Cluster studies: Determination of H0/q0

Physics

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Chandra Proposal Id #05800081

Scientific paper

These observations form part of a systematic study of distant clusters of galaxies which are planned to achieve several goals. These include the determination of H0 and q0 by combining the X-ray measurements of gas density and temperature with radio measurements of the Sunyaev Zel'dovich effect, as well as the determination of temperature-luminosity-gas mass correlations and the baryon mass function for high redshift samples, and the study of individual clusters (e.g. cooling flows/AGN interactions, merging systems).

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