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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: on the measurement of growth rate using galaxy correlation functions

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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : on the measurement of growth rate using galaxy correlation functions. / Satpathy, Siddharth; Alam, Shadab; Ho, Shirley; White, Martin; Bahcall, Neta A.; Beutler, Florian; Brownstein, Joel R.; Chuang, Chia-Hsun; Eisenstein, Daniel J.; Grieb, Jan Niklas; Kitaura, Francisco-Shu; Olmstead, Matthew D.; Percival, Will J.; Salazar-Albornoz, Salvador; Sánchez, Ariel G.; Seo, Hee-Jong; Thomas, Daniel; Tinker, Jeremy L.; Tojeiro, Rita.

In: Monthly Notices of the Royal Astronomical Society, Vol. 469, No. 2, 08.2017, p. 1369-1382.

Research output: Contribution to journalArticle

Harvard

Satpathy, S, Alam, S, Ho, S, White, M, Bahcall, NA, Beutler, F, Brownstein, JR, Chuang, C-H, Eisenstein, DJ, Grieb, JN, Kitaura, F-S, Olmstead, MD, Percival, WJ, Salazar-Albornoz, S, Sánchez, AG, Seo, H-J, Thomas, D, Tinker, JL & Tojeiro, R 2017, 'The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: on the measurement of growth rate using galaxy correlation functions', Monthly Notices of the Royal Astronomical Society, vol. 469, no. 2, pp. 1369-1382. https://doi.org/10.1093/mnras/stx883

APA

Satpathy, S., Alam, S., Ho, S., White, M., Bahcall, N. A., Beutler, F., Brownstein, J. R., Chuang, C-H., Eisenstein, D. J., Grieb, J. N., Kitaura, F-S., Olmstead, M. D., Percival, W. J., Salazar-Albornoz, S., Sánchez, A. G., Seo, H-J., Thomas, D., Tinker, J. L., & Tojeiro, R. (2017). The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: on the measurement of growth rate using galaxy correlation functions. Monthly Notices of the Royal Astronomical Society, 469(2), 1369-1382. https://doi.org/10.1093/mnras/stx883

Vancouver

Satpathy S, Alam S, Ho S, White M, Bahcall NA, Beutler F et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: on the measurement of growth rate using galaxy correlation functions. Monthly Notices of the Royal Astronomical Society. 2017 Aug;469(2):1369-1382. https://doi.org/10.1093/mnras/stx883

Author

Satpathy, Siddharth ; Alam, Shadab ; Ho, Shirley ; White, Martin ; Bahcall, Neta A. ; Beutler, Florian ; Brownstein, Joel R. ; Chuang, Chia-Hsun ; Eisenstein, Daniel J. ; Grieb, Jan Niklas ; Kitaura, Francisco-Shu ; Olmstead, Matthew D. ; Percival, Will J. ; Salazar-Albornoz, Salvador ; Sánchez, Ariel G. ; Seo, Hee-Jong ; Thomas, Daniel ; Tinker, Jeremy L. ; Tojeiro, Rita. / The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : on the measurement of growth rate using galaxy correlation functions. In: Monthly Notices of the Royal Astronomical Society. 2017 ; Vol. 469, No. 2. pp. 1369-1382.

Bibtex

@article{6571885759cd4a539d6b17e0cbf58cee,
title = "The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: on the measurement of growth rate using galaxy correlation functions",
abstract = "We present a measurement of the linear growth rate of structure, f, from the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 (DR12) using convolution Lagrangian perturbation theory (CLPT) with Gaussian streaming redshift space distortions (GSRSD) to model the two-point statistics of BOSS galaxies in DR12. The BOSS-DR12 data set includes 1198 006 massive galaxies spread over the redshift range 0.2 < z < 0.75. These galaxy samples are categorized in three redshift bins. Using CLPT-GSRSD in our analysis of the combined sample of the three redshift bins, we report measurements of fσ8 for the three redshift bins. We find fσ8 = 0.430 ± 0.054 at zeff = 0.38, fσ8 = 0.452 ± 0.057 at zeff = 0.51 and fσ8 = 0.457 ± 0.052 at zeff = 0.61. Our results are consistent with the predictions of Planck Λ cold dark matter-general relativity. Our constraints on the growth rates of structure in the Universe at different redshifts serve as a useful probe, which can help distinguish between a model of the Universe based on dark energy and models based on modified theories of gravity. 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.",
keywords = "astro-ph.CO",
author = "Siddharth Satpathy and Shadab Alam and Shirley Ho and Martin White and Bahcall, {Neta A.} and Florian Beutler and Brownstein, {Joel R.} and Chia-Hsun Chuang and Eisenstein, {Daniel J.} and Grieb, {Jan Niklas} and Francisco-Shu Kitaura and Olmstead, {Matthew D.} and Percival, {Will J.} and Salvador Salazar-Albornoz and S{\'a}nchez, {Ariel G.} and Hee-Jong Seo and Daniel Thomas and Tinker, {Jeremy L.} and Rita Tojeiro",
note = "This is one of the companion papers of the SDSS DR12 final cosmological result. Submitted to MNRAS. 15 pages, 7 figures, 2 tables.",
year = "2017",
month = aug,
doi = "10.1093/mnras/stx883",
language = "English",
volume = "469",
pages = "1369--1382",
journal = "MNRAS",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "2",

}

RIS

TY - JOUR

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

T2 - on the measurement of growth rate using galaxy correlation functions

AU - Satpathy, Siddharth

AU - Alam, Shadab

AU - Ho, Shirley

AU - White, Martin

AU - Bahcall, Neta A.

AU - Beutler, Florian

AU - Brownstein, Joel R.

AU - Chuang, Chia-Hsun

AU - Eisenstein, Daniel J.

AU - Grieb, Jan Niklas

AU - Kitaura, Francisco-Shu

AU - Olmstead, Matthew D.

AU - Percival, Will J.

AU - Salazar-Albornoz, Salvador

AU - Sánchez, Ariel G.

AU - Seo, Hee-Jong

AU - Thomas, Daniel

AU - Tinker, Jeremy L.

AU - Tojeiro, Rita

N1 - This is one of the companion papers of the SDSS DR12 final cosmological result. Submitted to MNRAS. 15 pages, 7 figures, 2 tables.

PY - 2017/8

Y1 - 2017/8

N2 - We present a measurement of the linear growth rate of structure, f, from the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 (DR12) using convolution Lagrangian perturbation theory (CLPT) with Gaussian streaming redshift space distortions (GSRSD) to model the two-point statistics of BOSS galaxies in DR12. The BOSS-DR12 data set includes 1198 006 massive galaxies spread over the redshift range 0.2 < z < 0.75. These galaxy samples are categorized in three redshift bins. Using CLPT-GSRSD in our analysis of the combined sample of the three redshift bins, we report measurements of fσ8 for the three redshift bins. We find fσ8 = 0.430 ± 0.054 at zeff = 0.38, fσ8 = 0.452 ± 0.057 at zeff = 0.51 and fσ8 = 0.457 ± 0.052 at zeff = 0.61. Our results are consistent with the predictions of Planck Λ cold dark matter-general relativity. Our constraints on the growth rates of structure in the Universe at different redshifts serve as a useful probe, which can help distinguish between a model of the Universe based on dark energy and models based on modified theories of gravity. 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.

AB - We present a measurement of the linear growth rate of structure, f, from the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 (DR12) using convolution Lagrangian perturbation theory (CLPT) with Gaussian streaming redshift space distortions (GSRSD) to model the two-point statistics of BOSS galaxies in DR12. The BOSS-DR12 data set includes 1198 006 massive galaxies spread over the redshift range 0.2 < z < 0.75. These galaxy samples are categorized in three redshift bins. Using CLPT-GSRSD in our analysis of the combined sample of the three redshift bins, we report measurements of fσ8 for the three redshift bins. We find fσ8 = 0.430 ± 0.054 at zeff = 0.38, fσ8 = 0.452 ± 0.057 at zeff = 0.51 and fσ8 = 0.457 ± 0.052 at zeff = 0.61. Our results are consistent with the predictions of Planck Λ cold dark matter-general relativity. Our constraints on the growth rates of structure in the Universe at different redshifts serve as a useful probe, which can help distinguish between a model of the Universe based on dark energy and models based on modified theories of gravity. 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.

KW - astro-ph.CO

U2 - 10.1093/mnras/stx883

DO - 10.1093/mnras/stx883

M3 - Article

VL - 469

SP - 1369

EP - 1382

JO - MNRAS

JF - MNRAS

SN - 0035-8711

IS - 2

ER -

ID: 7171230