Search results for "Gamma-ray"

showing 10 items of 374 documents

Effects of dead time losses on terrestrial gamma ray flash measurements with the Burst and Transient Source Experiment

2010

[1] Measurements from the Burst and Transient Source Experiment (BATSE) instrument on the Compton Gamma Ray Observatory (CGRO) are the only ones where characteristics of single terrestrial gamma ray flashes (TGFs) have been obtained thus far. However, it has been reported that the measurements suffer from significant dead time losses which complicates the analysis and raises question about earlier BATSE studies. These losses are due to the high-intensity flux combined with limitations of the time resolution of the instrument. Since these losses will affect both the spectrum and the temporal distribution of the individual TGFs, results based on BATSE data need to be revisited, including our …

Atmospheric SciencePhotonMonte Carlo methodSoil ScienceFluxAstrophysicsAquatic ScienceOceanographyOpticsGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Earth-Surface ProcessesWater Science and TechnologyPhysicsEcologybusiness.industryGamma rayPaleontologyForestryDead timeLight curveGeophysicsSpace and Planetary ScienceTransient (oscillation)businessTerrestrial gamma-ray flashJournal of Geophysical Research: Space Physics
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Experiences of radioactivity measurement in various environmental samples

2013

An overview on our activity of environmental radioactivity measurement is reported. Radionuclide concentration have been evaluated in the particulate air, soils and rocks, drinking and surface water, wastewater, marine sediments and so on. Most of radionuclide concentration evaluation were performed using facilities of DEIM Department of Palermo University. In particular, particulate collection was performed by suction of atmospheric air through 45x45 Sofiltra-Poelman HYN-75 (Bleu type) cellulose filter paper using a high-volume air sampler located on the roof of our department building (20 m above ground-level), located within an undisturbed large park area in the city of Palermo (latitude…

Beryllium-7Environmental radioactivitySettore ING-IND/20 - Misure E Strumentazione NucleariLead-210Gamma-ray Spectrometry
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Alternative single-reference coupled cluster approaches for multireference problems: the simpler, the better.

2011

We report a general implementation of alternative formulations of single-reference coupled cluster theory (extended, unitary, and variational) with arbitrary-order truncation of the cluster operator. These methods are applied to compute the energy of Ne and the equilibrium properties of HF and C(2). Potential energy curves for the dissociation of HF and the BeH(2) model computed with the extended, variational, and unitary coupled cluster approaches are compared to those obtained from the multireference coupled cluster approach of Mukherjee et al. [J. Chem. Phys. 110, 6171 (1999)] and the internally contracted multireference coupled cluster approach [F. A. Evangelista and J. Gauss, J. Chem. …

Bond lengthCoupled clusterChemistryQuantum mechanicsMolecular vibrationGaussAnharmonicityGeneral Physics and AstronomyPhysics::Chemical PhysicsPhysical and Theoretical ChemistryUnitary statePotential energyFermi Gamma-ray Space TelescopeThe Journal of chemical physics
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Relativistic beaming and gamma-ray brightness of blazars

2009

We investigate the dependence of gamma-ray brightness of blazars on intrinsic properties of their parsec-scale radio jets and the implication for relativistic beaming. By combining apparent jet speeds derived from high-resolution VLBA images from the MOJAVE program with millimetre-wavelength flux density monitoring data from Metsahovi Radio Observatory, we estimate the jet Doppler factors, Lorentz factors, and viewing angles for a sample of 62 blazars. We study the trends in these quantities between the sources which were detected in gamma-rays by the Fermi Large Area Telescope (LAT) during its first three months of science operations and those which were not detected. The LAT-detected blaz…

BrightnessCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenajets [galaxies]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionTelescopesymbols.namesakeRelativistic beaminglawquasars: general0103 physical sciencesBlazar010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GalaxiasHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physicsGamma rayAstronomy and Astrophysicsgalaxies: jetsViewing angle:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Lorentz factorSpace and Planetary Scienceactive [galaxies]BL Lacertae objectssymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaAstrophysics - High Energy Astrophysical Phenomenagalaxies: active; ; ; BL Lacertae objects : generalFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo

2019

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38 10-6 (modeled) and 3.1 10-4 (unmodeled). We do not find any significant evidence for gravitational-wave signals associate…

Burst astrophysicAstrofísicaneutron star: binary010504 meteorology & atmospheric sciencesBinary numberAstrophysics01 natural sciencesLIGOQCSUPERNOVArelativistic jetsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01counterpartGRBGravitational waves (678)Physical SciencesRELATIVISTIC JETSAstrophysics - High Energy Astrophysical PhenomenaGravitational waveGravitationstarsblack-holeAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology (gr-qc)precursor activityGravitational wavesSettore FIS/05 - Astronomia e AstrofisicasupernovaCORE-COLLAPSEGamma-ray burstGravitational wave sourcesScience & TechnologyVirgoRCUKAstronomy and AstrophysicsHigh energy astrophysics (739)RedshiftDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie Kartographiedetector: sensitivityVIRGOSpace and Planetary Sciencegravitational radiation: emissionBLACK-HOLEddc:520Gravitational wave astronomyGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSGravitacióAstronomySignalGeneral Relativity and Quantum CosmologyBurst astrophysicslocalizationemission010303 astronomy & astrophysicsPhysicsDetectorGamma-ray bursts (629)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourcePRECURSOR ACTIVITYGamma-ray burstsLIGO (920)High energy astrophysicsdata analysis methodBurst astrophysics (187)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstAstronomy & AstrophysicsMASSgravitational radiation: direct detectionGravitational wave astronomy Gravitational wave sources LIGO; Gravitational waves Gamma-ray bursts Burst astrophysics High energy astrophysicsGravitational wave astronomy (675)electromagnetic field: production0103 physical sciencesnumerical calculationsGRB; gravitational waves; LIGO; VirgoSTFC0105 earth and related environmental sciencesgravitational wavesneutron starsGravitational waveCOUNTERPARTgravitational radiationLIGOcore-collapsegravitational radiation detectorGravitational wave sources (677)radiationNeutron starPhysics and AstronomymassRADIATIONEMISSIONGravitational wave astronomy; Gravitational wave sources; LIGO; Gravitational waves; Gamma-ray bursts; Burst astrophysics; High energy astrophysics
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Development of a 3D CZT detector prototype for Laue Lens telescope

2010

We report on the development of a 3D position sensitive prototype suitable as focal plane detector for Laue lens telescope. The basic sensitive unit is a drift strip detector based on a CZT crystal, (similar to 19x8 mm(2) area, 2.4 mm thick), irradiated transversally to the electric field direction. The anode side is segmented in 64 strips, that divide the crystal in 8 independent sensor (pixel), each composed by one collecting strip and 7 (one in common) adjacent drift strips. The drift strips are biased by a voltage divider, whereas the anode strips are held at ground. Furthermore, the cathode is divided in 4 horizontal strips for the reconstruction of the third interaction position coord…

CDTE DETECTORSPhysicsPhysics::Instrumentation and Detectorsbusiness.industryDetectorVoltage dividerGamma ray spectroscopySTRIPSCZT detectorCZT detectors 3D detectors Laue lensCathodeParticle detectorlaw.inventionAnodeLens (optics)TelescopeOpticsHard X- and soft gamma-ray astronomy3D imagingDrift striplawCDZNTEbusiness
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Deformation and mixing of coexisting shapes in neutron-deficient polonium isotopes

2015

Coulomb-excitation experiments are performed with postaccelerated beams of neutron-deficient Po196,198,200,202 isotopes at the REX-ISOLDE facility. A set of matrix elements, coupling the low-lying states in these isotopes, is extracted. In the two heaviest isotopes, Po200,202, the transitional and diagonal matrix elements of the 2+1 state are determined. In Po196,198 multistep Coulomb excitation is observed, populating the 4+1,0+2, and 2+2 states. The experimental results are compared to the results from the measurement of mean-square charge radii in polonium isotopes, confirming the onset of deformation from Po196 onwards. Three model descriptions are used to compare to the data. Calculati…

CHARGE RADIINuclear and High Energy PhysicsTRANSITION-PROBABILITYchemistry.chemical_elementCoulomb excitation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciences114 Physical sciencessymbols.namesakeMatrix (mathematics)NUCLEAR-DATA SHEETSCOULOMB-EXCITATION0103 physical sciencesSTATE PROPERTIESNuclear Physics - ExperimentNeutronfysiikka010306 general physicsEVEN-EVEN NUCLIDESMixing (physics)isotopesPoloniumINTRUDER STATESGAMMA-RAY SPECTROSCOPYPhysicsSPIN STATESisotoopitPO ISOTOPESIsotopeta114010308 nuclear & particles physicsBohr modelchemistryPhysics and AstronomysymbolsAtomic physicsInteracting boson modelphysicspolonium25.70.De 23.20.Js 25.60.−t 27.80.+w
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Advances in High-Energy-Resolution CdZnTe Linear Array Pixel Detectors with Fast and Low Noise Readout Electronics

2023

Radiation detectors based on Cadmium Zinc Telluride (CZT) compounds are becoming popular solutions thanks to their high detection efficiency, room temperature operation, and to their reliability in compact detection systems for medical, astrophysical, or industrial applications. However, despite a huge effort to improve the technological process, CZT detectors&rsquo; full potential has not been completely exploited when both high spatial and energy resolution are required by the application, especially at low energies (&lt;10 keV), limiting their application in energy-resolved photon counting (ERPC) systems. This gap can also be attributed to the lack of dedicated front-end electronics whic…

CZTSettore FIS/01 - Fisica SperimentaleX-ray spectroscopyCdZnTeGamma-ray spectroscopyElectrical and Electronic EngineeringBiochemistryInstrumentationSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)nuclear microelectronicsAtomic and Molecular Physics and Opticssemiconductor radiation detectorsAnalytical ChemistrySensors
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The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s

2018

e-ASTROGAM is a concept for a breakthrough observatory space mission carrying a gamma-ray telescope dedicated to the study of the non-thermal Universe in the photon energy range from 0.15 MeV to 3 GeV. The lower energy limit can be pushed down to energies as low as 30 keV for gamma-ray burst detection with the calorimeter. The mission is based on an advanced space-proven detector technology, with unprecedented sensitivity, angular and energy resolution, combined with remarkable polarimetric capability. Thanks to its performance in the MeV-GeV domain, substantially improving its predecessors, e-ASTROGAM will open a new window on the non-thermal Universe, making pioneering observations of the…

Cherenkov Telescope ArrayHigh-energy astrophysical phenomenaCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomyenergy resolution7. Clean energy01 natural sciencesSpace missionlaw.inventionIceCubeEinstein TelescopelawObservatoryLIGO010303 astronomy & astrophysicsKM3NeTPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Applied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionGamma-ray astronomyGamma-ray polarizationCondensed Matter Physicsphoton: energyobservatoryNuclear astrophysicsApace missionAstrophysics - High Energy Astrophysical Phenomenaperformancedetector: technologyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstspace missionCompton and pair creation telescopeTelescope0103 physical sciencessupernovaElectroniccalorimetergamma ray: detectorOptical and Magnetic MaterialsKAGRAElectrical and Electronic Engineering010306 general physicsTime domain astronomyLISAGamma-ray astronomyEinstein TelescopeAstronomyInstitut für Physik und AstronomieTime-domain astronomyCherenkov Telescope ArraysensitivityLIGOmessengerKM3NeTVIRGO13. Climate actionCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic Engineeringddc:520galaxyCompton and pair creation telescope; Gamma-ray astronomy; gamma-ray polarization; high-energy astrophysical phenomena; space mission; time-domain astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic Engineering[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

2021

Full list of authors: Acharyya, A.; Adam, R.; Adams, C.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Alves Batista, R.; Amati, L.; Ambrosi, G.; Angüner, E. O.; Antonelli, L. A.; Aramo, C.; Araudo, A.; Armstrong, T.; Arqueros, F.; Asano, K.; Ascasíbar, Y. Ashley, M.; Balazs, C.; Ballester, O.; Baquero Larriva, A.; Barbosa Martins, V.; Barkov, M.; Barres de Almeida, U.; Barrio, J. A.; Bastieri, D.; Becerra, J.; Beck, G.; Becker Tjus, J.; Benbow, W.; Benito, M.; Berge, D.; Bernardini, E.; Bernlöhr, K.; Berti, A.; Bertucci, B.; Beshley, V.; Biasuzzi, B.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Blazek, J.; Bocchino, F.; Boisson, C.; Bonneau Arbe…

Cherenkov Telescope ArrayMATÉRIA ESCURAscale: TeVAstronomyatmosphere [Cherenkov counter]dark matter experimentDark matter theoryenergy resolutionGamma ray experimentsParticleAstrophysicscosmic background radiation01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)benchmarkWIMPHESSenergy: fluxTeV [scale]relativistic [charged particle]gamma ray experimentMAGIC (telescope)Monte CarloEvent reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Contractionspatial distributiontrack data analysisPhysicsdensity [dark matter]ClumpyAstrophysics::Instrumentation and Methods for AstrophysicsimagingHigh Energy Physics - Phenomenologydark matter experiments; dark matter theory; gamma ray experiments; galaxy morphologyDark matter experimentsFísica nuclearVERITASAstrophysics - High Energy Astrophysical PhenomenaSimulationsnoiseWIMPAstrophysics::High Energy Astrophysical PhenomenaDark mattersatelliteCosmic background radiationFOS: Physical sciencesAnnihilationdark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsCherenkov counter: atmosphereheavy [dark matter]530annihilation [dark matter]GLASTDark matter experiments; Dark matter theory; Galaxy morphology; Gamma ray experimentscosmic radiation [p]0103 physical sciencesCherenkov [radiation]Candidatesddc:530AGNCherenkov radiationRadiative Processesthermal [cross section]010308 nuclear & particles physicsFísicadark matter: annihilationGamma-Ray SignalsCherenkov Telescope Array ; dark matter ; Galactic Center ; TeV gamma-ray astronomyAstronomy and AstrophysicsMassCherenkov Telescope Arrayradiation: CherenkovsensitivityMAGICGalaxyAstronomíadark matter: heavygamma rayp: cosmic radiation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]correlationcharged particle: relativisticflux [energy]Galaxy morphology/dk/atira/pure/subjectarea/asjc/3100/3103galaxysupersymmetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cross section: thermal
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