2012MNRAS.422L..48P

We study the quasi-simultaneous near-IR, optical, ultraviolet and X-ray photometry of 11 γ-ray selected blazars for which redshift estimates larger than 1.2 have been recently provided. Four of these objects turn out to be high-power blazars with the peak of their synchrotron emission between ∼ 3 {x} 10¹⁵ and ∼ 10¹⁶ Hz, and therefore of a kind predicted to exist but never seen before. This discovery has important implications for our understanding of physical processes in blazars, including the so-called `blazar sequence', and might also help in constraining the extragalactic background light through γ-ray absorption since two sources are strongly detected even in the 10-100 GeV Fermi-LAT band. Based on our previous work and their high powers, these sources are very likely high-redshift flat-spectrum radio quasars, with their emission lines swamped by the non-thermal continuum.