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Star Formation in Cluster Galaxies at 0.2<z<0.55
Mike. L. Balogh, Simon L. Morris, H. K. C. Yee +2
The rest frame equivalent width of the [OII]3727 emission line, W(OII), has been measured for cluster and field galaxies in the CNOC redshift survey of rich clusters at 0.2<z<0.55.…
The CNOC Cluster Survey: Omega, sigma_8, Phi(L,z) Results, and Prospects for Lambda Measurement
R. G. Carlberg, H. K. C. Yee, H. Lin +14
Rich galaxy clusters are powerful probes of both cosmological and galaxy evolution parameters. The CNOC cluster survey was primarily designed to distinguish between Omega=1 and Ome…
The Average Mass Profile of Galaxy Clusters
R. G. Carlberg, H. K. C. Yee, E. Ellingson +9
The average mass density profile measured in the CNOC cluster survey is well described with the analytic form rho(r)=A/[r(r+a_rho)^2], as advocated on the basis on n-body simulatio…
Redshift Evolution of Galaxy Cluster Densities
R. G. Carlberg, S. L. Morris, H. K. C. Yee +1
The number of rich galaxy clusters per unit volume is a strong function of Omega, the cosmological density parameter, and sigma_8, the linear extrapolation to z=0 of the density co…