Weak Gravitational Lensing: Current Status and Future Prospects
arXiv:astro-ph/9509019
Abstract
In this review I will describe progress that has been made in determining masses of galaxy clusters using `weak lensing' and how this technique my be applied in the future to determine the dark matter distribution both on supercluster scales and on the scale of galaxy haloes.
plain latex; 15 pages; 6 postscript figures