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Modeling the Imprints of Large-scale Magnetized Structures on γ-Rays from Extragalactic Transients

  • Authors: Saikat Das, Soebur Razzaque, Nestor Mirabal, Nicola Omodei, Kohta Murase, Israel Martinez-Castellanos

Saikat Das et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 5.

UHE γ-ray (εγ ≳ 1018 eV) injection model. Pair echo synchrotron emission flux assuming Lγ,iso = 1054 erg s−1, Ep,iso ≃ 6 × 1051 erg, fesc → 1. The dashed vertical line corresponds to the characteristic energy of synchrotron radiation at a time Δt ≃ 192 days after the initial trigger. The dashed vertical line marks the synchrotron photon energy for which the characteristic pair echo time spread is Δtsyn ≃ 192 days.

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