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U.S. Department of Energy
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Very high energy gamma ray astrophysics

Technical Report ·
DOI:https://doi.org/10.2172/5076918· OSTI ID:5076918
Our scientific goal is to discover and study by means of gamma-ray astronomy those regions of the universe where particles are accelerated to extreme energies. The atmospheric Cherenkov technique provides a unique and potentially sensitive window in the region of 10{sup 11} to approximately 10{sup 14} eV for this purpose. The Whipple Observatory Collaboration is currently engaged in the development of a Cherenkov camera which has the ultimate capability of distinguishing gamma-ray showers from the numerous cosmic-ray background showers by imaging the Cherenkov light from each shower. We have recently demonstrated the potential of the imaging technique with our 18 sigma detection of TeV photons from the Crab Nebula using a camera of 10 elements, pixel spacing 0.25 degrees. This detection represents a factor of 10 improvement in sensitivity compared to a non-imaging detector. The next step in the development of the detector is to obtain a second large reflector, similar to the present 10 meter instrument, for stereoscopic viewing of showers. This project, named GRANITE, is now approved by DOE. With GRANITE it should be possible to probe more deeply in space by a factor of 7, and to fully investigate the possibility of new physics which has been suggested by reports of anomalous radiation from Hercules X-1. 18 refs.
Research Organization:
Iowa State Univ. of Science and Technology, Ames, IA (USA)
Sponsoring Organization:
DOE/ER
DOE Contract Number:
AC02-80ER10774
OSTI ID:
5076918
Report Number(s):
DOE/ER/10774-10; ON: DE90006645
Country of Publication:
United States
Language:
English