activity
20172020
most citedDark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood Analyses

129 citations · 153 across the 3 of their papers we have counts for

collaborators

14 papers

astro-ph.CO202013 cited

Masses: Weak Lensing Calibration of the Dark Energy Survey Year 1 redMaPPer Clusters using Stellar Masses

M. E. S. Pereira, A. Palmese, T. N. Varga +78

We present the weak lensing mass calibration of the stellar mass based mass proxy for redMaPPer galaxy clusters in the Dark Energy Survey Year 1. For the first time we…

astro-ph.GA2020

The impact of spectroscopic incompleteness in direct calibration of redshift distributions for weak lensing surveys

W. G. Hartley, C. Chang, S. Samani +74

Obtaining accurate distributions of galaxy redshifts is a critical aspect of weak lensing cosmology experiments. One of the methods used to estimate and validate redshift distribut…

astro-ph.CO2020

Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak Lensing

DES Collaboration, Tim Abbott, Michel Aguena +129

We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected from the Dark Energy Survey (DES) Year 1 dataset. Our analysis uses the same shear…

astro-ph.CO2019

Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps -- validation on simulations

M. Gatti, C. Chang, O. Friedrich +69

We present a simulated cosmology analysis using the second and third moments of the weak lensing mass (convergence) maps. The analysis is geared towards the third year (Y3) data fr…

astro-ph.CO2019

Dark Energy Survey Year 1 results: The relationship between mass and light around cosmic voids

Y. Fang, N. Hamaus, B. Jain +74

What are the mass and galaxy profiles of cosmic voids? In this paper we use two methods to extract voids in the Dark Energy Survey (DES) Year 1 redMaGiC galaxy sample to address th…

astro-ph.CO2019

The Aemulus Project IV: Emulating Halo Bias

Thomas McClintock, Eduardo Rozo, Arka Banerjee +6

Models of the spatial distribution of dark matter halos must achieve new levels of precision and accuracy in order to satisfy the requirements of upcoming experiments. In this work…