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肺切除术后肺部并发症发生的危险因素分析

中国胸心血管外科临床杂志 2010年第4期17卷 301-306页

作者：王邵华阮征郑健黄海龙宋康声上海交通大学附属第一人民医院胸外科上海200080

目的分析肺切除术后肺部并发症(PPC)发生的危险因素,尽可能减少术后PPC的发生,降低病死率。方法回顾性分析2007年1月至2009年12月在我科行肺切除术302例患者的临床资料,其中男228例,女74例;年龄23～91岁,平均年龄63.38岁。统计术后各种... 详细信息

目的分析肺切除术后肺部并发症(PPC)发生的危险因素,尽可能减少术后PPC的发生,降低病死率。方法回顾性分析2007年1月至2009年12月在我科行肺切除术302例患者的临床资料,其中男228例,女74例;年龄23～91岁,平均年龄63.38岁。统计术后各种肺部并发症的发生率,并收集术前、术中及术后相关资料和数据,采用logistic多元回归分析肺切除术后PPC发生的独立危险因素。结果围术期共死亡22例(7.28%),75例(24.83%)发生110例次PPC,最主要的PPC为胸膜腔持续漏气/支气管胸膜瘘(8.94%,27/302),院内肺炎(6.95%,21/302)和急性呼吸衰竭(6.29%,19/302)。logistic多因素分析结果显示:ASA分级≥3级(OR=2.400,P=0.020)、术后即刻气管内插管机械通气时间延长(OR=1.620,P=0.030)是肺切除术后发生PPC的独立危险因子。结论以患者一般情况和各器官功能状态为基础的ASA分级和术后机械通气时间是肺切除术后PPC的独立预测因子。对高危患者需特别注意完善术前准备,改善患者各器官功能状况,保护肺功能,术后尽量缩短机械通气时间,尽可能减少PPC的发生。

关键词：肺切除术肺部并发症危险因素

食管壁内夹层的诊断与治疗——附一例报告及文献复习

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中国胸心血管外科临床杂志 2011年第5期18卷 417-421页

作者：王邵华刘法兵阮征黄海龙郑健居潮强宋康声上海交通大学附属第一人民医院胸外科上海200080

目的探讨食管壁内夹层(intramural esophageal dissection,IED)的可能发病机制、临床表现、诊断方法和治疗预后,以提高IED的诊疗水平。方法回顾性分析2010年2月上海交通大学附属第一人民医院收治的1例全胸段食管环状壁内夹层、假腔严重... 详细信息

目的探讨食管壁内夹层(intramural esophageal dissection,IED)的可能发病机制、临床表现、诊断方法和治疗预后,以提高IED的诊疗水平。方法回顾性分析2010年2月上海交通大学附属第一人民医院收治的1例全胸段食管环状壁内夹层、假腔严重感染合并局限性食管破裂患者的临床资料,女,56岁。行右侧开胸探查,经第5肋间后外侧切口进胸,切除病变食管,游离胃后经胸骨后路径上提至左颈部与颈段健康食管吻合。使用PubMed检索系统,检索关键词为intramural esophageal dissection或intramural esophageal hematoma,复习2000～2010国外所发表的临床资料完整的个案报道。结果本例患者行全胸段病变食管切除后治愈,术后14d出院;已随访6个月,一般情况好。复习临床资料完整的个案13例,主要临床表现为胸背痛、吞咽疼痛和吞咽困难,偶有呕血;诊断主要依靠内镜和食管X线钡餐造影检查。12例行保守治疗、内镜下治疗或手术切除病变食管治愈或缓解;1例行手术探查后死亡。结论 IED是一种罕见的疾病,诊断主要依靠食管X线造影、内镜和CT扫描。IED为良性病变,可予保守治疗或内镜下治疗。对部分病情严重的患者,手术切除病变食管更加安全可靠。

关键词：食管壁内夹层食管破裂食管切除术

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食管雪旺细胞瘤的诊断与治疗

同济大学学报（医学版） 2011年第4期32卷 91-95页

作者：王邵华阮征郑健黄海龙宋康声居潮强上海交通大学医学院附属第一人民医院胸外科上海200085

目的探讨食管雪旺细胞瘤的临床表现、诊断及预后,以提高食管恶性雪旺细胞瘤的诊疗水平。方法回顾性分析我院1例恶性食管恶性雪旺细胞瘤患者的临床资料。使用PubMed检索系统,检索关键词为esophageal schwannoma或nerve sheath tumor,复... 详细信息

目的探讨食管雪旺细胞瘤的临床表现、诊断及预后,以提高食管恶性雪旺细胞瘤的诊疗水平。方法回顾性分析我院1例恶性食管恶性雪旺细胞瘤患者的临床资料。使用PubMed检索系统,检索关键词为esophageal schwannoma或nerve sheath tumor,复习英语发表的临床资料完整的个案报道。结果患者为恶性食管雪旺细胞瘤(核分裂相6个/每50个高倍视野),经肿块剜除术后随访6年无复发。复习临床资料完整的雪旺细胞瘤25例,其中恶性者4例。根据病灶切除后组织学诊断,临床表现主要是吞咽困难(64.0%)。食管良性和恶性雪旺细胞瘤的年龄、性别、生长方式、生长部位、病变长度、临床表现和手术方式差异均无统计学意义(P>0.05)。病灶剜除术是主要的手术方式。随访中仅1例良性食管雪旺细胞瘤复发;恶性雪旺细胞瘤最长随访72个月无复发。结论食管黏膜下肿瘤的鉴别诊断中需考虑雪旺细胞瘤的可能,食管雪旺细胞瘤的诊断依赖于病理检查。对部分有选择的恶性雪旺细胞瘤患者,外科手术病灶剜除不失为替代食管切除的手术方式选择。

关键词：食管手术病理食管肉瘤

Timing analysis of the black hole candidate EXO 1846–031 with Insight-HXMT monitoring

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Research in Astronomy and Astrophysics 2021年第3期21卷 193-204页

作者： He-Xin liu Yue huang Guang-Cheng Xiao Qing-Cui Bu Jin-Lu Qu Shu Zhang Shuang-Nan Zhang Shu-Mei Jia fang-Jun Lu Xiang Ma Lian Tao Wei Zhang Li Chen Li-Ming song Ti-Pei Li Yu-Peng Xu Xue-Lei Cao Yong Chen Cong-Zhan liu Ce Cai Zhi Chang Gang Chen Tian-Xiang Chen Yi-Bao Chen Yu-Peng Chen Wei Cui Wei-Wei Cui Jing-kang Deng Yong-Wei Dong Yuan-Yuan Du Min-Xue Fu Guan-hua Gao He Gao Min Gao Ming-Yu Ge Yu-Dong Gu Ju Guan Cheng-Cheng Guo Da-Wei Han Jia Huo Lu-hua jiang Wei-Chun jiang Jing Jin Yong-Jie Jin Ling-Da Kong bing Li Cheng-Kui Li Gang Li Mao-Shun Li Wei Li Xian Li Xiao-Bo Li Xu-fang Li Yang-Guo Li zheng-Wei Li Xiao-hua Liang Jing-Yuan Liao Bai-sheng liu Guo-Qing liu Hong-Wei liu Xiao-Jing liu Yi-Nong liu Bo Lu Xue-Feng Lu Qi Luo Tao Luo Bin Meng Yi Nang jian-Yin Nie Ge Ou Na Sai Ren-Cheng Shang Xin-Ying song Liang Sun Ying Tan You-Li Tuo Chen wang Guo-Feng wang Juan wang Ling-Jun wang Weng-Shuai wang Yu-Sa wang Xiang-Yang Wen Bai-Yang Wu Bo-bing Wu Mei Wu Shuo Xiao shao-Lin Xiong He Xu Jia-Wei Yang sheng Yang Yan-Ji Yang Yi-Jung Yang Qi-Bin Yi Qian-Qing Yin Yuan You Ai-Mei Zhang Cheng-Mo Zhang fan Zhang Hong-Mei Zhang Juan Zhang Tong Zhang Wan-Chang Zhang Wen-Zhao Zhang Yi Zhang Yi-Fei Zhang Yong-Jie Zhang Yuan-Hang Zhang Yue Zhang Zhao Zhang Zhi Zhang Zi-Liang Zhang hai-sheng Zhao Xiao-fan Zhao Shi-Jie zheng Yao-Guang zheng Deng-Ke Zhou jian-Feng Zhou Yu-Xuan Zhu Ren-Lin Zhuang Yue Zhu Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Chinese Academy of SciencesBeijing 100049China Institut fur Astronomie und Astrophysik Kepler Center for Astro and Particle PhysicsEberhard Karls Universität72076 TubingenGermany Department of Astronomy Beijing Normal UniversityBeijing 100088China Department of Astronomy Tsinghua UniversityBeijing 100084China Department of Physics Tsinghua UniversityBeijing 100084China Department of Engineering Physics Tsinghua UniversityBeijing 100084China Key Laboratory of Space Astronomy and Technology National Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China College of Physics Sciences&Technology Hebei UniversityBaoding 071002Hebei ProvinceChina

We present the observational results from a detailed timing analysis of the black hole candidate EXO 1846-031 during its outburst in 2019 with the observations of Insight-HXMT,NICER and *** outburst can be classified roughly into four different ***-C quasi-periodic oscillations(QPOs)observed by NICER(about 0.1-6 Hz)and Insight-HXMT(about 0.7-8 Hz)are also reported in this ***,we study various physical quantities related to QPO *** QPO rms-frequency relationship in the energy band 1-10 keV indicates that there is a turning pointing in frequency around2 Hz,which is similar to that of GRS 1915+105.A possible hypothesis for the relationship above may be related to the inclination of the source,which may require a high inclination to explain *** relationships between QPO frequency and QPO rms,hardness,total fractional rms and count rate have also been found in other transient sources,which can indicate that the origin of type-C QPOs is non-thermal.

关键词： X-ray binaries black hole candidate QPO EXO 1846–031

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

Atlas of dynamic spectra of fast radio burst FRB 20201124A

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Chinese Physics B 2023年第2期32卷 1-4页

作者：王铂钧胥恒姜金辰徐江伟牛佳瑞陈平李柯伽张冰朱炜玮东苏勃张春风傅海周德江张永坤王培冯毅李晔李冬子鲁文宾杨元培 RNCaballero 蔡策陈卯蒸戴子高艾力·伊沙木丁甘恒谦韩金林郝龙飞黄玉祥姜鹏李承奎李菂李辉李新乔李志玄刘志勇罗睿门云鹏牛晨辉彭文溪钱磊宋黎明孙京海王发印汪敏王娜王维扬吴雪峰肖硕熊少林徐永华徐仁新杨俊杨轩姚蕊易祁彬岳友岭于东俊余文飞袁建平张彬彬张松波张双南赵一郑伟康朱岩邹金航 Kavli Institute for Astronomy and Astrophysics Peking UniversityBeijing 100871China National Astronomical Observatories Chinese Academy of SciencesBeijing 100101China Department of Astronomy Peking UniversityBeijing 100871China University of Chinese Academy of Sciences Chinese Academy of SciencesBeijing 100049China Department of Particle Physics and Astrophysics Weizmann Institute of ScienceRehovot 76100Israel Nevada Center for Astrophysics University of NevadaLas VegasNV 89154USA Department of Physics and Astronomy University of NevadaLas VegasNV 89154USA Department of Physics&Astronomy University of IowaIowa CityIA 52242USA Zhejiang Laboratory HangzhouZhejiang 311121China Purple Mountain Observatory Chinese Academy of SciencesNanjing 210008China TAPIR Walter Burke Institute for Theoretical PhysicsMail Code 350-17CaltechPasadenaCA 91125USA Department of Astronomy University of California at BerkeleyBerkeleyCA 94720USA South-Western Institute For Astronomy Research Yunnan UniversityYunnan 650504China Key Laboratory of Particle Astrophysics Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China Xinjiang Astronomical Observatory Chinese Academy of SciencesUrumqi 830011China University of Science and Technology of China Anhui 230026China Yunnan Observatories Chinese Academy of SciencesKunming 650216China Guizhou Normal University Guiyang 550001China CSIRO Space and Astronomy EppingNSW 1710Australia Max-Planck institut fur Radioastronomie Auf Dem HugelBonn53121Germany School of Astronomy and Space Science Nanjing UniversityNanjing 210093China State Key Laboratory of Nuclear Physics and Technology School of PhysicsPeking UniversityBeijing 100871China Shanghai Astronomical Observatory Chinese Academy of SciencesShanghai 200030China Key Laboratory of Modern Astronomy and Astrophysics(Nanjing University) Ministry of EducationNanjing 210093China College of Physics Hebei Normal UniversityShijiazhuang 050024China

fast radio bursts(FRBs) are highly dispersed millisecond-duration radio bursts,[1,2]of which the physical origin is still not fully understood. FRB 20201124A is one of the most actively repeating FRBs. In this paper, we present the collection of 1863 burst dynamic spectra of FRB 20201124A measured with the Five-hundred-meter Aperture Spherical radio Telescope(faST). The current collection, taken from the observation during the FRB active phase from April to June 2021, is the largest burst sample detected for any FRB so far. The standard PSRFITs format is adopted, including dynamic spectra of the burst, and the time information of the dynamic spectra, in addition, mask files help readers to identify the pulse positions are also provided. The dataset is available in Science Data Bank, with the link https://***/10.57760/sciencedb.j00113.00076.

关键词： fast radio burst faST

静脉吸毒人群HIV自愿咨询检测对其高危行为影响的研究

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疾病控制杂志 2006年第5期10卷 448-450页

作者：陈康林尹潞阮玉华王云霞秦光明张莉陈显煌姜正清宋本莉刘石柱郝春邵一鸣西昌市皮肤病性病防治站四川西昌615000 中国疾病预防控制中心性病艾滋病预防控制中心北京100050 四川省疾病预防控制中心四川成都610031

目的了解静脉吸毒人群接受HIV自愿咨询检测前后其高危行为的变化情况。方法以社区为基础招募HIV血清抗体阴性的静脉吸毒人群,调查其社会人口学、近3个月吸毒相关行为和近6个月性行为情况,比较VCT前后12个月研究对象的高危行为变化情况... 详细信息

目的了解静脉吸毒人群接受HIV自愿咨询检测前后其高危行为的变化情况。方法以社区为基础招募HIV血清抗体阴性的静脉吸毒人群,调查其社会人口学、近3个月吸毒相关行为和近6个月性行为情况,比较VCT前后12个月研究对象的高危行为变化情况。结果静脉吸毒人群212人接受VCT前后12个月高危行为变化为:近3个月静脉吸毒、注射海洛因、海洛因混合其他毒品使用频率≥7次/w的比例分别从79.3%、40.6%、52.4%分别下降至64.6%、25.9%、41.5%;近3个月新的共用注射器具吸毒伙伴、共用针头或注射器、共用洗针头或注射器的水、共用吸毒器皿、共用棉球和共用注射器前或后装入毒品的比例分别从14.2%、38.7%、28.3%、27.4%、7.55%、5.7%分别下降至4.3%、11.32%、11.3%、17.0%、1.9%、0.9%;近6个月以性交为条件给性伴提供钱物和有新性伴的比例分别从18.4%、27.8%下降到11.3%、18.9%。结论VCT可减少静脉吸毒人群HIV相关高危行为。

关键词：获得性免疫缺陷综合征流行病学

Sub-percent precision measurement of neutrino oscillation parameters with JUNO

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Chinese Physics C 2022年第12期46卷 28-49页

作者： Angel Abusleme Thomas Adam Shakeel Ahmad Rizwan Ahmed Sebastiano Aiello Muhammad Akram Abid Aleem Fengpeng An Qi An Giuseppe Andronico Nikolay Anfimov Vito Antonelli Tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Auguste Weidong Bai Nikita Balashov Wander Baldini Andrea Barresi Davide Basilico Eric Baussan Marco Bellato Antonio Bergnoli Thilo Birkenfeld Sylvie Blin David Blum Simon Blyth Anastasia Bolshakova Mathieu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Jose Busto Ilya Butorov Anatael Cabrera Barbara Caccianiga Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Riccardo Callegari Antonio Cammi Agustin Campeny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Chi Chan Jinfan Chang Yun Chang Guoming Chen Pingping Chen Po-An Chen shaomin Chen Xurong Chen Yixue Chen Yu Chen Zhiyuan Chen Zikang Chen Jie Cheng Yaping Cheng Yu Chin Cheng Alexey Chetverikov Davide Chiesa Pietro Chimenti Artem Chukanov Gérard Claverie Catia Clementi Barbara Clerbaux Selma Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalager Christophe De La Taille Zhi Deng Ziyan Deng Wilfried Depnering Marco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara Sergey Dmitrievsky Tadeas Dohnal Dmitry Dolzhikov Georgy Donchenko jianmeng Dong Evgeny Doroshkevich Marcos Dracos Frédéric Druillole Ran Du Shuxian Du Stefano Dusini Martin Dvorak Timo Enqvist Heike Enzmann Andrea fabbri Donghua fan Lei fan jian fang Wenxing fang Marco fargetta Dmitry Fedoseev zhengyong Fei Li-Cheng Feng Qichun Feng Richard Ford Amélie Fournier Haonan Gan Feng Gao Alberto Garfagnini Arsenii Gavrikov Marco Giammarchi Nunzio Giudice Maxim Gonchar Guanghua Gong Hui Gong Yuri Gornushkin Alexandre Göttel Marco Grassi Vasily Gromov Minghao Gu Xiaofei Gu Yu Gu Mengyun Guan Yuduo Guan Nunzio Guardone Cong Guo Jingyuan Guo Wanlei Guo Xinheng Guo Yuhang Guo Paul Hackspacher Caren Hagner Ran Han Yang Han Miao He Wei He Tobias Heinz Patrick Hellmuth Yuekun Heng Rafael Herrera YuenKeung Ho Yerevan Physics Institute YerevanArmenia UniversiéLibre de Bruxelles BrusselsBelgium Universidade Estadual de Londrina LondrinaBrazil Pontificia Universidade Catolica do Rio de Janeiro Rio de JaneiroBrazil 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 JinanChinaand Key Laboratory of Particle Physics and Particle Irradiation of Ministry of EducationShandong UniversityQingdaoChina 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 UniversityZhengzhou

JUNO is a multi-purpose neutrino observatory under construction in the south of *** publication presents new sensitivity estimates for the measurement of the △m_(31)^(2),△m_(21)^(2),sin^(2)θ_(12),and sin^(2)θ_(13) oscillation parameters using reactor antineutrinos,which is one of the primary physics goals of the *** sensitivities are obtained using the best knowledge available to date on the location and overburden of the experimental site,the nuclear reactors in the surrounding area and beyond,the detector response uncertainties,and the reactor antineutrino spectral shape constraints expected from the TAO satellite *** is found that the △m_(21)^(2) and sin^(2)θ_(12) oscillation parameters will be determined to 0.5%precision or better in six years of data *** the same period,the △m_(31)^(2) parameter will be determined to about 0.2%precision for each mass ordering *** new precision represents approximately an order of magnitude improvement over existing constraints for these three parameters.

关键词： neutrino oscillation reactor antineutrino precision measurement JUNO

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早期肺癌围术期治疗专家共识

循证医学 2019年第4期19卷 193-198页

作者：无吴一龙陆舜王长利王俊程颖陈晓媛陈明王群范云揣少坤汪笑男张力杨跃杨帆王洁陈海泉支修益胡成平杨衿记刘宏旭蔡开灿张绪超刘永煜黄诚许林毛伟敏周清华康晓征李强张兰军周建娅黄云超汪步海邬麟徐松涛钟文昭徐世东杨农朱正飞林冬梅廖日强宋启斌杨林刘再毅蔡修宇蒋峰胡毅陈元马智勇乔贵宾宋勇林根赵明芳周清卢铀闫小龙王志杰刘晓晴马海涛彭忠民岳东升施巍炜廖美琳管忠震陈婧华中国临床肿瘤学会、中国抗癌协会肺癌专业委员会广州燃石医学检验有限公司广州510300 南京世和基因生物技术有限公司南京210032 中山大学肿瘤防治中心广州510060 北京大学肿瘤医院北京100142 中国医学科学院肿瘤医院北京100021 复旦大学附属肿瘤医院上海200032 首都医科大学宣武医院北京100053 中南大学湘雅医院长沙410008 中国医科大学肿瘤医院沈阳110042 南方医科大学南方医院广州510515 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 沈阳市第十人民医院沈阳110044 福建省肿瘤医院福州350014 江苏省肿瘤医院南京210009 四川大学华西医院成都610041 四川省肿瘤医院成都610041 浙江大学附属第一医院杭州310003 云南省肿瘤医院昆明650118 苏北人民医院江苏扬州225001 湖南省肿瘤医院长沙410013 哈尔滨医科大学附属肿瘤医院哈尔滨150081 上海交通大学附属胸科医院上海200030 武汉大学人民医院武汉430060 深圳市人民医院广东深圳518020 解放军总医院第一医学中心北京100853 华中科技大学同济医学院附属同济医院武汉430030 河南省肿瘤医院郑州450003 东部战区总医院南京210002 中国医科大学附属第一医院沈阳110001 空军军医大学唐都医院西安710038 解放军总医院第五医学中心北京100071 苏州大学附属第一医院江苏苏州215006 天津医科大学肿瘤医院天津300060 山东省立医院济南250021 至本医疗科技(上海)有限公司上海201114 北京大学人民医院北京100044 吉林省肿瘤医院长春130021 国家食品药品监督管理总局药品审评中心北京100038 浙江省肿瘤医院杭州310022 复旦大学附属中山医院上海200032

由中国临床肿瘤学会和中国抗癌协会肺癌专业委员会主办,中国胸部肿瘤研究协作组、广东省抗癌协会肺癌专业委员会、广东省医学科学院、广东省人民医院和广东省肺癌研究所承办的第16届中国肺癌高峰论坛于2019年3月1-2日在广州召开。此次... 详细信息

由中国临床肿瘤学会和中国抗癌协会肺癌专业委员会主办,中国胸部肿瘤研究协作组、广东省抗癌协会肺癌专业委员会、广东省医学科学院、广东省人民医院和广东省肺癌研究所承办的第16届中国肺癌高峰论坛于2019年3月1-2日在广州召开。此次论坛从早期肺癌围手术期治疗的实践、探索、展望、共识四个角度开展相关学术探讨,达成了专家共识。

关键词：早期肺癌围术期治疗循证医学共识