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Center for Astro-geodynamics
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News
The Milky Way’s star dust distribution precisely measured by SHAO astronomers
Figure 1 : Image of the Sombrero Galaxy ( also known as M104 ) from Hubble space telescope ( upper ) .Recently , the structure of dust component in the Milky Way Galaxy has been accurately modeled revealing the most accurate scale of the Galactic dust distribution so far .News Contact : ZUO Wenwe...
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East Asia VLBI Radio Telescope Network to Start Scientific Commission
East Asia Very Long Baseline Interferometry ( EA VLBI Network , EAVN ) , a network composed of 21 radio telescopes from China , Japan and South Korea , has been astronomically operational and will begin scientific commissioning soon .To learn more about the EAVN , please contact : AN Tao , Shangh...
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Scientific Progress
TAP LCOGT 2017AB Call for Proposals [2017.02.03]
Research Fund for International Young Scientists Call for Proposals FY 2017 [2017.01.20]
Call for proposals of TianMa 65 meter telescope [2016.12.30]
SHAO Astronomers discovered 15 candidate X-ray transients in the nearby satellite... [2016.04.07]
Seminars
Galaxy-Halo Connection for Next Generation Galaxy Surveys [2018.05.21]
Reverberation Mapping of AGNs [2018.05.14]
Probing Cosmic Reionization with Lyman Alpha Galaxies [2018.05.07]
From Dark to Light: The Evolution from Molecular Clouds to Massive Protostars & C... [2018.05.02]
Colloquia
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
  Introduction
SHAO was formally established in 1962 following the amalgamation of the former Xujiahui (originally spelt Zi-Ka-Wei) and Sheshan observatories, which were founded by the French Mission Catholique in 1872 and 1900 respectively.
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