Fig. 2

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Two-dimensional cross-correlation function of H I, Li I, Na I, Mg I, K I, Ca I, Ti I, V I, Cr I, Mn I, Fe I, Fe II, Co I, Ni I, Ba II, Sr I and Sr II for ingress and egress combined in Kp − Vsys space. The last panel shows the cross-correlation function for the entire atmospheric model – including all species – at 2500 K. We highlight the different scales on the colour maps for the deviation from the mean in terms of standard deviations away from the planetary trace, denoted as σ.
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