Submitted to Cornell University’s online archive www.arXiv.org in 2000 by Ray Protheroe Post-print sourced from www.arxiv.org. Copyright © 2000 Published by Elsevier Science B.V.We consider the implications of the recent determination of the universal infrared background for the propagation of photons up to 20 TeV from the active galaxy Markarian 501 as observed by HEGRA. At 20 TeV the mean free path for photon-photon collisions on the infrared background would be much shorter than the distance to Markarian 501, implying absorption factors of the order of exp(-10), or greater, and consequently an excessive power output for this active galaxy. Possible solutions of this problem are discussed.R. J. Protheroe and H. Meyerhttp://www.elsevier.co...
There are observations indicating a possible anomalous transparency of intergalactic space (filled w...
The active galaxy Markarian 501 was discovered with air-Cerenkov telescopes at photon energies of 10...
The scope of this paper is to discuss two important questions relevant for TeV γ-ray astronomy; the ...
We present a semi-empirical model for the evolving far-infrared to ultraviolet diffuse background pr...
We use the new results of the HEGRA detector on the TeV gamma-ray emission from Mrk 501 to set upper...
Context: The background radiation in the optical and the infrared cause energy loss in the propagati...
The energy spectrum of Mkn501 in the TeV energy regime, as measured by the HEGRA (High Energy Gamma ...
Attenuation of high-energy gamma-rays by pair production with ultraviolet, optical and infrared (IR)...
Following our previously proposed technique, we have used the recent gamma-ray observations of Mrk 4...
Context. The background radiation in the optical and the infrared cause energy loss in the propagati...
The recent observations of 50 TeV gamma radiation by HEGRA have the potential of determining the ext...
Very high energy gamma-ray data obtained by CAT and HEGRA from active galactic nucleus Mkn 501 are u...
We present a new calculation of the intergalactic gamma-ray absorption coefficient as a function of ...
The flux of high energy (HE, energy $100\,\mathrm{MeV} \lesssim E\lesssim 100\,\mathrm{GeV}$) and ve...
We discuss the determination of the intergalactic pair-production absorption coefficient as derived ...
There are observations indicating a possible anomalous transparency of intergalactic space (filled w...
The active galaxy Markarian 501 was discovered with air-Cerenkov telescopes at photon energies of 10...
The scope of this paper is to discuss two important questions relevant for TeV γ-ray astronomy; the ...
We present a semi-empirical model for the evolving far-infrared to ultraviolet diffuse background pr...
We use the new results of the HEGRA detector on the TeV gamma-ray emission from Mrk 501 to set upper...
Context: The background radiation in the optical and the infrared cause energy loss in the propagati...
The energy spectrum of Mkn501 in the TeV energy regime, as measured by the HEGRA (High Energy Gamma ...
Attenuation of high-energy gamma-rays by pair production with ultraviolet, optical and infrared (IR)...
Following our previously proposed technique, we have used the recent gamma-ray observations of Mrk 4...
Context. The background radiation in the optical and the infrared cause energy loss in the propagati...
The recent observations of 50 TeV gamma radiation by HEGRA have the potential of determining the ext...
Very high energy gamma-ray data obtained by CAT and HEGRA from active galactic nucleus Mkn 501 are u...
We present a new calculation of the intergalactic gamma-ray absorption coefficient as a function of ...
The flux of high energy (HE, energy $100\,\mathrm{MeV} \lesssim E\lesssim 100\,\mathrm{GeV}$) and ve...
We discuss the determination of the intergalactic pair-production absorption coefficient as derived ...
There are observations indicating a possible anomalous transparency of intergalactic space (filled w...
The active galaxy Markarian 501 was discovered with air-Cerenkov telescopes at photon energies of 10...
The scope of this paper is to discuss two important questions relevant for TeV γ-ray astronomy; the ...