Upper panel: error-weighted average of Runs 2012 and 2013 RV measurements (black points), following the subtraction of the systemic velocities and assuming no reflex stellar motion (K = 0 km s^-1). The RM adjustment with and vsini_⋆ = 123.5 ± 22.5 km s^-1 is overplotted with a red line. Keplerian residuals are first calculated in each run and then grouped in common phase bins. We excluded the two anomalous RV measurements in dataset 2013 (Fig. 2). Lower panel: residuals from the Keplerian + RM fit, without binning. Green points correspond to Run 2012, orange points to Run 2013.