A GRB follow-up system at the xinglong observatory and detection of the high-redshift GRB 060927

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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).

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Zheng, W. K., Deng, J. S., Zhai, M., Xin, L. P., Qiu, Y. L., Wang, J., … Hu, J. Y. (2008). A GRB follow-up system at the xinglong observatory and detection of the high-redshift GRB 060927. Chinese Journal of Astronomy and Astrophysics, 8(6), 693–699. https://doi.org/10.1088/1009-9271/8/6/08

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