Fig. 6.
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BHARD and BHMD as a function of redshift for the high redshift simulations, L12.5n768. The models that give similar BHARDs in the SMBH regime result in BHARDs that are orders of magnitude different in the IMBH regime. The models with accretion disks show a delay in BHARD compared to the models without accretion disks at the highest redshift, where timescales are shortest.
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