Table A.2
Orbital parameters of the planetary candidates using a simple MCMC analysis to fit Keplerian orbits to the RV data.
| Parameters | YBP401 | YBP1194 | YBP1514 |
|
|
|||
| P [days] | 4.0873 |
6.959 |
5.1189 |
| T [JD] | 2 455 974.23 |
2455290.0 |
245986.34 |
| e | 0.141 |
0.294 |
0.332 |
| ω [deg] | –31.69 |
99.14 |
–34.76 |
|
–0.197 |
0.535 |
–0.329 |
|
0.319 |
–0.086 |
0.474 |
| K [ m s-1] | 48.911 |
35.607 |
50.97 |
| msini [MJup] | 0.41 |
0.32 |
0.42 |
| γ [ km s-1] | 33.172 |
34.185 |
34.058 |
Notes. We considered as free parameters the orbital period P, the time of transit Tc, the radial velocity semi-amplitude K, the centre-of-mass velocity γ, and the orthogonal quantities and , where e is the eccentricity and ω is the argument of periastron. We quote the mode of the resulting parameter distributions as the final value and the 68.3% interval with equal probability density at the ± 1σ bound to derive the uncertainty. T: time at periastron passage, K: semi-amplitude of the RV curve, msini: planetary minimum mass.
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