Table 1
Relevant orbital, planetary, and stellar parameters of the five planetary systems in our sample.
| a | Porb | e | Pps | ω | Rp | Mp | R* | Teff | mV | References | |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (au) | (d) | (…) | (d) | (°) | (RJ) | (MJ) | (R⊙) | (K) | (…) | ||
| HAT-P-2 b | 0.06740 | 5.6334729 | 0.5171 | 1.8927 | 185.2 | 0.951 | 8.74 | 1.54 | 6414 | 8.69 | 1, 2, 3, 4, 5 |
| HD 80606 b | 0.4603 | 111.436765 | 0.9318 | 1.7314 | 301.213 | 1.032 | 4.1641 | 0.98 | 5645 | 9.00 | 5, 6, 7, 8 |
| TOI-3362 b | 0.153 | 18.09547 | 0.815 | 1.2997 | 51 | 1.142 | 5.03 | 1.830 | 6532 | 10.86 | 5, 9 |
| TOI-4127 b | 0.3081 | 56.39879 | 0.7471 | 6.6118 | 129.6 | 1.096 | 2.30 | 1.293 | 6096 | 11.44 | 5, 10 |
| HD 17156 b | 0.1623 | 21.216398 | 0.6768 | 3.6775 | 121.71 | 1.095 | 3.191 | 1.508 | 6079 | 8.16 | 5, 11, 12 |
Notes. From left to right, these parameters are the semi-major axis, orbital period, eccentricity, planetary rotation period, argument of periastron, planetary reference radius, planetary mass, planetary surface gravity, stellar radius, stellar effective temperature and apparent V-band magnitude.
References. (1) Southworth (2010); (2) Pál et al. (2010); (3) Triaud et al. (2010); (4) Tsantaki et al. (2014); (5) Høg et al. (2000); (6) Pearson et al. (2022); (7) Moutou et al. (2009); (8) Naef et al. (2001); (9) Dong et al. (2021); (10) Gupta et al. (2023); (11) Winn et al. (2009); (12) Nutzman et al. (2011).
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