Table C.1
Same derived posterior table as Table 5 but assuming the second signal to be of planetary origin.
| Parameter | Posterior(a) | Unit | |
|---|---|---|---|
| b | [c](b) | ||
| Pp |  |
 |
d |
| t0,p (BJD) |  |
 |
d |
| r1,p |  |
… | … |
| r2,p |  |
… | … |
| Kp |  |
 |
m s−1 |
| ep | 0.0 (fixed) | 0.0 (fixed) | … |
| ωp | 90.0 (fixed) | 90.0 (fixed) | … |
| p = Rp∕R⋆ |  |
… | … |
| b = (ap∕R⋆)cosip |  |
… | … |
| ap∕R⋆ |  |
… | … |
| ip |  |
… | deg |
 |
 |
… | h |
| Mp |  |
 |
M⊕ |
| Rp |  |
… | R⊕ |
| ρp |  |
… | g cm−3 |
| gp |  |
… | m s−2 |
| ap |  |
 |
|
 |
 |
 |
K |
 |
 |
 |
S⊕ |
Notes. (a)Parameters obtained with the posterior values from Table B.3. Error bars denote the 68 % posterior credibility intervals. (b)The square brackets denote the assumption that the long-term signal is of planetary origin. (c)Transit duration from first contact to fourth contact. (d)Equilibrium temperature calculated assuming zero Bond albedo. (e)Insolation.
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