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Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
Open accessAbstract
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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“with just six free parameters, it manages to fit well all the current cosmological observations [8][9][10][11][12][13][14][15][16][17].”
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Liu, R., Hu, W., & Grin, D. (2025) · Physical review. D/Physical review. D. · doi:10.1103/1z4c-1w7f · Cited by 7
Zhong, K., Saraivanov, E., Caputi, J., Miranda, V., Boruah, S. S., Eifler, T. F., & Krause, E. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.123519 · Cited by 7
Self-citationCSST cosmological emulator II: Generalized accurate halo mass function emulation
Zhao, C., & Yu, Y. (2025) · Science China Physics Mechanics and Astronomy · doi:10.1007/s11433-025-2764-x · Cited by 7
The impact of 2D and 3D BAO measurements on the Cosmic Distance Duality Relation with HII galaxies
Zheng, J., Qiang, D.-C., You, Z.-Q., & Kumar, D. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/10/029 · Cited by 7
“The increasing tensions between cosmological parameters inferred from early-and late-Universe observations [10–17] have raised growing concerns about the robustness of the standard cosmology.”
Dixit, A., Yadav, M., Pradhan, A., & Barak, M. S. (2025) · Annals of Physics · doi:10.1016/j.aop.2025.170275 · Cited by 7
“This model has excellent agreement with a wide range of observational data from various regions of the universe [22–25].”
The BIG SOBOL SEQUENCE: How many simulations do we need for simulation-based inference in cosmology?
Bairagi, A., Wandelt, B. D., & Villaescusa-Navarro, F. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202554602 · Cited by 28
Effective Field Theory Constraints on Primordial Black Holes from the High-Redshift Lyman- α Forest
Ivanov, M. M., & Trifinopoulos, S. (2026) · Physical Review Letters · doi:10.1103/8g8z-bmxd · Cited by 7
Cardone, V. F., Joudaki, S., Blot, L., Bonici, M., Camera, S., Cañas-Herrera, G., Carrilho, P., Casas, S., Davini, S., Domizio, S. D., et al. (2026) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202556856 · Cited by 7
Self-citationTwo-point Separation Functions for Modeling Wide Binary Systems in Nearby Dwarf Galaxies
Kervick, C., Walker, M. G., Peñarrubia, J., & Koposov, S. E. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac5b5f · Cited by 7
The X-ray angular power spectrum of extended sources in the eROSITA Final Equatorial Depth survey
Lau, E. T., Bogdán, Á., Chadayammuri, U., Nagai, D., Kraft, R., & Cappelluti, N. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac3147 · Cited by 7
Sánchez, C., Alarcon, A., Bernstein, G. M., Sánchez, J., Pandey, S., Raveri, M., Prat, J., Weaverdyck, N., Sevilla-Noarbe, I., Chang, C., et al. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad2402 · Cited by 7
Self-citationThe catalog-to-cosmology framework for weak lensing and galaxy clustering for LSST
Prat, J., Zuntz, J., Chang, C., Tröster, T., Pedersen, E. M., García-García, C., Longley, E. P., Sánchez, J., Alonso, D., Fang, X., et al. (2023) · The Open Journal of Astrophysics · doi:10.21105/astro.2212.09345 · Cited by 16
Self-citationWang, Z., Yao, J., Liu, X., Liu, D., Fan, Z., & Hu, B. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad1592 · Cited by 7
Mass-varying dark matter from a phase transition
Mandal, S., & Sehgal, N. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.107.123003 · Cited by 7
Iqbal, A., Pratt, G. W., Bobin, J., Arnaud, M., Rasia, E., Rossetti, M., Duffy, R., Bartalucci, I., Bourdin, H., Luca, F. D., et al. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202347234 · Cited by 7
Cluster cosmology without cluster finding
Xhakaj, E., Leauthaud, A., Lange, J., Krause, E., Hearin, A. P., Huang, S., Wechsler, R. H., & Heydenreich, S. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae882 · Cited by 7
Self-citationBoruah, S. S., Fiedorowicz, P., & Rozo, E. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.023524 · Cited by 7
Dark scattering: accelerated constraints from KiDS-1000 with ReACT and CosmoPower
Carrion, K., Carrilho, P., Mancini, A. S., Pourtsidou, A., & Hidalgo, J. C. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae1663 · Cited by 8
The DAMIC-M Low Background Chamber
Arnquist, I. J., Avalos, N., Bailly, P., Baxter, D., Bertou, X., Bogdan, M., Bourgeois, C., Brandt, J., Cadiou, A., Castelló-Mor, N., et al. (2024) · Journal of Instrumentation · doi:10.1088/1748-0221/19/11/t11010 · Cited by 7
“To minimize temperature-induced stress on CCDs, we use the cooling rate of 0.1 K/min during temperature cycles.”
InfluentialSelf-citationKugel, R., Schaye, J., Schaller, M., McCarthy, I. G., Braspenning, J., Helly, J. C., Moreno, V. J. F., & McGibbon, R. J. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae2218 · Cited by 7
Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data
Tutusaus, I., Bonvin, C., & Grimm, N. (2024) · Nature Communications · doi:10.1038/s41467-024-53363-6 · Cited by 7
“However, some residual systematic uncertainties were identified in the two bins with the highest redshift and this led to the use of only the first 4 bins in the baseline 3 × 2pt analysis [14].”
InfluentialSelf-citationExamining Lyman-alpha emitters through simulations in anticipation of the DESI-II survey
Ravi, J., Hadzhiyska, B., White, M. J., Hernquist, L., & Bose, S. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.103509 · Cited by 7
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.
What counts as a claim ›How we measure confidence ›How we check this ›
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