6 papers
Observation of High Energy Atmospheric Neutrinos with the Antarctic Muon and Neutrino Detector Array
AMANDA Collaboration, J. Ahrens
The Antarctic Muon and Neutrino Detector Array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming thr…
Results from AMANDA
Gary C. Hill
The AMANDA (Antarctic Muon And Neutrino Detector Array) detector, located at the South Pole station, Antarctica, was recently expanded with the addition of six new strings, complet…
Search for Supernova Neutrino-Bursts with the AMANDA Detector
AMANDA collaboration
The core collapse of a massive star in the Milky Way will produce a neutrino burst, intense enough to be detected by existing underground detectors. The AMANDA neutrino telescope l…
The AMANDA Neutrino Telescope: Principle of Operation and First Results
E. Andres
AMANDA is a high-energy neutrino telescope presently under construction at the geographical South Pole. In the Antarctic summer 1995/96, an array of 80 optical modules (OMs) arrang…
The AMANDA Neutrino Telescope
F. Halzen
With an effective telescope area of order m for TeV neutrinos, a threshold near 50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector r…
The AMANDA Neutrino Telescope and the Indirect Search for Dark Matter
F. Halzen
With an effective telescope area of order 10^4 m^2, a threshold of ~50 GeV and a pointing accuracy of 2.5 degrees, the AMANDA detector represents the first of a new generation of h…