Fig. 14.

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AGN populations. Left: AGN fraction, defined in terms of AGN bolometric luminosity as a function of galaxy mass. We recall that we have assumed an intrinsic active fraction of unity. Solid lines only require Lbol > 1044 erg s−1, dotted lines add m444W < 28 (galaxy and AGN combined) and dashed lines are for cLRDs (including the same bolometric and m444W cuts). Right: fraction of AGN-dominated sources at F444W as a function of m277W-m444W. Above m277W-m444W > 1.5 all sources are AGN-dominated.
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