NewEvery arXiv paper, its researchers & institutions — mapped.
papers

Publications (15)

astro-ph.CO2014

Characterizing SL2S galaxy groups using the Einstein radius

T. Verdugo, V. Motta, G. Foëx +11

astro-ph.CO2014

Dark matter-baryons separation at the lowest mass scale: the Bullet Group

F. Gastaldello, M. Limousin, G. Foëx +13

astro-ph.GA2016

The Red Radio Ring: a gravitationally lensed hyperluminous infrared radio galaxy at z=2.553 discovered through citizen science

J. E. Geach, A. More, A. Verma +49

astro-ph.CO2017

DES meets Gaia: discovery of strongly lensed quasars from a multiplet search

A. Agnello, H. Lin, N. Kuropatkin +69

astro-ph.CO2015

Observation and Confirmation of Six Strong Lensing Systems in The Dark Energy Survey Science Verification Data

B. Nord, E. Buckley-Geer, H. Lin +89

astro-ph2007

Multi-Frequency VLBI Observations of the Gravitational Lens B2016+112

A. More, R. W. Porcas

astro-ph2009

A New Window of Exploration in the Mass Spectrum: Strong Lensing by Galaxy Groups in the SL2S

M. Limousin, R. Cabanac, R. Gavazzi +21

astro-ph2007

Probing a massive radio galaxy with gravitational lensing

A. More, J. P. McKean, T. W. B. Muxlow +3

astro-ph2009

The role of luminous substructure in the gravitational lens system MG 2016+112

A. More, J. P. McKean, S. More +3

astro-ph.CO2013

SARCS strong lensing galaxy groups: I - optical, weak lensing, and scaling laws

G. Foëx, V. Motta, M. Limousin +5

astro-ph.GA2017

Discovery of the Lensed Quasar System DES J0408-5354

H. Lin, E. Buckley-Geer, A. Agnello +78

astro-ph.IM2018

The Hyper Suprime-Cam SSP Survey: Overview and Survey Design

H. Aihara, N. Arimoto, R. Armstrong +139

astro-ph.CO2010

The mass distribution of a moderate redshift galaxy group and brightest group galaxy from gravitational lensing and kinematics

J. P. McKean, M. W. Auger, L. V. E. Koopmans +6

astro-ph.GA2017

Models of the strongly lensed quasar DES J0408-5354

Adriano Agnello, Huan Lin, L. Buckley-Geer +82

astro-ph.CO2011

Gravitational lens candidates in the E-CDFS

A. More, K. Jahnke, S. More +4