Fig. A.1
MCMC posterior distribution of the CARMENES VIS RVs for G264-012 for a model including two circular planetary orbits (parameters Kb, Pb, Tc,b, Kc, Pc, and Tc,c), a Gaussian Process using the george-code and a quasi-periodic kernel (hyper-parameters h, w, P, and λ), offset μ and additional jitter σ. Only solutions with 
are shown.
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