J/A+A/669/A104      Stellar parameters from Gaia DR3         (Kordopatis+, 2023)

Stellar ages, masses, extinctions, and orbital parameters based on spectroscopic parameters of Gaia DR3. Kordopatis G., Schultheis M., McMillan P.J., Palicio P.A., de Laverny P., Recio-Blanco A., Creevey O., Alvarez M.A., Andrae R., Poggio E., Spitoni E., Contursi G., Zhao H., Oreshina-Slezak I., Ordenovic C., Bijaoui A. <Astron. Astrophys. 669, A104 (2023)> =2023A&A...669A.104K 2023A&A...669A.104K (SIMBAD/NED BibCode)
ADC_Keywords: Milky Way ; Stars, standard ; Radial velocities ; Positional data Keywords: Galaxy: kinematics and dynamics - Galaxy: stellar content - stars: fundamental parameters Abstract: Gaia's third data release provides radial velocities for 33 million stars and spectroscopically derived atmospheric parameters for more than 5 million targets. When combined with the astrometric data, these allow us to derive orbital and stellar parameters that are key to understanding the stellar populations of the Milky Way and to perform Galactic archaeology. We used the calibrated atmospheric parameters, 2MASS and Gaia-EDR3 photometry, and parallax-based distances to compute the ages, initial stellar masses, and reddenings for the stars with spectroscopic parameters. We also derived the orbits for all of the stars with measured radial velocities and astrometry, adopting two sets of line-of-sight distances from the literature. Four different sets of ages, masses, and absolute magnitudes in different photometric bands are obtained through an isochrone fitting method, considering different combinations of input parameters. The reddenings are obtained by comparing the observed colours with those obtained from the isochrone projection. Finally, the orbits are computed adopting an axisymmetric potential of the Galaxy. Comparisons with reference catalogues of field and cluster stars suggest that reliable ages are obtained for stars younger than 9-10Gyr when the estimated relative age uncertainty is <50 per cent. For older stars, ages tend to be underestimated. The most reliable stellar type for age determination are turn-off stars, even when the input atmospheric parameters have large uncertainties. Ages for giants and main-sequence stars are retrieved with uncertainties of the order of 2Gyr when extinction towards the star's line of sight is less than AV≲2.5mag. The catalogue of ages, initial stellar masses, reddenings, galactocentric positions and velocities, as well as the stellar orbital actions, eccentricities, apocentre, pericentre and maximum distance from the Galactic plane reached during their orbits, is made publicly available to be downloaded. With this catalogue, the full chemo-dynamical properties of the extended solar neighbourhood unfold and allow us to better identify the properties of the spiral arms, to parametrise the dynamical heating of the disc, and to thoroughly study the chemical enrichment of the Milky Way. Description: We build upon the Gaia public catalogues, and focus on the RVS sample of GDR3. This sample contains 33*106 stars with radial velocity measurements and 5*106 stars with spectroscopic parameters and abundances (Recio-Blanco et al., 2022, arXiv:2206.05541; Fouesneau et al., 2022, arXiv:2206.05992). We performed an improved projection on the isochrones that takes into account the necessary GSP-Spec calibrations of metallicity and surface gravities2, stellar distance (in a different way to FLAME, using the Bailer-Jones et al. (2021, Cat. I/352) values), infrared (2MASS, Skrutskie et al., 2006, Cat. VII/233), and EDR3 photometry. Furthermore, for the community's convenience, we also computed and provide the catalogue of the three-dimensional galactocentric positions, (cylindrical) velocities, and orbital parameters of all of the GDR3 RVS stars using an updated version of the axisymmetric Galactic potential of McMillan (2017MNRAS.465...76M 2017MNRAS.465...76M) and the Galpy code (Bovy, 2015ApJS..216...29B 2015ApJS..216...29B). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 1665 33652071 Catalog (table A1) -------------------------------------------------------------------------------- See also: I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021) I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- GaiaDR3 Gaia DR3 source ID (source_id) 21- 30 F10.6 kpc Xdgeo ?=- Median galactocentric Cartesian X position (Xmeddgeo) 32- 41 F10.6 kpc b_Xdgeo ?=- Lower confidence limit of Xdgeo (Xlodgeo) 43- 52 F10.6 kpc B_Xdgeo ?=- Upper confidence limit of Xdgeo (Xhidgeo) 54- 63 F10.6 kpc Ydgeo ?=- Median galactocentric Cartesian Y position (Ymeddgeo) 65- 74 F10.6 kpc b_Ydgeo ?=- Lower confidence limit of Ydgeo (Ylodgeo) 76- 85 F10.6 kpc B_Ydgeo ?=- Upper confidence limit of Ydgeo (Yhidgeo) 87- 96 F10.6 kpc Zdgeo ?=- Median galactocentric Cartesian Z position (Zmeddgeo) 98- 107 F10.6 kpc b_Zdgeo ?=- Lower confidence limit of Zdgeo (Zlodgeo) 109- 118 F10.6 kpc B_Zdgeo ?=- Upper confidence limit of Zdgeo (Zhidgeo) 120- 128 F9.6 kpc rdgeo ?=- Median heliocentric line-of-sight distance with geometric prior from Bailer-Jones et al. (2021, Cat. I/352) (rmeddgeo) 130- 138 F9.6 kpc b_rdgeo ?=- Lower confidence limit of rdgeo (rlodgeo) 140- 148 F9.6 kpc B_rdgeo ?=- Upper confidence limit of rdgeo (rhidgeo) 150- 158 F9.3 km/s VRdgeo ?=- Median galactocentric radial velocity obtained using rmeddgeo (VRmeddgeo) 160- 168 F9.3 km/s b_VRdgeo ?=- Lower confidence limit of VRdgeo (VRlodgeo) 170- 178 F9.3 km/s B_VRdgeo ?=- Upper confidence limit of VRdgeo (VRhidgeo) 180- 188 F9.3 km/s Vphidgeo ?=- Median galactocentric azimuthal velocity obtained using rmeddgeo (Vphimeddgeo) 190- 198 F9.3 km/s b_Vphidgeo ?=- Lower confidence limit of Vphidgeo (Vphilodgeo) 200- 208 F9.3 km/s B_Vphidgeo ?=- Upper confidence limit of Vphidgeo (Vphihidgeo) 210- 218 F9.3 km/s VZdgeo ?=- Median galactocentric vertical velocity obtained using rmeddgeo (VZmeddgeo) 220- 228 F9.3 km/s b_VZdgeo ?=- Lower confidence limit of VZdgeo (VZlodgeo) 230- 238 F9.3 km/s B_VZdgeo ?=- Upper confidence limit of VZdgeo (VZhidgeo) 240- 249 F10.8 --- edgeo ?=9.99999999 Median eccentricity, obtained using rmeddgeo (emeddgeo) 251- 260 F10.8 --- b_edgeo ?=9.99999999 Lower confidence limit of edgeo (elodgeo) 262- 271 F10.8 --- B_edgeo ?=9.99999999 Upper confidence limit of edgeo (ehidgeo) 273- 282 F10.6 kpc Zmaxdgeo ?=- Median maximum distance from the galactic plane obtained using rmeddgeo (Zmaxmeddgeo) 284- 293 F10.6 kpc b_Zmaxdgeo ?=- Lower confidence limit of Zmaxdgeo (Zmaxlodgeo) 295- 304 F10.6 kpc B_Zmaxdgeo ?=- Upper confidence limit of Zmaxdgeo (Zmaxhidgeo) 306- 314 F9.6 kpc rperidgeo ?=- Median perigalactic radius reached by the star, obtained using rmeddgeo (rperimeddgeo) 316- 324 F9.6 kpc b_rperidgeo ?=- Lower confidence limit of rperidgeo (rperilodgeo) 326- 334 F9.6 kpc B_rperidgeo ?=- Upper confidence limit of rperidgeo (rperihidgeo) 336- 345 F10.6 kpc rapodgeo ?=- Median apogalactic radius reached by the star, obtained using rmeddgeo (rapomeddgeo) 347- 356 F10.6 kpc b_rapodgeo ?=- Lower confidence limit of rapodgeo (rapolodgeo) 358- 366 F9.5 kpc B_rapodgeo ?=- Upper confidence limit of rapodgeo (rapohidgeo) 368- 379 E12.6 km.kpc/s Jrdgeo ?=- Median radial action obtained using rmeddgeo (Jrmeddgeo) 381- 392 E12.6 km.kpc/s b_Jrdgeo ?=- Lower confidence limit of Jrdgeo (Jrlodgeo) 394- 405 E12.6 km.kpc/s B_Jrdgeo ?=- Upper confidence limit of Jrdgeo (Jrhidgeo) 407- 414 F8.2 km.kpc/s Lzdgeo ?=- Median angular momentum in z-direction obtained using rmeddgeo (Lzmeddgeo) 416- 424 F9.2 km.kpc/s b_Lzdgeo ?=- Lower confidence limit of Lzdgeo (-9999.99 for infinity) (Lzlodgeo) 426- 433 F8.2 km.kpc/s B_Lzdgeo ?=- Upper confidence limit of Lzdgeo (Lzhidgeo) 435- 446 E12.6 km.kpc/s Jzdgeo ?=- Median radial action obtained using rmeddgeo (Jzmeddgeo) 448- 459 E12.6 km.kpc/s b_Jzdgeo ?=- Lower confidence limit of Jzdgeo (Jzlodgeo) 461- 472 E12.6 km.kpc/s B_Jzdgeo ?=- Upper confidence limit of Jzdgeo (Jzhidgeo) 474- 483 F10.6 kpc Xdpgeo ?=- Median galactocentric Cartesian X position (Xmeddphotogeo) 485- 494 F10.6 kpc b_Xdpgeo ?=- Lower confidence limit of Xdpgeo (Xlodphotogeo) 496- 505 F10.6 kpc B_Xdpgeo ?=- Upper confidence limit of Xdpgeo (Xhidphotogeo) 507- 516 F10.6 kpc Ydpgeo ?=- Median galactocentric Cartesian Y position (Ymeddphotogeo) 518- 527 F10.6 kpc b_Ydpgeo ?=- Lower confidence limit of Ydpgeo (Ylodphotogeo) 529- 538 F10.6 kpc B_Ydpgeo ?=- Upper confidence limit of Ydpgeo (Yhidphotogeo) 540- 549 F10.6 kpc Zdpgeo ?=- Median galactocentric Cartesian Z position (Zmeddphotogeo) 551- 560 F10.6 kpc b_Zdpgeo ?=- Lower confidence limit of Zdpgeo (Zlodphotogeo) 562- 571 F10.6 kpc B_Zdpgeo ?=- Upper confidence limit of Zdpgeo (Zhidphotogeo) 573- 581 F9.6 kpc rdpgeo ?=- Median heliocentric line-of-sight distance with photogeometric prior from Bailer-Jones et al. (2021, Cat. I/352) (rmeddphotogeo) 583- 591 F9.6 kpc b_rdpgeo ?=- Lower confidence limit of Rdpgeo (rlodphotogeo) 593- 601 F9.6 kpc B_rdpgeo ?=- Upper confidence limit of Rdpgeo (rhidphotogeo) 603- 612 F10.4 km/s VRdpgeo ?=- Median galactocentric radial velocity obtained using rmeddpgeo (VRmeddphotogeo) 614- 623 F10.4 km/s b_VRdpgeo ?=- Lower confidence limit of VRdpgeo (VRlodphotogeo) 625- 634 F10.4 km/s B_VRdpgeo ?=- Upper confidence limit of VRdpgeo (VRhidphotogeo) 636- 645 F10.4 km/s Vphidpgeo ?=- Median galactocentric azimuthal velocity obtained using rmeddpgeo (Vphimeddphotogeo) 647- 656 F10.4 km/s b_Vphidpgeo ?=- Lower confidence limit of Vphidpgeo (Vphilodphotogeo) 658- 667 F10.4 km/s B_Vphidpgeo ?=- Upper confidence limit of Vphidpgeo (Vphihidphotogeo) 669- 678 F10.4 km/s VZdpgeo ?=- Median galactocentric azimuthal velocity obtained using rmeddpgeo (VZmeddphotogeo) 680- 689 F10.4 km/s b_VZdpgeo ?=- Lower confidence limit of VZdpgeo (VZlodphotogeo) 691- 700 F10.4 km/s B_VZdpgeo ?=- Upper confidence limit of VZdpgeo (VZhidphotogeo) 702- 711 F10.8 --- edpgeo ?=9.99999999 Median eccentricity, obtained using rmeddpgeo (emeddphotogeo) 713- 722 F10.8 --- b_edpgeo ?=9.99999999 Lower confidence limit of edpgeo (elodphotogeo) 724- 733 F10.8 --- B_edpgeo ?=9.99999999 Upper confidence limit of edpgeo (ehidphotogeo) 735- 744 F10.6 kpc Zmaxdpgeo ?=- Median maximum distance from the galactic plane obtained using rmeddpgeo (Zmaxmeddphotogeo) 746- 755 F10.6 kpc b_Zmaxdpgeo ?=- Lower confidence limit of Zmaxdpgeo (Zmaxlodphotogeo) 757- 766 F10.6 kpc B_Zmaxdpgeo ?=- Upper confidence limit of Zmaxdpgeo (Zmaxhidphotogeo) 768- 776 F9.6 kpc rperidpgeo ?=- Median perigalactic radius reached by the star, obtained using rmeddpgeo (rperimeddphotogeo) 778- 786 F9.6 kpc b_rperidpgeo ?=- Lower confidence limit of rperidpgeo (rperilodphotogeo) 788- 796 F9.6 kpc B_rperidpgeo ?=- Upper confidence limit of rperidpgeo (rperihidphotogeo) 798- 807 F10.6 kpc rapodpgeo ?=- Median apogalactic radius reached by the star, obtained using rmeddpgeo (rapomeddphotogeo) 809- 818 F10.6 kpc b_rapodpgeo ?=- Lower confidence limit of rapodpgeo (rapolodphotogeo) 820- 829 F10.6 kpc B_rapodpgeo ?=- Upper confidence limit of rapodpgeo (rapohidphotogeo) 831- 842 E12.6 km.kpc/s Jrdpgeo ?=- Median radial action obtained using rmeddpgeo (Jrmeddphotogeo) 844- 855 E12.6 km.kpc/s b_Jrdpgeo ?=- Lower confidence limit of Jrdpgeo (Jrlodphotogeo) 857- 868 E12.6 km.kpc/s B_Jrdpgeo ?=- Upper confidence limit of Jrdpgeo (Jrhidphotogeo) 870- 877 F8.2 km.kpc/s Lzdpgeo ?=- Median angular momentum in z-direction obtained using rmeddpgeo (Lzmeddphotogeo) 879- 886 F8.2 km.kpc/s b_Lzdpgeo ?=- Lower confidence limit of Lzdpgeo (Lzlodphotogeo) 888- 895 F8.2 km.kpc/s B_Lzdpgeo ?=- Upper confidence limit of Lzdpgeo (Lzhidphotogeo) 897- 908 E12.6 km.kpc/s Jzdpgeo ?=- Median vertical action obtained using rmeddpgeo (Jzmeddphotogeo) 910- 921 E12.6 km.kpc/s b_Jzdpgeo ?=- Lower confidence limit of Jzdpgeo (Jzlodphotogeo) 923- 934 E12.6 km.kpc/s B_Jzdpgeo ?=- Upper confidence limit of Jzdpgeo (Jzhidphotogeo) 936- 942 F7.2 K Teffspec ?=- Projected Teff adopting the calibrated GSP-Spec parameters only (Teff_spec) 944- 952 F9.6 --- loggspec ?=- Projected logg adopting the calibrated GSP-Spec parameters only (logg_spec) 954- 962 F9.6 --- metaspec ?=- Projected [M/H] adopting the calibrated GSP-Spec parameters only (meta_spec) 964- 972 F9.6 Gyr agespec ?=- Inferred age adopting the calibrated GSP-Spec parameters only (age_spec) 974- 981 F8.6 Gyr e_agespec ?=- rms uncertainty on agespec (ageerrorspec) 983- 990 F8.6 Msun Minispec ?=- Inferred initial stellar mass adopting the calibrated GSP-Spec parameters only (Minispec) 992- 999 F8.6 Msun e_Minispec ?=- rms uncertainty on (Minierror_spec) 1001-1010 F10.6 mag GMAGspec ?=- Inferred absolute G magnitude adopting the calibrated GSP-Spec parameters only (G_spec) 1012-1021 F10.6 mag BPMAGspec ?=- Inferred absolute BP magnitude adopting the calibrated GSP-Spec parameters only (GBPspec) 1023-1032 F10.6 mag RPMAGspec ?=- Inferred absolute RP magnitude adopting the calibrated GSP-Spec parameters only (GRPspec) 1034-1042 F9.6 mag e_GMAGspec ?=- rms uncertainty on GMAGspec (Gerrorspec) 1044-1052 F9.6 mag e_BPMAGspec ?=- rms uncertainty on BPMAGspec (GBPerror_spec) 1054-1062 F9.6 mag e_RPMAGspec ?=- rms uncertainty on RPMAGspec (GRPerror_spec) 1064-1071 F8.2 K Teffspecjhk ?=- Projected Teff adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (Teff_specjhk) 1073-1081 F9.6 --- loggspecjhk ?=- Projected logg adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (logg_specjhk) 1083-1091 F9.6 --- metaspecjhk ?=- Projected [M/H] adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (meta_specjhk) 1093-1101 F9.6 Gyr agespecjhk ?=- Inferred age adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (age_specjhk) 1103-1110 F8.6 Gyr e_agespecjhk ?=- rms uncertainty on adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (ageerrorspecjhk) 1112-1119 F8.6 Msun Minispecjhk ?=- Inferred initial stellar mass adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (Minispecjhk) 1121-1128 F8.6 Msun e_Minispecjhk ?=- rms uncertainty on Minispecjhk (Minierror_specjhk) 1130-1139 F10.6 mag GMAGspecjhk ?=- Inferred absolute G magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (G_specjhk) 1141-1150 F10.6 mag BPMAGspecjhk ?=- Inferred absolute BP magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (GBPspecjhk) 1152-1161 F10.6 mag RPMAGspecjhk ?=- Inferred absolute RP magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (GRPspecjhk) 1163-1170 F8.6 mag e_GMAGspecjhk ?=- rms uncertainty on GMAGspecjhk (Gerrorspecjhk) 1172-1179 F8.6 mag e_BPMAGspecjhk ?=- rms uncertainty on BPMAGspecjhk (GBPerror_specjhk) 1181-1188 F8.6 mag e_RPMAGspecjhk ?=- rms uncertainty on RPMAGspecjhk (GRPerror_specjhk) 1190-1197 F8.2 K Teffspecjhkg ?=- Projected Teff adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (Teff_specjhkg) 1199-1207 F9.6 --- loggspecjhkg ?=- Projected logg adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (logg_specjhkg) 1209-1217 F9.6 --- metaspecjhkg ?=- Projected [M/H] adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (meta_specjhkg) 1219-1227 F9.6 Gyr agespecjhkg ?=- Inferred age adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (age_specjhkg) 1229-1236 F8.6 Gyr e_agespecjhkg ?=- rms uncertainty on agespecjhkg (ageerrorspecjhkg) 1238-1245 F8.6 Msun Minispecjhkg ?=- Inferred initial stellar mass adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (Minispecjhkg) 1247-1254 F8.6 Msun e_Minispecjhkg ?=- rms uncertainty on Minispecjhkg (Minierror_specjhkg) 1256-1265 F10.6 mag GMAGspecjhkg ?=- Inferred absolute G magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (G_specjhkg) 1267-1276 F10.6 mag BPMAGspecjhkg ?=- Inferred absolute BP magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (GBPspecjhkg) 1278-1287 F10.6 mag RPMAGspecjhkg ?=- Inferred absolute RP magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (GRPspecjhkg) 1289-1296 F8.6 mag e_GMAGspecjhkg ?=- rms uncertainty on GMAGspecjhkg (Gerrorspecjhkg) 1298-1305 F8.6 mag e_BPMAGspecjhkg ?=- rms uncertainty on BPMAGspecjhkg (GBPerror_specjhkg) 1307-1314 F8.6 mag e_RPMAGspecjhkg ?=- rms uncertainty on RPMAGspecjhkg (GRPerror_specjhkg) 1316-1323 F8.2 K Teffspeck ?=- Projected Teff adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (Teff_speck) 1325-1333 F9.6 --- loggspeck ?=- Projected logg adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (logg_speck) 1335-1343 F9.6 --- metaspeck ?=- Projected [M/H] adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (meta_speck) 1345-1353 F9.6 Gyr agespeck ?=- Inferred age adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (age_speck) 1355-1362 F8.6 Gyr e_agespeck ?=- rms uncertainty on agespeck (ageerrorspeck) 1364-1371 F8.6 Msun Minispeck ?=- Inferred initial stellar mass adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (Minispeck) 1373-1380 F8.6 Msun e_Minispeck ?=- rms uncertainty on Minispeck (Minierror_speck) 1382-1391 F10.6 mag GMAGspeck ?=- Inferred absolute G magnitude adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (G_speck) 1393-1402 F10.6 mag BPMAGspeck ?=- Inferred absolute BP magnitude adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (GBPspeck) 1404-1413 F10.6 mag RPMAGspeck ?=- Inferred absolute RP magnitude adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (GRPspeck) 1415-1423 F9.6 mag e_GMAGspeck ?=- rms uncertainty on GMAGspeck (Gerrorspeck) 1425-1433 F9.6 mag e_BPMAGspeck ?=- rms uncertainty on BPMAGspeck (GBPerror_speck) 1435-1443 F9.6 mag e_RPMAGspeck ?=- rms uncertainty on RPMAGspeck (GRPerror_speck) 1445-1452 F8.2 K Teff ?=- Adopted projected Teff (Teff) 1454-1462 F9.6 --- logg ?=- Adopted projected logg (logg) 1464-1472 F9.6 --- meta ?=- Adopted projected [M/H] (meta) 1474-1482 F9.6 Gyr age ?=- Inferred age (age) 1484-1491 F8.6 Gyr e_age ?=- rms uncertainty on age (age_error) 1493-1500 F8.6 Msun Mini ?=- Inferred initial stellar mass (M_ini) 1502-1509 F8.6 Msun e_Mini ?=- rms uncertainty on Mini (Minierror) 1511-1520 F10.6 mag GMAG ?=- Inferred absolute G magnitude (G) 1522-1531 F10.6 mag BPMAG ?=- Inferred absolute BP magnitude (G_BP) 1533-1542 F10.6 mag RPMAG ?=- Inferred absolute RP magnitude (G_RP) 1544-1552 F9.6 mag e_GMAG ?=- rms uncertainty on GMAG (G_error) 1554-1562 F9.6 mag e_BPMAG ?=- rms uncertainty on BPMAG (GBPerror) 1564-1572 F9.6 mag e_RPMAG ?=- rms uncertainty on RPMAG (GRPerror) 1574-1583 F10.6 mag E(BP-RP) ?=- Inferred reddening using the projected GBP and GRP (EBPRP) 1585-1593 F9.6 mag e_E(BP-RP) ?=- rms uncertainty on E(BP-RP) (EBPRP_error) 1595-1602 A8 --- pflavour Adopted projection flavour for inferred ages and masses (spec, specjhk, specjhkg, speck or nan) (pflavour) 1604-1613 F10.3 pc rgeo Median of the geometric distance posterior (rmedgeo) 1615-1623 F9.3 pc b_rgeo Lower limit of the geometric distance posterior (rlogeo) 1625-1634 F10.3 pc B_rgeo Upper limit of the geometric distance posterior (rhigeo) 1636-1644 F9.3 pc rpgeo ?=- Median of the photogeometric distance posterior (rmedphotogeo) 1646-1654 F9.3 pc b_rpgeo ?=- Lower limit of the photogeometric distance posterior (rlophotogeo) 1656-1665 F10.3 pc B_rpgeo ?=- Upper limit of the photogeometric distance posterior (99999.999 for infinity) (rhiphotogeo) -------------------------------------------------------------------------------- Acknowledgements: Georges Kordopatis, georges.kordopatis(at)oca.eu
(End) Patricia Vannier [CDS] 12-Dec-2022
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line