Optical Measurements for CANGAROO-III

Details Optical Measurements for CANGAROO-III Optical Measurements for CANGAROO-III

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ebhe.conf..345k&link_type=abstract

ENERGY BUDGET IN THE HIGH ENERGY UNIVERSE . Proceedings of the International Workshop. Held 22-24 February 2006 in Kashiwa, Japa

Physics

Scientific paper

CANGAROO-III consists of four telescopes installed near Woomera, South Australia to observe celestial gamma-ray sources by detecting Cherenkov light from air showers. Stereo observations have been performed since March 2004 with an improved angular resolution and a lower energy threshold. In this paper, we present some preliminary results from optical measurements with a cooled CCD camera on the reflectivity of the telescope reflector and the atmospheric transmittance.

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