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Fig. 1


Left: IRAC colour-colour diagram of the 5MUSES sample. The wedge is the AGN selection region of Donley et al. (2012). Red and black circles represent sources with EW6.2 ≤ 0.2  μm and EW6.2 > 0.2  μm respectively. Grey circles correspond to sources for which the SED decomposition attributes more than 50% of their total infrared luminosity to AGN activity. Right: fractional contribution of an AGN component to the total LIR as a function of the 6.2 μm EW of the sources. The dashed grey line corresponds to fAGN = 0.5.

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