Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 473, Issue 2, Pages 2737-2752Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stx2333
Keywords
dark matter; large-scale structure of Universe; cosmology: observations; cosmology: theory
Categories
Funding
- World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan
- Alfred P. Sloan Foundation
- National Science Foundation
- US Department of Energy Office of Science
- University of Arizona
- Brazilian Participation Group
- Brookhaven National Laboratory
- Carnegie Mellon University
- University of Florida
- French Participation Group
- German Participation Group
- Harvard University
- Instituto de Astrofisica de Canarias
- Michigan State/Notre Dame/JINA Participation Group
- Johns Hopkins University
- Lawrence Berkeley National Laboratory
- Max Planck Institute for Astrophysics
- Max Planck Institute for Extraterrestrial Physics
- New Mexico State University
- New York University
- Ohio State University
- Pennsylvania State University
- University of Portsmouth
- Princeton University
- Spanish Participation Group
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- University of Washington
- Yale University
- [28-1890]
- [27-10917]
- Grants-in-Aid for Scientific Research [17H07319, 16J01890] Funding Source: KAKEN
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We measure statistically anisotropic signatures imprinted in three-dimensional galaxy clustering using bipolar spherical harmonics in both Fourier space and configuration space. We then constrain a well-known quadrupolar anisotropy parameter g(2M) in the primordial power spectrum, parametrized by P( k) = (P) over bar( k)[ 1 + Sigma(M) g(2M)Y(2M) ((k) over cap)], with M determining the direction of the anisotropy. Such an anisotropic signal is easily contaminated by artificial asymmetries due to specific survey geometry. We precisely estimate the contaminated signal and finally subtract it from the data. Using the galaxy samples obtained by the Baryon Oscillation Spectroscopic Survey Data Release 12, we find no evidence for violation of statistical isotropy, g(2M) for all M to be of zero within the 2 sigma level. The g(2M)-type anisotropy can originate from the primordial curvature power spectrum involving a directional-dependent modulation g(*)((k) over cap . (p) over cap)(2). The bound on g(2M) is translated into g(*) as -0.09 < g(*) < 0.08 with a 95 per cent confidence level when (p) over cap is marginalized over.
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