Fig. 10
Main plot: comparison between SFRIR + UV and SFRIR for SFGs with at least one IR detection. Filled points mark PACS-detected galaxies. Bottom plot: SFRIR + UV over SFRIR ratio as a function of SFRIR. Median ratio in bins of SFRIR are also shown. Upper plot: black histogram is the distribution of SFRIR over the entire sample of SFGs; red empty histogram is the distribution of PACS-detected sources only.
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