Search results for "Detectors"

showing 10 items of 2229 documents

High-speed and high-resolution interrogation of FBG sensors using wavelength-to-time mapping and Gaussian filters

2019

In this work we report a novel intensity-based technique for simultaneous high-speed and high-resolution interrogation of fiber Bragg grating (FBG) sensors. The method uses a couple of intensity Gaussian filters and the dispersion-induced wavelength-to-time mapping effect. The Bragg wavelength is retrieved by means of the amplitude comparison between the two filtered grating spectrums, which are mapped into a time-domain waveform. In this way, measurement distortions arising from residual power due to the grating sidelobes are completely avoided, and the wavelength measurement range is considerably extended with respect to the previously proposed schemes. We present the mathematical backgro…

Optical fiberoptical fibersPhysics - Instrumentation and DetectorsGaussianPhysics::OpticsFOS: Physical sciences//purl.org/becyt/ford/2.2 [https]Gratinglaw.inventionsymbols.namesakeOpticsFiber Bragg gratinglawWaveformphotonic sensorssensor monitoringfiber opticsPhysicsUNESCO::FÍSICA::ÓpticaSignal processingfiber sensorsbusiness.industryfiber bragg fratingInstrumentation and Detectors (physics.ins-det)Atomic and Molecular Physics and OpticsWavelengthLight intensity//purl.org/becyt/ford/2 [https]:FÍSICA::Óptica [UNESCO]symbolsbusinessfiber Bragg gratingsPhysics - OpticsOptics (physics.optics)
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Calibration of the RPC charge readout in the ARGO-YBJ experiment

2012

""The charge readout of Resistive Plate Chambers (RPCs) is implemented in the ARGO-YBJ experiment to measure the charged particle density of the shower front up to 10^4\\\/m^2, enabling the study of the primary cosmic rays with energies in the ''knee'' region. As the first time for RPCs being used this way, a telescope with RPCs and scintillation detectors is setup to calibrate the number of charged particles hitting a RPC versus its charge readout. Air shower particles are taken as the calibration beam. The telescope was tested at sea level and then moved to the ARGO-YBJ site for coincident operation with the ARGO-YBJ experiment. The charge readout shows good linearity with the particle de…

Optical telescopesNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsCamere a Piastre Resistive (RPC)Resistive plate chamberAstrophysics::High Energy Astrophysical PhenomenaCosmic raylaw.inventionTelescopeSettore FIS/05 - Astronomia E AstrofisicaOpticslawCoincidentAir showersCalibrationSea levelInstrumentationParticle densitiesCosmic raysResistive Plate Chambers Charge read-out Extended Air ShowersPhysicsAir showers Charge readout Dynamic range Knee regions Particle densities Resistive plate chambers; Calibration Charged particles Cosmic rays Experiments Optical telescopes Sea level Telescopes; Particle spectrometersResistive touchscreenScintillationDynamic rangeCharge readoutParticle spectrometersbusiness.industryCharged particlesSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsCharged particleAir showerCalibrazione della Risposta Analogica di RPCKnee regionsLettura Analogica di RPCCalibrationResistive plate chambersbusinessExperimentsTelescopes
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Time calibration of the ANTARES neutrino telescope

2011

The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a relative time calibration between the photomultipliers at the level of ~1 ns. The methods developed to attain this level of precision are described.

Optical telescopesPhysics - Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectors01 natural sciencesOptimal performanceHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Calibration procedureDimensional arraysAngular resolution[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino energyNEUTRINO TELESCOPE010303 astronomy & astrophysicsPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)Deep seaNeutrino detectorRelative timeCalibrationFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsTime calibrationPhotomultiplier[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cherenkov lightAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesScattering lengthNeutrino TelescopesOptical telescopeNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Tellurium compounds0103 physical sciencesOptical systemsCalibrationAngular resolution14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORCherenkov radiationtime calibration; neutrino telescopes; antaresANTARES010308 nuclear & particles physicsNeutrino interactionsAstronomyElementary particlesAstronomy and AstrophysicsPhotomultipliersFISICA APLICADAHigh Energy Physics::ExperimentUNDERWATER DETECTORNeutrino telescopesSYSTEM
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ANTARES: The first undersea neutrino telescope

2011

The ANTARES Neutrino Telescope was completed in May 2008 and is the first operational Neutrino Telescope in the Mediterranean Sea. The main purpose of the detector is to perform neutrino astronomy and the apparatus also offers facilities for marine and Earth sciences. This paper describes the design, the construction and the installation of the telescope in the deep sea, offshore from Toulon in France. An illustration of the detector performance is given. © 2011 Elsevier B.V. All rights reserved.

Optical telescopesPhysics::Instrumentation and DetectorsAstronomyMarine engineeringSubmarine cablesAstrophysics01 natural scienceslaw.inventionAstroparticlelaw010303 astronomy & astrophysicsInstrumentationPhysicsDense wavelength division multiplexingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsSubmarine cableDeep seaNeutrino astronomyFísica nuclearNeutrinoMarine technologyAstrophysics - Instrumentation and Methods for AstrophysicsNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Wet mateable connectorAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLINEOptical telescopePhysics::GeophysicsTelescopePhotomultiplier tube0103 physical sciencesNeutrinoDWDM14. Life underwaterDeep sea detectorInstrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORAstroparticle physics010308 nuclear & particles physicswet mateable connector.Marine technologyAstronomyElementary particles[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]PhotomultipliersKM3NeTFISICA APLICADAEarth (planet)High Energy Physics::ExperimentNeutrino astronomyastroparticle; neutrino astronomy; marine technology; dwdm; photomultiplier tube; deep sea detector; submarine cable; wet mateable connector; neutrinoSYSTEMTelescopes
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The ANTARES telescope neutrino alert system

2012

The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.

Optical telescopesPhysics::Instrumentation and DetectorsAstrophysics7. Clean energy01 natural sciencesGamma ray burstsFOLLOW-UP OBSERVATIONSlaw.inventionlawFlaring activeVery high energiesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGAMMA-RAY BURSTS[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsSupernovaNeutrino detectorNeutrino astronomyFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesOptical telescopeTelescopeMuon tracksCoincidentSEARCHDetection methods0103 physical sciencesCore collapse supernovae010306 general physicsOptical follow-upInstrumentation and Methods for Astrophysics (astro-ph.IM)Neutronsantares; neutrino astronomy; optical follow-up; transient sourcesANTARES010308 nuclear & particles physicsGamma raysAstronomyAstronomy and AstrophysicsAlert systemsStarsTransient sources[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Optical signalsPotential sources13. Climate actionFISICA APLICADAHigh Energy Physics::ExperimentNeutrino astronomyGamma-ray burst
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"Table 11" of "Search for a heavy charged boson in events with a charged lepton and missing transverse momentum from $pp$ collisions at $\sqrt{s} = 1…

2019

Product of acceptance and efficiency for the electron and muon selections as a function of the $W^\prime$ pole mass.

P P --> E- NU X13000.0Physics::Instrumentation and DetectorsMathematics::Number TheoryP P --> E+ NU XPhysics::Accelerator PhysicsEFFHigh Energy Physics::ExperimentP P --> MU- NU XACCP P --> MU+ NU X
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"Table 1" of "Search for Heavy Long-Lived Charged Particles with the ATLAS detector in pp collisions at sqrt(s) = 7 TeV"

2011

Distribution of BETA for all candidates in the slepton search. Data are presented for inclusive muon production and for di-muons from Z0 decays together with Monte Carlo predictions of the latter.

P P --> SLEPTON XInclusiveProton-Proton ScatteringPhysics::Instrumentation and DetectorsPhysics::Accelerator Physics7000.0High Energy Physics::ExperimentN
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"Table 4" of "Search for Supersymmetry in Events with Large Missing Transverse Momentum, Jets, and at Least One Tau Lepton in 7 TeV Proton-Proton Col…

2013

The Acceptance, Efficiency and Acceptance x Efficiency for the tau+muon channel as a function of Lambda and Tan(Beta).

P P --> TAU MUON JETS MMProton-Proton ScatteringPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyExclusiveSUSY7000.0High Energy Physics::ExperimentSupersymmetryJet ProductionTau productionMuon production
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"Table 3" of "Measurement of the Transverse Momentum Distribution of W Bosons in pp Collisions at sqrt(s) = 7 TeV with the ATLAS Detector"

1970

The normalized, differential cross secton from the Muon and Electron decay channel Combined for the Born-level PT definition.

P P --> W+ XInclusiveSingle Differential Cross SectionProton-Proton ScatteringPhysics::Instrumentation and DetectorsP P --> W- X7000.0High Energy Physics::ExperimentDSIG/DPTTransverse Momentum DependenceW Production
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"Table 2" of "Measurement of the Transverse Momentum Distribution of W Bosons in pp Collisions at sqrt(s) = 7 TeV with the ATLAS Detector"

1970

The normalized, differential cross secton measured in the W to Muon decay channel for the three different PT definitions, Born, Dressed and Bare.

P P --> W+ XInclusiveSingle Differential Cross SectionProton-Proton ScatteringPhysics::Instrumentation and DetectorsP P --> W- X7000.0High Energy Physics::ExperimentDSIG/DPTTransverse Momentum DependenceW ProductionMuon production
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