Fig. 1
RV measurements of HD 3167 taken on 2016 October 1 as function of time. Upper panel: solid black circles represent the HARPS-N data, the dashed red line indicates the Keplerian fit, and the solid green line depicts the final best fit with the RM effect. Lower panel: black solid circles are the residuals after subtracting the Keplerian, and green solid circles are the residuals after subtracting the best-fit RM model.
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