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FIT: the scintillating fiber tracker of the HERD space mission
Perrina, C.1; Azzarello, P.2; Cadoux, F.2; Favre, Y.2; Frieden, J. M.1; La Marra, D.2; Sukhonos, D.2; Wu, X.2; Adriani, O.28; Alemanno, F.29,30; Aloisio, R.29,30; Altomare, C.25; Ambrosi, G.37; An, Q.12; Antonelli, M.48; Azzarello, P.40; Bai, L.10; Bai, Y. L.5; Bao, T. W.3; Barbanera, M.37; Barbato, F. C.29,30; Bernardini, P.33; Berti, E.28; Bertucci, B.38; Bi, X. J.3; Bigongiari, G.39; Bongi, M.28; Bonvicini, V.48; Bordas, P.43; Bosch-Ramon, V.43; Bottai, S.27; Brogi, P.39; Cadoux, F.40; Campana, D.34; Cao, W. W.5; Cao, Z.3; Casaus, J.42; Catanzani, E.38; Cattaneo, P. W.36; Chang, J.11,15; Chang, Y. H.23; Chen, G. M.3; Chen, Y.17; Cianetti, F.38; Comerma, A.43,44; Cortis, D.31; Cui, X. H.15; Cui, X. Z.3; Dai, C.7; Dai, Z. G.17; D’Alessandro, R.28; De Gaetano, S.26; De Mitri, I.29,30; de Palma, F.33; Di Felice, V.53; Di Giovanni, A.29,30; Di Santo, M.29,30; Di Venere, L.26; Dong, J. N.8,9; Dong, Y. W.3; Donvito, G.25; Duranti, M.37; D’Urso, D.52; Evoli, C.29,30; Fang, K.3; Fariña, L.45; Favre, Y.40; Feng, C. Q.12; Feng, H.18; Feng, H. B.7; Feng, Z. K.7; Finetti, N.24; Formato, V.53; Frieden, J. M.47; Fusco, P.26; Gao, J. R.5; Gargano, F.25; Gascon-Fora, D.43; Gasparrini, D.53; Giglietto, N.26; Giovacchini, F.42; Gomez, S.43; Gong, K.3; Gou, Q. B.3; Guida, R.49; Guo, D. Y.3; Guo, J. H.11; Guo, Y. Q.3; He, H. H.3; Hu, H. B.3; Hu, J. Y.3,4; Hu, P.3,4; Hu, Y. M.11; Huang, G. S.12; Huang, J.3; Huang, W. H.8,9; Huang, X. T.8,9; Huang, Y. B.7; Huang, Y. F.17; Ionica, M.37; Jouvin, L.45; Kotenko, A.40; Kyratzis, D.29,30; La Marra, D.40; Li, M. J.8,9; Li, Q. Y.8,9; Li, R.5; Li, S. L.3,4; Li, T.8,9; Li, X.11; Li, Z.19; Li, Z. H.3,4; Liang, E. W.7; Liang, M. J.3,4; Liao, C. L.10; Licciulli, F.25; Lin, S. J.3; Liu, D.8,9; Liu, H. B.7; Liu, H.10; Liu, J. B.12; Liu, S. B.12; Liu, X.3,4; Liu, X. W.7; Liu, Y. Q.3; Loparco, F.26; Loporchio, S.25; Lu, X.7; Lyu, J. G.6; Lyu, L. W.5; Maestro, P.39; Mancini, E.37; Manera, R.43; Marin, J.42; Marrocchesi, P. S.39; Marsella, G.56,57; Martinez, G.42; Martinez, M.45; Marzullo, D.50; Mauricio, J.43; Mocchiutti, E.48; Morettini, G.38; Mori, N.27; Mussolin, L.38; Mazziotta, M. N.25; Oliva, A.54; Orlandi, D.31; Osteria, G.34; Pacini, L.27; Panico, B.34; Pantaleo, F. R.26; Papa, S.49; Papini, P.27; Paredes, J. M.43; Parenti, A.29,30; Pauluzzi, M.38; Pearce, M.46; Peng, W. X.3; Perfetto, F.34; Perrina, C.47; Perrotta, G.49; Pillera, R.26; Pizzolotto, C.48
会议录名称Proceedings of Science
2022-03-18
卷号395
DOI10.22323/1.395.0067
产权排序第16完成单位
收录类别EI
会议名称37th International Cosmic Ray Conference, ICRC 2021
会议日期2021-07-12
会议地点Virtual, Berlin, Germany
摘要

The High Energy cosmic-Radiation Detection (HERD) facility is a space payload proposed to be installed onboard the China’s Space Station (CSS). The aims of HERD are the indirect detection of dark matter, the direct detection of cosmic rays towards the "knee" of the spectrum (∼ 1 PeV) and the monitoring of the full gamma-ray sky from 100 MeV. The HERD core is a calorimeter capable of accepting particles incident on its top and four lateral sides, each equipped with a sector of the scintillating fiber tracker: FIT. The FIT sectors host 7 tracking planes made of modules. The module, composed of a fiber mat and three arrays of silicon photomultipliers (SiPMs), is the elementary brick of FIT. Several FIT modules have been built and tested with particle beams at CERN. A FIT demonstrator, made of two partially instrumented tracking planes, has been assembled and sent through vibration tests. The results of the performed tests as well as the current design of FIT are presented in this contribution. © Copyright owned by the author(s).

资助项目N/A
项目资助者N/A
语种英语
学科领域天文学 ; 天体物理学 ; 高能天体物理学 ; 核科学技术
文章类型Conference article (CA)
出版者Sissa Medialab Srl
URL查看原文
EI入藏号20225213290580
EI主题词Cosmic rays
EI分类号656.1 Space Flight - 657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 741.1 Light/Optics - 931.3 Atomic and Molecular Physics - 932.1 High Energy Physics
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文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/25685
专题高能天体物理研究组
作者单位1.Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, CH-1015, Switzerland;
2.Département de Physique Nucléaire et Corpusculaire (DPNC), Université de Genève, Genève 4, CH-1211, Switzerland;
3.Key Laboratory of Particle and Astrophysics, Chinese Academy of Sciences, Beijing, China;
4.University of Chinese Academy of Sciences, Beijing, China;
5.Xi’an Institute of Optics and Precision Mechanics of CAS, Xi’an, China;
6.Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China;
7.School of Physical Science and Technology, Guangxi University, Nanning, China;
8.Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, China;
9.Key Laboratory of Particle Physics and Particle Irradiation, Ministry of Education, China;
10.School of Physical Science and Technology, Southwest Jiaotong University, Chengdu, China;
11.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, China;
12.Department of Modern Physics, University of Science and Technology of China, Hefei, China;
13.Department of Astronomy, Yunan University, Kunming, China;
14.North Night Vision Technology co. ltd., Kunming, China;
15.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
16.Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming, China;
17.School of Astronomy and Space Science, Nanjing University, Nanjing, China;
18.Department of Astronomy, Tsinghua University, Beijing, China;
19.Department of Astronomy, Peking University, Beijing, China;
20.Institute of Astrophysics, Central China Normal University, Wuhan, China;
21.Department of Physics, China University of Geosciences, Wuhan, China;
22.The University of Hong Kong, Hong Kong;
23.Institute of Physics, Academia Sinica, Taipei, Taiwan;
24.Università dell’Aquila, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy;
25.Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Bari, Italy;
26.Dipartimento di Fisica,
27.Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy;
28.Università di Firenze, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy;
29.Gran Sasso Science Institute, L’Aquila, Italy;
30.INFN Laboratori Nazionali del Gran Sasso, Assergi, L’Aquila, Italy;
31.INFN Laboratori Nazionali del Gran Sasso, L’Aquila, Italy;
32.Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Lecce, Italy;
33.Universitá del Salento, Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Lecce, Italy;
34.Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Napoli, Italy;
35.Università di Napoli
36.Istituto Nazionale di Fisica Nucleare, Sezione di Pavia, Pavia, Italy;
37.Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
38.Università degli Studi di Perugia, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
39.Università di Siena, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Pisa, Italy;
40.Département de Physique Nucléaire et Corpusculaire (DPNC), Université de Genève, Genève, Switzerland;
41.Department of Astronomy, University of Geneva, Geneva, Switzerland;
42.Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, E-28040, Spain;
43.Dept. Física Quàntica i Astrofísica, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Barcelona, Spain;
44.Universitat Pompeu Fabra (UPF), Barcelona, Spain;
45.Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), Bellaterra, Barcelona, E-08193, Spain;
46.KTH Royal Institute of Technology, Stockholm, Sweden;
47.Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland;
48.Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Trieste, Italy;
49.Università degli Studi di Napoli Federico II, Napoli, Italy;
50.Università degli Studi di Trieste, Italy;
51.Italian Space Agency, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
52.Università degli Studi di Sassari, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
53.Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, Rome, Italy;
54.Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Bologna, Italy;
55.Università di Bologna, Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Bologna, Italy;
56.Dipartimento di Fisica e Chimica
57.INFN sez. Catania, Catania, Italy
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GB/T 7714		 Perrina, C.,Azzarello, P.,Cadoux, F.,et al. FIT: the scintillating fiber tracker of the HERD space mission[C]:Sissa Medialab Srl,2022.
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