A GRB Follow-up System at the Xinglong Observatory and Detection of the High-Redshift GRB 060927 ⋆

W. Zheng, J. Deng, M. Zhai, L. Xin, Y. Qiu, J. Wang, X. Lu, J. Wei, J. Hu
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引用次数: 18

Abstract

A gamma-ray burst (GRB) optical photometric follow-up system at the Xinglong Observatory of National Astronomical Observatories of China (NAOC) has been constructed. It uses the 0.8-m Tsinghua-NAOC Telescope (TNT) and the 1-m EST telescope, and can automatically respond to GRB Coordinates Network (GCN) alerts. Both telescopes slew relatively fast, being able to point to a new target field within ~1 min upon a request. Whenever available, the 2.16-m NAOC telescope is also used. In 2006 the system responded to 15 GRBs and detected seven early afterglows. In 2007 six GRBs have been detected among 18 follow-up observations. TNT observations of the second most distant GRB 060927 (z = 5.5) are shown, which started as early as 91 s after the GRB trigger. The afterglow was detected in the combined image of the first 19×20 s unfiltered exposures. This GRB follow-up system has joined the East-Asia GRB Follow-up Observation Network (EAFON).
星龙天文台GRB后续系统与高红移GRB 060927的探测
在中国国家天文台兴隆天文台建设了伽玛暴(GRB)光学光度跟踪系统。它使用0.8 m清华-国家天文台望远镜(TNT)和1 m EST望远镜,并能自动响应GRB坐标网络(GCN)警报。两个望远镜旋转相对较快,能够根据请求在1分钟内指向一个新的目标场。只要有条件,也会使用2.16米的NAOC望远镜。2006年,该系统对15次伽马射线爆发做出了反应,并探测到7次早期余辉。2007年,在18次后续观测中发现了6次伽马射线暴。图中显示了第二遥远的GRB 060927 (z = 5.5)的TNT观测结果,它早在GRB触发后91秒就开始了。余辉是在第一张19×20 5张未过滤照片的组合图像中检测到的。该GRB后续系统已加入东亚GRB后续观测网(EAFON)。
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