Search results for "spectrometer"

showing 10 items of 751 documents

Measurements with a hybrid detector prototype composed of a MOS CCD and a CZT spectrometer

2008

The scientific objectives of the future X-ray astronomy instruments require new type of focusing telescopes able to extend the observational range starting from 0.1 keV at least up to 100 keV to solve crucial question concerning the nature of the high energy emission. A challenging technology to extend the classical grazing incidence range to higher energy is today offered by the development of multilayer optics that are effective as X-ray concentrators between few keV up to 100 keV. A useful arrangement for this type of mission concept can foresee the soft (e.g. 0.1-10 keV) X-ray optics nested and coaxial with the hard-X mirrors. The focal plane of the telescope shall operate on a very wid…

PhysicsSpace technologyPixelSpectrometerPhysics::Instrumentation and Detectorsbusiness.industryAstrophysics::High Energy Astrophysical PhenomenaDetectorAstrophysics::Instrumentation and Methods for Astrophysicslaw.inventionTelescopeOpticsCardinal pointlawOptoelectronicsCoaxialbusinessImage resolutionCZT detectors2008 IEEE Nuclear Science Symposium Conference Record
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The x-ray microcalorimeter spectrometer onboard Athena

2012

Trabajo presentado a la conferencia: "Space Telescopes and Instrumentation: Ultraviolet to Gamma Ray" celebrada en Amsterdam (Holanda) el 1 de julio de 2012.-- et al.

PhysicsSpacecraftSpectrometerCalorimeter (particle physics)business.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsMissionslaw.inventionX-rayTelescopeX-ray missions micro-calorimeter AthenaOpticsCardinal pointSettore FIS/05 - Astronomia E AstrofisicaMicro-calorimeterAthena; Micro-calorimeter; Missions; X-raylawAthenaTransition edge sensorSpectral resolutionbusiness
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Isomers and high-spin structures in the N=81 isotones Xe135 and Ba137

2017

The high-spin structures of the N = 81 isotones 135Xe and 137Ba are investigated after multinucleontransfer (MNT) and fusion-evaporation reactions. Both nuclei are populated in (i) 136Xe+238U and (ii) 136Xe+208Pb MNT reactions employing the high-resolution Advanced Gamma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA, (iii), in the 136Xe+198Pt MNT reaction employing the -ray array GAMMASPHERE in combination with the gas detector array Chico, and (iv) via a 11B+130Te fusion-evaporation reaction. The high-spin level schemes of 135Xe and 137Ba are considerably extended to higher energies. The 2058-keV (19=2 ) state in 135Xe is identified as an isomer, completing the systema…

PhysicsSpectrometer010308 nuclear & particles physics0103 physical sciencesQuadrupoleSHELL modelGammasphereAGATAAtomic physics010306 general physicsSpin (physics)01 natural sciencesPhysical Review C
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High resolution spectroscopic study ofBeΛ10

2016

Spectroscopy of a Be-10(Lambda) hypernucleus was carried out at JLab Hall C using the (e, e' K+) reaction. A new magnetic spectrometer system (SPL+ HES+ HKS), specifically designed for high resolution hypernuclear spectroscopy, was used to obtain an energy spectrum with a resolution of similar to 0.78 MeV (FWHM). The well-calibrated spectrometer system of the present experiment using p(e, e' K+)Lambda, Sigma(0) reactions allowed us to determine the energy levels; and the binding energy of the ground-state peak (mixture of 1(-) and 2(-) states) was found to be B-Lambda = 8.55 +/- 0.07(stat.) +/- 0.11(sys.) MeV. The result indicates that the ground-state energy is shallower than that of an em…

PhysicsSpectrometer010308 nuclear & particles physicsBinding energyResolution (electron density)HypernucleusLambda01 natural sciencesExcited state0103 physical sciencesAtomic physicsNuclear Experiment010306 general physicsSpectroscopyGround statePhysical Review C
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Total absorption γ -ray spectroscopy of the β -delayed neutron emitters I137 and Rb95

2019

The decays of the β-delayed neutron emitters I137 and Rb95 have been studied with the total absorption γ-ray spectroscopy technique. The purity of the beams provided by the JYFLTRAP Penning trap at the ion guide isotope separator on-line facility in Jyvaskyla allowed us to carry out a campaign of isotopically pure measurements with the decay total absorption γ-ray spectrometer, a segmented detector composed of 18 NaI(Tl) modules. The contamination coming from the interaction of neutrons with the spectrometer has been carefully studied, and we have tested the use of time differences between prompt γ rays and delayed neutron interactions to eliminate this source of contamination. Due to the s…

PhysicsSpectrometer010308 nuclear & particles physicsNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaPenning trap01 natural sciencesNuclear physics13. Climate action0103 physical sciencesNeutronGamma spectroscopyNuclear Experiment010306 general physicsSpectroscopyAbsorption (electromagnetic radiation)Delayed neutronPhysical Review C
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Recoil-isomer tagging techniques at RITU

2003

Techniques have been developed to study isomeric states in nuclei with the use of RITU (gas filled separator) at the University of Jyvaskyla. The first was the recoil-isomer tagging technique initially, utilised by D.M. Cullen to study the K π = 8− isomeric state in 138Gd [1]. The juro-sphere array was employed in conjunction with ritu and a focal plane array which consisted of several Compton-suppressed Germanium detectors, placed in close geometry around a multi wire proportional counter (mwpc) and a silicon strip detector used for the implantation of recoiling nuclei. This technique correlates prompt and delayed γ-ray transitions across isomeric states and identifies the lifetime of the …

PhysicsSpectrometer010308 nuclear & particles physicsProportional counter7. Clean energy01 natural sciencesParticle detectorParticle identificationCharged particleSemiconductor detectorNuclear physicsRecoil0103 physical sciencesNeutron010306 general physics
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Near-threshold $\pi^-$ photoproduction on the deuteron

2018

The first experimental investigation of the near-threshold cross section for incoherent $\pi^-$ photoproduction on the deuteron $\gamma$ d -> $\pi^-$ pp is presented. The experimental technique involved detection of the ~131 MeV gamma ray resulting from the radiative capture of photoproduced $\pi^-$ in the target. The total cross section has been measured using an unpolarized tagged-photon beam, a liquid-deuterium target, and three very large NaI(Tl) spectrometers. The data are compared to theoretical models that give insight into the elementary reaction $\gamma$ n -> $\pi^-$ p and pion-nucleon and nucleon-nucleon final-state interactions.

PhysicsSpectrometer010308 nuclear & particles physicsRadiative captureNuclear TheoryTheoretical models01 natural sciences3. Good healthNuclear physicsNear thresholdCross section (physics)Deuterium0103 physical sciencesElementary reaction010306 general physicsNuclear ExperimentNuclear ExperimentBeam (structure)
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Lifetime measurements of excited states in neutron-rich Ti53 : Benchmarking effective shell-model interactions

2020

Level lifetimes of the yrast (5/2(-)) to 13/2(-) states in the neutron-rich nucleus Ti-53, produced in a multinucleon-transfer reaction, have been measured for the first time. The recoil distance Doppler-shift method was employed and lifetimes of the excited states were extracted by a lineshape analysis aided by GEANT4-based Monte-Carlo simulations. The experiment was performed at the Grand Accelerateur National d'Ions Lourds facility in Caen, France, by using the Advanced Gamma Tracking Array for the gamma-ray detection coupled to the large-acceptance variable mode spectrometer for an event-by-event particle identification and the Cologne plunger for deep-inelastic reactions. Reduced trans…

PhysicsSpectrometer010308 nuclear & particles physicsYrastNuclear structureShell (structure)01 natural sciences7. Clean energyParticle identificationRecoilExcited state0103 physical sciencesNeutronAtomic physicsNuclear Experiment010306 general physicsPhysical Review C
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First Glimpse of the N=82 Shell Closure below Z=50 from Masses of Neutron-Rich Cadmium Isotopes and Isomers

2020

We probe the $N=82$ nuclear shell closure by mass measurements of neutron-rich cadmium isotopes with the ISOLTRAP spectrometer at ISOLDE-CERN. The new mass of $^{132}\mathrm{Cd}$ offers the first value of the $N=82$, two-neutron shell gap below $Z=50$ and confirms the phenomenon of mutually enhanced magicity at $^{132}\mathrm{Sn}$. Using the recently implemented phase-imaging ion-cyclotron-resonance method, the ordering of the low-lying isomers in $^{129}\mathrm{Cd}$ and their energies are determined. The new experimental findings are used to test large-scale shell-model, mean-field, and beyond-mean-field calculations, as well as the ab initio valence-space in-medium similarity renormalizat…

PhysicsSpectrometerAb initioShell (structure)Closure (topology)General Physics and AstronomyRenormalization group7. Clean energy01 natural sciencesISOLTRAPIsotopes of cadmium0103 physical sciencesPhysics::Atomic and Molecular ClustersNeutronAtomic physicsNuclear Experiment010306 general physicsPhysical Review Letters
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A Broad Iron Line in the Chandra High Energy Transmission Grating Spectrum of 4U 1705-44

2005

We present the results of a Chandra 30 ks observation of the low-mass X-ray binary and atoll source 4U 1705-44. Here we concentrate on the study of discrete features in the energy spectrum at energies below ~3 keV, as well as on the iron Kalpha line, using the High Energy Transmission Grating Spectrometer on board the Chandra satellite. Below 3 keV, three narrow emission lines are found at 1.47, 2.0, and 2.6 keV. The 1.47 and 2.6 keV lines are probably identified with Lyalpha emission from Mg XII and S XVI, respectively. The identification of the feature at ~2.0 keV is uncertain because of the presence of an instrumental feature at the same energy. The iron Kalpha line at ~6.5 keV is found …

PhysicsSpectrometerAstrophysics::High Energy Astrophysical PhenomenaX-rays : starsAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsaccretion accretion diskstars : individual (4U 1705-44)Coronastars : neutronNeutron starFull width at half maximumSpace and Planetary Scienceindividual (4U 1705-44); stars : neutron; X-rays : binaries; X-rays : general; X-rays : stars [accretion accretion disks; stars]Reflection (physics)Emission spectrumLow MassX-rays : binarieLine (formation)X-rays : general
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