AGN winds ionised by the accretion disk and X-ray corona, may carry and deposit sufficient energy and metals to the interstellar medium, thereby affecting the evolution of galaxies. However, the observational evidence and associated modelling are not yet conclusive.
Key Questions include:

— How and where do winds launch as a result of the accretion process?

— What are the physical conditions of the outflowing material?

— Does AGN feedback impact the interstellar medium of the host galaxy?

This thematic area will develop Artificial Intelligence emulators of outflow physical models to constrain the physical properties and launching site of AGN winds using archival data from state-of-the-art X-ray facilities (XMM, NuSTAR, Chandra, XRISM). These results will provide a solid basis for comparison to multiwavelength observations of galaxy-scale winds (ALMA, HST, JWST) and the latest numerical simulations of AGN feedback and galaxy evolution.