Gaia Data Release 2: Properties and validation of the radial velocities
dc.contributor.author | Katz, D | |
dc.contributor.author | Sartoretti, P | |
dc.contributor.author | Cropper, Mark | |
dc.contributor.author | Panuzzo, P | |
dc.contributor.author | Seabroke, G. M | |
dc.contributor.author | Viala, Y | |
dc.contributor.author | Benson, K | |
dc.contributor.author | Blomme, R | |
dc.contributor.author | Jasniewicz, G | |
dc.contributor.author | Jean-Antoine, A | |
dc.contributor.author | Zerjal, Maruska | |
dc.date.accessioned | 2022-05-02T00:49:53Z | |
dc.date.available | 2022-05-02T00:49:53Z | |
dc.date.issued | 2019 | |
dc.date.updated | 2020-12-27T07:22:35Z | |
dc.description.abstract | Context. 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.sponsorship | Funding 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.mimetype | application/pdf | en_AU |
dc.identifier.issn | 0004-6361 | en_AU |
dc.identifier.uri | http://hdl.handle.net/1885/264198 | |
dc.language.iso | en_AU | en_AU |
dc.provenance | https://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.publisher | EDP Sciences | en_AU |
dc.rights | © ESO 2019 | en_AU |
dc.source | Astronomy and Astrophysics | en_AU |
dc.subject | techniques: spectroscopic | en_AU |
dc.subject | techniques: radial velocities | en_AU |
dc.subject | catalogs | en_AU |
dc.subject | surveys | en_AU |
dc.title | Gaia Data Release 2: Properties and validation of the radial velocities | en_AU |
dc.type | Journal article | en_AU |
local.bibliographicCitation.lastpage | 19 | en_AU |
local.bibliographicCitation.startpage | 1 | en_AU |
local.contributor.affiliation | Katz, D, Observatoire de Paris | en_AU |
local.contributor.affiliation | Sartoretti, P, Observatoire de Paris | en_AU |
local.contributor.affiliation | Cropper, Mark, University College London | en_AU |
local.contributor.affiliation | Panuzzo, P, Observatoire de Paris | en_AU |
local.contributor.affiliation | Seabroke, G. M, University College London | en_AU |
local.contributor.affiliation | Viala, Y, Observatoire de Paris | en_AU |
local.contributor.affiliation | Benson, K, University College London | en_AU |
local.contributor.affiliation | Blomme, R, Observatoire Royal de Belgique | en_AU |
local.contributor.affiliation | Jasniewicz, G, Universite de Montpellier II | en_AU |
local.contributor.affiliation | Jean-Antoine, A, CNES Centre Spatial de Toulouse | en_AU |
local.contributor.affiliation | Zerjal, Maruska, College of Science, ANU | en_AU |
local.contributor.authoremail | u1047253@anu.edu.au | en_AU |
local.contributor.authoruid | Zerjal, Maruska, u1047253 | en_AU |
local.description.notes | Imported from ARIES | en_AU |
local.identifier.absfor | 020104 - Galactic Astronomy | en_AU |
local.identifier.absseo | 970102 - Expanding Knowledge in the Physical Sciences | en_AU |
local.identifier.ariespublication | u3102795xPUB1040 | en_AU |
local.identifier.citationvolume | 622 | en_AU |
local.identifier.doi | 10.1051/0004-6361/201833273 | en_AU |
local.identifier.scopusID | 2-s2.0-85062169388 | |
local.identifier.uidSubmittedBy | u3102795 | en_AU |
local.publisher.url | http://www.aanda.org/ | en_AU |
local.type.status | Published Version | en_AU |
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