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Title: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Double-probe measurements from BOSS galaxy clustering and Planck data – towards an analysis without informative priors

Journal Article · · Monthly Notices of the Royal Astronomical Society
DOI:https://doi.org/10.1093/mnras/stx751· OSTI ID:1324283
 [1];  [2];  [3];  [4];  [5];  [5];  [6];  [7];  [8];  [8];  [9];  [10];  [11];  [12];  [13];  [14];  [15];  [16];  [17];  [13] more »;  [18];  [19];  [9];  [20];  [21];  [22];  [23];  [24];  [16];  [25] « less
  1. Instituto de Astrofisica de Canarias (IAC), Tenerife (Spain); Univ. de La Laguna, Tenerife (Spain); Univ. Autonoma de Madrid, Madrid (Spain); Leibniz-Institut fur Astrophysik Potsdam (AIP), Potsdam (Germany)
  2. Univ. Autonoma de Madrid, Madrid (Spain); Leibniz-Institut fur Astrophysik Potsdam (AIP), Potsdam (Germany)
  3. Instituto de Astrofisica de Canarias (IAC), Tenerife (Spain); Univ. de La Laguna, Tenerife (Spain)
  4. Univ. de Barcelona (IEEC-UB), Barcelona (Spain)
  5. Chinese Academy of Sciences (CAS), Beijing (China); Univ. of Portsmouth, Portsmouth (United Kingdom)
  6. Univ. Autonoma de Madrid, Madrid (Spain); Campus of International Excellence UAM+CSIC, Madrid (Spain)
  7. Univ. Autonoma de Madrid, Madrid (Spain); Campus of International Excellence UAM+CSIC, Madrid (Spain); Instituto de Astrofisica de Andalucia (CSIC), Granada (Spain)
  8. Brookhaven National Lab. (BNL), Upton, NY (United States)
  9. Carnegie Mellon Univ., Pittsburgh, PA (United States)
  10. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of Portsmouth, Portsmouth (United Kingdom)
  11. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  12. Sorbonne Univ., Paris (France); Univ. Pierre et Marie Curie, Paris (France)
  13. Univ.-Sternwarte Munchen, Munich (Germany); Max-Planck-Institut fur extraterrestrische Physik, Garching (Germany)
  14. Carnegie Mellon Univ., Pittsburgh, PA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
  15. Leibniz-Institut fur Astrophysik Potsdam (AIP), Potsdam (Germany); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
  16. Univ. of Portsmouth, Portsmouth (United Kingdom)
  17. Sejong Univ., Seoul (Korea)
  18. Kansas State Univ., Manhattan, KS (United States); Hia State Univ., Tbilisi (Georgia); Univ. of Portsmouth, Portsmouth (United Kingdom)
  19. Max-Planck-Institut fur extraterrestische Physik, Garching (Germany)
  20. Ohio Univ., Athens, OH (United States)
  21. New York Univ., New York, NY (United States)
  22. Univ. of St. Andrews, St. Andrews (United Kingdom)
  23. Univ. Nacional Autonoma de Mexico (Mexico)
  24. Univ. of Utah, Salt Lake City, UT (United States)
  25. King's College, Wilkes Barre, PA (United States)
+ Show Author Affiliations

Here, we develop a new methodology called double-probe analysis with the aim of minimizing informative priors in the estimation of cosmological parameters. We extract the dark-energy-model-independent cosmological constraints from the joint data sets of Baryon Oscillation Spectroscopic Survey (BOSS) galaxy sample and Planck cosmic microwave background (CMB) measurement. We measure the mean values and covariance matrix of {R, la, Ωbh2, ns, log(As), Ωk, H(z), DA(z), f(z)σ8(z)}, which give an efficient summary of Planck data and 2-point statistics from BOSS galaxy sample, where R = √ΩmH20, and la = πr(z*)/rs(z*), z* is the redshift at the last scattering surface, and r(z*) and rs(z*) denote our comoving distance to z* and sound horizon at z* respectively. The advantage of this method is that we do not need to put informative priors on the cosmological parameters that galaxy clustering is not able to constrain well, i.e. Ωbh2 and ns. Using our double-probe results, we obtain Ωm = 0.304 ± 0.009, H0 = 68.2 ± 0.7, and σ8 = 0.806 ± 0.014 assuming ΛCDM; and Ωk = 0.002 ± 0.003 and w = –1.00 ± 0.07 assuming owCDM. The results show no tension with the flat ΛCDM cosmological paradigm. By comparing with the full-likelihood analyses with fixed dark energy models, we demonstrate that the double-probe method provides robust cosmological parameter constraints which can be conveniently used to study dark energy models. We extend our study to measure the sum of neutrino mass and obtain Σmν < 0.10/0.22 (68%/95%) assuming ΛCDM and Σmν < 0.26/0.52 (68%/95%) assuming wCDM. This paper is part of a set that analyses the final galaxy clustering dataset from BOSS.

Research Organization:
Brookhaven National Lab. (BNL), Upton, NY (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
SC0012704
OSTI ID:
1324283
Report Number(s):
BNL-112528-2016-JA; KA2301020
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 468, Issue 4; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 10 works
Citation information provided by
Web of Science

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Neutrinos in Cosmology text January 2019
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The seventh data release of the sloan digital sky survey text January 2009
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Planck pre-launch status: High Frequency Instrument polarization calibration text January 2010
Planck Early Results: The Planck mission text January 2011
Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance text January 2011
Planck early results: first assessment of the High Frequency Instrument in-flight performance text January 2011
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
The Baryon Oscillation Spectroscopic Survey of SDSS-III text January 2012
Modeling the Anisotropic Two-Point Galaxy Correlation Function on Small Scales and Improved Measurements of H(z), D_A(z), and f(z)sigma_8(z) from the Sloan Digital Sky Survey DR7 Luminous Red Galaxies text January 2012
CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey - Imaging Data and Catalogue Products text January 2012
Cosmological Structure Formation with Augmented Lagrangian Perturbation Theory text January 2012
Planck 2013 results. I. Overview of products and scientific results text January 2013
Modelling Baryon Acoustic Oscillations with Perturbation Theory and Stochastic Halo Biasing text January 2013
The Clustering of Galaxies in the SDSS-III DR10 Baryon Oscillation Spectroscopic Survey: No Detectable Colour Dependence of Distance Scale or Growth Rate Measurements text January 2013
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples 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: Signs of neutrino mass in current cosmological datasets 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
Planck 2015 results. I. Overview of products and scientific results text January 2015
Planck 2015 results. XIII. Cosmological parameters text January 2015
Planck 2015 results. XV. Gravitational lensing text January 2015
Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies text January 2015
Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters text January 2015
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies text January 2015
SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 12: galaxy target selection and large scale structure catalogues preprint January 2015
Measuring Baryon Acoustic Oscillations from the clustering of voids text January 2015
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function text January 2016
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
Observational Constraints on Dark Energy and Cosmic Curvature text January 2007
Baryonic Features in the Matter Transfer Function text January 1997
Weighing Neutrinos with Galaxy Surveys text January 1997
The Sloan Digital Sky Survey Photometric Camera text January 1998

Cited By (3)

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering journal September 2018
Producing a BOSS CMASS sample with DES imaging journal September 2019
Producing a BOSS-CMASS sample with DES imaging text January 2019

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79 ASTRONOMY AND ASTROPHYSICS
cosmology: observations
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