Outflows and feedback in active galaxies with MUSE and SINFONI Integral Field Spectroscopy. My group provided the first evidences of Positive and Negative feedback on AGN host galaxies
MAGNUM (Measuring Active Galactic Nuclei Under MUSE Microscope) is a MUSE@VLT integral field survey of 10 among the closest and best studied Active Galaxies
SUPER (SINFONI Survey for Unveiling the Physics and the Effect of Radiative feedback) is a SINFONI Large Program to carry out the first statistically-sound investigation of ionised outflows in AGN host galaxies at the peak epoch of AGN and galaxy assembly, z~2. It consists of 280 hours of SINFONI observations in LGS Seeing Enhancer mode to reach a spatial resolution of 1 kpc at z~2.