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  2. 寺田 幸功

寺田 幸功

テラダ ユキカツ  (Yukikatsu Terada)

基本情報

所属
埼玉大学 大学院理工学研究科 理工学研究科  教授
国立研究開発法人宇宙航空研究開発機構 宇宙科学研究所 特任教授
学位
博士(2002年3月 東京大学)
J-GLOBAL ID
200901062224980497
researchmap会員ID
1000368169
外部リンク

研究キーワード

 14

研究分野

 2

経歴

 8
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学歴

 3

委員歴

 2

論文

 372
  • Makoto Tashiro, Richard Kelley, Shin Watanabe, Hironori Maejima, Lillian Reichenthal, Kenichi Toda, Leslie Hartz, Andrea Santovincenzo, Kyoko Matsushita, Hiroya Yamaguchi, Robert Petre, Brian Williams, Matteo Guainazzi, Elisa Costantini, Yoh Takei, Yoshitaka Ishisaki, Ryuichi Fujimoto, Joy Henegar-Leon, Gary Sneiderman, Hiroshi Tomida, Koji Mori, Hiroshi Nakajima, Yukikatsu Terada, Matthew Holland, Michael Loewenstein, Eric Miller, Makoto Sawada, Timothy Kallman, Jelle Kaastra, Chris Done, Teruaki Enoto, Aya Bamba, Lia Corrales, Yoshihiro Ueda, Erin Kara, Irina Zhuravleva, Yutaka Fujita, Yoshitaka Arai, Marc Audard, Hisamitsu Awaki, Ralf Ballhausen, Chris Baluta, Nobutaka Bando, Ehud Behar, Thomas Bialas, Rozenn Boissay-Malaquin, Laura Brenneman, Gregory V Brown, Meng Chiao, Renata Cumbee, Cor de Vries, Jan-Willem den Herder, María Díaz Trigo, Michael DiPirro, Tadayasu Dotani, Jacobo Ebrero Carrero, Ken Ebisawa, Megan Eckart, Dominique Eckert, Satoshi Eguchi, Yuichiro Ezoe, Carlo Ferrigno, Adam Foster, Yasushi Fukazawa, Kotaro Fukushima, Akihiro Furuzawa, Luigi Gallo, Javier Garcia Martinez, Nathalie Gorter, Martin Grim, Liyi Gu, Kouichi Hagino, Kenji Hamaguchi, Isamu Hatsukade, Katsuhiro Hayashi, Takayuki Hayashi, Natalie Hell, Edmund Hodges-Kluck, Takafumi Horiuchi, Ann Hornschemeier, Akio Hoshino, Yuto Ichinohe, Chisato Ikuta, Ryo Iizuka, Daiki Ishi, Manabu Ishida, Naoki Ishihama, Kumi Ishikawa, Kosei Ishimura, Tess Jaffe, Satoru Katsuda, Yoshiaki Kanemaru, Steven Kenyon, Caroline Kilbourne, Mark Kimball, Shunji Kitamoto, Shogo Kobayashi, Takayoshi Kohmura, Aya Kubota, Maurice Leutenegger, Yoshitomo Maeda, Maxim Markevitch, Hironori Matsumoto, Keiichi Matsuzaki, Dan McCammon, Brian McLaughlin, Brian McNamara, Francois Mernier, Joseph Miko, Jon Miller, Kenji Minesugi, Shinji Mitani, Ikuyuki Mitsuishi, Misaki Mizumoto, Tsunefumi Mizuno, Koji Mukai, Hiroshi Murakami, Richard Mushotzky, Kazuhiro Nakazawa, Chikara Natsukari, Jan-Uwe Ness, Kenichiro Nigo, Mari Nishiyama, Kumiko Nobukawa, Masayoshi Nobukawa, Hirofumi Noda, Hirokazu Odaka, Mina Ogawa, Shoji Ogawa, Anna Ogorzalek, Takashi Okajima, Atsushi Okamoto, Naomi Ota, Masanobu Ozaki, Stephane Paltani, Paul Plucinsky, F Scott Porter, Katja Pottschmidt, Jose Antonio Quero, Takahiro Sasaki, Kosuke Sato, Rie Sato, Toshiki Sato, Yoichi Sato, Hiromi Seta, Maki Shida, Megumi Shidatsu, Shuhei Shigeto, Russel Shipman, Keisuke Shinozaki, Peter Shirron, Aurora Simionescu, Randall Smith, Yang Soong, Hiromasa Suzuki, Andrew Szymkowiak, Hiromitsu Takahashi, Mai Takeo, Toru Tamagawa, Keisuke Tamura, Takaaki Tanaka, Atsushi Tanimoto, Yuichi Terashima, Yohko Tsuboi, Masahiro Tsujimoto, Hiroshi Tsunemi, Takeshi Tsuru, Hiroyuki Uchida, Nagomi Uchida, Yuusuke Uchida, Hideki Uchiyama, Shinichiro Uno, Jacco Vink, Michael Witthoeft, Rob Wolfs, Satoshi Yamada, Shinya Yamada, Kazutaka Yamaoka, Noriko Yamasaki, Makoto Yamauchi, Shigeo Yamauchi, Keiichi Yanagase, Tahir Yaqoob, Susumu Yasuda, Tomokage Yoneyama, Tessei Yoshida, Miohoko Yukita
    Publications of the Astronomical Society of Japan 2025年4月11日  査読有り
    Abstract The X-Ray Imaging and Spectroscopy Mission (XRISM) is a joint mission between the Japan Aerospace Exploration Agency (JAXA) and the National Aeronautics and Space Administration (NASA) in collaboration with the European Space Agency (ESA). In addition to the three space agencies, universities and research institutes from Japan, North America, and Europe have joined to contribute to developing satellite and onboard instruments, data-processing software, and the scientific observation program. XRISM is the successor to the ASTRO-H (Hitomi) mission, which ended prematurely in 2016. Its primary science goal is to examine astrophysical problems with precise, high-resolution X-ray spectroscopy. XRISM promises to discover new horizons in X-ray astronomy. It carries a 6 × 6 pixelized X-ray microcalorimeter on the focal plane of an X-ray mirror assembly (Resolve) and a co-aligned X-ray CCD camera (Xtend) that covers the same energy band over a large field of view. XRISM utilizes the Hitomi heritage, but all designs were reviewed. The attitude and orbit control system was improved in hardware and software. The spacecraft was launched from the JAXA Tanegashima Space Center on 2023 September 6 (UTC). During the in-orbit commissioning phase, the onboard components were activated. Although the gate valve protecting the Resolve sensor with a thin beryllium X-ray entrance window was not yet opened, scientific observation started in 2024 February with the planned performance verification observation program. The nominal observation program commenced with the following guest observation program beginning in 2024 September.
  • Saito, T., Takahashi, M., Inome, Y., Abe, H., Artero, M., Blanch, O., Becerra González, J., Fukami, S., Hadasch, D., Hanabata, Y., Hattori, Y., Herrera Llorente, J., Ishio, K., Iwasaki, H., Katagiri, H., Kawamura, K., Kerszberg, D., Kimura, S., Kiyomoto, T., Kojima, T., Konno, Y., Kobayashi, Y., Koyama, S., Kubo, H., Kushida, J., López-Oramas, A., Masuda, S., Matsuoka, S., Mazin, D., Nakajima, D., Nakamori, T., Nagayoshi, T., Ninci, D., Nishijima, K., Nishiyama, G., Nogami, Y., Nozaki, S., Ogino, M., Ohoka, H., Oka, T., Ono, S., Okumura, A., Orito, R., Rugliancich, A., Sakurai, S., Sasaki, N., Sunada, Y., Suzuki, M., Tamura, K., Takeda, J., Terada, Y., Teshima, M., Tokanai, F., Tomono, Y., Tsujimoto, S., Tsukamoto, Y., Umetsu, Y., Yamamoto, T., Yoshida, T.
    Nuclear Instruments and Methods in Physics Research A 2025年4月  査読有り
    The camera of the Large-Sized Telescopes (LSTs) of the Cherenkov Telescope Array Observatory (CTAO) consists of 1855 pixels that are grouped into 265 high-performance photomultiplier tube (PMT) modules. Each module comprises a seven-light-guide plate, seven PMT units, a slow control board, and a readout board with a trigger board. The requirements for the PMT modules include various aspects, such as photon detection efficiency, dynamic range, buffer depth, and test pulse functionality. We have developed a high-performance PMT module that fulfills all these requirements. Mass-production and quality control (QC) of modules for all four LSTs of the northern CTAO have been completed. Here we report on the technical details of each element of the module and its performance, together with the methods and results of QC measurements....
  • Yoneyama, T., Fukushima, K., Hayashi, K., Kanemaru, Y., Ogawa, S., Yoshida, T., Audard, M., Behar, E., Inoue, S., Ishihara, Y., Kohmura, T., Maeda, Y., Mizumoto, M., Nagashima, N., Nobukawa, M., Pottschmidt, K., Shidatsu, M., Sugai, H., Terada, Y., Terashima, Y., Tsuboi, Y., Uchida, H., Yanagi, T., Yoshimoto, M.
    2025年3月  
    XRISM/Xtend Transient Search (XTS) detected an X-ray flare from an X-ray source XRISM J1747-2832 located at the Galactic central region on 2025-03-19 TT. The source position is determined to be (R.A., Dec.) = (266.761, -28.538), with a systematic error of & sim; 40 arcsec....
  • Mandel, S., Mori, K., Hailey, C., Bachetti, M., Degenaar, N., Draghis, P., Grindlay, J., Hong, J., Ponti, G., Reynolds, M., Tomsick, J., Wijnands, R., Fukushima, K., Hayashi, K., Kanemaru, Y., Ogawa, S., Yoshida, T., Iizuka, R., Baluta, C., Terada, Y., Costantini, E., Guainazzi, M., Kelley, R., Matsushita, K., Petre, R., Williams, B., Yamaguchi, H., Watanabe, S., Tashiro, M.
    2025年3月  
    A follow-up XRISM observation has been performed for the new Galactic centre transient MAXI J1744-294 detected by MAXI on January 2, 2025 (ATels #16975 and #16983)....
  • Sugai, H., Fukushima, K., Hayashi, K., Kanemaru, Y., Ogawa, S., Yoshida, T., Audard, M., Behar, E., Inoue, S., Ishihara, Y., Kohmura, T., Maeda, Y., Mizumoto, M., Nagashima, N., Nobukawa, M., Pottschmidt, K., Shidatsu, M., Terada, Y., Terashima, Y., Tsuboi, Y., Uchida, H., Yanagi, T., Yoneyama, T., Yoshimoto, M.
    2025年3月  
    XRISM/Xtend Transient Search (XTS) detected an increase in X-ray intensity from an X-ray source XRISM J1717-3717 on 2025-02-28 TT. The source position is determined to be (R.A., Dec.) = (259.347, -37.28648), with a systematic error of & sim; 40 arcsec....
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MISC

 263

書籍等出版物

 4

講演・口頭発表等

 150
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担当経験のある科目(授業)

 53
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所属学協会

 6
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共同研究・競争的資金等の研究課題

 13
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