Fig. 2.

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Raw (top) and activity-filtered (bottom) LBL RVs (red circles) derived from all spectral features of IRAS 04125+2902. The top plot shows the MCMC fit to the RV data, including GPR modeling of the activity (cyan full line, with dotted lines depicting the 68% confidence intervals). The bottom plot shows the activity-filtered RVs with the best fit of the planet signature (cyan full line). The rms of RV residuals is 4 m s−1.
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