Home >

news ヘルプ

論文・著書情報


タイトル
和文: 
英文:The search for optical emission on and before the GRB trigger with the WIDGET telescope 
著者
和文: Tamagawa, T., Usui, F., Urata, Y., Abe, K., Onda, K., Tashiro, M., Terada, Y., Fujiwara, H., Miura, N., Hirose, S., 河合 誠之, Yoshida, A., Mori, M., Makishima, K..  
英文: Tamagawa, T., Usui, F., Urata, Y., Abe, K., Onda, K., Tashiro, M., Terada, Y., Fujiwara, H., Miura, N., Hirose, S., Kawai, N., Yoshida, A., Mori, M., Makishima, K..  
言語 English 
掲載誌/書名
和文: 
英文:Nuovo Cimento C Geophysics Space Physics C 
巻, 号, ページ Vol. 28        pp. 771
出版年月 2005年7月 
出版者
和文: 
英文: 
会議名称
和文: 
英文: 
開催地
和文: 
英文: 
DOI https://doi.org/10.1393/ncc/i2005-10150-1
アブストラクト WIDGET is a robotic telescope for monitoring the HETE-2 field-of-view to detect Gamma-Ray Burst optical flashes or possible optical precursors. The system has 62°×62° wide field-of-view which covers about 80% of HETE-2 one with a 2k×2k Apogee U10 CCD camera and a Canon EF 24 mm f/1.4 wide-angle lens without a bandpass filter. WIDGET has been in operation since June 2004 at Akeno observing site where is about 200 km apart from Tokyo. Typical limiting magnitude with S/N = 3 at the site is V = 10mag for 5 seconds exposure and V = 11mag for 30 seconds exposure. We had already six coincident observations with HETE-2 position alerts. It was, however, cloudy for all cases due to rainy season in Japan. The expected number of coincident observations under clear sky is about 5 events per year. We will extend the system in early 2005 for Swift era to monitor optical transients in wider field-of-view, multi-color or polarization modes.

©2007 Tokyo Institute of Technology All rights reserved.