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WoS	SCOPUS	Document Type	Document Title	Abstract	Authors	Affiliation	ResearcherID (WoS)	AuthorsID (SCOPUS)	Author Email(s)	Journal Name	JCR Abbreviation	ISSN	eISSN	Volume	Issue	WoS Edition	WoS Category	JCR Year	IF	FWCI ⓘ	FWCI Update Date	WoS Citation	SCOPUS Citation	Keywords (WoS)	KeywordsPlus (WoS)	Keywords (SCOPUS)	KeywordsPlus (SCOPUS)	Language	Publication Stage	Publication Year	Publication Date	DOI	JCR Link	DOI Link	WOS Link	SCOPUS Link
	○	Article ⓘ	Prognostic Value of Baseline Neutrophil-to-Lymphocyte Ratio Combined With Anemia in Patients With ST-Segment Elevation Myocardial Infarction: A Nationwide Prospective Cohort Study ⓘ	Objective: Data pertaining to the prognostic value of the combination of high neutrophil-to-lymphocyte ratio (NLR) and anemia on admission in patients with ST-segment elevation myocardial infarction (STEMI) are limited. The objective of this study was to investigate the clinical value of baseline NLR in combination with anemia in predicting clinical outcomes after STEMI. Methods: A total of 5,194 consecutive patients with STEMI within 12 hours of symptom onset from the Korea Acute Myocardial Infarction Registry-National Institute of Health database between 2011 and 2015 were categorized into 4 groups according to their NLR and hemoglobin levels: low NLR (<4) without anemia (n=2,722; reference group); high NLR (≥4) without anemia (n=1,527); low NLR with anemia (n=508); and high NLR with anemia (n=437). The co-primary outcomes were 180-day and 3-year all-cause mortality. Results: Mortality rates significantly increased at the 3-year follow-up across the groups (3.3% vs. 5.4% vs. 16.5% vs. 21.7% for 180-day mortality and 5.3% vs. 9.0% vs. 23.8% vs. 33.4% for 3-year mortality; all p-trends <0.001). After adjusting for baseline covariates, the combination of high NLR and anemia was a significant predictor of 180-day mortality after STEMI with low NLR and no anemia as the reference (adjusted hazard ratio, 2.16; 95% confidence interval, 1.58–2.95; p<0.001). Similar findings were observed for the 3-year mortality. Conclusions: This nationwide prospective cohort study showed that the combination of high NLR (≥4) and anemia is a strong predictor of all-cause mortality after STEMI. © 2022 The Korean Society of Lipid and Atherosclerosis. ⓘ	Cho, Kyung Hoon; Shin, Min-Ho; Kim, Min Chul; Sim, Doo Sun; Hong, Young Joon; Kim, Ju Han; Ahn, Youngkeun; Chae, Shung Chull; Seong, In Whan; Park, Jong-Seon; Yoon, Chang-Hwan; Hur, Seung Ho; Lee, Sang Rok; Jeong, Myung Ho ⓘ	Department of Cardiology, Chonnam National University Hospital, Gwangju, South Korea; Department of Preventive Medicine, Chonnam National University Medical School, Hwasun, South Korea; Department of Cardiology, Chonnam National University Hospital, Gwangju, South Korea, Department of Cardiology, Chonnam National University Medical School, Hwasun, South Korea; Department of Cardiology, Chonnam National University Hospital, Gwangju, South Korea, Department of Cardiology, Chonnam National University Medical School, Hwasun, South Korea; Department of Cardiology, Chonnam National University Hospital, Gwangju, South Korea, Department of Cardiology, Chonnam National University Medical School, Hwasun, South Korea; Department of Cardiology, Chonnam National University Hospital, Gwangju, South Korea, Department of Cardiology, Chonnam National University Medical School, Hwasun, South Korea; Department of Cardiology, Chonnam National University Hospital, Gwangju, South Korea, Department of Cardiology, Chonnam National University Medical School, Hwasun, South Korea; Department of Cardiology, Kyungpook National University Hospital, Daegu, South Korea; Department of Cardiology, Chungnam National University Hospital, Daejeon, South Korea; Department of Cardiology, Yeungnam University Hospital, Daegu, South Korea; Department of Cardiology, Seoul National University Bundang Hospital, Seongnam, South Korea; Department of Cardiology, Keimyung University Dongsan Medical Center, Daegu, South Korea; Department of Cardiology, Jeonbuk National University Hospital, Jeonju, South Korea; Department of Cardiology, Chonnam National University Hospital, Gwangju, South Korea, Department of Cardiology, Chonnam National University Medical School, Hwasun, South Korea ⓘ	ⓘ	55595842500; 7401537616; 57202224572; 7006825347; 13310329100; 57196169644; 56937721300; 7101962036; 35254371300; 15763054600; 7202882965; 34570274500; 55887032200; 56485157500 ⓘ	myungho@chollian.net; ⓘ	Journal of Lipid and Atherosclerosis ⓘ	ⓘ	2287-2892		11	2		ⓘ			0.55	2025-06-25 ⓘ		5	ⓘ	ⓘ	Anemia; Lymphocytes; Neutrophils; ST elevation myocardial infarction ⓘ	ⓘ	English	Final	2022		10.12997/jla.2022.11.2.147 ⓘ		바로가기		바로가기
	○	Article ⓘ	Prognostic Value of Short-Term Follow-up of Multiple Biomarkers After Discharge in Hospitalized Patients With Acute Heart Failure (POSTBIO-HF): Rationale and Study Design ⓘ	Several surrogate biomarkers possess prognostic significance for heart failure (HF), and a decline in their respective values may predict clinical improvement. However, data on the prognostic value of these biomarkers during short-term follow-up after discharge in acute decompensated HF are scarce. We aim to evaluate the prognostic value of short-term follow-up of surrogate biomarkers for predicting the prognosis of hospitalized patients with acute decompensated HF. This multi-center, prospective study will enroll consecutive hospitalized patients with acute decompensated HF. All patients will undergo sampling and comparison of biomarkers, including plasma N-terminal pro-brain natriuretic peptide, growth differentiation factor 15, troponin-T, high-sensitivity C-reactive protein, and urinary albumin/creatinine ratio obtained within 1 month and 6 months after discharge from the index admission. The primary endpoint is a composite of cardiovascular mortality or HF hospitalization during 1 year of follow-up. We will investigate the prognostic value of multiple biomarkers for the primary endpoint. This trial will provide robust evidence for novel multi-biomarker strategies for acute decompensated HF in real-world settings. © 2022. Korean Society of Heart Failure. ⓘ	Cho, Dong-Hyuk; Son, Jung-Woo; Lee, Chan Joo; Choi, Jimi; Kim, Mi-Na; Lee, Ju-Hee; Lee, Sunki; Yang, Dong Heon; Cho, Hyun-Jai; Choi, Jin-Oh; Kim, Eung Ju; Choi, Dong-Ju; Yoo, Byung-Su ⓘ	Division of Cardiology, Department of Internal Medicine, Yonsei University Wonju College of Medicine, Wonju, South Korea; Division of Cardiology, Department of Internal Medicine, Yonsei University Wonju College of Medicine, Wonju, South Korea; Division of Cardiology, Department of Internal Medicine, Severance Hospital, Yonsei University College of Medicine, Seoul, South Korea; Division of Endocrinology and Metabolism, Department of Internal Medicine, Korea University College of Medicine, Seoul, South Korea; Division of Cardiology, Department of Internal Medicine, Korea University Anam Hospital, Seoul, South Korea; Division of Cardiology, Department of Internal Medicine, Chungbuk National University Hospital, Cheongju, South Korea; Division of Cardiology, Department of Internal Medicine, Dongtan Hospital, Hallym University, Hwaseong, South Korea; Division of Cardiology, Department of Internal Medicine, Kyungpook National University Hospital, Taegu, South Korea; Division of Cardiology, Department of Internal Medicine, Seoul National University Hospital, Seoul, South Korea; Division of Cardiology, Department of Internal Medicine, Sungkyunkwan University College of Medicine, Seoul, South Korea; Division of Cardiology, Department of Internal Medicine, Korea University Guro Hospital, Seoul, South Korea; Division of Cardiology, Cardiovascular Center, Seoul National University Bundang Hospital, Seongnam, South Korea; Division of Cardiology, Department of Internal Medicine, Yonsei University Wonju College of Medicine, Wonju, South Korea ⓘ	ⓘ	55314257200; 57201929388; 57226133622; 57221520689; 55686260600; 57204073070; 55642622400; 35277423400; 35285421400; 15848011800; 7404507139; 35274349200; 7102851884 ⓘ	yubs@yonsei.ac.kr; ⓘ	International Journal of Heart Failure ⓘ	ⓘ	2636-154X		4	2		ⓘ			0.23	2025-06-25 ⓘ		2	ⓘ	ⓘ	Biomarkers; Heart failure ⓘ	ⓘ	English	Final	2022		10.36628/ijhf.2022.0005 ⓘ		바로가기		바로가기
	○	Conference paper ⓘ	Properties of Cosmic Aluminum Nuclei: Results from the Alpha Magnetic Spectrometer ⓘ	We report the properties of aluminum (Al) nuclei in cosmic rays measured in the rigidity range 2.15 GV to 3.0 TV with 0.51 million nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. We observed that above 6 GV the Al spectrum is well described by the weighted sum of the silicon spectrum (primary cosmic rays) and the fluorine spectrum (secondary cosmic rays). The fraction of the primary component increases with rigidity and becomes dominant at highest rigidities. Al/Si abundance ratio at the source is determined independent of cosmic ray propagation. © Copyright owned by the author(s). ⓘ	Liu, Zhen; Paniccia, Mercedes; Zhang, Cheng; Aguilar, M.; Ali Cavasonza, L.; Alpat, B.; Ambrosi, G.; Arruda, L.; Attig, N.; Barao, F.; Barrin, L.; Bartoloni, A.; Başeğmez-Du Pree, S.; Battiston, R.; Behlmann, M.; Beranek, B.; Berdugo, J.; Bertucci, B.; Bindi, V.; Bollweg, K.; Borgia, B.; Boschini, M.J.; Bourquin, M.; Bueno, E.F.; Burger, J.; Burger, W.J.; Burmeister, S.; Cai, X.D.; Capell, M.; Casaus, J.; Castellini, G.; Cervelli, F.; Chang, Y.H.; Chen, G.M.; Chen, G.R.; Chen, H.S.; Chen, Y.; Cheng, L.; Chou, H.Y.; Chouridou, S.; Choutko, V.; Chung, C.H.; Clark, C.; Coignet, G.; Consolandi, C.; Contin, A.; Corti, C.; Cui, Z.; Dadzie, K.; Delgado, C.; Della Torre, S.; Demirköz, M.B.; Derome, L.; Di Falco, S.; Di Felice, V.; Díaz, C.; Dimiccoli, F.; von Doetinchem, P.; Dong, F.; Donnini, F.; Duranti, M.; Egorov, A.; Eline, A.; Feng, J.; Fiandrini, E.; Fisher, P.; Formato, V.; Freeman, C.; Gámez, C.; García-López, R.J.; Gargiulo, C.; Gast, H.; Gervasi, M.; Giovacchini, F.; Gómez-Coral, D.M.; Gong, J.; Goy, C.; Grabski, V.; Grandi, D.; Graziani, M.; Haino, S.; Han, K.C.; Hashmani, R.K.; He, Z.H.; Heber, B.; Hsieh, T.H.; Hu, J.Y.; Incagli, M.; Jang, W.Y.; Jia, Yi; Jinchi, H.; Khiali, B.; Kim, G.N.; Kirn, Th.; Konyushikhin, M.; Kounina, O.; Kounine, A.; Koutsenko, V.; Krasnopevtsev, D.; Kuhlman, A.; Kulemzin, A.; La Vacca, G.; Laudi, E.; Laurenti, G.; Lazzizzera, I.; Lebedev, A.; Lee, H.T.; Lee, S.C.; Li, J.Q.; Li, M.; Li, Q.; Li, S.; Li, J.H.; Li, Z.H.; Liang, J.; Light, C.; Lin, C.H.; Lippert, T.; Liu, J.H.; Lu, S.Q.; Lu, Y.S.; Luebelsmeyer, K.; Luo, J.Z.; Luo, Xi; Machate, F.; Mañá, C.; Marín, J.; Marquardt, J.; Martin, T.; Martínez, G.; Masi, N.; Maurin, D.; Medvedeva, T.; Menchaca-Rocha, A.; Meng, Q.; Mikhailov, V.V.; Molero, M.; Mott, P.; Mussolin, L.; Negrete, J.; Nikonov, N.; Nozzoli, F.; Oliva, A.; Orcinha, M.; Palermo, M.; Palmonari, F.; Pashnin, A.; Pauluzzi, M.; Pensotti, S.; Phan, H.D.; Plyaskin, V.; Pohl, M.; Poluianov, S.; Qin, X.; Qu, Z.Y.; Quadrani, L.; Rancoita, P.G.; Rapin, D.; Reina Conde, A.; Robyn, E.; Rosier-Lees, S.; Rozhkov, A.; Rozza, D.; Sagdeev, R.; Schael, S.; von Dratzig, A. Schulz; Schwering, G.; Seo, E.S.; Shakfa, Z.; Shan, B.S.; Siedenburg, T.; Solano, C.; Song, J.W.; Song, X.J.; Sonnabend, R.; Strigari, L.; Su, T.; Sun, Q.; Sun, Z.T.; Tacconi, M.; Tang, X.W.; Tang, Z.C.; Tian, J.; Ting, Samuel C.C.; Ting, S.M.; Tomassetti, N.; Torsti, J.; Tüysüz, C.; Urban, T.; Usoskin, I.; Vagelli, V.; Vainio, R.; Valencia-Otero, M.; Valente, E.; Valtonen, E.; Acosta, M. Vázquez; Vecchi, M.; Velasco, M.; Vialle, J.P.; Wang, C.X.; Wang, L.; Wang, L.Q.; Wang, N.H.; Wang, Q.L.; Wang, S.; Wang, X.; Wang, Yu; Wang, Z.M.; Wei, J.; Weng, Z.L.; Wu, H.; Xiong, R.Q.; Xu, W.; Yan, Q.; Yang, Y.; Yashin, I.I.; Yi, H.; Yu, Y.M.; Yu, Z.Q.; Zannoni, M.; Zhang, F.; Zhang, F.Z.; Zhang, J.H.; Zhang, Z.; Zhao, F.; Zheng, C.; Zheng, Z.M.; Zhuang, H.L.; Zhukov, V.; Zichichi, A.; Zuccon, P. ⓘ	DPNC, Université de Genève, Genève 4, 1211, Switzerland; DPNC, Université de Genève, Genève 4, 1211, Switzerland; Institute of High Energy Physics, Beijing, China; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; INFN Sezione di Perugia, Perugia, 06100, Italy; INFN Sezione di Perugia, Perugia, 06100, Italy; Laboratório de Instrumentação e Física Experimental de Partículas (LIP), Lisboa, 1649-003, Portugal; Jülich Supercomputing Centre, JARA-FAME, Research Centre Jülich, Jülich, 52425, Germany; Laboratório de Instrumentação e Física Experimental de Partículas (LIP), Lisboa, 1649-003, Portugal; European Organization for Nuclear Research (CERN), Geneva 23, 1211, Switzerland; INFN Sezione di Roma 1, Roma, 00185, Italy; Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, Groningen, 9700 AV, Netherlands; INFN TIFPA, Povo, Trento, 38123, Italy, Università di Trento, Povo, Trento, 38123, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; INFN Sezione di Perugia, Perugia, 06100, Italy, Università di Perugia, Perugia, 06100, Italy; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; National Aeronautics and Space Administration Johnson Space Center (JSC), Houston, 77058, TX, United States; INFN Sezione di Roma 1, Roma, 00185, Italy, Università di Roma La Sapienza, Roma, 00185, Italy; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy; DPNC, Université de Genève, Genève 4, 1211, Switzerland; Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, Groningen, 9700 AV, Netherlands; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN TIFPA, Povo, Trento, 38123, Italy; Institut für Experimentelle und Angewandte Physik, Christian-Alberts-Universität zu Kiel, Kiel, 24118, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; CNR–IROE, Firenze, 50125, Italy; INFN Sezione di Pisa, Pisa, 56100, Italy; Institute of Physics, Academia Sinica, Nankang, Taipei, 11529, Taiwan; Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing, 100049, China, University of Chinese Academy of Sciences (UCAS), Beijing, 100049, China; National Aeronautics and Space Administration Johnson Space Center (JSC), Houston, 77058, TX, United States; Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing, 100049, China, University of Chinese Academy of Sciences (UCAS), Beijing, 100049, China; DPNC, Université de Genève, Genève 4, 1211, Switzerland; National Aeronautics and Space Administration Johnson Space Center (JSC), Houston, 77058, TX, United States; Physics Department, Center for High Energy and High Field Physics, National Central University (NCU), Tao Yuan, 32054, Taiwan; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States, National Aeronautics and Space Administration Johnson Space Center (JSC), Houston, 77058, TX, United States; Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, LAPP-IN2P3, Annecy, 74000, France; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; INFN Sezione di Bologna, Bologna, 40126, Italy, Università di Bologna, Bologna, 40126, Italy; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; National Aeronautics and Space Administration Johnson Space Center (JSC), Houston, 77058, TX, United States, Shandong University (SDU), Shandong, Jinan, 250100, China; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy; Department of Physics, Middle East Technical University (METU), Ankara, 06800, Turkey; Univ. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, Grenoble, 38000, France; INFN Sezione di Pisa, Pisa, 56100, Italy; INFN Sezione di Roma Tor Vergata, Roma, 00133, Italy, ASI Space Science Data Center (SSDC), Roma, 00133, Italy; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; INFN TIFPA, Povo, Trento, 38123, Italy; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; Southeast University (SEU), Nanjing, 210096, China; INFN Sezione di Roma Tor Vergata, Roma, 00133, Italy, ASI Space Science Data Center (SSDC), Roma, 00133, Italy; INFN Sezione di Perugia, Perugia, 06100, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Perugia, Perugia, 06100, Italy, Università di Perugia, Perugia, 06100, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Roma Tor Vergata, Roma, 00133, Italy, ASI Space Science Data Center (SSDC), Roma, 00133, Italy; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; Instituto de Astrofísica de Canarias (IAC), La Laguna, 38205, Spain, Departamento de Astrofísica, Universidad de La Laguna, Tenerife, La Laguna, 38206, Spain; European Organization for Nuclear Research (CERN), Geneva 23, 1211, Switzerland; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy, Università di Milano–Bicocca, Milano, 20126, Italy; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; Southeast University (SEU), Nanjing, 210096, China; Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, LAPP-IN2P3, Annecy, 74000, France; Instituto de Física, Universidad Nacional Autónoma de México (UNAM), Ciudad de México, 01000, Mexico; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy, Università di Milano–Bicocca, Milano, 20126, Italy; INFN Sezione di Perugia, Perugia, 06100, Italy, Università di Perugia, Perugia, 06100, Italy; Institute of Physics, Academia Sinica, Nankang, Taipei, 11529, Taiwan; National Chung–Shan Institute of Science and Technology (NCSIST), Longtan, Tao Yuan, 32546, Taiwan; Department of Physics, Middle East Technical University (METU), Ankara, 06800, Turkey; Sun Yat–Sen University (SYSU), Guangzhou, 510275, China; Institut für Experimentelle und Angewandte Physik, Christian-Alberts-Universität zu Kiel, Kiel, 24118, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing, 100049, China, University of Chinese Academy of Sciences (UCAS), Beijing, 100049, China; INFN Sezione di Pisa, Pisa, 56100, Italy; CHEP, Kyungpook National University, Daegu, 41566, South Korea; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; National Chung–Shan Institute of Science and Technology (NCSIST), Longtan, Tao Yuan, 32546, Taiwan; INFN Sezione di Roma Tor Vergata, Roma, 00133, Italy, ASI Space Science Data Center (SSDC), Roma, 00133, Italy; CHEP, Kyungpook National University, Daegu, 41566, South Korea; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy, Università di Milano–Bicocca, Milano, 20126, Italy; European Organization for Nuclear Research (CERN), Geneva 23, 1211, Switzerland; INFN Sezione di Bologna, Bologna, 40126, Italy, Università di Bologna, Bologna, 40126, Italy; INFN TIFPA, Povo, Trento, 38123, Italy, Università di Trento, Povo, Trento, 38123, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Academia Sinica Grid Center (ASGC), Nankang, Taipei, 11529, Taiwan; Institute of Physics, Academia Sinica, Nankang, Taipei, 11529, Taiwan; Southeast University (SEU), Nanjing, 210096, China; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Southeast University (SEU), Nanjing, 210096, China; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Shandong University (SDU), Shandong, Jinan, 250100, China; Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing, 100049, China, University of Chinese Academy of Sciences (UCAS), Beijing, 100049, China; Shandong University (SDU), Shandong, Jinan, 250100, China; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; Institute of Physics, Academia Sinica, Nankang, Taipei, 11529, Taiwan; Jülich Supercomputing Centre, JARA-FAME, Research Centre Jülich, Jülich, 52425, Germany; Institute of Electrical Engineering (IEE), Chinese Academy of Sciences, Beijing, 100190, China; Institute of Physics, Academia Sinica, Nankang, Taipei, 11529, Taiwan; Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing, 100049, China; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Southeast University (SEU), Nanjing, 210096, China; National Aeronautics and Space Administration Johnson Space Center (JSC), Houston, 77058, TX, United States; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; Institut für Experimentelle und Angewandte Physik, Christian-Alberts-Universität zu Kiel, Kiel, 24118, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States, National Aeronautics and Space Administration Johnson Space Center (JSC), Houston, 77058, TX, United States; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; INFN Sezione di Bologna, Bologna, 40126, Italy, Università di Bologna, Bologna, 40126, Italy; Univ. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, Grenoble, 38000, France; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Instituto de Física, Universidad Nacional Autónoma de México (UNAM), Ciudad de México, 01000, Mexico; Southeast University (SEU), Nanjing, 210096, China; NRNU, MEPhI (Moscow Engineering Physics Institute), Moscow, 115409, Russian Federation; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States, National Aeronautics and Space Administration Johnson Space Center (JSC), Houston, 77058, TX, United States; INFN Sezione di Perugia, Perugia, 06100, Italy, Università di Perugia, Perugia, 06100, Italy; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; INFN TIFPA, Povo, Trento, 38123, Italy; INFN Sezione di Bologna, Bologna, 40126, Italy, Università di Bologna, Bologna, 40126, Italy; Laboratório de Instrumentação e Física Experimental de Partículas (LIP), Lisboa, 1649-003, Portugal; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; INFN Sezione di Bologna, Bologna, 40126, Italy, Università di Bologna, Bologna, 40126, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Perugia, Perugia, 06100, Italy, Università di Perugia, Perugia, 06100, Italy; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy, Università di Milano–Bicocca, Milano, 20126, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; DPNC, Université de Genève, Genève 4, 1211, Switzerland; Sodankylä Geophysical Observatory, Space Physics and Astronomy Research Unit, University of Oulu, Oulu, 90014, Finland; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Institute of Physics, Academia Sinica, Nankang, Taipei, 11529, Taiwan; INFN Sezione di Bologna, Bologna, 40126, Italy, Università di Bologna, Bologna, 40126, Italy; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy; DPNC, Université de Genève, Genève 4, 1211, Switzerland; Instituto de Astrofísica de Canarias (IAC), La Laguna, 38205, Spain, Departamento de Astrofísica, Universidad de La Laguna, Tenerife, La Laguna, 38206, Spain; DPNC, Université de Genève, Genève 4, 1211, Switzerland; Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, LAPP-IN2P3, Annecy, 74000, France; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy, Università di Milano–Bicocca, Milano, 20126, Italy; East–West Center for Space Science, University of Maryland, College Park, 207, MD, United States; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; IPST, University of Maryland, College Park, 20742, MD, United States; Department of Physics, Middle East Technical University (METU), Ankara, 06800, Turkey; Beihang University (BUAA), Beijing, 100191, China; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Shandong University (SDU), Shandong, Jinan, 250100, China; Shandong Institute of Advanced Technology (SDIAT), Shandong, Jinan, 250100, China; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; INFN Sezione di Roma 1, Roma, 00185, Italy; Shandong Institute of Advanced Technology (SDIAT), Shandong, Jinan, 250100, China; Shandong University (SDU), Shandong, Jinan, 250100, China; Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing, 100049, China, University of Chinese Academy of Sciences (UCAS), Beijing, 100049, China; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy, Università di Milano–Bicocca, Milano, 20126, Italy; Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing, 100049, China; Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing, 100049, China; INFN Sezione di Perugia, Perugia, 06100, Italy, Università di Perugia, Perugia, 06100, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States, European Organization for Nuclear Research (CERN), Geneva 23, 1211, Switzerland; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Perugia, Perugia, 06100, Italy, Università di Perugia, Perugia, 06100, Italy; Space Research Laboratory, Department of Physics and Astronomy, University of Turku, Turku, 20014, Finland; Department of Physics, Middle East Technical University (METU), Ankara, 06800, Turkey; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States, National Aeronautics and Space Administration Johnson Space Center (JSC), Houston, 77058, TX, United States; Sodankylä Geophysical Observatory, Space Physics and Astronomy Research Unit, University of Oulu, Oulu, 90014, Finland; INFN Sezione di Perugia, Perugia, 06100, Italy, Agenzia Spaziale Italiana (ASI), Roma, 001, Italy; Space Research Laboratory, Department of Physics and Astronomy, University of Turku, Turku, 20014, Finland; Physics Department, Center for High Energy and High Field Physics, National Central University (NCU), Tao Yuan, 32054, Taiwan; INFN Sezione di Roma 1, Roma, 00185, Italy, Università di Roma La Sapienza, Roma, 00185, Italy; Space Research Laboratory, Department of Physics and Astronomy, University of Turku, Turku, 20014, Finland; Instituto de Astrofísica de Canarias (IAC), La Laguna, 38205, Spain, Departamento de Astrofísica, Universidad de La Laguna, Tenerife, La Laguna, 38206, Spain; Kapteyn Astronomical Institute, University of Groningen, P.O. 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Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; INFN Sezione di Bologna, Bologna, 40126, Italy, Università di Bologna, Bologna, 40126, Italy; INFN TIFPA, Povo, Trento, 38123, Italy, Università di Trento, Povo, Trento, 38123, Italy ⓘ	ⓘ	57739250200; 56266617500; 56097029500; 22996439600; 57191410260; 7004466804; 7006385307; 7004947256; 57223376954; 35314473000; 55646582300; 35285626700; 29667446900; 7006819163; 55646746400; 57222348704; 57215449045; 35226994400; 57222995845; 57189869313; 7007048697; 57203921827; 35876701500; 57191419057; 35352197500; 7201366306; 56881766800; 35227001900; 35227003900; 35227047800; 7004686796; 7005849628; 36760341300; 56896268700; 57770857500; 59666635000; 56137098800; 59609731200; 56365790700; 59880360300; 57216843622; 7403613567; 26665276200; 7004915931; 57222996264; 57191631180; 56872614900; 57225771159; 36481146400; 55635066900; 55891367200; 15843124700; 57217206029; 10041262700; 23479571900; 56463148700; 56365795400; 57222997362; 57222997042; 56437611300; 35338969500; 9277807200; 35227188500; 56365757500; 7004110494; 34770275300; 38561219400; 57202653707; 57211714717; 7006562654; 6602129426; 22834585300; 7003542102; 7801414508; 57193066571; 57194348346; 7004647768; 12545785500; 8435313700; 55646269300; 6602286685; 56365702500; 57217054073; 9638950300; 8371200500; 57214622344; 57217061944; 7003367998; 59777356000; 57200080694; 55646334500; 56678677500; 35313854400; 7004426528; 22134943600; 55646570800; 6507961476; 35227523800; 57384463600; 12239763300; 16019713900; 25960147300; 26967798300; 7003952900; 35227498500; 7402203861; 56365458100; 55337748800; 59649303200; 57217055777; 59447556300; 59630035000; 57221810319; 57189355627; 56959673200; 57196712846; 37099295200; 57202385981; 56103245100; 56662601100; 57212185186; 6603714395; 56437050600; 44561341800; 57192255225; 35227644500; 7201368610; 56027602600; 57213093167; 7201759290; 54929862600; 23019068500; 59889210700; 56254267800; 59063266500; 8088744900; 57205664408; 57197414498; 57194701604; 58711964100; 38561788700; 6603891162; 57923509300; 56365718600; 57206439911; 7005895860; 57205658335; 35227915000; 7004136045; 57200079784; 35227897900; 59621291700; 55991195200; 58602560100; 56662705400; 9338192300; 57195453781; 7004095328; 57205657945; 57221808079; 15835400200; 57212750153; 55084788000; 57226207657; 56029998100; 6507857834; 35228049900; 7005953753; 57221799961; 55647041700; 14629476900; 57205656263; 56978396500; 57221805527; 57217054674; 59812536800; 57221800567; 59045426200; 55504541600; 54899147500; 35228080500; 57224667833; 57203395141; 35228106000; 35228151000; 25230473300; 7003546454; 58194973400; 57198326830; 7004683817; 55646766500; 7004090779; 57194199213; 35351623000; 35314156500; 35314150800; 7005558667; 57827162300; 24516496600; 57221808490; 59881421000; 56365823000; 7404340936; 7406915784; 58316262400; 57939847100; 35436531400; 59666826000; 59667047600; 36626819200; 59815832900; 36574222800; 57215821711; 57199874977; 57219734051; 6603852312; 57221300223; 57211439512; 57199729020; 7003655337; 59806546900; 57217058141; 56365642600; 57219233647; 57207165786; 57196415759; 56437095300; 57225700563; 7201458058; 57210687222; 23007073000 ⓘ	zhen.liu@cern.ch; ⓘ	Proceedings of Science ⓘ	ⓘ	1824-8039		395			ⓘ			0	2025-06-25 ⓘ		0	ⓘ	ⓘ	ⓘ	Cosmic rays; Cosmology; Particle spectrometers; Rigidity; Space stations; Abundance ratios; Alpha magnetic spectrometer experiment; Alpha magnetic spectrometers; Cosmic ray propagation; Cosmics; International Space stations; Property; Spectra's; Weighted Sum; Aluminum ⓘ	English	Final	2022		ⓘ				바로가기
	○	Conference paper ⓘ	Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer ⓘ	We report the observation of new properties of primary iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62 million iron nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. Above 80.5 GV the rigidity dependence of the cosmic ray Fe flux is identical to the rigidity dependence of the primary cosmic ray He, C, and O fluxes, with the Fe/O flux ratio being constant at 0.155±0.006. This shows that unexpectedly Fe and He, C, and O belong to the same class of primary cosmic rays which is different from the primary cosmic rays Ne, Mg, and Si class. © Copyright owned by the author(s). ⓘ	Chen, Yao; Paniccia, Mercedes; Aguilar, M.; Ali Cavasonza, L.; Allen, M.S.; Alpat, B.; Ambrosi, G.; Arruda, L.; Attig, N.; Barao, F.; Barrin, L.; Bartoloni, A.; Başeğmez-Du Pree, S.; Battiston, R.; Behlmann, M.; Beischer, B.; Berdugo, J.; Bertucci, B.; Bindi, V.; de Boer, W.; Bollweg, K.; Borgia, B.; Boschini, M.J.; Bourquin, M.; Bueno, E.F.; Burger, J.; Burger, W.J.; Burmeister, S.; Cai, X.D.; Capell, M.; Casaus, J.; Castellini, G.; Cervelli, F.; Chang, Y.H.; Chen, G.M.; Chen, G.R.; Chen, H.S.; Cheng, L.; Chou, H.Y.; Chouridou, S.; Choutko, V.; Chung, C.H.; Clark, C.; Coignet, G.; Consolandi, C.; Contin, A.; Corti, C.; Cui, Z.; Dadzie, K.; Delgado, C.; Della Torre, S.; Demirköz, M.B.; Derome, L.; Di Falco, S.; Di Felice, V.; Díaz, C.; Dimiccoli, F.; von Doetinchem, P.; Dong, F.; Donnini, F.; Duranti, M.; Egorov, A.; Eline, A.; Feng, J.; Fiandrini, E.; Fisher, P.; Formato, V.; Freeman, C.; Galaktionov, Y.; Gámez, C.; García-López, R.J.; Gargiulo, C.; Gast, H.; Gervasi, M.; Giovacchini, F.; Gómez-Coral, D.M.; Gong, J.; Goy, C.; Grabski, V.; Grandi, D.; Graziani, M.; Haino, S.; Han, K.C.; Hashmani, R.K.; He, Z.H.; Heber, B.; Hsieh, T.H.; Hu, J.Y.; Incagli, M.; Jang, W.Y.; Jia, Yi; Jinchi, H.; Kanishev, K.; Khiali, B.; Kim, G.N.; Kirn, Th.; Konyushikhin, M.; Kounina, O.; Kounine, A.; Koutsenko, V.; Kuhlman, A.; Kulemzin, A.; La Vacca, G.; Laudi, E.; Laurenti, G.; Lazzizzera, I.; Lebedev, A.; Lee, H.T.; Lee, S.C.; Li, J.Q.; Li, M.; Li, Q.; Li, S.; Li, J.H.; Li, Z.H.; Liang, J.; Light, C.; Lin, C.H.; Lippert, T.; Liu, J.H.; Liu, Z.; Lu, S.Q.; Lu, Y.S.; Luebelsmeyer, K.; Luo, J.Z.; Luo, Xi; Lyu, S.S.; Machate, F.; Mañá, C.; Marín, J.; Marquardt, J.; Martin, T.; Martínez, G.; Masi, N.; Maurin, D.; Menchaca-Rocha, A.; Meng, Q.; Mikhailov, V.V.; Mo, D.C.; Molero, M.; Mott, P.; Mussolin, L.; Negrete, J.; Nikonov, N.; Nozzoli, F.; Oliva, A.; Orcinha, M.; Palermo, M.; Palmonari, F.; Pashnin, A.; Pauluzzi, M.; Pensotti, S.; Phan, H.D.; Piandani, R.; Plyaskin, V.; Poluianov, S.; Qin, X.; Qu, Z.Y.; Quadrani, L.; Rancoita, P.G.; Rapin, D.; Reina Conde, A.; Robyn, E.; Rosier-Lees, S.; Rozhkov, A.; Rozza, D.; Sagdeev, R.; Schael, S.; von Dratzig, A. Schulz; Schwering, G.; Seo, E.S.; Shakfa, Z.; Shan, B.S.; Siedenburg, T.; Solano, C.; Song, J.W.; Song, X.J.; Sonnabend, R.; Strigari, L.; Su, T.; Sun, Q.; Sun, Z.T.; Tacconi, M.; Tang, X.W.; Tang, Z.C.; Tian, J.; Ting, Samuel C.C.; Ting, S.M.; Tomassetti, N.; Torsti, J.; Tüysüz, C.; Urban, T.; Usoskin, I.; Vagelli, V.; Vainio, R.; Valencia-Otero, M.; Valente, E.; Valtonen, E.; Vázquez Acosta, M.; Vecchi, M.; Velasco, M.; Vialle, J.P.; Wang, C.X.; Wang, L.; Wang, L.Q.; Wang, N.H.; Wang, Q.L.; Wang, S.; Wang, X.; Wang, Yu; Wang, Z.M.; Wei, J.; Weng, Z.L.; Wu, H.; Xiong, R.Q.; Xu, W.; Yan, Q.; Yang, Y.; Yashin, I.I.; Yi, H.; Yu, Y.M.; Yu, Z.Q.; Zannoni, M.; Zhang, C.; Zhang, F.; Zhang, J.H.; Zhang, Z.; Zhao, F.; Zheng, C.; Zheng, Z.M.; Zhuang, H.L.; Zhukov, V.; Zichichi, A.; Zimmermann, N.; Zuccon, P. ⓘ	Shandong Institute of Advanced Technology (SDIAT), Shandong, Jinan, 250100, China, Nikhef, Amsterdam, 1098 XG, Netherlands; DPNC, Université de Genève, Genève 4, 1211, Switzerland; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Perugia, Perugia, 06100, Italy; INFN Sezione di Perugia, Perugia, 06100, Italy; Laboratório de Instrumentação e Física Experimental de Partículas (LIP), Lisboa, 1649-003, Portugal; Jülich Supercomputing Centre, JARA-FAME, Research Centre Jülich, Jülich, 52425, Germany; Laboratório de Instrumentação e Física Experimental de Partículas (LIP), Lisboa, 1649-003, Portugal; European Organization for Nuclear Research (CERN), Geneva 23, 1211, Switzerland; INFN Sezione di Roma 1, Roma, 00185, Italy; Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, Groningen, 9700 AV, Netherlands, Nikhef, Amsterdam, 1098 XG, Netherlands; INFN TIFPA, Povo, Trento, 38123, Italy, Università di Trento, Povo, Trento, 38123, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; I. 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Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, Grenoble, 38000, France; INFN Sezione di Pisa, Pisa, 56100, Italy; INFN Sezione di Roma Tor Vergata, Roma, 00133, Italy, ASI Space Science Data Center (SSDC), Roma, 00133, Italy; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; INFN TIFPA, Povo, Trento, 38123, Italy; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; Southeast University (SEU), Nanjing, 210096, China; INFN Sezione di Roma Tor Vergata, Roma, 00133, Italy, ASI Space Science Data Center (SSDC), Roma, 00133, Italy; INFN Sezione di Perugia, Perugia, 06100, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Perugia, Perugia, 06100, Italy, Università di Perugia, Perugia, 06100, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Roma Tor Vergata, Roma, 00133, Italy, ASI Space Science Data Center (SSDC), Roma, 00133, Italy; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; Instituto de Astrofísica de Canarias (IAC), La Laguna, 38205, Spain, Departamento de Astrofísica, Universidad de La Laguna, Tenerife, La Laguna, 38206, Spain; European Organization for Nuclear Research (CERN), Geneva 23, 1211, Switzerland; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy, Università di Milano–Bicocca, Milano, 20126, Italy; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; Southeast University (SEU), Nanjing, 210096, China; Univ. Grenoble Alpes, Univ. Savoie Mont Blanc, CNRS, LAPP-IN2P3, Annecy, 74000, France; Instituto de Física, Universidad Nacional Autónoma de México (UNAM), Ciudad de México, 01000, Mexico; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy, Università di Milano–Bicocca, Milano, 20126, Italy; INFN Sezione di Perugia, Perugia, 06100, Italy, Università di Perugia, Perugia, 06100, Italy; Institute of Physics, Academia Sinica, Nankang, Taipei, 11529, Taiwan; National ChungShan Institute of Science and Technology (NCSIST), Longtan, Tao Yuan, 32546, Taiwan; Department of Physics, Middle East Technical University (METU), Ankara, 06800, Turkey; Sun Yat-Sen University (SYSU), Guangzhou, 510275, China; Institut für Experimentelle und Angewandte Physik, Christian-Alberts-Universität zu Kiel, Kiel, 24118, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing, 100049, China, University of Chinese Academy of Sciences (UCAS), Beijing, 100049, China; INFN Sezione di Pisa, Pisa, 56100, Italy; CHEP, Kyungpook National University, Daegu, 41566, South Korea; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; National ChungShan Institute of Science and Technology (NCSIST), Longtan, Tao Yuan, 32546, Taiwan; INFN TIFPA, Povo, Trento, 38123, Italy; INFN Sezione di Roma Tor Vergata, Roma, 00133, Italy, ASI Space Science Data Center (SSDC), Roma, 00133, Italy; CHEP, Kyungpook National University, Daegu, 41566, South Korea; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Physics and Astronomy Department, University of Hawaii, Honolulu, 96822, HI, United States; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; INFN Sezione di Milano–Bicocca, Milano, 20126, Italy, Università di Milano–Bicocca, Milano, 20126, Italy; European Organization for Nuclear Research (CERN), Geneva 23, 1211, Switzerland; INFN Sezione di Bologna, Bologna, 40126, Italy; INFN TIFPA, Povo, Trento, 38123, Italy, Università di Trento, Povo, Trento, 38123, Italy; Massachusetts Institute of Technology (MIT), Cambridge, 02139, MA, United States; Academia Sinica Grid Center (ASGC), Nankang, Taipei, 11529, Taiwan; Institute of Physics, Academia Sinica, Nankang, Taipei, 11529, Taiwan; Southeast University (SEU), Nanjing, 210096, China; I. 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Box 800, Groningen, 9700 AV, Netherlands; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, 28040, Spain; Univ. Grenoble Alpes, Univ. 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Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; INFN Sezione di Bologna, Bologna, 40126, Italy, Università di Bologna, Bologna, 40126, Italy; I. Physics Institute, JARA-FAME, RWTH Aachen University, Aachen, 52056, Germany; INFN TIFPA, Povo, Trento, 38123, Italy, Università di Trento, Povo, Trento, 38123, Italy ⓘ	ⓘ	56137098800; 56266617500; 22996439600; 57191410260; 55677088495; 7004466804; 7006385307; 7004947256; 57223376954; 35314473000; 55646582300; 35285626700; 29667446900; 7006819163; 55646746400; 22984136100; 57215449045; 35226994400; 57222995845; 8790523400; 57189869313; 7007048697; 57203921827; 35876701500; 57191419057; 35352197500; 7201366306; 56881766800; 35227001900; 35227003900; 35227047800; 7004686796; 7005849628; 36760341300; 56896268700; 57770857500; 59666635000; 59783845300; 56365790700; 59880360300; 57216843622; 7403613567; 26665276200; 7004915931; 57222996264; 57191631180; 56872614900; 57225771159; 36481146400; 55635066900; 55891367200; 15843124700; 57217206029; 10041262700; 23479571900; 56463148700; 56365795400; 57222997362; 57222997042; 56437611300; 35338969500; 9277807200; 35227188500; 56365757500; 7004110494; 34770275300; 38561219400; 57202653707; 7005152953; 57211714717; 7006562654; 6602129426; 22834585300; 7003542102; 7801414508; 57193066571; 57194348346; 7004647768; 12545785500; 8435313700; 55646269300; 6602286685; 56365702500; 57217054073; 9638950300; 8371200500; 57214622344; 57217061944; 7003367998; 59777356000; 57200080694; 55646334500; 14041902800; 56678677500; 35313854400; 7004426528; 22134943600; 55646570800; 6507961476; 35227523800; 12239763300; 16019713900; 25960147300; 26967798300; 7003952900; 35227498500; 7402203861; 56365458100; 55337748800; 59649303200; 57217055777; 59447556300; 59630035000; 57221810319; 57189355627; 56959673200; 57196712846; 37099295200; 57202385981; 56103245100; 57739250200; 56662601100; 57212185186; 6603714395; 56437050600; 44561341800; 57217660157; 57192255225; 35227644500; 7201368610; 56027602600; 57213093167; 7201759290; 54929862600; 23019068500; 56254267800; 59063266500; 8088744900; 23470418700; 57205664408; 57197414498; 57194701604; 58711964100; 38561788700; 6603891162; 57923509300; 56365718600; 57206439911; 7005895860; 57205658335; 35227915000; 7004136045; 57200079784; 24401662400; 35227897900; 55991195200; 58602560100; 56662705400; 9338192300; 57195453781; 7004095328; 57205657945; 57221808079; 15835400200; 57212750153; 55084788000; 57226207657; 56029998100; 6507857834; 35228049900; 7005953753; 57221799961; 55647041700; 14629476900; 57205656263; 56978396500; 57221805527; 57217054674; 59812536800; 57221800567; 59045426200; 55504541600; 54899147500; 35228080500; 57224667833; 57203395141; 35228106000; 35228151000; 25230473300; 7003546454; 58194973400; 57198326830; 7004683817; 55646766500; 7004090779; 57194199213; 35351623000; 35314156500; 35314150800; 7005558667; 57827162300; 24516496600; 57221808490; 59877174600; 56365823000; 7404340936; 7406915784; 58316262400; 57939847100; 35436531400; 59666826000; 59667047600; 36626819200; 59815832900; 36574222800; 57215821711; 57199874977; 57219734051; 6603852312; 57221300223; 57211439512; 57199729020; 7003655337; 56097029500; 57217058141; 56365642600; 57219233647; 57207165786; 57196415759; 56437095300; 57225700563; 7201458058; 57210687222; 57191284590; 23007073000 ⓘ	yao.chen@cern.ch; ⓘ	Proceedings of Science ⓘ	ⓘ	1824-8039		395			ⓘ			0	2025-06-25 ⓘ		0	ⓘ	ⓘ	ⓘ	C (programming language); Cosmic ray measurement; Cosmology; Iron; Rigidity; Space stations; Alpha magnetic spectrometer experiment; Alpha magnetic spectrometers; Fe fluxes; Fe O; Flux ratio; International Space stations; Iron nuclei; Property; Cosmic rays ⓘ	English	Final	2022		ⓘ				바로가기
	○	Book chapter ⓘ	Prospects and challenges of polymer nanocomposites for innovative food packaging ⓘ	Sustainable and affordable food packaging is a prerequisite for world food markets. Several plastic-based packaging approaches are functional during the transport and storing of food products as an orthodox packaging approach. Owing to food safety and quality, consumers’ preference, and shelf-life issues, conventional plastic-based packaging are highly discouraged. Thus, polymer-based nanocomposites are considered as potential alternatives to conventional food packaging toward innovative packaging of food materials. Several nanocomposites such as nanoparticles, nanotubes, nanoclays, nanoproteins, nanosheets, nanopolymers, and nanocarbohydrates are used in the food packaging market to replace petroleum-based plastic packaging throughout the world. However, the assessment of various nanocomposites in terms of food contact, microbial, and hygiene safety is still under investigation. Although biodegradable nanocomposites have multifunctional benefits to enhance the packaging of foods over the traditional packaging, food safety and compatibility of these nanocomposites are not explored vastly. Additionally, the merger of various polymers and their nanocomposites is in the initial research phase due to the incompatibility of heterogeneous chemical properties. Therefore, a customized and technological advancement is necessary to sustain the application of polymer nanocomposites as a sustainable packaging alternative for food products. This study emphasizes the contemporary trends and prospects of polymer nanocomposites for safe and affordable food packaging along with challenges toward innovative and state-of-the-art packaging developments. © 2023 Elsevier Inc. All rights reserved. ⓘ	Sarker, Aniruddha; Mondal, Shakti Chandra; Ahmmed, Raju; Rana, Juwel; Waheda Rahman Ansary, Most.; Bilal, Muhammad ⓘ	School of Applied Biosciences, College of Agriculture and Life Sciences, Kyungpook National University, Daegu, South Korea; Department of Integrative Food, Bioscience and Biotechnology, College of Agriculture and Life Sciences, Chonnam National University, Gwangju, South Korea, Department of Food Processing and Preservation, Hajee Mohammad Danesh Science and Technology University, Dinajpur, Bangladesh; Department of Chemical and Food Engineering, Dhaka University of Engineering & Technology, Gazipur, Bangladesh; Department of Nutrition & Food Engineering, Daffodil International University, Dhaka, Bangladesh; Department of Convergence Study on the Ocean Science and Technology, Korea Maritime and Ocean University, Busan, South Korea; Institute of Chemical Technology and Engineering, Faculty of Chemical Technology, Poznan University of Technology, Poznan, Poland ⓘ	ⓘ	57211874397; 57207912327; 57222186125; 57216908353; 58172069300; 58042993600 ⓘ	ⓘ	Smart Polymer Nanocomposites: Design, Synthesis, Functionalization, Properties, and Applications ⓘ	ⓘ						ⓘ			6.68	2025-06-25 ⓘ		14	ⓘ	ⓘ	biodegradable polymer; Food packaging; food safety; nanocomposites ⓘ	ⓘ	English	Final	2022		10.1016/b978-0-323-91611-0.00021-9 ⓘ		바로가기		바로가기
	○	Conference paper ⓘ	Prospects for neutrino astrophysics with Hyper-Kamiokande ⓘ	Hyper-Kamiokande is a multi-purpose next generation neutrino experiment. The detector is a two-layered cylindrical shape ultra-pure water tank, with its height of 64 m and diameter of 71 m. The inner detector will be surrounded by tens of thousands of twenty-inch photosensors and multi-PMT modules to detect water Cherenkov radiation due to the charged particles and provide our fiducial volume of 188 kt. This detection technique is established by Kamiokande and Super-Kamiokande. As the successor of these experiments, Hyper-K will be located deep underground, 600 m below Mt. Tochibora at Kamioka in Japan to reduce cosmic-ray backgrounds. Besides our physics program with accelerator neutrino, atmospheric neutrino and proton decay, neutrino astrophysics is an important research topic for Hyper-K. With its fruitful physics research programs, Hyper-K will play a critical role in the next neutrino physics frontier. It will also provide important information via astrophysical neutrino measurements, i.e., solar neutrino, supernova burst neutrinos and supernova relic neutrino. Here, we will discuss the physics potential of Hyper-K neutrino astrophysics. © Copyright owned by the author(s). ⓘ	Yano, Takatomi; Abe, K.; Adrich, P.; Aihara, H.; Akutsu, R.; Alekseev, I.; Ali, A.; Alj Hakim, Y.I.; Ameli, F.; Anthony, L.H.V.; Araya, A.; Asaoka, Y.; Aushev, V.; Ballester, F.; Bandac, I.; Barbi, M.; Barr, G.; Batkiewicz-Kwasniak, M.; Bellato, M.; Berardi, V.; Bernard, L.; Bernardini, E.; Berns, L.; Bhadra, S.; Bian, J.; Blanchet, A.; Blondel, A.; Boiano, A.; Bolognesi, S.; Bonavera, L.; Booth, N.; Bordoni, S.; Borjabad, S.; Boschi, T.; Bose, D.; Boyd, S.B.; Bozza, C.; Bravar, A.; Bronner, C.; Brown, L.; Bubak, A.; Buchowicz, A.; Buizza Avanzini, M.; Cafagna, F.S.; Calabria, N.F.; Calvo-Mozota, J.M.; Cao, S.; Carroll, A.; Catanesi, M.G.; Cebriàn, S.; Chakraborty, S.; Choi, J.H.; Choubey, S.; Cicerchia, M.; Coleman, J.; Collazuol, G.; Cuen-Rochin, S.; Danilov, M.; Díaz López, G.; De la Fuente, E.; de Perio, P.; De Rosa, G.; Dealtry, T.; Densham, C.J.; Dergacheva, A.; Deshmukh, N.; Devi, M.M.; Di Lodovico, F.; Di Meo, P.; Di Palma, I.; Doyle, T.A.; Drakopoulou, E.; Drapier, O.; Dumarchez, J.; Eklund, L.; El Hedri, S.; Ellis, J.; Emery, S.; Esmaili, A.; Esteve, R.; Fedotov, S.; Feng, J.; Fernandez, P.; Fernández-Martinez, E.; Ferrario, P.; Ferrazzi, B.; Finch, A.; Finley, C.; Fiorillo, G.; Fitton, M.; Friend, M.; Fujii, Y.; Fujisawa, C.; Fukuda, Y.; Galinski, G.; Gao, J.; Garde, C.; Garfagnini, A.; Garode, S.; Gialanella, L.; Giganti, C.; Gomez-Cadenas, J.J.; Gonin, M.; González-Nuevo, J.; Gorin, A.; Gornea, R.; Gousy-Leblanc, V.; Gramegna, F.; Grassi, M.; Grella, G.; Guigue, M.; Hadley, D.R.; Harada, M.; Hartz, M.; Hassani, S.; Hastings, N.C.; Hayato, Y.; Hernando-Morata, J.A.; Herrero, V.; Hiraide, K.; Holin, A.; Hoshina, K.; Hultqvist, K.; Iacob, F.; Ichikawa, A.K.; Idrissi Ibnsalih, W.; Ieki, K.; Ikeda, M.; Ioannisian, A.; Ishida, T.; Ishidoshiro, K.; Ishino, H.; Ishitsuka, M.; Israel, H.T.; Ito, H.; Itow, Y.; Izumi, N.; Izumiyama, S.; Jakkapu, M.; Jamieson, B.; Jang, J.S.; Jo, H.S.; Jonsson, P.; Joo, K.K.; Kajita, T.; Kakuno, H.; Kameda, J.; Kaneshima, R.; Kano, Y.; Karlen, D.; Kataoka, Y.; Kato, A.; Katori, T.; Kazarian, N.; Khabibullin, M.; Khotjantsev, A.; Kikawa, T.; Kekic, M.; Kim, J.Y.; Kim, S.B.; King, S.; Kinoshita, T.; Kisiel, J.; Klekotko, A.; Kobayashi, T.; Koerich, L.; Kolev, N.; Konaka, A.; Kormos, L.L.; Koshio, Y.; Kotsar, Y.; Kouzakov, K.A.; Kowalik, K.L.; Kravchuk, L.; Kryukov, A.P.; Kudenko, Y.; Kumita, T.; Kurjata, R.; Kutter, T.; Kuze, M.; Kwak, K.; La Commara, M.; Labarga, L.; Lagoda, J.; Lamers James, M.; Lamoureux, M.; Laveder, M.; Lavitola, L.; Lee, J.; Leitner, R.; Lezaun, V.; Li, B.; Lim, I.T.; Lindner, T.; Litchfield, R.P.; Long, K.R.; Longhin, A.; Loverre, P.; Lu, X.; Ludovici, L.; Maekawa, Y.; Magaletti, L.; Magar, K.; Makida, Y.; Malek, M.; Malinský, M.; Marchi, T.; Mariani, C.; Marinelli, A.; Martens, K.; Marti, Ll.; Martin, J.F.; Martin, D.; Marzec, J.; Matsubara, T.; Matsumoto, R.; McCauley, N.; Medhi, A.; Mehta, P.; Mellet, L.; Menjo, H.; Mezzetto, M.; Migenda, J.; Migliozzi, P.; Miki, S.; Miller, E.W.; Minamino, A.; Mine, S.; Mineev, O.; Munteanu, L.; Mitra, A.; Miura, M.; Moharana, R.; Mollo, C.M.; Mondal, T.; Mongelli, M.; Monrabal, F.; Moon, D.H.; Moon, C.S.; Mora, F.J.; Mori, M.; Moriyama, S.; Mueller, Th.A.; Nakadaira, T.; Nakagiri, K.; Nakahata, M.; Nakai, S.; Nakajima, Y.; Nakamura, K.; Nakamura, K.I.; Nakamura, H.; Nakanishi, S.; Nakano, Y.; Nakaya, T.; Nakayama, S.; Nakayoshi, K.; Nascimento Machado, L.; Naseby, C.E.R.; Navarro-Garcia, B.; Needham, M.; Niewczas, K.; Ninomiya, K.; Nishimori, S.; Nishimura, Y.; Noguchi, Y.; Nova, F.; Nugent, J.C.; Nunokawa, H.; Obrebski, W.; Ochoa-Ricoux, J.P.; O’Connor, E.; Ogawa, N.; Ogitsu, T.; Okamoto, K.; O’Keeffe, H.M.; Okumura, K.; Onishchuk, Y.; Orozco-Luna, F.; Oshlianskyi, A.; Ospina, N.; Ostrowski, M.; O’Sullivan, E.; Oyama, Y.; Ozaki, H.; Pac, M.Y.; Paganini, P.; Palladino, V.; Pari, M.; Pasternak, J.; Pastore, C.; Pastuszak, G.; Patel, D.A.; Pavin, M.; Payne, D.; Peña-Garay, C.; Pidcott, C.; Playfer, S.; Pointon, B.W.; Popov, A.; Popov, B.; Porwit, K.; Posiadala-Zezula, M.; Pronost, G.; Prouse, N.W.; Quilain, B.; Quiroga, A.A.; Radicioni, E.; Radics, B.; Rajda, P.J.; Renner, J.; Rescigno, M.; Ricciardi, G.; Richards, B.; Rondio, E.; Roskovec, B.; Roth, S.; Rott, C.; Rubbia, A.; Ruggeri, A.C.; Russo, S.; Rychter, A.; Ryu, D.; Sakashita, K.; Samani, S.; Sánchez, F.; Sánchez, M.L.; Sano, S.; Santos, J.D.; Santucci, G.; Sarmah, P.; Sato, K.; Scott, M.; Seiya, Y.; Sekiguchi, T.; Sekiya, H.; Seo, J.W.; Sgalaberna, D.; Shan, Z.; Shaykina, A.; Shiba, H.; Shimizu, I.; Shimizu, K.; Shin, C.D.; Shinoki, M.; Shiozawa, M.; Skrobova, N.; Skwarczynski, K.; Smy, M.B.; Sobczyk, J.; Sobel, H.W.; Soler, F.J.P.; Sonoda, Y.; Spina, R.; Spisso, B.; Spradlin, P.; Stankevich, K.L.; Stawarz, L.; Stellacci, S.M.; Studenikin, A.I.; Suárez Gómez, S.L.; Suganuma, T.; Suvorov, S.; Suwa, Y.; Suzuki, A.T.; Suzuki, S.Y.; Suzuki, Y.; Svirida, D.; Taani, M.; Tada, M.; Takeda, A.; Takemoto, Y.; Taketa, A.; Takeuchi, Y.; Tanaka, H.; Tanaka, H.I.; Tanaka, M.; Tashiro, T.; Thiesse, M.; Thompson, L.F.; Tiwari, D.; Toledo, J.F.; Tomatani-Sánchez, A.K.; Tortone, G.; Tsui, K.M.; Tsukamoto, T.; Tzanov, M.; Uchida, Y.; Vagins, M.R.; Valder, S.; Valentino, V.; Vasseur, G.; Vijayvargi, A.; Vinning, W.G.S.; Vivolo, D.; Vogelaar, R.B.; Vyalkov, M.M.; Wachala, T.; Wark, D.; Wascko, M.O.; Wendell, R.A.; Wilson, J.R.; Wronka, S.; Xia, J.; Xie, Z.; Yamaguchi, Y.; Yamamoto, K.; Yamauchi, K.; Yano, T.; Yershov, N.; Yokoyama, M.; Yonenaga, M.; Yoo, J.; Yu, I.; Zakrzewski, T.; Zaldivar, B.; Zalipska, J.; Zaremba, K.; Zarnecki, G.; Ziembicki, M.; Zietara, K.; Zito, M.; Zhu, T.; Zsoldos, S. ⓘ	Kamioka Observatory, ICRR, The University of Tokyo, Mozumi, Kamioka, Hida, Gifu, 456, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; National Centre for Nuclear Research, Warsaw, Poland; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Department of Physics, Tokyo, Japan; TRIUMF, Vancouver, BC, Canada; P.N.Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russian Federation; Kyoto University, Department of Physics, Kyoto, Japan; Imperial College London, Department of Physics, London, United Kingdom; INFN Sezione di Roma, Università Sapienza, Dipartimento di Fisica, Roma, Italy; Imperial College London, Department of Physics, London, United Kingdom; University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Earthquake Research Institute, Tokyo, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; Kyiv National University, Department of Nuclear Physics, Kyiv, Ukraine; Universitat Politècnica de València, Instituto de Instrumentaciòn para Imagen Molecular (i3M), Valencia, Spain; Laboratorio Subterráneo de Canfranc, Estación, Canfranc, Spain; University of Regina, Department of Physics, Regina, SK, Canada; Oxford University, Department of Physics, Oxford, United Kingdom; H. Niewodniczański Institute of Nuclear Physics PAN, Cracow, Poland; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; INFN Sezione di Bari, Università e Politecnico di Bari, Bari, Italy; Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; Tokyo Institute of Technology, Department of Physics, Tokyo, Japan; York University, Department of Physics and Astronomy, Toronto, ON, Canada; University of California, Irvine, Department of Physics and Astronomy, Irvine, CA, United States; Laboratoire de Physique Nucleaire et de Hautes Energie, IN2P3, CNRS, Sorbonne Universitè, Paris, France; Laboratoire de Physique Nucleaire et de Hautes Energie, IN2P3, CNRS, Sorbonne Universitè, Paris, France; INFN Sezione di Napoli, Napoli, Italy; IRFU, CEA, Universitè Paris-Saclay, Gif-sur-Yvette, France; University of Oviedo, Applied Mathematical Modeling Group, Department of Physics, Oviedo, Spain; University of Victoria, Department of Physics and Astronomy, Victoria, BC, Canada; University of Geneva, Section de Physique, DPNC, Geneva, Switzerland; Laboratorio Subterráneo de Canfranc, Estación, Canfranc, Spain; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; S. N. Bose National Centre for Basic Sciences, Salt Lake City, Kolkata, India; University of Warwick, Department of Physics, Coventry, United Kingdom; Università degli Studi di Salerno, INFN Gruppo Collegato di Salerno, Fisciano, Italy; University of Geneva, Section de Physique, DPNC, Geneva, Switzerland; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; University of Victoria, Department of Physics and Astronomy, Victoria, BC, Canada; University of Silesia in Katowice, A. Chełkowski Institute of Physics, Poland; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France; INFN Sezione di Bari, Università e Politecnico di Bari, Bari, Italy; INFN Sezione di Napoli, Università Federico II di Napoli, Dipartimento di Fisica, Napoli, Italy; Laboratorio Subterráneo de Canfranc, Estación, Canfranc, Spain; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Liverpool, Department of Physics, Liverpool, United Kingdom; INFN Sezione di Bari, Università e Politecnico di Bari, Bari, Italy; University of Zaragoza, Centro de Astropartículas y Física de Altas Energías (CAPA), Zaragoza, Spain; Indian Institute of Technology Guwahati, Guwahati, India; Dongshin University, Laboratory for High Energy Physics, Naju, South Korea; KTH Royal Institute of Technology, Department of Physics, Stockholm, Sweden; INFN Laboratori Nazionali di Legnaro, (PD), Legnaro, Italy; University of Liverpool, Department of Physics, Liverpool, United Kingdom; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; TRIUMF, Vancouver, BC, Canada, Universidad Autonoma de Sinaloa, Culiacan, Mexico; P.N.Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russian Federation; Universitat de Santiago de Compostela, Instituto Gallego de Física de Altas Enerxías, Santiago de Compostela, Spain; Universidad de Guadalajara, CUCEI, Departamento de Fisica, Jal., Guadalajara, Mexico, Universidad de Guadalajara, CUCEA, IT.Ph.D. program, Jal., Guadalajara, Mexico, University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan; TRIUMF, Vancouver, BC, Canada; INFN Sezione di Napoli, Università Federico II di Napoli, Dipartimento di Fisica, Napoli, Italy; Lancaster University, Physics Department, Lancaster, United Kingdom; STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; Vishwakarma Institute of Information Technology, Pune, India; Tezpur University, Department of Physics, Sonitpur, India; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; INFN Sezione di Napoli, Napoli, Italy; INFN Sezione di Roma, Università Sapienza, Dipartimento di Fisica, Roma, Italy; Lancaster University, Physics Department, Lancaster, United Kingdom; University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom; Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France; Laboratoire de Physique Nucleaire et de Hautes Energie, IN2P3, CNRS, Sorbonne Universitè, Paris, France; University of Glasgow, School of Physics and Astronomy, Glasgow, United Kingdom; Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; IRFU, CEA, Universitè Paris-Saclay, Gif-sur-Yvette, France; Pontifícia Universidade Católica do Rio de Janeiro, Departamento de Física, Rio de Janeiro, Brazil; Universitat Politècnica de València, Instituto de Instrumentaciòn para Imagen Molecular (i3M), Valencia, Spain; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; Kyoto University, Department of Physics, Kyoto, Japan; University of Liverpool, Department of Physics, Liverpool, United Kingdom; University Autonoma Madrid, Department of Theoretical Physics, Madrid, Spain; Donostia International Physics Center, Ikerbasque Foundation, Basque Country, Spain; University of Regina, Department of Physics, Regina, SK, Canada; Lancaster University, Physics Department, Lancaster, United Kingdom; Stockholm University, Oskar Klein Centre, Department of Physics, Stockholm, Sweden; INFN Sezione di Napoli, Università Federico II di Napoli, Dipartimento di Fisica, Napoli, Italy; STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; Keio University, Department of Physics, Yokohama, Japan; Miyagi University of Education, Department of Physics, Sendai, Japan; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; Vishwakarma Institute of Information Technology, Pune, India; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; Vishwakarma Institute of Information Technology, Pune, India; Università della Campania”L. Vanvitelli”, INFN Sezione di Napoli, Napoli, Italy; Laboratoire de Physique Nucleaire et de Hautes Energie, IN2P3, CNRS, Sorbonne Universitè, Paris, France; Donostia International Physics Center, Ikerbasque Foundation, Basque Country, Spain; Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France; University of Oviedo, Applied Mathematical Modeling Group, Department of Physics, Oviedo, Spain; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; Carleton University, Department of Physics, Ottawa, ON, Canada; University of Victoria, Department of Physics and Astronomy, Victoria, BC, Canada; INFN Laboratori Nazionali di Legnaro, (PD), Legnaro, Italy; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; Università degli Studi di Salerno, INFN Gruppo Collegato di Salerno, Fisciano, Italy; Laboratoire de Physique Nucleaire et de Hautes Energie, IN2P3, CNRS, Sorbonne Universitè, Paris, France; University of Warwick, Department of Physics, Coventry, United Kingdom; Okayama University, Department of Physics, Okayama, Japan; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, TRIUMF, Vancouver, BC, Canada; IRFU, CEA, Universitè Paris-Saclay, Gif-sur-Yvette, France; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; Universitat de Santiago de Compostela, Instituto Gallego de Física de Altas Enerxías, Santiago de Compostela, Spain; Universitat Politècnica de València, Instituto de Instrumentaciòn para Imagen Molecular (i3M), Valencia, Spain; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom; University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Earthquake Research Institute, Tokyo, Japan; Stockholm University, Oskar Klein Centre, Department of Physics, Stockholm, Sweden; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; Tohoku University, Department of Physics, Sendai, Japan; Università della Campania”L. Vanvitelli”, INFN Sezione di Napoli, Napoli, Italy; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; Institute for Theoretical Physics and Modeling, Yerevan, Armenia; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; Tohoku University, Research Center for Neutrino Science, Sendai, Japan; Okayama University, Department of Physics, Okayama, Japan; Tokyo University of Science, Department of Physics, Chiba, Japan; University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan; Nagoya University, Kobayashi-Maskawa Institute for the Origin of Particles, The Universe, Nagoya, Japan, Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan; Tokyo University of Science, Department of Physics, Chiba, Japan; Tokyo Institute of Technology, Department of Physics, Tokyo, Japan; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, SOKENDAI (The Graduate University for Advanced Studies), Tokai, Japan; University of Winnipeg, Department of Physics, Winnipeg, MB, Canada; GIST College, Gwangju Institute of Science and Technology, Gwangju, South Korea; Kyungpook National University, Department of Physics, Daegu, South Korea; Imperial College London, Department of Physics, London, United Kingdom; Chonnam National University, Department of Physics, Gwangju, South Korea; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan; Tokyo Metropolitan University, Department of Physics, Tokyo, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan; University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Earthquake Research Institute, Tokyo, Japan; TRIUMF, Vancouver, BC, Canada, University of Victoria, Department of Physics and Astronomy, Victoria, BC, Canada; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Earthquake Research Institute, Tokyo, Japan; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; Institute for Theoretical Physics and Modeling, Yerevan, Armenia; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; Kyoto University, Department of Physics, Kyoto, Japan; Universitat de Santiago de Compostela, Instituto Gallego de Física de Altas Enerxías, Santiago de Compostela, Spain; Chonnam National University, Department of Physics, Gwangju, South Korea; Sungkyunkwan University, Department of Physics, Suwon, South Korea; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; Tokyo University of Science, Department of Physics, Chiba, Japan; H. Niewodniczański Institute of Nuclear Physics PAN, Cracow, Poland, University of Silesia in Katowice, A. Chełkowski Institute of Physics, Poland; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Regina, Department of Physics, Regina, SK, Canada; University of Regina, Department of Physics, Regina, SK, Canada; TRIUMF, Vancouver, BC, Canada; Lancaster University, Physics Department, Lancaster, United Kingdom; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, Okayama University, Department of Physics, Okayama, Japan; Kobe University, Department of Physics, Kobe, Japan; Moscow State University, Department of Theoretical Physics, Moscow, Russian Federation; National Centre for Nuclear Research, Warsaw, Poland; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; Moscow State University, Department of Theoretical Physics, Moscow, Russian Federation; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; Tokyo Metropolitan University, Department of Physics, Tokyo, Japan; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; Louisiana State University, Department of Physics and Astronomy, Baton Rouge, LA, United States; Tokyo Institute of Technology, Department of Physics, Tokyo, Japan; Ulsan National Institute of Science and Technology, Department of Physics, Ulsan, South Korea; INFN Sezione di Napoli, Università Federico II di Napoli, Dipartimento di Fisica, Napoli, Italy; University Autonoma Madrid, Department of Theoretical Physics, Madrid, Spain; National Centre for Nuclear Research, Warsaw, Poland; Lancaster University, Physics Department, Lancaster, United Kingdom, STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; INFN Sezione di Napoli, Università Federico II di Napoli, Dipartimento di Fisica, Napoli, Italy; Kyungpook National University, Department of Physics, Daegu, South Korea; Charles University, IPNP, FMF, Prague, Czech Republic; Laboratorio Subterráneo de Canfranc, Estación, Canfranc, Spain; ETH Zurich, Institute for Particle and Astroparticle Physics, Zurich, Switzerland; Chonnam National University, Department of Physics, Gwangju, South Korea; TRIUMF, Vancouver, BC, Canada; University of Glasgow, School of Physics and Astronomy, Glasgow, United Kingdom; Imperial College London, Department of Physics, London, United Kingdom; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; INFN Sezione di Roma, Università Sapienza, Dipartimento di Fisica, Roma, Italy; Oxford University, Department of Physics, Oxford, United Kingdom; INFN Sezione di Roma, Università Sapienza, Dipartimento di Fisica, Roma, Italy; Keio University, Department of Physics, Yokohama, Japan; INFN Sezione di Bari, Università e Politecnico di Bari, Bari, Italy; Vishwakarma Institute of Information Technology, Pune, India; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom; Charles University, IPNP, FMF, Prague, Czech Republic; INFN Laboratori Nazionali di Legnaro, (PD), Legnaro, Italy; Virginia Tech, Center for Neutrino Physics, Blacksburg, VA, United States; INFN Sezione di Napoli, Napoli, Italy; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; University of Toronto, Department of Physics, Toronto, ON, Canada; Imperial College London, Department of Physics, London, United Kingdom; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; Tokyo University of Science, Department of Physics, Chiba, Japan; University of Liverpool, Department of Physics, Liverpool, United Kingdom; Tezpur University, Department of Physics, Sonitpur, India; University of Liverpool, Department of Physics, Liverpool, United Kingdom; Laboratoire de Physique Nucleaire et de Hautes Energie, IN2P3, CNRS, Sorbonne Universitè, Paris, France; Nagoya University, Graduate School of Science, Nagoya, Japan; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; INFN Sezione di Napoli, Napoli, Italy; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; Yokohama National University, Faculty of Engineering, Yokohama, Japan; University of California, Irvine, Department of Physics and Astronomy, Irvine, CA, United States; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; IRFU, CEA, Universitè Paris-Saclay, Gif-sur-Yvette, France; University of Warwick, Department of Physics, Coventry, United Kingdom; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; Indian Institute of Technology Jodhpur, Department of Physics, Rajasthan, Karwar, India; INFN Sezione di Napoli, Napoli, Italy; S. N. Bose National Centre for Basic Sciences, Salt Lake City, Kolkata, India; INFN Sezione di Bari, Università e Politecnico di Bari, Bari, Italy; Donostia International Physics Center, Ikerbasque Foundation, Basque Country, Spain; Chonnam National University, Department of Physics, Gwangju, South Korea; Kyungpook National University, Department of Physics, Daegu, South Korea; Universitat Politècnica de València, Instituto de Instrumentaciòn para Imagen Molecular (i3M), Valencia, Spain; Kyoto University, Department of Physics, Kyoto, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Department of Physics, Tokyo, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Earthquake Research Institute, Tokyo, Japan; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Department of Physics, Tokyo, Japan; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, High Energy Accelerator Research Organization (KEK), Tsukuba, Japan; Tohoku University, Department of Physics, Sendai, Japan; Tokyo University of Science, Department of Physics, Chiba, Japan; Tokyo University of Science, Department of Physics, Chiba, Japan; Kobe University, Department of Physics, Kobe, Japan; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, Kyoto University, Department of Physics, Kyoto, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; INFN Sezione di Napoli, Università Federico II di Napoli, Dipartimento di Fisica, Napoli, Italy; Imperial College London, Department of Physics, London, United Kingdom; Universidad de Guadalajara, CUCEI, Departamento de Fisica, Jal., Guadalajara, Mexico; University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom; Wroclaw University, Faculty of Physics and Astronomy, Wroclaw, Poland; Nagoya University, Graduate School of Science, Nagoya, Japan; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan; Keio University, Department of Physics, Yokohama, Japan; Kyoto University, Department of Physics, Kyoto, Japan; STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom; University of Glasgow, School of Physics and Astronomy, Glasgow, United Kingdom; Pontifícia Universidade Católica do Rio de Janeiro, Departamento de Física, Rio de Janeiro, Brazil; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; University of California, Irvine, Department of Physics and Astronomy, Irvine, CA, United States; Stockholm University, Oskar Klein Centre, Department of Astronomy, Stockholm, Sweden; University of Tokyo, Department of Physics, Tokyo, Japan; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan; Lancaster University, Physics Department, Lancaster, United Kingdom; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan; Kyiv National University, Department of Nuclear Physics, Kyiv, Ukraine; Universidad de Guadalajara, CUCEA, IT.Ph.D. program, Jal., Guadalajara, Mexico; Kyiv National University, Department of Nuclear Physics, Kyiv, Ukraine; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; Astronomical Observatory of the Jagiellonian University, Krakow, Poland; Uppsala University, Department of Physics and Astronomy, Uppsala, Sweden; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; Kobe University, Department of Physics, Kobe, Japan; Dongshin University, Laboratory for High Energy Physics, Naju, South Korea; Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France; INFN Sezione di Napoli, Università Federico II di Napoli, Dipartimento di Fisica, Napoli, Italy; INFN Sezione di Padova, Università di Padova, Dipartimento di Fisica, Padova, Italy; Imperial College London, Department of Physics, London, United Kingdom; INFN Sezione di Bari, Università e Politecnico di Bari, Bari, Italy; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; University of Regina, Department of Physics, Regina, SK, Canada; TRIUMF, Vancouver, BC, Canada; University of Liverpool, Department of Physics, Liverpool, United Kingdom; Laboratorio Subterráneo de Canfranc, Estación, Canfranc, Spain; University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom; University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom; TRIUMF, Vancouver, BC, Canada, British Columbia Institute of Technology, Physics Department, Burnaby, BC, Canada; Moscow State University, Department of Theoretical Physics, Moscow, Russian Federation; Laboratoire de Physique Nucleaire et de Hautes Energie, IN2P3, CNRS, Sorbonne Universitè, Paris, France; University of Silesia in Katowice, A. Chełkowski Institute of Physics, Poland; University of Warsaw, Faculty of Physics, Warsaw, Poland; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; TRIUMF, Vancouver, BC, Canada; Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France; Pontifícia Universidade Católica do Rio de Janeiro, Departamento de Física, Rio de Janeiro, Brazil; INFN Sezione di Bari, Università e Politecnico di Bari, Bari, Italy; ETH Zurich, Institute for Particle and Astroparticle Physics, Zurich, Switzerland; AGH University of Science and Technology, Faculty of Computer Science, Electronics and Telecommunications, Krakow, Poland; Universitat de Santiago de Compostela, Instituto Gallego de Física de Altas Enerxías, Santiago de Compostela, Spain; INFN Sezione di Roma, Università Sapienza, Dipartimento di Fisica, Roma, Italy; INFN Sezione di Napoli, Università Federico II di Napoli, Dipartimento di Fisica, Napoli, Italy; University of Warwick, Department of Physics, Coventry, United Kingdom; National Centre for Nuclear Research, Warsaw, Poland; Charles University, IPNP, FMF, Prague, Czech Republic; RWTH Aachen University, III. Physikalisches Institut, Aachen, Germany; Sungkyunkwan University, Department of Physics, Suwon, South Korea; ETH Zurich, Institute for Particle and Astroparticle Physics, Zurich, Switzerland; INFN Sezione di Napoli, Napoli, Italy; Laboratoire de Physique Nucleaire et de Hautes Energie, IN2P3, CNRS, Sorbonne Universitè, Paris, France; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; Ulsan National Institute of Science and Technology, Department of Physics, Ulsan, South Korea; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; Oxford University, Department of Physics, Oxford, United Kingdom; University of Geneva, Section de Physique, DPNC, Geneva, Switzerland; University of Oviedo, Applied Mathematical Modeling Group, Department of Physics, Oviedo, Spain; Yokohama National University, Faculty of Engineering, Yokohama, Japan; University of Oviedo, Applied Mathematical Modeling Group, Department of Physics, Oviedo, Spain; York University, Department of Physics and Astronomy, Toronto, ON, Canada; Indian Institute of Technology Guwahati, Guwahati, India; Nagoya University, Graduate School of Science, Nagoya, Japan; Imperial College London, Department of Physics, London, United Kingdom; Osaka City University, Department of Physics, Osaka, Japan; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; Sungkyunkwan University, Department of Physics, Suwon, South Korea; ETH Zurich, Institute for Particle and Astroparticle Physics, Zurich, Switzerland; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan; Tohoku University, Research Center for Neutrino Science, Sendai, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan; Chonnam National University, Department of Physics, Gwangju, South Korea; Tokyo University of Science, Department of Physics, Chiba, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; P.N.Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russian Federation; National Centre for Nuclear Research, Warsaw, Poland; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of California, Irvine, Department of Physics and Astronomy, Irvine, CA, United States; Wroclaw University, Faculty of Physics and Astronomy, Wroclaw, Poland; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of California, Irvine, Department of Physics and Astronomy, Irvine, CA, United States; University of Glasgow, School of Physics and Astronomy, Glasgow, United Kingdom; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan; INFN Sezione di Bari, Università e Politecnico di Bari, Bari, Italy; INFN Gruppo Collegato di Salerno, Fisciano, Italy; University of Glasgow, School of Physics and Astronomy, Glasgow, United Kingdom; Moscow State University, Department of Theoretical Physics, Moscow, Russian Federation; Astronomical Observatory of the Jagiellonian University, Krakow, Poland; INFN Gruppo Collegato di Salerno, Fisciano, Italy; Moscow State University, Department of Theoretical Physics, Moscow, Russian Federation; University of Oviedo, Applied Mathematical Modeling Group, Department of Physics, Oviedo, Spain; Tokyo University of Science, Department of Physics, Chiba, Japan; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; Kyoto Sangyo University, Department of Astrophysics and Atmospheric Sciences, Kyoto, Japan; Kobe University, Department of Physics, Kobe, Japan; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Tokyo, Tokyo, Japan; P.N.Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russian Federation; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Earthquake Research Institute, Tokyo, Japan; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, Kobe University, Department of Physics, Kobe, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Earthquake Research Institute, Tokyo, Japan; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan; University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom; University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom; University of Regina, Department of Physics, Regina, SK, Canada; Universitat Politècnica de València, Instituto de Instrumentaciòn para Imagen Molecular (i3M), Valencia, Spain; Tecnologico de Monterrey, Escuela de Ingenieria y Ciencias, Jalisco, Zapopan, Mexico; INFN Sezione di Napoli, Napoli, Italy; University of Liverpool, Department of Physics, Liverpool, United Kingdom; High Energy Accelerator Research Organization (KEK), Tsukuba, Japan, J-PARC Center, Tokai, Japan; Louisiana State University, Department of Physics and Astronomy, Baton Rouge, LA, United States; Imperial College London, Department of Physics, London, United Kingdom; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of California, Irvine, Department of Physics and Astronomy, Irvine, CA, United States; University of Warwick, Department of Physics, Coventry, United Kingdom; INFN Sezione di Bari, Università e Politecnico di Bari, Bari, Italy; IRFU, CEA, Universitè Paris-Saclay, Gif-sur-Yvette, France; Indian Institute of Technology Jodhpur, Department of Physics, Rajasthan, Karwar, India; University of Warwick, Department of Physics, Coventry, United Kingdom; Università della Campania”L. Vanvitelli”, INFN Sezione di Napoli, Napoli, Italy; Virginia Tech, Center for Neutrino Physics, Blacksburg, VA, United States; Moscow State University, Department of Theoretical Physics, Moscow, Russian Federation; H. Niewodniczański Institute of Nuclear Physics PAN, Cracow, Poland; Oxford University, Department of Physics, Oxford, United Kingdom, STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom; Imperial College London, Department of Physics, London, United Kingdom; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, Kyoto University, Department of Physics, Kyoto, Japan; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; National Centre for Nuclear Research, Warsaw, Poland; University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom; Tokyo Institute of Technology, Department of Physics, Tokyo, Japan; Osaka City University, Department of Physics, Osaka, Japan; Tokyo University of Science, Department of Physics, Chiba, Japan; University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan; Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation; University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo Institutes for Advanced Study, Kashiwa, Japan, University of Tokyo, Next-generation Neutrino Science Organization, Kamioka, Japan, University of Tokyo, Department of Physics, Tokyo, Japan; Tokyo University of Science, Department of Physics, Chiba, Japan; Korea Institute of Science and Technology, Department of Physics, Daejeon, South Korea; Sungkyunkwan University, Department of Physics, Suwon, South Korea; National Centre for Nuclear Research, Warsaw, Poland; University Autonoma Madrid, Department of Theoretical Physics, Madrid, Spain; National Centre for Nuclear Research, Warsaw, Poland; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; National Centre for Nuclear Research, Warsaw, Poland; Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland; Astronomical Observatory of the Jagiellonian University, Krakow, Poland; Laboratoire de Physique Nucleaire et de Hautes Energie, IN2P3, CNRS, Sorbonne Universitè, Paris, France; Imperial College London, Department of Physics, London, United Kingdom; King’s College London, Department of Physics, Strand Building, Strand, London, United Kingdom ⓘ	ⓘ	55968950500; 35316842700; 13609522800; 26431253400; 57191279607; 7004810214; 57191253786; 58027846900; 7004440709; 57195331264; 7006379524; 7005503172; 6602773267; 59569332600; 6508172339; 7006694639; 7102234805; 57208582625; 6603078804; 7006563072; 57203392800; 57188547921; 57203321898; 10040410200; 55436856500; 57203395818; 7004379668; 6603201393; 24478500100; 15843147700; 57198148175; 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57192182484; 57219794859; 6602714744; 7003749196; 57194426867; 55217173800; 57191488233; 56227897900; 57192837686; 35227961100; 57203396608; 35243922200; 55453339300; 6603029548; 57194109845; 57221150748; 57188827382; 15823196300; 57201839222; 57214923578; 57224776880; 6602114983; 57194320179; 57205642820; 35228176800; 56967652300; 56042471600; 59317777600; 58027849400; 57714569800; 57225875741; 57221141307; 57193893003; 35315137400; 57206030757; 56229202900; 57221148620; 6503884494; 56963525800; 57216231240; 6506254435; 57189229483; 6701650464; 57213620331; 7003776359; 35353976400; 57221142645; 57198865806; 55514765000; 6603098471; 57221140763; 15123454000; 7004772244; 6603085091; 35228290900; 57198231124; 8977997200; 57295741200; 57222079561; 57219648437; 59843779100; 58828711600; 59340236500; 8387485300; 55743752400; 57193333004; 59067101600; 35228244700; 57221151144; 51462236400; 55936708500; 6603387833; 57204472898; 16680503100; 54416814100; 35228232200; 58828271600; 57159999800 ⓘ	tyano@km.icrr.u-tokyo.ac.jp; ⓘ	Proceedings of Science ⓘ	ⓘ	1824-8039		395			ⓘ			0	2025-06-25 ⓘ		0	ⓘ	ⓘ	ⓘ	Atomic physics; Charged particles; Cosmic rays; Cosmology; Neutrons; Particle detectors; Supernovae; Cherenkov radiations; Cosmic Ray Background; Cylindrical shapes; Inner Detector; Multi-purpose; Neutrino astrophysics; Neutrino experiments; Photosensor; Physics project; Ultra-pure water; Water tanks ⓘ	English	Final	2022		ⓘ				바로가기
○		Article ⓘ	Proximity of maxillary molar apexes to the cortical bone surface and the maxillary sinus ⓘ	Objectives: This study aimed to analyze the proximity of maxillary molar roots to their overlying cortical bone surfaces and the maxillary sinus. Materials and Methods: Cone-beam computed tomographic images of 151 patients with completely erupted upper molars that had 3 separate roots were studied. The following distances were measured: from the root apex to the cortical plate and maxillary sinus floor, and from the apical 3-mm level of the root to the cortical plate. Differences between groups were analyzed with 1-way analysis of variance and the Scheffe post hoc test, the significance of differences between cone-beam computed tomography views with the paired t-test, and the significance of differences among age groups with linear regression analysis. The significance level was set at p < 0.05. Results: The mesiobuccal and distobuccal root apexes of maxillary second molars were more distant from the buccal cortical plate than the maxillary first molars (p < 0.05). The apical 3-mm level of the mesiobuccal root of the first molar was closer to the buccal cortical bone than the second molar (p < 0.05). In the maxillary first molars, the thickness of the buccal cortical bone decreased in all roots with age (p < 0.05). In all root apexes of both molars, the difference in the vertical level between the maxillary sinus floor and the root apex increased with age (p < 0.05). Conclusions: Awareness of the anatomical profile of maxillary molar apices in relation to the cortical bones and maxillary sinus will be beneficial for apical surgery. ⓘ	Lee, Han Shin; Kim, Dokyung; Kim, Sung Kyo ⓘ	Kyungpook Natl Univ, Sch Dent, Dept Conservat Dent, Daegu, South Korea; Kyungpook Natl Univ, Sch Dent, Dept Conservat Dent, 2175 Dalgubeol-Daero, Daegu 41940, South Korea ⓘ	Lee, Han/W-4924-2019 ⓘ	ⓘ	skykim@knu.ac.kr; ⓘ	RESTORATIVE DENTISTRY AND ENDODONTICS ⓘ	ⓘ	2234-7658	2234-7666	47	3		ⓘ				ⓘ	1		Maxillary molar; Proximity; Cortical plate; Maxillary sinus; Endodontic surgery ⓘ	BEAM COMPUTED-TOMOGRAPHY; PERIAPICAL LESIONS; POSTERIOR TEETH; ROOT; MORPHOLOGY; THICKNESS; ASSOCIATION; RADIOGRAPHY; ENDODONTICS; DIMENSIONS ⓘ	ⓘ	ⓘ	English		2022	2022-08	10.5395/rde.2022.47.e33 ⓘ		바로가기	바로가기
○	○	Article ⓘ	Pseudohermitian Curvatures on Bounded Strictly Pseudocon- vex Domains in C² ⓘ	In this paper, we present a formula for pseudohermitian curvatures on bounded strictly pseudoconvex domains in C-2 with respect to the coefficients of adapted frames given by Graham and Lee in [3] and their structure equations. As an application, we will show that the pseudohermitian curvatures on strictly plurisubharmonic exhaustions of Thullen domains diverges when the points converge to a weakly pseudoconvex boundary point of the domain. ⓘ	Seo, Aeryeong ⓘ	Kyungpook Natl Univ, Dept Math, Daegu 41566, South Korea ⓘ	Seo, Aeryeong/GON-4707-2022 ⓘ	55266222700 ⓘ	aeryeong.seo@knu.ac.kr; ⓘ	KYUNGPOOK MATHEMATICAL JOURNAL ⓘ	KYUNGPOOK MATH J ⓘ	1225-6951	0454-8124	62	2	ESCI	MATHEMATICS ⓘ	2022	0.7	0	2025-06-25 ⓘ	0	0	phrases; Pseudohermitian manifolds; Thullen domains ⓘ	ⓘ	Pseudohermitian manifolds; Thullen domains ⓘ	ⓘ	English		2022	2022-06	10.5666/kmj.2022.62.2.323 ⓘ	바로가기	바로가기	바로가기	바로가기
	○	Article ⓘ	Pseudohyperkalemia after total splenectomy in a dog: a case report ⓘ	A 16-year-old, 7.4 kg, castrated male Cocker Spaniel presenting anorexia and weight loss was referred due to a splenic mass, and total splenectomy was performed to resolve clinical signs. Following surgery, the dog developed mild hyperkalemia (6.27 mmol/L) without any clinical symptoms. Further investigations were conducted to determine the cause of hyperkalemia. The serum-plasma potassium difference was measured (1.05 mmol/L), and pseudohyperkalemia was diagnosed. The cause of pseudohyperkalemia was considered as thrombocytosis after splenectomy. The dog did not receive any specific treatment to lower blood potassium. To our knowledge, we report the first case of post-splenectomy pseudohyperkalemia in a dog. © 2022 Korean Society of Veterinary Science. All rights reserved. ⓘ	Moon, Chang-Hwan; Lee, Je Hun; Jeong, You-Jeong; Kwon, Young-Sam; Lee, Haebeom; Kim, Dae-Hyun; Jeong, Seong Mok ⓘ	Department of Veterinary Surgery, College of Veterinary Medicine, Chungnam National University, Daejeon, 34134, South Korea; Department of Veterinary Surgery, College of Veterinary Medicine, Chungnam National University, Daejeon, 34134, South Korea; Department of Veterinary Surgery, College of Veterinary Medicine, Chungnam National University, Daejeon, 34134, South Korea; Department of Veterinary Surgery, College of Veterinary Medicine, Kyungpook National University, Daegu, 41566, South Korea; Department of Veterinary Surgery, College of Veterinary Medicine, Chungnam National University, Daejeon, 34134, South Korea; Department of Veterinary Surgery, College of Veterinary Medicine, Chungnam National University, Daejeon, 34134, South Korea; Department of Veterinary Surgery, College of Veterinary Medicine, Chungnam National University, Daejeon, 34134, South Korea ⓘ	ⓘ	57211242244; 57218824105; 57811004300; 7403459426; 17343812000; 57215570370; 7402425314 ⓘ	jsmok@cnu.ac.kr; ⓘ	Korean Journal of Veterinary Research ⓘ	ⓘ	2466-1384		62	2		ⓘ			0	2025-06-25 ⓘ		0	ⓘ	ⓘ	dogs; hyperkalemia; pseudohyperkalemia; splenectomy; thrombocytosis ⓘ	ⓘ	English	Final	2022		10.14405/kjvr.20210051 ⓘ		바로가기		바로가기
○	○	Article ⓘ	Psychological Effects of COVID-19 Patient Management Experience among Paramedics and Emergency Medical Technicians: A Nationwide Survey in Korea ⓘ	Background: Throughout the coronavirus disease 2019 (COVID-19) pandemic, not only medical personnel but also paramedics or emergency medical technicians (EMT) have faced multiple physical and psychological challenges while performing their duties. The current study aimed to evaluate the psychological effects of managing patients with COVID-19 on the paramedics and EMT. Materials and Methods: A survey targeting paramedics and EMT in Korea was conducted in December 2020. An official letter requesting participation and with the link to an online-based survey was sent to the Public Emergency Medical Services. Only one response was accepted from each participant. Results: A total of 326 paramedics and EMT responded to the survey. Among them, 66.3% (216/326) had experience in managing patients with COVID-19. No differences in the distribution of sex, age, working area, duration of working experience, and underlying comorbidities were observed between those who did (COVID-19 group) and did not (non-COVID-19 group) experience managing patients with COVID-19. The percentage of participants who showed severe posttraumatic stress disorder (PTSD) symptoms was significantly higher in the COVID group than in the non-COVID group (11.1% vs. 3.6%, P = 0.029). The participants in the COVID group had a significantly higher mean Global Assessment of Recent Stress Scale score than those in the non-COVID group (18.7 +/- 11.1 vs. 16.1 +/- 9.9, P = 0.042). The proportion of paramedics and EMT willing to leave their job if given a chance was higher in the COVID group than the non-COVID group (24.1% vs. 9.1%, P = 0.001). Additionally, paramedics and EMT in the COVID group tended to show concern regarding exposure to COVID-19 infection. Conclusion: The experience of managing patients with COVID-19 resulted in psychological distress among paramedics and EMT in Korea. ⓘ	Kim, Bongyoung; Kwon, Ki Tae; Hwang, Soyoon; Ryoo, Hyun Wook; Chung, Un Sun; Lee, So Hee; Lee, Ju-Yeon; Park, Hye Yoon; Shin, Ji-Yeon; Bae, Sang-geun ⓘ	Hanyang Univ, Coll Med, Dept Internal Med, Seoul, South Korea; Kyungpook Natl Univ, Chilgok Hosp, Dept Internal Med, Div Infect Dis,Sch Med, Daegu, South Korea; Kyungpook Natl Univ, Sch Med, Dept Emergency Med, Daegu, South Korea; Kyungpook Natl Univ, Sch Med, Dept Psychiat, Daegu, South Korea; Natl Med Ctr, Dept Psychiat, Seoul, South Korea; Chonnam Natl Univ, Med Sch, Dept Psychiat, Gwangju, South Korea; Seoul Natl Univ Hosp, Dept Psychiat, Seoul, South Korea; Kyungpook Natl Univ, Sch Med, Dept Prevent Med, Daegu, South Korea ⓘ	; Kim, Hanjin/KYP-2633-2024; Lee, So Hee/B-5940-2016; Lee, Jung-Seok/L-6826-2019; Hwang, Soyoon/HHM-5762-2022; Kim, Woo/AAG-1822-2019; Kim, Bongyoung/H-3409-2018 ⓘ	55622077200; 9733850500; 57203160675; 55350557500; 24477437300; 56442744300; 57203144588; 57189505933; 55567961600; 55278023500 ⓘ	ktkwon@knu.ac.kr; ⓘ	INFECTION AND CHEMOTHERAPY ⓘ	INFECT CHEMOTHER ⓘ	2093-2340	2092-6448	54	2	ESCI	INFECTIOUS DISEASES ⓘ	2022	4.2	1.2	2025-06-25 ⓘ	8	9	COVID-19; Psychological distress; Paramedics; EMT; Korea ⓘ	WORKERS ⓘ	COVID-19; EMT; Korea; Paramedics; Psychological distress ⓘ	adult; Article; artificial ventilation; comorbidity; controlled study; coronavirus disease 2019; distress syndrome; emergency health service; extracorporeal oxygenation; female; global assessment of recent stress scale; health care personnel; health survey; human; job satisfaction; Korea; male; mental health; paramedical personnel; patient care; Patient Health Questionnaire 9; perception; rescue personnel ⓘ	English		2022	2022-06	10.3947/ic.2022.0049 ⓘ	바로가기	바로가기	바로가기	바로가기
○	○	Article ⓘ	PTO Torque and Draft Analyses of an Integrated Tractor-Mounted Implement for Round Ridge Preparation ⓘ	PurposeResearch on labor-saving of upland cultivation has been more actively conducted in Korea, since the consumption of and interest in local food have increased. The objectives of this study were to investigate characteristics of rotary-base implement for intensive farming and to suggest an operational strategy by analyzing draft (Ph) and power take-off (PTO) torque (Tq) of an integrated implement for round ridge preparation.MethodsA dynamometer and torque meter were installed between a tractor hitch and an attachment to measure Ph and Tq and to analyze performance of the integrated implement.ResultsIncrease in forward speed (SPD), decrease in Ph, and increase in Tq were observed. Rotary tilth depth (DEP) was a major factor in increasing Ph and Tq. In the operation of the integrated implement based on rotavator, the specific draft (SD) tended to decrease but the specific torque (ST) approached to a maximum value as the rotary pitch (p) increased.ConclusionThe optimum p and velocity ratio (lambda) for draft reduction were 36.15 cm/rev and 3.9, respectively for the actual SPD of 4.18 km/h at 540 rpm of PTO rotating speed (RPM). The regression of the rear wheel reaction (Rr) and slip showed a decaying exponential relation. If the Rr is reduced to 27 kN, slip will be properly maintained at 12-15%. Furthermore, the implement could be operated using a category I tractor with a front loader ballast. ⓘ	Koo, Young Mo ⓘ	Kyungpook Natl Univ, Sch Agr Civil & Bioind Engn, 80 Daehak Ro, Daegu 41566, South Korea ⓘ	ⓘ	57197976008 ⓘ	ymkoo@knu.ac.kr; ⓘ	JOURNAL OF BIOSYSTEMS ENGINEERING ⓘ	ⓘ	1738-1266	2234-1862	47	3		ⓘ			0.97	2025-06-25 ⓘ	8	8	Draft; Integrated implement; PTO torque; Rear wheel reaction; Rotary pitch ⓘ	TILLER DESIGN PARAMETERS; ROTARY-TILLER; PERFORMANCE; REQUIREMENT; RATIO ⓘ	Draft; Integrated implement; PTO torque; Rear wheel reaction; Rotary pitch ⓘ	Ballast (railroad track); Cultivation; Power takeoffs; Tractors (agricultural); Tractors (truck); Wheels; Draft; Integrated implement; Labor saving; Local foods; Operational strategies; Power take-off torque; Power take-offs; Rear wheel reaction; Rear wheels; Rotary pitch; Torque ⓘ	English		2022	2022-09	10.1007/s42853-022-00146-w ⓘ		바로가기	바로가기	바로가기
○	○	Article ⓘ	Purity Evaluation of Highly Oriented Cubic Silicon Carbide Using Micro-Raman Spectroscopy ⓘ	The purity level of 3C-SiC (beta phase) powder is an important factor for its use as a raw material for fabricating high-quality single crystals. Herein, we used micro-Raman spectroscopy to systematically investigate the purity of 3C-SiC powders subjected to three different purification treatments. The transverse optical (TO; 795 cm(-1)) and longitudinal optical (LO; 970 cm(-1)) phonon modes of 3C-SiC were measured, and the peak intensity ratio (TO/LO) showed good correlation with the purity. The highly purified 3C-SiC had a TO/LO value of 1.0 at a narrow full width half maximum of the LO peak. Furthermore, the pristine 3C-SiC powder exhibited Raman peaks corresponding to the D and G bands, indicating carbon bonding by graphite impurities. Thus, we demonstrated that the proposed micro-Raman spectroscopy is an effective analysis technique for characterizing the crystal quality and purity level of 3C-SiC powders. ⓘ	Kim, Seul-Ki; Jung, Eun Young; Lee, Myung-Hyun ⓘ	Korea Inst Ceram Engn Sr Technol, Semicond Mat Ctr, Jinju 52851, South Korea; Kyungpook Natl Univ, Coll IT Engn, Sch Elect & Elect Engn, Daegu 41566, South Korea ⓘ	ⓘ	57640906000; 57203199724; 57144971400 ⓘ	eyjung@knu.ac.kr;mhlee@kicet.re.kr; ⓘ	TRANSACTIONS ON ELECTRICAL AND ELECTRONIC MATERIALS ⓘ	TRANS ELECTR ELECTRO ⓘ	1229-7607	2092-7592	23	3	ESCI	MATERIALS SCIENCE, MULTIDISCIPLINARY ⓘ	2022	1.9	0.24	2025-06-25 ⓘ	3	3	Cubic silicon carbide (3C-SiC); Purity level; Micro-Raman spectroscopy ⓘ	BORON ⓘ	Cubic silicon carbide (3C-SiC); Micro-Raman spectroscopy; Purity level ⓘ	Crystal impurities; Optical correlation; Powders; Purification; Quality control; Raman spectroscopy; Single crystals; Cubic silicon carbide; Cubic silicon carbide (3c-SiC); High quality single crystals; Micro Raman Spectroscopy; Phase powders; Purification treatments; Purity level; SiC powder; Transverse optical; Silicon carbide ⓘ	English		2022	2022-06	10.1007/s42341-022-00394-9 ⓘ	바로가기	바로가기	바로가기	바로가기
	○	Conference paper ⓘ	Q DROP TENDENCY OF HALF-WAVE RESONATOR CAVITY ⓘ	Half-wave resonator superconducting cavities (HWRs) have been fabricated and tested. HWRs have been installed in the low energy section of the LINAC and being ready to be cooled down for the next step. All HWR cavities have been completely tested in two ways: vertical test and horizontal test. For the vetical test, HWRs were tested both at 4.2 K and 2.1 K cryogenic surroundings although the operating temperature is 2.1 K. Good cavity having higher quality factor than that of the target value showed the Q0 drop tendency of 2.1 K was very similar to that of 4.2 K. However, in many cases, Q0 drop tendency of 2.1 K was not similar with 4.2 K, rather Q0 decreased more rapidly than 4.2 K which means the surface resistance of the cavity rapidly increased at 2 K surrounding. In this study, we will report that various Q0 results of HWRs and discuss their Q0 drop tendencies as a function of temperature, 2.1 K and 4.2 K along with field emission. © 2022 Proceedings - Linear Accelerator Conference, LINAC. All rights reserved. ⓘ	Jung, Yoochul; Kim, Heetae; Kim, Hyunik; Jang, Hyojae; Kim, Juwan; Jeon, Sungmin ⓘ	Institute for Basic Science, Daejeon, South Korea; Institute for Basic Science, Daejeon, South Korea; Institute for Basic Science, Daejeon, South Korea; Institute for Basic Science, Daejeon, South Korea; Institute for Basic Science, Daejeon, South Korea; Kyungpook National University, Daegu, South Korea ⓘ	ⓘ	55970173300; 57203246684; 57547363500; 56221023600; 57204427562; 57222536170 ⓘ	ⓘ	Proceedings - Linear Accelerator Conference, LINAC ⓘ	ⓘ	2226-0366					ⓘ			0	2025-06-25 ⓘ		0	ⓘ	ⓘ	ⓘ	Linear accelerators; Superconducting resonators; Half-wave resonators; High quality factors; Lower energies; Operating temperature; Resonator cavities; Superconducting cavities; Target values; Two ways; Drops ⓘ	English	Final	2022		10.18429/jacow-linac2022-mopopa20 ⓘ		바로가기		바로가기
○	○	Article ⓘ	QTL Mapping for Resistance to Bacterial Wilt Caused by Two Isolates of Ralstonia solanacearum in Chili Pepper (Capsicum annuum L.) ⓘ	Bacterial wilt caused by the beta-proteobacterium Ralstonia solanacearum is one of the most destructive soil-borne pathogens in peppers (Capsicum annuum L.) worldwide. Cultivated pepper fields in Korea face a continuous spread of this pathogen due to global warming. The most efficient and sustainable strategy for controlling bacterial wilt is to develop resistant pepper varieties. Resistance, which is quantitatively inherited, occurs differentially depending on R. solanacearum isolates. Therefore, in this study, we aimed to identify resistance quantitative trait loci (QTLs) in two F-2 populations derived from self-pollination of a highly resistant pepper cultivar 'Konesian hot' using a moderately pathogenic 'HS' isolate and a highly pathogenic 'HWA' isolate of R. solanacearum for inoculation, via genotyping-by-sequencing analysis. QTL analysis revealed five QTLs, Bwr6w-7 .2, Bwr6w-8.1, Bwr6w-9.1, Bwr6w-9.2, and Bwr6w-10 .1, conferring resistance to the 'HS' isolate with R-2 values of 13.05, 12.67, 15.07, 10.46, and 9.69%, respectively, and three QTLs, Bwr6w-5.1, Bwr6w-6 .1, and Bwr6w-7.1, resistant to the 'HWA' isolate with phenotypic variances of 19.67, 16.50, and 12.56%, respectively. Additionally, six high-resolution melting (HRM) markers closely linked to the QTLs were developed. In all the markers, the mean disease index of the paternal genotype was significantly lower than that of the maternal genotype. The QTLs and HRM markers are expected to be useful for the development of pepper varieties with high resistance to bacterial wilt. ⓘ	Lee, Saeyoung; Chakma, Nidhi; Joung, Sunjeong; Lee, Je Min; Lee, Jundae ⓘ	Jeonbuk Natl Univ, Inst Agr Sci & Technol, Dept Hort, Jeonju 54896, South Korea; Kyungpook Natl Univ, Dept Hort Sci, Coll Agr & Life Sci, Daegu 41566, South Korea ⓘ	; Lee, Je Min/F-9797-2014; Lee, Je/AAE-7496-2020 ⓘ	57734170100; 57734270100; 57734362200; 8885729900; 23028197900 ⓘ	lsy4674@hanmail.net;nidhi.chakma@griffithuni.edu.au;sunjeong7571@gmail.com;jemin@knu.ac.kr;ajfall@jbnu.ac.kr; ⓘ	PLANTS-BASEL ⓘ	ⓘ	2223-7747		11	12		ⓘ			1.83	2025-06-25 ⓘ	15	16	bacterial wilt; chili pepper; genotyping-by-sequencing; high-resolution melting; quantitative trait loci; single nucleotide polymorphism ⓘ	PSEUDOMONAS-SOLANACEARUM; TOMATO PLANTS; ADAPTATION; DIVERSITY; INFECTION; DENSITY ⓘ	bacterial wilt; chili pepper; genotyping-by-sequencing; high-resolution melting; quantitative trait loci; single nucleotide polymorphism ⓘ	ⓘ	English		2022	2022-06	10.3390/plants11121551 ⓘ		바로가기	바로가기	바로가기
	○	Article ⓘ	Quality characteristics of dried onion and garlic slices according to thermal and nonthermal treatment methods ⓘ	In the present study, the application of suitable thermal and nonthermal pretreatment methods was explored to develop a dried products comprising onion and garlic slices. Pretreatment was performed via blanching for 30 sec, steaming for 1 min, dipping in warm water (45℃) for 30 min, and dipping in cold water (8℃) for 1 hr. Furthermore, physicochemical and microbiological analyses were performed in conjunction with sensory evaluations. The group subjected to pretreatment via cold-water dipping exhibited the lowest moisture content and water activity with a negligible redness, yellowness, and browning index. Furthermore, the results of sensory evaluation revealed that this group exhibited relatively high color and overall acceptability. The group subjected to pretreatment via blanching presented severe browning and shape distortion. The samples in the group subjected to pretreatment via cold-water dipping did not exhibit a significant difference in pH; furthermore, the number of microorganisms during storage was lower than that in the control group. It was concluded that the hot-air drying of onion and garlic slices after cold-water dipping resulted in an increase in drying efficiency and the suppression of browning, without inducing major component changes. The facile technique demonstrated in the present study is expected to be fast and cost-effective, thereby facilitating practical application in farms. Copyright © 2022 The Korean Society of Food Preservation ⓘ	Choi, Ji-Young; Kim, Jiyoon; Kim, Jungsoo; Jeong, Saeul; Gwak, Da-Hyeon; Kang, Seok; Han, So-Jin; Kim, Hyun-Joong; Moon, Kwang-Deog ⓘ	Food Safety and Distribution Research Group, Korea Food Research Institute, Wanju, 55365, South Korea; School of Food Science and Technology, Kyungpook National University, Daegu, 41566, South Korea; School of Food Science and Technology, Kyungpook National University, Daegu, 41566, South Korea; School of Food Science and Technology, Kyungpook National University, Daegu, 41566, South Korea; School of Food Science and Technology, Kyungpook National University, Daegu, 41566, South Korea; School of Food Science and Technology, Kyungpook National University, Daegu, 41566, South Korea; School of Food Science and Technology, Kyungpook National University, Daegu, 41566, South Korea; School of Food Science and Technology, Kyungpook National University, Daegu, 41566, South Korea; School of Food Science and Technology, Kyungpook National University, Daegu, 41566, South Korea ⓘ	ⓘ	57219113098; 57208110209; 57211108486; 57219605598; 57576688700; 57575197800; 57576045800; 57576688800; 55999192900 ⓘ	kdmoon@knu.ac.kr; ⓘ	Korean Journal of Food Preservation ⓘ	ⓘ	1738-7248		29	1		ⓘ			0.26	2025-06-25 ⓘ		3	ⓘ	ⓘ	browning inhibition; cold water dipping; garlic slice; hot air drying; onion slice ⓘ	ⓘ	Korean	Final	2022		10.11002/kjfp.2022.29.1.34 ⓘ		바로가기		바로가기

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JCR Year	해당 저널의 JCR(Journal Citation Reports) 지표가 산출된 연도입니다.
IF (Impact Factor)	저널 영향력 지수. 최근 2년간 발표된 논문이 해당 연도에 평균적으로 인용된 횟수를 나타냅니다. 저널의 학술적 영향력을 나타내는 대표적인 지표입니다.
JCR (%)	해당 카테고리에서 저널이 위치하는 상위 백분율입니다. 값이 낮을수록 우수한 저널임을 의미합니다 (예: 5%는 상위 5%를 의미).
FWCI	Field-Weighted Citation Impact. 분야별 가중 인용 영향력 지수입니다. 논문이 받은 인용을 동일 분야, 동일 연도, 동일 문헌 유형의 평균과 비교한 값입니다. 1.0이 평균이며, 1.0보다 높으면 평균 이상의 인용을 받았음을 의미합니다.
FWCI UpdateDate	FWCI 값이 마지막으로 업데이트된 날짜입니다. FWCI는 인용이 누적됨에 따라 주기적으로 업데이트됩니다.
WOS Citation	Web of Science에서 집계된 해당 논문의 총 인용 횟수입니다.
SCOPUS Citation	SCOPUS에서 집계된 해당 논문의 총 인용 횟수입니다.
Keywords (WoS)	저자가 논문에서 직접 지정한 키워드입니다. Web of Science에 등록된 저자 키워드 목록입니다.
KeywordsPlus (WoS)	Web of Science에서 자동으로 추출한 추가 키워드입니다. 논문의 참고문헌 제목에서 자주 등장하는 단어들로 생성됩니다.
Keywords (SCOPUS)	저자가 논문에서 직접 지정한 키워드입니다. SCOPUS에 등록된 저자 키워드 목록입니다.
KeywordsPlus (SCOPUS)	SCOPUS에서 자동으로 추출하거나 추가한 색인 키워드입니다.
Language	논문이 작성된 언어입니다. 대부분 English이며, 그 외 다양한 언어로 작성된 논문이 포함될 수 있습니다.
Publication Year	논문이 출판된 연도입니다.
Publication Date	논문의 정확한 출판 날짜입니다 (년-월-일 형식).
DOI	Digital Object Identifier. 디지털 객체 식별자로, 논문을 고유하게 식별하는 영구적인 식별번호입니다. 이를 통해 논문의 온라인 위치를 찾을 수 있습니다.

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