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Constraints on the optical-IR extragalactic background from γ-ray absorption studies

Published online by Cambridge University Press:  17 August 2012

Luigi Costamante
Luigi Costamante*
Affiliation:
Stanford University, Stanford, USA INAF, Brera Observatory, Milano, Italy email: luigic2011@gmail.com
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Abstract

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Very high energy (VHE ≳0.1 TeV) gamma-rays from extragalactic sources, interacting by γ-γ collisions with diffuse intergalactic radiation fields, provide an alternative way to constrain the diffuse background light, completely independent of direct measurements. The limits depend however on our knowledge of the physics of the gamma-ray sources. After clarifying the interplay between background light and VHE spectra, I summarize the extent and validity of the obtainable limits, and where future improvements can be expected.

Keywords

galaxies: activeBL Lacertae objects: generalcosmology: diffuse radiationgamma rays: observationsinfrared: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S284: The Spectral Energy Distribution of Galaxies , September 2011 , pp. 420 - 428
Copyright
Copyright © International Astronomical Union 2012

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