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  • HomeResearch News
  • Research News
    • Mar 14, 2022
      What Happened before Solar Flare?
      A research team led by Dr. SHEN Jinhua from Xinjiang Astronomical Observatory of the Chinese Academy of Sciences investigated the evolution of flaring active region NOAA 12158 using the high-resolution observations from the Big Bear Lake...
    • Mar 02, 2022
      Research progress in the Study of Dense Clumps in the W33 Giant Molecular Cloud
      Using the 100-m Effelsberg telescope near Bonn/Germany, Kadirya Tursun, a PhD student supervised by Prof. Jarken Esimbek from Xinjiang Astronomical Observatory (XAO), along with their collaborators from Max Planck Institute of Radioastro...Using the 100-m Effelsberg telescope near Bonn/Germany, Kadirya Tursun, a PhD student supervised by Prof. Jarken Esimbek from Xinjiang Astronomical Observatory (XAO), along with their collaborators from Max Planck Institute of Radioastro...
    • Jan 07, 2022
      Investigation of nulling and sub-pulse drifting properties of PSR J1727-2739
      Using the archived observational data at 1369 MHz with the Parkes 64-m radio telescope, Rukiye Rejep, a PhD student from the Pulsar Group at the Xinjiang Astronomical Observatory (XAO) of the Chinese Academy of Sciences, and her co-resea...
    • Dec 21, 2021
      Transient RFI mitigation algorithm based on pulse phase and standard deviation
      The rapid development of communication technology escalates the challenges for the radio astronomy observing environment. During pulsar observations, transient radio frequency interference (RFI) sometimes appears in the observational dat...
    • Dec 17, 2021
      Constraint on Dark Energy from Quantum Uncertainty
      Recently, new model and constraint on dark energy from quantum uncertainty was finished by fresh PhD HUANG Long and his supervisors Prof. YANG Xiaofeng, Prof. LIU Xiang in the galaxies and cosmology group at Xinjiang Astronomical Observa...
    • Dec 16, 2021
      Researchers Reveal Morphological Evolution of Open Clusters
      Open clusters are ideal “laboratories” not only for star formation and evolution, but also as an important component of the Milky Way. The morphology of open clusters is a useful tool to study the dynamic evolution of open clusters. In...
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