Could we identify hot ocean-planets with CoRoT, Kepler and Doppler velocimetry?
Franck Selsis(Centre National de la Recherche Scientifique), A. Léger(Université Paris-Saclay), P. Bordé(Institut d'Astrophysique Spatiale), Bruno Chazelas, Frank Brachet(Centre National de la Recherche Scientifique), C. Moutou(Laboratoire d’Astrophysique de Marseille), M. Decaudin(Université Paris-Sud), Dimitri Mawet(European Southern Observatory), D. Despois(Centre National de la Recherche Scientifique), M. Ollivier, J.–M. Grießmeier(Université d'Orléans), M. Deleuil(Centre National de la Recherche Scientifique), James F. Kasting(Pennsylvania State University), D. Ehrenreich(University of Geneva), O. Grasset, H. Lammer(Austrian Academy of Sciences), P. Barge, C. Sotin, F. Bouchy
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