Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-30T04:51:27.247Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 

References

Becklin, E. E. and Neugebauer, G.: 1968, Astrophys. J. 151, 145.CrossRefGoogle Scholar
Bleeker, J. A. M., Burger, J. J., Deerenberg, A. J. M., Scheepmaker, A., Swanenburg, B. N., Tanaka, Y., Hayakawa, S., Makino, F., and Ogawa, H.: 1968, Canadian J. Phys. 46, S461.Google Scholar
Clark, G. W., Garmire, G. P., Kraushaar, W. L.: 1968, Astrophys. J. Letters 153, L203.CrossRefGoogle Scholar
Cowsik, R. and Pal, Y.: 1969, Phys. Rev. Letters 22, 550.Google Scholar
De Jager, C. and De Loore, C.: 1970, this volume, p. 238.CrossRefGoogle Scholar
Delvaille, J. P., Albats, P., Greisen, K. I., and Ogelman, H. B.: 1968, Canadian J. Phys. 46, S425.CrossRefGoogle Scholar
Fichtel, C. E., Kniffen, D. A., and Ogelman, H. B.: 1970, this volume p. 315.CrossRefGoogle Scholar
Gorenstein, P., Kellogg, E. M., and Gursky, H.: 1969, Astrophys. J. 156, 315.Google Scholar
Hoffman, W. F. and Frederick, C. L.: 1969, Astrophys. J. Letters 155, L9.Google Scholar
Hutchinson, G. W., Ramsden, D., and Wills, R. D.: 1970, this volume p. 300.Google Scholar
Metzger, A. E., Anderson, E. C., Van Dilla, M. A., and Arnold, J. R.: 1964, Nature 204, 766.CrossRefGoogle Scholar
Ögelman, H.: 1969, Nature 221, 753.Google Scholar
Peterson, L. E.: 1967, University of California at San Diego report SP68-1, July.Google Scholar
Peterson, L. E.: 1969, private communication.Google Scholar
Rocchia, R., Rothenflug, R., Boclet, D., Ducros, G., and Labeyrie, J., Space Research VII, North Holland Publishing Co., Amsterdam 1967, Vol. 1, pp. 1327–1333.Google Scholar
Shen, C. S.: 1969, Phys. Rev. Letters 22, 568.Google Scholar
Shivanandan, K., Houck, J. R., and Harwit, M. O.: 1968, Phys. Rev. Letters 21, 1460.CrossRefGoogle Scholar
Stecker, F. W.: 1970, this volume p. 382.CrossRefGoogle Scholar
Valdez, J. V. and Waddington, C. J.: 1969, Astrophys. J. Letters 156, L85.Google Scholar
Vette, J., Matteson, J. L., Gruber, D., and Peterson, L. E.: 1970, this volume p. 335.CrossRefGoogle Scholar