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Cited by 1,124Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaDark Matter and Cosmic Phenomena

The DOI matches its Crossref record; 214 of the 215 references it cites were found in a registry or an index.

Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing

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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·2022·Physical Review D
DOI 10.1103/physrevd.105.023520
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Abstract

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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  1. A. Einstein, 1917, Sitzungsber. Preuss. Akad. Wiss. Berlin (Math. Phys.), 1917, 142
  2. S. J. Maddox, 1990, Mon. Not. R. Astron. Soc., 243, 692
  3. L. van Waerbeke, 2000, Astron. Astrophys., 358, 30
  4. 10.1093/mnras/stz2162 · DOI
  5. 10.3847/2041-8213/ab04fa · DOI
  6. 10.3847/1538-4357/aab9bb · DOI
  7. 10.3847/1538-4357/aab9bb · DOI
  8. 10.3847/1538-4357/aab9bb · DOI
  9. 10.1093/mnras/stx721 · DOI · Paper page
  10. R. A. C. Croft, 2015, Quarterly Phys. Rev., 1, 1

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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
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
DOI
10.1103/physrevd.105.023520
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
Licence
link.aps.org/licenses/aps-default-license (vor)
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

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