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Active galactic nucleus (AGN) driven outflows can have a significant impacton the evolution of the host galaxy. In this work, we compare the properties ofgalaxies that hosts AGNs with and without outflows. Our sample consists of 103AGNs identified by mid-IR color-color selection, and confirmed with opticalspectroscopy at a redshift range of 0.3 $\lesssim$ z $\lesssim$ 0.9. We fit the[OIII] $\lambda$5007 line using spectra from the zCOSMOS survey to identify andto study the occurrence of outflows. We find that ionized outflows are presentin $\sim$25\% of our sample, with the largest incidence at the highest [OIII]and X-ray luminosity bins. The fastest outflows are found in the more extendedand massive galaxies. We do not observe a difference in the star formation rateof AGNs with outflows compared to AGNs without outflows. From visual inspectionand non-parametric morphological studies, we obtain that outflows arepreferentially observed in galaxies with disk-type and elliptical morphologies.

Host galaxy and nuclear properties of IR-selected AGNs with and without outflow signatures