“About Me”的版本间差异
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'''Prof. Dr. Shiyin Shen ''' |
'''Prof. Dr. Shiyin Shen ''' |
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* orcid: 0000-0002-3073-5871 |
* orcid: 0000-0002-3073-5871 |
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* leader of the research group '''[http://cluster.shao.ac.cn Star cluster and Galaxies]'''; |
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== Research Interests == |
== Research Interests == |
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==Research highlights== |
==Research highlights== |
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* 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] |
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* The Chocolate Chip Cookie Model: Dust Geometry of Milky Way-like Disk Galaxies [https://ui.adsabs.harvard.edu/#abs/2022ApJ...938..139L/abstract] |
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* How to quntify the interaction level of paired galaxies? Kinemetry~ [https://ui.adsabs.harvard.edu/#abs/2020ApJ...892L..20F/abstract] |
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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] |
* 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] |
* 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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2025年9月10日 (三) 11:17的最新版本
Prof. Dr. Shiyin Shen
- orcid: 0000-0002-3073-5871
- leader of the research group Star cluster and Galaxies;
Research Interests
- 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]
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. [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]