K. Sato N. Y. Yamasaki M. Ishida Y. Maeda K. Mitsuda Y. Ishisaki Y. Fujita Y. Ezoe I. Mitsuishi Y. Tawara K. Osato N. Kawai K. Matsushita D. Nagai K. Yoshikawa R. Fujimoto T. G. Tsuru N. Ota S. Yamada Y. Ichinohe Y. Uchida Y. Nakashima
Journal of Low Temperature Physics 209(5-6) 971-979 2022年12月
Takashi Hasebe Ryuta Imamura Masahiro Tsujimoto Hisamitsu Awaki Meng P. Chiao Ryuichi Fujimoto Leslie S. Hartz Gary A. Sneiderman Yoh Takei Susumu Yasuda
Proceedings of SPIE - The International Society for Optical Engineering 12181 2022年
Resolve is a payload hosting an x-ray microcalorimeter detector operated at 50 mK in the X-Ray Imaging and Spectroscopy Mission (XRISM), which is currently under development by an international collaboration and is planned to be launched in 2023. ...
Ryuta Imamura Masahiro Tsujimoto Hisamitsu Awaki Meng P. Chiao Ryuichi Fujimoto Yoshitaka Ishisaki Richard L. Kelley Caroline A. Kilbourne Frederick S. Porter Makoto Sawada Gary A. Sneiderman Yoh Takei Shinya Yamada
X-RAY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY X 12191 2022年
The Resolve instrument onboard the XRISM satellite is equipped with 6 x 6 x-ray microcalorimeter detectors aiming at an energy resolution of 7 eV (FWHM) at 5.9 keV. It is currently under development by an international collaboration and will be la...
Aharonian, F.A. Akamatsu, H. Akimoto, F. Allen, S.W. Angelini, L. Arnaud, K.A. Audard, M. Awaki, H. Axelsson, M. Bamba, A. Bautz, M.W. Blandford, R.D. Bulbul, E. Brenneman, L.W. Brown, G.V. Cackett, E.M. Chernyakova, M. Chiao, M.P. Coppi, P. Costantini, E. Plaa, J.D. Herder, J.-W.D. Done, C. Dotani, T. Ebisawa, K. Eckart, M.E. Enoto, T. Ezoe, Y. Fabian, A.C. Ferrigno, C. Foster, A.R. Fujimoto, R. Fukazawa, Y. Furuzawa, A. Galeazzi, M. Gallo, L.C. 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.E. Hoshino, A. Hughes, J.P. 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.S. Kallman, T. Kamae, T. Kara, E. Kataoka, J. Katsuda, S. Katsuta, J. Kawaharada, M. Kawai, N. Kelley, R.L. Khangulyan, D. Kilbourne, C.A. King, A.L. Kitaguchi, T. Kitamoto, S. Kitayama, T. Kohmura, T. Kokubun, M. Koyama, S. Koyama, K. Kretschmar, P. Krimm, H.A. Kubota, A. Kunieda, H. Laurent, P. Lebrun, F. Lee, S.-H. Leutenegger, M.A. Limousin, O. Loewenstein, M. Long, K.S. Lumb, D.H. Madejski, G.M. Maeda, Y. Maier, D. Makishima, K. Markevitch, M. Matsumoto, H. Matsushita, K. McCammon, D. McNamara, B.R. Mehdipour, M. Miller, E.D. Miller, J.M. Mineshige, S. Mitsuda, K. Mitsuishi, I. Miyazawa, T. Mizuno, T. Mori, H. Mori, K. Moseley, H. Mukai, K. Murakami, H. Murakami, T. Mushotzky, R.F. Nakagawa, T. Nakajima, H. Nakamori, T. Nakano, T. Nakashima, S. Nakazawa, K. Nobukawa, K. Nobukawa, M. Noda, H. Nomachi, M. Dell, S.L.O. Odaka, H. Ohashi, T. Ohno, M. OKajima, T. Ota, N. Ozaki, M. Paerels, F. Paltani, S. Parmar, A. Petre, R. Pinto, C. Pohl, M. Porter, F.S. Pottschmidt, K. Ramsey, B.D. Reynolds, C.S. Russell, H.R. Safi-Harb, S. Saito, S. Sakai, K. Sameshima, H. Sasaki, T. Sato, G. Sato, K. Sato, R. Sawada, M. Schartel, N. Serlemitsos, P.J. Seta, H. Shidatsu, M. Simionescu, A. Smith, R.K. Soong, Y. Stawarz, Ł. Sugawara, Y. Sugita, S. Szymkowiak, A.E. Tajima, H. Takahashi, H. Takahashi, T. Takeda, S. Takei, Y. Tamagawa, T. Tamura, K. Tamura, T. Tanaka, T. Tanaka, Y. Tanaka, Y. Tashiro, M. Tawara, Y. Terada, Y. Terashima, Y. Tombesi, F. Tomida, H. Tsuboi, Y. Tsujimoto, M. Tsunemi, H. Tsuru, T. Uchida, H. Uchiyama, H. Uchiyama, Y. Ueda, S. Ueda, Y. Ueno, S. Uno, S. Urry, C.M. Ursino, E. Vries, C.P.D. Watanabe, S. Werner, N. Wik, D.R. Wilkins, D.R. Williams, B.J. Yamada, S. Yamaguchi, H. Yamaoka, K. Yamasaki, N.Y. Yamauchi, M. Yamauchi, S. Yaqoob, T. Yatsu, Y. Yonetoku, D. Yoshida, A. Zhuravleva, I. Zoghbi, A.
Astrophysical Journal Letters 837(1) 2017年
X-ray spectroscopy with Hitomi was expected to resolve the origin of the faint unidentified E approximate to 3.5 keV emission line reported in several low-resolution studies of various massive systems, such as galaxies and clusters, including the ...
Caroline A. Kilbourne Joseph S. Adams Petar Arsenovic Travis Ayers Meng P. Chiao Michael J. DiPirro Megan E. Eckart Ryuichi Fujimoto John D. Kazeva Richard L. Kelley Kari L. Kripps Bruce Lairson Maurice A. Leutenegger Heidi Lopez Dan McCammon Daniel S. McGuinness Kazuhisa Mitsuda Samuel J. Moseley F. Scott Porter Andrea N. Schweiss Yoh Takei Rosemary S. Thorpe Tomomi Watanabe Noriko Y. Yamasaki Seiji Yoshida
SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY 9905 2016年 [査読有り]
The calorimeter array of the JAXA Astro-H (renamed Hitomi) Soft X-ray Spectrometer (SXS) was designed to provide unprecedented spectral resolution of spatially extended cosmic x-ray sources and of all cosmic x-ray sources in the Fe-K band around 6...
Aharonian, F. Akamatsu, H. Akimoto, F. Allen, S.W. Anabuki, N. Angelini, L. Arnaud, K. Audard, M. Awaki, H. Axelsson, M. Bamba, A. Bautz, M. Blandford, R. Brenneman, L. Brown, G.V. Bulbul, E. Cackett, E. Chernyakova, M. Chiao, M. Coppi, P. Costantini, E. De Plaa, J. Den Herder, J.-W. Done, C. Dotani, T. Ebisawa, K. Eckart, M. Enoto, T. Ezoe, Y. Fabian, A.C. 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. Lebrun, F. Lee, S.-H. Leutenegger, M. Limousin, O. Loewenstein, M. Long, K.S. Lumb, D. Madejski, G. Maeda, Y. Maier, D. Makishima, K. Markevitch, M. Matsumoto, H. Matsushita, K. McCammon, D. McNamara, B. Mehdipour, M. Miller, E. Miller, J. Mineshige, S. Mitsuda, K. Mitsuishi, I. Miyazawa, T. Mizuno, T. Mori, H. Mori, K. Moseley, H. Mukai, K. Murakami, H. Murakami, T. Mushotzky, R. Nagino, R. Nakagawa, T. Nakajima, H. Nakamori, T. Nakano, T. Nakashima, S. Nakazawa, K. Nobukawa, M. Noda, H. Nomachi, M. ODell, S. Odaka, H. Ohashi, T. Ohno, M. Okajima, T. Ota, N. Ozaki, M. Paerels, F. Paltani, S. Parmar, A. Petre, R. Pinto, C. Pohl, M. Porter, F.S. Pottschmidt, K. Ramsey, B. Reynolds, C. Russell, H. Safi-Harb, S. Saito, S. Sakai, K. Sameshima, H. Sato, G. Sato, K. Sato, R. Sawada, M. Schartel, N. Serlemitsos, P. Seta, H. Shidatsu, M. Simionescu, A. Smith, R. Soong, Y. Stawarz, L. Sugawara, Y. Sugita, S. Szymkowiak, A. Tajima, H. Takahashi, H. Takahashi, T. Takeda, S. Takei, Y. Tamagawa, T. Tamura, K. Tamura, T. Tanaka, T. Tanaka, Y. Tanaka, Y. Tashiro, M. Tawara, Y. Terada, Y. Terashima, Y. Tombesi, F. Tomida, H. Tsuboi, Y. Tsujimoto, M. Tsunemi, H. Tsuru, T. Uchida, H. Uchiyama, H. Uchiyama, Y. Ueda, S. Ueda, Y. Ueno, S. Uno, S. Urry, M. Ursino, E. De Vries, C. Watanabe, S. Werner, N. Wik, D. Wilkins, D. Williams, B. Yamada, S. Yamaguchi, H. Yamaoka, K. Yamasaki, N.Y. Yamauchi, M. Yamauchi, S. Yaqoob, T. Yatsu, Y. Yonetoku, D. Yoshida, A. Yuasa, T. Zhuravleva, I. Zoghbi, A.
Nature 535(7610) 117-121 2016年
Clusters of galaxies are the most massive gravitationally-bound objects in<br />
the Universe and are still forming. They are thus important probes of<br />
cosmological parameters and a host of astrophysical processes. Knowledge of the<br />
dyna...
J. W. Den Herdera D. Bagnali S. Bandler M. Barbera X. Barcons D. Barret P. Bastia M. Bisotti K. Boyce C. Cara M. Ceballos L. Corcione B. Cobo L. Colasanti J. De Plaa M. DiPirro W. B. Doriese Y. Ezoe R. Fujimoto F. Gatti L. Gottardi P. Guttridge R. Den Hartog I. Hepburn R. Kelley K. Irwin Y. Ishisaki C. Kilbourne P. A J De Korte J. Van Der Kuur S. Lotti C. Macculi K. Mitsuda T. Mineo L. Natalucci T. Ohashi M. Page S. Paltani E. Perinati L. Piro C. Pigot F. S. Porter G. Rauw L. Ravera E. Renotte J. L. Sauvageot C. Schmid S. Sciortino P. Shirron Y. Takei G. Torrioli M. Tsujimoto L. Valenziano D. Willingale C. De Vries H. Van Weers J. Wilms N. Y. Yamasaki
Proceedings of SPIE - The International Society for Optical Engineering 8443 2012年12月
one of the instruments on the Advanced Telescope for High-Energy Astrophysics (Athena) which was one of the three missions under study as one of the L-class missions of ESA, is the X-ray Microcalorimeter Spectrometer (XMS). This instrument, which ...
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