TeV spectral energy flux of HESS J1614−518 plotted together with the GeV spectral energy flux of 2FHL J1614.3−5146e (Ackermann et al. 2016) and 3FGL J1614.3−5146e (Acero et al. 2015). The integral fluxes given in the Fermi-LAT catalogs were converted using the power-law models given in the catalogs. The energy of the flux points was determined by calculating the geometrical center of the energy boundaries in log-space.