Open Access
Table A.8
Inferred system parameters with the photodynamical modelling with three planets.
Parameter | Median and 68.3% CI | |
---|---|---|
Star | ||
Mass, M* | (M0) | 0.976 ± 0.053 |
Radius, R* | ![]() |
0.918 ± 0.017 |
Stellar mean density, ρ* | [g cm−3] | 1.79 ± 0.13 |
Planet b | ||
Semi-major axis, a | [au] | 0.0828 ± 0.0015 |
Eccentricity, e | ![]() |
|
Argument of pericentre, ω | ![]() |
|
Inclination, i | 88.87 ± 0.21 | |
Longitude of the ascending node, Ω | [º] | 180 (fixed at tref) |
Mean anomaly, M0 | [º] | ![]() |
Impact parameter, b | 0.323 ± 0.064 | |
T′0 − 2 450 000 | [BJDtdb] | 7957.48176 ± 0.00025 |
P′ | [d] | 8.80358 ± 0.00018 |
K′ | [ms−1] | 29.1 ± 1.9 |
Mass, Mp | (MJ) | ![]() |
Radius, Rp | ![]() |
0.765 ± 0.016 |
Planet mean density, ρp | [g cm−3] | 0.788 ± 0.071 |
Planet c | ||
Semi-major axis, a | [au] | 0.2059 ± 0.0037 |
Eccentricity, e | ![]() |
|
Argument of pericentre, ω | [°] | 25.4 ± 5.6 |
Inclination, i | [°] | ![]() |
Longitude of the ascending node, Ω | [°] | ![]() |
Mean anomaly, M0 | [°] | 259.0 ± 3.8 |
Impact parameter, b | ![]() |
|
T′0 − 2 450 000 | [BJDtdb] | 7971 56 ± 0 31 |
P′ | [d] | 34 5441 ± 0 0026 |
K′ | [ms−1] | ![]() |
Mass, Mp | (MJ) | ![]() |
Planet (d) | ||
Semi-major axis, a | [au] | ![]() |
Eccentricity, e | ![]() |
|
Argument of pericentre, ω | [°] | 148 ± 96 |
Inclination, i | [°] | ![]() |
Longitude of the ascending node, Ω | [°] | ![]() |
Mean anomaly, M0 | [°] | ![]() |
Impact parameter, b | ![]() |
|
T′0 − 2 450 000 | [BJDtdb] | ![]() |
P′ | [d] | ![]() |
K′ | [ms−1] | 8.9 ± 2.2 |
Mass, Mp | (MJ) | ![]() |
Mutual inclination b, c, lb‚c | [°] | 21 ± 12 |
Mutual inclination b, d, lb‚d | [°] | 93 ± 46 |
Mutual inclination c, d, lc‚d | [°] | 95 ± 43 |
Notes. The table lists: Posterior median and 68.3% CI for the photody-namical modelling with three planets (Section 7.8). The orbital parameters are given for the reference time tref = 2 457 957 48167 BJDtdb.
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