“MaNGA science discussion”的版本间差异

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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 SFH dust MaNGA.pdf
  • 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