“About Me”的版本间差异
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==Links== |
==Links== |
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*[http://cluster.shao.ac.cn/~shen/PhD/THESIS.pdf| My Ph.D thesis: |
*[http://cluster.shao.ac.cn/~shen/PhD/THESIS.pdf| My Ph.D thesis: The statsical study of the size distribution of galaxies, Chinese] |
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*[http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?library&libname=My+paper&libid=4804c2b092| My Publications] |
*[http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?library&libname=My+paper&libid=4804c2b092| My Publications] |
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*[[CV: English]] |
*[[CV: English]] |
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2014年9月9日 (二) 14:12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 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 inclination of spiral galaxies
- inclination dependence luminosity function of spiral galaxies: implications on the dust attenuation of galaxies.[6]
- inclination of the host spirals of type II AGNs: implications on the nuclear obscurer of the AGNs.[7]
X-ray Astronomy
- Soft X-ray properties of QSOs[8]
- X-ray properties of clusters of galaxies
- X-ray luminosities of optically selected clusters of galaxies[9], and correlations with radio-loud AGN[10]