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===Galaxy pair and galaxy interaction===  | 
  ===Galaxy pair and galaxy interaction===  | 
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* How to quantify the merging stage of   | 
  * How to quantify the merging stage of galaxy pairs?  Kinemetry, Morphlogy?  | 
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* Physical process in different stages?  | 
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[[File:Pair_stage.png|300px|thumb|center|  galaxy pair merging stage(2020ApJ...892L..20F)]]  | 
  [[File:Pair_stage.png|300px|thumb|center|  galaxy pair merging stage(2020ApJ...892L..20F)]]  | 
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===Compact groups of galaxies ===  | 
  ===Compact groups of galaxies ===  | 
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*the largest and most complete low redshift compact groups of galaxies(CGs) sample selected from SDSS and LAMOST  | 
  *the largest and most complete low redshift compact groups of galaxies(CGs) sample selected from SDSS and LAMOST.  | 
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*Dynamics and physical nature CGs  | 
  *Dynamics and physical nature CGs?  | 
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[[File:CG.jpg|  | 
  [[File:CG.jpg|300px|thumb|center| compact groups of galaxies in SDSS+LAMOST (2020ApJS..246...12Z)]]  | 
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===Dust geometry of galaxies ===  | 
  ===Dust geometry of galaxies ===  | 
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*How to measure or quantify the geometry of the dust components?  | 
  *How to measure or quantify the geometry of the dust components?  | 
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*How the dust geometries affect the observed properties of galaxies?  | 
  *How the dust geometries affect the observed properties of galaxies?  | 
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[[File:图片1.png|  | 
  [[File:图片1.png|300px|thumb|center| dust geometry model of disk galaxies]]  | 
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===HII regions of galaxies ===  | 
  ===HII regions of galaxies ===  | 
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*Identify HII regions in local star-forming galaxies using MaNGA data  | 
  *Identify HII regions in local star-forming galaxies using MaNGA data.  | 
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* Characterize the star formation process of HII regions  | 
  * Characterize the star formation process of HII regions.  | 
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[[File:HII.png|300px|thumb|center| HII regions identified from MaNGA maps]]  | 
  [[File:HII.png|300px|thumb|center| HII regions identified from MaNGA maps]]  | 
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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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2020年6月24日 (三) 08:39的最新版本
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
 - ---