Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S292(8), p. 105-105, 2012
DOI: 10.1017/s1743921313000653
Full text: Unavailable
AbstractLAMOST has 4 meters in diameter with 4000 fibers in the focal plane. The telescope is now on the way towards full spectroscopy survey periods. This survey project has the potential to largely increase our understanding of the substructure of the Galactic stellar spheroid and different disk components through accurate measurements of radial velocities, metallicities and effective temperatures of millions of stars.