The experimental search for point sources above 1 TeV

Details The experimental search for point sources above 1 TeV The experimental search for point sources above 1 TeV

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..203..203g&link_type=abstract

IN: Particle astrophysics - The NASA cosmic ray program for the 1990s and beyond (A92-20526 06-93). New York, American Institute

Astronomy and Astrophysics

Astrophysics

Astrophysics, Cosmic Ray Showers, Point Sources, Radiation Detectors, Cerenkov Counters, Muons, Neutrinos, Scintillation Counters

Scientific paper

Experimental studies of point sources of very high energy and ultrahigh energy radiation are discussed. The Cygnus array, operational since 1986, is sensitive to the electromagnetic and muonic component of extensive air showers above 5 x 10 exp 13 eV. The proposed Grande detector will be capable of detecting all components of extensive air showers above 10 exp 13 eV and detecting upward moving muons from neutrino-induced events in the rock below. The proposed Milagro experiment will study the electromagnetic and muonic component of extensive air showers above 10 exp 12 eV.

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