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arXiv · astro-ph/0506613

The STACEE Ground-Based Gamma-Ray Detector

STACEE Collaboration·D. M. Gingrich·L. M. Boone·D. Bramel·J. Carson·C. E. Covault·P. Fortin·D. S. Hanna·J. A. Hinton·A. Jarvis·J. Kildea·T. Lindner·C. Mueller·R. Mukherjee·R. A. Ong·K. Ragan·R. A. Scalzo·C. G. Theoret·D. A. Williams·J. A. Zweerink
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Abstract

We describe the design and performance of the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) in its complete configuration. STACEE uses the heliostats of a solar energy research facility to collect and focus the Cherenkov photons produced in gamma-ray induced air showers. The light is concentrated onto an array of photomultiplier tubes located near the top of a tower. The large Cherenkov photon collection area of STACEE results in a gamma-ray energy threshold below that of previous ground-based detectors. STACEE is being used to observe pulsars, supernova remnants, active galactic nuclei, and gamma-ray bursts.

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STACEE Collaboration, D. M. Gingrich, L. M. Boone, D. Bramel, J. Carson, C. E. Covault, P. Fortin, D. S. Hanna, J. A. Hinton, A. Jarvis, J. Kildea, T. Lindner, C. Mueller, R. Mukherjee, R. A. Ong, K. Ragan, R. A. Scalzo, C. G. Theoret, D. A. Williams, J. A. Zweerink. 2005-06-24. The STACEE Ground-Based Gamma-Ray Detector. https://doi.org/10.1109/tns.2005.855705

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