論文 - 田中 孝明
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Rapid Deceleration of Blast Waves Witnessed in Tycho’s Supernova Remnant 査読あり
T. Tanaka, T. Okuno, H. Uchida, H. Yamaguchi, S. H. Lee, K. Maeda, B. J. Williams
The Astrophysical Journal Letters 906 ( 1 ) L3 2021年
共著
担当区分：筆頭著者, 責任著者
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Soft X-ray Imager aboard Hitomi (ASTRO-H) 査読あり
T. Tanaka, H. Uchida, H. Nakajima, H. Tsunemi, K. Hayashida, T. G. Tsuru, T. Dotani, R. Nagino, S. Inoue, S. Katada, R. Washino, M. Ozaki, H. Tomida, C. Natsukari, S. Ueda, M. Iwai, K. Mori, M. Yamauchi, I. Hatsukade, Y. Nishioka, E. Isoda, M. Nobukawa, J. S. Hiraga, T. Kohmura, H. Murakami, K. K. Nobukawa, A. Bamba, J. P. Doty
Journal of Astronomical Telescopes, Instruments, and Systems 4 ( 1 ) 011211 2018年
共著
担当区分：筆頭著者, 責任著者
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NuSTAR Detection of Nonthermal Bremsstrahlung from the Supernova Remnant W49B 査読あり
T. Tanaka, H. Yamaguchi, D. R. Wik, F. A. Aharonian, A. Bamba, D. Castro, A. R. Foster, R. Petre, J. Rho, R. K. Smith, H. Uchida, Y. Uchiyama, B. J. Williams
The Astrophysical Journal Letters 866 ( 2 ) L26 2018年
共著
担当区分：筆頭著者, 責任著者
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Detection of the Characteristic Pion-Decay Signature in Supernova Remnants 査読あり
M. Ackermann, et al. (including T. Tanaka as a corresponding author)
Science 339 ( 6121 ) 807 - 811 2013年
共著
担当区分：責任著者
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Gamma-Ray Emission from the Shell of Supernova Remnant W44 Revealed by the Fermi LAT 査読あり
A. A. Abdo, et al. (including T. Tanaka as a corresponding author),
Science 327 ( 5969 ) 1103 - 1106 2010年
共著
担当区分：責任著者
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XRISM Reveals Low Nonthermal Pressure in the Core of the Hot, Relaxed Galaxy Cluster A2029 査読あり
XRISM Collaboration (including T. Tanaka)
The Astrophysical Journal Letters 982 ( 1 ) L5 2025年3月
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Soft X-ray Imager of the Xtend system on board XRISM 査読あり
K. Noda, et al. (including T. Tanaka as a corresponding author)
Publications of the Astronomical Society of Japan 2025年3月
担当区分：責任著者
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A detailed study on spectroscopic performance of SOI pixel detector with a pinned depleted diode structure for X-ray astronomy 査読あり
M. Yukumoto, K. Mori, A. Takeda, Y. Nishioka, M. Kimura, Y. Fuchita, T. Yoshida, T. G. Tsuru, I. Kurachi, K. Hagino, Y. Arai, T. Kohmura, T. Tanaka, K. K. Nobukawa
Nuclear Instruments and Methods in Physics Research A 1072 170203 2025年3月
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The bulk motion of gas in the core of the Centaurus galaxy cluster 査読あり 国際共著
XRISM Collaboration (including T. Tanaka)
Nature 638 ( 8050 ) 365 - 369 2025年2月
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Detection of Extended X-Ray Emission around the PeVatron Microquasar V4641 Sgr with XRISM
Hiromasa Suzuki, Naomi Tsuji, Yoshiaki Kanemaru, Megumi Shidatsu, Laura Olivera-Nieto, Samar Safi-Harb, Shigeo S. Kimura, Eduardo de la Fuente, Sabrina Casanova, Kaya Mori, Xiaojie Wang, Sei Kato, Dai Tateishi, Hideki Uchiyama, Takaaki Tanaka, Hiroyuki Uchida, Shun Inoue, Dezhi Huang, Marianne Lemoine-Goumard, Daiki Miura, Shoji Ogawa, Shogo B. Kobayashi, Chris Done, Maxime Parra, Maria Díaz Trigo, Teo Muñoz-Darias, Montserrat Armas Padilla, Ryota Tomaru, Yoshihiro Ueda
The Astrophysical Journal Letters 978 ( 2 ) L20 - L20 2025年1月
出版者・発行元：American Astronomical Society
Abstract
A recent report on the detection of very-high-energy gamma rays from V4641 Sagittarii (V4641 Sgr) up to ≈0.8 PeV has made it the second confirmed “PeVatron” microquasar. Here we report on the observation of V4641 Sgr with X-Ray Imaging and Spectroscopy Mission (XRISM) in 2024 September. Thanks to the large field of view and low background, the CCD imager Xtend successfully detected for the first time X-ray extended emission around V4641 Sgr with a significance of ≳4.5σ and >10σ based on our imaging and spectral analysis, respectively. The spatial extent is estimated to have a radius of 7′ ± 3′ (13 ± 5 pc at a distance of 6.2 kpc) assuming a Gaussian-like radial distribution, which suggests that the particle acceleration site is within ~10 pc of the microquasar. If the X-ray morphology traces the diffusion of accelerated electrons, this spatial extent can be explained by either an enhanced magnetic field (∼80 μG) or a suppressed diffusion coefficient (∼10<sup>27</sup> cm<sup>2</sup> s<sup>−1</sup> at 100 TeV). The integrated X-ray flux, (4–6) × 10<sup>−12</sup> erg s<sup>−1</sup> cm<sup>−2</sup> (2–10 keV), would require a magnetic field strength higher than the Galactic mean (≳8 μG) if the diffuse X-ray emission originates from synchrotron radiation and the gamma-ray emission is predominantly hadronic. If the X-rays are of thermal origin, the measured extension, temperature, and plasma density can be explained by a jet with a luminosity of ∼2 × 10<sup>39</sup> erg s<sup>−1</sup>, which is comparable to the Eddington luminosity of this system.その他リンク： https://iopscience.iop.org/article/10.3847/2041-8213/ad9d11/pdf
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Overionized plasma in the supernova remnant Sagittarius A East anchored by XRISM observations 査読あり
XRISM Collaboration (including T. Tanaka)
Publications of the Astronomical Society of Japan 77 ( 1 ) L1 - L8 2024年12月
DOI： 10.1093/pasj/psae111
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The XRISM/Resolve View of the Fe K Region of Cyg X-3 査読あり 国際共著
XRISM Collaboration (including T. Tanaka)
The Astrophysical Journal Letters 977 ( 2 ) L34 2024年12月
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Recent Results on Supernova Remnants at Highest Energies 招待あり 査読あり
T. Tanaka
Proceedings of Science 417 022 2024年12月
担当区分：筆頭著者
DOI： 10.22323/1.417.0022
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The XRISM first-light observation: Velocity structure and thermal properties of the supernova remnant N 132D 査読あり 国際共著
XRISM Collaboration (including T. Tanaka)
Publications of the Astronomical Society of Japan 76 ( 6 ) 1186 - 1201 2024年10月
DOI： 10.1093/pasj/psae080
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XRISM Spectroscopy of the Fe Kα Emission Line in the Seyfert Active Galactic Nucleus NGC 4151 Reveals the Disk, Broad-line Region, and Torus 査読あり 国際共著
XRISM Collaboration (including T. Tanaka)
The Astrophysical Journal Letters 973 ( 1 ) L25 2024年9月
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Evaluation of the X-ray SOI pixel detector with the on-chip ADC
Hiroumi Matsuhashi, Kouichi Hagino, Aya Bamba, Ayaki Takeda, Masataka Yukumoto, Koji Mori, Yusuke Nishioka, Takeshi Go Tsuru, Mizuki Uenomachi, Tomonori Ikeda, Masamune Matsuda, Takuto Narita, Hiromasa Suzuki, Takaaki Tanaka, Ikuo Kurachi, Takayoshi Kohmura, Yusuke Uchida, Yasuo Arai, Shoji Kawahito
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 1064 169426 - 169426 2024年7月
出版者・発行元：Elsevier BV
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Search for Synchrotron Emission from Secondary Electrons of Proton–Proton Interactions in Galactic PeVatron Candidate HESS J1641-463 査読あり 国際共著
N. Tsuji, T. Tanaka, S. Safi-Harb, F. Aharonian, S. Casanova, R. Kothes, E. Moulin, H. Uchida, Y. Uchiyama
The Astrophysical Journal 967 ( 2 ) 138 2024年6月
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Design study and spectroscopic performance of SOI pixel detector with a pinned depleted diode structure for X-ray astronomy 査読あり
M. Yukumoto, K. Mori, A. Takeda, Y. Nishioka, S. Yonemura, D. Izumi, U. Iwakiri, T. G. Tsuru, I. Kurachi, K. Hagino, Y. Arai, T. Kohmura, T. Tanaka, M. Kimura, Y. Fuchita, T. Yoshida, T. Ikeda
Nuclear Instruments and Methods in Physics Research A 1060 169033 2024年3月
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Three-dimensional Velocity Diagnostics to Constrain the Type Ia Origin of Tycho's Supernova Remnant 査読あり
H. Uchida, T. Kasuga, K. Maeda, S.-H. Lee, T. Tanaka, A. Bamba
The Astrophysical Journal 962 ( 2 ) 159 2024年2月
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Exploring the Circumstellar Environment of Tycho's Supernova Remnant. I. The Hydrodynamic Evolution of the Shock 査読あり
R. Kobashi, S.-H. Lee, T. Tanaka, K. Maeda
The Astrophysical Journal 961 ( 1 ) 32 2024年1月