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000297017 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2008-02/roncadelli_marco
000297017 0247_ $$2arXiv$$aarXiv:0911.1056
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000297017 0881_ $$aarXiv:0911.1056
000297017 088__ $$2arXiv$$aarXiv:0911.1056
000297017 1001_ $$0P:(DE-HGF)0$$aRoncadelli, Marco$$b0
000297017 1112_ $$a4th Patras Workshop on Axions, WIMPs and WISPs$$cHamburg$$d2008-06-18 - 2008-06-21$$gAXION-WIMP 2008$$wGermany
000297017 245__ $$aDetection of distant AGN by MAGIC: the transparency of the Universe to high-energy photons
000297017 260__ $$aHamburg$$bDeutsches Elektronen-Synchrotron, DESY$$c2009
000297017 300__ $$a53-56
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000297017 520__ $$aThe recent detection of blazar 3C279 by MAGIC has confirmed previous indications by H.E.S.S. that the Universe is more transparent to very-high-energy gamma rays than previously thought. We show that this fact can be reconciled with standard blazar emission models provided photon oscillations into a veri light Axion-Like Particle occur in extragalactic magnetic fields. A quantitative estimate of this effect explains the observed spectrum of 3C279. Our prediction can be tested in the near future by the satellite-borne GLAST detector as well as by the ground-based Imaging Atmospheric Cherenkov Telescpoes H.E.S.S., MAGIC, CANGAROO III, VERITAS and by the Extensive Air Shower arrays ARGO-YBJ and MILAGRO.
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000297017 588__ $$aDataset connected to DataCite, INSPIRE
000297017 650_7 $$2INSPIRE$$aphoton: oscillation
000297017 650_7 $$2INSPIRE$$ablazar: emission
000297017 650_7 $$2INSPIRE$$aemission: model
000297017 650_7 $$2INSPIRE$$agamma ray: VHE
000297017 650_7 $$2INSPIRE$$ashowers: air
000297017 650_7 $$2INSPIRE$$amagnetic field
000297017 650_7 $$2INSPIRE$$atransparency
000297017 650_7 $$2INSPIRE$$aCherenkov
000297017 650_7 $$2INSPIRE$$aVERITAS
000297017 650_7 $$2INSPIRE$$aGLAST
000297017 650_7 $$2INSPIRE$$aaxion
000297017 650_7 $$2INSPIRE$$aWIMP
000297017 650_7 $$2INSPIRE$$aAGN
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000297017 7001_ $$0P:(DE-HGF)0$$aDe Angelis, Alessandro$$b1
000297017 7001_ $$0P:(DE-HGF)0$$aMansutti, Oriana$$b2
000297017 773__ $$a10.3204/DESY-PROC-2008-02/roncadelli_marco
000297017 7870_ $$0PUBDB-2016-01759$$aLindner, Axel et.al.$$dVerlag Deutsches Elektronen-Synchrotron, 2008$$iIsPartOf$$rDESY-PROC-2008-02$$tProceedings, 4th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2008)
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