Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
M. A. Troxel, N. MacCrann, J. Zuntz, T. F. Eifler, E. Krause, S., Dodelson, D. Gruen, J. Blazek, O. Friedrich, S. Samuroff, J. Prat, L. F., Secco, C. Davis, A. Fert\'e, J. DeRose, A. Alarcon, A. Amara, E. Baxter, M., R. Becker, G. M. Bernstein, S. L. Bridle, R. Cawthon, C. Chang

TL;DR
This paper presents the most significant cosmic shear measurements from DES Year 1, constraining cosmological parameters with high precision and confirming consistency with previous data and models.
Contribution
It provides the first high-precision cosmic shear results from DES Year 1 using multiple independent methods and catalogs, improving constraints on cosmological parameters.
Findings
3.5% uncertainty on $\sigma_8(\Omega_m/0.3)^{0.5}$
Results consistent with previous cosmic shear and CMB data
No evidence for deviation from $w=-1$ in dark energy equation of state
Abstract
We use 26 million galaxies from the Dark Energy Survey (DES) Year 1 shape catalogs over 1321 deg 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 CDM and CDM models, while also varying the neutrino mass density. These results are shown to be robust using two independent shape catalogs, two independent \photoz\ calibration methods, and two independent analysis pipelines in a blind analysis. We find a 3.5\% fractional uncertainty on at 68\% CL, which is a factor of 2.5 improvement over the fractional constraining power of our DES Science Verification results. In CDM, we find a 4.8\% fractional uncertainty on and a dark energy equation-of-state…
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