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20142018
most citedFirst Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters

276 citations · 1.7k across the 17 of their papers we have counts for

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11 papers · 1 filter

astro-ph.CO2018★ 23 cited

First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Effects of Chromatic Corrections to Supernova Photometry on Measurements of Cosmological Parameters

J. Lasker, R. Kessler, D. Scolnic +78

Calibration uncertainties have been the leading systematic uncertainty in recent analyses using type Ia Supernovae (SNe Ia) to measure cosmological parameters. To improve the calib…

astro-ph.CO2018★ 29 cited

Steve: A hierarchical Bayesian model for Supernova Cosmology

S. R. Hinton, T. M. Davis, A. G. Kim +66

We present a new Bayesian hierarchical model (BHM) named Steve for performing type Ia supernova (SNIa) cosmology fits. This advances previous works by including an improved treatme…

astro-ph.CO2018★ 132 cited

First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Analysis, Systematic Uncertainties, and Validation

D. Brout, D. Scolnic, R. Kessler +122

We present the analysis underpinning the measurement of cosmological parameters from 207 spectroscopically classified type Ia supernovae (SNe Ia) from the first three years of the…

astro-ph.CO2018★ 237 cited

First Cosmological Results using Type Ia Supernovae from the Dark Energy Survey: Measurement of the Hubble Constant

E. Macaulay, R. C. Nichol, D. Bacon +106

We present an improved measurement of the Hubble constant (H_0) using the 'inverse distance ladder' method, which adds the information from 207 Type Ia supernovae (SNe Ia) from the…

astro-ph.CO2018★ 276 cited

First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters

T. M. C. Abbott, S. Allam, P. Andersen +141

We present the first cosmological parameter constraints using measurements of type Ia supernovae (SNe Ia) from the Dark Energy Survey Supernova Program (DES-SN). The analysis uses…

astro-ph.CO2018★ 146 cited

Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSS

M. Costanzi, E. Rozo, M. Simet +83

We perform the first blind analysis of cluster abundance data. Specifically, we derive cosmological constraints from the abundance and weak-lensing signal of \redmapper\ clusters o…

astro-ph.CO2018★ 97 cited

Survey geometry and the internal consistency of recent cosmic shear measurements

M. A. Troxel, E. Krause, C. Chang +76

We explore the impact of an update to the typical approximation for the shape noise term in the analytic covariance matrix for cosmic shear experiments that assumes the absence of…

astro-ph.CO2018★ 51 cited

Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions

E. J. Baxter, Y. Omori, C. Chang +91

Optical imaging surveys measure both the galaxy density and the gravitational lensing-induced shear fields across the sky. Recently, the Dark Energy Survey (DES) collaboration used…

astro-ph.CO2017★ 204 cited

Dark Energy Survey Year 1 Results: Weak Lensing Shape Catalogues

J. Zuntz, E. Sheldon, S. Samuroff +104

We present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set, covering 1500 square degrees with a median redshift of . The catalogues cover two main fie…

astro-ph.CO2015★ 115 cited

Space Warps II. New Gravitational Lens Candidates from the CFHTLS Discovered through Citizen Science

Anupreeta More, Aprajita Verma, Philip J. Marshall +18

We report the discovery of 29 promising (and 59 total) new lens candidates from the CFHT Legacy Survey (CFHTLS) based on about 11 million classifications performed by citizen scien…

astro-ph.CO2014★ 56 cited

Orientation Bias of Optically Selected Galaxy Clusters and Its Impact on Stacked Weak Lensing Analyses

Jörg P. Dietrich, Yuanyuan Zhang, Jeeseon Song +15

Weak-lensing measurements of the averaged shear profiles of galaxy clusters binned by some proxy for cluster mass are commonly converted to cluster mass estimates under the assumpt…