Fig. 5
The MCMC solution for all IRa01 candidates in (b,(Rp/R ∗ )) space. Note the strong parameter degeneracy at high b. Yellow CoRoT WinIDs are the two confirmed planets CoRoT-1b and CoRoT-4b, blue objects are confirmed blends from the follow-up work presented in Moutou et al. (2009), and red sources are either unsettled cases or confirmed genuine binaries with non-planetary secondary masses from the radial velocity variations.
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