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'''Prof. Dr. Shiyin Shen ''' |
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* orcid: 0000-0002-3073-5871 |
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*Vice director of the Research Center of the Galaxy and Cosmology[http://astro.shao.cas.cn/] ; |
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*Deputy leader of the research group |
* Deputy leader of the research group '''[http://cluster.shao.ac.cn Star cluster and Galaxies]'''; |
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== Research |
== Research Interests == |
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* AI-related applications on galaxy structure and morphology [https://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.6391X/abstract][https://arxiv.org/abs/2412.15533][https://arxiv.org/abs/2410.21962][https://arxiv.org/abs/2404.07780] |
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===galaxy astronomy === |
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* dust geometry of MW and local disk galaxies [http://adsabs.harvard.edu/abs/2017AJ....153...88L][http://adsabs.harvard.edu/abs/2018ApJ...858...75L][https://ui.adsabs.harvard.edu/#abs/2022ApJ...938..139L/abstract][https://ui.adsabs.harvard.edu/#abs/2023ApJ...946L...7L/abstract] |
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*statistical porperties of galaxies and AGNs |
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* galaxy interaction, galaxy pair, compact groups of galaxies [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][https://ui.adsabs.harvard.edu/#abs/2022ApJ...926..119Z/abstract][https://ui.adsabs.harvard.edu/#abs/2021ApJ...911..105Z/abstract][https://ui.adsabs.harvard.edu/#abs/2020ApJS..246...12Z/abstract] |
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===X-ray astronomy=== |
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* IFS study of nearby galaxies [https://ui.adsabs.harvard.edu/abs/2018A%26A...613A..13Y/abstract] [https://ui.adsabs.harvard.edu/#abs/2020ApJ...892L..20F/abstract] [https://ui.adsabs.harvard.edu/#abs/2024ApJ...976...15Q/abstract][https://ui.adsabs.harvard.edu/#abs/2024ApJ...977..175L/abstract] [https://ui.adsabs.harvard.edu/#abs/2022ApJS..262....6F/abstract] |
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*image stacking technic; QSO, clusters of galaxies |
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===LAMOST extragalactic survey=== |
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*Suvey Strategy, input source catalog |
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*South galactic Cap U-band Sky Suvey (SCUSS[http://batc.bao.ac.cn/Uband/]) |
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== |
==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] |
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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] |
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* Whether the universe is transparent? [https://ui.adsabs.harvard.edu/abs/2015ApJ...802L..16X/abstract] |
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* Are the brightest group/cluster galaxies special? Is it only because of their definition? [http://adsabs.harvard.edu/abs/2014ApJ...782...23S] |
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* The size distribution (size-mass relation) of local galaxies [https://ui.adsabs.harvard.edu/abs/2003MNRAS.343..978S/abstract] |
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==Curriculum Vitae 个人简历 == |
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==curriculum vitae== |
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*[[CV: English]] |
*[[CV: English]] |
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*[[ |
*[[个人简历]] |
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==[[Publications]]== |
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==Links== |
==Links== |
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*[http://cluster.shao.ac.cn/~shen/PhD/THESIS.pdf 博士论文：星系大小分布的统计研究] |
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*[https://ui.adsabs.harvard.edu/search/q=orcid%3A0000-0002-3073-5871&sort=date+desc My Publications] |
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2024年12月26日 (四) 02:18的最新版本
Prof. Dr. Shiyin Shen
- orcid: 0000-0002-3073-5871
- Deputy 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]