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
Open accessAbstract
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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“This tension is becoming statistically significant and is now at the level of 3.1σ with KiDS-100 [77], that gives S 8 = 0.766 +0.020 -0.014 , and 2.5σ with DES-Y3 [78], that gives S 8 = 0.759 +0.025 -0.025 , while Planck prefers a higher value for S 8 = 0.834 +0.016 -0.016 .”
From Challenges of the Standard Cosmological Model (2022) · cites this paper as [78]
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“S 8 in disagreement at about 3.8σ with KiDS-1000 [77], and more than 3.5σ with DES-Y3 [78].”
From Challenges of the Standard Cosmological Model (2022) · cites this paper as [78]
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“by varying Ω k , both the well-known tensions on H 0 and S 8 are exacerbated”
From Challenges of the Standard Cosmological Model (2022) · cites this paper as [78]
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Citations
Cites
1 retracted
Survey geometry and the internal consistency of recent cosmic shear measurements
Troxel, M. A., Krause, E., Chang, C., Eifler, T. F., Friedrich, O., Gruen, D., MacCrann, N., Chen, A., Davis, C. P., DeRose, J., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1889 · Cited by 96
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Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R. L., Hogan, C. J., Jha, S., Kirshner, R. P., et al. (1998) · The Astronomical Journal · doi:10.1086/300499 · Cited by 19,704
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
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The Astropy Collaboration, Robitaille, T. P., Tollerud, E. J., Greenfield, P., Droettboom, M., Bray, E., Aldcroft, T., Davis, M., Ginsburg, A., Price-Whelan, A. M., et al. (2013) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201322068 · Cited by 14,620
Self-citationThe Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package
Price-Whelan, A., Sipőcz, B., Günther, H. M., Lim, P., Crawford, S., Conseil, S., Shupe, D., Craig, M., Dencheva, N., Ginsburg, A., et al. (2018) · Astronomical Journal · doi:10.3847/1538-3881/aabc4f · Cited by 6,887
Self-citationThe cosmological simulation code gadget-2
Springel, V. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09655.x · Cited by 6,368
Górski, K., Hivon, E., Banday, A., Wandelt, B. D., Hansen, F., Reinecke, M., & Bartelmann, M. (2004) · The Astrophysical Journal · doi:10.1086/427976 · Cited by 5,217
Lewis, A., Challinor, A., & Lasenby, A. (2000) · The Astrophysical Journal · doi:10.1086/309179 · Cited by 4,920
Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity
Weinberg, S., & Dicke, R. H. (1973) · American Journal of Physics · doi:10.1119/1.1987308 · Cited by 3,103
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Bahamonde, S., Dialektopoulos, K. F., Escamilla‐Rivera, C., Farrugia, G., Gakis, V., Hendry, M., Hohmann, M., Said, J. L., Mifsud, J., & Valentino, E. D. (2022) · Reports on Progress in Physics · doi:10.1088/1361-6633/ac9cef · Cited by 631
Secco, L. F., Samuroff, S., Krause, E., Jain, B., Blazek, J., Raveri, M., Campos, A., Amon, A., Chen, A., Doux, C., et al. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.105.023515 · Cited by 388
Self-citationThe Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters
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Metadata
- 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
- Amon, A.
- Gruen, D.
- Troxel, M. A.
- MacCrann, N.
- Dodelson, S.
- Choi, A.
- Doux, C.
- 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.
- Cawthon, R.
- Chang, C.
- Chen, R.
- Chintalapati, P.
- Crocce, M.
- Davis, C.
- Diehl, H. T.
- Drlica-Wagner, A.
- Eckert, K.
- Elvin-Poole, J.
- Everett, S.
- Fang, X.
- Fosalba, P.
- Giannini, G.
- Gruendl, R. A.
- Harrison, I.
- Hartley, W. G.
- Herner, K.
- Huang, H.
- Kuropatkin, N.
- Liddle, A. R.
- McCullough, J.
- Muir, J.
- Pandey, S.
- Porredon, A.
- Refregier, A.
- Rollins, R. P.
- Roodman, A.
- Rosenfeld, R.
- Ross, A. J.
- Rykoff, E. S.
- Sevilla-Noarbe, I.
- Sheldon, E.
- Shin, T.
- Troja, A.
- Varga, T. N.
- Weaverdyck, N.
- Yanny, B.
- Yin, B.
- Zuntz, J.
- Aguena, M.
- Allam, S.
- Annis, J.
- Bacon, D.
- Bertin, E.
- Bhargava, S.
- Brooks, D.
- Burke, D. L.
- Carretero, J.
- Costanzi, M.
- Desai, S.
- Dietrich, J. P.
- Doel, P.
- Ferrero, I.
- Frieman, J.
- García-Bellido, J.
- Giannantonio, T.
- Gschwend, J.
- Gutierrez, G.
- Hinton, S. R.
- Honscheid, K.
- Hoyle, B.
- James, D. J.
- Kron, R.
- Kuehn, K.
- Lahav, O.
- Lima, M.
- Lin, H.
- 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.
- Schubnell, M.
- Serrano, S.
- Smith, M.
- Soares-Santos, M.
- Thomas, D.
- To, C.
- Weller, J.
- 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
- 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
- bronze
- doi.org
- 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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