Supervised machine learning techniques for radio source classification

dc.contributor.advisorVaccari, Mattia
dc.contributor.authorMofokeng, Chaka
dc.date.accessioned2023-05-17T10:51:16Z
dc.date.accessioned2024-10-30T10:23:09Z
dc.date.available2023-05-17T10:51:16Z
dc.date.available2024-10-30T10:23:09Z
dc.date.issued2023
dc.descriptionMasters of Scienceen_US
dc.description.abstractClassification is one of the most fundamental aspects of scientific investigation. Astronomers have thus developed several classification schemes to try and make sense of the evolving properties of planets, stars and galaxies. One of the most popular ways to classify galaxies is according to their shape, or morphology, which has long been performed visually to produce annotated galaxy catalogues. However, visual inspection and manual annotation by astronomers will not be able to keep up with the expected data flow from next-generation sky surveys. In this context, the main objective of our study was to use deep learning to automate radio source characterization (that is detection, classification and identification) from image data efficiently. We adopted a pre-trained deep learning model called CLARAN (Classifying Radio Sources Automatically with Neural Networks) based on the Radio Galaxy Zoo Citizen Science Classification Project and applied it to a GMRT 610 MHz survey in the ELAIS-N1 region covering an area of 12.8 square degrees at a resolution of approximately 6 arcsec at a rootmean-square noise of about 40 µJy/beam.en_US
dc.identifier.urihttps://hdl.handle.net/10566/16584
dc.language.isoenen_US
dc.publisherUniversity of the Western Capeen_US
dc.rights.holderUniversity of the Western Capeen_US
dc.subjectRadio surveysen_US
dc.subjectCosmic radio sourcesen_US
dc.subjectDeep learningen_US
dc.subjectAstronomyen_US
dc.subjectCLARANen_US
dc.titleSupervised machine learning techniques for radio source classificationen_US

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