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000083101 088__ $$2arXiv$$aarXiv:0711.0353
000083101 1001_ $$0P:(DE-HGF)0$$aWissing, H.$$b0
000083101 1112_ $$0C07-07-03$$2inspire$$a30th International Cosmic Ray Conference$$cMerida$$d2007-07-03 - 2007-07-11$$gICRC2007$$wMexico
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000083101 245__ $$aSearch for Relativistic Magnetic Monoploles with the AMANDA-II Detector
000083101 260__ $$aCiudad de Mexico$$bUniversidad Nacional Autonoma de Mexico$$c2007
000083101 300__ $$a139-142
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000083101 500__ $$3Converted on 2013-06-21 19:20
000083101 520__ $$aCherenkov emissions of magnetic charges moving through matter will exceed those of electric charges by several orders of magnitude. The AMANDA neutrino telescope is therefore capable of efficiently detecting relativistic magnetic monopoles that pass through its sensitive volume.  We present the to date most stringent limit on the flux of relativistic magnetic monopoles based on the analysis of one year of data taken with AMANDA-II.
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000083101 693__ $$0EXP:(DE-H253)AMANDA-20170101$$5EXP:(DE-H253)AMANDA-20170101$$eAntarctic Muon And Neutrino Detector Array$$x0
000083101 7001_ $$0P:(DE-HGF)0$$aIceCube Collaboration$$b1$$eCollaboration author
000083101 7870_ $$0PUBDB-2016-01641$$aCaballero, Rogelio et.al.$$dCiudad de Mexico : Universidad Nacional Autonoma de Mexico, 2007$$iIsMemberOf$$rarXiv:0711.0353$$tProceedings, 30th International Cosmic Ray Conference (ICRC 2007)
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