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Observations of the diffuse galactic light.Systematic observations during five nights were made with a field of 137 arc seconds at a fixed declination of 20 deg 42 min through one arm of the Milky Way over a range of right ascension from 257 to 336 deg. Corrections for zodiacal light, airglow, and integrated starlight leave a residual which is interpreted as the diffuse galactic light. The residual, plotted against galactic latitude, suggests that the diffuse light in the sample studied emanates from several discrete sources.
Document ID
19720042447
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Roach, F. E.
Smith, L. L.
(Battelle Pacific Northwest Laboratories Richland, Wash., United States)
Pfleiderer, J.
(Bonn, Universitaet Bonn, Germany)
Batishko, C.
(Kitt Peak National Observatory Tucson, Ariz., United States)
Batishko, K.
Date Acquired
August 6, 2013
Publication Date
April 15, 1972
Publication Information
Publication: Astrophysical Journal
Volume: 173
Subject Category
Space Sciences
Accession Number
72A26113
Funding Number(s)
CONTRACT_GRANT: NGR-48-003-013
CONTRACT_GRANT: NSF GP-17561
Distribution Limits
Public
Copyright
Other

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