Tracing Matter with Weak Lensing Surveys
Astrophysics
2007-05-23 v1
Abstract
Gravitational weak lensing maps the location of (dark) matter at all scales. The lens-induced distortion field traces gravity fields and can be used to reconstruct the mass distribution in galaxies, groups, clusters of galaxies or large-scale structures. From these reconstructions, one can in principle recover where the matter is, what are its properties and how it is coupled with light and baryons. In the following, we review the present status of weak lensing analysis and discuss the most recent results regarding matter properties in the universe.
Cite
@article{arxiv.astro-ph/0111091,
title = {Tracing Matter with Weak Lensing Surveys},
author = {Y. Mellier and L. van Waerbeke},
journal= {arXiv preprint arXiv:astro-ph/0111091},
year = {2007}
}
Comments
Latex, 10 pages. To appear in "Where's the Matter? Tracing Dark and Bright Matter with the New Generation of Large Scale Surveys", June 2001, Treyer & Tresse Eds., Frontier Group