Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/341306
Full metadata record
DC FieldValueLanguage
dc.contributor.CRUESPUNIVERSIDADE ESTADUAL DE CAMPINASpt_BR
dc.contributor.authorunicampSanchez, Flávia Sobreirapt_BR
dc.typeArtigopt_BR
dc.titleDark Energy Survey year 1 results: methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functionspt_BR
dc.contributor.authorBaxter, E. J.pt_BR
dc.contributor.authorOmori, Y.pt_BR
dc.contributor.authorChang, C.pt_BR
dc.contributor.authorGiannantonio, T.pt_BR
dc.contributor.authorKirk, D.pt_BR
dc.contributor.authorKrause, E.pt_BR
dc.contributor.authorBlazek, J.pt_BR
dc.contributor.authorBleem, L.pt_BR
dc.contributor.authorChoi, A.pt_BR
dc.contributor.authorCrawford, T. M.pt_BR
dc.contributor.authorDodelson, S.pt_BR
dc.contributor.authorEifler, T. F.pt_BR
dc.contributor.authorFriedrich, O.pt_BR
dc.contributor.authorGruen, D.pt_BR
dc.contributor.authorHolder, G. P.pt_BR
dc.contributor.authorJain, B.pt_BR
dc.contributor.authorJarvis, M.pt_BR
dc.contributor.authorMacCrann, N.pt_BR
dc.contributor.authorNicola, A.pt_BR
dc.contributor.authorPandey, S.pt_BR
dc.contributor.authorPrat, J.pt_BR
dc.contributor.authorReichardt, C. L.pt_BR
dc.contributor.authorSamuroff, S.pt_BR
dc.contributor.authorSanchez, C.pt_BR
dc.contributor.authorSecco, L. F.pt_BR
dc.contributor.authorSheldon, E.pt_BR
dc.contributor.authorTroxel, M. A.pt_BR
dc.contributor.authorZuntz, J.pt_BR
dc.contributor.authorAbbott, T. M. C.pt_BR
dc.contributor.authorAbdalla, F. B.pt_BR
dc.contributor.authorAnnis, J.pt_BR
dc.contributor.authorAvila, S.pt_BR
dc.contributor.authorBechtol, K.pt_BR
dc.contributor.authorBenson, B. A.pt_BR
dc.contributor.authorBertin, E.pt_BR
dc.contributor.authorBrooks, D.pt_BR
dc.contributor.authorBuckley-Geer, E.pt_BR
dc.contributor.authorBurke, D. L.pt_BR
dc.contributor.authorRosell, A. C.pt_BR
dc.contributor.authorKind, M. C.pt_BR
dc.contributor.authorCarretero, J.pt_BR
dc.contributor.authorCastander, F. J.pt_BR
dc.contributor.authorCawthon, R.pt_BR
dc.contributor.authorCunha, C. E.pt_BR
dc.contributor.authorD'Andrea, C. B.pt_BR
dc.contributor.authorda Costa, L. N.pt_BR
dc.contributor.authorDavis, C.pt_BR
dc.contributor.authorDe Vicente, J.pt_BR
dc.contributor.authorDePoy, D. L.pt_BR
dc.contributor.authorDiehl, H. T.pt_BR
dc.contributor.authorDoel, P.pt_BR
dc.contributor.authorEstrada, J.pt_BR
dc.contributor.authorEvrard, A. E.pt_BR
dc.contributor.authorFlaugher, B.pt_BR
dc.contributor.authorFosalba, P.pt_BR
dc.contributor.authorFrieman, J.pt_BR
dc.contributor.authorGarcia-Bellido, J.pt_BR
dc.contributor.authorGaztanaga, E.pt_BR
dc.contributor.authorGerdes, D. W.pt_BR
dc.contributor.authorGruendl, R. R. A.pt_BR
dc.contributor.authorGschwend, J.pt_BR
dc.contributor.authorGutierrez, G.pt_BR
dc.contributor.authorHartley, W. G.pt_BR
dc.contributor.authorHollowood, D.pt_BR
dc.contributor.authorHoyle, B.pt_BR
dc.contributor.authorJames, D. J.pt_BR
dc.contributor.authorKent, S.pt_BR
dc.contributor.authorKuehn, K.pt_BR
dc.contributor.authorKuropatkin, N.pt_BR
dc.contributor.authorLahav, O.pt_BR
dc.contributor.authorLima, M.pt_BR
dc.contributor.authorMaia, M. A. G.pt_BR
dc.contributor.authorMarch, M.pt_BR
dc.contributor.authorMarshall, J. L.pt_BR
dc.contributor.authorMelchior, P.pt_BR
dc.contributor.authorMenanteau, F.pt_BR
dc.contributor.authorMiquel, R.pt_BR
dc.contributor.authorPlazas, A. A.pt_BR
dc.contributor.authorRoodman, A.pt_BR
dc.contributor.authorRykoff, E. S.pt_BR
dc.contributor.authorSanchez, E.pt_BR
dc.contributor.authorSchindler, R.pt_BR
dc.contributor.authorSchubnell, M.pt_BR
dc.contributor.authorSevilla-Noarbe, I.pt_BR
dc.contributor.authorSmith, M.pt_BR
dc.contributor.authorSmith, R. C.pt_BR
dc.contributor.authorSoares-Santos, M.pt_BR
dc.contributor.authorSobreira, F.pt_BR
dc.contributor.authorSuchyta, E.pt_BR
dc.contributor.authorSwanson, M. E. C.pt_BR
dc.contributor.authorTarle, G.pt_BR
dc.contributor.authorWalker, A. R.pt_BR
dc.contributor.authorWu, W. L. K.pt_BR
dc.contributor.authorWeller, J.pt_BR
dc.subjectGaláxiaspt_BR
dc.subjectCisalhamentopt_BR
dc.subject.otherlanguageGalaxiespt_BR
dc.subject.otherlanguageShear (Mechanics)pt_BR
dc.description.abstractOptical imaging surveys measure both the galaxy density and the gravitational lensing-induced shear fields across the sky. Recently, the Dark Energy Survey (DES) Collaboration used a joint fit to two-point correlations between these observables to place tight constraints on cosmology (T. M. C. Abbott et al. (Dark Energy Survey Collaboration), Phys. Rev. D 98, 043526 (2018)). In this work, we develop the methodology to extend the DES Year 1 joint probes analysis to include cross-correlations of the optical survey observables with gravitational lensing of the cosmic microwave background as measured by the South Pole Telescope (SPT) and Planck. Using simulated analyses, we show how the resulting set of five two-point functions increases the robustness of the cosmological constraints to systematic errors in galaxy lensing shear calibration. Additionally, we show that contamination of the SPT+Planck cosmic microwave background lensing map by the thermal Sunyaev-Zel'dovich effect is a potentially large source of systematic error for two-point function analyses but show that it can be reduced to acceptable levels in our analysis by masking clusters of galaxies and imposing angular scale cuts on the two-point functions. The methodology developed here will be applied to the analysis of data from the DES, the SPT, and Planck in a companion work.pt_BR
dc.relation.ispartofPhysical review. D, Covering particles, fields, gravitation, and cosmologypt_BR
dc.relation.ispartofabbreviationPhys. rev. Dpt_BR
dc.publisher.cityCollege Park, MDpt_BR
dc.publisher.countryEstados Unidospt_BR
dc.publisherAmerican Physical Societypt_BR
dc.date.issued2019pt_BR
dc.date.monthofcirculationJan.pt_BR
dc.language.isoengpt_BR
dc.description.volume99pt_BR
dc.description.issuenumber2pt_BR
dc.description.firstpage1pt_BR
dc.description.lastpage22pt_BR
dc.rightsabertopt_BR
dc.sourceWOSpt_BR
dc.identifier.issn2470-0010pt_BR
dc.identifier.eissn2470-0029pt_BR
dc.identifier.doi10.1103/PhysRevD.99.023508pt_BR
dc.identifier.urlhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.023508pt_BR
dc.description.sponsorshipFINANCIADORA DE ESTUDOS E PROJETOS - FINEPpt_BR
dc.description.sponsorshipFUNDAÇÃO CARLOS CHAGAS FILHO DE AMPARO À PESQUISA DO ESTADO DO RIO DE JANEIRO - FAPERJpt_BR
dc.description.sponsorshipCONSELHO NACIONAL DE DESENVOLVIMENTO CIENTÍFICO E TECNOLÓGICO - CNPQpt_BR
dc.description.sponsorship1FINEP - FINANCIADORA DE ESTUDOS E PROJETOSpt_BR
dc.description.sponsorship1FAPERJ - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DO RIO DE JANEIROpt_BR
dc.description.sponsorship1CNPQ - CONSELHO NACIONAL DE DESENVOLVIMENTO CIENTÍFICO E TECNOLÓGICOpt_BR
dc.description.sponsorship1MCTIC - MINISTÉRIO DA CIÊNCIA, TECNOLOGIA, INOVAÇÕES E COMUNICAÇÕESpt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.date.available2020-05-13T19:35:09Z-
dc.date.accessioned2020-05-13T19:35:09Z-
dc.description.provenanceMade available in DSpace on 2020-05-13T19:35:09Z (GMT). No. of bitstreams: 1 000455061600003.pdf: 1534611 bytes, checksum: 0b41570d14ad6d815e5134f1f035c1e9 (MD5) Previous issue date: 2019en
dc.identifier.urihttp://repositorio.unicamp.br/jspui/handle/REPOSIP/341306-
dc.contributor.departmentDepartamento de Raios Cósmicos e Cronologiapt_BR
dc.contributor.unidadeInstituto de Física "Gleb Wataghin"pt_BR
dc.identifier.source000455061600003pt_BR
dc.creator.orcid0000-0002-7822-0658pt_BR
dc.type.formArtigopt_BR
dc.identifier.articleid23508pt_BR
dc.description.sponsorNoteThe contour plots in this paper were made using CHAINCONSUMER7 [90]. E. B. is partially supported by the U.S. Department of Energy Grant No. DE-SC0007901. The Reichardt and Bianchini acknowledge support from the Australian Research Council's Future Fellowships scheme (Grant No. FT150100074). P.F. is funded by MINECO, Projects No. ESP2013-48274-C3-1-P, No. ESP2014-58384-C3-1-P, and No. ESP2015-66861-C3-1-R. E. R. is supported by DOE Grant No. DE-SC0015975 and by the Sloan Foundation, Grant No. FG-2016-6443. Support for D. G. was provided by NASA through Einstein Postdoctoral Fellowship Grant No. PF5-160138 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under Contract No. NAS8-03060. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology andAstro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, FINEP - FINANCIADORA DE ESTUDOS E PROJETOS, Fundacao Carlos Chagas Filho de Amparo 'a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico and the Ministerio da Ciencia, Tecnologia e Inovacao, the Deutsche Forschungsgemeinschaft, and the collaborating institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenossische Technische Hochschule Zurich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l'Espai, the Institut de Fisica d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universitat Munchen and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. This work is based in part on observations at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under Grants No. AYA2015-71825, No. ESP2015-88861, No. FPA2015-68048, No. SEV-2012-0234, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. Institut de Fisica d'Altes Energies is partially funded by the Centres de Recerca de Catalunya program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Program (Grant No. FP7/2007-2013) including ERC Grants No. 240672, No. 291329, and No. 306478. We acknowledge support from the Australian Research Council Centre of Excellence for All-sky Astrophysics, through Project No. CE110001020. The South Pole Telescope program is supported by the National Science Foundation through Grant No. PLR-1248097. Partial support is also provided by the NSF Physics Frontier Center Grant No. PHY-0114422 to the Kavli Institute of Cosmological Physics at the University of Chicago, the Kavli Foundation, and the Gordon and Betty Moore Foundation through Grant No. 947 to the University of Chicago. Argonne National Laboratory's work was supported under the U.S. Department of Energy Contract No. DE-AC02-06CH11357. This manuscript has been authored by Fermi Research Alliance, LLC, under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. The United States Government retains and the publisher, by accepting the article for publication, acknowledges that the United States Government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes.pt_BR
dc.description.sponsorNoteMCTIC - MINISTÉRIO DA CIÊNCIA, TECNOLOGIA, INOVAÇÕES E COMUNICAÇÕESpt_BR
Appears in Collections:IFGW - Artigos e Outros Documentos

Files in This Item:
File SizeFormat 
000455061600003.pdf1.5 MBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.