“About Me”的版本间差异

2024年12月26日 (四) 02:18的最新版本

Prof. Dr. Shiyin Shen

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]

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 ==Research highlights==
+* 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. [https://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.6391X/abstract]
+* The Chocolate Chip Cookie Model: Dust Geometry of Milky Way-like Disk Galaxies [https://ui.adsabs.harvard.edu/#abs/2022ApJ...938..139L/abstract]
+* How to quntify the interaction level of paired galaxies? Kinemetry~ [https://ui.adsabs.harvard.edu/#abs/2020ApJ...892L..20F/abstract]
 * 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]
 * LAMOST Complementary galaxy sample: these galaxies in SDSS main galaxy sample without spectroscopy [https://ui.adsabs.harvard.edu/abs/2016RAA....16...43S/abstract]