Fig. 6
Examples of cross-correlation functions of the best fit masks for three of the FEROS spectra. The first row shows the full CCFs while the second row shows the profiles from which the radial velocities were determined. The final AMBRE:FEROS stellar parameters (Teff,log g, [M/H], [α/Fe]) and radial velocities are stated for each spectrum. The red lines are used to calculate the contrast and FWHM for each profile.
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