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Observations of TeV photons at the Whipple Observatory

Conference ·
OSTI ID:6966224
; ; ;  [1]; ;  [2];  [3]; ; ; ; ;  [4];
  1. Iowa State Univ. of Science and Technology, Ames, IA (United States)
  2. Michigan Univ., Ann Arbor, MI (United States)
  3. Saint Patrick's Coll., Maynooth (Ireland)
  4. Harvard-Smithsonian Center for Astrophysics, Amado, AZ (United States)
The Whipple Observatory 10 m gamma-ray telescope has been used to search for TeV gamma-ray emission from a number of objects. This paper reports observations of six galactic and three extragalactic objectsusing the Cherenkov image technique. With the introduction of a high-resolution camera (1/4[degree] pixel) in 1988, the Crab Nebula was detected at a significance level of 20 [omega], in 30 hours of on-source observation. Upper limits at a fraction of the Crab flux are set for most of the other objects, based on the absence of any significant dc excess or periodic effect when an a priori Monte Carlo determined imaging selection criterion (the azwidth cut'') is employed. There are weak indications that one source, Hercules X-1, may be an episodic emitter. The Whipple detection system will be improved shortly with the addition of a second reflector 11 m in diameter (GRANITE) for stereoscopic viewing of showers. The combination of the two-reflector system should have a signal-to-noise advantage of 10[sup 3] over a simple nonimaging Cherenkov receiver.
Research Organization:
Iowa State Univ. of Science and Technology, Ames, IA (United States)
Sponsoring Organization:
DOE; USDOE, Washington, DC (United States)
DOE Contract Number:
AC02-80ER10774
OSTI ID:
6966224
Report Number(s):
CONF-9010289-5; ON: DE93003720
Country of Publication:
United States
Language:
English