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- W2109005107 abstract "Abstract We used the method of Silva & Cruz (2006), which distinguishes between planetary and stellar companions by fitting transit light curves, to select the most promising CoRoT candidates to be monitored with radial-velocity measurements. Testing this method on the light curves of confirmed CoRoT exoplanetary systems shows that the estimated radius for such planets is smaller than 2 R Jup , while for most of the light curves in which no planet has been detected, the secondary companion has an estimated radius larger than 2 R Jup . We present preliminary results concerning other light curves for which no planet has been detected yet." @default.
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- W2109005107 date "2009-11-01" @default.
- W2109005107 modified "2023-09-25" @default.
- W2109005107 title "Selection of most promising CoRoT candidates for radial-velocity follow-up" @default.
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- W2109005107 doi "https://doi.org/10.1017/s1743921310010975" @default.
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