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    • Brief Introduction
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  • HomeResearch News
  • Research News
    • Mar 21, 2018
      Research progress of the all-axis radio interferometric data reduction pipeline - SAND
      Recently, a research on automatic Very Long Baseline Interferometry (VLBI) imaging and analysis pipeline - SAND and its related algorithms have been published in Monthly Notices of the Royal Astronomical Society (MNRAS 473 450 2018). The...
    • Mar 14, 2018
      Evolution and Photoevaporation of Protoplanetary Disks in Clusters:The Role of Pre-stellar Core Properties
      Associated research fellow, Xiao Lin from Astrochemistry group at Xinjiang Astronomical Observatory, analyzed the influences of molecular clouds property to external photoevaporation efficiency in the research of the evolution and format...
    • Mar 06, 2018
      Research Progress of the Nanshan One-meter Wide-field Telescope on the Observations of the Transiting Exoplanet Monitoring Project (TEMP), Kepler-9 b Transit
      Recently, Dr. Liu, Jinzhong, associated research fellow, and his co-researchers from the optical astronomy and astronomical applications group at Xinjiang Astronomical Observatory (XAO) joined the transiting exoplanet monitoring project ...
    • Feb 07, 2018
      2017 Annual Summary Meeting of the QTT-973 Program
      The 973 Program on Research of the Key Technologies for 110-m Aperture Fully Steerable Radio Telescope (hereinafter referred to as QTT-973 program) was held in Cheng Du between 25-26 January, 2018. More than 100 participants were present...
    • Feb 04, 2018
      Network broadcast of the total lunar eclipse: An observation activity from Xinjiang Astronomical observatory
      A 3-in-1 exhibition from the moon, popularly known as the Blue Moon, that involves a total eclipse,supermoon, and blue moon, was staged in the sky over China on January 31. The last time that the same event happened was about 152 years a...
    • Feb 01, 2018
      Dependence of pulsar death line on the equation of state
      A useful starting point for understanding the diverse flavors of pulsars is to place them on the plane, where the spin period, P, and the period derivative, , of a pulsar can be obtained at very high levels of precision through timing me...
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