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Anisotropy of the diffuse background at millimeter wavelengthsThe anisotropy of the diffuse background radiation has been measured with a 10-deg FWHM beam in a broad spectral band from 0.6 to 4.0 mm. A dipole anisotropy is detected with magnitude consistent with previous measurements; the present data may, however, be contaminated by atmospheric emission. Upper limits are set to fluctuations at higher-order multipoles. The most stringent limit is at l = 4, where a 95-percent confidence-level limit of less than 0.00025 is set. The observed level of isotropy sharply constrains the possibility of local astronomical origin for the submillimeter excess.
Document ID
19890039547
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Bernstein, G. M.
(California Univ. Berkeley, CA, United States)
Fischer, M. L.
(California Univ. Berkeley, CA, United States)
Richards, P. L.
(California, University Berkeley, United States)
Peterson, J. B.
(Princeton University NJ, United States)
Timusk, T.
(McMaster University Hamilton, Canada)
Date Acquired
August 14, 2013
Publication Date
February 1, 1989
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 337
ISSN: 0004-637X
Subject Category
Space Radiation
Accession Number
89A26918
Funding Number(s)
CONTRACT_GRANT: NSG-7205
Distribution Limits
Public
Copyright
Other

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