Search results for "ddc:5"

showing 10 items of 1717 documents

Uptake mechanism of ApoE-modified nanoparticles on brain capillary endothelial cells as a blood-brain barrier model.

2012

Background The blood-brain barrier (BBB) represents an insurmountable obstacle for most drugs thus obstructing an effective treatment of many brain diseases. One solution for overcoming this barrier is a transport by binding of these drugs to surface-modified nanoparticles. Especially apolipoprotein E (ApoE) appears to play a major role in the nanoparticle-mediated drug transport across the BBB. However, at present the underlying mechanism is incompletely understood. Methodology/Principal Findings In this study, the uptake of the ApoE-modified nanoparticles into the brain capillary endothelial cells was investigated to differentiate between active and passive uptake mechanism by flow cytome…

Apolipoprotein EDrugs and DevicesDrug Research and DevelopmentLipoproteinsMaterials Sciencelcsh:MedicinePlasma protein bindingBiologyBlood–brain barrierBiochemistryFlow cytometryApolipoproteins EMaterial by AttributeMiceApolipoproteins EDrug Delivery Systemsddc:570Cell Line TumormedicineAnimalsHumansNanotechnologyPharmacokineticsReceptorlcsh:ScienceBiologySerum AlbuminBrain DiseasesMultidisciplinaryMicroscopy Confocalmedicine.diagnostic_testlcsh:RBrainEndothelial CellsProteinsBiological TransportFlow CytometryCell biologymedicine.anatomical_structureBlood-Brain BarrierNanoparticles for drug delivery to the brainLDL receptorNanoparticlesMedicinelcsh:QProtein BindingResearch ArticleBiotechnologyPLoS ONE
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Science Advances

2019

River ecosystems receive and process vast quantities of terrestrial organic carbon, the fate of which depends strongly on microbial activity. Variation in and controls of processing rates, however, are poorly characterized at the global scale. In response, we used a peer-sourced research network and a highly standardized carbon processing assay to conduct a global-scale field experiment in greater than 1000 river and riparian sites. We found that Earth’s biomes have distinct carbon processing signatures. Slow processing is evident across latitudes, whereas rapid rates are restricted to lower latitudes. Both the mean rate and variability decline with latitude, suggesting temperature constrai…

Aquatic Ecology and Water Quality Managementriparian zonesORGANIC-MATTER DECOMPOSITIONBiodiversité et EcologieOceanografi hydrologi och vattenresurser/dk/atira/pure/sustainabledevelopmentgoals/life_on_landCarbon CycleCARBONekosysteemitOceanography Hydrology and Water Resourcesbiomesbiomitddc:570carbon cycleHumansSTREAMSLife ScienceHuman ActivitiesRiparian zonesTEMPERATUREInstitut für Biochemie und BiologieEcosystemComputingMilieux_MISCELLANEOUSSDG 15 - Life on Landaquatic ecosystemsScience & TechnologyWIMEKhiilen kiertovesiekosysteemitAquatic EcologyAquatische Ecologie en WaterkwaliteitsbeheerriversMultidisciplinary Sciencesekosysteemit (ekologia)BiomonitoringarticlesScience & Technology - Other Topics[SDE.BE]Environmental Sciences/Biodiversity and EcologyecosystemsjoetEnvironmental Monitoring
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Low-temperature Zr mobility: An in-situ synchrotron-radiation XRF study of the effect of radiation damage in zircon on the element release in $H_{2}O…

2006

The release of Zr, U, and Pb from nearly metamict zircon and its recrystallized analog and of Zr from fully crystalline and slightly radiation-damaged zircon in H 2 O + HCl ± SiO 2 fluids was investigated in situ at temperatures between 200 and 500 °C using a hydrothermal diamond-anvil cell and time-resolved synchrotron-radiation XRF analyses. Dissolution of nearly metamict zircon proceeded much faster than that of zircon with little or no radiation damage and resulted in a 1.5 to 2 log units higher Zr molality in 6 to 7 m HCl fluids. Extensive recrystallization of the almost fully amorphous material started at 260 to 300 °C in H 2 O + HCl, and at about 360 °C if quartz was added, and was c…

Aqueous solutionAnalytical chemistryRecrystallization (metallurgy)Mineralogy550 - Earth sciencesHydrothermal circulationAmorphous solidMetamictizationGeophysicsGeochemistry and Petrologyddc:550QuartzDissolutionGeologyZircon
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A no-carrier-added72Se/72As radionuclide generator based on solid phase extraction

2005

Summary72As-labelled radiopharmaceuticals could be a valuable resource for Positron Emission Tomography (PET). In particular, the long half-life of72As (T1/2= 26 h) facilitates the observation of long-term physiological or metabolic processes, such as the enrichment and distribution of antibodies in tumor tissue. This work describes the primary radiochemical separation of no-carrier-added (nca)72Se from cyclotron irradiated germanium targets and the development of a polystyrene type solid-phase extraction based72Se/72As radionuclide generator, avoiding the addition of any selenium carrier. The irradiated germanium target is dissolved in HFconcand selenium is reduced with hydrazine dihydroch…

Aqueous solutionChemistryElutionExtraction (chemistry)Radiochemistrychemistry.chemical_elementJYield (chemistry)ddc:540Solid phase extractionPhysical and Theoretical ChemistryRadionuclide GeneratorArsenicSeleniumNuclear chemistryRadiochimica Acta
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Solubilization control by redox-switching of polysoaps

2008

Reversible changes in the self-organization of polysoaps may be induced by controlling their charge numbers via covalently bound redox moieties. This is illustrated with two viologen polysoaps, which in response to an electrochemical stimulus, change their solubility and aggregation in water, leading from homogeneously dissolved and aggregated molecules to collapsed ones and vice verse. Using the electrochemical quartz crystal microbalance (EQCM), it could be shown that the reversibility of this process is better than 95% in 16 cycles.

Aqueous solutionPolymers and PlasticsChemistryInorganic chemistryViologenGeneral ChemistryQuartz crystal microbalanceCondensed Matter PhysicsElectrochemistryPhotochemistryRedoxCovalent bondddc:540Materials ChemistrymedicineMoleculeInstitut für ChemieSolubilitymedicine.drug
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1200 years of decadal-scale variability of Mediterranean vegetation and climate at Pantelleria Island, Italy.

2013

A new sedimentary sequence from Lago di Venere on Pantelleria Island, located in the Strait of Sicily between Tunisia and Sicily was recovered. The lake is located in the coastal infra-Mediterranean vegetation belt at 2 m a.s.l. Pollen, charcoal and sedimentological analyses are used to explore linkages among vegetation, fire and climate at a decadal scale over the past 1200 years. A dry period from ad 800 to 1000 that corresponds to the 'Medieval Warm Period' (WMP) is inferred from sedimentological analysis. The high content of carbonate recorded in this period suggests a dry phase, when the ratio of evaporation/precipitation was high. During this period the island was dominated by thermop…

ArcheologyInstitut für Erd- und UmweltwissenschaftenSettore AGR/05 - Assestamento Forestale E Selvicoltura'Little Ice Age' (LIA)'Medieval Warm Period' (MWP)Climate changePinus pinasterQuercus pubescenschemistry.chemical_compoundcentral Mediterraneancentral Mediterranean fire history ‘Little Ice Age’ (LIA) ‘Medieval Warm Period’ (MWP) Pinus pinaster Quercus ilex Quercus pubescens vegetation historyddc:550Precipitationvegetation historyEarth-Surface ProcessesGlobal and Planetary ChangeEcologybiologyEcologyPaleontologySedimentPlant communityVegetationbiology.organism_classificationQuercus ilexfire historychemistryQuercus pubescensPeriod (geology)CarbonateInstitut für GeowissenschaftenPhysical geographyGeology
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Competitive relaxation processes of oxygen deficient centers in silica

2003

Physical review / B 67, 033202 (2003). doi:10.1103/PhysRevB.67.033202

Arrhenius equationMaterials sciencePhotoluminescenceQuenching (fluorescence)Oxygen deficientRelaxation (NMR)530symbols.namesakeAmplitudeExcited statesymbolsddc:530Atomic physicsLuminescencePhysical Review B
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SAN plot: A graphical representation of the signal, noise, and artifacts content of spectra

2019

The signal-to-noise ratio is an important property of NMR spectra. It allows to compare the sensitivity of experiments, the performance of hardware, etc. Its measurement is usually done in a rudimentary manner involving manual operation of selecting separately a region of the spectrum with signal and noise, respectively, applying some operation and returning the signal-to-noise ratio. We introduce here a simple method based on the analysis of the distribution of point intensities in one- and two-dimensional spectra. The signal/artifact/noise plots, (SAN plots) allows one to present in a graphical manner qualitative and quantitative information about spectra. It will be shown that besides me…

Artifact (error)ChemistryNoise (signal processing)General ChemistrySignalPlot (graphics)NMRSignal-to-noise ratioSAN plotddc:540General Materials SciencePoint (geometry)Representation (mathematics)AlgorithmSensitivity (electronics)
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Measurement of the atmospheric ?µ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope

2013

Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric energy spectrum in the energy range 0.1-200 TeV is presented, using data collected by the ANTARES underwater neutrino telescope from 2008 to 2011. Overall, the measured flux is similar to 25 % higher than predicted by the conventional neutrino flux, and compatible with the measurements reported in ice. The flux is compatible with a single power-law dependence with spectral index gamma (meas)=3.58 +/- 0.12. With the present statistics the contribution of prompt neutrinos cannot be established.

Astrofísica:Desenvolupament humà i sostenible::Medi ambient [Àrees temàtiques de la UPC]Physics and Astronomy (miscellaneous)Raigs còsmicsFluxOceanografia7. Clean energy01 natural scienceslaw.inventionlawUnderwater acousticsEnergy range 0.1 to 200 TeVNeutrino TelescopePhysicsRange (particle radiation)Spectral index[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]atmospheric neutrinoNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsLorentz Invariance ViolationFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]OscillationsSoroll -- Aspectes ambientalsAstrophysics::High Energy Astrophysical PhenomenaCosmic rayddc:500.2MACRONuclear physicsTelescopeMUONSSEARCH0103 physical sciencesNeutrinsNeutrinos010306 general physicsEngineering (miscellaneous)Cosmic raysDETECTOR:Física::Acústica [Àrees temàtiques de la UPC]ANTARESAtmospheric neutrino antineutrino010308 nuclear & particles physicsAntares telescopeHigh Energy Physics::Phenomenology[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionFISICA APLICADAlorentz invariance violation; neutrino oscillation; muonsHigh Energy Physics::ExperimentEnergy (signal processing)Bar (unit)European Physical Journal C
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A first search for coincident gravitational waves and high energy neutrinos using LIGO, Virgo and ANTARES data from 2007

2013

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two sup…

AstrofísicaEXPLOSIONSHigh energyPhotonPOINT SOURCESSUPERCONDUCTING COSMIC STRINGSGravitational waves / experimentsGravitational waves/experimentsAstrophysics01 natural scienceshigh energy neutrinosgravitational wavesgravitational waves / experiment010303 astronomy & astrophysicsQCmedia_commonLine (formation)QBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)GAMMA-RAY BURSTSdark matter detectorsGravitational waves / experiments; Neutrino astronomy; Astronomy and Astrophysicshigh energy neutrinos[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsgravitational waves; gravitational waves / experiments; neutrino astronomy; high energy neutrinos; high energy neutrinosgravitational wavesgravitational wavesparticle physics - cosmology connectionNeutrino astronomyCOSMIC STRINGSRELATIVISTIC JETSNeutrinoAstrophysics - High Energy Astrophysical Phenomenasupersymmetry and cosmology[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]gravitational waves / experiments; neutrino astronomyTELESCOPEmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaSCIENCE RUNFOS: Physical sciencesddc:500.2GAMMA-RAY BURSTS; CORE-COLLAPSE SUPERNOVAE; SUPERCONDUCTING COSMIC STRINGS; MAGNETAR GIANT FLARES; SCIENCE RUN; RELATIVISTIC JETS; POINT SOURCES; BLACK-HOLES; LOCAL-RATE; TELESCOPEGravitational wavesGeneral Relativity and Quantum CosmologyCORE-COLLAPSE SUPERNOVAESettore FIS/05 - Astronomia e AstrofisicaCoincidentneutrino experiments0103 physical sciences010306 general physicsMAGNETAR GIANT FLARESBLACK-HOLESHigh Energy Astrophysical PhenomenaGravitational waveAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsDRIVENUniverseLIGOGIANT FLARESLOCAL-RATEFISICA APLICADALUMINOSITYRADIATIONHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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