activity
20032009
most citedA direct empirical proof of the existence of dark matter

2.4k citations · 3.7k across the 7 of their papers we have counts for

collaborators

10 papers

astro-ph.CO20093 cited

The Evolution of Galaxy Clusters Across Cosmic Time

M. Arnaud, H. Bohringer, C. Jones +40

The large scale structure of the present Universe is determined by the growth of dark matter density fluctuations and by the dynamical action of dark energy and dark matter. While…

astro-ph2008124 cited

Chandra's View of the Ram Pressure Stripped Galaxy M86

S. Randall, P. Nulsen, W. R. Forman +4

We present results from a mosaic of nine Chandra observations of M86 and the surrounding field. We detect three main diffuse components: the Virgo ICM at ~2.4 keV, the extended hal…

astro-ph200855 cited

The Impact of Galaxy Cluster Mergers on Cosmological Parameter Estimation from Surveys of the Sunyaev-Zel'dovich Effect

Daniel R. Wik, Craig L. Sarazin, Paul M. Ricker +1

Sensitive surveys of the Cosmic Microwave Background will detect thousands of galaxy clusters via the Sunyaev-Zel'dovich (SZ) effect. Two SZ observables, the central or maximum and…

astro-ph2007789 cited

Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-5

Scott W. Randall, Maxim Markevitch, Douglas Clowe +2

(Abridged) We compare recent results from X-ray, strong lensing, weak lensing, and optical observations with numerical simulations of the merging galaxy cluster 1E0657-56. X-ray ob…

astro-ph200647 cited

Catching a bullet: direct evidence for the existence of dark matter

D. Clowe, S. W. Randall, M. Markevitch

We present X-ray and weak lensing observations of the merging cluster system 1E0657-556. Due to the recently collision of a merging subcluster with the main cluster, the X-ray plas…

astro-ph20062.4k cited

A direct empirical proof of the existence of dark matter

Douglas Clowe, Marusa Bradac, Anthony H. Gonzalez +4

We present new weak lensing observations of 1E0657-558 (z=0.296), a unique cluster merger, that enable a direct detection of dark matter, independent of assumptions regarding the n…