研究者データベース

粟木 久光アワキ ヒサミツ

所属部署名大学院理工学研究科 数理物質科学専攻
職名教授
Last Updated :2020/07/04

研究者基本情報

基本情報

氏名

  • 氏名

    粟木 久光
  • 氏名(カナ)

    アワキ ヒサミツ

基本情報

所属

所属・職名

  • 部署

    大学院理工学研究科 数理物質科学専攻
  • 職名

    教授

学歴等

学歴

  • 1991年, 名古屋大学, 理学研究科
  • 1991年, 名古屋大学
  • 1986年, 金沢大学, 理学部
  • 1986年, 金沢大学

学位

  • 博士(理学)

その他基本情報

所属学協会

  • 米国天文学会
  • 国際天文学会連合
  • 日本物理学会
  • 日本天文学会
  • The American Astronomical Society

委員歴

  • 2007年 - 2008年, 日本天文学会, 早川基金選考委員会, 日本天文学会
  • 2004年 - 2005年, 日本天文学会, 早川基金選考委員, 日本天文学会
  • 2002年 - 2003年, 日本天文学会, 地域開催地理事, 日本天文学会

研究活動情報

研究分野等

研究分野

  • 自然科学一般, 天文学

研究キーワード

  • X線天文学
  • X-ray Astronomy

著書・発表論文等

論文

  • Detection of polarized gamma-ray emission from the Crab nebula with the Hitomi Soft Gamma-ray Detector, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年12月, [査読有り], 0004-6264, 10.1093/pasj/psy118
  • Hitomi X-ray observation of the pulsar wind nebula G21.5-0.9, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年06月, [査読有り], 0004-6264, 10.1093/pasj/psy027
  • HITOMI (ASTRO-H) X-ray astronomy satellite, Tadayuki Takahashi, Motohide Kokubun, Kazuhisa Mitsuda, Richard L. Kelley, Takaya Ohashi, Felix Aharonian, Hiroki Akamatsu, Fumie Akimoto, Steven W. Allen, Naohisa Anabuki, Lorella Angelini, Keith Arnaud, Makoto Asai, Marc Audard, Hisamitsu Awaki, Magnus Axelsson, Philipp Azzarello, Chris Baluta, Aya Bamba, Nobutaka Bando, Marshall W. Bautz, Thomas Bialas, Roger Blandford, Kevin Boyce, Laura W. Brenneman, Gregory V. Brown, Esra Bulbul, Edward M. Cackett, Edgar Canavan, Maria Chernyakova, Meng P. Chiao, Paolo S. Coppi, Elisa Costantini, Steve O' Dell, Michael DiPirro, Chris Done, Tadayasu Dotani, John Doty, Ken Ebisawa, Megan E. Eckart, Teruaki Enoto, Yuichiro Ezoe, Andrew C. Fabian, Carlo Ferrigno, Adam R. Foster, Ryuichi Fujimoto, Yasushi Fukazawa, Stefan Funk, Akihiro Furuzawa, Massimiliano Galeazzi, Luigi C. Gallo, Poshak Gandhi, Kirk Gilmore, Margherita Giustini, Andrea Goldwurm, Liyi Gu, Matteo Guainazzi, Daniel Haas, Yoshito Haba, Kouichi Hagino, Kenji Hamaguchi, Ilana M. Harrus, Isamu Hatsukade, Takayuki Hayashi, Katsuhiro Hayashi, Kiyoshi Hayashida, Jan Willem Den Herder, Junko S. Hiraga, Kazuyuki Hirose, Ann Hornschemeier, Akio Hoshino, John P. Hughes, Yuto Ichinohe, Ryo Iizuka, Hajime Inoue, Yoshiyuki Inoue, Kazunori Ishibashi, Manabu Ishida, Kumi Ishikawa, Kosei Ishimura, Yoshitaka Ishisaki, Masayuki Itoh, Masachika Iwai, Naoko Iwata, Naoko Iyomoto, Chris Jewell, Jelle Kaastra, Tim Kallman, Tsuneyoshi Kamae, Erin Kara, Jun Kataoka, Satoru Katsuda, Junichiro Katsuta, Madoka Kawaharada, Nobuyuki Kawai, Taro Kawano, Shigeo Kawasaki, Dmitry Khangulyan, Caroline A. Kilbourne, Mark Kimball, Journal of Astronomical Telescopes, Instruments, and Systems, Journal of Astronomical Telescopes, Instruments, and Systems, 2018年04月, [査読有り], 2329-4124, 10.1117/1.JATIS.4.2.021402
  • Hitomi observation of radio galaxy NGC 1275: The first X-ray microcalorimeter spectroscopy of Fe-K alpha line emission from an active galactic nucleus, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psx147
  • Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psx072
  • Glimpse of the highly obscured HMXB IGR J16318-4848 with Hitomi, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psx154
  • Hitomi X-ray studies of giant radio pulses from the Crab pulsar, Felix Aharonian, Hiroki Akamatsu, Fumie Akimoto, Steven W. Allen, Lorella Angelini, Marc Audard, Hisamitsu Awaki, Magnus Axelsson, Aya Bamba, Marshall W. Bautz, Roger Blandford, Laura W. Brenneman, Gregory V. Brown, Esra Bulbul, Edward M. Cackett, Maria Chernyakova, Meng P. Chiao, Paolo S. Coppi, Elisa Costantini, Jelle De Plaa, Cor P. De Vries, Jan Willem Den Herder, Chris Done, Tadayasu Dotani, Ken Ebisawa, Megan E. Eckart, Teruaki Enoto, Yuichiro Ezoe, Andrew C. Fabian, Carlo Ferrigno, Adam R. Foster, Ryuichi Fujimoto, Yasushi Fukazawa, Akihiro Furuzawa, Massimiliano Galeazzi, Luigi C. Gallo, Poshak Gandhi, Margherita Giustini, Andrea Goldwurm, Liyi Gu, Matteo Guainazzi, Yoshito Haba, Kouichi Hagino, Kenji Hamaguchi, Ilana M. Harrus, Isamu Hatsukade, Katsuhiro Hayashi, Takayuki Hayashi, Kiyoshi Hayashida, Junko S. Hiraga, Ann Hornschemeier, Akio Hoshino, John P. Hughes, Yuto Ichinohe, Ryo Iizuka, Hajime Inoue, Yoshiyuki Inoue, Manabu Ishida, Kumi Ishikawa, Yoshitaka Ishisaki, Masachika Iwai, Jelle Kaastra, Tim Kallman, Tsuneyoshi Kamae, Jun Kataoka, Satoru Katsuda, Nobuyuki Kawai, Richard L. Kelley, Caroline A. Kilbourne, Takao Kitaguchi, Shunji Kitamoto, Tetsu Kitayama, Takayoshi Kohmura, Motohide Kokubun, Katsuji Koyama, Shu Koyama, Peter Kretschmar, Hans A. Krimm, Aya Kubota, Hideyo Kunieda, Philippe Laurent, L. E.E. Shiu-Hang, Maurice A. Leutenegger, Olivier O. Limousin, Michael Loewenstein, Knox S. Long, David Lumb, Greg Madejski, Yoshitomo Maeda, Daniel Maier, Kazuo Makishima, Maxim Markevitch, Hironori Matsumoto, Kyoko Matsushita, Dan McCammon, Brian R. McNamara, Missagh Mehdipour, Eric D. Miller, Jon M. Miller, Shin Mineshige, Publications of the Astronomical Society of Japan, Publications of the Astronomical Society of Japan, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psx083
  • Atmospheric gas dynamics in the Perseus cluster observed with Hitomi, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psx138
  • Temperature structure in the Perseus cluster core observed with Hitomi, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psy004
  • Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psx127
  • Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psx151
  • Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psx156
  • In-orbit performance of the soft X-ray imaging system aboard Hitomi (ASTRO-H), Nakajima Hiroshi, Maeda Yoshitomo, Uchida Hiroyuki, Tanaka Takaaki, Tsunemi Hiroshi, Hayashida Kiyoshi, Tsuru Takeshi G, Dotani Tadayasu, Nagino Ryo, Inoue Shota, Ozaki Masanobu, Tomida Hiroshi, Natsukari Chikara, Ueda Shutaro, Mori Koji, Yamauchi Makoto, Hatsukade Isamu, Nishioka Yusuke, Sakata Miho, Beppu Tatsuhiko, Honda Daigo, Nobukawa Masayoshi, Hiraga Junko S, Kohmura Takayoshi, Murakami Hiroshi, Nobukawa, Kumiko K, Bamba Aya, Doty John P, Iizuka Ryo, Sato Toshiki, Kurashima Sho, Nakaniwa Nozomi, Asai Ryota, Ishida Manadu, Mori Hideyuki, Soong Yang, Okajima Takashi, Serlemitsos Peter, Tawara Yuzuru, Mitsuishi Ikuyuki, Ishibashi Kazunori, Tamura Keisuke, Hayashi Takayuki, Furuzawa Akihiro, Sugita Satoshi, Miyazawa Takuya, Awaki Hisamitsu, Miller Eric D, Yamaguchi Hiroya, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2018年03月, [査読有り], 0004-6264, 10.1093/pasj/psx116
  • Suzaku Observations of Heavily Obscured (Compton-thick) Active Galactic Nuclei Selected by the Swift/BAT Hard X-Ray Survey, The Astrophysical Journal, The Astrophysical Journal, 2018年02月, [査読有り]
  • Sub-arcsecond Imaging with Multi Image X-ray Interferometer Module (MIXIM) for Very Small Satellites, Hayashida Kiyoshi, Kawabata Tomoki, Hanasaka Takashi, Asakura Kazunori, Yoneyama Tomokage, Okazaki Koki, Ide Shuntaro, Matsumoto Hironori, Nakajima Hiroshi, Awaki Hisamitsu, Tsunemi Hiroshi, SPACE TELESCOPES AND INSTRUMENTATION 2018: ULTRAVIOLET TO GAMMA RAY, SPACE TELESCOPES AND INSTRUMENTATION 2018: ULTRAVIOLET TO GAMMA RAY, 2018年, 0277-786X, 10.1117/12.2314181
  • Concept of X-ray Astronomy Recovery Mission, SPACE TELESCOPES AND INSTRUMENTATION 2018: ULTRAVIOLET TO GAMMA RAY, SPACE TELESCOPES AND INSTRUMENTATION 2018: ULTRAVIOLET TO GAMMA RAY, 2018年, 0277-786X, 10.1117/12.2309455
  • Supermirror design for Hard X-Ray Telescopes on-board Hitomi (ASTRO-H), Journal of Astronomical Telescopes, Instruments, and Systems, Journal of Astronomical Telescopes, Instruments, and Systems, 2018年01月, [査読有り]
  • On-ground calibration of the Hitomi Hard X-ray Telescopes, Journal of Astronomical Telescopes, Instruments, and Systems, Journal of Astronomical Telescopes, Instruments, and Systems, 2018年01月, [査読有り]
  • Inorbit performance of the Hard X-ray Telescope (HXT) on board the Hitomi (ASTRO-H) satellite, 松本浩典, 粟木久光, Journal of Astronomical Telescopes, Instruments, and Systems, Journal of Astronomical Telescopes, Instruments, and Systems, 2018年01月, [査読有り]
  • Solar abundance ratios of the iron-peak elements in the Perseus cluster, Nature, Nature, 2017年11月, [査読有り]
  • Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster, Astrophysical Journal Letters, Astrophysical Journal Letters, 2017年, [査読有り]
  • The nature of the torus in the heavily obscured AGN Markarian 3: an X-ray study, M. Guainazzi, G. Risaliti, H. Awaki, P. Arevalo, F. E. Bauer, S. Bianchi, S. E. Boggs, W. N. Brandt, M. Brightman, F. E. Christensen, W. W. Craig, K. Forster, C. J. Hailey, F. Harrison, M. Koss, A. Longinotti, C. Markwardt, A. Marinucci, G. Matt, C. S. Reynolds, C. Ricci, D. Stern, J. Svoboda, D. Walton, W. Zhang, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016年08月, [査読有り], 0035-8711, 10.1093/mnras/stw1033
  • The quiescent intracluster medium in the core of the Perseus cluster, Felix Aharonian, Hiroki Akamatsu, Fumie Akimoto, Steven W. Allen, Naohisa Anabuki, Lorella Angelini, Keith Arnaud, Marc Audard, Hisamitsu Awaki, Magnus Axelsson, Aya Bamba, Marshall Bautz, Roger Blandford, Laura Brenneman, Gregory V. Brown, Esra Bulbul, Edward Cackett, Maria Chernyakova, Meng Chiao, Paolo Coppi, Elisa Costantini, Jelle de Plaa, Jan-Willem den Herder, Chris Done, Tadayasu Dotani, Ken Ebisawa, Megan Eckart, Teruaki Enoto, Yuichiro Ezoe, Andrew C. Fabian, Carlo Ferrigno, Adam Foster, Ryuichi Fujimoto, Yasushi Fukazawa, Akihiro Furuzawa, Massimiliano Galeazzi, Luigi Gallo, Poshak Gandhi, Margherita Giustini, Andrea Goldwurm, Liyi Gu, Matteo Guainazzi, Yoshito Haba, Kouichi Hagino, Kenji Hamaguchi, Ilana Harrus, Isamu Hatsukade, Katsuhiro Hayashi, Takayuki Hayashi, Kiyoshi Hayashida, Junko Hiraga, Ann Hornschemeier, Akio Hoshino, John Hughes, Ryo Iizuka, Hajime Inoue, Yoshiyuki Inoue, Kazunori Ishibashi, Manabu Ishida, Kumi Ishikawa, Yoshitaka Ishisaki, Masayuki Itoh, Naoko Iyomoto, Jelle Kaastra, Timothy Kallman, Tuneyoshi Kamae, Erin Kara, Jun Kataoka, Satoru Katsuda, Junichiro Katsuta, Madoka Kawaharada, Nobuyuki Kawai, Richard Kelley, Dmitry Khangulyan, Caroline Kilbourne, Ashley King, Takao Kitaguchi, Shunji Kitamoto, Tetsu Kitayama, Takayoshi Kohmura, Motohide Kokubun, Shu Koyama, Katsuji Koyama, Peter Kretschmar, Hans Krimm, Aya Kubota, Hideyo Kunieda, Philippe Laurent, Francois Lebrun, Shiu-Hang Lee, Maurice Leutenegger, Olivier Limousin, Michael Loewenstein, Knox S. Long, David Lumb, Grzegorz Madejski, Yoshitomo Maeda, Daniel Maier, Kazuo Makishima, Maxim Markevitch, Hironori Matsumoto, Kyoko Matsushita, Dan McCammon, Brian McNamara, Missagh Mehdipour, Eric Miller, Jon Miller, Shin Mineshige, Kazuhisa Mitsuda, Ikuyuki Mitsuishi, Takuya Miyazawa, Tsunefumi Mizuno, Hideyuki Mori, Koji Mori, Harvey Moseley, Koji Mukai, Hiroshi Murakami, Toshio Murakami, Richard Mushotzky, Ryo Nagino, Takao Nakagawa, Hiroshi Nakajima, Takeshi Nakamori, Toshio Nakano, Shinya Nakashima, Kazuhiro Nakazawa, Masayoshi Nobukawa, Hirofumi Noda, Masaharu Nomachi, Steve O'Dell, Hirokazu Odaka, Takaya Ohashi, Masanori Ohno, Takashi Okajima, Naomi Ota, Masanobu Ozaki, Frits Paerels, Stephane Paltani, Arvind Parmar, Robert Petre, Ciro Pinto, Martin Pohl, F. Scott Porter, Katja Pottschmidt, Brian Ramsey, Christopher Reynolds, Helen Russell, Samar Safi-Harb, Shinya Saito, Kazuhiro Sakai, Hiroaki Sameshima, Goro Sato, Kosuke Sato, Rie Sato, Makoto Sawada, Norbert Schartel, Peter Serlemitsos, Hiromi Seta, Megumi Shidatsu, Aurora Simionescu, Randall Smith, Yang Soong, Lukasz Stawarz, Yasuharu Sugawara, Satoshi Sugita, Andrew Szymkowiak, Hiroyasu Tajima, Hiromitsu Takahashi, Tadayuki Takahashi, Shin'ichiro Takeda, Yoh Takei, Toru Tamagawa, Keisuke Tamura, Takayuki Tamura, Takaaki Tanaka, Yasuo Tanaka, Yasuyuki Tanaka, Makoto Tashiro, Yuzuru Tawara, Yukikatsu Terada, Yuichi Terashima, Francesco Tombesi, Hiroshi Tomida, Yohko Tsuboi, Masahiro Tsujimoto, Hiroshi Tsunemi, Takeshi Tsuru, Hiroyuki Uchida, Hideki Uchiyama, Yasunobu Uchiyama, Shutaro Ueda, Yoshihiro Ueda, Shiro Ueno, Shin'ichiro Uno, Meg Urry, Eugenio Ursino, Cor De Vries, Shin Watanabe, Norbert Werner, Daniel Wik, Dan Wilkins, Brian Williams, Shinya Yamada, Hiroya Yamaguchi, Kazutaka Yamaoka, Noriko Y. Yamasaki, Makoto Yamauchi, Shigeo Yamauchi, Tahir Yaqoob, Yoichi Yatsu, Daisuke Yonetoku, Atsumasa Yoshida, Takayuki Yuasa, Irina Zhuravleva, Abderahmen Zoghbi, NATURE, NATURE, 2016年07月, [査読有り], 0028-0836, 10.1038/nature18627
  • Studies of print-through and reflectivity of x-ray mirrors using thin carbon-fiber-reinforced plastic, Satoshi Sugita, Hisamitsu Awaki, Kenya Yoshioka, Keiji Ogi, Hideyo Kunieda, Hironori Matsumoto, Takuya Miyazawa, Ikuyuki Mitsuishi, Toshihiro Iwase, Shigetaka Saji, Sasagu Tachibana, Masato Maejima, Shun Yoshikawa, Naoki Shima, Takashi Ishikawa, Takayoshi Hamada, Naoki Ishida, Hiromichi Akiyama, Kazuaki Kishimoto, Shin Utsunomiya, Tomohiro Kamiya, Kentaro Uesugi, Yoshio Suzuki, Journal of Astronomical Telescopes, Instruments, and Systems, Journal of Astronomical Telescopes, Instruments, and Systems, 2016年01月, [査読有り], 2329-4124, 10.1117/1.JATIS.2.1.014002
  • A NEW SAMPLE OF OBSCURED AGNs SELECTED FROM THE XMM-NEWTON AND AKARI SURVEYS, Yuichi Terashima, Yoshitaka Hirata, Hisamitsu Awaki, Shinki Oyabu, Poshak Gandhi, Yoshiki Toba, Hideo Matsuhara, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2015年11月, [査読有り], 0004-637X, 10.1088/0004-637X/814/1/11
  • Studies of the moisture absorption of thin carbon fiber reinforced plastic substrates for x-ray mirrors, Satoshi Sugita, Hisamitsu Awaki, Daichi Kurihara, Kenya Yoshioka, Mizuki Nomura, Keiji Ogi, Yuuki Tomita, Tomoki Mita, Hideyo Kunieda, Hironori Matsumoto, Takuya Miyazawa, Ikuyuki Mitsuishi, Toshihiro Iwase, Masato Maejima, Naoki Shima, Takashi Ishikawa, Takayoshi Hamada, Naoki Ishida, Hiromichi Akiyama, Kazuaki Kishimoto, Shin Utsunomiya, Tomohiro Kamiya, Journal of Astronomical Telescopes, Instruments, and Systems, Journal of Astronomical Telescopes, Instruments, and Systems, 2015年, [査読有り], 2329-4124, 10.1117/1.JATIS.1.3.034003
  • Hard x-ray telescopes to be onboard ASTRO-H, Hisamitsu Awaki, Hideyo Kunieda, Manabu Ishida, Hironori Matsumoto, Yasunori Babazaki, Tadatsugu Demoto, Akihiro Furuzawa, Yoshito Haba, Takayuki Hayashi, Ryo Iizuka, Kazunori Ishibashi, Naoki Ishida, Masayuki Itoh, Toshihiro Iwase, Tatsuro Kosaka, Daichi Kurihara, Yuuji Kuroda, Yoshitomo Maeda, Yoshifumi Meshino, Ikuyuki Mitsuishi, Yuusuke Miyata, Takuya Miyazawa, Hideyuki Mori, Housei Nagano, Yoshiharu Namba, Yasushi Ogasaka, Keiji Ogi, Takashi Okajima, Shigetaka Saji, Fumiya Shimasaki, Takuro Sato, Toshiki Sato, Satoshi Sugita, Yoshio Suzuki, Kenji Tachibana, Sasagu Tachibana, Shunya Takizawa, Keisuke Tamura, Yuzuru Tawara, Tatsuharu Torii, Kentato Uesugi, Koujun Yamashita, Shigeo Yamauchi, Applied Optics, Applied Optics, 2014年11月, [査読有り], 1559-128X, 10.1364/AO.53.007664
  • Iron Kα emission in type-I and type-II active galactic nuclei, Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, 2014年07月, [査読有り], 0035-8711, 10.1093/mnras/stu735
  • The narrow Fe Kα line and the molecular torus in active galactic nuclei: an IR/X-ray view, Astronomy & Astrophysics, Astronomy & Astrophysics, 2014年07月, [査読有り], 1432-0746, 10.1051/0004-6361/201322701
  • On the role of the Γ - λEdd relation on the X-ray Baldwin effect in active galactic nuclei, Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, 2013年11月, [査読有り], 0035-8711, 10.1093/mnras/stt1326
  • Luminosity-dependent unification of active galactic nuclei and the X-ray Baldwin effect, C. Ricci, S. Paltani, H. Awaki, P. -O. Petrucci, Y. Ueda, M. Brightman, ASTRONOMY & ASTROPHYSICS, ASTRONOMY & ASTROPHYSICS, 2013年05月, [査読有り], 1432-0746, 10.1051/0004-6361/201220324
  • A NEW SAMPLE OF CANDIDATE INTERMEDIATE-MASS BLACK HOLES SELECTED BY X-RAY VARIABILITY, Naoya Kamizasa, Yuichi Terashima, Hisamitsu Awaki, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2012年05月, [査読有り], 0004-637X, 10.1088/0004-637X/751/1/39
  • A Candidate Active Galactic Nucleus with a Pure Soft Thermal X-Ray Spectrum, Astrophys. J., Astrophys. J., 2012年, [査読有り], 10.1088/0004-637X/752/2/154
  • SUZAKU VIEW OF THE SWIFT/BAT ACTIVE GALACTIC NUCLEI. III. APPLICATION OF NUMERICAL TORUS MODELS TO TWO NEARLY COMPTON THICK ACTIVE GALACTIC NUCLEI (NGC 612 AND NGC 3081), Satoshi Eguchi, Yoshihiro Ueda, Hisamitsu Awaki, James Aird, Yuichi Terashima, Richard Mushotzky, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2011年03月, [査読有り], 0004-637X, 10.1088/0004-637X/729/1/31
  • SUZAKU OBSERVATION OF GRS 1915+105: EVOLUTION OF ACCRETION DISK STRUCTURE DURING LIMIT-CYCLE OSCILLATION, Y. Ueda, K. Honda, H. Takahashi, C. Done, H. Shirai, Y. Fukazawa, K. Yamaoka, S. Naik, H. Awaki, K. Ebisawa, J. Rodriguez, S. Chaty, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2010年04月, [査読有り], 0004-637X, 10.1088/0004-637X/713/1/257
  • SCATTERED X-RAYS IN OBSCURED ACTIVE GALACTIC NUCLEI AND THEIR IMPLICATIONS FOR GEOMETRICAL STRUCTURE AND EVOLUTION, Kazuhisa Noguchi, Yuichi Terashima, Yukiko Ishino, Yasuhiro Hashimoto, Michael Koss, Yoshihiro Ueda, Hisamitsu Awaki, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2010年03月, [査読有り], 0004-637X, 10.1088/0004-637X/711/1/144
  • A NEW SAMPLE OF BURIED ACTIVE GALACTIC NUCLEI SELECTED FROM THE SECOND XMM-NEWTON SERENDIPITOUS SOURCE CATALOGUE, Kazuhisa Noguchi, Yuichi Terashima, Hisamitsu Awaki, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2009年11月, [査読有り], 0004-637X, 10.1088/0004-637X/705/1/454
  • Suzaku observation of the Phoenix galaxy, G. Matt, S. Bianchi, H. Awaki, A. Comastri, M. Guainazzi, K. Iwasawa, E. Jimenez-Bailon, F. Nicastro, ASTRONOMY & ASTROPHYSICS, ASTRONOMY & ASTROPHYSICS, 2009年03月, [査読有り], 1432-0746, 10.1051/0004-6361/200811049
  • Study on X-Ray Spectra of Obscured Active Galactic Nuclei Based on Monte Carlo Simulation—An Interpretation of Observed Wide-Band Spectra, Astrophys. J., Astrophys. J., 2009年02月, [査読有り], 0004-637X, 10.1088/0004-637X/692/1/608
  • Detection of Hard X-Rays from the Compton-Thick Seyfert 2 Galaxy NGC 2273 with Suzaku, Publ.Astron. Soc. Japan, Publ.Astron. Soc. Japan, 2009年, [査読有り]
  • Suzaku observation of HCG 62: Temperature, abundance, and extended hard X-ray emission profiles, Kazuyo Tokoi, Kosuke Sato, Yoshitaka Ishisaki, Takaya Ohashi, Noriko Y. Yamasaki, Kazuhiro Nakazawa, Kyoko Matsushita, Yasushi Fukazawa, Akio Hoshino, Takayuki Tamura, Chihiro Egawa, Naomi Kawano, Naomi Ota, Naoki Isobe, Madoka Kawaharada, Hisamitsu Awaki, John P. Hughes, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2008年02月, [査読有り], 0004-6264, 10.1093/pasj/60.sp1.S317
  • Wide-band spectroscopy of the Compton thick Seyfert 2 galaxy Markarian 3 with Suzaku, Hisamitsu Awaki, Naohisa Anabuki, Yasushi Fukazawa, Luigi C. Gallo, Shinya Ikeda, Naoki Isobe, Takeshi Itoh, Hideyo Kunieda, Kazuo Makishima, Alex Markowitz, Giovanni Miniutti, Tsunefumi Mizuno, Takashi Okajima, Andrew Ptak, James N. Reeves, Tadayuki Takahashi, Yuichi Terashima, Tahir Yaqoob, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2008年02月, [査読有り], 0004-6264, 10.1093/pasj/60.sp1.S293
  • The Suzaku observation of NGC 3516: Complex absorption and the broad and narrow FeK lines, Alex Markowitz, James N. Reeves, Giovanni Miniutti, Peter Serlemitsos, Hideyo Kunieda, Tahir Yaqoob, Andrew C. Fabian, Yasushi Fukazawa, Richard Mushotzky, Takashi Okajima, Luigi C. Gallo, Hisamitsu Awaki, Richard E. Griffiths, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2008年02月, [査読有り], 0004-6264, 10.1093/pasj/60.sp1.S277
  • Detailed hard X-ray measurements of nuclear emission from the Seyfert 2 galaxy NGC 4388 with Suzaku, Hirohisa Shirai, Yasushi Fukazawa, Mahito Sasada, Masanori Ohno, Daisuke Yonetoku, Satoshi Yokota, Ryuichi Fujimoto, Toshio Murakami, Yuichi Terashima, Hisamitsu Awaki, Shinya Ikeda, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2008年02月, [査読有り], 0004-6264, 10.1093/pasj/60.sp1.S263
  • Suzaku wide-band X-ray spectroscopy of the Seyfert 2 AGN in NGC 4945, Takeshi Itoh, Chris Done, Kazuo Makishima, Grzegorz Madejski, Hisamitsu Awaki, Poshak Gandhi, Naoki Isobe, Gulab C. Dewangan, Richard E. Griffthis, Naohisa Anabuki, Takashi Okajima, James N. Reeves, Tadayuki Takahashi, Yoshihiro Ueda, Satohi Eguchi, Tahir Yaqoob, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2008年02月, [査読有り], 0004-6264, 10.1093/pasj/60.sp1.S251
  • X-ray study of discrete sources in NGC 1808 with Chandra, Kazunori Heike, Hisamitsu Awaki, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2007年06月, [査読有り], 0004-6264, 10.1093/pasj/59.3.531
  • The Suzaku Observation of the Nucleus of the Radio-Loud Active Galaxy Centaurus A: Constraints on Abundances of the Accreting Material, A. Markowitz, T. Takahashi, S. Watanabe, K. Nakazawa, Y. Fukazawa, M. Kokubun, K. Makishima, H. Awaki, A. Bamba, N. Isobe, J. Kataoka, G. Madejski, R. Mushotzky, T. Okajima, A. Ptak, J. N. Reeves, Y. Ueda, T. Yamasaki, T. Yaqoob, Astrophys.J.665:209-224,2007, Astrophys.J.665:209-224,2007, 2007年04月, 10.1086/519271
  • X-Ray Spectral Study of the Extended Emission, `the Cap', Located 11.6kpc above the Disk of M82, Publ. Astron. Soc. Japan letters, Publ. Astron. Soc. Japan letters, 2007年, [査読有り]
  • X-Ray Imaging Spectrometer (XIS) on Board Suzaku, Publ.Astron. Soc. Japan, Publ.Astron. Soc. Japan, 2007年, [査読有り]
  • The X-Ray Observatory Suzaku, Publ. Astron. Soc. Japan letters, Publ. Astron. Soc. Japan letters, 2007年, [査読有り]
  • In-flight status of the X-ray observatory Suzaku, T. Dotani, K. Mitsuda, M. Bautz, H. Inoue, R. L. Kelley, K. Koyama, H. Kunieda, K. Makishima, Y. Ogawara, R. Petre, T. Takahashi, H. Tsunemi, N. E. White, N. Anabuki, L. Angelini, K. Arnaud, H. Awaki, A. Bamba, K. Boyce, G. V. Brown, K. -W. Chan, J. Cottam, J. Doty, K. Ebisawa, Y. Ezoe, A. C. Fabian, E. Figueroa, R. Fujimoto, Y. Fukazawa, T. Furusho, A. Furuzawa, K. Gendreau, R. E. Griffiths, Y. Haba, K. Hamaguchi, l. Harrus, G. Hasinger, I. Hatsukade, K. Hayashida, P. J. Henry, J. S. Hiraga, S. S. Holt, A. Hornschemeier, J. P. Hughes, U. Hwang, M. Ishida, Y. Ishisaki, N. Isobe, M. Itoh, N. Iyomoto, S. M. Kahn, T. Kamae, H. Katagiri, J. Kataoka, H. Katayama, N. Kawai, M. Kawaharada, C. Kilbourne, K. Kinugasa, S. Kissel, S. Kitamoto, M. Kohama, T. Kohmura, M. Kokubun, T. Kotani, J. Kotoku, A. Kubota, G. M. Madejski, Y. Maeda, F. Makino, A. Markowitz, C. Matsumoto, H. Matsumoto, M. Matsuoka, K. Matsushita, D. McCammon, T. Mihara, K. Misaki, E. Miyata, T. Mizuno, K. Mori, H. Mori, M. Morii, H. Moseley, K. Mukai, H. Murakami, T. Murakami, R. Mushotzky, F. Nagase, M. Namiki, H. Negoro, K. Nakazawa, J. A. Nousek, T. Okajima, Y. Ogasaka, T. Ohashi, T. Oshima, N. Ota, M. Ozaki, H. Ozawa, A. N. Parmar, W. D. Pence, F. Scott Porter, J. N. Reeves, G. R. Ricker, L. Sakurai, W. T. Sanders, A. Senda, P. Serlemitsos, R. Shibata, K. Shinozaki, Y. Soong, R. Smith, M. Suzuki, A. E. Szymkowiak, H. Takahashi, Y. Takei, T. Tamagawa, K. Tamura, T. Tamura, Y. Tanaka, M. Tashiro, Y. Tawara, Y. Terada, Y. Terashima, H. Tomida, K. Torii, Y. Tsuboi, Y. Tsujimoto, T. Tsuru, M. J. L. Turner, Y. Uchiyama, Y. Ueda, S. Ueno, M. Ueno, S. Uno, Y. Urata, S. Watanabe, N. Yamamoto, K. Yamaoka, N. Y. Yamasaki, K. Yamashita, M. Yamauchi, S. Yajmauchi, T. Yaqoob, D. Yonetoku, A. Yoshida, 2007 IEEE NUCLEAR SCIENCE SYMPOSIUM CONFERENCE RECORD, VOLS 1-11, 2007 IEEE NUCLEAR SCIENCE SYMPOSIUM CONFERENCE RECORD, VOLS 1-11, 2007年, [査読有り], 1082-3654, 10.1109/NSSMIC.2007.4436667
  • Variability study of Seyfert 2 galaxies with XMM-Newton, Hisamitsu Awaki, Hirokatsu Murakami, Yuu Ogawa, Karen M. Leighly, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2006年07月, [査読有り], 0004-637X, 10.1086/504405
  • A variability study of the Seyfert 2 galaxy NGC 6300 with XMM-Newton, H Awaki, H Murakami, KM Leighly, C Matsumoto, K Hayashida, D Grupe, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2005年10月, [査読有り], 0004-637X, 10.1086/433161
  • The development of a back-illuminated supportless CCD for SXI onboard the NeXT satellite, TG Tsuru, S Takagi, H Matsumoto, T Inui, K Koyama, H Tsunemi, K Hayashida, E Miyata, T Dotani, M Ozaki, H Awaki, S Kitamoto, T Kohmura, NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2005年04月, [査読有り], 0168-9002, 10.1016/j.nima.2005.01.080
  • X-ray imaging spectrometers (XIS) of Astro-E2, H Matsumoto, K Koyama, TG Tsuru, H Nakajima, H Yamaguchi, H Tsunemi, K Hayashida, E Miyata, K Torii, M Namiki, T Dotani, M Ozaki, H Murakami, N Anabuki, S Kitamoto, H Awaki, T Kohmura, H Katayama, A Bamba, MW Bautz, JP Doty, GR Ricker, RF Foster, GY Prigozhin, SE Kissel, BE Burke, AD Pillsbury, B LaMarr, NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2005年04月, [査読有り], 0168-9002, 10.1016/j.nima.2005.01.076
  • Revealing the High Energy Emission from the Obscured Seyfert Galaxy MCG-5-23-16 with Suzaku, Publ. Astron. Soc. Japan,, Publ. Astron. Soc. Japan,, 2005年, [査読有り]
  • Deconstructing NGC 7130, NA Levenson, KA Weaver, TM Heckman, H Awaki, Y Terashima, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2005年01月, [査読有り], 0004-637X, 10.1086/425913
  • An XMM-Newton observation of the Seyfert 2 galaxy NGC 6300. I. The nucleus, C Matsumoto, A Nava, LA Maddox, KM Leighly, D Grupe, H Awaki, S Ueno, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2004年12月, [査読有り], 0004-637X, 10.1086/425566
  • Accretion and outflow in the active galactic nucleus and starburst of NGC 5135, NA Levenson, KA Weaver, TM Heckman, H Awaki, Y Terashima, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2004年02月, [査読有り], 0004-637X, 10.1086/380836
  • ASCA observation of unusually X-ray-hard radio-quiet QSO Kaz 102, T Miyaji, Y Ishisaki, Y Ueda, Y Ogasaka, H Awaki, K Hayashida, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2003年04月, [査読有り], 0004-6264, 10.1093/pasj/55.2.L11
  • Discovery of Bright Variable X-ray Sources in NGC1569 with Chandra, K. Heike, H. Awaki, Y. Misao, K. Hayashida, K.A.Weaver, The Astrophysical Journal, The Astrophysical Journal, 2003年, [査読有り], 10.1086/377090
  • X-ray emission from a merger remnant, NGC 7252 (the "atoms-for-peace" galaxy), H Awaki, H Matsumoto, H Tomida, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2002年03月, [査読有り], 0004-637X, 10.1086/338694
  • A novel method to estimate the thickness of the deplation layer of an X-ray CCD, H. Awaki, K. Tachibana, Y. Tamai, K. Yamamoto, S. Kitamoto, M. Tsujimoto, Nuclear Instruments & Methods in Physics Research, Nuclear Instruments & Methods in Physics Research, 2002年, [査読有り], 10.1016/S0168-9002(02)01612-1
  • Extreme X-Ray Iron Lines in Active Galactic Nuclei, N.A. Levenson, J.H. Krolik, P.T. Zycki, T.M. Heckma, K.A. Weaver, H. Awaki, Y. Terashima, Astrophysical Journal, Astrophysical Journal, 2002年, [査読有り], 10.1086/342092
  • Estimation of Central Black Hole Masses in Low-luminosity Active Galactic Nuclei, H. Awaki, Y. Terashima, K. Hayashida, M. Sakano, Publication of the Astronomical Society of Japan, Publication of the Astronomical Society of Japan, 2001年, [査読有り]
  • Discovery of a Luminous, Variable, Off-Center Source in the Nucleus of M82 with the Chandra High-Resolution Camera, H. Matsumoto, T.G. Tsuru, K. Koyama, H. Awaki, C.R. Canizares, N. Kawai, S. Matsushita, R. Kawabe, Astrophysical Journal Letter, Astrophysical Journal Letter, 2001年, [査読有り], 10.1086/318878
  • X-ray emission from Seyfert 2 galaxies with optical polarized broad lines, H Awaki, S Ueno, Y Taniguchi, KA Weaver, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2000年10月, [査読有り], 0004-637X
  • A search for broad infrared recombination lines in NGC 1068, D Lutz, R Genzel, E Sturm, L Tacconi, E Wieprecht, T Alexander, H Netzer, A Sternberg, AFM Moorwood, RAE Fosbury, K Fricke, SJ Wagner, A Quirrenbach, H Awaki, KY Lo, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 2000年02月, [査読有り], 0004-637X
  • X-ray CCD calibration system using fluorescent lines, NIMPA, NIMPA, 2000年, [査読有り], 10.1016/S0168-9002(00)00306-5
  • The hard X-ray response of the XIS-CCD for Astro-E: qualification of the X-ray CCD detector, M Nishiuchi, K Koyama, H Awaki, T Tsuru, M Sakano, K Hamaguchi, H Murakami, H Tsunemi, K Hayashida, S Kitamoto, E Miyata, T Dotani, M Ozaki, M Bautz, J Doty, S Kissel, R Foster, G Ricker, NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1999年10月, 0168-9002, 10.1016/S0168-9002(99)00601-4
  • An RXTE observation of NGC 6300: A new bright compton reflection-dominated Seyfert 2 galaxy, KM Leighly, JP Halpern, H Awaki, M Cappi, S Ueno, J Siebert, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 1999年09月, [査読有り], 0004-637X
  • Development of a fast56- readout system of an X-ray CCD, AWAKI H, HAMAGUCHI K, KOYAMA K, TOMIDA H, TSURU T, Nuclear Instruments & Methods in Physics Research, Nuclear Instruments & Methods in Physics Research, 1999年, 0168-9002, 10.1016/S0168-9002(99)00616-6
  • Broad Band X-ray Observations of Seyfert 2 Galaxy NGC 5506, T. Wang, T. Mihara, C. Otani, M. Matsuoka, H. Awaki, Astrophysical Journal, Astrophysical Journal, 1999年, [査読有り]
  • The hardest X-ray source in the ASCA large sky survey: Discovery of a new type 2 Seyfert, M Sakano, K Koyama, T Tsuru, H Awaki, Y Ueda, T Takahashi, M Akiyama, K Ohta, T Yamada, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 1998年09月, [査読有り], 0004-637X, 10.1086/306158
  • NGC7582 : The Prototype Narrow-Line X-ray Galaxy, J.F. Schachter, F. Fiore, M. Elvis, S. Mathur, A.S. Wilson, J.A. Morse, H. Awaki, K. Iwasawa, Astrophysical Joural, Astrophysical Joural, 1998年, [査読有り]
  • On the nature of the X-ray absorption in the Seyfert 2 galaxy NGC 4507, A. Comastri, C. Vignali, M. Cappi, G. Matt, R. Audano, H. Awaki, S. Ueno, Monthly Notice Royal Astronomical Society., Monthly Notice Royal Astronomical Society., 1998年, [査読有り]
  • X-ray imaging spectroscopy of Stephan's Quintet and Seyfert 2 galaxy NGC 7319, H Awaki, K Koyama, H Matsumoto, H Tomida, T Tsuru, S Ueno, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1997年08月, [査読有り], 0004-6264, 10.1093/pasj/49.4.445
  • Radiation damage on X-ray CCDs and restoration technique for space astronomy, H Tomida, H Matsumoto, M Ozaki, Y Tazawa, H Awaki, T Tsuru, K Koyama, H Tsunemi, K Yamamoto, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1997年06月, [査読有り], 0004-6264, 10.1093/pasj/49.3.405
  • ASCA PV observations of the Seyfert 2 galaxy NGC 4388: The obscured nucleus and its X-ray emission, K Iwasawa, AC Fabian, S Ueno, H Awaki, Y Fukazawa, K Matsushita, K Makishima, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997年03月, [査読有り], 0035-8711
  • Wide-Band X-ray Spectra and Images of the Starburst Galaxy M82, T. Tsuru, H. Awaki, K. Koyama, A. Ptak, Publications of the Astonomical Society of Japan, Publications of the Astonomical Society of Japan, 1997年, [査読有り]
  • X-ray property of Early-type galaxies as observed with ASCA, H. Matsumoto, K. Koyama, H. Awaki, T. Tsuru, M. Loewenstein, K. Matsushita, Astrophysical Journal, Astrophysical Journal, 1997年, [査読有り], 10.1086/304132
  • ASCA observation of NGC 1808, H Awaki, S Ueno, K Koyama, T Tsuru, K Iwasawa, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1996年06月, [査読有り], 0004-6264, 10.1093/pasj/48.3.409
  • Detection of hard X-ray emission from Mkn 463, S Ueno, K Koyama, H Awaki, Hayashi, I, PR Blanco, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1996年06月, [査読有り], 0004-6264, 10.1093/pasj/48.3.389
  • X-ray observations of NGC 2110 with Ginga and ASCA, Hayashi, I, K Koyama, H Awaki, S Ueno, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1996年04月, [査読有り], 0004-6264, 10.1093/pasj/48.2.219
  • Discovery of an Abundance Gradient in the Central Region of the Virgo Cluster, H. Matsumoto, K. Koyama, H. Awaki, T. Tsuru, M. Loewenstein, K. Matsushita, Publication of Astronomical Society of Japan, Publication of Astronomical Society of Japan, 1996年, [査読有り]
  • AN IRAS-SELECTED SEYFERT-2 GALAXY IRAS-18325-5926 - THE X-RAY SOURCE AND NUCLEAR OBSCURATION, K IWASAWA, H KUNIEDA, Y TAWARA, H AWAKI, K KOYAMA, T MURAYAMA, Y TANIGUCHI, ASTRONOMICAL JOURNAL, ASTRONOMICAL JOURNAL, 1995年08月, [査読有り], 0004-6256
  • Characterization of the Advanced Satellite for Cosmology and Astrophysics X-ray telescope: preflight calibration and ray tracing, Appl. Opt., Appl. Opt., 1995年, [査読有り], 10.1364/AO.34.004848
  • The X-ray Telescope on board ASCA, P.J. Serlemitsos, L. Jalota, Yang Soong, H. Kunieda, Y. Tawara, Y. Tsusaka, H. Suzuki, Y. Sakima, T. Yamazaki, H. Yoshioka, A. Furuzawa, K. Yamashita, H. Awaki, M. Itoh, Y. Ogasaka, H. Honda, Y. Uchibori, Publication of Astronomical Society of Japan, Publication of Astronomical Society of Japan, 1995年, [査読有り]
  • ASCA observation of NGC4636 : dark matter and metallicity gradient, R.F. Mushotzky, M. Loewenstein, H. Awaki, K. Makishima, K. Matsushita, H. Matsumoto, Astrophysical Journal, Astrophysical Journal, 1994年, [査読有り]
  • Discovery and implications of very low metal abundarus in NGC1404 and NGC4374, M. Loewenstein, R.F. Mushotzky, T. Tamura, Y. Ikebe, K. Makishima, K. Matsushita, H. Awaki, P.J. Serlemitsos, Astrophysical Journal, Astrophysical Journal, 1994年, [査読有り]
  • Detections of hard X-ray emissions from bright early-type galaxies with ASCA, K. Matsushita, K. Makishima, H. Awaki, C.R. Canizares, A.C. Fabian, Y. Fukazawa, M. Loewenstein, H. Matsumoto, T. Mihara, R.F. Mushotzky, T. Ohashi, G.R. Ricker, P.J. Serlemitsos, T. Tsuru, Y. Tsusaka, T. Yamazaki, Astrophysical Journal, Astrophysical Journal, 1994年, [査読有り]
  • Evidence for X-ray flux and spectral modulation by obsorption in NGC6814.(]G0001[).The nature of the mos rapid variability, K. Leighly, H. Kunieda, Y. Tsusaka, H. Awaki, S. Tsuruta, Astrophysical Journal, Astrophysical Journal, 1994年, [査読有り]
  • ASCA Observation of Three Bright Early-Type Galaxies ; NGC4472, NGC4406, and NGC4636, H. Awaki, R. Mushotzky, T. Tsuru, A.C. Fabian, Y. Fukazawa, M. Loewenstein, K. Makishima, H. Matsumoto, K. Matsushita, T. Mihara, T. Ohashi, G.R. Ricker, P.J. Serlemitsos, Y. Tsusaka, T. Yamazaki, Publications of the Astronomical Society of Japan, Publications of the Astronomical Society of Japan, 1994年, [査読有り]
  • ASCA Observations of NGC 1068, S. Ueno, R.F.Mushotzky, K. Koyama, K. Iwasawa, H. Awaki, I. Hayashi, Publications of the Astronomical Society of Japan, Publications of the Astronomical Society of Japan, 1994年, [査読有り]
  • An ASCA Observation of the Seyfert 2 Galaxy Markarian 3, K. Iwasawa, T. Yaqoob, H. Awaki, Y. Ogasaka, Publications of the Astronomical Society of Japan, Publications of the Astronomical Society of Japan, 1994年, [査読有り]
  • SIMULTANEOUS GINGA AND IUE OBSERVATIONS OF THE SEYFERT-GALAXY NGC-3516, M KOLMAN, JP HALPERN, C MARTIN, H AWAKI, K KOYAMA, ASTROPHYSICAL JOURNAL, ASTROPHYSICAL JOURNAL, 1993年02月, [査読有り], 0004-637X
  • Thirty-meter X-ray pencil beam line at the Institute of Space and Astronautical Science, Jpn. J. Appl. Phys. 1, Regul. Pap. Short Notes, Jpn. J. Appl. Phys. 1, Regul. Pap. Short Notes, 1993年, [査読有り]
  • POSSIBLE X-RAY-EMISSION FROM A NEW SOUTHERN QSO HE 1029-1401, K IWASAWA, H KUNIEDA, H AWAKI, K KOYAMA, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1993年, [査読有り], 0004-6264
  • X-ray evidence for the Seyfert activity buried in an infrared galaxy, NGC4945, K. Iwasawa, K. Koyama, H. Awaki, H. Kunieda, K. Makishima, T. Tsuru, T. Ohashi, N.Nakai, Astrophysical Journal, Astrophysical Journal, 1993年, [査読有り]
  • Hard X-ray emission from a narrow-line radio galaxy IC5063 and obscured active nucleus, Astrophys. J. letter, Astrophys. J. letter, 1992年, [査読有り]
  • X-RAY OBSERVATIONS OF THE BROAD LINE RADIO GALAXY 3C-382 - VARIABILITY, AN IRON LINE AND SOFT-X-RAY EMISSION, JS KAASTRA, H KUNIEDA, H AWAKI, ASTRONOMY & ASTROPHYSICS, ASTRONOMY & ASTROPHYSICS, 1991年02月, [査読有り], 0004-6361
  • Discovery of large absorption in the X-ray spectrum of Seyfert 2 galaxy NGC 4507, Publ. Astron. Soc. Japan letters, Publ. Astron. Soc. Japan letters, 1991年, [査読有り]
  • X-ray continuum and evidence for an iron emission line from the quasar E1821+643, Astrophys. J., Astrophys. J., 1991年, [査読有り]
  • X-ray implications of a Unified Model of Seyfert Galaxies, H. Awaki, K. Koyama, H. Inoue, J. P. Halpern, Publications of the Astronomical Society of Japan, Publications of the Astronomical Society of Japan, 1991年, [査読有り]
  • Ginga observations of three X-ray luminous early-type galaxies : NGC4472, NGC4636, and NGC3998, H. Awaki, K. Koyama, H. Kunieda, T. Ohashi, S. Takano, Y. Tawara, Astrophysical Journal, Astrophysical Journal, 1991年, [査読有り]
  • RAPID VARIABILITY OF THE IRON FLUORESCENCE LINE FROM THE SEYFERT-1 GALAXY NGC6814, H KUNIEDA, TJ TURNER, H AWAKI, K KOYAMA, R MUSHOTZKY, Y TSUSAKA, NATURE, NATURE, 1990年06月, [査読有り], 0028-0836
  • Ginga observations of X-ray from the Seyfert 1 galaxy Markarian 509, Astrophysical Journal, Astrophysical Journal, 1990年, [査読有り]
  • X-ray evidence of an obscured nucleus in the type 2 Seyfert galaxy, Mkn3, H. Awaki, K. Koyama, H. Kunieda, Y. Tawara, Nature, Nature, 1990年, [査読有り], 10.1038/346544a0
  • LARGE-SCALE EXTENDED X-RAY-EMISSION FROM THE VIRGO CLUSTER OF GALAXIES, S TAKANO, H AWAKI, K KOYAMA, H KUNIEDA, Y TAWARA, S YAMAUCHI, K MAKISHIMA, T OHASHI, NATURE, NATURE, 1989年07月, [査読有り], 0028-0836, 10.1038/340289a0
  • Intense 6.7-keV iron line emission from the Galactic Centre, Nature, Nature, 1989年, [査読有り], 10.1038/339603a0
  • X-ray outburst of the quasar 3C 279, The Astrophys.J. Lett, The Astrophys.J. Lett, 1989年, [査読有り]
  • An intense iron line emission from NGC 1068, Publ. Astron. Soc. Jpn., Publ. Astron. Soc. Jpn., 1989年, [査読有り]
  • X-ray spectral study of M31 with Ginga, Publ. Astron. Soc. Jpn., Publ. Astron. Soc. Jpn., 1989年, [査読有り]
  • Discovery of 413.9-second X-ray pulsation from X 1722-36, Publ. Astron. Soc. Jpn., Publ. Astron. Soc. Jpn., 1989年, [査読有り]
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  • The Large Area Counter on Ginga, Publ. Astron. Soc. Jpn., Publ. Astron. Soc. Jpn., 1989年, [査読有り]

講演・口頭発表等

  • 可視光用2.5ミクロンピクセルCMOSセンサーによるX線偏光検出, 朝倉一統, 林田 清, 川端智樹, 花坂剛史, 米山友景, 岡崎貴樹, 井出峻太郎, 野田博文, 松本浩典, 常深 博, 粟木久光, 中嶋 大, 2019年03月
  • 多重像X線干渉計MIXIMの開発の現状–微小ピクセルサイズの効能とスケーラブルな計画立案–, 林田 清, 花坂剛史, 朝倉一統, 米山友景, 野田博文, 井出峻太郎, 岡崎貴樹, 石倉彩美, 服部兼吾, 松本浩典, 常深 博, 粟木久光, 中嶋 大, 日本天文学会2019年春季年会, 2019年03月
  • 炭素繊維強化プラスチック(CFRP)へのX線反射面形成法の開発 II, 粟木久光, 吉田鉄生, 相田 望, 松本浩典, 米山友景, 井出峻太郎, 三石郁之, 大塚康司, 清水貞行, 田村啓輔, 中澤知洋, 石田 学, 前田良知, 中庭 望, 日本天文学会2019年春季年会, 2019年03月
  • 硬X線集光偏光計X-Calibur気球実験の2018年フライトと将来計画, 田村啓輔, 高橋弘充, 内田和海, 深沢泰司, 水野恒史, 北口貴雄, 玉川 徹, 早藤麻美, 周 圓輝, 堤 まりな, 内山慶祐, 林田 清, 松本浩典, 常深 博, 榎戸輝揚, 前田良知, 石田 学, 斎藤芳隆, 宮澤 拓也, 粟木久光, 郡司修一, Krawczynski, H, Dowkontt, P, Abarr, Q, Errando, M, Rauch, B, Bose, R, Kislat, F, 岡島 崇, Lanzi, J, Stuchlik, D, Heatwole, S, Li, S, de Geronimo, G, Pearce, M, Kiss, M, Kushwah, R, Iyer, N. K, 日本物理学会第74回年次大会, 2019年03月
  • 硬X線偏光観測実験X-Caliburの2018-2019年気球フライトに向けた準備状況, 高橋弘充, 内田和海, 深沢泰司, 水野恒史, 北口貴雄, 玉川 徹, 早藤麻美, 周 圓輝, 堤まりな, 内山慶祐, 林田 清, 松本浩典, 常深 博, 榎戸輝揚, 田村啓輔, 前田 良知, 石田 学, 斎藤芳隆, 宮澤拓也, 粟木久光, 郡司修一, Krawczynski, H, Rauch, B, Errando, M, Bose, R, Dowkontt, P, Simburger, G, Braun, D, Abarr, Q, West, A, Lisalda, L, Guarino, V, Kislat, F, 岡島 崇, Stuchlik, D, Lanzi, J, Heatwole, S, Peterson, Z, McGee, J, Gadson, T, Pearce, M, Kiss, M, Iyer, N, Kushwah, R, Ryde, F, Stana, T, 日本天文学会2019年春季年会, 2019年03月
  • 南極周回気球による硬X線偏光観測実験X-Caliburの2021年将来フライトへ向けて, 田村啓輔, 高橋弘充, 内田和海, 深沢泰司, 水野恒史, 北口貴雄, 玉川 徹, 早藤麻美, 周 圓輝, 堤 まりな, 内山慶祐, 林田 清, 松本 浩典, 常深 博, 榎戸輝揚, 前田良知, 石田 学, 斎藤芳隆, 宮澤 拓也, 粟木久光, 郡司修一, Krawczynski, H, Rauch, B, Errando, M, Bose, R, Dowkontt, P, Simburger, G, Braun, D, Abarr, Q, West, A, Lisalda, L, Guarino, V, Kislat, F, 岡島 崇, Stuchlik, D, Lanzi, J, Heatwole, S, Peterson, Z, McGee, J, Gadson, T, Pearce, M, Kiss, M, Iyer, N, Kushwah, R, Ryde, F, Stana, T, 2019年03月
  • X線分光撮像衛星XRISM搭載Resolveの開発の現状 III, Ishisaki, Y, Kelley, R. L, Akamatsu, H, Awaki, H, Bialas, T. G, Brown, G.V, Chiao, M, Costantini, E, den Herder, J.-W, Dipirro, M.J, Eckart, M. E, Ezoe, Y, Ferrigno, C, Fujimoto, R, Furuzawa, A, Graham, S. M, Grim, M, Hayashi, T, Horiuchi, T, Hoshino, A, Ichinohe, Y, Iizuka, R, Ishibashi, K, Ishida, M, Ishikawa, K, Kilbourne, C. A, Kitamoto, S, Koyama, S, Leutenegger, M. A, Maeda, Y, McCammon, D, Mitsuishi, I, Mori, H, Nakashima, S, Ohashi, T, Okajima, T, Paltani, S, Porter, F. S, Sato, K, Sawada, M, Seta, H, Shibano, Y, Shirron, P. J, Sneiderman, G.A, Soong, Y, Szymkowiak, A. E, Takei, Y, Tamagawa, T, Tsujimoto, M, de Vries, C. P, Yamada, S, Yamasaki, N. Y, Yasuda, S, Yoshioka, N, 2019年03月
  • 小型衛星計画 FORCE 用の X 線反射鏡開発の現状, 松本浩典, 粟木久光, 田村啓輔, 岡島 崇, 森 英之, 森 浩二, 武田彩希, 村上弘志, 寺田幸功, 中島真也, 久保田あや, 馬場 彩, 小高裕和, 谷津陽一, 幸村孝由, 萩野浩一, 小林翔悟, 内山泰伸, 北山 哲, 高橋忠幸, 石田 学, 渡辺 伸, 飯塚 亮, 山口弘悦, 中嶋 大, 中澤知洋, 古澤彰浩, 鶴 剛, 上田佳宏, 田中孝明, 内田裕之, 常深 博, 伊藤真之, 信川正順, 太田直美, 寺島雄一, 深沢泰司, 水野恒史, 高橋弘充, 大野雅功, 他, FORCE WG, 日本天文学会2019年春季年会, 2019年03月
  • 軟X線から硬X線の広帯域を高感度で撮像分光する小型衛星計画FORCEの現状(8), 森 浩二, 武田彩希, 村上弘志, 寺田幸功, 中島真也, 久保田あや, 馬場 彩, 小高裕和, 谷津陽一, 幸村孝由, 萩野浩一, 小林翔悟, 内山泰伸, 北山 哲, 高橋忠幸, 石田 学, 渡辺 伸, 飯塚 亮, 山口弘悦, 中嶋 大, 中澤知洋, 古澤彰浩, 鶴 剛, 上田佳宏, 田中孝明, 内田裕之, 松本浩典, 常深 博, 伊藤真之, 信川正順, 太田直美, 粟木久光, 寺島雄一, 深沢泰司, 水野恒史, 高橋弘充, 大野雅功, 岡島 崇, 森 英之, 他FORCE WG, 日本天文学会2019年春季年会, 2019年03月
  • 可視光用微小ピクセルCMOS検出器によるX線偏光検出, 朝倉一統, 林田 清, 川端智樹, 花坂剛史, 米山友景, 岡崎貴樹, 井出峻太, 郎, 野田博文, 松本浩典, 常深 博, 粟木久光, 中嶋 大, 第19回宇宙科学シンポジウム, 2019年01月, 招待有り
  • 多重像X線干渉計の開発:サブ秒角の撮像達成とスケーラブルなミッション計画, 林田 清, 花坂剛史, 朝倉一統, 米山友景, 岡崎貴樹, 井出 峻太郎, 川端智樹, 野田博文, 石倉彩美, 服部兼吾, 松本浩典, 常深 博, 中嶋 大, 粟木久光, 第19回宇宙科学シンポジウム, 2019年01月
  • レプリカ法に変わるCFRP上でのX線反射面形成法, 粟木久光, 松本浩典, 三石郁之, 相田 望, 吉田鉄生, 中澤知洋, 大塚康司, 清水貞行, 米山友景, 井出峻太郎, 石田 学, 前田良知, 中庭 望, 第19回宇宙科学シンポジウム, 2019年01月
  • 硬X線集光偏光計X-Calibur気球実験の2018年フライトと将来計画, 高橋弘充, 内田和海, 深沢泰司, 水野恒史, 北口貴雄, 玉川 徹, 早藤麻美, 周 圓輝, 堤 まりな, 内山慶祐, 林田 清, 松本浩典, 常深 博, 榎戶輝揚, 田村啓輔, 前田良知, 石田 学, 斎藤芳隆, 宮澤拓也, 粟木久光, 郡司修一, Krawczynski Henric・Dowkontt Paul・Abarr Quin・Errando Manel・Rauch Bria・Bose Richard・Kislat Fabian, 岡島 崇, Lanzi James, Stuchlik David, Heatwole Scott・Li Shaorui・de Geronimo Gialuigi, Pearce Mark・Kiss Mozsi, Kushwah Rakhee, Kumar Iyer Nirmal, 2019年01月
  • 軟X線から硬X線の広帯域を高感度で撮像分光する小型衛星計画FORCEの現状(7), 森 浩二, 鶴 剛, 中澤知洋, 上田佳宏, 村上弘志, 深沢泰司, 粟木久光, 松本浩典, 岡島 崇, 石田 学, 高橋忠幸, 常深 博, 第19回宇宙科学シンポジウム, 2019年01月
  • X線分光撮像衛星(XRISM)搭載Resolveの開発状況, 石崎欣尚, Kelley Richard L, 赤松弘規, 粟木久光, Bialas Thomas G, Brown Gregory V, Chiao Meng P, Costantini Elisa, den Herder Jan-Willem, Dipirro Michael J, Eckart Megan E, 江副祐一郎, Ferrigno Carlo, 藤本龍一, 古澤彰浩, Graham Steven M, Grim Grim, 林多佳由, 星野晶夫, 一戶悠人, 飯塚 亮, 石橋和紀, 石田 学, 石川久美, Kilbourne Caroline A, 北本俊二, 小山志勇, Leutenegger Maurice A, 前田良知, McCammon Dan, 三石郁之, 森 英之, 中島真也, 大橋隆哉, 岡島 崇, Paltani Stephane, Porter F. Scott, 佐藤浩介, 澤田真理, 瀬田裕美, 柴野靖子, Shirron Peter J, Sneiderman Gary A, Soong Yang, Szymkowiak Andrew E, 竹井 洋, 玉川 徹, 辻本匡弘, Vries Cor P. de, 山田真也, 山崎典子, 安田 進, 吉岡奈紗, 第19回宇宙科学シンポジウム, 2019年01月
  • 炭素繊維強化プラスチック(CFRP)へのX線反射面形成法の開発, 粟木久光, 大上千智, 吉田鉄生, 岩切 駿, 相田 望, 松本浩典, 三石郁之, 大塚康司, 清水貞行, 田村啓輔, 中澤知洋, 石田 学, 石田直樹, 2018年09月
  • X線多重像干渉計MIXIMの開発現状(1) サブ秒角の撮像達成, 花坂剛史, 川端智樹, 林田 清, 朝倉一統, 米山友景, 井出峻太郎, 松本浩典, 常深 博, 粟木久光, 中嶋 大, 日本天文学会2018年秋季年会, 2018年09月
  • 南極周回気球による硬 X 線偏光観測ミッションX-Caliburの現状と今後, 内田和海, 高橋弘充, 深澤泰司, 水野恒史, 北口貴雄, 玉川 徹, 周 圓輝, 堤まりな, 内山慶祐, 林田 清, 松本浩典, 常深 博, 榎戸輝揚, 田村啓輔, 前田良知, 石田 学, 斎藤芳隆, 宮澤拓也, 粟木久光, 郡司修一, Krawczynski, H.・Dowkontt, Kislat, F, 岡島 崇・Lanzi, J, Stuchlik, D・Li, S.・de Geronimo, G, 他 X-Calibur チーム, 日本天文学会2018年秋季年会, 2018年09月
  • X線多重像干渉計MIXIMの開発現状(2) モデルプランの策定と概念検討, 林田 清, 花坂剛史, 朝倉一統, 米山友景, 井出峻太郎, 松本浩典, 常深 博, 粟木久光, 中嶋 大, 日本天文学会2018年秋季年会, 2018年09月
  • 軟X線から硬X線の広帯域を高感度で撮像分光する小型衛星計画FORCEの現状(7), 中澤知洋, 森 浩二, 鶴剛, 上田佳宏, 松本浩典, 粟木久光, 石田 学, 寺島雄一, 常深 博, 中嶋 大, 田中孝明, 内田裕之, 伊藤真之, 寺田幸功, 久保田あや, 馬場 彩, 小高裕和, 高橋忠幸, 谷津陽一, 幸村孝由, 萩野浩一, 小林翔悟, 北山 哲, 村上弘志, 信川正順, 太田直美, 深沢泰司, 水野恒史, 高橋弘充, 大野雅功, 古澤彰浩, 武田彩希, 中島真也, 内山泰伸, 渡辺 伸, 飯塚 亮, 岡島崇, 山口弘悦, 森 英之, 他 FORCE WG, 日本天文学会2018年秋季年会, 2018年09月
  • X線天文衛星代替機 XARM 搭載 Resolve の開発の現状 II, Ishisaki,Y, Kelley, R.L, Akamatsu, H, Awaki, H, Bialas, T.G, Brown, G.V, Chiao, M.P, Costantini, E, den Herder, J.-W, Dipirro, M.J, Eckart, M.E, Ezoe, Y, Ferrigno, C, Fujimoto, R, Furuzawa, A, Graham, S.M, Grim, M, Hayashi, T, Hoshino, A, Ichinohe, Y, Iizuka, R, Ishibashi, K, Ishida, M, Ishikawa, K, Kilbourne, C.A, Kitamoto, S, Koyama, S, Leutenegger, M.A, Maeda, Y, McCammon, D, Mitsuishi, I, Mori, S, Nakashima, H, Noda, H, Ohashi, T, Okajima, T, Paltani, S, Porter, F.S, Sato, K, Sawada, M, Seta, H, Shirron, P.J, Sneiderman, G.A, Soong, Y, Szymkowiak, A.E, Takei, Y, Tamagawa, T, Tsujimoto, M, de Vries, S. C.P, Yamada, S, Yamasaki, N, 日本物理学会2018年秋季大会, 2018年09月
  • サブ秒角でX線天体を撮像する多重像X線干渉計MIXIMの開発II, 林田清, 花坂剛史, 川端智樹, 朝倉一統, 松本浩典, 常深 博, 中嶋 大, 粟木久光, 日本物理学会2018年秋季大会, 2018年09月
  • 炭素繊維強化プラスチック(CFRP)を用いた軽量大面積X線望遠鏡の開発の現状, 粟木久光, 大上千智, 吉田鉄生, 岩切駿, 相田望, 松本浩典, 三石郁之, 大塚康司, 清水貞行, 田村啓輔, 中澤知洋, 石田学, 石田直樹, 日本物理学会2018年秋季大会, 2018年09月
  • The FORCE mission: science aim and instrument parameter for broadband x-ray imaging spectroscopy with good angular resolution, SPIE Astronomical Telescopes + Instrumentation, 2018年06月
  • Development of a lightweight x-ray mirror using thin carbon-fiber-reinforced plastic (CFRP), Awaki, H, Oue, C, Iwakiri, H, Omatsu, M, Yoshida, T, Yokota, T, Ishida, N, Matsumoto, H, SPIE Astronomical Telescopes + Instrumentation, 2018年06月

MISC

  • Concept of the X-ray Astronomy Recovery Mission, Proceedings of the SPIE, Proceedings of the SPIE, 10699, 1069922, 2018年07月
  • The FORCE mission: science aim and instrument parameter for broadband x-ray imaging spectroscopy with good angular resolution, Proceedings of the SPIE, Proceedings of the SPIE, 10699, 106992D, 2018年07月
  • Development of a lightweight x-ray mirror using thin carbon-fiber-reinforced plastic (CFRP), Proceedings of the SPIE, Proceedings of the SPIE, 10699, 106993R, 2018年07月
  • The Hitomi (ASTRO-H) hard x-ray telescope (HXT): current status of calibration, Proceedings of the SPIE, Proceedings of the SPIE, 10399, 103990R, 2017年08月
  • Focusing On Relativistic universe and Cosmic Evolution: the FORCE mission, Proceedings of the XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop, Proceedings of the XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop, 77, 2017年06月
  • Ray-tracing simulation and in-orbit performance of the ASTRO-H hard x-ray telescope (HXT), Proceedings of the SPIE, Proceedings of the SPIE, 9905, 990541, 2016年07月
  • Development of an X-ray telescope using the carbon fiber reinforced plastic, Awaki Hisamitsu, Sugita Satoshi, Ogi Keiji, Yoshioka Kenya, Matsumoto Hironori, Mitsuishi Ikuyuki, Tawara Yuzuru, SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, 9905, 2016年, 0277-786X, 10.1117/12.2232650
  • The ASTRO-H (Hitomi) X-ray Astronomy Satellite, Takahashi Tadayuki, Kokubun Motohide, Mitsuda Kazuhisa, Kelley Richard, Ohashi Takaya, Aharonian Felix, Akamatsu Hiroki, Akimoto Fumie, Allen Steve, Anabuki Naohisa, Angelini Lorella, Arnaud Keith, Asai Makoto, Audard Marc, Awaki Hisamitsu, Axelsson Magnus, Azzarello Philipp, Baluta Chris, Bamba Aya, Bando Nobutaka, Bautz Marshall, Bialas Thomas, Blandford Roger, Boyce Kevin, Brenneman Laura, Brown Greg, Bulbul Esra, Cackett Edward, Canavan Edgar, Chernyakova Maria, Chiao Meng, Coppi Paolo, Costantini Elisa, de Plaa Jelle, den Herder Jan-Willem, DiPirro Michael, Done Chris, Dotani Tadayasu, Doty John, Ebisawa Ken, Eckart Megan, Enoto Teruaki, Ezoe Yuichiro, Fabian Andrew, Ferrigno Carlo, Foster Adam, Fujimoto Ryuichi, Fukazawa Yasushi, Furuzawa Akihiro, Galeazzi Massimiliano, Gallo Luigi, Gandhi Poshak, Gilmore Kirk, Giustini Margherita, Goldwurm Andrea, Gu Liyi, Guainazzi Matteo, Haas Daniel, Haba Yoshito, Hagino Kouichi, Hamaguchi Kenji, Harayama Atsushi, Harrus Ilana, Hatsukade Isamu, Hayashi Takayuki, Hayashi Katsuhiro, Hayashida Kiyoshi, Hiraga Junko, Hirose Kazuyuki, Hornschemeier Ann, Hoshino Akio, Hughes John, Ichinohe Yuto, Iizuka Ryo, Inoue Yoshiyuki, Inoue Hajime, Ishibashi Kazunori, Ishida Manabu, Ishikawa Kumi, Ishimura Kosei, Ishisaki Yoshitaka, Itoh Masayuki, Iwata Naoko, Iyomoto Naoko, Jewell Chris, Kaastra Jelle, Kallman Timothy, Kamae Tuneyoshi, Kara Erin, Kataoka Jun, Katsuda Satoru, Katsuta Junichiro, Kawaharada Madoka, Kawai Nobuyuki, Kawano Taro, Kawasaki Shigeo, Khangulyan Dmitry, Kilbourne Caroline, Kimball Mark, King Ashley, Kitaguchi Takao, Kitamoto Shunji, Kitayama Tetsu, Kohmura Takayoshi, Kosaka Tatsuro, Koujelev Alex, Koyama Katsuji, Koyama Shu, Kretschmar Peter, Krimm Hans, Kubota Aya, Kunieda Hideyo, Laurent Philippe, Lebrun Francois, Lee Shiu-Hang, Leutenegger Maurice, Limousin Olivier, Loewenstein Michael, Long Knox, Lumb David, Madejski Grzegorz, Maeda Yoshitomo, Maier Daniel, Makishima Kazuo, Markevitch Maxim, Masters Candace, Matsumoto Hironori, Matsushita Kyoko, McCammon Dan, Mcguinness Daniel, McNamara Brian, Mehdipour Missagh, Miko Joseph, Miller Jon, Miller Eric, Mineshige Shin, Minesugi Kenji, Mitsuishi Ikuyuki, Miyazawa Takuya, Mizuno Tsunefumi, Mori Koji, Mori Hideyuki, Moroso Franco, Moseley Harvey, Muench Theodore, Mukai Koji, Murakami Hiroshi, Murakami Toshio, Mushotzky Richard, Nagano Housei, Nagino Ryo, Nakagawa Takao, Nakajima Hiroshi, Nakamori Takeshi, Nakano Toshio, Nakashima Shinya, Nakazawa Kazuhiro, Namba Yoshiharu, Natsukari Chikara, Nishioka Yusuke, Nobukawa Masayoshi, Nobukawa Kumiko, Noda Hirofumi, Nomachi Masaharu, O' Dell Steve, Odaka Hirokazu, Ogawa Hiroyuki, Ogawa Mina, Ogi Keiji, Ohno Masanori, Ohta Masayuki, Okajima Takashi, Okamoto Atsushi, Okazaki Tsuyoshi, Ota Naomi, Ozaki Masanobu, Paerels Frits, Paltani Stephane, Parmar Arvind, Petre Robert, Pinto Ciro, Pohl Martin, Pontius James, Porter F. Scott, Pottschmidt Katja, Ramsey Brian, Reynolds Christopher, Russell Helen, Safi-Harb Samar, Saito Shinya, Sakai Shin-ichiro, Sakai Kazuhiro, Sameshima Hiroaki, Sasaki Toru, Sato Goro, Sato Yoichi, Sato Kosuke, Sato Rie, Sawada Makoto, Schartel Norbert, Serlemitsos Peter, Seta Hiromi, Shibano Yasuko, Shida Maki, Shidatsu Megumi, Shimada Takanobu, Shinozaki Keisuke, Shirron Peter, Simionescu Aurora, Simmons Cynthia, Smith Randall, Sneiderman Gary, Soong Yang, Stawarz Lukasz, Sugawara Yasuharu, Sugita Hiroyuki, Sugita Satoshi, Szymkowiak Andrew, Tajima Hiroyasu, Takahashi Hiromitsu, Takeda Shin'ichiro, Takei Yoh, Tamagawa Toru, Tamura Takayuki, Tamura Keisuke, Tanaka Takaaki, Tanaka Yasuo, Tanaka Yasuyuki, Tashiro Makoto, Tawara Yuzuru, Terada Yukikatsu, Terashima Yuichi, Tombesi Francesco, Tomida Hiroshi, Tsuboi Yohko, Tsujimoto Masahiro, Tsunemi Hiroshi, Tsuru Takeshi, Uchida Hiroyuki, Uchiyama Yasunobu, Uchiyama Hideki, Ueda Yoshihiro, Ueda Shutaro, Ueno Shiro, Uno Shin'ichiro, Urry Meg, Ursino Eugenio, de Vries Cor, Wada Atsushi, Watanabe Shin, Watanabe Tomomi, Werner Norbert, Wik Daniel, Wilkins Dan, Williams Brian, Yamada Takahiro, Yamada Shinya, Yamaguchi Hiroya, Yamaoka Kazutaka, Yamasaki Noriko, Yamauchi Makoto, Yamauchi Shigeo, Yaqoob Tahir, Yatsu Yoichi, Yonetoku Daisuke, Yoshida Atsumasa, Yuasa Takayuki, Zhuravleva Irina, Zoghbi Abderahmen, SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, 9905, 2016年, 0277-786X, 10.1117/12.2232379
  • A broadband X-ray imaging spectroscopy with high-angular resolution: the FORCE mission, Koji Mori, Takeshi Go Tsuru, Kazuhiro Nakazawa, Yoshihiro Ueda, Takashi Okajima, Hiroshi Murakami, Hisamitsu Awaki, Hironori Matsumoto, Yasushi Fukazawa, Hiroshi Tsunemi, Tadayuki Takahashi, William W. Zhang, SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, SPIE-INT SOC OPTICAL ENGINEERING, SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, 9905, 311, 2016年, 0277-786X, 10.1117/12.2231262, We are proposing FORCE (Focusing On Relativistic universe and Cosmic Evolution) as a future Japan-lead Xray observatory to be launched in the mid 2020s. Hitomi (ASTRO-H) possesses a suite of sensitive instruments enabling the highest energy-resolution spectroscopy in soft X-ray band, a broadband X-ray imaging spectroscopy in soft and hard X-ray bands, and further high energy coverage up to soft gamma-ray band. FORCE is the direct successor to the broadband X-ray imaging spectroscopy aspect of Hitomi (ASTRO-H) with significantly higher angular resolution. The current design of FORCE defines energy band pass of 1-80 keV with angular resolution of < 15'' in half-power diameter, achieving a 10 times higher sensitivity above 10 keV compared to any previous missions with simultaneous soft X-ray coverage. Our primary scientific objective is to trace the cosmic formation history by searching for "missing black holes" in various mass-scales: "buried supermassive black holes (SMBHs)" (> 10(4) M-circle dot) residing in the center of galaxies in a cosmological distance, "intermediate-mass black holes" (10(2)-10(4) M-circle dot) acting as the possible seeds from which SMBHs grow, and "orphan stellar-mass black holes" (< 10(2) M-circle dot) without companion in our Galaxy. In addition to these missing BHs, hunting for the nature of relativistic particles at various astrophysical shocks is also in our scope, utilizing the broadband X-ray coverage with high angular-resolution. FORCE are going to open a new era in these fields. The satellite is proposed to be launched with the Epsilon vehicle that is a Japanese current solid-fuel rocket. FORCE carries three identical pairs of Super-mirror and wide-band X-ray detector. The focal length is currently planned to be 10 m. The silicon mirror with multi-layer coating is our primary choice to achieve lightweight, good angular optics. The detector is a descendant of hard X-ray imager onboard Hitomi (ASTRO-H) replacing its silicon strip detector with SOI-CMOS silicon pixel detector, allowing an extension of the low energy threshold down to 1 keV or even less.
  • Performance of ASTRO-H Hard X-ray Telescope (HXT), Awaki Hisamitsu, Kunieda Hideyo, Ishida Manabu, Matsumoto Hironori, Furuzawa Akihiro, Haba Yoshito, Hayashi Takayuki, Iizuka Ryo, Ishibashi Kazunori, Itoh Masayuki, Kosaka Tatsuro, Maeda Yoshitomo, Mitsuishi Ikuyuki, Miyazawa Takuya, Mori Hideyuki, Nagano Hosei, Namba Yoshiharu, Ogasaka Yasushi, Ogi Keiji, Okajima Takashi, Sugita Satoshi, Suzuki Yoshio, Tamura Keisuke, Tawara Yuzuru, Uesugi Kentato, Yamauchi Shigeo, SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, 9905, 2016年, 0277-786X, 10.1117/12.2231258
  • Development of an X-ray telescope using the carbon fiber reinforced plastic (CFRP), Hironori Matsumoto, Toshihiro Iwase, Masato Maejima, Hisamitsu Awaki, Hideyo Kunieda, Naoki Ishida, Satoshi Sugita, Takuya Miyazawa, Naoki Shima, Ikuyuki Mitsuishi, Yuzuru Tawara, OPTICS FOR EUV, X-RAY, AND GAMMA-RAY ASTRONOMY VII, SPIE-INT SOC OPTICAL ENGINEERING, OPTICS FOR EUV, X-RAY, AND GAMMA-RAY ASTRONOMY VII, 9603, 2015年, 0277-786X, 10.1117/12.2190762, We are developing an X-ray mirror using the carbon fiber reinforced plastic (CFRP) as a substrate in order to improve the angular resolution of tightly-nested thin-foil Wolter-I X-ray mirrors. We found that curing of the epoxy used in the replication process at the room temperature is effective to suppress the print through. We were able to make mirrors whose shape accuracy is 3 5 pm. Characterization at the synchrotron facility SPring-8 using the X-ray pencil beam of 20 keV showed that the angular resolution was 3 - 5 arcmin as a whole, but can reach to 20 arcsec locally.
  • ASTRO-H White Paper - AGN Winds, J. S. Kaastra, Y. Terashima, T. Kallman, Y. Haba, E. Costantini, L. Gallo, Y. Fukazawa, F. Tombesi, N. Anabuki, H. Awaki, G. Brown, L. di Gesu, K. Ebisawa, J. Ebrero, M. Eckart, K. Hagino, K. S. Long, J. Miller, T. Miyazawa, S. Paltani, C. Reynolds, C. Ricci, H. Sameshima, H. Seta, Y. Ueda, M. Urry, for the ASTRO-H, Science Working Group, 2014年12月, http://arxiv.org/abs/1412.1171v1, In this white paper we describe the prospects for ASTRO-H for the study of<br /> outflows from active galactic nuclei. The most important breakthroughs in this<br /> field are expected to arise from the high spectral resolution and sensitivity<br /> in the Fe-K band, combined with broad-band sensitivity over the full X-ray band<br /> and spectral capabilities also at lower energies. The sensitivity in the Fe-K<br /> region allows to extend the absorption measure distribution of the outflow out<br /> to the highest ionisation states accessible, where observations with current<br /> X-ray missions indicate that most of the outflowing gas is to be found. Due to<br /> the high-resolution and sensitivity it will also be able to give the definitive<br /> proof for the existence of ultra-fast outflows, and if so, characterise their<br /> physical properties in great detail. These ultra-fast outflows carry very large<br /> amounts of energy and momentum, and are of fundamental importance for feedback<br /> studies. We show how the ASTRO-H observations in general can help to constrain<br /> numerical models for outflows. The link to reflection and emission processes is<br /> also discussed, as well as the possible relation between outflows and<br /> relativistic emission lines. Finally, we discuss the prospects for other<br /> related categories of objects like BAL quasars, partially covered sources and<br /> Compton thick outflows.
  • The ASTRO-H X-ray Astronomy Satellite, Takahashi Tadayuki, Mitsuda Kazuhisa, Kelley Richard, Aharonian Felix, Akamatsu Hiroki, Akimoto Fumie, Allen Steve, Anabuki Naohisa, Angelini Lorella, Arnaud Keith, Asai Makoto, Audard Marc, Awaki Hisamitsu, Azzarello Philipp, Baluta Chris, Bamba Aya, Bando Nobutaka, Bautz Marshall, Bialas Thomas, Blandford Roger, Boyce Kevin, Brenneman Laura, Brown Greg, Cackett Edward, Canavan Edgar, Chernyakova Maria, Chiao Meng, Coppi Paolo, Costantini Elisa, de Plaa Jelle, den Herder Jan-Willem, DiPirro Michael, Done Chris, Dotani Tadayasu, Doty John, Ebisawa Ken, Enoto Teruaki, Ezoe Yuichiro, Fabian Andrew, Ferrigno Carlo, Foster Adam, Fujimoto Ryuichi, Fukazawa Yasushi, Funk Stefan, Furuzawa Akihiro, Galeazzi Massimiliano, Gallo Luigi, Gandhi Poshak, Gilmore Kirk, Guainazzi Matteo, Haas Daniel, Haba Yoshito, Hamaguchi Kenji, Harayama Atsushi, Hatsukade Isamu, Hayashi Katsuhiro, Hayashi Takayuki, Hayashida Kiyoshi, Hiraga Junko, Hirose Kazuyuki, Hornschemeier Ann, Hoshino Akio, Hughes John, Hwang Una, Iizuka Ryo, Inoue Yoshiyuki, Ishibashi Kazunori, Ishida Manabu, Ishikawa Kumi, Ishimura Kosei, Ishisaki Yoshitaka, Itoh Masayuki, Iwata Naoko, Iyomoto Naoko, Jewell Chris, Kaastra Jelle, Kallman Timothy, Kamae Tuneyoshi, Kataoka Jun, Katsuda Satoru, Katsuta Junichiro, Kawaharada Madoka, Kawai Nobuyuki, Kawano Taro, Kawasaki Shigeo, Khangaluyan Dmitry, Kilbourne Caroline, Kimball Mark, Kimura Masashi, Kitamoto Shunji, Kitayama Tetsu, Kohmura Takayoshi, Kokubun Motohide, Konami Saori, Kosaka Tatsuro, Koujelev Alexander, Koyama Katsuji, Krimm Hans, Kubota Aya, Kunieda Hideyo, LaMassa Stephanie, Laurent Philippe, Lebrun Francois, Leutenegger Maurice, Limousin Olivier, Loewenstein Michael, Long Knox, Lumb David, Madejski Grzegorz, Maeda Yoshitomo, Makishima Kazuo, Markevitch Maxim, Masters Candace, Matsumoto Hironori, Matsushita Kyoko, McCammon Dan, McGuinness Daniel, McNamara Brian, Miko Joseph, Miller Jon, Miller Eric, Mineshige Shin, Minesugi Kenji, Mitsuishi Ikuyuki, Miyazawa Takuya, Mizuno Tsunefumi, Mori Koji, Mori Hideyuki, Moroso Franco, Muench Theodore, Mukai Koji, Murakami Hiroshi, Murakami Toshio, Mushotzky Richard, Nagano Housei, Nagino Ryo, Nakagawa Takao, Nakajima Hiroshi, Nakamori Takeshi, Nakashima Shinya, Nakazawa Kazuhiro, Namba Yoshiharu, Natsukari Chikara, Nishioka Yusuke, Nobukawa Masayoshi, Noda Hirofumi, Nomachi Masaharu, Dell Steve O, Odaka Hirokazu, Ogawa Hiroyuki, Ogawa Mina, Ogi Keiji, Ohashi Takaya, Ohno Masanori, Ohta Masayuki, Okajima Takashi, Okazaki Tsuyoshi, Ota Naomi, Ozaki Masanobu, Paerels Frits, Paltani Stephane, Parmar Arvind, Petre Robert, Pinto Ciro, Pohl Martin, Pontius James, Porter F. Scott, Pottschmidt Katja, Ramsey Brian, Reis Rubens, Reynolds Christopher, Ricci Claudio, Russell Helen, Safi-Harb Samar, Saito Shinya, Sakai Shin-ichiro, Sameshima Hiroaki, Sato Kosuke, Sato Rie, Sato Goro, Sawada Makoto, Serlemitsos Peter, Seta Hiromi, Shibano Yasuko, Shida Maki, Shimada Takanobu, Shirron Peter, Simionescu Aurora, Simmons Cynthia, Smith Randall, Sneiderman Gary, Soong Yang, Stawarz Lukasz, Sugawara Yasuharu, Sugita Satoshi, Szymkowiak Andrew, Tajima Hiroyasu, Takahashi Hiroaki, Takahashi Hiromitsu, Takeda Shin-ichiro, Takei Yoh, Tamagawa Toru, Tamura Keisuke, Tamura Takayuki, Tanaka Takaaki, Tanaka Yasuyuki, Tanaka Yasuo, Tashiro Makoto, Tawara Yuzuru, Terada Yukikatsu, Terashima Yuichi, Tombesi Francesco, Tomida Hiroshi, Tsuboi Yoko, Tsujimoto Masahiro, Tsunemi Hiroshi, Tsuru Takeshi, Uchida Hiroyuki, Uchiyama Hideki, Uchiyama Yasunobu, Ueda Yoshihiro, Uedag Shutaro, Ueno Shiro, Uno Shinichiro, Urry Meg, Ursino Eugenio, de Vries Cor, Wada Atsushi, Watanabe Shin, Watanabe Tomomi, Werner Norbert, White Nicholas, Wilkins Dan, Yamada Shinya, Yamada Takahiro, Yamaguchi Hiroya, Yamaoka Kazutaka, Yamasaki Noriko, Yamauchi Makoto, Yamauchi Shigeo, Yadoob Tahir, Yatsu Yoichi, Yonetoku Daisuke, Yoshida Atsumasa, Yuasa Takayuki, Zhuravleva Irina, Zoghbi Abderahmen, ZuHone John, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, 9144, 2014年, 0277-786X, 10.1117/12.2055681
  • Recent Progress in the Ground Calibration of the ASTRO-H Hard X-ray Telescope (HXT-2), Hideyuki Mori, Yuji Kuroda, Takuya Miyazawa, Hisamitsu Awaki, Yasunori Babazaki, Akihiro Furuzawa, Tatsuya Hibino, Ryo Iizuka, Kazunori Ishibashi, Toshihiro Iwase, Hideyo Kunieda, Daichi Kurihara, Hironori Matsumoto, Yusuke Miyata, Sigetaka Saji, Satoshi Sugita, Yoshio Suzuki, Sasagu Tachibana, Keisuke Tamura, Yuzuru Tawara, Kentaro Uesugi, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, SPIE-INT SOC OPTICAL ENGINEERING, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, 9144, 2014年, 0277-786X, 10.1117/12.2055656, The 6th Japanese X-ray satellite, ASTRO-H, equips two Hard X-ray Telescopes (HXTs) to perform imaging spectroscopy up to 70 keV. The 2nd flight module (HXT-2) had been completed in July, 2013. After some environmental tests were passed, the X-ray performance of the HXT-2 was measured at the SPring-8 BL20B2, 3rd generation synchrotron facility. The angular resolution defined with a Half Power Diameter (HPD) was 1'.9 at 30 keV and 1'.8 at 50 keV. This small energy dependence is considered to be caused by the difference in image quality of each foil; the inner mirror shells have better quality than outer ones. The effective area was found to be 178 cm(2) at 30 keV and 82 cm(2) at 50 keV, both of which exceed the requirement. Furthermore, the detailed energy dependence of the effective area was examined for a limited aperture in the 30-70 keV band with a pitch of 1 keV. We also measured the off-axis dependence of the effective area at 50 keV, and then determined the optical axis. The field of view of the HXT-2 was found to be 5'.6 (FWHM of the vignetting function), consistent with the simulation. In this paper, we also report the detailed analysis of the ground calibration data, which will be used for image reconstruction by a ray-tracing simulator.
  • Studies of Lightweight X-ray Telescope with CFRP, Sugita Satoshi, Awaki Hisamitsu, Kurihara Daichi, Yoshioka Kenya, Tomita Yuuki, Ogi Keiji, Kunieda Hideyo, Matsumoto Hironori, Miyazawa Takuya, Iwase Toshihiro, Hibino Tatsuya, Ishikawa Takashi, Hamada Takayoshi, Ishida Naoki, Akiyama Hiromichi, Kishimoto Kazuaki, Utsunomiya Shin, Kamiya Tomohiro, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, 9144, 2014年, 0277-786X, 10.1117/12.2054837
  • ASTRO-H Soft X-ray Telescope (SXT), Yang Soong, Takashi Okajima, Peter J. Serlemitsos, Stephen L. Odell, Brian D. Ramsey, Mikhail V. Gubarev, Manabu Ishida, Yoshitomo Maeda, Ryo Iizuka, Takayuki Hayashi, Yuzuru Tawara, Akihiro Furuzawa, Hideyuki Mori, Takuya Miyazawa, Hideyo Kunieda, Hisamitsu Awaki, Satoshi Sugita, Keisuke Tamura, Kazunori Ishibashi, Takanori Izumiya, Sari Minami, Toshiki Sato, Kazuki Tomikawa, Naomichi Kikuchi, Toshihiro Iwase, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, SPIE-INT SOC OPTICAL ENGINEERING, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, 9144, 2014年, 0277-786X, 10.1117/12.2056804, ASTRO-H is an astrophysics satellite dedicated for non-dispersive X-ray spectroscopic study on selective celestial X-ray sources. Among the onboard instruments there are four Wolter-I X-ray mirrors of their reflectors' figure in conical approximation. Two of the four are soft X-ray mirrors(1), of which the energy range is from a few hundred eV to 15 keV within the effective aperture being defined by the nested reflectors' radius ranging between 5.8 cm to 22.5 cm. The focal point instruments will be a calorimeter (SXS) and a CCD camera (SXI), respectively. The mirrors were in quadrant configuration with photons being reflected consecutively in the primary and secondary stage before converging on the focal plane of 5.6 m away from the interface between the two stages. The reflectors of the mirror are made of heat-formed aluminum substrate of the thickness gauged of 152 mu m, 229 mu m, and 305 mu m of the alloy 5052 H-19, followed by epoxy replication on gold-sputtered smooth Pyrex cylindrical mandrels to acquire the X-ray reflective surface. The epoxy layer is 10 mu m nominal and surface gold layer of 0.2 mu m. Improvements on angular response over its predecessors, e.g. Astro-E1/Suzaku mirrors, come from error reduction on the figure, the roundness, and the grazing angle/radius mismatching of the reflecting surface, and tighter specs and mechanical strength on supporting structure to reduce the reflector positioning and the assembly errors. Each soft x-ray telescope (SXT), SXT-1 or SXT-2, were integrated from four independent quadrants of mirrors. The stray-light baffles, in quadrant configuration, were mounted onto the integrated mirror. Thermal control units were attached to the perimeter of the integrated mirror to keep the mirror within operating temperature in space. The completed instrument went through a series of optical alignment, thus made the quadrant images confocal and their optical axes in parallel to achieve highest throughput possible. Environmental tests were carried out, and optical quality of the telescopes has been confirmed. SXT-1 and -2 were tested with the broad but slightly divergent beam, up to 8 arc-minutes, at Goddard. The full characterization were carried out in Japan which includes: angular resolution, effective area in the energy range of similar to 0.4 - 12keV, off-axis response at various energies, etc. We report the calibration results of the SXT-1 and -2 that were obtained at NASA/Goddard and JAXA/ISAS. The detailed calibration are reported in the two papers in this conference: 9144-206, &quot;Ground-based x-ray calibration of the ASTRO-H soft x-ray telescopes&quot; by R. Iizuka et al. and 9144-207, &quot;Revealing a detailed performance of the soft x-ray telescopes of the ASTRO-H mission&quot; by T. Sato, et al. Some small but significant discrepancies existed between ISAS and Goddard measurements that were attributed to the difference of the X-ray beams - pencil beam vs divergent beam.
  • ASTRO-H Hard X-ray Telescope (HXT), Awaki Hisamitsu, Kunieda Hideyo, Furuzawa Akihiro, Haba Yoshito, Hayashi Takayuki, Iizuka Ryo, Ishibashi Kazunori, Ishida Manabu, Itoh Masayuki, Kosaka Tatsuro, Maeda Yoshitomo, Matsumoto Hironori, Miyazawa Takuya, Mori Hideyuki, Nagano Hosei, Namba Yoshiharu, Ogasaka Yasushi, Ogi Keiji, Okajima Takashi, Sugita Satoshi, Suzuki Yoshio, Tamura Keisuke, Tawara Yuzuru, Uesugi Kentato, Yamashita Koujun, Yamauchi Shigeo, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, 9144, 2014年, 0277-786X, 10.1117/12.2054633
  • The ASTRO-H X-ray Observatory, 粟木 久光, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, 8443, 84431Z, 2012年09月
  • Current status of ASTRO-H Hard X-ray Telescopes (HXTs), 粟木 久光, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, 8443, 844324, 2012年09月
  • Vibration properties of mirror foils for hard x-ray telescope onboard satellite, 粟木 久光, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, 8443, 84435A, 2012年09月
  • The pre-collimator for the ASTRO-H x-ray telescopes: shielding from stray lights, 粟木 久光, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, 8443, 84435B, 2012年09月
  • Recent results of hard x-ray characterization of ASTRO-H HXT at SPring-8, 粟木 久光, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of the SPIE, 8443, 84435C, 2012年09月
  • Vibration properties of Hard X-ray telescope on board satellite, SPIEThe Proceedings of SPIE, SPIEThe Proceedings of SPIE, 7732, 77323G1-9, 2010年
  • The thermal analysis of the hard X-ray telescope (HXT) and the investigation of the deformation of the mirror foil due to temperature change, SPIEThe Proceedings of SPIE, SPIEThe Proceedings of SPIE, 7732, 77323A1-13, 2010年
  • Hard x-ray telescope to be onboard ASTRO-H, SPIEThe Proceedings of SPIE 7732, SPIEThe Proceedings of SPIE 7732, 7732, 773214-1-12, 2010年
  • Vibration properties of Hard X-ray telescope on board satellite, SPIEThe Proceedings of SPIE, SPIEThe Proceedings of SPIE, 7732, 77323G1-9, 2010年
  • The thermal analysis of the hard X-ray telescope (HXT) and the investigation of the deformation of the mirror foil due to temperature change, SPIEThe Proceedings of SPIE, SPIEThe Proceedings of SPIE, 7732, 77323A1-13, 2010年
  • Hard x-ray telescope to be onboard ASTRO-H, SPIEThe Proceedings of SPIE 7732, SPIEThe Proceedings of SPIE 7732, 7732, 773214-1-12, 2010年
  • Current status of the Astro-H-X-ray Telescope system, SPIEThe Proceedings of SPIE, SPIEThe Proceedings of SPIE, 7437, 743703, 2009年
  • Current status of the Astro-H-X-ray Telescope system, SPIEThe Proceedings of SPIE, SPIEThe Proceedings of SPIE, 7437, 743703, 2009年
  • Design study of telescope housing for the NeXT/XRT, SPIEThe Proceedings of SPIE, SPIEThe Proceedings of SPIE, 7011, 70112Q, 2008年
  • Design study of telescope housing for the NeXT/XRT, SPIEThe Proceedings of SPIE, SPIEThe Proceedings of SPIE, 7011, 70112Q, 2008年
  • Soft X-ray mirrors onboard the NeXT satellite, Takashi Okajima, Peter J. Serlemitsos, Yang Soong, Kai-Wing Chan, Rob Petre, Yasushi Ogasaka, Takuya Miyazawa, Akihiro Furuzawa, Hideyo Kunieda, Manabu Ishida, Yoshitomo Maeda, Keisuke Tamura, Hideyuki Mori, Hisamitsu Awaki, SPACE TELESCOPES AND INSTRUMENTATION 2008: ULTRAVIOLET TO GAMMA RAY, PTS 1 AND 2, SPIE-INT SOC OPTICAL ENGINEERING, SPACE TELESCOPES AND INSTRUMENTATION 2008: ULTRAVIOLET TO GAMMA RAY, PTS 1 AND 2, 7011, 2008年, 0277-786X, 10.1117/12.789599, The New Exploration X-ray Telescope (NeXT) is an X-ray, astronomical observatory slated to be launched from Japan in 2013. Its objectives range from high resolution imaging and spectroscopy, below similar to 12 keV to studyiug the hard X-ray sky up to similar to 70 keV. To accomplish these goals, it will carry, among other instruments, 4 grazing incidence, imaging telescopes, two covering the soft X-ray band and the remaining the higher energies. The soft X-ray telescopes will be similar to ones flown onboard Suzaku, with a larger outer diameter (45 cm) and longer focal length (6 m). The NASA's GSFC foil mirror group is collaborating with the Nagoya University and ISAS/JAXA in the implementation of the the soft, X-ray mirrors. Our science driven goal is a &lt; 1.3' Half Power Diameter (HPD) Point Spread Function, improved from Suzaku similar to 1.7' HPD. We address important area in the fabrication process where we plan to make changes; (1) substrate shaping, (2) replication process, (3) reflector assembly, (4) alignment bar accuracy and (5) focal length miss match among segments. Having done some of them, we measured 1.26' HPD for 60-pair quadrant reflectors. But it still includes bad sectors (&gt; 1.8' HPD) towards the quadrant boundary, while most of middle sectors are at 1' HPD level. The bad sectors can be corrected with new assembly approach where we actively tune and then fix reflectors at their right position or whole conical shell reflectors instead of segmented ones. In this proceeding, we present a proposed NeXT soft X-ray telescope performance, report the current status of the development and introduce the new whole shell mirror.
  • Design of the pre-collimator for the NeXT X-ray telescopes, Hideyuki Mori, Yasushi Ogasaka, Manabu Ishida, Yoshitomo Maeda, Keisuke Tamura, Hideyo Kunieda, Akihiro Furuzawa, Yoshito Haba, Takuya Miyazawa, Koujun Yamashita, Hisamitsu Awaki, Peter J. Serlemitsos, Yang Soong, Kai-Wing Chan, Takashi Okajima, SPACE TELESCOPES AND INSTRUMENTATION 2008: ULTRAVIOLET TO GAMMA RAY, PTS 1 AND 2, SPIE-INT SOC OPTICAL ENGINEERING, SPACE TELESCOPES AND INSTRUMENTATION 2008: ULTRAVIOLET TO GAMMA RAY, PTS 1 AND 2, 7011, 2008年, 0277-786X, 10.1117/12.789184, We present the design of the pre-collimator for the X-ray telescopes (XRTs) onboard New X-ray Telescope (NeXT). The optical design adopted for the NeXT XRTs is conically-approximated Wolter-I type optics. The tightly-nested reflectors with thin substrates (150-300 mu m) enable us to achieve the large effective area and extremely light weight simultaneously. However. due to the packed reflector shells, X-rays from the outside of the XRT field of view occasionally arrive at the focal plane without the, normal double reflection (stray lights), and then produce a ghost image oil the detector. Thus. the stray-fights contamination degrades sensitivity of the source detection In order to reduce the stray lights efficiently, we plan to mount a, collimator onto each telescope (referred to as pre-collimator), which is similar to that equipped with the Suzaku XRTs. The pre-collimator consists of coaxially-nested cylindrical blades. each of which is aligned radially with the corresponding primary reflector. We, found the height of the pre-collimator blade to be similar to 100 mm that is required to block the X-rays with off-axis angles of 30'-50'. which are the main light pass of the stray lights for the NeXT XRTs.
  • The NeXT x-ray telescope system: status update, Yasushi Ogasaka, Hideyo Kunieda, Takuya Miyazawa, Peter Serlemitsos, Yang Soong, Takashi Okajima, Yoshitomo Maeda, Hideyuki Mori, Manabu Ishida, Hisamitsu Awaki, Akihiro Furuzawaa, Yoshiharu Namba, Kentato Uesugi, Yoshio Suzuki, Yoshito Haba, Keisuke Tamura, Hiroshi Tsunemi, Koujun Yamashita, Masayuki Ito, SPACE TELESCOPES AND INSTRUMENTATION 2008: ULTRAVIOLET TO GAMMA RAY, PTS 1 AND 2, SPIE-INT SOC OPTICAL ENGINEERING, SPACE TELESCOPES AND INSTRUMENTATION 2008: ULTRAVIOLET TO GAMMA RAY, PTS 1 AND 2, 7011, 2008年, 0277-786X, 10.1117/12.788736, Japan's NeXT mission has, been approved for the Phase-A in 2007. At, present NeXT is in the process of transition to the Phase-B. One of the unique freature of the mission is an imaging spectroscopy in unprecedentedly wide energy region from 0.5 to 80 keV. The X-Ray Telescope (XRT) system covers the energy by means of grazing incidence reflective optics. International collaboration has been formed for the project and design and basic study have been carried out so far. Current baseline specification includes two hard X-ray telescopes which are combined with the Hard X-ray. Imager (Si + CdTe pixel or strip) and cover 5 to 80 keV, and two soft, X-ray telescopes which cover 0.3 to about 20 keV, one combined with a high resolution X-ray micro-calorimeter and the other with an X-ray CCD. Both of hard and soft X-ray mirrors employ same optical design; tightly-nested conically-approximated thin-foil Wolter-I optics. The mission requirements for XRT system have been identified as 300 cm(2) at 30 keV for the hard X-ray telescope in total and 400 cm(2) at 6 keV for the soft X-ray telescope per unit. The requirement oil the point spread function is 1.7 arcmin in HPD, as well as the goal being 1.2 arcmin Based oil the current level of technology all the mission requirements are expected to be satisfied.
  • Broad-band spectra of Seyfert 2 galaxies observed with Suzaku, Hisamitsu Awaki, PROGRESS OF THEORETICAL PHYSICS SUPPLEMENT, PROGRESS THEORETICAL PHYSICS PUBLICATION OFFICE, PROGRESS OF THEORETICAL PHYSICS SUPPLEMENT, 169, 240, 243, 2007年, 0375-9687, We obtained broad-band spectra of Seyfert 2 galaxies observed with the X-ray satellite Suzaku. Their X-ray emissions were resolved into a weak power-law emission, an absorbed power-law emission, a reflection, and many emission lines. These are the first observations to resolve the spectra by a broad-band spectroscopy from 0.3 to 100 keV. Thank to the high quality spectra with Suzaku, we obtained information to investigate the structure of active galactic nuclei in detail.
  • Time variability of low-luminosity AGN, Astron.Nach., Astron.Nach., 320, 307, 1999年
  • Time variability of low-luminosity AGN, Astron.Nach., Astron.Nach., 320, 307, 1999年
  • ASCA Observations of Seyfert 2 Galaxies, "Emission Lines in Active Galaxies : New Methods and Techniques" B. M. Peterson, F. -Z. Cheng, and A. S. Wilson(eds), "Emission Lines in Active Galaxies : New Methods and Techniques" B. M. Peterson, F. -Z. Cheng, and A. S. Wilson(eds), 44, 1997年, 10.1016/S0273-1177(97)00042-2
  • ASCA Observations of Seyfert 2 Galaxies, "Emission Lines in Active Galaxies : New Methods and Techniques" B. M. Peterson, F. -Z. Cheng, and A. S. Wilson(eds), "Emission Lines in Active Galaxies : New Methods and Techniques" B. M. Peterson, F. -Z. Cheng, and A. S. Wilson(eds), 44, 1997年, 10.1016/S0273-1177(97)00042-2
  • Calibration of Astro-D telescope with an X-ray pencil beam, S. P. I. E-The International Society for Optical Engineering, S. P. I. E-The International Society for Optical Engineering, 2011, 517, 1993年
  • Calibration of Astro-D telescope with an X-ray pencil beam, S. P. I. E-The International Society for Optical Engineering, S. P. I. E-The International Society for Optical Engineering, 2011, 517, 1993年
  • SEARCH FOR LARGE-SCALE EXTENDED DIFFUSE-X-RAY EMISSION FROM THE COMA-A1367 SUPERCLUSTER, Y TAWARA, M KAWADA, S TAKANO, K KOYAMA, H AWAKI, PROCEEDINGS OF THE 23RD ESLAB SYMPOSIUM ON TWO TOPICS IN X-RAY ASTRONOMY, VOLS 1 AND 2, EUROPEAN SPACE AGENCY, PROCEEDINGS OF THE 23RD ESLAB SYMPOSIUM ON TWO TOPICS IN X-RAY ASTRONOMY, VOLS 1 AND 2, 296, 1065, 1067, 1989年
  • Sub-arcsecond imaging with multi-image x-ray interferometer module (MIXIM) for very small satellite, 粟木 久光, Proceedings of the SPIE, Proceedings of the SPIE, 10699, 106990U

その他研究情報

競争的資金

愛媛大学教員活動実績

教育活動(B)

担当授業科目(B01)

  • 2019年, 前期, 学部, 宇宙物理学セミナーⅢ
  • 2019年, 前期, 学部, 物理学実験Ⅱ
  • 2019年, 前期, 学部, 卒業研究Ⅰ
  • 2019年, 前期, 学部, 卒業研究Ⅱ
  • 2019年, 前期, 学部, 基礎電磁気学
  • 2019年, 前期, 修士, 物理学ゼミナールI
  • 2019年, 前期, 修士, 物理学ゼミナールⅢ


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