“MaNGA science discussion”的版本间差异
跳到导航
跳到搜索
无编辑摘要 |
|||
第5行: | 第5行: | ||
*Yunliang Zheng: Marvin |
*Yunliang Zheng: Marvin |
||
*Jun Yin: Metallicity |
*Jun Yin: Metallicity |
||
*Shiyin Shen: SFH and dust |
*Shiyin Shen: SFH and dust [[File:SFH_dust_MaNGA.pdf]] |
||
*Shuai Feng: Kinematics |
*Shuai Feng: Kinematics |
||
*Ling Zhu: dynamics modelling |
*Ling Zhu: dynamics modelling |
||
*Fangting Yuan: Mergers |
*Fangting Yuan: Mergers |
||
*Zhenzhen Li: AGN |
*Zhenzhen Li: AGN |
||
==Projects== |
==Projects== |
2019年5月24日 (五) 09:09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
- 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