@article{0787dbad58f847c0b9c54645b0841ba4,
title = "Dark Energy Survey Year 3 results: Measurement of the baryon acoustic oscillations with three-dimensional clustering",
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",
author = "{DES Collaboration} and Chan, {K. C.} and S. Avila and {Carnero Rosell}, A. and I. Ferrero and J. Elvin-Poole and E. Sanchez and H. Camacho and A. Porredon and M. Crocce and Abbott, {T. M.C.} and M. Aguena and S. Allam and F. Andrade-Oliveira and E. Bertin and S. Bocquet and D. Brooks and Burke, {D. L.} and {Carrasco Kind}, M. and J. Carretero and Castander, {F. J.} and R. Cawthon and C. Conselice and M. Costanzi and Pereira, {M. E.S.} and {De Vicente}, J. and S. Desai and Diehl, {H. T.} and P. Doel and S. Everett and B. Flaugher and P. Fosalba and J. Garc{\'i}a-Bellido and E. Gaztanaga and Gerdes, {D. W.} and T. Giannantonio and D. Gruen and Gruendl, {R. A.} and G. Gutierrez and Hinton, {S. R.} and Hollowood, {D. L.} and K. Honscheid and D. Huterer and James, {D. J.} and K. Kuehn and O. Lahav and C. Lidman and M. Lima and Marshall, {J. L.} and J. Mena-Fern{\'a}ndez and F. Menanteau",
note = "K.\u2009C.\u2009C. acknowledges the support from the National Science Foundation of China under the Grants No. 11873102 and No. 12273121, the science research grants from the China Manned Space Project with No. CMS-CSST-2021-B01, and the Science and Technology Program of Guangzhou, China (Grant No. 202002030360). S.\u2009A. is supported by the Spanish Agencia Estatal de Investigacion through the grant \u201CIFT Centro de Excelencia Severo Ochoa by CEX2020-001007-S\u201D and \u201CEU-HORIZON-2020-776247 Enabling Weak Lensing Cosmology (EWC)\u201D, and was also supported by Atraccion de Talento Program No. 2019-T1/TIC-12702 granted by the Comunidad de Madrid in Spain. 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 and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Funda\u00E7\u00E3o Carlos Chagas Filho de Amparo \u00E0 Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cient\u00EDfico e Tecnol\u00F3gico and the Minist\u00E9rio da Ci\u00EAncia, Tecnologia e Inova\u00E7\u00E3o, 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 Energ\u00E9ticas, Medioambientales y Tecnol\u00F3gicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgen\u00F6ssische Technische Hochschule (ETH) Z\u00FCrich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ci\u00E8ncies de l\u2019Espai (IEEC/CSIC), the Institut de F\u00EDsica d\u2019Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universit\u00E4t M\u00FCnchen and the associated Excellence Cluster Universe, the University of Michigan, NSF\u2019s NOIRLab, 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. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF\u2019s NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) 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 MICINN under Grants No. ESP2017-89838, No. PGC2018-094773, No. PGC2018-102021, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union\u2019s Seventh Framework Program (No. FP7/2007-2013) including ERC Grant Agreements No. 240672, No. 291329, and No. 306478. We acknowledge support from the Brazilian Instituto Nacional de Ci\u00EAncia e Tecnologia (INCT) do e-Universo (CNPq Grant No. 465376/2014-2). 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.",
year = "2022",
month = dec,
day = "15",
doi = "10.1103/PhysRevD.106.123502",
language = "English (US)",
volume = "106",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "12",
}