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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering

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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering. / Wang, Yuting; Zhao, Gong Bo; Chuang, Chia Hsun; Pellejero-Ibanez, Marcos; Zhao, Cheng; Kitaura, Francisco Shu; Rodriguez-Torres, Sergio.

In: Monthly Notices of the Royal Astronomical Society, Vol. 481, No. 3, 11.12.2018, p. 3160-3166.

Research output: Contribution to journalArticle

Harvard

Wang, Y, Zhao, GB, Chuang, CH, Pellejero-Ibanez, M, Zhao, C, Kitaura, FS & Rodriguez-Torres, S 2018, 'The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering', Monthly Notices of the Royal Astronomical Society, vol. 481, no. 3, pp. 3160-3166. https://doi.org/10.1093/mnras/sty2449

APA

Wang, Y., Zhao, G. B., Chuang, C. H., Pellejero-Ibanez, M., Zhao, C., Kitaura, F. S., & Rodriguez-Torres, S. (2018). The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering. Monthly Notices of the Royal Astronomical Society, 481(3), 3160-3166. https://doi.org/10.1093/mnras/sty2449

Vancouver

Wang Y, Zhao GB, Chuang CH, Pellejero-Ibanez M, Zhao C, Kitaura FS et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering. Monthly Notices of the Royal Astronomical Society. 2018 Dec 11;481(3):3160-3166. https://doi.org/10.1093/mnras/sty2449

Author

Wang, Yuting ; Zhao, Gong Bo ; Chuang, Chia Hsun ; Pellejero-Ibanez, Marcos ; Zhao, Cheng ; Kitaura, Francisco Shu ; Rodriguez-Torres, Sergio. / The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering. In: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 481, No. 3. pp. 3160-3166.

Bibtex

@article{eb168b5810474396ade231eacc75aa73,
title = "The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering",
abstract = "We perform a tomographic analysis of structure growth and expansion rate from the anisotropic galaxy clustering of the combined sample of Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12, which covers the redshift range of 0.2 < z < 0.75. In order to extract the redshift information of anisotropic galaxy clustering, we analyse this data set in nine overlapping redshift slices in configuration space and perform the joint constraints on the parameters (DV × (r d fid /rd), FAP, fσ8) using the correlation function multipoles. The analysis pipeline is validated using the MultiDark-Patchy mock catalogues. We obtain a measurement precision of 1.5 per cent-2.9 per cent for DV × (r d fid /rd), 5.2 per cent-9 per cent for FAP, and 13.3 per cent-24 per cent for fσ8, depending on the effective redshift of the slices. We report a joint measurement of (DV × (r d fid /rd), FAP, fσ8) with the full covariance matrix in nine redshift slices. We use our joint baryon acoustic oscillations and redshift-space distortions measurement combined with external data sets to constrain the gravitational growth index γ, and find γ = 0.656 ± 0.057, which is consistent with the Λ Cold Dark Matter (ΛCDM) prediction within 95 per cent confidence level.",
keywords = "Cosmological parameters, Large-scale structure of Universe",
author = "Yuting Wang and Zhao, {Gong Bo} and Chuang, {Chia Hsun} and Marcos Pellejero-Ibanez and Cheng Zhao and Kitaura, {Francisco Shu} and Sergio Rodriguez-Torres",
year = "2018",
month = dec
day = "11",
doi = "10.1093/mnras/sty2449",
language = "English",
volume = "481",
pages = "3160--3166",
journal = "MNRAS",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "3",

}

RIS

TY - JOUR

T1 - The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey

T2 - a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering

AU - Wang, Yuting

AU - Zhao, Gong Bo

AU - Chuang, Chia Hsun

AU - Pellejero-Ibanez, Marcos

AU - Zhao, Cheng

AU - Kitaura, Francisco Shu

AU - Rodriguez-Torres, Sergio

PY - 2018/12/11

Y1 - 2018/12/11

N2 - We perform a tomographic analysis of structure growth and expansion rate from the anisotropic galaxy clustering of the combined sample of Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12, which covers the redshift range of 0.2 < z < 0.75. In order to extract the redshift information of anisotropic galaxy clustering, we analyse this data set in nine overlapping redshift slices in configuration space and perform the joint constraints on the parameters (DV × (r d fid /rd), FAP, fσ8) using the correlation function multipoles. The analysis pipeline is validated using the MultiDark-Patchy mock catalogues. We obtain a measurement precision of 1.5 per cent-2.9 per cent for DV × (r d fid /rd), 5.2 per cent-9 per cent for FAP, and 13.3 per cent-24 per cent for fσ8, depending on the effective redshift of the slices. We report a joint measurement of (DV × (r d fid /rd), FAP, fσ8) with the full covariance matrix in nine redshift slices. We use our joint baryon acoustic oscillations and redshift-space distortions measurement combined with external data sets to constrain the gravitational growth index γ, and find γ = 0.656 ± 0.057, which is consistent with the Λ Cold Dark Matter (ΛCDM) prediction within 95 per cent confidence level.

AB - We perform a tomographic analysis of structure growth and expansion rate from the anisotropic galaxy clustering of the combined sample of Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12, which covers the redshift range of 0.2 < z < 0.75. In order to extract the redshift information of anisotropic galaxy clustering, we analyse this data set in nine overlapping redshift slices in configuration space and perform the joint constraints on the parameters (DV × (r d fid /rd), FAP, fσ8) using the correlation function multipoles. The analysis pipeline is validated using the MultiDark-Patchy mock catalogues. We obtain a measurement precision of 1.5 per cent-2.9 per cent for DV × (r d fid /rd), 5.2 per cent-9 per cent for FAP, and 13.3 per cent-24 per cent for fσ8, depending on the effective redshift of the slices. We report a joint measurement of (DV × (r d fid /rd), FAP, fσ8) with the full covariance matrix in nine redshift slices. We use our joint baryon acoustic oscillations and redshift-space distortions measurement combined with external data sets to constrain the gravitational growth index γ, and find γ = 0.656 ± 0.057, which is consistent with the Λ Cold Dark Matter (ΛCDM) prediction within 95 per cent confidence level.

KW - Cosmological parameters

KW - Large-scale structure of Universe

UR - http://www.scopus.com/inward/record.url?scp=85054210914&partnerID=8YFLogxK

U2 - 10.1093/mnras/sty2449

DO - 10.1093/mnras/sty2449

M3 - Article

AN - SCOPUS:85054210914

VL - 481

SP - 3160

EP - 3166

JO - MNRAS

JF - MNRAS

SN - 0035-8711

IS - 3

ER -

ID: 11888468