Radial Velocity Standard Stars for the Gaia RVS

Gérard Jasniewicz (1) , F. Crifo (2) , C. Soubiran (3, 4, 5, 6) , D. Hestroffer (7) , A. Siebert (8) , L. Veltz (9) , Lionel Bigot (10) , L. Chemin (3, 4, 5, 6) , P. David (11) , A. Guerrier (12) , D. Katz (2, 13) , H.-G. Ludwig (14) , Patrick Richard (12) , F. Royer (15) , P. Sartoretti (2) , S. Udry (16)

1 GRAAL - Groupe de Recherche en Astronomie et Astrophysique du Languedoc
2 GEPI - Galaxies, Etoiles, Physique, Instrumentation
3 OASU - Observatoire aquitain des sciences de l'univers
4 LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac]
5 UB - Université Sciences et Technologies - Bordeaux 1
6 L3AB - Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux
7 IMCCE - Institut de Mécanique Céleste et de Calcul des Ephémérides
8 ObAS - Observatoire astronomique de Strasbourg
9 AIP - Astrophysikalisches Institut Potsdam
10 PhLAM - Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523
11 LPNHE - Laboratoire de Physique Nucléaire et de Hautes Énergies
12 CNES - Centre National d'Études Spatiales [Toulouse]
13 OP - Observatoire de Paris - Site de Paris
14 ZAH - Zentrum für Astronomie der Universität Heidelberg
15 LT2C - Laboratoire Telecom Claude Chappe
16 ObsGE - Observatoire Astronomique de l'Université de Genève

The calibration of the Radial Velocity Zero-Point (RVZP) of the Radial Velocity Spectrometer (RVS) will be performed with the help of Radial Velocity (RV) standard stars and asteroids. A full-sky list of RV standard stars candidates has been built for this purpose within the Development Unit (DU) 640 of the Gaia DPAC Consortium. A ground-based campaign of RV observations has been initiated to eliminate unsuitable candidates. Simulations have also been performed in order to estimate in advance the number of RV standard stars and asteroids crossing the RVS field of view. These standard stars and asteroids will also be very helpful for controlling any harmful effect (especially the CCD radiation damage) on calibration and RVZP during the lifetime of the Gaia project. Kinematic RV are expected to be published at the end of the project for the brightest stars, taking into account gravitational redshift and convective shifts for the lines present in the RVS spectral wavelength range.

Domaines: Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]; Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]

Gérard Jasniewicz, F. Crifo, C. Soubiran, D. Hestroffer, A. Siebert, et al.. Radial Velocity Standard Stars for the Gaia RVS. GAIA: At the Frontiers of Astrometry, 2010, ., France. pp.195-200, ⟨10.1051/EAS/1045033⟩. ⟨hal-00572360⟩