SED-derived M_dust vs. M_star in logarithmic space. The σ values of the best-fit robust correlation are shown in the lower right corner. The robust correlations are shown as solid lines, and the (gray) dashed one corresponds to the relation given by da Cunha et al. (2010) for SDSS galaxies, reported to M_star through the SFMS by Hunt et al. (2016). The gray area is defined the same way as in Fig. 15. As in previous figures, filled symbols correspond to high specific SFR (Log(sSFR/yr⁻¹) > −10.6), and open ones to low specific SFR (Log(sSFR/yr⁻¹) ≤ −10.6).