Fig. 8
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Stellar surface RVs of the regions occulted by GJ 436b in ESPRESSO visits 1 (blue) and 2 (red), HARPS Visit A (magenta), and HARPS-N visits B (orange) and C (green) derived from the fits to individual exposures (same details as Fig. 4). The solid black curve is the best-fit model derived from the joint Revolutions fit to all visits.
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