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Fig. 6


Left: L24/LIR ratio as a function of the 6.2 μm PAH feature EW. Purple squares correspond to sources for which the SED decomposition suggests that the AGN contribution to the total LIR is >50%. Leftward arrows denote upper limits in EW6.2 measurements. Middle: Td versus EW6.2. Td estimates are derived based on a modified blackbody model for 79 sources (out of the total 154 sources shown in the left panel), which are detected in at least three bands at λrest> 60 μm. Right: Td versus fraction of LIR arising from AGN activity, as derived based on SED decomposition.

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