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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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