Two examples of our SED modelling using BAGPIPES: NGC 2841 (top) and UGC 05721 (bottom). The blue points with error bars show our measured fluxes in the various bands (FUV, NUV, g, r, z, J, H, K_s, 3.6 μm, 22 μm). The z band is used only in UGC 05721. The orange-shaded region encompasses the set of SED models that best reproduce the data, with the dark orange points showing the predicted fluxes in the same wavebands as the measurements. The insets show the SFH of the model set. The two galaxies have markedly different SFHs and corresponding values of Υ_phot, listed on the left side of each panel.