Evolution of the X-ray Luminosity Function of MACS Clusters

Details Evolution of the X-ray Luminosity Function of MACS Clusters Evolution of the X-ray Luminosity Function of MACS Clusters

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..379..312m&link_type=abstract

Cosmic Frontiers ASP Conference Series, Vol. 379, proceedings of the conference held 31 July-4 August 2006 at Durham University,

Computer Science

Scientific paper

We report the X-ray luminosity function for the Massive Cluster Sample
taking into account the Malmquist bias and the Eddington bias. The XLF
of the MACS sample is fitted using the Schechter function and shows
significant evolution comparing to the Extended Brightest Cluster
Sample.

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