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Application of statistical pattern recognition and deep learning for morphological classification in radio astronomy

Thesis (MSc)--Stellenbosch University, 2022.

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Main Author: Becker, Adolf Burger
Other Authors: Grobler, Trienko
Format: Thesis
Language:en_ZA
Published: Stellenbosch : Stellenbosch University 2022
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access_status_str Open Access
author Becker, Adolf Burger
author2 Grobler, Trienko
author_browse Becker, Adolf Burger
Grobler, Trienko
author_facet Grobler, Trienko
Becker, Adolf Burger
author_sort Becker, Adolf Burger
collection Thesis
dc_rights_str_mv Stellenbosch University
description Thesis (MSc)--Stellenbosch University, 2022.
format Thesis
id oai:scholar.sun.ac.za:10019.1/124690
institution Stellenbosch University (South Africa)
language en_ZA
last_indexed 2026-06-10T12:43:34.445Z
license_str Other — see source repository
provenance_str_mv Harvested via OAI-PMH from SUNScholar — Stellenbosch University Repository
publishDate 2022
publishDateRange 2022
publishDateSort 2022
publisher Stellenbosch : Stellenbosch University
publisherStr Stellenbosch : Stellenbosch University
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source_str SUNScholar — Stellenbosch University Repository
spelling oai:scholar.sun.ac.za:10019.1/124690 Application of statistical pattern recognition and deep learning for morphological classification in radio astronomy Becker, Adolf Burger Grobler, Trienko Stellenbosch University. Faculty of Science. Dept. of Computer Science. Machine Learning UCTD Radio astronomy Pattern recognition systems Deep learning (Machine learning) Morphological classification Thesis (MSc)--Stellenbosch University, 2022. ENGLISH ABSTRACT: The morphological classification of radio sources is important to gain a full under standing of galaxy evolution processes and their relation with local environmental properties. Furthermore, the complex nature of the problem, its appeal for citi zen scientists and the large data rates generated by existing and upcoming radio telescopes combine to make the morphological classification of radio sources an ideal test case for the application of machine learning techniques. One approach that has shown great promise recently is Convolutional Neural Networks (CNNs). Literature, however, lacks two major things when it comes to CNNs and radio galaxy morphological classification. Firstly, a proper analysis to identify whether overfitting occurs when training CNNs to perform radio galaxy morphological clas sification is needed. Secondly, a comparative study regarding the practical appli cability of the CNN architectures in literature is required. Both of these short comings are addressed in this thesis. Multiple performance metrics are used for the latter comparative study, such as inference time, model complexity, compu tational complexity and mean per class accuracy. A ranking system based upon recognition and computational performance is proposed. MCRGNet, ATLAS and ConvXpress (novel classifier) are the architectures that best balance computational requirements with recognition performance. AFRIKAANSE OPSOMMING: Die morfologiese klassifikasie van radiobronne is belangrik om ’n volledige begrip van die evolusieprosesse binnein sterrestelsels te ontwikkel, asook die rol wat hul plaaslike omgewings hierin speel. As gevolg van die ingewikkelde aard van die probleem, asook die aantrekkingskrag daarvan vir “burgerwetenskaplikes” en die groot hoeveelhede data wat deur bestaande en opkomende radioteleskope gege nereer word, maak die morfologiese klassifikasie van radiobronne ’n ideale proef gebied vir die toepassing van masjienleertegnieke. ’n Benadering wat belowend lyk, is Konvolusionele Neurale Netwerke (KNNe). Literatuur ontbreek egter twee belangrike dinge as dit kom by KNNe en die morfologiese klassifikasie van radio sterrestelsels. Eerstens is daar ’n analise nodig rondom die identifikasie van oor passing wanneer KNNe afgerig word om radio sterrestelsels volgens morfologie te klassifiseer. Tweedens word ’n vergelykende studie oor die praktiese toepaslik heid van die KNN-argitekture in literatuur benodig. Albei hierdie tekortkominge word in hierdie tesis aagespreek. Veelvuldige prestasiemetings word vir laasgenoemde vergelykende studie gebruik, soos inferensietyd, modelkompleksiteit, berekeningkompleksiteit en gemiddelde akkuraatheid per klas. ’n Rangorde skema word voorgestel gebaseer op herkenning en berekeningsprestasie. MCRGNet, AT LAS en ConvXpress (nuwe bydrae) is die argitekture wat berekeningsvereistes en herkenningsprestasie die beste balanseer. Masters 2022-03-01T10:36:37Z 2022-04-29T09:26:43Z 2022-03-01T10:36:37Z 2022-04-29T09:26:43Z 2022-04 Thesis http://hdl.handle.net/10019.1/124690 en_ZA Stellenbosch University 127 pages application/pdf Stellenbosch : Stellenbosch University
spellingShingle Machine Learning
UCTD
Radio astronomy
Pattern recognition systems
Deep learning (Machine learning)
Morphological classification
Becker, Adolf Burger
Application of statistical pattern recognition and deep learning for morphological classification in radio astronomy
title Application of statistical pattern recognition and deep learning for morphological classification in radio astronomy
title_full Application of statistical pattern recognition and deep learning for morphological classification in radio astronomy
title_fullStr Application of statistical pattern recognition and deep learning for morphological classification in radio astronomy
title_full_unstemmed Application of statistical pattern recognition and deep learning for morphological classification in radio astronomy
title_short Application of statistical pattern recognition and deep learning for morphological classification in radio astronomy
title_sort application of statistical pattern recognition and deep learning for morphological classification in radio astronomy
topic Machine Learning
UCTD
Radio astronomy
Pattern recognition systems
Deep learning (Machine learning)
Morphological classification
url http://hdl.handle.net/10019.1/124690
work_keys_str_mv AT beckeradolfburger applicationofstatisticalpatternrecognitionanddeeplearningformorphologicalclassificationinradioastronomy