Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Fermi-LAT high-z active galactic nuclei and the extragalactic background light.

Armstrong, Thomas and Brown, Anthony M. and Chadwick, Paula M. (2017) 'Fermi-LAT high-z active galactic nuclei and the extragalactic background light.', Monthly notices of the Royal Astronomical Society., 470 (4). pp. 4089-4098.

Abstract

Observations of distant gamma-ray sources are hindered by the presence of the extragalactic background light (EBL). In order to understand the physical processes that result in the observed spectrum of sources, it is imperative that a good understanding of the EBL is included. In this work, an investigation into the imprint of the EBL on the observed spectra of high-redshift Fermi-LAT active galactic nuclei is presented. By fitting the spectrum below ∼10 GeV, an estimation of the unabsorbed intrinsic source spectrum is obtained; by applying this spectrum to data up to 300 GeV, it is then possible to derive a scaling factor for different EBL models. A second approach uses five sources (PKS 0426−380, 4C +55.17, Ton 116, PG 1246+586 and RBS 1432) that were found to exhibit very high energy (VHE) emission (Eγ > 100 GeV). Through Monte Carlo simulations, it is shown that the observation of VHE photons, despite the large distances of these objects, is consistent with current EBL models. Many of these sources would be observable with the upcoming ground-based observatory, the Cherenkov Telescope Array, leading to a better understanding of the EBL.

Item Type:Article
Full text:(VoR) Version of Record
Download PDF
(1446Kb)
Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1093/mnras/stx1309
Publisher statement:This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Date accepted:24 May 2017
Date deposited:11 October 2017
Date of first online publication:29 May 2017
Date first made open access:11 October 2017

Save or Share this output

Export:
Export
Look up in GoogleScholar