The ASTRID simulation's present-day universe broadly matches observed black-hole–galaxy scaling relations, galaxy counts, cluster stellar masses, and clustering, with known excesses in low-redshift star formation and accretion.
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The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
The ASTRID simulation's present-day universe broadly matches observed black-hole–galaxy scaling relations, galaxy counts, cluster stellar masses, and clustering, with known excesses in low-redshift star formation and accretion.