activity
20152019
most citedA gravitational-wave standard siren measurement of the Hubble constant

1.2k citations · 1.6k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2019107 cited

Three new VHS-DES Quasars at 6.7 < z < 6.9 and Emission Line Properties at z > 6.5

S. L. Reed, M. Banerji, G. D. Becker +58

We report the results from a search for z > 6.5 quasars using the Dark Energy Survey (DES) Year 3 dataset combined with the VISTA Hemisphere Survey (VHS) and WISE All-Sky Survey. O…

astro-ph.CO201985 cited

Dark Energy Survey Year 1 Results: Calibration of Cluster Mis-centering in the redMaPPer Catalogs

Y. Zhang, T. Jeltema, D. L. Hollowood +83

The center determination of a galaxy cluster from an optical cluster finding algorithm can be offset from theoretical prescriptions or -body definitions of its host halo center.…

astro-ph.CO20171.2k cited

A gravitational-wave standard siren measurement of the Hubble constant

B. P. Abbott, R. Abbott, T. D. Abbott +1308

The detection of GW170817 in both gravitational waves and electromagnetic waves heralds the age of gravitational-wave multi-messenger astronomy. On 17 August 2017 the Advanced LIGO…

astro-ph.GA201727 cited

Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey Science Verification Data

J. Etherington, D. Thomas, C. Maraston +61

Measurements of the galaxy stellar mass function are crucial to understand the formation of galaxies in the Universe. In a hierarchical clustering paradigm it is plausible that the…

astro-ph.CO201624 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…

astro-ph.IM201580 cited

Characterization and correction of charge-induced pixel shifts in DECam

Daniel Gruen, Gary M. Bernstein, Mike Jarvis +4

Interaction of charges in CCDs with the already accumulated charge distribution causes both a flux dependence of the point-spread function (an increase of observed size with flux,…