Table 3
Input physical and orbital parameters of the planets.
| Planets | Mp (MJ) | Rp (RJ) | Teq (K) | T0 (BJDTDB) (a) | P (day) | a/Rs | i (deg) | Ref. |
|---|---|---|---|---|---|---|---|---|
| CoRoT-1b | 1.03 ± 0.12 | 1.49 ± 0.08 | 1898 ± 50 | 4159.4532 | 1.5089557 | 4.92 ± 0.08 | 85.1 ± 0.5 | [1] |
| HAT-P-18b | 0.197 ± 0.013 | 0.995 ± 0.052 | 852 ± 28 | 4715.02174 | 5.508023 | 16.04 ± 0.75 | 88.8 ± 0.3 | [2] |
| HAT-P-57b | 1.41 ± 1.52 | 1.74 ± 0.36 | 1855 ± 40 (b) | 5113.48127 | 2.465300 | 5.82 ± 0.09 | 88.26 ± 0.85 | [3] |
| Qatar-1b | 1.294 ± 0.050 | 1.143 ± 0.026 | 1418 ± 28 | 6234.10322 | 1.42002420 | 6.25 ± 0.07 | 84.08 ± 0.16 | [4] |
| TrES-4b | 0.78± 0.19 | 1.61 ± 0.18 | 1785 ± 40 (b) | 4230.90530 | 3.553950 | 6.04 ± 0.23 | 82.81 ± 0.33 | [3] |
| WASP-2b | 0.880 ± 0.038 | 1.063 ± 0.028 | 1286±17 | 3991.51455 | 2.15222144 | 8.08 ± 0.12 | 84.81 ± 0.17 | [5] |
| WASP-10b | 3.15 ± 0.12 | 1.080 ± 0.020 | 1370 ± 50 | 4664.03091 | 3.0927616 | 11.65 ± 0.11 | 88.49 ± 0.20 | [6] |
| WASP-32b | 3.60 ± 0.07 | 1.18 ± 0.07 | 1560 ± 50 | 5151.0546 | 2.718659 | 7.8 ± 0.3 | 85.3 ± 0.5 | [7] |
| WASP-36b | 2.361 ± 0.070 | 1.327 ± 0.021 | 1733±19 | 5569.83771 | 1.53736596 | 5.85 ± 0.06 | 83.15 ± 0.13 | [8] |
| WASP-39b | 0.281 ± 0.032 | 1.279 ± 0.040 | 1166±14 | 5342.96913 | 4.0552941 | 11.07 ± 0.17 | 87.32 ± 0.17 | [9] |
| WASP-49b | 0.396 ± 0.026 | 1.198 ± 0.046 | 1399 ± 41 | 6267.68389 | 2.7817362 | 8.01 ± 0.20 | 84.48 ± 0.13 | [10] |
| WASP-156b | 0.128 ± 0.010 | 0.51 ± 0.02 | 970 ± 25 | 4677.707 | 3.836169 | 12.8 ± 0.5 | 89.1 ± 0.8 | [11] |
Notes. (a)Initial transit epochs subtracting 2 450 000. (b)Black-body equilibrium temperature calculated with the input stellar effective temperature and normalized semimajor axis (Teq = Teff (Rs/2a)1/2 [ƒ(1 – AB)]1/4, Charbonneau et al. 2005) assuming a Bond albedo of 0 and uniform heat redistribution (ƒ = 1).
References. [1] Barge et al. (2008) [2] Hartman et al. (2011) [3] Stassun et al. (2017) [4] Collins et al. (2017) [5] Southworth (2012) [6] Johnson et al. (2009) [7] Maxted et al. (2010) [8] Mancini et al. (2016) [9] Mancini et al. (2018) [10] Lendl et al. (2016) [11] Demangeon et al. (2018).
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