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Table 3

Adopted priors and results of the Markov chain Monte Carlo orbital fits.

Parameter Priors 1 planet 2 planets 2 planets + year-long signal
(adopted solution)
Kb (m s−1)
         
Pb (d) 1628 ± 12 1631 ± 13
         
         
         
T0,b (BJD-2450000)
         
eb Derived 0.10 ± 0.06
         
ωb (deg) Derived
         
Mb sin i (MJup) Derived 0.63 ± 0.05 0.63 ± 0.05
         
ab (au) Derived 2.35 ± 0.04 2.36 ± 0.04 2.36 ± 0.04

Kc (m s−1)
         
Pc (d)
         
T0,c (BJD-2 450 000)
         
         
         
ec Derived
         
ωc (deg) Derived
         
Mc sin i (M) Derived
         
ac (au) Derived 0.30 ± 0.01 0.30 ± 0.01

Kyr (m s−1)
         
Pyr (d)
         
T0,yr (BJD-2450000)

γHARPS (m s−1) 3.96 ± 0.62
         
γHARPS-N (m s−1)
         
JitterHARPS (m s−1)
         
JitterHARPS-N (m s−1)

Residuals rms (m s −1) 4.00 3.56 3.01
         
Maximum −199.39 −180.18 −167.35
         
BIC 440.83 425.78 414.13

Notes. The listed best fit values and uncertainties are the medians and 16th–84th percentiles of the posterior distributions, respectively.

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