Jet power as a function of disk luminosity of FSRQs (red) and “BL Lacs” (blue) considered in Ghisellini et al. (2014) compared with the NuSTAR blazars considered here. We also show the blazars with z >  4 and z >  5, considered in Sbarrato et al. (2016) and in Ghisellini et al. (2015). Segments connect different states of the same source. The NuSTAR blazars are among the most powerful, both in terms of their disk luminosity and jet power, with PKS 0836+710 having the most powerful jet, and S5 0014+81 having the most powerful accretion disk. We note that the BL Lacs shown here were the only BL Lacs observed by Sbarrato et al. (2013) with broad emission lines. They must be considered the low disk luminosity tail of FSRQ.