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Werkzeuggestützte interaktive Formalisierung textueller Anwendungsfallbeschreibungen für den Systemtest, , , , , and . Beiträge der 35. Jahrestagung der Gesellschaft für Informatik e.V. (Band2), Bonn, 19. bis 22. September 2005., (2005)Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty, , , , , , , , , and 144 other author(s). (2021)cite arxiv:2105.13544Comment: 32+9 pages, 13+4 figures, see https://www.darkenergysurvey.org/des-year-3-cosmology-results-papers/ for the full DES Y3 cosmology release.Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing, , , , , , , , , and 160 other author(s). (2021)cite arxiv:2105.13549Comment: See https://www.darkenergysurvey.org/des-year-3-cosmology-results-papers/ for the full DES Y3 3x2pt cosmology release.Cosmology from Cosmic Shear with DES Science Verification Data, , , , , , , , , and 119 other author(s). (2015)cite arxiv:1507.05552Comment: 20 pages, 12 figures. Additional information at http://deswl.github.io/.Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing, , , , , , , , , and 190 other author(s). (2017)cite arxiv:1708.01530Comment: 31 pages, 22 figures.The Dark Energy Survey: more than dark energy - an overview, , , , , , , , , and 131 other author(s). Monthly Notices of the Royal Astronomical Society, 460 (2): 1270--1299 (Aug 19, 2016)Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration, , , , , , , , , and 138 other author(s). (2021)cite arxiv:2105.13543Comment: 42 pages, 19 figures.Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample, , , , , , , , , and 134 other author(s). (2021)cite arxiv:2105.13546Comment: 25 pages, 16 figures, to be submitted to PRD. See https://www.darkenergysurvey.org/des-year-3-cosmology-results-papers/ for the full DES Y3 cosmology release.Eight new luminous z > 6 quasars selected via SED model fitting of VISTA, WISE and Dark Energy Survey Year 1 Observations, , , , , , , , , and 53 other author(s). (2017)cite arxiv:1701.04852Comment: 19 pages, 15 figures.Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835, , , , , , , , , and 101 other author(s). (2021)cite arxiv:2107.04646Comment: 23 pages, 10 figures, to be submitted to PRD.