期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 428, 期 2, 页码 1116-1127出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/sts094
关键词
cosmology: observations; (cosmology:) inflation; (cosmology:) large-scale structure of Universe
资金
- UK Science and Technology Facilities Council [ST/I001204/1]
- UK Science and Technology Facilities Research Council
- European Research Council
- National Aeronautics and Space Administration
- Alfred P. Sloan Foundation
- National Science Foundation
- US Department of Energy Office of Science
- University of Arizona
- Brazilian Participation Group
- Brookhaven National Laboratory
- Cambridge University
- Carnegie Mellon University
- Case Western University
- University of Florida
- Fermilab
- French Participation Group
- German Participation Group
- Harvard University
- UC Irvine
- Instituto de Astrofisica de Andalucia
- Instituto de Astrofisica de Canarias
- Institucio Catalana de Recerca y Estudis Avancat, Barcelona
- Instituto de Fisica Corpuscular
- Michigan State/Notre Dame/JINA Participation Group
- Johns Hopkins University
- Korean Institute for Advanced Study
- 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 Pittburgh
- University of Portsmouth
- Princeton University
- UC Santa Cruz
- Spanish Participation Group
- Texas Christian University
- Trieste Astrophysical Observatory
- University of Tokyo/IPMU
- University of Utah
- Vanderbilt University
- University of Virginia
- University of Washington
- University of Wisconson
- Yale University
- STFC [ST/H008586/1, ST/I001204/1, ST/K00333X/1, ST/J005673/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/J005673/1, ST/H008586/1, ST/I001204/1, ST/K00333X/1] Funding Source: researchfish
- Division Of Astronomical Sciences [0901965] Funding Source: National Science Foundation
We analyse the density field of 264 283 galaxies observed by the Sloan Digital Sky Survey (SDSS)-III Baryon Oscillation Spectroscopic Survey (BOSS) and included in the SDSS Data Release 9 (DR9). In total, the SDSS DR9 BOSS data include spectroscopic redshifts for over 400 000 galaxies spread over a footprint of more than 3000 deg(2). We measure the power spectrum of these galaxies with redshifts 0.43 < z < 0.7 in order to constrain the amount of local non-Gaussianity, f(NL)(local), in the primordial density field, paying particular attention to the impact of systematic uncertainties. The BOSS galaxy density field is systematically affected by the local stellar density and this influences the ability to accurately measure f(NL)(local). In the absence of any correction, we find (erroneously) that the probability that f(NL)(local) is greater than zero, P(f(NL)(local) > 0), is 99.5 per cent. After quantifying and correcting for the systematic bias and including the added uncertainty, we find -45 < f(NL)(local) < 195 at 95 per cent confidence and P(f(NL)(local) > 0) = 91.0 per cent. A more conservative approach assumes that we have only learnt the k dependence of the systematic bias and allows any amplitude for the systematic correction; we find that the systematic effect is not fully degenerate with that of f(NL)(local), and we determine that - 82 < f(NL)(local) < 178 (at 95 per cent confidence) and P(f(NL)(local) > 0) = 68 per cent. This analysis demonstrates the importance of accounting for the impact of Galactic foregrounds on f(NL)(local) measurements. We outline the methods that account for these systematic biases and uncertainties. We expect our methods to yield robust constraints on f(NL)(local) for both our own and future large-scale structure investigations.
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