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A&A 479, 41-47 (2008)
DOI: 10.1051/0004-6361:20065605
BL Lacertae contribution to the extragalactic gamma-ray background
T. M. Kneiske1, 2 and K. Mannheim11 Universität Würzburg, Am Hubland, 97057 Würzburg, Germany
2 Department of Physics and Mathematical Physics, University of Adelaide, SA 5005, Australia
e-mail: tkneiske@physics.adelaide.edu.au
(Received 15 May 2006 / Accepted 28 September 2007)
Abstract
Very high energy gamma-rays from blazars
traversing cosmological distances through the metagalactic radiation
field can convert into electron-positron pairs in photon-photon collisions.
The converted gamma-rays initiate electromagnetic cascades
driven by inverse-Compton scattering off the microwave background photons.
Using a model for the time-dependent metagalactic radiation field consistent with all
currently available far-infrared-to-optical data, we calculate
the cascade contribution from faint, unresolved high- and low-peaked blazars to the extragalactic
gamma-ray background as measured by EGRET.
For low-peaked blazars, we adopt a spectral index consistent with the mean
spectral index of EGRET detected blazars, and the EGRET luminosity function.
For high-peaked blazars,
we adopt template spectra matching prototype sources observed
with air-Cherenkov telescopes up to 30 TeV, and a luminosity function
based on X-ray measurements.
The low number of
20 for nearby high-peaked blazars
with a flux exceeding
above 300 GeV inferred from the luminosity function
is consistent with the results from air-Cherenkov telescope observations.
Including the cascade emission from higher redshifts,
the total high-peaked blazar contribution to the observed gamma-ray background at GeV energies
can account for ~30%.
Key words: galaxies: BL Lacertae objects: general -- cosmology: diffuse radiation -- gamma rays: observations
© ESO 2008
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