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There is an ongoing debate on whether feedback from active galactic nuclei(AGNs) can effectively regulate the star formation activities in their hostgalaxies. To investigate the feedback effect of AGN-driven outflows, we performintegral-field spectroscopic observations of 40 moderate-luminosity(10$^{41.5}$ $<$ L$_{\rm [OIII];cor}$ $<$ 10$^{43.1}$ erg s$^{-1}$) Type-2 AGNsat z $<$ 0.1, which present strong outflow signatures in the integrated [OIII]kinematics. Based on the radial profile of the normalized [OIII] velocitydispersion by stellar velocity dispersion, we measure the kinematic outflowsize and extend the kinematic outflow size-luminosity relation reported in Kang& Woo (2018) into a wider luminosity range (over four orders of magnitude in[OIII] luminosity). The shallow slope of the kinematic outflow size-luminosityrelation indicates that while ionizing photons can reach out further, kineticenergy transfer is much less efficient due to various effects, demonstratingthe importance of kinematical analysis in quantifying the outflow size andenergetics. By comparing the outflow kinematics with the host galaxyproperties, we find that AGNs with strong outflows have higher star formationrate and higher HI gas fraction than those AGNs with weak outflows. Theseresults suggest that the current feedback from AGN-driven outflows do notinstantaneously suppress or quench the star formation in the host galaxieswhile its effect is delayed.

Unraveling the complex structure of AGN-driven outflows: V. Integral-field spectroscopy of 40 moderate-luminosity Type-2 AGNs