Table 5
Best-fit posterior parameters and determined planet parameters for the two planetary systems.
Parameter(a) | GJ 724 | GJ 3988 |
---|---|---|
Planetary posteriors | ||
Pb (d) | ![]() |
![]() |
t0,b (BJD) | ![]() |
![]() |
Kb (m s−1) | ![]() |
![]() |
![]() |
![]() |
0 (fixed) |
![]() |
![]() |
0 (fixed) |
Derived parameters (b) | ||
Mb sin i (M⊕) | ![]() |
![]() |
ab (au) | ![]() |
![]() |
eb | ![]() |
0 (fixed) |
ωb (deg) | ![]() |
0 (fixed) |
< Sb (S⊕)> | ![]() |
![]() |
< Teq,b (c) (K)> | ![]() |
![]() |
Teq,b (d) (K) | ![]() |
![]() |
GP posteriors | ||
PGP,rv (d) | ![]() |
![]() |
σGP, rv, CARM-VIS (m s−1) | ![]() |
![]() |
σGP, rv, HARPS (m s−1) | ![]() |
… |
σGP,rv,IRD (m s−1) | … | ![]() |
ƒGP, rv | ![]() |
![]() |
Q0,GP, rv | ![]() |
![]() |
dQGP, rv | ![]() |
![]() |
Instrumental posteriors | ||
γcarm-vis (m s−1) | ![]() |
![]() |
σCARM-VIS (m s−1) | ![]() |
![]() |
γHARPS (m s−1) | ![]() |
… |
σHARPS (m s−1) | ![]() |
… |
γIRD (m s−1) | … | ![]() |
σIRD (m s−1) | … | ![]() |
Notes. (a) Error bars denote the 68% posterior credibility intervals.(b) These derived parameters were computed using the stellar parameters that were sampled from a normal distribution centred around the values from Table 1 with the width of the uncertainty.(c) Assuming a zero Bond albedo. (d) Computed using Eq. (4) from Quirrenbach (2022).
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