The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift-space distortions between redshift 0.8 and 2.2

被引：21

作者：

Ruggeri, Rossana ^{[1
]}

Percival, Will J. ^{[1
]}

Gil-Marin, Hector ^{[2
,3
]}

Beutler, Florian ^{[1
,4
]}

Mueller, Eva-Maria ^{[1
]}

Zhu, Fangzhou ^{[5
]}

Padmanabhan, Nikhil ^{[5
]}

Zhao, Gong-Bo ^{[1
,6
]}

Zarrouk, Pauline ^{[7
]}

Sanchez, Ariel G. ^{[8
]}

Bautista, Julian ^{[9
]}

Brinkmann, Jonathan ^{[10
]}

Brownstein, Joel R. ^{[9
]}

Baumgarten, Falk ^{[11
]}

Chuang, Chia-Hsun ^{[11
,12
,13
]}

Dawson, Kyle ^{[9
]}

Seo, Hee-Jong ^{[14
]}

Tojeiro, Rita ^{[15
]}

Zhao, Cheng ^{[16
,17
]}

机构：

[1] Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England

[2] Sorbonne Univ, ILP, 98 Bis Blvd Arago, F-75014 Paris, France

[3] Univ Paris 06, Lab Phys Nucl & Hautes Energies, 4 Pl Jussieu, F-75005 Paris, France

[4] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA

[5] Yale Univ, Dept Phys, New Haven, CT 06511 USA

[6] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China

[7] Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France

[8] Max Planck Inst Extraterr Phys, Postfach 1312,Giessenbachstr, D-85741 Garching, Germany

[9] Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA

[10] Apache Point Observ, POB 59, Sunspot, NM 88349 USA

[11] Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany

[12] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA

[13] Stanford Univ, Phys Dept, Stanford, CA 94305 USA

[14] Ohio Univ, Dept Phys & Astron, Clippinger Labs, Athens, OH 45701 USA

[15] Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland

[16] Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China

[17] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2019年 / 483卷 / 03期

基金：

美国安德鲁·梅隆基金会; 欧洲研究理事会; 英国科学技术设施理事会; 美国国家科学基金会;

关键词：

cosmology: observations; dark energy; dark matter; large-scale structure of Universe; POWER-SPECTRUM; ACOUSTIC-OSCILLATIONS; GALAXIES;

D O I：

10.1093/mnras/sty3395

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We measure the growth rate and its evolution using the anisotropic clustering of the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Data Release 14 (DR14) quasar sample, which includes 148 659 quasars covering the wide redshift range of 0.8 < z < 2.2 and a sky area of 2112.90 deg(2). To optimize measurements we deploy a redshift-dependent weighting scheme, which allows us to avoid binning and perform the data analysis consistently including the redshift evolution across the sample. We perform the analysis in Fourier space, and use the redshift evolving power spectrum multipoles to measure the redshift-space distortion parameter f sigma(8) and parameters controlling the anisotropic projection of the cosmological perturbations. We measure f sigma(8)(z = 1.52) = 0.43 +/- 0.05 and df sigma(8)/dz (z = 1.52) = -0.16 +/- 0.08, consistent with the expectation for a lambda cold dark matter cosmology as constrained by the Planck experiment.

引用

页码：3878 / 3887

页数：10

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