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Observation of TeV gamma rays from the Crab nebula using the atmospheric Cerenkov imaging technique

Weekes, T. C., Cawley, M. F., Fegan, D. J., Gibbs, K. G., Hillas, A. M., Kowk, P. W., Lamb, R. C., Lewis, D. A., Macomb, D., Porter, N. A., Reynolds, P. T., Vacanti, G.·1989·The Astrophysical Journal

Abstract

The Whipple Observatory 10-m reflector, operating as a 37-pixel camera, has been used to observe the Crab Nebula in TeV gamma rays. By selecting gamma-ray images based on their predicted properties, more than 98 percent of the background is rejected; a detection is reported at the 9.0-sigma level, corresponding to a flux of 1.8 x 10 to the -11th photons sq cm/s above 0.7 TeV (with a factor of 1.5 uncertainty in both flux and energy). Less than 25 percent of the observed flux is pulsed at the period of PSR 0531. There is no evidence for variability on time scales from months to years. Although continuum emission from the pulsar cannot be ruled out, it seems more likely that the observed flux comes from the hard Compton synchrotron spectrum of the nebula.

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Metadata

Authors
Weekes, T. C., Cawley, M. F., Fegan, D. J., Gibbs, K. G., Hillas, A. M., Kowk, P. W., Lamb, R. C., Lewis, D. A., Macomb, D., Porter, N. A., Reynolds, P. T., & Vacanti, G.
Venue
The Astrophysical Journal
Published
1989-07
Volume
342
Pages
379
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1974281020
Cited by
715
References
0
FWCI
10.31
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Observation of TeV gamma rays from the Crab nebula using the atmospheric Cerenkov imaging technique. https://app.cochat.ai/papers/10.1086/167599
The paper
Weekes, T. C., Cawley, M. F., Fegan, D. J., Gibbs, K. G., Hillas, A. M., Kowk, P. W., Lamb, R. C., Lewis, D. A., Macomb, D., Porter, N. A., Reynolds, P. T., & Vacanti, G. (1989). Observation of TeV gamma rays from the Crab nebula using the atmospheric Cerenkov imaging technique. The Astrophysical Journal. https://doi.org/10.1086/167599

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