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The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAmoST)

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Research in Astronomy and Astrophysics 2012年第9期12卷 1197-1242页

作者： xiang-Qun Cui Yong-Heng Zhao Yao-Quan Chu Guo-Ping Li Qi Li Li-Ping zhang hong-Jun Su Zheng-Qiu Yao Ya-Nan Wang xiao-Zheng Xing Xin-Nan Li Yong-Tian Zhu Gang Wang Bo-Zhong Gu A-Li Luo Xin-Qi xu Zhen-Chao zhang gen-Rong Liu Hao-Tong zhang De-hua Yang Shu-yun Cao Hai-yuan Chen jian-Jun Chen Kun-Xin Chen ying Chen jia-Ru Chu Lei feng xue-Fei gong Yong-Hui Hou hong-Zhuan Hu Ning-Sheng Hu Zhong-wen Hu Lei jia Fang-hua jiang xiang jiang Zi-Bo jiang ge Jin Ai-hua Li Yan Li Ye-Ping Li Guan-QunLiu Zhi-Gang Liu Huo-Ming Shi Zheng-hong tang Qing-Sheng Tao xiang-Yan yuan Chao Zhai jing zhang Yan-xia zhang Yong zhang Ming Zhao Fang zhou Guo-hua zhou Jie Zhu Si-Cheng Zou National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China yzhao @ *** Nanjing Institute of Astronomical Optics and Technology National Astronomical ObservatoriesChinese Academy of Sciences Nanjing 210042 China University of Science and Tecfinologyof China Hefei 230026 China Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai 200030 China Institute of Architecture Design and Research Chinese Academy of Sciences Beijing 100190China

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAmoST, also called the Guo Shou jing Telescope) is a special reflecting Schmidt telescope. LAmoST’s special design allows both a large aperture (effective aperture of 3.6 m–4.9 m) and a wide field of view (FOV) (5°). It has an innovative active reflecting Schmidt configuration which continuously changes the mirror’s surface that adjusts during the observation process and combines thin deformable mirror active optics with segmented active optics. Its primary mirror (6.67m×6.05 m) and active Schmidt mirror (5.74m×4.40 m) are both segmented, and composed of 37 and 24 hexagonal sub-mirrors respectively. By using a parallel controllable fiber positioning technique, the focal surface of 1.75 m in diameter can accommodate 4000 optical fibers. Also, LAmoST has 16 spectrographs with 32 CCD cameras. LAmoST will be the telescope with the highest rate of spectral acquisition. As a national large scientific project, the LAmoST project was formally proposed in 1996, and approved by the Chinese government in 1997. The construction started in 2001, was completed in 2008 and passed the official acceptance in June 2009. The LAmoST pilot survey was started in October 2011 and the spectroscopic survey will launch in September 2012. Up to now, LAmoST has released more than 480 000 spectra of objects. LAmoST will make an important contribution to the study of the large-scale structure of the Universe, structure and evolution of the Galaxy, and cross-identification of multiwaveband properties in celestial objects.

关键词： techniques: wide field telescope - active optics - multi fiber - spectroscopy survey - data reduction

The first data release(DR1) of the LAmoST regular survey

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Research in Astronomy and Astrophysics 2015年第8期15卷 1095-1124页

作者： A-Li Luo Yong-Heng Zhao Gang Zhao Li-cai Deng xiao-Wei Liu yi-Peng jing Gang Wang Hao-Tong zhang jian-Rong Shi xiang-Qun Cui Yao-Quan Chu Guo-Ping Li Zhong-Rui Bai yue Wu Yan cai Shu-yun Cao Zi-huang Cao Jeffrey L.Carlin Hai-yuan Chen jian-Jun Chen Kun-Xin Chen Li Chen xue-Lei Chen xiao-Yan Chen ying Chen Norbert Christlieb jia-Ru Chu Chen-zhou Cui yi-Qiao Dong Bing Du Dong-Wei Fan Lei feng jian-Ning Fu Peng Gao xue-Fei gong Bo-Zhong Gu Yan-Xin Guo Zhan-wen Han Bo-Liang He Jin-Liang Hou Yong-Hui Hou wen Hou hong-Zhuan Hu Ning-Sheng Hu Zhong-wen Hu Zhi-ying Huo Lei jia Fang-hua jiang xiang jiang Zhi-Bo jiang ge Jin xiao Kong xu Kong Ya-Juan Lei Ai-hua Li chang-hua Li Guang-Wei Li Hai-Ning Li jian Li Qi Li Shuang Li Sha-Sha Li Xin-Nan Li Yan Li yin-Bi Li Ye-Ping Li yuan Liang Chien-Cheng Lin Chao Liu gen-Rong Liu Guan-Qun Liu Zhi-Gang Liu wen-Zhi Lu yu Luo yin-Dun Mao Heidi Newberg Ji-Jun Ni Zhao-xiang Qi Yong-Jun Qi Shi-yin Shen Huo-Ming Shi jing song yi-Han song Ding-Qiang Su hong-Jun Su Zheng-hong tang Qing-Sheng Tao yuan Tian dan Wang da-Qi Wang feng-Fei Wang Guo-Min Wang Hai Wang hong-Chi Wang jian Wang jia-Ning Wang jian-Ling Wang jian-Ping Wang Jun-xian Wang Lei Wang Meng-Xin Wang Shou-Guan Wang Shu-Qing Wang xia Wang Ya-Nan Wang You Wang yue-Fei Wang You-Fen Wang Peng Wei Ming-Zhi Wei hong Wu Ke-Fei Wu xue-Bing Wu yu-Zhong Wu xiao-Zheng Xing Ling-Zhe xu Xin-Qi xu Yan xu Tai-Sheng Yan De-hua Yang Hai-feng Yang Hui-Qin Yang Ming Yang Zheng-Qiu Yao Yong yu Hui yuan Hai-Bo yuan Hai-Long yuan Wei-Min yuan Chao Zhai En-Peng zhang hua-Wei zhang jian-Nan zhang Li-Pin zhang Wei zhang Yong zhang Yan-xia zhang Zheng-Chao zhang Ming Zhao Fang zhou xu zhou Jie Zhu Yong-Tian Zhu Si-Cheng Zou Fang Zuo National Astronomical Observatories Chinese Academy of Sciences Department of Astronomy Peking University Shanghai Astronomical Observatory Chinese Academy of Sciences Nanjing Institute of Astronomical Optics & Technology National Astronomical ObservatoriesChinese Academy of Sciences University of Science and Technology of China Department of Physics Applied Physics and AstronomyRensselaer Polytechnic InstituteTroyNY 12180USA Department of Physics and Astronomy Earlham CollegeRichmondIN 47374USA Universitt Heidelberg Zentrum für AstronomieLandessternwarteKnigstuhl 1269117 HeidelbergGermany Department of Astronomy Beijing Normal University yunnan Observatories Chinese Academy of Sciences Purple mountain Observatory Chinese Academy of Sciences

The Large sky Area Multi-Object Fiber Spectroscopic Telescope（LAmoST） general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs. Objects in both the pilot survey and the first year regular survey are included in the LAmoST DR1. The pilot survey started in October 2011 and ended in June 2012, and the data have been released to the public as the LAmoST Pilot data Release in August 2012. The regular survey started in September 2012, and completed its first year of operation in June 2013. The LAmoST DR1 includes a total of 1202 plates containing 2 955 336 spectra, of which 1 790 879 spectra have observed signalto-noise ratio（SNR） ≥ 10. All data with SNR ≥ 2 are formally released as LAmoST DR1 under the LAmoST data policy. This data release contains a total of 2 204 696 spectra, of which 1 944 329 are stellar spectra, 12 082 are galaxy spectra and 5017 are quasars. The DR1 not only includes spectra, but also three stellar catalogs with measured parameters： late A,FGK-type stars with high quality spectra（1 061 918 entries）, A-type stars（100 073 entries）, and M-type stars（121 522 entries）. This paper introduces the survey design, the observational and instrumental limitations, data reduction and analysis, and some caveats. A description of the FITS structure of spectral files and parameter catalogs is also provided.

关键词： techniques: spectroscopic survey—data release—catalog

data release of the LAmoST pilot survey

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Research in Astronomy and Astrophysics 2012年第9期12卷 1243-1246页

作者： A-Li Luo Hao-Tong zhang Yong-Heng Zhao Gang Zhao xiang-Qun Cui Guo-Ping Li Yao-Quan Chu jian-Rong Shi Gang Wang jian-Nan zhang Zhong-Rui Bai xiao-Yan Chen feng-Fei Wang Yan-Xin Guo jian-Jun Chen Bing Du xiao Kong Ya-Juan Lei yin-Bi Li yi-Han song yue Wu Yan-xia zhang Xin-Lin zhou Fang Zuo Peng Du Lin He wen Hou yi-Qiao Dong jian Li Guang-Wei Li Shuang Li jing song yuan Tian Meng-Xin Wang Yong-Hui Hou Zhi-ying Huo hong-Zhuan Hu Ning-Sheng Hu Zhong-wen Hu Lei jia Fang-hua jiang xiang jiang Zi-Bo jiang ge Jin Ai-hua Li Qi Li yin-Dun Mao Zheng-hong tang Qing-Sheng Tao Liang-Ping Tu da-Qing Wang dan Wang jian-Ping Wang Lei Wang Shou-Guan Wang Shu-Qing Wang Ya-Nan Wang You Wang yue-Fei Wang Ming-Zhi Wei xiang-xiang xue xiao-Zheng Xing Ling-Zhe xu Xin-Qi xu Yan xu De-hua Yang Shi-Hai Yang Zheng-Qiu Yao Yong yu Hui yuan Chao Zhai En-Peng zhang jing zhang Li-Ping zhang Weizhang Yong zhang Zhen-Chao zhang Ming Zhao Fang zhou Yong-Tian Zhu Jie Zhu Si-Cheng Zou National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China lal @ lamost o rg Nanjing Institute of Astronomical Optics and Technology National Astronomical ObservatoriesChinese Academy of Sciences Nanjing 210042 China University of Science and Technologyof China Hefei 230026 China Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai 200030 China Institute of Architecture Design and Research Chinese Academy of Sciences Beijing 100190China

This paper describes the data release of the LAmoST pilot survey, which includes data reduction, calibration, spectral analysis, data products and data access. The accuracy of the released data and the information about the FITS headers of spectra are also introduced. The released data set includes 319 000 spectra and a catalog of these objects.

关键词： techniques: spectroscopic survey — data reduction — data release

细胞培养法检测和分离狂犬病街毒的可行性研究

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中华流行病学杂志 2009年第6期30卷 611-615页

作者：汪霞徐葛林吴杰罗静朱家鸿周剑军施南峰唐青张永振唐建蓉吴泰才明贺田沈蕊华陈焕春武汉生物制品研究所 430060 浙江省慈溪市疾病预防控制中心中国疾病预防控制中心病毒病预防控制所传染病预防控制所中国药品生物制品检定所广西壮族自治区疾病预防控制中心安徽省阜阳市疾病预防控制中心上海市疾病预防控制中心华中农业大学兽医学院

目的研究MNA细胞培养法检测和分离狂犬病街毒的可行性。方法用MNA细胞培养法、荧光抗体实验（FAT）和双抗体夹心ELISA方法分别检测33份狂犬病街毒样品、20份狂犬病毒阴性犬脑样品和4份正常鼠脑样品。结果MNA细胞培养法检测57份待检样品... 详细信息

目的研究MNA细胞培养法检测和分离狂犬病街毒的可行性。方法用MNA细胞培养法、荧光抗体实验（FAT）和双抗体夹心ELISA方法分别检测33份狂犬病街毒样品、20份狂犬病毒阴性犬脑样品和4份正常鼠脑样品。结果MNA细胞培养法检测57份待检样品，培养48h的实验结果显示，33份狂犬病街毒样品均为阳性，狂犬病毒阴性犬脑样品和正常鼠脑样品均为阴性，与FAT、双抗体夹心ELISA方法的检测结果完全一致。结论MNA细胞培养法对样品中狂犬病街毒的检测具有较高的灵敏度和特异性，可用于狂犬病街毒的检测和分离。

关键词：狂犬病街毒细胞培养法检测

CEPC Technical Design Report

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Radiation Detection Technology and Methods 2024年第1期8卷 I0003-I0016,1-1091页

作者： Waleed Abdallah Tiago Carlos Adorno de Freitas Konstantin Afanaciev Shakeel Ahmad Ijaz Ahmed xiaocong Ai Abid Aleem Wolfgang Altmannshofer Fabio Alves Weiming An Rui An daniele Paolo Anderle Stefan Antusch Yasuo Arai Andrej Arbuzov Abdesslam Arhrib Mustafa Ashry Sha Bai yu Bai Yang Bai Vipul Bairathi Csaba Balazs Philip Bambade Yong Ban Tripamo Bandyopadhyay Shou-Shan Bao Desmond P.Barber Ayse Bat Varvara Batozskaya Subash Chandra Behera Alexander Belyaev Michele Bertucci xiao-Jun Bi yuanjie Bi Tianjian Bian Fabrizio Bianchi Thomas Biekotter Michela Biglietti Shalva Bilanishvili Deng Binglin Denis Bodrov Anton Bogomyagkov Serge Bondarenko Stewart Boogert Maarten Boonekamp Marcello Borri Angelo Bosotti Vincent Boudry mohammed Boukidi Igor Boyko Ivanka Bozovic Giuseppe Bozzi Jean-Claude Brient Anastasiia Budzinskaya Masroor Bukhari Vladimir Bytev Giacomo Cacciapaglia hua cai wenyong cai Wujun cai yijian cai yizhou cai yuchen cai Haiying cai huacheng cai Lorenzo Calibbi Junsong Cang Guofu Cao jianshe Cao Antoine Chance xuejun chang yue chang Zhe chang Xinyuan chang Wei Chao Auttakit Chatrabhuti yimin Che yuzhi Che Bin Chen danping Chen Fuqing Chen Fusan Chen Gang Chen Guoming Chen hua-Xing Chen Huirun Chen Jinhui Chen Ji-yuan Chen Kai Chen Mali Chen Mingjun Chen Mingshui Chen Ning Chen Shanhong Chen Shanzhen Chen Shao-Long Chen Shaomin Chen Shiqiang Chen Tianlu Chen Wei Chen xiang Chen xiaoyu Chen Xin Chen xun Chen xurong Chen Ye Chen ying Chen yukai Chen Zelin Chen Zilin Chen Gang Chen Boping Chen Chunhui Chen Hok Chuen Cheng huajie Cheng Shan Cheng Tongguang Cheng yunlong Chi Pietro Chimenti wen Han Chiu Guk Cho Ming-Chung Chu xiaotong Chu Ziliang Chu Guglielmo Coloretti Andreas Crivellin Hanhua Cui xiaohao Cui Zhaoyuan Cui Brunella D'Anzi Ling-yun dai Xinchen dai xuwen dai Antonio De Maria Nicola De Filippis Christophe De La Taille Francesca De mori Chiara De Sio Elisa Del Core Shuangxue Deng Wei-Tian Deng Zhi Deng Ziyan Deng Bhupal Dev tang Dewen Biagio Di Micco Ran Ding Siqin Dingl Yadong Ding Haiyi Dong jianin AGH University of Science and Technology Faculty of Physics and Applied Computer ScienceKrakow Anhui University HefeiAnhui Applied Physics Department Federal Urdu University of ArtsScience and TechnologyIslamabad Banaras Hindu University Institute of ScienceVaranasi Bandirma Onyedi Eylul University Bandirma Beihang University Beijing Beijing Computational Science Research Center Beijing Beijing Conveyi LTD Beijing Beijing Glass Research Institute Co. LtdBeijing Beijing Institute of Technology Beijing Beijing Normal University Beijing Brown University ProvidenceRI Budker Institute of Nuclear Physics Novosibirsk Cadi Ayyad University Laboratory of Fundamental and Applied PhysicsPolydisciplinary FacultyMarrakech cairo University Giza Center for Theory and Computation National Tsing Hua UniversityHsinchu Central China Normal University WuhanHubei Central South University ChangshaHunan Centro de Fisica Teorica de Particulas Universidade Tecnica de LisboaLisboa Chengdu KaitengSifang Digital Radio&TV Equipment Co. LtdChengduSichuan China academy of engineering physics MianyangSichuan China building materials academy Beijing China Center of Advanced Science and Technology Beijing China Institute of Atomic Energy Beijing China Jiliang University HangzhouZhejiang China Nuclear Instrument CO. LTDBeijing China University of geosciences Beijing China University of geosciences WuhanHubei China University of Mining and Technology XuzhouJiangsu China West Normal University NanchongSichuan Chongqing University Department of PhysicsChongqing Chulalongkorn University Bangkok City University of hong Kong Department of PhysicsHong Kong Cockcroft Institute Daresbury Cornell University IthacaNY CPPM(AMU/IPhU&CNRS/INP) Marseille dalian Minzu University DalianLiaoning dalian University of Technology Department of PhysicsDalian Deutsches Elektronen-Synchrotron DESY Hamburg Dzhelepov Laboratory of Nuclear Problems of Joint Institute for Nuclear Research(DLNP JINR) Dubna East China University Of Science And Technol

The Circular Electron Positron Collider(CEPC)is a large scientific project initiated and hosted by China,fostered through extensive collaboration with international *** complex comprises four accelerators:a 30 geV Linac,a 1.1 geV damping Ring,a Booster capable of achieving energies up to 180 geV,and a Collider operating at varying energy modes(Z,W,H,and tt).The Linac and damping Ring are situated on the surface,while the subterranean Booster and Collider are housed in a 100 km circumference underground tunnel,strategically accommodating future expansion with provisions for a potential Super Proton Proton Collider(SPPC).The CEPC primarily serves as a Higgs *** its baseline design with synchrotron radiation(SR)power of 30 MW per beam,it can achieve a luminosity of 5×10^(34)cm^(-2)s^(-1)per interaction point(IP),resulting in an integrated luminosity of 13 ab^(-1)for two IPs over a decade,producing 2.6 million Higgs *** the SR power to 50 MW per beam expands the CEPC's capability to generate 4.3 million Higgs bosons,facilitating precise measurements of Higgs coupling at sub-percent levels,exceeding the precision expected from the HL-LHC by an order of *** Technical Design Report(TDR)follows the Preliminary Conceptual Design Report(Pre-CDR,2015)and the Conceptual Design Report(CDR,2018),comprehensively detailing the machine's layout,performance metrics,physical design and analysis,technical systems design,R&D and prototyping efforts,and associated civil engineering ***,it includes a cost estimate and a preliminary construction timeline,establishing a framework for forthcoming engineering design phase and site selection *** is anticipated to begin around 2027-2028,pending government approval,with an estimated duration of 8 *** commencement of experiments and data collection could potentially be initiated in the mid-2030s.

关键词： initiated exceeding precise

Feasibility and physics potential of detecting ^(8)B solar neutrinos at JUNO

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Chinese Physics C 2021年第2期45卷 93-110页

作者： Angel Abusleme Thomas Adam Shakeel Ahmad Sebastiano Aiello Muhammad Akram Nawab Ali fengpeng An Guangpeng An Qi An Giuseppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Auguste Andrej Babic Wander Baldini Andrea Barresi Eric Baussan Marco Bellato Antonio Bergnoli Enrico Bernieri david Biare Thilo Birkenfeld Sylvie Blin david Blum Simon Blyth Anastasia Bolshakova Mathieu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Max Buesken Mario Buscemi Jose Busto Ilya Butorov Anatael Cabrera Hao cai xiao cai Yanke cai Zhiyan cai Antonio Cammi Agustin Campeny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Jinfan chang yun chang Pingping Chen Po-An Chen Shaomin Chen Shenjian Chen xurong Chen yi-wen Chen yixue Chen yu Chen zhang Chen Jie Cheng Yaping Cheng Alexander Chepurnov davide Chiesa Pietro Chimenti Artem Chukanov Anna Chuvashova Gérard Claverie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo daniele Corti Salvatore Costa Flavio dal Corso Christophe De La Taille jiawei Deng Zhi Deng Ziyan Deng Wilfried Depnering Marco Diaz xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal georgy Donchenko jianmeng Dong damien Dornic Evgeny Doroshkevich Marcos Dracos Frédéric Druillole Shuxian Du Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea Fabbri Lukas Fajt Donghua Fan Lei Fan Can Fang jian Fang Marco Fargetta Anna Fatkina Dmitry Fedoseev Vladko Fekete Li-Cheng feng Qichun feng Richard Ford Andrey Formozov Amélie Fournier Haonan Gan feng Gao Alberto Garfagnini Alexandre Göttel Christoph genster Marco Giammarchi Agnese Giaz Nunzio Giudice Franco Giuliani Maxim Gonchar Guanghua gong Hui gong Oleg Gorchakov yuri Gornushkin Marco Grassi Christian Grewing Maxim Gromov Vasily Gromov Minghao Gu xiaofei Gu yu Gu Mengyun Guan Nunzio Guardone Maria Gul Cong Guo jingyuan Guo Wanlei Guo Xinheng Guo yuhang Guo Paul Hackspacher Caren Hagner Ran Han Yan Yerevan Physics Institute YerevanArmenia UniversitéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontificia Universidade Catolica do Rio de Janeiro RioBrazil Pontificia Universidad Católica de Chile SantiagoChile Universidad Tecnica Federico Santa Maria ValparaisoChile Beijing Institute of Spacecraft Environment Engineering BeijingChina Beijing Normal University BeijingChina China Institute of Atomic Energy BeijingChina Institute of High Energy Physics BeijingChina North China Electric Power University BeijingChina School of Physics Peking UniversityBeijingChina Tsinghua University BeijingChina University of Chinese Academy of Sciences BeijingChina Jilin University ChangchunChina College of Electronic Science and Engineering National University of Defense TechnologyChangshaChina Chongqing University ChongqingChina Dongguan University of Technology DongguanChina Jinan University GuangzhouChina Sun Yat-Sen University GuangzhouChina Harbin Institute of Technology HarbinChina University of Science and Technology of China HefeiChina The Radiochemistry and Nuclear Chemistry Group in University of South China HengyangChina Wuyi University JiangmenChina Shandong University JinanChina Institute of modern Physics Chinese Academy of SciencesLanzhouChina Nanjing University NanjingChina Guangxi University NanningChina East China University of Science and Technology ShanghaiChina School of Physics and Astronomy Shanghai Jiao Tong UniversityShanghaiChina Tsung-dao Lee Institute Shanghai Jiao Tong UniversityShanghaiChina Institute of Hydrogeology and Environmental geology Chinese Academy of Geological SciencesShijiazhuangChina Nankai University TianjinChina Wuhan University WuhanChina Xi’an jiaotong University Xi’anChina xiamen University XiamenChina School of Physics and Microelectronics Zhengzhou UniversityZhengzhouChina Institute of Physics National Chiao-Tung University Hsinchu National United University Miao-Li Department of Physics National T

The jiangmen Underground Neutrino Observatory(JUNO)features a 20 kt multi-purpose underground liquid scintillator sphere as its main *** of JUNO's features make it an excellent location for^8B solar neutrino measurements,such as its low-energy threshold,high energy resolution compared with water Cherenkov detectors,and much larger target mass compared with previous liquid scintillator *** this paper,we present a comprehensive assessment of JUNO's potential for detecting^8B solar neutrinos via the neutrino-electron elastic scattering process.A reduced 2 MeV threshold for the recoil electron energy is found to be achievable,assuming that the intrinsic radioactive background^(238)U and^(232)Th in the liquid scintillator can be controlled to 10^(-17)g/*** ten years of data acquisition,approximately 60,000 signal and 30,000 background events are *** large sample will enable an examination of the distortion of the recoil electron spectrum that is dominated by the neutrino flavor transformation in the dense solar matter,which will shed new light on the inconsistency between the measured electron spectra and the predictions of the standard three-flavor neutrino oscillation *** m^(2)_(21)=4.8times10^(-5);(7.5times10^(-5))eV^(2),JUNO can provide evidence of neutrino oscillation in the Earth at approximately the 3sigma(2sigma)level by measuring the non-zero signal rate variation with respect to the solar zenith ***,JUNO can simultaneously measureDelta m^2_(21)using^8B solar neutrinos to a precision of 20% or better,depending on the central value,and to sub-percent precision using reactor antineutrinos.A comparison of these two measurements from the same detector will help understand the current mild inconsistency between the value of Delta m^2_(21)reported by solar neutrino experiments and the KamLAND experiment.

关键词： neutrino oscillation solar neutrino JUNO

老年人新型冠状病毒感染小分子抗病毒药物治疗建议

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中国药理学通报 2023年第3期39卷 425-430页

作者：潘敏张田婧常双冯晓霞魏伟李俊赵红梅费广鹤李家斌陈飞虎戴敏孟晓明王华项轶曹孟淑陈晓阳叶贤伟许杜娟胡晓文姜玲王昌会汪永忠刘浩谢海棠方平钱震东唐超杨刚腾小宝钱朝霞丁国正孙艳范晓云张玲玲安徽医科大学第一附属医院安徽合肥230022 安徽医科大学临床药理研究所安徽合肥230032 安徽医科大学药学院安徽合肥230032 北京中日友好医院北京100029 安徽中医药大学安徽合肥230012 上海交通大学附属瑞金医院上海200025 南京鼓楼医院江苏南京210008 福建医科大学附属第二医院福建泉州362000 贵州省人民医院贵州贵阳550025 中国科学技术大学附属第一医院安徽合肥230001 安徽中医药大学第一附属医院安徽合肥230012 蚌埠医学院药学院安徽蚌埠233000 皖南医学院弋矶山医院安徽芜湖241001 铜陵市人民医院安徽铜陵244099 铜陵市立医院安徽铜陵244000 亳州市中医院安徽亳州236800 芜湖市第二人民医院安徽芜湖241000 阜阳市第二人民医院安徽阜阳236015 蚌埠市第三人民医院安徽蚌埠233000 安庆市立医院安徽安庆246004

新型冠状病毒感染已流行三年之久,虽然病毒的不断变异使得其致病力减弱,但伴有基础病的老年患者仍是新冠病毒重症感染的高危人群。随着对新冠病毒分子结构和致病机制的不断认识,抗新冠病毒药物相继上市,这些药物可以有效降低老年患者的... 详细信息

新型冠状病毒感染已流行三年之久,虽然病毒的不断变异使得其致病力减弱,但伴有基础病的老年患者仍是新冠病毒重症感染的高危人群。随着对新冠病毒分子结构和致病机制的不断认识,抗新冠病毒药物相继上市,这些药物可以有效降低老年患者的重症率及死亡率。该文就目前我国附条件批准上市的5种小分子抗病毒药物的作用机制、临床用药、药物相互作用、不良反应等多方面进行阐述,为老年人抗新冠病毒治疗的临床合理用药提供参考建议。

关键词：老年人新型冠状病毒感染抗病毒药物临床合理用药药物相互作用治疗建议

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Ⅲ期非小细胞肺癌的处理:共识与争鸣

循证医学 2022年第3期22卷 129-136页

作者：吴一龙陆舜周清华张力程颖王洁汪步海胡成平林丽珠钟文昭宋勇杨农董晓荣赵健杨海虹郭卉闫小龙刘宏旭马锐林劼刘思旸陈椿王立峰周承志周明吴芳杨学宁杜瀛瀛姚煜邵阳洪少东崔久嵬全雪萍陈蓉蓉吴佳妍张嘉涛周建娅汪斌超程超王慧娟柳菁菁邬麟黄岩匡煜坤张永昌胡洁杨衿记冯卫能苏文媚范云杨帆陈明唐可京潘燚申鹏刘安文张海波梁文华周清马智勇蔡修宇刘慧陈龙飞揣少坤单建贞郑燕芳尤长宣朱晓霞李力张同梅涂海燕林武荣张绪超周鹏辉柯尊富梁会营中国抗癌协会肺癌专业委员会广东省临床试验协会/中国胸部肿瘤研究协作组广东省人民医院、广东省医学科学院、广东省肺癌研究所广州510080 上海交通大学附属胸科医院上海200030 四川大学华西医院成都610041 中山大学肿瘤防治中心广州510060 吉林省肿瘤医院长春130021 中国医学科学院肿瘤医院北京100021 南京大学医学院附属苏北人民医院江苏扬州225001 中南大学湘雅医院长沙410008 广州中医药大学第一附属医院广州510405 东部战区总医院南京210002 湖南省肿瘤医院长沙410013 华中科技大学同济医学院附属协和医院武汉430022 广州医科大学附属肿瘤医院广州510095 广州医科大学附属第一医院广州510120 西安交通大学第一附属医院西安710061 空军军医大学唐都医院西安710038 辽宁省肿瘤医院沈阳110042 昆明医科大学第二附属医院昆明650101 福建医科大学附属协和医院福州350014 南京大学医学院附属鼓楼医院南京210008 中南大学湘雅二医院长沙410011 安徽医科大学第一附属医院合肥230022 南京世和基因生物技术股份有限公司南京210032 吉林大学白求恩第一医院长春130021 上海桐树生物科技有限公司上海200444 北京吉因加科技有限公司北京102206 福建和瑞基因科技有限公司福州350207 浙江大学医学院附属第一医院杭州310031 中山大学附属第一医院广州510080 郑州大学附属肿瘤医院/河南省肿瘤医院郑州450003 复旦大学附属中山医院上海200032 佛山市第一人民医院广东佛山528000 广东医科大学附属医院广东湛江524000 中国科学院大学附属肿瘤医院/浙江省肿瘤医院杭州310022 北京大学人民医院北京100044 南方医科大学南方医院广州510515 南昌大学附属第二医院南昌330006 广东省中医院广州510120 广州燃石医学检验有限公司广州510300 南方医科大学珠江医院广州510280 陆军军医大学大坪医院重庆400042 首都医科大学附属北京胸科医院北京101149 至本医疗科技(上海)有限公司上海201114 不详

由中国抗癌协会肺癌专业委员会和广东省临床试验协会/中国胸部肿瘤研究协作组主办的“第19届中国肺癌高峰论坛”于2022年3月5日在广州顺利召开。此次论坛中,来自肺癌临床研究、转化性研究、基础研究的专家们围绕可切除/不可切除Ⅲ期非... 详细信息

由中国抗癌协会肺癌专业委员会和广东省临床试验协会/中国胸部肿瘤研究协作组主办的“第19届中国肺癌高峰论坛”于2022年3月5日在广州顺利召开。此次论坛中,来自肺癌临床研究、转化性研究、基础研究的专家们围绕可切除/不可切除Ⅲ期非小细胞肺癌(non-small cell lung cancer,NSCLC)的多学科综合治疗和生物标志物进行了深入交流和讨论,并最终达成了专家共识。

关键词： Ⅲ期非小细胞肺癌多学科综合治疗共识

严重创伤患者紧急救治血液保障模式与输血策略中国专家共识(2024版)

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中华创伤杂志 2024年第10期40卷 865-881页

作者：卢尧李阳张雷英唐昊敬慧丹王耀丽贾向志巴立卞茂红蔡丹蔡辉蔡晓红查占山陈秉宇陈大庆陈凤陈国安陈海鸣陈静陈敏陈青陈舒陈玺程金凤褚晓凌崔红旺崔欣达珍戴莹邓素容董伟群范为民冯珂付丹晖付涌水傅奇傅雪梅甘佳甘新宇高伟巩怀证桂嵘郭庚韩宁郝一文何武兵洪强侯瑞琴侯卫胡婕胡培阳胡熙胡晓玉黄光斌黄婕黄象艳黄远帅浑守永蒋学兵金平赖冬乐爱平黎红梅李碧娟李翠莹李代红李海宏李贺李辉李剑平李宁李喜莹李湘民李小飞李晓娟李志强李忠俊李尊严梁华钦梁晓华廖冬发廖群廖燕林甲进刘春霞刘凤华刘培贤刘铁梅刘小信刘志伟刘中砥陆华栾建凤骆建军骆群吕定丰吕琪吕先萍马爱军马立强马曙轩马现君马小刚马晓莉毛国庆穆士杰聂少林欧阳淑娟欧阳锡林潘春球潘健潘晓华彭磊彭涛钱宝华乔姝秦莉任颖任召祺戎瑞明苏常山孙明伟孙文武孙振威唐海平唐晓峰唐长玖陶翠华田志彬汪娟王宝燕王春燕王革非王海燕王鸿捷王鹏王鹏里王秋实王晓宁王新华王学锋王勇王勇军王远杰王志华韦少俊魏亚明文键波文军吴江吴巨峰夏爱军夏飞夏荣谢珏邢颜超熊雁徐峰徐永柱许永安晏永和燕备战杨江杨江存杨军杨新文杨勇毅姚春艳叶明亮尹昌林尹明尹文于连玲于淑红余泽波郁毅刚喻安永袁红袁燚张婵张进军张军张凯张磊冰张泉张荣江张三明张生吉张硕张伟张伟东张晰张兴文章桂喜章晓军赵国庆赵建鹏赵树铭郑蓓蓓郑山根周华友周吉成周砺宏周谋周小玉周雪莲周源周政周祖皇朱海燕朱培元朱长举祝丽丽王正国蒋建新汪德清兰炯采王全立于洋张连阳文爱清中华医学会临床输血学分会中华医学会创伤学分会创伤急救与多发伤学组中华医学会灾难医学分会青年学组陆军军医大学陆军特色医学中心重庆400042 陆军军医大学陆军特色医学中心创伤与化学中毒全国重点实验室重庆400042 中国人民解放军总医院第一医学中心北京100853 军事医学研究院卫生勤务与血液研究所北京100850 浙江大学医学院附属第二医院杭州310009 安徽医科大学第一附属医院合肥230022 湘潭市中心医院湘潭411100 中国医学科学院北京协和医学院输血研究所成都610052 上海交通大学医学院附属瑞金医院上海200025 海军军医大学第一附属医院上海200433 浙江省人民医院杭州310014 温州医科大学附属第二医院温州325027 内蒙古自治区人民医院呼和浩特010017 武汉市血液中心武汉430030 南昌大学第一附属医院南昌330006 河北医科大学第三医院石家庄050051 乌鲁木齐市血液中心乌鲁木齐830000 南京大学医学院附属鼓楼医院南京210008 浙江省血液中心杭州310052 重庆两江新区人民医院重庆401121 株洲市中心医院株洲412000 福建省疾病预防控制中心福州350012 海南医学院第一附属医院海口570102 贵州省血液中心贵阳550001 西藏自治区血液中心拉萨850000 中国人民解放军联勤保障部队第九二〇医院昆明650000 重庆医科大学附属永川医院重庆402160 昆明医科大学第一附属医院昆明650032 江西省血液中心南昌330052 宁夏医科大学总医院银川750001 福建医科大学附属协和医院福州350001 广州市第一人民医院广州510080 重庆市血液中心重庆400015 成都市血液中心成都610042 中国医学科学院北京协和医院北京100730 中国人民解放军西部战区总医院成都610083 华中科技大学同济医学院附属同济医院武汉430030 山东省血液中心济南250014 中南大学湘雅三医院长沙410013 山西医科大学第一医院太原030001 上海同济大学附属东方医院上海200120 中国医科大学附属第一医院沈阳110001 福建省立医院福州350001 厦门大学附属第一医院厦门361003 北京大学人民医院北京100044 青海省血液中心西宁810007 浙江省天台县人民医院天台317200 昆明市儿童医院昆明650228 安徽省血液中心合肥230031 重庆大学附属中心医院重庆市急救医疗中心重庆400014 湖南省人民医院(湖南师范大学附属第一医院) 长沙410001 中国人民解放军联勤保障部队第九六〇医院济南250031 西南医科大学附属医院泸州646000 山东第一医科大学附属省立医院济南250021 中国人民解放军总医院第六医学中心北京100048 余姚市人民医院余姚315400 厦门医学院附属第二医院厦门361005 重庆市垫江县人民医院重庆408300 中南大学湘雅医院长沙410008 空军军医大学空军特色医学中心北京100142 天津市第一中心医院天津300192 山西省中西医结合医院太原030013 安徽医科大学第二附属医院合肥230601 辽宁省血液中心沈阳110044 中国医学科学院肿瘤医院北京100021 首都医科大学附属北京友谊医院北京100050 兰州大学第二医院兰州730030 上海市第六人民医院上海201599 陆军军医大学第二附属医院重庆400037 北华大学附属医院吉林132000 广州血液中心广州510095 大连市血液中心大连116001 广西医科大学第三附属医院南宁530007 兰州大学第一医院兰州730030 哈尔滨医科大学附属第一医院哈尔滨150010 山西医科大学第二医院太原030000 吉林大学中日联谊医院长春130062 山东第一医科大学第一附属医院(山东省千佛山医院) 济南250013 浙江大学医学院附属邵逸夫医院杭州310016 重庆医科大学附属第二医院重庆400010 中国人民解放军东部战区总医院南京210002 中国人民解放军联勤保障部队第九〇三医院杭州310013 中国人民解放军总医院第五医学中心北京100071 宁波大学附属第一医院宁波315010 天津大学应急医学研究院天津300072 郑州大学第一附属医院郑州450052 河北省血液中心石家庄050004 中国人民解放军联勤保障部队第九〇〇医院福州350025 首都医科大学附属北京儿童医院北京100045 山东大学齐鲁医院济南250012 西藏自治区人民医院拉萨850000 河南省红十字血液中心郑州450012 荆州市中心血站荆州434099 空军军医大学第二附属医院西安710038 株洲市中心血站株洲412007 湖南省肿瘤医院/中南大学湘雅医

严重创伤患者对救治时效性要求极高,输血在此类患者的紧急救治阶段发挥着不可替代的作用。越来越多的循证医学证据和临床经验表明,早期输注低效价O型全血或平衡比例红细胞、血浆和血小板等成分血的止血复苏策略将使严重创伤大出血患者... 详细信息

严重创伤患者对救治时效性要求极高,输血在此类患者的紧急救治阶段发挥着不可替代的作用。越来越多的循证医学证据和临床经验表明,早期输注低效价O型全血或平衡比例红细胞、血浆和血小板等成分血的止血复苏策略将使严重创伤大出血患者获益。然而,当前国内血液保障模式不能完全满足临床对严重创伤患者紧急救治输血的时效性和有效性需求。针对我国严重创伤紧急救治血液保障模式与输血策略中存在的关键问题,中华医学会临床输血学分会、中华医学会创伤学分会创伤急救与多发伤学组和中华医学会灾难医学分会青年学组组织国内输血医学和创伤救治专家,基于循证医学证据并结合Delphi法专家咨询投票,共同制订《严重创伤患者紧急救治血液保障模式与输血策略中国专家共识(2024版)》,从血液保障模式和输血策略两个方面共提出10条推荐意见,为严重创伤紧急救治阶段的输血复苏提供参考,以期进一步提高严重创伤患者的救治成功率。

关键词：创伤和损伤急救输血专家共识