AGN feedback
AGN feedback (either radiative or mechanical) is largely used in numerical and semi-analytical simulations of galaxies evolution. Although There is mounting evidence that AGN outflows are ubiquitous, observational proofs of the impact that such AGN-driven outflows have on their host galaxies are still largely missing. This is one of my main research interests at the moment, and I am using FIR photometry (Herschel), IFU observations (SINFONI/VLT), sub-mm interferometry (PdBI and ALMA).