Table 3
Parameter priors and posteriors for the spectral retrievals.
| Parameter | Prior | Posterior |
|---|---|---|
| Planetary atmosphere | ||
| Rp,1bar (RJ) |  |
 |
| Tiso (K) |  |
 |
| logPcloud∕1bar |  |
 |
| logARS |  |
 |
 |
 |
 |
 |
 |
 |
| Stellar contamination | ||
| Tspot (K) |  |
 |
| fspot (%) |  |
 |
| Tfacu (K) |  |
 |
| ffacu (%) |  |
 |
Notes. In the spectral retrieval analyses, the model assumption could be a purely planetary atmosphere, purely stellar contamination, or a combinationof the two. The table presents the posterior estimates for the model assumption in which both planetary atmosphere (with NH3 and H2O) and stellar contamination are considered, i.e., Model 17 in Table 2.
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