The left panel shows the apparent radial velocities of HD 3167 b spanning five separate transits (colored points) and the best-fit consensus model including the RM effect (black curves). The right panel shows the residuals after subtracting the best-fit model. Arbitrary vertical offsets were applied to separate data from different nights. The lowermost dataset was analyzed by V. Bourrier et al. (2021). The uppermost is a composite of all the data, including phase-binned points for display purposes. The gray region is the transit interval.