| 报告题目： |
Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields |
| 报告人： |
薛永泉 教授 |
| 报告人单位： |
中国科学技术大学天文学系 |
| 报告时间： |
2018年5月31日上午9:00 |
| 报告地点： |
东七楼427 |
| 邀请单位： |
粒子与天体物理研究所 |
| 报告摘要： |
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Highly obscured and Compton-thick (CT) active galactic nuclei (AGNs) escaping even the deepest X-ray surveys are often thought to be comparably numerous to unobscured and moderately obscured AGNs. These sources are necessary for fitting the cosmic X-ray background emission in the 10-30 keV band and play a crucial role in the black hole/galaxy co-evolution history. In this talk I present, in a personal point of view, some recent efforts in searching for highly obscured and CT AGNs in the Chandra Deep Fields. I discuss the properties and implications of the highly obscured and CT AGNs/AGN candidates identified through these efforts. I also discuss future prospects of pushing this area forward.
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| 报告人简介： |
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薛永泉，2000年与2003年分别获得北京大学学士与硕士学位，2008年获得美国普度大学博士学位，之后在美国宾州州立大学从事博士后研究，2012年5月到中国科学技术大学天文系任教授。主要研究方向为利用多波段（尤其是X射线）深场巡天来研究活动星系核的相关物理过程和现象，例如，活动星系核的统计，超大质量黑洞和星系的协同演化，宇宙X射线背景辐射，遮蔽活动星系核以及活动星系核X射线光变等。
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