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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration space

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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample : anisotropic clustering analysis in configuration space. / Hou, Jiamin; Sánchez, Ariel G.; Scoccimarro, Román; Salazar-Albornoz, Salvador; Burtin, Etienne; Gil-Marín, Héctor; Percival, Will J.; Ruggeri, Rossana; Zarrouk, Pauline; Zhao, Gong Bo; Bautista, Julian; Brinkmann, Jonathan; Brownstein, Joel R.; Dawson, Kyle S.; Chandrachani Devi, N.; Myers, Adam D.; Habib, Salman; Heitmann, Katrin; Tojeiro, Rita; Rossi, Graziano; Schneider, Donald P.; Seo, Hee Jong; Wang, Yuting.

In: Monthly Notices of the Royal Astronomical Society, Vol. 480, No. 2, 01.10.2018, p. 2521-2534.

Research output: Contribution to journalArticle

Harvard

Hou, J, Sánchez, AG, Scoccimarro, R, Salazar-Albornoz, S, Burtin, E, Gil-Marín, H, Percival, WJ, Ruggeri, R, Zarrouk, P, Zhao, GB, Bautista, J, Brinkmann, J, Brownstein, JR, Dawson, KS, Chandrachani Devi, N, Myers, AD, Habib, S, Heitmann, K, Tojeiro, R, Rossi, G, Schneider, DP, Seo, HJ & Wang, Y 2018, 'The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration space', Monthly Notices of the Royal Astronomical Society, vol. 480, no. 2, pp. 2521-2534. https://doi.org/10.1093/MNRAS/STY1984

APA

Hou, J., Sánchez, A. G., Scoccimarro, R., Salazar-Albornoz, S., Burtin, E., Gil-Marín, H., Percival, W. J., Ruggeri, R., Zarrouk, P., Zhao, G. B., Bautista, J., Brinkmann, J., Brownstein, J. R., Dawson, K. S., Chandrachani Devi, N., Myers, A. D., Habib, S., Heitmann, K., Tojeiro, R., ... Wang, Y. (2018). The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration space. Monthly Notices of the Royal Astronomical Society, 480(2), 2521-2534. https://doi.org/10.1093/MNRAS/STY1984

Vancouver

Hou J, Sánchez AG, Scoccimarro R, Salazar-Albornoz S, Burtin E, Gil-Marín H et al. The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration space. Monthly Notices of the Royal Astronomical Society. 2018 Oct 1;480(2):2521-2534. https://doi.org/10.1093/MNRAS/STY1984

Author

Hou, Jiamin ; Sánchez, Ariel G. ; Scoccimarro, Román ; Salazar-Albornoz, Salvador ; Burtin, Etienne ; Gil-Marín, Héctor ; Percival, Will J. ; Ruggeri, Rossana ; Zarrouk, Pauline ; Zhao, Gong Bo ; Bautista, Julian ; Brinkmann, Jonathan ; Brownstein, Joel R. ; Dawson, Kyle S. ; Chandrachani Devi, N. ; Myers, Adam D. ; Habib, Salman ; Heitmann, Katrin ; Tojeiro, Rita ; Rossi, Graziano ; Schneider, Donald P. ; Seo, Hee Jong ; Wang, Yuting. / The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample : anisotropic clustering analysis in configuration space. In: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 480, No. 2. pp. 2521-2534.

Bibtex

@article{a56b1c562d6a4b69a7bf8a46385b45da,
title = "The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration space",
abstract = "We explore the cosmological implications of anisotropic clustering measurements of the quasar sample from Data Release 14 (DR14) of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (eBOSS) in configuration space. The ~147 000 quasar sample observed by eBOSS offers a direct tracer of the density field and bridges the gap of previous baryon acoustic oscillation measurements between redshift 0.8 < z < 2.2. By analysing the two-point correlation function characterized by clustering wedges ξwi (s) and multipoles ξℓ(s), we measure the angular diameter distance, Hubble parameter, and cosmic structure growth rate. We define a systematic error budget for our measurements based on the analysis of N-body simulations and mock catalogues. Based on the DR14 large-scale structure quasar sample at the effective redshift zeff = 1.52, we find the growth rate of cosmic structure fσ8(zeff) = 0.396 ± 0.079, and the geometric parameters DV(z)/rd = 26.47 ± 1.23, and FAP(z) = 2.53 ± 0.22, where the uncertainties include both statistical and systematic errors. These values are in excellent agreement with the best-fitting standard Λ cold dark matter model to the latest cosmic microwave background data from Planck.",
keywords = "Cosmology, Data analysis, Large-scale structure of Universe, Quasars",
author = "Jiamin Hou and S{\'a}nchez, {Ariel G.} and Rom{\'a}n Scoccimarro and Salvador Salazar-Albornoz and Etienne Burtin and H{\'e}ctor Gil-Mar{\'i}n and Percival, {Will J.} and Rossana Ruggeri and Pauline Zarrouk and Zhao, {Gong Bo} and Julian Bautista and Jonathan Brinkmann and Brownstein, {Joel R.} and Dawson, {Kyle S.} and {Chandrachani Devi}, N. and Myers, {Adam D.} and Salman Habib and Katrin Heitmann and Rita Tojeiro and Graziano Rossi and Schneider, {Donald P.} and Seo, {Hee Jong} and Yuting Wang",
year = "2018",
month = oct
day = "1",
doi = "10.1093/MNRAS/STY1984",
language = "English",
volume = "480",
pages = "2521--2534",
journal = "MNRAS",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "2",

}

RIS

TY - JOUR

T1 - The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample

T2 - anisotropic clustering analysis in configuration space

AU - Hou, Jiamin

AU - Sánchez, Ariel G.

AU - Scoccimarro, Román

AU - Salazar-Albornoz, Salvador

AU - Burtin, Etienne

AU - Gil-Marín, Héctor

AU - Percival, Will J.

AU - Ruggeri, Rossana

AU - Zarrouk, Pauline

AU - Zhao, Gong Bo

AU - Bautista, Julian

AU - Brinkmann, Jonathan

AU - Brownstein, Joel R.

AU - Dawson, Kyle S.

AU - Chandrachani Devi, N.

AU - Myers, Adam D.

AU - Habib, Salman

AU - Heitmann, Katrin

AU - Tojeiro, Rita

AU - Rossi, Graziano

AU - Schneider, Donald P.

AU - Seo, Hee Jong

AU - Wang, Yuting

PY - 2018/10/1

Y1 - 2018/10/1

N2 - We explore the cosmological implications of anisotropic clustering measurements of the quasar sample from Data Release 14 (DR14) of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (eBOSS) in configuration space. The ~147 000 quasar sample observed by eBOSS offers a direct tracer of the density field and bridges the gap of previous baryon acoustic oscillation measurements between redshift 0.8 < z < 2.2. By analysing the two-point correlation function characterized by clustering wedges ξwi (s) and multipoles ξℓ(s), we measure the angular diameter distance, Hubble parameter, and cosmic structure growth rate. We define a systematic error budget for our measurements based on the analysis of N-body simulations and mock catalogues. Based on the DR14 large-scale structure quasar sample at the effective redshift zeff = 1.52, we find the growth rate of cosmic structure fσ8(zeff) = 0.396 ± 0.079, and the geometric parameters DV(z)/rd = 26.47 ± 1.23, and FAP(z) = 2.53 ± 0.22, where the uncertainties include both statistical and systematic errors. These values are in excellent agreement with the best-fitting standard Λ cold dark matter model to the latest cosmic microwave background data from Planck.

AB - We explore the cosmological implications of anisotropic clustering measurements of the quasar sample from Data Release 14 (DR14) of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (eBOSS) in configuration space. The ~147 000 quasar sample observed by eBOSS offers a direct tracer of the density field and bridges the gap of previous baryon acoustic oscillation measurements between redshift 0.8 < z < 2.2. By analysing the two-point correlation function characterized by clustering wedges ξwi (s) and multipoles ξℓ(s), we measure the angular diameter distance, Hubble parameter, and cosmic structure growth rate. We define a systematic error budget for our measurements based on the analysis of N-body simulations and mock catalogues. Based on the DR14 large-scale structure quasar sample at the effective redshift zeff = 1.52, we find the growth rate of cosmic structure fσ8(zeff) = 0.396 ± 0.079, and the geometric parameters DV(z)/rd = 26.47 ± 1.23, and FAP(z) = 2.53 ± 0.22, where the uncertainties include both statistical and systematic errors. These values are in excellent agreement with the best-fitting standard Λ cold dark matter model to the latest cosmic microwave background data from Planck.

KW - Cosmology

KW - Data analysis

KW - Large-scale structure of Universe

KW - Quasars

UR - http://www.scopus.com/inward/record.url?scp=85054080662&partnerID=8YFLogxK

U2 - 10.1093/MNRAS/STY1984

DO - 10.1093/MNRAS/STY1984

M3 - Article

AN - SCOPUS:85054080662

VL - 480

SP - 2521

EP - 2534

JO - MNRAS

JF - MNRAS

SN - 0035-8711

IS - 2

ER -

ID: 15862336