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@INPROCEEDINGS{Milke:94764,
      author       = {Milke, N. and Rhode, W. and Ruhe, T. and DESY},
      collaboration = {{IceCube Collaboration}},
      title        = {{S}tudies on the {U}nfolding of the {A}tmospheric
                      {N}eutrino {S}pectrum with {I}ce{C}ube 59 using the {TRUEE}
                      {A}lgorithm},
      address      = {Beijing},
      publisher    = {Institute of Physics},
      reportid     = {PHPPUBDB-18937},
      pages        = {833},
      year         = {2011},
      abstract     = {The measurement of the atmospheric neutrino energy spectrum
                      provides information about the diffuseneutrino flux from
                      extragalactic sources. A relative increase of the spectrum
                      toward higher energies could be evidencefor neutrino
                      producing hadronic processes in the cosmic high energy
                      accelerators, such as active galactic nuclei orgamma ray
                      bursts. IceCube is currently the largest neutrino detector
                      on Earth and is placed in the antarctic ice at thegeographic
                      South Pole. IceCube permits the detection of neutrinos with
                      energies beyond 106 GeV. Since the acceptanceand the
                      resolution of neutrino telescopes suffer from the finite
                      resolution and limited acceptance, a regularized
                      unfoldingmethod is used to extract the energy distribution
                      of neutrinos from the measured observables. For AMANDA,
                      theunfolding was done with the RUN algorithm. Based on the
                      basic concept of this program and for data analyses in
                      theROOT frame, a new deconvolution algorithm (TRUEE) has
                      been written and tested. With this new algorithm, studieson
                      the analysis of the atmospheric neutrino spectrum measured
                      with the IceCube 59 string configuration will be presented.},
      month         = {Aug},
      date          = {2011-08-11},
      organization  = {32nd International Cosmic Ray
                       Conference, Beijing (China), 11 Aug
                       2011 - 18 Aug 2011},
      cin          = {ZNP(-2012)},
      cid          = {$I:(DE-H253)ZNP_-2012_-20130307$},
      pnm          = {52x - Programm Astroteilchenphysik - Topic unbekannt
                      (POF2-52x)},
      pid          = {G:(DE-HGF)POF2-52x},
      experiment   = {EXP:(DE-H253)IceCube-20150101},
      typ          = {PUB:(DE-HGF)8},
      eprint       = {1111.2736},
      howpublished = {arXiv:1111.2736},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1111.2736;\%\%$},
      url          = {https://bib-pubdb1.desy.de/record/94764},
}