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抗肿瘤坏死因子治疗与多发性硬化症的进展相关

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世界核心医学期刊文摘（胃肠病学分册） 2005年第9期1卷 55-55页

作者： Enayati p.J. papadakis K.A. 徐瑞 Department of Medicine David Geffen School of Medicine University of California Los Angeles 8700 Beverly Blvd. Los Angeles CA 90048 United States Dr.

A 35-year-old woman with a history of indeterminate colitis developed symptoms of multiple sclerosis after treatment with infliximab. Neurologic examination confirmed upper and lower extremity motor and sensory deficits. MRI showed multiple enhancing white matter lesions distributed throughout her brain as well as her thoracic spine. There may be a link between inflammatory demyelinating disease of the central nervous system and anti-tumor necrosis-αtherapy. This case report describes the onset or worsening of a demyelinating process after the initiation of infliximab therapy in a patient with indeterminate colitis.

关键词：多发性硬化症抗肿瘤坏死因子脱髓鞘疾病下肢运动中枢神经系统肿瘤坏死因子α 检查表感觉功能徐瑞

希腊啃老族和边缘青年的教育、培训、就业现状

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当代教育与文化 2018年第3期10卷 1-10页

作者：尼克斯.帕帕扎基斯佩拉.卡拉奇纳基斯希腊克里特大学政治学系希腊克里特大学初等教育系

文章主要论述希腊青年(啃老族)在教育、就业和培训的现状,着重探讨希腊受经济危机和持续萧条的影响下青年失业和啃老族问题。从希腊青年和啃老族的教育水平、受培训情况、失业问题和社会弱势的现状出发,分析了希腊人贫困代际传递现象、... 详细信息

文章主要论述希腊青年(啃老族)在教育、就业和培训的现状,着重探讨希腊受经济危机和持续萧条的影响下青年失业和啃老族问题。从希腊青年和啃老族的教育水平、受培训情况、失业问题和社会弱势的现状出发,分析了希腊人贫困代际传递现象、生存战略和青年与啃老族的生活历程。

关键词：边缘青少年希腊青少年教育培训失业问题社会弱势

CT增强扫描碘吸收量对病人组织吸收辐射剂量的影响研究:CT放射剂量学的启示

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国际医学放射学杂志 2018年第2期 237-237页

作者： K.perisinakis A.Tzedakis K.Spanakis A.E.papadakis A.Hatzidakis J.Damilakis 韩雨 Department of Medical physics Medical School University of Crete

摘要目的探讨碘摄取对CT照射组织/器官吸收剂量的影响及其在CT剂量测定中的意义。方法回顾性分析120例CT检查的病人,确定对CT增强敏感的组织,检查包括CT

关键词：辐射剂量 CT

CT自动曝光控制技术:病人体型、解剖区域、指定的调制强度对管电流及影像质量的影响

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国际医学放射学杂志 2014年第6期 608-608页

作者： A.E.papadakis K.perisinakis J.Damilakis 孟珊 Department of Medical physics University Hospital of HeraklionStavrakiaP.O.Box 1352Heraklion 71110CreteGreece

摘要目的研究在使用自动管电流调制(ATCM)CT检查时,病人体型、身体部位、调制强度对管电流及影像质量的影响。方法采用了模拟新生儿,1、5、10岁儿童及成人体型的

关键词：影像质量管电流病人 CT

具有低动脉粥样硬化风险特征的专业耐力运动员的亚临床冠状动脉疾病发病率

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中华高血压杂志 2017年第6期25卷 588-588页

作者：刘莉叶鹏 Merghani A Maestrini V Rosmini S Cox AT Dhutia H Bastiaenen R David S Yeo TJ Narain R Malhotra A papadakis M Wilson MG Tome M AlFakih K Moon JC Sharma S

研究表明,具有冠状动脉疾病（coronary artery disease,CAD）危险因素的中老年（健将）运动员比久坐个体冠状动脉钙化（coronary artery calcium,CAC）评分更高。尚没有研究评估具有低动脉粥样硬化风险特征的专业运动员的CAD患病率。

关键词：动脉粥样硬化冠状动脉疾病耐力运动员疾病发病率风险亚临床 artery 冠状动脉钙化

通过模型研究妊娠期腹部CT中病人的中心定位对胚胎辐射剂量和影像质量的影响

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国际医学放射学杂志 2015年第3期 296-296页

作者： G.Solomou A.E.papadakis J.Damilakis 刘陈汉 Faculty of Medicine Department of Medical PhysicsUniversity of CreteHeraklionP.O.Box 2208 71003 Crete Greece

目的研究妊娠期病人行腹部CT检查时病人的中心位置对胚胎辐射剂量和影像质量的影响。材料与方法分别对3个代表早中晚期孕妇的人体模型行常规腹部CT检

关键词：影像质量辐射剂量人体模型中心定位晚期孕妇噪声比热释光剂量计中心偏移信噪比降低率

进行升主动脉瘤手术的患者冠状动脉扩张的发生率

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世界核心医学期刊文摘（心脏病学分册） 2005年第4期1卷 32-32页

作者： papadakis M. C. Leontiadis E. Manginas A. 王永兴

We retrospectively studied the coronary arteriograms of 82 consecutive patient s who underwent planned surgical repair of an ascending aorta aneurysm and an ag e-matched control group of 92 consecutive patients who underwent coronary angio graphy during the same time period. The present study examines the incidence of coronary artery ectasia in patients with aneurysms of the ascending aorta.

关键词：升主动脉瘤手术冠状动脉扩张外科修复

早孕期间多层CT对孕体的辐射剂量:一种可用于不同母体体型及孕体位置的方法

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国际医学放射学杂志 2011年第1期34卷 76-页

作者： J.Damilakis K.perisinakis A.Tzedakis A.E.papadakis A.Karantanas 刘宁宁 Department of Medical physics Faculty of MedicineUniversity of Crete

目的建立一种评估多层CT对孕7周内患有腹部及盆腔疾病的孕妇所受辐射剂量的方法。材料与方法该研究获得学院伦理委员会批准并得到病人知情同意。

关键词：辐射剂量孕体 CT

Observatory science with eXTp

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Science China(physics,Mechanics & Astronomy) 2019年第2期62卷 97-138页

作者： Jean J.M.in 't Zand Enrico Bozzo JinLu Qu Xiang-Dong Li Lorenzo Amati Yang Chen Immacolata Donnarumma Victor Doroshenko Stephen A.Drake Margarita Hernanz peter A.Jenke Thomas J.Maccarone Simin Mahmoodifar Domitilla de Martino Alessandra De Rosa Elena M.Rossi Antonia Rowlinson Gloria Sala Giulia Stratta Thomas M.Tauris Joern Wilms XueFeng Wu ping Zhou Iván Agudo Diego Altamirano Jean-Luc Atteia Nils A.andersson M.Cristina Baglio David R.Ballantyne Altan Baykal Ehud Behar Tomaso Belloni Sudip Bhattacharyya Stefano Bianchi Anna Bilous pere Blay Joao Braga Sφren Brandt Edward F.Brown Niccolo Bucciantini Luciano Burderi Edward M.Cackett Riccardo Campana Sergio Campana piergiorgio Casella Yuri Cavecchi Frank Chambers Liang Chen Yu-peng Chen Jér?me Chenevez Maria Chernyakova ChiChuan Jin Riccardo Ciolfi Elisa Costantini Andrew Cumming Antonino D'Aì Zi-Gao Dai Filippo D'Ammando Massimiliano De pasquale Nathalie Degenaar Melania Del Santo Valerio D'Elia Tiziana Di Salvo Gerry Doyle Maurizio Falanga XiLong Fan Robert D.Ferdman Marco Feroci Federico Fraschetti Duncan K.Galloway Angelo F.Gambino poshak Gandhi MingYu Ge Bruce Gendre Ramandeep Gill Diego G?tz Christian Gouiffès paola Grandi Jonathan Granot Manuel Güdel Alexander Heger Craig O.Heinke Jeroen Homan Rosario Iaria Kazushi Iwasawa Luca Izzo Long Ji peter G.Jonker Jordi José Jelle S.Kaastra Emrah Kalemci Oleg Kargaltsev Nobuyuki Kawai Laurens Keek Stefanie Komossa Ingo Kreykenbohm Lucien Kuiper Devaky Kunneriath Gang Li En-Wei Liang Manuel Linares Francesco Longo FangJun Lu Alexander A.Lutovinov Denys Malyshev Julien Malzac Antonios Manousakis Ian McHardy Missagh Mehdipour Yunpeng Men Mariano Méndez Roberto p.Mignani Romana Mikusincova M.Coleman Miller Giovanni Miniutti Christian Motch Joonas Nättilä Emanuele Nardini Torsten Neubert paul T.O'Brien Mauro Orlandini Julian p.Osborne Luigi pacciani Stéphane paltani Maurizio paolillo Iossif E.papadakis Biswajit paul Alberto pellizzoni Uria peretz Miguel A.pérez Torres Emanuele perinati Chanda prescod-Weinstein pablo Reig SRON Netherlands Institute for Space Research Department of Astronomy University of Geneva Key Laboratory for particle Astrophysics Institute of High Energy PhysicsChinese Academy of Sciences School of Astronomy and Space Science Nanjing University INAF-IASF Bologna ASI Via del Politecnico snc INAF-Istituto di Astrofisica e planetologie Spaziali Institut für Astronomie und Astrophysik Tübingen Universit?t Tübingen NASA Goddard Space Flight Center ICREA&Institute of Space Sciences(IEEC-CSIC) Campus UABCarrer de Can Magrans CSpAR SPA University of Alabama in Huntsville Department of physics Texas Tech University INAF Osservatorio Astronomico di Capodimonte Leiden Observatory Leiden University Anton pannekoek Institute University of Amsterdam ASTRON Netherlands Institute for Radio Astronomy Universitat politecnica de Catalunya(UpC-IEEC) Universitádegli Studi di Urbino‘Carlo Bo’ Max-planck-Institut für Radioastronomie Dr.Karl-Remeis-Sternwarte and Erlangen Centre for Astroparticle physics(ECAp) Friedrich Alexander Universit?t Erlangen-Nurnberg purple Mountain Observatory Chinese Academy of Sciences Instituto de Astrofysíca de Andalucia-CSIC Department of physics and Astronomy University of Southampton IRAp Universitéde ToulouseCNRSUPSCNES Mathematical Sciences and STAG Research Centre University of Southampton New York University Abu Dhabi Center for Relativistic Astrophysics School of PhysicsGeorgia Institute of Technology physics Department Middle East Technical University Department of physics Technion-Israel Institute of Technology INAF Osservatorio Astronomico di Brera Tata Institute of Fundamental Research Dipartimento di Matematica e Fisica Universitàdegli Studi Roma Tre Instituto de Astrofísica de Canarias Instituto Nacional de pesquisas Espaciais-INpE National Space Institute Technical University of Denmark(DTU Space) Department of physics and Astronomy Michigan State University INAF Osservatorio Astrofisico di Arcetri Dipartimento di Fisica Universitádegli Studi di Cagliari Department of physics and A

In this White paper we present the potential of the enhanced X-ray Timing and polarimetry(eXTp) mission for studies related to Observatory Science targets. These include flaring stars, supernova remnants, accreting white dwarfs, low and high mass X-ray binaries, radio quiet and radio loud active galactic nuclei, tidal disruption events, and gamma-ray bursts. eXTp will be excellently suited to study one common aspect of these objects: their often transient nature. Developed by an international Consortium led by the Institute of High Energy physics of the Chinese Academy of Science, the eXTp mission is expected to be launched in the mid 2020s.

关键词： space research in struments nuclear astrophysics flare stars accretion and accretion disks mass loss and stellar winds cataclysmic binaries X-ray binaries supernova remnants active galactic nuclei X-ray bursts gamma-ray bursts gravitational waves