Development of the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE)

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dc.creatorOng, Rene A.
dc.creatorCollaboration, the STACEE
dc.date1997-01-30
dc.date.accessioned2026-07-07T02:22:50Z
dc.date.available2026-07-07T02:22:50Z
dc.descriptionSTACEE 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.
dc.description3 latex pages, uses sprocl.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9701236
dc.identifierhttp://arxiv.org/abs/astro-ph/9701236
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11024
dc.subjectAstrophysics
dc.titleDevelopment of the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE)
dc.typetext

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