HI intensity mapping: Impact of primary beam effects
| dc.contributor.advisor | Santos, Mario G. | |
| dc.contributor.author | Matshawule, Siyambonga Donald | |
| dc.date.accessioned | 2023-02-01T08:29:25Z | |
| dc.date.accessioned | 2024-05-14T13:26:41Z | |
| dc.date.available | 2023-02-01T08:29:25Z | |
| dc.date.available | 2024-05-14T13:26:41Z | |
| dc.date.issued | 2023 | |
| dc.description | Philosophiae Doctor - PhD | en_US |
| dc.description.abstract | Neutral hydrogen (HI) intensity mapping surveys with upcoming and future radio telescopes such as the MeerKAT, a precursor to the Square Kilometre Array Observatory (SKAO) MID telescope, have great potential for constraining cosmology, particularly in the post-reionization Universe provided that e ective cleaning methods are available to separate the strong foregrounds from the cosmological signal. The application of cleaning methods is usually conducted under the assumption of simplistic primary beam models. In this thesis, I simulate a single-dish wide-area survey with MeerKAT characteristics, and test foreground subtraction with a realistic model for the primary beam that contains a non-trivial frequency dependence. I also probe the impact of strong point sources on the cleaning. To conduct this evaluation, point source maps from a much more realistic full-sky point source catalogue are included as part of the foregrounds present in the sky model. | en_US |
| dc.identifier.uri | https://hdl.handle.net/10566/15021 | |
| dc.language.iso | en | en_US |
| dc.publisher | University of the Western Cape | en_US |
| dc.rights.holder | University of the Western Cape | en_US |
| dc.subject | Astronomy | en_US |
| dc.subject | Physics | en_US |
| dc.subject | Cosmology | en_US |
| dc.subject | Neutral hydrogen | en_US |
| dc.title | HI intensity mapping: Impact of primary beam effects | en_US |