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

Published online by Cambridge University Press:  01 May 2008

François Bouchy ,
Claire Moutou  and
Didier Queloz
François Bouchy
Affiliation:
Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, 98bis Bd Arago, 75014 Paris, France, email: bouchy@iap.fr
Claire Moutou
Affiliation:
Laboratoire d'Astrophysique de Marseille (UMR 6110), 38 rue Frederic Joliot-Curie, 13388 Marseille Cedex 13, France
Didier Queloz
Affiliation:
Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes, 1290 Sauverny, Switzerland
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Abstract

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Radial 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.

Information

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S253: Transiting Planets , May 2008 , pp. 129 - 139
Copyright
Copyright © International Astronomical Union 2009

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