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Abstract:
A significant limitation in our understanding of AGN-driven outflows is the complex coupling of the AGN luminosity or mechanical jet power with the multi-phase ISM. Here, I present the first results of our Close AGN Reference Survey (CARS) combining spatially-resolved observations from Chandra, VLT-MUSE, SOFIA, JVLA and ALMA for a representative sample of 40 most luminous type 1 AGN at 0.01