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Blazars as beamlights to probe the Extragalactic Background Light in the Fermi and Cherenkov telescopes era by Persic, Massimo; Mankuzhiyil, Nijil; Tavecchio, Fabrizio is a scholarly article available to read on EtoBox.

What is Blazars as beamlights to probe the Extragalactic Background Light in the Fermi and Cherenkov telescopes era about?

The Extragalactic Background Light (EBL) is the integrated light from all the stars that have ever formed, and spans the IR-UV range. The interaction of very-high-energy (VHE: E>100 GeV) gamma-rays, emitted by sources located at cosmological distances, with the intervening EBL results in electron-positron pair production that leads to energy-dependent attenuation of the observed VHE flux. This introduces a fundamental ambiguity in the interpretation of the measured VHE blazar spectra: neither the intrinsic spectra, nor the EBL, are separately known - only their combination is. In this paper we propose a method to measure the EBL photon number density. It relies on using simultaneous observations of blazars in the optical, X-ray, high-energy (HE: E>100 MeV) gamma-ray (from the Fermi telescope), and VHE gamma-ray (from Cherenkov telescopes) bands. For each source, the method involves best-fitting the spectral energy distribution (SED) from optical through HE gamma-rays (the latter being largely unaffected by EBL attenuation as long as z<1) with a Synchrotron Self-Compton (SSC) model. We extrapolate such best-fitting models into the VHE regime, and assume they represent the blazars' i

Author

Persic, Massimo; Mankuzhiyil, Nijil; Tavecchio, Fabrizio

Published

2009

Language

EN