Table 6
Derived planetary parameters for TOI-1685 b and TOI-1685 [c].
| Parameter(a) | TOI-1685 b |
|---|---|
| Planet parameters | |
| Pb (d) |  |
| t0,b (BJD) |  |
| ab∕R⋆ |  |
| p = Rb∕R⋆ |  |
| b = (ab∕R⋆)cos ib |  |
| ib (deg) |  |
| r1 |  |
| r2 |  |
| Kb (m s−1) |  |
| Derived physical parameters | |
| Mb (M⊕) |  |
| Rb (R⊕) |  |
| ρb (g cm−3) |  |
| gb (m s−2) |  |
| Teq,b (K)(b) |  |
| Sb (S⊕) |  |
| Parameter(b) | TOI-1685 [c](c) |
| Pc (d) |  |
| t0,c (BJD) |  |
| ac∕R⋆ |  |
| Kc (m s−1) |  |
| Teq,c (K)(c) |  |
| Sc (S⊕) |  |
| Mcsini (M⊕) |  |
Notes. (a) Parameters obtained with the posterior values from Table 5. (b) Parameters obtained with the posterior values of the 2cp+GP model fit. (c)We use square brackets to denote the tentative second planet as there is no agreed-upon nomenclature for unconfirmed planet candidates. It is understood that the values tabulated here have been computed under the assumption that the RV signal is indeed of a planetary origin. Error bars denote the 68% posterior credibility intervals. (c) The equilibrium temperature was calculated assuming zero Bond albedo.
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