Fig. 11
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[V/Fe] versus [Fe/H] of the 135 CARMENES-GTO stars derived from our line-by-line analysis, color- and symbol-coded for their membership attribution to Galactic kinematic groups. Top: analysis based on stellar parameters from Schw19. Bottom: analysis based on stellar parameters from Marfil+. The thick-disk members appear to be better distinguished in metallicity space with the parameters estimated by Marfil+.
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