The High Energy cosmic-Radiation Detector (HERD) Trigger System

doi:10.22323/1.395.0062

YNAO OpenIR > 高能天体物理研究组

	The High Energy cosmic-Radiation Detector (HERD) Trigger System
	Velasco, M. A.1; Bao, T.2; Berti, E.3; Bonvicini, V.4; Casaus, J.1; Giovacchini, F.1; Liu, X.2; Marco, R.1; Marín, J.1; Martínez, G.1; Mori, N.3; Oliva, A.5; Pacini, L.3; Quan, Z.2; Tang, Z.2; Xu, M.2; Zampa, G.4; Zampa, N.4; Adriani, O.31; Alemanno, F.32,33; Aloisio, R.32,33; Altomare, C.28; Ambrosi, G.40; An, Q.15; Antonelli, M.51; Azzarello, P.43; Bai, L.13; Bai, Y. L.8; Bao, T. W.6; Barbanera, M.40; Barbato, F. C.32,33; Bernardini, P.36; Bertucci, B.41; Bi, X. J.6; Bigongiari, G.42; Bongi, M.31; Bordas, P.46; Bosch-Ramon, V.46; Bottai, S.30; Brogi, P.42; Cadoux, F.43; Campana, D.37; Cao, W. W.8; Cao, Z.6; Catanzani, E.41; Cattaneo, P. W.39; Chang, J.14,18; Chang, Y. H.26; Chen, G. M.6; Chen, Y.20; Cianetti, F.41; Comerma, A.46,47; Cortis, D.34; Cui, X. H.18; Cui, X. Z.6; Dai, C.10; Dai, Z. G.20; D'Alessandro, R.31; De Gaetanoe, S.29; De Mitri, I.32,33; de Palma, F.36; Di Felice, V.56; Di Giovanni, A.32,33; Di Santo, M.32,33; Di Venere, L.29; Dong, J. N.11,12; Dong, Y. W.6; Donvito, G.28; Duranti, M.40; D'Urso, D.55; Evoli, C.32,33; Fang, K.6; Fariña, L.48; Favre, Y.43; Feng, C. Q.15; Feng, H.21; Feng, H. B.10; Feng, Z. K.10; Finetti, N.27; Formato, V.56; Frieden, J. M.50; Fusco, P.29; Gao, J. R.8; Gargano, F.28; Gascon-Fora, D.46; Gasparrini, D.56; Giglietto, N.29; Gomez, S.46; Gong, K.6; Gou, Q. B.6; Guida, R.52; Guo, D. Y.6; Guo, J. H.14; Guo, Y. Q.6; He, H. H.6; Hu, H. B.6; Hu, J. Y.6,7; Hu, P.6,7; Hu, Y. M.14; Huang, G. S.15; Huang, J.6; Huang, W. H.11,12; Huang, X. T.11,12; Huang, Y. B.10; Huang, Y. F.20; Ionica, M.40; Jouvin, L.48; Kotenko, A.43; Kyratzis, D.32,33; La Marra, D.43; Li, M. J.11,12; Li, Q. Y.11,12; Li, R.8; Li, S. L.6,7; Li, T.11,12; Li, X.14; Li, Z.22; Li, Z. H.6,7; Liang, E. W.10; Liang, M. J.6,7; Liao, C. L.13; Licciulli, F.28; Lin, S. J.6; Liu, D.11,12; Liu, H. B.10; Liu, H.13; Liu, J. B.15; Liu, S. B.15; Liu, X. W.10; Liu, Y. Q.6; Loparco, F.29; Loporchio, S.28; Lu, X.10; Lyu, J. G.9; Lyu, L. W.8; Maestro, P.42; Mancini, E.40; Manera, R.46; Marrocchesi, P. S.42; Marsella, G.59,60; Martinez, M.48; Marzullo, D.53; Mauricio, J.46; Mocchiutti, E.51; Morettini, G.41; Mussolin, L.41; Nicola Mazziotta, M.28; Orlandi, D.34; Osteria, G.37; Panico, B.37; Pantalei, F. R.29; Papa, S.52; Papini, P.30; Paredes, J. M.46; Parenti, A.32,33; Pauluzzi, M.41; Pearce, M.49; Peng, W. X.6; Perfetto, F.37; Perrina, C.50; Perrotta, G.52; Pillera, R.29; Pizzolotto, C.51; Qiao, R.6
会议录名称	Proceedings of Science
	2022-03-18
卷号	395
DOI	10.22323/1.395.0062
产权排序	第19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 next generation spaceborne detector to be installed onboard the Chinese Space Station for about 10 years. HERD will address major problems in fundamental physics and astrophysics, providing precise measurements of charged-cosmic rays up to PeV energies, performing indirect searches for dark matter in the electron spectrum up to few tens of TeV and monitoring the gamma-ray skymap for surveys and transient searches. HERD is composed of a 3D imaging calorimeter (CALO) surrounded by a scintillating fiber tracker (FIT), a plastic scintillator detector (PSD) and a silicon charge detector (SCD). In addition, a transition radiation detector (TRD) is placed on a lateral side to provide accurate energy calibration. Based on this innovative design, the effective geometric factor of HERD will be one order of magnitud larger than that of current space-based detectors. The HERD trigger strategy is designed to accomplish the scientific goals of the mission, and is based on trigger definitions that rely on the energy deposited in CALO and the PSD. The trigger performances are evaluated using a detailed Monte Carlo simulation that includes the latest HERD geometry. In addition, alternative trigger definitions based on the event topology can be established thanks to the photodiode readout of CALO crystals. The feasibility of these topological triggers is also investigated and presented. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
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	20225113275758
EI主题词	Cosmic rays
EI分类号	656.1 Space Flight - 657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 723.4 Artificial Intelligence - 921.4 Combinatorial Mathematics, Includes Graph Theory, Set Theory - 922.2 Mathematical Statistics - 931.3 Atomic and Molecular Physics - 932.1 High Energy Physics
引用统计
文献类型	会议论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/25687
专题	高能天体物理研究组
作者单位	1.Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Avda. Complutense 40, Madrid, E-28040, Spain; 2.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China; 3.Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Firenze, Via G. Sansone 1, Florence, Sesto Fiorentino, I-50019, Italy; 4.Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Trieste, Padriciano 99, Trieste, I-34012, Italy; 5.Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Bologna, Viale Carlo Berti Pichat, 6/2, BO, Bologna, 40127, Italy; 6.Key Laboratory of Particle and Astrophysics, Chinese Academy of Sciences, Beijing, China; 7.University of Chinese Academy of Sciences, Beijing, China; 8.Xi'an Institute of Optics and Precision Mechanics, CAS, Xi'an, China; 9.Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China; 10.School of Physical Science and Technology, Guangxi University, Nanning, China; 11.Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, China; 12.Key Laboratory of Particle Physics and Particle Irradiation, Ministry of Education, China; 13.School of Physical Science and Technology, Southwest Jiaotong University, Chengdu, China; 14.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, China; 15.Department of Modern Physics, University of Science and Technology of China, Hefei, China; 16.Department of Astronomy, Yunan University, Kunming, China; 17.North Night Vision Technology Co. Ltd., Kunming, China; 18.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China; 19.Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming, China; 20.School of Astronomy and Space Science, Nanjing University, Nanjing, China; 21.Department of Astronomy, Tsinghua University, Beijing, China; 22.Department of Astronomy, Peking University, Beijing, China; 23.Institute of Astrophysics, Central China Normal University, Wuhan, China; 24.Department of Physics, China University of Geosciences, Wuhan, China; 25.The University of Hong Kong, Hong Kong; 26.Institute of Physics, Academia Sinica, Taipei, Taiwan; 27.Universitá dell'Aquila, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy; 28.Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Bari, Italy; 29.Dipartimento di Fisica 30.Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy; 31.Universitá di Firenze, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy; 32.Gran Sasso Science Institute, L'Aquila, Italy; 33.INFN, Laboratori Nazionali del Gran Sasso, Assergi, L'Aquila, Italy; 34.INFN, Laboratori Nazionali del Gran Sasso, L'Aquila, Italy; 35.Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Lecce, Italy; 36.Universitá del Salento, Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Lecce, Italy; 37.Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Napoli, Italy; 38.Universitá di Napoli 39.Istituto Nazionale di Fisica Nucleare, Sezione di Pavia, Pavia, Italy; 40.Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 41.Universitá degli Studi di Perugia, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 42.Universitá di Siena, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Pisa, Italy; 43.Département de Physique Nucléaire et Corpusculaire (DPNC), Université de Genève, Genève, Switzerland; 44.Department of Astronomy, University of Geneva, Geneva, Switzerland; 45.Centro de Investigaciones Energéticas Medioambientales y Tecnoló Gicas (CIEMAT), Madrid, E-28040, Spain; 46.Dept. Física Quàntica i Astrofísica, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Barcelona, Spain; 47.Universitat Pompeu Fabra (UPF), Barcelona, Spain; 48.Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), Bellaterra, Barcelona, E-08193, Spain; 49.KTH Royal Institute of Technology, Stockholm, Sweden; 50.Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland; 51.Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Trieste, Italy; 52.Universitá degli Studi di Napoli Federico II, Napoli, Italy; 53.Universitá degli Studi di Trieste, Italy; 54.Italian Space Agency, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 55.Universitá degli Studi di Sassari, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy; 56.Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, Rome, Italy; 57.INFN Sezione di Bologna, Bologna, 40126, Italy; 58.Universitá di Bologna, Bologna, 40126, Italy; 59.Dipartimento di Fisica e Chimica 60.INFN sez. Catania, Catania, Italy
推荐引用方式 GB/T 7714	Velasco, M. A.,Bao, T.,Berti, E.,et al. The High Energy cosmic-Radiation Detector (HERD) Trigger System[C]:Sissa Medialab Srl,2022.

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