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The Hard VHE γ‐Ray Emission in High‐Redshift TeV Blazars: Comptonization of Cosmic Microwave Background Radiation in an Extended Jet?

  • Authors: Markus Böttcher, Charles D. Dermer, and Justin D. Finke

Böttcher, Dermer, & Finke 2008 The Astrophysical Journal Letters 679 L9.

  • Provider: AAS Journals

Caption: Fig. 2.

Same as Fig. 1, but for the SED of 2004 June 5–10. Here, optical and X‐ray data were obtained from simultaneous XMM‐Newton observations (Aharonian et al. 2007a). Inner‐jet parameters used for the synchrotron fit were ﹩\Gamma =25﹩, ﹩\gamma ^{\,\prime }_{1}=1.8\times 10^{5}﹩, ﹩\gamma ^{\,\prime }_{2}=1.5\times 10^{6}﹩, ﹩q=2.5﹩, ﹩L_{\mathrm{jet}\,}=1.45\times 10^{40}﹩ ergs s−1, ﹩R^{\,\prime }_{B}=6\times 10^{16}﹩ cm, and ﹩B^{\,\prime }=0.05﹩ G.

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