huibintemacv
Differences
This shows you the differences between two versions of the page.
Both sides previous revisionPrevious revision | Next revisionBoth sides next revision | ||
huibintemacv [2019/12/11 03:36] – [Personal information] huibintema | huibintemacv [2019/12/11 03:37] – [Summary of research interests] huibintema | ||
---|---|---|---|
Line 26: | Line 26: | ||
* Large-scale structure – merging galaxy clusters: Mpc-scale diffuse radio sources (halos, relics), tailed radio galaxies, ICM physics | * Large-scale structure – merging galaxy clusters: Mpc-scale diffuse radio sources (halos, relics), tailed radio galaxies, ICM physics | ||
* Radio sky surveys: low-frequency radio sky, large-area surveys, high-redshift radio galaxies | * Radio sky surveys: low-frequency radio sky, large-area surveys, high-redshift radio galaxies | ||
- | * Radio interferometry: | + | * Radio interferometry: |
----- | ----- |
huibintemacv.txt · Last modified: 2019/12/11 04:48 by huibintema