The power spectrum and bispectrum of SDSS DR11 BOSS galaxies - I. Bias and gravity

被引:180
作者
Gil-Marin, Hector [1 ]
Norena, Jorge [2 ,3 ,4 ]
Verde, Licia [2 ,5 ,6 ]
Percival, Will J. [1 ]
Wagner, Christian [7 ]
Manera, Marc [8 ]
Schneider, Donald P. [9 ,10 ]
机构
[1] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England
[2] Univ Barcelona, IEEC UB, Inst Ciencies Cosmos, E-08028 Barcelona, Spain
[3] Univ Geneva, Dept Theoret Phys, CH-1211 Geneva 4, Switzerland
[4] Ctr Astroparticle Phys, CH-1211 Geneva 4, Switzerland
[5] Inst Catalana Recerca & Estudis Avancats, E-08010 Barcelona, Spain
[6] Univ Oslo, Inst Theoret Astrophys, N-0316 Oslo, Norway
[7] Max Planck Inst Astrophys, D-85741 Garching, Germany
[8] UCL, London WC1E 6BT, England
[9] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[10] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
基金
美国安德鲁·梅隆基金会; 英国科学技术设施理事会; 欧洲研究理事会; 美国国家科学基金会;
关键词
galaxies: haloes; cosmological parameters; cosmology: theory; large-scale structure of Universe; OSCILLATION SPECTROSCOPIC SURVEY; DIGITAL SKY SURVEY; 3-POINT CORRELATION-FUNCTION; LARGE-SCALE STRUCTURE; BARYON ACOUSTIC-OSCILLATIONS; SHANE-WIRTANEN CATALOG; DATA RELEASE; NONLINEAR EVOLUTION; GRAVITATIONAL-INSTABILITY; COSMOLOGICAL PARAMETERS;
D O I
10.1093/mnras/stv961
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We analyse the anisotropic clustering of the Baryon Oscillation Spectroscopic Survey CMASS Data Release 11 sample, which consists of 690 827 galaxies in the redshift range 0.43 < z < 0.70 and has a sky coverage of 8498 deg(2) corresponding to an effective volume of similar to 6 Gpc(3). We fit the Fourier space statistics, the power spectrum and bispectrum monopoles to measure the linear and quadratic bias parameters, b(1) and b(2), for a non-linear non-local bias model, the growth of structure parameter f and the amplitude of dark matter density fluctuations parametrized by as. We obtain b(1)(z(eff))(1.40)sigma-8(z(eff)) = 1.672 +/- 0.060 and bc.231) (zerf)a8(zerf) = 0.579 0.082 at the effective redshift of the survey, zeff = 0.57. The main cosmological result is the constraint on the combination /41(zeff)a8(z(eff)) = 0.582 +/- 0.084, which is complementary to fas constraints obtained from two-point redshift-space distortion analyses. A less conservative analysis yields f(0.43)(zeft)sigma 8(zeff) = 0.584 +/- 0.051. We ensure that our result is robust by performing detailed systematic tests using a large suite of survey galaxy mock catalogues and N-body simulations. The constraints on f(0.43) sigma(8) are useful for setting additional constraints on neutrino mass, gravity, curvature as well as the number of neutrino species from galaxy surveys analyses (as presented in a companion paper).
引用
收藏
页码:539 / 580
页数:42
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