@inproceedings{oai:jaxa.repo.nii.ac.jp:00011539,
 author = {倉本, 祐輔 and 谷津, 陽一 and 五十川, 知子 and 斎藤, 孝男 and 片岡, 淳 and 河合, 誠之 and 山本, 佳久 and 宮澤, 航 and 松永, 三郎 and 宇井, 恭一 and Kuramoto, Yusuke and Yatsu, Yoichi and Ikagawa, Tomoko and Saito, Takao and Kataoka, Jun and Kawai, Nobuyuki and Yamamoto, Yoshihisa and Miyazawa, Wataru and Matsunaga, Saburo and Ui, Kyoichi},
 book = {第4回宇宙科学シンポジウム, Proceedings of the 4th Space Science Symposium},
 month = {Aug},
 note = {Lab for Space Systems (LSS) in the Tokyo Institute of Technology successfully launched 1 kg pico-satellite CUTE-1 on June 30, 2003. Work is being collaborated with LSS for developing 50 kg-class satellite, Hu-ring, which can detect GRBs in 0.5 to 400 keV band. Such a small satellite has benefits of being quickly developed, flexibly designed at small cost. Furthermore, it provides good opportunities to test new/challenging technologies in space environment. It is planned to use avalanche photodiodes (APD), for the first time in space as a low-energy particle monitor. Basic characteristics of APDs will be tested thoroughly by the forthcoming pico-satellite, CUTE-2. The distribution of low-energy (E less than 30 keV) electrons/protons will be studied especially in South Atlantic Anomaly (SAA) and auroral zone with CUTE-2., 資料番号: AA0047899103},
 pages = {435--436},
 publisher = {宇宙航空研究開発機構宇宙科学研究本部, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)},
 title = {Development of Tokyo-tech pico-satellite CUTE-2 for GRB observation satellite Hu-ring: Instructions for participants of the ISAS symposium},
 year = {2004}
}