Fig. 13.
Radial metallicity gradients plotted against stellar mass for the O3N2 calibration (top panel) and the KK04 calibration (bottom panel) for DustPedia LTG (green) and ETG (magenta). The radii are relative to reff instead of r25. The weak correlations found for these calibrations are consistent with Belfiore et al. (2017; shown in blue) and Poetrodjojo et al. (2018).
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