Stellar mass, SFR, age, and dust mass (from top left to bottom right) plotted for galaxies assuming THIMF against Chabrier IMF. The estimates are derived from the SED fitting code CIGALE with errors calculated using a Bayesian analysis. The histograms on each axis show the distribution of the galaxies. Offsets in M_*, SFR, and M_Dust among both IMFs are shown as ratios of the median values (and corresponding uncertainties from the 25th and 75th percentile of the distributions). The black dotted line in each panel represents the 1:1 relation.