| hal.structure.identifier | Max Planck Institute for Astronomy [MPIA] | |
| dc.contributor.author | FOUESNEAU, M. | |
| hal.structure.identifier | Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB] | |
| dc.contributor.author | FRÉMAT, Y. | |
| hal.structure.identifier | Max Planck Institute for Astronomy [MPIA] | |
| dc.contributor.author | ANDRAE, R. | |
| dc.contributor.author | KORN, A.J. | |
| hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
| dc.contributor.author | SOUBIRAN, C. | |
| hal.structure.identifier | Joseph Louis LAGRANGE [LAGRANGE] | |
| dc.contributor.author | KORDOPATIS, G. | |
| hal.structure.identifier | INAF - Osservatorio Astronomico di Padova [OAPD] | |
| dc.contributor.author | VALLENARI, A. | |
| hal.structure.identifier | Uppsala University | |
| dc.contributor.author | HEITER, U. | |
| dc.contributor.author | CREEVEY, O.L. | |
| dc.contributor.author | SARRO, L.M. | |
| hal.structure.identifier | Joseph Louis LAGRANGE [LAGRANGE] | |
| dc.contributor.author | DE LAVERNY, P. | |
| dc.contributor.author | LANZAFAME, A.C. | |
| hal.structure.identifier | Royal Observatory of Belgium = Observatoire Royal de Belgique [ROB] | |
| dc.contributor.author | LOBEL, A. | |
| hal.structure.identifier | INAF - Osservatorio Astronomico di Padova [OAPD] | |
| dc.contributor.author | SORDO, R. | |
| dc.contributor.author | RYBIZKI, J. | |
| hal.structure.identifier | Joseph Louis LAGRANGE [LAGRANGE] | |
| dc.contributor.author | SLEZAK, I. | |
| dc.contributor.author | ALVAREZ, M.A. | |
| hal.structure.identifier | INAF - Osservatorio Astrofisico di Torino [OATo] | |
| dc.contributor.author | DRIMMEL, R. | |
| hal.structure.identifier | Universidade da Coruña | |
| dc.contributor.author | GARABATO, D. | |
| hal.structure.identifier | Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics [LESIA] | |
| hal.structure.identifier | Institut de Physique de Rennes [IPR] | |
| dc.contributor.author | LEBRETON, Y. | |
| hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
| dc.contributor.author | BOURET, J.-C. | |
| dc.date.issued | 2023-06 | |
| dc.identifier.issn | 0004-6361 | |
| dc.description.abstractEn | The third Gaia data release contains, beyond the astrometry and photometry, dispersed light for hundreds of millions of sources from the Gaia prism spectra (BP and RP) and the spectrograph (RVS). This data release opens a new window on the chemo-dynamical properties of stars in our Galaxy, essential knowledge for understanding the structure, formation, and evolution of the Milky Way. To provide insight into the physical properties of Milky Way stars, we used these data to produce a uniformly-derived, all-sky catalog of stellar astrophysical parameters (APs): Teff, logg, [M/H], [$\alpha$/Fe], activity index, emission lines, rotation, 13 chemical abundance estimates, radius, age, mass, bolometric luminosity, distance, and dust extinction. We developed the Apsis pipeline to infer APs of Gaia objects by analyzing their astrometry, photometry, BP/RP, and RVS spectra. We validate our results against other literature works, including benchmark stars, interferometry, and asteroseismology. Here we assessed the stellar analysis performance from Apsis statistically. We describe the quantities we obtained, including our results' underlying assumptions and limitations. We provide guidance and identify regimes in which our parameters should and should not be used. Despite some limitations, this is the most extensive catalog of uniformly-inferred stellar parameters to date. These comprise Teff, logg, and [M/H] (470 million using BP/RP, 6 million using RVS), radius (470 million), mass (140 million), age (120 million), chemical abundances (5 million), diffuse interstellar band analysis (1/2 million), activity indices (2 million), H{$\alpha$} equivalent widths (200 million), and further classification of spectral types (220 million) and emission-line stars (50 thousand). More precise and detailed astrophysical parameters based on epoch BP, RP, and RVS are planned for the next Gaia data release. | |
| dc.language.iso | en | |
| dc.publisher | EDP Sciences | |
| dc.rights.uri | http://creativecommons.org/licenses/by/ | |
| dc.subject.en | Astrophysics - Solar and Stellar Astrophysics | |
| dc.subject.en | Astrophysics - Astrophysics of Galaxies | |
| dc.title.en | Gaia Data Release 3: Apsis II -- Stellar Parameters | |
| dc.type | Article de revue | |
| dc.identifier.doi | 10.1051/0004-6361/202243919 | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph] | |
| dc.identifier.arxiv | 2206.05992 | |
| bordeaux.journal | Astronomy and Astrophysics - A&A | |
| bordeaux.page | A28 | |
| bordeaux.volume | 674 | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-03857352 | |
| hal.version | 1 | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-03857352v1 | |
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