Search results for "methods [Gene Expression Profiling]"

showing 10 items of 838 documents

1981

A new interferometer has been designed in order to perform measurements of refractive indices and refractive index increments on liquid systems under elevated pressure at different temperatures. The method of measurement, the calibration of the instrument and the treatment of data are described. With a series of test measurements on trans-decalin it is shown that with this instrument reliable results are obtained.

chemistry.chemical_compoundInterferometryTemperature and pressureOpticsMaterials scienceDecalinchemistrybusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsCalibrationFunction (mathematics)businessRefractive indexDie Makromolekulare Chemie
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L’ADULTO COME SPECCHIO. MODALITÀ COMUNICATIVE E APPRENDIMENTO

2021

Numerose ricerche sull’infanzia condotte a partire dal secolo scorso, hanno mostrato come i bambini, fin dai primi mesi di vita, siano attivi e propositivi nella interazione con gli altri esseri umani. In una prospettiva educativa, di promozione dei processi di apprendimento e di sostegno alla costruzione di una immagine di sé positiva e fiduciosa nelle proprie potenzialità, sono di grande importanza le modalità comunicative e relazionali degli adulti significativi. A tali modalità farò riferimento nel mio contributo, soffermandomi sul rispecchiamento verbale e non verbale, nelle sue diverse forme, approfondendone le ragioni teoriche e metodologiche e riflettendo su come possa attuarsi una …

corpo e linguaggiodevelopment and learningbody and languageverbal and non-verbal mirroringsviluppo e apprendimentoAdult-child relationshiprispecchiamento verbale e non verbale.Relazione adulto-bambinomodalità comunicative in ambito educativoSettore M-PED/01 - Pedagogia Generale E Socialecommunication methods in the educational field
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Status of Advanced Virgo

2017

The LIGO and the Virgo collaborations have recently announced the first detections of Gravitational Waves. Due to their weak amplitude, Gravitational Waves are expected to produce a very small effect on free-falling masses, which undergo a displacement of the order of 10-18 m for a Km-scale mutual distance. This discovery showed that interferometric detectors are suitable to reveal such a feeble effect, and therefore represent a new tool for astronomy, astrophysics and cosmology in the understanding of the Universe. To better reconstruct the position of the Gravitational Wave source and increase the signal-to-noise ratio of the events by means of multiple coincidence, a network of detectors…

cosmological modeldetector: performanceVirgo LIGO gravitational waveAstronomyinterferometerQC1-999detector: networkgravitational radiation: direct detection01 natural sciencesCoincidenceCosmologyPhysics and Astronomy (all)0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]LIGO010306 general physicsSettore FIS/01Physics010308 nuclear & particles physicsGravitational wavePhysicsDetectorgravitational radiationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomygravitational radiation detectorLIGOdetector: sensitivityInterferometryVIRGOAmplitudePhysics and Astronomygravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory

2019

With the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between 1017 eV and 1020 eV from point-like sources across the sky, from close to the Southern Celestial Pole up to 60 in declination, with peak sensitivities at declinations around ∼-53 and ∼+55, and an unmatched sensitivity for arrival directions in the Northern hemisphere. A search has been performed for highly-inclined air showers induced by neutrinos of all flavours with no candidate events found in data taken between 1 Jan 2004 and 31 Aug 2018. Upper limits on the neutrino flux from point-like steady sources have been derived as a function of source declination. An unrivaled sensit…

cosmological neutrinosAstronomypoleFluxAstrophysics01 natural sciencesneutrino: fluxcosmic ray experiments; cosmological neutrinos; neutrino astronomy; ultra high energy cosmic raysmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSastro-ph.HEcosmological neutrinoSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAYSneutrino: UHEAugerobservatoryNEUTRINOSNeutrinoAstrophysics - High Energy Astrophysical Phenomenaairmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical Phenomenacosmic ray experimentFOS: Physical sciencesultra high energy cosmic raysDeclinationneutrino astronomyCelestial pole0103 physical sciencesflux: upper limitHigh Energy PhysicsDETECTORZenithAstrophysiquePierre Auger Observatoryflavorshowers: atmosphere010308 nuclear & particles physicsdetector: surfaceNorthern HemisphereAstronomy and AstrophysicsAstronomiesensitivitySkyExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Promoting the Cultural Understanding of a Student in a General Education School: Teachers’ Experiences and Challenges

2020

Cultural understanding is a basis for competence-oriented general education. Teachers are responsible for applied content and methods that are used to purposefully lead school students to that result.The aim of this study is to identify actual goals for the development of teacher education curriculum, professional development, and teaching aids by investigating in-service teachers’ challenges in the successful promotion of students’ cultural understanding in general schools.The readiness of teachers to promote the cultural understanding of primary school students was explored in a mixed-methods study. The findings indicated aspects that teachers consider relevant as well as the main problem…

cultural understandingmedia_common.quotation_subject05 social sciencesProfessional development050301 educationGeneral education010501 environmental sciencesmixed-methods study01 natural sciencesTeacher educationlcsh:Education (General)EducationSchool teachersPromotion (rank)PedagogyComputingMilieux_COMPUTERSANDEDUCATIONPsychologylcsh:L7-9910503 educationCurriculumgeneral educationteachers’ experience0105 earth and related environmental sciencesmedia_commonActa Paedagogica Vilnensia
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Computational Techniques for the Analysis of Small Signals in High-Statistics Neutrino Oscillation Experiments

2020

The current and upcoming generation of Very Large Volume Neutrino Telescopes – collecting unprecedented quantities of neutrino events – can be used to explore subtle effects in oscillation physics, such as (but not restricted to) the neutrino mass ordering. The sensitivity of an experiment to these effects can be estimated from Monte Carlo simulations. With the high number of events that will be collected, there is a trade-off between the computational expense of running such simulations and the inherent statistical uncertainty in the determined values. In such a scenario, it becomes impractical to produce and use adequately-sized sets of simulated events with traditional methods, such as M…

data analysis methodNuclear and High Energy PhysicsMonte Carlo methodFVLV nu TData analysis; Detector; KDE; MC; Monte Carlo; Neutrino; Neutrino mass ordering; Smoothing; Statistics; VLVνTData analysisKDEFOS: Physical sciences01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)statistical analysisnumerical methods0103 physical sciencesStatisticsNeutrinoddc:530Sensitivity (control systems)MC010306 general physicsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMonte CarloPhysicsVLVνT010308 nuclear & particles physicsOscillationStatisticsoscillation [neutrino]ObservableDetectorMonte Carlo [numerical calculations]WeightingNeutrino mass orderingPhysics and AstronomyPhysics - Data Analysis Statistics and ProbabilityPhysique des particules élémentairesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsMATTERData Analysis Statistics and Probability (physics.data-an)SmoothingSmoothing
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Intrinsic backgrounds from Rn and Kr in the XENON100 experiment

2018

In this paper, we describe the XENON100 data analyses used to assess the target-intrinsic background sources radon ([InlineMediaObject not available: see fulltext.]), thoron ([InlineMediaObject not available: see fulltext.]) and krypton ([InlineMediaObject not available: see fulltext.]). We detail the event selections of high-energy alpha particles and decay-specific delayed coincidences. We derive distributions of the individual radionuclides inside the detector and quantify their abundances during the main three science runs of the experiment over a period of ∼4years, from January 2010 to January 2014. We compare our results to external measurements of radon emanation and krypton concentr…

data analysis methodPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)WIMPFOS: Physical scienceschemistry.chemical_elementlcsh:AstrophysicsRadonSciences de l'ingénieur01 natural sciencesIonNuclear physicsradon: nuclideXENONlcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Engineering (miscellaneous)nuclidebackground: radioactivitybackground: suppressionkryptonPhysicsRadionuclidePhysique010308 nuclear & particles physicsKryptonInstrumentation and Detectors (physics.ins-det)Alpha particleAstronomieDark Matter direct search experimentrespiratory tract diseasesRadon DaughtersBackgroundchemistrylcsh:QC770-798TPCAstrophysics - Instrumentation and Methods for Astrophysics
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Search for magnetically-induced signatures in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory

2020

We search for signals of magnetically-induced effects in the arrival directions of ultra-high-energy cosmic rays detected at the Pierre Auger Observatory. We apply two different methods. One is a search for sets of events that show a correlation between their arrival direction and the inverse of their energy, which would be expected if they come from the same point-like source, they have the same electric charge and their deflection is relatively small and coherent. We refer to these sets of events as "multiplets". The second method, called "thrust", is a principal axis analysis aimed to detect the elongated patterns in a region of interest. We study the sensitivity of both methods using a …

electric [charge]AstronomydeflectionThrustmagnetic fieldAstrophysics01 natural sciencesmass spectrumhelium: nucleusbenchmarksurface [detector]Cosmic ray experimentsUltra-high-energy cosmic ray010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstrophysics::Instrumentation and Methods for AstrophysicsCosmic ray experiments; Ultra high energy cosmic raysAugerobservatoryacceleration [cosmic radiation]Astrophysics - High Energy Astrophysical PhenomenasignaturePrincipal axis theoremActive galactic nucleusCherenkov counter: waterAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]energy spectrumFOS: Physical sciencesnucleus [helium]Cosmic rayElectric chargeCosmic ray experimentGLASTdetector: fluorescence0103 physical sciencesddc:530thrustcosmic radiation: UHEHigh Energy Physicscosmic radiation: accelerationAGNAstrophysiquePierre Auger Observatoryfluorescence [detector]010308 nuclear & particles physicsdetector: surfacecharge: electricwater [Cherenkov counter]Astronomy and AstrophysicsUltra high energy cosmic raysAstronomiesensitivityGalaxycoherencefluxgamma raymultipletcorrelationExperimental High Energy Physicsgalaxy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOS
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Offensive Transitions in High-Performance Football: Differences Between UEFA Euro 2008 and UEFA Euro 2016

2019

[Abstract] Coaches, footballers and researchers agree that offensive transitions are one of the most important moments in football today. In a sport where defense over attack dominates, with low scores on the scoreboard, the importance of these actions from the offensive point of view becomes very important. Despite this, scientific literature is still very limited on this topic. Therefore, the objectives set out in the present investigation have been two: first, by means of a proportion analysis and the application of a chisquare test, it was intended to describe the possible differences between the offensive transitions made in the UEFA Euro 2008 and UEFA Euro 2016; then, through differen…

footballMixed methodsmixed methodslcsh:BF1-990FootballMixed methods researchFootballScientific literaturePhase (combat)050105 experimental psychologyObservational methodologyCompetition (economics)03 medical and health sciencesHigh performance0302 clinical medicineSoccerEconometricsPsychologyObservació (Mètode científic)Sport strategyObservation (Scientific method)0501 psychology and cognitive sciencesSet (psychology)Observational methodologyGeneral PsychologyOriginal ResearchEstratègia esportiva05 social sciencesOffensiveoffensive transitionsQuarter (United States coin)Offensive transitionslcsh:PsychologyFutbolobservational methodologyPsychologyInvestigació amb mètodes mixtoshigh performance030217 neurology & neurosurgeryFrontiers in Psychology
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Pinpointing the SMBH in NGC1052

2016

Supermassive black holes (SMBH) are essential for the production of jets in radio-loud active galactic nuclei (AGN). Theoretical models based on Blandford & Znajek (1977MNRAS.179..433B) extract the rotational energy from a Kerr black hole, which could be the case for NGC1052, to launch these jets. This requires magnetic fields on the order of 1000G to 10000G. We imaged the vicinity of the SMBH of the AGN NGC1052 with the Global Millimetre VLBI Array and found a bright and compact central feature that is smaller than 1.9 light days (100 Schwarzschild radii) in radius. Interpreting this as a blend of the unresolved jet bases, we derive the magnetic field at 1 Schwarzschild radius to lie betwe…

galactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxiesComputer Science::Digital Librariesobservational astronomyGeneral Relativity and Quantum CosmologyRadio galaxiesNatural SciencesAstrophysics::Galaxy AstrophysicsVery long baseline interferometry
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