“About Me”的版本间的差异
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*X-ray properties of clusters of galaxies | *X-ray properties of clusters of galaxies | ||
:X-ray luminosities of optically selected clusters of galaxies[http://adsabs.harvard.edu/abs/2014MNRAS.439..611W], and correlations with radio-loud AGN[http://adsabs.harvard.edu/abs/2008MNRAS.389.1074S] | :X-ray luminosities of optically selected clusters of galaxies[http://adsabs.harvard.edu/abs/2014MNRAS.439..611W], and correlations with radio-loud AGN[http://adsabs.harvard.edu/abs/2008MNRAS.389.1074S] | ||
==Curriculum Vitae == | ==Curriculum Vitae == | ||
2014年9月9日 (二) 14:36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]