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Title: Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear

Journal Article · · Physical Review D
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We use 26×106 galaxies from the Dark Energy Survey (DES) Year 1 shape catalogs over 1321 deg2 of the sky to produce the most significant measurement of cosmic shear in a galaxy survey to date. We constrain cosmological parameters in both the flat ΛCDM and the wCDM models, while also varying the neutrino mass density. These results are shown to be robust using two independent shape catalogs, two independent photo-z calibration methods, and two independent analysis pipelines in a blind analysis. We find a 3.5% fractional uncertainty on σ8m/0.3)0.5=0.782$$_{-0.027}^{+0.027}$$ at 68% C.L., which is a factor of 2.5 improvement over the fractional constraining power of our DES Science Verification results. In wCDM, we find a 4.8% fractional uncertainty on σ8m/0.3)0.5=0.777$$_{-0.038}^{+0.036}$$ and a dark energy equation-of-state w=-0.95$$_{-0.39}^{+0.33}$$. We find results that are consistent with previous cosmic shear constraints in σ8—Ωm, and we see no evidence for disagreement of our weak lensing data with data from the cosmic microwave background. Finally, we find no evidence preferring a wCDM model allowing w≠-1. We expect further significant improvements with subsequent years of DES data, which will more than triple the sky coverage of our shape catalogs and double the effective integrated exposure time per galaxy.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Brookhaven National Laboratory (BNL), Upton, NY (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Univ. of Michigan, Ann Arbor, MI (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Organization:
DES Collaboration
Grant/Contract Number:
AC02-07CH11359; SC0007859; SC0012704; SC0007901; AC02-05CH11231; PF5-160138
OSTI ID:
1468419
Alternate ID(s):
OSTI ID: 1392234; OSTI ID: 1466860; OSTI ID: 1487087; OSTI ID: 1646568
Report Number(s):
arXiv:1708.01538; FERMILAB-PUB-17-279-PPD; BNL-114247-2017-JA; PRVDAQ; 1614461
Journal Information:
Physical Review D, Vol. 98, Issue 4; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 383 works
Citation information provided by
Web of Science

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Evidence for the accelerated expansion of the Universe from weak lensing tomography with COSMOS text January 2009
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Bayesian Galaxy Shape Measurement for Weak Lensing Surveys - III. Application to the Canada-France-Hawaii Telescope Lensing Survey text January 2012
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CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics text January 2016
Cosmology constraints from shear peak statistics in Dark Energy Survey Science Verification data text January 2016
KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing text January 2016
Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology text January 2017
Dark Energy Survey Year 1 Results: Redshift distributions of the weak lensing source galaxies text January 2017
Detection of Weak Gravitational Lensing by Large-scale Structure text January 2000
Spin induced galaxy alignments and their implications for weak lensing measurements text January 2000
Intrinsic alignment-lensing interference as a contaminant of cosmic shear text January 2004
HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere text January 2004
Systematic Errors in Future Weak Lensing Surveys: Requirements and Prospects for Self-Calibration text January 2005
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