The cluster environments of the z ∼ 1 3 CR radio galaxies

An analysis of the environments around a sample of 28 3CR radio galaxies with red-shifts 0.6 < z < 1.8 is presented, based primarily upon K–band images down to K ∼ 20 taken using the UK Infrared Telescope (UKIRT). A net overdensity of K– band galaxies is found in the fields of the radio galaxies, with the mean excess counts being comparable to that expected for clusters of Abell Class 0 richness. A sharp peak is found in the angular cross–correlation amplitude centred on the radio galaxies , which, for reasonable assumptions about the luminosity function of the galaxies, corresponds to a spatial cross–correlation amplitude between those determined for low redshift Abell Class 0 and Abell Class 1 clusters. These data are complimented by J–band images also from UKIRT, and by optical images from the Hubble Space Telescope. The fields of the lower redshift (z ∼ < 0.9) radio galaxies in the sample generally show well–defined near–infrared colour–magnitude relations with little scatter, indicating a significant number of galaxies at the redshift of the radio galaxy; the relations involving colours shortward of the 4000Å break show considerably greater scatter, suggesting that many of the cluster galaxies have low levels of recent or on–going star formation. At higher redshifts the colour–magnitude sequences are less prominent due to the increased field galaxy contribution at faint magnitudes, but there is a statistical excess of galaxies with the very red infrared colours (J − K ∼ > 1.75) expected of old cluster galaxies at these redshifts. Although these results are appropriate for the mean of all of the radio galaxy fields, there exist large field–to–field variations in the richness of the environments. Many, but certainly not all, powerful z ∼ 1 radio galaxies lie in (proto–)cluster environments.