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Possible Contribution to IPERCOOL from SHAO TANG Zheng-Hong

Possible Contribution to IPERCOOL from SHAO TANG Zheng-Hong. 1. Person and Manpower. Group of Astrometry: Parallax & Proper Motion TANG Zheng-Hong (1969): 1 mon/yr QI Zhao-Xiang/Kevin(1979): 6 mon/yr YU Yong (1977): 3 mon/yr

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Possible Contribution to IPERCOOL from SHAO TANG Zheng-Hong

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  1. Possible Contribution to IPERCOOL from SHAO TANG Zheng-Hong

  2. 1. Person and Manpower Group of Astrometry: Parallax & Proper Motion • TANG Zheng-Hong (1969): 1 mon/yr • QI Zhao-Xiang/Kevin(1979): 6 mon/yr • YU Yong (1977): 3 mon/yr Group of Evolution and Structure of Stellar Cluster and Galaxy: Spectroscopy & Photometry • CHEN Li (1962): 1 mon/yr • WANG You-Fen (1980): 10 mon/yr (Ph.D Thesis) • SHEN Shi-Yin (1976): 2 mon/yr Observation Data reduction Implementation

  3. 2. Visiting Plan

  4. 3. Observational facilities (1) LAMOST: A 4m Schmidt telescope with a 20 square degrees field and a 4000 fibres  low resolution spectroscopy. • Group of Astrometry is responsible for the pointing/tracking of LAMOST. • Group of Galactic Structure and Revolution is one of the key research units for Galactic Survey of LAMOST.

  5. 3. Observational facilities (2) 2.4m (F=19.2m), YFOSC (3) 1.0/1.2/1.8 Schmidt, 20mag (Exp=10s) Anti-galactic-center Survey

  6. Thanks

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