Fig. 18.
Left: gas extinction radial distribution (in units of Re), colour-coded as a function of the stellar mass log(M⋆/M⊙), as reported in the legend. The shaded regions represent the 16th and 84th percentiles of the distribution in each stellar mass bin taking into account the number of galaxies lying in the bin. Right: slope of the radial profiles of E(B − V) in units of mag/Re as a function of stellar mass.
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