Atmospheric Neutrino and Muon Spectra Measured with the AMANDA-II Detector

Details Atmospheric Neutrino and Muon Spectra Measured with the AMANDA-II Detector Atmospheric Neutrino and Muon Spectra Measured with the AMANDA-II Detector

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1313g&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

AMANDA is a large neutrino telescope designed to measure the flux of high energy neutrinos from astrophysical sources. The background for such measurements consists of down-going atmospheric muons and up-going atmospheric neutrino-induced muons. A new method to reconstruct the muon and neutrino energy spectra based on neural networks and regularized unfolding has been developed. The atmospheric muon spectrum has been used as a cross-check on the method and the atmospheric neutrino spectrum has been measured up to 100 TeV.

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