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The Close AGN Reference Survey (CARS www.cars-survey.org) has assembled a rich comma hyperdimensional dataset for 33 nearby Type 1 AGN comma anchored by VLT-MUSE IFU datacubes for every target comma along with pan-chromatic complementary datasets including ALMA for a large subset of the sample. We now propose an orders-of-magnitude increase in the spatial and temporal resolution of young stars and their ages (respectively) for the entire sample. The proposed WFC3-UVIS UV imaging will map sites of very recent star formation along multiphase quasar-driven outflows comma instability-driven gas inflows comma and merger-driven tidal interactions comma testing whether each might lead to the suppression or even triggering of star formation. It is comma therefore comma a direct test of both negative and positive black hole feedback models.