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Cambridge University Press, Proceedings of the International Astronomical Union, S276(6), p. 549-550, 2010

DOI: 10.1017/s174392131102117x

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Resolving blended radial velocities

Journal article published in 2010 by Alexandre Santerne ORCID, Claire Moutou, François Bouchy
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

AbstractIn space, photometric surveys are very efficient to detect small transiting planets or stars which are contaminated by blended eclipsing binaries. We present some simulations compared to radial velocity (RV) observations obtained with the SOPHIE spectrograph (OHP, France) in order to determine the true nature of a brown dwarf candidate revealed by CoRoT: a background eclipsing binary diluted by a foreground star.