論文 - 廿日出 勇
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Concept of the X-ray Astronomy Recovery Mission 査読あり
Tashiro, Makoto, Maejima, Hironori, Toda, Kenichi, 他
Proceedings of the SPIE 10699 2018年7月
記述言語：英語 掲載種別：研究論文（国際会議プロシーディングス）
DOI： 10.1117/12.2309455
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Soft x-ray imaging telescope (Xtend) onboard X-ray Astronomy Recovery Mission (XARM) 査読あり
Hayashida, Kiyoshi, Tomida, Hiroshi, Mori, Koji, 他
Proceedings of the SPIE 10699 2018年7月
記述言語：英語 掲載種別：研究論文（国際会議プロシーディングス）
DOI： 10.1117/12.2311446
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Hitomi X-ray observation of the pulsar wind nebula G21.5-0.9 査読あり
Hitomi Collaboration, Aaronian, Felix, Akamatsu, Hiroki, 他
Publications of the Astronomical Society of Japan 70 ( 3 ) 2018年6月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psy027
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Hitomi (ASTRO-H) X-ray Astronomy Satellite 査読あり
Takahashi, Tadayuki, Kokubun, Motohide, Mitsuda, Kazuhisa, 他
Journal of Astronomical Telescopes, Instruments, and Systems 4 2018年4月
記述言語：英語 掲載種別：研究論文（学術雑誌）
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In-orbit performance of the soft X-ray imaging system aboard Hitomi (ASTRO-H) 査読あり
Nakajima, H., Maeda, Y., Uchida, H., et al.
Publications of the Astronomical Society of Japan 70 ( 2 ) 21 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psx116
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Glimpse of the highly obscured HMXB IGR J16318-4848 with Hitomi 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Publications of the Astronomical Society of Japan 70 ( 2 ) 17 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psx154
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Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Publications of the Astronomical Society of Japan 70 ( 2 ) 16 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psx151
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Hitomi X-ray studies of giant radio pulses from the Crab pulsar 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Publications of the Astronomical Society of Japan 70 ( 2 ) 15 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psx083
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Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Publications of the Astronomical Society of Japan 70 ( 2 ) 14 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psx072
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Hitomi observation of radio galaxy NGC 1275: The first X-ray microcalorimeter spectroscopy of Fe-Kalpha line emission from an active galactic nucleus 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Publications of the Astronomical Society of Japan 70 ( 2 ) 13 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psx147
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Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Publications of the Astronomical Society of Japan 70 ( 2 ) 12 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psx156
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Temperature structure in the Perseus cluster core observed with Hitomi 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Publications of the Astronomical Society of Japan 70 ( 2 ) 11 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psy004
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Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Publications of the Astronomical Society of Japan 80 ( 2 ) 10 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psx127
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Atmospheric gas dynamics in the Perseus cluster observed with Hitomi 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Publications of the Astronomical Society of Japan 70 ( 2 ) 9 2018年3月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1093/pasj/psx138
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Soft X-ray Imager aboard Hitomi (ASTRO-H) 査読あり
Tanaka, T., Uchida, H., Nakajima, H., et al.
Journal of Astronomical Telescopes, Instruments, and Systems 4 ( 011211 ) 2018年1月
記述言語：英語 掲載種別：研究論文（学術雑誌）
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X線天文衛星代替機(XARM) 搭載の軟Ｘ線撮像装置の開発状況
幸村 孝由, 村上 弘志, 山内 誠, 廿日出 勇, 萩野 浩一, 石田 学, 前田 良知, 内山 秀樹, 山岡 和貴, 松本 浩典, 信川 正順, 林田 清, 信川 久美子, 平賀 純子, 小林 翔悟, 堂谷 忠靖, 尾崎 正伸, 常深 博, 他 XARM 軟X線撮像装置開発チーム, 冨田 洋, 森 浩二, 岡島 崇, 中嶋 大, 鶴 剛, 田中 孝明, 内田 裕之
日本物理学会講演概要集 73 ( 0 ) 495 - 495 2018年
記述言語：日本語 掲載種別：研究論文（学術雑誌） 出版者・発行元：一般社団法人 日本物理学会
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Solar abundance ratios of the iron-peak elements in the Perseus cluster 査読あり
Aharonian, F., Akamatsu, H., Akimoto, F., et al.
Nature 551 ( 7681 ) 478 - 480 2017年11月
記述言語：英語 掲載種別：研究論文（学術雑誌）
DOI： 10.1038/nature24301
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Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster 査読あり
Aharonian F., Akamatsu H., Akimoto F., Allen S., Angelini L., Arnaud K., Audard M., Awaki H., Axelsson M., Bamba A., Bautz M., Blandford R., Bulbul E., Brenneman L., Brown G., Cackett E., Chernyakova M., Chiao M., Coppi P., Costantini E., Plaa J., Herder J., Done C., Dotani T., Ebisawa K., Eckart M., Enoto T., Ezoe Y., Fabian A., Ferrigno C., Foster A., Fujimoto R., Fukazawa Y., Furuzawa A., Galeazzi M., Gallo L., Gandhi P., Giustini M., Goldwurm A., Gu L., Guainazzi M., Haba Y., Hagino K., Hamaguchi K., Harrus I., Hatsukade I., Hayashi K., Hayashi T., Hayashida K., Hiraga J., Hornschemeier A., Hoshino A., Hughes J., Ichinohe Y., Iizuka R., Inoue H., Inoue S., Inoue Y., Ishibashi K., Ishida M., Ishikawa K., Ishisaki Y., Itoh M., Iwai M., Iyomoto N., Kaastra J., Kallman T., Kamae T., Kara E., Kataoka J., Katsuda S., Katsuta J., Kawaharada M., Kawai N., Kelley R., Khangulyan D., Kilbourne C., King A., Kitaguchi T., Kitamoto S., Kitayama T., Kohmura T., Kokubun M., Koyama S., Koyama K., Kretschmar P., Krimm H., Kubota A.
Astrophysical Journal Letters 837 ( 1 ) 2017年3月
記述言語：英語 掲載種別：研究論文（学術雑誌） 出版者・発行元：Astrophysical Journal Letters
© 2017. The American Astronomical Society. All rights reserved. High-resolution X-ray spectroscopy with Hitomi was expected to resolve the origin of the faint unidentified E ≈ 3.5 keV emission line reported in several low-resolution studies of various massive systems, such as galaxies and clusters, including the Perseus cluster. We have analyzed the Hitomi first-light observation of the Perseus cluster. The emission line expected for Perseus based on the XMM-Newton signal from the large cluster sample under the dark matter decay scenario is too faint to be detectable in the Hitomi data. However, the previously reported 3.5 keV flux from Perseus was anomalously high compared to the sample-based prediction. We find no unidentified line at the reported high flux level. Taking into account the XMM measurement uncertainties for this region, the inconsistency with Hitomi is at a 99% significance for a broad dark matter line and at 99.7% for a narrow line from the gas. We do not find anomalously high fluxes of the nearby faint K line or the Ar satellite line that were proposed as explanations for the earlier 3.5 keV detections. We do find a hint of a broad excess near the energies of high-n transitions of S xvi (E ≃ 3.44 keV rest-frame) - a possible signature of charge exchange in the molecular nebula and another proposed explanation for the unidentified line. While its energy is consistent with XMM pn detections, it is unlikely to explain the MOS signal. A confirmation of this interesting feature has to wait for a more sensitive observation with a future calorimeter experiment.
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The quiescent intracluster medium in the core of the Perseus cluster 査読あり
Aharonian F., Akamatsu H., Akimoto F., Allen S., Anabuki N., Angelini L., Arnaud K., Audard M., Awaki H., Axelsson M., Bamba A., Bautz M., Blandford R., Brenneman L., Brown G., Bulbul E., Cackett E., Chernyakova M., Chiao M., Coppi P., Costantini E., De Plaa J., Den Herder J., Done C., Dotani T., Ebisawa K., Eckart M., Enoto T., Ezoe Y., Fabian A., Ferrigno C., Foster A., Fujimoto R., Fukazawa Y., Furuzawa A., Galeazzi M., Gallo L., Gandhi P., Giustini M., Goldwurm A., Gu L., Guainazzi M., Haba Y., Hagino K., Hamaguchi K., Harrus I., Hatsukade I., Hayashi K., Hayashi T., Hayashida K., Hiraga J., Hornschemeier A., Hoshino A., Hughes J., Iizuka R., Inoue H., Inoue Y., Ishibashi K., Ishida M., Ishikawa K., Ishisaki Y., Itoh M., Iyomoto N., Kaastra J., Kallman T., Kamae T., Kara E., Kataoka J., Katsuda S., Katsuta J., Kawaharada M., Kawai N., Kelley R., Khangulyan D., Kilbourne C., King A., Kitaguchi T., Kitamoto S., Kitayama T., Kohmura T., Kokubun M., Koyama S., Koyama K., Kretschmar P., Krimm H., Kubota A., Kunieda H., Laurent P.
Nature 535 ( 7610 ) 117 - 121 2016年7月
記述言語：英語 掲載種別：研究論文（学術雑誌） 出版者・発行元：Nature
© 2016 Macmillan Publishers Limited. All rights reserved. Clusters of galaxies are the most massive gravitationally bound objects in the Universe and are still forming. They are thus important probes of cosmological parameters and many astrophysical processes. However, knowledge of the dynamics of the pervasive hot gas, the mass of which is much larger than the combined mass of all the stars in the cluster, is lacking. Such knowledge would enable insights into the injection of mechanical energy by the central supermassive black hole and the use of hydrostatic equilibrium for determining cluster masses. X-rays from the core of the Perseus cluster are emitted by the 50-million-kelvin diffuse hot plasma filling its gravitational potential well. The active galactic nucleus of the central galaxy NGC 1275 is pumping jetted energy into the surrounding intracluster medium, creating buoyant bubbles filled with relativistic plasma. These bubbles probably induce motions in the intracluster medium and heat the inner gas, preventing runaway radiative cooling - a process known as active galactic nucleus feedback. Here we report X-ray observations of the core of the Perseus cluster, which reveal a remarkably quiescent atmosphere in which the gas has a line-of-sight velocity dispersion of 164 ± 10 kilometres per second in the region 30-60 kiloparsecs from the central nucleus. A gradient in the line-of-sight velocity of 150 ± 70 kilometres per second is found across the 60-kiloparsec image of the cluster core. Turbulent pressure support in the gas is four per cent of the thermodynamic pressure, with large-scale shear at most doubling this estimate. We infer that a total cluster mass determined from hydrostatic equilibrium in a central region would require little correction for turbulent pressure.
DOI： 10.1038/nature18627
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The ASTRO-H (Hitomi) X-ray astronomy satellite 査読あり
Takahashi T., Kokubun M., Mitsuda K., Kelley R., Ohashi T., Aharonian F., Akamatsu H., Akimoto F., Allen S., Anabuki N., Angelini L., Arnaud K., Asai M., Audard M., Awaki H., Axelsson M., Azzarello P., Baluta C., Bamba A., Bando N., Bautz M., Bialas T., Blandford R., Boyce K., Brenneman L., Brown G., Bulbul E., Cackett E., Canavan E., Chernyakova M., Chiao M., Coppi P., Costantini E., De Plaa J., Den Herder J., DiPirro M., Done C., Dotani T., Doty J., Ebisawa K., Eckart M., Enoto T., Ezoe Y., Fabian A., Ferrigno C., Foster A., Fujimoto R., Fukazawa Y., Furuzawa A., Galeazzi M., Gallo L., Gandhi P., Gilmore K., Giustini M., Goldwurm A., Gu L., Guainazzi M., Haas D., Haba Y., Hagino K., Hamaguchi K., Harayama A., Harrus I., Hatsukade I., Hayashi T., Hayashi K., Hayashida K., Hiraga J., Hirose K., Hornschemeier A., Hoshino A., Hughes J., Ichinohe Y., Iizuka R., Inoue Y., Inoue H., Ishibashi K., Ishida M., Ishikawa K., Ishimura K., Ishisaki Y., Itoh M., Iwata N., Iyomoto N., Jewell C., Kaastra J., Kallman T., Kamae T., Kara E., Kataoka J., Katsuda S., Katsuta J., Kawaharada M., Kawai N., Kawano T., Kawasaki S., Khangulyan D., Kilbourne C., Kimball M., King A.
Proceedings of SPIE - The International Society for Optical Engineering 9905 2016年7月
記述言語：英語 掲載種別：研究論文（国際会議プロシーディングス） 出版者・発行元：Proceedings of SPIE - The International Society for Optical Engineering
© 2016 SPIE. The Hitomi (ASTRO-H) mission is the sixth Japanese X-ray astronomy satellite developed by a large international collaboration, including Japan, USA, Canada, and Europe. The mission aimed to provide the highest energy resolution ever achieved at E > 2 keV, using a microcalorimeter instrument, and to cover a wide energy range spanning four decades in energy from soft X-rays to gamma-rays. After a successful launch on 2016 February 17, the spacecraft lost its function on 2016 March 26, but the commissioning phase for about a month provided valuable information on the on-board instruments and the spacecraft system, including astrophysical results obtained from first light observations. The paper describes the Hitomi (ASTRO-H) mission, its capabilities, the initial operation, and the instruments/spacecraft performances confirmed during the commissioning operations for about a month.
DOI： 10.1117/12.2232379