Mightee: Deep 1.4 ghz source counts and the sky temperature contribution of star-forming galaxies and active galactic nuclei

dc.contributor.authorHale, Catherine
dc.contributor.authorWhittam, Imogen
dc.contributor.authorJarvis, Matt
dc.date.accessioned2023-06-14T09:02:43Z
dc.date.available2023-06-14T09:02:43Z
dc.date.issued2023
dc.description.abstractWe 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.identifier.citationHale, 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/stac3320en_US
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1093/mnras/stac3320
dc.identifier.urihttp://hdl.handle.net/10566/9079
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.subjectAstronomyen_US
dc.subjectPhysicsen_US
dc.subjectCosmologyen_US
dc.subjectGravitationen_US
dc.subjectGalaxiesen_US
dc.titleMightee: Deep 1.4 ghz source counts and the sky temperature contribution of star-forming galaxies and active galactic nucleien_US
dc.typeArticleen_US

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