Title: | Gaia Data Release 3. A golden sample of astrophysical parameters |
Authors: | Gaia Collaboration Creevey, O. L. Sarro, L. M. Lobel, A. PANCINO, Elena Andrae, R. SMART, Richard Laurence CLEMENTINI, Gisella Heiter, U. Korn, A. J. Fouesneau, M. Frémat, Y. De Angeli, F. VALLENARI, Antonella Harrison, D. L. Thévenin, F. Reylé, C. SORDO, Rosanna GAROFALO, Alessia Brown, A. G. A. Eyer, L. Prusti, T. de Bruijne, J. H. J. Arenou, F. Babusiaux, C. Biermann, M. Ducourant, C. Evans, D. W. Guerra, R. Hutton, A. Jordi, C. Klioner, S. A. Lammers, U. L. Lindegren, L. Luri, X. Mignard, F. Panem, C. Pourbaix, D. RANDICH, Maria Sofia Sartoretti, P. Soubiran, C. Tanga, P. Walton, N. A. Bailer-Jones, C. A. L. Bastian, U. DRIMMEL, Ronald Jansen, F. Katz, D. LATTANZI, Mario Gilberto van Leeuwen, F. Bakker, J. Cacciari, C. Castañeda, J. Fabricius, C. Galluccio, L. Guerrier, A. Masana, E. Messineo, R. Mowlavi, N. Nicolas, C. Nienartowicz, K. Pailler, F. Panuzzo, P. Riclet, F. Roux, W. Seabroke, G. M. Gracia-Abril, G. Portell, J. Teyssier, D. Altmann, M. Audard, M. Bellas-Velidis, I. Benson, K. Berthier, J. Blomme, R. Burgess, P. W. BUSONERO, Deborah Busso, G. Cánovas, H. Carry, B. CELLINO, Alberto Cheek, N. Damerdji, Y. Davidson, M. de Teodoro, P. Nuñez Campos, M. Delchambre, L. DELL'ORO, Aldo Esquej, P. Fernández-Hernández, J. Fraile, E. Garabato, D. García-Lario, P. Gosset, E. Haigron, R. Halbwachs, J. -L. Hambly, N. C. Hernández, J. Hestroffer, D. Hodgkin, S. T. Holl, B. Janßen, K. Jevardat de Fombelle, G. Jordan, S. Krone-Martins, A. LANZAFAME, Alessandro Löffler, W. Marchal, O. MARRESE, Paola Maria Moitinho, A. Muinonen, K. Osborne, P. Pauwels, T. Recio-Blanco, A. Riello, M. Rimoldini, L. Roegiers, T. Rybizki, J. Siopis, C. Smith, M. SOZZETTI, Alessandro Utrilla, E. van Leeuwen, M. ABBAS, Ummi Ábrahám, P. Abreu Aramburu, A. Aerts, C. Aguado, J. J. Ajaj, M. Aldea-Montero, F. ALTAVILLA, Giuseppe Álvarez, M. A. Alves, J. Anders, F. Anderson, R. I. Anglada Varela, E. Antoja, T. Baines, D. Baker, S. G. Balaguer-Núñez, L. Balbinot, E. Balog, Z. Barache, C. Barbato, D. Barros, M. Barstow, M. A. Bartolomé, S. Bassilana, J. -L. Bauchet, N. BECCIANI, Ugo BELLAZZINI, Michele Berihuete, A. Bernet, M. BERTONE, Stefano Bianchi, L. Binnenfeld, A. Blanco-Cuaresma, S. Boch, T. Bombrun, A. Bossini, D. Bouquillon, S. BRAGAGLIA, Angela Bramante, L. Breedt, E. Bressan, A. Brouillet, N. BRUGALETTA, Elisa BUCCIARELLI, Beatrice Burlacu, A. Butkevich, A. G. BUZZI, Raffaella Caffau, E. Cancelliere, R. Cantat-Gaudin, T. Carballo, R. Carlucci, T. CARNERERO MARTIN, Maria Isabel Carrasco, J. M. Casamiquela, L. CASTELLANI, Marco Castro-Ginard, A. Chaoul, L. Charlot, P. Chemin, L. Chiaramida, V. Chiavassa, A. Chornay, N. COMORETTO, Giovanni Contursi, G. Cooper, W. J. Cornez, T. Cowell, S. Crifo, F. Cropper, M. CROSTA, Mariateresa Crowley, C. Dafonte, C. Dapergolas, A. David, P. de Laverny, P. DE LUISE, Fiore De March, R. De Ridder, J. de Souza, R. de Torres, A. del Peloso, E. F. del Pozo, E. Delbo, M. Delgado, A. Delisle, J. -B. Demouchy, C. Dharmawardena, T. E. Di Matteo, P. Diakite, S. Diener, C. DISTEFANO, Elisa Maria Carmela Dolding, C. Enke, H. Fabre, C. FABRIZIO, Michele Faigler, S. Fedorets, G. Fernique, P. Figueras, F. Fournier, Y. Fouron, C. Fragkoudi, F. GAI, Mario Garcia-Gutierrez, A. Garcia-Reinaldos, M. García-Torres, M. Gavel, A. Gavras, P. Gerlach, E. Geyer, R. GIACOBBE, Paolo Gilmore, G. Girona, S. Giuffrida, G. Gomel, R. Gomez, A. González-Núñez, J. González-Santamaría, I. González-Vidal, J. J. Granvik, M. Guillout, P. Guiraud, J. Gutiérrez-Sánchez, R. Guy, L. P. Hatzidimitriou, D. Hauser, M. Haywood, M. Helmer, A. Helmi, A. Hilger, T. Sarmiento, M. H. Hidalgo, S. L. Hładczuk, N. Hobbs, D. Holland, G. Huckle, H. E. Jardine, K. Jasniewicz, G. Jean-Antoine Piccolo, A. Jiménez-Arranz, Ó. Juaristi Campillo, J. Julbe, F. Karbevska, L. Kervella, P. Khanna, S. Kordopatis, G. Kóspál, Á. Kostrzewa-Rutkowska, Z. Kruszyńska, K. Kun, M. Laizeau, P. Lambert, S. LANZA, Antonino Francesco Lasne, Y. Le Campion, J. -F. Lebreton, Y. Lebzelter, T. LECCIA, Silvio Leclerc, N. Lecoeur-Taibi, I. Liao, S. Licata, E. L. Lindstrøm, H. E. P. Lister, T. A. Livanou, E. Lorca, A. Loup, C. Madrero Pardo, P. Magdaleno Romeo, A. Managau, S. Mann, R. G. Manteiga, M. Marchant, J. M. MARCONI, Marcella Marcos, J. Marcos Santos, M. M. S. Marín Pina, D. MARINONI, Silvia Marocco, F. Marshall, D. J. Martin Polo, L. Martín-Fleitas, J. M. Marton, G. Mary, N. Masip, A. Massari, D. Mastrobuono-Battisti, A. Mazeh, T. McMillan, P. J. MESSINA, Sergio Michalik, D. Millar, N. R. Mints, A. Molina, D. MOLINARO, Roberto Molnár, L. Monari, G. Monguió, M. MONTEGRIFFO, Paolo Montero, A. Mor, R. Mora, A. MORBIDELLI, Roberto Morel, T. Morris, D. MURAVEVA, Tatiana Murphy, C. P. MUSELLA, ILARIA Nagy, Z. Noval, L. Ocaña, F. Ogden, A. Ordenovic, C. Osinde, J. O. Pagani, C. PAGANO, Isabella Palaversa, L. Palicio, P. A. Pallas-Quintela, L. Panahi, A. Payne-Wardenaar, S. Peñalosa Esteller, X. Penttilä, A. Pichon, B. PIERSIMONI, Anna Marina Pineau, F. -X. Plachy, E. Plum, G. POGGIO, Eloisa Prša, A. Racero, E. Ragaini, S. RAINER, Monica RAITERI, Claudia Maria Ramos, P. Ramos-Lerate, M. RE FIORENTIN, Paola Regibo, S. Richards, P. J. Rios Diaz, C. RIPEPI, Vincenzo RIVA, Alberto Rix, H. -W. Rixon, G. Robichon, N. Robin, A. C. Robin, C. Roelens, M. Rogues, H. R. O. Rohrbasser, L. Romero-Gómez, M. Rowell, N. Royer, F. Ruz Mieres, D. Rybicki, K. A. Sadowski, G. Sáez Núñez, A. Sagristà Sellés, A. Sahlmann, J. Salguero, E. Samaras, N. Sanchez Gimenez, V. SANNA, Nicoletta Santoveña, R. SARASSO, Maria Margherita Schultheis, M. SCIACCA, Eva Segol, M. Segovia, J. C. Ségransan, D. Semeux, D. Shahaf, S. Siddiqui, H. I. Siebert, A. Siltala, L. Silvelo, A. Slezak, E. Slezak, I. Snaith, O. N. Solano, E. Solitro, F. Souami, D. Souchay, J. SPAGNA, Alessandro Spina, L. Spoto, F. Steele, I. A. Steidelmüller, H. Stephenson, C. A. Süveges, M. Surdej, J. Szabados, L. Szegedi-Elek, E. Taris, F. Taylor, M. B. Teixeira, R. Tolomei, L. Tonello, N. Torra, F. Torra, J. Torralba Elipe, G. Trabucchi, M. Tsounis, A. T. Turon, C. Ulla, A. Unger, N. Vaillant, M. V. van Dillen, E. van Reeven, W. Vanel, O. VECCHIATO, Alberto Viala, Y. Vicente, D. Voutsinas, S. Weiler, M. Wevers, T. Wyrzykowski, Ł. Yoldas, A. Yvard, P. Zhao, H. Zorec, J. Zucker, S. Zwitter, T. |
Issue Date: | 2023 |
Journal: | ASTRONOMY & ASTROPHYSICS |
Number: | 674 |
First Page: | A39 |
Abstract: | Context.Gaia Data Release 3 (DR3) provides a wealth of new data products for the astronomical community to exploit, including astrophysical parameters for half a billion stars. In this work, we demonstrate the high quality of these data products and illustrate their use in different astrophysical contexts. <BR /> Aims: We produce homogeneous samples of stars with high-quality astrophysical parameters by exploiting Gaia DR3, while focusing on many regimes across the Hertzsprung-Russell (HR) diagram; spectral types OBA, FGKM, and ultracool dwarfs (UCDs). We also focus on specific subsamples of particular interest to the community: solar analogues, carbon stars, and the Gaia spectrophotometric standard stars (SPSS). <BR /> Methods: We query the astrophysical parameter tables along with other tables in Gaia DR3 to derive the samples of the stars of interest. We validate our results using the Gaia catalogue itself and by comparison with external data. <BR /> Results: We produced six homogeneous samples of stars with high-quality astrophysical parameters across the HR diagram for the community to exploit. We first focus on three samples that span a large parameter space: young massive disc stars (OBA; about 3 Million), FGKM spectral type stars (about 3 Million), and UCDs (about 20 000). We provide these sources along with additional information (either a flag or complementary parameters) as tables that are made available in the Gaia archive. We also identify 15 740 bone fide carbon stars and 5863 solar analogues, and provide the first homogeneous set of stellar parameters of the SPSS sample. We demonstrate some applications of these samples in different astrophysical contexts. We use a subset of the OBA sample to illustrate its usefulness in analysing the Milky Way rotation curve. We then use the properties of the FGKM stars to analyse known exoplanet systems. We also analyse the ages of some unseen UCD-companions to the FGKM stars. We additionally predict the colours of the Sun in various passbands (Gaia, 2MASS, WISE) using the solar-analogue sample. Conclusions.Gaia DR3 contains a wealth of new high-quality astrophysical parameters for the community to exploit. <P />Full Table 8 is only available at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr/">cdsarc.u-strasbg.fr</A> ( ftp://130.79.128.5 ) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/674/A39">http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/674/A39</A> <P />This paper contains tables that are made available only through the Gaia archive under Performance verification.... |
URI: | http://hdl.handle.net/20.500.12386/36234 |
URL: | https://www.aanda.org/articles/aa/full_html/2023/06/aa43800-22/aa43800-22.html https://api.elsevier.com/content/abstract/scopus_id/85164201977 |
ISSN: | 0004-6361 |
DOI: | 10.1051/0004-6361/202243800 |
Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista
|