Difference between revisions of "MaNGA science discussion"
Jump to navigation
Jump to search
m (Shiyin moved page MaNGA monthly discussion to MaNGA science discussion) |
|||
Line 1: | Line 1: | ||
=Minutes= | |||
==17.01.11== | |||
*[[ALFALFA and MaNGA]] | |||
==Minutes== | |||
===17.01.11=== | |||
'''1. How to bin MaNGA spectra''' | '''1. How to bin MaNGA spectra''' |
Revision as of 01:41, 29 October 2018
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