Publication | Open Access
Extragalactic optical-infrared background radiation, its time evolution and the cosmic photon-photon opacity
881
Citations
75
References
2008
Year
EngineeringBackground LightInfrared PhysicsSpace OpticCosmologyInfrared OpticCosmic Photon-photon OpacityLarge Scale StructureObservational CosmologyGalaxy FormationPhotometryPhysicsHigh Energy ParticlesTime EvolutionCosmic RayBackground RadiationHigh-energy AstrophysicsHigh-energy Cosmic RayEarly UniverseEmissivity
Context. The background radiation in the optical and the infrared cause energy loss in the propagation of high energy particles through space. In particular, TeV observations with Cherenkov telescopes of extragalactic sources are influenced by the opacity effects due to the interaction of the very high-energy source photons with the background light.
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