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Table 1
Assumed parameters of the planetary systems used for the simulations throughout this paper.
| Planet | R* | T* | Distance | Rp | Tp | log(g) | Separation | Planet υsin(i) |
|---|---|---|---|---|---|---|---|---|
| β Pic b | 1.80 R⊙ | 8100 K | 19.4 pc | 1.36 Rjup | 1700 K | 4.0 | 0.30″ | 25 km s−1 |
| HR8799 e | 1.34 R⊙ | 7400 K | 40.88 pc | 1.12 Rjup | l200 K | 4.0 | 0.40″ | 15 km s−1 |
| 51 Eri b | 1.45 R⊙ | 7200 K | 29.4 pc | 1.10 Rjup | 700 K | 4.0 | 0.45″ | 10 km s−1 |
References. β Pic b: Bonnefoy et al. (2013), Snellen et al. (2014); HR8799e: Gravity Collaboration et al. (2019); Mollière et al. (2020); Wang et al. (2021); and 51 Eri b: Samland et al. (2017); Rajan et al. (2017).
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