“About Me”的版本间差异

2020年4月29日 (三) 14:52的最新版本

Prof. Dr. Shiyin Shen

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]

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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]
 * 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 applications on large sample of galaxies and AGNs [http://adsabs.harvard.edu/abs/2006MNRAS.369.1639S] [http://adsabs.harvard.edu/abs/2014ApJ...782...23S][]
 * 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]
+* 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][]
 * scaling relation of disk galaxies [http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] [http://adsabs.harvard.edu/abs/2009ApJ...705.1496S]