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arXiv · hep-ex/9809025

The AMANDA Neutrino Telescope

F. Halzen
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Abstract

With an effective telescope area of order $10^4$ m$^2$ for TeV neutrinos, a threshold near $\sim$50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe early results on the calibration of natural deep ice as a particle detector as well as on AMANDA's performance as a neutrino telescope.

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F. Halzen. 1998-09-23. The AMANDA Neutrino Telescope. https://doi.org/10.1016/s0920-5632(99)00469-7

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