Difference between revisions of "MaNGA Technical Group"
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===1. Possible Porjects=== | ===1. Possible Porjects=== | ||
====A list:==== | ====A list:==== | ||
1 | 1. Emission-line measurements, and the morphology distribution of different emission lines (science drive not yet clear) | ||
2 | 2. The stellar population analysis of type I AGNs | ||
3 | 3. The lick indices of type I AGNs | ||
4 | 4. Balmer decrements of broad and narrow emission lines of type I AGNs | ||
5 | 5. Outflow | ||
6 | 6. LSB in type I AGNs | ||
7 | 7. Velocity dispersion distributions of type I AGNs | ||
=Sources= | =Sources= | ||
Revision as of 15:34, 27 June 2018
Minutes
2018-06-26
1. 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