Fig. 23.
MBH spin evolution with MBH mass for all MBH at redshift z = 0.25 (black markers), and the spin evolution history with mass for the six most massive MBH (coloured lines). Shown for comparison are observations from Reynolds (2013; grey triangles) and Soares & Nemmen (2020; grey crosses). MBHs experience a fast initial spin growth phase followed by a more stochastic evolution.
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