Introduction.- Integral field spectroscopy and spectral energy distributions.- Energetic galaxy-wide outflows in high-z ULIRGs hosting AGN activity.- Kiloparsec scale outflows are prevalent in luminous AGN: outflows and feedback in the context of the overall AGN population.- Storm in a "Teacup" a radio-quiet quasar with ≈10 kpc radio-emitting bubbles and extreme gas kinematics.- No submillimetre signature of star formation suppression among X-ray luminous AGN.- Conclusions.- Ongoing and future work.
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