Search results for "methods [Diffusion Tensor Imaging]"

showing 10 items of 992 documents

The energy spectrum of cosmic rays beyond the turn-down around 1017 eV as measured with the surface detector of the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina – Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia – the Australian Research Council; Be…

Physics and Astronomy (miscellaneous)AstronomyAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesFluxCosmic rayAstrophysics7. Clean energy01 natural sciencesdetector: fluorescenceAugercosmic rayssurface [detector]Observatory0103 physical sciencescalorimeterddc:530High Energy Physicscosmic radiation: UHEspectrum [cosmic radiation]010303 astronomy & astrophysicsEngineering (miscellaneous)Engineering & allied operationsHigh Energy Astrophysical Phenomena (astro-ph.HE)fluorescence [detector]Pierre Auger ObservatoryPhysicsastro-ph.HEcosmic radiation: energy spectrumcosmic radiation: spectrumdetector: surface010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugerCalorimeterfluxobservatoryspectralddc:620[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomenaenergy spectrum [cosmic radiation]Energy (signal processing)RAIOS CÓSMICOSultra-high energy cosmic rays energy spectrum features.
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A method for approximating optimal statistical significances with machine-learned likelihoods

2022

The European physical journal / C 82(11), 993 (2022). doi:10.1140/epjc/s10052-022-10944-3

Physics and Astronomy (miscellaneous)Gluonsboosted particleFOS: Physical sciencesTop Quark530High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)statistical analysisddc:530numerical calculationsEngineering (miscellaneous)Monte CarloInstrumentation and Methods for Astrophysics (astro-ph.IM)new physicsFísicadijet: final statefinal state [dijet]sensitivityHigh Energy Physics - Phenomenologymachine learningCERN LHC CollPhysics - Data Analysis Statistics and ProbabilitySubstructureAstrophysics - Instrumentation and Methods for AstrophysicsData Analysis Statistics and Probability (physics.data-an)
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Classification of gravitational-wave glitches via dictionary learning

2018

We present a new method for the classification of transient noise signals (or glitches) in advanced gravitational-wave interferometers. The method uses learned dictionaries (a supervised machine learning algorithm) for signal denoising, and untrained dictionaries for the final sparse reconstruction and classification. We use a data set of 3000 simulated glitches of three different waveform morphologies, comprising 1000 glitches per morphology. These data are embedded in non-white Gaussian noise to simulate the background noise of advanced LIGO in its broadband configuration. Our classification method yields a 96% accuracy for a large range of initial parameters, showing that learned diction…

Physics and Astronomy (miscellaneous)Noise reductionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Data_CODINGANDINFORMATIONTHEORY01 natural sciencesGeneral Relativity and Quantum CosmologyBackground noiseTransient noisesymbols.namesake0103 physical sciencesWaveformAstrophysics::Solar and Stellar Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPattern recognitionLIGOGlitchGaussian noisesymbolsArtificial intelligenceAstrophysics - Instrumentation and Methods for Astrophysicsbusiness
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Cutoff dependence of the thrust peak position in the dipole shower

2020

We analyse the dependence of the peak position of the thrust distribution on the cutoff value in the Nagy-Soper dipole shower. We compare the outcome of the parton shower simulations to a relation of the dependence from an analytic computation, derived within soft-collinear effective theory. We show that the result of the parton shower simulations and the analytic computation are in good agreement.

Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsComputationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical scienceslcsh:AstrophysicsThrust01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Position (vector)lcsh:QB460-4660103 physical sciencesEffective field theoryCutofflcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsParton showerEngineering (miscellaneous)Physics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsComputational physicsDipoleHigh Energy Physics - PhenomenologyDistribution (mathematics)lcsh:QC770-798High Energy Physics::Experiment
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'School adopts an experiment': the magnetic levitation of superconductors

2010

The event 'School adopts an experiment' is an event targeted at high schools and secondary schools. It is based on a tight and direct collaboration between researchers and school students and teachers. Several schools were involved in the event by 'adopting' an experiment in physics research laboratories. Groups of selected students were first trained by university researchers, then they demonstrated the experiments to other students and teachers during the event. Students who adopted an experiment acquired knowledge of the subjects connected with the experiment in a most impressive way compared with the usual didactics at school. Further positive points were: (i) to establish a close and d…

Physics educationLaboratory experiments and apparatuEvent (relativity)Physics educationComputingMilieux_COMPUTERSANDEDUCATIONMathematics educationGeneral Physics and AstronomySuperconducting magnets magnetic levitationSecondary schoolEducation and communication.Magnetic levitationTeaching methods and strategieEducation
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'School adopts an experiment': the photoluminescence in extra-virgin olive oil and in tonic water

2011

We report a laboratory activity, carried out along with high- and secondary-school students, that can be done to increase the interest of the young in scientific studies. Groups of selected students ‘adopted’ experiments at physics research laboratories, under the guidance of university researchers. Subsequently, the students demonstrated the experiments to the public at large during the annual science festival organized in Palermo by the association PalermoScienza, in collaboration with the University of Palermo. Experiments on the magnetic levitation of superconductors and on the photoluminescence of several substances were proposed. We discuss the experiment on photoluminescence as a cas…

Physics education; Teaching methods and strategies; Fluorescence and phosphorescence spectraPhysicsScience instructionPhysics educationTeaching methodPhysics educationGeneral Physics and AstronomyTeaching methods and strategieEducationTonic waterfoodMathematics educationfood.beverageFluorescence and phosphorescence spectraOlive oil
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ARGO-YBJ constraints on very high energy emission from GRBs

2009

The ARGO-YBJ (Astrophysical Radiation Ground-based Observatory at YangBaJing) experiment is designed for very high energy $\gamma$-astronomy and cosmic ray researches. Due to the full coverage of a large area ($5600 m^2$) with resistive plate chambers at a very high altitude (4300 m a.s.l.), the ARGO-YBJ detector is used to search for transient phenomena, such as Gamma-ray bursts (GRBs). Because the ARGO-YBJ detector has a large field of view ($\sim$2 sr) and is operated with a high duty cycle ($>$90%), it is well suited for GRB surveying and can be operated in searches for high energy GRBs following alarms set by satellite-borne observations at lower energies. In this paper, the sensitivit…

Physics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaSettore FIS/01 - Fisica SperimentaleDetectorGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsCosmic rayField of viewAstrophysicsRadiation7. Clean energy01 natural sciencesSettore FIS/05 - Astronomia e Astrofisica13. Climate actionDuty cycleObservatory0103 physical sciencesGAMMA RAY BURSTS GAMMA RAYS COSMIC RAYS EXTENDED AIR SHOWERSGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysics
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Application of dictionary learning to denoise LIGO’s blip noise transients

2020

Data streams of gravitational-wave detectors are polluted by transient noise features, or ``glitches,'' of instrumental and environmental origin. In this work we investigate the use of total variation methods and learned dictionaries to mitigate the effect of those transients in the data. We focus on a specific type of transient, ``blip" glitches, as this is the most common type of glitch present in the LIGO detectors and their waveforms are easy to identify. We randomly select 100 blip glitches scattered in the data from advanced LIGO's O1 run, as provided by the citizen-science project Gravity Spy. Our results show that dictionary-learning methods are a valid approach to model and subtrac…

Physics010308 nuclear & particles physicsData stream miningAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesBinary numberGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)01 natural sciencesGeneral Relativity and Quantum CosmologyLIGOGlitchNoiseTransient noise0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsTransient (computer programming)010306 general physicsAlgorithmPhysical Review D
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New method to observe gravitational waves emitted by core collapse supernovae

2018

While gravitational waves have been detected from mergers of binary black holes and binary neutron stars, signals from core collapse supernovae, the most energetic explosions in the modern Universe, have not been detected yet. Here we present a new method to analyse the data of the LIGO, Virgo, and KAGRA network to enhance the detection efficiency of this category of signals. The method takes advantage of a peculiarity of the gravitational wave signal emitted in the core collapse supernova and it is based on a classification procedure of the time-frequency images of the network data performed by a convolutional neural network trained to perform the task to recognize the signal. We validate …

Physics010308 nuclear & particles physicsGravitational waveAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsType II supernova01 natural sciencesSignalGeneral Relativity and Quantum CosmologyLIGOGravitational wavesGravitational waves; SupernovaeGeneral Relativity and Quantum CosmologySupernovaNeutron starSupernovaeBinary black hole0103 physical sciencesKAGRAAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysics
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Evaluation of a commercial APD array (Avalanche PhotoDiode) for a readout detector in a hadrontherapy beam characterization application

2010

The aim of the present work is the characterization of the S8898–128–02 Avalanche PhotoDiode array (APDs) from Hamamatsu Photonics. This work includes the implementation of a readout system as well as electronic noise estimation in APDs under several conditions varying integration times and clock frequencies.

PhysicsAPDSPhysics::Instrumentation and Detectorsbusiness.industryPhysics::Medical PhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAvalanche photodiodeNoise (electronics)law.inventionlawNuclear electronicsOptoelectronicsPhotonicsbusinessField-programmable gate arrayBeam (structure)IEEE Nuclear Science Symposuim & Medical Imaging Conference
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