The evolution of galaxy clusters from cosmic dawn to noon
            
    Our overall aim is to understand the role of environment in regulating galaxy growth from the first overdensities at z~6, cosmic dawn, to the galaxy clusters forming at the epoch of peak star formation, z~2, cosmic noon. To accomplish this goal, we have and will assemble a vast data set spanning a wide range of frequencies from the UV to the radio
            
            Helmut
            
                        Dannerbauer 
            
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