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19942020
most citedDark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

1.2k citations · 4.3k across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.CO2020★ 39 cited

Constraints on dark matter to dark radiation conversion in the late universe with DES-Y1 and external data

Angela Chen, Dragan Huterer, Sujeong Lee +81

We study a phenomenological class of models where dark matter converts to dark radiation in the low redshift epoch. This class of models, dubbed DMDR, characterizes the evolution o…

astro-ph.IM2018★ 497 cited

The Dark Energy Survey Data Release 1

T. M. C. Abbott, F. B. Abdalla, S. Allam +199

We describe the first public data release of the Dark Energy Survey, DES DR1, consisting of reduced single epoch images, coadded images, coadded source catalogs, and associated pro…

astro-ph.CO2017★ 204 cited

Dark Energy Survey Year 1 Results: Weak Lensing Shape Catalogues

J. Zuntz, E. Sheldon, S. Samuroff +104

We present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set, covering 1500 square degrees with a median redshift of . The catalogues cover two main fie…

astro-ph.CO2017★ 1.2k cited

Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

DES Collaboration, T. M. C. Abbott, F. B. Abdalla +197

We present cosmological results from a combined analysis of galaxy clustering and weak gravitational lensing, using 1321 deg of imaging data from the first year of the D…

astro-ph.CO2017★ 68 cited

CMB Polarization B-mode Delensing with SPTpol and Herschel

A. Manzotti, K. T. Story, W. L. K. Wu +60

We present a demonstration of delensing the observed cosmic microwave background (CMB) B-mode polarization anisotropy. This process of reducing the gravitational-lensing generated…

astro-ph.CO2016★ 24 cited

Inference from the small scales of cosmic shear with current and future Dark Energy Survey data

N. MacCrann, J. Aleksić, A. Amara +61

Cosmic shear is sensitive to fluctuations in the cosmological matter density field, including on small physical scales, where matter clustering is affected by baryonic physics in g…