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Fig. B.1.

image

Best-fit SED models for the 67 galaxies in the current sample containing the unattenuated emission by the old (red) and the young (blue) stellar populations, the nebular line emission (dark-yellow), the diffuse dust (orange), the emission from the PDR regions (green), as well as the AGN emission (purple) are also presented. The best-fit SED is indicated as a black curve, while the observations for each galaxy, along with their uncertainties, are indicated by violet open squares. Light-green dots stand for the best-model flux densities.

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