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1. Full Text The quiescent intracluster medium in the core of the Perseus cluster
by Aharonian, Felix and Akamatsu, Hiroki and Akimoto, Fumie and Allen, Steven W and Anabuki, Naohisa and Angelini, Lorella and Arnaud, Keith and Audard, Marc and Awaki, Hisamitsu and Axelsson, Magnus and Bamba, Aya and Bautz, Marshall and Blandford, Roger and Brenneman, Laura and Brown, Gregory V and Bulbul, Esra and Cackett, Edward and Chernyakova, Maria and Chiao, Meng and Coppi, Paolo and Costantini, Elisa and De Plaa, Jelle and Den Herder, Jan-Willem and Done, Chris and Dotani, Tadayasu and Ebisawa, Ken and Eckart, Megan and Enoto, Teruaki and Ezoe, Yuichiro and Fabian, Andrew C and Ferrigno, Carlo and Foster, Adam and Fujimoto, Ryuichi and Fukazawa, Yasushi and Furuzawa, Akihiro and Galeazzi, Massimiliano and Gallo, Luigi and Gandhi, Poshak and Giustini, Margherita and Goldwurm, Andrea and Gu, Liyi and Guainazzi, Matteo and Haba, Yoshito and Hagino, Kouichi and Hamaguchi, Kenji and Harrus, Ilana and Hatsukade, Isamu and Hayashi, Katsuhiro and Hayashi, Takayuki and Hayashida, Kiyoshi and Hiraga, Junko and Hornschemeier, Ann and Hoshino, Akio and Hughes, John and Iizuka, Ryo and Inoue, Hajime and Inoue, Yoshiyuki and Ishibashi, Kazunori and Ishida, Manabu and Ishikawa, Kumi and Ishisaki, Yoshitaka and Itoh, Masayuki and Iyomoto, Naoko and Kaastra, Jelle and Kallman, Timothy and Kamae, Tuneyoshi and Kara, Erin and Kataoka, Jun and Katsuda, Satoru and Katsuta, Junichiro and Kawaharada, Madoka and Kawai, Nobuyuki and Kelley, Richard and Khangulyan, Dmitry and Kilbourne, Caroline and King, Ashley and Kitaguchi, Takao and Kitamoto, Shunji and Kitayama, Tetsu and Kohmura, Takayoshi and Kokubun, Motohide and Koyama, Shu and Koyama, Katsuji and Kretschmar, Peter and Krimm, Hans and Kubota, Aya and Kunieda, Hideyo and Laurent, Philippe and Lebrun, François and Lee, Shiu-Hang and Leutenegger, Maurice and Limousin, Olivier and Loewenstein, Michael and Long, Knox S and Lumb, David and Madejski, Grzegorz and Maeda, Yoshitomo and Maier, Daniel and Makishima, Kazuo and Markevitch, Maxim and ... and Hitomi Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States)
Nature, ISSN 0028-0836, 07/2016, Volume 535, Issue 7610, pp. 117 - 121
Clusters of galaxies are the most massive gravitationally bound objects in the Universe and are still forming. They are thus important probes(1) of... 
NGC 1275 | GALAXY CLUSTERS | TURBULENT VELOCITY | MULTIDISCIPLINARY SCIENCES | LINE | GAS | NGC-1275 | CONSTRAINTS | X-RAY SPECTROSCOPY | XMM-NEWTON | FEEDBACK | Clusters | Observations | Stars | Cosmology | Astrophysics | Velocity | Stars & galaxies | ASTRONOMY AND ASTROPHYSICS | GRQC | ASTRO
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2. Full Text Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer
by Aharonian, F and Akamatsu, H and Akimoto, F and Allen, SW and Angelini, L and Audard, M and Awaki, H and Axelsson, M and Bamba, A and Bautz, MW and Blandford, R and Brenneman, LW and Brown, GV and Bulbul, E and Cackett, EM and Chernyakova, M and Chiao, MP and Coppi, PS and Costantini, E and de Plaa, J and de Vries, CP and den Herder, JW and Done, C and Dotani, T and Ebisawa, K and Eckart, ME and Enoto, T and Ezoe, Y and Fabian, AC and Ferrigno, C and Foster, AR and Fujimoto, R and Fukazawa, Y and Furuzawa, A and Galeazzi, M and Gallo, LC and Gandhi, P and Giustini, M and Goldwurm, A and Gu, LY and Guainazzi, M and Haba, Y and Hagino, K and Hamaguch, K and Harrus, IM and Hatsukade, I and Hayashi, K and Hayashi, T and Hayashida, K and Hiraga, JS and Hornschemeier, A and Hoshino, A and Hughes, JP and Ichinohe, Y and Iizuka, R and Inoue, H and Inoue, Y and Ishida, M and Ishikawa, K and Ishisaki, Y and Kaastra, J and Kallman, T and Kamae, T and Kataoka, J and Katsuda, S and Kawai, N and Kelley, RL and Kilbourne, CA and Kitaguchi, T and Kitamoto, S and Kitayama, T and Kohmura, T and Kokubun, M and Koyama, K and Koyama, S and Kretschmar, P and Krimm, HA and Kubota, A and Kunieda, H and Laurent, P and Lee, SH and Leutenegger, MA and Limousin, O and Loewenstein, M and Long, KS and Lumb, D and Madejski, G and Maeda, Y and Maier, D and Makishima, K and Markevitch, M and Matsumoto, H and Matsushita, K and McCammon, D and McNamara, BR and Mehdipour, M and Miller, ED and Miller, JM and Mineshige, S and Mitsuda, K and ... and Hitomi Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Fysikum and Naturvetenskapliga fakulteten and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, ISSN 0004-6264, 03/2018, Volume 70, Issue 2
The Crab nebula originated from a core-collapse supernova (SN) explosion observed in 1054 AD. When viewed as a supernova remnant (SNR), it has an anomalously... 
CALIBRATION | ISM: supernova remnants | methods: observational | ENVIRONMENT | PULSAR | INTERSTELLAR-MEDIUM | instrumentation: spectrographs | ISM: individual (Crab nebula) | EVOLUTION | SPECTROSCOPY | MODELS | SUPERNOVA-REMNANTS | ASTRONOMY & ASTROPHYSICS | CONSTRAINTS | ABSORPTION | ASTRONOMY AND ASTROPHYSICS | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
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3. Full Text Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster
by Aharonian, F.A and Akamatsu, H and Akimoto, F and Allen, S.W and Angelini, L and Arnaud, K.A and Audard, M and Awaki, H and Axelsson, M and Bamba, A and Bautz, M.W and Blandford, R.D and Bulbul, E and Brenneman, L.W and Brown, G.V and Cackett, E.M and Chernyakova, M and Chiao, M.P and Coppi, P and Costantini, E and Plaa, J. De and Herder, J.-W. Den and Done, C and Dotani, T and Ebisawa, K and Eckart, M.E and Enoto, T and Ezoe, Y and Fabian, A.C and Ferrigno, C and Foster, A.R and Fujimoto, R and Fukazawa, Y and Furuzawa, A and Galeazzi, M and Gallo, L.C and Gandhi, P and Giustini, M and Goldwurm, A and Gu, L and Guainazzi, M and Haba, Y and Hagino, K and Hamaguchi, K and Harrus, I and Hatsukade, I and Hayashi, K and Hayashi, T and Hayashida, K and Hiraga, J and Hornschemeier, A.E and Hoshino, A and Hughes, J.P and Ichinohe, Y and Iizuka, R and Inoue, H and Inoue, S and Inoue, Y and Ishibashi, K and Ishida, M and Ishikawa, K and Ishisaki, Y and Itoh, M and Iwai, M and Iyomoto, N and Kaastra, J.S and Kallman, T and Kamae, T and Kara, E and Kataoka, J and Katsuda, S and Katsuta, J and Kawaharada, M and Kawai, N and Kelley, R.L and Khangulyan, D and Kilbourne, C.A and King, A.L and Kitaguchi, T and Kitamoto, S and Kitayama, T and Kohmura, T and Kokubun, M and Koyama, S and Koyama, K and Kretschmar, P and Krimm, H.A and Kubota, A and Kunieda, H and Laurent, P and Lebrun, F and Lee, S.-H and Leutenegger, M.A and Limousin, O and Loewenstein, M and Long, K.S and Lumb, D.H and Madejski, G.M and Maeda, Y and Maier, D and ... and Hitomi Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States)
Astrophysical Journal Letters, ISSN 2041-8205, 03/2017, Volume 837, Issue 1, pp. L15 - L15
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... 
galaxies: clusters: individual (A426) | galaxies: clusters: intracluster medium | X-rays: galaxies: clusters | dark matter | DECAYING DARK-MATTER | TEMPERATURE | SEARCH | ASTRONOMY & ASTROPHYSICS | Galactic clusters | Charge exchange | Emission spectroscopy | Dark matter | Decay | Flux | XMM (spacecraft) | Signatures | ASTRONOMY AND ASTROPHYSICS | galaxies | clusters | X-rays
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4. Full Text Solar abundance ratios of the iron-peak elements in the Perseus cluster
by Aharonian, Felix and Akamatsu, Hiroki and Akimoto, Fumie and Allen, Steven W and Angelini, Lorella and Audard, Marc and Awaki, Hisamitsu and Axelsson, Magnus and Bamba, Aya and Bautz, Marshall W and Blandford, Roger and Brenneman, Laura W and Brown, Gregory V and Bulbul, Esra and Cackett, Edward M and Chernyakova, Maria and Chiao, Meng P and Coppi, Paolo S and Costantini, Elisa and De Plaa, Jelle and Den Herder, Jan-Willem and Done, Chris and Dotani, Tadayasu and Ebisawa, Ken and Eckart, Megan E and Enoto, Teruaki and Ezoe, Yuichiro and Fabian, Andrew C and Ferrigno, Carlo and Foster, Adam R and Fujimoto, Ryuichi and Fukazawa, Yasushi and Furuzawa, Akihiro and Galeazzi, Massimiliano and Gallo, Luigi C and Gandhi, Poshak and Giustini, Margherita and Goldwurm, Andrea and Gu, Liyi and Guainazzi, Matteo and Haba, Yoshito and Hagino, Kouichi and Hamaguchi, Kenji and Harrus, Ilana M and Hatsukade, Isamu and Hayashi, Katsuhiro and Hayashi, Takayuki and Hayashida, Kiyoshi and Hiraga, Junko S and Hornschemeier, Ann and Hoshino, Akio and Hughes, John P and Ichinohe, Yuto and Iizuka, Ryo and Inoue, Hajime and Inoue, Yoshiyuki and Ishida, Manabu and Ishikawa, Kumi and Ishisaki, Yoshitaka and Iwai, Masachika and Kaastra, Jelle and Kallman, Tim and Kamae, Tsuneyoshi and Kataoka, Jun and Katsuda, Satoru and Kawai, Nobuyuki and Kelley, Richard L and Kilbourne, Caroline A and Kitaguchi, Takao and Kitamoto, Shunji and Kitayama, Tetsu and Kohmura, Takayoshi and Kokubun, Motohide and Koyama, Katsuji and Koyama, Shu and Kretschmar, Peter and Krimm, Hans A and Kubota, Aya and Kunieda, Hideyo and Laurent, Philippe and Lee, Shiu-Hang and Leutenegger, Maurice A and Limousine, Olivier and Loewenstein, Michael and Long, Knox S and Lumb, David and Madejski, Greg and Maeda, Yoshitomo and Maier, Daniel and Makishima, Kazuo and Markevitch, Maxim and Matsumoto, Hironori and Matsushita, Kyoko and McCammon, Dan and McNamara, Brian R and Mehdipour, Missagh and Miller, Eric D and Miller, Jon M and Mineshige, Shin and Mitsuda, Kazuhisa and ... and Hitomi Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States) and Fysikum and Naturvetenskapliga fakulteten and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
Nature, ISSN 0028-0836, 11/2017, Volume 551, Issue 7681, pp. 478 - 480
The metal abundance of the hot plasma that permeates galaxy clusters represents the accumulation of heavy elements produced by billions of supernovae(1).... 
X-RAY SPECTROMETER | RESONANT SCATTERING | CHANDRASEKHAR-MASS PROGENITORS | INTRACLUSTER MEDIUM | IA SUPERNOVAE | MULTIDISCIPLINARY SCIENCES | ASTRO-H | WHITE-DWARFS | 4 RICH CLUSTERS | CHEMICAL ENRICHMENT | GAS MOTIONS | Physiological aspects | Perseus (Constellation) | Iron | Natural history | Supernova | Spectroscopy | Heavy elements | Parameter estimation | Statistical analysis | White dwarf stars | Galaxies | Supernovae | Stars & galaxies | Milky Way Galaxy | Abundance | X-ray spectroscopy | Milky Way | Sun | Cosmic rays | Galactic clusters | Spectrum analysis | Emission measurements | Chromium | Nickel | Manganese | Physics - High Energy Astrophysical Phenomena | ASTRONOMY AND ASTROPHYSICS | Galaxies and clusters | High-energy astrophysics | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
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5. Full Text The ASTRO-H Mission
by Takahashi, Tadayuki and Mitsuda, Kazuhisa and Kelley, Richard and Aharonian, Felix and Akimoto, Fumie and Allen, Steve and Anabuki, Naohisa and Angelini, Lorella and Arnaud, Keith and Awaki, Hisamitsu and Bamba, Aya and Bando, Nobutaka and Bautz, Mark and Blandford, Roger and Boyce, Kevin and Brown, Greg and Chernyakova, Mara and Coppi, Paolo and Costantini, Elisa and Cottam, Jean and Crow, John and de Plaa, Jelle and de Vries, Cor and den Herder, Jan-Willem and DiPirro, Michael and Done, Chris and Dotani, Tadayasu and Ebisawa, Ken and Enoto, Teruaki and Ezoe, Yuichiro and Fabian, Andrew and Fujimoto, Ryuichi and Fukazawa, Yasushi and Funk, Stefan and Furuzawa, Akihiro and Galeazzi, Massimiliano and Gandhi, Poshak and Gendreau, Keith and Gilmore, Kirk and Haba, Yoshito and Hamaguchi, Kenji and Hatsukade, Isamu and Hayashida, Kiyoshi and Hiraga, Junko and Hirose, Kazuyuki and Hornschemeier, Ann and Hughes, John and Hwang, Una and Iizuka, Ryo and Ishibashi, Kazunori and Ishida, Manabu and Ishimura, Kosei and Ishisaki, Yoshitaka and Isobe, Naoki and Ito, Masayuki and Iwata, Naoko and Kaastra, Jelle and Kallman, Tim and Kamae, Tuneyoshi and Katagiri, Hideaki and Kataoka, Jun and Katsuda, Satoru and Kawaharada, Madoka and Kawai, Nobuyuki and Kawasaki, Shigeo and Khangaluyan, Dmitry and Kilbourne, Caroline and Kinugasa, Kenzo and Kitamoto, Shunji and Kitayama, Tetsu and Kohmura, Takayoshi and Kokubun, Motohide and Kosaka, Tatsuro and Kotani, Taro and Koyama, Katsuji and Kubota, Aya and Kunieda, Hideyo and Laurent, Philippe and Lebrun, Francois and Limousin, Olivier and Loewenstein, Michael and Long, Knox and Madejski, Grzegorz and Maeda, Yoshitomo and Makishima, Kazuo and Markevitch, Maxim and Matsumoto, Hironori and Matsushita, Kyoko and McCammon, Dan and Miller, Jon and Mineshige, Shin and Minesugi, Kenji and Miyazawa, Takuya and Mizuno, Tsunefumi and Mori, Koji and Mori, Hideyuki and Mukai, Koji and Murakami, Hiroshi and Murakami, Toshio and Mushotzky, Richard and ...
Proceedings of SPIE, ISSN 0277-786X, 07/2010, Volume 7732, Issue 1, pp. 77320Z - 77320Z-18
The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science... 
X-ray astronomy | Micro-calorimete | X-ray | Hard X-ray | Gamma-ray | Gamma-ray astronomy | Physics - Instrumentation and Methods for Astrophysics
Conference Proceeding
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6. Full Text Atmospheric gas dynamics in the Perseus cluster observed with Hitomi
by Aharonian, F and Akamatsu, H and Akimoto, F and Allen, SW and Angelini, L and Audard, M and Awaki, H and Axelsson, M and Bamba, A and Bautz, MW and Blandford, R and Brenneman, LW and Brown, GV and Bulbul, E and Cackett, EM and Canning, REA and Chernyakova, M and Chiao, MP and Coppi, PS and Costantini, E and de Plaa, J and de Vries, CP and den Herder, JW and Done, C and Dotani, T and Ebisawa, K and Eckart, ME and Enoto, T and Ezoe, Y and Fabian, AC and Ferrigno, C and Foster, AR and Fujimoto, R and Fukazawa, Y and Furuzawa, A and Galeazzi, M and Gallo, LC and Gandhi, P and Giustini, M and Goldwurm, A and Gu, LY and Guainazzi, M and Haba, Y and Hagino, K and Hamaguchi, K and Harrus, IM and Hatsukade, I and Hayashi, K and Hayashi, T and Hayashida, K and Hiraga, JS and Hornschemeier, A and Hoshino, A and Hughes, JP and Ichinohe, Y and Iizuka, R and Inoue, H and Inoue, S and Inoue, Y and Ishida, M and Ishikawa, K and Ishisaki, Y and Iwai, M and Kaastra, J and Kallman, T and Kamae, T and Kataoka, J and Katsuda, S and Kawai, N and Kelley, RL and Kilbourne, CA and Kitaguchi, T and Kitamoto, S and Kitayama, T and Kohmura, T and Kokubun, M and Koyama, K and Koyama, S and Kretschmar, P and Krimm, HA and Kubota, A and Kunieda, H and Laurent, P and Lee, SH and Leutenegger, MA and Limousin, O and Loewenstein, M and Long, KS and Lumr, D and Madejski, G and Maeda, Y and Maier, D and Makishima, K and Markevitch, M and Matsumoto, H and Matsushita, K and McCammon, D and McNamara, BR and Mehdipour, M and Miller, ED and ... and Hitomi Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Fysikum and Naturvetenskapliga fakulteten and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, ISSN 0004-6264, 03/2018, Volume 70, Issue 2
Extending the earlier measurements reported in Hitomi collaboration (2016, Nature, 535, 117), we examine the atmospheric gas motions within the central 100 kpc... 
RAY-EMITTING GAS | ELLIPTIC GALAXIES | GALAXY CLUSTERS | ACTIVE GALACTIC NUCLEUS | galaxies: clusters: intracluster medium | DEEP CHANDRA OBSERVATION | galaxies: clusters: individual (Perseus) | galaxies: individual (NGC 1275) | INTRACLUSTER MEDIUM | ASTRONOMY & ASTROPHYSICS | X-RAY | X-rays: galaxies: clusters | COOL CORE CLUSTERS | XMM-NEWTON | SUZAKU OBSERVATIONS | Physics - High Energy Astrophysical Phenomena | ASTRONOMY AND ASTROPHYSICS | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
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7. Full Text The ASTRO-H X-ray Observatory
by Takahashi, Hiromitsu and Takahashi, Tadayuki and Mitsuda, Kazuhisa and Kelley, Richard and Aarts, Henri and Aharonian, Felix and Akamatsu, Hiroki and Akimoto, Fumie and Allen, Steve and Anabuki, Naohisa and Angelini, Lorella and Arnaud, Keith and Asai, Makoto and Audard, Marc and Awaki, Hisamitsu and Azzarello, Philipp and Baluta, Chris and Bamba, Aya and Bando, Nobutaka and Bautz, Mark and Blandford, Roger and Boyce, Kevin and Brown, Greg and Cackett, Ed and Chernyakova, Mara and Coppi, Paolo and Costantini, Elisa and de Plaa, Jelle and den Herder, Jan-Willem and DiPirro, Michael and Done, Chris and Dotani, Tadayasu and Doty, John and Ebisawa, Ken and Eckart, Megan and Enoto, Teruaki and Ezoe, Yuichiro and Fabian, Andrew and Ferrigno, Carlo and Foster, Adam and Fujimoto, Ryuichi and Fukazawa, Yasushi and Funk, Stefan and Furuzawa, Akihiro and Galeazzi, Massimiliano and Gallo, Luigi and Gandhi, Poshak and Gendreau, Keith and Gilmore, Kirk and Haas, Daniel and Haba, Yoshito and Hamaguchi, Kenji and Hatsukade, Isamu and Hayashi, Takayuki and Hayashida, Kiyoshi and Hiraga, Junko and Hirose, Kazuyuki and Hornschemeier, Ann and Hoshino, Akio and Hughes, John and Hwang, Una and Iizuka, Ryo and Inoue, Yoshiyuki and Ishibashi, Kazunori and Ishida, Manabu and Ishimura, Kosei and Ishisaki, Yoshitaka and Ito, Masayuki and Iwata, Naoko and Iyomoto, Naoko and Kaastra, Jelle and Kallman, Timothy and Kamae, Tuneyoshi and Kataoka, Jun and Katsuda, Satoru and Kawahara, Hajime and Kawaharada, Madoka and Kawai, Nobuyuki and Kawasaki, Shigeo and Khangaluyan, Dmitry and Kilbourne, Caroline and Kimura, Masashi and Kinugasa, Kenzo and Kitamoto, Shunji and Kitayama, Tetsu and Kohmura, Takayoshi and Kokubun, Motohide and Kosaka, Tatsuro and Koujelev, Alex and Koyama, Katsuji and Krimm, Hans and Kubota, Aya and Kunieda, Hideyo and LaMassa, Stephanie and Laurent, Philippe and Lebrun, Francois and Leutenegger, Maurice and Limousin, Olivier and Loewenstein, Michael and Long, Knox and ...
Proceedings of SPIE - The International Society for Optical Engineering, ISSN 0277-786X, 9/2012, Volume 8443, pp. 84431Z - 84431Z-22
The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science... 
Gamma-ray Astronomy | X-ray | X-ray Astronomy | Hard X-ray | Micro-calorimeter | Gamma-ray | Physics - Instrumentation and Methods for Astrophysics
Conference Proceeding
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8. Full Text The ASTRO-H (Hitomi) x-ray astronomy satellite
by Takahashi, Hiromitsu and Takahashi, Tadayuki and Kokubun, Motohide and Mitsuda, Kazuhisa and Kelley, Richard and Ohashi, Takaya and Aharonian, Felix and Akamatsu, Hiroki and Akimoto, Fumie and Allen, Steve and Anabuki, Naohisa and Angelini, Lorella and Arnaud, Keith and Asai, Makoto and Audard, Marc and Awaki, Hisamitsu and Axelsson, Magnus and Azzarello, Philipp and Baluta, Chris and Bamba, Aya and Bando, Nobutaka and Bautz, Marshall and Bialas, Thomas and Blandford, Roger and Boyce, Kevin and Brenneman, Laura and Brown, Greg and Bulbul, Esra and Cackett, Edward and Canavan, Edgar and Chernyakova, Maria and Chiao, Meng and Coppi, Paolo and Costantini, Elisa and de Plaa, Jelle and den Herder, Jan-Willem and DiPirro, Michael and Done, Chris and Dotani, Tadayasu and Doty, John and Ebisawa, Ken and Eckart, Megan and Enoto, Teruaki and Ezoe, Yuichiro and Fabian, Andrew and Ferrigno, Carlo and Foster, Adam and Fujimoto, Ryuichi and Fukazawa, Yasushi and Furuzawa, Akihiro and Galeazzi, Massimiliano and Gallo, Luigi and Gandhi, Poshak and Gilmore, Kirk and Giustini, Margherita and Goldwurm, Andrea and Gu, Liyi and Guainazzi, Matteo and Haas, Daniel and Haba, Yoshito and Hagino, Kouichi and Hamaguchi, Kenji and Harayama, Atsushi and Harrus, Ilana and Hatsukade, Isamu and Hayashi, Katsuhiro and Hayashi, Takayuki and Hayashida, Kiyoshi and Hiraga, Junko and Hirose, Kazuyuki and Hornschemeier, Ann and Hoshino, Akio and Hughes, John and Ichinohe, Yuto and Iizuka, Ryo and Inoue, Hajime and Inoue, Yoshiyuki and Ishibashi, Kazunori and Ishida, Manabu and Ishikawa, Kumi and Ishimura, Kosei and Ishisaki, Yoshitaka and Itoh, Masayuki and Iwata, Naoko and Iyomoto, Naoko and Jewell, Chris and Kaastra, Jelle and Kallman, Timothy and Kamae, Tuneyoshi and Kara, Erin and Kataoka, Jun and Katsuda, Satoru and Katsuta, Junichiro and Kawaharada, Madoka and Kawai, Nobuyuki and Kawano, Taro and Kawasaki, Shigeo and Khangulyan, Dmitry and Kilbourne, Caroline and Kimball, Mark and ...
Proceedings of SPIE - The International Society for Optical Engineering, ISSN 0277-786X, 7/2016, Volume 9905, pp. 99050U - 99050U-17
The Hitomi (ASTRO-H) mission is the sixth Japanese X-ray astronomy satellite developed by a large international collaboration, including Japan, USA, Canada,... 
Gamma-ray Astronomy | microcalorimeter | X-ray | X-ray Astronomy | Hard X-ray | Gamma-ray
Conference Proceeding
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9. Full Text Measurements of resonant scattering in the Perseus Cluster core with Hitomi SXS
by Aharonian, F and Akamatsu, H and Akimoto, F and Allen, SW and Angelini, L and Audard, M and Awaki, H and Axelsson, M and Bamba, A and Bautz, MW and Blandford, R and Brenneman, LW and Brown, GV and Bulbul, E and Cackett, EM and Chernyakova, M and Chiao, MP and Coppi, PS and Costantini, E and de Plaa, J and de Vries, CP and den Herder, JW and Done, C and Dotani, T and Ebisawa, K and Eckart, ME and Enoto, T and Ezoe, Y and Fabian, AC and Ferrigno, C and Foster, AR and Fujimoto, R and Fukazawa, Y and Furukawa, M and Furuzawa, A and Galeazzi, M and Gallo, LC and Gandhi, P and Giustini, M and Goldwurm, A and Gu, LY and Guainazzi, M and Haba, Y and Hagino, K and Hamaguchi, K and Harrus, IM and Hatsukade, I and Hayashi, K and Hayashi, T and Hayashida, K and Hiraga, JS and Hornschemeier, A and Hoshino, A and Hughes, JP and Ichinohe, Y and Iizuka, R and Inoue, H and Inoue, Y and Ishida, M and Ishikawa, K and Ishisaki, Y and Iwai, M and Kaastra, J and Kallman, T and Kamae, T and Kataoka, J and Katsuda, S and Kawai, N and Kelley, RL and Kilbourne, CA and Kitaguchi, T and Kitamoto, S and Kitayama, T and Kohmura, T and Kokubun, M and Koyama, K and Koyama, S and Kretschmar, P and Krimm, HA and Kubota, A and Kunieda, H and Laurent, P and Lee, SH and Leutenegger, MA and Limousin, OO and Loewenstein, M and Long, KS and Lumb, D and Madejski, G and Maeda, Y and Maier, D and Makishima, K and Markevitch, M and Matsumoto, H and Matsushita, K and McCammon, D and McNamara, BR and Mehdipour, M and Miller, ED and Miller, JM and ... and Hitomi Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Fysikum and Naturvetenskapliga fakulteten and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, ISSN 0004-6264, 03/2018, Volume 70, Issue 2
Thanks to its high spectral resolution (similar to 5 eV at 6 keV), the Soft X-ray Spectrometer (SXS) on board Hitomi enables us to measure the detailed... 
METAL DISTRIBUTION | COOLING FLOW | CROSS-SECTIONS | X-RAY-LINES | ELLIPTIC GALAXIES | galaxies: clusters: intracluster medium | SURFACE BRIGHTNESS | GAS MOTIONS | CHARGED HELIUM-LIKE | ASTRONOMY & ASTROPHYSICS | XMM-NEWTON OBSERVATIONS | DIELECTRONIC-RECOMBINATION | galaxies: clusters: individual (Perseus Cluster) | X-rays: galaxies: clusters | Physics - High Energy Astrophysical Phenomena | ASTRONOMY AND ASTROPHYSICS | individual X-rays | galaxies | intracluster medium | clusters | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
Journal Article
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