“SHAO-KIAA galaxies”的版本间差异
		
		
		
		
		
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==Zheng Zhenya ==  | 
  ==Zheng Zhenya ==  | 
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===Epoch of Reionization   | 
  ===Epoch of Reionization (EoR)===   | 
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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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  * Evolution 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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2020年6月24日 (三) 08:39的最新版本
Guo Hong
- large scale structure of galaxy distribution
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Hao Lei
- ionized gas of galaxies
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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
 - ---