“MaNGA science discussion”的版本间差异

来自cluster
跳到导航 跳到搜索
无编辑摘要
无编辑摘要
 
(未显示2个用户的10个中间版本)
第1行: 第1行:
==MaNGA workshop 2019 May/24==
==projects==

*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]]
*[[star formation history]]
*[[dust extinction]]
*[[dust extinction]]
*[[metalicity]]
*[[metalicity]]
*[[ALFALFA and MaNGA]]
*[[ALFALFA and MaNGA]]

==Data==
* https://trac.sdss.org/wiki/MANGA/Data/Access
:MPL-2 --》 click 'redux/v1_1_2'
:drpall-v1_1_2.fits: target information
:platelist3d: list of target with images

*Also check:
:https://sas.sdss.org/manga/
:https://trac.sdss.org/wiki/MANGA/Data/MangaSASTutorial
:file server [https://data.sdss.org/sas/mangawork/manga/spectro/](password protected, ask someone)
:data Tutorial [https://trac.sdss.org/wiki/MANGA/Data/DataTutorial]

*data on [[Iserver_Service | iserver上]]
:/data/data_SDSS/MANGA, try /data/data_SDSS/MANGA/IDL_pro/ml2.tar.gz




==Minutes==
==Minutes==

2019年6月3日 (一) 03:04的最新版本

MaNGA workshop 2019 May/24

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