Fig. C.5
Auto-correlation of the TiO model spectrum (left panel) and cross-correlation between the Fe model spectrum and a rotationally broadened version of itself (vrot = 7 km s−1; right panel). For comparison, we plot the observed CCFs from the CARMENES observations in gray lines. The auto-correlation of the TiO model spectrum has a width of 5.4 km s−1. This is close to the FWHM value of the observed CCF (4.0 ± 0.7 km s−1). Also the FWHM of the cross-correlation with the broadened Fe model spectrum is close to the value of the observed CCF (10.5 km s−1 and 8.6 ± 1.0 km s−1, respectively).
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