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Fig. 2

image

RV measurement of HD 3167 taken on 2017 November 23 as a function of time. Upper panel: solid black circles represent the HARPS-N data, the dashed red line indicates the Keplerian fit, and the green line is the over plotted best-fit RM model from the 2016 transit. The blue dotted line marks the transit ingress and egress of planet b. The expected RM amplitude due to the transit of planet b is 0.6 m s−1. Lower panel: residuals after the best-fit RM is subtracted.

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