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Back Cover: Plasma Process. Polym. 1∕2015

Plasma Processes and Polymers 2015年第1期12卷

作者： Xunzhi Huang Yongsheng Li Xiaoxia Zhong Amanda E. Rider Kostya (Ken) Ostrikov State Key Laboratory of Advanced Optical Communication Systems and Networks Key Laboratory for Laser Plasmas (Ministry of Education) Department of Physics and Astronomy Shanghai Jiao Tong University Shanghai 200240 China School of Physics University of Sydney New South Wales 2006 Australia Industrial Innovation Program Manufacturing Flagship CSIRO Lindfield New South Wales 2070 Australia Institute for Future Environments and School of Chemistry Physics and Mechanical Engineering Queensland University of Technology Brisbane Queensland 4000 Australia

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Emerging contaminants:A One Health perspective

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The Innovation 2024年第4期5卷 140-170,139页

作者： Fang Wang Leilei Xiang Kelvin Sze-Yin Leung Martin Elsner Ying Zhang Yuming Guo Bo Pan Hongwen Sun Taicheng An Guangguo Ying Bryan WBrooks Deyi Hou Damian EHelbling Jianqiang Sun Hao Qiu Timothy MVogel Wei Zhang Yanzheng Gao Myrna JSimpson Yi Luo Scott XChang Guanyong Su Bryan MWong Tzung-May Fu Dong Zhu Karl JJobst Chengjun Ge Frederic Coulon Jean Damascene Harindintwali Xiankui Zeng Haijun Wang Yuhao Fu Zhong Wei Rainer Lohmann Changer Chen Yang Song Concepcion Sanchez-Cid Yu Wang Ali El-Naggar Yiming Yao Yanran Huang Japhet Cheuk-Fung Law Chenggang Gu Huizhong Shen Yanpeng Gao Chao Qin Hao Li Tong Zhang Natàlia Corcoll Min Liu Daniel SAlessi Hui Li Kristian KBrandt Yolanda Pico Cheng Gu Jianhua Guo Jianqiang Su Philippe Corvini Mao Ye Teresa Rocha-Santos Huan He Yi Yang Meiping Tong Weina Zhang Fidèle Suanon Ferdi Brahushi Zhenyu Wang Syed AHashsham Marko Virta Qingbin Yuan Gaofei Jiang Louis A.Tremblay Qingwei Bu Jichun Wu Willie Peijnenburg Edward Topp Xinde Cao Xin Jiang Minghui Zheng Taolin Zhang Yongming Luo Lizhong Zhu Xiangdong Li DamiàBarceló Jianmin Chen Baoshan Xing Wulf Amelung Zongwei Cai Ravi Naidu Qirong Shen Janusz Pawliszyn Yong-guan Zhu Andreas Schaeffer Matthias C.Rillig Fengchang Wu Gang Yu James M.Tiedje State Key Laboratory of Soil and Sustainable Agriculture Institute of Soil ScienceChinese Academy of SciencesNanjing 210008China University of Chinese Academy of Sciences Beijing 100049China Department of Chemistry Hong Kong Baptist UniversityHong KongChina HKBU Institute of Research and Continuing Education Shenzhen Virtual University ParkShenzhenChina Technical University of Munich TUM School of Natural SciencesInstitute of Hydrochemistry85748 GarchingGermany School of Resources&Environment Northeast Agricultural UniversityHarbin 150030China Climate Air Quality Research UnitSchool of Public Health and Preventive MedicineMonash UniversityMelbourneVICAustralia Faculty of Environmental Science&Engineering Kunming University of Science&TechnologyKunming 650500China Ministry of Education Key Laboratory of Pollution Processes and Environmental Criteria College of Environmental Science and EngineeringNankai UniversityTianjin 300350China Guangdong Key Laboratory of Environmental Catalysis and Health Risk Control School of Environmental Science and EngineeringInstitute of Environmental Health and Pollution ControlGuangdong University of TechnologyGuangzhou 510006China Ministry of Education Key Laboratory of Environmental Theoretical Chemistry South China Normal UniversityGuangzhouGuangdong 510006China Department of Environmental Science Baylor UniversityWacoTXUSA Center for Reservoir and Aquatic Systems Research(CRASR) Baylor UniversityWacoTXUSA School of Environment Tsinghua UniversityBeijing 100084China School of Civil and Environmental Engineering Cornell UniversityIthacaNY 14853USA Key Laboratory of Microbial Technology for Industrial Pollution Control of Zhejiang Province Zhejiang University of TechnologyHangzhou 310014China School of Environmental Science and Engineering Shanghai Jiao Tong UniversityShanghai 200240China Laboratoire d’Ecologie Microbienne Universite Claude Bernard Lyon 1UMR CNRS 5557UMR INRAE 1418VetAgro Sup69622 VilleurbanneFrance Department of Pla

Environmental pollution is escalating due to rapid global development that often prioritizes human needs over planetary *** global efforts to mitigate legacy pollutants,the continuous introduction of new substances remains a major threat to both people and the *** response,global initiatives are focusing on risk assessment and regulation of emerging contaminants,as demonstrated by the ongoing efforts to establish the UN’s Intergovernmental Science-Policy Panel on Chemicals,Waste,and Pollution *** review identifies the sources and impacts of emerging contaminants on planetary health,emphasizing the importance of adopting a One Health *** for monitoring and addressing these pollutants are discussed,underscoring the need for robust and socially equitable environmental policies at both regional and international *** actions are needed to transition toward sustainable pollution management practices to safeguard our planet for future generations.

关键词： pollution planet contaminants

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THE INTRODUCTION OF HEAT RECOVERABLE COUPLINGS TO SHIP REPAIR AND MAINTENANCE

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NAVAL ENGINEERS JOURNAL 1982年第6期94卷 63-71页

作者： LIBERATORE, DJ BASKERVILLE, JE LCdr. Donald J. Liberatore USN: began his career in the U.S. Navy in 1965. He has had many diverse assignments involving surface ships and submarines during the past seventeen years. During his tour at Naval Shipyard Portsmouth (N.H.) he was Assistant Design Superintendent and responsible for the introduction of Heat Recoverable Coupling technology into the shipyard. Presently he is assigned to the Naval Sea Systems Command (NAVSEA) in the Sonar Dome Office. Prior assignments within NAVSEA have been as Assistant Ship Systems Design Manager for the SSNX and FA-SSN preliminary designs in the Submarine Propulsion Analysis Branch in the Submarine Hydrodynamics Branch and in the Gear Coupling and Clutch Branch. He received his Bachelor of Engineering degree from Vanderbilt University in 1971 and in 1977 graduated from Massachusetts Institute of Technology with his M.S. degree in Naval Architecture and Marine Engineering and his Professional degree of Ocean Engineer. A member of ASNE since 1975 LCdr. Liberatore also is a member of IEEE SNAME the Naval Institute and Sigma Xi. Cdr. James E. Baskerville USN: is presently assigned to NAVSEA as the Ship Manager for the DDG 51 the Navy's next generation surface combatant. In a previous tour at Naval Shipyard Pearl Harbor he was the Navy's Program Manager for Heat Recoverable Coupling introduction in ship repair and maintenance. A graduate of the U.S. Naval Academy Class of 1969 he is a qualified Surface Warfare Officer and a designated Engineering Duty Officer (ED). He received his M.S. degree in Mechanical Engineering and his Professional degree of Ocean Engineer from Massachusetts Institute of Technology and also holds a patent right on an Electronic Control and Response System. His naval assignments have included tours in the USS Ramey (FFG-2) as Aide and Flag Lieutenant to the Commander Naval Electronic Systems Command and as Ship Superintendent Surface Type Desk Officer and Assistant Design Superintendent at Naval Shipyard Pearl Harbor. Cdr. Baskervi

Although Heat Recoverable Couplings (HRCs), used to join pipe, may be labeled innovative “state-of-the-art” technology for U.S. Naval Shipyards, they have been in use in foreign ships and high technology industries for over a decade. HRCs provide a permanent leak-proof pipe joint in specified applications without the use of high temperature and the inherent hazards of an open flame. Manufactured from NITINOL, a nickel-titanium alloy developed by the U.S. Navy, the couplings exhibit a “shape memory” characteristic. That is, they return (shrink) to a specified shape (pipe diameter) thus forming a mechanical seal when the expanded coupling is removed from a cryogenic environment and warmed above approximately —130°C. This paper provides background information into the development of NITINOL, technical explanation of shape memory metallurgy, and a summary of results, with specific examples, describing the trial use of HRCs at Pearl Harbor and Norfolk Naval Shipyards. Limited return cost data and recommendations for future use are presented. Then, using the HRC program as a basis, the Authors discuss the conservative nature of the ship repair and maintenance environment. This environment, in the Authors' opinion, couples with complex contractual constraints and requirements which serve to restrict the introduction of new ideas. An analogy is made to Russian tenacity of recent years which promotes “exploring and doing” while we in the U.S. Navy are frequently content to study.

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Insights from a multiscale framework on metabolic rate variation driving glioblastoma multiforme growth and invasion

Communications Engineering

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Communications engineering 2024年第1期3卷 176页

作者： Amereh, Meitham Shojaei, Shahla Seyfoori, Amir Walsh, Tavia Dogra, Prashant Cristini, Vittorio Nadler, Ben Akbari, Mohsen Department of Mechanical Engineering University of Victoria 3800 Finnerty Road Victoria V8P 5C2 BC Canada Laboratory for Innovations in MicroEngineering (LiME) University of Victoria 3800 Finnerty Road Victoria V8P 5C2 BC Canada Centre for Advanced Materials and Related Technologies (CAMTEC) University of Victoria 3800 Finnerty Road Victoria V8P 5C2 BC Canada Department of Anatomy and Cell Sciences University of Manitoba 66 Chancellors Cir Winnipeg R3B 2E9 MB Canada Mathematics in Medicine Program Department of Medicine Houston Methodist Research Institute 6670 Bertner Ave. Houston 77030 TX United States Department of Physiology and Biophysics Weill Cornell Medical College 1300 York Ave. New York 10065 NY United States Neal Cancer Center Houston Methodist Research Institute 6670 Bertner Ave. Houston 77030 TX United States Department of Imaging Physics University of Texas M.D. Anderson Cancer Center 1515 Holcombe Blvd Houston 77030 TX United States Physiology Biophysics and Systems Biology Program Graduate School of Medical Sciences Weill Cornell Medicine 1300 York Ave. New York 10065 NY United States School of Biomedical Engineering University of British Columbia 2329 West Mall Vancouver V6T 1Z4 BC Canada

Non-physiological levels of oxygen and nutrients within the tumors result in heterogeneous cell populations that exhibit distinct necrotic, hypoxic, and proliferative zones. Among these zonal cellular properties, metabolic rates strongly affect the overall growth and invasion of tumors. Here, we report on a hybrid discrete-continuum (HDC) mathematical framework that uses metabolic data from a biomimetic two-dimensional (2D) in-vitro cancer model to predict three-dimensional (3D) behaviour of in-vitro human glioblastoma (hGB). The mathematical model integrates modules of continuum, discrete, and neurons. Results indicated that the HDC model is capable of quantitatively predicting growth, invasion length, and the asymmetric finger-type invasion pattern in in-vitro hGB tumors. Additionally, the model could predict the reduction in invasion length of hGB tumoroids in response to temozolomide (TMZ). This model has the potential to incorporate additional modules, including immune cells and signaling pathways governing cancer/immune cell interactions, and can be used to investigate targeted therapies. © The Author(s) 2024.

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THE MANAGEMENT OF SURFACE SHIP MAINTENANCE

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NAVAL ENGINEERS JOURNAL 1980年第6期92卷 71-83页

作者： WOODRUFF, RB USN THE AUTHORgraduated from the U.S. Naval Academy with distinction in 1964. He served initially in theUSS Davis (DD-937)as Main Propulsion Assistant attended the Naval Destroyer School. and then was a member of the Pre-Commissioning Crew and Engineer Officer in theUSS Julius A. Furer (DEG-6).Selected as an Engineering Duty Officer (ED) in 1968. he had a tour in the Maintenance Department Staff of Commander Cruiser-Destroyer Force U.S. Atlantic Fleet at Newport. R.I. after which he attended Massachusetts Institute of Technology for graduate studies which culminated in his receiving his M.S. degree in Mechanical Engineering and his degree of Ocean Engineer in 1972. Following graduation he was assigned to the Boston Naval Shipyard followed by two years in theUSS Puget Sound (AD-38) asRepair Officer after which he was ordered to the Norfolk Naval Shipyard as the Production Engineering Officer. Currently he is on duty in the Naval Sea Systems Command (PMS 399) where he is the Trials Officer and Deputy Hull Technical Director for the OLIVER HAZARD PERRY (FFG 7) Class Acquisition Program. Cdr. Woodruff is a qualified Surface Warfare Officer. and among his military decorations holds the Naval Achievement Medal and the Vietnamese Meritorious Unit Citation Gallantry Cross. In addition to ASNE which he joined in 1967. he is a member of SNAME and the U.S. Naval Institute. and his two previous papers on Naval Shipyard Production presented at ASNE Day 1978 and 1979 were published in theNaval Engineers JournalVol. 90 No. 2 (April 1978) and Vol. 91. No. 2 (April 1979).

The purpose of the paper is to address the current dilemma facing the Surface Ship Navy as it approaches the twenty-first century. The basic underlying thesis is that the Maintenance Community has lost sight of the goal it must have: to support the Commanding Officer of a ship to get his ship from point A to point B with its weapons system ready. To do this, three basic things must occur: 1) the ship must be capable of getting underway and steaming (i.e., turn the screw); 2) the ship must have its weapons systems working and “up” in all respects (i.e., fight the ship); and 3) the Crew must be prepared (i.e., have sufficient training). It Is submitted that we have lost sight of this fact. There remains an inordinate amount of concern over appearance (external and internal), habitability, plaques, inspections, and various human factors programs, and funds may be spent in there areas when the main machinery plant and missile systems are “down.” A recent example is the effort to remove every speck of wood from all Navy ships including picture frames. Training is addressed also as the third key element missing, particularly in the main machinery spaces. A brief examination is made of the ship cycle as it gas into the maintenance mode, i.e., delivery plus one to two years. A comparison is made with the basic Submarine Force approach to this problem and when the Surface Community may take a page out of the Submarine Force book. An addressed are: 1) Current Ship's Maintenance Project (CSMP); 2) Planned Maintenance System (PMS); 3) Pre-Overhaul Test and Inspection (POT&I); 4) Long lead time SHIPALT material, 5) Intermediate Maintenance Activity (IMA) role (Tenders and SIMAS); and 6) Shipyard role and facilities.

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THE FFG 7 CLASS DESIGN IMPACT BY INSURV TRIALS

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NAVAL ENGINEERS JOURNAL 1982年第2期94卷 87-100页

作者： WOODRUFF, RB The authorgraduated from the U.S. Naval Academy with distinction in 1964. He served initially in theUSS Davis (DD-937)as Main Propulsion Assistant attended the Naval Destroyer School and then was a member of the Pre-Commissioning Crew and Engineer Officer in theUSS Julius A. Furer (DEG-6).Selected as an Engineering Duty Officer (ED) in 1968 he had a tour in the Maintenance Department Staff of Commander Cruisr-Destroyer Force U.S. Atlantic Fleet at Newport R.I. after which he attended Massachusetts Institute of Technology for graduate studies which culminated in his receiving his M.S. degree in Mechanical Engineering and his degree of Ocean Engineer in 1972. Following graduation he was assigned to the Boston Naval Shipyard followed by two years in theUSS Puget Sound (AD-38)as Repair Officer after which he was ordered to the Norfolk Naval Shipyard as the Production Engineering Officer. Currently he is on duty in the Naval Sea Systems Command (PMS 399) where he is the Trials Officer and Hull Technical Director for theOliver Hazard Perry (FFG-7)Class Acquisition Program. Cdr. Woodruff is a qualified Surface Warfare Officer and among his military decorations holds the Naval Achievement Medal and the Vietnamese Meritorious Unit Citation Gallantry Cross. In addition to ASNE which he joined in 1967 he is a member of the U.S. Naval Institute. Two previous papers on Naval Shipyard Production presented at ASNE Day 1978 and 1979 were published in the Naval Engineers Journal Vol. 90 No. 2 (April 1978) and Vol. 91 No. 2 (April 1979). A paper on the Management of Surface Ship Maintenance was published in theNaval Engineers JournalDecember 1980.

This paper describes the impact made on the OLIVER HAZARD PERRY (FFG 7) Class design after numerous trials by the President, Board of Inspection and Survey and his Staff. In the early 1970s, faced with a Fleet of World War II Destroyers, the Navy embarked on a program to build large numbers of Frigates to perform an Ocean Escort role. This ship had three major design constraints placed on it by Chief of Naval Operations (CNO): fixed meaning, fixed displacement, and fixed cost or “designed to cost.” The purpose of this paper is to pass on some “lessons learned.” The acid test of any ship design is how well it does with the Fleet in regard to performance and reliability. How well has the “design-constrained” FFG-7 fared with 20 plus ship trials under its belt? Very well in some areas; not so well in others. Examples of the good aspects of this ship design (LM 2500 and main propulsion train, Standard Option Equipment, et cetera) as well as those which must be considered poor will be addressed. Some examples of the latter are the “breezeway” cargo doors, ship's service diesel generators, MK 92 Combat systems, decontamination stations, and topside corrosion control. In many cases INSURV caused design changes to be made that were sorely needed; in other cases, changes were made (or not made) over issues that had little or no impact on making this ship more ready for war. A brief examination of the Naval Sea systems Command (NAVSEA) surface ship design policies is made from the point of view of the Trials Officer (the Author) who rode most of the trials with PRESINSURV. Some of the issues addressed: •Improved NAVSEA corporate memory between ship designs. •Longer Acceptance Trial for Lead Ship. •Early deployment of Lead Ship without TECHREPS. •Improved NAVSEA/INSURV/CNO communication on Trial/Technical Issues and insertion of INSURV early into the design process. •Need for NAVSEA to stand up and say “no” to costly design changes that do little to make for a better warship.

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U.S. SHIPBUILDING: THE SEVENTIES IN RETROSPECT —THE PROSPECTS FOR THE EIGHTIES

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Naval Engineers Journal 1980年第4期92卷 25-38页

作者： FISHER, JAMES R. COADY, PHILIP USN Capt. James Ronald Fisher USN is a graduate of the U.S. Naval Academy. Class of 1958. has his M.A. degree in Management and is an Engineering Duty Officer (ED). He has served in a Destroyer and four Attack and Fleet Ballistic Missile Submarines as Training Officer of the Nuclear Propulsion Unit. West Milton N. Y. and at the Charleston Naval Shipyard where he also was the Chairman of the ASNE Charleston Section. He was ordered to the National Defense University from duty in the Industrial Management Directorate Naval Sea Systems Command (NAVSEA). and has just recently been reassigned to the Submarine Platform Directorate at NA VSEA. Cdr. Philip Coady USN is a graduate of Tufts University from which he received his A.B. degree in 1963 and also the Naval Postgraduate School. Monterey. Calif. from which he received his M.S. degree in 1972. His sea experience has been predominently in Destroyers. most recently as Executive Officer of the USS Claude V. Ricketts (DDG-S) and has had two tours in the Office of the Chief of Naval Operations (OP-090) his latest being that of Special Assistant for Financial Management to the Director of Navy Program Planning (OP-090). Currently he is under orders to assume command of the USS Conolly (DD-979).

This paper reviews the recent turbulent history of the U.S. Shipbuilding Industry, its present status, and its prospects for the decade ahead. The Authors suggest that current maritime policy and the trend of market f...

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Application of Interpolation Image by using Bi-Cubic Algorithm

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Journal of Physics: Conference Series 2018年第1期1114卷

作者： Dahlan Abdullah F Fajriana M Maryana Lidya Rosnita Andysah Putera Utama Siahaan Robbi Rahim P Harliana H Harmayani Zainuddin Ginting Cut Ita Erliana Defi Irwansyah Z Zulmiardi Muammar Khaddafi Feby Milanie Henry Aspan Ismul Huda Kundharu Saddhono Indrya Mulyaningsih Roy Marthen Moonti Parwito Hardianto Djanggih Ainna Amalia Edy Winarno Wiwien Hadikurniawati Department of Informatics Universitas Malikussaleh Aceh Indonesia School of Computer and Communication Engineering Universiti Malaysia Perlis Malaysia Department of Informatics Engineering Sekolah Tinggi Teknik Harapan Medan Indonesia Department of Informatics AMIK Intel Com Global Indo Indonesia Department of Chemical Engineering Universitas Malikussaleh Aceh Indonesia Department of Industrial Engineering Universitas Malikussaleh Aceh Indonesia Department of Mechanical Engineering Universitas Malikussaleh Aceh Indonesia Department of Accounting Universitas Malikussaleh Aceh Indonesia Universitas Pembangunan Panca Budi Medan Indonesia Universitas Syiah Kuala Aceh Indonesia Graduate Program Universitas Sebelas Maret Surakarta Indonesia Indonesian Language Teaching Department Institut Agama Islam Negeri Syekh Nurjati Cirebon Indonesia Department of Law Universitas Gorontalo Gorontalo Indonesia Department of Agrotechnology Universitas Ratu Samban Bengkulu Indonesia Department of Law Universitas Tompotika Luwuk Banggai Luwuk Indonesia Islamic Institut of Miftahul Ula Kertosono Nganjuk East Java Indonesia Faculty of Information Technology Universitas Stikubank Semarang Indonesia

Image magnification is one of the branches in digital image processing that is often required in various applications such as in the field of medicine, multimedia, and in satellite imagery. As technology grows, more and more methods are used for image enlargement. In this study, the image enlargement process performs by using Bi-Cubic spline interpolation method, and the result of image try to compare between the original one and picture after enlargement.

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LST-1 observations of an enormous flare of BL Lacertae in 2021 38

LST-1 observations of an enormous flare of BL Lacertae in 20...

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38th International Cosmic Ray Conference, ICRC 2023

作者： Nozaki, Seiya Asano, Katsuaki Escudero, Juan Emery, Gabriel Priyadarshi, Chaitanya Abe, K. Abe, S. Aguasca-Cabot, A. Agudo, I. Alvarez Crespo, N. Antonelli, L.A. Aramo, C. Arbet-Engels, A. Arcaro, C. Artero, M. Asano, K. Aubert, P. Baktash, A. Bamba, A. Baquero Larriva, A. Baroncelli, L. Barres de Almeida, U. Barrio, J.A. Batkovic, I. Baxter, J. Becerra González, J. Bernardini, E. Bernardos, M.I. Bernete Medrano, J. Berti, A. Bhattacharjee, P. Biederbeck, N. Bigongiari, C. Bissaldi, E. Blanch, O. Bonnoli, G. Bordas, P. Bulgarelli, A. Burelli, I. Burmistrov, L. Buscemi, M. Cardillo, M. Caroff, S. Carosi, A. Carrasco, M.S. Cassol, F. Cauz, D. Cerasole, D. Ceribella, G. Chai, Y. Cheng, K. Chiavassa, A. Chikawa, M. Chytka, L. Cifuentes, A. Contreras, J.L. Cortina, J. Costantini, H. Dalchenko, M. Dazzi, F. De Angelis, A. de Bony de Lavergne, M. De Lotto, B. De Lucia, M. de Menezes, R. Del Peral, L. Deleglise, G. Delgado, C. Delgado Mengual, J. della Volpe, D. Dellaiera, M. Di Piano, A. Di Pierro, F. Di Pilato, A. Di Tria, R. Di Venere, L. Díaz, C. Dominik, R.M. Dominis Prester, D. Donini, A. Dorner, D. Doro, M. Eisenberger, L. Elsässer, D. Emery, G. Escudero, J. Fallah Ramazani, V. Ferrara, G. Ferrarotto, F. Fiasson, A. Foffano, L. Freixas Coromina, L. Fröse, S. Fukami, S. Fukazawa, Y. Garcia, E. Garcia López, R. Gasbarra, C. Gasparrini, D. Geyer, D. Giesbrecht Paiva, J. Giglietto, N. Giordano, F. Gliwny, P. Godinovic, N. Grau, R. Green, J. Green, D. Gunji, S. Günther, P. Hackfeld, J. Hadasch, D. Hahn, A. Hashiyama, K. Hassan, T. Hayashi, K. Heckmann, L. Heller, M. Herrera Llorente, J. Hirotani, K. Hoffmann, D. Horns, D. Houles, J. Hrabovsky, M. Hrupec, D. Hui, D. Hütten, M. Iarlori, M. Imazawa, R. Inada, T. Inome, Y. Ioka, K. Iori, M. Ishio, K. Jimenez Martinez, I. Jurysek, J. Kagaya, M. Karas, V. Katagiri, H. Kataoka, J. Kerszberg, D. Kobayashi, Y. Kohri, K. Kong, A. Kubo, H. Kushida, J. Lainez, M. Lamanna, G. Lamastra, A. Le Flour, T. Linhoff, M. Longo, F. López-Coto, R. Max-Planck-Institut für Physik Föhringer Ring 6 München80805 Germany Institute for Cosmic Ray Research University of Tokyo 5-1-5 Kashiwa-no-ha Chiba Kashiwa277-8582 Japan Instituto de Astrofísica de Andalucía-CSIC Glorieta de la Astronomía s/n Granada18008 Spain Aix Marseille Univ CNRS IN2P3 CPPM Marseille France The Barcelona Institute of Science and Technology Campus UAB Bellaterra Barcelona08193 Spain Department of Physics Tokai University Japan Departament de Física Quàntica i Astrofísica Institut de Ciències del Cosmos Universitat de Barcelona IEEC-UB Spain EMFTEL department IPARCOS Universidad Complutense de Madrid Spain INAF Osservatorio Astronomico di Roma Italy INFN Sezione di Napoli Italy INFN Sezione di Padova Università degli Studi di Padova Italy LAPP Univ. Grenoble Alpes Univ. Savoie Mont Blanc CNRS-IN2P3 Annecy France Universität Hamburg Institut für Experimentalphysik Germany Graduate School of Science University of Tokyo Japan Universidad del Azuay Ecuador INAF Osservatorio di Astrofisica e Scienza dello spazio di Bologna Italy Centro Brasileiro de Pesquisas Físicas Brazil Instituto de Astrofísica de Canarias Departamento de Astrofísica Universidad de La Laguna Spain CIEMAT Spain Department of Physics TU Dortmund University Germany INFN Sezione di Bari Politecnico di Bari Italy INAF Osservatorio Astronomico di Brera Italy INFN Sezione di Trieste Università degli Studi di Udine Italy University of Geneva Département de physique nucléaire et corpusculaire Switzerland INFN Sezione di Catania Italy Italy INFN Sezione di Bari Università di Bari Italy INFN Sezione di Torino Italy Palacky University Olomouc Faculty of Science Czech Republic University of Alcalá UAH Spain Port d’Informació Científica Spain University of Rijeka Department of Physics Croatia Institute for Theoretical Physics and Astrophysics Universität Würzburg Germany Institut für Theoretische Physik Lehrstuhl IV: Plasma-Astroteilchenphysik Ruhr-Universit

The first prototype of LST (LST-1) for the Cherenkov Telescope Array has been in commissioning phase since 2018 and already started scientific observations with the low energy threshold around a few tens of GeV. In 2021, LST-1 observed BL Lac following the alerts based on multi-wavelength observations and detected prominent gamma-ray flares. In addition to the daily flux variability, LST-1 also detected sub-hour-scale intra-night variability reaching 3–4 times higher than the gamma-ray flux from the Crab Nebula above 100 GeV. In this proceeding, we will report the analysis results of LST-1 observations of BL Lac in 2021, especially focusing on flux variability. © Copyright owned by the author(s) under the terms of the Creative Commons.

关键词： Cosmology

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Performance of the Large-Sized Telescope prototype of the Cherenkov Telescope Array 38

Performance of the Large-Sized Telescope prototype of the Ch...

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38th International Cosmic Ray Conference, ICRC 2023

作者： Morcuende, D. López-Coto, R. Moralejo, A. Nozaki, S. Vuillaume, T. Abe, K. Abe, S. Aguasca-Cabot, A. Agudo, I. Alvarez Crespo, N. Antonelli, L.A. Aramo, C. Arbet-Engels, A. Arcaro, C. Artero, M. Asano, K. Aubert, P. Baktash, A. Bamba, A. Baquero Larriva, A. Baroncelli, L. Barres de Almeida, U. Barrio, J.A. Batkovic, I. Baxter, J. Becerra González, J. Bernardini, E. Bernardos, M.I. Bernete Medrano, J. Berti, A. Bhattacharjee, P. Biederbeck, N. Bigongiari, C. Bissaldi, E. Blanch, O. Bonnoli, G. Bordas, P. Bulgarelli, A. Burelli, I. Burmistrov, L. Buscemi, M. Cardillo, M. Caroff, S. Carosi, A. Carrasco, M.S. Cassol, F. Cauz, D. Cerasole, D. Ceribella, G. Chai, Y. Cheng, K. Chiavassa, A. Chikawa, M. Chytka, L. Cifuentes, A. Contreras, J.L. Cortina, J. Costantini, H. Dalchenko, M. Dazzi, F. De Angelis, A. de Bony de Lavergne, M. De Lotto, B. De Lucia, M. de Menezes, R. Del Peral, L. Deleglise, G. Delgado, C. Delgado Mengual, J. della Volpe, D. Dellaiera, M. Di Piano, A. Di Pierro, F. Di Pilato, A. Di Tria, R. Di Venere, L. Díaz, C. Dominik, R.M. Dominis Prester, D. Donini, A. Dorner, D. Doro, M. Eisenberger, L. Elsässer, D. Emery, G. Escudero, J. Fallah Ramazani, V. Ferrara, G. Ferrarotto, F. Fiasson, A. Foffano, L. Freixas Coromina, L. Fröse, S. Fukami, S. Fukazawa, Y. Garcia, E. Garcia López, R. Gasbarra, C. Gasparrini, D. Geyer, D. Giesbrecht Paiva, J. Giglietto, N. Giordano, F. Gliwny, P. Godinovic, N. Grau, R. Green, J. Green, D. Gunji, S. Günther, P. Hackfeld, J. Hadasch, D. Hahn, A. Hashiyama, K. Hassan, T. Hayashi, K. Heckmann, L. Heller, M. Herrera Llorente, J. Hirotani, K. Hoffmann, D. Horns, D. Houles, J. Hrabovsky, M. Hrupec, D. Hui, D. Hütten, M. Iarlori, M. Imazawa, R. Inada, T. Inome, Y. Ioka, K. Iori, M. Ishio, K. Jimenez Martinez, I. Jurysek, J. Kagaya, M. Karas, V. Katagiri, H. Kataoka, J. Kerszberg, D. Kobayashi, Y. Kohri, K. Kong, A. Kubo, H. Kushida, J. Lainez, M. Lamanna, G. Lamastra, A. Le Flour, T. Linhoff, M. Longo, F. López-Oramas, A. IPARCOS-UCM Instituto de Física de Partículas y del Cosmos EMFTEL Department Universidad Complutense de Madrid MadridE-28040 Spain Instituto de Astrofísica de Andalucía-CSIC Glorieta de la Astronomía s/n Granada18008 Spain The Barcelona Institute of Science and Technology Campus UAB Bellaterra Barcelona08193 Spain Max-Planck-Institut für Physik Föhringer Ring 6 München80805 Germany Univ. Savoie Mont Blanc CNRS Laboratoire d’Annecy de Physique des Particules IN2P3 Annecy74000 France Department of Physics Tokai University Japan Institute for Cosmic Ray Research University of Tokyo Japan Departament de Física Quàntica i Astrofísica Institut de Ciències del Cosmos Universitat de Barcelona IEEC-UB Spain EMFTEL department IPARCOS Universidad Complutense de Madrid Spain INAF Osservatorio Astronomico di Roma Italy INFN Sezione di Napoli Italy INFN Sezione di Padova Università degli Studi di Padova Italy Universität Hamburg Institut für Experimentalphysik Germany Graduate School of Science University of Tokyo Japan Universidad del Azuay Ecuador INAF Osservatorio di Astrofisica e Scienza dello spazio di Bologna Italy Centro Brasileiro de Pesquisas Físicas Brazil Instituto de Astrofísica de Canarias Departamento de Astrofísica Universidad de La Laguna Spain CIEMAT Spain Department of Physics TU Dortmund University Germany INFN Sezione di Bari Politecnico di Bari Italy INAF Osservatorio Astronomico di Brera Italy INFN Sezione di Trieste Università degli Studi di Udine Italy University of Geneva Département de physique nucléaire et corpusculaire Switzerland INFN Sezione di Catania Italy Italy Aix Marseille Univ CNRS IN2P3 CPPM France INFN Sezione di Bari Università di Bari Italy INFN Sezione di Torino Italy Palacky University Olomouc Faculty of Science Czech Republic University of Alcalá UAH Spain Port d’Informació Científica Spain University of Rijeka Department of Physics Croatia Institute for Theoretical Physics and Astrophysics Universität W

The next-generation ground-based gamma-ray Cherenkov Telescope Array Observatory (CTAO) will consist of imaging atmospheric Cherenkov telescopes (IACTs) of three different sizes distributed in two sites. The Large-Sized Telescopes will cover the low-energy end of the CTA energy range, starting at about 20 GeV. After its first years of operation at the CTA northern site, the Large-Sized Telescope prototype (LST-1) is in the final stage of its commissioning phase, having collected a significant amount of scientific data to date. In this contribution, we present the physics performance of the telescope using low-zenith Crab Nebula observations and Monte Carlo simulations fine-tuned accordingly. We show performance figures of merit such as the energy threshold, effective area, energy and angular resolution, and sensitivity based on the standard Hillas-parameters approach and following the source-independent and dependent analysis methods. The analysis threshold is estimated at 30 GeV. The energy resolution is around 30%, and the angular resolution is 0.3 degrees at 100 GeV. The best integral sensitivity of LST-1 is about 1.1% of the Crab Nebula flux above 250 GeV for 50 hours of observations. We also show the spectral energy distribution and light curve from Crab Nebula observations, which agree with results from other IACTs and link smoothly with Fermi-LAT when considering statistical and systematic uncertainties near the energy threshold. © Copyright owned by the author(s) under the terms of the Creative Commons.

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