Orbital configuration and behind-the-planet local profiles of the 6297.8013 Å Fe I line for 11 August are shown simulated with SOAPv4. Left: representation of the stellar disc in terms of velocities, along with the position of the planet as a function of the observed orbital phases. Right: simulated behind-the-planet line profiles as a function of the orbital phase. The colours on the plot correspond to the phases and positions shown on the left plot.