Simulations Applied to the Bright SHARC XCLF: Results and Implications
M. P. Ulmer, C. Adami, R. Pildis, A. K. Romer, R. C. Nichol, B. P. Holden
Abstract
We have performed simulations of the effectiveness of the Serendipitous High-redshift Archival ROSAT Cluster (SHARC) survey for various model universes. We find, in agreement with work based on a preliminary set of simulations no statistically significant evolution of the luminosity function out to z = 0.8.
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