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A high resolution imaging detector for TeV gamma-ray astronomy
Authors:M F Cawley  D J Fegan  K Harris  A M Hillas  P W Kwok  R C Lamb  M J Lang  D A Lewis  D Macomb  P T Reynolds  D J Schmid  G Vacanti  T C Weekes
Institution:(1) Physics Department, St. Patrick's College, Maynooth, Co. Kildare, Ireland;(2) Physics Department, University College, Belfield, 4 Dublin, Ireland;(3) Harvard-Smithsonian Center for Astrophysics, Whipple Observatory, 85645-0097 Amado, AZ, USA;(4) Physics Department, University of Leeds, LS2 9JT Leeds, U.K.;(5) Physics Department, Iowa State University, 50011 Ames, IA, USA;(6) Present address: Physics Department, University of Minnesota, 55455 Minneapolis, MN, USA
Abstract:Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques.
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