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Evolution of supermassive black holes : the role of galaxy mergers

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Figure

Figure 1.1: Madau plot, taken from (Bouwens et al., 2014)
Figure 1.2: Depiction of the geometry of AGNs proposed by Barthel (1989) including, from nearestthe SMBH outwards, the accretion disk, the broad line region, the torus, the narrow line region andpotentially kpc scale jets
Figure 1.3: Typical AGN spectral energy distributions, taken from (Ho, 1999).
Figure 1.4: The decline in sSFR with increasing stellar mass, split by morphology. Colours indicategalaxy morphology: ellipticals - maroon; S0 - red; S0a and Sa - orange; Sab and Sb - yellow; Sbc -green; Sc and Scd - cyan; Sd and Sdm - blue; Sm, Im, I and
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