“About Me”的版本间差异

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'''Prof. Dr. Shiyin Shen '''
'''Prof. Dr. Shiyin Shen '''
* orcid: 0000-0002-3073-5871
* orcid: 0000-0002-3073-5871
*Vice director of the '''[http://astro.shao.cas.cn/ Astrophysical Division]''', Shanghai Astronomical Observatory ;
* Deputy leader of the research group '''[http://cluster.shao.ac.cn Star cluster and Galaxies]''';
*Deputy leader of the research group '''[http://cluster.shao.ac.cn Star cluster and Galaxies]''';


== Research Fields ==
== Research Interests ==
⚫
* 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]
===galaxy astronomy ===
* 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]
* statistical properties of galaxies and AGNs
* 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][]
* dust dsitribution in MW and local spiral galaxies
* 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]

* scaling relation of disk galaxies [http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] [http://adsabs.harvard.edu/abs/2009ApJ...705.1496S]
===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 ([http://batc.bao.ac.cn/Uband/ SCUSS])


==Research highlights==
==Research highlights==
* 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]
===Statistical properties of galaxies and AGNs===
*The statistical nature of the brightest group galaxies [http://adsabs.harvard.edu/abs/2014ApJ...782...23S]
* LAMOST Complementary galaxy sample: these galaxies in SDSS main galaxy sample without spectroscopy [https://ui.adsabs.harvard.edu/abs/2016RAA....16...43S/abstract]
*The size distribution of galaxies [http://adsabs.harvard.edu/abs/2003MNRAS.343..978S]
* Whether the universe is transparent? [https://ui.adsabs.harvard.edu/abs/2015ApJ...802L..16X/abstract]
* Are the brightest group/cluster galaxies special? Is it only because of their definition? [http://adsabs.harvard.edu/abs/2014ApJ...782...23S]
*The Tully-Fisher relation of Spiral galaxies
:The third parameter, fundamental plane?[http://adsabs.harvard.edu/abs/2002MNRAS.331..259S]
* The size distribution (size-mass relation) of local galaxies [https://ui.adsabs.harvard.edu/abs/2003MNRAS.343..978S/abstract]
:Morphological dependence?[http://adsabs.harvard.edu/abs/2009ApJ...705.1496S]
*The inclination of spiral galaxies
:inclination dependence luminosity function of spiral galaxies: implications on the dust attenuation of galaxies.[http://adsabs.harvard.edu/abs/2007ApJ...659.1159S]
:inclination of the host spirals of type II AGNs: implications on the nuclear obscurer of the AGNs.[http://adsabs.harvard.edu/abs/2010ApJ...725L.210S]

===dust in galaxies===
⚫
*MW dust extinction and distribution [http://adsabs.harvard.edu/abs/2017AJ....153...88L][http://adsabs.harvard.edu/abs/2018ApJ...858...75L]
* dust in merging galaxies [http://adsabs.harvard.edu/abs/2018ApJS..234....5Y]


===X-ray Astronomy===
*Soft X-ray properties of QSOs[http://adsabs.harvard.edu/abs/2006MNRAS.369.1639S]
*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]


==Curriculum Vitae 个人简历 ==
==Curriculum Vitae 个人简历 ==
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==Links==
==Links==
*[http://cluster.shao.ac.cn/~shen/PhD/THESIS.pdf 博士论文：星系大小分布的统计研究]
*[http://cluster.shao.ac.cn/~shen/PhD/THESIS.pdf 博士论文：星系大小分布的统计研究]
*[https://ui.adsabs.harvard.edu/public-libraries/8aEX4kmqTDGm2ZOHA-8Rmw My Publications]
*[https://ui.adsabs.harvard.edu/search/q=orcid%3A0000-0002-3073-5871&sort=date+desc My Publications]

2020年4月29日 (三) 14:29的版本

Prof. Dr. Shiyin Shen

Research Interests

  • galaxy structure, dust geometry of MW and local disk galaxies [1][2]
  • galaxy pair and galaxy interaction [3] [4] [5]
  • statistical applications on large sample of galaxies and AGNs [6] [7][]
  • IFS study of galaxies [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]


Curriculum Vitae 个人简历

Links

取自“http://202.127.29.3/~shen/wiki/index.php?title=About_Me&oldid=3277”