Fig. 4.
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Left: Fraction of galaxies with an AGN of X-ray luminosity > 2 × 1038 erg s−1 vs. stellar mass at redshifts 0, 2, and 4 (from top to bottom). We compare our results with data from the AMUSE survey (Gallo et al. 2010; Miller et al. 2015). Right: Fraction of systems with the most massive BH in kinetic feedback mode vs stellar mass at the same redshifts.
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