Search results for "BURSTS"

showing 10 items of 76 documents

Burst analysis tool for developing neuronal networks exhibiting highly varying action potential dynamics

2012

In this paper we propose a firing statistics based neuronal network burst detection algorithm for neuronal networks exhibiting highly variable action potential dynamics. Electrical activity of neuronal networks is generally analyzed by the occurrences of spikes and bursts both in time and space. Commonly accepted analysis tools employ burst detection algorithms based on predefined criteria. However, maturing neuronal networks, such as those originating from human embryonic stem cells (hESC), exhibit highly variable network structure and time-varying dynamics. To explore the developing burst/spike activities of such networks, we propose a burst detection algorithm which utilizes the firing s…

Computer scienceNeuroscience (miscellaneous)Interval (mathematics)ta3112lcsh:RC321-57103 medical and health sciencesCellular and Molecular Neuroscience0302 clinical medicineMoving averageHistogramBiological neural networkMethods Articleburst analysislcsh:Neurosciences. Biological psychiatry. Neuropsychiatry030304 developmental biology0303 health sciencesspike trainsQuantitative Biology::Neurons and Cognitionmicroelectrode arrayMEAaction potential burstsdeveloping neuronal networksMultielectrode arrayhuman embryonic stem cellsPower (physics)nervous systemSkewnesshESCsSpike (software development)Biological systemNeuroscience030217 neurology & neurosurgeryNeuroscienceFrontiers in Computational Neuroscience
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Quantification and automatized adaptive detection of in vivo and in vitro neuronal bursts based on signal complexity.

2015

In this paper, we propose employing entropy values to quantify action potential bursts in electrophysiological measurements from the brain and neuronal cultures. Conventionally in the electrophysiological signal analysis, bursts are quantified by means of conventional measures such as their durations, and number of spikes in bursts. Here our main aim is to device metrics for burst quantification to provide for enhanced burst characterization. Entropy is a widely employed measure to quantify regularity/complexity of time series. Specifically, we investigate the applicability and differences of spectral entropy and sample entropy in the quantification of bursts in in vivo rat hippocampal meas…

Computer scienceQuantitative Biology::Tissues and OrgansAstrophysics::High Energy Astrophysical PhenomenaEntropyCell Culture TechniquesElectrophysiological PhenomenaAction Potentialsta3112HippocampusEntropy (classical thermodynamics)In vivoEntropy (information theory)AnimalsEntropy (energy dispersal)Rats WistarEntropy (arrow of time)ta217NeuronsSignal processingQuantitative Biology::Neurons and Cognitionta213Entropy (statistical thermodynamics)Signal Processing Computer-Assistedadaptive detectionelectrophysiological signal analysisquantificationneuronal burstsElectrophysiological PhenomenaSample entropyElectrophysiologyElectrophysiologyMicroelectrodeBiological systemNeuroscienceMicroelectrodesEntropy (order and disorder)Annual International Conference of the IEEE Engineering in Medicine and Biology Society. IEEE Engineering in Medicine and Biology Society. Annual International Conference
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The transient gravitational-wave sky

2013

Interferometric detectors will very soon give us an unprecedented view of the gravitational-wave sky, and in particular of the explosive and transient Universe. Now is the time to challenge our theoretical understanding of short-duration gravitational-wave signatures from cataclysmic events, their connection to more traditional electromagnetic and particle astrophysics, and the data analysis techniques that will make the observations a reality. This paper summarizes the state of the art, future science opportunities, and current challenges in understanding gravitational-wave transients.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Explosive materialmedia_common.quotation_subjectELECTROMAGNETIC COUNTERPARTSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologySPIN-DOWN LIMIT0103 physical sciencesPRESUPERNOVA EVOLUTIONCORE-COLLAPSE010306 general physics010303 astronomy & astrophysicsARMED SPIRAL INSTABILITYmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysicsGAMMA-RAY BURSTSNEUTRINO PAIR ANNIHILATIONGravitational waveAstronomyMASS BLACK-HOLESUniverseBAR-MODE INSTABILITYInterferometrySkyData analysisTransient (oscillation)Astrophysics - High Energy Astrophysical PhenomenaDRIVEN SUPERNOVAgravitational waves neutron stars black holesAstrophysics - Cosmology and Nongalactic AstrophysicsClassical and Quantum Gravity
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Timing techniques applied to distributed modular high-energy astronomy: the H.E.R.M.E.S. project

2021

The HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites -- Technologic and Scientific Pathfinder) is an in-orbit demonstration of the so-called distributed astronomy concept. Conceived as a mini-constellation of six 3U nano-satellites hosting a new miniaturized detector, HERMES-TP/SP aims at the detection and accurate localisation of bright high-energy transients such as Gamma-Ray Bursts. The large energy band, the excellent temporal resolution and the wide field of view that characterize the detectors of the constellation represent the key features for the next generation high-energy all-sky monitor with good localisation capabilities that will play a pivotal role in the future …

CubeSatsHigh energyHigh-energy astronomyReal-time computingFOS: Physical sciences01 natural sciences7. Clean energy010309 opticsX-rays0103 physical sciencesNano-satellitesTemporal triangulationInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsConstellationHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsModular designPathfinderTemporal resolutionGamma Ray BurstsTransient (oscillation)Astrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsbusinessSpace Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
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Quantum gravity with THESEUS

2021

AbstractIn this paper we explore the possibility to search for a dispersion law for light propagation in vacuo with a sample of Gamma-Ray Bursts detected by the THESEUS satellite. Within Quantum Gravity theories, different models for space-time quantization predict relative discrepancies of the speed of photons w.r.t. the speed of light that (in a series expansion) depend on a given power of the ratio of the photon energy to the Planck energy. This ratio is as small as 10− 23 for photons in the soft γ −ray band (100 keV). The dominant effect is determined by the first significant term of this expansion. If the first order in this expansion is relevant, these theories imply a Lorentz Invaria…

CubeSatsSettore FIS/05 - Astronomia E AstrofisicaAll-sky monitorSpace and Planetary ScienceAstrophysics::High Energy Astrophysical PhenomenaX-raysQuantum gravityGravitational wave counterpartsAstronomy and AstrophysicsGamma-ray burstsNano-satellitesTemporal triangulationExperimental Astronomy
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The HERMES-Technologic and Scientific Pathfinder

2020

HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites Technologic and Scientific Pathfinder) is a constellation of six 3U nano-satellites hosting simple but innovative X-ray detectors, characterized by a large energy band and excellent temporal resolution, and thus optimized for the monitoring of Cosmic High Energy transients such as Gamma Ray Bursts and the electromagnetic counterparts of Gravitational Wave Events, and for the determination of their positions. The projects are funded by the Italian Ministry of University and Research and by the Italian Space Agency, and by the European Union Horizon 2020 Research and Innovation Program under Grant Agreement No. 821896. HERMES-TP/S…

CubeSatsmedia_common.quotation_subjectCubeSats; Gamma Ray Bursts; Nano-satellites; X-raysFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyAstrophysics - Instrumentation and MethodsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesX-raysmedia_common.cataloged_instanceEuropean unionAerospace engineeringNano-satellites010306 general physics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)media_commonConstellationPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)COSMIC cancer databasebusiness.industryGravitational waveModular designPathfinderSkyTemporal resolutionGamma Ray BurstsbusinessAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysics
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

2018

The LIGO Scientific and Virgo Collaborations have announced the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutron stars estimated from this event suggests that distant, unresolvable binary neutron stars create a significant astrophysical stochastic gravitational-wave background. The binary neutron star background will add to the background from binary black holes, increasing the amplitude of the total astrophysical background relative to previous expectations. In the Advanced LIGO-Virgo frequency band most sensitive to stochastic backgrounds (near 25 Hz), we predict a total astrophysical background with amplitude $\Omega_{\rm…

Design sensitivityneutron star: binarygravitational radiation: stochasticAstronomyX-ray binaryGeneral Physics and AstronomyAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationGravitational wave backgroundGravitational Waves Neutron Stars Stochastic Background Virgo LIGOblack holeLIGOstochastic modelQCQBPhysicsGAMMA-RAY BURSTSSignal to noise ratioStochastic systemsBlack holesGravitational effectsarticleAstrophysics::Instrumentation and Methods for AstrophysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSING[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sources Experimental studies of gravity Gravitational WavesGravitationBinary neutron starsX-ray bursterBinsAstrophysics::High Energy Astrophysical PhenomenaMERGERSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionBinary pulsarNeutron starsSTAR-FORMATIONPhysics and Astronomy (all)General Relativity and Quantum CosmologyBinary black holebinary: coalescence0103 physical sciencesFrequency bandsddc:530RATESINTERFEROMETERS010306 general physicsAstrophysics::Galaxy AstrophysicsNeutronsGravitational Waves010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundgravitational radiationAstronomyNeutron Stars530 Physikbinary: compactsensitivityStarsLIGObackground: stochasticEVOLUTIONsignal noise ratioVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionStellar black holeStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHIGH-REDSHIFTneutron star: coalescencePhysical Review Letters
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Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

2014

A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012-2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV - PeV range at the level of $10^{-8}\, \mathrm{GeV}\, \mathrm{cm}^{-2}\, \mathrm{s}^{-1}\, \mathrm{sr}^{-1}$ per flavor and reject a purely atmospheric explanation for the combined 3-year data at $5.7 \sigma$. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotrop…

FLUXACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)TELESCOPESolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyIceCubeIceCube Neutrino ObservatoryHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SEARCH0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGlashow resonanceHigh Energy Physics::PhenomenologyASTRONOMYAstronomySolar neutrino problemBLAZARSPhysics and AstronomyNeutrino detector13. Climate actionLEPTONSJETSMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyEMISSIONAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Constraints on ultra-high-energy cosmic ray sources from a search for neutrinos above 10 PeV with IceCube

2016

We report constraints on the sources of ultra-high-energy cosmic ray (UHECR) above $10^{9}$ GeV, based on an analysis of seven years of IceCube data. This analysis efficiently selects very high energy neutrino-induced events which have deposited energies from $\sim 10^6$ GeV to above $10^{11}$ GeV. Two neutrino-induced events with an estimated deposited energy of $(2.6 \pm 0.3) \times 10^6$ GeV, the highest neutrino energies observed so far, and $(7.7 \pm 2.0) \times 10^5$ GeV were detected. The atmospheric background-only hypothesis of detecting these events is rejected at 3.6$\sigma$. The hypothesis that the observed events are of cosmogenic origin is also rejected at $>$99% CL because of…

FLUXSELECTIONFERMI-LATActive galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesCosmic rayAstrophysicsParameter space7. Clean energy01 natural sciencesCOSMOGENIC NEUTRINOS; TRACK RECONSTRUCTION; FERMI-LAT; BURSTS; SPECTRUM; MODEL; FLUX; TELESCOPES; SELECTION; EMISSIONPulsar0103 physical sciencesTRACK RECONSTRUCTIONBURSTSddc:550Ultrahigh energy010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)SPECTRUM010308 nuclear & particles physicsStar formationCOSMOGENIC NEUTRINOSAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyMODELPhysics and Astronomy13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEMISSIONEnergy (signal processing)Astrophysics - Cosmology and Nongalactic Astrophysics
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Network Physiology of Cortico–Muscular Interactions

2020

Skeletal muscle activity is continuously modulated across physiologic states to provide coordination, flexibility and responsiveness to body tasks and external inputs. Despite the central role the muscular system plays in facilitating vital body functions, the network of brain-muscle interactions required to control hundreds of muscles and synchronize their activation in relation to distinct physiologic states has not been investigated. Recent approaches have focused on general associations between individual brain rhythms and muscle activation during movement tasks. However, the specific forms of coupling, the functional network of cortico-muscular coordination, and how network structure a…

Flexibility (anatomy)Computer sciencePhysiologybrain wavesPhysiologynetwork physiologylcsh:Physiology03 medical and health sciencesMuscle tone0302 clinical medicineRhythmInteraction networkPhysiology (medical)medicinesleepSettore MAT/07 - Fisica Matematica030304 developmental biologySlow-wave sleepOriginal Research0303 health scienceslcsh:QP1-981burstsMuscular systemSkeletal muscledynamic networksSleep in non-human animalsmedicine.anatomical_structuremuscle tonetime delay stabilitysynchronization030217 neurology & neurosurgeryFrontiers in Physiology
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