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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

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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…

astro-ph2006309 cited

Strong and weak lensing united III: Measuring the mass distribution of the merging galaxy cluster 1E0657-56

Marusa Bradac, Douglas Clowe, Anthony H. Gonzalez +7

The galaxy cluster 1E0657-56 (z = 0.296) is remarkably well-suited for addressing outstanding issues in both galaxy evolution and fundamental physics. We present a reconstruction o…