Fig. 11.
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VHE light curve at hνobs = 1 TeV (top) and spectrum around the peak at tobs = 110 days (bottom) for the moderate (in blue) and optimistic (in red) reference cases (see Table 6). Both predict similar fluxes in the synchrotron range due to the observational constraints, but they differ in the SSC regime. The upper limit from H.E.S.S. is indicated for comparison (Abdalla et al. 2020).
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