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Cited by 437Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaDark Matter and Cosmic Phenomena

The DOI matches its Crossref record; 208 of the 208 references it cites were found in a registry or an index.

Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration

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Amon, A., Gruen, D., Troxel, M. A., MacCrann, N., Dodelson, S., Choi, A., Doux, C., Secco, L. F., Samuroff, S., Krause, E., Cordero, J., Myles, J., DeRose, J., Wechsler, R. H., Gatti, M., Navarro-Alsina, A., Bernstein, G. M., Jain, B., Blazek, J., Alarcon, A., Ferté, A., Lemos, P., Raveri, M., Campos, A., Prat, J., Sánchez, C., Jarvis, M., Alves, O., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bridle, S. L., Camacho, H., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chang, C., Chen, R., Chintalapati, P., Crocce, M., Davis, C., Diehl, H. T., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elvin-Poole, J., Everett, S., Fang, X., Fosalba, P., Friedrich, O., Gaztanaga, E., Giannini, G., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Huterer, D., Kuropatkin, N., Leget, P., Liddle, A. R., McCullough, J., Muir, J., Pandey, S., Park, Y., Porredon, A., Refregier, A., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Tutusaus, I., Tutusaus, I., Varga, T. N., Weaverdyck, N., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Kron, R., Kuehn, K., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Tarle, G., Thomas, D., To, C., Weller, J., DES Collaboration·2022·Physical Review D
DOI 10.1103/physrevd.105.023514
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Abstract

This work, together with its companion paper, Secco, Samuroff et al. [Phys. Rev. D 105, 023515 (2022)], present the Dark Energy Survey Year 3 cosmic-shear measurements and cosmological constraints based on an analysis of over 100 million source galaxies. With the data spanning $4143\text{ }\text{ }{\mathrm{deg}}^{2}$ on the sky, divided into four redshift bins, we produce a measurement with a signal-to-noise of 40. We conduct a blind analysis in the context of the Lambda-Cold Dark Matter ($\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$) model and find a 3% constraint of the clustering amplitude, ${S}_{8}\ensuremath{\equiv}{\ensuremath{\sigma}}_{8}({\mathrm{\ensuremath{\Omega}}}_{\mathrm{m}}/0.3{)}^{0.5}=0.75{9}_{\ensuremath{-}0.023}^{+0.025}$. A $\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$-Optimized analysis, which safely includes smaller scale information, yields a 2% precision measurement of ${S}_{8}=0.77{2}_{\ensuremath{-}0.017}^{+0.018}$ that is consistent with the fiducial case. The two low-redshift measurements are statistically consistent with the Planck Cosmic Microwave Background result, however, both recovered ${S}_{8}$ values are lower than the high-redshift prediction by $2.3\ensuremath{\sigma}$ and $2.1\ensuremath{\sigma}$ ($p$-values of 0.02 and 0.05), respectively. The measurements are shown to be internally consistent across redshift bins, angular scales and correlation functions. The analysis is demonstrated to be robust to calibration systematics, with the ${S}_{8}$ posterior consistent when varying the choice of redshift calibration sample, the modeling of redshift uncertainty and methodology. Similarly, we find that the corrections included to account for the blending of galaxies shifts our best-fit ${S}_{8}$ by $0.5\ensuremath{\sigma}$ without incurring a substantial increase in uncertainty. We examine the limiting factors for the precision of the cosmological constraints and find observational systematics to be subdominant to the modeling of astrophysics. Specifically, we identify the uncertainties in modeling baryonic effects and intrinsic alignments as the limiting systematics.

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  1. L. Van Waerbeke, 2000, Astron. Astrophys., 358, 30
  2. 10.1088/0004-637X/765/1/74 · DOI
  3. 10.1103/PhysRevD.98.043528 · DOI
  4. 10.1086/516598 · DOI
  5. 10.1051/0004-6361/201834379 · DOI
  6. 10.1086/427976 · DOI

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Authors
Amon, A., Gruen, D., Troxel, M. A., MacCrann, N., Dodelson, S., Choi, A., Doux, C., Secco, L. F., Samuroff, S., Krause, E., Cordero, J., Myles, J., DeRose, J., Wechsler, R. H., Gatti, M., Navarro-Alsina, A., Bernstein, G. M., Jain, B., Blazek, J., Alarcon, A., Ferté, A., Lemos, P., Raveri, M., Campos, A., Prat, J., Sánchez, C., Jarvis, M., Alves, O., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bridle, S. L., Camacho, H., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chang, C., Chen, R., Chintalapati, P., Crocce, M., Davis, C., Diehl, H. T., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elvin-Poole, J., Everett, S., Fang, X., Fosalba, P., Friedrich, O., Gaztanaga, E., Giannini, G., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Huterer, D., Kuropatkin, N., Leget, P., Liddle, A. R., McCullough, J., Muir, J., Pandey, S., Park, Y., Porredon, A., Refregier, A., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Tutusaus, I., Tutusaus, I., Varga, T. N., Weaverdyck, N., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Kron, R., Kuehn, K., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Tarle, G., Thomas, D., To, C., Weller, J., & DES Collaboration
Affiliations
  • Kavli Institute for Particle Astrophysics and Cosmology (US)
  • SLAC National Accelerator Laboratory (US)
  • Duke University (US)
  • University of Cambridge (GB)
  • Carnegie Mellon University (US)
  • The Ohio State University (US)
  • University of Pennsylvania (US)
  • University of Chicago (US)
  • University of Arizona (US)
  • University of Manchester (GB)
  • Lawrence Berkeley National Laboratory (US)
  • Universidade Estadual de Campinas (UNICAMP) (BR)
  • École Polytechnique Fédérale de Lausanne (CH)
  • Argonne National Laboratory (US)
  • Jet Propulsion Laboratory (US)
  • University of Sussex (GB)
  • University of Michigan (US)
  • Laboratório Interinstitucional de e-Astronomia (BR)
  • Department of Physics and Astronomy, Watanabe 416, 2505 Correa Road, Honolulu, Hawaii 96822, USA
  • University of Wisconsin–Madison (US)
  • Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain
  • Center for Astrophysical Surveys, National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
  • Fermi National Accelerator Laboratory (US)
  • Institute of Space Sciences (ES)
  • University of California, Santa Cruz (US)
  • Institute for High Energy Physics (ES)
  • University of Illinois Urbana-Champaign (US)
  • University of Geneva (CH)
  • Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
  • Kavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
  • University of Lisbon (PT)
  • Kavli Institute for the Physics and Mathematics of the Universe (JP)
  • ETH Zurich (CH)
  • Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
  • Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (ES)
  • Brookhaven National Laboratory (US)
  • Max Planck Institute for Extraterrestrial Physics (DE)
  • University of Edinburgh (GB)
  • University of Portsmouth (GB)
  • Centre National de la Recherche Scientifique (FR)
  • University College London (GB)
  • Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
  • University of Trieste (IT)
  • Laboratório Interinstitucional de e-Astronomia, Rua Gal. José Cristino 77, Rio de Janeiro, Rio de Janeiro 20921-400, Brazil
  • Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
  • Indian Institute of Technology Hyderabad (IN)
  • Ludwig-Maximilians-Universität München (DE)
  • University of Oslo (NO)
  • Consejo Superior de Investigaciones Científicas (ES)
  • National Observatory (BR)
  • The University of Queensland (AU)
  • Center for Astrophysics Harvard & Smithsonian (US)
  • Lowell Observatory (US)
  • Universidade de São Paulo (BR)
  • Texas A&M University (US)
  • Harvard University (US)
  • Princeton University (US)
  • Institució Catalana de Recerca i Estudis Avançats (ES)
  • National Center for Supercomputing Applications (US)
  • University of Southampton (GB)
ORCID
Venue
Physical Review D
Publisher
American Physical Society (APS)
Published
2022-01-13
Volume
105
Issue
2
Pages
023514
ISSN
  • 2470-0010 (ISSN-L)
  • 2470-0029
DOI
10.1103/physrevd.105.023514
OpenAlex
W3173079094
Cited by
437
References
202
Citations by year
2026: 66 · 2025: 107 · 2024: 98 · 2023: 84 · 2022: 71
FWCI
36.09
Type
journal article
Language
en
Open access
Licence
Locations
  • Physical review. D/Physical review. D. (publishedVersion)
  • Research Archive of Indian Institute of Technology Hyderabad (Indian Institute of Technology Hyderabad) (acceptedVersion)
  • UA Campus Repository (The University of Arizona) (acceptedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • ArTS Archivio della ricerca di Trieste (University of Trieste https://www.units.it/) (submittedVersion, other-oa)
  • OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
  • Sussex Research Online (University of Sussex) (submittedVersion)
  • HAL (submittedVersion)
  • DIGITAL.CSIC (Spanish National Research Council (CSIC)) (submittedVersion)
  • UCL Discovery (University College London) (submittedVersion)
  • Figshare (submittedVersion)
  • Hispana (submittedVersion)
  • Infoscience (Ecole Polytechnique Fédérale de Lausanne) (submittedVersion, cc-by-nc-nd)
  • CINECA IRIS Institutial Research Information System (University of Genoa) (submittedVersion)
  • Biblos-e Archivo (Universidad Autónoma de Madrid) (submittedVersion)
  • LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) (submittedVersion, other-oa)
  • NORA - Norwegian Open Research Archives (submittedVersion, other-oa)
  • Padua Research Archive (University of Padova) (submittedVersion)
  • arXiv (Cornell University) (cc-by)
Funders
  • U.S. Department of Energy (DE-AC02-07CH11359)
  • National Science Foundation (AST-1138766, AST-1536171)
  • Science and Technology Facilities Council
  • Higher Education Funding Council for England
  • National Centre for Supercomputing Applications
  • University of Illinois at Urbana-Champaign
  • University of Chicago
  • Center for Cosmology and Astroparticle Physics, Ohio State University
  • Ohio State University
  • Texas A&M University
  • Financiadora de Estudos e Projetos
  • Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro
  • Conselho Nacional de Desenvolvimento Científico e Tecnológico
  • Ministério da Ciência, Tecnologia e Inovação
  • Deutsche Forschungsgemeinschaft
  • Ministerio de Ciencia e Innovación (ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, MDM-2015-0509)
  • European Commission
  • Generalitat de Catalunya
  • Seventh Framework Programme
  • European Research Council (240672, 291329, 306478)
  • Office of Science
  • High Energy Physics
  • Ministry of Science and Education of Spain
  • Mitchell Institute for Fundamental Physics and Astronomy
  • Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (465376/2014-2)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
Keywords
cosmic shear, S8, clustering amplitude, LambdaCDM model, cosmological constraints, redshift calibration, galaxy blending, weak gravitational lensing, observational systematics, baryon acoustic oscillations, redshift-space distortions

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