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LAMOST and China-VO

Published online by Cambridge University Press:  05 March 2015

Yongheng Zhao*
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 1000012, China email: yzhao@bao.ac.cn
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Abstract

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LAMOST is a special reflecting Schmidt telescope used to observe ten million spectra of celestial objects. There are about half million spectra released in the pilot survey of LAMOST. In the “Big Data“ era of astronomy, Virtual Observatory will play an important role to make use of those massive spectral data of LAMOST.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Cui, C. & Zhao, Y. 2004, Public. of NAOC 1 (3), 203Google Scholar
Cui, X., Zhao, Y., Chu, Y.et al. 2012, Research of Astron. & Astrophys. 12, 1197Google Scholar
Lawrence, A. 2009, in: Simpson, R.J., Ward-Thompson, Length D. (eds.), Astronomy: Networked Astronomy and the New MediaGoogle Scholar
Luo, A., Zhang, H., Zhao, Y.et al. 2012, Research of Astron. & Astrophys. 12, 1243CrossRefGoogle Scholar
Newberg, H. J., Carlin, J. L., Chen, L., et al. 2012, ASPC 458, 405Google Scholar
Peng, N., Zhang, Y., Zhao, Y., & Wu, X. 2012, MNRAS 425, 2599Google Scholar
Zhang, Y. & Zhao, Y. 2006, ASPC 351, 173Google Scholar
Zhao, Y. 1999, Public. of Yunnan Obs. Suppl., p. 1Google Scholar
Zhao, G., Zhao, Y., Chu, Y., et al. 2012, Research of Astron. & Astrophys. 12, 723Google Scholar