IceCube CollaborationAbbasi, R.Ackermann, M.Adams, J.Ahlers, M.Ahrens, J.Andeen, K.Auffenberg, J.Bai, X.Baker, M.Baret, B.Barwick, S.Bay, R.Bazo Alba, J.Beattie, K.Becka, T.Becker, J.Becker, K.-H.Berdermann, J.Berghaus, P.Berley, D.Bernardini, E.Bertrand, D.Besson, D.Blaufuss, E.Boersma, D.Bohm, C.Bolmont, J.Böser, S.Botner, O.Braun, J.Breder, D.Burgess, T.Castermans, T.Chirkin, D.Christy, B.Clem, J.Cowen, D.D’Agostino, M.Danninger, M.Davour, A.Day, C.Depaepe, O.De Clercq, C.Demirörs, L.Descamps, F.Desiati, P.De Vries-Uiterweerd, G.Deyoung, T.Diaz-Velez, J.Dreyer, J.Dumm, J.Duvoort, M.Edwards, W.Ehrlich, R.Eisch, J.Ellsworth, R.Engdegård, O.Euler, S.Evenson, P.Fadiran, O.Fazely, A.Filimonov, K.Finley, C.Foerster, M.Fox, B.Franckowiak, A.Franke, R.Gaisser, T.Gallagher, J.Ganugapati, R.Gerhardt, L.Gladstone, L.Goldschmidt, A.Goodman, J.Gozzini, R.Grant, D.Griesel, T.Groß, A.Grullon, S.Gunasingha, R.Gurtner, M.Ha, C.Hallgren, A.Halzen, F.Han, K.Hanson, K.Hardtke, R.Hasegawa, Y.Heise, J.Helbing, K.Hellwig, M.Herquet, P.Hickford, S.Hill, G.Hodges, J.Hoffman, K.Hoshina, K.Hubert, D.Huelsnitz, W.Hughey, B.Hülß, J.-P.Hulth, P.Hultqvist, K.Hundertmark, S.Hussain, S.Imlay, R.Inaba, M.Ishihara, A.Jacobsen, J.Japaridze, G.Johansson, H.Joseph, J.Kampert, K.-H.Kappes, A.Karg, T.Karle, A.Kawai, H.Kelley, J.Kiryluk, J.Kislat, F.Klein, S.Klepser, S.Kohnen, G.Kolanoski, H.Köpke, L.Kowalski, M.Kowarik, T.Krasberg, M.Kuehn, K.Kuwabara, T.Labare, M.Laihem, K.Landsman, H.Lauer, R.Leich, H.Leier, D.Lewis, C.Lucke, A.Lundberg, J.Lünemann, J.Madsen, J.Maruyama, R.Mase, K.Matis, H.Mcparland, C.Meagher, K.Meli, A.Merck, M.Messarius, T.Mészáros, P.Miyamoto, H.Mohr, A.Montaruli, T.Morse, R.Movit, S.Münich, K.Nahnhauer, R.Nam, J.Nießen, P.Nygren, D.Odrowski, S.Olivas, A.Olivo, M.Ono, M.Panknin, S.Patton, S.Pérez De Los Heros, C.Petrovic, J.Piegsa, A.Pieloth, D.Pohl, A.Porrata, R.Potthoff, N.Pretz, J.Price, P.Przybylski, G.Rawlins, K.Razzaque, S.Redl, P.Resconi, E.Rhode, W.Ribordy, M.Rizzo, A.Robbins, W.Rodriguez, J.Roth, P.Rothmaier, F.Rott, C.Roucelle, C.Rutledge, D.Ryckbosch, D.Sander, H.-G.Sarkar, S.Satalecka, K.Schlenstedt, S.Schmidt, T.Schneider, D.Schultz, O.Seckel, D.Semburg, B.Seo, S.Sestayo, Y.Seunarine, S.Silvestri, A.Smith, A.Song, C.Spiczak, G.Spiering, C.Stamatikos, M.Stanev, T.Stezelberger, T.Stokstad, R.Stoufer, M.Stoyanov, S.Strahler, E.Straszheim, T.Sulanke, K.-H.Sullivan, G.Swillens, Q.Taboada, I.Tarasova, O.Tepe, A.Ter-Antonyan, S.Tilav, S.Tluczykont, M.Toale, P.Tosi, D.Turčan, D.Van Eijndhoven, N.Vandenbroucke, J.Van Overloop, A.Viscomi, V.Vogt, C.Voigt, B.Walck, C.Waldenmaier, T.Walter, M.Wendt, C.Westerhoff, S.Whitehorn, N.Wiebusch, C.Wiedemann, C.Wikström, G.Williams, D.Wischnewski, R.Wissing, H.Woschnagg, K.Xu, X.Yodh, G.Yoshida, S.2010-11-052010-11-052010-11-05200910.1103/PhysRevD.79.062001https://infoscience.epfl.ch/handle/20.500.14299/56969WOS:000264762500005We present a search for point sources of high energy neutrinos using 3.8 yr of data recorded by AMANDA-II during 2000-2006. After reconstructing muon tracks and applying selection criteria designed to optimally retain neutrino-induced events originating in the northern sky, we arrive at a sample of 6595 candidate events, predominantly from atmospheric neutrinos with primary energy 100 GeV to 8 TeV. Our search of this sample reveals no indications of a neutrino point source. We place the most stringent limits to date on E-2 neutrino fluxes from points in the northern sky, with an average upper limit of E-2 Phi(nu mu)+nu(tau)<= 5.2x10(-11) TeV cm(-2) s(-1) on the sum of nu(mu) and nu(tau) fluxes, assumed equal, over the energy range from 1.9 TeV to 2.5 PeV.Cosmic-RaysTelescopesSelectionDetectorObjectsLimitstext::journal::journal article::research article