X-ray Emission from Optically-Selected, High-Redshift Galaxy Clusters from the RCS Survey

Details X-ray Emission from Optically-Selected, High-Redshift Galaxy Clusters from the RCS Survey X-ray Emission from Optically-Selected, High-Redshift Galaxy Clusters from the RCS Survey

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1802g&link_type=abstract

Chandra Proposal ID #06901058

Physics

Chandra Proposal Id #06901058

Scientific paper

We propose to continue our study of optically-selected, high-redshift (z ~1) galaxy clusters from the RCS survey, which prior CXO observations have shown to be relatively underluminous for their optical richness. Here we propose a 50ks followup observation of RCS1419+5326 (z=0.64), initially observed for 10ks in GO3. The proposed observation will provide a precise global temperature for this object, as well as surface brightness and temperature maps that can diagnose the dynamical state of the cluster.

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