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Weak Gravitational Lensing: Current Status and Future Prospects

Nick Kaiser

Published 1995-09-05Version 1

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.

Comments: plain latex; 15 pages; 6 postscript figures
Categories: astro-ph
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