NAOC Open IR  > 星系宇宙学研究部
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: observational systematics and baryon acoustic oscillations in the correlation function
Ross, Ashley J.1,2; Beutler, Florian2,3; Chuang, Chia-Hsun4,5; Pellejero-Ibanez, Marcos6,7; Seo, Hee-Jong8; Vargas-Magana, Mariana9; Cuesta, Antonio J.10; Percival, Will J.2; Burden, Angela2,11; Sanchez, Ariel G.12; Grieb, Jan Niklas12,13; Reid, Beth3; Brownstein, Joel R.14; Dawson, Kyle S.14; Eisenstein, Daniel J.15; Ho, Shirley3,16,17; Kitaura, Francisco-Shu5; Nichol, Robert C.2; Olmstead, Matthew D.18; Prada, Francisco4,19,20; Rodriguez-Torres, Sergio A.4,19,21; Saito, Shun22,23; Salazar-Albornoz, Salvador12,13; Schneider, Donald P.24,25; Thomas, Daniel2; Tinker, Jeremy26; Tojeiro, Rita27; Wang, Yuting2,28; White, Martin3,17,29; Zhao, Gong-bo2,28
2017
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume464Issue:1Pages:1168-1191
AbstractWe present baryon acoustic oscillation (BAO) scale measurements determined from the clustering of 1.2 million massive galaxies with redshifts 0.2 < z < 0.75 distributed over 9300 deg(2), as quantified by their redshift-space correlation function. In order to facilitate these measurements, we define, describe, and motivate the selection function for galaxies in the final data release (DR12) of the SDSS III Baryon Oscillation Spectroscopic Survey (BOSS). This includes the observational footprint, masks for image quality and Galactic extinction, and weights to account for density relationships intrinsic to the imaging and spectroscopic portions of the survey. We simulate the observed systematic trends in mock galaxy samples and demonstrate that they impart no bias on BAO scale measurements and have a minor impact on the recovered statistical uncertainty. We measure transverse and radial BAO distance measurements in 0.2 < z < 0.5, 0.5 < z < 0.75, and (overlapping) 0.4 < z < 0.6 redshift bins. In each redshift bin, we obtain a precision that is 2.7 per cent or better on the radial distance and 1.6 per cent or better on the transverse distance. The combination of the redshift bins represents 1.8 per cent precision on the radial distance and 1.1 per cent precision on the transverse distance. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. The measurements and likelihoods presented here are combined with others in Alam et al. to produce the final cosmological constraints from BOSS.
SubtypeArticle
KeywordCosmology: Observations Large-scale Structure Of Universe
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationOhio State University Center for Cosmology and Particle Physics ; Ohio State University Center for Cosmology and Particle Physics ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064) ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064) ; MINECO Centro de Excelencia Severo Ochoa Programme(SEV-2012-0249 ; MINECO Centro de Excelencia Severo Ochoa Programme(SEV-2012-0249 ; MINECO(AYA2012-39702-C02-01) ; MINECO(AYA2012-39702-C02-01) ; US Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0014329) ; US Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0014329) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Proyecto Conacyt Fronteras(281) ; Proyecto Conacyt Fronteras(281) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Cambridge University ; Cambridge University ; Carnegie Mellon University ; Carnegie Mellon University ; Case Western University ; Case Western University ; University of Florida ; University of Florida ; Fermilab ; Fermilab ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; UC Irvine ; UC Irvine ; Instituto de Astrofisica de Andalucia ; Instituto de Astrofisica de Andalucia ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Institucio Catalana de Recerca y Estudis Avancat, Barcelona ; Institucio Catalana de Recerca y Estudis Avancat, Barcelona ; Instituto de Fisica Corpuscular ; Instituto de Fisica Corpuscular ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Korean Institute for Advanced Study ; Korean Institute for Advanced Study ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; UC Santa Cruz ; UC Santa Cruz ; Spanish Participation Group ; Spanish Participation Group ; Texas Christian University ; Texas Christian University ; Trieste Astrophysical Observatory University of Tokyo/IPMU ; Trieste Astrophysical Observatory University of Tokyo/IPMU ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Yale University ; Yale University ; AYA2014-60641-C2-1-P) ; AYA2014-60641-C2-1-P) ; Ohio State University Center for Cosmology and Particle Physics ; Ohio State University Center for Cosmology and Particle Physics ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064) ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064) ; MINECO Centro de Excelencia Severo Ochoa Programme(SEV-2012-0249 ; MINECO Centro de Excelencia Severo Ochoa Programme(SEV-2012-0249 ; MINECO(AYA2012-39702-C02-01) ; MINECO(AYA2012-39702-C02-01) ; US Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0014329) ; US Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0014329) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Proyecto Conacyt Fronteras(281) ; Proyecto Conacyt Fronteras(281) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Cambridge University ; Cambridge University ; Carnegie Mellon University ; Carnegie Mellon University ; Case Western University ; Case Western University ; University of Florida ; University of Florida ; Fermilab ; Fermilab ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; UC Irvine ; UC Irvine ; Instituto de Astrofisica de Andalucia ; Instituto de Astrofisica de Andalucia ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Institucio Catalana de Recerca y Estudis Avancat, Barcelona ; Institucio Catalana de Recerca y Estudis Avancat, Barcelona ; Instituto de Fisica Corpuscular ; Instituto de Fisica Corpuscular ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Korean Institute for Advanced Study ; Korean Institute for Advanced Study ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; UC Santa Cruz ; UC Santa Cruz ; Spanish Participation Group ; Spanish Participation Group ; Texas Christian University ; Texas Christian University ; Trieste Astrophysical Observatory University of Tokyo/IPMU ; Trieste Astrophysical Observatory University of Tokyo/IPMU ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Yale University ; Yale University ; AYA2014-60641-C2-1-P) ; AYA2014-60641-C2-1-P)
DOI10.1093/mnras/stw2372
WOS KeywordDIGITAL SKY SURVEY ; MEASURING D-A ; DATA RELEASE ; GROWTH-RATE ; COSMOLOGICAL PARAMETERS ; FULL SHAPE ; FINAL DATA ; SAMPLE ; RECONSTRUCTION ; DISTANCE
Indexed BySCI
Language英语
Funding OrganizationOhio State University Center for Cosmology and Particle Physics ; Ohio State University Center for Cosmology and Particle Physics ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064) ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064) ; MINECO Centro de Excelencia Severo Ochoa Programme(SEV-2012-0249 ; MINECO Centro de Excelencia Severo Ochoa Programme(SEV-2012-0249 ; MINECO(AYA2012-39702-C02-01) ; MINECO(AYA2012-39702-C02-01) ; US Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0014329) ; US Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0014329) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Proyecto Conacyt Fronteras(281) ; Proyecto Conacyt Fronteras(281) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Cambridge University ; Cambridge University ; Carnegie Mellon University ; Carnegie Mellon University ; Case Western University ; Case Western University ; University of Florida ; University of Florida ; Fermilab ; Fermilab ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; UC Irvine ; UC Irvine ; Instituto de Astrofisica de Andalucia ; Instituto de Astrofisica de Andalucia ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Institucio Catalana de Recerca y Estudis Avancat, Barcelona ; Institucio Catalana de Recerca y Estudis Avancat, Barcelona ; Instituto de Fisica Corpuscular ; Instituto de Fisica Corpuscular ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Korean Institute for Advanced Study ; Korean Institute for Advanced Study ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; UC Santa Cruz ; UC Santa Cruz ; Spanish Participation Group ; Spanish Participation Group ; Texas Christian University ; Texas Christian University ; Trieste Astrophysical Observatory University of Tokyo/IPMU ; Trieste Astrophysical Observatory University of Tokyo/IPMU ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Yale University ; Yale University ; AYA2014-60641-C2-1-P) ; AYA2014-60641-C2-1-P) ; Ohio State University Center for Cosmology and Particle Physics ; Ohio State University Center for Cosmology and Particle Physics ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064) ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064) ; MINECO Centro de Excelencia Severo Ochoa Programme(SEV-2012-0249 ; MINECO Centro de Excelencia Severo Ochoa Programme(SEV-2012-0249 ; MINECO(AYA2012-39702-C02-01) ; MINECO(AYA2012-39702-C02-01) ; US Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0014329) ; US Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0014329) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Proyecto Conacyt Fronteras(281) ; Proyecto Conacyt Fronteras(281) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Cambridge University ; Cambridge University ; Carnegie Mellon University ; Carnegie Mellon University ; Case Western University ; Case Western University ; University of Florida ; University of Florida ; Fermilab ; Fermilab ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; UC Irvine ; UC Irvine ; Instituto de Astrofisica de Andalucia ; Instituto de Astrofisica de Andalucia ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Institucio Catalana de Recerca y Estudis Avancat, Barcelona ; Institucio Catalana de Recerca y Estudis Avancat, Barcelona ; Instituto de Fisica Corpuscular ; Instituto de Fisica Corpuscular ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Korean Institute for Advanced Study ; Korean Institute for Advanced Study ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; University of Pittsburgh ; University of Pittsburgh ; Princeton University ; Princeton University ; UC Santa Cruz ; UC Santa Cruz ; Spanish Participation Group ; Spanish Participation Group ; Texas Christian University ; Texas Christian University ; Trieste Astrophysical Observatory University of Tokyo/IPMU ; Trieste Astrophysical Observatory University of Tokyo/IPMU ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Yale University ; Yale University ; AYA2014-60641-C2-1-P) ; AYA2014-60641-C2-1-P)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000393646300089
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8298
Collection星系宇宙学研究部
Affiliation1.Ohio State Univ, Ctr Cosmol & AstroParticle Phys, Columbus, OH 43210 USA
2.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
3.Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
4.Univ Autonoma Madrid, CSIC, Inst Fis Teor, Cantoblanco, E-28049 Madrid, Spain
5.Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany
6.IAC, C Via Lactea S-N, E-38205 Tenerife, Spain
7.Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
8.Ohio Univ, Dept Phys & Astron, 251B Clippinger Labs, Athens, OH 45701 USA
9.Univ Nacl Autonoma Mexico, Inst Fis, Apdo Postal 20-364, Mexico City 04510, DF, Mexico
10.Univ Barcelona, Inst Ciencies Cosmos ICCUB, IEEC UB, Marti i Franques 1, E-08028 Barcelona, Spain
11.Yale Univ, Dept Phys, 260 Whitney Ave, New Haven, CT 06520 USA
12.Max Planck Inst Extraterr Phys, Postfach 1312,Giessenbachstr, D-85741 Garching, Germany
13.Ludwig Maximilians Univ Munchen, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany
14.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
15.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
16.Carnegie Mellon Univ, Dept Phys, McWilliams Ctr Cosmol, 5000 Forbes Ave, Pittsburgh, PA 15213 USA
17.Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
18.Kings Coll, Dept Chem & Phys, 133 North River St, Wilkes Barre, PA 18711 USA
19.UAM CSIC, Campus Int Excellence, E-28049 Madrid, Spain
20.CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
21.Univ Autonoma Madrid, Inst Fis Teor M8, Cantoblanco, E-28049 Madrid, Spain
22.Max Planck Inst Astrophys, Karl Schwarzschild Starsse 1, D-85740 Garching, Germany
23.Univ Tokyo, Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan
24.Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
25.Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
26.NYU, Ctr Cosmol & Particle Phys, Dept Phys, 4 Washington Pl, New York, NY 10003 USA
27.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
28.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
29.Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
Recommended Citation
GB/T 7714
Ross, Ashley J.,Beutler, Florian,Chuang, Chia-Hsun,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: observational systematics and baryon acoustic oscillations in the correlation function[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,464(1):1168-1191.
APA Ross, Ashley J..,Beutler, Florian.,Chuang, Chia-Hsun.,Pellejero-Ibanez, Marcos.,Seo, Hee-Jong.,...&Zhao, Gong-bo.(2017).The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: observational systematics and baryon acoustic oscillations in the correlation function.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,464(1),1168-1191.
MLA Ross, Ashley J.,et al."The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: observational systematics and baryon acoustic oscillations in the correlation function".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 464.1(2017):1168-1191.
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