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Fig. 5
Left panel. Radio VLBA luminosity against γ-optical loudness (Go ≡ S′γ/S′opt) for the M1-1FGL quasars and BL Lacs. Right panel. Optical luminosity against γ-radio loudness (Gr ≡ S′γ/S′VLBA). The dotted and dashed lines represent the ordinary least-square fit to the data for quasars and BL Lacs respectively.
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