Trinity's unconstrained predictions for quasar clustering agree with observations at z=0-3.5, and future surveys are unlikely to detect luminosity-dependent clustering unless they target very bright quasars.
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Trinity VII. Predictions for the Observable Correlation Functions of Accreting Black Holes
Trinity's unconstrained predictions for quasar clustering agree with observations at z=0-3.5, and future surveys are unlikely to detect luminosity-dependent clustering unless they target very bright quasars.