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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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Self-citationPandey, S., Krause, E., DeRose, J., MacCrann, N., Jain, B., Crocce, M., Blazek, J., Choi, A., Huang, H.-J., To, C., et al. (2022) · UA Campus Repository (The University of Arizona) · doi:10.1103/physrevd.106.043520 · Cited by 83
Self-citationCosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
Carrilho, P., Moretti, C., & Pourtsidou, A. (2023) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2023/01/028 · Cited by 81
The MillenniumTNG Project: high-precision predictions for matter clustering and halo statistics
Hernández‐Aguayo, C., Springel, V., Pakmor, R., Barrera, M., Ferlito, F., White, S. D. M., Hernquist, L., Hadzhiyska, B., Delgado, A. M., Kannan, R., et al. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad1657 · Cited by 82
DES Y3 cosmic shear down to small scales: Constraints on cosmology and baryons
Aricò, G., Angulo, R. E., Zennaro, M., Contreras, S., Chen, A., & Hernández-Monteagudo, C. (2023) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202346539 · Cited by 80
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Self-citationSolà, J., Gómez-Valent, A., Pérez, J. D. C., & Moreno-Pulido, C. (2023) · Universe · doi:10.3390/universe9060262 · Cited by 77
Piattella, O. F. (2018) · UNITEXT for physics · doi:10.1007/978-3-319-95570-4 · Cited by 109
Consistency of effective field theory analyses of the BOSS power spectrum
Simon, T., Zhang, P., Poulin, V., & Smith, T. L. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.107.123530 · Cited by 76
Cosmology from CMB lensing and delensed E E power spectra using 2019–2020 SPT-3G polarization data
Ge, F., Millea, M., Camphuis, E., Daley, C., Huang, N., Omori, Y., Quan, W., Anderes, E., Anderson, A. J., Ansarinejad, B., et al. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.083534 · Cited by 76
Self-citationOmnipotent dark energy: A phenomenological answer to the Hubble tension
Adil, S. A., Akarsu, Ö., Valentino, E. D., Nunes, R. C., Özülker, E., Sen, A. A., & Specogna, E. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.109.023527 · Cited by 71
Simon, T., Abellán, G. F., Du, P., Poulin, V., & Tsai, Y. (2022) · arXiv (Cornell University) · doi:10.1103/physrevd.106.023516 · Cited by 74
Simon, T., Zhang, P., Poulin, V., & Smith, T. L. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.107.063505 · Cited by 72
Measurement of gravitational lensing of the cosmic microwave background using SPT-3G 2018 data
Pan, Z., Bianchini, F., Wu, W. L. K., Ade, P. A. R., Ahmed, Z., Anderes, E., Anderson, A. J., Ansarinejad, B., Archipley, M., Aylor, K., et al. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.108.122005 · Cited by 72
“3, and σ 8 (left to right) across different cosmological probes and surveys. from The direct H 0 measurement is taken Murakami et al. [37], while the LSS-based constraint on S 8 is taken from the reanalysis of the DES-Y3 (+ BAO) data of [40] presented in Madhavacheril et al. [72].”
InfluentialSelf-citationWeak lensing combined with the kinetic Sunyaev–Zel’dovich effect: a study of baryonic feedback
Bigwood, L., Amon, A., Schneider, A., Salcido, J., McCarthy, I. G., Preston, C., Sanchez, D., Sijacki, D., Schaan, E., Ferraro, S., et al. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae2100 · Cited by 72
Self-citationCosmological preference for a negative neutrino mass
Green, D., & Meyers, J. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.083507 · Cited by 72
Resolving the Hubble tension with early dark energy
Herold, L., & Ferreira, E. G. M. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.108.043513 · Cited by 73
Doux, C., Jain, B., Zürcher, D., Lee, J., Fang, X., Rosenfeld, R., Amon, A., Camacho, H., Choi, A., Secco, L. F., et al. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac1826 · Cited by 86
Self-citationTanseri, I., Hagstotz, S., Vagnozzi, S., Giusarma, E., & Katherine Freese, B. (2022) · Journal of High Energy Astrophysics · doi:10.1016/j.jheap.2022.07.002 · Cited by 70
Strong Gravitational Lensing as a Probe of Dark Matter
Vegetti, S., Birrer, S., Despali, G., Fassnacht, C. D., Gilman, D., Hezaveh, Y., Perreault-Levasseur, L., McKean, J. P., Powell, D., O’Riordan, C. M., et al. (2024) · Space Science Reviews · doi:10.1007/s11214-024-01087-w · Cited by 142
“…Koopmans 2004; Mandelbaum et al. 2006; Clowe et al. 2006; Auger et al. 2009; Barnabè et al. 2011; Sonnenfeld et al. 2022; Shajib et al. 2024), hot gas in galaxy clusters (e.g. Ettori et al. 2013), weak lensing and galaxy clustering (e.g. Alam et al. 2017; Heymans et al. 2021; Abbott et al. 2022).”
Self-citationInvestigating late-time dark energy and massive neutrinos in light of DESI Y1 BAO
Rebouças, J., de Souza, D. H. F., Zhong, K., Miranda, V., & Rosenfeld, R. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/02/024 · Cited by 68
“…Type Ia supernovae luminosity distances [3–9], distance measurements from Baryonic Acoustic Oscillations (BAOs) [10–29], Cosmic Microwave Background (CMB) temperature and polarization anisotropies [30–37], two-point correlation functions of galaxy shapes and positions [38–43], among other probes.”
Self-citationDark Energy Survey Year 3 Results: Deep Field optical + near-infrared images and catalogue
Hartley, W. G., Choi, A., Amon, A., Gruendl, R. A., Sheldon, E. S., Harrison, I., Bernstein, G. M., Sevilla-Noarbe, I., Yanny, B., Eckert, K., et al. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab3055 · Cited by 71
Self-citationDark Energy Survey Year 3 results: Cosmology with moments of weak lensing mass maps
Gatti, M., Jain, B., Chang, C., Raveri, M., Zürcher, D., Secco, L. F., Whiteway, L., Jeffrey, N., Doux, C., Kacprzak, T., et al. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.106.083509 · Cited by 66
Self-citationThe DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
Huang, L., Cai, R.-G., & Wang, S.-J. (2025) · Science China Physics Mechanics and Astronomy · doi:10.1007/s11433-025-2754-5 · Cited by 73
Chiu, I.-N. T., Klein, M., Mohr, J. J., & Bocquet, S. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad957 · Cited by 65
Self-citationThe Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and OverviewPreprint
Crichton, D., Aich, M., Amara, A., Bandura, K., Bassett, B. A., Bengaly, C. A. P., Berner, P., Bhatporia, S., Bucher, M., Chang, T., et al. (2021) · arXiv (Cornell University) · doi:10.1117/1.jatis.8.1.011019 · Cited by 65
Goldstein, S., Hill, J. C., Iršič, V., & Sherwin, B. D. (2023) · Physical Review Letters · doi:10.1103/physrevlett.131.201001 · Cited by 65
DESI luminous red galaxy samples for cross-correlations
Zhou, R., Ferraro, S., White, M. J., DeRose, J., Sailer, N., Aguilar, J., Ahlen, S. P., Bailey, S., Brooks, D., Claybaugh, T., et al. (2023) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2023/11/097 · Cited by 62
Self-citationModel-independent cosmological inference post DESI DR1 BAO measurements
Mukherjee, P., & Sen, A. A. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.123502 · Cited by 79
Sabogal, M. A., Silva, E., Nunes, R. C., Kumar, S., Valentino, E. D., & Giarè, W. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.123508 · Cited by 62
Negative neutrino masses as a mirage of dark energy
Elbers, W., Frenk, C. S., Jenkins, A. R., Li, B., & Pascoli, S. (2025) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.111.063534 · Cited by 61
Early dark sector, the Hubble tension, and the swampland
McDonough, E., Lin, M., Hill, J. C., Hu, W., & Zhou, S. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.106.043525 · Cited by 59
Late-time interacting cosmologies and the Hubble constant tension
Gariazzo, S., Valentino, E. D., Mena, O., & Nunes, R. C. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.106.023530 · Cited by 61
Fuzzy dark matter and the Dark Energy Survey Year 1 data
Dentler, M., Marsh, D. J. E., Hložek, R., Laguë, A., Rogers, K. K., & Grin, D. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac1946 · Cited by 58
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
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