Optimisation of galaxy identification methods on large interferometric surveys
The astronomical size of spectral data cubes that will result from the SKA pathfinders planned large HI surveys such as LADUMA; Fornax HI survey; DINGO; WALLABY; etc. necessitate fully automated three-dimensional (3D) source finding and parametrization tools. A fraction of the percentage difference...
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Dissertation |
| Language: | English |
| Published: |
Faculty of Science
2019
|
| Subjects: | |
| Online Access: | http://hdl.handle.net/11427/30072 |