Preliminary results from the Chicago air shower array and the Michigan muon array

Details Preliminary results from the Chicago air shower array and the Michigan muon array Preliminary results from the Chicago air shower array and the Michigan muon array

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..220..122k&link_type=abstract

High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Volume 220, pp. 122-126 (1991).

Astronomy and Astrophysics

Astronomy

X-Ray Binaries, Pulsars, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

The Chicago Air Shower Array (CASA) is a large area surface array designed to detect extensive air showers (EAS) produced by primaries with energy ~100 TeV. It operates in coincidence with the underground Michigan Muon Array (MIA). Preliminary results are presented from a search for steady emission and daily emission from three astrophysical sources: Cygnus X-3, Hercules X-1, and the Crab nebula and pulsar. There is no evidence for a significant signal from any of these sources in the 1989 data.

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