Orateur
Description
I will discuss the progress that has been made by coming SZ data from the South Pole Telescope (SPT) with X-ray data from Chandra and XMM-Newton. To date, we have followed up hundreds of SPT-selected clusters with these two X-ray telescopes, providing the strongest constraints on the enrichment history of the intracluster medium (ICM), the dynamical evolution of clusters, the cooling and feedback history of cluster cores, and the deviations from self-similar evolution in cluster cores. These observations have become extremely challenging as we discover clusters at z~2, and so I will also include a discussion of how a next generation of X-ray surveys with STAR-X and AXIS, coupled with resolved SZ experiments, could enable us to trace cluster evolution to the epoch of their formation.
