activity
20122026
most citedThe DESI Experiment Part I: Science,Targeting, and Survey Design

1.3k citations · 4k across the 78 of their papers we have counts for

collaborators
Showing 2022Show all

8 papers · 1 filter

astro-ph.CO2022★ 13 cited

Dark Energy Survey Year 3 Results: Redshift Calibration of the MagLim Lens Sample from the combination of SOMPZ and clustering and its impact on Cosmology

G. Giannini, A. Alarcon, M. Gatti +111

We present an alternative calibration of the MagLim lens sample redshift distributions from the Dark Energy Survey (DES) first three years of data (Y3). The new calibration is base…

astro-ph.CO2022★ 5 cited

A Machine Learning Approach to Enhancing eROSITA Observations

John Soltis, Michelle Ntampaka, John Wu +5

The eROSITA X-ray telescope, launched in 2019, is predicted to observe roughly 100,000 galaxy clusters. Follow-up observations of these clusters from Chandra, for example, will be…

astro-ph.CO2022

Dark Energy Survey Year 3 Results: Constraints on extensions to CDM with weak lensing and galaxy clustering

DES Collaboration, T. M. C. Abbott, M. Aguena +159

We constrain extensions to the CDM model using measurements from the Dark Energy Survey's first three years of observations and external data. The DES data are the two-point cor…

astro-ph.CO2022★ 8 cited

Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos

Arya Farahi, Daisuke Nagai, Dhayaa Anbajagane

Halos of similar mass and redshift exhibit a large degree of variability in their differential properties, such as dark matter, hot gas, and stellar mass density profiles. This var…

astro-ph.CO2022★ 4 cited

C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning

Daniel Farid, Han Aung, Daisuke Nagai +2

We present Classification of Cluster GAlaxy MEmbers (C-GaMe), a classification algorithm based on a suite of machine learning models that differentiates galaxies into orbiting,…

astro-ph.CO2022★ 51 cited

Optical selection bias and projection effects in stacked galaxy cluster weak lensing

Hao-Yi Wu, Matteo Costanzi, Chun-Hao To +16

Cosmological constraints from current and upcoming galaxy cluster surveys are limited by the accuracy of cluster mass calibration. In particular, optically identified galaxy cluste…