报告题目：Galactic Tomography with the LAMOST and SDSS

报 告 人：Haibo Yuan，Peking University

报告时间：2015年4月1日（周三）13:30-15:00

报告地点：理科楼物理系三楼报告厅C302

报告摘要：The Milky Way provides us a unique opportunity to study galaxy formation and evolution in unprecedented details. The field has been greatly advanced by surveys like 2MASS and SDSS in recent years, and will be further revolutionized by on-going and up-coming surveys like LAMOST, Gaia and LSST in the near future. In this talk, I will present our work on mapping the stellar populations, structure, kinematics and chemistry of the Milky Way with the LAMOST and SDSS surveys.