Three years' systematic GRB follow-up at the Xinglong Observatory and the optical afterglow observations of GRB 080330

被引：3
|
作者：
Xin LiPing [1 ,2 ]
Deng JingSong [1 ]
Zheng WeiKang [1 ,2 ]
Wei JianYan [1 ]
Wang Jing [1 ]
Qiu YuLei [1 ]
Hu JingYao [1 ]
机构：
[1] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
[2] Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China
来源：
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY | 2010年 / 53卷
基金：
中国国家自然科学基金;
关键词：
GRB; afterglow; follow-up observation; TNT; 080330; GAMMA-RAY BURST;
D O I：
10.1007/s11433-010-0031-3
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We present a brief overview of follow-up observations of GRB afterglows made by the 0.8-m TNT and other telescopes at the Xinglong observatory during the last three years. Our system, dedicated to the measurement of early-time optical afterglow emission, responded to 50 GRBs from Jan. 2006 to Apr. 2009. Among them, about 50% have been successfully detected. The fastest response time is 76 sec (GRB 061110A and GRB 090426) after the space-borne GRB detector was triggered. The redshift distribution spans the range from z = 0.033 (GRB 060218) to z = 5.6 (GRB 060927). We also report the optical photometric follow-up of GRB 080330, which is an X-ray flash, as an example of our observations.
引用
收藏
页码：56 / 59
页数：4
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