Year: 1995
Type: preprint
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.
Source: arXiv (Cornell University)
Author: Kaiser, Nick
Institution: Canadian Institute for Theoretical Astrophysics
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W1520097358