“About Me”的版本间差异

来自Shiyin's note
跳到导航 跳到搜索
无编辑摘要
无编辑摘要
第1行: 第1行:
'''Prof. Dr. Shiyin Shen '''
'''Prof. Dr. Shiyin Shen '''
* orcid:0000-0002-3073-5871
* orcid: 0000-0002-3073-5871
*Vice director of the '''[http://astro.shao.cas.cn/ Astrophysical Division]''', Shanghai Astronomical Observatory ;
*Vice director of the '''[http://astro.shao.cas.cn/ Astrophysical Division]''', Shanghai Astronomical Observatory ;
*Deputy leader of the research group '''[http://cluster.shao.ac.cn Star cluster and Galaxies]''';
*Deputy leader of the research group '''[http://cluster.shao.ac.cn Star cluster and Galaxies]''';

2019年7月16日 (二) 14:43的版本

Prof. Dr. Shiyin Shen

Research Fields

galaxy astronomy

  • statistical properties of galaxies and AGNs
  • dust dsitribution in MW and local spiral galaxies

X-ray astronomy

  • image stacking technique; QSO, clusters of galaxies

LAMOST extragalactic survey

  • Survey Strategy, input source catalog
  • South galactic Cap U-band Sky Survey (SCUSS)

Research highlights

Statistical properties of galaxies and AGNs

  • The statistical nature of the brightest group galaxies [1]
  • The size distribution of galaxies [2]
  • The Tully-Fisher relation of Spiral galaxies
The third parameter, fundamental plane?[3]
Morphological dependence?[4]
  • The inclination of spiral galaxies
inclination dependence luminosity function of spiral galaxies: implications on the dust attenuation of galaxies.[5]
inclination of the host spirals of type II AGNs: implications on the nuclear obscurer of the AGNs.[6]

dust in galaxies

  • MW dust extinction and distribution [7][8]
  • dust in merging galaxies [9]

X-ray Astronomy

  • Soft X-ray properties of QSOs[10]
  • X-ray properties of clusters of galaxies
X-ray luminosities of optically selected clusters of galaxies[11], and correlations with radio-loud AGN[12]

Curriculum Vitae 个人简历

Links