“MaNGA science discussion”的版本间差异
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*Shiyin Shen: SFH and dust [[File:SFH_dust_MaNGA.pdf]] |
*Shiyin Shen: SFH and dust [[File:SFH_dust_MaNGA.pdf]] |
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*Shuai Feng: Kinematics [[File:GalKin.pdf]] |
*Shuai Feng: Kinematics [[File:GalKin.pdf]] |
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*Ling Zhu: dynamics modelling |
*Ling Zhu: dynamics modelling[[File:Example.jpg]] |
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*Fangting Yuan: Mergers |
*Fangting Yuan: Mergers |
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*Zhenzhen Li: AGN |
*Zhenzhen Li: AGN |
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2019年5月27日 (一) 06:24的版本
MaNGA workshop 2019 May/24
- Lei Hao: overview of MaNGA and CSST-IFS
- Mengting Ju: MaNDA data structure
- Yunliang Zheng: Marvin
- Jun Yin: Metallicity
- Shiyin Shen: SFH and dust
- Shuai Feng: Kinematics
- Ling Zhu: dynamics modelling文件:Example.jpg
- 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