Integrated UV to NIR spectral energy distribution (SED) of the galaxies NGC 7469 and IC 5283. In this two-panel plot, the top panel shows the photometric data from Table 5 for the two galaxies are shown as yellow dots which were used to fit a SED using the code MAGPHYS (da Cunha & Charlot 2011). The blue dashed line represents the unabsorbed stellar component, while the red dashed lines show the dust re-emission. The black solid line represents the total emission. The bottom panel shows the residuals concerning the best fit. The parameters χ² and z_s represent the chi-square of the best-fit model and the redshift of the galaxy, respectively. Table 6 provides the extracted physical parameters derived from this SED fitting.