X-ray Galaxy Clusters as Cosmological Probes
22-Oct-99
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Table of Contents
Overview
X-ray Properties and Galaxy Cluster Masses
The Mass Function of Galaxy Clusters
Advantage of an X-ray Cluster Survey
The NORAS I and REFLEX I Cluster Surveys
The NORAS Cluster Survey
Growth Curve Analysis
Fraction of Undetected Flux
Distribution of Spectral Hardness and Extent
Identification Scheme
The REFLEX Cluster Survey
L
X
vs redshift for the REFLEX Survey
REFLEX X-ray Bright Cluster Sample
LogN-LogS Distribution of REFLEX Clusters
The X-ray Luminosity Function from REFLEX
Effective Sky Coverage of the REFLEX Survey
Power Spectrum for X-ray Bright Clusters
Outlook
Author:
Hans Boehringer
Email:
hxb@xray.mpe.mpg.de