Fig. C.1

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Visualisation of the CCF residuals profiles obtained before (top panel) and after (bottom panel) the decorrelation by the S-index for HD4628. The colour code is the Z-normalised S-index vector (in arbitrary units). The stellar activity signature, initially visible in the top panel by the blue-to-green colour gradient at the line centre (v = 0 km s−1), is removed, whereas the clear instrumental defocus is preserved. The instrumental time-domain vectors can be extracted after performing a PCA decomposition of those profiles (see Fig. C.2).
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