TY - JOUR AU - Aharonian, F AU - Akamatsu, H AU - Akimoto, F AU - Allen, SW AU - Angelini, L AU - Audard, M AU - Awaki, H AU - Axelsson, M AU - Bamba, A AU - Bautz, MW AU - Blandford, R AU - Brenneman, LW AU - Brown, GV AU - Bulbul, E AU - Cackett, EM AU - Chernyakova, M AU - Chiao, MP AU - Coppi, PS AU - Costantini, E AU - De Plaa, J AU - Den Herder, JW AU - Done, C AU - Dotani, T AU - Ebisawa, K AU - Eckart, ME AU - Enoto, T AU - Ezoe, Y AU - Fabian, AC AU - Ferrigno, C AU - Foster, AR AU - Fujimoto, R AU - Fukazawa, Y AU - Furuzawa, A AU - Galeazzi, M AU - Gallo, LC AU - Gandhi, P AU - Giustini, M AU - Goldwurm, A AU - Gu, L AU - Guainazzi, M AU - Haba, Y AU - Hagino, K AU - Hamaguchi, K AU - Harrus, IM AU - Hatsukade, I AU - Hayashi, K AU - Hayashi, T AU - Hayashida, K AU - Hiraga, JS AU - Hornschemeier, A AU - Hoshino, A AU - Hughes, JP AU - Ichinohe, Y AU - Iizuka, R AU - Inoue, H AU - Inoue, Y AU - Ishida, M AU - Ishikawa, K AU - Ishisaki, Y AU - Iwai, M AU - Kaastra, J AU - Kallman, T AU - Kamae, T AU - Kataoka, J AU - Katsuda, S AU - Kawai, N AU - Kelley, RL AU - Kilbourne, CA AU - Kitaguchi, T AU - Kitamoto, S AU - Kitayama, T AU - Kohmura, T AU - Kokubun, M AU - Koyama, K AU - Koyama, S AU - Kretschmar, P AU - Krimm, HA AU - Kubota, A AU - Kunieda, H AU - Laurent, P AU - Lee, SH AU - Leutenegger, MA AU - Limousine, O AU - Loewenstein, M AU - Long, KS AU - Lumb, D AU - Madejski, G AU - Maeda, Y AU - Maier, D AU - Makishima, K AU - Markevitch, M AU - Matsumoto, H AU - Matsushita, K AU - McCammon, D AU - McNamara, BR AU - Mehdipour, M AU - Miller, ED AU - Miller, JM AU - Mineshige, S AU - Mitsuda, K AU - Mitsuishi, I AU - Miyazawa, T AU - Mizuno, T AU - Mori, H AU - Mori, K AU - Mukai, K AU - Murakami, H AU - Mushotzky, RF AU - Nakagawa, T AU - Nakajima, H AU - Nakamori, T AU - Nakashima, S AU - Nakazawa, K AU - Nobukawa, KK AU - Nobukawa, M AU - Noda, H AU - Odaka, H AU - Ohashi, T AU - Ohno, Masanori AU - Okajima, T AU - Ota, N AU - Ozaki, M AU - Paerels, F AU - Paltani, S AU - Petre, R AU - Pinto, C AU - Frederick, SP AU - Pottschmidt, K AU - Christopher, SR AU - Safi-Harb, S AU - Saito, S AU - Sakai, K AU - Sasaki, T AU - Sato, G AU - Sato, K AU - Sato, R AU - Sawada, M AU - Schartel, N AU - Serlemitsos, PJ AU - Seta, H AU - Shidatsu, M AU - Simionescu, A AU - Smith, RK AU - Soong, Y AU - Stawarz, L AU - Sugawara, Y AU - Sugita, S AU - Szymkowiak, A AU - Tajima, H AU - Takahashi, H AU - Takahashi, T AU - Ichirotakeda, S AU - Takei, Y AU - Tamagawa, T AU - Tamura, T AU - Tanaka, T AU - Tanaka, Y AU - Tanaka, YT AU - Tashiro, MS AU - Tawara, Y AU - Terada, Y AU - Terashima, Y AU - Tombesi, F AU - Tomida, H AU - Tsuboi, Y AU - Tsujimoto, M AU - Tsunemi, H AU - Tsuru, TG AU - Uchida, H AU - Uchiyama, H AU - Uchiyama, Y AU - Ueda, S AU - Ueda, Y AU - Uno, S AU - Urry, CM AU - Ursino, E AU - Vries, CPD AU - Watanabe, S AU - Werner, Norbert AU - Wik, DR AU - Wilkins, DR AU - Williams, BJ AU - Yamada, S AU - Yamaguchi, H AU - Yamaoka, K AU - Yamasaki, NY AU - Yamauchi, M AU - Yamauchi, S AU - Yaqoob, T AU - Yatsu, Y AU - Yonetoku, D AU - Zhuravleva, I AU - Zoghbi, A TI - Solar abundance ratios of the iron-peak elements in the Perseus cluster JF - NATURE J2 - NATURE VL - 551 PY - 2017 IS - 7681 SP - 478 EP - 480 PG - 3 SN - 0028-0836 DO - 10.1038/nature24301 UR - https://m2.mtmt.hu/api/publication/3335576 ID - 3335576 N1 - 1Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin, Ireland Max-Planck-Institut für Kernphysik, PO Box 103980, Heidelberg, 69029, Germany Gran Sasso Science Institute, viale Francesco Crispi 7, L' Aquila, 67100, Italy SRON Netherlands Institute for Space Research, Sorbonnelaan 2, Utrecht, 3584, Netherlands Institute for Space-Earth Environmental Research, Nagoya University, Furo-cho, Chikusa-ku, 464-8601, Japan Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, United States Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, United States SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94025, United States NASA, Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, United States Department of Astronomy, University of Geneva, ch. d'Écogia 16, Versoix, CH-1290, Switzerland Department of Physics, Ehime University, Bunkyo-cho, Matsuyama, Ehime, 790-8577, Japan Department of Physics, Oskar Klein Center, Stockholm University, Stockholm, 10691, Sweden Department of Physics, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan Research Center for the Early Universe, School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, United States Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138, United States Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, CA 94550, United States Department of Physics and Astronomy, Wayne State University, 666 West Hancock Street, Detroit, MI 48201, United States Astronomy Department, Yale University, New Haven, CT 06520-8101, United States Physics Department, Yale University, New Haven, CT 06520-8120, United States Centre for Extragalactic Astronomy, Department of Physics, University of Durham, South Road, Durham, DH13LE, United Kingdom Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, 3-1-1 Yoshino-dai, Chuo-ku, Sagamihara, Kanagawa, 252-5210, Japan Department of Astronomy, Kyoto University, Sakyo-ku, Kyoto, 606-8502, Japan Hakubi Center for Advanced Research, Kyoto University, Kyoto, 606-8302, Japan Department of Physics, Tokyo Metropolitan University, 1-1 Minami-Osawa, Tokyo, 192-0397, Japan Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB30HA, United Kingdom Faculty of Mathematics and Physics, Kanazawa University, Kanazawa, Ishikawa, 920-1192, Japan School of Science, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, 739-8526, Japan Fujita Health University, Toyoake, Aichi, 470-1192, Japan Physics Department, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, United States Department of Astronomy and Physics, Saint Mary's University, 923 Robie Street, Halifax, NS B3H3C3, Canada Department of Physics and Astronomy, University of Southampton, Highfield, Southampton, SO171BJ, United Kingdom Laboratoire APC, 10 rue Alice Domon, Paris, 75013, France CEA Saclay, Gif Yvette, 91191, France European Space Research and Technology Center, Keplerlaan 1, Noordwijk, 2201, Netherlands Department of Physics and Astronomy, Aichi University of Education, Aichi, 448-8543, Japan Department of Physics, Tokyo University of Science, Yamazaki, Noda, 2641, 278-8510, Japan Department of Physics, University of Maryland Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, United States Department of Applied Physics and Electronic Engineering, University of Miyazaki, 1-1 Gakuen Kibanadai-Nishi, Miyazaki, 889-2192, Japan Department of Physics, Nagoya University, Aichi, 464-8602, Japan Department of Earth and Space Science, Osaka University, 1-1 Machikaneyama-cho, Toyonaka, Osaka, 560-0043, Japan Department of Physics, Kwansei Gakuin University, 2-1 Gakuen, Sanda, 669-1337, Japan Department of Physics, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima-ku, Tokyo, 171-8501, Japan Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854, United States Meisei University, 2-1-1 Hodokubo, Hino, Tokyo, 191-8506, Japan Leiden Observatory, Leiden University, PO Box 9513, Leiden, 2300, Netherlands Research Institute for Science and Engineering, Waseda University, 3-4-1 Ohkubo, Tokyo, 169-8555, Japan Department of Physics, Chuo University, 1-13-27 Kasuga, Tokyo, 112-8551, Japan Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Tokyo, 152-8550, Japan Department of Physics, Toho University, 2-2-1 Miyama, Chiba, 274-8510, Japan Department of Physics, Kyoto University, Kitashirakawa-Oiwake-Cho, Sakyo, Kyoto, 606-8502, Japan European Space Astronomy Center, Camino Bajo Del Castillo, Madrid, 28692, Spain Universities Space Research Association, 7178 Columbia Gateway Drive, Columbia, MD 21046, United States National Science Foundation, 4201 Wilson Blvd, Arlington, VA 22230, United States Department of Electronic Information Systems, Shibaura Institute of Technology, 307 Fukasaku, Saitama, 337-8570, Japan Department of Astronomy, University of Maryland, College Park, MD 20742, United States Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States Institute of Physical and Chemical Research, 2-1 Hirosawa, Saitama, 351-0198, Japan Department of Physics, Tokyo University of Science, 1-3 Kagurazaka, Tokyo, 162-8601, Japan Department of Physics, University of Wisconsin, Madison, WI 53706, United States Department of Physics and Astronomy, University of Waterloo, 200 University Avenue West, Waterloo, ON N2L3G1, Canada Department of Astronomy, University of Michigan, 1085 South University Avenue, Ann Arbor, MI 48109, United States Okinawa Institute of Science, Technology Graduate University, 1919-1 Tancha, Onna-son Okinawa, 904-0495, Japan Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima, 739-8526, Japan Faculty of Liberal Arts, Tohoku Gakuin University, 2-1-1 Tenjinzawa, Miyagi, 981-3193, Japan Faculty of Science, Yamagata University, 1-4-12 Kojirakawa-machi, Yamagata, 990-8560, Japan Department of Physics, Nara Women's University, Kitauoyanishi-machi, Nara, 630-8506, Japan Department of Teacher Training, School Education, Nara University of Education, Takabatake-cho, Nara, 630-8528, Japan Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, 6-3 Aramakiazaaoba, Aoba-ku, Sendai, Miyagi, 980-8578, Japan Astronomical Institute, Tohoku University, 6-3 Aramakiazaaoba, Miyagi, 980-8578, Japan Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, United States Department of Physics and Astronomy, University of Manitoba, Winnipeg, R3T2N2, Canada Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Chuo-ku, Sagamihara, 252-5258, Japan Astronomical Observatory of Jagiellonian University, ul. Orla 171, Kraków, 30-244, Poland RIKEN Nishina Center, 2-1 Hirosawa, Wako, Saitama, 351-0198, Japan Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse 1, Garching, 85748, Germany Department of Physics, Saitama University, 255 Shimo-Okubo, Saitama, 338-8570, Japan Department of Physics, University of Rome Tor Vergata, Via della Ricerca Scientifica 1, Rome, I-00133, Italy Faculty of Education, Shizuoka University, 836 Ohya, Suruga-ku, Shizuok, 422-8529, Japan Faculty of Health Sciences, Nihon Fukushi University, 26-2 Higashi Haemi-cho, Handa, Aichi, 475-0012, Japan MTA, Eötvös University Lendület Hot, Universe Research Group, Pazmany Peter setany 1/A, Budapest, 1117, Hungary Department of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University, Kotlávrská 2, Brno, 61137, Czech Republic Department of Physics and Astronomy, University of Utah, 115 South, Salt Lake City, UT 1400, 84112, United States Johns Hopkins University, Homewood Campus, Baltimore, MD 21218, United States Cited By :25 Export Date: 26 November 2019 CODEN: NATUA Correspondence Address: Yamaguchi, H.; NASA, Goddard Space Flight Center, 8800 Greenbelt Road, United States; email: hiroya.yamaguchi@nasa.gov AB - The metal abundance of the hot plasma that permeates galaxy clusters represents the accumulation of heavy elements produced by billions of supernovae. Therefore, X-ray spectroscopy of the intracluster medium provides an opportunity to investigate the nature of supernova explosions integrated over cosmic time. In particular, the abundance of the iron-peak elements (chromium, manganese, iron and nickel) is key to understanding how the progenitors of typical type Ia supernovae evolve and explode. Recent X-ray studies of the intracluster medium found that the abundance ratios of these elements differ substantially from those seen in the Sun, suggesting differences between the nature of type Ia supernovae in the clusters and in the Milky Way. However, because the K-shell transition lines of chromium and manganese are weak and those of iron and nickel are very close in photon energy, high-resolution spectroscopy is required for an accurate determination of the abundances of these elements. Here we report observations of the Perseus cluster, with statistically significant detections of the resonance emission from chromium, manganese and nickel. Our measurements, combined with the latest atomic models, reveal that these elements have near-solar abundance ratios with respect to iron, in contrast to previous claims. Comparison between our results and modern nucleosynthesis calculations disfavours the hypothesis that type Ia supernova progenitors are exclusively white dwarfs with masses well below the Chandrasekhar limit (about 1.4 times the mass of the Sun). The observed abundance pattern of the iron-peak elements can be explained by taking into account a combination of near- A nd sub-Chandrasekhar-mass type Ia supernova systems, adding to the mounting evidence that both progenitor types make a substantial contribution to cosmic chemical enrichment. © 2017 Macmillan Publishers Limited, part of Springer Nature. LA - English DB - MTMT ER - TY - JOUR AU - Aharonian, F AU - Akamatsu, H AU - Akimoto, F AU - Allen, SW AU - Anabuki, N AU - Angelini, L AU - Arnaud, K AU - Audard, M AU - Awaki, H AU - Axelsson, M AU - Bamba, A AU - Bautz, M AU - Blandford, R AU - Brenneman, L AU - Brown, GV AU - Bulbul, E AU - Cackett, E AU - Chernyakova, M AU - Chiao, M AU - Coppi, P AU - Costantini, E AU - de Plaa, J AU - den Herder, JW AU - Done, C AU - Dotani, T AU - Ebisawa, K AU - Eckart, M AU - Enoto, T AU - Ezoe, Y AU - Fabian, AC AU - Ferrigno, C AU - Foster, A AU - Fujimoto, R AU - Fukazawa, Y AU - Furuzawa, A AU - Galeazzi, M AU - Gallo, L AU - Gandhi, P AU - Giustini, M AU - Goldwurm, A AU - Gu, L AU - Guainazzi, M AU - Haba, Y AU - Hagino, K AU - Hamaguchi, K AU - Harrus, I AU - Hatsukade, I AU - Hayashi, K AU - Hayashi, T AU - Hayashida, K AU - Hiraga, J AU - Hornschemeier, A AU - Hoshino, A AU - Hughes, J AU - Iizuka, R AU - Inoue, H AU - Inoue, Y AU - Ishibashi, K AU - Ishida, M AU - Ishikawa, K AU - Ishisaki, Y AU - Itoh, M AU - Iyomoto, N AU - Kaastra, J AU - Kallman, T AU - Kamae, T AU - Kara, E AU - Kataoka, J AU - Katsuda, S AU - Katsuta, J AU - Kawaharada, M AU - Kawai, N AU - Kelley, R AU - Khangulyan, D AU - Kilbourne, C AU - King, A AU - Kitaguchi, T AU - Kitamoto, S AU - Kitayama, T AU - Kohmura, T AU - Kokubun, M AU - Koyama, S AU - Koyama, K AU - Kretschmar, P AU - Krimm, H AU - Kubota, A AU - Kunieda, H AU - Laurent, P AU - Lebrun, F AU - Lee, SH AU - Leutenegger, M AU - Limousin, O AU - Loewenstein, M AU - Long, KS AU - Lumb, D AU - Madejski, G AU - Maeda, Y AU - Maier, D AU - Makishima, K AU - Markevitch, M AU - Matsumoto, H AU - Matsushita, K AU - McCammon, D AU - McNamara, B AU - Mehdipour, M AU - Miller, E AU - Miller, J AU - Mineshige, S AU - Mitsuda, K AU - Mitsuishi, I AU - Miyazawa, T AU - Mizuno, T AU - Mori, H AU - Mori, K AU - Moseley, H AU - Mukai, K AU - Murakami, H AU - Murakami, T AU - Mushotzky, R AU - Nagino, R AU - Nakagawa, T AU - Nakajima, H AU - Nakamori, T AU - Nakano, T AU - Nakashima, S AU - Nakazawa, K AU - Nobukawa, M AU - Noda, H AU - Nomachi, M AU - O'Dell, S AU - Odaka, H AU - Ohashi, T AU - Ohno, Masanori AU - Okajima, T AU - Ota, N AU - Ozaki, M AU - Paerels, F AU - Paltani, S AU - Parmar, A AU - Petre, R AU - Pinto, C AU - Pohl, M AU - Porter, FS AU - Pottschmidt, K AU - Ramsey, B AU - Reynolds, C AU - Russell, H AU - Safi-Harb, S AU - Saito, S AU - Sakai, K AU - Sameshima, H AU - Sato, G AU - Sato, K AU - Sato, R AU - Sawada, M AU - Schartel, N AU - Serlemitsos, P AU - Seta, H AU - Shidatsu, M AU - Simionescu, A AU - Smith, R AU - Soong, Y AU - Stawarz, L AU - Sugawara, Y AU - Sugita, S AU - Szymkowiak, A AU - Tajima, H AU - Takahashi, H AU - Takahashi, T AU - Takeda, S AU - Takei, Y AU - Tamagawa, T AU - Tamura, K AU - Tamura, T AU - Tanaka, T AU - Tanaka, Y AU - Tanaka, Y AU - Tashiro, M AU - Tawara, Y AU - Terada, Y AU - Terashima, Y AU - Tombesi, F AU - Tomida, H AU - Tsuboi, Y AU - Tsujimoto, M AU - Tsunemi, H AU - Tsuru, T AU - Uchida, H AU - Uchiyama, H AU - Uchiyama, Y AU - Ueda, S AU - Ueda, Y AU - Ueno, S AU - Uno, S AU - Urry, M AU - Ursino, E AU - De Vries, C AU - Watanabe, S AU - Werner, Norbert AU - Wik, D AU - Wilkins, D AU - Williams, B AU - Yamada, S AU - Yamaguchi, H AU - Yamaoka, K AU - Yamasaki, NY AU - Yamauchi, M AU - Yamauchi, S AU - Yaqoob, T AU - Yatsu, Y AU - Yonetoku, D AU - Yoshida, A AU - Yuasa, T AU - Zhuravleva, I AU - Zoghbi, A TI - The quiescent intracluster medium in the core of the Perseus cluster JF - NATURE J2 - NATURE VL - 535 PY - 2016 IS - 7610 SP - 117 EP - 121 PG - 5 SN - 0028-0836 DO - 10.1038/nature18627 UR - https://m2.mtmt.hu/api/publication/3177712 ID - 3177712 N1 - Megjegyzés-26334289 Group Author: Hitomi Collaboration Megjegyzés-26334356 Group Author: Hitomi Collaboration AB - Clusters of galaxies are the most massive gravitationally bound objects in the Universe and are still forming. They are thus important probes(1) 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(2-6). 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. LA - English DB - MTMT ER - TY - JOUR AU - Chantler, C T AU - Kinnane, M N AU - Gillaspy, J D AU - Hudson, L T AU - Payne, A T AU - Smale, L F AU - Henins, A AU - Pomeroy, J M AU - Kimpton, J A AU - Takács, Endre AU - Makonyi, K TI - Comment on "Testing Three-Body Quantum Electrodynamics with Trapped Ti20+ Ions: Evidence for a Z-Dependent Divergence Between Experiment and Calculation" Reply JF - PHYSICAL REVIEW LETTERS J2 - PHYS REV LETT VL - 110 PY - 2013 IS - 15 PG - 2 SN - 0031-9007 DO - 10.1103/PhysRevLett.110.159302 UR - https://m2.mtmt.hu/api/publication/2416642 ID - 2416642 LA - English DB - MTMT ER - TY - JOUR AU - Chantler, Chris T AU - Kinnane, M N AU - Gillaspy, John Dale AU - Hudson, Larry T AU - Payne, A T AU - Smale, L F AU - Henins, A AU - Pomeroy, J M AU - Tan, J N AU - Kimpton, J A AU - Takács, Endre AU - Makónyi, Károly TI - Testing Three-Body Quantum Electrodynamics with Trapped Ti{20+} Ions: Evidence for a Z-dependent Divergence Between Experiment and Calculation JF - PHYSICAL REVIEW LETTERS J2 - PHYS REV LETT VL - 109 PY - 2012 IS - 15 PG - 5 SN - 0031-9007 DO - 10.1103/PhysRevLett.109.153001 UR - https://m2.mtmt.hu/api/publication/2375958 ID - 2375958 LA - English DB - MTMT ER - TY - JOUR AU - Rodriguez, D AU - Blaum, K AU - Nortershauser, W AU - Ahammed, M AU - Algora, Alejandro AU - Audi, G AU - Aysto, J AU - Beck, D AU - Bender, M AU - Billowes, J AU - Block, M AU - Bohm, C AU - Bollen, G AU - Brodeur, M AU - Brunner, T AU - Bushaw, BA AU - Cakirli, RB AU - Campbell, P AU - Cano-Ott, D AU - Cortes, G AU - Lopez-Urrutia, JRC AU - Das, P AU - Dax, A AU - De, A AU - Delheij, P AU - Dickel, T AU - Dilling, J AU - Eberhardt, K AU - Eliseev, S AU - Ettenauer, S AU - Flanagan, KT AU - Ferrer, R AU - Garcia-Ramos, JE AU - Gartzke, E AU - Geissel, H AU - George, S AU - Geppert, C AU - Gomez-Hornillos, MB AU - Gusev, Y AU - Habs, D AU - Heenen, PH AU - Heinz, S AU - Herfurth, F AU - Herlert, A AU - Hobein, M AU - Huber, G AU - Huyse, M AU - Jesch, C AU - Jokinen, A AU - Kester, O AU - Ketelaer, J AU - Kolhinen, V AU - Koudriavtsev, I AU - Kowalska, M AU - Kramer, J AU - Kreim, S AU - Krieger, A AU - Kuhl, T AU - Lallena, AM AU - Lapierre, A AU - Le Blanc, F AU - Litvinov, YA AU - Lunney, D AU - Martinez, T AU - Marx, G AU - Matos, M AU - Minaya-Ramirez, E AU - Moore, I AU - Nagy, S AU - Naimi, S AU - Neidherr, D AU - Nesterenko, D AU - Neyens, G AU - Novikov, YN AU - Petrick, M AU - Plass, WR AU - Popov, A AU - Quint, W AU - Ray, A AU - Reinhard, PG AU - Repp, J AU - Roux, C AU - Rubio, B AU - Sanchez, R AU - Schabinger, B AU - Scheidenberger, C AU - Schneider, D AU - Schuch, R AU - Schwarz, S AU - Schweikhard, L AU - Seliverstov, M AU - Solders, A AU - Suhonen, M AU - Szerypo, J AU - Tain, JL AU - Thirolf, PG AU - Ullrich, J AU - Van, Duppen P AU - Vasiliev, A AU - Vorobjev, G AU - Weber, C AU - Wendt, K AU - Winkler, M AU - Yordanov, D AU - Ziegler, F TI - MATS and LaSpec: High-precision experiments using ion traps and lasers at FAIR JF - EUROPEAN PHYSICAL JOURNAL-SPECIAL TOPICS J2 - EUR PHYS J-SPEC TOP VL - 183 PY - 2010 SP - 1 EP - 123 PG - 123 SN - 1951-6355 DO - 10.1140/epjst/e2010-01231-2 UR - https://m2.mtmt.hu/api/publication/3109219 ID - 3109219 LA - English DB - MTMT ER - TY - JOUR AU - Orts, RS AU - Lopez-Urrutia, JRC AU - Bruhns, H AU - Martinez, AJG AU - Harman, Z AU - Jentschura, Ulrich David AU - Keitel, CH AU - Lapierre, A AU - Tawara, H AU - Tupitsyn, II AU - Ullrich, J AU - Volotka, AV TI - Zeeman splitting and g factor of the 1s(2)2s(2)2p (2)P(3/2) and (2)P(1/2) levels in Ar(13+) JF - PHYSICAL REVIEW A J2 - PHYS REV A VL - 76 PY - 2007 IS - 5 SN - 2469-9926 DO - 10.1103/PhysRevA.76.052501 UR - https://m2.mtmt.hu/api/publication/3178250 ID - 3178250 N1 - : Volotka, Andrey/N-1650-2013; 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