S. L. Xiong

ORCID: 0009-0005-9942-7059
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About
Contact & Profiles
Research Areas
  • Astrophysical Phenomena and Observations
  • Geoscience and Mining Technology
  • Pulsars and Gravitational Waves Research
  • Geomechanics and Mining Engineering
  • Astrophysics and Cosmic Phenomena
  • Gamma-ray bursts and supernovae
  • Testicular diseases and treatments
  • Sperm and Testicular Function
  • Remote Sensing and Land Use
  • Geochemistry and Geochronology of Asian Mineral Deposits
  • Solar and Space Plasma Dynamics
  • Particle Detector Development and Performance
  • Sexual Differentiation and Disorders
  • Advanced Optical Sensing Technologies
  • Geophysics and Gravity Measurements
  • Particle accelerators and beam dynamics
  • Genetic and Clinical Aspects of Sex Determination and Chromosomal Abnormalities
  • Advanced Algorithms and Applications
  • Infrared Target Detection Methodologies
  • Radar Systems and Signal Processing
  • Gyrotron and Vacuum Electronics Research
  • Mechanics and Biomechanics Studies
  • Atomic and Subatomic Physics Research
  • Geological and Geophysical Studies
  • Radiation Detection and Scintillator Technologies

Chengdu University of Traditional Chinese Medicine
2024-2025

China Academy of Engineering Physics
2024

Institute of High Energy Physics
2019-2020

Chinese Academy of Sciences
2019-2020

CAE (Canada)
1991

Despite over 50 years of research, many open questions remain about the origin and nature GRBs. Polarization measurements prompt emission these extreme phenomena have long been thought to be key answering a range questions. The POLAR detector was designed produce first set detailed reliable polarization in an energy approximately 50-500 keV. During late 2016 early 2017, detected total 55 Analysis results 5 GRBs reported past. were found consistent with low or unpolarized flux. However,...

10.1051/0004-6361/202037915 article EN Astronomy and Astrophysics 2020-09-29

In this work, we report the in-orbit demonstration of X-ray pulsar navigation with Insight-Hard Modulation Telescope (Insight-HXMT), which was launched on Jun. 15th, 2017. The new method 'Significance Enhancement Pulse-profile Orbit-dynamics' (SEPO) is adopted to determine orbit observations only one pulsar. test, Crab chosen and observed by Insight-HXMT from Aug. 31th Sept. 5th in Using 5-day-long observation data, determined successfully three telescopes onboard - High Energy (HE), Medium...

10.3847/1538-4365/ab3718 article EN The Astrophysical Journal Supplement Series 2019-08-21

A sizeable fraction of gamma-ray burst (GRB) light curves (LCs) feature a sequence peaks that hold information on the unknown way energy is released and dissipated into gamma-rays over time. Traditionally, searches for periodic signals in GRB LCs have turned out to be inconclusive, partly because they are challenging as consequence short-lived, coloured-noise, non-stationary nature themselves. Yet, recent claims revived issue. We aim search components through new approach GRBs avoids most...

10.1051/0004-6361/202452326 article EN Astronomy and Astrophysics 2025-04-18

10.1109/icops58192.2024.10626607 article EN 2020 IEEE International Conference on Plasma Science (ICOPS) 2024-06-16

After 34 years, the black-hole candidate EXO 1846-031 went into outburst again in 2019. We investigate its spectral properties hard intermediate and soft states with NuSTAR Insight-HXMT. A reflection component has been detected two but possibly originating from different illumination spectra: state, illuminating source is attributed to a coronal component, which commonly observed other X-ray binaries, whereas state probably produced by disk self-irradiation. Both cases support as low...

10.3847/1538-4357/abc55e article EN The Astrophysical Journal 2020-12-29

A new black hole X-ray binary (BHXRB) MAXI J1535-571 was discovered by during its outburst in 2017. Using observations taken the first Chinese satellite, Hard Modulation Telescope (dubbed as Insight-HXMT), we perform a joint spectral analysis (2-150 keV) both energy and time domains. The spectra provide essential input for probing intrinsic Quasi-Periodic Oscillation (QPO) fractional rms (FRS). Our results show that intermediate state, are general consistent with those reported Swift/XRT...

10.48550/arxiv.2001.06637 preprint EN cc-by arXiv (Cornell University) 2020-01-01

The Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) satellite consists of two small satellites. Each GECAM payload contains 25 gamma ray detectors (GRD) and 8 charged particle (CPD). GRD is the main detector which can detect gamma-rays particles localize Gamma-Ray Bursts (GRB),while CPD used to help discriminate gamma-ray bursts bursts. makes use lanthanum bromide (LaBr3) crystal readout by SiPM. As all available SiPM devices belong commercial grade,...

10.48550/arxiv.2109.00235 preprint EN cc-by-nc-sa arXiv (Cornell University) 2021-01-01
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