Comparison of SEDs computed by BEAGLE for two galaxy types. The upper panel displays the SED of a passive galaxy (green line), whereas the lower panel shows the SED of a star-forming galaxy (navy line). The U (3584 Å), V (5477 Å), and J (12 474 Å) filters, utilised for calculating photometric magnitudes, are marked on each graph to highlight the spectral regions where these galaxies exhibit significant differences in the rest-frame.