X-ray fitting and SED modeling of HSP and EHSP blazars indicate a subsample may reach detectable TeV fluxes for CTA.
B.4.Broadband spectral energy distribution of 5BZBJ1636–1248 (z=0.246,γ 0 ∼10 5,γ break ∼10 6)
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Constraining the synchrotron peak and estimating the VHE brightness of a sample of extreme high synchrotron peak blazars
X-ray fitting and SED modeling of HSP and EHSP blazars indicate a subsample may reach detectable TeV fluxes for CTA.