Gaia Data Release 2: Properties and validation of the radial velocities

dc.contributor.authorKatz, D
dc.contributor.authorSartoretti, P
dc.contributor.authorCropper, Mark
dc.contributor.authorPanuzzo, P
dc.contributor.authorSeabroke, G. M
dc.contributor.authorViala, Y
dc.contributor.authorBenson, K
dc.contributor.authorBlomme, R
dc.contributor.authorJasniewicz, G
dc.contributor.authorJean-Antoine, A
dc.contributor.authorZerjal, Maruska
dc.date.accessioned2022-05-02T00:49:53Z
dc.date.available2022-05-02T00:49:53Z
dc.date.issued2019
dc.date.updated2020-12-27T07:22:35Z
dc.description.abstractContext. For Gaia DR2, 280 million spectra collected by the Radial Velocity Spectrometer instrument on board Gaia were processed, and median radial velocities were derived for 9.8 million sources brighter than GRVS = 12 mag. Aims. This paper describes the validation and properties of the median radial velocities published in Gaia DR2. Methods. Quality tests and filters were applied to select those of the 9.8 million radial velocities that have the quality to be published in Gaia DR2. The accuracy of the selected sample was assessed with respect to ground-based catalogues. Its precision was estimated using both ground-based catalogues and the distribution of the Gaia radial velocity uncertainties. Results. Gaia DR2 contains median radial velocities for 7 224 631 stars, with Teff in the range [3550, 6900] K, which successfully passed the quality tests. The published median radial velocities provide a full-sky coverage and are complete with respect to the astrometric data to within 77.2% (for G larger than or equal to 12.5 mag). The median radial velocity residuals with respect to the ground-based surveys vary from one catalogue to another, but do not exceed a few 100 m s-1. In addition, the Gaia radial velocities show a positive trend as a function of magnitude, which starts around GRVS - 9 mag and reaches about +500 m s-1 at GRVS = 11.75 mag. The origin of the trend is under investigation, with the aim to correct for it in Gaia DR3. The overall precision, estimated from the median of the Gaia radial velocity uncertainties, is 1.05 km s-1. The radial velocity precision is a function of many parameters, in particular, the magnitude and effective temperature. For bright stars, GRVS E [4, 8] mag, the precision, estimated using the full dataset, is in the range 220-350 m s-1, which is about three to five times more precise than the pre-launch specification of 1 km s-1. At the faint end, GRVS = 11.75 mag, the precisions for Teff = 5000 and 6500 K are 1.4 and 3.7 km s-1, respectively.en_AU
dc.description.sponsorshipFunding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. Most of the authors are current or past members of the ESA Gaia mission team and of the Gaia DPAC and their work has been supported by the French Centre National de la Recherche Scientifique (CNRS), the Centre National d’Etudes Spatiales (CNES), the Agence Nationale de la Recherche, the Région Aquitaine, the Université de Bordeaux, the Utinam Institute of the Université de Franche-Comté, and the Institut des Sciences de l’ Univers (INSU); the Science and Technology Facilities Council and the United Kingdom Space Agency; the Belgian Federal Science Policy Office (BELSPO) through various Programme de Développement d’Expériences Scientifiques (PRODEX) grants; the German Aerospace Agency (Deutsches Zentrum fur Luft- und Raumfahrt e.V., DLR); the Algerian Centre de Recherche en Astronomie, Astrophysique et Géophysique of Bouzareah Observatory; the Swiss State Secretariat for Education, Research, and Innovation through the ESA PRODEX programme, the Mesures d’Accompagnement, the Swiss Activités Nationales Complémentaires, and the Swiss National Science Foundation; the Slovenian Research Agency (research core funding No. P1-0188)en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-6361en_AU
dc.identifier.urihttp://hdl.handle.net/1885/264198
dc.language.isoen_AUen_AU
dc.provenancehttps://v2.sherpa.ac.uk/id/publication/11142..."The Published Version can be archived in any website" from SHERPA/RoMEO site (as at 2/05/2022).en_AU
dc.publisherEDP Sciencesen_AU
dc.rights© ESO 2019en_AU
dc.sourceAstronomy and Astrophysicsen_AU
dc.subjecttechniques: spectroscopicen_AU
dc.subjecttechniques: radial velocitiesen_AU
dc.subjectcatalogsen_AU
dc.subjectsurveysen_AU
dc.titleGaia Data Release 2: Properties and validation of the radial velocitiesen_AU
dc.typeJournal articleen_AU
local.bibliographicCitation.lastpage19en_AU
local.bibliographicCitation.startpage1en_AU
local.contributor.affiliationKatz, D, Observatoire de Parisen_AU
local.contributor.affiliationSartoretti, P, Observatoire de Parisen_AU
local.contributor.affiliationCropper, Mark, University College Londonen_AU
local.contributor.affiliationPanuzzo, P, Observatoire de Parisen_AU
local.contributor.affiliationSeabroke, G. M, University College Londonen_AU
local.contributor.affiliationViala, Y, Observatoire de Parisen_AU
local.contributor.affiliationBenson, K, University College Londonen_AU
local.contributor.affiliationBlomme, R, Observatoire Royal de Belgiqueen_AU
local.contributor.affiliationJasniewicz, G, Universite de Montpellier IIen_AU
local.contributor.affiliationJean-Antoine, A, CNES Centre Spatial de Toulouseen_AU
local.contributor.affiliationZerjal, Maruska, College of Science, ANUen_AU
local.contributor.authoremailu1047253@anu.edu.auen_AU
local.contributor.authoruidZerjal, Maruska, u1047253en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor020104 - Galactic Astronomyen_AU
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciencesen_AU
local.identifier.ariespublicationu3102795xPUB1040en_AU
local.identifier.citationvolume622en_AU
local.identifier.doi10.1051/0004-6361/201833273en_AU
local.identifier.scopusID2-s2.0-85062169388
local.identifier.uidSubmittedByu3102795en_AU
local.publisher.urlhttp://www.aanda.org/en_AU
local.type.statusPublished Versionen_AU

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