BP spectrum representation
bp_chi_squared	xp_summary_bp_chi_squared	float		Chi squared for the BP spectrum representation
bp_n_transits	xp_summary_bp_n_transits	short		Number of transits contributing to the mean in BP
bp_n_contaminated_transits	xp_summary_bp_n_contaminated_transits	short		Number of contaminated transits in BP
bp_n_blended_transits	xp_summary_bp_n_blended_transits	short		Number of blended transits in BP
rp_n_relevant_bases	xp_summary_rp_n_relevant_bases	short		Number of bases that are relevant for the representation of this mean RP spectrum
rp_relative_shrinking	xp_summary_rp_relative_shrinking	float		Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean RP spectrum
rp_n_measurements	xp_summary_rp_n_measurements	short		Number of measurements used for the RP spectrum generation
rp_n_rejected_measurements	xp_summary_rp_n_rejected_measurements	short		Number of rejected measurements in the RP spectrum generation
rp_standard_deviation	xp_summary_rp_standard_deviation	float	'electron'.s-1.pixel-1	Standard deviation for the RP spectrum representation
rp_chi_squared	xp_summary_rp_chi_squared	float		Chi squared for the RP spectrum representation
rp_n_transits	xp_summary_rp_n_transits	short		Number of transits contributing to the mean in RP
rp_n_contaminated_transits	xp_summary_rp_n_contaminated_transits	short		Number of contaminated transits in RP
rp_n_blended_transits	xp_summary_rp_n_blended_transits	short		Number of blended transits in RP

About Catalog

Gaia Data Release 3 from the European Space Agency
Important links to official Gaia Data Release documentation:

Preset field selections:

gaia_source: This table has an entry for every Gaia observed source as published with this data release. It contains the basic source parameters, in their final state as processed by the Gaia Data Processing and Analysis Consortium from the raw data coming from the spacecraft. The table is complemented with others containing information specific to certain kinds of objects (e.g. Solar--system objects, non--single stars, variables etc.) and value--added processing (e.g. astrophysical parameters etc.). Further array data types (spectra, epoch measurements) are presented separately via `Datalink' resources.

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_file_upper Upper bound for HEALpix index level 8 of source file for this row (used in determining source file name: "%s_%06d-%06d" % (table_name, source_id >> 43, _file_max))	source_id Unique source identifier (unique within a particular Data Release)	random_index Random index for use when selecting subsets	ref_epoch yr Reference epoch	pos Barycentric position								parallax mas Parallax	parallax_error mas Standard error of parallax	parallax_over_error Parallax divided by its standard error	pm mas/year Proper motion					corr astrometric correlation coefficients										astrometric solution metadata																																					duplicated_source Source with multiple source identifiers	phot_g G-band photometry					phot_bp BP photometry							phot_rp RP photometry								phot_proc_mode Photometry processing mode	bp_rp mag BP - RP colour	bp_g mag BP - G colour	g_rp mag G - RP colour	rv Radial velocity															vbroad km.s**-1 Spectral line broadening parameter	vbroad_error km.s**-1 Uncertainty on the spectral line broadening	vbroad_nb_transits Number of transits used to compute vbroad	grvs_mag mag Integrated Grvs magnitude	grvs_mag_error mag Grvs magnitude uncertainty	grvs_mag_nb_transits Number of transits used to compute Grvs	rvs_spec_sig_to_noise Signal to noise ratio in the mean RVS spectrum	phot_variable_flag Photometric variability flag	metadata_flags Flags that indicate presence of more specialized data for a given source											astrophysical_parameters This is the main table containing the 1D astrophysical parameters produced by the Apsis processing chain developed in Gaia DPAC CU8. Additional parameters can be found in table AstrophysicalParametersSupp.																																																																astrophysical_parameters_supp This table contains additional parameters from the Apsis processing chain, compared to the main table AstrophysicalParameters, from modules that produce more than one result for a parameter. It contains (1) the individual library results from GSP-Phot, (2) FLAME results from processing GSP-Spec parameters given in the AstrophysicalParameters table, and (3) results from the GSP-Spec ANN algorithm.	epoch_photometry Epoch photometry. Each row in this table contains the light curve for a given object in bands G, BP and RP as stored in the DataLink Massive data base. This table makes extensive use of array types. It can be obtained selecting the RAW data structure option. A flat table (sparse cube), which one photometric point per source per row can be obtained using INDIVIDUAL or COMBINED. Note this table is not available through the main archive TAP interface, but via the Massive Data service, indexed by the VO Datalink protocol.	galaxy_candidates This table contains parameters derived from various modules dedicated to the classification and characterisation of sources considered as galaxy candidates. This table has been constructed with the intention to be complete rather than pure and, as such, it will contain a large fraction of non-genuine extragalactic sources. Purer samples can be drawn using dedicated flags or queries.	nss_acceleration_astro This table contains non-single-star astrometric models for sources having a non-linear proper motion which is compatible with an acceleration solution. Several possible models are hosted within the same table and they are indicated by the field nssSolutionType. The description of this latter lists all possible solution types considered for this release. Only a selection of parameters hosted in this table are provided here, depending on the solution. The details of those is given in the description of field bitIndex, which can also be used to extract the relevant elements of the correlation vector corrVec.																		nss_non_linear_spectro This table contains non-single-star orbital models for spectroscopic binaries compatible with a trend. Several possible models are hosted within the same table and they are indicated by the field nssSolutionType. The description of this latter lists all possible solution types considered for this release. Only a selection of parameters hosted in this table are provided here, depending on the solution. The details of those is given in the description of field bitIndex, which can also be used to extract the relevant elements of the correlation vector corrVec.															nss_two_body_orbit This table contains non-single-star orbital models for sources compatible with an orbital two-body solution. This covers astrometric binaries, spectroscopic binaries, eclipsing binaries and certain combinations thereof. Several possible models are hosted within the same table and they are indicated by the field nssSolutionType. The description of this latter lists all possible solution types considered for this release. Only a selection of parameters hosted in this table are provided here, depending on the solution. The details of those is given in the description of field bitIndex, which can also be used to extract the relevant elements of the correlation vector corrVec. Warning: as a source may receive independent astrometric, spectroscopic or photometric orbits, a query using a given sourceId may return several solutions. This has to be accounted for when doing a crossmatch by sourceId.	nss_vim_fl This table contains non-single-star models for sources compatible with an Variability Induced Mover (VIM) solution. Several possible models are in principle hosted within the same table and they are indicated by the field nssSolutionType. The description of this latter lists all possible solution types considered for this release. Only a selection of parameters hosted in this table are provided here, depending on the solution. The details of those is given in the description of field bitIndex, which can also be used to extract the relevant elements of the correlation vector corrVec. For DR3, only VIMF solutions are provided here.																qso_candidates This table contains parameters derived from various modules dedicated to the classification and characterisation of sources considered as QSO candidates. Together with those, the QSOs used to define the Gaia-CRF3 are also listed in this table. This table has been constructed with the intention to be complete rather than pure and, as such, it will contain a large fraction of non-genuine extragalactic sources. Purer samples can be drawn using dedicated flags or queries.																																								rvs_mean_spectrum This is the RVS mean sampled spectrum table. The spectra are in the rest frame, they are normalised and their wavelength grid ranges from 846 to 870 nm in steps of 0.01 nm (2401 elements).								vari_agn This table provides information on AGN properties.	vari_cepheid This table describes the Cepheid stars.	vari_classifier_result Table with variability classification results of all classifiers, which are identified by the classifierName column. In DR3, multiple classifiers (depending on class) are combined into a single classifier with classifierName=`nTransits:5+', which is described in VariClassifierDefinition and identifies the classes defined in VariClassifierClassDefinition.	vari_compact_companion This table describes the compact companion candidates.	vari_eclipsing_binary This table describes the properties of the eclipsing binaries resulting from the variability analysis.	vari_long_period_variable This table describes the Long Period Variable stars. Some entries can be NaN when absent.	vari_microlensing This table describes the microlensing events.	vari_ms_oscillator This table describes the main-sequence oscillators.	vari_planetary_transit This table describes the Planetary Transit candidate events.	vari_rad_vel_statistics Statistical parameters of radial velocity time series, using only transits not rejected, see rejectedByVariability column in VariEpochRadialVelocity. Note that NaN will be reported when the parameter value is missing or cannot be calculated.	vari_rotation_modulation This table describes the solar-like stars with rotational modulation.	vari_rrlyrae This table describes the RR Lyrae stars.	vari_short_timescale This table describes the short-timescale sources.	vari_summary Summary table that provides the information on where a sourceId can be found in the different Variability tables and statistical parameters of time series, using only transits not rejected. Note that NULL is reported when the statistical parameter value is missing or cannot be calculated.	xp_continuous_mean_spectrum Table hosting the mean BP and RP spectra based on the continuous representation in basis functions.																							xp_sampled_mean_spectrum This is the BP/RP externally calibrated sampled mean spectrum. All mean spectra are sampled to the same set of absolute wavelength positions, which can be found in the field wavelength of table XpMerge.					xp_summary This tables contains auxiliary information about the mean BP/RP spectrum of a given source. It should be used in order to refine queries on spectra and build dedicated samples before interrogating the DataLink protocol to download the results of those queries.
				ra deg Right ascension	ra_error mas Standard error of right ascension	dec deg Declination	dec_error mas Standard error of declination	l deg Galactic longitude	b deg Galactic latitude	ecl_lon deg Ecliptic longitude	ecl_lat deg Ecliptic latitude				pm mas.yr**-1 Total proper motion	pmra mas.yr**-1 Proper motion in right ascension direction	pmra_error mas.yr**-1 Standard error of proper motion in right ascension direction	pmdec mas.yr**-1 Proper motion in declination direction	pmdec_error mas.yr**-1 Standard error of proper motion in declination direction	ra_dec_corr Correlation between right ascension and declination	ra_parallax_corr Correlation between right ascension and parallax	ra_pmra_corr Correlation between right ascension and proper motion in right ascension	ra_pmdec_corr Correlation between right ascension and proper motion in declination	dec_parallax_corr Correlation between declination and parallax	dec_pmra_corr Correlation between declination and proper motion in right ascension	dec_pmdec_corr Correlation between declination and proper motion in declination	parallax_pmra_corr Correlation between parallax and proper motion in right ascension	parallax_pmdec_corr Correlation between parallax and proper motion in declination	pmra_pmdec_corr Correlation between proper motion in right ascension and proper motion in declination	astrometric_n_obs_al Total number of observations in the along-scan (AL) direction	astrometric_n_obs_ac Total number of observations in the across-scan (AC) direction	astrometric_n_good_obs_al Number of good observations in the along-scan (AL) direction	astrometric_n_bad_obs_al Number of bad observations in the along-scan (AL) direction	astrometric_gof_al Goodness of fit statistic of model wrt along-scan observations	astrometric_chi2_al AL chi-square value	astrometric_excess_noise mas Excess noise of the source	astrometric_excess_noise_sig Significance of excess noise	astrometric_params_solved Which parameters have been solved for?	astrometric_primary_flag Primary or secondary	nu_eff_used_in_astrometry um**-1 Effective wavenumber of the source used in the astrometric solution	pseudocolour um**-1 Astrometrically estimated pseudocolour of the source	pseudocolour_error um**-1 Standard error of the pseudocolour of the source	ra_pseudocolour_corr Correlation between right ascension and pseudocolour	dec_pseudocolour_corr Correlation between declination and pseudocolour	parallax_pseudocolour_corr Correlation between parallax and pseudocolour	pmra_pseudocolour_corr Correlation between proper motion in right asension and pseudocolour	pmdec_pseudocolour_corr Correlation between proper motion in declination and pseudocolour	astrometric_matched_transits Matched FOV transits used in the AGIS solution	visibility_periods_used Number of visibility periods used in Astrometric solution	astrometric_sigma5d_max mas The longest semi-major axis of the 5-d error ellipsoid	matched_transits The number of transits matched to this source	new_matched_transits The number of transits newly incorporated into an existing source in the current cycle	matched_transits_removed The number of transits removed from an existing source in the current cycle	ipd_gof_harmonic_amplitude Amplitude of the IPD GoF versus position angle of scan	ipd_gof_harmonic_phase deg Phase of the IPD GoF versus position angle of scan	ipd_frac_multi_peak Percent of successful-IPD windows with more than one peak	ipd_frac_odd_win Percent of transits with truncated windows or multiple gate	ruwe Renormalised unit weight error	scan_direction_strength_k1 Degree of concentration of scan directions across the source	scan_direction_strength_k2 Degree of concentration of scan directions across the source	scan_direction_strength_k3 Degree of concentration of scan directions across the source	scan_direction_strength_k4 Degree of concentration of scan directions across the source	scan_direction_mean_k1 deg Mean position angle of scan directions across the source	scan_direction_mean_k2 deg Mean position angle of scan directions across the source	scan_direction_mean_k3 deg Mean position angle of scan directions across the source	scan_direction_mean_k4 deg Mean position angle of scan directions across the source		phot_g_n_obs Number of observations contributing to G photometry	phot_g_mean_flux 'electron'.s**-1 G-band mean flux	phot_g_mean_flux_error 'electron'.s**-1 Error on G-band mean flux	phot_g_mean_flux_over_error G-band mean flux divided by its error	phot_g_mean_mag mag G-band mean magnitude	phot_bp_n_obs Number of observations contributing to BP photometry	phot_bp_mean_flux 'electron'.s**-1 Integrated BP mean flux	phot_bp_mean_flux_error 'electron'.s**-1 Error on the integrated BP mean flux	phot_bp_mean_flux_over_error Integrated BP mean flux divided by its error	phot_bp_mean_mag mag Integrated BP mean magnitude	phot_bp_n_contaminated_transits Number of BP contaminated transits	phot_bp_n_blended_transits Number of BP blended transits	phot_rp_n_obs Number of observations contributing to RP photometry	phot_rp_mean_flux 'electron'.s**-1 Integrated RP mean flux	phot_rp_mean_flux_error 'electron'.s**-1 Error on the integrated RP mean flux	phot_rp_mean_flux_over_error Integrated RP mean flux divided by its error	phot_rp_mean_mag mag Integrated RP mean magnitude	phot_bp_rp_excess_factor BP/RP excess factor	phot_rp_n_contaminated_transits Number of RP contaminated transits	phot_rp_n_blended_transits Number of RP blended transits					radial_velocity km.s**-1 Radial velocity	radial_velocity_error km.s**-1 Radial velocity error	rv_method_used Method used to obtain the radial velocity	rv_nb_transits Number of transits used to compute the radial velocity	rv_nb_deblended_transits Number of valid transits that have undergone deblending	rv_visibility_periods_used Number of visibility periods used to estimate the radial velocity	rv_expected_sig_to_noise Expected signal to noise ratio in the combination of the spectra used to obtain the radial velocity	rv_renormalised_gof Radial velocity renormalised goodness of fit	rv_chisq_pvalue P-value for constancy based on a chi-squared criterion	rv_time_duration d Time coverage of the radial velocity time series	rv_amplitude_robust km.s**-1 Total amplitude in the radial velocity time series after outlier removal	rv_template_teff K Teff of the template used to compute the radial velocity	rv_template_logg log(cm.s**-2) Logg of the template used to compute the radial velocity	rv_template_fe_h 'dex' [Fe/H] of the template used to compute the radial velocityy	rv_atm_param_origin Origin of the atmospheric parameters associated to the template									in_qso_candidates Flag indicating the availability of additional information in the QsoCandidates table	in_galaxy_candidates Flag indicating the availability of additional information in the GalaxyCandidates table	non_single_star Flag indicating the availability of additional information in the various Non-Single Star tables	has_xp_continuous Flag indicating the availability of mean BP/RP spectrum in continuous representation for this source	has_xp_sampled Flag indicating the availability of mean BP/RP spectrum in sampled form for this source	has_rvs Flag indicating the availability of mean RVS spectrum for this source	has_epoch_photometry Flag indicating the availability of epoch photometry for this source	has_epoch_rv Flag indicating the availability of epoch radial velocity for this source	has_mcmc_gspphot Flag indicating the availability of GSP-Phot MCMC samples for this source	has_mcmc_msc Flag indicating the availability of MSC MCMC samples for this source	in_andromeda_survey Flag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS)	_index Offset of this row in the source file for this table (see _file_max)	classprob Class probabilities for source classification													teff K stellar effective temperature						logg log(cm.s**-2) stellar surface gravity						mh dex stellar metallicity						distance pc distance to star			azero mag monochromatic extinction			ag mag extinction in G band			abp mag extinction in Bp			arp mag extinction in Rp			ebpminrp mag reddening			mg mag Absolute magnitude			radius solRad Stellar radius			gspphot_metadata Metadata related to the gspphot processing			alphafe dex Abundance of alpha-elements [alpha/Fe]			fem dex Abundance of neutral iron					sife dex Abundance of Silicon					cafe dex Abundance of Calcium					tife dex Abundance of Titanium					mgfe dex Abundance of Magnesium					ndfe dex Abundance of Neodymium					feiim dex Abundance of ionised Iron					sfe dex Abundance of Sulphur					zrfe dex Abundance of Zirconium					nfe dex Abundance of Nitrogen					crfe dex Abundance of Chromium					cefe dex Abundance of Cerium					nife dex Abundance of Nickel					cn0ew dex Equivalent witdh of cyanogen absorption line				dib Diffuse interstellar band (DIB)									gspspec_metadata Metadata related to the gspspec processing	espels Data from the ESP-ELS (emission line stars) processing													esphs Data from the ESP-HS (hot stars) processing													espcs Data from the ESP-CS (cool stars) processing			espucd Data from the ESP-UCD (ultra cool dwarfs) processing			flame Stellar parameters from the Final Luminosity Age Mass Estimator (FLAME)																		msc Stellar parameters from the Multiple Star Classifier (MSC)																												oa ID and information for Outlier Analysis (OA) cross-match				_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table	nss_solution_type NSS model adopted	accel_ra mas.yr**-2 Acceleration in RA	accel_ra_error mas.yr**-2 Standard error of Acceleration in RA	accel_dec mas.yr**-2 Acceleration in DEC	accel_dec_error mas.yr**-2 Standard error of Acceleration in DEC	deriv_accel_ra mas.yr**-3 Time derivative of the accel. in RA	deriv_accel_ra_error mas.yr**-3 Standard error of Time derivative of the acceleration in RA	deriv_accel_dec mas.yr**-3 Time derivative of the accel. in DEC	deriv_accel_dec_error mas.yr**-3 Standard error of Time derivative of the acceleration in DEC	astrometric_n_obs_al Total astrometric CCD observations in AL considered	astrometric_n_good_obs_al Total astrometric CCD observations in AL actually used	bit_index Boolean mask for the fields above in the corrVec matrix	corr_vec Vector form of the upper triangle of the correlation matrix	obj_func Value of the objective function at the solution	goodness_of_fit Goodness of fit in the Hipparcos sense	significance The significance of the solution (i.e. how worth keeping a model is)	flags Quality flag for the achieved NSS solution	_index Offset of this row in the source file for this table	nss_solution_type NSS model adopted	mean_velocity km.s**-1 Mean velocity	mean_velocity_error km.s**-1 Standard error of Mean velocity	first_deriv_velocity Km.s-1.d-1 First order derivative of the velocity	first_deriv_velocity_error Km.s-1.d-1 Standard error of First order derivative of the velocity	second_deriv_velocity Km.s-1.d-2 Second order derivative of the velocity	second_deriv_velocity_error Km.s-1.d-2 Standard error of Second order derivative of the velocity	rv_n_obs_primary Total number of radial velocities considered for the primary	rv_n_good_obs_primary Total number of radial velocities actually used for the primary	bit_index Boolean mask for the fields above in the corrVec matrix	corr_vec Vector form of the upper triangle of the correlation matrix	obj_func Value of the objective function at the solution	goodness_of_fit Goodness of fit in the Hipparcos sense	flags Quality flag for the achieved NSS solution	_index Offset of rows for this source_id in the source file for this table	_index Offset of this row in the source file for this table	nss_solution_type NSS model adopted	ref_flux_g 'electron'.s**-1 Reference flux in the G band	vim_d_ra mas VIM coordinate in RA	vim_d_ra_error mas Standard error of VIM coordinate in RA	vim_d_dec mas VIM coordinate in DEC	vim_d_dec_error mas Standard error of VIM coordinate in DEC	astrometric_n_obs_al Total astrometric CCD observations in AL considered	astrometric_n_good_obs_al Total astrometric CCD observations in AL actually used	bit_index Boolean mask for the fields above in the corrVec matrix	corr_vec Vector form of the upper triangle of the correlation matrix	obj_func Value of the objective function at the solution	goodness_of_fit Goodness of fit in the Hipparcos sense	efficiency Efficiency of the solution	significance The significance of the solution (i.e. how worth keeping a model is)	flags Quality flag for the achieved NSS solution	_index Offset of this row in the source file for this table (see _file_max)	astrometric_selection_flag Flag indicating if the source is part of the astrometric selection	gaia_crf_source Flag indicative of whether the source was used define the Gaia-CRF3	vari_best_class_name Name of best class, see table VariClassifierClassDefinition for details of the class	vari_best_class_score Score of the best class	fractional_variability_g Fractional variability in the G band	structure_function_index Index of the first-order structure function in the G band	structure_function_index_scatter Standard deviation of the index of the structure function	qso_variability Quasar variability metric in the G band	non_qso_variability Non-quasar variability metric in the G band	vari_agn_membership_score Membership score (0=lowest,1=highest) of source to be of AGN type	classprob_dsc_combmod_quasar Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)	classprob_dsc_combmod_galaxy Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)	classlabel_dsc Class assigned by DSC based on the probability from its Combmod classifier	classlabel_dsc_joint Class assigned by DSC based on the probability from its Specmod and Allosmod classifiers	classlabel_oa Class assigned by OA the neuron that represents the source	redshift_qsoc Redshift from QSOC	redshift_qsoc_lower Redshift lower confidence level from QSOC	redshift_qsoc_upper Redshift upper confidence level from QSOC	ccfratio_qsoc Value of the cross-correlation function used to derive the redshift from QSOC, relative to the maximum value	zscore_qsoc Redshift zscore from QSOC	flags_qsoc Processing flags for the analysis based on BP/RP Spectra from QSOC	n_transits Number of transits used for the morphological analysis	intensity_quasar 'electron'.s**-1 Fitted intensity of the quasar at its center	intensity_quasar_error 'electron'.s**-1 Error on the fitted intensity of the quasar at its center	intensity_hostgalaxy 'electron'.s**-1 Fitted intensity of the host galaxy at the effective radius	intensity_hostgalaxy_error 'electron'.s**-1 Error on the fitted intensity of the host galaxy at effective radius	radius_hostgalaxy mas Fitted effective radius of the host galaxy	radius_hostgalaxy_error mas Error on the fitted effective radius of the host galaxy	sersic_index Fitted sersic Index	sersic_index_error Error on the fitted sersic Index	ellipticity_hostgalaxy Fitted ellipticity of the host galaxy	ellipticity_hostgalaxy_error Error on the fitted ellipticity of the host galaxy	posangle_hostgalaxy deg Fitted position angle of the host galaxy	posangle_hostgalaxy_error deg Error on the fitted position angle of the host galaxy	host_galaxy_detected Flag indicating whether a host galaxy has been detected	l2_norm L2 norm for the fitted Sersic profile	morph_params_corr_vec Vector form of the upper triangle of the correlation matrix for the fitted morphological parameters	host_galaxy_flag Flag indicative of processing or scientific quality for the morphological parameters fitting	source_selection_flags Bit indicative of whether the input data from a given module met the source list eligibility criteria for the source of interest	_index Offset of this row in the source file for this table (see _file_max)	ra deg Right Ascension	dec deg Declination	flux array of fluxes	flux_error array of uncertainties in flux	combined_transits number of combined transits	combined_ccds number of combined CCD spectra	deblended_ccds number of deblended CCD spectra	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	_index Offset of this row in the source file for this table (see _file_max)	bp_basis_function_id Identifier defining the set of basis functions for the BP spectrum representation	bp_degrees_of_freedom Degrees of freedom for the BP spectrum representation	bp_n_parameters Number of parameters for the BP spectrum representation	bp_n_measurements Number of measurements used for the BP spectrum generation	bp_n_rejected_measurements Number of rejected measurements in the BP spectrum generation	bp_standard_deviation Standard deviation for the BP spectrum representation	bp_chi_squared Chi squared for the BP spectrum representation	bp_coefficients Basis function coefficients for the BP spectrum representation	bp_coefficient_errors Basis function coefficient errors for the BP spectrum representation	bp_n_relevant_bases Number of bases that are relevant for the representation of this mean BP spectrum	bp_relative_shrinking Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean BP spectrum	rp_basis_function_id Identifier defining the set of basis functions for the BP spectrum representation	rp_degrees_of_freedom Degrees of freedom for the RP spectrum representation	rp_n_parameters Number of parameters for the RP spectrum representation	rp_n_measurements Number of measurements used for the RP spectrum generation	rp_n_rejected_measurements Number of rejected measurements in the RP spectrum generation	rp_standard_deviation Standard deviation for the RP spectrum representation	rp_chi_squared Chi squared for the RP spectrum representation	rp_coefficients Basis function coefficients for the RP spectrum representation	rp_coefficient_errors Basis function coefficient errors for the RP spectrum representation	rp_n_relevant_bases Number of bases that are relevant for the representation of this mean RP spectrum	rp_relative_shrinking Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean RP spectrum	_index Offset of this row in the source file for this table (see _file_max)	ra deg Right Ascension	dec deg Declination	flux W.m-2.nm-1 mean BP + RP combined spectrum flux	flux_error W.m-2.nm-1 mean BP + RP combined spectrum flux error	_index Offset of this row in the source file for this table (see _file_max)	bp_n_relevant_bases Number of bases that are relevant for the representation of this mean BP spectrum	bp_relative_shrinking Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean BP spectrum	bp_n_measurements Number of measurements used for the BP spectrum generation	bp_n_rejected_measurements Number of rejected measurements in the BP spectrum generation	bp_standard_deviation 'electron'.s-1.pixel-1 Standard deviation for the BP spectrum representation	bp_chi_squared Chi squared for the BP spectrum representation	bp_n_transits Number of transits contributing to the mean in BP	bp_n_contaminated_transits Number of contaminated transits in BP	bp_n_blended_transits Number of blended transits in BP	rp_n_relevant_bases Number of bases that are relevant for the representation of this mean RP spectrum	rp_relative_shrinking Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean RP spectrum	rp_n_measurements Number of measurements used for the RP spectrum generation	rp_n_rejected_measurements Number of rejected measurements in the RP spectrum generation	rp_standard_deviation 'electron'.s-1.pixel-1 Standard deviation for the RP spectrum representation	rp_chi_squared Chi squared for the RP spectrum representation	rp_n_transits Number of transits contributing to the mean in RP	rp_n_contaminated_transits Number of contaminated transits in RP	rp_n_blended_transits Number of blended transits in RP
				ra deg Right ascension	ra_error mas Standard error of right ascension	dec deg Declination	dec_error mas Standard error of declination	l deg Galactic longitude	b deg Galactic latitude	ecl_lon deg Ecliptic longitude	ecl_lat deg Ecliptic latitude				pm mas.yr**-1 Total proper motion	pmra mas.yr**-1 Proper motion in right ascension direction		pmdec mas.yr**-1 Proper motion in declination direction																	astrometric_chi2_al AL chi-square value	astrometric_excess_noise mas Excess noise of the source	astrometric_excess_noise_sig Significance of excess noise		astrometric_primary_flag Primary or secondary																			ruwe Renormalised unit weight error											phot_g_mean_flux 'electron'.s**-1 G-band mean flux			phot_g_mean_mag mag G-band mean magnitude		phot_bp_mean_flux 'electron'.s**-1 Integrated BP mean flux			phot_bp_mean_mag mag Integrated BP mean magnitude		phot_bp_n_blended_transits Number of BP blended transits		phot_rp_mean_flux 'electron'.s**-1 Integrated RP mean flux			phot_rp_mean_mag mag Integrated RP mean magnitude	phot_bp_rp_excess_factor BP/RP excess factor		phot_rp_n_blended_transits Number of RP blended transits					radial_velocity km.s**-1 Radial velocity	radial_velocity_error km.s**-1 Radial velocity error	rv_method_used Method used to obtain the radial velocity																																	classprob_dsc_combmod_quasar Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)	classprob_dsc_combmod_galaxy Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)	classprob_dsc_combmod_star 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 Probability from DSC-Combmod of being a white dwarf (data used: BP/RP spectrum, photometry, astrometry)	classprob_dsc_combmod_binarystar Probability from DSC-Combmod of being a binary star (data used: BP/RP spectrum, photometry, astrometry)	classprob_dsc_specmod_quasar Probability from DSC-Specmod of being a quasar (data used: BP/RP spectrum)	classprob_dsc_specmod_galaxy Probability from DSC-Specmod of being a galaxy (data used: BP/RP spectrum)	classprob_dsc_specmod_star Probability from DSC-Specmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum)	classprob_dsc_specmod_whitedwarf Probability from DSC-Specmod of being a white dwarf (data used: BP/RP spectrum)	classprob_dsc_specmod_binarystar Probability from DSC-Specmod of being a binary star (data used: BP/RP spectrum)	classprob_dsc_allosmod_quasar Probability from DSC-Allosmod of being a quasar (data used: photometry, astrometry)	classprob_dsc_allosmod_galaxy Probability from DSC-Allosmod of being a galaxy (data used: photometry, astrometry)	classprob_dsc_allosmod_star Probability from DSC-Allosmod of being a star (data used: photometry, astrometry)	teff_gspphot K Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra	teff_gspphot_lower K Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra	teff_gspphot_upper K Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra	teff_gspspec K Effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	teff_gspspec_lower K 16th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	teff_gspspec_upper K 84th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	logg_gspphot log(cm.s**-2) Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra	logg_gspphot_lower log(cm.s**-2) Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra	logg_gspphot_upper log(cm.s**-2) Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra	logg_gspspec log(cm.s**-2) Logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	logg_gspspec_lower 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 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_gspphot dex Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra	mh_gspphot_lower dex Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra	mh_gspphot_upper dex Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra	mh_gspspec 'dex' Global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	mh_gspspec_lower 'dex' 16th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	mh_gspspec_upper 'dex' 84th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	distance_gspphot pc Distance from GSP-Phot Aeneas best library using BP/RP spectra	distance_gspphot_lower pc Lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra	distance_gspphot_upper pc Upper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectra	azero_gspphot mag Monochromatic extinction \(A_0\) at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra	azero_gspphot_lower mag Lower confidence level (16%) of monochromatic extinction \(A_0\) at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra	azero_gspphot_upper mag Upper confidence level (84%) of monochromatic extinction \(A_0\) at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra	ag_gspphot mag Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra	ag_gspphot_lower mag Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra	ag_gspphot_upper mag Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra	abp_gspphot mag Extinction in \(G_{\rm BP}\) band from GSP-Phot Aeneas best library using BP/RP spectra	abp_gspphot_lower mag Lower confidence level (16%) of extinction in \(G_{\rm BP}\) band from GSP-Phot Aeneas best library using BP/RP spectra	abp_gspphot_upper mag Upper confidence level (84%) of extinction in \(G_{\rm BP}\) band from GSP-Phot Aeneas best library using BP/RP spectra	arp_gspphot mag Extinction in \(G_{\rm RP}\) band from GSP-Phot Aeneas best library using BP/RP spectra	arp_gspphot_lower mag Lower confidence level (16%) of extinction in \(G_{\rm RP}\) band from GSP-Phot Aeneas best library using BP/RP spectra	arp_gspphot_upper mag Upper confidence level (84%) of extinction in \(G_{\rm RP}\) band from GSP-Phot Aeneas best library using BP/RP spectra	ebpminrp_gspphot mag Reddening \(E(G_{\rm BP} - G_{\rm RP})\) from GSP-Phot Aeneas best library using BP/RP spectra	ebpminrp_gspphot_lower mag Lower confidence level (16%) of reddening \(E(G_{\rm BP} - G_{\rm RP})\) from GSP-Phot Aeneas best library using BP/RP spectra	ebpminrp_gspphot_upper mag Upper confidence level (84%) of reddening \(E(G_{\rm BP} - G_{\rm RP})\) from GSP-Phot Aeneas best library using BP/RP spectra	mg_gspphot mag Absolute magnitude \(M_{\rm G}\) from GSP-Phot Aeneas best library using BP/RP spectra	mg_gspphot_lower mag Lower confidence level (16%) of absolute magnitude \(M_{\rm G}\) from GSP-Phot Aeneas best library using BP/RP spectra	mg_gspphot_upper mag Upper confidence level (84%) of absolute magnitude \(M_{\rm G}\) from GSP-Phot Aeneas best library using BP/RP spectra	radius_gspphot solRad Radius from GSP-Phot Aeneas best library using BP/RP spectra	radius_gspphot_lower solRad Lower confidence level (16%) of radius from GSP-Phot Aeneas best library using BP/RP spectra	radius_gspphot_upper solRad Upper confidence level (84%) of radius from GSP-Phot Aeneas best library using BP/RP spectra	logposterior_gspphot Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC best library	mcmcaccept_gspphot MCMC acceptance rate of GSP-Phot Aeneas MCMC best library	libname_gspphot Name of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this table	alphafe_gspspec '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 '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 '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 '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 '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 '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 dex Number of lines used for [Fe/M] abundance estimation	fem_gspspec_linescatter 'dex' Uncertainty estimation of [Fe/M] abundance using N lines of the element, given in femGspspecNlines	sife_gspspec '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 'dex' 16th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	sife_gspspec_upper 'dex' 84th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	sife_gspspec_nlines dex Number of lines used for [Si/Fe] abundance estimation	sife_gspspec_linescatter 'dex' Uncertainty estimation of [Si/Fe] abundance using N lines of the element, given in sifeGspspecNlines	cafe_gspspec '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 'dex' 16th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	cafe_gspspec_upper 'dex' 84th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	cafe_gspspec_nlines dex Number of lines used for [Ca/Fe] abundance estimation	cafe_gspspec_linescatter 'dex' Uncertainty estimation of [Ca/Fe] abundance using N lines of the element, given in cafeGspspecNlines	tife_gspspec '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 'dex' 16th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	tife_gspspec_upper 'dex' 84th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	tife_gspspec_nlines dex Number of lines used for [Ti/Fe] abundance estimation	tife_gspspec_linescatter 'dex' Uncertainty estimation of [Ti/Fe] abundance using N lines of the element, given in tifeGspspecNlines	mgfe_gspspec '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 'dex' 16th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	mgfe_gspspec_upper 'dex' 84th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	mgfe_gspspec_nlines dex Number of lines used for [Mg/Fe] abundance estimation	mgfe_gspspec_linescatter 'dex' Uncertainty estimation of [Mg/Fe] abundance using N lines of the element, given in mgfeGspspecNlines	ndfe_gspspec '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 'dex' 16th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	ndfe_gspspec_upper 'dex' 84th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	ndfe_gspspec_nlines dex Number of lines used for [Nd/Fe] abundance estimation	ndfe_gspspec_linescatter 'dex' Uncertainty estimation of [Nd/Fe] abundance using N lines of the element, given in ndfeGspspecNlines	feiim_gspspec '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 '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 '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 dex Number of lines used for [FeII/M] abundance estimation	feiim_gspspec_linescatter 'dex' Uncertainty estimation of [FeII/M] abundance using N lines of the element, given in feiimGspspecNlines	sfe_gspspec '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 'dex' 16th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	sfe_gspspec_upper 'dex' 84th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	sfe_gspspec_nlines dex Number of lines used for [S/Fe] abundance estimation	sfe_gspspec_linescatter 'dex' Uncertainty estimation of [S/Fe] abundance using N lines of the element, given in sfeGspspecNlines	zrfe_gspspec '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 'dex' 16th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	zrfe_gspspec_upper 'dex' 84th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	zrfe_gspspec_nlines dex Number of lines used for [Zr/Fe] abundance estimation	zrfe_gspspec_linescatter 'dex' Uncertainty estimation of [Zr/Fe] abundance using N lines of the element, given in zrfeGspspecNlines	nfe_gspspec '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 'dex' 16th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	nfe_gspspec_upper 'dex' 84th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	nfe_gspspec_nlines dex Number of lines used for [N/Fe] abundance estimation	nfe_gspspec_linescatter 'dex' Uncertainty estimation of [N/Fe] abundance using N lines of the element, given in nfeGspspecNlines	crfe_gspspec '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 'dex' 16th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	crfe_gspspec_upper 'dex' 84th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	crfe_gspspec_nlines dex Number of lines used for [Cr/Fe] abundance estimation	crfe_gspspec_linescatter 'dex' Uncertainty estimation of [Cr/Fe] abundance using N lines of the element, given in crfeGspspecNlines	cefe_gspspec '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 'dex' 16th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	cefe_gspspec_upper 'dex' 84th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	cefe_gspspec_nlines dex Number of lines used for [Ce/Fe] abundance estimation	cefe_gspspec_linescatter 'dex' Uncertainty estimation of [Ce/Fe] abundance using N lines of the element, given in cefeGspspecNlines	nife_gspspec '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 'dex' 16th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	nife_gspspec_upper 'dex' 84th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations	nife_gspspec_nlines dex Number of lines used for [Ni/Fe] abundance estimation	nife_gspspec_linescatter 'dex' Uncertainty estimation of [Ni/Fe] abundance using N lines of the element, given in nifeGspspecNlines	cn0ew_gspspec nm Equivalent witdh of cyanogen absorption line, derived from RVS spectra	cn0ew_gspspec_uncertainty nm Uncertainty of equivalent witdh of cyanogen absorption line, derived from RVS spectra	cn0_gspspec_centralline nm Central wavelength of cyanogen line, derived from RVS spectra using DIB algorithm	cn0_gspspec_width nm Width of cyoanogen line, derived from RVS spectra using DIB algorithm	dib_gspspec_lambda nm DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra	dib_gspspec_lambda_uncertainty nm Uncertainty on DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra	dibew_gspspec angstrom Equivalent width of the DIB from GSP-Spec MatisseGauguin using RVS spectra	dibew_gspspec_uncertainty angstrom Global uncertainty on DIB equivalent width value using DIB algorithm	dibewnoise_gspspec_uncertainty angstrom Uncertainty on DIB equivalent width value occuring from noise part	dibp0_gspspec Depth (\(p_0\) parameter) of the DIB derived from a Gaussian model fit	dibp2_gspspec angstrom Width (\(p_2\) parameter) of the DIB derived from a Gaussian model fit	dibp2_gspspec_uncertainty angstrom Uncertainty on the dibp2Gspspec parameter	dibqf_gspspec Quality flag of the DIB computation	logchisq_gspspec Logarithm of the goodness-of-fit for the GSP-Spec MatisseGauguin parameters	ew_espels_halpha nm Halpha pseudo-equivalent width from ESP-ELS	ew_espels_halpha_uncertainty nm Uncertainty of the Halpha pseudo-equivalent width from ESP-ELS	ew_espels_halpha_flag Quality flag of the Halpha pseudo-equivalent width from ESP-ELS	ew_espels_halpha_model nm Halpha pseudo-equivalent width from ESP-ELS measured on the synthetic spectrum	classlabel_espels Adopted ELS class label from ESP-ELS	classlabel_espels_flag Quality flag of the adopted ELS class label from ESP-ELS	classprob_espels_wcstar Probability from ESP-ELS of being a Wolf-Rayet star of type WC	classprob_espels_wnstar Probability from ESP-ELS of being a Wolf-Rayet star of type WN	classprob_espels_bestar Probability from ESP-ELS of being a Be Star	classprob_espels_ttauristar Probability from ESP-ELS of being a T Tauri Star	classprob_espels_herbigstar Probability from ESP-ELS of being a Herbig Ae/Be Star	classprob_espels_dmestar Probability from ESP-ELS of being an active M dwarf Star	classprob_espels_pne Probability from ESP-ELS of being a planetary nebula	azero_esphs mag Monochromatic interstellar extinction, A\(_\mathrm{0}\), from ESP-HS	azero_esphs_uncertainty mag Uncertainty at a 68% confidence level on A\(_\mathrm{0}\) from ESP-HS	ag_esphs mag Intersterstellar extinction in G band from ESP-HS	ag_esphs_uncertainty mag Uncertainty on \(A_{\rm G}\) from ESP-HS	ebpminrp_esphs mag Reddening \(E(G_{\rm BP} - G_{\rm RP})\) from ESP-HS	ebpminrp_esphs_uncertainty mag Uncertainty on \(E(G_{\rm BP} - G_{\rm RP})\) from ESP-HS	teff_esphs K Effective temperature from ESP-HS	teff_esphs_uncertainty K Uncertainty at a 68% confidence level on the effective temperature from ESP-HS	logg_esphs log(cm.s**-2) Surface gravity from ESP-HS	logg_esphs_uncertainty log(cm.s**-2) Uncertainty at a 68% confidence level on the surface gravity from ESP-HS	vsini_esphs km.s**-1 Projected rotational velocity from ESP-HS	vsini_esphs_uncertainty km.s**-1 Uncertainty on the projected rotational velocity from ESP-HS	spectraltype_esphs Spectral type from ESP-ELS	activityindex_espcs nm Chromospheric activity index from ESP-CS, measured on the calcium triplet using RVS spectra	activityindex_espcs_uncertainty nm Uncertainty in the chromospheric activity index from ESP-CS	activityindex_espcs_input Source of input stellar parameters for the computation of the activity index by ESP-CS	teff_espucd K Effective temperature estimate from ESP-UCD based on the RP spectrum	teff_espucd_uncertainty K Uncertainty of the effective temperature estimate produced by ESP-UCD	flags_espucd Quality flags of the ESP-UCD parameter estimates	radius_flame solRad Radius of the star from FLAME using teffGspphot and lumFlame	radius_flame_lower solRad Lower confidence level (16%) of radiusFlame	radius_flame_upper solRad Upper confidence level (84%) of radiusFlame	lum_flame solLum Luminosity of the star from FLAME using G band magnitude, extinction (agGspphot), parallax or distance, and a bolometric correction bcFlame	lum_flame_lower solLum Lower confidence level (16%) of lumFlame	lum_flame_upper solLum Upper confidence level (84%) of lumFlame	mass_flame solMass Mass of the star from FLAME using stellar models, lumFlame, and teffGspphot	mass_flame_lower solMass Lower confidence level (16%) of massFlame	mass_flame_upper solMass Upper confidence level (84%) of massFlame	age_flame Gyr Age of the star from FLAME using stellar models, see massFlame for details	age_flame_lower Gyr Lower confidence level (16%) of ageFlame	age_flame_upper Gyr Upper confidence level (84%) of ageFlame	flags_flame Flags indicating quality and processing information from FLAME	evolstage_flame Evolutionary stage of the star from FLAME using stellar models, see massFlame for details	gravredshift_flame km.s**-1 Gravitational redshift from FLAME using radiusFlame and loggGspphot	gravredshift_flame_lower km.s**-1 Lower confidence level (16%) of gravredshiftFlame	gravredshift_flame_upper km.s**-1 Upper confidence level (84%) of gravredshiftFlame	bc_flame mag Bolometric correction used to derive lumFlame	mh_msc 'dex' Metallicity of the source treated as a binary system from MSC using BP/RP spectra and parallax	mh_msc_upper 'dex' Upper confidence level (84%) of the metallicity from MSC using BP/RP spectra and parallax	mh_msc_lower 'dex' Lower confidence level (16%) of the metallicity from MSC using BP/RP spectra and parallax	azero_msc mag Monochromatic extinction \(A_0\) at 547.7nm of the source treated as a binary system from MSC using BP/RP spectra and parallax	azero_msc_upper mag Upper confidence level (84%) of monochromatic extinction \(A_0\) at 547.7nm from MSC using BP/RP spectra and parallax	azero_msc_lower mag Lower confidence level (16%) of monochromatic extinction \(A_0\) at 547.7nm from MSC using BP/RP spectra and parallax	distance_msc pc Distance from MSC using BP/RP spectra and parallax	distance_msc_upper pc Upper confidence level (84%) of distance from MSC using BP/RP spectra and parallax	distance_msc_lower pc Lower confidence level (16%) of distance from MSC using BP/RP spectra and parallax	teff_msc1 K Effective temperature of the primary from MSC using BP/RP spectra and parallax	teff_msc1_upper K Upper confidence level (84%) of effective temperature of the primary from MSC using BP/RP spectra and parallax	teff_msc1_lower K Lower confidence level (16%) of effective temperature of the primary from MSC using BP/RP spectra and parallax	teff_msc2 K Effective temperature of the secondary from MSC using BP/RP spectra and parallax	teff_msc2_upper K Upper confidence level (84%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax	teff_msc2_lower K Lower confidence level (16%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax	logg_msc1 log(cm.s**-2) Surface gravity of the primary from MSC using BP/RP spectra and parallax	logg_msc1_upper 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 log(cm.s**-2) Lower confidence level (16%) of surface gravity of the primary from MSC using BP/RP spectra and parallax	logg_msc2 log(cm.s**-2) Surface gravity of the secondary from MSC using BP/RP spectra and parallax	logg_msc2_upper 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 log(cm.s**-2) Lower confidence level (16%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax	ag_msc mag Extinction in G band of the source treated as a binary system from MSC using BP/RP spectra and parallax	ag_msc_upper mag Upper confidence level (84%) of extinction in G band from MSC using BP/RP spectra and parallax	ag_msc_lower mag Lower confidence level (16%) of extinction in G band from MSC using BP/RP spectra and parallax	logposterior_msc Goodness-of-fit score (normalised log-posterior) of MSC MCMC	mcmcaccept_msc Mean MCMC acceptance rate of MSC MCMC	mcmcdrift_msc Mean drift of the MSC MCMC chain in units of parameter standard deviation	flags_msc Flag indicating quality information from MSC	neuron_oa_id Identifier of the OA SOM map neuron that represents the source	neuron_oa_dist Distance between the source XP spectra and the OA neuron XP prototype that represents the source	neuron_oa_dist_percentile_rank Percentile rank according to the distance distribution of the OA neuron that represents the source	flags_oa Flags indicating quality and processing information from OA				_index Offset of this row in the source file for this table	nss_solution_type NSS model adopted	accel_ra mas.yr**-2 Acceleration in RA		accel_dec mas.yr**-2 Acceleration in DEC										obj_func Value of the objective function at the solution	goodness_of_fit Goodness of fit in the Hipparcos sense		flags Quality flag for the achieved NSS solution	_index Offset of this row in the source file for this table	nss_solution_type NSS model adopted	mean_velocity km.s**-1 Mean velocity										obj_func Value of the objective function at the solution	goodness_of_fit Goodness of fit in the Hipparcos sense	flags Quality flag for the achieved NSS solution		_index Offset of this row in the source file for this table	nss_solution_type NSS model adopted	ref_flux_g 'electron'.s**-1 Reference flux in the G band	vim_d_ra mas VIM coordinate in RA	vim_d_ra_error mas Standard error of VIM coordinate in RA	vim_d_dec mas VIM coordinate in DEC	vim_d_dec_error mas Standard error of VIM coordinate in DEC					obj_func Value of the objective function at the solution	goodness_of_fit Goodness of fit in the Hipparcos sense	efficiency Efficiency of the solution		flags Quality flag for the achieved NSS solution					vari_best_class_score Score of the best class				qso_variability Quasar variability metric in the G band								redshift_qsoc Redshift from QSOC				zscore_qsoc Redshift zscore from QSOC									sersic_index Fitted sersic Index	sersic_index_error Error on the fitted sersic Index						l2_norm L2 norm for the fitted Sersic profile					ra deg Right Ascension	dec deg Declination	flux array of fluxes	flux_error array of uncertainties in flux	combined_transits number of combined transits	combined_ccds number of combined CCD spectra	deblended_ccds number of deblended CCD spectra																																							ra deg Right Ascension	dec deg Declination	flux W.m-2.nm-1 mean BP + RP combined spectrum flux											bp_n_blended_transits Number of blended transits in BP									rp_n_blended_transits Number of blended transits in RP

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