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Galaxy clusters are composed of dark matter and of baryons, divided between the stars (10% of the mass) and the hot intra-cluster medium (ICM, 90%). Gravitational lensing allows to directly probe the potential of galaxy clusters, as it is directly se
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______293::f0b935e9847a0f9ce04a9c521c54565b
https://hdl.handle.net/2123/31102
https://hdl.handle.net/2123/31102
