Top left panel: V_sys-K_p map for for the single-species Fe model with a VMR of 0.01 and a cloud top pressure of 10^−1∙5 bar for all post-eclipse data containing a significant false-positive signal. The red crosshairs indicate the expected location of the planetary signal. The remaining three panels show the corresponding maps for each of the observing nights individually. There is no map for night 3 as no posteclipse data were taken.