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Table 5

G 264–012: priors, best likelihoods, and posterior distribution uncertainties of the combined planets plus activity fit to RVs and derived planetary parameters.

Parameter Prior Posterior Unit
Planets
Pb d
       
Kb m s−1
       
tc,b − 2 458 000 d
       
Pc d
       
Kc m s−1
       
tc,c − 2 458 000 d
       
GP kernel hyperparameters
h m s−1
       
P d
       
λ d
       
w
Instruments
σ m s−1
       
μ m s−1
Derived
ab au
       
Mb sini M
       
Sb S
       
Teq,b K
ac au
       
Mc sini M
       
Sc S
Teq,c K

Notes. , and , with and σRV, as the average and the rms of the RV time series, respectively.

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