Key words: quasars: emission lines — galaxies: nuclei — galaxies: bulges — black hole physics

1 INTRODUCTION

2 SAMPLE AND DATA ANALYSIS

3 SMBH MASS, EDDINGTON RATIO AND STELLAR VELOCITY DISPERSION

4 MBH-σ* RELATION
4.1 The mass deviation from MBH-σ* relation
4.2 Uncertainties

5 ORIGIN OF RADIO LUMINOSITY
5.1 L5GHz-L[OIII] relation
5.2 The radio luminosity dependence on the SMBH mass and the Eddington ratio

6 CONCLUSIONS