The Compton-thick AGN NGC 1068 is highly obscured and viewed at a large viewing angle. Thus the primary emission from source is not directly observed at X-rays, which makes studying the source difficult. Also, recently the source has been detected by IceCube as a source of high-energy neutrinos. Numerous models have been proposed as ways to produce neutrinos in this source. Due to the low-powered jets, the models focus on the corona as the origin of neutrino production. We report on MYTorus fits to the NuSTAR and INTEGRAL spectral fits to determine the characteristics of the corona.
Rodi et al. (Wed,) studied this question.