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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering - towards an accurate model

文献类型：期刊论文

作者Tinker, Jeremy L.7; Thomas, Daniel14; Satpathy, Siddharth25,26; Sanchez, Ariel G.24; Samushia, Lado1,14,30; Salazar-Albornoz, Salvador23,24; Rossi, Graziano29; Slosar, Anze19; Percival, Will J.14; Chuang, Chia-Hsun2,8
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2017-10-01
卷号471期号:2页码:2370-2390
关键词Cosmological Parameters Distance Scale Large-scale Structure Of Universe Cosmology: Observations
DOI10.1093/mnras/stx1641
文献子类Article
英文摘要We analyse the broad-range shape of the monopole and quadrupole correlation functions of the Baryon Oscillation Spectroscopic Survey Data Release 12 (DR12) CMASS and LOWZ galaxy sample to obtain constraints on the Hubble expansion rate H(z), the angular-diameter distance D-A(z), the normalized growth rate f(z) sigma(8)(z) and the physical matter density Omega(m) h(2). We adopt wide and flat priors on all model parameters in order to ensure the results are those of a ` single-probe' galaxy clustering analysis. We also marginalize over three nuisance terms that account for potential observational systematics affecting the measured monopole. However, such Monte Carlo Markov Chain analysis is computationally expensive for advanced theoretical models. We develop a new methodology to speed up the analysis. Using the range 40 h(-1) Mpc < s < 180 h(-1) Mpc, we obtain {DA(z) r(s,fid)/ r(s) (Mpc), H(z) r(s)/r(s),(fid) km s(-1) Mpc(-1), f(z)sigma 8(z)Omega(m)h(2)} = {956 +/- 28, 75.0 +/- 4.0, 0.397 +/- 0.073, 0.143 +/- 0.017} at z = 0.32 and {1421 +/- 23, 96.7 +/- 2.7, 0.497 +/- 0.058, 0.137 +/- 0.015} at z = 0.59 where r(s) is the comoving sound horizon at the drag epoch and r(s,fid) = 147.66 Mpc for the fiducial cosmology used in this study. Combining our measurements with Planck data, we obtain Omega(m) = 0.306 +/- 0.009, H-0 = 67.9 +/- 0.7 kms(-1) Mpc(-1) and sigma(8) = 0.815 +/- 0.009 assuming Lambda cold dark matter (CDM); Omega(k) = 0.000 +/- 0.003 and w= -1.02 +/- 0.08 assuming owCDM. Our results show no tension with the flat Lambda CDM cosmological paradigm. This paper is part of a set that analyses the final galaxy clustering data set from Baryon Oscillation Spectroscopic Survey.
WOS关键词DIGITAL SKY SURVEY ; DARK ENERGY SURVEY ; LUMINOUS RED GALAXIES ; SURVEY COSMOLOGICAL IMPLICATIONS ; REDSHIFT-SPACE DISTORTIONS ; DATA RELEASE 9 ; 3-POINT CORRELATION-FUNCTION ; FINAL DATA RELEASE ; MEASURING D-A ; ACOUSTIC-OSCILLATIONS
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000409022700075
资助机构Spanish MICINN's Consolider-Ingenio Programme under grant MultiDark(CSD2009-00064 ; Spanish MICINN's Consolider-Ingenio Programme under grant MultiDark(CSD2009-00064 ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; MINECO(AYA2012-39702- C02-01) ; MINECO(AYA2012-39702- C02-01) ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST)(NRF-SGER 2014055950) ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST)(NRF-SGER 2014055950) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; 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 ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; 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 Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University ; (LANCAD-UNAM-DGTIC-319) ; (LANCAD-UNAM-DGTIC-319) ; AYA2010-21231-C02-01) ; AYA2010-21231-C02-01) ; Spanish MICINN's Consolider-Ingenio Programme under grant MultiDark(CSD2009-00064 ; Spanish MICINN's Consolider-Ingenio Programme under grant MultiDark(CSD2009-00064 ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; Comunidad de Madrid(HEPHACOS S2009/ESP-1473) ; MINECO(AYA2012-39702- C02-01) ; MINECO(AYA2012-39702- C02-01) ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST)(NRF-SGER 2014055950) ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST)(NRF-SGER 2014055950) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; 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 ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; 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 Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University ; (LANCAD-UNAM-DGTIC-319) ; (LANCAD-UNAM-DGTIC-319) ; AYA2010-21231-C02-01) ; AYA2010-21231-C02-01)
源URL[http://ir.bao.ac.cn/handle/114a11/20148]  
专题国家天文台_星系宇宙学研究部
作者单位1.Kansas State Univ, Manhattan, KS 66506 USA
2.Univ Autonoma Madrid, UAM CSIC, Inst Fis Teor, E-28049 Madrid, Spain
3.Kings Coll, Dept Chem & Phys, 133 North River St, Wilkes Barre, PA 18711 USA
4.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
5.Univ Nacl Autonoma Mexico, Inst Fis, Mexico City 20364, DF, Mexico
6.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
7.NYU, Dept Phys, Ctr Cosmol & Particle Phys, 4 Washington Pl, New York, NY 10003 USA
8.Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany
9.IAC, C Via Lactea S-N, E-38200 Tenerife, Spain
10.ULL, Dept Astrofis, E-38206 Tenerife, Spain
推荐引用方式
GB/T 7714		 Tinker, Jeremy L.,Thomas, Daniel,Satpathy, Siddharth,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering - towards an accurate model[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,471(2):2370-2390.
APA Tinker, Jeremy L..,Thomas, Daniel.,Satpathy, Siddharth.,Sanchez, Ariel G..,Samushia, Lado.,...&Tojeiro, Rita.(2017).The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering - towards an accurate model.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,471(2),2370-2390.
MLA Tinker, Jeremy L.,et al."The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering - towards an accurate model".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 471.2(2017):2370-2390.

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来源：国家天文台

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