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A search for high-energy γ-rays from pulsars

Published online by Cambridge University Press:  14 August 2015

G. G. Fazio ,
D. R. Hearn ,
H. F. Helmken ,
G. H. Rieke  and
T. C. Weekes
G. G. Fazio
Affiliation:
Mt. Hopkins Observatory, Smithsonian Astrophysical Observatory, Amado, Ariz., and Harvard University, Cambridge, Mass., U.S.A.
D. R. Hearn
Affiliation:
Mt. Hopkins Observatory, Smithsonian Astrophysical Observatory, Amado, Ariz., and Harvard University, Cambridge, Mass., U.S.A.
H. F. Helmken
Affiliation:
Mt. Hopkins Observatory, Smithsonian Astrophysical Observatory, Amado, Ariz., and Harvard University, Cambridge, Mass., U.S.A.
G. H. Rieke
Affiliation:
Mt. Hopkins Observatory, Smithsonian Astrophysical Observatory, Amado, Ariz., and Harvard University, Cambridge, Mass., U.S.A.
T. C. Weekes
Affiliation:
Mt. Hopkins Observatory, Smithsonian Astrophysical Observatory, Amado, Ariz., and Harvard University, Cambridge, Mass., U.S.A.

Abstract

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The 10-m optical reflector at Mt. Hopkins, Ariz., was used to search for cosmic γ radiation from pulsars by detection of atmospheric Čerenkov light generated by energetic particle showers. In the energy region of 1011–1012 eV, no evidence of pulsed γ-ray emission was found from either NP0532 (Crab Nebula) or CP1133.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 37: Non-Solar X- and Gamma-Ray Astronomy , 1970 , pp. 192 - 195
Copyright
Copyright © Reidel 1970 

References

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