Radial Velocity Follow-up for Confirmation and Characterization of Transiting Exoplanets

Details Radial Velocity Follow-up for Confirmation and Characterization of Transiting Exoplanets Radial Velocity Follow-up for Confirmation and Characterization of Transiting Exoplanets

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..366..193b&link_type=abstract

Transiting Extrapolar Planets Workshop ASP Conference Series, Vol. 366, Proceedings of the conference held 25-28 September, 2006

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Radial Velocity follow-up is essential to confirm or exclude the planetary nature of a transiting companion as well as to determine its accurate mass. We present here some elements of an efficient Doppler follow-up strategy based on high-resolution spectroscopy devoted to the characterization of transiting candidates. Some Doppler facilities involved in the follow-up of ground-based and space-based photometric surveys are presented. Performances of the mass characterization of earth-like transiting exoplanets are discussed.

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