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Fig. A.2
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Model spectra of secondary γ-rays produced by interaction of monoenergetic primary γ-rays with energy Eγo = 10 TeV. Same as Fig. 2, but calculated with CRbeam and ELMAG 3.03. After corrections to the implementation of the EBL model of Franceschini et al. (2008) in ELMAG 3.03, CRbeam, and ELMAG show much better agreement.
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