Search results for " format"

showing 10 items of 2156 documents

Development of microfluidics for sorting of carbon nanotubes

2018

Sorting of carbon nanotubes by their chirality is the current bottleneck in the way to their broad employment based on their exceptional electronic and optical properties. Despite the extensive effort, there is no known method, which would result in really pure chirality ensembles. Previously reported sorting protocols result in enrichment rather than in sorting, alter electronic structure, and suffer from low yield. This is mostly due to the statistical approach, where the nanotubes with mixed chiralities are treated as a set. In this thesis, we propose a new sorting technique based on nanotube-by-nanotube compartmelization, characterization, and sorting in a continuously running droplet-b…

sonicationlow droplet formation frequencyspektroskopiamicrofluidicsinterfacial tensionpassive trappingTADBwater-in-oilPhysics::Fluid DynamicsSDBSerotusmenetelmätsurface tensionSpan 80rajapintailmiötcentrifugationdielectrophoresisnestefysiikkadroplet stabilitycarbon nanotubesdecanedispersiotlinkoaminenfluoresenssiultraäänilong-term stabilitypisaratlajitteludroplet-basedmikropiiritindividualizationsilinizationnear-infrared fluorescenceglass microfabricationdispersionwet etchingmetallic electrodesmikrotekniikkananoputketsorting
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A Theoretical and Experimental Investigation of the Spectroscopic Properties of a DNA-Intercalator Salphen-Type ZnIIComplex

2014

The photophysical and DNA-binding properties of the cationic zinc(II) complex of 5-triethylammonium methyl salicylidene ortho-phenylenediiminato (ZnL 2 + ) were investi- gated by a combination of experimental and theoretical methods. DFT calculations were performed on both the ground and the first excited states of ZnL 2 + and on its possi- ble mono- and dioxidation products, both in vacuo and in selected solvents mimicked by the polarizable continuum model. Comparison of the calculated absorption and fluores- cence transitions with the corresponding experimental data led to the conclusion that visible light induces a two-elec- tron photooxidation process located on the phenylenediimi- nato…

spectroscopyNO ligandStereochemistryIntercalation (chemistry)Ionic bondingmetal complex Fluorescence spectroscopy DNA recognition metal complexes organometallics complex formation DNA binding drugs fluorescence spectroscopy equilibrium constants reaction mechanisms nucleic acids affinity binding mode thermodynamics speciationmetal complexesbinding modePhenylenediaminesPolarizable continuum modelCatalysisdrugsmetal complexthermodynamicsintercalationcomplex formationOrganometallic CompoundsA-DNADNA bindingFluorescence spectroscopyDNA recognitionphotochemistryLigandChemistrySpectrum AnalysisphotooxidationOrganic ChemistryCationic polymerizationequilibrium constantsGeneral Chemistrydensity functional calculationFluorescenceZincCrystallographyreaction mechanismsnucleic acidsspeciationSettore CHIM/03 - Chimica Generale E InorganicaExcited stateaffinityfluorescenceorganometallics
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The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

2007

(abridged:) The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) surveys the most populated ~5 square degrees of the Taurus star formation region, using the XMM-Newton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association. Many targets are also studied in the optical, and high-resolution X-ray grating spectroscopy has been obtained for selected bright sources. The X-ray spectra have been coherently analyzed with two different thermal models (2-component thermal model, and a continuous emission measure distribution model). We present ov…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaBrown dwarfFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Observatory0103 physical sciencesProtostarAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsstars : formationStar formationMolecular cloudAstrophysics (astro-ph)Astronomy and AstrophysicsAccretion (astrophysics)Starsgravitational waves13. Climate actionSpace and Planetary ScienceX-rays : star
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The close classical T Tauri binary V4046 Sgr: Complex magnetic fields & distributed mass accretion

2011

We report here the first results of a multi-wavelength campaign focussing on magnetospheric accretion processes within the close binary system V4046 Sgr, hosting two partly-convective classical T Tauri stars of masses ~0.9 Msun and age ~12 Myr. In this paper, we present time-resolved spectropolarimetric observations collected in 2009 September with ESPaDOnS at the Canada-France-Hawaii Telescope (CFHT) and covering a full span of 7d or ~2.5 orbital/rotational cycles of V4046 Sgr. Small circularly polarised Zeeman signatures are detected in the photospheric absorption lines but not in the accretion-powered emission lines of V4046 Sgr, thereby demonstrating that both system components host lar…

stars: formation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]stars: individual: V4046 SgrAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsstars: imagingtechniques: polarimetricSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar Astrophysicsstars: rotation[SDU]Sciences of the Universe [physics]stars: magnetic fieldsAstrophysics::Solar and Stellar Astrophysicstechniques: polarimetric stars: formation stars: imaging stars: individual: V4046 Sgr stars: magnetic fields stars: rotationAstrophysics::Earth and Planetary AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics
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Spectral analysis of the dipping LMXB system XB 1916-053

2019

Context: XB 1916-053 is a low mass X-ray binary system (LMXB) hosting a neutron star (NS) and showing periodic dips. The spectrum of the persistent emission was modeled with a blackbody component having a temperature between 1.31 and 1.67 keV and with a Comptonization component with an electron temperature of 9.4 keV and a photon index $\Gamma$ between 2.5 and 2.9. The presence of absorption features associated with highly ionized elements suggested the presence of partially ionized plasma in the system. Aims: In this work we performed a study of the spectrum of XB 1916-053, which aims to shed light on the nature of the seed photons that contribute to the Comptonization component. Methods: …

stars: individual: XB 1916-053Absorption spectroscopyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsX-rays: general01 natural sciencesSpectral lineformation identification Line neutron Stars Stars: individual: XB 1916-053 X-rays: binaries X-rays: generalX-rays: binariesstars: neutron0103 physical sciencesBlack-body radiationAbsorption (logic)010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstronomy and AstrophysicsNeutron starAbsorption edgeSpace and Planetary ScienceElectron temperatureline: formationAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]line: identification
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Spectral analysis of the AMXP during its 2018 outburst

2023

The Accreting Millisecond X-ray Pulsar IGR J17591-2342 is a Low Mass X-ray Binary (LMXB) system that went in outburst on 2018 August and it was monitored by the NICER observatory and partially by other facilities. We aim to study how the spectral emission of this source evolved during the outburst by exploiting the whole X-ray data repository of simultaneous observations. The continuum emission of the combined broad-band spectra is on average well described by an absorbed Comptonization component scattering blackbody-distributed photons peaking at (0.8 +/- 0.5) keV by a moderately optically thick corona (tau = 2.3 +/- 0.5) with temperature of (34 +/- 9) keV. A blackbody component with tempe…

stars: neutronX-rays: binariesSettore FIS/05 - Astronomia E Astrofisicaline: profilesline: formationstars: individual: IGR J17591-2342
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Contrastare le difficoltà di apprendimento in matematica degli studenti stranieri nel primo ciclo di istruzione

2016

Contrastare le difficoltà di apprendimento in matematica degli studenti stranieri nel primo ciclo di istruzione

successo formativo studenti stranieri problem solvingproblem solvingsuccesso formativosuccesso formativo studenti stranieri problem posing argomentazionestudenti stranieri
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Titanocene Selenide Sulfides Revisited: Formation, Stabilities, and NMR Spectroscopic Properties

2019

[TiCp2S5] (phase A), [TiCp2Se5] (phase F), and five solid solutions of mixed titanocene selenide sulfides [TiCp2SexS5−x] (Cp = C5H5−) with the initial Se:S ranging from 1:4 to 4:1 (phases B–E) were prepared by reduction of elemental sulfur or selenium or their mixtures by lithium triethylhydridoborate in thf followed by the treatment with titanocene dichloride [TiCp2Cl2]. Their 77Se and 13C NMR spectra were recorded from the CS2 solution. The definite assignment of the 77Se NMR spectra was based on the PBE0/def2-TZVPP calculations of the 77Se chemical shifts and is supported by 13C NMR spectra of the samples. The following complexes in varying ratios were identified in the CS2 solutions of …

sulfidit77Se-NMR spectroscopyPharmaceutical ScienceCrystal structureSulfidesorganometalliyhdisteet010402 general chemistry01 natural sciencesArticleAnalytical Chemistrylcsh:QD241-441Seleniumcrystal structureschemistry.chemical_compoundChalcogenlcsh:Organic chemistrytitanocene selenide sulfidesSelenide0103 physical sciencesDrug DiscoveryOrganometallic CompoundsCarbon-13 Magnetic Resonance SpectroscopyNMR-spektroskopiaPhysical and Theoretical Chemistryta116DLPNO-CCSD(T) calculations13C-NMR spectroscopyCrystallographyMolecular Structure010304 chemical physics<sup>13</sup>C-NMR spectroscopyChemistryChemical shiftOrganic ChemistryTitanocene dichlorideCarbon-13 NMRkiteetStandard enthalpy of formation0104 chemical sciencesNMR spectra databasetitaani<sup>77</sup>Se-NMR spectroscopyChemistry (miscellaneous)Carbon DisulfideseleeniQuantum TheoryMolecular MedicinePhysical chemistryMolecules
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Image formation with plasmonic nanostructures

2015

En 1873, Ernst Abbe concluyó que debido a la difracción de la luz el límite de resolución de un sistema óptico es aproximadamente la mitad de la longitud de onda de trabajo. Este límite, llamado el límite de difracción produce porque las ondas evanescentes no contribuyen a la formación de la imagen. En cualquier sistema óptico formado por materiales presentes en la naturaleza los detalles espaciales del objeto que sean más pequeños que el límite de resolución son transportados por ondas evanescentes. Normalmente estas ondas se pierden debido a la fuerte atenuación que experimentan viajando del objeto a la imagen. // En 1968, Veselago mostró que un material con permitividad y permeabilidad n…

superlentesUNESCO::FÍSICA::Óptica:FÍSICA::Óptica [UNESCO]PlasmónicasuperlensUNESCO::FÍSICA::Óptica ::Propiedades ópticas de los sólidos:FÍSICA::Óptica ::Propiedades ópticas de los sólidos [UNESCO]nanoestructurasimage formationplasmonicsFormación de imágenesnanoestructures
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Monitoraggio e percezione delle esperienze formative internazionali tra gli specializzandi italiani in igiene e medicina preventiva. Indagine condott…

2013

Introduzione Molti studi hanno dimostrato che le esperienze formative internazionali (International Health Electives - IHE) contribuiscono all'acquisizione di conoscenze e competenze fondamentali per i futuri professionisti in Sanità proprio attraverso l'opportunità di confronto fra sistemi sanitari e contesti socio-culturali differenti. Sebbene le IHE siano in crescita, non ci sono dati che riguardino quelle svolte dagli specializzandi italiani in Igiene. L'obiettivo dello studio è di raccogliere informazioni sulle loro pregresse esperienze formative internazionali e di comprendere motivazioni ed eventuali criticità relative alla decisione di effettuare una IHE. Materiali e metodi Gli spec…

survey attività formative internazionali medici in formazione igiene e medicina preventivaSettore MED/42 - Igiene Generale E Applicata
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