Table 4
Currently known most suitable observational targets for the observational and data analysis method presented in this paper.
| Exoplanet | Rplanet | Rstar | 2MASS KS |
|
|
|||
| Hot-Jupiters | |||
| HD 209458 b | 1.4 RJup | 1.2 R⊙ | 6.3 |
| HD 189733 b | 1.1 RJup | 0.76 R⊙ | 5.5 |
| HD 80606 b | 1.0 RJup | 1.0 R⊙ | 7.3 |
| WASP-80 b | 0.95 RJup | 0.57 R⊙ | 8.4 |
| Hot-Neptunes | |||
| HAT-P-26 b | 1.6 RNep | 0.79 R⊙ | 9.6 |
| HAT-P-11 b | 1.2 RNep | 0.75 R⊙ | 7.0 |
| GJ 436 b | 1.1 RNep | 0.46 R⊙ | 6.1 |
| GJ 3470 b | 1.1 RNep | 0.50 R⊙ | 8.0 |
| Super-Earths | |||
| GJ 1214 b | 2.6 R⊕ | 0.21 R⊙ | 8.8 |
| Kepler-49 b | 2.7 R⊕ | 0.53 R⊙ | 12.4 |
| Kepler-125 b | 2.3 R⊕ | 0.51 R⊙ | 11.7 |
| HD 97658 b | 2.3 R⊕ | 0.70 R⊙ | 5.7 |
| 55 cnc e | 2.0 R⊕ | 0.94 R⊙ | 4.0 |
| Earth-size planets | |||
| Kepler-205 c | 1.6 R⊕ | 0.55 R⊙ | 10.8 |
| Kepler-186 d | 1.4 R⊕ | 0.47 R⊙ | 11.6 |
| Kepler-42 b | 0.76 R⊕ | 0.17 R⊙ | 11.5 |
| Kepler-42 c | 0.71 R⊕ | 0.17 R⊙ | 11.5 |
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