Fig. 2
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Radial-velocity measurements of K2-110. Top panel: radial velocities as a function of time, showing no long-term trends. The blue and light blue points display the measurements obtained with the HARPS-N and HARPS spectrographs, respectively, and the black line indicates the Keplerian best-fit model. Bottom panel: same radial velocities as in the top panel, but phase folded at the ephemeris of K2-110b (P = 13.86 d).
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