Results of fitting the T04 model for galaxies in the GAMA, SDSS and COSMOS datasets using different assumptions for the intrinsic emission separated in bins of SFR. The fitted parameters are the (top), F (middle), and r_bulge (bottom). The assumptions for intrinsic emission are made using different star-formation main-sequences: Leslie et al. (2018a) (purple), Schreiber et al. (2015) (green), and Speagle et al. (2014) (orange), where square markers indicate the sample around z ≈ 0.0 and the crosses for the sample around z ≈ 0.7. We see that none of the normalizations result in a consistent trend between SFR and any of the fitted parameters.