245 citations · 602 across the 8 of their papers we have counts for
8 papers
Limits on diffuse fluxes of high energy extraterrestrial neutrinos with the AMANDA-B10 detector
J. Ahrens et al.
Data from the AMANDA-B10 detector taken during the austral winter of 1997 have been searched for a diffuse flux of high energy extraterrestrial muon-neutrinos, as predicted from, e…
Search for Point Sources of High Energy Neutrinos with AMANDA
J. Ahrens, X. Bai, G. Barouch +1
This paper describes the search for astronomical sources of high-energy neutrinos using the AMANDA-B10 detector, an array of 302 photomultiplier tubes, used for the detection of Ch…
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…
Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector
The AMANDA Collaboration, J. Ahrens
A search for nearly vertical up-going muon-neutrinos from neutralino annihilations in the center of the Earth has been performed with the AMANDA-B10 neutrino detector. The data sam…
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…
Results from the AMANDA High Energy Neutrino Detector
E. Andres, P. Askebjer, X. Bai +2
This paper briefly summarizes the search for astronomical sources of high-energy neutrinos using the AMANDA-B10 detector. The complete data set from 1997 was analyzed. For E_mu>10…
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…