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
Background radiation fields pervade the Universe, and above a certain energy any γ-ray flux emitted ...
The search for detection of ?-rays from distant AGNs by Imaging Atmospheric Cherenkov Telescopes (IA...
Axion Like Particles (ALPs) are predicted to couple with photons in the presence of magnetic fields....
The recent detection of blazar 3C279 by MAGIC has confirmed previous indications by H.E.S.S. that th...
The recent detection of blazar 3C279 by MAGIC has confirmed previous indications by H.E.S.S. that th...
The MAGIC collaboration has recently reported the detection of the strong gamma-ray blazar 3C279 dur...
The detection of the blazar 3C279 at a record distance z=0.54 by MAGIC, and of other distant blazars...
MAGIC is currently the world's largest single dish ground based imaging atmospheric Cherenkov telesc...
Recent findings by gamma-ray Cherenkov telescopes suggest a higher transparency of the Universe to v...
The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detect...
The atmospheric Cherenkov gamma- ray telescope MAGIC, designed for a low- energy threshold, has dete...
TeV photons coming from a distant extragalactic source are not able to propagate over large distance...
The MAGIC collaboration has recently reported the detection of the strong -ray blazar 3C279 during a...
Axionlike particles (ALPs) are predicted to couple with photons in the presence of magnetic fields. ...
Very high energy gamma-rays are expected to be absorbed by the extragalactic background light over c...
Background radiation fields pervade the Universe, and above a certain energy any γ-ray flux emitted ...
The search for detection of ?-rays from distant AGNs by Imaging Atmospheric Cherenkov Telescopes (IA...
Axion Like Particles (ALPs) are predicted to couple with photons in the presence of magnetic fields....
The recent detection of blazar 3C279 by MAGIC has confirmed previous indications by H.E.S.S. that th...
The recent detection of blazar 3C279 by MAGIC has confirmed previous indications by H.E.S.S. that th...
The MAGIC collaboration has recently reported the detection of the strong gamma-ray blazar 3C279 dur...
The detection of the blazar 3C279 at a record distance z=0.54 by MAGIC, and of other distant blazars...
MAGIC is currently the world's largest single dish ground based imaging atmospheric Cherenkov telesc...
Recent findings by gamma-ray Cherenkov telescopes suggest a higher transparency of the Universe to v...
The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detect...
The atmospheric Cherenkov gamma- ray telescope MAGIC, designed for a low- energy threshold, has dete...
TeV photons coming from a distant extragalactic source are not able to propagate over large distance...
The MAGIC collaboration has recently reported the detection of the strong -ray blazar 3C279 during a...
Axionlike particles (ALPs) are predicted to couple with photons in the presence of magnetic fields. ...
Very high energy gamma-rays are expected to be absorbed by the extragalactic background light over c...
Background radiation fields pervade the Universe, and above a certain energy any γ-ray flux emitted ...
The search for detection of ?-rays from distant AGNs by Imaging Atmospheric Cherenkov Telescopes (IA...
Axion Like Particles (ALPs) are predicted to couple with photons in the presence of magnetic fields....