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The Energetic Universe in Focus: Twenty years of Science with the Chandra X-ray Observatory

Stellar energetic particles in the magnetically turbulent habitable zones of TRAPPIST-1-like planetary systems

The ADVANCE Program and the PhD Network at Northeastern University

Why there are so many successful AGN Feedback models?

The velocity structure of the X-ray emitting gas in simulated galaxy cluster mergers

Thesis talks

Connecting across Scales: From Galaxies into the Cosmic Web with the Magneticum Simulations.

The role of ionized and molecular outflows in quasar evolution.

AGN winds, feedback and the baryon cycle in the galaxy ecosystem

Measuring the Impact of Mass Outflows in Nearby Active Galaxies