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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the Fourier space wedges of the final sample
Grieb, Jan Niklas1,2; Sanchez, Ariel G.2; Salazar-Albornoz, Salvador1,2; Scoccimarro, Roman3,4; Crocce, Martin; Dalla Vecchia, Claudio5,6; Montesano, Francesco2; Gil-Marin, Hector7,8,9; Ross, Ashley J.7,10; Beutler, Florian11; Rodriguez-Torres, Sergio12,13,14; Chuang, Chia-Hsun14,15; Prada, Francisco12,14,16; Kitaura, Francisco-Shu15; Cuesta, Antonio J.17; Eisenstein, Daniel J.18; Percival, Will J.7; Vargas-Magana, Mariana19; Tinker, Jeremy L.3,4; Tojeiro, Rita20; Brownstein, Joel R.21; Maraston, Claudia7; Nichol, Robert C.7; Olmstead, Matthew D.22; Samushia, Lado7,23,24; Seo, Hee-Jong25; Streblyanska, Alina; Zhao, Gong-bo7,26
2017-05-01
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷号467期号:2页码:2085-2112
摘要We extract cosmological information from the anisotropic power-spectrummeasurements from the recently completed Baryon Oscillation Spectroscopic Survey (BOSS), extending the concept of clustering wedges to Fourier space. Making use of new fast-Fourier-transform-based estimators, we measure the power-spectrum clustering wedges of the BOSS sample by filtering out the information of Legendre multipoles l > 4. Our modelling of these measurements is based on novel approaches to describe non-linear evolution, bias and redshift-space distortions, which we test using synthetic catalogues based on large-volume N-body simulations. We are able to include smaller scales than in previous analyses, resulting in tighter cosmological constraints. Using three overlapping redshift bins, we measure the angular-diameter distance, the Hubble parameter and the cosmic growth rate, and explore the cosmological implications of our full-shape clustering measurements in combination with cosmic microwave background and Type Ia supernova data. Assuming a Lambda cold dark matter (Lambda CDM) cosmology, we constrain the matter density to Omega M = 0.311(-0.010)(+ 0.009) and the Hubble parameter to H-0 = 67.6(-0.6)(+0.7) km s(-1) Mpc(-1), at a confidence level of 68 per cent. We also allow for nonstandard dark energy models and modifications of the growth rate, finding good agreement with the Lambda CDM paradigm. For example, we constrain the equation-of-state parameter to omega =-1.019(-0.039)(+0.048) . 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.
文章类型Article
关键词Cosmological Parameters Cosmology: Observations Dark Energy Large -scale-structure Of Universe
WOS标题词Science & Technology ; Physical Sciences
资助者Transregional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Transregional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish MICINN's Consolider-Ingenio Programme(CSD2009-00064 ; Spanish MICINN's Consolider-Ingenio Programme(CSD2009-00064 ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Campus de Excelencia Internacional UAM/CSIC ; Campus de Excelencia Internacional UAM/CSIC ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; 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 ; ESA Member States ; ESA Member States ; NASA and Canada ; NASA and Canada ; SEV-2015-0548 ; SEV-2015-0548 ; AYA201021231-C02-01) ; AYA201021231-C02-01) ; AYA2013-46886 ; AYA2013-46886 ; AYA2014-58308) ; AYA2014-58308) ; Transregional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Transregional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish MICINN's Consolider-Ingenio Programme(CSD2009-00064 ; Spanish MICINN's Consolider-Ingenio Programme(CSD2009-00064 ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Campus de Excelencia Internacional UAM/CSIC ; Campus de Excelencia Internacional UAM/CSIC ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; 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 ; ESA Member States ; ESA Member States ; NASA and Canada ; NASA and Canada ; SEV-2015-0548 ; SEV-2015-0548 ; AYA201021231-C02-01) ; AYA201021231-C02-01) ; AYA2013-46886 ; AYA2013-46886 ; AYA2014-58308) ; AYA2014-58308)
DOI10.1093/mnras/stw3384
关键词[WOS]DIGITAL SKY SURVEY ; MICROWAVE BACKGROUND ANISOTROPIES ; POWER SPECTRUM MULTIPOLES ; ACOUSTIC-OSCILLATIONS ; DATA RELEASE ; REDSHIFT-SPACE ; GROWTH-RATE ; CMASS GALAXIES ; DARK ENERGY ; FULL SHAPE
收录类别SCI
语种英语
资助者Transregional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Transregional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish MICINN's Consolider-Ingenio Programme(CSD2009-00064 ; Spanish MICINN's Consolider-Ingenio Programme(CSD2009-00064 ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Campus de Excelencia Internacional UAM/CSIC ; Campus de Excelencia Internacional UAM/CSIC ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; 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 ; ESA Member States ; ESA Member States ; NASA and Canada ; NASA and Canada ; SEV-2015-0548 ; SEV-2015-0548 ; AYA201021231-C02-01) ; AYA201021231-C02-01) ; AYA2013-46886 ; AYA2013-46886 ; AYA2014-58308) ; AYA2014-58308) ; Transregional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Transregional Collaborative Research Centre TR33 'The Dark Universe' of the German Research Foundation (DFG) ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish MICINN's Consolider-Ingenio Programme(CSD2009-00064 ; Spanish MICINN's Consolider-Ingenio Programme(CSD2009-00064 ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Campus de Excelencia Internacional UAM/CSIC ; Campus de Excelencia Internacional UAM/CSIC ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; 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 ; ESA Member States ; ESA Member States ; NASA and Canada ; NASA and Canada ; SEV-2015-0548 ; SEV-2015-0548 ; AYA201021231-C02-01) ; AYA201021231-C02-01) ; AYA2013-46886 ; AYA2013-46886 ; AYA2014-58308) ; AYA2014-58308)
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000398416700060
引用统计
被引频次:23[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8230
专题星系宇宙学研究部
作者单位1.Ludwig Maximilians Univ Munchen, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany
2.Max Planck Inst Extraterr Phys, Postfach 1312, D-85741 Garching, Germany
3.NYU, Dept Phys, Ctr Cosmol & Particle Phys, New York, NY 10003 USA
4.CSIC, IEEC, Inst Ciencies Espai, Campus UAB Ciencies,Torre C5 Par 2, Barcelona 08193, Spain
5.Inst Astrofis Canarias, C Via Lactea S N, E-38205 Tenerife, Spain
6.Univ La Laguna, Dept Astrofis, Av Astrofis Francisco Sanchez S N, E-38206 Tenerife, Spain
7.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
8.Sorbonne Univ, Inst Lagrange Paris, 98 Bis Blvd Arago, F-75014 Paris, France
9.Univ Paris 06, Lab Phys Nucl & Hautes Energies, 4 Pl Jussieu, F-75005 Paris, France
10.Ohio State Univ, Ctr Cosmol & AstroParticle Phys, Columbus, OH 43210 USA
11.Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
12.Univ Autonoma Madrid, CSIC, Inst Fis Teor, E-28049 Madrid, Spain
13.CSIC, Campus Int Excellence UAM, E-28049 Madrid, Spain
14.Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain
15.Leibniz Inst Astrophys AIP, Sternwarte 16, D-14482 Potsdam, Germany
16.Inst Astrofis Andalucia, CSIC, E-18080 Granada, Spain
17.Univ Barcelona IEEC UB, Inst Ciencies Cosmos ICCUB, Martii Franques 1, E-08028 Barcelona, Spain
18.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
19.Univ Nacl Autonoma Mexico, Inst Fis, POB 20364, Mexico City 01000, DF, Mexico
20.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
21.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
22.Kings Coll, Dept Chem & Phys, 133 North River St, Wilkes Barre 18711, PA USA
23.Kansas State Univ, Manhattan, KS 66506 USA
24.Ilia State Univ, Natl Abastumani Astrophys Observ, 2A Kazbegi Ave, GE-1060 Tbilisi, Rep of Georgia
25.Ohio Univ, Dept Phys & Astron, 251B Clippinger Labs, Athens, OH 45701 USA
26.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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Grieb, Jan Niklas,Sanchez, Ariel G.,Salazar-Albornoz, Salvador,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the Fourier space wedges of the final sample[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,467(2):2085-2112.
APA Grieb, Jan Niklas.,Sanchez, Ariel G..,Salazar-Albornoz, Salvador.,Scoccimarro, Roman.,Crocce, Martin.,...&Zhao, Gong-bo.(2017).The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the Fourier space wedges of the final sample.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,467(2),2085-2112.
MLA Grieb, Jan Niklas,et al."The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the Fourier space wedges of the final sample".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 467.2(2017):2085-2112.
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