Table 5
Derived planet parameters for GJ 3929 b and the planet candidate.
| Parameter | Posterior  |
Posterior  |
Units |
|---|---|---|---|
| Derived transit parameters | |||
| p = Rp∕R⋆ |  |
… | … |
| b = (ap∕R⋆)cosip |  |
… | … |
| ap∕R⋆ |  |
… | … |
| ip |  |
… | deg |
| Derived physical parameters(b) | |||
| Mp |  |
… | M⊕ |
| Mp sin i |  |
 |
M⊕ |
| Rp |  |
… | R⊕ |
| ρp |  |
… | g cm−3 |
| gp |  |
… | km s−2 |
| ap |  |
 |
au |
 |
 |
 |
K |
| S |  |
 |
S⊕ |
| ESM(d) |  |
… | … |
| TSM(d) |  |
… | … |
Notes. (a) Error bars denote the 68% posterior credibility intervals. (b)Sampled from normal distributions for stellar mass, radius, and luminosity based on the results from Sect. 3. (c) Assuming a zero Bond albedo. (d)Emission and transmission spectroscopy metrics (Kempton et al. 2018).
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