0000000000003031

AUTHOR

Wenxi Peng

0000-0002-7453-9709

showing 4 related works from this author

A charge reconstruction algorithm for DAMPE silicon microstrip detectors

2019

Abstract The DArk Matter Particle Explorer (DAMPE) can detect electrons and photons from 5 GeV to 10 TeV and charged nuclei from a few tens of GeV to 100 TeV. The silicon–tungstentracker (STK), which is composed of 768 singled-sided silicon microstrip detectors, is one of four subdetectors in DAMPE providing photon conversion , track reconstruction, and charge identification for relativistic charged particles. This paper focuses on the charge identification performance of the STK detector. The charge response depends mainly on the incident angle and the impact position of the incoming particle. To improve the charge resolution, a reconstruction algorithm to correct for these parameters was …

PhysicsNuclear and High Energy PhysicsPhotonLarge Hadron ColliderIon beamPhysics::Instrumentation and Detectors010308 nuclear & particles physicsCharge reconstructionSTKSettore FIS/01 - Fisica SperimentaleReconstruction algorithmElectron01 natural sciencesCharged particleCharge sharingIonNuclear physicsSilicon microstrip detector0103 physical sciencesDAMPEHigh Energy Physics::ExperimentCharge sharing010303 astronomy & astrophysicsInstrumentation
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The DAMPE silicon–tungsten tracker

2016

Abstract The DArk Matter Particle Explorer (DAMPE) is a spaceborne astroparticle physics experiment, launched on 17 December 2015. DAMPE will identify possible dark matter signatures by detecting electrons and photons in the 5 GeV–10 TeV energy range. It will also measure the flux of nuclei up to 100 TeV, for the study of the high energy cosmic ray origin and propagation mechanisms. DAMPE is composed of four sub-detectors: a plastic strip scintillator, a silicon–tungsten tracker–converter (STK), a BGO imaging calorimeter and a neutron detector. The STK is composed of six tracking planes of 2 orthogonal layers of single-sided micro-strip detectors, for a total detector surface of ca. 7 m2. T…

Nuclear and High Energy PhysicsCosmic rays; Dark matter; Silicon tracker; Spaceborne experiment; Nuclear and High Energy Physics; InstrumentationPhysics::Instrumentation and DetectorsCosmic rayParticle detectorsTracking (particle physics)01 natural sciencesParticle detectorOpticscosmic rays0103 physical sciencesDark matterNeutron detection010303 astronomy & astrophysicsInstrumentationAstroparticle physicsPhysicsLarge Hadron ColliderCalorimeter (particle physics)010308 nuclear & particles physicsbusiness.industryDetectorSettore FIS/01 - Fisica SperimentaleParticle detectors cosmic raysSpaceborne experimentSilicon trackerHigh Energy Physics::Experimentbusiness
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Comparison of proton shower developments in the BGO calorimeter of the Dark Matter Particle Explorer between GEANT4 and FLUKA simulations

2020

The DArk Matter Particle Explorer (DAMPE) is a satellite-borne detector for high-energy cosmic rays and $\gamma$-rays. To fully understand the detector performance and obtain reliable physical results, extensive simulations of the detector are necessary. The simulations are particularly important for the data analysis of cosmic ray nuclei, which relies closely on the hadronic and nuclear interactions of particles in the detector material. Widely adopted simulation softwares include the GEANT4 and FLUKA, both of which have been implemented for the DAMPE simulation tool. Here we describe the simulation tool of DAMPE and compare the results of proton shower properties in the calorimeter from t…

Physics - Instrumentation and DetectorsProton85Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHadronDark matterS-General Physics and AstronomyFOS: Physical sciencesCosmic rayNuclear physicsSpectral analysisInstrumentation and Methods for Astrophysics (astro-ph.IM)Monte Carlo simulationPhysicsTp9550Calorimeter (particle physics)96DetectorInstrumentation and Detectors (physics.ins-det)5513Cosmic Rays-n-tParticleHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for Astrophysics
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Calibration of the Lunar Orbital X-ray Fluorescence Imaging Spectrometer (LOXIA) of Chang'E-1 satellite at INAF-OAPA

2007

The Lunar Orbital X-ray Fluorescence Imaging Spectrometer (LOXIA) designed and constructed at the Institute of High Energy Physics of the Chinese Academy of Sciences to perform chemical composition analysis of the Moon surface will operate on-board the Chang'E-1 mission, the first Chinese lunar spacecraft to be launched in 2007. We report the main results of the calibration measurements that we have performed using the X-ray beamline of the XACT facility of INAFOsservatorio Astronomico di Palermo G.S. Vaiana to determine the quantum efficiency of the XRS detector in the soft X-rays as a function of photon energy and angle of incidence.

PhysicsX-rays Instrumentation Spectroscopy Space missions MoonPhotonSpacecraftSpectrometerbusiness.industryAstrophysics::High Energy Astrophysical PhenomenaImaging spectrometerPhoton energyOpticsBeamlineAngle of incidence (optics)Physics::Space PhysicsSatelliteAstrophysics::Earth and Planetary Astrophysicsbusiness
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