Fig. 12.
Top left: maximum observed apparent speed as a function of total VLBI luminosity. Top right: Fermi-LAT flux as a function of average VLBI core flux. Center left: Fermi-LAT flux as a function of average VLBI jet flux. Center right: average VLBI core brightness temperature as a function of Fermi-LAT luminosity. Center bottom: Fermi-LAT luminosity as a function of average VLBI core dominance.
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