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Fig. 11.

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Radio-luminosity ratio of L5 GHz, FIRST/L5 GHz, FP as a function of sBHAR. The yellow shaded area represents the corresponding Eddington limit accretion (λEdd = 1) region assuming the local scaling relation of MBH − M (Kormendy & Ho 2013) for the range of 9 < log(M/M) < 12 where our sources reside, as shown in Fig. 8. The gray cross represents the typical error bar of the two values.

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