Fig. 4


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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.