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Review of observational results on γ-ray background∗: (Invited discourse)

Published online by Cambridge University Press:  14 August 2015

G. W. Clark ,
G. P. Garmire  and
W. L. Kraushaar
G. W. Clark
Affiliation:
Dept. of Physics and Center for Space Research, Massachusetts Institute of Technology, Cambridge, Mass., U.S.A.
G. P. Garmire
Affiliation:
Dept. of Physics, California Institute of Technology, Pasadena, Cal., U.S.A.
W. L. Kraushaar
Affiliation:
Department of Physics, University of Wisconsin, Madison, Wis., U.S.A.

Abstract

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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.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 37: Non-Solar X- and Gamma-Ray Astronomy , 1970 , pp. 269 - 279
Copyright
Copyright © Reidel 1970 

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