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Galaxy clusters are valuable cosmological probes. However, cluster massestimates rely on observable quantities that are affected by complicatedbaryonic physics in the intracluster medium (ICM), including feedback fromactive galactic nuclei (AGN). Cosmological simulations have started to includeAGN feedback using subgrid models. In order to make robust predictions, thesystematics of different implementations and parametrizations need to beunderstood. We have developed an AGN subgrid model in FLASH that supports a fewdifferent black hole accretion models and feedback models. We use this model tostudy the effect of AGN on X-ray cluster observables and its dependence onmodel variations.

The Influence of AGN Feedback on Galaxy Cluster Observables