Speaker
Description
The Three Hundred Simulation Suites include 324 re-simulated regions identified around massive clusters and resimulated with different hydrodynamical codes and resolution. Their purpose is to provide a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications. Extensive work has been done to create mocks images to compare with observations and catalogs of simulated clusters have been extracted to match the characteristics of observed samples, such as NIKA2 and CHEX-MATE. I will give an overview of the products at disposal to the community, provide information on how to access them, discuss some comparison between the results of the hydrodynamical codes, and present how the simulations helped with both the analysis and the interpretation of observed data.