Dust mass (M_dust) vs. SFR for the main sample. Red crosses show the results of Smith et al. (2012) for a sample of ~1400 objects selected at 250 μm from the H-ATLAS survey (Eales et al. 2010) at z< 0.5. The dashed line shows the best fit obtained in da Cunha et al. (2010) from a sample of about ~1700 low redshift galaxies. Blue triangles and the magenta circles show two subsamples of approximately the same size with M_∗< 5 × 10⁹ M_⊙ and M_∗> 5 × 10¹⁰ M_⊙, respectively. The cross in the bottom right corner shows the average error.