The sensitivity of atmospheric Cerenkov detectors for gamma-ray astronomy

Details The sensitivity of atmospheric Cerenkov detectors for gamma-ray astronomy The sensitivity of atmospheric Cerenkov detectors for gamma-ray astronomy

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ncimb..35...95w&link_type=abstract

Nuovo Cimento, Sezione B, vol. 35 B, Sept. 11, 1976, p. 95-109.

Astronomy and Astrophysics

Astronomy

5

Cerenkov Counters, Cosmic Ray Showers, Gamma Rays, X Ray Astronomy, Background Radiation, Luminous Intensity, Monte Carlo Method, Radiant Flux Density, Radiation Distribution, Reflectors

Scientific paper

The collection area and energy threshold of a number of atmospheric Cerenkov detectors are estimated based on some recent Monte Carlo calculations of the light distributions from gamma-ray-induced air showers. These parameters permit absolute fluxes to be evaluated and the results of different experiments to be compared. Although the parameters used are for a 10-m optical reflector at an altitude of 2.3 km, the method outlined is general and can be applied to other detectors.

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