The cluster environments of powerful radio - loud and radio - quiet AGN

The spatial clustering amplitude (B gq) is determined for a sample of 44 powerful AGN at z ≃ 0.2. No significant difference is detected in the richness of the cluster environments of the radio-loud and radio-quiet sub-samples, both of which typically inhabit environments as rich as Abell Class ≃ 0. Comparison with radio luminosity-matched samples from Hill & Lilly (1991) and Wold et al. (2000a) suggests that there is no epoch-dependent change in environment richness out to at least z ≥ 0.5 for either radio galaxies or radio quasars. Comparison with the APM cluster survey shows that, contrary to current folklore, powerful AGN do not avoid rich clusters, but rather display a spread in cluster environment which is perfectly consistent with being drawn at random from the massive elliptical population. Finally, we argue that virtually all Abell class ≃ 0 clusters contained an active galaxy during the epoch of peak quasar activity at z ∼ 2.5.