Difference between revisions of "MaNGA Technical Group"

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


# Possible Porjects
=== Possible Porjects ===
## A list:
A list:
### 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)
### The stellar population analysis of type I AGNs
# The stellar population analysis of type I AGNs
### The lick indices of type I AGNs
# The lick indices of type I AGNs
### Balmer decrements of broad and narrow emission lines of type I AGNs  
# Balmer decrements of broad and narrow emission lines of type I AGNs  
### Outflow
# Outflow
### LSB in type I AGNs
# LSB in type I AGNs
### 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

Possible Porjects

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