User Tools

Site Tools


huibintemacv

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revisionPrevious revision
Next revisionBoth sides next revision
huibintemacv [2019/12/11 03:36] – [Personal information] huibintemahuibintemacv [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: wide-field calibration and imaging, automated data reduction, algorithm development, the ionosphere +  * Radio interferometry: wide-field calibration and imaging, automated data processing, algorithm development, the ionosphere 
  
 ----- -----
huibintemacv.txt · Last modified: 2019/12/11 04:48 by huibintema

Donate Powered by PHP Valid HTML5 Valid CSS Driven by DokuWiki