Fig. 8.
SED of all 11 blazars at z > 2 observed so far by NuSTAR. It can be noted that (1) the synchrotron hump is remarkably similar; (2) for several sources the accretion disk sticks out in the optical-UV band; (3) 0014+813 has an exceptionally powerful accretion disk; and (4) the X-ray and γ-ray emission is more dispersed and variable.
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