A High-Redshift Cluster Revealed by a WAT Radio Source

Details A High-Redshift Cluster Revealed by a WAT Radio Source A High-Redshift Cluster Revealed by a WAT Radio Source

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..133b&link_type=abstract

XMM-Newton Proposal ID #05035101

Computer Science

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, 1137+3000, Xmm-Newton Proposal 05035101

Scientific paper

Wide-angle tailed (WAT) radio sources are found in clusters of galaxies at low redshifts, and therefore can be used as probes for finding high-redshift clusters. We propose to observe the most distant WAT cluster known at z=0.96. Measurement of the luminosity, mass, and temperature of this cluster is an important complement to those values measured from clusters selected from optical and X-ray surveys and will aid in the study of cluster formation and evolution. Determining the gas mass fraction of the cluster will help in constraining the equation of state of dark energy.

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