The optical reflector system for the CANGAROO-II imaging atmospheric Cherenkov telescope

Abstract

A new imaging atmospheric Cherenkov telescope (CANGAROO-II) with a light-weight reflector has been constructed. Light, robust, and durable mirror facets of containing CFRP (Carbon Fiber Reinforced Plastic) laminates were developed for the telescope. The attitude of each facet can be adjusted by stepping motors. In this paper, we describe the design, manufacturing, alignment procedure, and the performance of the CANGAROO-II optical reflector system.

arXiv commentAstroparticle Physics, (2000) in press., 22 pages (11 figures), LaTeX uses elsart.sty

References in corpus (6)

• Impact of atmospheric parameters on the atmospheric Cherenkov technique
• Very High Energy Gamma-Ray Astronomy
• The CAT Imaging Telescope for Very-High-Energy Gamma-Ray Astronomy
• The Cangaroo-III Project
• An Optical Reflector System for the CANGAROO-II Telescope
• Initial Performance of CANGAROO-II 7m telescope

Cited by in corpus (31)

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• Development of an atmospheric Cherenkov imaging camera for the CANGAROO-III experiment
• Evidence of TeV gamma-ray emission from the nearby starburst galaxy NGC 253
• Detection of diffuse TeV gamma-ray emission from the nearby starburst galaxy NGC 253
• Observation of gamma-rays greater than 10 TeV from Markarian 421
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• CANGAROO-III search for TeV Gamma-rays from two clusters of galaxies
• Cherenkov Telescopes as Optical Telescopes for Bright Sources: Today's Specialised Thirty Metre Telescopes?
• Observation of an extended VHE gamma-ray emission from MSH 15-52 with CANGAROO-III
• Fourier transform method for imaging atmospheric Cherenkov telescopes
• Erratum: Detection of diffuse TeV gamma-ray emission from the nearby starburst galaxy NGC 253
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• Searches for very high energy gamma rays from blazars with CANGAROO-III telescope in 2005-2009