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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

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

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

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

Centralized isolation of Helicobacter pylori from multiple centers and transport condition influences

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World Journal of Gastroenterology 2015年第3期21卷 944-952页

作者： Ya-Nan Gong You-Ming Li Ning-Min Yang Hong-Zhang Li Feng Guo Lang Lin Qun-Ying Wang Jia-Kun Zhang Zi-Zhong Ji Ji-bo Mao Jun-Liang Mao Zheng-Chao Shi Wu-heng Tang xin-jian zhu Wei Shao Xiao-Feng Zhang xing-Hua Wang Yue-Feng Tong Mi-Zu jiang Guang-Lan Chen Zhi-yong Wang Hui-Min tu Guo-Fa jiang jian-Sheng Wu Xu-Peng Chen Qiu-Long Ding Hong Ouyang Feng-Zhe Jin Yan-Li Xu jian-Zhong Zhang State Key Laboratory for Infectious Disease Prevention and Control National Institute for Communicable Disease Control and PreventionChinese Center for Disease Control and Prevention Collaborative Innovation Center for Diagnosis and Treatment of Infectious Diseases The First Affiliated Hospital College of MedicineZhejiang University Zhiyuan Medical Inspection Institute Co. Ltd. Sanmen People’s Hospital The First People’s Hospital of Xiaoshan District The First People’s Hospital of Cangnan Jinhua Municipal Central Hospital The First People’s Hospital of Pingyang The First Hospital of Jiaxing Zhoushan Hospital The First People’s Hospital of Wenling Rui’an People’s Hospital Maternal and Child Health Hospital of Zhoushan City Shangyu People’s Hospital People’s Hospital of Putuo District Zhoushan Hangzhou First People’s Hospital Qingtian People’s Hospital The First People’s Hospital of yongkang The Children’s Hospital Zhejiang University School of Medicine Lishui People’s Hospital The Affiliated Hospital of Hangzhou Normal University Wuxi No.4 Hospital Affiliated to Suzhou University Jinhua Wenrong Hospital The First Affiliated Hospital of Wenzhou Medical College Yueqing People’s Hospital Tiantai People’s Hospital Lin’an people’s Hospital Rui’an City TCM Hospital Medical College of Hebei University of Engineering

AIM:To evaluate the efficacy of centralized culture and possible influencing ***:From January 2010 to July 2012,66452 patients with suspected Helicobacter pylori(***) infection from 26 hospitals in Zhejiang and jiangsu Provinces in China underwent gastrointestinal *** mucosal biopsies were taken from the antrum for *** biopsies were transported under natural environmental temperature to the central laboratory in Hangzhou city and divided into three groups based on their transport time:5,24 and 48 *** culture results were reported after 72 h and the positive culture rates were analyzed by a χ2 *** additional 5736 biopsies from ***-positive patients(5646 rapid urease test-positive and 90 14C-urease breath test-positive) were also cultured for quality control in the central laboratory ***:The positive culture rate was 31.66%(21036/66452) for the patient samples and 71.72%(4114/5736) for the ***-positive quality control *** the 5 h transport group,the positiveculture rate was 30.99%(3865/12471),and 32.84%(14960/45553) in the 24 h transport *** contrast,the positive culture rate declined significantly in the 48 h transport group(26.25%; P tural temperature increased from 4.67 to 29.14℃,while the positive culture rate declined from 36.67%(1462/3987) to 24.12%(1799/7459).When the temperature exceeded 24℃,the positive culture rate decreased significantly,especially in the 48 h transport group(23.17%).CONCLUSION:Transportation of specimens within 24 h and below 24℃ is reasonable and acceptable for centralized culture of multicenter *** samples.

关键词： Centralized isolation Helicobacter pylori Influenc

准南霍-玛-吐构造带紫泥泉子组油气成藏流体动力学特征

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中国石油大学学报（自然科学版） 2013年第3期37卷 30-36,43页

作者：陈勇王鑫涛方世虎张健赵孟军柳少波白振华中国石油大学地球科学与技术学院山东青岛266580 中国石油勘探开发研究院提高石油采收率国家重点实验室北京100083 新疆油田勘探开发研究院新疆乌鲁木齐830011

在区域热演化史和埋藏史基础上,通过对准噶尔盆地南缘霍-玛-吐构造带白垩系东沟组-古近系紫泥泉子组砂岩储层流体包裹体样品的系统分析,确定各期次油气成藏的主要时间,并对古近系紫泥泉子组在油气成藏期中的古流体势演化和油气运聚特征... 详细信息

在区域热演化史和埋藏史基础上,通过对准噶尔盆地南缘霍-玛-吐构造带白垩系东沟组-古近系紫泥泉子组砂岩储层流体包裹体样品的系统分析,确定各期次油气成藏的主要时间,并对古近系紫泥泉子组在油气成藏期中的古流体势演化和油气运聚特征进行研究。结果表明:研究区主要经历了两期油气成藏,第一期主要在中新世中—晚期(距今约14～9 Ma),第二期主要在上新世中—晚期(距今约3.7～2.5 Ma);两期油气成藏的古流体势分布格局具有显著差异,第一期在吐谷鲁背斜区的古流体势最低,以聚集白垩系烃源岩生成的油为主,第二期在玛纳斯背斜区的古流体势演变为最低,以聚集中下侏罗统煤系烃源岩生成的气为主。

关键词：油气藏成藏期次古流体势流体包裹体霍-玛-吐构造带准噶尔盆地南缘

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

Chinese Multidisciplinary Expert Consensus on the Diagnosis and Treatment of Hyperuricemia and Related Diseases

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Chinese Medical Journal 2017年第20期130卷 2473-2488页

作者： Zou, He-jian Wu, Hu-Sheng Zhou, Jing-Guo Zeng, Xue-Jun Dai, Lie Wu, Hua-Xiang zhu, Xiao-Xia Mei, Chang-Lin Hao, Chuan-Ming Chen, Nan Liu, Bi-Cheng Chen, jiang-Hua Yang, Li Nie, Jing Yu, Chen Peng, Ai Yu, Sheng-Qiang Li, Lin Ge, Jun-bo huo, yong Zhang, Shu-Yang Chen, Yun-Dai Dong, Yu-Gang Liang, Chun Dai, Yu-Xiang Gao, xin Li, Chang-Gui Zhao, Jia-Jun Chen, hai-Bing Cheng, Zhi-Feng Lin, Huan-Dong Guan, Yang-Tai Wang, Kai Luo, Ben-Yan Dai, Ruo-Lian jiang, Quan Xue, Luan Liang, Chao-Chao Chen, Ming Fan, Song Multidisciplinary Expert Task Force on Hyperuricemia and Related Diseases

INTRODUCTIONThe prevalence of hyperuricenlia （HUA） has increased in China in the recent years in relation to socioeconomic developments and changing lifestyles and diets, with a trend toward onset at younger age. HUA has become the second most common metabolic disease after diabetes mellitus. Like gout, HUA is also associated with the occurrence and progression of disorders of the urinary, endocrine, metabolic, cardio-cerebrovascular, and other systems.

关键词： Consensus Gout Hyperuricemia Recommendation Uric Acid

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肺癌适应性治疗中国专家共识

循证医学 2024年第4期24卷 193-200页

作者：吴一龙陆舜程颖周清张嘉涛潘燚汪斌超韩宝惠陈海泉周清华王绿化陈明王洁周彩存刘晓晴马智勇黄诚宋启斌莫树锦钟文昭朱正飞宋勇陈蓉蓉陈克终刘基巍杨帆胡晓桦胡毅杨懿岳东升王群赵军范江陈椿孟庆威闫小龙董晓荣朱波邢力刚李兆澄李子明褚倩陈元林根段建春田攀文范云刘安文刘慧刘哲峰杨农汪步海张同梅信涛刘思阳王志杰马锐于起涛林劼涂海燕姚煜赵明芳王慧娟张海波蔡尚立张绪超李慧杜瀛瀛吴芳严令华崔久嵬王燕邬麟周建娅汪笑男黄媚娟冯卫能周进李力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肺癌研究所南方医科大学附属广东省人民医院(广东省医学科学院)广州510080 上海交通大学医学院附属胸科医院上海200030 吉林省肿瘤医院长春130021 复旦大学附属肿瘤医院上海200032 四川大学华西医院成都610041 中国医学科学院肿瘤医院深圳医院广东深圳518116 中山大学肿瘤防治中心广州510060 中国医学科学院肿瘤医院北京100021 同济大学附属上海市肺科医院上海200433 解放军总医院第五医学中心北京100039 郑州大学附属肿瘤医院/河南省肿瘤医院郑州450003 福建省肿瘤医院福州350011 武汉大学人民医院肿瘤中心武汉430060 香港中文大学医学院中国香港东部战区总医院南京210002 北京吉因加科技有限公司北京102206 北京大学人民医院北京100044 大连医科大学附属第一医院辽宁大连116011 广西医科大学第一附属医院南宁530020 解放军总医院北京100071 成都市第三人民医院/西南交通大学医学院成都610031 天津医科大学肿瘤医院天津300060 复旦大学附属中山医院上海200032 北京大学肿瘤医院北京100142 上海交通大学附属上海市第一人民医院上海200025 福建医科大学附属协和医院福州350001 哈尔滨医科大学附属肿瘤医院哈尔滨150081 空军军医大学唐都医院西安710038 华中科技大学同济医学院附属协和医院武汉430022 陆军军医大学第二附属医院-新桥医院重庆400037 山东省肿瘤医院济南250117 华中科技大学同济医学院附属同济医院武汉430030 中国医学科学院肿瘤医院山西医院太原030013 中国科学院大学附属肿瘤医院/浙江省肿瘤医院杭州310022 南昌大学附属第二医院南昌330006 湖南省第二人民医院长沙410035 南京大学医学院附属苏北人民医院江苏扬州225001 首都医科大学附属北京胸科医院北京101149 哈尔滨医科大学附属第二医院哈尔滨150001 暨南大学附属第一医院广州510630 辽宁省肿瘤医院沈阳110042 广西医科大学附属肿瘤医院南宁530012 昆明医科大学第二附属医院昆明650101 西安交通大学第一附属医院西安710061 中国医科大学附属第一医院沈阳110001 广东省中医院广州510120 广州燃石医学检验所有限公司广州510300 安徽医科大学第一附属医院合肥230022 中南大学湘雅二医院长沙410011 上海桐树生物科技有限公司上海200444 吉林大学白求恩第一医院长春130021 湖南省肿瘤医院长沙410013 浙江大学医学院附属第一医院杭州310031 南京世和基因生物技术股份有限公司南京210032 佛山市第一人民医院广东佛山528000 四川省肿瘤医院成都610042 陆军军医大学大坪医院重庆400042 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21届中国肺癌高峰论坛”于2024年3月2日在广州顺利召开。此次论坛以肺癌适应性治疗为主题,从肺癌适应性治疗定义、早中晚期临床应用以及生物标志物... 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21届中国肺癌高峰论坛”于2024年3月2日在广州顺利召开。此次论坛以肺癌适应性治疗为主题,从肺癌适应性治疗定义、早中晚期临床应用以及生物标志物对适应性治疗的指导价值等角度展开探讨并达成了专家共识。

关键词：肺癌适应性治疗共识