“About Me”的版本间差异
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无编辑摘要 |
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==Research highlights== |
==Research highlights== |
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===Statsitical properties of galaxies=== |
===Statsitical properties of galaxies=== |
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*The statistical nature of the brightest group galaxies |
*The statistical nature of the brightest group galaxies [http://adsabs.harvard.edu/abs/2014ApJ...782...23S] |
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*The size distruibution of galaxies |
*The size distruibution of galaxies [http://adsabs.harvard.edu/abs/2003MNRAS.343..978S] |
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*The Tully-Fisher relation of Spiral galaxies |
*The Tully-Fisher relation of Spiral galaxies |
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:The third parameter, fundamental plane? |
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:Morphological dependence? |
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*The inclination of spiral galaxies |
*The inclination of spiral galaxies |
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:inclination dependence luminosity function of spiral galaxies: implications on the dust attenuation of galaxies. |
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:inclination of the host spirals of type II AGNs: implications on the nuclear obscurer of the AGNs. |
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===X-ray Astronomy=== |
===X-ray Astronomy=== |
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2014年9月9日 (二) 14:02的版本
Prof. Dr. Shiyin Shen
- Vice director of the Center of the Galaxy and Cosmology ;
- Deputy leader of the group Star cluster and Galactic Structure;
Research Fields
galaxy astronomy
- statistical porperties of galaxies and AGNs
X-ray astronomy
- image stacking technic; QSO, clusters of galaxies
LAMOST extragalactic survey
- Suvey Strategy, input source catalog
- South galactic Cap U-band Sky Suvey ([1])
Research highlights
Statsitical properties of galaxies
- The statistical nature of the brightest group galaxies [2]
- The size distruibution of galaxies [3]
- The Tully-Fisher relation of Spiral galaxies
- The third parameter, fundamental plane?
- Morphological dependence?
- The inclination of spiral galaxies
- inclination dependence luminosity function of spiral galaxies: implications on the dust attenuation of galaxies.
- inclination of the host spirals of type II AGNs: implications on the nuclear obscurer of the AGNs.
X-ray Astronomy
- Soft X-ray properties of QSOs
- X-ray properties of clusters of galaxies