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==恒星演化及其应用== |
==恒星演化及其应用== |
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:advisor: Zhanwen Han |
:advisor: Zhanwen Han |
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:2017.04.26@SJTU |
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Download the PPT [http://cluster.shao.ac.cn/~jyin/20170425_Han.tar.gz] |
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==[[Photometry of overlapping galaxy pairs]]== |
==[[Photometry of overlapping galaxy pairs]]== |
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==Searching of cluster structures in multiple sky survey data== |
==Searching of cluster structures in multiple sky survey data== |
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:advisor: Zhengyi Shao |
:advisor: Zhengyi Shao |
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==students== |
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===Zhang kaiqi=== |
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*project: [[astropy.cosmolgy]] |
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2019年6月5日 (三) 02:39的最新版本
恒星演化及其应用
- advisor: Zhanwen Han
- 2017.04.26@SJTU
Download the PPT [1]
Photometry of overlapping galaxy pairs
- advisor: Shiyin Shen[2]
- collaborator: Shuai Feng (postgraduate student)
Galaxy pair is a kind of self-gravitational system, which contains two member galaxies. Because of simplest configuration, galaxy pairs are very useful to study the interaction effect, such as merge, tidal force, dynamic fiction. However, projected effect often causes overlapping in galaxy pairs, especially in compact pairs. That seriously biases photometric parameters due to comtamination of each star light and obstructs further study about galaxy pairs. So how to get rid of overlapping influence has become a very important task. More accurate photometry of overlapping galaxy pairs will be more helpful for future research.
Spectral Energy Distribution (SED) of Brown Dwarfs
- advisor: Zhengyi Shao
Searching of cluster structures in multiple sky survey data
- advisor: Zhengyi Shao
students
Zhang kaiqi
- project: astropy.cosmolgy