arXiv · astro-ph/9701236
Development of the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE)
Abstract
STACEE is a proposed atmospheric Cherenkov telescope for ground-based gamma-ray astrophysics between 25 and 500 GeV. The telescope will make use of the large solar mirrors (heliostats) available at a solar research facility to achieve an energy threshold lower than any existing ground-based instrument. This paper describes the development of STACEE, including an overview of the complete instrument design and a discussion of results from recent prototype tests at the large solar heliostat field of Sandia National Laboratories.
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Rene A. Ong, the STACEE Collaboration. 1997-01-30. Development of the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). https://arxiv.org/abs/astro-ph/9701236
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