all wavelengths and compact (milliarcsecond scale) radio emission of extreme brightness
temperatures, often exceeding the Compton limit (Urry 1999). Their radio spectra are
generally well described by a power-law shape, with a “flat” spectral index α< 0. 5 (where
the flux density Fν∝ ν− α). Multi-epoch Very Long Baseline Interferometry (VLBI)
observations often show superluminal expansion, and the radio and optical emission is …