pith. machine review for the scientific record. sign in

arxiv: 0906.2962 · v1 · submitted 2009-06-16 · 🌌 astro-ph.HE · astro-ph.IM

Recognition: unknown

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
show 1 more author
Authors on Pith no claims yet
classification 🌌 astro-ph.HE astro-ph.IM
keywords follow-upsystemdetectedtelescopebeenearlygrbsnaoc
0
0 comments X
read the original 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 about 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 91s after the GRB trigger. The afterglow was detected in the combined image of first 19x20s unfiltered exposures. This GRB follow-up system has joined the East-Asia GRB Follow-up Observation Network (EAFON).

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.