Non-LRD AGN at z>4.5 show elevated Mbh/M* ratios relative to the local relation, with the transition over ~500 Myr driven by changes in M* from BEAGLE-AGN modeling rather than Mbh evolution.
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A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling
Non-LRD AGN at z>4.5 show elevated Mbh/M* ratios relative to the local relation, with the transition over ~500 Myr driven by changes in M* from BEAGLE-AGN modeling rather than Mbh evolution.