Search results for "GAMMA-RAY"

showing 10 items of 374 documents

Neutrinos from GRBs with ANTARES

2013

A search for muon neutrinos in coincidence with gamma-ray bursts with the ANTARES neutrino detector using data from the end of 2007 to 2011 is performed. Expected neutrino fluxes are calculated for each burst individually. The most recent numerical calculations of the spectra using the NeuCosmA code are employed, which include Monte Carlo simulations of the full underlying photohadronic interaction processes. The discovery probability for a selection of 296 gamma-ray bursts in the given period is optimised using an extended maximum-likelihood strategy. No significant excess over background is found in the data, and 90% confidence level upper limits are placed on the total expected flux acco…

observational astronomyAstronomical modelsAstrophysics and AstronomyGamma-ray astronomyPhysics::Instrumentation and DetectorsPhysicsAstrophysics::High Energy Astrophysical PhenomenaGamma ray astronomyAstrophysics::Instrumentation and Methods for AstrophysicsHigh Energy Physics::ExperimentNatural Sciences
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3rd HAWC cat. of VHE gamma-ray sources (3HWC)

2022

We present a new catalog of TeV gamma-ray sources using 1523 days of data from the High-Altitude Water Cherenkov (HAWC) Observatory. The catalog represents the most sensitive survey of the northern gamma-ray sky at energies above several TeV, with three times the exposure compared to the previous HAWC catalog, 2HWC. We report 65 sources detected at >=5{sigma} significance, along with the positions and spectral fits for each source. The catalog contains eight sources that have no counterpart in the 2HWC catalog, but are within 1{deg} of previously detected TeV emitters, and 20 sources that are more than 1{deg} away from any previously detected TeV source. Of these 20 new sources, 14 have a p…

observational astronomyAstrophysics and AstronomyGamma-ray astronomyPhysicsGamma ray astronomyNatural Sciences
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Gamma-Ray spectral energy in HAWC J1825-134 region

2022

The Earth is bombarded by ultrarelativistic particles, known as cosmic rays (CRs). CRs with energies up to a few PeV (=1015eV), the knee in the particle spectrum, are believed to have a Galactic origin. One or more factories of PeV CRs, or PeVatrons, must thus be active within our Galaxy. The direct detection of PeV protons from their sources is not possible since they are deflected in the Galactic magnetic fields. Hundred TeV {gamma}-rays from decaying {pi}0, produced when PeV CRs collide with the ambient gas, can provide the decisive evidence of proton acceleration up to the knee. Here we report the discovery by the High Altitude Water Cerenkov (HAWC) observatory of the {gamma}-ray source…

observational astronomyAstrophysics and AstronomyGamma-ray astronomyPhysicsGamma ray astronomyNatural SciencesSpectral energy distribution
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INTEGRAL observations of GRB 070311

2008

We present prompt {gamma}-ray, early NIR/optical, late optical and X-ray observations of the peculiar GRB 070311 discovered by INTEGRAL, in order to gain clues on the mechanisms responsible for the prompt {gamma}-ray pulse as well as for the early and late multi-band afterglow of GRB 070311. We fitted with empirical functions the gamma-ray and optical light curves and scaled the result to the late time X-rays.

observational astronomyAstrophysics and AstronomyX ray sourcesGamma-ray astronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsGamma ray astronomyNatural SciencesX-ray sourcescosmology
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Development of 2D & 3D cadmium–zinc–telluride spectroscopic imagers for X-ray and gamma ray applications

2021

spectroscopic X-ray imagingcharge sharingcharge lossespectroscopic X-ray and gamma-ray imaging.X-ray and gamma ray detectorCdZnTe pixel detector3D CdZnTe detectorSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)charge-sharing correctiondrift strip detector
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A Decade of GRB Follow-Up by BOOTES in Spain (2003–2013)

2016

This article covers ten years of GRB follow-ups by the Spanish BOOTES stations: 71 follow-ups providing 23 detections. Follow-ups by BOOTES-1B from 2005 to 2008 were given in a previous article and are here reviewed and updated, and additional detection data points are included as the former article merely stated their existence. The all-sky cameras CASSANDRA have not yet detected any GRB optical afterglows, but limits are reported where available.

spectroscopyArticle Subjectlcsh:Astronomy100418AFOS: Physical sciencesgamma-ray burst02 engineering and technology01 natural scienceslcsh:QB1-991emission0103 physical sciences0202 electrical engineering electronic engineering information engineeringpanchromatic observations010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsshooterenergy injectionAstronomyAstronomy and AstrophysicsBOOTEShost-galaxySpace and Planetary Science28 February 1997020201 artificial intelligence & image processingAstrophysics - High Energy Astrophysical PhenomenaafterglowGamma-ray burstAdvances in Astronomy
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Global analysis of the pMSSM in light of the Fermi GeV excess: prospects for the LHC Run-II and astroparticle experiments

2016

We present a new global fit of the 19-dimensional phenomenological Minimal Supersymmetric Standard Model (pMSSM-19) that comply with all the latest experimental results from dark matter indirect, direct and accelerator dark matter searches. We show that the model provides a satisfactory explanation of the excess of gamma-rays from the Galactic centre observed by the Fermi~Large Area Telescope, assuming that it is produced by the annihilation of neutralinos in the Milky Way halo. We identify two regions that pass all the constraints: the first corresponds to neutralinos with a mass ~80-100 GeV annihilating into WW with a branching ratio of 95% ; the second to heavier neutralinos, with mass ~…

supersymmetry and cosmologyParticle physicsMilky WayAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesgamma ray experiments7. Clean energy01 natural sciences0202 Atomic Molecular Nuclear Particle And Plasma PhysicsHigh Energy Physics - Phenomenology (hep-ph)Settore FIS/05 - Astronomia e Astrofisica0103 physical sciencesHigh Energy Physics010306 general physicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)PhysicsAnnihilationLarge Hadron Colliderdark matter detectorsdark matter theory010308 nuclear & particles physicsBranching fractionHigh Energy Physics::Phenomenologyhep-phAstronomy and AstrophysicsNuclear & Particles Physics0201 Astronomical And Space SciencesHigh Energy Physics - Phenomenology13. Climate actionExperimental High Energy PhysicsHigh Energy Physics::ExperimentHaloFermi Gamma-ray Space TelescopeMinimal Supersymmetric Standard Model
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Experimental study of 100Tc β decay with total absorption γ -ray spectroscopy

2017

The β decay of 100Tc has been studied by using the total absorption γ -ray spectroscopy technique at the Ion Guide Isotope Separator On-Line facility in Jyväskylä. In this work the new Decay Total Absorption γ -ray Spectrometer in coincidence with a cylindrical plastic β detector has been employed. The β intensity to the ground state obtained from the analysis is in good agreement with previous high-resolution measurements. However, differences in the feeding to the first-excited state as well as weak feeding to a new level at high excitation energy have been deduced from this experiment. Theoretical calculations performed in the quasiparticle random-phase approximation framework are also r…

total absorption gamma-ray spectroscopybeta decay
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r Process (n, γ) Rate Constraints from the γ Emission of Neutron Unbound States in β decay

2017

Total absorption gamma-ray spectroscopy is used to measure accurately the intensity of γγ emission from neutron-unbound states populated in the ββ-decay of delayed-neutron emitters. From the comparison of this intensity with the intensity of neutron emission a constraint on the (n, γγ) cross section for highly unstable neutron-rich nuclei can be deduced. A surprisingly large γγ branching was observed for a number of isotopes which might indicate the need to increase by a large factor the Hauser-Feshbach (n, γγ) cross-section estimates that impact on r process abundance calculations. peerReviewed

total absorption gamma-ray spectroscopybeta-delayed neutron emittersAstrophysics::High Energy Astrophysical Phenomenar-processutron-capture ratesNuclear Experiment
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Total absorption spectroscopy study of the β decay of 86Br and 91Rb

2017

The beta decays of 86Br and 91Rb have been studied using the total absorption spectroscopy technique. The radioactive nuclei were produced at the Ion Guide Isotope Separator On-Line facility in Jyväskylä and further purified using the JYFLTRAP. 86Br and 91Rb are considered to be major contributors to the decay heat in reactors. In addition, 91Rb was used as a normalization point in direct measurements of mean gamma energies released in the beta decay of fission products by Rudstam et al. assuming that this decay was well known from high-resolution measurements. Our results show that both decays were suffering from the Pandemonium effect and that the results of Rudstam et al. should be renor…

total absorption gamma-ray spectroscopyrubidiumneutron emissionHigh Energy Physics::Experimentbeta decaybromiNuclear Experiment
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