The X-Ray, SZ, and Optical Scaling Relations of Massive Galaxy Clusters

Details The X-Ray, SZ, and Optical Scaling Relations of Massive Galaxy Clusters The X-Ray, SZ, and Optical Scaling Relations of Massive Galaxy Clusters

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cxo..prop.2918r&link_type=abstract

Chandra proposal ID #11800852

Physics

Scientific paper

A multi-wavelength approach to cluster cosmology is necessary to overcome systematic uncertainties in the relation between cluster mass and observable mass tracers. We propose short observations of 12 of the 25 richest optical clusters in the redshift range 0.2

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