0000000000304124

AUTHOR

Jiawei Yang

showing 3 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 enhanced X-ray Timing and Polarimetry mission—eXTP

2019

In this paper we present the enhanced X-ray Timing and Polarimetry mission - eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to det…

Gravity (chemistry)Computer sciencespace mission: eXTPX-ray timingPolarimetryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences7. Clean energyPhysics and Astronomy (all)Settore FIS/05 - Astronomia E AstrofisicaObservatoryX-ray instrumentation0103 physical sciencesX-ray polarimetryGround segmentAerospace engineering010306 general physics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)High Energy Astrophysical Phenomena (astro-ph.HE)Spacecraftsezelebusiness.industryPayloadGravitational waveAstrophysics::Instrumentation and Methods for Astrophysicsspace mission: eXTP; X-ray instrumentation; X-ray polarimetry; X-ray timing; Physics and Astronomy (all)Space SciencebusinessAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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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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