The Evolution of Cluster Radio Galaxies at 0.5<z<1

dc.creatorPerlman, Eric S.
dc.creatorFrye, Christopher
dc.creatorEbeling, Harald
dc.creatorJones, Laurence R.
dc.creatorScharf, Caleb A.
dc.creatorHorner, Donald
dc.date2003-03-24
dc.date.accessioned2026-07-07T02:08:05Z
dc.date.available2026-07-07T02:08:05Z
dc.descriptionWe are conducting a deep radio survey of a sample of 25 distant ($0.5<z<1$) clusters of galaxies. Here we present a progress report. So far 17 of 25 clusters have been observed, to varying depths. We have found 33 radio sources within 0.3 Abell radii of the cluster center, of which 28 are likely associated with cluster member galaxies. A comparison of the radio luminosity function of these clusters with the results of two surveys at lower redshift, reveals no evidence for strong evolution in the population of cluster radio galaxies at $z \sim 0.65$.
dc.description5 pages, 2 figures, to be published in Carnegie Observatories Astrophysics Series, Vol. 3: Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution, ed. J. S. Mulchaey, A. Dressler, and A. Oemler (Pasadena: Carnegie Observatories, http://www.ociw.edu/ociw/symposia/series/symposium3/proceedings.html)
dc.identifierhttps://arxiv.org/abs/astro-ph/0303533
dc.identifierhttp://arxiv.org/abs/astro-ph/0303533
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5907
dc.subjectAstrophysics
dc.titleThe Evolution of Cluster Radio Galaxies at 0.5<z<1
dc.typetext

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