Gaia Data Release 2: The astrometric solution

L. Lindegren J. Hernandez 1 A. Bombrun 2 S. Klioner U. Bastian 3 M. Ramos-Lerate A. De Torres H. Steidelmuller C. Stephenson D. Hobbs 4 U. Lammers 5 M. Biermann 6 R. Geyer 7 T. Hilger D. Michalik U. Stampa P. J. Mcmillan J. Castaneda M. Clotet G. Comoretto 8 M. Davidson C. Fabricius 9 G. Gracia N. C. Hambly A. Hutton A. Mora 10 J. Portell F. Van Leeuwen U. Abbas 11 A. Abreu M. Altmann 3 A. Andrei 12 E. Anglada 13 L. Balaguer-Núñez 14 C. Barache 15 U. Becciani S. Bertone L. Bianchi 16 S. Bouquillon 15 G. Bourda 17 T. Brusemeister B. Bucciarelli D. Busonero R. Buzzi R. Cancelliere T. Carlucci 15 P. Charlot 17 N. Cheek M. Crosta C. Crowley 18 J. De Bruijne F. De Felice R. Drimmel P. Esquej A. Fienga 19 E. Fraile M. Gai 20 N. Garralda J. J. Gonzalez-Vidal R. Guerra 21 M. Hauser W. Hofmann B. Holl 22 S. Jordan 23 M. G. Lattanzi H. Lenhardt S. Liao E. Licata T. Lister W. Loffler J. Marchant 24 J.-M. Martin-Fleitas R. Messineo F. Mignard 25 R. Morbidelli E. Poggio A. Riva 26 N. Rowell E. Salguero M. Sarasso E. Sciacca H. Siddiqui 27 R. L. Smart 20 A. Spagna I. Steele 28 F. Taris J. Torra A. Van Elteren W. Van Reeven A. Vecchiato 29
17 M2A 2018
LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac]
29 Astrometry
OATo - INAF - Osservatorio Astrofisico di Torino
Abstract : Gaia Data Release 2 (Gaia DR2) contains results for 1693 million sources in the magnitude range 3 to 21 based on observations collected by the European Space Agency Gaia satellite during the first 22 months of its operational phase. We describe the input data, models, and processing used for the astrometric content of Gaia DR2, and the validation of these results performed within the astrometry task. Some 320 billion centroid positions from the pre-processed astrometric CCD observations were used to estimate the five astrometric parameters (positions, parallaxes, and proper motions) for 1332 million sources, and approximate positions at the reference epoch J2015.5 for an additional 361 million mostly faint sources. Special validation solutions were used to characterise the random and systematic errors in parallax and proper motion. For the sources with five-parameter astrometric solutions, the median uncertainty in parallax and position at the reference epoch J2015.5 is about 0.04 mas for bright (G<14 mag) sources, 0.1 mas at G=17 mag, and 0.7 mas at G=20 mag. In the proper motion components the corresponding uncertainties are 0.05, 0.2, and 1.2 mas/yr, respectively. The optical reference frame defined by Gaia DR2 is aligned with ICRS and is non-rotating with respect to the quasars to within 0.15 mas/yr. From the quasars and validation solutions we estimate that systematics in the parallaxes depending on position, magnitude, and colour are generally below 0.1 mas, but the parallaxes are on the whole too small by about 0.03 mas. Significant spatial correlations of up to 0.04 mas in parallax and 0.07 mas/yr in proper motion are seen on small (<1 deg) and intermediate (20 deg) angular scales. Important statistics and information for the users of the Gaia DR2 astrometry are given in the appendices.
Type de document :
Article dans une revue
Astronomy and Astrophysics - A&A, EDP Sciences, 2018
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Contributeur : Marie-Paule Pomies <>
Soumis le : mardi 22 mai 2018 - 12:25:17
Dernière modification le : mardi 29 mai 2018 - 12:51:09

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L. Lindegren, J. Hernandez, A. Bombrun, S. Klioner, U. Bastian, et al.. Gaia Data Release 2: The astrometric solution. Astronomy and Astrophysics - A&A, EDP Sciences, 2018. 〈hal-01797082〉



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