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Fig. 2


Top panel: Phased-folded radial velocities of K2-132 obtained with HARPS (red dots), FEROS (gray dots), and Keck/HIRES (blue dots). The red line corresponds to the Keplerian model using the posterior parameters of the MCMC analysis of Sect. 3.5. Bottom panel: Residuals for the observed radial velocities. The small blue band around zero has a width equal to the fitted jitter term of 5.1 m s−1.

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