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News
A Novel Method to Weigh the Milky Way...
 
A Novel Method to Weigh the Milky Way with Its “Missing” Baryons (12.17)
Prof. Tao An and collaborators are in the finalists for the 2020 "Gordon Bell Prize" (11.18)
Evidence for Past Supermassive Black Hole Jets in the Milky Way Galaxy Revealed by CAS Researchers (05.06)
Searching for the Polyphony Players——Compact Group of Galaxies (12.10)
Chinese Scientists Complete First SKA Regional Center Prototype (11.22)
Seminars
Solar System Science with Next Generation Sky Surveys [2022.02.16]
High-precision Astrometry (高精度天体测量) [2021.11.03]
Mapping the dark matter universe [2021.06.07]
Science and Exploration of Solar System’s Small Bodies – Rosetta and ... [2021.05.10]
A Turbulent Convective Model on Circumpolar Vortices of Jupiter(木星极... [2021.01.06]
Characteristic mass in galaxy quenching: environmental versus internal ... [2020.07.09]
VLBI astrometry of long period variables using VERA [2019.11.26]
Hydrodynamical galaxy formation simulations: Current results and future... [2019.10.31]
Colloquia
地球2.0凌星巡天空间卫星科学研讨会
The 2nd notice of “2020 CPGPS Forum”
The importance of telescopes of all sizes, from small to extremely large:
International Workshop on GNSS Ionosphere (IWGI2018), Nov 4-6, 2018, Shanghai
EVN Technical Operations Group Meeting
APSG-2017 1st Announcement
International Workshop on Solar System Small Bodies Exploration_Second Announcement
IVOA Interoperability Meeting 2017
  Introduction
SHAO was formally established in 1962 following the amalgamation of the former Xujiahui (originally spelt Zi-Ka-Wei) and Sheshan (Zỏ-Sẻ) observatories, which were founded by the French Mission Catholique in 1872 and 1900 respectively.
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