Fig. 2.

Scaling relation between dust and HI masses within r25, in logarithmic scale, for 429 DustPedia late-type galaxies (those with dust and HI mass data). The light blue circles are log(MHI) detections with error bars drawn in light gray. Red squares with downward arrows show log(MHI) upper limits. The (black) continuum line is the line fit derived for the plotted 429 galaxies, and the (magenta) dashed line that for the sample galaxies with dust, HI, and H2 data (252 galaxies, those plotted in both panels of Fig. 3). Equations of the line fits and the Pearson correlation coefficients R are also given in the figure.
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