Kinematic maps obtained from the nonparametric analysis of the [O III] emission line profiles of J1430. Top panels: integrated flux on the left, with the ∼1″ resolution 6 GHz VLA contours at 3,5,10,20, and 60σ from Jarvis et al. (2019) superimposed (white solid lines), and vel_p on the right, which traces the narrow component. Middle panels: vel₀₅ (left) and vel₉₅ (right), which trace blueshifted and redshifted outflowing gas. The same 6 GHz contours shown in the flux map are shown in cyan, and the ∼0.25″ resolution 6 GHz VLA contours at 3, 5, 15, 30, and 60σ from Jarvis et al. (2019) are shown in solid white. The black contours correspond to the brightness temperature ratio (T₃₂/T₂₁) from ALMA CO observations at 0.5″ resolution (Audibert et al. 2023). Bottom panels: W₈₀ on the left, with the same contours as in the vel₀₅ map, and the number of Gaussians fit in each spaxel on the right. White and black crosses indicate the AGN location, defined as the maximum of the [O III] emission. North is up and east to the left.