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Table 7
Expected flux ratios, eclipse depths, and equilibrium temperatures for the planets without detected eclipse candidates.
| Planet | Flux ratio [%] | Depth [h] | Teq [K] |
|
|
|||
| CoRoT-4b | 0.01–0.15 | 0.00–0.02 | 1010–1350 |
| CoRoT-5b | 0.05–0.58 | 0.01–0.11 | 1380–1850 |
| CoRoT-7b | 0.44–3.13 | 0.00–0.01 | 1720–2350 |
| CoRoT-8b | 0.00–0.14 | 0.00–0.01 | 820–1110 |
| CoRoT-9b | 0.00–0.01 | 0.00–0.00 | 390–530 |
| CoRoT-10b | 0.00–0.05 | 0.00–0.01 | 610–840 |
| CoRoT-12b | 0.07–0.78 | 0.01–0.18 | 1380–1860 |
| CoRoT-14b | 0.46–2.92 | 0.04–0.25 | 1850–2560 |
| CoRoT-16b | 0.02–0.43 | 0.00–0.04 | 1110–1610 |
| CoRoT-17b | 0.15–1.33 | 0.01–0.06 | 1550–2110 |
| CoRoT-19b | 0.15–1.13 | 0.01–0.07 | 1590–2140 |
| CoRoT-20b | 0.00–0.13 | 0.00–0.01 | 910–1240 |
| CoRoT-23b | 0.11–1.27 | 0.01–0.06 | 1500–2130 |
Notes. Shown are the 95% credible intervals for the expected θf, ΔF, and Teq when the planet is assumed to radiate as a blackbody.
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