Fig. 1.
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Flux upper limits obtained from H.E.S.S. observations of NGC 1068. This figure also shows MAGIC flux upper limits (Acciari et al. 2019) along with a Fermi-LAT data bow tie and an 0.1-1 TeV data point from the Fermi-LAT catalog (Abdollahi et al. 2022). Models A and B show the absorbed γ-ray flux from the neutrino source (see Sect. 4.2). A model for jet-driven bubbles (Sect. 4.1.1) is provided. The calorimetric bound is also shown.
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