Search results for "GAM"

showing 10 items of 5334 documents

Multiple accelerated particle populations in the Cygnus Loop with Fermi-LAT

2021

The Cygnus Loop (G74.0-8.5) is a very well-known nearby supernova remnant (SNR) in our Galaxy. Thanks to its large size, brightness, and angular offset from the Galactic plane, it has been studied in detail from radio to $\gamma$-ray emission. The $\gamma$ -rays probe the populations of energetic particles and their acceleration mechanisms at low shock speeds. We present an analysis of the $\gamma$-ray emission detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope over 11 years in the region of the Cygnus Loop. We performed detailed morphological and spectral studies of the $\gamma$-ray emission toward the remnant from 100 MeV to 100 GeV and compared it with X-ra…

Astrophysics::High Energy Astrophysical Phenomenabrightnesscosmic radiation: energyFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeV01 natural sciencesGLASTthermalX-raycosmic raysSpitzer Space Telescope0103 physical sciencesultravioletsupernovaRadiative transferopticalcloudcosmic radiation: acceleration010306 general physicsSupernova remnant010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsacceleration of particlesISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cygnus LoopAstronomy and Astrophysicsshock wavesGalactic planeGalaxy13. Climate actionSpace and Planetary Sciencegamma raystatisticsspectralgalaxyAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Fermi Gamma-ray Space Telescope
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Observation of TeV gamma rays from the Cygnus region with the ARGO-YBJ experiment

2012

We report the observation of TeV gamma-rays from the Cygnus region using the ARGO-YBJ data collected from 2007 November to 2011 August. Several TeV sources are located in this region including the two bright extended MGRO J2019+37 and MGRO J2031+41. According to the Milagro data set, at 20 TeV MGRO J2019+37 is the most significant source apart from the Crab Nebula. No signal from MGRO J2019+37 is detected by the ARGO-YBJ experiment, and the derived flux upper limits at 90% confidence level for all the events above 600 GeV with medium energy of 3 TeV are lower than the Milagro flux, implying that the source might be variable and hard to be identified as a pulsar wind nebula. The only statist…

Astrophysics::High Energy Astrophysical Phenomenageneral – pulsars: individual (MGRO J2019+37 [Gamma rays]FluxFOS: Physical sciencesAstrophysics01 natural sciencesPulsar wind nebulageneral – pulsar0103 physical sciencesMILAGRO010303 astronomy & astrophysicsDETECTORArgoPhysicsCALIBRATIONHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsMGRO J2031+41)Settore FIS/01 - Fisica SperimentaleGamma rayAstronomy and Astrophysicsindividual (MGRO J2019+37 MGRO J2031+41)PLANE3. Good healthMedium energyCrab Nebulagamma ray13. Climate actionSpace and Planetary ScienceGALACTIC SOURCESJ2032+4130Milagrogamma rays; general – pulsars; individual (MGRO J2019+37 MGRO J2031+41)EMISSIONAstrophysics - High Energy Astrophysical Phenomena
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TeV gamma-ray survey of the Northern sky using the ARGO-YBJ detector

2013

The ARGO-YBJ detector is an extensive air shower array that has been used to monitor the northern $\gamma$-ray sky at energies above 0.3 TeV from 2007 November to 2013 January. In this paper, we present the results of a sky survey in the declination band from $-10^{\circ}$ to $70^{\circ}$, using data recorded over the past five years. With an integrated sensitivity ranging from 0.24 to $\sim$1 Crab units depending on the declination, six sources have been detected with a statistical significance greater than 5 standard deviations. Several excesses are also reported as potential $\gamma$-ray emitters. The features of each source are presented and discussed. Additionally, $95\%$ confidence le…

Astrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectFOS: Physical sciencesFluxField of viewAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGamma rays: general – surveys01 natural sciencesDeclination0103 physical sciencesAbsorption (logic)010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicsgeneral – su [gamma rays]Air showerExtragalactic background light13. Climate actionSpace and Planetary ScienceSkygeneral – surveys [Gamma rays]Astrophysics - High Energy Astrophysical Phenomena
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"Table 2" of "Measurement and Interpretation of Fermion-Pair Production at LEP Energies of 183 and 189 GeV"

2003

No description provided.

Asymmetry MeasurementE+ E- ScatteringIntegrated Cross SectionE+ E- --> TAU- TAU+ (GAMMAS)ExclusiveE+ E- --> MU- MU+ (GAMMAS)Cross SectionTau production183.0-189.0SIGMuon productionASYM
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Discontinuous Gradient Constraints and the Infinity Laplacian

2012

Motivated by tug-of-war games and asymptotic analysis of certain variational problems, we consider a gradient constraint problem involving the infinity Laplace operator. We prove that this problem always has a solution that is unique if a certain regularity condition on the constraint is satisfied. If this regularity condition fails, then solutions obtained from game theory and $L^p$-approximation need not coincide.

Asymptotic analysisGeneral Mathematicsta111010102 general mathematicsMathematical analysisinfinity Laplace operator01 natural sciences010101 applied mathematicsConstraint (information theory)Mathematics - Analysis of PDEsOperator (computer programming)Infinity LaplacianFOS: Mathematics0101 mathematicsGame theorygradient constraint problemsAnalysis of PDEs (math.AP)MathematicsInternational Mathematics Research Notices
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Contribuições e efeitos dos videogames na atenção à diversidade

2021

[Resumen] Este artículo presenta los resultados de una revisión de la literatura sobre estudios centrados en las contribuciones y los efectos de los videojuegos en la atención a la diversidad. Para ello, se tomó como muestra las investigaciones recogidas en las bases de datos Scopus, wos, eric, ProQuest Dissertations & Theses Global (pqdt), Dialnet y csic-isoc y en los buscadores académicos Rebiun, Teseo y ScienceDirect. Después de considerar algunos aspectos del análisis bibliométrico, con el propósito de contextualizar la autoría y la procedencia de los artículos, se procedió a analizar en profundidad el contenido de los documentos seleccionados, de acuerdo con los objetivos de este estud…

Atenção à diversidadeeducationinclusive educationeducação;atenção à diversidadevideojuegoseducação inclusivavideo gamesEducationatención a la diversidadeducación inclusivaattention to diversityEducaçãovideogamesEducacióeducación
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Traitement de données RGB et Lidar à extrêmement haute résolution: retombées de la compétition de fusion de données 2015 de l'IEEE GRSS - Partie A / …

2016

International audience; In this paper, we discuss the scientific outcomes of the 2015 data fusion contest organized by the Image Analysis and Data Fusion Technical Committee (IADF TC) of the IEEE Geoscience and Remote Sensing Society (IEEE GRSS). As for previous years, the IADF TC organized a data fusion contest aiming at fostering new ideas and solutions for multisource studies. The 2015 edition of the contest proposed a multiresolution and multisensorial challenge involving extremely high-resolution RGB images and a three-dimensional (3-D) LiDAR point cloud. The competition was framed in two parallel tracks, considering 2-D and 3-D products, respectively. In this paper, we discuss the sci…

Atmospheric Science010504 meteorology & atmospheric sciencesComputer scienceMULTIMODAL-DATA FUSIONGeophysics. Cosmic physics0211 other engineering and technologies02 engineering and technologyCONTESTcomputer.software_genre01 natural sciencesOutcome (game theory)LIDARTraitement des imagesIMAGE ANALYSIS AND DATA FUSION (IADF)DEEP NEURAL NETWORKSDeep neural networksTraitement du signal et de l'imageMULTIRESOLUTION910 Geography & travelMultiresolutionGround truthLANDCOVER CLASSIFICATIONIMAGE AERIENNE1903 Computers in Earth SciencesBenchmarkingVision par ordinateur et reconnaissance de formesOcean engineering10122 Institute of GeographyLidarDeep neural networksData miningExtremely high spatial resolutionMultimodal-data fusionLiDARComputers in Earth Sciences; Atmospheric ScienceImage analysis and data fusion (IADF)EXTREMELY HIGH SPATIAL RESOLUTIONCLASSIFICATIONTRAITEMENT IMAGE1902 Atmospheric ScienceAPPRENTISSAGE STATISTIQUEComputers in Earth SciencesTELEDETECTIONSynthèse d'image et réalité virtuelleTC1501-1800021101 geological & geomatics engineering0105 earth and related environmental sciencesLandcover classificationmultiresolution-[INFO.INFO-DB]Computer Science [cs]/Databases [cs.DB]QC801-809Intelligence artificielleMULTISOURCESensor fusionRGB color modelcomputerMultisource
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Observationally Weak TGFs in the RHESSI Data

2019

Abstract Terrestrial gamma ray flashes (TGFs) are sub‐millisecond bursts of high energetic gamma radiation associated with intracloud flashes in thunderstorms. In this paper we use the simultaneity of lightning detections by World Wide Lightning Location Network to find TGFs in the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) data that are too faint to be identified by standard search algorithms. A similar approach has been used in an earlier paper, but here we expand the data set to include all years of RHESSI + World Wide Lightning Location Network data and show that there is a population of observationally weak TGFs all the way down to 0.22 of the RHESSI detection thresh…

Atmospheric Science010504 meteorology & atmospheric sciences[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]Atmospheric ElectricityPopulationHard radiationAstrophysics01 natural sciencesLightningterrestrial gamma‐ray flahesAerosol and CloudsLatitude0103 physical sciencesEarth and Planetary Sciences (miscellaneous)RHESSIobservationally weakeducation010303 astronomy & astrophysicsResearch Articles0105 earth and related environmental sciencesPhysicseducation.field_of_studyGamma rayNetwork datathunderstormsLightningWorld widehard radiationGeophysicsSpace and Planetary ScienceAtmospheric ProcessesThunderstormResearch ArticleJournal of Geophysical Research: Atmospheres
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Astrophysical neutrinos and cosmic rays observed by IceCube

2018

The core mission of the IceCube neutrino observatory is to study the origin and propagation of cosmic rays. IceCube, with its surface component IceTop, observes multiple signatures to accomplish this mission. Most important are the astrophysical neutrinos that are produced in interactions of cosmic rays, close to their sources and in interstellar space. IceCube is the first instrument that measures the properties of this astrophysical neutrino flux and constrains its origin. In addition, the spectrum, composition, and anisotropy of the local cosmic-ray flux are obtained from measurements of atmospheric muons and showers. Here we provide an overview of recent findings from the analysis of Ic…

Atmospheric ScienceAstrophysics::High Energy Astrophysical PhenomenaAerospace EngineeringCosmic rayAstrophysicsPhysics and Astronomy(all)7. Clean energy01 natural sciencesIceCube Neutrino ObservatoryIceCubecosmic raysObservatory0103 physical sciencesNeutrinos010303 astronomy & astrophysicsCosmic raysPhysicsMuon010308 nuclear & particles physicsGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsneutrinosAstronomyAstronomy and AstrophysicsGeophysicsCosmic rays; IceCube; Neutrinos; Aerospace Engineering; Space and Planetary ScienceNeutrino detector13. Climate actionSpace and Planetary SciencePhysique des particules élémentairesGeneral Earth and Planetary SciencesNeutrinoNeutrino astronomy
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Observation of Terrestrial Gamma-Ray Flashes at Mid Latitude

2021

We present a sample of Terrestrial Gamma-ray Flashes (TGFs) observed at mid latitudes by the Atmosphere Space Interaction Monitor (ASIM). The events were detected between June 2018 and August 2020 in the latitude bands between 35° and 51° in both hemispheres, which we hereafter refer to as “mid latitudes.” The sample includes the first observations above urn:x-wiley:2169897X:media:jgrd57293:jgrd57293-math-0001 and consists of 14 events clustered in four geographical regions: north-west Atlantic and eastern USA; Mediterranean Sea; the ocean around South Africa; and north-eastern China and Siberia. We examine the characteristics of each event, both standalone and in the context of the global …

Atmospheric ScienceGeophysicsSpace and Planetary ScienceMiddle latitudesEarth and Planetary Sciences (miscellaneous)Gamma rayEnvironmental scienceAtmospheric electricityAtmospheric sciencesLightningRadiofrequency radiation
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