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Fig. B.1.
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SED at VHE gamma rays obtained with LST-1 (blue squares) and MAGIC (orange diamonds; Acciari et al. 2022) using all observations between observation-day intervals t − t0 ∼ [1, 4] d (see Table 1 for LST-1). The best-fit model for LST-1 is displayed as a blue line together with a grey spectral error band.
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