| Autor: |
Brown, A. G. A. Vallenari, A. Prusti, T. de Bruijne, J. H. J. Babusiaux, C. Biermann, M. Creevey, O. L. Evans, D. W. Eyer, L. Hutton, A. Jansen, F. Jordi, C. Klioner, S. A. Lammers, U. Lindegren, L. Luri, X. Mignard, F. and Panem, C. Pourbaix, D. Randich, S. Sartoretti, P. and Soubiran, C. Walton, N. A. Arenou, F. Bailer-Jones, C. A. L. and Bastian, U. Cropper, M. Drimmel, R. Katz, D. and Lattanzi, M. G. van Leeuwen, F. Bakker, J. Cacciari, C. and Castaneda, J. De Angeli, F. Ducourant, C. Fabricius, C. and Fouesneau, M. Fremat, Y. Guerra, R. Guerrier, A. and Guiraud, J. Jean-Antoine Piccolo, A. Masana, E. Messineo, R. and Mowlavi, N. Nicolas, C. Nienartowicz, K. Pailler, F. and Panuzzo, P. Riclet, F. Roux, W. Seabroke, G. M. Sordo, R. Tanga, P. Thevenin, F. Gracia-Abril, G. Portell, J. and Teyssier, D. Altmann, M. Andrae, R. Bellas-Velidis, I. and Benson, K. Berthier, J. Blomme, R. Brugaletta, E. and Burgess, P. W. Busso, G. Carry, B. Cellino, A. Cheek, N. and Clementini, G. Damerdji, Y. Davidson, M. Delchambre, L. and Dell'Oro, A. Fernandez-Hernandez, J. Galluccio, L. and Garcia-Lario, P. Garcia-Reinaldos, M. Gonzalez-Nunez, J. and Gosset, E. Haigron, R. Halbwachs, J. -L. Hambly, N. C. and Harrison, D. L. Hatzidimitriou, D. Heiter, U. Hernandez, J. and Hestroffer, D. Hodgkin, S. T. Holl, B. Janssen, K. and Jevardat de Fombelle, G. Jordan, S. Krone-Martins, A. and Lanzafame, A. C. Loeffler, W. Lorca, A. Manteiga, M. and Marchal, O. Marrese, P. M. Moitinho, A. Mora, A. and Muinonen, K. Osborne, P. Pancino, E. Pauwels, T. Petit, J. -M. Recio-Blanco, A. Richards, P. J. Riello, M. and Rimoldini, L. Robin, A. C. Roegiers, T. Rybizki, J. and Sarro, L. M. Siopis, C. Smith, M. Sozzetti, A. Ulla, A. and Utrilla, E. van Leeuwen, M. van Reeven, W. Abbas, U. and Abreu Aramburu, A. Accart, S. Aerts, C. Aguado, J. J. and Ajaj, M. Altavilla, G. Alvarez, M. A. Alvarez Cid-Fuentes, J. Alves, J. Anderson, R. I. Anglada Varela, E. Antoja, T. Audard, M. Baines, D. Baker, S. G. Balaguer-Nunez, L. and Balbinot, E. Balog, Z. Barache, C. Barbato, D. and Barros, M. Barstow, M. A. Bartolome, S. Bassilana, J. -L. and Bauchet, N. Baudesson-Stella, A. Becciani, U. and Bellazzini, M. Bernet, M. Bertone, S. Bianchi, L. and Blanco-Cuaresma, S. Boch, T. Bombrun, A. Bossini, D. and Bouquillon, S. Bragaglia, A. Bramante, L. Breedt, E. and Bressan, A. Brouillet, N. Bucciarelli, B. Burlacu, A. and Busonero, D. Butkevich, A. G. Buzzi, R. Caffau, E. and Cancelliere, R. Canovas, H. Cantat-Gaudin, T. Carballo, R. and Carlucci, T. Carnerero, I, M. Carrasco, J. M. and Casamiquela, L. Castellani, M. Castro-Ginard, A. Castro Sampol, P. Chaoul, L. Charlot, P. Chemin, L. Chiavassa, A. Cioni, M. -R. L. Comoretto, G. Cooper, W. J. Cornez, T. Cowell, S. Crifo, F. Crosta, M. Crowley, C. and Dafonte, C. Dapergolas, A. David, M. David, P. de Laverny, P. De Luise, F. De March, R. De Ridder, J. de Souza, R. de Teodoro, P. de Torres, A. del Peloso, E. F. and del Pozo, E. Delbo, M. Delgado, A. Delgado, H. E. and Delisle, J. -B. Di Matteo, P. Diakite, S. Diener, C. and Distefano, E. Dolding, C. Eappachen, D. Edvardsson, B. and Enke, H. Esquej, P. Fabre, C. Fabrizio, M. Faigler, S. and Fedorets, G. Fernique, P. Fienga, A. Figueras, F. and Fouron, C. Fragkoudi, F. Fraile, E. Franke, F. Gai, M. and Garabato, D. Garcia-Gutierrez, A. Garcia-Torres, M. and Garofalo, A. Gavras, P. Gerlach, E. Geyer, R. Giacobbe, P. Gilmore, G. Girona, S. Giuffrida, G. Gomel, R. and Gomez, A. Gonzalez-Santamaria, I. Gonzalez-Vidal, J. J. and Granvik, M. Gutierrez-Sanchez, R. Guy, L. P. Hauser, M. and Haywood, M. Helmi, A. Hidalgo, S. L. Hilger, T. and Hladczuk, N. Hobbs, D. Holland, G. Huckle, H. E. and Jasniewicz, G. Jonker, P. G. Juaristi Campillo, J. Julbe, F. and Karbevska, L. Kervella, P. Khanna, S. Kochoska, A. and Kontizas, M. Kordopatis, G. Korn, A. J. Kostrzewa-Rutkowska, Z. Kruszynska, K. Lambert, S. Lanza, A. F. Lasne, Y. and Le Campion, J. -F. Le Fustec, Y. Lebreton, Y. Lebzelter, T. and Leccia, S. Leclerc, N. Lecoeur-Taibi, I. Liao, S. and Licata, E. Lindstrom, E. P. Lister, T. A. Livanou, E. and Lobel, A. Madrero Pardo, P. Managau, S. Mann, R. G. and Marchant, J. M. Marconi, M. Marcos Santos, M. M. S. and Marinoni, S. Marocco, F. Marshall, D. J. Martin Polo, L. and Martin-Fleitas, J. M. Masip, A. Massari, D. and Mastrobuono-Battisti, A. Mazeh, T. McMillan, P. J. Messina, S. Michalik, D. Millar, N. R. Mints, A. Molina, D. and Molinaro, R. Molnar, L. Montegriffo, P. Mor, R. and Morbidelli, R. Morel, T. Morris, D. Mulone, A. F. Munoz, D. Muraveva, T. Murphy, C. P. Musella, I. Noval, L. and Ordenovic, C. Orru, G. Osinde, J. Pagani, C. Pagano, I. and Palaversa, L. Palicio, P. A. Panahi, A. Pawlak, M. and Penalosa Esteller, X. Penttila, A. Piersimoni, A. M. Pineau, F. -X. Plachy, E. Plum, G. Poggio, E. Poretti, E. and Poujoulet, E. Prsa, A. Pulone, L. Racero, E. Ragaini, S. and Rainer, M. Raiteri, C. M. Rambaux, N. Ramos, P. and Ramos-Lerate, M. Re Fiorentin, P. Regibo, S. Reyle, C. and Ripepi, V. Riva, A. Rixon, G. Robichon, N. Robin, C. and Roelens, M. Rohrbasser, L. Romero-Gomez, M. Rowell, N. and Royer, F. Rybicki, K. A. Sadowski, G. Sagrista Selles, A. and Sahlmann, J. Salgado, J. Salguero, E. Samaras, N. and Sanchez Gimenez, V. Sanna, N. Santovena, R. Sarasso, M. and Schultheis, M. Sciacca, E. Segol, M. Segovia, J. C. and Segransan, D. Semeux, D. Shahaf, S. Siddiqui, H. I. and Siebert, A. Siltala, L. Slezak, E. Smart, R. L. Solano, E. Solitro, F. Souami, D. Souchay, J. Spagna, A. and Spoto, F. Steele, I. A. Steidelmueller, H. Stephenson, C. A. and Suveges, M. Szabados, L. Szegedi-Elek, E. Taris, F. and Tauran, G. Taylor, M. B. Teixeira, R. Thuillot, W. and Tonello, N. Torra, F. Torra, J. Turon, C. Unger, N. and Vaillant, M. van Dillen, E. Vanel, O. Vecchiato, A. and Viala, Y. Vicente, D. Voutsinas, S. Weiler, M. Wevers, T. Wyrzykowski, L. Yoldas, A. Yvard, P. Zhao, H. and Zorec, J. Zucker, S. Zurbach, C. Zwitter, T. Gaia Collaboration |
| Jazyk: |
angličtina |
| Rok vydání: |
2021 |
| Popis: |
Context. We present the early installment of the third Gaia data release, Gaia EDR3, consisting of astrometry and photometry for 1.8 billion sources brighter than magnitude 21, complemented with the list of radial velocities from Gaia DR2. Aims. A summary of the contents of Gaia EDR3 is presented, accompanied by a discussion on the differences with respect to Gaia DR2 and an overview of the main limitations which are present in the survey. Recommendations are made on the responsible use of Gaia EDR3 results. Methods. The raw data collected with the Gaia instruments during the first 34 months of the mission have been processed by the Gaia Data Processing and Analysis Consortium and turned into this early third data release, which represents a major advance with respect to Gaia DR2 in terms of astrometric and photometric precision, accuracy, and homogeneity. Results. Gaia EDR3 contains celestial positions and the apparent brightness in G for approximately 1.8 billion sources. For 1.5 billion of those sources, parallaxes, proper motions, and the (G(BP) - G(RP)) colour are also available. The passbands for G, G(BP), and G(RP) are provided as part of the release. For ease of use, the 7 million radial velocities from Gaia DR2 are included in this release, after the removal of a small number of spurious values. New radial velocities will appear as part of Gaia DR3. Finally, Gaia EDR3 represents an updated materialisation of the celestial reference frame (CRF) in the optical, the Gaia-CRF3, which is based solely on extragalactic sources. The creation of the source list for Gaia EDR3 includes enhancements that make it more robust with respect to high proper motion stars, and the disturbing effects of spurious and partially resolved sources. The source list is largely the same as that for Gaia DR2, but it does feature new sources and there are some notable changes. The source list will not change for Gaia DR3. Conclusions. Gaia EDR3 represents a significant advance over Gaia DR2, with parallax precisions increased by 30 per cent, proper motion precisions increased by a factor of 2, and the systematic errors in the astrometry suppressed by 30-40% for the parallaxes and by a factor similar to 2.5 for the proper motions. The photometry also features increased precision, but above all much better homogeneity across colour, magnitude, and celestial position. A single passband for G, G(BP), and G(RP) is valid over the entire magnitude and colour range, with no systematics above the 1% level |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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