X-Ray Observations of the Most Massive DLS Shear-Selected Galaxy Clusters
Astrophysics
2009-09-29 v1
Abstract
We report on preliminary results of our X-ray survey of the most massive clusters currently identified from the Deep Lens Survey (DLS). The DLS cluster sample is selected based on weak lensing shear, which makes it possible for the first time to study clusters in a baryon-independent way. In this article we present X-ray properties of a subset of the shear-selected cluster sample.
Keywords
Cite
@article{arxiv.astro-ph/0401473,
title = {X-Ray Observations of the Most Massive DLS Shear-Selected Galaxy Clusters},
author = {John P. Hughes and Ian Dell'Antonio and Joseph Hennawi and Vera Margoniner and Sandor Molnar and Dara Norman and David Spergel and J. Anthony Tyson and Gillian Wilson and David Wittman},
journal= {arXiv preprint arXiv:astro-ph/0401473},
year = {2009}
}
Comments
4 pages, including 6 postscript figs, LaTeX, to appear in the proceedings of the conference "Multiwavelength Cosmology" held 17-20 June, 2003, ed M. Plionis