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J. Carson (UCLA), L.M. Boone (College of Wooster), D. Bramel (Columbia U.), C.E. Covault (CWRU), P. Fortin, G. Gauthier (McGill U.), D. Gingrich (Tri-Universities Meson Facility), D. Hanna (McGill U.), A. Jarvis (UCLA), J. Kildea, T. Lindner, C. Mueller (McGill U.), R. Mukherjee (Barnard College), R.A. Ong (UCLA), K.J. Ragan (McGill U.), R.A. Scalzo (U. Chicago), D.A. Williams (UCSC), J. Zweerink (UCLA)
The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is a ground-based experiment sensitive to ~100 GeV gamma rays. STACEE is in a unique position to measure gamma rays from blazars at lower energies than those probed by other ground-based instruments, ultimately providing new information about the particle acceleration mechanisms in these powerful objects. We explain the STACEE experiment itself, review recent results and discuss future plans.
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.