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@ARTICLE{Ahrens:329829,
      author       = {Ahrens, J. and Bai, X. and Barwick, S. W. and Becka, T. and
                      Becker, K. H. and Bernardini, Elisa and Bertrand, D. and
                      Binon, F. G. and Biron, A. and Boersma, D. J. and Boeser,
                      Sebastian and Botner, O. and Bouchta, A. and Bouhali, O. and
                      Burgess, T. and Carius, S. and Castermans, T. and Chen, A.
                      and Chirkin, D. and Collin, B. and Conrad, J. and Cooley, J.
                      and Cowen, D. F. and Davour, A. and De Clercq, C. and
                      DeYoung, T. and Desiati, P. and Dewulf, J. P. and Ekstrom,
                      P. and Feser, T. and Gaisser, T. K. and Ganugapati, R. and
                      Gaug, M. and Geenen, Heiko and Gerhardt, L. and Goldschmidt,
                      A. and Gross, A. and Hallgren, A. and Halzen, F. and Hanson,
                      K. and Hardtke, R. and Harenberg, T. and Hauschildt, Tonio
                      and Helbing, K. and Hellwig, M. and Herquet, P. and Hill, G.
                      C. and Hubert, D. and Hughey, B. and Hulth, P. O. and
                      Hultqvist, K. and Hundertmark, S. and Jacobsen, J. and
                      Karle, A. and Kestel, M. and Kopke, L. and Kowalski, M. and
                      Kuehn, K. and Lamoureux, J. I. and Leich, H. and Leuthold,
                      M. and Lindahl, P. and Liubarsky, I. and Madsen, J. and
                      Mandli, K. and Marciniewski, P. and Matis, H. S. and
                      McParland, C. P. and Messarius, T. and Minaeva, Y. and
                      Miocinovic, P. and Morse, R. and Munich, K. and Nahnhauer,
                      R. and Neunhoffer, T. and Niessen, P. and Nygren, D. R. and
                      Ogelman, H. and Olbrechts, Ph. and Perez de los Heros, C.
                      and Pohl, A. C. and Porrata, R. and Price, P. B. and
                      Przybylski, G. T. and Rawlins, K. and Resconi, E. and Rhode,
                      W. and Ribordy, M. and Richter, S. and Rodriguez Martino, J.
                      and Sander, H. G. and Schinarakis, K. and Schlenstedt, S.
                      and Schmidt, T. and Schneider, D. and Schwarz, R. and
                      Silvestri, A. and Solarz, M. and Spiczak, G. and Spiering,
                      C. and Stamatikos, M. and Steele, D. and Steffen, P. and
                      Stokstad, R. G. and Sulanke, K. H. and Taboada, I. and
                      Thollander, L. and Tilav, S. and Wagner, W. and Walck, C.
                      and Wang, Y. R. and Wiebusch, C. H. and Wiedemann, C. and
                      Wischnewski, R. and Wissing, H. and Yodh, G.},
      collaboration = {{AMANDA Collaboration}},
      title        = {{S}earch for extraterrestrial point sources of neutrinos
                      with {AMANDA}-{II}},
      journal      = {Physical review letters},
      volume       = {92},
      number       = {7},
      issn         = {1079-7114},
      address      = {College Park, Md.},
      publisher    = {APS},
      reportid     = {PUBDB-2017-06379, astro-ph/0309585},
      pages        = {071102},
      year         = {2004},
      note         = {Standort Zeuthen; AMANDA Collaboration},
      abstract     = {We present the results of a search for point sources of
                      high energy neutrinos in the northern hemisphere using
                      AMANDA-II data collected in the year 2000. Included are flux
                      limits on several AGN blazars, microquasars, magnetars and
                      other candidate neutrino sources. A search for excesses
                      above a random background of cosmic-ray-induced atmospheric
                      neutrinos and misreconstructed downgoing cosmic-ray muons
                      reveals no statistically significant neutrino point sources.
                      We show that AMANDA-II has achieved the sensitivity required
                      to probe known TeV gamma-ray sources such as the blazar
                      Markarian 501 in its 1997 flaring state at a level where
                      neutrino and gamma-ray fluxes are equal.},
      keywords     = {neutrino: cosmic radiation (INSPIRE) / cosmic radiation:
                      particle source (INSPIRE) / cosmic radiation: flux (INSPIRE)
                      / upper limit (INSPIRE) / AGN: blazar (INSPIRE) / quasar
                      (INSPIRE) / matter: magnetic (INSPIRE) / Cherenkov counter:
                      water (INSPIRE) / photomultiplier (INSPIRE) / data
                      management (INSPIRE) / muon: cosmic radiation (INSPIRE) /
                      numerical methods (INSPIRE) / AMANDA (INSPIRE) /
                      experimental results (INSPIRE)},
      cin          = {DESY(-2012)},
      ddc          = {550},
      cid          = {$I:(DE-H253)DESY_-2012_-20170516$},
      pnm          = {899 - ohne Topic (POF3-899)},
      pid          = {G:(DE-HGF)POF3-899},
      experiment   = {EXP:(DE-H253)AMANDA-20170101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)16},
      UT           = {WOS:000189139500007},
      pubmed       = {pmid:14995836},
      doi          = {10.1103/PhysRevLett.92.071102},
      url          = {https://bib-pubdb1.desy.de/record/329829},
}