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Fig. 3.

image

Left panel: same as Fig. 2 for the scaling relation between dust and H2 masses for 252 DustPedia late-type galaxies (those with dust and H2 data). The H2 gas masses were derived assuming the constant XCO (value from Bolatto et al. 2013). Right panel: same as left panel but for the scaling relation between dust and total gas masses.

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