Table A.1.
Description of the columns used in the catalogues we release in this work.
Column Identifier | Description | Units |
---|---|---|
KIC/K2_ID/TIC | Kepler/K2/TESS ID | None |
K2_campaign | K2 campaign number | None |
GEDR3_source_id | Gaia EDR3 source ID | None |
GEDR3_ra | Gaia EDR3 right ascension | deg |
GEDR3_dec | Gaia EDR3 declination | deg |
GEDR3_l | Gaia EDR3 galactic longitude | deg |
GEDR3_b | Gaia EDR3 galactic latitude | deg |
GEDR3_ecl_lon | Gaia EDR3 ecliptic longitude | deg |
GEDR3_ecl_lat | Gaia EDR3 ecliptic latitude | deg |
GEDR3_parallax | Gaia EDR3 parallax | mas |
GEDR3_parallax_Z5 | L21 correction (5p) | mas |
GEDR3_phot_g_mean_mag | Gaia EDR3 G-band magnitude | mag |
GEDR3_phot_bp_mean_mag | Gaia EDR3 GBP-band magnitude | mag |
GEDR3_phot_rp_mean_mag | Gaia EDR3 GRP-band magnitude | mag |
GEDR3_nu_eff_used_in_astrometry | Gaia EDR3 effective wavenumber | μm−1 |
GEDR3_pseudocolour | Gaia EDR3 pseudocolour | μm−1 |
GEDR3_astrometric_params_solved | Gaia EDR3 number of astrometric parameters solved | None |
GEDR3_ruwe | Gaia EDR3 renormalised unit weight error | None |
GEDR3_ipd_frac_multi_peak | Gaia EDR3 percent of successful-IPD windows with more than one peak | None |
GEDR3_ipd_gof_harmonic_amplitude | Gaia EDR3 amplitude of the IPD GoF versus position angle of scan | None |
GEDR3_ipd_frac_odd_win | Gaia EDR3 percent of transits with truncated windows or multiple gates | None |
GEDR3_phot_bp_n_blended_transits | Gaia EDR3 number of BP blended transits | None |
GEDR3_phot_rp_n_blended_transits | Gaia EDR3 number of RP blended transits | None |
GEDR3_phot_bp_n_obs | Gaia EDR3 number of observations contributing to BP photometry | None |
GEDR3_phot_rp_n_obs | Gaia EDR3 number of observations contributing to RP photometry | None |
GEDR3_blending_fraction | Gaia EDR3 blending fraction | None |
GEDR3_phot_bp_rp_excess_factor | Gaia EDR3 BP/RP excess factor | None |
GEDR3_phot_bp_rp_excess_factor_corrected | Gaia EDR3 corrected BP/RP excess factor | None |
GEDR3_phot_bp_rp_excess_factor_corrected_scatter | Gaia EDR3 1σ scatter for the corrected BP/RP excess factor | None |
GDR3_non_single_star | Gaia DR3 flag indicating the availability in Non-Single Star tables | None |
GDR3_distance_gspphot | Gaia DR3 distance from GSP-Phot | pc |
GDR3_ag_gspphot | Gaia DR3 extinction in G-band from GSP-Phot | mag |
2MASS_kmag | 2MASS KS-band magnitude | mag |
APOGEE_ID | APOGEE ID | None |
APOGEE_teff | APOGEE Teff | K |
APOGEE_feh | APOGEE [Fe/H] | None |
APOGEE_alpha | APOGEE [α/Fe] | None |
APOGEE_mh | APOGEE [M/H] | None |
APOGEE_ASPCAPFLAGS | APOGEE flag for issues associated with the ASPCAP fits | None |
GALAH_teff | GALAH Teff | K |
GALAH_feh | GALAH [Fe/H] | None |
GALAH_alpha | GALAH [α/Fe] | None |
GALAH_mh | GALAH [M/H] | None |
GALAH_flag_sp | GALAH stellar parameter quality flag | None |
GALAH_flag_fe_h | GALAH [Fe/H] quality flag | None |
GALAH_flag_alpha_fe | GALAH [α/Fe] quality flag | None |
MA09_numax | νmax from MA09 pipeline | μHz |
MA09_Dnu | Δν from MA09 pipeline | μHz |
MA09_PARAM_mass | Mass from PARAM, based on MA09 and APOGEE/GALAH | M⊙ |
MA09_PARAM_rad | Radius from PARAM, based on MA09 and APOGEE/GALAH | R⊙ |
MA09_PARAM_mbol | Bolometric magnitude from PARAM, based on MA09 and APOGEE/GALAH | mag |
MA09_PARAM_dist | Distance from PARAM, based on MA09 and APOGEE/GALAH | pc |
MA09_PARAM_Av | Visual extinction from PARAM, based on MA09 and APOGEE/GALAH | mag |
MA09_PARAM_Ks | KS absolute magnitude from PARAM, based on MA09 and APOGEE/GALAH | mag |
MA09_PARAM_parallax | Parallax from PARAM, based on MA09 and APOGEE/GALAH | mas |
E20_numax | νmax from E20 pipeline | μHz |
E20_Dnu | Δν from E20 pipeline | μHz |
E20_PARAM_mass | Mass from PARAM, based on E20 and APOGEE/GALAH | M⊙ |
E20_PARAM_rad | Radius from PARAM, based on E20 and APOGEE/GALAH | R⊙ |
E20_PARAM_mbol | Bolometric magnitude from PARAM, based on E20 and APOGEE/GALAH | mag |
E20_PARAM_dist | Distance from PARAM, based on E20 and APOGEE/GALAH | pc |
E20_PARAM_Av | Visual extinction from PARAM, based on E20 and APOGEE/GALAH | mag |
E20_PARAM_Ks | KS absolute magnitude from PARAM, based on E20 and APOGEE/GALAH | mag |
E20_PARAM_parallax | Parallax from PARAM, based on E20 and APOGEE/GALAH | mas |
E17_evstate | Elsworth et al. (2017) evolutionary state | None |
Notes. There are four datasets in total: Kepler+ APOGEE, K2+ APOGEE, K2+ GALAH, and TESS+ APOGEE. In these tables we compile asteroseismic information from MA09 and E20, spectroscopic constraints from APOGEE DR17 (Abdurro’uf et al. 2022) or GALAH DR3 (Buder et al. 2021), and astrometric properties from Gaia (E)DR3 (Gaia Collaboration 2021, 2023). Where relevant, uncertainties defined either as the standard deviation (‘err’) or as the 16th or 84th percentiles (68L, 68U) are provided. For APOGEE we adopt conservative uncertainty values of 50 K and 0.05 dex for Teff and [M/H], but keep the original values if they are larger. For GALAH, if [α/Fe] is not available, then the value and uncertainty on [M/H] are simply equal to those of [Fe/H]. GEDR3_blending_fraction, GEDR3_phot_bp_rp_excess_factor_corrected, GEDR3_phot_bp_rp_excess_factor_corrected_scatter are computed following Sect. 9.3 in Riello et al. (2021).
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