A South Pole facility to observe very high energy gamma ray sources

Details A South Pole facility to observe very high energy gamma ray sources A South Pole facility to observe very high energy gamma ray sources

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..198...24m&link_type=abstract

IN: Astrophysics in Antarctica (A92-22401 07-89). New York, American Institute of Physics, 1989, p. 24-34.

Astronomy and Astrophysics

Astronomy

2

Cerenkov Counters, Cerenkov Radiation, Gamma Ray Astronomy, Particle Telescopes, Binary Stars, Radio Sources (Astronomy), Relativistic Particles, Stellar Radiation

Scientific paper

The construction of an atmospheric Cerenkov telescope (ACT) at a South Polar site is under consideration, in view of the long polar night's accommodation of nearly continuous observation of very high energy gamma-ray sources (400 hrs/month), the large concentration of candidate sources at high southern declinations, and the circumpolarity of the sky, which simplifies data analysis. ACT is envisioned as operating in conjunction with the South Polar Air Shower Experiment, thereby constituting a comprehensive-coverage cosmic gamma-ray facility.

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