Table 4
Planets in the transmission region between ice giants and gas giants.
| Planet | M P | R P | P | M ∗ | R ∗ | T eff | V | K | Transm. |
| (MJup) | (RJup) | (d) | (M⊙) | (R⊙) | (K) | signal | |||
|
|
|||||||||
| WASP-107b | 0.12 ± 0.01 | 0.94 ± 0.02 | 5.72 | 0.69 ± 0.05 | 0.66 ± 0.02 | 4430 ± 120 | 11.6 | 8.6 | 1000 |
| WASP-139b | 0.12 ± 0.02 | 0.80 ± 0.05 | 5.92 | 0.92 ± 0.10 | 0.80 ± 0.04 | 5300 ± 100 | 12.4 | 10.5 | 94 |
| HATS-7b | 0.12 ± 0.01 | 0.56 ± 0.04 | 3.19 | 0.85 ± 0.03 | 0.82 ± 0.04 | 4985 ± 50 | 13.3 | 11.0 | 21 |
| HATS-8b | 0.14 ± 0.02 | 0.87 |
3.58 | 1.06 ± 0.04 | 1.09 |
5679 ± 50 | 14.0 | 12.7 | 10 |
| Kepler-35b | 0.13 ± 0.02 | 0.73 ± 0.01 | 131.46 | 0.888 ± 0.005 | 1.028 ± 0.002 | 5606 ± 150 | 15.9 | 13.9 | 1 |
| WASP-43b† | 2.03 ± 0.05 | 1.04 ± 0.02 | 0.81 | 0.72 ± 0.03 | 0.67 ± 0.01 | 4520 ± 120 | 12.4 | 9.3 | 74 |
Notes. The data for WASP-107b are from this paper and the data for the other systems were taken from TEPCat. The transmission signal (final column) is the product of the star’s K-band flux and the area ratio of the planetary atmosphere’s annulus to the stellar disc; the transmission signal values were normalised such that the predicted signal for WASP-107b is 1000.
We included WASP-43b for comparison as its atmospheric water abundance was recently measured from a transmission spectrum (Kreidberg et al. 2014).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.