SLIM Project Team
  1. Researcher List
  2. Makoto Tashiro

Makoto Tashiro

  (田代 信)

Profile Information

Affiliation
Professor, Graduate School of Science and Engineering, Saitama University
Specially Appointed Professor, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
Degree
Master (Science)(the University of Tokyo)
Dr. (Science)(the University of Tokyo)
J-GLOBAL ID
200901083726265608
researchmap Member ID
1000161587
External link

Research Interests

 14

Research Areas

 1

Research History

 4

Education

 3

Committee Memberships

 2

Awards

 2

Papers

 224
  • Naoki Isobe, Motoki Kino, Takao Nakagawa, Shunsuke Baba, Makoto Tashiro, Hiroshi Nagai
    Publications of the Astronomical Society of Japan, Jun 19, 2026  
  • Taishu Kayanoki, Yasushi Fukazawa, Junjie Mao, Jon M. Miller, Luigi Gallo, Tahir Yaqoob, Richard Mushotzky, David Bogensberger, Misaki Mizumoto, Kouichi Hagino, Hirofumi Noda, Yoshihiro Ueda, Makoto Tashiro, Yuya Nakatani, Toshiya Iwata, Misaki Urata
    The Astrophysical Journal, 1002(1) 91-91, Apr 28, 2026  
    Abstract We present the first clear detection of ionized Fe-K emission and absorption components in the nearby radio galaxy Centaurus A, revealed by the high-resolution XRISM/Resolve detector. In the 6.5–6.9 keV band, XRISM reveals multiple Fe xxv and Fe xxvi emission components. One is a broad (with a width of σ  = 3000 km s −1 ) and redshifted (+3400 km s −1 ) component, originating at D = 0.02 pc from the central black hole. The other two components are narrow (with a width of σ  = 500 km s −1 ) and exhibit redshifted and blueshifted velocities (+2600 and −1500 km s −1 ), originating from more distant regions ( D = 0.1 pc). The photoionized model explains the broader component, while the two narrower components can be explained by either photoionization or collisional ionization. One interpretation is that the broader component is an outflow at ∼10 2 R S (Schwarzschild radius) and the narrow component is a shock-heated plasma close to the torus, with a possible connection to the JWST-discovered outflow outside the torus. Two blueshifted absorption lines are detected at ∼7.1 keV (∼10 4 km s −1 ) and ∼10.6 keV (∼10 5 km s −1 ). The line significance of the 10.6 keV line is above 98%. The absorption line components might be attributed to the broad emission component. These results demonstrate the high potential of XRISM/Resolve to characterize ionized emission and absorption features in the Fe-K band. Our findings establish a new benchmark in the study of circumnuclear environments in low-luminosity radio galaxies, thereby contributing to a broader understanding of active galactic nuclei unification.
  • Marc Audard, Hisamitsu Awaki, Ralf Ballhausen, Aya Bamba, Ehud Behar, Rozenn Boissay-Malaquin, Laura Brenneman, Gregory V. Brown, Lia Corrales, Elisa Costantini, Renata Cumbee, Maria Diaz Trigo, Chris Done, Tadayasu Dotani, Ken Ebisawa, Megan E. Eckart, Dominique Eckert, Satoshi Eguchi, Teruaki Enoto, Yuichiro Ezoe, Adam Foster, Ryuichi Fujimoto, Yutaka Fujita, Yasushi Fukazawa, Kotaro Fukushima, Akihiro Furuzawa, Luigi Gallo, Javier A. García, Liyi Gu, Matteo Guainazzi, Kouichi Hagino, Kenji Hamaguchi, Isamu Hatsukade, Katsuhiro Hayashi, Takayuki Hayashi, Natalie Hell, Edmund Hodges-Kluck, Ann Hornschemeier, Yuto Ichinohe, Daiki Ishi, Manabu Ishida, Kumi Ishikawa, Yoshitaka Ishisaki, Jelle Kaastra, Timothy Kallman, Erin Kara, Satoru Katsuda, Yoshiaki Kanemaru, Richard Kelley, Caroline Kilbourne, Shunji Kitamoto, Shogo Kobayashi, Takayoshi Kohmura, Aya Kubota, Maurice Leutenegger, Michael Loewenstein, Yoshitomo Maeda, Maxim Markevitch, Hironori Matsumoto, Kyoko Matsushita, Dan McCammon, Brian McNamara, François Mernier, Eric D. Miller, Jon M. Miller, Ikuyuki Mitsuishi, Misaki Mizumoto, Tsunefumi Mizuno, Koji Mori, Koji Mukai, Hiroshi Murakami, Richard Mushotzky, Hiroshi Nakajima, Kazuhiro Nakazawa, Jan-Uwe Ness, Kumiko Nobukawa, Masayoshi Nobukawa, Hirofumi Noda, Hirokazu Odaka, Shoji Ogawa, Anna Ogorzałek, Takashi Okajima, Naomi Ota, Stephane Paltani, Robert Petre, Paul Plucinsky, Frederick S. Porter, Katja Pottschmidt, Kosuke Sato, Toshiki Sato, Makoto Sawada, Hiromi Seta, Megumi Shidatsu, Aurora Simionescu, Randall Smith, Hiromasa Suzuki, Andrew Szymkowiak, Hiromitsu Takahashi, Mai Takeo, Toru Tamagawa, Keisuke Tamura, Takaaki Tanaka, Atsushi Tanimoto, Makoto Tashiro, Yukikatsu Terada, Yuichi Terashima, Yohko Tsuboi, Masahiro Tsujimoto, Hiroshi Tsunemi, Takeshi Tsuru, Ayşegül Tümer, Hiroyuki Uchida, Nagomi Uchida, Yuusuke Uchida, Hideki Uchiyama, Shutaro Ueda, Yoshihiro Ueda, Shinichiro Uno, Jacco Vink, Shin Watanabe, Brian J. Williams, Satoshi Yamada, Shinya Yamada, Hiroya Yamaguchi, Kazutaka Yamaoka, Noriko Yamasaki, Makoto Yamauchi, Shigeo Yamauchi, Tahir Yaqoob, Tomokage Yoneyama, Tessei Yoshida, Mihoko Yukita, Irina Zhuravleva, Matthew Charbonneau, Neo Dizdar, Masashi Fujita, Daisuke Ito, Jessica Martin, Hannah McCall, Helen Russell, John ZuHone
    The Astrophysical Journal, 998(2) 210-210, Feb 11, 2026  Peer-reviewed
    Abstract The XRISM/Resolve microcalorimeter directly measured the gas velocities in the core of the Virgo Cluster, the closest example of active galactic nucleus (AGN) feedback in a cluster. This proximity allows us to resolve the kinematic impact of feedback on scales down to 5 kpc. Our spectral analysis reveals a high velocity dispersion of km s −1 near the AGN, which steeply declines to ∼60 km s −1 between 5 and 25 kpc in the northwest direction. The observed line-of-sight bulk velocity in all regions is broadly consistent with the central galaxy, M87, with a mild trend toward blueshifted motions at larger radii. Systematic uncertainties have been carefully assessed and do not affect the measurements. The central velocities, if attributed entirely to isotropic turbulence, correspond to a transonic intracluster medium at sub-6 kpc scales with 3D Mach number and a nonthermal pressure fraction of . Simple models of weak shocks and sound waves and calculations assuming isotropic turbulence both support the hypothesis that the velocity field reflects a mix of shock-driven expansion and turbulence. Compared to other clusters observed by XRISM to date, M87’s central region stands out as the most kinematically disturbed, exhibiting both the highest velocity dispersion and the largest 3D Mach number, concentrated at the smallest physical scales.
  • Marc Audard, Hisamitsu Awaki, Ralf Ballhausen, Aya Bamba, Ehud Behar, Rozenn Boissay-Malaquin, Laura Brenneman, Gregory V. Brown, Lia Corrales, Elisa Costantini, Renata Cumbee, María Díaz Trigo, Chris Done, Tadayasu Dotani, Ken Ebisawa, Megan E. Eckart, Dominique Eckert, Satoshi Eguchi, Teruaki Enoto, Yuichiro Ezoe, Adam Foster, Ryuichi Fujimoto, Yutaka Fujita, Yasushi Fukazawa, Kotaro Fukushima, Akihiro Furuzawa, Luigi Gallo, Javier A. García, Liyi Gu, Matteo Guainazzi, Kouichi Hagino, Kenji Hamaguchi, Isamu Hatsukade, Katsuhiro Hayashi, Takayuki Hayashi, Natalie Hell, Edmund Hodges-Kluck, Ann Hornschemeier, Yuto Ichinohe, Daiki Ishi, Manabu Ishida, Kumi Ishikawa, Yoshitaka Ishisaki, Jelle Kaastra, Timothy Kallman, Erin Kara, Satoru Katsuda, Yoshiaki Kanemaru, Richard Kelley, Caroline Kilbourne, Shunji Kitamoto, Shogo Kobayashi, Takayoshi Kohmura, Aya Kubota, Maurice Leutenegger, Michael Loewenstein, Yoshitomo Maeda, Maxim Markevitch, Hironori Matsumoto, Kyoko Matsushita, Dan McCammon, Brian McNamara, François Mernier, Eric D. Miller, Jon M. Miller, Ikuyuki Mitsuishi, Misaki Mizumoto, Tsunefumi Mizuno, Koji Mori, Koji Mukai, Hiroshi Murakami, Richard Mushotzky, Hiroshi Nakajima, Kazuhiro Nakazawa, Jan-Uwe Ness, Kumiko Nobukawa, Masayoshi Nobukawa, Hirofumi Noda, Hirokazu Odaka, Shoji Ogawa, Anna Ogorzalek, Takashi Okajima, Naomi Ota, Stephane Paltani, Robert Petre, Paul Plucinsky, Frederick S. Porter, Katja Pottschmidt, Kosuke Sato, Toshiki Sato, Makoto Sawada, Hiromi Seta, Megumi Shidatsu, Aurora Simionescu, Randall Smith, Hiromasa Suzuki, Andrew Szymkowiak, Hiromitsu Takahashi, Mai Takeo, Toru Tamagawa, Keisuke Tamura, Takaaki Tanaka, Atsushi Tanimoto, Makoto Tashiro, Yukikatsu Terada, Yuichi Terashima, Yohko Tsuboi, Masahiro Tsujimoto, Hiroshi Tsunemi, Takeshi G. Tsuru, Ayşegül Tümer, Hiroyuki Uchida, Nagomi Uchida, Yuusuke Uchida, Hideki Uchiyama, Yoshihiro Ueda, Shinichiro Uno, Jacco Vink, Shin Watanabe, Brian J. Williams, Satoshi Yamada, Shinya Yamada, Hiroya Yamaguchi, Kazutaka Yamaoka, Noriko Yamasaki, Makoto Yamauchi, Shigeo Yamauchi, Tahir Yaqoob, Tomokage Yoneyama, Tessei Yoshida, Mihoko Yukita, Ian Drury, Julie Hlavacek-Larrondo, Julian Meunier, Kostas Migkas, Lior Shefler, Phillip C. Stancil, Nhut Truong, Shutaro Ueda, Benjamin Vigneron, John ZuHone, Congyao Zhang, Annie Heinrich, Irina Zhuravleva, Elena Bellomi
    Nature, 650(8101) 309-313, Jan 28, 2026  Peer-reviewed
  • Yoshiaki Kanemaru, Ryo Iizuka, Yoshitomo Maeda, Takashi Okajima, Takayuki Hayashi, Kazuhiro Kiyokane, Yuto Nihei, Takashi Kominato, Manabu Ishida, Chikara Natsukari, Shin Watanabe, Kousuke Sato, Yukikatsu Terada, Katsuhiro Hayashi, Chris Baluta, Tessei Yoshida, Akio Hoshino, Shoji Ogawa, Kotaro Fukushima, Hiromitsu Takahashi, Masayoshi Nobukawa, Tsunefumi Mizuno, Kazuhiro Nakazawa, Shin’ichiro Uno, Ken Ebisawa, Satoshi Eguchi, Satoru Katsuda, Aya Kubota, Naomi Ota, Megumi Shidatsu, Atsushi Tanimoto, Yuichi Terashima, Yohko Tsuboi, Yuusuke Uchida, Hideki Uchiyama, Shigeo Yamauchi, Yoneyama Tomokage, Satoshi Yamada, Nagomi Uchida, Rie Sato, Matthew P. Holland, Michael Loewenstein, Eric D. Miller, Tahir Yaqoob, Robert S. Hill, Morgan D. Waddy, Mark M. Mekosh, Joseph B. Fox, Isabella S. Brewer, Emily Aldoretta, Makoto Tashiro, Kenichi Toda, Hironori Maejima
    Journal of Astronomical Telescopes, Instruments, and Systems, 11(04), Dec 18, 2025  Peer-reviewed
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Misc.

 306
  • 勝田哲, 品川裕之, 金丸善朗, 森浩二, 鈴木寛大, 田代信, 望月優子, 望月優子, 大城勇憲, 信川久実子, 中澤知洋, 三好由純, MILLER Eric D., 峠千尋, 陣英克, 三好勉信, 藤原均, PETRE Robert, BEHAR Ehud
    日本天文学会年会講演予稿集, 2025, 2025  
  • 寺田幸功, 寺田幸功, 田代信, 田代信, 高橋弘充, 信川正順, 水野恒史, 宇野伸一郎, 中澤知洋, 久保田あや, 渡辺伸, 飯塚亮, 佐藤理江, 林克洋, 米山友景, 吉田鉄生, 金丸善朗, 小川翔司, 星野晶夫, 福島光太郎, BALUTA Chris, 海老沢研, 江口智士, 勝田哲, 太田直美, 志達めぐみ, 谷本敦, 寺島雄一, 坪井陽子, 内田和海, 内田悠介, 内山秀樹, 山田智史, 山内茂雄, HOLLAND Matt, LOEWENSTEIN Michael, MILLER Eric, YAQOOB Tahir
    宇宙航空研究開発機構研究開発報告 JAXA-RR-(Web), (24-004), 2025  
  • 小川翔司, 金丸善朗, 林克洋, 福島光太郎, 吉田鉄生, 寺田幸功, 田代信, 高橋弘充, 水野恒史, 深沢泰司, 信川正順, 宇野伸一郎, 中澤知洋, 大宮悠希, 大熊佳吾, 内山秀樹, 久保田あや, 勝田哲, 本上侑吾, 寺島雄一, 志達めぐみ, 新居田祐基, 高木利紘, 山内茂雄, 太田直美, 白木天音, 鈴木那梨, 山田智史, 坪井陽子, 米山友景, 内田悠介, 江口智士, 谷本敦, 善本真梨那, 飯塚亮, 内田和海, 海老沢研, 渡辺伸, HOLLAND Matt, YAQOOB Tahir, BALUTA Chris, LOEWENSTEIN Michael, LOEWENSTEIN Michael, MILLER Eric
    日本天文学会年会講演予稿集, 2025, 2025  
  • 寺田, 幸功, 田代, 信, 高橋, 弘充, 信川, 正順, 水野, 恒史, 宇野, 伸一郎, 久保田, あや, 中澤, 知洋, 渡辺, 伸, 飯塚, 亮, 佐藤, 理江, 林, 克洋, 米山, 友景, 吉田, 鉄生, 金丸, 善朗, 小川, 翔司, BALUTA, Chris, 海老沢, 研, 江口, 智士, 勝田, 哲, 北口, 貴雄, 太田, 直美, 志達, めぐみ, 谷本, 敦, 寺島, 雄一, 坪井, 陽子, 内田, 和海, 内田, 悠介, 内山, 秀樹, 山田, 智史, 山内, 茂雄, HOLLAND, Matt, LOEWENSTEIN, Michael, MILLER, Eric, YAQOOB, Tahir
    2023年度 宇宙科学情報解析シンポジウム, Feb, 2024  
  • 田代信, 寺田幸功, 前島弘則, 戸田謙一, 山口弘悦, 竹井洋, 冨田洋, 藤本龍一, 辻本匡弘, 渡辺伸, KELLEY R., REICHENTHAL L., HARTZ L., SNEIDERMAN G., PETRE R., WILLIAMS B., HOLLAND M., LOEWENSTEIN M., 松下恭子, GUAINAZZI M., COSTANTINI E., 石崎欣尚, 森浩二, 中嶋大, MILLER E., 澤田真理
    日本天文学会年会講演予稿集, 2024, 2024  Lead author
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Presentations

 101
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Teaching Experience

 67
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Professional Memberships

 2

Research Projects

 16
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Social Activities

 1
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