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Gamma-ray performance study of the HERD payload
Adriani, O.26; Alemanno, F.27,28; Aloisio, R.27,28; Altomare, C.23; Ambrosi, G.35; An, Q.10; Antonelli, M.46; Azzarello, P.38; Bai, L.8; Bai, Y. L.3; Bao, T. W.1; Barbanera, M.35; Barbato, F. C.27,28; Bernardini, P.31; Berti, E.26; Bertucci, B.36; Bi, X. J.1; Bigongiari, G.37; Bongi, M.26; Bonvicini, V.46; Bordas, P.41; Bosch-Ramon, V.41; Bottai, S.25; Brogi, P.37; Cadoux, F.38; Campana, D.32; Cao, W. W.3; Cao, Z.1; Casaus, J.40; Catanzani, E.36; Cattaneo, P. W.34; Chang, J.9,13; Chang, Y. H.21; Chen, G. M.1; Chen, Y.15; Cianetti, F.36; Comerma, A.41,42; Cortis, D.29; Cui, X. H.13; Cui, X. Z.1; Dai, C.5; Dai, Z. G.15; D'Alessandro, R.26; De Gaetano, S.24; De Mitri, I.27,28; de Palma, F.31; Di Felice, V.51; Di Giovanni, A.27,28; Di Santo, M.27,28; Di Venere, L.24; Dong, J. N.6,7; Dong, Y. W.1; Donvito, G.23; Duranti, M.35; D'Urso, D.50; Evoli, C.27,28; Fang, K.1; Fariña, L.43; Favre, Y.38; Feng, C. Q.10; Feng, H.16; Feng, H. B.5; Feng, Z. K.5; Finetti, N.22; Formato, V.51; Frieden, J. M.45; Fusco, P.24; Gao, J. R.3; Gargano, F.23; Gascon-Fora, D.41; Gasparrini, D.51; Giglietto, N.24; Giovacchini, F.40; Gomez, S.41; Gong, K.1; Gou, Q. B.1; Guida, R.47; Guo, D. Y.1; Guo, J. H.9; Guo, Y. Q.1; He, H. H.1; Hu, H. B.1; Hu, J. Y.1,2; Hu, P.1,2; Hu, Y. M.9; Huang, G. S.10; Huang, J.1; Huang, W. H.6,7; Huang, X. T.6,7; Huang, Y. B.5; Huang, Y. F.15; Ionica, M.35; Jouvin, L.43; Kotenko, A.38; Kyratzis, D.27,28; La Marra, D.38; Li, M. J.6,7; Li, Q. Y.6,7; Li, R.3; Li, S. L.1,2; Li, T.6,7; Li, X.9; Li, Z.17; Li, Z. H.1,2; Liang, E. W.5; Liang, M. J.1,2; Liao, C. L.8; Licciulli, F.23; Lin, S. J.1; Liu, D.6,7; Liu, H. B.5; Liu, H.8; Liu, J. B.10; Liu, S. B.10; Liu, X.1,2; Liu, X. W.5; Liu, Y. Q.1; Loparco, F.24; Loporchio, S.23; Lu, X.5; Lyu, J. G.4; Lyu, L. W.3; Maestro, P.37; Mancini, E.35; Manera, R.41; Marin, J.40; Marrocchesi, P. S.37; Marsella, G.54,55; Martinez, G.40; Martinez, M.43; Marzullo, D.48; Mauricio, J.41; Mocchiutti, E.46; Morettini, G.36; Mori, N.25; Mussolin, L.36; Nicola Mazziotta, M.23; Oliva, A.52; Orlandi, D.29; Osteria, G.32; Pacini, L.25; Panico, B.32; Pantaleo, F. R.24; Papa, S.47; Papini, P.25; Paredes, J. M.41; Parenti, A.27,28; Pauluzzi, M.36; Pearce, M.44; Peng, W. X.1; Perfetto, F.32; Perrina, C.45; Perrotta, G.47; Pillera, R.24; Pizzolotto, C.46; Qiao, R.1; Qin, J. J.3; Quadrani, L.52,53; Quan, Z.1; Rappoldi, A.34; Raselli, G.34; Ren, X. X.6,7; Renno, F.47; Ribo, M.41
会议录名称Proceedings of Science
2022-03-18
卷号395
DOI10.22323/1.395.0651
产权排序第14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 has been proposed as a space astronomy payload onboard the future China's Space Station. HERD is planned for operation starting around 2027 for about 10 years In addition to the unprecedented sensitivity for dark matter searches and cosmic-ray measurements up to the knee energy, it should perform gamma-ray monitoring and full sky survey from few hundred MeV up to tens of TeV. We present the first study of the HERD gamma-ray performance obtained with full simulations of the whole detector geometry. HERD will be a cubic detector composed with 5 active faces. We present a study conducted inside the HERD analysis software package, which includes a detailed description of the detector materials. In this work we present the HERD effective area, the point spread function and the resulting gamma-ray sensitivity. © 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20230113326372
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
引用统计
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/25721
专题高能天体物理研究组
作者单位1.Key Laboratory of Particle and Astrophysics, Chinese Academy of Sciences, Beijing, China;
2.University of Chinese Academy of Sciences, Beijing, China;
3.Xi'an Institute of Optics and Precision Mechanics of CAS, Xi'an, China;
4.Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China;
5.School of Physical Science and Technology, Guangxi University, Nanning, China;
6.Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, China;
7.Key Laboratory of Particle Physics and Particle Irradiation, Ministry of Education, China;
8.School of Physical Science and Technology, Southwest Jiaotong University, Chengdu, China;
9.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, China;
10.Department of Modern Physics, University of Science and Technology of China, Hefei, China;
11.Department of Astronomy, Yunan University, Kunming, China;
12.North Night Vision Technology co. ltd., Kunming, China;
13.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
14.Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming, China;
15.School of Astronomy and Space Science, Nanjing University, Nanjing, China;
16.Department of Astronomy, Tsinghua University, Beijing, China;
17.Department of Astronomy, Peking University, Beijing, China;
18.Institute of Astrophysics, Central China Normal University, Wuhan, China;
19.Department of Physics, China University of Geosciences, Wuhan, China;
20.The University of Hong Kong, Hong Kong;
21.Institute of Physics, Academia Sinica, Taipei, Taiwan;
22.Universitá dell'Aquila, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy;
23.Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Bari, Italy;
24.Dipartimento di Fisica
25.Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy;
26.Universitá di Firenze, Istituto Nazionale di Fisica Nucleare, Sezione di Firenze, Firenze, Italy;
27.Gran Sasso Science Institute, L'Aquila, Italy;
28.INFN Laboratori Nazionali del Gran Sasso, L'Aquila, Assergi, Italy;
29.INFN Laboratori Nazionali del Gran Sasso, L'Aquila, Italy;
30.Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Lecce, Italy;
31.Universitá del Salento, Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Lecce, Italy;
32.Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Napoli, Italy;
33.Universitá di Napoli
34.Istituto Nazionale di Fisica Nucleare, Sezione di Pavia, Pavia, Italy;
35.Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
36.Universitá degli Studi di Perugia, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
37.Universitá di Siena, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Pisa, Italy;
38.Département de Physique Nucléaire et Corpusculaire (DPNC), Université de Genève, Genève, Switzerland;
39.Department of Astronomy, University of Geneva, Geneva, Switzerland;
40.Centro de Investigaciones Energéticas, Medioambientales y Tecnoló gicas (CIEMAT), Madrid, E-28040, Spain;
41.Dept. Física Quàntica i Astrofísica, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Barcelona, Spain;
42.Universitat Pompeu Fabra (UPF), Barcelona, Spain;
43.Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), Bellaterra, Barcelona, E-08193, Spain;
44.KTH Royal Institute of Technology, Stockholm, Sweden;
45.Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland;
46.Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Trieste, Italy;
47.Universitá degli Studi di Napoli Federico II, Napoli, Italy;
48.Universitá degli Studi di Trieste, Italy;
49.Italian Space Agency, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
50.Universitá degli Studi di Sassari, Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, Perugia, Italy;
51.Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, Rome, Italy;
52.INFN Sezione di Bologna, Bologna, 40126, Italy;
53.Universitá di Bologna, Bologna, 40126, Italy;
54.Dipartimento di Fisica e Chimica
55.INFN sez. Catania, Catania, Italy
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Adriani, O.,Alemanno, F.,Aloisio, R.,et al. Gamma-ray performance study of the HERD payload[C]:Sissa Medialab Srl,2022.
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