Holger Israel, Thomas Erben, Thomas H. Reiprich, Alexey Vikhlinin, Craig L. Sarazin, Peter Schneider
Evolution in the mass function of galaxy clusters sensitively traces both the
expansion history of the Universe and cosmological structure formation. Robust
cluster mass determinations are a key ingredient for a reliable measurement of
this evolution, especially at high redshift. Weak gravitational lensing is a
promising tool for, on average, unbiased mass estimates. This weak lensing
project aims at measuring reliable weak lensing masses for a complete X-ray
selected sample of 36 high redshift (0.35View original: http://arxiv.org/abs/1112.4444
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