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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 | JCR (%) | 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 |
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| ○ | Article | Construction Method of ECVAM using Land Cover Map and KOMPSAT-3A Image | In this study, the periodic and simplified update and production way of the ECVAM (Environmental Conservation Value Assessment Map) was presented through the classification of environmental values using KOMPSAT-3A satellite imagery and land cover map. ECVAM is a map that evaluates the environmental value of the country in five stages based on 62 legal evaluation items and 8 environmental and ecological evaluation items, and is provided on two scales: 1:25000 and 1:5000. However, the 1:5000 scale environmental assessment map is being produced and serviced with a slow renewal cycle of one year due to various constraints such as the absence of reference materials and different production years. Therefore, in this study, one of the deep learning techniques, KOMPSAT-3A satellite image, SI (Spectral Indices), and land cover map were used to conduct this study to confirm the possibility of establishing an environmental assessment map. As a result, the accuracy was calculated to be 87.25% and 85.88%, respectively. Through the results of the study, it was possible to confirm the possibility of constructing an environmental assessment map using satellite imagery, optical index, and land cover classification. © 2022 Korean Society of Surveying. All rights reserved. | Kwon, Hee Sung; Song, Ah Ram; Jung, Se Jung; Lee, Won Hee | Dept. of Spatial Information, Kyungpook National University, South Korea; Dept. of Convergence & Fusion System Engineering, Kyungpook National University, South Korea; Dept. of Convergence & Fusion System Engineering, Kyungpook National University, South Korea; Dept. of Convergence & Fusion System Engineering, Kyungpook National University, South Korea | 58117719300; 56496312900; 57209137546; 57190774365 | wlee33@knu.ac.kr; | Journal of the Korean Society of Surveying, Geodesy, Photogrammetry and Cartography | 1598-4850 | 40 | 5 | 0.09 | 2025-06-25 | 1 | Deep Learning; Environmental Conservation Value Assessment Map; Environmental Geographic Information; Land cover map | environmental assessment; environmental values; land cover; learning; satellite imagery | Korean | Final | 2022 | 10.7848/ksgpc.2022.40.5.367 | 바로가기 | 바로가기 | |||||||||||||||
| ○ | Conference paper | Construction of Disaster Knowledge Graphs to Enhance Disaster Resilience | As a result of the recent surge in disaster-related data, numerous studies have been conducted to deal with the massive amount of data. In the meantime, the issue of managing data in various formats and representing their relevance is being raised. In this paper, we present a disaster knowledge graph to analyze the impact of a disaster and predict how much effort it will take to recover from the disaster. To that end, we define the structure of a disaster knowledge graph containing data collected from sensors, social networks, web, and risk analysis results. To extract meaningful information from structured and unstructured data, we use a risk analysis platform that can compute hazard values in accordance with various hazard models. Then, we store automatically graphs into a graph database as a form of a time-series data. Therefore, it will be possible to predict the progress of a complex disaster that can occur in a chain using a series of disaster knowledge graphs. © 2022 IEEE. | Kim, Seonhyeong; Kwon, Young-Woo | Kyungpook National University, School of Computer Science and Engineering, Daegu, South Korea; Kyungpook National University, School of Computer Science and Engineering, Daegu, South Korea | 57256850100; 57208480210 | kimsh951027@knu.ac.kr; | Proceedings - 2022 IEEE International Conference on Big Data, Big Data 2022 | 1.65 | 2025-06-25 | 5 | disaster; knowledge graph; risk analysis | Disasters; Hazards; Knowledge graph; Risk assessment; Disaster resiliences; Graph database; Hazard modeling; Knowledge graphs; Social risks; Social webs; Structured data; Time-series data; Unstructured data; Risk analysis | English | Final | 2022 | 10.1109/bigdata55660.2022.10021017 | 바로가기 | 바로가기 | ||||||||||||||||||
| ○ | Conference paper | Construction status and prospects of the Hyper-Kamiokande project | The Hyper-Kamiokande project is a 258-kton Water Cherenkov together with a 1.3-MW high-intensity neutrino beam from the Japan Proton Accelerator Research Complex (J-PARC). The inner detector with 186-kton fiducial volume is viewed by 20-inch photomultiplier tubes (PMTs) and multi-PMT modules, and thereby provides state-of-the-art of Cherenkov ring reconstruction with thresholds in the range of few MeVs. The project is expected to lead to precision neutrino oscillation studies, especially neutrino CP violation, nucleon decay searches, and low energy neutrino astronomy. In 2020, the project was officially approved and construction of the far detector was started at Kamioka. In 2021, the excavation of the access tunnel and initial mass production of the newly developed 20-inch PMTs was also started. In this paper, we present a basic overview of the project and the latest updates on the construction status of the project, which is expected to commence operation in 2027. © Copyright owned by the author(s). | Itow, Yoshitaka; 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. | Institute for Space-Earth Environmental Research, Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Aichi, Nagoya, 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 , 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 , 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 | 8503624700; 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; 55508216000; 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; 55968950500; 8387485300; 55743752400; 57193333004; 59067101600; 35228244700; 57221151144; 51462236400; 55936708500; 6603387833; 57204472898; 16680503100; 54416814100; 35228232200; 58828271600; 57159999800 | itow@isee.nagoya-u.ac.jp; | Proceedings of Science | 1824-8039 | 395 | 0 | 2025-06-25 | 0 | Neutrons; Particle detectors; Cherenkov; Construction status; CP violations; High intensity; Inner Detector; Japan proton accelerator research complexes; Neutrino beams; Neutrino oscillations; State of the art; Status and prospect; Photomultipliers | English | Final | 2022 | 바로가기 | |||||||||||||||||||
| ○ | Conference paper | Continuous Differential Image-based Fast Convolution for Convolutional Neural Networks | Convolutional neural networks with powerful visual image analysis of deep structures are gaining popularity in many research fields. The main difference in convolutional neural networks compared to other artificial neural networks is the addition of many convolutional layers. The convolutional layer improves the performance of artificial neural networks by extracting feature maps required for image classification. However, for applications that require very low-latency on limited processing resources, the success of a convolutional neural network depends on how fast we can compute. In this paper, we propose a novel convolution technique of fast algorithms for convolutional neural networks using continuous differential images. The proposed method improves the response speed of the algorithm by reducing the computational complexity of the convolutional layer. It is compatible with all types of convolutional neural networks, and the lower the difference in the continuous images, the better the performance. We use the darknet network to benchmark the CPU implementation of our algorithm and show state-of-the-art throughput at pixel difference thresholds from 0 to 25 pixels. © 2022 IEEE. | Hong, Sunghoon; Park, Daejin | School of Electronic and Electrical Engineering, Kyungpook National University, Daegu, South Korea; School of Electronic and Electrical Engineering, Kyungpook National University, Daegu, South Korea | 55726350900; 55463943600 | International Conference on ICT Convergence | 2162-1233 | 2022-October | 0.44 | 2025-06-25 | 2 | Convolution techniques; Convolutional neural networks; Deep learning; Fast convolution; Machine learning | Convolution; Deep learning; Image enhancement; Learning systems; Multilayer neural networks; Pixels; Convolution techniques; Convolutional neural network; Deep learning; Differential image; Fast convolution; Image-analysis; Image-based; Machine-learning; Performance; Visual image; Convolutional neural networks | English | Final | 2022 | 10.1109/ictc55196.2022.9952518 | 바로가기 | 바로가기 | |||||||||||||||||
| ○ | Book chapter | Convergence in a neo-Kaleckian model with endogenous technical progress and autonomous demand growth | This paper introduces technical progress along the lines of the Kaldor Verdoorn law within a neo-Kaleckian model of growth and distribution that incorporates the Sraffian supermultiplier mechanism. The key features of the model include the interactive effects of endogenous technical progress, the non-capacity-creating demand component that grows at an exogenous rate and, in its long-run version, a Harrodian adjustment mechanism. It turns out that, whereas the model converges towards the normal rate of capacity utilization, the main tenets of the Keynesian model are still valid in the long run as well as in the short run in the sense that all of the average rates of accumulation, capacity utilization, and technical progress are lower during the traverse after the propensity to save or the share of profits goes up. The conditions under which the productivity regime can be wage-led are examined, and the possible effects of an exogenous technical shift are also discussed. © Marc Lavoie 2022. | Nah, Won Jun; Lavoie, Marc | School of Economics and Trade, Kyungpook National University, Daegu, South Korea; University of Sorbonne Paris Cité, University of Paris 13, CEPN, France, Department of Economics, University of Ottawa, Ottawa, ON, Canada | 36497335900; 35775352400 | Post-Keynesian Growth Theory:Selected Essays | 0 | 2025-06-25 | 0 | Autonomous expenditures; Capacity utilization; Growth; Neo-Kaleckian; Technical progress | English | Final | 2022 | 바로가기 | ||||||||||||||||||||||
| ○ | ○ | Review | Core Elements for Implementing Antimicrobial Stewardship Programs in Korean General Hospitals | Currently, antimicrobial resistance (AMR) is a major threat to global public health. The antimicrobial stewardship program (ASP) has been proposed as an important approach to overcome this crisis. ASP supports the optimal use of antimicrobials, including appropriate dosing decisions, administration duration, and administration routes. In Korea, efforts are being made to overcome AMR using ASPs as a national policy. The current study aimed to develop core elements of ASP that could be introduced in domestic medical facilities. A Delphi survey was conducted twice to select the core elements through expert consensus. The core elements for implementing the ASP included (1) leadership commitment, (2) operating system, (3) action, (4) tracking, (5) reporting, and (6) education. To ensure these core elements are present at medical facilities, multiple departments must collaborate as teams for ASP operations. Establishing a reimbursement system and a workforce for ASPs are prerequisites for implementing ASPs. To ensure that ASP core elements are actively implemented in medical facilities, it is necessary to provide financial support for ASPs in medical facilities, nurture the healthcare workforce in performing ASPs, apply the core elements to healthcare accreditation, and provide incentives to medical facilities by quality evaluation criteria. | Cheong, Hae Suk; Park, Kyung-Hwa; Kim, Hong Bin; Kim, Shin-Woo; Kim, Bongyoung; Moon, Chisook; Lee, Mi Suk; Yoon, Young Kyung; Jeong, Su Jin; Kim, Yong Chan; Eun, Byung Wook; Lee, Hyukmin; Shin, Ji-Yeon; Kim, Hyung-sook; Hwang, In Sun; Park, Choon-Seon; Kwon, Ki Tae | Sungkyunkwan Univ, Kangbuk Samsung Hosp, Dept Internal Med, Div Infect Dis,Sch Med, Seoul, South Korea; Chonnam Natl Univ, Dept Infect Dis, Med Sch, Gwangju, South Korea; Seoul Natl Univ, Bundang Hosp, Dept Internal Med, Coll Med, Seongnam, South Korea; Kyungpook Natl Univ, Sch Med, Dept Internal Med, Daegu, South Korea; Hanyang Univ, Dept Internal Med, Coll Med, Seoul, South Korea; Inje Univ, Dept Internal Med, Div Infect Dis, Coll Med, Busan, South Korea; Kyung Hee Univ, Kyung Hee Univ Hosp, Dept Internal Med, Coll Med, Seoul, South Korea; Korea Univ, Dept Internal Med, Div Infect Dis, Coll Med, Seoul, South Korea; Yonsei Univ, Dept Internal Med, Div Infect Dis, Coll Med, Seoul, South Korea; Nowon Eulji Univ Hosp, Dept Pediat, Seoul, South Korea; Yonsei Univ, Dept Lab Med, Coll Med, Seoul, South Korea; Kyungpook Natl Univ, Sch Med, Dept Prevent Med, Daegu, South Korea; Seoul Natl Univ, Dept Pharm, Bundang Hosp, Seongnam, South Korea; Korea Inst Healthcare Accreditat, Seoul, South Korea; Hlth Insurance Review & Assessment Serv, Hlth Insurance Review & Assessment Res Inst, Wonju, South Korea; Kyungpook Natl Univ, Chilgok Hosp, Sch Med,Div Infect Dis, Dept Internal Med, Daegu, South Korea | ; Kim, Hong Bin/J-5452-2012; Kim, Bongyoung/H-3409-2018; Kim, Woo/AAG-1822-2019; Kyung, Yoon/AAS-3428-2020; Kim, Hee/AAU-6368-2021; Kim, Sooyeon/AAA-8521-2022; Kim, Hanjin/KYP-2633-2024; Eun, Byungwook/NAZ-8644-2025 | 57233155100; 57219637574; 35307429400; 8710731500; 55622077200; 22980995800; 55759244100; 25947937900; 57226001028; 36486497700; 12762260900; 8872234300; 55567961600; 55945673500; 58083509900; 23498882100; 9733850500 | ktkwon@knu.ac.kr; | INFECTION AND CHEMOTHERAPY | INFECT CHEMOTHER | 2093-2340 | 2092-6448 | 54 | 4 | ESCI | INFECTIOUS DISEASES | 2022 | 4.2 | 0.83 | 2025-06-25 | 16 | 17 | Antimicrobial resistance; Leadership; Multidisciplinary; Financial support; Accreditation | CLOSTRIDIUM-DIFFICILE INFECTION; COMMUNITY-ACQUIRED PNEUMONIA; HEALTH-CARE EPIDEMIOLOGY; VENTILATOR-ASSOCIATED PNEUMONIA; CLINICAL-PRACTICE GUIDELINES; ANTIBIOTIC STEWARDSHIP; DISEASES SOCIETY; COMBINATION THERAPY; PRESCRIBING PRACTICE; IMPACT | Accreditation; Antimicrobial resistance; Financial support; Leadership; Multidisciplinary | accreditation; antibiotic resistance; antimicrobial stewardship; consensus; Delphi study; education; financial management; general hospital; health workforce; human; human experiment; Korea; leadership; reimbursement; review | English | 2022 | 2022-12 | 10.3947/ic.2022.0171 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||
| ○ | Proceedings Paper | Cosmic-ray Heavy Nuclei Spectra Using the ISS-CREAM Instrument | Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) was designed to study high-energy cosmic rays up to PeV and recorded data from August 22nd, 2017 to February 12th, 2019 on the ISS. In this analysis, the Silicon Charge Detector (SCD), CALorimeter (CAL), and Top and Bottom Counting Detectors (TCD/BCD) are used. The SCD is composed of four layers and provides the measurement of cosmic-ray charges with a resolution of similar to 0.2e. The CAL comprises 20 interleaved tungsten plates and scintillators, measures the incident cosmic-ray particles' energies, and provides a high energy trigger. The TCD/BCDs consist of photodiode arrays and plastic scintillators and provide a low-energy trigger. In this analysis, the SCD top layer is used for charge determination. Here, we present the heavy nuclei analysis using the ISS-CREAM instrument. | Kang, S. C.; Aggarwal, S.; Amare, Y.; Angelaszek, D.; Bowman, D.; Chen, Y. C.; Choi, G. H.; Copley, M.; Dermoe, L.; Eraud, L.; Falana, C.; Gerrety, A.; Han, J. H.; Huh, H. G.; Haque, A.; Hwang, Y. S.; Hyun, H. J.; Jeon, H. B.; Jeon, J. A.; Jeong, S.; Kim, H. J.; Kim, K. C.; Kim, M. H.; Lee, H. Y.; Lee, J.; Lee, M. H.; Lu, L.; Lundquist, J. P.; Lutz, L.; Menchaca-Rocha, A.; Ofoha, O.; Park, H.; Park, I. H.; Park, J. M.; Picot-Clemente, N.; Scrandis, R.; Seo, E. S.; Smith, J. R.; Takeishi, R.; Walpole, P.; Weinmann, R. P.; Wu, H.; Wu, J.; Yin, Z.; Yoon, Y. S.; Zhang, H. G. | Kyungpook Natl Univ, Dept Phys, Daegu, South Korea; Univ Maryland, Inst Phys Sci & Tech, College Pk, MD USA; Univ Maryland, Dept Phys, College Pk, MD USA; Sungkyunkwan Univ, Dept Phys, Seoul, South Korea; Lab Phys Subatom Cosmol, Grenoble, France; Univ Nacl Autonoma Mexico, Inst Fis, Mexico City, DF, Mexico | Meninno, Elisa/AAJ-4478-2021; Ha, Jeong/F-6918-2013; Lee, Moo/AAK-4266-2020; Kang, Jeong/AAU-4400-2020; , ES/AAN-2324-2020; Lundquist, Jon/AAR-1595-2020; Park, Hae/AAM-2956-2021; Smith, Rory/AAU-8567-2021 | sinchul1216@gmail.com; | 37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021 | 0 | English | 2022 | 2022 | 바로가기 | ||||||||||||||||||||||||
| ○ | Conference paper | Cosmic-ray Heavy Nuclei Spectra Using the ISS-CREAM Instrument | Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) was designed to study high-energy cosmic rays up to PeV and recorded data from August 22nd, 2017 to February 12th, 2019 on the ISS. In this analysis, the Silicon Charge Detector (SCD), CALorimeter (CAL), and Top and Bottom Counting Detectors (TCD/BCD) are used. The SCD is composed of four layers and provides the measurement of cosmic-ray charges with a resolution of ∼0.2e. The CAL comprises 20 interleaved tungsten plates and scintillators, measures the incident cosmic-ray particles’ energies, and provides a high energy trigger. The TCD/BCDs consist of photodiode arrays and plastic scintillators and provide a low-energy trigger. In this analysis, the SCD top layer is used for charge determination. Here, we present the heavy nuclei analysis using the ISS-CREAM instrument. © Copyright owned by the author(s). | Kang, S.C.; Aggarwal, S.; Amare, Y.; Angelaszek, D.; Bowman, D.; Chen, Y.C.; Choi, G.H.; Copley, M.; Dermoe, L.; Eraud, L.; Falana, C.; Gerrety, A.; Han, J.H.; Huh, H.G.; Haque, A.; Hwang, Y.S.; Hyun, H.J.; Jeon, H.B.; Jeon, J.A.; Jeong, S.; Kim, H.J.; Kim, K.C.; Kim, M.H.; Lee, H.Y.; Lee, J.; Lee, M.H.; Lu, L.; Lundquist, J.P.; Lutz, L.; Menchaca-Rocha, A.; Ofoha, O.; Park, H.; Park, I.H.; Park, J.M.; Picot-Clemente, N.; Scrandis, R.; Seo, E.S.; Smith, J.R.; Takeishi, R.; Walpole, P.; Weinmann, R.P.; Wu, H.; Wu, J.; Yin, Z.; Yoon, Y.S.; Zhang, H.G. | Dept. of Physics, Kyungpook National University, South Korea; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Dept. of Physics, University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Dept. of Physics, Sungkyunkwan University, South Korea; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Laboratoire de Physique Subatomique ed de Cosmologie, Grenoble, France; Laboratoire de Physique Subatomique ed de Cosmologie, Grenoble, France; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Dept. of Physics, Kyungpook National University, South Korea; Dept. of Physics, Kyungpook National University, South Korea; Dept. of Physics, Kyungpook National University, South Korea; Dept. of Physics, Sungkyunkwan University, South Korea; Dept. of Physics, Sungkyunkwan University, South Korea; Dept. of Physics, Kyungpook National University, South Korea; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Dept. of Physics, Sungkyunkwan University, South Korea; Dept. of Physics, Sungkyunkwan University, South Korea; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Dept. of Physics, Kyungpook National University, South Korea; Dept. of Physics, Sungkyunkwan University, South Korea; Dept. of Physics, Kyungpook National University, South Korea; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Dept. of Physics, Sungkyunkwan University, South Korea; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States, Dept. of Physics, University of Maryland, College Park, MD, United States; Inst. for Phys. Sci. and Tech., University of Maryland, College Park, MD, United States | 57191418531; 59436068600; 56636827400; 56015950400; 57893619300; 59072706100; 7202652482; 59074552300; 58034770800; 7801514590; 57217106639; 57217101028; 55590479100; 36126235400; 57212636034; 55584791466; 35233487300; 57014196800; 24478376500; 35104920200; 59051568100; 24780757400; 57206000814; 57199646872; 36664730200; 57198252980; 57201616440; 56110612200; 7005973973; 56254267800; 55891853300; 58642658300; 56419230500; 9942606600; 35722936000; 57894097700; 7005953753; 57207399046; 56271261200; 15844727300; 57196415279; 59815772800; 56122537700; 57217101369; 35243798200; 57217099781 | sinchul1216@gmail.com; | Proceedings of Science | 1824-8039 | 395 | 0 | 2025-06-25 | 0 | Cosmology; Ionization; Scintillation counters; Silicon detectors; Space stations; Charge detectors; Cosmic-ray particles; Energy; Heaviest nuclei; High-energy cosmic rays; International Space stations; Measurements of; Particle energy; Photodiode arrays; Spectra's; Cosmic rays | English | Final | 2022 | 바로가기 | |||||||||||||||||||
| ○ | ○ | Proceedings Paper | Cost Effective High Torque Density Multi-Layer Motors Utilzing both Rare-Earth and Ferrite Permanenet Magnets | This paper, we propose a design method for a multilayer internal permanent magnet synchronous motor using two types of permanent magnet materials. Since it is a model that uses two types of permanent magnet materials, the characteristics and output of the motor are affected by the positioning of the permanent magnets. Therefore, in this paper, by selecting the proper location of the rare-earth permanent magnet and the non-rare earth permanent magnet, the design was designed to maintain the performance similar to that of the existing rare-earth permanent magnet machine at a lower cost. The final designed model was verified through finite element analysis and experiments. | Seok, Chang-Hoon; Kim, Gui-Hwan; Choi, Hong-Soon; Seo, Jangho | Kyungpook Natl Univ, Sch Elect & Elect Engn, Daegu, South Korea; Kyungpook Natl Univ, Dept Elect Engn, Daegu, South Korea; Kyungpook Natl Univ, Sch Automot Engn, Sangju, South Korea | 57581239400; 57193239440; 7404338767; 12791073600 | haneulpretty@naver.com;ddx1000@knu.ac.kr;tochs@knu.ac.kr;j.seo@knu.ac.kr; | TWENTIETH BIENNIAL IEEE CONFERENCE ON ELECTROMAGNETIC FIELD COMPUTATION (IEEE CEFC 2022) | 0 | 2025-06-25 | 0 | 0 | Ferrite permanent magnet; multilayer interior permanent magnet synchronous motor; rare-earth magnet | Ferrite permanent magnet; multilayer interior permanent magnet synchronous motor; rare-earth magnet | Ferrite; Multilayers; Permanent magnets; Rare earths; Synchronous motors; Cost effective; Ferrite permanent magnets; High torque density; Interior permanent magnet synchronous motor; Multi-layers; Multilayer interior permanent magnet synchronoi motor; Permanent magnet materials; Rare earth magnet; Rare earth permanent magnet; Rare-earths; Cost effectiveness | English | 2022 | 2022 | 10.1109/cefc55061.2022.9940736 | 바로가기 | 바로가기 | 바로가기 | ||||||||||||||
| ○ | Conference paper | Cotton Production and Demand Forecasting | The primary goal of this study is visualizing the tabular data compound growth and forecast area, product demand forecast(from Pakistan and Globally), output and average yield in Punjab, Pakistan. Cotton output in Pakistan's Punjab province and worldwide. Data obtained from government reports from 1990 to 2017 were scrutinized for this purpose. In Pakistan, empirical data showed that area under cultivation grew at a negative compound rate, but production and average yield grew at a positive compound rate. In Punjab, however, the compound growth rate of cotton planting and output was negative, although the average yield increased. Cotton forecasting revealed that acreage, output, and average yield will all increase in Pakistan by 2025. Cotton crop area in Punjab will expand by 2025, but cotton output and average yield will continue to fall. We used power Bi to visualize these outputs. Our results show there has been a significant shift in cotton mill activity towards Asia in recent decades, in particular the People's Republic of China. The OECD/FAO agricultural outlook for this year assumes a slight upward trend for mill consumption in China since 2016. With support for the cotton industry in India, another major cotton consumer, cotton mill usage is expected to grow continuously. © 2022 IEEE. | Gul, Malik Urfa; Paul, Anand; John Pratheep, K.; Jeon, Gwanggil | Kyungpook National University, Department of Computer Science and Engineering, Daegu, South Korea; Kyungpook National University, Department of Computer Science and Engineering, Daegu, South Korea; Intel, Santa Clara, CA, United States; Incheon National University, Department of Computer Science and Engineering, South Korea | 58087464900; 56650522400; 57485834500; 15022497800 | paul.editor@gmail.com; | 2022 10th International Conference on Orange Technology, ICOT 2022 | 0.64 | 2025-06-25 | 2 | Data analysis; demand and crop forecasting; visualization of data | Cotton; Crops; Cultivation; Data visualization; Growth rate; Average yield; Compound growths; Cotton production; Demand and crop forecasting; Demand forecasting; Pakistan; Product demand; Production forecasting; Tabular data; Visualization of data; Forecasting | English | Final | 2022 | 10.1109/icot56925.2022.10008177 | 바로가기 | 바로가기 | ||||||||||||||||||
| ○ | ○ | Proceedings Paper | CSS-A Cheap-Surrogate-Based Selection Operator for Multi-objective Optimization | Due to the complex topology of the search space, expensive multi-objective evolutionary algorithms (EMOEAs) emphasize enhancing the exploration capability. Many algorithms use ensembles of surrogate models to boost the performance. Generally, the surrogate-based model either works out the solution's fitness by approximating the evaluation function or selects the solution by weighting the uncertainty degree of candidate solutions. This paper proposes a selection operator called Cheap surrogate selection (CSS) for multi-objective problems by utilizing the density probability on a k-dimensional tree. As opposed to the first type of surrogate models, which approximate the objective function, the proposed CSS only estimates the uncertainty of the candidate solutions. As a result, CSS does not require extensive sampling or training. Besides, CSS makes use of neighbors' density and builds the tree with low computational complexity, resulting in an accelerated surrogate process. Moreover, a new EMOEA is proposed by integrating spherical search as the core optimizer with the proposed selection scheme. Over a wide variety of benchmark problems, we show that the proposed method outperforms several state-of-the-art EMOEAs. | Kong, Lingping; Kumar, Abhishek; Snasel, Vaclav; Das, Swagatam; Kromer, Pavel; Ojha, Varun | VSB Tech Univ Ostrava, Dept Comp Sci, Ostrava, Czech Republic; Kyungpook Natl Univ, Dept Artificial Intelligence, Daegu 701702, South Korea; Indian Stat Inst, Elect & Commun Sci Unit, 203 BT Rd, Kolkata 700108, India; Univ Reading, Dept Comp Sci, Reading, England | Kumar, Abhishek/ABA-5251-2021; Ojha, Varun/M-2319-2013; Kong, Lingping/KPB-3641-2024; Ojha, Varun/AAD-4994-2020; Krömer, Pavel/D-8347-2016; Das, Swagatam/AAG-6753-2019; Snasel, Vaclav/B-8094-2009 | 56031337800; 57206266703; 57195632134; 24729258600; 8907452600; 55339927100 | lingping.kong@vsb.cz;abhishek.kumar.eee13@iitbhu.ac.in;vaclav.snasel@vsb.cz;swagatam.das@isical.ac.in;pavel.kromer@vsb.cz; | BIOINSPIRED OPTIMIZATION METHODS AND THEIR APPLICATIONS | 0302-9743 | 1611-3349 | 13627 | 0 | 2025-06-25 | 0 | 0 | Multi-objective optimization; Evolutionary algorithm; Cheap surrogate selection; Spherical search | EVOLUTIONARY ALGORITHM; MODEL | Cheap surrogate selection; Evolutionary algorithm; Multi-objective optimization; Spherical search | Forestry; Genetic algorithms; Uncertainty analysis; Cheap surrogate selection; Complex topology; Multi-Objective Evolutionary Algorithm; Multi-objectives optimization; Performance; Search spaces; Selection operators; Spherical search; Surrogate modeling; Surrogate-based modeling; Multiobjective optimization | English | 2022 | 2022 | 10.1007/978-3-031-21094-5_5 | 바로가기 | 바로가기 | 바로가기 | |||||||||
| ○ | ○ | Article | CT Imaging Findings in Non-Atherosclerotic Coronary Artery Disease | Acute coronary syndrome (ACS) is mainly caused by atherosclerotic coronary artery disease (CAD); however, it can also occur in patients with non -atherosclerotic CAD. Conventional coronary angiography only shows the lumen of arteries, indicating the presence of stenosis or dilatation. Thus, it has limited value in evaluating the coronary artery wall and offers low specificity for diagnosing CAD. Coronary CT angiography provides additional information, including the depiction of the concerned vessel and the aorta, as well as the pulmonary artery, which permits the diagnosis of non -atherosclerotic CAD and the differentiation of various causes of the disease. In this review, we present the pathophysiology and CT imaging features of non -atherosclerotic CAD. | Park, Jongmin; Park, Byunggeon; Kang, Eun-Ju; Lee, Jongmin | Kyungpook Natl Univ, Sch Med, Dept Radiol, 130 Dongdeok Ro, Daegu 41944, South Korea; Kyungpook Natl Univ, Kyungpook Natl Univ Chilgok Hosp, Sch Med, Dept Radiol, Daegu, South Korea; Dong A Univ, Coll Med, Med Ctr, Dept Radiol, Busan, South Korea | Kang, Eun-Ju/N-7376-2015; Lee, Jongmin/AAR-6361-2020 | 57216463879; 57211532915; 8395421600; 55689919700 | jonglee@knu.ac.kr; | JOURNAL OF THE KOREAN SOCIETY OF RADIOLOGY | 2951-0805 | 83 | 1 | 0 | 2025-06-25 | 0 | 0 | Coronary Artery Disease; Coronary Vasospasm; Takayasu's Arteritis; Kawasaki Disease; Computed Tomography; X-Ray | ST-SEGMENT ELEVATION; KAWASAKI-DISEASE; INTRAVASCULAR ULTRASOUND; ANGIOGRAPHIC FINDINGS; COMPUTED-TOMOGRAPHY; TAKAYASU ARTERITIS; RISK-FACTORS; SPASM; DIAGNOSIS; FEATURES | Computed Tomography, X-Ray; Coronary Artery Disease; Coronary Vasospasm; Kawasaki Disease; Takayasu's Arteritis | English | 2022 | 2022-01 | 10.3348/jksr.2021.0165 | 바로가기 | 바로가기 | 바로가기 | ||||||||||
| ○ | Book chapter | Curcumin usage for inflammation and spinal cord injury | Curcumin is an herbal medicine that has been used for a very long time in Asian countries, including India. Curcumin is a key active ingredient that is extracted from turmeric. Turmeric is a rhizomatous plant of the ginger family, and modern scientific studies have demonstrated its extensive pharmacological activity, such as inflammation relief and anti-oxidant effects. The neuroprotective effect of turmeric has also been reported in several experimental studies on the animal brain and neuronal tissue. These functional properties of curcumin have great potential in the treatment of spinal cord injury (SCI). Curcumin is a valid and effective therapeutic agent that could alleviate the catastrophic secondary injury process of the spinal cord, including inflammation, edema, free radical injury, fibrosis, and glial scar formation. This potential is supported by the immune pathological results obtained from several animal experiments, and significantly better outcomes were achieved in the evaluation using the Basso, Beattie, and Bresnahan locomotor rating scale for neurological function recovery. However, the evidence-based effectiveness of curcumin for SCI remains in the experimental stage, and questions pertaining to its clinical application, such as dose-safety verification and bioavailability remain unanswered. © 2022 Elsevier Inc. All rights reserved. | Lee, Subum; Kim, Kyoung-Tae | Department of Neurosurgery, Korea University Anam Hospital, Seoul, South Korea; Department of Neurosurgery, School of Medicine, Kyungpook National University, Kyungpook National University Hospital, Daegu, South Korea | 57193631061; 57201369790 | Diagnosis and Treatment of Spinal Cord Injury | 0 | 2025-06-25 | 0 | Curcumin; Functional recovery; Inflammation; Neuroprotective effect; Oxidative stress; Spinal cord injury | English | Final | 2022 | 10.1016/b978-0-12-822498-4.00033-6 | 바로가기 | 바로가기 | ||||||||||||||||||||
| ○ | Review | Current Status and Prospects Regarding Radiocarbon Studies in the East Sea | Together with the development of measurement techniques, radiocarbon (14C) has been increasingly used as a key tool to investigate carbon cycling and associated biogeochemistry in the ocean. In this paper, the current status of radiocarbon studies in the East Sea (Japan Sea) is reviewed. Previously, spatiotemporal distribution and change of the water masses in the East Sea from 1979 to 1999 were investigated by using the14C in the dissolved inorganic carbon (DIC). Researches on sinking particulate organic carbon (POC) revealed that POC in the deep ocean has more complex and heterogeneous origins than we expected. In particular, since 2011, Korean researchers have been collecting sinking particle samples for more than 10 years, so it is expected that14C of POC will provide important information to understand carbon cycling in relation to climate change. Although the quantity of14C data published in the East Sea is still limited, the importance and the future direction of using14C to understand the biogeochemical mechanisms of carbon cycling and its role as a carbon reservoir in the East Sea are detailed herein. © 2022, Korea Ocean Research and Development Institute. All rights reserved. | Kim, Minkyoung | School of Earth System Sciences, College of Natural Sciences, Kyungpook National University, Daegu, 41566, South Korea | 57212315624 | minkyoung@knu.ac.kr; | Ocean and Polar Research | 1598-141X | 44 | 1 | 0 | 2025-06-25 | 0 | carbon cycling; DIC (dissolved inorganic carbon); East Sea; radiocarbon; sinking POC (particulate organic carbon) | Pacific Ocean; Sea of Japan; biogeochemistry; carbon cycle; carbon sink; dissolved inorganic carbon; particulate organic carbon; radiocarbon dating | Korean | Final | 2022 | 10.4217/opr.2022008 | 바로가기 | 바로가기 | |||||||||||||||
| ○ | ○ | Article | Current status of cytopathology practice in Korea: impact of the coronavirus pandemic on cytopathology practice | Background: The Continuous Quality Improvement program for cytopathology in 2020 was completed during the coronavirus pandemic. In this study, we report the result of the quality improvement program. Methods: Data related to cytopathology practice from each institute were collected and processed at the web-based portal. The proficiency test was conducted using glass slides and whole-slide images (WSIs). Evaluation of the adequacy of gynecology (GYN) slides from each institution and submission of case glass slides and WSIs for the next quality improvement program were performed. Results: A total of 214 institutions participated in the annual cytopathology survey in 2020. The number of entire cytopathology specimens was 8,220,650, a reduction of 19.0% from the 10,111,755 specimens evaluated in 2019. Notably, the number of respiratory cytopathology specimens, including sputum and bronchial washing/ brushing significantly decreased by 86.9% from 2019, which could be attributed to the global pandemic of coronavirus disease. The ratio of cases with atypical squamous cells to squamous intraepithelial lesions was 4.10. All participating institutions passed the proficiency test and the evaluation of adequacy of GYN slides. Conclusions: Through the Continuous Quality Improvement program, the effect of coronavirus disease 2019 pandemic, manifesting with a reduction in the number of cytologic examinations, especially in respiratory-related specimen has been identified. The Continuous Quality Improvement Program of the Korean Society for Cytopathology can serve as the gold standard to evaluate the current status of cytopathology practice in Korea. | Hong, Soon Auck; Jung, Haeyoen; Kim, Sung Sun; Jin, Min-Sun; Pyo, Jung-Soo; Jeong, Ji Yun; Choi, Younghee; Gong, Gyungyub; Chong, Yosep | Chung Ang Univ, Coll Med, Dept Pathol, Seoul, South Korea; Eone Reference Lab, Dept Pathol, Incheon, South Korea; Chonnam Natl Univ, Med Sch, Dept Pathol, Gwangju, South Korea; Catholic Univ Korea, Coll Medidne, Dept Hosp Pathol, Seoul, South Korea; Eulji Univ, Uijeongbu Eulji Univ Hosp, Sch Med, Dept Pathol, Uijongbu, South Korea; Kyungpook Natl Univ, Chilgok Hosp, Sch Med, Dept Pathol, Daegu, South Korea; Hallym Univ, Dongtan Sacred Heart Hosp, Dept Pathol, Hwasung, South Korea; Ulsan Univ, Coll Med, Asan Med Ctr, Dept Pathol, Seoul, South Korea | ; Chong, Yosep/ISA-4170-2023; Choi, Sung-hee/J-5689-2012; Kim, Suhnggwon/J-5407-2012 | 35181418800; 57218776368; 35069766900; 56927442600; 55127950000; 57205472984; 55685949600; 7103214892; 23666142300 | ychong@catholic.ac.kr; | JOURNAL OF PATHOLOGY AND TRANSLATIONAL MEDICINE | J PATHOL TRANSL MED | 2383-7837 | 2383-7845 | 56 | 6 | ESCI | PATHOLOGY | 2022 | 2.4 | 0.49 | 2025-06-25 | 3 | 3 | Cytology; Surveys; Statistics; Quality; Coronavirus; Pandemic | CYTOLOGY; PROGRAM; RATIO | Coronavirus; Cytology; Pandemic; Quality; Statistics; Surveys | adenocarcinoma; Article; atypical squamous cells of the cervix; comparative study; coronavirus disease 2019; correlational study; cytodiagnosis; cytopathology; endobronchial ultrasonography; endometrium; endoscopic ultrasonography; general hospital; health care practice; health survey; human; Korea; laboratory; ovary; pandemic; quality control; questionnaire; sputum analysis; squamous cell carcinoma; squamous cell lesion; total quality management; tracheobronchial toilet; university hospital; uterine cervix cytology; vaginal secretion | English | 2022 | 2022-11 | 10.4132/jptm.2022.09.21 | 바로가기 | 바로가기 | 바로가기 | 바로가기 |
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