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Devon L. Hollowood

Researcher at University of California, Santa Cruz

Publications -  60
Citations -  1887

Devon L. Hollowood is an academic researcher from University of California, Santa Cruz. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 18, co-authored 60 publications receiving 1343 citations. Previous affiliations of Devon L. Hollowood include Santa Cruz Institute for Particle Physics.

Papers
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Journal ArticleDOI

The RedMaPPer Galaxy Cluster Catalog From DES Science Verification Data

Eli S. Rykoff, +94 more
TL;DR: The redMaPPer algorithm as discussed by the authors was applied to 150 deg(2) of Science Verification (SV) data from the Dark Energy Survey (DES), and to the Sloan Digital Sky Survey (SDSS) DR8 photometric data set.
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The redMaPPer Galaxy Cluster Catalog From DES Science Verification Data

Eli S. Rykoff, +94 more
TL;DR: In this paper, the authors describe updates to the Redmapper{} algorithm, a photometric red-sequence cluster finder specifically designed for large photometric surveys, applied to data from the Dark Energy Survey (DES), and to the Sloan Digital Sky Survey (SDSS) DR8 photometric data set.
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The SPTpol Extended Cluster Survey

Lindsey Bleem, +159 more
TL;DR: In this article, the authors describe the observations and resultant galaxy cluster catalog from the 2770 deg$^2$ SPTpol Extended Cluster Survey (SPT-ECS).
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Methods for cluster cosmology and application to the SDSS in preparation for DES Year 1 release

M. Costanzi, +103 more
TL;DR: In this paper, the authors derived cosmological constraints from the abundance and weak-lensing signal of clusters of richness in the red-shift range of the Sloan Digital Sky Survey (SDSS).
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Dark Energy Survey Year 1 Results: Constraints on Intrinsic Alignments and their Colour Dependence from Galaxy Clustering and Weak Lensing

S. Samuroff, +76 more
TL;DR: In this article, a joint analysis of intrinsic alignments and cosmology using tomographic weak lensing, galaxy clustering and galaxy-galaxy lensing measurements from Year 1 (Y1) of the Dark Energy Survey is performed.