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Additional auxiliary data for the GAIA-RVS

hal.structure.identifierGalaxies, Etoiles, Physique, Instrumentation [GEPI]
dc.contributor.authorCRIFO, F.,
hal.structure.identifierM2A 2014
dc.contributor.authorCHEMIN, L.
hal.structure.identifierLaboratoire Univers et Particules de Montpellier [LUPM]
dc.contributor.authorJASNIEWICZ, Gérard
dc.contributor.authorKATZ, D.,
hal.structure.identifierProbabilités, statistique, physique mathématique [PSPM]
dc.contributor.authorMARCHAL, O.,
dc.contributor.authorSARTORETTI, P.,
hal.structure.identifierM2A 2014
dc.contributor.authorSOUBIRAN, C.
dc.contributor.authorTHÉVENIN, F.,
dc.contributor.authorZWITTER, T.,
dc.date.issued2014-12
dc.date.conference2014-06-03
dc.description.abstractEnThe Gaia-RVS will measure some 10^8 stellar radial velocities using the correlation method with well-adapted template spectra for each individual case. Ground-based RV standards will be used to fix the zero-point. Gaia instruments are ``self-calibrating'' and no calibration device is available on board. But for the beginning of the mission, until the needed calibration parameters become available, the calibrations have to come from external sources, i.e. existing ground-based observations of already very well-known objects. Therefore beside the basic list of 1400 very stable and well-measured primary standards, several secondary RV lists have been built recently. The basic list itself will be extended with around 500 new "primary standard". The libraries of existing spectra have been carefully investigated: a lot of high-quality material is available for the start of the reductions and for the validation of the pipeline results. In addition, as the data expected from the photometric instrument are not available at the beginning, very large lists with atmospheric parameters (Teff, log g, metallicity) have been produced from the literature. Grids of 3D atmospheric models have been calculated, in order to select the best template for the correlation; they will be used in the future and will automatically take into account the stellar convective shift across the HR diagram.
dc.language.isoen
dc.subject.enStars: fundamental parameters
dc.subject.enTechniques: radial velocities
dc.subject.enSurveys: Gaia.
dc.title.enAdditional auxiliary data for the GAIA-RVS
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.page417 - 420
bordeaux.conference.titleSF2A-2014: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: J. Ballet, F. Martins, F. Bournaud, R. Monier, C. Reylé, pp.417-420, held in Paris 03-06- june 2014
bordeaux.countryFR
bordeaux.conference.cityParis
bordeaux.peerReviewedoui
hal.identifierhal-01095829
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01095829v1
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