  The AGN-galaxy cross-correlation function of radio-quiet AGN and radio
galaxies has been measured with the Panoramic Deep Fields. Colour selection
criteria and photometric redshifts have been used to significantly increase the
signal-to-noise of the angular cross-correlation function. Radio-quiet AGN
environments are comparable to the environments of early-type galaxies at low
redshift. The radio galaxy-galaxy spatial cross-correlation function is very
strong though large variations are observed from field-to-field. These
variations appear to be caused by large-scale-structure on scales comparable to
the 5 degree field-of-view. The distribution and spatial cross-correlation
function of radio galaxies and clusters in the Panoramic Deep Fields is
consistent with these objects tracing the same structures at z<0.7. No evidence
is found for evolution of the AGN-galaxy spatial cross-correlation function
across the redshift range observed.
