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We explore the connection between the black hole mass and its relativisticjet for a sample of radio-loud AGN (z < 1), in which the relativistic jetparameters are well estimated by means of long term monitoring with the 14mMets\"ahovi millimeter wave telescope and the Very Long Base-line Array (VLBA).NIR host galaxy images taken with the NOTCam on the Nordic Optical Telescope(NOT) and retrieved from the 2MASS all-sky survey allowed us to perform adetailed surface brightness decomposition of the host galaxies in our sampleand to estimate reliable black hole masses via their bulge luminosities. Wepresent early results on the correlations between black hole mass and therelativistic jet parameters. Our preliminary results suggest that the moremassive the black hole is, the faster and the more luminous jet it produces.

Linking the central engine to the jet properties in radio loud AGN