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  • 标题:Extragalactic background light models and GeV-TeV observation of blazars
  • 本地全文:下载
  • 作者:K. K. Singh ; P. J. Meintjes
  • 期刊名称:NRIAG Journal of Astronomy and Geophysics
  • 印刷版ISSN:2090-9977
  • 电子版ISSN:2090-9985
  • 出版年度:2020
  • 卷号:9
  • 期号:1
  • 页码:309-320
  • DOI:10.1080/20909977.2020.1743468
  • 语种:English
  • 出版社:Elsevier
  • 摘要:In this work, we use two different methods to determine the opacity of the TeV gamma-rays caused by the extragalactic background light (EBL) via e—e+ production due to photon-photon interaction. The first method, Model-Dependent Approach, uses various EBL models for estimating the opacity as a function of the redshift and energy of the TeV photons. The second method, Model-Independent Approach, relies on using the simultaneous observations of blazars in the MeV-GeV energy range from the Fermi-LAT and in the TeV band from the ground-based gammaray telescopes. We make the underline assumption that the extrapolation of the LAT spectrum of blazars to TeV energies is either a good estimate or an upper limit for the intrinsic TeV spectrum of a source. We apply this method on the simultaneous observations of a few blazars at different redshifts to demonstrate a comparative study of six prominent EBL models. Opacities of the TeV photons predicted by the model-independent approach are systematically larger than the ones estimated from the modeldependent method. Therefore, the gamma-ray observations of blazars can be used to set a strict upper limit on the opacity of the Universe to the TeV photons at a given redshift.
  • 关键词:Galaxies: blazars;observations: gamma-rays;general: EBL
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