November 1, 2021 (v1)
Journal article
Abstract In large-scale hydrodynamical cosmological simulations, the fate of massive galaxies is mainly dictated by the modeling of feedback from active galactic nuclei (AGN). The amount of energy released by AGN feedback is proportional to the mass that has been accreted on to the BHs, but the exact sub-grid modeling of AGN feedback differs in...
Uploaded on: December 4, 2022