Prototype Test Results of the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE)
Abstract
There are currently no experiments, either satellite or ground-based, that are sensitive to astrophysical gamma-rays at energies between 20 and 250 GeV. We are developing the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) to explore this energy range. STACEE will use heliostat mirrors at a solar research facility to collect Cherenkov light from extensive air showers produced by high energy gamma-rays. Here we report on the results of prototype test work at the solar facility of Sandia National Laboratories (Albuquerque, NM). The work demonstrates that the facility is suitable for use as an astrophysical observatory. In addition, using a full scale prototype of part of STACEE, we detected atmospheric Cherenkov radiation at energies lower than any other ground-based experiment to date.
Keywords
Cite
@article{arxiv.astro-ph/9704037,
title = {Prototype Test Results of the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE)},
author = {STACEE Collaboration},
journal= {arXiv preprint arXiv:astro-ph/9704037},
year = {2015}
}
Comments
28 LaTeX pages, 24 PostScript figures, uses psfig.sty submitted to Nucl. Inst. Meth. A