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

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A fast onboard star-extraction algorithm optimized for the SVOM Visible Telescope

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

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

Content Provider	Springer Nature Link
Author	Xin, LiPing Deng, JingSong Zheng, WeiKang Wei, JianYan Wang, Jing Qiu, YuLei Hu, JingYao
Copyright Year	2010
Abstract	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.
Starting Page	56
Ending Page	59
Page Count	4
File Format	PDF
ISSN	16747348
Journal	Science in China Series G
Volume Number	53
Issue Number	1
e-ISSN	18622844
Language	English
Publisher	SP Science China Press
Publisher Date	2010-05-20
Publisher Place	Heidelberg
Access Restriction	One Nation One Subscription (ONOS)
Subject Keyword	GRB afterglow follow-up observation TNT GRB 080330 Astronomy, Observations and Techniques Classical Continuum Physics Physics
Content Type	Text
Resource Type	Article
Subject	Physics and Astronomy

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