Very high-energy gamma rays from the Crab nebula and pulsar.
This project is to search for Very High Energy (VHE) (10¹¹ eV to 10¹⁴ eV) gamma rays from the Crab nebula and pulsar using the atmospheric Cherenkov imaging technique. The technique uses an array of 37 photomultiplier tubes to record the images of the Cherenkov light pulses generated by energetic pa...
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Language: | en |
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The University of Arizona.
1989
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Online Access: | http://hdl.handle.net/10150/184863 |