Resolving the cosmic X-ray background with a next-generation high-energy X-ray observatory
by Ryan Hickox, Francesca Civano, D. Ballantyne, M. Balokovic, P. Boorman, W. Brandt, R. Canning, F. Fornasini, P. Gandhi, M. Jones, G. Lansbury, L. Lanz, G. Lanzuisi, K. Madsen, S. Marchesi, A. Masini, T. Ananna, D. Stern, and C. Ricci
Published onMay 31, 2019
Resolving the cosmic X-ray background with a next-generation high-energy X-ray observatory
·
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.
The full text of this article is only available in PDF format:
Creative Commons Attribution 4.0 International License (CC-BY 4.0)
