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

Troxel, MA; MacCrann, N; Zuntz, J; Eifler, TF; Krause, E; Dodelson, S; Gruen, D; ... Zhang, Y; + view all (2018) Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear. Physical Review D , 98 (4) , Article 043528. 10.1103/PhysRevD.98.043528. Green open access

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Abstract

We use 26 × 10 6 galaxies from the Dark Energy Survey (DES) Year 1 shape catalogs over 1321     deg 2 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 Λ CDM and the w CDM 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 σ 8 ( Ω m / 0.3 ) 0.5 = 0.78 2 + 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 w CDM , we find a 4.8% fractional uncertainty on σ 8 ( Ω m / 0.3 ) 0.5 = 0.77 7 + 0.036 − 0.038 and a dark energy equation-of-state w = − 0.9 5 + 0.33 − 0.39 . We find results that are consistent with previous cosmic shear constraints in σ 8 — Ω m , 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 w CDM 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.

Type: Article
Title: Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear
Open access status: An open access version is available from UCL Discovery
DOI: 10.1103/PhysRevD.98.043528
Publisher version: http://dx.doi.org/10.1103/PhysRevD.98.043528
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: Science & Technology, Physical Sciences, Astronomy & Astrophysics, Physics, Particles & Fields, Physics, MATTER POWER SPECTRUM, LARGE-SCALE STRUCTURE, WEAK-LENSING MEASUREMENTS, CHALLENGE LIGHTCONE SIMULATION, SCIENCE VERIFICATION DATA, INTRINSIC ALIGNMENTS, PARAMETER CONSTRAINTS, REDSHIFT DISTRIBUTIONS, GALAXY ELLIPTICITIES, MODEL PREDICTIONS
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/1571428
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