Fig. 22.
[α/M] ratio as a function of [Fe/H] for several bins of R and |Z|. [α/M] and [Fe/H] were derived through our CNN while the R and |Z| come from the DR6 of RAVE (Steinmetz et al. 2020b). Hexagonal bins and contour plots of the data are presented together. In total, we present trends for 185 569 stars with S/N > 30, parallax errors lower than 20%, and RAVE “n&o” classification.
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