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Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
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We present the first cosmology results from large-scale structure using the full 5000 deg 2 of imaging data from the Dark Energy Survey (DES) Data Release 1.We perform an analysis of large-scale structure combining three two-point correlation functions (3 × 2pt): (i) cosmic shear using 100 million source galaxies, (ii) galaxy clustering, and (iii) the cross-correlation of source galaxy shear with lens galaxy positions, galaxy-galaxy lensing.To achieve the cosmological precision enabled by these measurements has required updates to nearly every part of the analysis from DES Year 1, including the use of two independent galaxy clustering samples, modeling advances, and several novel improvements in the calibration of gravitational shear and photometric redshift inference.The analysis was performed under strict conditions to mitigate confirmation or observer bias; we describe specific changes made to the lens galaxy sample following unblinding of the results and tests of the robustness of our results to this decision.We model the data within the flat ΛCDM and wCDM cosmological models, marginalizing over 25 nuisance parameters.We find consistent cosmological results between the three two-point correlation functions; their combination yields clustering amplitude S 8 ¼ 0.776 þ0.017 -0.017 and matter density Ω m ¼ 0.339
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Alok, A. K., Chall, T. J., Chundawat, N. R. S., & Mandal, A. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.109.055011 · Cited by 5
Mass calibration of DES Year-3 clusters via SPT-3G CMB cluster lensing
Ansarinejad, B., Raghunathan, S., Abbott, T. M. C., Ade, P. A. R., Aguena, M., Alves, O., Anderson, A. J., Andrade-Oliveira, F., Archipley, M., Balkenhol, L., et al. (2024) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2024/07/024 · Cited by 5
Self-citationBerlfein, F., Mandelbaum, R., Dodelson, S., & Schafer, C. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae1444 · Cited by 5
Self-citationGravitational lensing from clusters of galaxies to test disformal couplings theories
Zamani, S., Salzano, V., & Bettoni, D. (2024) · The European Physical Journal C · doi:10.1140/epjc/s10052-024-13000-4 · Cited by 5
Inverse galaxy-galaxy lensing: Magnification, intrinsic alignments, and cosmology
Cross, D., & Sánchez, C. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.123534 · Cited by 5
“The three main observables at the 2-point level are those of galaxy clustering (position-position correlations), galaxy-galaxy lensing (position-shape) and cosmic shear (shape-shape) [60].”
Self-citationTele-correlation: calibrating shear-shear correlation with real data
Shen, Z. X., Zhang, J., Liu, C., Li, H., Wang, H., Liu, Z., & Sun, J. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/01/068 · Cited by 5
“Many large scale galaxy surveys set weak lensing as their primary scientific goals, including Canada-France-Hawaii Telescope Lensing Survey (CFHTLenS 1 )[1], Dark Energy Survey (DES 2 ) [2], Hyper Suprime-Cam Subaru Strategic Program (HSC 3 )[3], Kilo-Degree Survey (KiDS 4 )[4].”
BackgroundHi intensity mapping with the MIGHTEE Survey: first results of the Hi power spectrum
Mazumder, A., Wolz, L., Chen, Z., Paul, S., Santos, M. G., Jarvis, M. J., Townsend, J., Sekhar, S., & Taylor, R. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf975 · Cited by 5
Self-citationGiocoli, C., Despali, G., Meneghetti, M., Rasia, E., Moscardini, L., Borgani, S., Lesci, G. F., Marulli, F., Cui, W., & Yepes, G. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202553871 · Cited by 5
Ten-parameter simulation suite for cosmological emulation beyond Λ CDM
Yang, Y., Bird, S., & Ho, M.-F. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.083529 · Cited by 5
Toda, Y., & Seto, O. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.083551 · Cited by 5
Inflation in non-local hybrid metric-Palatini gravity
Bombacigno, F., Angelis, M. D., van de Bruck, C., & Giarè, W. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/05/025 · Cited by 7
Primordial sharp features through the nonlinear regime of structure formation
Stahl, C., Werth, D., & Poulin, V. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.123514 · Cited by 5
Thakore, B., Negro, M., Regis, M., Camera, S., Gruen, D., Nicolao Fornengo, B., Roodman, A. J., Porredon, A., Schutt, T., Cuoco, A., et al. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/06/037 · Cited by 5
Self-citationJohnston, H., Chisari, N. E., Joudaki, S., Reischke, R., Stölzner, B., Loureiro, A., Mahony, C., Unruh, S., Wright, A. H., Asgari, M., et al. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202452466 · Cited by 5
Self-citationPure-mode correlation functions for cosmic shear and application to KiDS-1000
Schneider, P., Asgari, M., Jozani, Y. N., Dvornik, A., Giblin, B., Harnois-Déraps, J., Heymans, C., Hildebrandt, H., Hoekstra, H., Kuijken, K. H., et al. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202142479 · Cited by 5
Impact of lensing magnification on the analysis of galaxy clustering in redshift space
Breton, M.-A., de la Torre, S., & Piat, J. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202142487 · Cited by 5
Methodological refinement of the submillimeter galaxy magnification bias
Cueli, M. M., González-Nuevo, J., Bonavera, L., Lapi, A., Crespo, D., & Casas, J. M. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202347876 · Cited by 5
A new analysis of the BOSS survey, including full-shape information and post-reconstruction BAOPreprint
Chen, S.-F., Vlah, Z., & White, M. J. (2021) · arXiv (Cornell University) · Cited by 5
$Λ$CDM is alive and wellPreprint
Blanchard, A., Héloret, J.-Y., Ilić, S., Lamine, B., & Tutusaus, I. (2022) · arXiv (Cornell University) · doi:10.48550/arxiv.2205.05017 · Cited by 9
Self-citationSpecial Issue on Modified Gravity Approaches to the Tensions of ΛCDM: Goals and Highlights
Valentino, E. D., Perivolaropoulos, L., & Said, J. L. (2024) · Universe · doi:10.3390/universe10040184 · Cited by 5
“The standard cosmological model, known as Λ CDM, has been remarkably successful in providing a coherent and predictive framework for understanding the Universe’s evolution, its large-scale structure, and cosmic microwave background (CMB) radiation [1–6].”
MethodPSTN-056: Survey Cadence Optimization Committee's Phase 3 Recommendations
Rubin's Survey Cadence Optimization Committee, N., Bianco, F. B., Jones, L., Anguita, T., Bauer, F. E., Edwards, L. O. V., Jha, S. W., Mandelbaum, R., Miller, A. A., Olsen, K. A. G., et al. (2025) · DOE SLAC National Accelerator Laboratory Repository · doi:10.71929/rubin/2585402 · Cited by 5
Kopana, M., Jolicoeur, S., & Maartens, R. (2025) · The European Physical Journal C · doi:10.1140/epjc/s10052-025-14241-7 · Cited by 4
“In (2.1), T ( k ) is the matter transfer function (normalized to 1 on very large scales), D is the growth factor (normalized to 1 today) and g in = ( 1 + z in ) D in is the initial growth suppression factor, with z in deep in the matter era.”
InfluentialLi, H.-H., Zhang, X.-Z., Qiu, T., & Xia, J.-Q. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/07/056 · Cited by 4
“017 ( DES-Y3 ) [69].”
Searching for dark matter interactions with ACT, SPT and DES
Zhou, Z., & Weiner, N. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/08/075 · Cited by 4
Geometric interpretations of the k -nearest neighbour distributions
Gangopadhyay, K., Banerjee, A., & Abel, T. (2025) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staf1637 · Cited by 4
Metadata
- Authors
- Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Bhargava, S., Birrer, S., Blazek, J., Brandao-Souza, A., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Cawthon, R., Chang, C., Chen, A., Chen, R., Choi, A., Conselice, C., Cordero, J., Costanzi, M., Crocce, M., da Costa, L. N., da Silva Pereira, M. E., Davis, C., Davis, T. M., De Vicente, J., DeRose, J., Desai, S., Di Valentino, E., Diehl, H. T., Dietrich, J. P., Dodelson, S., Doel, P., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Evrard, A. E., Fang, X., Farahi, A., Fernandez, E., Ferrero, I., Ferté, A., Fosalba, P., Friedrich, O., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Harrison, I., Hartley, W. G., Herner, K., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., Huff, E. M., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeffrey, N., Jeltema, T., Kovacs, A., Krause, E., Kron, R., Kuehn, K., Kuropatkin, N., Lahav, O., Leget, P.-F., Lemos, P., Liddle, A. R., Lidman, C., Lima, M., Lin, H., MacCrann, N., Maia, M. A. G., Marshall, J. L., Martini, P., McCullough, J., Melchior, P., Mena-Fernández, J., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Muir, J., Myles, J., Nadathur, S., Navarro-Alsina, A., Nichol, R. C., Ogando, R. L. C., Omori, Y., Palmese, A., Pandey, S., Park, Y., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Porredon, A., Prat, J., Raveri, M., Rodriguez-Monroy, M., Rollins, R. P., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Sanchez, J., Sanchez Cid, D., Scarpine, V., Schubnell, M., Scolnic, D., Secco, L. F., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tabbutt, M., Tarle, G., Thomas, D., To, C., Troja, A., Troxel, M. A., Tucker, D. L., Tutusaus, I., Varga, T. N., Walker, A. R., Weaverdyck, N., Wechsler, R., Weller, J., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., & DES Collaboration
- Affiliations
- Cerro Tololo Inter-American Observatory (CL)
- Laboratório Interinstitucional de e-Astronomia (BR)
- Argonne National Laboratory (US)
- Fermi National Accelerator Laboratory (US)
- University of Michigan (US)
- Kavli Institute for Particle Astrophysics and Cosmology (US)
- Consejo Superior de Investigaciones Científicas (ES)
- University of Portsmouth (GB)
- University of Hawaiʻi at Mānoa (US)
- University of Wisconsin–Madison (US)
- University of Pennsylvania (US)
- University of Sussex (GB)
- Stanford University (US)
- Northeastern University (US)
- Universidade Estadual de Campinas (UNICAMP) (BR)
- University of Manchester (GB)
- University College London (GB)
- SLAC National Accelerator Laboratory (US)
- Carnegie Mellon University (US)
- Institute for High Energy Physics (ES)
- Institute of Space Sciences (ES)
- University of Chicago (US)
- Duke University (US)
- The Ohio State University (US)
- University of Nottingham (GB)
- University of Trieste (IT)
- The University of Queensland (AU)
- Lawrence Berkeley National Laboratory (US)
- Indian Institute of Technology Hyderabad (IN)
- Ludwig-Maximilians-Universität München (DE)
- California Institute of Technology (US)
- University of California, Santa Cruz (US)
- University of Arizona (US)
- University of Geneva (CH)
- University of Oslo (NO)
- University of Cambridge (GB)
- University of Illinois Urbana-Champaign (US)
- National Observatory (BR)
- Center for Astrophysics Harvard & Smithsonian (US)
- Centre National de la Recherche Scientifique (FR)
- Lowell Observatory (US)
- University of Lisbon (PT)
- Australian National University (AU)
- Universidade de São Paulo (BR)
- Texas A&M University (US)
- Harvard University (US)
- Princeton University (US)
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (ES)
- Institució Catalana de Recerca i Estudis Avançats (ES)
- Max Planck Institute for Extraterrestrial Physics (DE)
- Kavli Institute for the Physics and Mathematics of the Universe (JP)
- National Center for Supercomputing Applications (US)
- Brookhaven National Laboratory (US)
- University of Southampton (GB)
- Oak Ridge National Laboratory (US)
- ORCID
- Abbott, T. M. C.
- Aguena, M.
- Alarcon, A.
- Allam, S.
- Alves, O.
- Amon, A.
- Andrade-Oliveira, F.
- Annis, J.
- Avila, S.
- Bacon, D.
- Baxter, E.
- Bechtol, K.
- Becker, M. R.
- Bernstein, G. M.
- Bhargava, S.
- Birrer, S.
- Blazek, J.
- Bridle, S. L.
- Brooks, D.
- Burke, D. L.
- Camacho, H.
- Campos, A.
- Carretero, J.
- Castander, F. J.
- Cawthon, R.
- Chang, C.
- Chen, A.
- Choi, A.
- Conselice, C.
- Cordero, J.
- Costanzi, M.
- Crocce, M.
- Davis, C.
- Davis, T. M.
- DeRose, J.
- Desai, S.
- Diehl, H. T.
- Dietrich, J. P.
- Dodelson, S.
- Doel, P.
- Doux, C.
- Drlica-Wagner, A.
- Eckert, K.
- Eifler, T. F.
- Elsner, F.
- Elvin-Poole, J.
- Everett, S.
- Evrard, A. E.
- Fang, X.
- Farahi, A.
- Fernandez, E.
- Ferrero, I.
- Ferté, A.
- Fosalba, P.
- Frieman, J.
- García-Bellido, J.
- Gatti, M.
- Gerdes, D. W.
- Giannantonio, T.
- Giannini, G.
- Gruen, D.
- Gruendl, R. A.
- Gschwend, J.
- Gutierrez, G.
- Harrison, I.
- Hartley, W. G.
- Herner, K.
- Hinton, S. R.
- Honscheid, K.
- Hoyle, B.
- Huff, E. M.
- Jain, B.
- James, D. J.
- Jarvis, M.
- Jeffrey, N.
- Jeltema, T.
- Krause, E.
- Kron, R.
- Kuehn, K.
- Kuropatkin, N.
- Lahav, O.
- Lemos, P.
- Liddle, A. R.
- Lidman, C.
- Lima, M.
- Lin, H.
- MacCrann, N.
- Maia, M. A. G.
- Marshall, J. L.
- Martini, P.
- McCullough, J.
- Melchior, P.
- Mena-Fernández, J.
- Menanteau, F.
- Miquel, R.
- Mohr, J. J.
- Morgan, R.
- Muir, J.
- Myles, J.
- Nadathur, S.
- Navarro-Alsina, A.
- Nichol, R. C.
- Ogando, R. L. C.
- Omori, Y.
- Palmese, A.
- Pandey, S.
- Paz-Chinchón, F.
- Petravick, D.
- Pieres, A.
- Porredon, A.
- Prat, J.
- Raveri, M.
- Rollins, R. P.
- Romer, A. K.
- Roodman, A.
- Rosenfeld, R.
- Ross, A. J.
- Rykoff, E. S.
- Samuroff, S.
- Sánchez, C.
- Sanchez, E.
- Schubnell, M.
- Scolnic, D.
- Serrano, S.
- Sevilla-Noarbe, I.
- Sheldon, E.
- Shin, T.
- Smith, M.
- Soares-Santos, M.
- Suchyta, E.
- Swanson, M. E. C.
- Tabbutt, M.
- Thomas, D.
- To, C.
- Troja, A.
- Troxel, M. A.
- Tutusaus, I.
- Varga, T. N.
- Walker, A. R.
- Weaverdyck, N.
- Wechsler, R.
- Weller, J.
- Yanny, B.
- Yin, B.
- Zuntz, J.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2022-01-13
- Volume
- 105
- Issue
- 2
- Pages
- 023520
- ISSN
- 2470-0010 (ISSN-L)
- 2470-0029
- OpenAlex
- W3165898284
- Cited by
- 1,124
- References
- 212
- Citations by year
- 2026: 199 · 2025: 252 · 2024: 236 · 2023: 224 · 2022: 168
- FWCI
- 87.07
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Physical review. D/Physical review. D. (publishedVersion)
- arXiv (Cornell University) (acceptedVersion)
- UA Campus Repository (The University of Arizona) (acceptedVersion)
- HAL (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)
- Biblos-e Archivo (Universidad Autónoma de Madrid) (submittedVersion, public-domain)
- DIGITAL.CSIC (Spanish National Research Council (CSIC)) (submittedVersion)
- Hispana (submittedVersion)
- Infoscience (Ecole Polytechnique Fédérale de Lausanne) (submittedVersion, cc-by-nc-nd)
- CINECA IRIS Institutial Research Information System (University of Genoa) (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)
- Funders
- U.S. Department of Energy
- National Science Foundation (AST-1138766, AST-1536171)
- Science and Technology Facilities Council
- Higher Education Funding Council for England
- University of Illinois at Urbana-Champaign
- University of Chicago
- Ohio State University
- Texas A and 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 (465376/2014-2)
- Ministério da Ciência, Tecnologia e Inovação
- Departamento Administrativo de Ciencia, Tecnología e Innovación
- Deutsche Forschungsgemeinschaft
- Argonne National Laboratory
- Kavli Institute for Theoretical Physics, University of California, Santa Barbara
- University of Cambridge
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
- University College London
- University of Edinburgh
- Eidgenössische Technische Hochschule Zürich
- Fermilab
- Lawrence Berkeley National Laboratory
- Ludwig-Maximilians-Universität München
- University of Michigan
- University of Nottingham
- University of Pennsylvania
- University of Portsmouth
- SLAC National Accelerator Laboratory
- Stanford University
- University of Sussex
- Association of Universities for Research in Astronomy
- Ministerio de Ciencia e Innovación (ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, MDM-2015-0509)
- European Regional Development Fund
- Generalitat de Catalunya
- H2020 European Research Council (240672, 291329, 306478)
- Instituto Nacional de Ciência e Tecnologia de Fármacos e Medicamentos
- Office of Science
- High Energy Physics
- Ministry of Science and Education of Spain
- Collaborating Institution
- DES-Brazil Consortium
- Institut de Ciències de l’Espai
- Institut de Física d’Altes Energies
- Excellence Cluster Universe
- NFS’s NOIRLab
- OzDES Membership Consortium
- Fermi Research Alliance (DE-AC02-07CH11359)
- 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
- cosmological constraints, large-scale structure, galaxy clustering, weak gravitational lensing, cosmic shear, galaxy-galaxy lensing, cross correlation function, matter density, wCDM model, photometric redshift calibration, confirmation bias, observer bias, Dark Energy Survey
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
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