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Physics and Results from the AMANDA-II High Energy Neutrino Telescope


This paper briefly describes the principle of operation and science goals of the AMANDA high energy neutrino telescope located at the South Pole, Antarctica. Results from an earlier phase of the telescope, called AMANDA-BIO, demonstrate both reliable operation and the broad astrophysical reach of this device, which includes searches for a variety of sources of ultrahigh energy neutrinos: generic point sources, Gamma-Ray Bursts and diffuse sources. The predicted sensitivity and angular resolution of the telescope were confirmed by studies of atmospheric muon and neutrino backgrounds. We also report on the status of the analysis from AMANDA-II, a larger version with far greater capabilities. At this stage of analysis, details of the ice properties and other systematic uncertainties of the AMANDA-II telescope are under study, but we have made progress toward critical science objectives. In particular, we present the first preliminary flux limits from AMANDA-II on the search for continuous emission from astrophysical point sources, and report on the search for correlated neutrino emission from Gamma Ray Bursts detected by BATSE before decommissioning in May 2000. During the next two years, we expect to exploit the full potential of AMANDA-II with the installation of a new data acquisition system that records full waveforms from the in-ice optical sensors.



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Ahrens, J. et al. 2001, Astropart. Phys., 16, 345
Ahrens, J. et al. 2002a, Phys. Rev. D, 012005
Ahrens, J. et al. 2002b, Phys. Rev. D, 032006.
Ahrens, J. et al. 2003a, ApJ, in press (astro-ph/0208006).
Ahrens, J. et al. 2003b, Phys. Rev. D, in press
Andres, E. et al. 2000, Astropart. Phys., 13, 1 (see amanda for more information)
Andres, E. et al. 2001, Nature, 410, 441
Balkanov, V. et al. 2001, in Proc. 9th Int. Workshop on Neutrino Telescopes (Venice, Italy) Vol. 3 p. 591
Barwick, S. W., 2000, Phys. Scripta, T, 85, 106 (astro-ph/9903467)
Bertin, V., Negri, E., & Orloff, J. 2002, submitted to European Phy. J. C
Dermer, C. & Atoyan, A. 2001, Phys. Rev. Lett. 87, 221102.
Gaisser, T. K., Halzen, F., & Stanev, T., 1995, Phys. Rept. 258, 173
GCN, 2002, see
Gorham, P. et al. 2002, Proc. SPIE (Kona, Hawaii,)
Hardke, R. 2001, in Proc. 27th Int. Cosmic Ray Conf. (Hamburg, Germany)
Hill, G. C. & Leuthold, M. J. 2001, in Proc. of ICRC, (Hamburg, Germany) p. 1113
Hurley, K., 2002, private communication.
Hundertmark, S., 2001, in Proc. Second Workshop Methodical Aspects Underwater/Underice Neutrino Telescopes, Hamburg (
Karle, A. et al. 2002, Proc. XXth Int. Conf. Neutrino Phys. Astrophys. (Munich) (astro-ph/0209556)
Letessier-Selvon, A. et al. 2001, Proc. 27th ICRC, 1204
Levinson, A. & Waxman, E., 2001, Phys. Rev. Lett., 87 1711101.01
Lipari, P., 1993, Astro. Part. Phys. 1, 193
Mannheim, K., Protheroe, R. J., & Rachen, J. P., 2000, Phys. Rev. D, 63, 023003
Matsuno, S. 2001, Proc. Inter. Cosmic Ray Conf. (Hamburg, Germany) 1069
Niessen, P. & Spiering, C., 2001, in Proc. of ICRC (Hamburg, Germany), p. 1496
Perrone, et al. 2001, in Proc. 27th Int. Cosmic Ray Conf. (Hamburg, Germany), p. 1073
Price, P. B., Woschnagg, K., & Chirkin, D., 2000, Geophys. Res. Lett., 27, 2129
Ringwald, A. & Tu, H., 2002, Phys. Lett. B, 525, 135
Spiering, C. 2002, Prog. Part. Nucl. Phys., 48, 43
Waxman, E. & Bahcall, J. 1997, Phys. Rev. Lett., 78, 2292
Waxman, E. & Bahcall, J. 1999, Phys. Rev. D, 59, 023002


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