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Fig. B.1

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Maps of WASP-69 intrinsic CCF profiles measured in individual epochs with NIRPS (red frame), HARPS (blue frame), and HARPS-N (purple frame), plotted as a function of RV in the star rest frame (abscissa) and orbital phase (ordinate). Each map is associated with a residual map showing the difference between out-of-transit CCFs and their master or between intrinsic CCFs and their best-fit model (scaled to the level of out-of-transit residuals). Horizontal dashed green lines show transit contacts. The solid green line indicates the surface RV track associated with the best RMR fit.

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