SHAO-KIAA galaxies: Difference between revisions
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==Zheng Zhenya == |
==Zheng Zhenya == |
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===Epoch of Reionization (EoR)=== |
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* --- |
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* How to probe EoR via galaxies? |
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* 21cm & Ly-α in EoR |
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===High-Redshift Galaxies=== |
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* Physical properties of high-redshift galaxies |
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* Galaxy protoclusters at high-redshift |
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==Zhu Lin == |
==Zhu Lin == |
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Latest revision as of 08:39, 24 June 2020
Guo Hong
- large scale structure of galaxy distribution
- ---
Hao Lei
- ionized gas of galaxies
- ---
Shen Shiyin
Galaxy pair and galaxy interaction
- How to quantify the merging stage of galaxy pairs? Kinemetry, Morphlogy?
- Physical process in different stages?
Compact groups of galaxies
- the largest and most complete low redshift compact groups of galaxies(CGs) sample selected from SDSS and LAMOST.
- Dynamics and physical nature CGs?
Dust geometry of galaxies
- How to measure or quantify the geometry of the dust components?
- How the dust geometries affect the observed properties of galaxies?
HII regions of galaxies
- Identify HII regions in local star-forming galaxies using MaNGA data.
- Characterize the star formation process of HII regions.
Zheng Zhenya
Epoch of Reionization (EoR)
- How to probe EoR via galaxies?
- 21cm & Ly-α in EoR
High-Redshift Galaxies
- Physical properties of high-redshift galaxies
- Evolution of high-redshift galaxies
- Galaxy protoclusters at high-redshift
Zhu Lin
- galactic dynamics
- ---