A search for astrophysical point sources of 100 TeV gamma rays by the UMC collaboration

Details A search for astrophysical point sources of 100 TeV gamma rays by the UMC collaboration A search for astrophysical point sources of 100 TeV gamma rays by the UMC collaboration

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..272.1203m&link_type=abstract

Proceedings of the XXVI International Conference on High Energy Physics. Vol. II. AIP Conference Proceedings, Volume 272, pp. 1

Physics

High Energy Physics

Scientific paper

The CASA-MIA experiment is a very large extensive air shower detector with good angular resolution. This instrument has been used to search the entire visible sky for astrophysical point sources of 100 TeV gamma rays. Approximately 90% of the isotropic charged cosmic ray background is rejected by measuring the muon content of the showers. Stringent limits are placed on the possible flux of 100 TeV sources across a large part of the Northern sky.

Affiliated with

Also associated with

No associations

Rating

A search for astrophysical point sources of 100 TeV gamma rays by the UMC collaboration does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A search for astrophysical point sources of 100 TeV gamma rays by the UMC collaboration, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A search for astrophysical point sources of 100 TeV gamma rays by the UMC collaboration will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1045284