Abstract
With an effective telescope area of order 104 m2 for TeV neutrinos, a threshold near ∼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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 474-485 |
| Number of pages | 12 |
| Journal | Nuclear Physics B - Proceedings Supplements |
| Volume | 77 |
| Issue number | 1-3 |
| DOIs | |
| State | Published - May 1999 |
All Science Journal Classification (ASJC) codes
- Atomic and Molecular Physics, and Optics
- Nuclear and High Energy Physics