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Oxford University Press, Monthly Notices of the Royal Astronomical Society, 3(504), p. 4312-4336, 2021

DOI: 10.1093/mnras/stab918

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Dark Energy Survey Year 3 Results: Weak Lensing Shape Catalogue

Journal article published in 2020 by M. Gatti, E. Sheldon, A. Amon, M. Becker ORCID, M. Troxel ORCID, A. Choi, C. Doux ORCID, N. MacCrann ORCID, A. Navarro Alsina, I. Harrison ORCID, D. Gruen ORCID, G. Bernstein ORCID, M. Jarvis, L. F. Secco, A. Ferté and other authors.
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

ABSTRACT We present and characterize the galaxy shape catalogue from the first 3 yr of Dark Energy Survey (DES) observations, over an effective area of 4143 deg2 of the southern sky. We describe our data analysis process and our self-calibrating shear measurement pipeline metacalibration, which builds and improves upon the pipeline used in the DES Year 1 analysis in several aspects. The DES Year 3 weak-lensing shape catalogue consists of 100 204 026 galaxies, measured in the riz bands, resulting in a weighted source number density of neff = 5.59 gal arcmin−2 and corresponding shape noise σe = 0.261. We perform a battery of internal null tests on the catalogue, including tests on systematics related to the point spread function (PSF) modelling, spurious catalogue B-mode signals, catalogue contamination, and galaxy properties.