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Fig. A.3


The dust-to-stellar mass ratio as a function of stellar mass (left), NUV − r colour (center) and stellar mass surface density (right), for dust masses estimated from the 350 μm luminosities without taking into account any colour/temperature variation in the sample. Symbols are as in Fig. 3. The orange lines and dashed regions show the average scaling relations and  ± 1σ area presented in Fig. 3.

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