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modification of Serum Galectin-3 and Reversal of Cardiac Remodeling Following Pediatric Transcatheter Atrial Septal Defect Closure

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Congenital Heart Disease 2022年第2期17卷 173-185页

作者： Omnia Shafei Alyaa A.Kotby mona mEl Ganzoury nevin m.ha.eeb Eman Elsayed Department of Pediatrics Faculty of MedicineAin Shams UniversityCairoEgypt Children’s Hospital Cardiology UnitAin Shams University HospitalsCairoEgypt

Objectives:We aimed to evaluate the effect of percutaneous atrial septal defect(ASD)closure in children using right heart indices and serum galectin-3(Gal-3),as potential biomarkers of right heart ***:This case–control prospective study included 40 children with ASD and 25 control *** echocardiographic evaluation was performed before the procedure,as well as 24 h,1 month,and 6 months after *** Gal-3 was measured before,and 1 month after the ***:Serum Gal-3 concentration,right atrial(RA)dimensions,right ventricular(RV)dimensions,indexed RA area,and right index of myocardial performance(RImP)were significantly increased in children with ASD compared with control subjects while tricuspid annular plane systolic excursion(TAPSE)was significantly *** months after closure,RA,and RV dimensions significantly decreased and RVfunction improved(RImP decreased and TAPSE increased).Gal-3 oncentration significantly decreased 1 month after ASD closure,but it did not reach normal range compared with control subjects.A positive correlation between Gal-3 and age at closure,RA area,RV dimensions,and RImP was observed.A positive correlation was observed between the decrease in Gal-3 concentration and the decrease in RA area and RV dimensions 1 month after ASD closure.A significant negative correlation was observed between TAPSE and Gal-3 concentration before and after ***:Percutaneous ASD closure can improve right-sided indices and decrease serum Gal-3 ***-3 can be used as a sensitive biomarker of right heart remodeling,with a decrease in Gal-3 concentration suggesting reversal of maladaptive remodeling.

关键词： Percutaneous device closure Galectin-3 cardiac remodeling children atrial septal defect

Going…Going…Gone:The End of the Banana?

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疯狂英语（初中天地） 2003年第28期 18-18页

作者： nevin

Nobody ever thought it could happen, but botanical and agricultural experts have issued a grave warning:the banana, one of the world's best-loved fruits, might practically go extinct in as short as 10 *** bananas we eat today originated from the wild banana(musa acuminata), which is inedible because of the many sturdy seeds it contains. Apparently, about 10,000 years ago, people somewhere in South-East Asia discovered a rare mutated variety that yielded soft, delicious fruits without seeds. This m...

关键词： Gone:The End of the Banana Going

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营养与健康—新的知识新的挑战——1987年10月在第五届亚洲营养会议上的专题报告

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营养学报 1988年第2期 184-186页

作者： Dr nevin,S. Scrimshaw,m. D. PH. D.,梅节 ,陈起萱 massachusetts Institute of Technology Director Food and Nutrition Programme United Nations University Japan Institute Professor massachusetts Institute of Technology Director Food and Nutrition Programme United Nations University Japan Institute Professor massachusetts Institute of Technology Director Food and Nutrition Programme United Nations University Japan Institute Professor

在营养上,亚洲地区最艰难的日子已经过去,而且正在继续改进。目前,对于战胜常见营养缺乏病的方法学问题已经基本解决,营养与退行性疾病、富裕和过度营养所引起的严重健康等问题正在受到关注,这对亚洲的营养学者来说,是一个空前的机会和... 详细信息

在营养上,亚洲地区最艰难的日子已经过去,而且正在继续改进。目前,对于战胜常见营养缺乏病的方法学问题已经基本解决,营养与退行性疾病、富裕和过度营养所引起的严重健康等问题正在受到关注,这对亚洲的营养学者来说,是一个空前的机会和巨大的挑战。日前,亚洲热量不足的人们还在增加,只有日本和小国例外;一部分亚洲的孩子仍然因

关键词：营养发病率死亡率人口自然变动营养与健康营养教育亚洲缺碘性疾病会议

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

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