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

dc.contributor.authorChan, K. C.
dc.contributor.authorAvila, S.
dc.contributor.authorCarnero Rosell, A.
dc.contributor.authorFerrero, I.
dc.contributor.authorElvin-Poole, J.
dc.contributor.authorSanchez, E.
dc.contributor.authorCamacho, H. [UNESP]
dc.contributor.authorPorredon, A.
dc.contributor.authorCrocce, M.
dc.contributor.authorAbbott, T. M.C.
dc.contributor.authorAguena, M.
dc.contributor.authorAllam, S.
dc.contributor.authorAndrade-Oliveira, F.
dc.contributor.authorBertin, E.
dc.contributor.authorBocquet, S.
dc.contributor.authorBrooks, D.
dc.contributor.authorBurke, D. L.
dc.contributor.authorCarrasco Kind, M.
dc.contributor.authorCarretero, J.
dc.contributor.authorCastander, F. J.
dc.contributor.authorCawthon, R.
dc.contributor.authorConselice, C.
dc.contributor.authorCostanzi, M.
dc.contributor.authorPereira, M. E.S.
dc.contributor.authorDe Vicente, J.
dc.contributor.authorDesai, S.
dc.contributor.authorDiehl, H. T.
dc.contributor.authorDoel, P.
dc.contributor.authorEverett, S.
dc.contributor.authorFlaugher, B.
dc.contributor.authorFosalba, P.
dc.contributor.authorGarcía-Bellido, J.
dc.contributor.authorGaztanaga, E.
dc.contributor.authorGerdes, D. W.
dc.contributor.authorGiannantonio, T.
dc.contributor.authorGruen, D.
dc.contributor.authorGruendl, R. A.
dc.contributor.authorGutierrez, G.
dc.contributor.authorHinton, S. R.
dc.contributor.authorHollowood, D. L.
dc.contributor.authorHonscheid, K.
dc.contributor.authorHuterer, D.
dc.contributor.authorJames, D. J.
dc.contributor.authorKuehn, K.
dc.contributor.authorLahav, O.
dc.contributor.authorLidman, C.
dc.contributor.authorLima, M.
dc.contributor.authorMarshall, J. L.
dc.contributor.authorMena-Fernández, J.
dc.contributor.authorMenanteau, F.
dc.contributor.authorMiquel, R.
dc.contributor.authorPalmese, A.
dc.contributor.authorPaz-Chinchón, F.
dc.contributor.authorPieres, A.
dc.contributor.authorPlazas Malagón, A. A.
dc.contributor.authorRaveri, M.
dc.contributor.authorRodriguez-Monroy, M.
dc.contributor.authorRoodman, A.
dc.contributor.authorRoss, A. J.
dc.contributor.authorScarpine, V.
dc.contributor.authorSevilla-Noarbe, I.
dc.contributor.authorSmith, M.
dc.contributor.authorSuchyta, E.
dc.contributor.authorSwanson, M. E.C.
dc.contributor.authorTarle, G.
dc.contributor.authorThomas, D.
dc.contributor.authorTucker, D. L.
dc.contributor.authorVincenzi, M.
dc.contributor.authorWeaverdyck, N.
dc.contributor.institutionSun Yat-sen University
dc.contributor.institutionSYSU
dc.contributor.institutionUniversidad Autonoma de Madrid
dc.contributor.institutionUniversidad Autónoma de Madrid
dc.contributor.institutionInstituto de Astrofisica de Canarias
dc.contributor.institutionLaboratório Interinstitucional de E-Astronomia-LIneA
dc.contributor.institutionDpto. Astrofísica
dc.contributor.institutionUniversity of Oslo
dc.contributor.institutionThe Ohio State University
dc.contributor.institutionMedioambientales y Tecnológicas (CIEMAT)
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.contributor.institutionUniversity of Edinburgh
dc.contributor.institutionInstitut d'Estudis Espacials de Catalunya (IEEC)
dc.contributor.institutionCSIC)
dc.contributor.institutionNSF's National Optical-Infrared Astronomy Research Laboratory
dc.contributor.institutionFermi National Accelerator Laboratory
dc.contributor.institutionUniversity of Michigan
dc.contributor.institutionInstitut d'Astrophysique de Paris
dc.contributor.institutionLudwig-Maximilians-Universität
dc.contributor.institutionUniversity College London
dc.contributor.institutionStanford University
dc.contributor.institutionSLAC National Accelerator Laboratory
dc.contributor.institutionNational Center for Supercomputing Applications
dc.contributor.institutionUniversity of Illinois at Urbana-Champaign
dc.contributor.institutionThe Barcelona Institute of Science and Technology
dc.contributor.institutionWilliam Jewell College
dc.contributor.institutionUniversity of Manchester
dc.contributor.institutionSchool of Physics and Astronomy
dc.contributor.institutionUniversity of Trieste
dc.contributor.institutionINAF-Osservatorio Astronomico di Trieste
dc.contributor.institutionInstitute for Fundamental Physics of the Universe
dc.contributor.institutionUniversität Hamburg
dc.contributor.institutionIIT Hyderabad
dc.contributor.institutionCalifornia Institute of Technology
dc.contributor.institutionUniversity of Cambridge
dc.contributor.institutionUniversity of Queensland
dc.contributor.institutionSanta Cruz Institute for Particle Physics
dc.contributor.institutionCenter for Astrophysics and Harvard and Smithsonian
dc.contributor.institutionMacquarie University
dc.contributor.institutionLowell Observatory
dc.contributor.institutionThe Australian National University
dc.contributor.institutionAustralian National University
dc.contributor.institutionUniversidade de São Paulo (USP)
dc.contributor.institutionTexas A and M University
dc.contributor.institutionInstitució Catalana de Recerca i Estudis Avançats
dc.contributor.institution501 Campbell Hall
dc.contributor.institutionObservatório Nacional
dc.contributor.institutionPeyton Hall
dc.contributor.institutionUniversity of Pennsylvania
dc.contributor.institutionUniversity of Southampton
dc.contributor.institutionOak Ridge National Laboratory
dc.contributor.institutionUniversity of Portsmouth
dc.contributor.institutionLawrence Berkeley National Laboratory
dc.date.accessioned2023-07-29T13:32:08Z
dc.date.available2023-07-29T13:32:08Z
dc.date.issued2022-12-15
dc.description.abstractThe 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.en
dc.description.affiliationSchool of Physics and Astronomy Sun Yat-sen University, 2 Daxue Road, Tangjia
dc.description.affiliationCSST Science Center for the Guangdong-Hongkong-Macau Greater Bay Area SYSU
dc.description.affiliationInstituto de Fisica Teorica UAM/CSIC Universidad Autonoma de Madrid
dc.description.affiliationDepartamento de Física Teórica Universidad Autónoma de Madrid
dc.description.affiliationInstituto de Astrofisica de Canarias, Tenerife
dc.description.affiliationLaboratório Interinstitucional de E-Astronomia-LIneA, Rua Gal. José Cristino 77, RJ
dc.description.affiliationUniversidad de la Laguna Dpto. Astrofísica, Tenerife
dc.description.affiliationInstitute of Theoretical Astrophysics University of Oslo, P.O. Box 1029 Blindern
dc.description.affiliationCenter for Cosmology and Astro-Particle Physics The Ohio State University
dc.description.affiliationDepartment of Physics The Ohio State University
dc.description.affiliationCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)
dc.description.affiliationInstituto de Física Teórica Universidade Estadual Paulista
dc.description.affiliationInstitute for Astronomy University of Edinburgh
dc.description.affiliationInstitut d'Estudis Espacials de Catalunya (IEEC)
dc.description.affiliationInstitute of Space Sciences (ICE CSIC) Campus UAB, Carrer de Can Magrans, s/n
dc.description.affiliationCerro Tololo Inter-American Observatory NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603
dc.description.affiliationFermi National Accelerator Laboratory, P. O. Box 500
dc.description.affiliationDepartment of Physics University of Michigan
dc.description.affiliationCNRS UMR 7095 Institut d'Astrophysique de Paris
dc.description.affiliationSorbonne Universités UPMC Univ Paris 06 UMR 7095 Institut d'Astrophysique de Paris
dc.description.affiliationUniversity Observatory Faculty of Physics Ludwig-Maximilians-Universität, Scheinerstr. 1
dc.description.affiliationDepartment of Physics and Astronomy University College London, Gower Street
dc.description.affiliationKavli Institute for Particle Astrophysics and Cosmology Stanford University, P. O. Box 2450
dc.description.affiliationSLAC National Accelerator Laboratory
dc.description.affiliationCenter for Astrophysical Surveys National Center for Supercomputing Applications, 1205 West Clark St.
dc.description.affiliationDepartment of Astronomy University of Illinois at Urbana-Champaign, 1002 W. Green Street
dc.description.affiliationInstitut de Física d'Altes Energies (IFAE) The Barcelona Institute of Science and Technology Campus UAB, Bellaterra
dc.description.affiliationPhysics Department William Jewell College
dc.description.affiliationJodrell Bank Center for Astrophysics School of Physics and Astronomy University of Manchester, Oxford Road
dc.description.affiliationUniversity of Nottingham School of Physics and Astronomy
dc.description.affiliationAstronomy Unit Department of Physics University of Trieste, via Tiepolo 11
dc.description.affiliationINAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11
dc.description.affiliationInstitute for Fundamental Physics of the Universe, Via Beirut 2
dc.description.affiliationHamburger Sternwarte Universität Hamburg, Gojenbergsweg 112
dc.description.affiliationDepartment of Physics IIT Hyderabad, Telangana
dc.description.affiliationJet Propulsion Laboratory California Institute of Technology, 4800 Oak Grove Dr.
dc.description.affiliationDepartment of Astronomy University of Michigan
dc.description.affiliationInstitute of Astronomy University of Cambridge, Madingley Road
dc.description.affiliationKavli Institute for Cosmology University of Cambridge, Madingley Road
dc.description.affiliationSchool of Mathematics and Physics University of Queensland
dc.description.affiliationSanta Cruz Institute for Particle Physics
dc.description.affiliationCenter for Astrophysics and Harvard and Smithsonian, 60 Garden Street
dc.description.affiliationAustralian Astronomical Optics Macquarie University
dc.description.affiliationLowell Observatory, 1400 Mars Hill Rd
dc.description.affiliationCentre for Gravitational Astrophysics College of Science The Australian National University
dc.description.affiliationThe Research School of Astronomy and Astrophysics Australian National University
dc.description.affiliationDepartamento de Física Matemática Instituto de Física Universidade de São Paulo, CP 66318, SP
dc.description.affiliationGeorge P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy Department of Physics and Astronomy Texas A and M University
dc.description.affiliationInstitució Catalana de Recerca i Estudis Avançats
dc.description.affiliationDepartment of Astronomy University of California Berkeley 501 Campbell Hall
dc.description.affiliationObservatório Nacional, Rua Gal. José Cristino 77, RJ
dc.description.affiliationDepartment of Astrophysical Sciences Princeton University Peyton Hall
dc.description.affiliationDepartment of Physics and Astronomy University of Pennsylvania
dc.description.affiliationSchool of Physics and Astronomy University of Southampton
dc.description.affiliationComputer Science and Mathematics Division Oak Ridge National Laboratory
dc.description.affiliationInstitute of Cosmology and Gravitation University of Portsmouth
dc.description.affiliationLawrence Berkeley National Laboratory, 1 Cyclotron Road
dc.description.affiliationUnespInstituto de Física Teórica Universidade Estadual Paulista
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.106.123502
dc.identifier.citationPhysical Review D, v. 106, n. 12, 2022.
dc.identifier.doi10.1103/PhysRevD.106.123502
dc.identifier.issn2470-0029
dc.identifier.issn2470-0010
dc.identifier.scopus2-s2.0-85143737093
dc.identifier.urihttp://hdl.handle.net/11449/248014
dc.language.isoeng
dc.relation.ispartofPhysical Review D
dc.sourceScopus
dc.titleDark Energy Survey Year 3 results: Measurement of the baryon acoustic oscillations with three-dimensional clusteringen
dc.typeArtigo
dspace.entity.typePublication
unesp.author.orcid0000-0001-8757-408X 0000-0001-8757-408X[1]
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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