PTA-detectable continuous gravitational wave sources in the ASTRID simulation are dominated by black hole mergers above 1e10 solar masses in central galaxies of massive clusters, often with dual AGN.
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Central Cluster Galaxies: A Hotspot for Detectable Gravitational Waves from Black Hole Mergers
PTA-detectable continuous gravitational wave sources in the ASTRID simulation are dominated by black hole mergers above 1e10 solar masses in central galaxies of massive clusters, often with dual AGN.