Fig. B.4
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Planetary candidate in the GJ 548A system. a) GLS periodogram of the RV time-series after subtracting the Base Model. The vertical blue dashed line marks the orbital period of the candidate. b) Phase-folded for the RV curve of the planetary candidate. The red solid line represents the best-fit Keplerian model, while the red circles indicates the binned RVs with the corresponding rms.
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