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Fig. 8


Left: LIR versus L8 for the whole 5MUSES sample. Black circles correspond to purely star-forming and composite sources, while red triangles correspond to AGN. The solid grey line depicts the median and 68% dispersion of composite and star-forming galaxies. Right: LIR/L8 versus EW of 6.2 μm. The horizontal lines enclose the values of LIR/L8 within the 68% dispersion from the median. The orange lines depict the best-fit linear regression and its scatter in the EW6.2 ≥ 0.4  μm regime. Purple squares correspond to sources with fAGN > 0.5.

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