Observed near-infrared-to-millimeter SEDs and best-fit models derived from CIGALE SED fitting analysis of galaxies E+W, E, and W. Gray line: Best-fit model for the galaxies E+W. Red line: Best-fit model for galaxy E. Green line: Best-fit model for galaxy W. The circles represent the observed photometric fluxes for galaxies E+W, E, and W, with the associated uncertainties given in Table 1. The crosses represent the modeled fluxes. Also indicated are the Hα observed and predicted fluxes (top right) and the corresponding [O III] 88 μm fluxes (bottom right).