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Fig. A.4
Posterior distributions from the MCMC analysis on LSPM J2116+0234 b. Plotted are the planetary parameters, instrumentaloffsets (γVIS, γNIR), GP hyper-parameters (KQP, λQP, wQP, PQP), and additional data jitters (σJit, VIS, σJit, NIR). The vertical dashed lines indicate the mean and 1σ uncertainties of the fitted parameters.
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