Relation between the jet and accretion disk properties. Left: correlation between the luminosities at 1.4 GHz (L_1.4 GHz [erg s⁻¹]) and absorption corrected 2−10 keV (). The two black dashed lines in the lower and higher with the boundary of erg s⁻¹ represent the fitting lines of Eqs. (3) and (4), respectively. Right: correlation between the jet power (P_jet) and bolometric AGN luminosity (L_AGN,bol). The black solid, dashed, and dot-dashed line shows the case with the jet production efficiency η_jet = 1, η_jet = 0.1, and η_jet = 0.01, respectively, by assuming the radiation efficiency of η_rad = 0.1 (Soltan 1982). The other symbols are the same as in Fig. 1.