保健衛生学部　リハビリテーション学科
  1. Researcher List
  2. Akihiro Furuzawa

Akihiro Furuzawa

  (古澤 彰浩)

Profile Information

Affiliation
School of Medicine Faculty of Medicine, Fujita Health University
Degree
博士（理学）(名古屋大学)
J-GLOBAL ID
200901003971539256
researchmap Member ID
6000001840

Research Interests

 8

Research Areas

 4

Research History

 1

Education

 1

Papers

 164
  • 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, Elena Bellomi, Ian Drury, Annie Heinrich, Julie Hlavacek-Larrondo, Julian Meunier, Konstantinos Migkas, Lior Shefler, Phillip C. Stancil, Nhut Truong, Benjamin Vigneron, Congyao Zhang, John ZuHone
    Astronomy & Astrophysics, Jun 22, 2026  Peer-reviewed
    The intracluster medium (ICM) is rich in chemical elements, produced by core-collapse (SNcc) and Type Ia supernovae (SNIa) over the last ∼12 Gyr. While cluster outskirts are uniformly enriched with Fe at ∼0.3 solar, strongly suggesting that the gas had been pre-enriched during or before the assembly of galaxies into clusters, the Fe abundance is known to centrally increase in the core of relaxed clusters. The origin of these central Fe peaks however, as well as the apparent presence of mysterious drops previously reported in the very centre of a number of systems, remain to be clarified.In this paper, we address these two questions by measuring the spatial distribution of Fe and its relative Si/Fe, S/Fe, Ar/Fe, Ca/Fe, Cr/Fe, Mn/Fe, and Ni/Fe ratios in the X-ray bright, nearby Perseus cluster.We take advantage of the unprecedented spectral resolution (∼5 eV) offered by the Resolve microcalorimeter on board which observed four distinct pointings of Perseus out to ∼250 kpc (∼0.2r_500) during its performance verification phase.Although the presence of an X-ray bright AGN challenges a precise quantification of absolute abundances in the very core, our baseline analysis rules out a strong drop with $>2σ$ confidence, at variance with previous charge-coupled device (CCD) measurements. In addition, we find a remarkable spatial uniformity of X/Fe ratios, supporting the idea of negligible late SNIa enrichment from the brightest cluster galaxy NGC,1275. We also compare the overall chemical composition of the Perseus ICM with SNcc and SNIa nucleosynthesis yield models, finding that the co-existence of two separate SNIa enrichment channels is not needed to reproduce the ICM ratios satisfactorily.
  • Marc Audard, Hisamitsu Awaki, Ralf Ballhausen, Aya Bamba, Ehud Behar, Rozenn Boissay-Malaquin, Laura Brenneman, Gregory V. Brown, Michael F. Corcoran, 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, Emi Goto, Liyi Gu, Matteo Guainazzi, Kouichi Hagino, Kenji Hamaguchi, Isamu Hatsukade, Katsuhiro Hayashi, Takayuki Hayashi, Natalie Hell, Edmund Hodges-Kluck, Ann Hornschemeier, Yuto Ichinohe, Shun Inoue, Daiki Ishi, Manabu Ishida, Yukiko Ishihara, Kumi Ishikawa, Yoshitaka Ishisaki, Francisco Junqueira, Jelle Kaastra, Timothy Kallman, Yoshiaki Kanemaru, Erin Kara, Satoru Katsuda, Richard L. Kelley, Caroline A. 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, Bert Vander Meulen, Eric D. Miller, Jon M. Miller, Ikuyuki Mitsuishi, Asca Miyamoto, 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
    The Astrophysical Journal, 1003(2) 156-156, May 22, 2026  Peer-reviewed
    Abstract The supermassive binary system, η Carinae, is experiencing enormous wind-driven mass loss at a rate unparalleled in the rest of the Galaxy. Their wind–wind collision (WWC) continuously produces shock heated, X-ray-emitting plasmas. The XRISM X-ray observatory observed the system in 2023 and 2024 when the X-ray emission began to increase toward periastron passage in 2025. This paper reports unprecedentedly high-resolution X-ray spectra in the Fe K α band between 6.2 and 7.1 keV, obtained with the Resolve X-ray microcalorimeter. The hydrogen-like (Ly α ) and helium-like (He α ) lines reveal three velocity components. Two of them are broadened with maximum velocities of 2000–3000 km s −1 , likely originating from the postshock companion wind. The other is relatively narrow, with a Gaussian broadening of only ∼290 km s −1 in 1 σ , which may originate from the postshock companion wind at the WWC stagnation point or penetrating the primary wind. The Fe fluorescent lines exhibit a moderate blueshift and broadening with velocities at 100–200 km s −1 , consistent with the primary wind’s velocity field. The spectra also confirm a Compton shoulder of the He α line complex for the first time. Both fluorescing and scattering spectral profiles indicate that the binary system is seen from the companion side during these observations. The flux ratio of the Compton-scattering emission to the fluorescent line suggests substantial hydrogen depletion of the primary wind, expected from CNO-cycled hydrogen nuclear fusion gas.
  • 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, Teruaki Enoto, Satoshi Eguchi, Yuichiro Ezoe, Adam Foster, Ryuichi Fujimoto, Yutaka Fujita, Yasushi Fukazawa, Kotaro Fukushima, Akihiro Furuzawa, Luigi Gallo, Javier A. Garcia, 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 Scott 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, Irina Zhuravleva, Kanta Fujiwara, Takuma Izumi, Taiki Kawamuro, Keiichi Maeda, Yuya Nakatani, Frits Paerels, Ryosuke Uematsu, Bert Vander Meulen
    Nature Astronomy, 10(6) 880-891, Mar 31, 2026  Peer-reviewed
  • 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 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, Irina Zhuravleva, Kazuki Ampuku, Erin Boettcher, Skylar Grayson, Gabriel Grell, Peter Kosec, Seiya Sasamata, Evan Scannapieco
    Nature, 651(8107) 909-913, Mar 25, 2026  Peer-reviewed
  • 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.
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Misc.

 1
  • 高橋, 弘充, ABARR, Quin, 粟木, 久光, BARING, Matthew, BOSE, Richard, BRAUN, Dana, DE, GERONIMO Gianluigi, DOWKNOTT, Paul, ELLIOT, John, 榎戸, 輝揚, ERRAND, Manel, 深沢, 泰司, 古澤, 彰浩, GADSON, Thomas, GAU, Epharaim, GUARINO, Victor, 郡司, 修一, HALL, Kenny, HARMON, Keon, 服部, 兼吾, 林田, 清, HEATWOLE, Scott, HOSSEN, Arman, 今里, 郁弥, 石橋, 和紀, 石田, 学, LYER, Nirmal Kumar, KISLAT, Fabian, MOZSI, Kiss, 北口, 貴雄, KOTSIFAKIS, David, KRAWCZYNSKI, Henric, LANZI, James, LISALDA, Lindsey, 前田, 良知, 眞武, 寛人, 松本, 浩典, 峯田, 大晴, 宮澤, 拓也, 水野, 恒史, 岡島, 崇, PASTRANI, Izabella, PEARCE, Mark, PETERSON, Zachary, PURDY, Chris, RAUCH, Brian, RYDE, Felix, 斎藤, 芳隆, SHREEVES, Chris, SIMBUERGER, Garry, SNOW, Carl, SPOONER, Sean, STANA, Theodor-Adrian, STUCHILK, David, 武田, 朋志, 武尾, 舞, 玉川, 徹, 田村, 啓輔, 常深, 博, 内田, 和海, 内田, 悠介, 内山, 慶祐, VINCENT, Brett, WEST, Andrew, WULF, Eric, 山本, 龍哉, 吉田, 勇登, TAKAHASHI, Hiromitsu, AWAKI, Hisamitsu, ENOTO, Teruaki, FUKAZAWA, Yasushi, FURUZAWA, Akihiro, GUNJI, Shuichi, HATTORI, Kengo, HAYASHIDA, Kiyoshi, IMAZATO, Fumiya, ISHIBASHI, Kazunori, ISHIDA, Manabu, MOZI, Kiss, KITAGUCHI, Takao, MAEDA, Yoshitomo, MATAKE, Hiroto, MATSUMOTO, Hironori, MINETA, Taisei, MIYAZAWA, Takuya, MIZUNO, Tsunefumi, OKAJIMA, Takashi, SAITO, Yoshitaka, SIMBURGER, Garry, STUCHKIH, David, TAKEDA, Tomoshi, TAKEO, Mai, TAMAGAWA, Toru, TAMURA, Keisuke, TSUNEMI, Hiroshi, UCHIDA, Nagomi, UCHIDA, Yuusuke, UCHIYAMA, Keisuke, YAMAMOTO, Ryuya, YOSHIDA, Yuto
    大気球シンポジウム: 2020年度 = Balloon Symposium: 2020, Nov, 2020  
    大気球シンポジウム 2020年度（2020年11月5-6日. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)）, 相模原市, 神奈川県 Balloon Symposium 2020 (November 5-6, 2020. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS)), Sagamihara, Kanagawa Japan 著者人数: 67名 資料番号: SA6000151012 レポート番号: isas20-sbs-012

Presentations

 61
  • 倉本春希, 松本浩典, 小高裕和, 袴田知宏, 島耕平, 宮本愛子, 河村穂登, 村上海都, 内田賢佑, 高塚紗弥菜, 長尾梓生, 宮澤拓也, 石橋和紀, 伊師大貴, 前田良知, 石田学, 宮本明日香, 田中虎次郎, 内田悠介, 呉屋和保, 横田雅人, 高橋弘充, 粟木久光, 古澤彰浩, OKAJIMA Takashi, KRAWCZYNSKI Henric, KISLAT Fabian, PEARCE Mark, 上杉健太朗, 星野真人
    日本天文学会年会講演予稿集, 2025
  • 高橋, 弘充, AF MALMBORG, Filip, 青柳, 美緒, 粟木, 久光, BOSE, Richard, BRAUN, Dana, CHUN, Sohee, DE GERONIMO, Gianluigi, 榎戸, 輝揚, ERRANDO, Manel, 深沢, 泰司, 古澤, 彰浩, GADSON, Thomas, GAU, Epharaim, GUARINO, Victor, 郡司, 修一, 袴田, 知宏, 林, 多佳由, HEATWOLE, Scott, HOSSEN, Arman, HU, Kun, 今村, 竜太, 今澤, 遼, 伊師, 大貴, 石橋, 和紀, 石田, 学, 石渡, 幸太, IYER, Nirmal Kumar, HARMON, Keon, 鴨川, 航, KISLAT, Fabian, KISS, Mozsi, 北口, 貴雄, KLEPPER, Kassi, KRAWCZYNSKI, Henric, 倉本, 春希, LANZI, James, LISALDA, Lindsey, 前田, 良知, 眞武, 寛人, 松本, 浩典, 松本, 岳人, 宮本, 明日香, 宮澤, 拓也, 水野, 恒史, 岡島, 崇, PEARCE, Mark, PETERSON, Zachary, RAHBARDAR MOJAVER, Mehrnossh, RAUCH, Brian, RODRIGUEZ CAVERO, Nicole, RYDE, Felix, 斎藤, 芳隆, 阪本, 菜月, 島, 耕平, 白濱, 健太郎, SIMBURGER, Garry, SPOONER, Sean, STANA, Theodor-Adrian, STUCHLIK, David, 武尾, 舞, 玉川, 徹, 田村, 啓輔, 田中, 虎次郎, 常深, 博, 内田, 和海, 内田, 悠介, WEST, Andrew, WULF, Eric, 善本, 真梨那, XL-Caliburチーム,
    大気球シンポジウム: 2024年度, Oct, 2024, 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS)
    レポート番号: isas24-sbs-008
  • 倉本春希, 松本浩典, 鴨川航, 善本真梨那, 袴田知宏, 青柳美緒, 石渡幸太, 島耕平, 白濱健太郎, 野田博文, 林田清, 常深博, 宮澤拓也, 石橋和紀, 伊師大貴, 前田良知, 石田学, 宮本明日香, 松本岳人, 田中虎次郎, 武尾舞, 内田悠介, 今澤遼, 阪本菜月, 高橋弘充, 今村竜太, 粟木久光, 古澤彰浩, 岡島崇, 田村啓輔, 林多佳由, KRAWCZYNSKI Henric, KISLAT Fabian
    日本天文学会年会講演予稿集, 2024
  • 三浦裕一, 齋藤芳子, 安田淳一郎, 中村泰之, 古澤彰浩, 千代勝実, 伊東正人, 小西哲郎, 大薮進喜
    日本物理学会講演概要集(CD-ROM), 2024
  • 高橋弘充, AF MALMBORG Filip, AF MALMBORG Filip, 青柳美緒, 粟木久光, BOSE Richard, BRAUN Dana, CHUN Sohee, DE GERONIMO Gianluigi, 榎戸輝揚, ERRANDO Manel, 深沢泰司, 古澤彰浩, GADSON Thomas, GAU Epharaim, GUARINO Victor, 郡司修一, 袴田知宏, HEATWOLE Scott, HOSSEN Arman, HU Kun, 今村竜太, 今澤遼, 石橋和紀, 石田学, 石渡幸太, IYER Nirmal Kumar, IYER Nirmal Kumar, HARMON Keon, 鴨川航, KISLAT Fabian, KISS Mozsi, KISS Mozsi, 北口貴雄, KLEPPER Kassi, KLEPPER Kassi, KRAWCZYNSKI Henric, 倉本春希, LANZI James, LISALDA Lindsey, 前田良知, 眞武寛人, 松本浩典, 松本岳人, 宮本明日香, 宮澤拓也, 水野恒史, 岡島崇, PEARCE Mark, PEARCE Mark, PETERSON Zachary, MOJAVER Mehrnossh Rahbardar, RAUCH Brian, CAVERO Nicole Rodriguez, RYDE Felix, RYDE Felix, 斎藤芳隆, 阪本菜月, 島耕平, 白濱健太郎, SIMBURGER Garry, SPOONER Sean, STANA Theodor-Adrian, STANA Theodor-Adrian, STUCHLIK David, 武尾舞, 玉川徹, 田村啓輔, 田中虎次郎, 常深博, 内田和海, 内田悠介, WEST Andrew, WULF Eric, 善本真梨那
    日本物理学会講演概要集(CD-ROM), 2024
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