Table 1
Results of our PTMCMC fitting procedure to the combined Kepler and Hubble data.
| TK18b HST photometry | Our HST photometry | |
|---|---|---|
| rs (%) |  |
 |
| aps (R⋆) |  |
 |
| Ps (d) |  |
 |
| φ (rad) |  |
 |
| fM (%) |  |
 |
| is (rad) |  |
 |
| Ωs (rad) |  |
 |
Notes. The Hubble data was either based on the photometry extracted by Teachey & Kipping (2018, TK18b; central column) or based on our own extraction (right column). Figure 4 illustrates quite clearly that the posterior distributions are not normally distributed and often not even representative of skewed normal distributions. The confidence intervals stated in this table have thus to be taken with care.
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