Modeled RM+CLV effects for Fe I for Night 1 and Night 2. In the top plots, we present the modeled RM+CLV effects after cross-correlation with the model of Fe I. In the middle plots, we show the cross-correlation residual plots for Night 1 and Night 2 separately in order to compare the shape of the modeled RM+CLV effects. In the bottom panels, we present the CC, after summing the in-transit data of the RM effect for K_p = 185 km s⁻¹. The feature in the RM+CLV model of Night 1 is due to a gap in the data during the observations.