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

Simulations Applied to the Bright SHARC XCLF: Results and Implications

Astrophysics 2007-05-23 v1

Authors: 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.

Keywords

SHARC survey simulations luminosity function statistical evolution high-redshift

Cite

@article{arxiv.astro-ph/9910117,
  title  = {Simulations Applied to the Bright SHARC XCLF: Results and Implications},
  author = {M. P. Ulmer and C. Adami and R. Pildis and A. K. Romer and R. C. Nichol and B. P. Holden},
  journal= {arXiv preprint arXiv:astro-ph/9910117},
  year   = {2007}
}

Comments

5 pages, 4 Postscript figures, IGRAP-Marseille conf. June 1999

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