AGN-Galaxy Clustering with the Panoramic Deep Fields
| dc.creator | Brown, M. J. I. | |
| dc.date | 2002-01-29 | |
| dc.date.accessioned | 2026-07-07T02:02:31Z | |
| dc.date.available | 2026-07-07T02:02:31Z | |
| dc.description | 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. | |
| dc.description | 4 pages, 2 figures, uses newpasp.sty, to appear in "A New Era In Cosmology" (ASP Conference Series) eds. T. Shanks and N. Metcalfe | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0201460 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0201460 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4066 | |
| dc.subject | Astrophysics | |
| dc.title | AGN-Galaxy Clustering with the Panoramic Deep Fields | |
| dc.type | text |