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Improved Peptidyl Linkers for Self-Assembly of Semiconductor Quantum Dot Bioconjugates

Nano Research 2009年第2期2卷 121-129页

作者： lorenzo berti Paola Serena D'Agostino Kelly Boeneman Igor L.Medintz CNR-INFM National Research Center on nanoStructures and bioSystems at Surfaces(S3)Via Campi213/A 41100 ModenaItaly University of California Davis Medical Center SacramentoCA 95817USA Center for Bio/Molecular Science and Engineering Code 6900 U.S.Naval Research LaboratoryWashingtonDC 20375USA

We demonstrate improved peptide linkers which allow both conjugation to biomolecules such as DNA and self-assembly with luminescent semiconductor quantum dots.A hexahistidine peptidyl sequence was generated by standard solid phase peptide synthesis and modified with the succinimidyl ester of iodoacetamide to yield a thiol-reactive iodoacetyl polyhistidine *** reactive peptide was conjugated to dye-labeled thiolated DNA which was utilized as a model target *** gel electrophoresis and fluorescence resonance energy transfer analysis confirmed that the linker allowed the DNA to self-assemble with quantum dots via metal-affinity driven *** contrast to previous peptidyl linkers that were based on disulfide exchange and were thus labile to reduction,the reactive haloacetyl chemistry demonstrated here results in a more stable thioether bond linking the DNA to the peptide which can withstand strongly reducing environments such as the intracellular *** thiol groups occur naturally in proteins,can be engineered into cloned proteins,inserted into nascent peptides or added to DNA during synthesis,the chemistry demonstrated here can provide a simple method for self-assembling a variety of stable quantum dot bioconjugates.

关键词： Semiconductor quantum dot peptide DNA nanocrystal bioconjugation iodoacetyl sulfhydryl polyhistidine metal-affinity fluorescence fluorescence resonance energy transfer(FRET)

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Feasibility of en bloc thulium laser enucleation of the prostate in a large case series. Are results enhanced by experience?

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Asian Journal of Urology 2019年第4期6卷 339-345页

作者： Giovanni Saredi Giacomo Maria Pirola Francesca Ambrosini Simone Barbieri lorenzo berti Andrea Pacchetti Domenico Iovino Giuseppe Ietto Letizia Libassi Giulio Carcano Department of Urology Ospedale di Circolo e Fondazione MacchiVareseItaly Department of Urology Usl Toscana Sud EstSan Donato HospitalArezzoItaly Centro Cardiologico Monzino IRCCSMilanItaly Department of Urology University of GenovaGenovaItaly Department of Surgery University of InsubriaVareseItaly

Objective:To provide the first large single-operator case series of patients who undergo“en bloc”thulium laser enucleation of the prostate(ThuLEP)and to demonstrate an improvement in enucleation efficacy with ***:We prospectively evaluated a cohort of patients with symptomatic benign prostatic hyperplasia(BPH)who underwent“en bloc”ThuLEP between May 2015 and November *** between dependent variables(delivered energy and operating time)and independent variables(adenoma volume and experience)were estimated with regression *** experience was calculated as the time interval between the date of the first operation of the series and the date of the operation being ***:A total of 100 patients were registered for the *** operative time was 56.5 min(interquartile range[IQR]:40-85 min).Median enucleation time was 17.4 min(IQR:15-21.5 min).Median enucleation index(enucleation time per adenoma gram)was 0.3 min/g(0.2-0.3 min/g).The overall operative time is not influenced by experience,but we registered a significant trend towards a reduction in the total amount of energy delivered energy normalized per adenoma gram(p=0.0148).Conclusion:We believe that further attention is needed for these new“en bloc”prostatic enucleation techniques,which can facilitate some surgical steps,leading to a widespread use of laser technology for BPH surgical treatment.

关键词： Benign prostatic hyperplasia Endoscopic enucleation of the prostate Laser surgery Thulium laser enucleation of the prostate

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Accretion in strong field gravity with eXTP

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Science China(Physics,Mechanics & Astronomy) 2019年第2期62卷 45-73页

作者： Alessandra De Rosa Phil Uttley LiJun Gou Yuan Liu Cosimo Bambi Didier Barret Tomaso Belloni Emanuele berti Stefano Bianchi Ilaria Caiazzo Piergiorgio Casella Marco Feroci Valeria Ferrari Leonardo Gualtieri Jeremy Heyl Adam Ingram Vladimir Karas FangJun Lu Bin Luo Giorgio Matt Sara Motta Joseph Neilsen Paolo Pani Andrea Santangelo XinWen Shu JunFeng Wang Jian-Min Wang YongQuan Xue YuPeng Xu WeiMin Yuan YeFei Yuan Shuang-Nan Zhang Shu Zhang Ivan Agudo lorenzo Amati Nils Andersson Cristina Baglio Pavel Bakala Altan Baykal Sudip Bhattacharyya Ignazio Bombaci NiccolóBucciantini Fiamma Capitanio Riccardo Ciolfi Wei K.Cui Filippo D'Ammando Thomas Dauser Melania Del Santo Barbara De Marco Tiziana Di Salvo Chris Done Michal Dovciak Andrew C.Fabian Maurizio Falanga Angelo Francesco Gambino Bruce Gendre Victoria Grinberg Alexander Heger Jeroen Homan Rosario Iaria JiaChen Jiang ChiChuan Jin Elmar Koerding Manu Linares Zhu Liu Thomas J.Maccarone Julien Malzac Antonios Manousakis Frédéric Marin Andea Marinucci Missagh Mehdipour Mariano Méndez Simone Migliari Cole Miller Giovanni Miniutti Emanuele Nardini Paul T.O'Brien Julian P.Osborne Pierre Olivier Petrucci Andrea Possenti Alessandro Riggio Jerome Rodriguez Andrea Sanna LiJing Shao Malgosia Sobolewska Eva Sramkova Abigail L.Stevens Holger Stiele Giulia Stratta Zdenek Stuchlik Jiri Svoboda Fabrizio Tamburini Thomas M.Tauris Francesco Tombesi Gabriel Torok Martin Urbanec Frederic Vincent QingWen Wu Feng Yuan Jean J.M.in't Zand Andrzej A.Zdziarski XinLin Zhou INAF-Istituto di Astrofisica e Planetologie Spaziali Via Fosso del Cavaliere Anton Pannekoek Institute for Astronomy University of Amsterdam National Astronomical Observatories Chinese Academy of Science Institute of High Energy Physics Chinese Academy of Science Center for Field Theory and Particle Physics and Department of Physics Fudan University IRAP Universitéde ToulouseCNRSUPSCNES INAF-Osservatorio Astronomico di Brera Department of Physics and Astronomy The University of MississippiUniversity Dipartimento di Matematica e Fisica Universitàdegli studi Roma Tre University of British Columbia INAF-Osservatorio Astronomico di Roma INFN-Roma 2 c/o Dipartimento di Fisica II Universit?di Roma"Tor Vergata" Dipartimento di Fisica Universitàdegli Studi di Roma"La Sapienza"&Sezione INFN Roma1 Department of Physics University of OxfordClarendon Laboratory Astronomical Institute Academy of Sciences School of Astronomy and Space Science Nanjing University MIT Kavli Institute for Astrophysics and Space Research Institut für Astronomie und Astrophysik Eberhard Karls Universität Department of Physics Anhui Normal University Department of Astronomy and Institute of Theoretical Physics and Astrophysics Xiamen University CAS Key Laboratory for Research in Galaxies and Cosmology Department of AstronomyUniversity of Science and Technology of China Instituto de Astrofísica de Andalucia(CSIC) Glorieta de la Astronomía s/n INAF-Istituto di Astrofisica Spaziale e Fisica cosmica di Bologna Mathematical Sciences and STAG Research Centre University of Southampton New York University Abu Dhabi Institute of Physics and Research Centre for Computational Physics and Data Processing Faculty of Philosophy&ScienceSilesian University in OpavaíBezru?ovo nám. Department of Physics Middle East Technical University Department of Astronomy and Astrophysics Tata Institute of Fundamental Research Dipartimento di Fisica Universit?di Pisa&INFN INAF-Osservatorio Astrofisico di Arcetri INAF-Osservatorio Astronomico di Padova INFN-TIFPA Trento Ins

In this paper we describe the potential of the enhanced X-ray Timing and Polarimetry(eXTP) mission for studies related to accretion flows in the strong field gravity regime around both stellar-mass and supermassive black-holes. eXTP has the unique capability of using advanced "spectral-timing-polarimetry" techniques to analyze the rapid variations with three orthogonal diagnostics of the flow and its geometry, yielding unprecedented insight into the inner accreting regions, the effects of strong field gravity on the material within them and the powerful outflows which are driven by the accretion process.

关键词： X-ray black holes physics accretion

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