“Intern program for college students”的版本间差异

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==恒星演化及其应用==
:advisor: Zhanwen Han
:2017.04.26@SJTU
Download the PPT [http://cluster.shao.ac.cn/~jyin/20170425_Han.tar.gz]

==[[Photometry of overlapping galaxy pairs]]==
==[[Photometry of overlapping galaxy pairs]]==
⚫
[[File:overlapping_pair.png|150px|right]]
:advisor: Shiyin Shen[http://cluster.shao.ac.cn/~shen/]
:advisor: Shiyin Shen[http://cluster.shao.ac.cn/~shen/]
:collaborator: Shuai Feng (postgraduate student)
:collaborator: Shuai Feng (postgraduate student)

⚫
[[File:overlapping_pair.png|150px|right]]
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==
==Spectral Energy Distribution (SED) of Brown Dwarfs==
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==Searching of cluster structures in multiple sky survey data==
==Searching of cluster structures in multiple sky survey data==
:advisor: Zhengyi Shao
:advisor: Zhengyi Shao

==students==
===Zhang kaiqi===
*project: [[astropy.cosmolgy]]

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

Overlapping pair.png
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

取自“http://cluster.shao.ac.cn/wiki/index.php?title=Intern_program_for_college_students&oldid=3121”