activity
20082016
most citedGravitationally lensed quasars and supernovae in future wide-field optical imaging surveys

428 citations · 542 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2016★ 6 cited

Probabilistic Cosmological Mass Mapping from Weak Lensing Shear

Michael D. Schneider, Karen Y. Ng, William A. Dawson +3

We infer gravitational lensing shear and convergence fields from galaxy ellipticity catalogs under a spatial process prior for the lensing potential. We demonstrate the performance…

astro-ph.GA2015★ 6 cited

Strong gravitational lensing with the SKA

J. P. McKean, N. Jackson, S. Vegetti +7

Strong gravitational lenses provide an important tool to measure masses in the distant Universe, thus testing models for galaxy formation and dark matter; to investigate structure…

astro-ph.CO2011★ 78 cited

The SWELLS Survey. I. A large spectroscopically selected sample of edge-on late-type lens galaxies

T. Treu, A. A. Dutton, M. W. Auger +5

The relative contribution of baryons and dark matter to the inner regions of spiral galaxies provides critical clues to their formation and evolution, but it is generally difficult…

astro-ph.CO2010★ 428 cited

Gravitationally lensed quasars and supernovae in future wide-field optical imaging surveys

Masamune Oguri, Philip J. Marshall

Cadenced optical imaging surveys in the next decade will be capable of detecting time-varying galaxy-scale strong gravitational lenses in large numbers, increasing the size of the…

astro-ph.CO2009★ 7 cited

Strong Gravitational Lensing as a Probe of Gravity, Dark-Matter and Super-Massive Black Holes

L. V. E. Koopmans, M. Auger, M. Barnabe +26

Whereas considerable effort has been afforded in understanding the properties of galaxies, a full physical picture, connecting their baryonic and dark-matter content, super-massive…

astro-ph2008★ 17 cited

Cluster detection in weak lensing surveys

F. Feroz, P. J. Marshall, M. P. Hobson

We present an efficient and robust approach for extracting clusters of galaxies from weak lensing survey data and measuring their properties. We use simple, physically-motivated cl…