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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

Abstract

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-likelihoodmore » 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.« less

Authors:
 [1];  [2];  [3];  [4];  [5];  [5]; ;  [6];  [7];  [8];  [8];  [9];  [10];  [11];  [12];  [13];  [14];  [15];  [16];  [17] more »;  [13];  [18];  [19];  [9];  [20];  [21];  [22];  [23];  [24];  [16];  [25] « less
+ Show Author Affiliations
  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)
Publication Date:
Research Org.:
Brookhaven National Lab. (BNL), Upton, NY (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1324283
Report Number(s):
BNL-112528-2016-JA
Journal ID: ISSN 0035-8711; KA2301020
Grant/Contract Number:  
SC0012704
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 468; Journal Issue: 4; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations; distance scale; large-scale structure of Universe; cosmological parameters

Citation Formats

Pellejero-Ibanez, Marco, Chuang, Chia -Hsun, Rubino-Martin, J. A., Cuesta, Antonio J., Wang, Yuting, Zhao, Gongbo, Ashley J. Ross, Rodriquez-Torres, Sergio, Prada, Francisco, Slosar, Anze, Vazquez, Jose A., Alam, Shadab, Beutler, Florian, Eisenstein, Daniel J., Gil-Martin, Hector, Grieb, Jan Niklas, Ho, Shirley, Kitaura, Francisco -Shu, Percival, Will J., Rossi, Graziano, Salazar-Albornoz, Salvador, Samushia, Lado, Sanchez, Ariel G., Sapathy, Siddharth, Seo, Hee -Jong, Tinker, Jeremy L., Tojeiro, Rita, Vargas-Magana, Mariana, Brownstein, Joel R., Nichol, Robert C., and Olmstead, Matthew D. 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. United States: N. p., 2016. Web. doi:10.1093/mnras/stx751.
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Pellejero-Ibanez, Marco, Chuang, Chia -Hsun, Rubino-Martin, J. A., Cuesta, Antonio J., Wang, Yuting, Zhao, Gongbo, Ashley J. Ross, Rodriquez-Torres, Sergio, Prada, Francisco, Slosar, Anze, Vazquez, Jose A., Alam, Shadab, Beutler, Florian, Eisenstein, Daniel J., Gil-Martin, Hector, Grieb, Jan Niklas, Ho, Shirley, Kitaura, Francisco -Shu, Percival, Will J., Rossi, Graziano, Salazar-Albornoz, Salvador, Samushia, Lado, Sanchez, Ariel G., Sapathy, Siddharth, Seo, Hee -Jong, Tinker, Jeremy L., Tojeiro, Rita, Vargas-Magana, Mariana, Brownstein, Joel R., Nichol, Robert C., & Olmstead, Matthew D. 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. United States. https://doi.org/10.1093/mnras/stx751
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Pellejero-Ibanez, Marco, Chuang, Chia -Hsun, Rubino-Martin, J. A., Cuesta, Antonio J., Wang, Yuting, Zhao, Gongbo, Ashley J. Ross, Rodriquez-Torres, Sergio, Prada, Francisco, Slosar, Anze, Vazquez, Jose A., Alam, Shadab, Beutler, Florian, Eisenstein, Daniel J., Gil-Martin, Hector, Grieb, Jan Niklas, Ho, Shirley, Kitaura, Francisco -Shu, Percival, Will J., Rossi, Graziano, Salazar-Albornoz, Salvador, Samushia, Lado, Sanchez, Ariel G., Sapathy, Siddharth, Seo, Hee -Jong, Tinker, Jeremy L., Tojeiro, Rita, Vargas-Magana, Mariana, Brownstein, Joel R., Nichol, Robert C., and Olmstead, Matthew D. Mon . "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". United States. https://doi.org/10.1093/mnras/stx751. https://www.osti.gov/servlets/purl/1324283.
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@article{osti_1324283,
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},
author = {Pellejero-Ibanez, Marco and Chuang, Chia -Hsun and Rubino-Martin, J. A. and Cuesta, Antonio J. and Wang, Yuting and Zhao, Gongbo and Ashley J. Ross and Rodriquez-Torres, Sergio and Prada, Francisco and Slosar, Anze and Vazquez, Jose A. and Alam, Shadab and Beutler, Florian and Eisenstein, Daniel J. and Gil-Martin, Hector and Grieb, Jan Niklas and Ho, Shirley and Kitaura, Francisco -Shu and Percival, Will J. and Rossi, Graziano and Salazar-Albornoz, Salvador and Samushia, Lado and Sanchez, Ariel G. and Sapathy, Siddharth and Seo, Hee -Jong and Tinker, Jeremy L. and Tojeiro, Rita and Vargas-Magana, Mariana and Brownstein, Joel R. and Nichol, Robert C. and Olmstead, Matthew D.},
abstractNote = {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.},
doi = {10.1093/mnras/stx751},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 4,
volume = 468,
place = {United States},
year = {Mon Mar 28 00:00:00 EDT 2016},
month = {Mon Mar 28 00:00:00 EDT 2016}
}
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Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance
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Reconstruction of primordial density fields
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Quantifying distortions of the Lagrangian dark-matter mesh in cosmology
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Review of Particle Physics
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The WiggleZ Dark Energy Survey: Final data release and cosmological results
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Planck 2015 results : I. Overview of products and scientific results
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Planck 2015 results : XI. CMB power spectra, likelihoods, and robustness of parameters
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Planck 2015 results : XIII. Cosmological parameters
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Planck 2015 results : XV. Gravitational lensing
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Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: modelling the clustering and halo occupation distribution of BOSS CMASS galaxies in the Final Data Release
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: analysis of potential systematics: Systematic analysis of BOSS 3D clustering
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: observational systematics and baryon acoustic oscillations in the correlation function
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Planck pre-launch status: High Frequency Instrument polarization calibration
journal, September 2010

Neutrino mass constraint from the Sloan Digital Sky Survey power spectrum of luminous red galaxies and perturbation theory
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring growth rate and geometry with anisotropic clustering
journal, February 2014

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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
journal, April 2014

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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
journal, September 2016

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  • Monthly Notices of the Royal Astronomical Society, Vol. 464, Issue 2
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the configuration-space clustering wedges
journal, September 2016

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  • Monthly Notices of the Royal Astronomical Society, Vol. 464, Issue 2
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The Multi-Object, Fiber-Fed Spectrographs for the Sloan Digital sky Survey and the Baryon Oscillation Spectroscopic Survey
journal, July 2013

Planck pre-launch status: The Planck mission
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CFHTLS weak-lensing constraints on the neutrino masses
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Upper Bound of 0.28 eV on Neutrino Masses from the Largest Photometric Redshift Survey
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: galaxy clustering measurements in the low-redshift sample of Data Release 11
journal, April 2014

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Distance measurements from supernovae and dark energy constraints
journal, December 2009

Observational constraints on dark energy and cosmic curvature
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Neutrinos Help Reconcile Planck Measurements with the Local Universe
journal, February 2014

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journal, September 2000

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  • The Astronomical Journal, Vol. 120, Issue 3
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample
journal, October 2013

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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
journal, December 2016

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Planck 2015 results : XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation
journal, September 2016

Neutrinos in cosmology
journal, January 2004

The Seventh Data Release of the Sloan Digital Sky Survey
text, January 2009

  • Abazajian, Kevork N.; Adelman-McCarthy, Jennifer K.; Agüeros, Marcel Andre
  • Columbia University
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Review of Particle Physics
text, January 2008

Neutrinos in Cosmology
text, January 2019

Planck 2015 results : VI. LFI mapmaking
journal, September 2016

Planck 2015 results : X. Diffuse component separation: Foreground maps
journal, September 2016

Neutrinos in Cosmology
text, January 2019

Planck 2015 results : XVI. Isotropy and statistics of the CMB
journal, September 2016

Review of Particle Physics
text, January 2018

Planck 2015 results : XXVI. The Second
journal, September 2016

Review of Particle Physics
text, January 2012

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  • Deutsches Elektronen-Synchrotron, DESY, Hamburg
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The seventh data release of the sloan digital sky survey
text, January 2009

  • Abazajian, K. N.; Al, Et; Adelman-McCarthy, J. K.
  • Institute of Physics Publishing
  • DOI: 10.5167/uzh-30878

The WiggleZ Dark Energy Survey: Survey Design and First Data Release
text, January 2009

Upper Bound of 0.28 eV on the Neutrino Masses from the Largest Photometric Redshift Survey
text, January 2009

Planck pre-launch status: High Frequency Instrument polarization calibration
text, January 2010

Planck Early Results: The Planck mission
text, January 2011

Planck early results: first assessment of the High Frequency Instrument in-flight performance
text, January 2011

The Baryon Oscillation Spectroscopic Survey of SDSS-III
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

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

Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
text, January 2015

Measuring Baryon Acoustic Oscillations from the clustering of voids
text, January 2015

Memory of Initial Conditions in Gravitational Clustering
text, January 2005

The 2.5 m Telescope of the Sloan Digital Sky Survey
text, January 2006

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

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    Works referencing / citing this record:

    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

    • Wang, Yuting; Zhao, Gong-Bo; Chuang, Chia-Hsun
    • Monthly Notices of the Royal Astronomical Society, Vol. 481, Issue 3
    • DOI: 10.1093/mnras/sty2449

    Producing a BOSS CMASS sample with DES imaging
    journal, September 2019

    • Lee, S.; Huff, E. M.; Ross, A. J.
    • Monthly Notices of the Royal Astronomical Society, Vol. 489, Issue 2
    • DOI: 10.1093/mnras/stz2288

    Producing a BOSS-CMASS sample with DES imaging
    text, January 2019

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