Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29463| Title: | Resolving the cosmic X-ray background with a next-generation high-energy X-ray observatory | Authors: | Hickox, Ryan Civano, Francesca Ballantyne, D. Balokovic, M. Boorman, P. Brandt, W. Canning, R. Fornasini, F. Gandhi, P. Jones, M. Lansbury, G. Lanz, L. LANZUISI, Giorgio Madsen, K. MARCHESI, STEFANO Masini, A. Ananna, T. Stern, D. Ricci, C. |
Issue Date: | 2019 | Journal: | BULLETIN OF THE AMERICAN ASTRONOMICAL SOCIETY | Number: | 51 | Issue: | 3 | First Page: | 468 | 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. | URI: | http://hdl.handle.net/20.500.12386/29463 | URL: | https://baas.aas.org/pub/2020n3i468/release/1 | ISSN: | 2330-9458 | Bibcode ADS: | 2019BAAS...51c.468H | Fulltext: | open |
| Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 61598544698940.pdf | postprint | 1.62 MB | Adobe PDF | View/Open |
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