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'''Prof. Dr. Shiyin Shen ''' |
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* orcid: 0000-0002-3073-5871 |
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* Deputy leader of the research group '''[http://cluster.shao.ac.cn Star cluster and Galaxies]'''; |
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== Research Interests == |
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* galaxy structure, dust geometry of MW and local disk galaxies [http://adsabs.harvard.edu/abs/2017AJ....153...88L][http://adsabs.harvard.edu/abs/2018ApJ...858...75L] |
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* galaxy pair and galaxy interaction [https://ui.adsabs.harvard.edu/abs/2016RAA....16...43S/abstract] [https://ui.adsabs.harvard.edu/#abs/2019ApJ...880..114F/abstract] [https://ui.adsabs.harvard.edu/abs/2020ApJS..246...12Z/abstract] |
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* IFS study of galaxies [https://ui.adsabs.harvard.edu/abs/2018A%26A...613A..13Y/abstract] [https://ui.adsabs.harvard.edu/#abs/2020ApJ...892L..20F/abstract] |
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* statistical applications on large sample of galaxies and AGNs [http://adsabs.harvard.edu/abs/2006MNRAS.369.1639S] [http://adsabs.harvard.edu/abs/2014ApJ...782...23S][] |
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* scaling relation of disk galaxies [http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] [http://adsabs.harvard.edu/abs/2009ApJ...705.1496S] |
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==Research highlights== |
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* How to model the three-dimensional dust distribution of MW? What is the vertical distance of the Sun to the Galactic plane? [http://adsabs.harvard.edu/abs/2018ApJ...858...75L] |
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* LAMOST Complementary galaxy sample: these galaxies in SDSS main galaxy sample without spectroscopy [https://ui.adsabs.harvard.edu/abs/2016RAA....16...43S/abstract] |
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* Whether the universe is transparent? [https://ui.adsabs.harvard.edu/abs/2015ApJ...802L..16X/abstract] |
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* Are the brightest group/cluster galaxies special? Is it only because of their definition? [http://adsabs.harvard.edu/abs/2014ApJ...782...23S] |
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* The size distribution (size-mass relation) of local galaxies [https://ui.adsabs.harvard.edu/abs/2003MNRAS.343..978S/abstract] |
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==Curriculum Vitae 个人简历 == |
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*[[CV: English]] |
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*[[个人简历]] |
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==Links== |
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*[http://cluster.shao.ac.cn/~shen/PhD/THESIS.pdf 博士论文：星系大小分布的统计研究] |
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*[https://ui.adsabs.harvard.edu/search/q=orcid%3A0000-0002-3073-5871&sort=date+desc My Publications] |
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2020年4月29日 (三) 14:52的最新版本
Prof. Dr. Shiyin Shen
- orcid: 0000-0002-3073-5871
- Deputy leader of the research group Star cluster and Galaxies;
Research Interests
- galaxy structure, dust geometry of MW and local disk galaxies [1][2]
- galaxy pair and galaxy interaction [3] [4] [5]
- IFS study of galaxies [6] [7]
- statistical applications on large sample of galaxies and AGNs [8] [9][]
- scaling relation of disk galaxies [10] [11]
Research highlights
- How to model the three-dimensional dust distribution of MW? What is the vertical distance of the Sun to the Galactic plane? [12]
- LAMOST Complementary galaxy sample: these galaxies in SDSS main galaxy sample without spectroscopy [13]
- Whether the universe is transparent? [14]
- Are the brightest group/cluster galaxies special? Is it only because of their definition? [15]
- The size distribution (size-mass relation) of local galaxies [16]