Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty

Detalhes bibliográficos
Autor(a) principal: Secco, L. F.
Data de Publicação: 2022
Outros Autores: Samuroff, S., Krause, E., Jain, B., Blazek, J., Raveri, M., Campos, A., Amon, A., Chen, A., Doux, C., Choi, A., Gruen, D., Bernstein, G. M., Chang, C., Derose, J., Myles, J., Ferté, A., Lemos, P., Huterer, D., Prat, J., Troxel, M. A., Maccrann, N., Liddle, A. R., Kacprzak, T., Fang, X., Sánchez, C., Pandey, S., Dodelson, S., Chintalapati, P., Hoffmann, K., Alarcon, A., Alves, O. [UNESP], Andrade-Oliveira, F. [UNESP], Baxter, E. J., Bechtol, K., Becker, M. R., Brandao-Souza, A., Camacho, H. [UNESP], Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Cordero, J. P., Crocce, M., Davis, C., Di Valentino, E., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elidaiana, M., Elsner, F., Elvin-Poole, J., Everett, S., Fosalba, P., Friedrich, O., Gatti, M., Giannini, G., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Jarvis, M., Jeffrey, N., Kuropatkin, N., Leget, P. F., Muir, J., McCullough, J., Navarro Alsina, A., Omori, Y., Park, Y., Porredon, A., Rollins, R., Roodman, A., Rosenfeld, R. [UNESP], Ross, A. J., Rykoff, E. S., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E. S., Shin, T., Tutusaus, I., Varga, T. N., Weaverdyck, N., Wechsler, R. H., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M.C., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bhargava, S., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., Da Costa, L. N., De Vicente, J., Diehl, H. T., 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., Jeltema, T., 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., Plazas Malagón, A. A., Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Scolnic, D., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E.C., Tarle, G., Thomas, D., To, C.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.105.023515
http://hdl.handle.net/11449/230302
Resumo: This work and its companion paper, Amon et al. [Phys. Rev. D 105, 023514 (2022)PRVDAQ2470-001010.1103/PhysRevD.105.023514], present cosmic shear measurements and cosmological constraints from over 100 million source galaxies in the Dark Energy Survey (DES) Year 3 data. We constrain the lensing amplitude parameter S8σ8ωm/0.3 at the 3% level in ΛCDM: S8=0.759-0.023+0.025 (68% CL). Our constraint is at the 2% level when using angular scale cuts that are optimized for the ΛCDM analysis: S8=0.772-0.017+0.018 (68% CL). With cosmic shear alone, we find no statistically significant constraint on the dark energy equation-of-state parameter at our present statistical power. We carry out our analysis blind, and compare our measurement with constraints from two other contemporary weak lensing experiments: the Kilo-Degree Survey (KiDS) and Hyper-Suprime Camera Subaru Strategic Program (HSC). We additionally quantify the agreement between our data and external constraints from the Cosmic Microwave Background (CMB). Our DES Y3 result under the assumption of ΛCDM is found to be in statistical agreement with Planck 2018, although favors a lower S8 than the CMB-inferred value by 2.3σ (a p-value of 0.02). This paper explores the robustness of these cosmic shear results to modeling of intrinsic alignments, the matter power spectrum and baryonic physics. We additionally explore the statistical preference of our data for intrinsic alignment models of different complexity. The fiducial cosmic shear model is tested using synthetic data, and we report no biases greater than 0.3σ in the plane of S8×ωm caused by uncertainties in the theoretical models.
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spelling Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertaintyThis work and its companion paper, Amon et al. [Phys. Rev. D 105, 023514 (2022)PRVDAQ2470-001010.1103/PhysRevD.105.023514], present cosmic shear measurements and cosmological constraints from over 100 million source galaxies in the Dark Energy Survey (DES) Year 3 data. We constrain the lensing amplitude parameter S8σ8ωm/0.3 at the 3% level in ΛCDM: S8=0.759-0.023+0.025 (68% CL). Our constraint is at the 2% level when using angular scale cuts that are optimized for the ΛCDM analysis: S8=0.772-0.017+0.018 (68% CL). With cosmic shear alone, we find no statistically significant constraint on the dark energy equation-of-state parameter at our present statistical power. We carry out our analysis blind, and compare our measurement with constraints from two other contemporary weak lensing experiments: the Kilo-Degree Survey (KiDS) and Hyper-Suprime Camera Subaru Strategic Program (HSC). We additionally quantify the agreement between our data and external constraints from the Cosmic Microwave Background (CMB). Our DES Y3 result under the assumption of ΛCDM is found to be in statistical agreement with Planck 2018, although favors a lower S8 than the CMB-inferred value by 2.3σ (a p-value of 0.02). This paper explores the robustness of these cosmic shear results to modeling of intrinsic alignments, the matter power spectrum and baryonic physics. We additionally explore the statistical preference of our data for intrinsic alignment models of different complexity. The fiducial cosmic shear model is tested using synthetic data, and we report no biases greater than 0.3σ in the plane of S8×ωm caused by uncertainties in the theoretical models.Kavli Institute for Cosmological Physics University of ChicagoDepartment of Physics and Astronomy University of PennsylvaniaMcWilliams Center for Cosmology Department of Physics Carnegie Mellon UniversityDepartment of Physics Northeastern UniversityDepartment of Astronomy Steward Observatory University of Arizona, 933 North Cherry AvenueLaboratory of Astrophysics École Polytechnique Fédérale de Lausanne (EPFL)Kavli Institute for Particle Astrophysics and Cosmology Stanford University, P. O. Box 2450Department of Physics University of MichiganCenter for Cosmology and Astro-Particle Physics The Ohio State UniversityDepartment of Physics The Ohio State UniversityDepartment of Physics Stanford University 382 Via Pueblo MallSLAC National Accelerator LaboratoryBerkeley Center for Cosmological Physics University of California, CAJet Propulsion Laboratory California Institute of Technology, 4800 Oak Grove Dr.Department of Physics and Astronomy University College London, Gower StreetDepartment of Physics Duke UniversityDepartment of Applied Mathematics and Theoretical Physics University of CambridgeInstituto de Astrofísica e Ciências Do Espaço Faculdade de Ciências Universidade de LisboaInstitute for Astronomy University of EdinburghPerimeter Institute for Theoretical Physics, 31 Caroline Street NorthInstitute for Particle Physics and Astrophysics ETH Zürich, Wolfgang-Pauli-Strasse 27Department of Physics Northern Illinois UniversityInstitute for Computational Science University of Zürich, Winterthurerstr. 190Argonne National Laboratory, 9700 South Cass AvenueInstituto de Física Teórica Universidade Estadual PaulistaLaboratório Interinstitucional de E-Astronomia - LIneA, Rua Gal. José Cristino 77, RJInstitute for Astronomy University of Hawai'i, 2680 Woodlawn DrivePhysics Department 2320 Chamberlin Hall University of Wisconsin-Madison, 1150 University AvenueInstituto de Física Gleb Wataghin Universidade Estadual de Campinas, CampinasCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)Instituto de Astrofísica de Canarias, La LagunaUniversidad de la Laguna Dpto. Astrofísica, La LagunaDepartment of Astronomy University of Illinois at Urbana-Champaign, 1002 W. Green StreetNational Center for Supercomputing Applications, 1205 West Clark StreetJodrell Bank Centre for Astrophysics School of Physics and Astronomy University of Manchester, Oxford RoadInstitut d'Estudis Espacials de Catalunya (IEEC)Institute of Space Sciences (ICE CSIC) Campus UAB, Carrer de Can Magrans, s/nDepartment of Astronomy and Astrophysics University of ChicagoFermi National Accelerator Laboratory, P. O. Box 500Max Planck Institute für Extraterrestrial Physics, GiessenbachstrasseSanta Cruz Institute for Particle PhysicsInstitute of Astronomy University of Cambridge, Madingley RoadInstitut de Física d'Altes Energies (IFAE) The Barcelona Institute of Science and Technology Campus UAB, BellaterraDepartment of Physics University of Oxford Denys Wilkinson Building, Keble RoadDépartement de Physique Théorique Center for Astroparticle Physics Université de Genève, 24 quai Ernest AnsermetLaboratoire de Physique de l'Ecole Normale Supérieure ENS Université PSL CNRS Sorbonne Université Université de ParisUniversité Clermont Auvergne CNRS/IN2P3 Laboratoire de Physique de ClermontKavli Institute for Particle Astrophysics and Cosmology Department of Physics Stanford UniversityLPNHE CNRS/IN2P3 Sorbonne Université Paris Diderot Laboratoire de Physique Nucléaire et de Hautes ÉnergiesKavli Institute for the Physics and Mathematics of the Universe (WPI) UTIAS The University of Tokyo, KashiwaICTP South American Institute for Fundamental Research Instituto de Física Teórica Universidade Estadual PaulistaCenter for Cosmology and Astro-Particle Physics Ohio State UniversityBrookhaven National LaboratoryUniversitäts-Sternwarte Fakultät für Physik Ludwig-Maximilians Universität München, Scheinerstrasse 1Institute for Astronomy University of Edinburgh, Blackford HillCerro Tololo Inter-American Observatory NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603Institute of Cosmology and Gravitation University of PortsmouthCNRS UMR 7095 Institut d'Astrophysique de ParisSorbonne Universités UPMC Univ Paris 06 UMR 7095 Institut d'Astrophysique de ParisDepartment of Physics and Astronomy Pevensey Building University of SussexAstronomy Unit Department of Physics University of Trieste, via Tiepolo 11INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11Institute for Fundamental Physics of the Universe, Via Beirut 2Observatório Nacional, Rua Gal. José Cristino 77, RJFaculty of Physics Ludwig-Maximilians-Universität, Scheinerstrasse 1Institute of Theoretical Astrophysics University of Oslo, P.O. Box 1029 BlindernInstituto de Fisica Teorica UAM/CSIC Universidad Autonoma de MadridDepartment of Astronomy University of MichiganKavli Institute for Cosmology University of Cambridge, Madingley RoadSchool of Mathematics and Physics University of QueenslandMax Planck Institute for Extraterrestrial Physics, GiessenbachstrasseCenter for Astrophysics | Harvard and Smithsonian, 60 Garden StreetAustralian Astronomical Optics Macquarie UniversityLowell Observatory, 1400 Mars Hill RdDepartamento de Física Matemática Instituto de Física Universidade de São Paulo, CP 66318, SPGeorge P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy Department of Physics and Astronomy Texas A and M UniversityDepartment of Astronomy The Ohio State UniversityRadcliffe Institute for Advanced Study Harvard UniversityDepartment of Astrophysical Sciences Princeton University Peyton HallCenter for Astrophysical Surveys National Center for Supercomputing Applications, 1205 West Clark StreetInstitució Catalana de Recerca i Estudis AvançatsSchool of Physics and Astronomy University of SouthamptonComputer Science and Mathematics Division Oak Ridge National LaboratoryInstituto de Física Teórica Universidade Estadual PaulistaICTP South American Institute for Fundamental Research Instituto de Física Teórica Universidade Estadual PaulistaUniversity of ChicagoUniversity of PennsylvaniaCarnegie Mellon UniversityNortheastern UniversityUniversity of ArizonaÉcole Polytechnique Fédérale de Lausanne (EPFL)Stanford UniversityUniversity of MichiganThe Ohio State University382 Via Pueblo MallSLAC National Accelerator LaboratoryUniversity of CaliforniaCalifornia Institute of TechnologyUniversity College LondonDuke UniversityUniversity of CambridgeUniversidade de LisboaUniversity of EdinburghPerimeter Institute for Theoretical PhysicsETH ZürichNorthern Illinois UniversityUniversity of ZürichArgonne National LaboratoryUniversidade Estadual Paulista (UNESP)Laboratório Interinstitucional de E-Astronomia - LIneAUniversity of Hawai'iUniversity of Wisconsin-MadisonUniversidade Estadual de Campinas (UNICAMP)Medioambientales y Tecnológicas (CIEMAT)Instituto de Astrofísica de CanariasDpto. AstrofísicaUniversity of Illinois at Urbana-ChampaignNational Center for Supercomputing ApplicationsUniversity of ManchesterInstitut d'Estudis Espacials de Catalunya (IEEC)Institute of Space Sciences (ICE CSIC)Fermi National Accelerator LaboratoryMax Planck Institute für Extraterrestrial PhysicsSanta Cruz Institute for Particle PhysicsThe Barcelona Institute of Science and TechnologyDenys Wilkinson BuildingUniversité de GenèveUniversité de ParisLaboratoire de Physique de ClermontLaboratoire de Physique Nucléaire et de Hautes ÉnergiesThe University of TokyoOhio State UniversityBrookhaven National LaboratoryLudwig-Maximilians Universität MünchenNSF's National Optical-Infrared Astronomy Research LaboratoryUniversity of PortsmouthInstitut d'Astrophysique de ParisUniversity of SussexUniversity of TriesteINAF-Osservatorio Astronomico di TriesteInstitute for Fundamental Physics of the UniverseObservatório NacionalLudwig-Maximilians-UniversitätUniversity of OsloUniversidad Autonoma de MadridUniversity of QueenslandMax Planck Institute for Extraterrestrial PhysicsCenter for Astrophysics | Harvard and SmithsonianMacquarie UniversityLowell ObservatoryUniversidade de São Paulo (USP)Texas A and M UniversityHarvard UniversityPeyton HallInstitució Catalana de Recerca i Estudis AvançatsUniversity of SouthamptonOak Ridge National LaboratorySecco, L. F.Samuroff, S.Krause, E.Jain, B.Blazek, J.Raveri, M.Campos, A.Amon, A.Chen, A.Doux, C.Choi, A.Gruen, D.Bernstein, G. M.Chang, C.Derose, J.Myles, J.Ferté, A.Lemos, P.Huterer, D.Prat, J.Troxel, M. A.Maccrann, N.Liddle, A. R.Kacprzak, T.Fang, X.Sánchez, C.Pandey, S.Dodelson, S.Chintalapati, P.Hoffmann, K.Alarcon, A.Alves, O. [UNESP]Andrade-Oliveira, F. [UNESP]Baxter, E. J.Bechtol, K.Becker, M. R.Brandao-Souza, A.Camacho, H. [UNESP]Carnero Rosell, A.Carrasco Kind, M.Cawthon, R.Cordero, J. P.Crocce, M.Davis, C.Di Valentino, E.Drlica-Wagner, A.Eckert, K.Eifler, T. F.Elidaiana, M.Elsner, F.Elvin-Poole, J.Everett, S.Fosalba, P.Friedrich, O.Gatti, M.Giannini, G.Gruendl, R. A.Harrison, I.Hartley, W. G.Herner, K.Huang, H.Huff, E. M.Jarvis, M.Jeffrey, N.Kuropatkin, N.Leget, P. F.Muir, J.McCullough, J.Navarro Alsina, A.Omori, Y.Park, Y.Porredon, A.Rollins, R.Roodman, A.Rosenfeld, R. [UNESP]Ross, A. J.Rykoff, E. S.Sanchez, J.Sevilla-Noarbe, I.Sheldon, E. S.Shin, T.Tutusaus, I.Varga, T. N.Weaverdyck, N.Wechsler, R. H.Yanny, B.Yin, B.Zhang, Y.Zuntz, J.Abbott, T. M.C.Aguena, M.Allam, S.Annis, J.Bacon, D.Bertin, E.Bhargava, S.Bridle, S. L.Brooks, D.Buckley-Geer, E.Burke, D. L.Carretero, J.Costanzi, M.Da Costa, L. N.De Vicente, J.Diehl, H. T.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.Jeltema, T.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.Plazas Malagón, A. A.Rodriguez-Monroy, M.Romer, A. K.Sanchez, E.Scarpine, V.Schubnell, M.Scolnic, D.Serrano, S.Smith, M.Soares-Santos, M.Suchyta, E.Swanson, M. E.C.Tarle, G.Thomas, D.To, C.2022-04-29T08:39:05Z2022-04-29T08:39:05Z2022-01-15info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.105.023515Physical Review D, v. 105, n. 2, 2022.2470-00292470-0010http://hdl.handle.net/11449/23030210.1103/PhysRevD.105.0235152-s2.0-85123757043Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-29T08:39:09Zoai:repositorio.unesp.br:11449/230302Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T16:19:20.785255Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
title Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
spellingShingle Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
Secco, L. F.
title_short Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
title_full Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
title_fullStr Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
title_full_unstemmed Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
title_sort Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
author Secco, L. F.
author_facet Secco, L. F.
Samuroff, S.
Krause, E.
Jain, B.
Blazek, J.
Raveri, M.
Campos, A.
Amon, A.
Chen, A.
Doux, C.
Choi, A.
Gruen, D.
Bernstein, G. M.
Chang, C.
Derose, J.
Myles, J.
Ferté, A.
Lemos, P.
Huterer, D.
Prat, J.
Troxel, M. A.
Maccrann, N.
Liddle, A. R.
Kacprzak, T.
Fang, X.
Sánchez, C.
Pandey, S.
Dodelson, S.
Chintalapati, P.
Hoffmann, K.
Alarcon, A.
Alves, O. [UNESP]
Andrade-Oliveira, F. [UNESP]
Baxter, E. J.
Bechtol, K.
Becker, M. R.
Brandao-Souza, A.
Camacho, H. [UNESP]
Carnero Rosell, A.
Carrasco Kind, M.
Cawthon, R.
Cordero, J. P.
Crocce, M.
Davis, C.
Di Valentino, E.
Drlica-Wagner, A.
Eckert, K.
Eifler, T. F.
Elidaiana, M.
Elsner, F.
Elvin-Poole, J.
Everett, S.
Fosalba, P.
Friedrich, O.
Gatti, M.
Giannini, G.
Gruendl, R. A.
Harrison, I.
Hartley, W. G.
Herner, K.
Huang, H.
Huff, E. M.
Jarvis, M.
Jeffrey, N.
Kuropatkin, N.
Leget, P. F.
Muir, J.
McCullough, J.
Navarro Alsina, A.
Omori, Y.
Park, Y.
Porredon, A.
Rollins, R.
Roodman, A.
Rosenfeld, R. [UNESP]
Ross, A. J.
Rykoff, E. S.
Sanchez, J.
Sevilla-Noarbe, I.
Sheldon, E. S.
Shin, T.
Tutusaus, I.
Varga, T. N.
Weaverdyck, N.
Wechsler, R. H.
Yanny, B.
Yin, B.
Zhang, Y.
Zuntz, J.
Abbott, T. M.C.
Aguena, M.
Allam, S.
Annis, J.
Bacon, D.
Bertin, E.
Bhargava, S.
Bridle, S. L.
Brooks, D.
Buckley-Geer, E.
Burke, D. L.
Carretero, J.
Costanzi, M.
Da Costa, L. N.
De Vicente, J.
Diehl, H. T.
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.
Jeltema, T.
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.
Plazas Malagón, A. A.
Rodriguez-Monroy, M.
Romer, A. K.
Sanchez, E.
Scarpine, V.
Schubnell, M.
Scolnic, D.
Serrano, S.
Smith, M.
Soares-Santos, M.
Suchyta, E.
Swanson, M. E.C.
Tarle, G.
Thomas, D.
To, C.
author_role author
author2 Samuroff, S.
Krause, E.
Jain, B.
Blazek, J.
Raveri, M.
Campos, A.
Amon, A.
Chen, A.
Doux, C.
Choi, A.
Gruen, D.
Bernstein, G. M.
Chang, C.
Derose, J.
Myles, J.
Ferté, A.
Lemos, P.
Huterer, D.
Prat, J.
Troxel, M. A.
Maccrann, N.
Liddle, A. R.
Kacprzak, T.
Fang, X.
Sánchez, C.
Pandey, S.
Dodelson, S.
Chintalapati, P.
Hoffmann, K.
Alarcon, A.
Alves, O. [UNESP]
Andrade-Oliveira, F. [UNESP]
Baxter, E. J.
Bechtol, K.
Becker, M. R.
Brandao-Souza, A.
Camacho, H. [UNESP]
Carnero Rosell, A.
Carrasco Kind, M.
Cawthon, R.
Cordero, J. P.
Crocce, M.
Davis, C.
Di Valentino, E.
Drlica-Wagner, A.
Eckert, K.
Eifler, T. F.
Elidaiana, M.
Elsner, F.
Elvin-Poole, J.
Everett, S.
Fosalba, P.
Friedrich, O.
Gatti, M.
Giannini, G.
Gruendl, R. A.
Harrison, I.
Hartley, W. G.
Herner, K.
Huang, H.
Huff, E. M.
Jarvis, M.
Jeffrey, N.
Kuropatkin, N.
Leget, P. F.
Muir, J.
McCullough, J.
Navarro Alsina, A.
Omori, Y.
Park, Y.
Porredon, A.
Rollins, R.
Roodman, A.
Rosenfeld, R. [UNESP]
Ross, A. J.
Rykoff, E. S.
Sanchez, J.
Sevilla-Noarbe, I.
Sheldon, E. S.
Shin, T.
Tutusaus, I.
Varga, T. N.
Weaverdyck, N.
Wechsler, R. H.
Yanny, B.
Yin, B.
Zhang, Y.
Zuntz, J.
Abbott, T. M.C.
Aguena, M.
Allam, S.
Annis, J.
Bacon, D.
Bertin, E.
Bhargava, S.
Bridle, S. L.
Brooks, D.
Buckley-Geer, E.
Burke, D. L.
Carretero, J.
Costanzi, M.
Da Costa, L. N.
De Vicente, J.
Diehl, H. T.
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.
Jeltema, T.
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.
Plazas Malagón, A. A.
Rodriguez-Monroy, M.
Romer, A. K.
Sanchez, E.
Scarpine, V.
Schubnell, M.
Scolnic, D.
Serrano, S.
Smith, M.
Soares-Santos, M.
Suchyta, E.
Swanson, M. E.C.
Tarle, G.
Thomas, D.
To, C.
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dc.contributor.none.fl_str_mv University of Chicago
University of Pennsylvania
Carnegie Mellon University
Northeastern University
University of Arizona
École Polytechnique Fédérale de Lausanne (EPFL)
Stanford University
University of Michigan
The Ohio State University
382 Via Pueblo Mall
SLAC National Accelerator Laboratory
University of California
California Institute of Technology
University College London
Duke University
University of Cambridge
Universidade de Lisboa
University of Edinburgh
Perimeter Institute for Theoretical Physics
ETH Zürich
Northern Illinois University
University of Zürich
Argonne National Laboratory
Universidade Estadual Paulista (UNESP)
Laboratório Interinstitucional de E-Astronomia - LIneA
University of Hawai'i
University of Wisconsin-Madison
Universidade Estadual de Campinas (UNICAMP)
Medioambientales y Tecnológicas (CIEMAT)
Instituto de Astrofísica de Canarias
Dpto. Astrofísica
University of Illinois at Urbana-Champaign
National Center for Supercomputing Applications
University of Manchester
Institut d'Estudis Espacials de Catalunya (IEEC)
Institute of Space Sciences (ICE CSIC)
Fermi National Accelerator Laboratory
Max Planck Institute für Extraterrestrial Physics
Santa Cruz Institute for Particle Physics
The Barcelona Institute of Science and Technology
Denys Wilkinson Building
Université de Genève
Université de Paris
Laboratoire de Physique de Clermont
Laboratoire de Physique Nucléaire et de Hautes Énergies
The University of Tokyo
Ohio State University
Brookhaven National Laboratory
Ludwig-Maximilians Universität München
NSF's National Optical-Infrared Astronomy Research Laboratory
University of Portsmouth
Institut d'Astrophysique de Paris
University of Sussex
University of Trieste
INAF-Osservatorio Astronomico di Trieste
Institute for Fundamental Physics of the Universe
Observatório Nacional
Ludwig-Maximilians-Universität
University of Oslo
Universidad Autonoma de Madrid
University of Queensland
Max Planck Institute for Extraterrestrial Physics
Center for Astrophysics | Harvard and Smithsonian
Macquarie University
Lowell Observatory
Universidade de São Paulo (USP)
Texas A and M University
Harvard University
Peyton Hall
Institució Catalana de Recerca i Estudis Avançats
University of Southampton
Oak Ridge National Laboratory
dc.contributor.author.fl_str_mv Secco, L. F.
Samuroff, S.
Krause, E.
Jain, B.
Blazek, J.
Raveri, M.
Campos, A.
Amon, A.
Chen, A.
Doux, C.
Choi, A.
Gruen, D.
Bernstein, G. M.
Chang, C.
Derose, J.
Myles, J.
Ferté, A.
Lemos, P.
Huterer, D.
Prat, J.
Troxel, M. A.
Maccrann, N.
Liddle, A. R.
Kacprzak, T.
Fang, X.
Sánchez, C.
Pandey, S.
Dodelson, S.
Chintalapati, P.
Hoffmann, K.
Alarcon, A.
Alves, O. [UNESP]
Andrade-Oliveira, F. [UNESP]
Baxter, E. J.
Bechtol, K.
Becker, M. R.
Brandao-Souza, A.
Camacho, H. [UNESP]
Carnero Rosell, A.
Carrasco Kind, M.
Cawthon, R.
Cordero, J. P.
Crocce, M.
Davis, C.
Di Valentino, E.
Drlica-Wagner, A.
Eckert, K.
Eifler, T. F.
Elidaiana, M.
Elsner, F.
Elvin-Poole, J.
Everett, S.
Fosalba, P.
Friedrich, O.
Gatti, M.
Giannini, G.
Gruendl, R. A.
Harrison, I.
Hartley, W. G.
Herner, K.
Huang, H.
Huff, E. M.
Jarvis, M.
Jeffrey, N.
Kuropatkin, N.
Leget, P. F.
Muir, J.
McCullough, J.
Navarro Alsina, A.
Omori, Y.
Park, Y.
Porredon, A.
Rollins, R.
Roodman, A.
Rosenfeld, R. [UNESP]
Ross, A. J.
Rykoff, E. S.
Sanchez, J.
Sevilla-Noarbe, I.
Sheldon, E. S.
Shin, T.
Tutusaus, I.
Varga, T. N.
Weaverdyck, N.
Wechsler, R. H.
Yanny, B.
Yin, B.
Zhang, Y.
Zuntz, J.
Abbott, T. M.C.
Aguena, M.
Allam, S.
Annis, J.
Bacon, D.
Bertin, E.
Bhargava, S.
Bridle, S. L.
Brooks, D.
Buckley-Geer, E.
Burke, D. L.
Carretero, J.
Costanzi, M.
Da Costa, L. N.
De Vicente, J.
Diehl, H. T.
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.
Jeltema, T.
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.
Plazas Malagón, A. A.
Rodriguez-Monroy, M.
Romer, A. K.
Sanchez, E.
Scarpine, V.
Schubnell, M.
Scolnic, D.
Serrano, S.
Smith, M.
Soares-Santos, M.
Suchyta, E.
Swanson, M. E.C.
Tarle, G.
Thomas, D.
To, C.
description This work and its companion paper, Amon et al. [Phys. Rev. D 105, 023514 (2022)PRVDAQ2470-001010.1103/PhysRevD.105.023514], present cosmic shear measurements and cosmological constraints from over 100 million source galaxies in the Dark Energy Survey (DES) Year 3 data. We constrain the lensing amplitude parameter S8σ8ωm/0.3 at the 3% level in ΛCDM: S8=0.759-0.023+0.025 (68% CL). Our constraint is at the 2% level when using angular scale cuts that are optimized for the ΛCDM analysis: S8=0.772-0.017+0.018 (68% CL). With cosmic shear alone, we find no statistically significant constraint on the dark energy equation-of-state parameter at our present statistical power. We carry out our analysis blind, and compare our measurement with constraints from two other contemporary weak lensing experiments: the Kilo-Degree Survey (KiDS) and Hyper-Suprime Camera Subaru Strategic Program (HSC). We additionally quantify the agreement between our data and external constraints from the Cosmic Microwave Background (CMB). Our DES Y3 result under the assumption of ΛCDM is found to be in statistical agreement with Planck 2018, although favors a lower S8 than the CMB-inferred value by 2.3σ (a p-value of 0.02). This paper explores the robustness of these cosmic shear results to modeling of intrinsic alignments, the matter power spectrum and baryonic physics. We additionally explore the statistical preference of our data for intrinsic alignment models of different complexity. The fiducial cosmic shear model is tested using synthetic data, and we report no biases greater than 0.3σ in the plane of S8×ωm caused by uncertainties in the theoretical models.
publishDate 2022
dc.date.none.fl_str_mv 2022-04-29T08:39:05Z
2022-04-29T08:39:05Z
2022-01-15
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.105.023515
Physical Review D, v. 105, n. 2, 2022.
2470-0029
2470-0010
http://hdl.handle.net/11449/230302
10.1103/PhysRevD.105.023515
2-s2.0-85123757043
url http://dx.doi.org/10.1103/PhysRevD.105.023515
http://hdl.handle.net/11449/230302
identifier_str_mv Physical Review D, v. 105, n. 2, 2022.
2470-0029
2470-0010
10.1103/PhysRevD.105.023515
2-s2.0-85123757043
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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