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Fig. 7.
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Teff − log(g) distribution of ARGOS (left) and A2A (right) stars coloured by mean [Fe/H]. 10 Gyr PARSEC isochrones with −2 < [Fe/H] (dex) < 0.6 are plotted beneath. We note that the isochrones are plotted at 35% transparency in order to visually differentiate them from the 2D histograms.
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