Presentation description

Radio galaxies are active galactic nuclei with jets misaligned with respect to the line of sight, making them a good laboratory for studying jet structure. Only a handful of radio galaxies have been detected at TeV gamma-ray energies. IC 310, a radio galaxy in the Perseus cluster known to exhibit fast TeV gamma-ray variability, was detected at an elevated TeV gamma-ray flux in March 2024 by the LHAASO gamma-ray observatory. Multi-wavelength follow-up observations of IC 310 during the flaring state were organized. We analyzed the X-Ray follow-up observations from the NuSTAR and Swift-XRT telescopes and constructed a broadband spectral energy distribution (SED) using contemporaneous optical and gamma-ray data for IC 310. We also fit the SED with one-zone and two-zone synchrotron self-Compton (SSC) models in order to gain insight to the underlying physics in extreme environments in the universe.