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Resolving the cosmic X-ray background with a next-generation high-energy X-ray observatory

Published onMay 31, 2019
Resolving the cosmic X-ray background with a next-generation high-energy X-ray observatory
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Abstract

We review progress in understanding the high-energy X-ray emission from active galactic nuclei, and highlight exciting opportunities for a future high-resolution, hard (1-200 keV) X-ray observatory to resolve the cosmic X-ray background and characterize accreting supermassive black holes across cosmic time.

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