Difference between revisions of "MaNGA science discussion"
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==MaNGA workshop 2019 May/24== | |||
*Lei Hao: overview of MaNGA and CSST-IFS [[File:haolei2.pptx]] | |||
*Mengting Ju: MaNDA data structure [[File:Manga数据介绍_2.pdf]] | |||
*Yunliang Zheng: Marvin | |||
*Jun Yin: Metallicity [[File:190524_Metallicity.in.MaNGA.pptx]] | |||
*Shiyin Shen: SFH and dust [[File:SFH_dust_MaNGA.pdf]] | |||
*Shuai Feng: Kinematics [[File:GalKin.pdf]] | |||
*Ling Zhu: dynamics modelling[[File:MaNGA_dynamics.pptx]] | |||
*Fangting Yuan: Mergers | |||
*Zhenzhen Li: AGN | |||
==Projects== | |||
*[[star formation history]] | |||
*[[dust extinction]] | |||
*[[metalicity]] | |||
*[[ALFALFA and MaNGA]] | *[[ALFALFA and MaNGA]] | ||
Latest revision as of 03:04, 3 June 2019
MaNGA workshop 2019 May/24
- Lei Hao: overview of MaNGA and CSST-IFS File:Haolei2.pptx
- Mengting Ju: MaNDA data structure File:Manga数据介绍 2.pdf
- Yunliang Zheng: Marvin
- Jun Yin: Metallicity File:190524 Metallicity.in.MaNGA.pptx
- Shiyin Shen: SFH and dust File:SFH dust MaNGA.pdf
- Shuai Feng: Kinematics File:GalKin.pdf
- Ling Zhu: dynamics modellingFile: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