Fig. A.1.
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qIR as a function of redshift for all the 500 targets (grey points), the 4 VLBA-detected AGN (dark blue stars) and the 277 non-detections that constitute the M★-matched sample (red points). The green dots are the 42 non-detections which make the (M★, rms)-matched control sample. The black line is the NLS fit of all the targets described by the power law (1 + z)−0.13.
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