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Multimessenger Constraints on Production Sites of High-energy Neutrinos from NGC 1068

  • Authors: Abhishek Das, Kohta Murase, B. Theodore Zhang

Abhishek Das et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 2.

Cascaded photon spectra (colored lines) and all-flavor neutrino spectra (dashed black lines) for different values of the emission radius R for different parameter sets explored in this work. Among the photon spectra, solid lines correspond to ξB = 1, while dashed lines correspond to ξB = 0.01. All panels are made for injected cosmic-ray protons with sCR = 2 and ﹩{\varepsilon }_{p}^{{\rm{\max }}}=30﹩ TeV. The solid black lines correspond to the 95% contour lines and the best-fit line from the IceCube data (R. Abbasi et al. 2022). Gamma-ray data from the Fermi-LAT (M. Ajello et al. 2023) and MAGIC (V. A. Acciari et al. 2019) observations are also shown.

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