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Title: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Single-probe measurements from DR12 galaxy clustering – towards an accurate model

Journal Article · · Monthly Notices of the Royal Astronomical Society
 [1];  [2];  [3];  [4];  [4];  [5];  [6];  [7];  [8];  [9];  [7];  [10];  [11];  [12];  [13];  [14];  [10];  [15];  [16];  [17] more »;  [18];  [19];  [20];  [21];  [18];  [22];  [13];  [23] « less
  1. Instituto de Astrofisica de Canarias (IAC), Tenerife (Spain); Univ. de La Laguna (ULL), Tenerife (Spain); Univ. Autonoma de Madrid, Madrid (Spain); Leibniz-Institut fur Astrophysik Potsdam (AIP), Potsdam (Germany)
  2. Univ. Autonoma de Madrid, Madrid (Spain); Campus of International Excellence UAM+CSIC, Madrid (Spain); Univ. de Madrid (UAM), Madrid (Spain)
  3. The Ohio State Univ., Columbus, OH (United States); Univ. of Portsmouth, Portsmouth (United Kingdom)
  4. Chinese Academy of Sciences (CAS), Beijing (China); Univ. of Portsmouth, Portsmouth (United Kingdom)
  5. Instituto de Astrofisica de Canarias (IAC), Tenerife (Spain); Univ. de La Laguna (ULL), Tenerife (Spain)
  6. Univ. Autonoma de Madrid, Madrid (Spain); Instituto de Astrofisica de Andalucia (CSIC), Granada (Spain)
  7. Sorbonne Univ., Paris (France); Univ. Pierre et Marie Curie, Paris (France)
  8. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of Portsmouth, Portsmouth (United Kingdom)
  9. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  10. Univ.-Sternwarte Munchen, Munich (Germany); Max-Planck-Institut fur extraterrestrische Physik, Garching (Germany)
  11. Carnegie Mellon Univ., Pittsburgh, PA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
  12. Leibniz-Institut fur Astrophysik Potsdam (AIP), Potsdam (Germany); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
  13. Univ. of Portsmouth, Portsmouth (United Kingdom)
  14. Sejong Univ., Seoul (Korea)
  15. Kansas State Univ., Manhattan, KS (United States); Brookhaven National Lab. (BNL), Upton, NY (United States); Univ. of Portsmouth, Portsmouth (United Kingdom)
  16. Max-Planck-Institut fur extraterrestrische Physik, Garching (Germany)
  17. Carnegie Mellon Univ., Pittsburgh, PA (United States)
  18. Brookhaven National Lab. (BNL), Upton, NY (United States)
  19. New York Univ. (NYU), NY (United States)
  20. Univ. of St. Andrews, St. Andrews (United Kingdom)
  21. Univ. Nacional Autonoma de Mexico (Mexico)
  22. Univ. of Utah, Salt Lake City, UT (United States)
  23. King's College, Wilkes Barre, PA (United States)
+ Show Author Affiliations

With the largest spectroscopic galaxy survey volume drawn from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS), we can extract cosmological constraints from the measurements of redshift and geometric distortions at quasi-linear scales (e.g. above 50 h -1 Mpc). We analyse the broad-range shape of the monopole and quadrupole correlation functions of the BOSS Data Release 12 (DR12) CMASS galaxy sample, at the effective redshift z = 0.59, to obtain constraints on the Hubble expansion rate H(z), the angular- diameter distance D A (z), the normalized growth rate f(z)σ 8 (z), and the physical matter density Ω m h 2 .We obtain robust measurements by including a polynomial as the model for the systematic errors, and find it works very well against the systematic effects, e.g. ones induced by stars and seeing. We provide accurate measurements (D A (0.59)r s,fid /r s , H(0.59)r s /r s,fid , f(0.59)σ 8 (0.59), Ω m h 2 ) = (1427 ± 26 Mpc, 97.3 ± 3.3 kms -1 Mpc -1 , 0.488 ± 0.060, 0.135 ± 0.016), where r s is the comoving sound horizon at the drag epoch and r s,fid = 147.66 Mpc is the sound scale of the fiducial cosmology used in this study. The parameters which are not well constrained by our galaxy clustering analysis are marginalized over with wide flat priors. Since no priors from other data sets, e.g. cosmic microwave background (CMB), are adopted and no dark energy models are assumed, our results from BOSS CMASS galaxy clustering alone may be combined with other data sets, i.e. CMB, SNe, lensing or other galaxy clustering data to constrain the parameters of a given cosmological model. The uncertainty on the dark energy equation of state parameter, w, from CMB+CMASS is about 8 per cent. The uncertainty on the curvature fraction, Ω k , is 0.3 per cent. We do not find deviation from flat ΛCDM.

Research Organization:
Brookhaven National Lab. (BNL), Upton, NY (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
SC00112704; AC02-05CH11231
OSTI ID:
1324269
Alternate ID(s):
OSTI ID: 1377516
Report Number(s):
BNL-112529-2016-JA; KA2301020
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 461, Issue 4; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 76 works
Citation information provided by
Web of Science

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Testing cosmological structure formation using redshift-space distortions text January 2008
Reliability of the detection of the Baryon Acoustic Peak text January 2008
The WiggleZ Dark Energy Survey: Survey Design and First Data Release text January 2009
Acoustic scale from the angular power spectra of SDSS-III DR8 photometric luminous galaxies text January 2012
Using Multipoles of the Correlation Function to Measure H(z), D_A(z), and β(z) from Sloan Digital Sky Survey Luminous Red Galaxies text January 2012
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring D_A and H at z=0.57 from the Baryon Acoustic Peak in the Data Release 9 Spectroscopic Galaxy Sample text January 2013
Planck 2013 results. I. Overview of products and scientific results text January 2013
Planck 2013 results. XVI. Cosmological parameters text January 2013
Modelling Baryon Acoustic Oscillations with Perturbation Theory and Stochastic Halo Biasing text January 2013
Simultaneous constraints on the growth of structure and cosmic expansion from the multipole power spectra of the SDSS DR7 LRG sample text January 2013
Measurement of $H(z)$ and $D_A(z)$ from the two-dimensional power spectrum of Sloan Digital Sky Survey luminous red galaxies text January 2013
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples text January 2013
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: galaxy clustering measurements in the low redshift sample of Data Release 11 text January 2014
A 2.5% measurement of the growth rate from small-scale redshift space clustering of SDSS-III CMASS galaxies text January 2014
Model-Independent Measurements of Cosmic Expansion and Growth at z=0.57 Using the Anisotropic Clustering of CMASS Galaxies From the Sloan Digital Sky Survey Data Release 9 text January 2014
Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies text January 2015
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Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample text January 2001
Cosmological parameters from CMB and other data: a Monte-Carlo approach text January 2002
The Third Data Release of the Sloan Digital Sky Survey text January 2004
Memory of Initial Conditions in Gravitational Clustering text January 2005
The 2.5 m Telescope of the Sloan Digital Sky Survey text January 2006
On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter text January 2006
The Clustering of Luminous Red Galaxies in the Sloan Digital Sky Survey Imaging Data text January 2006
Cosmological baryonic and matter densities from 600,000 SDSS Luminous Red Galaxies with photometric redshifts text January 2006
Baryonic Features in the Matter Transfer Function text January 1997
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Cited By (30)

Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS journal November 2016
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: towards a computationally efficient analysis without informative priors journal March 2017
Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters journal February 2020
Conjoined constraints on modified gravity from the expansion history and cosmic growth journal September 2017
Unraveling the effective fluid approach for f ( R ) models in the subhorizon approximation journal February 2019
Dipolar modulation in the size of galaxies: the effect of Doppler magnification journal August 2017
Internal robustness of growth rate data journal October 2018
A semi-analytical perspective on massive galaxies at z ∼ 0.55 journal March 2019
Planck 2015 results : XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation journal September 2016
Observational constraints on the oscillating dark energy cosmologies journal February 2019
Cosmological constraints from a joint analysis of cosmic growth and expansion journal July 2017
Constraining power of cosmological observables: Blind redshift spots and optimal ranges journal March 2019
Cosmological signatures of dark sector physics: the evolution of haloes and spin alignment journal January 2020
The VIMOS Public Extragalactic Redshift Survey (VIPERS): Gravity test from the combination of redshift-space distortions and galaxy-galaxy lensing at 0.5 <  z  < 1.2⋆ journal December 2017
Growth of matter perturbations in the bi-Galileons field model journal December 2019
Effective gravitational coupling in modified teleparallel theories journal April 2018
Planck 2015 results : XIII. Cosmological parameters journal September 2016
Model-independent reconstruction of the linear anisotropic stress η journal November 2018
Coupled quintessence with a ΛCDM background: removing the σ 8 tension journal January 2019
Planck 2015 results : X. Diffuse component separation: Foreground maps journal September 2016
Planck 2015 results : XVI. Isotropy and statistics of the CMB journal September 2016
Planck 2015 results : XXVI. The Second journal September 2016
Planck 2015 results. XIII. Cosmological parameters text January 2015
Validating estimates of the growth rate of structure with modified gravity simulations text January 2016
Dipolar modulation in the size of galaxies: The effect of Doppler magnification text January 2016
Cosmological constraints from a joint analysis of cosmic growth and expansion text January 2017
Effective gravitational coupling in modified teleparallel theories text January 2018
Constraining power of cosmological observables: blind redshift spots and optimal ranges text January 2018
Observational constraints on the oscillating dark energy cosmologies text January 2019
Designing Horndeski and the effective fluid approach text January 2019

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