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arXiv · astro-ph/0211264

Results from the Antarctic Muon and Neutrino Detector Array (AMANDA)

D. F. Cowen
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Abstract

We show new results from both the older and newer incarnations of AMANDA (AMANDA-B10 and AMANDA-II, respectively). These results demonstrate that AMANDA is a functioning, multipurpose detector with significant physics and astrophysics reach. They include a new higher-statistics measurement of the atmospheric muon neutrino flux and preliminary results from searches for a variety of sources of ultrahigh energy neutrinos: generic point sources, gamma-ray bursters and diffuse sources producing muons in the detector, and diffuse sources producing electromagnetic or hadronic showers in or near the detector.

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D. F. Cowen. 2002-11-12. Results from the Antarctic Muon and Neutrino Detector Array (AMANDA). https://doi.org/10.1016/s0920-5632(03)01335-5

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