Difference between revisions of "MaNGA Technical Group"

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==2018-06-26==
==2018-06-26==


===1. Possible Porjects===
# Possible Porjects
====A list:====
## A list:
1. Emission-line measurements, and the morphology distribution of different emission lines (science drive not yet clear)
### Emission-line measurements, and the morphology distribution of different emission lines (science drive not yet clear)
2. The stellar population analysis of type I AGNs
### The stellar population analysis of type I AGNs
3. The lick indices of type I AGNs
### The lick indices of type I AGNs
4. Balmer decrements of broad and narrow emission lines of type I AGNs  
### Balmer decrements of broad and narrow emission lines of type I AGNs  
5. Outflow
### Outflow
6. LSB in type I AGNs
### LSB in type I AGNs
7. Velocity dispersion distributions of type I AGNs
### Velocity dispersion distributions of type I AGNs


=Sources=
=Sources=

Revision as of 15:36, 27 June 2018

Minutes

2018-06-26

  1. Possible Porjects
    1. A list:
      1. Emission-line measurements, and the morphology distribution of different emission lines (science drive not yet clear)
      2. The stellar population analysis of type I AGNs
      3. The lick indices of type I AGNs
      4. Balmer decrements of broad and narrow emission lines of type I AGNs
      5. Outflow
      6. LSB in type I AGNs
      7. Velocity dispersion distributions of type I AGNs

Sources

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