Fig. 8
Bolometric luminosity vs. νpeak for our sample (magenta empty circles) compared with the sample reported by Giommi et al. (2012b; blue open and filled symbols) and the high-power HSP from Padovani et al. (2012b; red filled circles). Sources with only lower limits for the redshift are plotted as upward arrows, while sources with lower limits for νpeak are shown as right pointing arrows.
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