Abstract
The Crab pulsar (PSR0531+21) has been observed with the Whipple Observatory 10 m Reflector in imaging mode for ~102h. A suggestion of a broad light curve has been found, but with a low statistical significance. An upper limit (95% confidence level) for the pulsed flux (energy > 0.7TeV) is 4.5x10-12 photons-cm-2-s-1.
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© 1989 Kluwer Academic Publishers
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Vacanti, G. et al. (1989). Search for Pulsed TeV Emission from PSR0531+21. In: Shapiro, M.M., Wefel, J.P. (eds) Cosmic Gamma Rays, Neutrinos, and Related Astrophysics. NATO ASI Series, vol 270. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0921-2_18
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DOI: https://doi.org/10.1007/978-94-009-0921-2_18
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6903-8
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