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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: towards a computationally efficient analysis without informative priors
Pellejero-Ibanez, Marcos1,2,3,4; Chuang, Chia-Hsun3,4; Rubino-Martin, J. A.1,2; Cuesta, Antonio J.5; Wang, Yuting6,7; Zhao, Gongbo6,7; Ross, Ashley J.7,8; Rodriguez-Torres, Sergio3,9,10; Prada, Francisco3,9,11; Slosar, Anze12; Vazquez, Jose A.12; Alam, Shadab13,14; Beutler, Florian7,15; Eisenstein, Daniel J.16; Gil-Marin, Hector17,18; Grieb, Jan Niklas19,20; Ho, Shirley13,14; Kitaura, Francisco-Shu4,15,21,22; Percival, Will J.7; Rossi, Graziano23; Salazar-Albornoz, Salvador19,20; Samushia, Lado7,24,25; Sanchez, Ariel G.20; Satpathy, Siddharth13,14; Seo, Hee-Jong26; Tinker, Jeremy L.27; Tojeiro, Rita28; Vargas-Magana, Mariana29; Brownstein, Joel R.30; Nichol, Robert C.7; Olmstead, Matthew D.31
2017-07-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume468Issue:4Pages:4116-4133
AbstractWe develop a new computationally efficient methodology called double-probe analysis with the aim of minimizing informative priors (those coming from extra probes) in the estimation of cosmological parameters. Using our new methodology, we extract the dark energy model-independent cosmological constraints from the joint data sets of the Baryon Oscillation Spectroscopic Survey (BOSS) galaxy sample and Planck cosmic microwave background (CMB) measurements. We measure the mean values and covariance matrix of {R, l(a), Omega(b)h(2), n(s), log(A(s)), Omega(k), H(z), D-A(z), f(z)sigma(8)(z)}, which give an efficient summary of the Planck data and two- point statistics from the BOSS galaxy sample. The CMB shift parameters are R = root Omega H-m(0)2 r(z(*)) and l(a) = pi r(z(*))/r(s)(z(*)), where z(*) is the redshift at the last scattering surface, and r(z(*)) and rs(z(*)) denote our comoving distance to the z(*) and sound horizon at z(*), respectively; Omega(b) is the baryon fraction at z=0. This approximate methodology guarantees that we will not need to put informative priors on the cosmological parameters that galaxy clustering is unable to constrain, i.e. Omega(b)h(2) and ns. The main advantage is that the computational time required for extracting these parameters is decreased by a factor of 60 with respect to exact full-likelihood analyses. The results obtained show no tension with the flat Lambda cold dark matter (Lambda CDM) cosmological paradigm. By comparing with the full-likelihood exact analysis with fixed dark energy models, on one hand we demonstrate that the double-probe method provides robust cosmological parameter constraints that can be conveniently used to study dark energy models, and on the other hand we provide a reliable set of measurements assuming dark energy models to be used, for example, in distance estimations. We extend our study to measure the sum of the neutrino mass using different methodologies, including double-probe analysis (introduced in this study), full-likelihood analysis and single-probe analysis. From full-likelihood analysis, we obtain Sigma m(v) < 0.12 ( 68 per cent), assuming Lambda CDM and Sigma m(v) < 0.20 ( 68 per cent) assuming owCDM. We also find that there is degeneracy between observational systematics and neutrino masses, which suggests that one should take great care when estimating these parameters in the case of not having control over the systematics of a given sample.
SubtypeArticle
KeywordCosmological Parameters Distance Scale Large-scale Structure Of Universe Cosmology: Observations
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationSpanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064 ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064 ; Comunidad de Madrid(HEPHACOS 52009/ESP-1473) ; Comunidad de Madrid(HEPHACOS 52009/ESP-1473) ; MINECO(AYA2012-39702-C02-01) ; MINECO(AYA2012-39702-C02-01) ; National Research Foundation of Korea (NRF) through NRF-SGER - Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; National Research Foundation of Korea (NRF) through NRF-SGER - Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; Programa de Apoyo a Proyectos de Investigation e Innovation Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigation e Innovation Tecnologica (PAPITT)(IA102516) ; Proyecto Conacyt Fronteras(281) ; Proyecto Conacyt Fronteras(281) ; Proyecto LANCAD-UNAM-DGTIC(319) ; Proyecto LANCAD-UNAM-DGTIC(319) ; 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 ; AYA2010-21231-C02-01) ; AYA2010-21231-C02-01) ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064 ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064 ; Comunidad de Madrid(HEPHACOS 52009/ESP-1473) ; Comunidad de Madrid(HEPHACOS 52009/ESP-1473) ; MINECO(AYA2012-39702-C02-01) ; MINECO(AYA2012-39702-C02-01) ; National Research Foundation of Korea (NRF) through NRF-SGER - Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; National Research Foundation of Korea (NRF) through NRF-SGER - Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; Programa de Apoyo a Proyectos de Investigation e Innovation Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigation e Innovation Tecnologica (PAPITT)(IA102516) ; Proyecto Conacyt Fronteras(281) ; Proyecto Conacyt Fronteras(281) ; Proyecto LANCAD-UNAM-DGTIC(319) ; Proyecto LANCAD-UNAM-DGTIC(319) ; 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 ; AYA2010-21231-C02-01) ; AYA2010-21231-C02-01)
DOI10.1093/mnras/stx751
WOS KeywordDIGITAL SKY SURVEY ; SURVEY COSMOLOGICAL IMPLICATIONS ; LUMINOUS RED GALAXIES ; PRE-LAUNCH STATUS ; 2-POINT CORRELATION-FUNCTION ; TELESCOPE LENSING SURVEY ; FINAL DATA RELEASE ; REDSHIFT-SPACE ; CMASS GALAXIES ; NEUTRINO MASS
Indexed BySCI
Language英语
Funding OrganizationSpanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064 ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064 ; Comunidad de Madrid(HEPHACOS 52009/ESP-1473) ; Comunidad de Madrid(HEPHACOS 52009/ESP-1473) ; MINECO(AYA2012-39702-C02-01) ; MINECO(AYA2012-39702-C02-01) ; National Research Foundation of Korea (NRF) through NRF-SGER - Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; National Research Foundation of Korea (NRF) through NRF-SGER - Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; Programa de Apoyo a Proyectos de Investigation e Innovation Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigation e Innovation Tecnologica (PAPITT)(IA102516) ; Proyecto Conacyt Fronteras(281) ; Proyecto Conacyt Fronteras(281) ; Proyecto LANCAD-UNAM-DGTIC(319) ; Proyecto LANCAD-UNAM-DGTIC(319) ; 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 ; AYA2010-21231-C02-01) ; AYA2010-21231-C02-01) ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064 ; Spanish MICINNs Consolider-Ingenio Programme(MultiDark CSD2009-00064 ; Comunidad de Madrid(HEPHACOS 52009/ESP-1473) ; Comunidad de Madrid(HEPHACOS 52009/ESP-1473) ; MINECO(AYA2012-39702-C02-01) ; MINECO(AYA2012-39702-C02-01) ; National Research Foundation of Korea (NRF) through NRF-SGER - Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; National Research Foundation of Korea (NRF) through NRF-SGER - Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; Programa de Apoyo a Proyectos de Investigation e Innovation Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigation e Innovation Tecnologica (PAPITT)(IA102516) ; Proyecto Conacyt Fronteras(281) ; Proyecto Conacyt Fronteras(281) ; Proyecto LANCAD-UNAM-DGTIC(319) ; Proyecto LANCAD-UNAM-DGTIC(319) ; 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 ; AYA2010-21231-C02-01) ; AYA2010-21231-C02-01)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000402819700029
Citation statistics
Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8806
Collection星系宇宙学研究部
Affiliation1.IAC, C Via Lactea S-N, E-38200 Tenerife, Spain
2.ULL, Dept Astrofis, E-38206 Tenerife, Spain
3.Univ Autonoma Madrid, UAM, CSIC, Inst Fis Teor, E-28049 Madrid, Spain
4.Leibniz Inst Astrophys Potsdam AIP, Art Sternwarte 16, D-14482 Potsdam, Germany
5.Univ Barcelona, IEEC UB, Inst Ciencies Cosmos ICCUB, Marti & Franques 1, E-08028 Barcelona, Spain
6.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
7.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3EX, Hants, England
8.Ohio State Univ, Dept Phys, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA
9.Campus Int Excellence UAM CSIC, E-28049 Madrid, Spain
10.Univ Autonoma Madrid, Dept Fis Teor M8, E-28049 Madrid, Spain
11.CSIC, Glorieta Astron, Inst Astrofis Andalucia, E-18080 Granada, Spain
12.Brookhaven Natl Lab, Upton, NY 11973 USA
13.Carnegie Mellon Univ, Dept Phys, 5000 Forbes Ave, Pittsburgh, PA 15213 USA
14.Carnegie Mellon Univ, McWilliams Ctr Pr, 5000 Forbes Ave, Pittsburgh, PA 15213 USA
15.Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
16.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
17.Sorbonne Univ, ILP, 98 Bis Blvd Arago, F-75014 Paris, France
18.Univ Paris 06, Lab Phys Nucl & Hautes Energies, 4 Pl Jussieu, F-75005 Paris, France
19.Univ Sternwarte Munich, Scheinerstr 1, D-81679 Munich, Germany
20.Max Planck Inst Extraterr Phys, Postfach 1312 Giessenbadistr, D-85741 Garching, Germany
21.Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
22.Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
23.Sejong Univ, Dept Phys & Astron, Seoul 143747, South Korea
24.Kansas State Univ, Manhattan, KS 66506 USA
25.Ilia State Univ, Natl Abastumani Astrophys Observ, 2A Kazbegi Ave, GE-1060 Tbilisi, Rep of Georgia
26.Ohio Univ, Dept Phys & Astron, 251B Clippinger Labs, Athens, OH 45701 USA
27.New York Univ, Dept Phys, Ctr Cosmol & Particle Phys, 4 Washington Pl, New York, NY 10003 USA
28.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
29.Univ Nacl Autonoma Mexico, Inst Fis, Apdo Postal 20-364, Mexico City, DF, Mexico
30.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
31.Kings Coll, Dept Chem & Phys, 133 North River St, Wilkes Barre, PA 18711 USA
Recommended Citation
GB/T 7714
Pellejero-Ibanez, Marcos,Chuang, Chia-Hsun,Rubino-Martin, J. A.,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: towards a computationally efficient analysis without informative priors[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,468(4):4116-4133.
APA Pellejero-Ibanez, Marcos.,Chuang, Chia-Hsun.,Rubino-Martin, J. A..,Cuesta, Antonio J..,Wang, Yuting.,...&Olmstead, Matthew D..(2017).The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: towards a computationally efficient analysis without informative priors.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,468(4),4116-4133.
MLA Pellejero-Ibanez, Marcos,et al."The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: towards a computationally efficient analysis without informative priors".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 468.4(2017):4116-4133.
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