Galaxy merger-driven quasar model reproduces observed quasar luminosity density evolution, luminosity functions, clustering, and host properties from z=0 to 6.
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Close dual-AGN systems exhibit increased obscuration, higher bolometric luminosity, and elevated Eddington ratios for the less massive black hole as projected separation decreases, with excess AGN pairs relative to controls.
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A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
Galaxy merger-driven quasar model reproduces observed quasar luminosity density evolution, luminosity functions, clustering, and host properties from z=0 to 6.
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Enhanced activity in close dual-AGN systems in the local Universe
Close dual-AGN systems exhibit increased obscuration, higher bolometric luminosity, and elevated Eddington ratios for the less massive black hole as projected separation decreases, with excess AGN pairs relative to controls.