A Search for Astronomical Neutrino Sources with the Super-Kamiokande Detector

Details A Search for Astronomical Neutrino Sources with the Super-Kamiokande Detector A Search for Astronomical Neutrino Sources with the Super-Kamiokande Detector

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1285w&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

1

Scientific paper

Upward-going muons logged by the super-Kamiokande detector during the SK-I running period (1996-2001), are used in a search for astrophysical point sources of neutrinos. The results of two indep endent analyses of all-sky surveys are presented. The data are also examined for an excess of muons associated with the extended flaring episo de of Markarian 501 in 1997. No significant evidence for astrophysical point sources of neutrinos is found. Confidence limits on the maximum observationally consistent neutrino flux that might be coming from selected source candidates are presented.

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