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.1801g&link_type=abstract

Chandra Proposal ID #06900442

Computer Science

Chandra Proposal Id #06900442

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. We will observed two clusters (one at z=1.09, for 70 ks, and one at z=0.64, for 50 ks) for a total exposure of 120 ksec. Our aim is to determine luminosity and bound the global temperature of these objects, to progress toward completion of X-ray observations of a well-defined z=1 subsample of the RCS, and to help select RCS candidates for subsequent, very deep followup observations with Chandra and XMM.

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