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A VO-driven Astronomical Data Grid in China

2010/01/08 by Chenzhou Cui, Cui, Chenzhou, Boliang He +5
Computer Science · Engineering · Physics and Astronomy · #Advanced Computational Techniques and Applications #Astronomical Observations and Instrumentation #FOS: Physical sciences #Inertial Sensor and Navigation #Instrumentation and Methods for Astrophysics (astro-ph.IM) #astro-ph.IM

paper · pdf · doi:10.48550/arxiv.1001.1192

4 pages, 3 figures. To appear in Proc. ADASS XIX (Sapporo, Japan, 2009)

openalex publication_date 2010/01/08 · arxiv created 2010/01/13 · arxiv updated 2010/01/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

With the implementation of many ambitious observation projects, including LAMOST, FAST, and Antarctic observatory at Doom A, observational astronomy in China is stepping into a brand new era with emerging data avalanche. In the era of e-Science, both these cutting-edge projects and traditional astronomy research need much more powerful data management, sharing and interoperability. Based on data-grid concept, taking advantages of the IVOA interoperability technologies, China-VO is developing a VO-driven astronomical data grid environment to enable multi-wavelength science and large database science. In the paper, latest progress and data flow of the LAMOST, architecture of the data grid, and its supports to the VO are discussed.

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