Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi

被引:81
作者
Aharonian, Felix [1 ,2 ,3 ]
Akamatsu, Hiroki [4 ]
Akimoto, Fumie [5 ]
Allen, Steven W. [6 ,7 ,8 ]
Angelini, Lorella [9 ]
Audard, Marc [10 ]
Awaki, Hisamitsu [11 ]
Axelsson, Magnus [12 ,13 ]
Bamba, Aya [14 ,15 ]
Bautz, Marshall W. [16 ]
Blandford, Roger [6 ,7 ,8 ]
Brenneman, Laura W. [17 ]
Brown, Gregory, V [18 ]
Bulbul, Esra [16 ]
Cackett, Edward M. [19 ]
Chernyakova, Maria [1 ]
Chiao, Meng P. [9 ]
Coppi, Paolo S. [20 ,21 ]
Costantini, Elisa [4 ]
de Plaa, Jelle [4 ]
de Vries, Cor P. [4 ]
den Herder, Jan-Willem [4 ]
Done, Chris [22 ]
Dotani, Tadayasu [23 ]
Ebisawa, Ken [23 ]
Eckart, Megan E. [9 ]
Enoto, Teruaki [24 ,25 ]
Ezoe, Yuichiro [26 ]
Fabian, Andrew C. [27 ]
Ferrigno, Carlo [10 ]
Foster, Adam R. [17 ]
Fujimoto, Ryuichi [28 ]
Fukazawa, Yasushi [29 ]
Furuzawa, Akihiro [30 ]
Galeazzi, Massimiliano [31 ]
Gallo, Luigi C. [32 ]
Gandhi, Poshak [33 ]
Giustini, Margherita [4 ]
Goldwurm, Andrea [34 ,35 ]
Gu, Liyi [4 ]
Guainazzi, Matteo [36 ]
Haba, Yoshito [37 ]
Hagino, Kouichi [38 ]
Hamaguchi, Kenji [9 ,39 ]
Harrus, Ilana M. [9 ,39 ]
Hatsukade, Isamu [40 ]
Hayashi, Katsuhiro [23 ,41 ]
Hayashi, Takayuki [41 ]
Hayashida, Kiyoshi [42 ]
Hell, Natalie [18 ]
机构
[1] Dublin Inst Adv Studies, 31 Fitzwilliam Pl, Dublin 2, Ireland
[2] Max Planck Inst Kernphys, POB 103980, D-69029 Heidelberg, Germany
[3] Gran Sasso Sci Inst, Viale Francesco Crispi 7, I-67100 Laquila, AQ, Italy
[4] SRON Netherlands Inst Space Res, Sorbonnelaan 2, NL-3584 CA Utrecht, Netherlands
[5] Nagoya Univ, Inst Space Earth Environm Res, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648601, Japan
[6] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94305 USA
[7] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA
[8] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA
[9] NASA, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA
[10] Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland
[11] Ehime Univ, Dept Phys, 2-5 Bunkyo Cho, Matsuyama, Ehime 7908577, Japan
[12] Stockholm Univ, Dept Phys, S-10691 Stockholm, Sweden
[13] Stockholm Univ, Oskar Klein Ctr, S-10691 Stockholm, Sweden
[14] Univ Tokyo, Dept Phys, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
[15] Univ Tokyo, Res Ctr Early Universe, Sch Sci, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
[16] MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[17] Smithsonian Astrophys Observ, 60 Garden St,MS-4, Cambridge, MA 02138 USA
[18] Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA
[19] Wayne State Univ, Dept Phys & Astron, 666 W Hancock St, Detroit, MI 48201 USA
[20] Yale Univ, Dept Astron, New Haven, CT 06520 USA
[21] Yale Univ, Dept Phys, New Haven, CT 06520 USA
[22] Univ Durham, Ctr Extragalact Astron, Dept Phys, South Rd, Durham DH1 3LE, England
[23] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshino Dai, Sagamihara, Kanagawa 2525210, Japan
[24] Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto, Kyoto 6068502, Japan
[25] Kyoto Univ, Hakubi Ctr Adv Res, Sakyo Ku, Kyoto, Kyoto 6068501, Japan
[26] Tokyo Metropolitan Univ, Dept Phys, 1-1 Minami Osawa, Hachioji, Tokyo 1920397, Japan
[27] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England
[28] Kanazawa Univ, Fac Math & Phys, Kakuma Machi, Kanazawa, Ishikawa 9201192, Japan
[29] Hiroshima Univ, Sch Sci, 1-3-1 Kagamiyama, Higashihiroshima, Hiroshima 7398526, Japan
[30] Fujita Hlth Univ, 1-98 Dengakugakubo,Kutsukake Cho, Toyoake, Aichi 4701192, Japan
[31] Univ Miami, Phys Dept, 1320 Campo Sano Dr, Coral Gables, FL 33146 USA
[32] St Marys Univ, Dept Astron & Phys, 923 Robie St, Halifax, NS B3H 3C3, Canada
[33] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England
[34] Lab APC, 10 Rue Alice Domon & Leonie Duquet, F-75013 Paris, France
[35] CEA Saclay, F-91191 Gif Sur Yvette, France
[36] European Space Technol Ctr, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands
[37] Aichi Univ Educ, Dept Phys & Astron, 1 Hirosawa,Igaya Cho, Kariya, Aichi 4488543, Japan
[38] Tokyo Univ Sci, Dept Phys, 2641 Yamazaki, Noda, Chiba 2788510, Japan
[39] Univ Maryland Baltimore Cty, Dept Phys, 1000 Hilltop Circle, Baltimore, MD 21250 USA
[40] Univ Miyazaki, Dept Appl Phys & Elect Engn, 1-1 Gakuen Kibanadai Nishi, Miyazaki, Miyazaki 8892192, Japan
[41] Nagoya Univ, Dept Phys, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan
[42] Osaka Univ, Dept Earth & Space Sci, 1-1 Machikaneyama Cho, Toyonaka, Osaka 5600043, Japan
[43] Kwansei Gakuin Univ, Dept Phys, 2-1 Gakuen, Sanda, Hyogo 6691337, Japan
[44] Rikkyo Univ, Dept Phys, Toshima Ku, 3-34-1 Nishi Ikebukuro, Tokyo 1718501, Japan
[45] Rutgers State Univ, Dept Phys & Astron, 136 Frelinghuysen Rd, Piscataway, NJ 08854 USA
[46] Meisei Univ, 2-1-1 Hodokubo, Hino, Tokyo 1918506, Japan
[47] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands
[48] Waseda Univ, Res Inst Sci & Engn, Shinjuku Ku, 3-4-1 Ohkubo, Tokyo 1698555, Japan
[49] Chuo Univ, Dept Phys, Bunkyo Ku, 1-13-27 Kasuga, Tokyo 1128551, Japan
[50] Tokyo Inst Technol, Dept Phys, Meguro Ku, 2-12-1 Ookayama, Tokyo 1528550, Japan
基金
加拿大自然科学与工程研究理事会;
关键词
instrumentation: spectrographs; methods: data analysis; X-rays: general; HELIUM-LIKE IONS; DIELECTRONIC SATELLITE SPECTRA; ELECTRON-IMPACT EXCITATION; IN-FLIGHT CALIBRATION; K-VACANCY STATES; H-LIKE FE; GALAXY CLUSTERS; HYDROGEN-LIKE; GROUND-STATE; AUGER DECAY;
D O I
10.1093/pasj/psx156
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Hitomi Soft X-ray Spectrometer spectrum of the Perseus cluster, with similar to 5 eV resolution in the 2-9 keV band, offers an unprecedented benchmark of the atomic modeling and database for hot collisional plasmas. It reveals both successes and challenges of the current atomic data and models. The latest versions of AtomDB/APEC (3.0.8), SPEX (3.03.00), and CHIANTI (8.0) all provide reasonable fits to the broad-band spectrum, and are in close agreement on best-fit temperature, emission measure, and abundances of a few elements such as Ni. For the Fe abundance, the APEC and SPEX measurements differ by 16%, which is 17 times higher than the statistical uncertainty. This is mostly attributed to the differences in adopted collisional excitation and dielectronic recombination rates of the strongest emission lines. We further investigate and compare the sensitivity of the derived physical parameters to the astrophysical source modeling and instrumental effects. The Hitomi results show that accurate atomic data and models are as important as the astrophysical modeling and instrumental calibration aspects. Substantial updates of atomic databases and targeted laboratory measurements are needed to get the current data and models ready for the data from the next Hitomi-level mission.
引用
收藏
页数:48
相关论文
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