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Upper limit on periodicity in the three-dimensional large-scale distribution of matterA search for large-scale periodicity in the 3D distribution of 268 Mg II QSO absorption systems which are distributed over 60 percent of the sky, at redshifts 0.1-2.0 is presented. The scalar 3D comoving separations of all pairs of absorption systems are calculated, and peaks in the power spectrum of the distribution of those separations are searched for. The present 95-percent confidence upper limit on the amplitude of a possible periodic fluctuation in the density of galaxies is between one-fourth and three-fourths of the amplitude implied by the data of Broadhurst et al. (1990), depending on the extent to which the wavelength varies and the phase of the signal drifts down lines of sight. A description is presented of how QSO absorption systems sample the 3D population of absorbers and how 3D positions can be represented by their scalar separations.
Document ID
19930044634
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Tytler, David
(NASA Headquarters Washington, DC United States)
Sandoval, John
(California Univ. La Jolla, United States)
Fan, Xiao-Ming
(California Univ. La Jolla; Columbia Univ., New York, United States)
Date Acquired
August 16, 2013
Publication Date
March 1, 1993
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 405
Issue: 1
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
93A28631
Funding Number(s)
CONTRACT_GRANT: NAGW-2119
Distribution Limits
Public
Copyright
Other

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