Robotic telescope for rapid gamma-ray burst follow-up observations

R. Sato*, N. Kawai, M. Suzuki, Y. Yatsu, J. Kataoka

*この研究の対応する著者

研究成果: Conference article査読

抄録

We have developed a robotic telescope at Tokyo Institute of Technology (Tokyo Tech) to perform rapid follow-up observations of early optical afterglows of gamma-ray bursts (GRBs). Our system was primarily designed to respond quickly to the GRB locations notified by the High Energy Transient Explorer 2 (HETE-2) satellite, but it can also respond to all the notifications provided by the GRB Coordinates Network (GCN). In order to cover the error circle of the HETE-2, wide-field and thermo-electrically cooled CCD camera is equipped on the focus of a small 30cm telescope. A field of view of our system is 44 arcminutes which can cover the most error circles of the HETE-2. The rapid response (less than 15 sec after the notice) and slew speeds (6 deg / sec) make our system appropriate for observing GRB afterglows. Using this convenient system, we detected the optical afterglow of GRB 030329. Observation was started 67 minutes after the burst, which was one of the earliest detection in the world. We report the performance of our telescope coupled to CCD camera, and estimate the limiting magnitude of our system. Although our system is located in a region affected by strong city lights, the limiting magnitude is approximately 17.3 mag.

本文言語English
ページ(範囲)859-870
ページ数12
ジャーナルProceedings of SPIE - The International Society for Optical Engineering
5492
PART 2
DOI
出版ステータスPublished - 2004 12月 24
外部発表はい
イベントGround-based Instrumentation for Astronomy - Glasgow, United Kingdom
継続期間: 2004 6月 212004 6月 25

ASJC Scopus subject areas

  • 電子材料、光学材料、および磁性材料
  • 凝縮系物理学
  • コンピュータ サイエンスの応用
  • 応用数学
  • 電子工学および電気工学

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