“About Me”的版本间的差异
跳到导航
跳到搜索
| 第6行： | 第6行： | ||
== Research Fields == | == Research Fields == | ||
===galaxy astronomy === | ===galaxy astronomy === | ||
*statistical | *statistical properties of galaxies and AGNs | ||
===X-ray astronomy=== | ===X-ray astronomy=== | ||
*image stacking | *image stacking technique; QSO, clusters of galaxies | ||
===LAMOST extragalactic survey=== | ===LAMOST extragalactic survey=== | ||
* | *Survey Strategy, input source catalog | ||
*South galactic Cap U-band Sky | *South galactic Cap U-band Sky Survey ([http://batc.bao.ac.cn/Uband/| SCUSS]) | ||
==Research highlights== | ==Research highlights== | ||
=== | ===Statistical properties of galaxies=== | ||
*The statistical nature of the brightest group galaxies [http://adsabs.harvard.edu/abs/2014ApJ...782...23S] | *The statistical nature of the brightest group galaxies [http://adsabs.harvard.edu/abs/2014ApJ...782...23S] | ||
*The size | *The size distribution of galaxies [http://adsabs.harvard.edu/abs/2003MNRAS.343..978S] | ||
*The Tully-Fisher relation of Spiral galaxies | *The Tully-Fisher relation of Spiral galaxies | ||
:The third parameter, fundamental plane?[http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] | :The third parameter, fundamental plane?[http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] | ||
2014年9月9日 (二) 15:02的版本
Prof. Dr. Shiyin Shen
- Vice director of the Research Center of the Galaxy and Cosmology ;
- Deputy leader of the research group Star cluster and Galactic Structure;
Research Fields
galaxy astronomy
- statistical properties of galaxies and AGNs
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
- The statistical nature of the brightest group galaxies [1]
- The size distribution of galaxies [2]
- The Tully-Fisher relation of Spiral galaxies
- 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]
X-ray Astronomy
- Soft X-ray properties of QSOs[7]
- X-ray properties of clusters of galaxies
- X-ray luminosities of optically selected clusters of galaxies[8], and correlations with radio-loud AGN[9]