Fig. 6
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Galactic iron radial gradient (in the form of [Fe/H] = α × RGC + β). The objects are colour-coded as in Fig. 3 and described in the legend. Grey points correspond to the DCEPs published in Ripepi et al. (2021) and Trentin et al. (2023) (except for those observed with UVES). The solid black line corresponds to the best-fitted line. Results of the fits are reported in both the figure and Table A.6.
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