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Center for Astro-geodynamics
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The Location of SHAO
To Measure the Galactic extinction? From Cosmological Principle!
A group from astronomers in Shanghai Astronomical Observatory have completed a systematical study on Galactic dust extinction recently. Taking advantage of the most up-to-date large sky area u band galaxy catalog from the South Galactic Cap U-band Sky Survey (SCUSS), this study has obtained stati...
ATCA: More Accurate OH Maser Positions from the SPLASH Pilot Region
OH masers, the first astrophysical maser ever detected in the space, opened an exciting and rapidly growing area of research. As a high-sensitivity survey of OH masers in our Galaxy, the Southern Parkes Large-Area Survey in Hydroxyl (SPLASH) has shown typical features of OH masers. However, due t...
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]
Gaps, Vortices, and Spiral Shocks: The Gas Dynamics of Protoplanetary Disks [2017.02.22]
Density Waves in Strongly Radiation Pressure Dominated AGN Accretion Disks [2017.02.10]
Observing Galaxies with the Atacama Large Millimeter Array (ALMA) [2017.02.10]
Not-so-simple stellar populations in nearby, resolved massive star clusters [2017.01.17]
Australia-China SKA Big Data Workshop Call for Proposals (1st Announcement)
First Announcement of 2017 IGMA Workshop & TFM
1st IUGG Symposium on Planetary Sciences (IUGG-PS 2017), July 3-5, 2017, Berlin, Germany
URSI 2017 GASS (August 2017 19-26,2017)
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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