从30 keV峰值滚降：对硬X射线和伽马射线背景的建模
天体物理学
2008-11-26 v1
摘要
我们将简要讨论在几十keV以上进行灵敏X射线观测的重要性，这有助于更好地理解与射电宁静和射电噪活动星系核中超大质量黑洞初级辐射相关的物理机制，以及最遮蔽源头的宇宙学演化。
引用
@article{arxiv.astro-ph/0604523,
title = {Rolling down from the 30 keV peak: modelling the hard X-ray and gamma-ray backgrounds},
author = {Andrea Comastri and Roberto Gilli and Guenther Hasinger},
journal= {arXiv preprint arXiv:astro-ph/0604523},
year = {2008}
}
备注
8 pages, 3 figures. Invited talk at the meeting "Gamma Wave 2005", Bonifacio, September 2005. To be published in "Experimental Astronomy"