Comparison between the stellar mass (left), hydrogen column density (centre), and intrinsic X-ray luminosity (right) derived using SED3FIT with the clumpy and smooth torus library. All considered SED templates are scaled to have L_IR = 10¹¹ L_⊙. Symbols indicate different galaxy populations: SF-AGN (dark-green circles), SB-AGN (orange squares), AGN type-1 (blue triangles), and AGN type-2 (magenta stars). In the central panel, empty symbols and arrows represent the upper limits to N_H for the objects for which N_H = 0 with one torus library, but not with the other torus library. These points are artificially set to log₁₀(N_H/cm⁻² = −20.5 for visual purposes. We do not show objects for which N_H = 0 using both torus libraries; this is comprised of three AGN1 templates and one SF-AGN template. The vertical dashed grey line indicates the maximum values of N_H of the smooth torus library. Error bars indicate the 16% and 84% percentiles and, in the right panel, the scatter of 0.33 dex in the relation to derive X-ray luminosity (Asmus et al. 2015). The black dotted line in each panel indicates the identity line.