GeV γ-ray astronomy with STACEE-64

Details GeV γ-ray astronomy with STACEE-64 GeV γ-ray astronomy with STACEE-64

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..868s&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 868-870 (2001).

Astronomy and Astrophysics

Astrophysics

Gamma-Ray, Cherenkov Detectors, Supernova Remnants, Galactic Nuclei, Circumnuclear Matter, And Bulges, Dark Matter

Scientific paper

The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is a new low-threshold atmospheric Cherenkov detector, using heliostat mirrors at a solar research facility to achieve a large collection area for Cherenkov light. The newest version of this detector, STACEE-64, should run at a threshold of 70 GeV or lower. Possible science for STACEE-64 in this energy range includes the study of AGN, supernova remnants, the extragalactic UV background, and exotic dark matter. .

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