Radial velocity time series derived from the DRS software (left columns) and SERVAL (right columns). Top panels: the best fit model to the RM is shown using the ARoME and PyAstronomy models, respectively. The red point is discarded in our analysis due to an anomalously low S/N, while the magenta points are given a lower weight in the RM fits due to being affected by a stellar flare. Lower panels: the data are the same but the fits incorporate the GP modelling. The different components of each best fit model are plotted in different colors and marked in the legend.