activity
20182022
most citedCMB-S4 Science Case, Reference Design, and Project Plan

443 citations · 549 across the 7 of their papers we have counts for

collaborators

24 papers

astro-ph.CO2021

The mass and galaxy distribution around SZ-selected clusters

T. Shin, B. Jain, S. Adhikari +136

We present measurements of the radial profiles of the mass and galaxy number density around Sunyaev-Zel'dovich-selected clusters using both weak lensing and galaxy counts. The clus…

astro-ph.CO2021

Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing

Sebastian Grandis, Sebastian Bocquet, Joseph J. Mohr +2

Cosmological inference from cluster number counts is systematically limited by the accuracy of the mass calibration, i.e. the empirical determination of the mapping between cluster…

astro-ph.CO202134 cited

Exploring the contamination of the DES-Y1 Cluster Sample with SPT-SZ selected clusters

S. Grandis, J. J. Mohr, M. Costanzi +73

We perform a cross validation of the cluster catalog selected by the red-sequence Matched-filter Probabilistic Percolation algorithm (redMaPPer) in Dark Energy Survey year 1 (DES-Y…

astro-ph.CO2020

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

C. To, E. Krause, E. Rozo +105

Combining multiple observational probes is a powerful technique to provide robust and precise constraints on cosmological parameters. In this letter, we present the first joint ana…

astro-ph.CO2020

Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8

V. Ghirardini, E. Bulbul, R. Kraft +11

The thermodynamic properties of the hot plasma in galaxy clusters retains information on the processes leading to the formation and evolution of the gas in their deep, dark matter…

astro-ph.CO2020

The Mira-Titan Universe. III. Emulation of the Halo Mass Function

Sebastian Bocquet, Katrin Heitmann, Salman Habib +5

We construct an emulator for the halo mass function over group and cluster mass scales for a range of cosmologies, including the effects of dynamical dark energy and massive neutri…