Search results for " data analysis"

showing 10 items of 231 documents

Search for pulsations at high radio frequencies from accreting millisecond X-ray pulsars in quiescence

2010

It is commonly believed that millisecond radio pulsars have been spun up by transfer of matter and angular momentum from a low-mass companion during an X-ray active mass transfer phase. A subclass of low-mass X-ray binaries is that of the accreting millisecond X-ray pulsars, transient systems that show periods of X-ray quiescence during which radio emission could switch on. The aim of this work is to search for millisecond pulsations from three accreting millisecond X-ray pulsars, XTE J1751-305, XTE J1814-338, and SAX J1808.4-3658, observed during their quiescent X-ray phases at high radio frequencies (5 - 8 GHz) in order to overcome the problem of the free-free absorption due to the matter…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MillisecondAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsLuminosityInterstellar medium85-05pulsars general methods data analysis methods observational stars neutron X-rays binariesNeutron starSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary ScienceMillisecond pulsarAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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Monte Carlo Markov Chain DEM reconstruction of isothermal plasmas

2012

In this paper, we carry out tests on the Monte Carlo Markov Chain (MCMC) technique with the aim of determining: 1) its ability to retrieve isothermal plasmas from a set of spectral line intensities, with and without random noise; 2) to what extent can it discriminate between an isothermal solution and a narrow multithermal distribution; and 3) how well it can detect multiple isothermal components along the line of sight. We also test the effects of 4) atomic data uncertainties on the results, and 5) the number of ions whose lines are available for the DEM reconstruction. We find that the MCMC technique is unable to retrieve isothermal plasmas to better than Delta log T = 0.05. Also, the DEM…

PhysicsLine-of-sightGaussianmethods: data analysis techniques: spectroscopic Sun: corona Sun: UV radiationFOS: Physical sciencesAstronomy and AstrophysicsMarkov chain Monte CarloPlasmaAstrophysicsSpectral lineIsothermal processComputational physicsIondata analysis techniques: spectroscopic Sun: corona Sun: UV radiation [methods]symbols.namesakeDistribution (mathematics)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencesymbolsSolar and Stellar Astrophysics (astro-ph.SR)
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Goodness-of-fit tests in many dimensions

2004

A method is presented to construct goodness-of-fit statistics in many dimensions for which the distribution of all possible test results in the limit of an infinite number of data becomes Gaussian if also the number of dimensions becomes infinite. Furthermore, an explicit example is presented, for which this distribution as good as only depends on the expectation value and the variance of the statistic for any dimension larger than one.

PhysicsNuclear and High Energy PhysicsGaussianFOS: Physical sciencesProbability and statisticsVariance (accounting)Expectation valuesymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Goodness of fitPhysics - Data Analysis Statistics and ProbabilitysymbolsLimit (mathematics)Statistical physicsDimension (data warehouse)InstrumentationData Analysis Statistics and Probability (physics.data-an)Statistic
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Monte Carlo simulation of virtual Compton scattering below pion threshold

2006

This paper describes the Monte Carlo simulation developed specifically for the VCS experiments below pion threshold that have been performed at MAMI and JLab. This simulation generates events according to the (Bethe-Heitler + Born) cross section behaviour and takes into account all relevant resolution-deteriorating effects. It determines the `effective' solid angle for the various experimental settings which are used for the precise determination of photon electroproduction absolute cross section.

PhysicsNuclear and High Energy PhysicsPhoton010308 nuclear & particles physicsMonte Carlo methodCompton scatteringSolid angleProbability and statistics01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsPionPhysics - Data Analysis Statistics and Probability[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]0103 physical sciencesNuclear Experiment010306 general physicsInstrumentation[PHYS.PHYS.PHYS-DATA-AN]Physics [physics]/Physics [physics]/Data Analysis Statistics and Probability [physics.data-an]Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Partition function based analysis of cosmic microwave background maps

1999

We present an alternative method to analyse cosmic microwave background (CMB) maps. We base our analysis on the study of the partition function. This function is used to examine the CMB maps, making use of the different information embedded at different scales and moments. Using the partition function in a likelihood analysis in two dimensions (Qrms-PS, n), we find the best-fitting model to the best data available at present (the COBE–DMR 4 years data set). By means of this analysis we find a maximum in the likelihood function for n=1.8-0.65+0.35 and Qrms-PS = 10-2.5+3μ K (95 per cent confidence level) in agreement with the results of other similar analyses [Smoot et al. (1 yr), Bennet et a…

PhysicsPartition function (quantum field theory)Cosmic microwave backgroundFísicaAstronomy and AstrophysicsMultifractal systemFunction (mathematics)Measure (mathematics)Cosmic microwave backgroundData setTheoretical physicsDistribution (mathematics)Methods: data analysisSpace and Planetary ScienceStatistical physicsdata analysis [Methods]Likelihood functionMonthly Notices of the Royal Astronomical Society
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Hierarchy and dynamics of trace distance correlations

2013

We define and analyze measures of correlations for bipartite states based on trace distance. For Bell diagonal states of two qubits, in addition to the known expression for quantum correlations using this metric, we provide analytic expressions for the classical and total correlations. The ensuing hierarchy of correlations based on trace distance is compared to the ones based on relative entropy and Hilbert-Schmidt norm. Although some common features can be found, the trace distance measure is shown to differentiate from the others in that the closest uncorrelated state to a given bipartite quantum state is not given by the product of the marginals, and further, the total correlations are s…

PhysicsQuantum PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciKullback–Leibler divergenceStatistical Mechanics (cond-mat.stat-mech)DiagonalGeneral Physics and AstronomyFOS: Physical sciencesProbability and statisticsMathematical Physics (math-ph)Entanglement measures witnesses and other characterizationQuantum stateQubitNorm (mathematics)Physics - Data Analysis Statistics and ProbabilityFoundations of quantum mechanicTrace distancemeasurement theoryStatistical physicsEntanglement and quantum nonlocalityQuantum Physics (quant-ph)QuantumCondensed Matter - Statistical MechanicsMathematical PhysicsData Analysis Statistics and Probability (physics.data-an)
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Active Brownian Motion Models and Applications to Ratchets

2008

We give an overview over recent studies on the model of Active Brownian Motion (ABM) coupled to reservoirs providing free energy which may be converted into kinetic energy of motion. First, we present an introduction to a general concept of active Brownian particles which are capable to take up energy from the source and transform part of it in order to perform various activities. In the second part of our presentation we consider applications of ABM to ratchet systems with different forms of differentiable potentials. Both analytical and numerical evaluations are discussed for three cases of sinusoidal, staircase-like and Mateos ratchet potentials, also with the additional loads modeled by…

PhysicsStatistical Mechanics (cond-mat.stat-mech)RatchetPerturbation (astronomy)FOS: Physical sciencesFluctuation phenomena random processes noise Brownian motion Nonlinear dynamics and chaosWhite noiseCondensed Matter - Soft Condensed MatterCondensed Matter PhysicsKinetic energyElectronic Optical and Magnetic MaterialsClassical mechanicsPhysics - Data Analysis Statistics and ProbabilityMolecular motorDirectionalitySoft Condensed Matter (cond-mat.soft)Differentiable functionBrownian motionData Analysis Statistics and Probability (physics.data-an)Condensed Matter - Statistical Mechanics
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Filaments in observed and mock galaxy catalogues

2010

Context. The main feature of the spatial large-scale galaxy distribution is an intricate network of galaxy filaments. Although many attempts have been made to quantify this network, there is no unique and satisfactory recipe for that yet. Aims. The present paper compares the filaments in the real data and in the numerical models, to see if our best models reproduce statistically the filamentary network of galaxies. Methods. We apply an object point process with interactions (the Bisous process) to trace and describe the filamentary network both in the observed samples (the 2dFGRS catalogue) and in the numerical models that have been prepared to mimic the data.We compare the networks. Result…

Physicsstatistical [Methods]Cosmology and Nongalactic Astrophysics (astro-ph.CO):ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Otras [UNESCO]FOS: Physical scienceslarge [Cosmology]Astronomy and AstrophysicsContext (language use)Scale structure of UniverseAstrophysicsNumerical models:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Cosmology : large; Scale structure of Universe; Methods : data analysis; Methods : statisticalGalaxyObject pointSpace and Planetary ScienceUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::OtrasUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniadata analysis [Methods]Astrophysics - Cosmology and Nongalactic Astrophysics
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A neural network clustering algorithm for the ATLAS silicon pixel detector

2014

A novel technique to identify and split clusters created by multiple charged particles in the ATLAS pixel detector using a set of artificial neural networks is presented. Such merged clusters are a common feature of tracks originating from highly energetic objects, such as jets. Neural networks are trained using Monte Carlo samples produced with a detailed detector simulation. This technique replaces the former clustering approach based on a connected component analysis and charge interpolation. The performance of the neural network splitting technique is quantified using data from proton-proton collisions at the LHC collected by the ATLAS detector in 2011 and from Monte Carlo simulations. …

Physics::Instrumentation and DetectorsCiencias FísicasMonte Carlo methodHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)jetParticle tracking detectors[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]scattering [p p]Statistical physicscluster [track data analysis]Particle tracking detectors (solid-state detectors)InstrumentationQCMathematical PhysicsPhysicsArtificial neural networkAtlas (topology)Detectordetectors)Monte Carlo [numerical calculations]ATLASperformance [neural network]CERN LHC CollParticle tracking detectors (Solid-state detectors)Feature (computer vision)Physical SciencesParticle tracking detectors (Solid-stateParticle tracking detectors; Particle tracking detectors (Solid-state detectors)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCConnected-component labelingAlgorithmNeural networksCIENCIAS NATURALES Y EXACTASParticle Physics - ExperimentInterpolationCiências Naturais::Ciências Físicas530 Physicssplitting:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesParticle tracking detectors; Particle tracking detectors (solid-state detectors); Instrumentation; Mathematical Physics530FysikHigh Energy Physicsddc:610Cluster analysispixel [semiconductor detector]Science & TechnologyFísica//purl.org/becyt/ford/1.3 [https]High Energy Physics - Experiment; High Energy Physics - ExperimentParticle tracking detectorcluster [charged particle]AstronomíaParticle tracking detectors; Particle tracking detectors (Solid-state; detectors)Experimental High Energy Physicsimpact parameter [resolution]
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Analyse spatiale des disparités régionales dans l'Europe élargie

2004

The aim of this paper is to study the regional inequalities in the enlarged European Union using Exploratory Spatial Data Analysis applied to per capita GDP for 258 regions of EU27 over the period 1995-2000. Strong evidence in favor of global and local autocorrelation as well as spatial heterogeneity is found for the wealth distribution. We also show that the enlargement process leads to a new North-West - East polarization scheme instead of the previous results obtained in the literature highlighting a North-South polarization scheme. Implications for regional development and cohesion policies are finally explored.

Politique régionaleExploratory spatial data analysisDisparités régionales[SHS.GEO] Humanities and Social Sciences/GeographyAutocorrélation spatialeSpatial heterogeneityAnalyse exploratoire des données spatiales[SHS.GEO]Humanities and Social Sciences/GeographyRegional policiesHétérogénéité spatialeSpatial autocorrelation[ SHS.GEO ] Humanities and Social Sciences/GeographyRegional disparities
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