Predicted EIC flux of GeV gamma rays for a jetted TDE at z ∼ 0.01. The blue line shows the EIC emission produced by inverse-Compton scattering of thermal photons from a super-Eddington accretion disk by the electrons responsible for the prompt X-ray emission. The black solid and dashed lines represent the sensitivities of Fermi/LAT and CTAO, respectively, for an exposure time of 10⁵ s. Since the EIC emission is produced by the same electrons that power the prompt emission, it is expected to be approximately contemporaneous with the prompt emission.