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Assembly of the Most Massive Clusters at Cosmic Noon

Published onMay 31, 2019
Assembly of the Most Massive Clusters at Cosmic Noon
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Abstract

The next decade will see a transformational shift in our understanding of protoclusters as deep spectroscopy over wide fields of view will be possible in conjunction with high resolution deep imaging in the optical and near-infrared, enabling the characterization of their overall structure, the galaxies within them, and the gas that feeds them.

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