Theoretical uncertainties due to AGN subgrid models in predictions of galaxy cluster observable properties
Theoretical uncertainties due to AGN subgrid models in predictions of galaxy cluster observable properties
Cosmological constraints derived from galaxy clusters rely on accurate predictions of cluster observable properties, in which feedback from active galactic nuclei (AGN) is a critical component. In order to model the physical effects due to supermassive black holes (SMBH) on cosmological scales, subgrid modelling is required, and a variety of …