“About Me”的版本间差异

2025年10月22日 (三) 02:01的最新版本

Prof. Dr. Shiyin Shen (ssy@shao.ac.cn)

AI-related applications on galaxy structure and morphology [1][2][3][4]
dust geometry of MW and local disk galaxies [5][6][7][8]
galaxy interaction, galaxy pair, compact groups of galaxies [9] [10] [11][12][13][14]
IFS study of nearby galaxies [15] [16] [17][18] [19]

AI applications on galaxy images: how many latent features can effectively represent a main sample galaxy image(r<17.77) in DESI? The answer is 40. [20]
The Chocolate Chip Cookie Model: Dust Geometry of Milky Way-like Disk Galaxies [21]
How to quntify the interaction level of paired galaxies? Kinemetry~ [22]
How to model the three-dimensional dust distribution of MW? What is the vertical distance of the Sun to the Galactic plane? [23]
LAMOST Complementary galaxy sample: these galaxies in SDSS main galaxy sample without spectroscopy [24]
Whether the universe is transparent? [25]
Are the brightest group/cluster galaxies special? Is it only because of their definition? [26]
The size distribution (size-mass relation) of local galaxies [27]

@@ 第1行： / 第1行： @@
-'''Prof. Dr. Shiyin Shen  '''
+'''Prof. Dr. Shiyin Shen  ''' (ssy@shao.ac.cn)
 * orcid: 0000-0002-3073-5871
 * leader of the research group '''[http://cluster.shao.ac.cn Star cluster and Galaxies]''';