Fig. 5.
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Redshifts of z = 0 (top), 2 (middle), 4 (bottom) BH mass-stellar mass (left) and BH mass-velocity dispersion (right) relations. Note: the Greene et al. (2020) fits to z = 0 MBHs do not take into account upper limits. We repeat the z = 0 relation in the higher redshift panels to highlight the redshift evolution in the simulations. The fit from Pacucci et al. (2023) is for z = 4 − 7 galaxies.
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