XMM-Newton Proposal 02014701

Details XMM-Newton Proposal 02014701 XMM-Newton Proposal 02014701

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop...79l&link_type=abstract

XMM-Newton Proposal ID #02014701

Computer Science

Cl0934+4804, Xmm-Newton Proposal 02014701

Scientific paper

We propose to continue our approved XMM program to obtain detailed X-ray spectral and structural data for distant, optically-selected clusters. These observations will, for the first time ever, allow is to place accurate constraints on the temperature, metallicity, and gas mass fraction in the intracluster medium of rich, optically-selected clusters at high redshift. The target clusters are the most well-studied systems at z greater than 0.7 in the optical and infrared; thus, the addition of XMM data will enable us to probe the relationship between the X-ray and optical properties and their implications for galaxy and cluster evolution. Our program provides an essential comparison sample to those well-studied, X-ray-selected clusters at similar redshifts.

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