“About Me”的版本间差异
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无编辑摘要 |
无编辑摘要 |
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== Research Fields == |
== Research Fields == |
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===galaxy astronomy === |
===galaxy astronomy === |
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*statistical |
*statistical properties of galaxies and AGNs |
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===X-ray astronomy=== |
===X-ray astronomy=== |
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*image stacking |
*image stacking technique; QSO, clusters of galaxies |
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===LAMOST extragalactic survey=== |
===LAMOST extragalactic survey=== |
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* |
*Survey Strategy, input source catalog |
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*South galactic Cap U-band Sky |
*South galactic Cap U-band Sky Survey ([http://batc.bao.ac.cn/Uband/| SCUSS]) |
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==Research highlights== |
==Research highlights== |
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=== |
===Statistical properties of galaxies=== |
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*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] |
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*The size |
*The size distribution 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?[http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] |
:The third parameter, fundamental plane?[http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] |
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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]