Open Access
Table C.5
Posteriors of the TOI-5624 system from the two tested dynamical scenarios.
| Configurations | 4 Planets | 5 Planets | ||
|---|---|---|---|---|
| Parameter | Prior | MAP (HDI±1σ) | Unit | |
| TOI-5624 d | ||||
| FITTED PARAMETERS | ||||
| Mp/M⋆ | U(0.30, 954.7) | ![]() |
![]() |
![]() |
| Orbital Period (P) | U(13.6, 13.8) | ![]() |
![]() |
days |
![]() |
U( ) |
![]() |
![]() |
|
![]() |
U( ) |
![]() |
![]() |
|
| Mean Longitude (λ) | U(0, 360) | ![]() |
![]() |
deg |
| DERIVED PARAMETERS | ||||
| Mass (Mp) | – | ![]() |
![]() |
M⊕ |
| Eccentricity (e) | U(0, 0.5) | ![]() |
![]() |
|
| Argument of Periastron (ω) | – | ![]() |
![]() |
deg |
| Mean Anomaly (M) | – | ![]() |
![]() |
deg |
| TOI-5624 e | ||||
| FITTED PARAMETERS | ||||
| Mp/M⋆ | U(0.30, 954.7) | ![]() |
![]() |
![]() |
| Orbital Period (P) | U(21.4, 21.6) | ![]() |
![]() |
days |
![]() |
U( ) |
![]() |
![]() |
|
![]() |
U( ) |
![]() |
![]() |
|
| Mean Longitude (λ) | U(0, 360) | ![]() |
![]() |
deg |
| DERIVED PARAMETERS | ||||
| Mass (Mp) | – | ![]() |
![]() |
M⊕ |
| Eccentricity (e) | U(0, 0.5) | ![]() |
![]() |
|
| Argument of Periastron (ω) | – | ![]() |
![]() |
deg |
| Mean Anomaly (M) | – | ![]() |
![]() |
deg |
| TOI-5624 f | ||||
| FITTED PARAMETERS | ||||
| Mp/M⋆ | U(0.30, 954.7) | ![]() |
![]() |
|
| Orbital Period (P) | U(43, 48) | ![]() |
days | |
![]() |
U( ) |
![]() |
||
![]() |
U( ) |
![]() |
||
| Mean Longitude (λ) | U(0, 360) | ![]() |
deg | |
| Inclination (i) | U(0, 180.0) | ![]() |
deg | |
| DERIVED PARAMETERS | ||||
| Mass (Mp) | – | ![]() |
M⊕ | |
| Eccentricity (e) | U(0, 0.5) | ![]() |
||
| Argument of Periastron (ω) | – | ![]() |
deg | |
| Mean Anomaly (M) | – | ![]() |
deg | |
Notes. Parameter estimates correspond to the maximum a posteriori (MAP) values, while the reported uncertainties represent the 68.3% highest density intervals (HDIs) of the marginalised posterior distributions.
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