Left: L₂₄/L_IR 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 L_IR is >50%. Leftward arrows denote upper limits in EW_6.2 measurements. Middle: T_d versus EW_6.2. T_d 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 λ_rest> 60 μm. Right: T_d versus fraction of L_IR arising from AGN activity, as derived based on SED decomposition.