Table 5
Main results form the combined Bayesian analysis for the planets with detected eclipse candidates.
| Planet | B 10 | P(M1) [%] | Phase | Eccentricity | Flux ratio [%] | Depth [h] | Tbr [K] | Teq [K] |
| Previously reported planets | ||||||||
| CoRoT-1b | 7.6 ± 0.2 | 88.4 ± 0.3 | 0.495 ± 0.002 | 0.04 ± 0.03 | 0.99 ± 0.39 | 0.20 ± 0.08 | 1580–2500 | 1830–2430 |
| CoRoT-2b | 2.0 ± 0.0 | 66.1 ± 0.2 | 0.501 ± 0.002 | 0.03 ± 0.03 | 0.25 ± 0.16 | 0.07 ± 0.05 | 1430–2110 | 1460–1930 |
| Statistically significant new eclipse candidates | ||||||||
| CoRoT-6b | 10.6 ± 0.7 | 91.4 ± 0.4 | 0.533 ± 0.000 | 0.06 ± 0.01 | 1.96 ± 0.69 | 0.27 ± 0.10 | 2230–2840 | 970–1270 |
| CoRoT-11b | (5.5 ± 1.1) × 104 | 100.0 ± 0.0 | 0.558 ± 0.002 | 0.35 ± 0.03 | 3.15 ± 0.58 | 0.36 ± 0.07 | 2580–3020 | 1650–2180 |
| CoRoT-15b | 27.2 ± 2.9 | 96.5 ± 0.4 | 0.495 ± 0.001 | 0.08 ± 0.05 | 22.00 ± 6.50 | 1.37 ± 0.40 | 3470–4710 | 1580–2340 |
| Statistically marginal new eclipse candidates | ||||||||
| CoRoT-3b | 2.3 ± 0.0 | 69.7 ± 0.3 | 0.509 ± 0.001 | 0.06 ± 0.06 | 1.85 ± 1.15 | 0.08 ± 0.05 | 1940–3070 | 1610–2170 |
| CoRoT-13b | 3.3 ± 0.1 | 77.0 ± 0.5 | 0.483 ± 0.001 | 0.08 ± 0.04 | 3.04 ± 1.47 | 0.25 ± 0.12 | 2150–3080 | 1220–1610 |
| CoRoT-18b | 3.1 ± 0.1 | 75.9 ± 0.4 | 0.469 ± 0.002 | 0.10 ± 0.04 | 3.93 ± 1.67 | 0.71 ± 0.30 | 2130–3020 | 1440–1950 |
| CoRoT-21b | 1.7 ± 0.0 | 63.1 ± 0.3 | 0.474 ± 0.002 | 0.05 ± 0.02 | 5.99 ± 3.29 | 0.27 ± 0.15 | 2210–3600 | 1930–2600 |
Notes. Listed are the maximum Bayes factor B10, and the M1 posterior probability P(M1); MCMC estimates for the eclipse center phase, orbit eccentricity, flux ratio, and eclipse depth; and estimates for the brightness and equilibrium temperatures.
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