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Fig. A.1


Marginalized and joint posterior probability density functions of the model parameters from the RV analysis. The adopted RV model includes a trained GP activity model ({ln a, lnλ, lnΓ, lnPGP, s}) plus the star’s systemic velocity ({γ0}) and three Keplerian planet solutions ({Pi, T0,i, Ki, hi, ki} for i = b, c, d).

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