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20012026
most citedMaximum-entropy weak lens reconstruction: improved methods and application to data

85 citations · 229 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2026★ 14 cited

The Vera C. Rubin Observatory Data Preview 1

Vera C Rubin Observatory Team, Tatiana Acero Cuellar, Emily Acosta +325

We present Rubin Data Preview 1 DP1, the first data from the NSF DOE Vera C Rubin Observatory, comprising raw and calibrated single epoch images, coadds, difference images, detecti…

astro-ph.CO2014★ 16 cited

The mass profile and dynamical status of the z~0.8 galaxy cluster LCDCS 0504

L. Guennou, A. Biviano, C. Adami +34

Constraints on the mass distribution in high-redshift clusters of galaxies are not currently very strong. We aim to constrain the mass profile, M(r), and dynamical status of the $z…

astro-ph.IM2012★ 29 cited

Atmospheric PSF Interpolation for Weak Lensing in Short Exposure Imaging Data

C. Chang, P. J. Marshall, J. G. Jernigan +25

A main science goal for the Large Synoptic Survey Telescope (LSST) is to measure the cosmic shear signal from weak lensing to extreme accuracy. One difficulty, however, is that wit…

astro-ph.CO2012★ 33 cited

The Hubble constant and new discoveries in cosmology

S. H. Suyu, T. Treu, R. D. Blandford +22

We report the outcome of a 3-day workshop on the Hubble constant (H_0) that took place during February 6-8 2012 at the Kavli Institute for Particle Astrophysics and Cosmology, on t…

astro-ph2002★ 52 cited

Cosmological parameter estimation and Bayesian model comparison using VSA data

Anze Slosar, Pedro Carreira, Kieran Cleary +28

We constrain the basic comological parameters using the first observations by the Very Small Array (VSA) in its extended configuration, together with existing cosmic microwave back…

astro-ph2001★ 85 cited

Maximum-entropy weak lens reconstruction: improved methods and application to data

P. J. Marshall, M. P. Hobson, S. F. Gull +1

We develop the maximum-entropy weak shear mass reconstruction method presented in earlier papers by taking each background galaxy image shape as an independent estimator of the red…