Table A.1.
Transiting sub-Neptune systems with outer giant planets (Table A.2).
| Name | Mass [ME] | Radius [RE] |
 [g cm−3] |
a [AU] | Period [days] | Mstar [M⊙] | TSM |
|---|---|---|---|---|---|---|---|
| 55-Cnc-e | 7.81 ± 0.56 | 2.08 ± 0.16 | 4.78 | 0.01543 | 0.736 | 1.015 | 354 |
| K-97b | 3.51 ± 1.9 | 1.48 ± 0.13 | 5.97 | 0.0361 | 2.586 | 0.94 | 1.2 |
| K-93b | 4.02 ± 0.68 | 1.48 ± 0.00006 | 6.83 | 0.0534 | 4.7267 | 0.91 | 3.6 |
| K-68b | 7.65 ± 1.32 | 2.31 ± 0.1 | 3.42 | 0.0617 | 5.498 | 1.079 | 25.8 |
| K-68c | 2.04 ± 1.72 | 0.958 ± 0.05 | 12.79 | 0.0906 | 9.60 | 1.079 | 0.87 |
| K-48b | 3.94 ± 2.10 | 1.88 ± 0.1 | 3.26 | 0.0532 | 4.778 | 0.88 | 11.5 |
| K-48c | 14.611 ± 2.3 | 2.71 ± 0.14 | 4.05 | 0.0851 | 9.67 | 0.88 | 7.38 |
| K-48d | 7.9 ± 4.6 | 2.04 ± 0.11 | 5.12 | 0.2298 | 42.89 | 0.88 | 3.55 |
| K-407b | < 3.2 | 1.07 ± 0.02 | 14.4 | 0.0150 | 0.6693 | 1.0 | 0.82 |
| K-94b | 10.841 ± 1.4 | 3.51 ± 0.15 | 1.38 | 0.0337 | 2.508 | 0.81 | 57 |
| π-Men-c | 4.52 ± 0.81 | 2.06 ± 0.03 | 2.85 | 0.067 | 6.268 | 1.094 | 252 |
| WASP-47e | 6.83 ± 0.66 | 1.81 ± 0.27 | 6.34 | 0.0173 | 0.789 | 1.10 | 14.2 |
| WASP-47d | 13.1 ± 1.5 | 3.576 ± 0.046 | 1.58 | 0.0886 | 9.03 | 1.10 | 25.5 |
| K-454b | 6.05 ± 1.51 | 2.4 ± 0.2 | 2.38 | 0.0954 | 10.57 | 1.028 | 19.4 |
| K-289b | 7.3 ± 6.8 | 2.15 ± 0.1 | 4.05 | 0.21 | 34.545 | 1.08 | 2.84 |
| K-289d | 4.1 ± 0.9 | 2.68 ± 0.17 | 1.17 | 0.33 | 66.06 | 1.08 | 7.94 |
| HD-86226c | 7.25 ± 1.15 | 2.16 ± 0.08 | 3.97 | 0.049 | 3.98 | 1.019 | 88.7 |
| HAT-P-11b | 23.4 ± 1.5 | 4.36 ± 0.06 | 1.59 | 0.053 | 4.88 | 0.81 | 192 |
| K-88b | 9.5 ± 1.10 | 3.44 ± 0.075 | 1.29 | 0.09 | 10.916 | 0.99 | 23.3 |
Notes. Data for the systems were taken from https://exoplanetarchive.ipac.caltech.edu. The mean density, 
, has been calculated from the mass and radius. As a reference, the Earth’s mean density is 5.51 g cm−3. Bold values indicate where the TSM is above the threshold, allowing good observational conditions.
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