Plot type:
Histogram bins the data by a single field and displays count of objects per bin.
Heatmap bins the data by two fields and displays count as color.
Conditional distribution bins the data by one field and displays the distribution of a second field within that bin as a boxplot (range and quartiles).
Shows a scatterplot of a (random subset) of actual data points.

For log functionality, set the filter to enable only positive values.

For log functionality, set the filter to enable only positive values.

For log functionality, set the filter to enable only positive values.

Count:
Choose whether the object count per bin is shown in linear or log scale.
Count is shown on the Y axis.
Count is shown on the color (Z) axis.

Use "*" as wildcard

Examples:{{ bucket.key }}

Range:

{{filter.render(filter.aggs.min)}}

{{filter.render(filter.aggs.max)}}

Select field to filter

Example python code to apply the above filters and retrieve data. To use, download and install this module.

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 |

Gaia Data Release 3 from the European Space Agency

Important links to official Gaia Data Release documentation:

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.

More under:

_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. | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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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 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||

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 |