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Table 3
Kepler planet frequency f(R,P), CoRoT detection ξCoRoT(R,P) rate, and number of expected CoRoT Neptunes nCoRoT [2−4 R⊕] for each cell of Rp and P as in Fig. 4 of Howard et al. (2012).
| Planetary radius | Orbital period | f(R,P) | ξCoRoT(R,P) | n CoRoT [2−4 R⊕] |
| [R⊕] | [days] | [%] | [%] | |
|
|
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| 2.0–2.8 | 1.2–2.0 | 0.037 ± 0.021 | 44 ± 6 | 0.45 ± 0.31 |
| 2.0–2.8 | 2.0–3.4 | 0.11 ± 0.04 | 28 ± 4 | 0.61 ± 0.31 |
| 2.8–4.0 | 2.0–3.4 | 0.035 ± 0.020 | 71 ± 3 | 0.49 ± 0.33 |
| 2.0–2.8 | 3.4–5.9 | 0.51 ± 0.11 | 19 ± 1 | 1.31 ± 0.50 |
| 2.8–4.0 | 3.4–5.9 | 0.18 ± 0.06 | 60 ± 2 | 1.48 ± 0.68 |
| 2.0–2.8 | 5.9–10.0 | 1.0 ± 0.2 | 14 ± 1 | 1.34 ± 0.50 |
| 2.8–4.0 | 5.9–10.0 | 0.62 ± 0.13 | 44 ± 2 | 2.62 ± 0.98 |
| 2.0–2.8 | 10.0–17.0 | 1.9 ± 0.3 | 7 ± 1 | 0.85 ± 0.30 |
| 2.8–4.0 | 10.0–17.0 | 1.1 ± 0.2 | 31 ± 1 | 2.43 ± 0.83 |
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