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A galaxy cluster, or cluster of galaxies, is a structure that consists of anywhere from hundreds to thousands of galaxies that are bound together by gravity with typical masses ranging from 10¹⁴–10¹⁵ solar masses. However, the number of galaxy clusters detected so far in the AKARI North Ecliptic Pole (NEP) field is limited. In this work, we provide. We develop a novel data-driven method for generating synthetic optical observations of galaxy clusters. In cluster weak lensing, the interplay. A lot goes on in a galaxy cluster. There can be anything from tens to thousands of galaxies bound together by gravity. The galaxies themselves. Like humans, galaxies can't stand to be alone. Nudged by gravity, galaxies tend to group together, and some even end up in the universe's. Galaxy clusters trace the highest density peaks in the large-scale structure of the Universe. Their clustering provides a powerful probe that can be exploited. These new RGS results bring us one step forward to understanding the charge exchange phenomenon in galaxy clusters. Key words: atomic processes / line. A galaxy cluster, or cluster of galaxies, is a structure that consists of anywhere from hundreds to thousands of galaxies that are bound together by gravity. Clusters grow through the infall of individual galaxies or groups of galaxies, Known as a brightest cluster galaxy, this is generally cD galaxy. Specifically, for each simulation you will find projections of simulated observable quantities of simulated galaxy clusters and cluster mergers. These synthetic.