Dark Energy Survey Year 3 results: Measurement of the baryon acoustic oscillations with three-dimensional clustering

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Autor(es): dc.contributorSun Yat-sen University-
Autor(es): dc.contributorSYSU-
Autor(es): dc.contributorUniversidad Autonoma de Madrid-
Autor(es): dc.contributorUniversidad Autónoma de Madrid-
Autor(es): dc.contributorInstituto de Astrofisica de Canarias-
Autor(es): dc.contributorLaboratório Interinstitucional de E-Astronomia-LIneA-
Autor(es): dc.contributorDpto. Astrofísica-
Autor(es): dc.contributorUniversity of Oslo-
Autor(es): dc.contributorThe Ohio State University-
Autor(es): dc.contributorMedioambientales y Tecnológicas (CIEMAT)-
Autor(es): dc.contributorUniversidade Estadual Paulista (UNESP)-
Autor(es): dc.contributorUniversity of Edinburgh-
Autor(es): dc.contributorInstitut d'Estudis Espacials de Catalunya (IEEC)-
Autor(es): dc.contributorCSIC)-
Autor(es): dc.contributorNSF's National Optical-Infrared Astronomy Research Laboratory-
Autor(es): dc.contributorFermi National Accelerator Laboratory-
Autor(es): dc.contributorUniversity of Michigan-
Autor(es): dc.contributorInstitut d'Astrophysique de Paris-
Autor(es): dc.contributorLudwig-Maximilians-Universität-
Autor(es): dc.contributorUniversity College London-
Autor(es): dc.contributorStanford University-
Autor(es): dc.contributorSLAC National Accelerator Laboratory-
Autor(es): dc.contributorNational Center for Supercomputing Applications-
Autor(es): dc.contributorUniversity of Illinois at Urbana-Champaign-
Autor(es): dc.contributorThe Barcelona Institute of Science and Technology-
Autor(es): dc.contributorWilliam Jewell College-
Autor(es): dc.contributorUniversity of Manchester-
Autor(es): dc.contributorSchool of Physics and Astronomy-
Autor(es): dc.contributorUniversity of Trieste-
Autor(es): dc.contributorINAF-Osservatorio Astronomico di Trieste-
Autor(es): dc.contributorInstitute for Fundamental Physics of the Universe-
Autor(es): dc.contributorUniversität Hamburg-
Autor(es): dc.contributorIIT Hyderabad-
Autor(es): dc.contributorCalifornia Institute of Technology-
Autor(es): dc.contributorUniversity of Cambridge-
Autor(es): dc.contributorUniversity of Queensland-
Autor(es): dc.contributorSanta Cruz Institute for Particle Physics-
Autor(es): dc.contributorCenter for Astrophysics and Harvard and Smithsonian-
Autor(es): dc.contributorMacquarie University-
Autor(es): dc.contributorLowell Observatory-
Autor(es): dc.contributorThe Australian National University-
Autor(es): dc.contributorAustralian National University-
Autor(es): dc.contributorUniversidade de São Paulo (USP)-
Autor(es): dc.contributorTexas A and M University-
Autor(es): dc.contributorInstitució Catalana de Recerca i Estudis Avançats-
Autor(es): dc.contributor501 Campbell Hall-
Autor(es): dc.contributorObservatório Nacional-
Autor(es): dc.contributorPeyton Hall-
Autor(es): dc.contributorUniversity of Pennsylvania-
Autor(es): dc.contributorUniversity of Southampton-
Autor(es): dc.contributorOak Ridge National Laboratory-
Autor(es): dc.contributorUniversity of Portsmouth-
Autor(es): dc.contributorLawrence Berkeley National Laboratory-
Autor(es): dc.creatorChan, K. C.-
Autor(es): dc.creatorAvila, S.-
Autor(es): dc.creatorCarnero Rosell, A.-
Autor(es): dc.creatorFerrero, I.-
Autor(es): dc.creatorElvin-Poole, J.-
Autor(es): dc.creatorSanchez, E.-
Autor(es): dc.creatorCamacho, H.-
Autor(es): dc.creatorPorredon, A.-
Autor(es): dc.creatorCrocce, M.-
Autor(es): dc.creatorAbbott, T. M.C.-
Autor(es): dc.creatorAguena, M.-
Autor(es): dc.creatorAllam, S.-
Autor(es): dc.creatorAndrade-Oliveira, F.-
Autor(es): dc.creatorBertin, E.-
Autor(es): dc.creatorBocquet, S.-
Autor(es): dc.creatorBrooks, D.-
Autor(es): dc.creatorBurke, D. L.-
Autor(es): dc.creatorCarrasco Kind, M.-
Autor(es): dc.creatorCarretero, J.-
Autor(es): dc.creatorCastander, F. J.-
Autor(es): dc.creatorCawthon, R.-
Autor(es): dc.creatorConselice, C.-
Autor(es): dc.creatorCostanzi, M.-
Autor(es): dc.creatorPereira, M. E.S.-
Autor(es): dc.creatorDe Vicente, J.-
Autor(es): dc.creatorDesai, S.-
Autor(es): dc.creatorDiehl, H. T.-
Autor(es): dc.creatorDoel, P.-
Autor(es): dc.creatorEverett, S.-
Autor(es): dc.creatorFlaugher, B.-
Autor(es): dc.creatorFosalba, P.-
Autor(es): dc.creatorGarcía-Bellido, J.-
Autor(es): dc.creatorGaztanaga, E.-
Autor(es): dc.creatorGerdes, D. W.-
Autor(es): dc.creatorGiannantonio, T.-
Autor(es): dc.creatorGruen, D.-
Autor(es): dc.creatorGruendl, R. A.-
Autor(es): dc.creatorGutierrez, G.-
Autor(es): dc.creatorHinton, S. R.-
Autor(es): dc.creatorHollowood, D. L.-
Autor(es): dc.creatorHonscheid, K.-
Autor(es): dc.creatorHuterer, D.-
Autor(es): dc.creatorJames, D. J.-
Autor(es): dc.creatorKuehn, K.-
Autor(es): dc.creatorLahav, O.-
Autor(es): dc.creatorLidman, C.-
Autor(es): dc.creatorLima, M.-
Autor(es): dc.creatorMarshall, J. L.-
Autor(es): dc.creatorMena-Fernández, J.-
Autor(es): dc.creatorMenanteau, F.-
Autor(es): dc.creatorMiquel, R.-
Autor(es): dc.creatorPalmese, A.-
Autor(es): dc.creatorPaz-Chinchón, F.-
Autor(es): dc.creatorPieres, A.-
Autor(es): dc.creatorPlazas Malagón, A. A.-
Autor(es): dc.creatorRaveri, M.-
Autor(es): dc.creatorRodriguez-Monroy, M.-
Autor(es): dc.creatorRoodman, A.-
Autor(es): dc.creatorRoss, A. J.-
Autor(es): dc.creatorScarpine, V.-
Autor(es): dc.creatorSevilla-Noarbe, I.-
Autor(es): dc.creatorSmith, M.-
Autor(es): dc.creatorSuchyta, E.-
Autor(es): dc.creatorSwanson, M. E.C.-
Autor(es): dc.creatorTarle, G.-
Autor(es): dc.creatorThomas, D.-
Autor(es): dc.creatorTucker, D. L.-
Autor(es): dc.creatorVincenzi, M.-
Autor(es): dc.creatorWeaverdyck, N.-
Data de aceite: dc.date.accessioned2025-08-21T20:25:21Z-
Data de disponibilização: dc.date.available2025-08-21T20:25:21Z-
Data de envio: dc.date.issued2023-07-29-
Data de envio: dc.date.issued2023-07-29-
Data de envio: dc.date.issued2022-12-14-
Fonte completa do material: dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.106.123502-
Fonte completa do material: dc.identifierhttp://hdl.handle.net/11449/248014-
Fonte: dc.identifier.urihttp://educapes.capes.gov.br/handle/11449/248014-
Descrição: dc.descriptionThe three-dimensional correlation function offers an effective way to summarize the correlation of the large-scale structure even for imaging galaxy surveys. We have applied the projected three-dimensional correlation function, ζp to measure the baryonic acoustic oscillations (BAO) scale on the first-three years Dark Energy Survey data. The sample consists of about 7 million galaxies in the redshift range 0.6<zp<1.1 over a footprint of 4108 deg2. Our theory modeling includes the impact of realistic true redshift distributions beyond Gaussian photo-z approximation. ζp is obtained by projecting the three-dimensional correlation to the transverse direction. To increase the signal-to-noise of the measurements, we have considered a Gaussian stacking window function in place of the commonly used top-hat. ζp is sensitive to DM(zeff)/rs, the ratio between the comoving angular diameter distance and the sound horizon. Using the full sample, DM(zeff)/rs is constrained to be 19.00±0.67 (top-hat) and 19.15±0.58 (Gaussian) at zeff=0.835. The constraint is weaker than the angular correlation w constraint (18.84±0.50), and we trace this to the fact that the BAO signals are heterogeneous across redshift. While ζp responds to the heterogeneous signals by enlarging the error bar, w can still give a tight bound on DM/rs in this case. When a homogeneous BAO-signal subsample in the range 0.7<zp<1.0 (zeff=0.845) is considered, ζp yields 19.80±0.67 (top-hat) and 19.84±0.53 (Gaussian). The latter is mildly stronger than the w constraint (19.86±0.55). We find that the ζp results are more sensitive to photo-z errors than w because ζp keeps the three-dimensional clustering information causing it to be more prone to photo-z noise. The Gaussian window gives more robust results than the top-hat as the former is designed to suppress the low signal modes. ζp and the angular statistics such as w have their own pros and cons, and they serve an important crosscheck with each other.-
Descrição: dc.descriptionSchool of Physics and Astronomy Sun Yat-sen University, 2 Daxue Road, Tangjia-
Descrição: dc.descriptionCSST Science Center for the Guangdong-Hongkong-Macau Greater Bay Area SYSU-
Descrição: dc.descriptionInstituto de Fisica Teorica UAM/CSIC Universidad Autonoma de Madrid-
Descrição: dc.descriptionDepartamento de Física Teórica Universidad Autónoma de Madrid-
Descrição: dc.descriptionInstituto de Astrofisica de Canarias, Tenerife-
Descrição: dc.descriptionLaboratório Interinstitucional de E-Astronomia-LIneA, Rua Gal. José Cristino 77, RJ-
Descrição: dc.descriptionUniversidad de la Laguna Dpto. Astrofísica, Tenerife-
Descrição: dc.descriptionInstitute of Theoretical Astrophysics University of Oslo, P.O. Box 1029 Blindern-
Descrição: dc.descriptionCenter for Cosmology and Astro-Particle Physics The Ohio State University-
Descrição: dc.descriptionDepartment of Physics The Ohio State University-
Descrição: dc.descriptionCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)-
Descrição: dc.descriptionInstituto de Física Teórica Universidade Estadual Paulista-
Descrição: dc.descriptionInstitute for Astronomy University of Edinburgh-
Descrição: dc.descriptionInstitut d'Estudis Espacials de Catalunya (IEEC)-
Descrição: dc.descriptionInstitute of Space Sciences (ICE CSIC) Campus UAB, Carrer de Can Magrans, s/n-
Descrição: dc.descriptionCerro Tololo Inter-American Observatory NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603-
Descrição: dc.descriptionFermi National Accelerator Laboratory, P. O. Box 500-
Descrição: dc.descriptionDepartment of Physics University of Michigan-
Descrição: dc.descriptionCNRS UMR 7095 Institut d'Astrophysique de Paris-
Descrição: dc.descriptionSorbonne Universités UPMC Univ Paris 06 UMR 7095 Institut d'Astrophysique de Paris-
Descrição: dc.descriptionUniversity Observatory Faculty of Physics Ludwig-Maximilians-Universität, Scheinerstr. 1-
Descrição: dc.descriptionDepartment of Physics and Astronomy University College London, Gower Street-
Descrição: dc.descriptionKavli Institute for Particle Astrophysics and Cosmology Stanford University, P. O. Box 2450-
Descrição: dc.descriptionSLAC National Accelerator Laboratory-
Descrição: dc.descriptionCenter for Astrophysical Surveys National Center for Supercomputing Applications, 1205 West Clark St.-
Descrição: dc.descriptionDepartment of Astronomy University of Illinois at Urbana-Champaign, 1002 W. Green Street-
Descrição: dc.descriptionInstitut de Física d'Altes Energies (IFAE) The Barcelona Institute of Science and Technology Campus UAB, Bellaterra-
Descrição: dc.descriptionPhysics Department William Jewell College-
Descrição: dc.descriptionJodrell Bank Center for Astrophysics School of Physics and Astronomy University of Manchester, Oxford Road-
Descrição: dc.descriptionUniversity of Nottingham School of Physics and Astronomy-
Descrição: dc.descriptionAstronomy Unit Department of Physics University of Trieste, via Tiepolo 11-
Descrição: dc.descriptionINAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11-
Descrição: dc.descriptionInstitute for Fundamental Physics of the Universe, Via Beirut 2-
Descrição: dc.descriptionHamburger Sternwarte Universität Hamburg, Gojenbergsweg 112-
Descrição: dc.descriptionDepartment of Physics IIT Hyderabad, Telangana-
Descrição: dc.descriptionJet Propulsion Laboratory California Institute of Technology, 4800 Oak Grove Dr.-
Descrição: dc.descriptionDepartment of Astronomy University of Michigan-
Descrição: dc.descriptionInstitute of Astronomy University of Cambridge, Madingley Road-
Descrição: dc.descriptionKavli Institute for Cosmology University of Cambridge, Madingley Road-
Descrição: dc.descriptionSchool of Mathematics and Physics University of Queensland-
Descrição: dc.descriptionSanta Cruz Institute for Particle Physics-
Descrição: dc.descriptionCenter for Astrophysics and Harvard and Smithsonian, 60 Garden Street-
Descrição: dc.descriptionAustralian Astronomical Optics Macquarie University-
Descrição: dc.descriptionLowell Observatory, 1400 Mars Hill Rd-
Descrição: dc.descriptionCentre for Gravitational Astrophysics College of Science The Australian National University-
Descrição: dc.descriptionThe Research School of Astronomy and Astrophysics Australian National University-
Descrição: dc.descriptionDepartamento de Física Matemática Instituto de Física Universidade de São Paulo, CP 66318, SP-
Descrição: dc.descriptionGeorge P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy Department of Physics and Astronomy Texas A and M University-
Descrição: dc.descriptionInstitució Catalana de Recerca i Estudis Avançats-
Descrição: dc.descriptionDepartment of Astronomy University of California Berkeley 501 Campbell Hall-
Descrição: dc.descriptionObservatório Nacional, Rua Gal. José Cristino 77, RJ-
Descrição: dc.descriptionDepartment of Astrophysical Sciences Princeton University Peyton Hall-
Descrição: dc.descriptionDepartment of Physics and Astronomy University of Pennsylvania-
Descrição: dc.descriptionSchool of Physics and Astronomy University of Southampton-
Descrição: dc.descriptionComputer Science and Mathematics Division Oak Ridge National Laboratory-
Descrição: dc.descriptionInstitute of Cosmology and Gravitation University of Portsmouth-
Descrição: dc.descriptionLawrence Berkeley National Laboratory, 1 Cyclotron Road-
Descrição: dc.descriptionInstituto de Física Teórica Universidade Estadual Paulista-
Idioma: dc.languageen-
Relação: dc.relationPhysical Review D-
???dc.source???: dc.sourceScopus-
Título: dc.titleDark Energy Survey Year 3 results: Measurement of the baryon acoustic oscillations with three-dimensional clustering-
Tipo de arquivo: dc.typelivro digital-
Aparece nas coleções:Repositório Institucional - Unesp

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