Cluster Weak Gravitational Lensing
Cosmology and Nongalactic Astrophysics
2013-04-12 v3
Abstract
Weak gravitational lensing of background galaxies is a unique, direct probe of the distribution of matter in clusters of galaxies. We review several important aspects of cluster weak gravitational lensing together with recent advances in weak lensing techniques for measuring cluster lensing profiles and constraining cluster structure parameters.
Cite
@article{arxiv.1002.3952,
title = {Cluster Weak Gravitational Lensing},
author = {Keiichi Umetsu},
journal= {arXiv preprint arXiv:1002.3952},
year = {2013}
}
Comments
Lectures given at the International School of Physics Enrico Fermi, Course CLXXII - "Astrophysics of Galaxy Clusters", Varenna, Italy, July 2008, ed. by A. Cavaliere and Y. Rephaeli; 30 pages, 14 figures; Reference format corrected