Master-out CCF_DI (thick magenta line) and its best fit (black line) obtained by tiling a model star with the limb-darkened master local CCF_loc, used as a proxy for the specific stellar intensity profile. The best-fit value for the projected stellar rotational velocity, which controls the spectral position of this profile over the model stellar disk, is in good agreement with its measured spectroscopic value and yields a good fit to the observed master-out CCF_DI.