posted on 2016-11-28, 13:45authored byGaia Collaboration, M. I. Wilkinson
Gaia is a cornerstone mission in the science programme of the EuropeanSpace Agency (ESA). The spacecraft construction was approved in 2006, following a study in which the original interferometric concept was changed to a direct-imaging approach. Both the spacecraft and the payload were built by European industry. The involvement of the scientific community focusses on data processing for which the international Gaia Data Processing and Analysis Consortium (DPAC) was selected in 2007. Gaia was launched on 19 December 2013 and arrived at its operating point, the second Lagrange point of the Sun-Earth-Moon system, a few weeks later. The commissioning of the spacecraft and payload was completed on 19 July 2014. The nominal five-year mission started with four weeks of special, ecliptic-pole scanning and subsequently transferred into full-sky scanning mode. We recall the scientific goals of Gaia and give a description of the as-built spacecraft that is currently (mid-2016) being operated to achieve these goals. We pay special attention to the payload module, the performance of which is closely related to the scientific performance of the mission. We provide a summary of the commissioning activities and findings, followed by a description of the routine operational mode. We summarise scientific performance estimates on the basis of in-orbit operations. Several intermediate Gaia data releases are planned and the data can be retrieved from the Gaia Archive, which is available through the Gaia home page.
Funding
This work has made use of results from the European Space
Agency (ESA) space mission Gaia, the data from which were processed by the
Gaia Data Processing and Analysis Consortium (DPAC). Funding for the DPAC
has been provided by national institutions, in particular the institutions participating
in the Gaia Multilateral Agreement. The Gaia mission website is http:
//www.cosmos.esa.int/gaia. The authors are current or past members of the
ESA and Airbus DS Gaia mission teams and of the Gaia DPAC. This work has
financially been supported by: the Algerian Centre de Recherche en Astronomie,
Astrophysique et Géophysique of Bouzareah Observatory; the Austrian FWF
Hertha Firnberg Programme through grants T359, P20046, and P23737; the
BELgian federal Science Policy Office (BELSPO) through various PROgramme
de Développement d’Expériences scientifiques (PRODEX) grants; the BrazilFrance
exchange programmes FAPESP-COFECUB and CAPES-COFECUB;
the Chinese National Science Foundation through grant NSFC 11573054; the
Czech-Republic Ministry of Education, Youth, and Sports through grant LG
15010; the Danish Ministry of Science; the Estonian Ministry of Education
and Research through grant IUT40-1; the European Commission’s Sixth Framework
Programme through the European Leadership in Space Astrometry (ELSA)
Marie Curie Research Training Network (MRTN-CT-2006-033481), through
Marie Curie project PIOF-GA-2009-255267 (SAS-RRL), and through a Marie
Curie Transfer-of-Knowledge (ToK) fellowship (MTKD-CT-2004-014188); the
European Commission’s Seventh Framework Programme through grant FP7-
606740 (FP7-SPACE-2013-1) for the Gaia European Network for Improved data
User Services (GENIUS) and through grant 264895 for the Gaia Research for
European Astronomy Training (GREAT-ITN) network; the European Research
Council (ERC) through grant 320360 and through the European Union’s Horizon
2020 research and innovation programme through grant agreement 670519
(Mixing and Angular
History
Citation
Astronomy and Astrophysics 595, A1 (2016)
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
VoR (Version of Record)
Published in
Astronomy and Astrophysics 595
Publisher
EDP Sciences for European Southern Observatory (ESO)