Relations between the values obtained from the BH fundamental plane and those obtained in this study. Top left: relation between two different BH mass estimations. M_BH,FP is obtained from the fundamental plane of Gültekin et al. (2019) and by using the obtained X-ray and radio luminosities in this study. M_BH, ⋆ is the BH mass estimated from the scaling relation of Kormendy & Ho (2013) and by using the obtained stellar mass. The gray cross represents the typical error bar of the two parameters. The gray dashed line represents the 1:1 line with the scatter area of the typical error bar. Top right: relation between the L_{5 GHz, FIRST} and L_{5 GHz, FP}, which is estimated from the fundamental plane relation of Gültekin et al. (2019) with the values of M_BH, ⋆ and . The gray cross represents the typical error bar of the two parameters. The gray dashed line represents the 1:1 line, with the scatter area of the typical error bar. Bottom left: black hole mass ratio of M_BH,FP/M_BH, ⋆ as a function of ℛ_obs. Bottom right: radio-luminosity ratio of L_{5 GHz, FIRST}/L_{5 GHz, FP} as a function of ℛ_obs. The orange shaded area represents the possible Doppler boost area by assuming typical radio-loud AGN. The red shaded area represents the possible range of the ℛ_obs for blazars by assuming a blazar sequence at 0 < z < 5. The gray cross represents the typical error bar of the two values in each panel.