001     297017
005     20211110133942.0
024 7 _ |a 10.3204/DESY-PROC-2008-02/roncadelli_marco
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024 7 _ |a arXiv:0911.1056
|2 arXiv
024 7 _ |a WOS:00
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024 7 _ |a inspire:836180
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037 _ _ |a PUBDB-2016-01770
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088 1 _ |a arXiv:0911.1056
088 _ _ |a arXiv:0911.1056
|2 arXiv
100 1 _ |a Roncadelli, Marco
|0 P:(DE-HGF)0
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111 2 _ |a 4th Patras Workshop on Axions, WIMPs and WISPs
|g AXION-WIMP 2008
|c Hamburg
|d 2008-06-18 - 2008-06-21
|w Germany
245 _ _ |a Detection of distant AGN by MAGIC: the transparency of the Universe to high-energy photons
260 _ _ |c 2009
|b Deutsches Elektronen-Synchrotron, DESY
|a Hamburg
300 _ _ |a 53-56
336 7 _ |a Conference Paper
|0 33
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336 7 _ |a Internal Report
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336 7 _ |a INPROCEEDINGS
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520 _ _ |a The 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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588 _ _ |a Dataset connected to DataCite, INSPIRE
650 _ 7 |a photon: oscillation
|2 INSPIRE
650 _ 7 |a blazar: emission
|2 INSPIRE
650 _ 7 |a emission: model
|2 INSPIRE
650 _ 7 |a gamma ray: VHE
|2 INSPIRE
650 _ 7 |a showers: air
|2 INSPIRE
650 _ 7 |a magnetic field
|2 INSPIRE
650 _ 7 |a transparency
|2 INSPIRE
650 _ 7 |a Cherenkov
|2 INSPIRE
650 _ 7 |a VERITAS
|2 INSPIRE
650 _ 7 |a GLAST
|2 INSPIRE
650 _ 7 |a axion
|2 INSPIRE
650 _ 7 |a WIMP
|2 INSPIRE
650 _ 7 |a AGN
|2 INSPIRE
693 _ _ |a HERA
|e Facility (machine) HERA
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700 1 _ |a De Angelis, Alessandro
|0 P:(DE-HGF)0
|b 1
700 1 _ |a Mansutti, Oriana
|0 P:(DE-HGF)0
|b 2
773 _ _ |a 10.3204/DESY-PROC-2008-02/roncadelli_marco
787 0 _ |a Lindner, Axel et.al.
|d Verlag Deutsches Elektronen-Synchrotron, 2008
|i IsPartOf
|0 PUBDB-2016-01759
|r DESY-PROC-2008-02
|t Proceedings, 4th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2008)
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