Results from the Antarctic muon and nuetrino detector array

Ahrens, J.; Bai, X.; Barwick, S. W.; Becka, T.; Becker, K. -H.; Bernardini, E.; Bertrand, D.; Binon, F.; Biron, A.; Boser, S.; Botner, O.; Bouhali, O.; Burgess, T.; Carius, S.; Castermans, T.; Chen, A.; Chirkin, D.; Conrad, J.; Cooley, J.; Cowen, D. F.; Davour, A.; De Clercq, C.; De Young, T.; Desiati, P.; Dewulf, J. -P.; Doksus, P.; Ekstrom, P.; Feser, T.; Gaisser, T. K.; Gaug, M.; Gerhardt, L.; Godschmidt, A.; Hallgren, A.; Halzen, F.; Hanson, K.; Hardtke, R.; Hauschildt, T.; Hellwig, M.; Herquet, P.; Hill, G. C.; Hulth, P. O.; Hundertmark, S.; Jacobson, J.; Karle, A.; Koci, B.; Kopke, L.; Kuehn, P.; Kowalski, M.; Lamoureux, J. I.; Leich, H.; Leuthold, M.; Lindahl, P.; Liubarsky, I.; Madsen, J.; Marciniewski, P.; Matis, H. S.; Mcparland, C. P.; Minaeva, Y.; Miocinovc, P.; Morse, R.; Nahnhauer, R.; Neunhoffer, T.; Niessen, P.; Nygren, D. R.; Ogelman, H.; Olbrechts, Ph.; Peres de los Heros, C.; Pohl, A. C.; Price, P. B.; Przybylski, G. T.; Rawlins, K.; Resconi, E.; Rhode, W.; Ribordy, M.; Richter, S.; Rodriguez Martino, J.; Ross, D.; Sander, H. -G.; Schmidt, T.; Schneider, D.; Schwarz, R.; Silvestri, A.; Solarz, M.; Spiczak, G. M.; Spiering, C.; Steele, D.; Steffen, P.; Stokstad, R. G.; Sudhoff, P.; Sulanke, K. -H.; Taboada, I.; Thollander, L.; Tilay, S.; Walck, C.; Weinheimer, C.; Wiebusch, C. H.; Wiedemann, C.; Wissing, H.

doi:10.1016/S0920-5632(03)01335-5

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.