Search results for "HALO"

showing 10 items of 2623 documents

FastEMD–CCA algorithm for unsupervised and fast removal of eyeblink artifacts from electroencephalogram

2020

Abstract Online detection and removal of eye blink (EB) artifacts from electroencephalogram (EEG) would be very useful in medical diagnosis and brain computer interface (BCI). In this work, approaches that combine unsupervised eyeblink artifact detection with empirical mode decomposition (EMD), and canonical correlation analysis (CCA), are proposed to automatically identify eyeblink artifacts and remove them in an online manner. First eyeblink artifact regions are automatically identified and an eyeblink artifact template is extracted via EMD, which incorporates an alternate interpolation technique, the Akima spline interpolation. The removal of eyeblink artifact components relies on the el…

Artifact (error)Cross-correlationmedicine.diagnostic_testComputer science0206 medical engineeringBiomedical EngineeringWord error rateHealth Informatics02 engineering and technologyElectroencephalography020601 biomedical engineeringHilbert–Huang transform[SPI]Engineering Sciences [physics]03 medical and health sciences0302 clinical medicineSignal ProcessingmedicineSpline interpolationAlgorithm030217 neurology & neurosurgeryInterpolationBrain–computer interfaceBiomedical Signal Processing and Control
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Online detection and removal of eye blink artifacts from electroencephalogram

2021

Abstract The most prominent type of artifact contaminating electroencephalogram (EEG) signals are the eye blink (EB) artifacts, which could potentially lead to misinterpretation of the EEG signal. Online identification and elimination of eye blink artifacts are crucial in applications such a Brain-Computer Interfaces (BCI), neurofeedback, and epilepsy diagnosis. In this paper, algorithms that combine unsupervised eye blink artifact detection (eADA) with modified Empirical Mode Decomposition (FastEMD) and Canonical Correlation Analysis (CCA) are proposed, i.e., FastEMD-CCA2 and FastCCA, to automatically identify eye blink artifacts and remove them in an online setting. The average accuracy, …

Artifact (error)medicine.diagnostic_testComputer sciencebusiness.industryBiomedical EngineeringWord error rateHealth InformaticsPattern recognitionElectroencephalographySignalHilbert–Huang transformSignal ProcessingmedicineArtificial intelligenceSensitivity (control systems)NeurofeedbackbusinessBrain–computer interfaceBiomedical Signal Processing and Control
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Automated and Online Eye Blink Artifact Removal from Electroencephalogram

2019

Eyeblink artifacts often contaminates electroencephalogram (EEG) signals, which could potentially confound EEG's interpretation. A lot offline methods are available to remove this artifact, but an online solution is required to remove eyeblink artifacts in near real time for EEG signal to be beneficial in applications such as brain computer interface, (BCI). In this work, approaches that combines unsupervised eyeblink artifact detection with Empirical Mode Decomposition (EMD) and Canonical Correlation Analysis (CCA) are proposed to automatically identify eyeblink artifacts and remove them in an online setting. The proposed approaches are analysed and evaluated in terms of artifact removal a…

Artifact (error)medicine.diagnostic_testComputer sciencebusiness.industryProcess (computing)Pattern recognition02 engineering and technologyElectroencephalography021001 nanoscience & nanotechnologySignalHilbert–Huang transform03 medical and health sciencesComputingMethodologies_PATTERNRECOGNITION0302 clinical medicinemedicineArtificial intelligence0210 nano-technologyCanonical correlationEye blinkbusiness030217 neurology & neurosurgeryBrain–computer interface2019 IEEE International Conference on Signal and Image Processing Applications (ICSIPA)
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Unsupervised Eye Blink Artifact Identification in Electroencephalogram

2018

International audience; The most prominent type of artifact contaminating electroencephalogram (EEG) signals is the eye blink (EB) artifact. Hence, EB artifact detection is one of the most crucial pre-processing step in EEG signal processing before this artifact can be removed. In this work, an approach that identifies EB artifacts without human supervision and automated varying threshold setting is proposed and evaluated. The algorithm functions on the basis of correlation between two EEG electrodes, Fp1 and Fp2, followed by EB artifact threshold determination utilizing the amplitude displacement from the mean. The proposed approach is validated and evaluated in terms of accuracy and error…

Artifact (error)medicine.diagnostic_testbusiness.industryComputer science05 social sciencesFeature extractionWord error ratePattern recognitionElectroencephalography050105 experimental psychologyEB Artifacts03 medical and health sciencesIdentification (information)Electroencephalogram0302 clinical medicine[INFO.INFO-TS]Computer Science [cs]/Signal and Image Processingmedicine0501 psychology and cognitive sciences[INFO]Computer Science [cs]Artificial intelligenceAutomated ThresholdbusinessEye blink030217 neurology & neurosurgery
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Emerging brominated flame retardants and dechlorane-related compounds in European eels (Anguilla anguilla) from Latvian lakes

2017

Abstract Fifteen halogenated flame retardants (HFRs) including seven emerging brominated flame retardants (EBFRs) and eight dechlorane-related compounds (DRCs) were analyzed in eels (Anguilla anguilla) sampled from five Latvian lakes. Out of the seven EBFRs, hexabromocyclododecane (HBCD) and decabromodiphenyl ethane (DBDPE) were found in eels in quantifiable concentrations, up to 6.58 and 33.0 ng g−1 lipid weight (l.w.), respectively. The mean total concentration of DRCs (∑DRC) in the samples was 0.62 ng g−1 l.w. and the geographical distribution of DRC contamination was nearly uniform among the selected lakes. Dechlorane 602 (Dec 602) was the predominant component, whereas the composition …

AsiaEnvironmental EngineeringHalogenation010504 meteorology & atmospheric sciencesHealth Toxicology and Mutagenesis010501 environmental sciencesAquatic biota01 natural scienceschemistry.chemical_compoundHalogenated Diphenyl EthersHydrocarbons ChlorinatedAnimalsEnvironmental ChemistryPolycyclic CompoundsFlame Retardants0105 earth and related environmental sciencesHexabromocyclododecanePublic Health Environmental and Occupational HealthGeneral MedicineGeneral ChemistryContaminationAnguillaLatviaPollutionHydrocarbons BrominatedEuropeLakesDecabromodiphenyl ethanechemistryAquatic environmentEnvironmental chemistryComposition (visual arts)Water Pollutants ChemicalBromobenzenesEnvironmental MonitoringChemosphere
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Quantitative EEG during Early Recovery from Hypoxic-Ischemic Injury in Immature Piglets: Burst Occurrence and Duration

1999

This study examined the course of EEG recovery in an animal model of hypoxic-ischemic injury. The model used periods of hypoxia, room air and asphyxia to induce cardiac arrest. One-week-old piglets (n = 16) were exposed to a period of hypoxia, room air and complete asphyxia for 7 minutes. After cardiac arrest and resuscitation, two EEG features were evaluated as prognostic indicators of behavioral outcome as assessed by a neuroscore at 24 hours after insult. A prominent EEG feature was the number and duration of bursts evident during recovery. Episodes of bursting were detected through the thresholds on sustained periods of elevated power. After the animal was resuscitated, the EEG was moni…

AsphyxiaResuscitationmedicine.diagnostic_testSwinebusiness.industryElectroencephalographyElectroencephalographyHypoxia (medical)030227 psychiatryQuantitative eeg03 medical and health sciencesBursting0302 clinical medicineAnimal modelAnimals NewbornAnesthesiaHypoxia-Ischemia BrainRoom air distributionmedicineAnimalsNeurology (clinical)medicine.symptombusiness030217 neurology & neurosurgeryClinical Electroencephalography
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Non-linear evolution of the cosmic neutrino background

2012

We investigate the non-linear evolution of the relic cosmic neutrino background by running large box-size, high resolution N-body simulations which incorporate cold dark matter (CDM) and neutrinos as independent particle species. Our set of simulations explore the properties of neutrinos in a reference Lambda CDM model with total neutrino masses between 0.05-0.60 eV in cold dark matter haloes of mass 10(11) – 10(15) h(-1) M-circle dot, over a redshift range z = 0 – 2. We compute the halo mass function and show that it is reasonably well fitted by the Sheth-Tormen formula, once the neutrino contribution to the total matter is removed. More importantly, we focus on the CDM and neutrino proper…

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark mattercosmological neutrinosFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesMomentumSettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesPeculiar velocity010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsneutrino propertiesPhysicsCosmologia010308 nuclear & particles physicsHalo mass functionAstronomy and Astrophysicsneutrino masses from cosmologyRedshiftCosmic neutrino background13. Climate actionHigh Energy Physics::ExperimentHaloNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Constraints on dark matter annihilation from CMB observations before Planck

2013

We compute the bounds on the dark matter (DM) annihilation cross section using the most recent Cosmic Microwave Background measurements from WMAP9, SPT'11 and ACT'10. We consider DM with mass in the MeV-TeV range annihilating 100% into either an e(+)e(-) or a mu(+)mu(-) pair. We consider a realistic energy deposition model, which includes the dependence on the redshift, DM mass and annihilation channel. We exclude the canonical thermal relic abundance cross section ( = 3 x 10(-26) cm(3)s(-1)) for DM masses below 30 GeV and 15 GeV for the e(+)e(-) and mu(+)mu(-) channels, respectively. A priori, DM annihilating in halos could also modify the reionization history of the Universe at late times…

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyPartícules (Física nuclear)symbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010303 astronomy & astrophysicsReionizationPhysicsdark matter theoryCosmologiaAnnihilation010308 nuclear & particles physicsAstronomy and AstrophysicsCMBR theoryRedshiftStarsHigh Energy Physics - PhenomenologysymbolsHalophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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N-body simulations with generic non-Gaussian initial conditions I: Power Spectrum and halo mass function

2010

We address the issue of setting up generic non-Gaussian initial conditions for N-body simulations. We consider inflationary-motivated primordial non-Gaussianity where the perturbations in the Bardeen potential are given by a dominant Gaussian part plus a non-Gaussian part specified by its bispectrum. The approach we explore here is suitable for any bispectrum, i.e. it does not have to be of the so-called separable or factorizable form. The procedure of generating a non-Gaussian field with a given bispectrum (and a given power spectrum for the Gaussian component) is not univocal, and care must be taken so that higher-order corrections do not leave a too large signature on the power spectrum.…

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)GaussianFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSeparable spacesymbols.namesakeComponent (UML)0103 physical sciencesStatistical physics010303 astronomy & astrophysicsPhysicsCosmologia010308 nuclear & particles physicsHalo mass functionSpectral densityAstronomy and AstrophysicsCosmologysymbolsSignature (topology)BispectrumAstrophysics - Cosmology and Nongalactic Astrophysics
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Halo-independent methods for inelastic dark matter scattering

2013

We present halo-independent methods to analyze the results of dark matter direct detection experiments assuming inelastic scattering. We focus on the annual modulation signal reported by DAMA/LIBRA and present three different halo-independent tests. First, we compare it to the upper limit on the unmodulated rate from XENON100 using (a) the trivial requirement that the amplitude of the annual modulation has to be smaller than the bound on the unmodulated rate, and (b) a bound on the annual modulation amplitude based on an expansion in the Earth's velocity. The third test uses the special predictions of the signal shape for inelastic scattering and allows for an internal consistency check of …

AstrofísicaParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesInelastic scattering01 natural sciencesSignalPartícules (Física nuclear)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsPhysicsdark matter theory010308 nuclear & particles physicsScatteringdark matter experimentsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsComputational physicsDark matter haloHigh Energy Physics - PhenomenologyAmplitudeModulationHaloAstronomia Aparells i instrumentsAstrophysics - Cosmology and Nongalactic Astrophysics
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