Difference between revisions of "Staff Members"
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==Group members== | ==Group members== | ||
== | ===侯金良Jinliang Hou=== | ||
[[file:Jlhou.jpg|right|150px|hou]] | [[file:Jlhou.jpg|right|150px|hou]] | ||
Office: 803 | Office: 803 | ||
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Research Interest: Star cluster, late-type stars, LAMOST | Research Interest: Star cluster, late-type stars, LAMOST | ||
==Related members== | ==Related members== | ||
Revision as of 07:13, 2 February 2021
Group members
侯金良Jinliang Hou
Office: 803
Tel: 5002
Email: houjl
Title: Chief Professor
Research interest: Galactic structure, Chemical evolution of galaxies，high redshift galaxies.
常瑞香 Ruixiang Chang
Office: 1502
Tel: 5307
Email: crx
Title: Professor
Research interest: Chemical evolution model of Milk way and nearby galaxies
陈力 Li Chen
Office: 1514
Tel: 5324
Email: chenli
Title: Professor
Resarch interest: star cluster，Galactic structure
富坚 Jian Fu
Office: 1501
Tel: 5113
Email: fujian
Title: Associate Professor
Research Interest: Galaxy Formation and Evolution, radio astrophysics on neutral gas
邵正义 Zhengyi Shao
Office: 1516
Tel: 5326
Email: zyshao
Title: Professor
Research: nearby galaxies, galaxy clusters
沈世银 Shiyin Shen
Office: 1801
Tel: 5318
Email: ssy
Title: Professor
Research interest: galaxy formation and evolution
Webpage: http://cluster.shao.ac.cn/~shen/
Rafael S de Souza
Office: 1504
Tel:
Email: drsouza
Title: Associate Professor
Research interest: Astrostatistics, Galactic and Extragalactic Astrophysics, Bayesian models
Webpage: https://cosmostatistics-initiative.org
钟靖 Jing Zhong
Office: 1501
Tel: 5113
Email: jzhong
Title: Associate Professor
Research Interest: Star cluster, late-type stars, LAMOST
Related members
尹君 Jun Yin
Office: 1504
Tel: 5309
Email: jyin
Title: Associate Professor
Research interest: Chemical evolution of galaxies
- Now a member of research group "Evolution of Galaxies and AGN"
袁方婷 Fangting Yuan
Office: 1504
Tel: 5309
Email: yuanft
Title: Associate Professor
Research Interest: Galaxy formation and evolution
- Now a member of research group "Early Universe and High-redshift Galaxies"[1]