| dc.contributor.author | Hale, Catherine | |
| dc.contributor.author | Whittam, Imogen | |
| dc.contributor.author | Jarvis, Matt | |
| dc.date.accessioned | 2023-06-14T09:02:43Z | |
| dc.date.available | 2023-06-14T09:02:43Z | |
| dc.date.issued | 2023 | |
| dc.identifier.citation | Hale, C. et al. (2023). Mightee: Deep 1.4 ghz source counts and the sky temperature contribution of star-forming galaxies and active galactic nuclei. Monthly Notices of the Royal Astronomical Society, 520(2), 2668–2691. https://doi.org/10.1093/mnras/stac3320 | en_US |
| dc.identifier.issn | 1365-2966 | |
| dc.identifier.uri | https://doi.org/10.1093/mnras/stac3320 | |
| dc.identifier.uri | http://hdl.handle.net/10566/9079 | |
| dc.description.abstract | We present deep 1.4 GHz source counts from ∼5 deg2 of the continuum Early Science data release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration survey down to S1.4GHz ∼15 μ
Jy. Using observations over two extragalactic fields (COSMOS and XMM-LSS), we provide a comprehensive investigation into correcting the incompleteness of the raw source counts within the survey to understand the true underlying source count population. We use a variety of simulations that account for: errors in source detection and characterization, clustering, and variations in the assumed source model used to simulate sources within the field and characterize source count incompleteness. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.subject | Astronomy | en_US |
| dc.subject | Physics | en_US |
| dc.subject | Cosmology | en_US |
| dc.subject | Gravitation | en_US |
| dc.subject | Galaxies | en_US |
| dc.title | Mightee: Deep 1.4 ghz source counts and the sky temperature contribution of star-forming galaxies and active galactic nuclei | en_US |
| dc.type | Article | en_US |
