A Search for Astrophysical Point Sources and a Solar Anisotropy Measurement

Details A Search for Astrophysical Point Sources and a Solar Anisotropy Measurement A Search for Astrophysical Point Sources and a Solar Anisotropy Measurement

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2537x&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

The L3 detector at LEP, CERN, has been employed for the search of point sources through the observation of muons with energies above 20, 30, 50, and 100 GeV. Excesses lasting for only one day, as well as steady emissions of single muon events pointing to a particular direction in the sky were searched for in the data obtained from mid July to October 1999 and from April to November 2000. special attention was also given to a selection of known γ -sources. No statistically significant excess has been observed for any direction or particular source in the time periods considered. In addition a dedicated study of the angular distribution of muons above 20 GeV revealed evidence for a Solar anisotropy of the primary flux.

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