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

309 citations · 615 across the 6 of their papers we have counts for

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astro-ph200799 cited

Dark Matter and Baryons in the Most X-ray Luminous and Merging Galaxy Cluster RX J1347.5-1145

Maruša Bradač, Tim Schrabback, Thomas Erben +12

The galaxy cluster RX J1347-1145 is one of the most X-ray luminous and most massive clusters known. Its extreme mass makes it a prime target for studying issues addressing cluster…

astro-ph200721 cited

Direct Observation of Cosmic Strings via their Strong Gravitational Lensing Effect: I. Predictions for High Resolution Imaging Surveys

Maria Alice Gasparini, Phil Marshall, Tommaso Treu +2

We use current theoretical estimates for the density of long cosmic strings to predict the number of strong gravitational lensing events in astronomical imaging surveys as a functi…

astro-ph2007171 cited

Analytic models of plausible gravitational lens potentials

Edward A. Baltz, Phil Marshall, Masamune Oguri

Gravitational lenses on galaxy scales are plausibly modelled as having ellipsoidal symmetry and a universal dark matter density profile, with a Sersic profile to describe the distr…

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…

astro-ph2005

The SNAP Strong Lens Survey

Phil Marshall, Roger Blandford, Masao Sako

Basic considerations of lens detection and identification indicate that a wide field survey of the types planned for weak lensing and Type Ia SNe with SNAP are close to optimal for…

astro-ph2004

Very Small Array observations of the Sunyaev-Zel'dovich effect in nearby galaxy clusters

Katy Lancaster, Ricardo Genova-Santos, Nelson Falcon +10

We present VSA observations (~34GHz) on scales ~20 arcmin towards a complete, X-ray-flux-limited sample of seven clusters at redshift z<0.1. Four have significant SZ detections in…