Precision Galaxy Cluster Mass Estimates with Weak Gravitational Lensing

Details Precision Galaxy Cluster Mass Estimates with Weak Gravitational Lensing Precision Galaxy Cluster Mass Estimates with Weak Gravitational Lensing

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21722702n&link_type=abstract

American Astronomical Society, AAS Meeting #217, #227.02; Bulletin of the American Astronomical Society, Vol. 43, 2011

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Clusters of galaxies are the largest collapsed structures in the universe. Their size and distribution provide cosmological information, while their internal dynamics provide astrophysical clues to galaxy formation and evolution. In both cases, an accurate estimate of the mass of these clusters is crucial in tying the theory to observation. Here we present an ongoing project where we carefully measure the masses of 20 of the most massive clusters in 0.15

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