From the first neutrino telescope, the antarctic muon and neutrino detector array AMANDA, to the IceCube observatory

Collaboration
May, 1999

Citations per year

0 Citations
Abstract:
With an effective telescope area of order 10,000 meter squared for very high energy 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 the calibration of natural deep ice as a particle detector as well as AMANDA’s performance as a neutrino telescope. We discuss its expansion to AMANDA II in the coming Antarctic summer and, subsequently, to a kilometer-scale detector ICECUBE.
  • talk: Venice 1999/02/23
  • talk: Salt Lake City 1999/08/17
  • neutrino: cosmic radiation
  • Cherenkov counter: water
  • muon: cosmic radiation
  • IceCube
  • AMANDA