Publicação: Dark Energy Survey Year 3 results: Measurement of the baryon acoustic oscillations with three-dimensional clustering
dc.contributor.author | Chan, K. C. | |
dc.contributor.author | Avila, S. | |
dc.contributor.author | Carnero Rosell, A. | |
dc.contributor.author | Ferrero, I. | |
dc.contributor.author | Elvin-Poole, J. | |
dc.contributor.author | Sanchez, E. | |
dc.contributor.author | Camacho, H. [UNESP] | |
dc.contributor.author | Porredon, A. | |
dc.contributor.author | Crocce, M. | |
dc.contributor.author | Abbott, T. M.C. | |
dc.contributor.author | Aguena, M. | |
dc.contributor.author | Allam, S. | |
dc.contributor.author | Andrade-Oliveira, F. | |
dc.contributor.author | Bertin, E. | |
dc.contributor.author | Bocquet, S. | |
dc.contributor.author | Brooks, D. | |
dc.contributor.author | Burke, D. L. | |
dc.contributor.author | Carrasco Kind, M. | |
dc.contributor.author | Carretero, J. | |
dc.contributor.author | Castander, F. J. | |
dc.contributor.author | Cawthon, R. | |
dc.contributor.author | Conselice, C. | |
dc.contributor.author | Costanzi, M. | |
dc.contributor.author | Pereira, M. E.S. | |
dc.contributor.author | De Vicente, J. | |
dc.contributor.author | Desai, S. | |
dc.contributor.author | Diehl, H. T. | |
dc.contributor.author | Doel, P. | |
dc.contributor.author | Everett, S. | |
dc.contributor.author | Flaugher, B. | |
dc.contributor.author | Fosalba, P. | |
dc.contributor.author | García-Bellido, J. | |
dc.contributor.author | Gaztanaga, E. | |
dc.contributor.author | Gerdes, D. W. | |
dc.contributor.author | Giannantonio, T. | |
dc.contributor.author | Gruen, D. | |
dc.contributor.author | Gruendl, R. A. | |
dc.contributor.author | Gutierrez, G. | |
dc.contributor.author | Hinton, S. R. | |
dc.contributor.author | Hollowood, D. L. | |
dc.contributor.author | Honscheid, K. | |
dc.contributor.author | Huterer, D. | |
dc.contributor.author | James, D. J. | |
dc.contributor.author | Kuehn, K. | |
dc.contributor.author | Lahav, O. | |
dc.contributor.author | Lidman, C. | |
dc.contributor.author | Lima, M. | |
dc.contributor.author | Marshall, J. L. | |
dc.contributor.author | Mena-Fernández, J. | |
dc.contributor.author | Menanteau, F. | |
dc.contributor.author | Miquel, R. | |
dc.contributor.author | Palmese, A. | |
dc.contributor.author | Paz-Chinchón, F. | |
dc.contributor.author | Pieres, A. | |
dc.contributor.author | Plazas Malagón, A. A. | |
dc.contributor.author | Raveri, M. | |
dc.contributor.author | Rodriguez-Monroy, M. | |
dc.contributor.author | Roodman, A. | |
dc.contributor.author | Ross, A. J. | |
dc.contributor.author | Scarpine, V. | |
dc.contributor.author | Sevilla-Noarbe, I. | |
dc.contributor.author | Smith, M. | |
dc.contributor.author | Suchyta, E. | |
dc.contributor.author | Swanson, M. E.C. | |
dc.contributor.author | Tarle, G. | |
dc.contributor.author | Thomas, D. | |
dc.contributor.author | Tucker, D. L. | |
dc.contributor.author | Vincenzi, M. | |
dc.contributor.author | Weaverdyck, N. | |
dc.contributor.institution | Sun Yat-sen University | |
dc.contributor.institution | SYSU | |
dc.contributor.institution | Universidad Autonoma de Madrid | |
dc.contributor.institution | Universidad Autónoma de Madrid | |
dc.contributor.institution | Instituto de Astrofisica de Canarias | |
dc.contributor.institution | Laboratório Interinstitucional de E-Astronomia-LIneA | |
dc.contributor.institution | Dpto. Astrofísica | |
dc.contributor.institution | University of Oslo | |
dc.contributor.institution | The Ohio State University | |
dc.contributor.institution | Medioambientales y Tecnológicas (CIEMAT) | |
dc.contributor.institution | Universidade Estadual Paulista (UNESP) | |
dc.contributor.institution | University of Edinburgh | |
dc.contributor.institution | Institut d'Estudis Espacials de Catalunya (IEEC) | |
dc.contributor.institution | CSIC) | |
dc.contributor.institution | NSF's National Optical-Infrared Astronomy Research Laboratory | |
dc.contributor.institution | Fermi National Accelerator Laboratory | |
dc.contributor.institution | University of Michigan | |
dc.contributor.institution | Institut d'Astrophysique de Paris | |
dc.contributor.institution | Ludwig-Maximilians-Universität | |
dc.contributor.institution | University College London | |
dc.contributor.institution | Stanford University | |
dc.contributor.institution | SLAC National Accelerator Laboratory | |
dc.contributor.institution | National Center for Supercomputing Applications | |
dc.contributor.institution | University of Illinois at Urbana-Champaign | |
dc.contributor.institution | The Barcelona Institute of Science and Technology | |
dc.contributor.institution | William Jewell College | |
dc.contributor.institution | University of Manchester | |
dc.contributor.institution | School of Physics and Astronomy | |
dc.contributor.institution | University of Trieste | |
dc.contributor.institution | INAF-Osservatorio Astronomico di Trieste | |
dc.contributor.institution | Institute for Fundamental Physics of the Universe | |
dc.contributor.institution | Universität Hamburg | |
dc.contributor.institution | IIT Hyderabad | |
dc.contributor.institution | California Institute of Technology | |
dc.contributor.institution | University of Cambridge | |
dc.contributor.institution | University of Queensland | |
dc.contributor.institution | Santa Cruz Institute for Particle Physics | |
dc.contributor.institution | Center for Astrophysics and Harvard and Smithsonian | |
dc.contributor.institution | Macquarie University | |
dc.contributor.institution | Lowell Observatory | |
dc.contributor.institution | The Australian National University | |
dc.contributor.institution | Australian National University | |
dc.contributor.institution | Universidade de São Paulo (USP) | |
dc.contributor.institution | Texas A and M University | |
dc.contributor.institution | Institució Catalana de Recerca i Estudis Avançats | |
dc.contributor.institution | 501 Campbell Hall | |
dc.contributor.institution | Observatório Nacional | |
dc.contributor.institution | Peyton Hall | |
dc.contributor.institution | University of Pennsylvania | |
dc.contributor.institution | University of Southampton | |
dc.contributor.institution | Oak Ridge National Laboratory | |
dc.contributor.institution | University of Portsmouth | |
dc.contributor.institution | Lawrence Berkeley National Laboratory | |
dc.date.accessioned | 2023-07-29T13:32:08Z | |
dc.date.available | 2023-07-29T13:32:08Z | |
dc.date.issued | 2022-12-15 | |
dc.description.abstract | The 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.affiliation | School of Physics and Astronomy Sun Yat-sen University, 2 Daxue Road, Tangjia | |
dc.description.affiliation | CSST Science Center for the Guangdong-Hongkong-Macau Greater Bay Area SYSU | |
dc.description.affiliation | Instituto de Fisica Teorica UAM/CSIC Universidad Autonoma de Madrid | |
dc.description.affiliation | Departamento de Física Teórica Universidad Autónoma de Madrid | |
dc.description.affiliation | Instituto de Astrofisica de Canarias, Tenerife | |
dc.description.affiliation | Laboratório Interinstitucional de E-Astronomia-LIneA, Rua Gal. José Cristino 77, RJ | |
dc.description.affiliation | Universidad de la Laguna Dpto. Astrofísica, Tenerife | |
dc.description.affiliation | Institute of Theoretical Astrophysics University of Oslo, P.O. Box 1029 Blindern | |
dc.description.affiliation | Center for Cosmology and Astro-Particle Physics The Ohio State University | |
dc.description.affiliation | Department of Physics The Ohio State University | |
dc.description.affiliation | Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT) | |
dc.description.affiliation | Instituto de Física Teórica Universidade Estadual Paulista | |
dc.description.affiliation | Institute for Astronomy University of Edinburgh | |
dc.description.affiliation | Institut d'Estudis Espacials de Catalunya (IEEC) | |
dc.description.affiliation | Institute of Space Sciences (ICE CSIC) Campus UAB, Carrer de Can Magrans, s/n | |
dc.description.affiliation | Cerro Tololo Inter-American Observatory NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603 | |
dc.description.affiliation | Fermi National Accelerator Laboratory, P. O. Box 500 | |
dc.description.affiliation | Department of Physics University of Michigan | |
dc.description.affiliation | CNRS UMR 7095 Institut d'Astrophysique de Paris | |
dc.description.affiliation | Sorbonne Universités UPMC Univ Paris 06 UMR 7095 Institut d'Astrophysique de Paris | |
dc.description.affiliation | University Observatory Faculty of Physics Ludwig-Maximilians-Universität, Scheinerstr. 1 | |
dc.description.affiliation | Department of Physics and Astronomy University College London, Gower Street | |
dc.description.affiliation | Kavli Institute for Particle Astrophysics and Cosmology Stanford University, P. O. Box 2450 | |
dc.description.affiliation | SLAC National Accelerator Laboratory | |
dc.description.affiliation | Center for Astrophysical Surveys National Center for Supercomputing Applications, 1205 West Clark St. | |
dc.description.affiliation | Department of Astronomy University of Illinois at Urbana-Champaign, 1002 W. Green Street | |
dc.description.affiliation | Institut de Física d'Altes Energies (IFAE) The Barcelona Institute of Science and Technology Campus UAB, Bellaterra | |
dc.description.affiliation | Physics Department William Jewell College | |
dc.description.affiliation | Jodrell Bank Center for Astrophysics School of Physics and Astronomy University of Manchester, Oxford Road | |
dc.description.affiliation | University of Nottingham School of Physics and Astronomy | |
dc.description.affiliation | Astronomy Unit Department of Physics University of Trieste, via Tiepolo 11 | |
dc.description.affiliation | INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11 | |
dc.description.affiliation | Institute for Fundamental Physics of the Universe, Via Beirut 2 | |
dc.description.affiliation | Hamburger Sternwarte Universität Hamburg, Gojenbergsweg 112 | |
dc.description.affiliation | Department of Physics IIT Hyderabad, Telangana | |
dc.description.affiliation | Jet Propulsion Laboratory California Institute of Technology, 4800 Oak Grove Dr. | |
dc.description.affiliation | Department of Astronomy University of Michigan | |
dc.description.affiliation | Institute of Astronomy University of Cambridge, Madingley Road | |
dc.description.affiliation | Kavli Institute for Cosmology University of Cambridge, Madingley Road | |
dc.description.affiliation | School of Mathematics and Physics University of Queensland | |
dc.description.affiliation | Santa Cruz Institute for Particle Physics | |
dc.description.affiliation | Center for Astrophysics and Harvard and Smithsonian, 60 Garden Street | |
dc.description.affiliation | Australian Astronomical Optics Macquarie University | |
dc.description.affiliation | Lowell Observatory, 1400 Mars Hill Rd | |
dc.description.affiliation | Centre for Gravitational Astrophysics College of Science The Australian National University | |
dc.description.affiliation | The Research School of Astronomy and Astrophysics Australian National University | |
dc.description.affiliation | Departamento de Física Matemática Instituto de Física Universidade de São Paulo, CP 66318, SP | |
dc.description.affiliation | George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy Department of Physics and Astronomy Texas A and M University | |
dc.description.affiliation | Institució Catalana de Recerca i Estudis Avançats | |
dc.description.affiliation | Department of Astronomy University of California Berkeley 501 Campbell Hall | |
dc.description.affiliation | Observatório Nacional, Rua Gal. José Cristino 77, RJ | |
dc.description.affiliation | Department of Astrophysical Sciences Princeton University Peyton Hall | |
dc.description.affiliation | Department of Physics and Astronomy University of Pennsylvania | |
dc.description.affiliation | School of Physics and Astronomy University of Southampton | |
dc.description.affiliation | Computer Science and Mathematics Division Oak Ridge National Laboratory | |
dc.description.affiliation | Institute of Cosmology and Gravitation University of Portsmouth | |
dc.description.affiliation | Lawrence Berkeley National Laboratory, 1 Cyclotron Road | |
dc.description.affiliationUnesp | Instituto de Física Teórica Universidade Estadual Paulista | |
dc.identifier | http://dx.doi.org/10.1103/PhysRevD.106.123502 | |
dc.identifier.citation | Physical Review D, v. 106, n. 12, 2022. | |
dc.identifier.doi | 10.1103/PhysRevD.106.123502 | |
dc.identifier.issn | 2470-0029 | |
dc.identifier.issn | 2470-0010 | |
dc.identifier.scopus | 2-s2.0-85143737093 | |
dc.identifier.uri | http://hdl.handle.net/11449/248014 | |
dc.language.iso | eng | |
dc.relation.ispartof | Physical Review D | |
dc.source | Scopus | |
dc.title | Dark Energy Survey Year 3 results: Measurement of the baryon acoustic oscillations with three-dimensional clustering | en |
dc.type | Artigo | |
dspace.entity.type | Publication | |
unesp.author.orcid | 0000-0001-8757-408X 0000-0001-8757-408X[1] | |
unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulo | pt |