Possible Contribution to IPERCOOL from SHAO

TANG Zheng-Hong

1. Person and ManpowerGroup 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

ObservationObservation Data reduction Data reduction I Implementationmplementation

2. Visiting PlanName Host Period (month) During

QI Zhao-Xiang OATo 2 (astrometry) now

OATo 3 (astrometry) 2011

CAR-UH 3 (spectroscopy) 2012

WANG You-Fen CAR-UH 9 (spectroscopy) 2011.1-9

YU Yong OATo 3 (astrometry 2011/12

SHEN Shi-Yin CAR-UH 2 (spectroscopy) 2011/12

TANG Zheng-Hong OATo 1 (astrometry) 2012

CHEN Li CAR-UH 1 (implementation)

2013

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.

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

Thanks