Automation of source-artefact classification
The high sensitivities of modern radio telescopes will enable the detection of very faint astrophysical sources in the distant Universe. However, these high sensitivities also imply that calibration artefacts, which were below the noise for less sensitive instruments, will emerge above the noise and...
| Main Author: | |
|---|---|
| Format: | Others |
| Language: | English |
| Published: |
Rhodes University
2017
|
| Online Access: | http://hdl.handle.net/10962/4920 |