Difference between revisions of "MaNGA science discussion"

Revision as of 01:43, 29 October 2018

MPL-2 --》 click 'redux/v1_1_2'

drpall-v1_1_2.fits: target information

platelist3d: list of target with images

file server [1]（password protected, ask someone）

data Tutorial [2]

/data/data_SDSS/MANGA, try /data/data_SDSS/MANGA/IDL_pro/ml2.tar.gz

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

@@ Line 1: / Line 1: @@
+==projects==
+*[[star formation history]]
+*[[dust extinction]]
+*[[metalicity]]
+*[[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
-*[[ALFALFA and MaNGA]]
 ==Minutes==