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We aim to identify and characterize secondary eclipses in the original lightcurves of all published CoRoT planets using uniform detection and evaluationcritetia. Our analysis is based on a Bayesian model selection between twocompeting models: one with and one without an eclipse signal. The search iscarried out by mapping the Bayes factor in favor of the eclipse model as afunction of the eclipse center time, after which the characterization ofplausible eclipse candidates is done by estimating the posterior distributionsof the eclipse model parameters using Markov Chain Monte Carlo.  We discover statistically significant eclipse events for two planets,CoRoT-6b and CoRoT-11b, and for one brown dwarf, CoRoT-15b. We also findmarginally significant eclipse events passing our plausibility criteria forCoRoT-3b, 13b, 18b, and 21b. The previously published CoRoT-1b and CoRoT-2beclipses are also confirmed.

Secondary eclipses in the CoRoT light curves: A homogeneous search based on Bayesian model selection