Fig. 12.
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Properties of color-selected cLRDs (red) with respect to all AGN with Lbol > 1044 erg s−1 (green) and with further m444W < 28 (blue) for SMC-like dust and model overm. A clear signature is the specific range in dust column density, Ndust, with respect to the global population. Further conditions are the elevated fEdd and ratio between MBH and Mstar.
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