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We explore the relationship between the ionized gas outflows and radioactivity using a sample of $\sim$ 6000 AGNs at z < 0.4 with the kinematicalmeasurement based on the [O III] line profile and the radio detection in theVLA FIRST Survey. To quantify radio activity, we divide our sample into aseries of binary subclasses based on the radio properties, i.e.,radio-luminous/radio-weak, AGN-dominated/star-formation-contaminated,compact/extended, and radio-loud/radio-quiet. None of the binary subclassesexhibits a significant difference in the normalized [O III] velocity dispersionat a given [O III] luminosity once we correct for the influence of the hostgalaxy gravitational potential. We only detect a significant difference of [OIII] kinematics between high and low radio-Eddington ratio (L$_{1.4GHz}$/L$_{Edd}$) AGNs. In contrast, we find a remarkable difference in ionizedgas kinematics between high and low bolometric-Eddington ratio AGNs. Theseresults suggest that accretion rate is the primary mechanism in driving ionizedgas outflows, while radio activity may play a secondary role providingadditional influence on gas kinematics

Investigating the Correlation of Outflow Kinematics with Radio Activity. Gas Outflows in AGNs. VII