A new look at the extragalactic very high energy sky: Searching for TeV-emitting candidates among the X-ray-bright, non-Fermi-detected blazar population

Open Access

Fig. 4

Spectral energy distributions of the 77 TeVCAT sources analyzed in this work. The SEDs are color-coded by class using the same coding described in Figure 2. We also show with black (red) dashed and dotted lines the median 0.2–12 keV and 20 GeV–300 TeV fluxes of the BZB subsample (overall population).

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