Search results for " profiles"

showing 10 items of 118 documents

La valutazione neuropsicologica tra significatività statistica e clinica

2008

Aspetti statistici e clinici pervadono tutte le fasi della valutazione neuropsicologica, dalla scelta dei test alla loro restituzione. Il presente articolo, utilizzando i dati di due ricerche come esempio, mette in evidenza l’importanza di ognuno dei due aspetti e di come questi influenzino le diverse fasi del processo di valutazione neuropsicologica e soprattutto la decisione finale e l’eventuale intervento.

Neuropsychological assessment statistical significance clinical significance neuropsychological profiles test sensitivity
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Comparison of LIBS results on ITER-relevant samples obtained by nanosecond and picosecond lasers

2019

This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement number 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission. Work performed under EUROfusion WP PFC.

Nuclear and High Energy PhysicsMaterials scienceMaterials Science (miscellaneous)chemistry.chemical_element01 natural sciences010305 fluids & plasmaslaw.inventionPulsed laser depositionsymbols.namesakeLIBS diagnosticslaw0103 physical sciences:NATURAL SCIENCES:Physics [Research Subject Categories]Temperature of laser-produced plasmaLaser-induced breakdown spectroscopyta216010302 applied physicsArgonta114Pulse durationNanosecondLaserlcsh:TK9001-9401Nuclear Energy and EngineeringchemistryStark effectPicosecondITER-relevant coatingssymbolslcsh:Nuclear engineering. Atomic powerDetection of hydrogen isotopesElemental depth profilesAtomic physicsNuclear Materials and Energy
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Revealing Employer’s Name in Social Networks

2017

Abstract The research investigates the question of the importance of mentioning the name of the employer in online and offline social networks. The exchange of information is an important part of social networks and social capital theory. Companies can use the networks of their employees to recruit new hires and to check habits and interests of likely new employees. To do that, the employee has to mention the name of the company in these social networks. The paper compares different real social networks used by family and friends and private and business social network sites (SNSs) as online social networks and compares the differences between men and women. The empirical research has been …

Online and offlinesocial networksHF5001-6182050801 communication & media studiesSocial networks0508 media and communicationsEmpirical researchhuman resource management0502 economics and businessBusinessSociologyHB71-74Social computingSocial networkDescriptive statisticsbusiness.industry05 social sciencesPublic relationsvirtual profilesEconomics as a scienceHuman resource managementSurvey data collectionsocial network sitesbusiness050203 business & managementSocial capitalEconomics and Business
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Theoretical profiles of the Mg + resonance lines perturbed by collisions with He

2016

International audience; The effects of collision broadening by He are central to understanding the opacity of cool stellar atmospheres. Aims. DZ white dwarfs show metal lines which are, in many cases, believed to come from some rocky material, a remnant of a former exoplanetary system. The analysis of the Mg + resonance lines is a valuable method to determine the chemical abundances in these systems. Methods. Unified profiles of the strongest of the UV lines of Mg + have been calculated in the semi-classical approach using very recent ab initio potential energies. Results. We present the first theoretical line profile calculations of the resonance lines of Mg + that have been perturbed by h…

Opacity[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Ab initiochemistry.chemical_elementAstrophysics01 natural sciencesResonance (particle physics)Metal0103 physical sciencesstars: atmospheresAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsHeliumAstrophysics::Galaxy AstrophysicsLine (formation)white dwarfsPhysicsStellar atmosphereWhite dwarfAstronomy and Astrophysicsline: profileschemistry13. Climate actionSpace and Planetary Sciencevisual_artvisual_art.visual_art_mediumAstrophysics::Earth and Planetary AstrophysicsAtomic physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Silesian Texans – przyczynek do relacji o stanie zachowania muzycznej kultury

2019

Śląscy Teksańczycy, od ponad 150 lat mieszkający w okolicach San Antonio w Teksasie, to dziś grupa szacowana przez niektórych badaczy na ok. 200 tysięcy (1%) mieszkańców tego stanu. Osie-dlali się zwykle grupowo, w przeciwieństwie do tzw. emigrantów brazylijskich z podobnego czasu. Tak powstały i istnieją do dziś osady o nazwach: Panna Maria (tu się wszystko zaczęło), Cesto-chowa, St. Hedwig, Kościuszko, Bandera i inne. Historię osadnictwa, losów rodzin, zachowania języka i kultury materialnej ujmują publikacje, niejednokrotnie niezwykle szczegółowe. Trudno podobny sąd wyrazić o badaniach stanu zachowania kultury muzycznej. Jednocześnie szczątkowe dane, zebrane niejednokrotnie niejako przy …

Panna Mariamusical cultureThe Father Leopold Moczygemba FoundationFranciszek KurzajSilesiamuzyczna kulturaŚląscy TeksańczycyAmerican PoloniaŚląskSan AntonioSilesian TexansPolonia amerykańskaSilesian ProfilesLiturgia Sacra. Liturgia -Musica -Ars
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Half-width plots, a simple tool to predict peak shape, reveal column kinetics and characterise chromatographic columns in liquid chromatography: Stat…

2013

Peak profiles in chromatography are characterised by their height, position, width and asymmetry; the two latter depend on the values of the left and right peak half-widths. Simple correlations have been found between the peak half-widths and the retention times. The representation of such correlations has been called half-width plots. For isocratic elution, the plots are parabolic, although often, the parabolas can be approximated to straight-lines. The plots can be obtained with the half-widths/retention time data for a set of solutes experiencing the same kinetics, eluted with a mobile phase at fixed or varying composition. When the analysed solutes experience different resistance to mas…

Peak profiles in chromatography are characterised by their height position width and asymmetry; the two latter depend on the values of the left and right peak half-widths. Simple correlations have been found between the peak half-widths and the retention times. The representation of such correlations has been called half-width plots. For isocratic elution the plots are parabolic although often the parabolas can be approximated to straight-lines. The plots can be obtained with the half-widths/retention time data for a set of solutes experiencing the same kinetics eluted with a mobile phase at fixed or varying composition. When the analysed solutes experience different resistance to mass transfer the plots will be solute dependent and should be obtained with the data for each solute eluted with mobile phases at varying composition. The half-width plots approach is a simple tool that facilitates the prediction of peak shape (width and asymmetry) with optimisation purposes reveal the interaction kinetics of solutes in different columns and characterise chromatographic columns. This work shows half-width plots for different situations in isocratic elution including the use of different flows the effect of temperature the modification of the stationary phase surface by an additive the existence of specific interactions within the column and the comparison of columns. The adaptation to gradient elution is also described. Previous knowledge on half-width plots is structured and analysed to which new results are added.Work (thermodynamics)Column characterisationmedia_common.quotation_subjectKineticsLiquid chromatographyAnalytical chemistryHalf-widthsInteraction kineticsBiochemistryAsymmetryAnalytical ChemistryPeak shapeColumn (typography)Position (vector)Mass transferPhase (matter)media_commonChromatographyElutionChemistryOrganic ChemistryGeneral MedicineModels TheoreticalKineticsPredictionChromatography LiquidJournal of Chromatography A
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Personality profiles of dyslexic children: a study with the Big Five Questionnaire

2009

Personality profiles dyslexicSettore MED/39 - Neuropsichiatria Infantile
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XMM-Newton detects a relativistically broadened iron line in the spectrum of the ms X-ray pulsar SAX J1808.4-3658

2008

We report on a 63-ks long XMM-Newton observation of the accreting millisecond pulsar SAX J1808.4-3658 during the latest X-ray outburst which started on September 21st 2008. The pn spectrum shows a highly significant emission line in the energy band where the iron K-alpha line is expected, and which we identify as emission from neutral (or mildly ionized) iron. The line profile appears to be quite broad (more than 1 keV FWHM) and asymmetric; the most probable explanation for this profile is Doppler and relativistic broadening from the inner accretion disc. From a fit with a diskline profile we find an inner radius of the disc of 8.7^(+3.7)_(-2.7) R_g, corresponding to 18.0^(+7.6)_(-5.6) km f…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)accretion accretion disks line: profiles stars: pulsars: individual: SAX J1808.4-3658 relativity X-rays: binariesFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsRadiusAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicssymbols.namesakeNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceMillisecond pulsarIonizationsymbolsAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAstrophysics::Earth and Planetary AstrophysicsDoppler effectAstrophysics::Galaxy AstrophysicsX-ray pulsarLine (formation)
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Large-scale normal fluid circulation in helium superflows

2017

We perform fully-coupled numerical simulations of helium II pure superflows in a channel, with vortex- line density typical of experiments. Peculiar to our model is the computation of the back-reaction of the superfluid vortex motion on the normal fluid and the presence of solid boundaries. We recover the uniform vortex-line density experimentally measured employing second sound resonators and we show that pure superflow in helium II is associated with a large-scale circulation of the normal fluid which can be detected using existing particle-tracking visualization techniques.

PhysicsComputationnormal and superfluid profilesFOS: Physical scienceschemistry.chemical_elementMechanics01 natural sciences010305 fluids & plasmasVortexCondensed Matter - Other Condensed MatterSuperfluidityResonatorClassical mechanicsCirculation (fluid dynamics)chemistry0103 physical sciencesSecond soundvortex pointpure superflow010306 general physicsSettore MAT/07 - Fisica MatematicaHeliumOther Condensed Matter (cond-mat.other)Line (formation)Superfluid Helium
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A relativistic iron emission line from the neutron star low-mass X-ray binary GX 3+1

2012

We present the results of a spectroscopic study of the Fe K{\alpha} emission of the persistent neutron-star atoll low-mass X-ray binary and type I X-ray burster GX 3+1 with the EPIC-PN on board XMM-Newton. The source shows a flux modulation over several years and we observed it during its fainter phase, which corresponds to an X-ray luminosity of Lx~10^37 ergs/s. When fitted with a two-component model, the X-ray spectrum shows broad residuals at \sim6-7 keV that can be ascribed to an iron K{\alpha} fluorescence line. In addition, lower energy features are observed at \sim3.3 keV, \sim3.9 keV and might originate from Ar XVIII and Ca XIX. The broad iron line feature is well fitted with a rela…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical Phenomenaidentification line: profiles X-rays: individuals: GX 3+1 X-rays: binaries stars: neutron [line]X-ray binaryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsRadiusAstrophysics::Cosmology and Extragalactic AstrophysicsType (model theory)01 natural sciencesLuminosityNeutron starSettore FIS/05 - Astronomia E Astrofisicaline: identification line: profiles X-rays: individuals: GX 3+1 X-rays: binaries stars: neutronSpace and Planetary Science0103 physical sciencesEmission spectrumAstrophysics - High Energy Astrophysical PhenomenaLow Mass010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsLine (formation)
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