The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the quasar sample between redshift 0.8 and 2.2

被引:189
作者
Neveux, Richard [1 ]
Burtin, Etienne [1 ]
de Mattia, Arnaud [1 ]
Smith, Alex [1 ]
Ross, Ashley J. [2 ]
Hou, Jiamin [3 ]
Bautista, Julian [4 ]
Brinkmann, Jonathan [5 ]
Chuang, Chia-Hsun [6 ]
Dawson, Kyle S. [7 ]
Gil-Marin, Hector [8 ,9 ]
Lyke, Brad W. [10 ]
de la Macorra, Axel [11 ]
des Bourboux, Helion du Mas [7 ]
Mohammad, Faizan G. [12 ,13 ]
Mueller, Eva-Maria [14 ]
Myers, Adam D. [10 ]
Newman, Jeffrey A. [15 ]
Percival, Will J. [12 ,13 ,16 ]
Rossi, Graziano [17 ]
Schneider, Donald [18 ]
Vivek, M. [19 ,20 ]
Zarrouk, Pauline [1 ,21 ]
Zhao, Cheng [22 ]
Zhao, Gong-Bo [23 ]
机构
[1] Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France
[2] Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA
[3] Max Planck Inst Extraterr Phys, Giessenbachstr,Postfach 1312, D-85748 Garching, Germany
[4] Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
[5] Apache Point Observ, POB 59, Sunspot, NM 88349 USA
[6] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94305 USA
[7] Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
[8] Univ Barcelona, Inst Ciencies Cosmos, ICCUB, Marti i Franques 1, E-08028 Barcelona, Spain
[9] Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona, Spain
[10] Univ Wyoming, 1000 E Univ Ave, Laramie, WY 82071 USA
[11] Univ Nacl Autonoma Mexico, Inst Fis, Apdo Postal 20-364, Mexico City, DF, Mexico
[12] Univ Waterloo, Waterloo Ctr Astrophys, Waterloo, ON N2L 3G1, Canada
[13] Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
[14] Univ Oxford, Dept Phys, Subdept Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
[15] Univ Pittsburgh, PITT PACC, Dept Phys & Astron, Pittsburgh, PA 15260 USA
[16] Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada
[17] Sejong Univ, Dept Phys & Astron, Seoul 143747, South Korea
[18] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
[19] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[20] Indian Inst Astrophys, Bangalore 560034, Karnataka, India
[21] Univ Durham, Inst Computat Cosmol, Dept Phys, South Rd, Durham DH1 3LE, England
[22] Ecole Polytech Fed Lausanne EPFL, Observ Sauverny, Inst Phys, Lab Astrophys, CH-1290 Versoix, Switzerland
[23] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
基金
美国国家科学基金会; 美国安德鲁·梅隆基金会;
关键词
galaxies: distances and redshifts; dark energy; distance scale; large-scale structure of Universe; cosmology: observations; FIBER COLLISIONS; GALAXIES; SPACE; EVOLUTION; CATALOGS;
D O I
10.1093/mnras/staa2780
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We measure the clustering of quasars of the final data release (DR16) of eBOSS. The sample contains 343 708 quasars between redshifts 0.8 <= z <= 2.2 over 4699 deg2. We calculate the Legendre multipoles (0,2,4) of the anisotropic power spectrum and perform a BAO and a Full-Shape (FS) analysis at the effective redshift z(eff) = 1.480. The errors include systematic errors that amount to 1/3 of the statistical error. The systematic errors comprise a modelling part studied using a blind N-body mock challenge and observational effects studied with approximate mocks to account for various types of redshift smearing and fibre collisions. For the BAO analysis, we measure the transverse comoving distance D-M(zeff)/r(drag) = 30.60 +/- 0.90 and the Hubble distance D-H(zeff)/r(drag) = 13.34 +/- 0.60. This agrees with the configuration space analysis, and the consensus yields: D-M(zeff)/r(drag) = 30.69 +/- 0.80 and D-H(zeff)/r(drag) = 13.26 +/- 0.55. In the FS analysis, we fit the power spectrum using a model based on Regularised Perturbation Theory, which includes redshift space distortions and the Alcock-Paczynski effect. The results are D-M(zeff)/r(drag) = 30.68 +/- 0.90 and D-H(zeff)/r(drag) = 13.52 +/- 0.51 and we constrain the linear growth rate of structure f(zeff)sigma 8(z(eff)) = 0.476 +/- 0.047. Our results agree with the configuration space analysis. The consensus analysis of the eBOSS quasar sample yields: D-M(zeff)/r(drag) = 30.21 +/- 0.79, D-H(zeff)/r(drag) = 3.23 +/- 0.47, and f(z(eff))sigma(8)(z(eff)) = 0.462 +/- 0.045 and is consistent with a flat Lambda CDM cosmological model using Planck results.
引用
收藏
页码:210 / 229
页数:20
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