J. Xu

ORCID: 0009-0008-0052-3609
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About
Contact & Profiles
Research Areas
  • Pulsars and Gravitational Waves Research
  • Marine and environmental studies
  • Astrophysics and Cosmic Phenomena
  • Oceanographic and Atmospheric Processes
  • Geophysics and Gravity Measurements
  • Atmospheric chemistry and aerosols
  • Atmospheric and Environmental Gas Dynamics
  • Atmospheric Ozone and Climate
  • Geophysics and Sensor Technology
  • Gamma-ray bursts and supernovae
  • Ocean Acidification Effects and Responses

National Science Library
2025

Chinese Academy of Sciences
2023-2024

National Astronomical Observatories
2023-2024

Green building materials refer to environmentally friendly low-consumption construction materials. Their widespread adoption is hindered by high costs, limited technological implementation, and the absence of standardized regulations. This study conducts a bibliometric analysis 5381 publications from 2003 2024, sourced Web Science Core Collection (WoS), applying Sustainability Transitions Theory (STT) classify research into Niche Innovation (new like phase change materials), Regime...

10.3390/buildings15060884 article EN cc-by Buildings 2025-03-12

ABSTRACT Double neutron star (DNS) systems offer excellent opportunities to test gravity theories. We report the timing results of PSR J1901+0658, first pulsar discovered in FAST Galactic Plane Pulsar Snapshot (GPPS) Survey. Based on observations by over 5 yr, we obtain phase-coherent solution and derive precise measurements its position, spin parameters, orbital dispersion measure. It has a period 75.7 ms, derivative 2.169(6) × 10−19 s s−1, characteristic age 5.5 Gyr. This is an orbit with...

10.1093/mnras/stae888 article EN cc-by Monthly Notices of the Royal Astronomical Society 2024-03-27

The pulsar B0458+46 was previously believed to have a distance of about 1.3$~$kpc and be associated with nearby supernova remnant, SNR HB9 (G160.9+2.6). We observe the neutral hydrogen (HI) absorption spectrum PSR by using Five-hundred-meter Aperture Spherical radio Telescope (FAST), detect two lines at radial velocities $V_{\rm LSR} = {-7.7}~{\rm km~s}^{-1}$ $-28.1~{\rm km~s^{-1}}$. Based on Galactic rotation curve modification factor correcting for systematic stream in anticenter region,...

10.1093/mnras/stad1782 article EN Monthly Notices of the Royal Astronomical Society 2023-06-13
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