and data from Büdenbender et al. (2014; B14) and Pasetto et al. (2012a,b); for the B14 SEGUE data, each colour represents a different [Fe/H] and [α/Fe] mono-abundance tracer population (and was chosen to reproduce the corresponding plots in B14), whereas the Pasetto et al. data are for undifferentiated RAVE stars.
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