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000094764 0247_ $$2arXiv$$aarXiv:1111.2736
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000094764 041__ $$aEnglish
000094764 1001_ $$0P:(DE-HGF)0$$aMilke, N.$$b0$$eCorresponding author
000094764 1112_ $$0C11-08-11$$2inspire$$a32nd International Cosmic Ray Conference$$cBeijing$$d2011-08-11 - 2011-08-18$$gICRC2011$$wChina
000094764 1101_ $$aDESY$$bStandort Zeuthen
000094764 245__ $$aStudies on the Unfolding of the Atmospheric Neutrino Spectrum with IceCube 59 using the TRUEE Algorithm
000094764 260__ $$aBeijing$$bInstitute of Physics$$c2011
000094764 300__ $$a833
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000094764 500__ $$3Converted on 2013-05-30 15:06
000094764 500__ $$3Converted on 2013-06-21 19:21
000094764 520__ $$aThe 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.
000094764 536__ $$0G:(DE-HGF)POF2-52x$$a52x - Programm Astroteilchenphysik - Topic unbekannt (POF2-52x)$$cPOF2-52x$$fPOF II$$x0
000094764 693__ $$0EXP:(DE-H253)IceCube-20150101$$5EXP:(DE-H253)IceCube-20150101$$eIceCube South Pole Neutrino Observatory$$x0
000094764 7001_ $$0P:(DE-HGF)0$$aRhode, W.$$b1$$eCorresponding author
000094764 7001_ $$0P:(DE-H253)PIP1012816$$aRuhe, T.$$b2$$eCorresponding author
000094764 7001_ $$0P:(DE-HGF)0$$aIceCube Collaboration$$b3$$eCollaboration author
000094764 7870_ $$0PUBDB-2016-01646$$aHussain, S. et.al.$$dBeijing : Institute of Physics, 2011$$iIsPartOf$$rarXiv:1111.2735$$tProceedings, 32nd International Cosmic Ray Conference (ICRC 2011)
000094764 7870_ $$0PUBDB-2016-01646$$aHussain, S. et.al.$$dBeijing : Institute of Physics, 2011$$iIsPartOf$$rarXiv:1111.2735$$tProceedings, 32nd International Cosmic Ray Conference (ICRC 2011)
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000094764 9132_ $$0G:(DE-HGF)POF3-613$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vMatter and Radiation from the Universe$$x0
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