“MaNGA science discussion”的版本间差异
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==MaNGA workshop 2019 May/24== |
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*Lei Hao: overview of MaNGA and CSST-IFS [[File:haolei2.pptx]] |
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*Mengting Ju: MaNDA data structure [[File:Manga数据介绍_2.pdf]] |
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*Yunliang Zheng: Marvin |
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*Jun Yin: Metallicity [[File:190524_Metallicity.in.MaNGA.pptx]] |
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*Shiyin Shen: SFH and dust [[File:SFH_dust_MaNGA.pdf]] |
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*Shuai Feng: Kinematics [[File:GalKin.pdf]] |
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*Ling Zhu: dynamics modelling[[File:MaNGA_dynamics.pptx]] |
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*Fangting Yuan: Mergers |
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*Zhenzhen Li: AGN |
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==Projects== |
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*[[star formation history]] |
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*[[dust extinction]] |
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*[[metalicity]] |
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*[[ALFALFA and MaNGA]] |
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'''1. How to bin MaNGA spectra''' |
'''1. How to bin MaNGA spectra''' |
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2019年6月3日 (一) 03:04的最新版本
MaNGA workshop 2019 May/24
- Lei Hao: overview of MaNGA and CSST-IFS 文件:Haolei2.pptx
- Mengting Ju: MaNDA data structure
- Yunliang Zheng: Marvin
- Jun Yin: Metallicity 文件:190524 Metallicity.in.MaNGA.pptx
- Shiyin Shen: SFH and dust
- Shuai Feng: Kinematics
- Ling Zhu: dynamics modelling文件:MaNGA dynamics.pptx
- Fangting Yuan: Mergers
- Zhenzhen Li: AGN
Projects
Minutes
17.01.11
1. How to bin MaNGA spectra
(1) Average flux (current method) (2) Maybe. using S/N as weight?
2. Generate a wiki page, upload emission line mask program (Shiyin Shen)
3. Current projects
Fangting: Spatially resolved star formation history of Mrk848, difference between star and gas extinction in mergers
Shiyin: Stellar population fitting, embed chemical evolution models to the fitting method
Huan: Halpha/Hbeta line ratio (still in preparation)
Jun & Mengting: BCD galaxies, stellar population
Ramya: LSB galaxies, mass-metallicity relation, SFR-mass relation
2-3 index to get stellar metallicity
Ting: Properties of Mid-infrared bright galaxies, using Halpha, Hdelta & D4000 to study star formation history of Mergers