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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space

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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : tomographic BAO analysis of DR12 combined sample in Fourier space. / Zhao, Gong-Bo; Wang, Yuting; Saito, Shun; Wang, Dandan; Ross, Ashley Jacob; Beutler, Florian; Grieb, Jan Niklas; Chuang, Chia-Hsun; Kitaura, Francisco-Shu; Rodriguez-Torres, Sergio; Percival, Will; Brownstein, Joel R.; Cuesta, Antonio J.; Eisenstein, Daniel J.; Gil Marin, Hector; Kneib, Jean-Paul; Nichol, Bob; Olmstead, Matthew D.; Prada, Francisco; Rossi, Graziano; Salazar-Albornoz, Salvador; Samushia, Lado; Sánchez, Ariel G.; Thomas, Daniel; Tinker, Jeremy L.; Tojeiro, Rita; Weinberg, David H.; Zhu, Fangzhou.

In: Monthly Notices of the Royal Astronomical Society, Vol. 466, No. 1, 04.2017, p. 762-779.

Research output: Contribution to journalArticle

Harvard

Zhao, G-B, Wang, Y, Saito, S, Wang, D, Ross, AJ, Beutler, F, Grieb, JN, Chuang, C-H, Kitaura, F-S, Rodriguez-Torres, S, Percival, W, Brownstein, JR, Cuesta, AJ, Eisenstein, DJ, Gil Marin, H, Kneib, J-P, Nichol, B, Olmstead, MD, Prada, F, Rossi, G, Salazar-Albornoz, S, Samushia, L, Sánchez, AG, Thomas, D, Tinker, JL, Tojeiro, R, Weinberg, DH & Zhu, F 2017, 'The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space', Monthly Notices of the Royal Astronomical Society, vol. 466, no. 1, pp. 762-779. https://doi.org/10.1093/mnras/stw3199

APA

Zhao, G-B., Wang, Y., Saito, S., Wang, D., Ross, A. J., Beutler, F., Grieb, J. N., Chuang, C-H., Kitaura, F-S., Rodriguez-Torres, S., Percival, W., Brownstein, J. R., Cuesta, A. J., Eisenstein, D. J., Gil Marin, H., Kneib, J-P., Nichol, B., Olmstead, M. D., Prada, F., ... Zhu, F. (2017). The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space. Monthly Notices of the Royal Astronomical Society, 466(1), 762-779. https://doi.org/10.1093/mnras/stw3199

Vancouver

Author

Zhao, Gong-Bo ; Wang, Yuting ; Saito, Shun ; Wang, Dandan ; Ross, Ashley Jacob ; Beutler, Florian ; Grieb, Jan Niklas ; Chuang, Chia-Hsun ; Kitaura, Francisco-Shu ; Rodriguez-Torres, Sergio ; Percival, Will ; Brownstein, Joel R. ; Cuesta, Antonio J. ; Eisenstein, Daniel J. ; Gil Marin, Hector ; Kneib, Jean-Paul ; Nichol, Bob ; Olmstead, Matthew D. ; Prada, Francisco ; Rossi, Graziano ; Salazar-Albornoz, Salvador ; Samushia, Lado ; Sánchez, Ariel G. ; Thomas, Daniel ; Tinker, Jeremy L. ; Tojeiro, Rita ; Weinberg, David H. ; Zhu, Fangzhou. / The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : tomographic BAO analysis of DR12 combined sample in Fourier space. In: Monthly Notices of the Royal Astronomical Society. 2017 ; Vol. 466, No. 1. pp. 762-779.

Bibtex

@article{e107a4ecc39f41a889b618ef01e338b8,
title = "The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space",
abstract = "We perform a tomographic baryon acoustic oscillations (BAO) analysis using the monopole, quadrupole and hexadecapole of the redshift-space galaxy power spectrum measured from the pre-reconstructed combined galaxy sample of the completed Sloan Digital Sky Survey (SDSS-III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release (DR)12 covering the redshift range of 0.20<z<0.75. By allowing for overlap between neighbouring redshift slices, we successfully obtained the isotropic and anisotropic BAO distance measurements within nine redshift slices to a precision of 1.5%−3.4% for DV/rd, 1.8%−4.2% for DA/rd and 3.7%−7.5% for H rd, depending on effective redshifts. We provide our BAO measurement of DA/rd and H rd with the full covariance matrix, which can be used for cosmological implications. Our measurements are consistent with those presented in Alam et al. (2016), in which the BAO distances are measured at three effective redshifts. We constrain dark energy parameters using our measurements, and find an improvement of the Figure-of-Merit of dark energy in general due to the temporal BAO information resolved. This paper is part of a set that analyses the final galaxy clustering dataset from BOSS.",
keywords = "galaxies: distances and redshifts, cosmological parameters, cosmology: observations, dark energy, distance scale, large-scale structure of Universe",
author = "Gong-Bo Zhao and Yuting Wang and Shun Saito and Dandan Wang and Ross, {Ashley Jacob} and Florian Beutler and Grieb, {Jan Niklas} and Chia-Hsun Chuang and Francisco-Shu Kitaura and Sergio Rodriguez-Torres and Will Percival and Brownstein, {Joel R.} and Cuesta, {Antonio J.} and Eisenstein, {Daniel J.} and {Gil Marin}, Hector and Jean-Paul Kneib and Bob Nichol and Olmstead, {Matthew D.} and Francisco Prada and Graziano Rossi and Salvador Salazar-Albornoz and Lado Samushia and S{\'a}nchez, {Ariel G.} and Daniel Thomas and Tinker, {Jeremy L.} and Rita Tojeiro and Weinberg, {David H.} and Fangzhou Zhu",
year = "2017",
month = apr,
doi = "10.1093/mnras/stw3199",
language = "English",
volume = "466",
pages = "762--779",
journal = "MNRAS",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "1",

}

RIS

TY - JOUR

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

T2 - tomographic BAO analysis of DR12 combined sample in Fourier space

AU - Zhao, Gong-Bo

AU - Wang, Yuting

AU - Saito, Shun

AU - Wang, Dandan

AU - Ross, Ashley Jacob

AU - Beutler, Florian

AU - Grieb, Jan Niklas

AU - Chuang, Chia-Hsun

AU - Kitaura, Francisco-Shu

AU - Rodriguez-Torres, Sergio

AU - Percival, Will

AU - Brownstein, Joel R.

AU - Cuesta, Antonio J.

AU - Eisenstein, Daniel J.

AU - Gil Marin, Hector

AU - Kneib, Jean-Paul

AU - Nichol, Bob

AU - Olmstead, Matthew D.

AU - Prada, Francisco

AU - Rossi, Graziano

AU - Salazar-Albornoz, Salvador

AU - Samushia, Lado

AU - Sánchez, Ariel G.

AU - Thomas, Daniel

AU - Tinker, Jeremy L.

AU - Tojeiro, Rita

AU - Weinberg, David H.

AU - Zhu, Fangzhou

PY - 2017/4

Y1 - 2017/4

N2 - We perform a tomographic baryon acoustic oscillations (BAO) analysis using the monopole, quadrupole and hexadecapole of the redshift-space galaxy power spectrum measured from the pre-reconstructed combined galaxy sample of the completed Sloan Digital Sky Survey (SDSS-III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release (DR)12 covering the redshift range of 0.20<z<0.75. By allowing for overlap between neighbouring redshift slices, we successfully obtained the isotropic and anisotropic BAO distance measurements within nine redshift slices to a precision of 1.5%−3.4% for DV/rd, 1.8%−4.2% for DA/rd and 3.7%−7.5% for H rd, depending on effective redshifts. We provide our BAO measurement of DA/rd and H rd with the full covariance matrix, which can be used for cosmological implications. Our measurements are consistent with those presented in Alam et al. (2016), in which the BAO distances are measured at three effective redshifts. We constrain dark energy parameters using our measurements, and find an improvement of the Figure-of-Merit of dark energy in general due to the temporal BAO information resolved. This paper is part of a set that analyses the final galaxy clustering dataset from BOSS.

AB - We perform a tomographic baryon acoustic oscillations (BAO) analysis using the monopole, quadrupole and hexadecapole of the redshift-space galaxy power spectrum measured from the pre-reconstructed combined galaxy sample of the completed Sloan Digital Sky Survey (SDSS-III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release (DR)12 covering the redshift range of 0.20<z<0.75. By allowing for overlap between neighbouring redshift slices, we successfully obtained the isotropic and anisotropic BAO distance measurements within nine redshift slices to a precision of 1.5%−3.4% for DV/rd, 1.8%−4.2% for DA/rd and 3.7%−7.5% for H rd, depending on effective redshifts. We provide our BAO measurement of DA/rd and H rd with the full covariance matrix, which can be used for cosmological implications. Our measurements are consistent with those presented in Alam et al. (2016), in which the BAO distances are measured at three effective redshifts. We constrain dark energy parameters using our measurements, and find an improvement of the Figure-of-Merit of dark energy in general due to the temporal BAO information resolved. This paper is part of a set that analyses the final galaxy clustering dataset from BOSS.

KW - galaxies: distances and redshifts

KW - cosmological parameters

KW - cosmology: observations

KW - dark energy

KW - distance scale

KW - large-scale structure of Universe

U2 - 10.1093/mnras/stw3199

DO - 10.1093/mnras/stw3199

M3 - Article

VL - 466

SP - 762

EP - 779

JO - MNRAS

JF - MNRAS

SN - 0035-8711

IS - 1

ER -

ID: 5193483