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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
Affiliation:
Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, 98bis Bd Arago, 75014 Paris, France, email: [email protected]
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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Aigrain, S., CollierCameron, A. Cameron, A., Ollivier, M., et al. , 2008, A&A, in press (arXiv:0807.3767)Google Scholar
Alonso, R., Brown, T. M., Torres, G., et al. , 2004, ApJ, 613, L153CrossRefGoogle Scholar
Alonso, R., Auvergne, M., Baglin, A., Ollivier, M., Moutou, C., et al. , 2008, A&A, 482, L21Google Scholar
Baglin, A., 2003, Advances in Space Research, Vol 31, Issue 2, 345.CrossRefGoogle Scholar
Barge, P., Baglin, A., Auvergne, M., Rauer, H., Leger, A., et al. , A&A, 482, L17CrossRefGoogle Scholar
Bakos, G., Noyes, R. W., Kovcs, G., et al. , 2004, PASP, 116, 266Google Scholar
Bouchy, F., Pont, F., Melo, C., et al. , 2005, A&A, 431, 1105Google Scholar
Bouchy, F., Queloz, D., Deleuil, M., Loeillet, B., Hatzes, A. P., et al. , 2008, A&A, 482, L25Google Scholar
Brown, T., 2003, ApJ 593, 125CrossRefGoogle Scholar
Deleuil, M., Deeg, H., Alonso, R., Bouchy, F., Rouan, D., et al. , 2008, A&A, in pressGoogle Scholar
McCullough, P. R., Stys, J. E., Valenti, J. A., et al. , 2006, ApJ, 648, 1228CrossRefGoogle Scholar
Moutou, C., Bruntt, H., Guillot, T., et al. , 2008, A&A, in press (arXiv:0807.3739)Google Scholar
Pollacco, D. L., Skillen, I., Cameron, A. C., et al. , 2006, PASP, 118, 1407Google Scholar
Pont, F., Melo, C., Bouchy, F., et al. , 2005, A&A, 433, L21Google Scholar
Pont, F., Zucker, S., Queloz, D., 2006, MNRAS, 373, 231Google Scholar
Santos, N. C., Mayor, M., Naef, D., et al. , 2002, A&A, 392, 215Google Scholar
Udalski, A., Paczynski, B., Zebrun, K., et al. , 2002, Acta Astronomica, 52, 1Google Scholar