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Fig. D.3.
Top: [Al/Fe] vs. [Fe/H] for the training sample. Bottom: [Al/Fe] vs. [Fe/H] for 301 076 stars of the observed sample with S/N > 30, RAVE DR6 “n&o” classification, and parallax errors lower than 20%. For each panel, we overplotted a Teff − log(g) diagram with the location of the plotted stars marked in red.
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