“About Me”的版本间差异
跳到导航
跳到搜索
| （未显示同一用户的52个中间版本） | |||
| 第1行： | 第1行： | ||
'''Prof. Dr. Shiyin Shen ''' |
|||
* orcid: 0000-0002-3073-5871 |
|||
| ⚫ | |||
* Deputy leader of the research group '''[http://cluster.shao.ac.cn Star cluster and Galaxies]'''; |
|||
===galaxy astronomy === |
|||
*statistical porperties of galaxies and AGNs |
|||
===X-ray astronomy=== |
|||
*image stacking technic; QSO, clusters of galaxies |
|||
===LAMOST extragalactic survey=== |
|||
*Suvey Strategy, input source catalog |
|||
*South galactic Cap U-band Sky Suvey (SCUSS[http://batc.bao.ac.cn/Uband/]) |
|||
== |
== Research Interests == |
||
* 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] |
|||
* 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] |
|||
* 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] |
|||
* 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] |
|||
| ⚫ | |||
==curriculum vitae== |
|||
* 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] |
|||
* Whether the universe is transparent? [https://ui.adsabs.harvard.edu/abs/2015ApJ...802L..16X/abstract] |
|||
* Are the brightest group/cluster galaxies special? Is it only because of their definition? [http://adsabs.harvard.edu/abs/2014ApJ...782...23S] |
|||
* The size distribution (size-mass relation) of local galaxies [https://ui.adsabs.harvard.edu/abs/2003MNRAS.343..978S/abstract] |
|||
==Curriculum Vitae 个人简历 == |
|||
*[[CV: English]] |
*[[CV: English]] |
||
*[[ |
*[[个人简历]] |
||
==[[Publications]]== |
|||
==Links== |
==Links== |
||
*[http://cluster.shao.ac.cn/~shen/PhD/THESIS.pdf 博士论文：星系大小分布的统计研究] |
|||
*[https://ui.adsabs.harvard.edu/search/q=orcid%3A0000-0002-3073-5871&sort=date+desc My Publications] |
|||
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]