activity
20122019
most citedThe DESI Experiment Part I: Science,Targeting, and Survey Design

1.3k citations · 2k across the 10 of their papers we have counts for

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Showing astro-ph.COShow all

8 papers · 1 filter

astro-ph.CO2019★ 104 cited

The Outer Rim Simulation: A Path to Many-Core Supercomputers

Katrin Heitmann, Hal Finkel, Adrian Pope +10

We describe the Outer Rim cosmological simulation, one of the largest high-resolution N-body simulations performed to date, aimed at promoting science to be carried out with large-…

astro-ph.CO2017★ 30 cited

Investigating Cluster Astrophysics and Cosmology with Cross-Correlation of the Thermal Sunyaev-Zel'dovich Effect and Weak Lensing

Ken Osato, Samuel Flender, Daisuke Nagai +2

Recent detections of the cross-correlation of the thermal Sunyaev-Zel'dovich (tSZ) effect and weak gravitational lensing (WL) enable unique studies of cluster astrophysics and cosm…

astro-ph.CO2016★ 43 cited

Constraints on the optical depth of galaxy groups and clusters

Samuel Flender, Daisuke Nagai, Michael McDonald

Future data from galaxy redshift surveys, combined with high-resolutions maps of the cosmic microwave background, will enable measurements of the pairwise kinematic Sunyaev-Zel'dov…

astro-ph.CO2016★ 124 cited

Detection of the kinematic Sunyaev-Zel'dovich effect with DES Year 1 and SPT

B. Soergel, S. Flender, K. T. Story +80

We detect the kinematic Sunyaev-Zel'dovich (kSZ) effect with a statistical significance of by combining a cluster catalogue derived from the first year data of the Dark Ene…

astro-ph.CO2015★ 39 cited

Simulations of the Pairwise Kinematic Sunyaev-Zel'dovich Signal

Samuel Flender, Lindsey Bleem, Hal Finkel +3

The pairwise kinematic Sunyaev-Zel'dovich (kSZ) signal from galaxy clusters is a probe of their line-of-sight momenta, and thus a potentially valuable source of cosmological inform…

astro-ph.CO2013★ 45 cited

The small scale power asymmetry in the cosmic microwave background

Samuel Flender, Shaun Hotchkiss

We investigate the hemispherical power asymmetry in the cosmic microwave background on small angular scales. We find an anomalously high asymmetry in the multipole range l=601-2048…