{"paper":{"title":"Gaia Data Release 3: Apsis II -- Stellar Parameters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A. Abreu Aramburu, A. Bijaoui, A. Burlacu, A. Chiavassa, A.C. Lanzafame, A. Gomez, A. Jean-Antoine Piccolo, A.J. Korn, A. Lobel, A. Lorca, A. Magdaleno Romeo, A. Recio-Blanco, A. Silvelo, A. Ulla, A. Vallenari, B. Pichon, C.A.L. Bailer-Jones, C. Dafonte, C. Demouchy, C. Martayan, C. Nicolas, C. Ordenovic, C. Robin, C. Soubiran, D. Garabato, D. Hatzidimitriou, D.J. Marshall, E. Brugaletta, E. Livanou, E.L. Licata, E. Poggio, E. Utrilla, E. van Dillen, F. Marocco, F. Pailler, F. Riclet, F. Th\\'evenin, G. Contursi, G. Kordopatis, G. Torralba Elipe, H.E.P. Lindstr{\\o}m, H. Zhao, I. Bellas-Velidis, I. Gonz\\'alez-Santamar\\'ia, I. Slezak, J. Bakker, J.-C. Bouret, J. Rybizki, J. Zorec, L. Casamiquela, L. Chaoul, L. Delchambre, L.M. Sarro, L. Pallas-Quintela, M.A. \\'Alvarez, M. Fouesneau, M. Garc\\'ia-Torres, M. Kontizas, M. Manteiga, M. Segol, M.S. Schultheis, M. S\\\"uveges, N. Brouillet, N. Mary, O.L. Creevey, P.A. Palicio, P. de Laverny, P. Garc\\'ia-Lario, R. Andrae, R. Blomme, R. Carballo, R. Drimmel, R.L. Smart, R. Santove\\~na, R. Sordo, T.E. Dharmawardena, U. Heiter, W.J. Cooper, Y. Fr\\'emat, Y. Lebreton, Y. Le Fustec","submitted_at":"2022-06-13T09:28:20Z","abstract_excerpt":"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], a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2206.05992","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2206.05992/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}