Search results for "Resolution"

showing 10 items of 1928 documents

Energy calibration of the NEXT-White detector with 1% resolution near Q ββ of 136Xe

2019

Excellent energy resolution is one of the primary advantages of electroluminescent high pressure xenon TPCs, and searches for rare physics events such as neutrinoless double-beta decay ($\beta\beta0\nu$) require precise energy measurements. Using the NEXT-White detector, developed by the NEXT (Neutrino Experiment with a Xenon TPC) collaboration, we show for the first time that an energy resolution of 1% FWHM can be achieved at 2.6 MeV, establishing the present technology as the one with the best energy resolution of all xenon detectors for $\beta\beta0\nu$ searches.

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysical measurementsPhysics::Instrumentation and DetectorsDark Matter and Double Beta DecayFísica -- Mesuramentschemistry.chemical_elementBioengineeringAtomic01 natural sciencesMathematical SciencesNuclear physicsParticle and Plasma PhysicsXenonAffordable and Clean Energy0103 physical sciencesDark Matter and Double Beta Decay (experiments)CalibrationNuclearlcsh:Nuclear and particle physics. Atomic energy. RadioactivityCalibratge010306 general physicsMathematical PhysicsPhysicsQuantum Physics010308 nuclear & particles physicsDetectorResolution (electron density)MolecularDetectorsNuclear & Particles PhysicsFull width at half maximumchemistryBeta (plasma physics)Physical SciencesCalibrationlcsh:QC770-798High Energy Physics::ExperimentNeutrinoEnergy (signal processing)
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Performance of prototypes for the ALICE electromagnetic calorimeter

2009

The performance of prototypes for the ALICE electromagnetic sampling calorimeter has been studied in test beam measurements at FNAL and CERN. A $4\times4$ array of final design modules showed an energy resolution of about 11% /$\sqrt{E(\mathrm{GeV})}$ $\oplus$ 1.7 % with a uniformity of the response to electrons of 1% and a good linearity in the energy range from 10 to 100 GeV. The electromagnetic shower position resolution was found to be described by 1.5 mm $\oplus$ 5.3 mm /$\sqrt{E \mathrm{(GeV)}}$. For an electron identification efficiency of 90% a hadron rejection factor of $>600$ was obtained.

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsHadronFOS: Physical sciencesElectron7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Physics - Instrumentation and Detectors; Physics - Instrumentation and Detectors; High Energy Physics - ExperimentDetectors and Experimental Techniques010306 general physicsNuclear ExperimentInstrumentationImage resolutionPhysicsRange (particle radiation)Large Hadron Collider010308 nuclear & particles physicsLinearityInstrumentation and Detectors (physics.ins-det)CalorimeterHigh Energy Physics::ExperimentALICE (propellant)
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Calibration strategy of the JUNO experiment

2021

We present the calibration strategy for the 20 kton liquid scintillator central detector of the Jiangmen Underground Neutrino Observatory (JUNO). By utilizing a comprehensive multiple-source and multiple-positional calibration program, in combination with a novel dual calorimetry technique exploiting two independent photosensors and readout systems, we demonstrate that the JUNO central detector can achieve a better than 1% energy linearity and a 3% effective energy resolution, required by the neutrino mass ordering determination. [Figure not available: see fulltext.]

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsmeasurement methodsscintillation counter: liquidenergy resolutionFOS: Physical sciencesPhotodetectorScintillator53001 natural sciencesNOHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)hal-03022811PE2_2Optics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Calibrationlcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAstrophysiqueJiangmen Underground Neutrino ObservatoryPhysicsJUNOliquid [scintillation counter]010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsLinearityInstrumentation and Detectors (physics.ins-det)calibrationNeutrino Detectors and Telescopes (experiments)lcsh:QC770-798High Energy Physics::ExperimentNeutrinobusinessEnergy (signal processing)Journal of High Energy Physics
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Temperature effect on RPC performance in the ARGO-YBJ experiment

2009

The ARGO-YBJ experiment has been taking data for nearly 2 years. In order to monitor continuously the performance of the Resistive Plate Chamber detectors and to study the daily temperature effects on the detector performance, a cosmic ray muon telescope was setup near the carpet detector array in the ARGO-YBJ laboratory. Based on the measurements performed using this telescope, it is found that, at the actual operating voltage of 7.2kV, the temperature effect on the RPC time resolution is about 0.04ns/degrees C and on the particle detection efficiency is about 0.03%/degrees C. Based on these figures we conclude that the environmental effects do not affect substantially the angular resoluti…

Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaCosmic rayEfficiencytelescopelaw.inventionTelescopeOpticslawAngular resolutionOperating voltagetime resolutionInstrumentationArgoPhysicsMuonbusiness.industryDetectorSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsTime resolutionTime resolutionCosmic Ray TelescopeefficiencyRPCHigh Energy Physics::Experimentbusiness
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Observation of the cosmic-ray shadow of the Moon with IceCube

2013

We report on the observation of a significant deficit of cosmic rays from the direction of the Moon with the IceCube detector. The study of this "Moon shadow" is used to characterize the angular resolution and absolute pointing capabilities of the detector. The detection is based on data taken in two periods before the completion of the detector: between April 2008 and May 2009, when IceCube operated in a partial configuration with 40 detector strings deployed in the South Pole ice, and between May 2009 and May 2010 when the detector operated with 59 strings. Using two independent analysis methods, the Moon shadow has been observed to high significance (> 6 sigma) in both detector config…

Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesNEUTRINO TELESCOPESPosition (vector)SEARCH0103 physical sciencesShadowAngular resolutionddc:530ARRIVAL DIRECTIONS010303 astronomy & astrophysicsDETECTORAnalysis methodHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsANISOTROPY010308 nuclear & particles physicsDetectorSUNAstronomyANGULAR RESOLUTIONEarth's magnetic fieldDeflection (physics)Physics and AstronomyAstrophysics - High Energy Astrophysical Phenomena
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Detector characterization and first coincidence tests of a Compton telescope based on LaBr3 crystals and SiPMs

2011

International audience; A Compton telescope for dose monitoring in hadron therapy consisting of several layers of continuous LaBr3 crystals coupled to silicon photomultiplier (SiPM) arrays is under development within the ENVISION project. In order to test the possibility of employing such detectors for the telescope, a detector head consisting of a continuous 16 mm×18 mm×5 mm LaBr3 crystal coupled to a SiPM array has been assembled and characterized, employing the SPIROC1 ASIC as readout electronics. The best energy resolution obtained at 511 keV is 6.5% FWHM and the timing resolution is 3.1 ns FWHM. A position determination method for continuous crystals is being tested, with promising res…

Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsCompton telescopeSiPM01 natural sciences7. Clean energyCoincidence030218 nuclear medicine & medical imaginglaw.inventionTelescope03 medical and health sciencesHadron therapy0302 clinical medicineOpticsSilicon photomultiplierApplication-specific integrated circuitlaw0103 physical sciencesCompton imaging[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det][SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/MicroelectronicsInstrumentationPhysicsContinuous crystal010308 nuclear & particles physicsbusiness.industryResolution (electron density)DetectorMPPCG-APDLaBr3Full width at half maximumbusiness
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Particle identification with the fast COMPASS RICH-1 detector

2009

International audience; A new photon detection system for the COMPASS RICH-1 detector has been designed and installed. In the central region, the project is based on multi-anode photo-multiplier technology accompanied by charge sensitive, high resolution and dead-time free time digitization. In the outer area, only the readout electronics for the existing photon detectors has been replaced. Details on the detector upgrade and its performance are presented.

Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsPhoton detectorMulti-anode photo-multiplierComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONHigh resolution[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesCOMPASSParticle identificationTDCParticle identificationOpticsCompass0103 physical sciences010306 general physicsInstrumentationRICHPhysics010308 nuclear & particles physicsbusiness.industryDetectorCharge (physics)Front-end electronicsUpgradeCOMPASS; RICH; Multi-anode photo-multiplier; Particle identification; Front-end electronics; TDCHigh Energy Physics::ExperimentbusinessPhoton detectionFront-end electronic
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High resolution detectors based on continuous crystals and SiPMs for small animal PET

2012

International audience; Sensitivity and spatial resolution are the two main factors to maximize in emission imaging. The improvement of one factor deteriorates the other with pixelated crystals. In this work we combine SiPM matrices with monolithic crystals, using an accurate γ-ray interaction position determination algorithm that provides depth of interaction. Continuous crystals provide higher sensitivity than pixelated crystals, while an accurate interaction position determination does not degrade the spatial resolution. Monte Carlo simulations and experimental data show good agreement both demonstrating sub-millimetre intrinsic spatial resolution. A system consisting in two rotating det…

Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSiPMMonte Carlo methodHigh resolution01 natural sciencesCoincidence030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineOpticsSilicon photomultiplierPosition (vector)0103 physical sciencesHigh resolutionSensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det][SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/MicroelectronicsInstrumentationImage resolutionPhysics010308 nuclear & particles physicsbusiness.industryDetectorPosition determinationPETMonolithic crystalsbusiness
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Fast Interaction Trigger for ALICE upgrade

2022

We present the structure, functionalities and the first in-beam performance of the ALICE Fast Interaction Trigger (FIT). FIT comprises three detectors: FT0, FV0 and FDD, which use Cherenkov and scintillation effects to detect charged particles originating from proton-proton (pp) and heavy-ion collisions. FIT generates triggers for ALICE, monitors luminosity and background, measures collision time, and determines global collision parameters, such as forward multiplicity, centrality and event plane. FIT uses dedicated front-end electronics to measure time and charge of pulses at pp bunch crossing interval of 25 ns and pp (Pb-Pb) interaction rates of up to 1 MHz (50 kHz). FIT has been installe…

Nuclear and High Energy PhysicsPhysics::Instrumentation and Detectorsdetector performanceTime resolutionhiukkasfysiikkaScintillatorALICE FIT114 Physical sciencesscintillatortrigger detectorAlice fitmittajärjestelmätDetectors and Experimental TechniquesNuclear ExperimentInstrumentationtime resolutionTrigger detectorDetector performanceCherenkov detector
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Depth resolution optimization for low-energy ERDA

2007

Abstract With the implementation of low-energy time-of-flight Elastic Recoil Detection Analysis (ERDA), routine analysis of thin films with high depth resolution becomes possible. The optimization of the measurement conditions is a key issue for an accurate sample characterization and is normally a compromise among depth resolution, mass resolution and sensitivity, for a given sample. In this work, we focus on the depth resolution optimization, presenting an extensive study of two different materials, SiO 2 and TiN, representative of light and medium mass targets. The film thickness varies between 10 and 50 nm. The samples were measured with different beams ( 35 Cl, 63 Cu, 79 Br and 127 I),…

Nuclear and High Energy PhysicsResolution (mass spectrometry)business.industryScatteringMonte Carlo methodchemistry.chemical_elementCharacterization (materials science)Elastic recoil detectionTime of flightOpticschemistryThin filmTinbusinessInstrumentationNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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