Author:
Clark G. W.,Garmire G. P.,Kraushaar W. L.
Abstract
Recent observations in the X- and γ-Ray region of the electromagnetic spectrum have given strong evidence for the existence of an extragalactic intensity with a slowly steepening power law spectrum in the region 103 to 108 eV. Further data from the OSO-III high energy γ-Ray detector are in agreement with earlier published reports, and suggest that the γ-Rays from high galactic latitudes have a softer spectrum than those from the galactic plane.
Publisher
Cambridge University Press (CUP)
Cited by
3 articles.
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