Fig. C.1
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Maximum a posteriori solution for the two-planet model on the TM RVs. The top panels show the RV observations for ESPRESSO18, ESPRESSO19, and ESPRESSO21, together with the GP component of the model (in pink) as well as the full model (in black). The RV residuals are shown just below, highlighting the full residual rms. The two bottom panels show the same for the FWHM.
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