Predicted X-ray backgrounds for the International X-ray Observatory
The background that will be observed by IXO's X-ray detectors naturally separates into two components: (1) a Cosmic X-ray Background (CXB), primarily due to unresolved point sources at high energies (E>2 keV), along with Galactic component(s) at lower energies that are generated in the disk...
| Những tác giả chính: | , , , , , |
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| Tác giả khác: | |
| Định dạng: | Bài viết |
| Ngôn ngữ: | en_US |
| Được phát hành: |
Society of Photo-optical Instrumentation Engineers
2011
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| Truy cập trực tuyến: | http://hdl.handle.net/1721.1/61647 https://orcid.org/0000-0002-1379-4482 |