The GATOS collaboration brings together the expertise of observers and modellers to investigate a variety of topics relating to the physical processes taking place in the nuclear regions of active galactic nuclei. These include the gas flow cycle, the polar dust emission, and the torus/obscuring material properties as well as the co-evolution of the star formation activity/AGN phenomena.
- Jan 2019: GATOS proposal "Resolving the ionized outflows in local Seyfert galaxies with GTC/MEGARA" accepted
- Sep 2017: Next GATOS meeting announced: University of Oxford (15 - 17 January 2018)
- Summer 2017: GATOS ALMA Cycle 5 proposal accepted (PI: S. García-Burillo)