1.4 GHz and [O III] luminosities of the sources with an [O III] detection. Sources with radio+optical AGN, radio-AGN, and optical-AGN are shown. For optical-AGN without a radio detection, the arrows show the upper limits on L_1.4 GHz. The shaded regions show the expected radio luminosity from the shocks scenario using the Nims et al. (2015) model, where the lower and upper edges show the limits for 5% and 25% coupling efficiency between AGN luminosity and wind kinetic luminosity, respectively. Different regions show the [O III] to bolometric luminosity conversion factors from Heckman et al. (2004) and Stasińska et al. (2025). The horizontal dotted lines show the luminosity divisions used in Sect. 4. To highlight the low-to-moderate luminosity nature of the sources in our study, we also show the parameter space occupied by the radio-AGN sample from Kukreti & Morganti (2024) in black contours, which examines the relation between radio properties and feedback on [O III] out to z = 0.8.