Radial velocity follow-up for confirmation and characterization of transiting exoplanets

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dc.creatorBouchy, F.
dc.creatorMoutou, C.
dc.creatorQueloz, D.
dc.creatorTeam, the CoRoT Exoplanet Science
dc.date2009-02-20
dc.date.accessioned2026-07-07T12:44:58Z
dc.date.available2026-07-07T12:44:58Z
dc.descriptionRadial Velocity follow-up is essential to establish or exclude the planetary nature of a transiting companion as well as to accurately determine its mass. Here we present some elements of an efficient Doppler follow-up strategy, based on high-resolution spectroscopy, devoted to the characterization of transiting candidates. Some aspects and results of the radial velocity follow-up of the CoRoT space mission are presented in order to illustrate the strategy used to deal with the zoo of transiting candidates.
dc.description10 pages, proceedings IAU symposium 253, Boston, May 2008
dc.identifierhttps://arxiv.org/abs/0902.3520
dc.identifierhttp://arxiv.org/abs/0902.3520
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/220954
dc.subjectEarth and Planetary Astrophysics
dc.titleRadial velocity follow-up for confirmation and characterization of transiting exoplanets
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