Fig. 2.
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Line-of-sight cosmogenic γ-ray flux from UHECR interactions (blue curve). The solid black line corresponds to the Fermi-LAT preliminary flux estimate for GRB 221009A (Pillera et al. 2022). The dashed red curve indicates the LHAASO sensitivity corresponding to 2000 s of observation. The vertical dotted line corresponds to the highest-energy detection by LHAASO. The synchrotron and SSC emission components are shown as dashed orange and brown curves, respectively.
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