AMANDA and IceCube: neutrino astronomy at the south pole

Details AMANDA and IceCube: neutrino astronomy at the south pole AMANDA and IceCube: neutrino astronomy at the south pole

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..39..438t&link_type=abstract

Journal of Physics: Conference Series, Volume 39, Issue 1, pp. 438-440 (2006).

Physics

Scientific paper

AMANDA is a high energy neutrino telescope consisting of 677 optical modules at 1.5-2 km depth in glacial ice at the south pole. We summarize AMANDA results for observation of atmospheric neutrinos and searches of extraterrestrial neutrinos from point sources, gamma ray bursts and diffuse fluxes. Upper limits at 90%CL are presented. The status of IceCube, the 1 km3 successor to AMANDA currently under construction is presented.

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