Fig. 9.
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Correlation between BH mass and galaxy mass at different redshift ranges: 3.5 < z < 4, 4 < z < 4.5, and 4.5 < z < 5. The notation is identical to Fig. 4. At constant M*, M• increases with redshift for z<. Delayed mergers are overmassive on average at certain galaxy masses at all redshifts, although the average lies within the scatter of the global relation.
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