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We have performed a very long baseline interferometry (VLBI) survey of local(z < 0.05) ultra hard X-ray (14-195 keV) selected active galactic nuclei (AGN)from the Swift Burst Alert Telescope (BAT) using KVN, KaVA, and VLBA. We firstexecuted fringe surveys of 142 BAT-detected AGN at 15 or 22 GHz. Based on thefringe surveys and archival data, we find 10/279 nearby AGN (~4%) VLBI have 22GHz flux above 30 mJy. This implies that the X-ray AGN with a bright nuclearjet are not common. Among these 10 radio-bright AGN, we obtained 22 GHz VLBIimaging data of our own for four targets and reprocessed archival data for sixtargets. We find that, although our 10 AGN observed with VLBI span a wide rangeof pc-scale morphological types, they lie on a tight linear relation betweenaccretion luminosity and nuclear jet luminosity. Our result suggests that apowerful nuclear radio jet correlates with the accretion disc luminosity. Wealso probed the fundamental plane of black hole activity at VLBI scales (e.g.,few milli-arcsecond). The jet luminosity and size distribution among our sampleroughly fit into the proposed AGN evolutionary scenario, finding powerful jetsafter the blow-out phase based on the Eddington ratio (\lambda_{Edd})-hydrogencolumn density (N_{H}) relation. In addition, we find some hints of gas inflowor galaxy-galaxy merger in the majority of our sample. This implies that gassupply via tidal interactions in galactic scale may help the central AGN tolaunch a powerful parsec-scale jet.

BAT AGN Spectroscopic Survey -- XVII: The Parsec-scale Jet Properties of the Ultra Hard X-ray Selected Local AGN