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Deep learning for supernovae detection

In future astronomical sky surveys it will be humanly impossible to classify the tens of thousands of candidate transients detected per night. This thesis explores the potential of using state-of-the-art machine learning algorithms to handle this burden more accurately and quickly than trained astro...

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Main Author: Amar, Gilad
Other Authors: Bassett, Bruce
Format: Thesis
Language:English
Published: Cosmology and Gravity Group 2018
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access_status_str Open Access
author Amar, Gilad
author2 Bassett, Bruce
author_browse Amar, Gilad
Bassett, Bruce
author_facet Bassett, Bruce
Amar, Gilad
author_sort Amar, Gilad
collection Thesis
description In future astronomical sky surveys it will be humanly impossible to classify the tens of thousands of candidate transients detected per night. This thesis explores the potential of using state-of-the-art machine learning algorithms to handle this burden more accurately and quickly than trained astronomers. To this end Deep Learning methods are applied to classify transients using real-world data from the Sloan Digital Sky Survey. Using cutting-edge training techniques several Convolutional Neural networks are trained and hyper-parameters tuned to outperform previous approaches and find that human labelling errors are the primary obstacle to further improvement. The tuning and optimisation of the deep models took in excess of 700 hours on a 4-Titan X GPU cluster.
format Thesis
id oai:open.uct.ac.za:11427/27090
institution University of Cape Town (South Africa)
language eng
last_indexed 2026-06-10T12:32:05.102Z
license_str Not specified — see source repository
provenance_str_mv Harvested via OAI-PMH from UCTD — University of Cape Town Open Access Repository
publishDate 2018
publishDateRange 2018
publishDateSort 2018
publisher Cosmology and Gravity Group
publisherStr Cosmology and Gravity Group
record_format dspace
source_str UCTD — University of Cape Town Open Access Repository
spelling oai:open.uct.ac.za:11427/27090 Deep learning for supernovae detection Amar, Gilad Bassett, Bruce Applied Mathematics Astronomy In future astronomical sky surveys it will be humanly impossible to classify the tens of thousands of candidate transients detected per night. This thesis explores the potential of using state-of-the-art machine learning algorithms to handle this burden more accurately and quickly than trained astronomers. To this end Deep Learning methods are applied to classify transients using real-world data from the Sloan Digital Sky Survey. Using cutting-edge training techniques several Convolutional Neural networks are trained and hyper-parameters tuned to outperform previous approaches and find that human labelling errors are the primary obstacle to further improvement. The tuning and optimisation of the deep models took in excess of 700 hours on a 4-Titan X GPU cluster. 2018-01-30T10:23:06Z 2018-01-30T10:23:06Z 2017 Master Thesis Masters MSc http://hdl.handle.net/11427/27090 eng application/pdf Cosmology and Gravity Group Faculty of Science University of Cape Town
spellingShingle Applied Mathematics
Astronomy
Amar, Gilad
Deep learning for supernovae detection
thesis_degree_str Master's
title Deep learning for supernovae detection
title_full Deep learning for supernovae detection
title_fullStr Deep learning for supernovae detection
title_full_unstemmed Deep learning for supernovae detection
title_short Deep learning for supernovae detection
title_sort deep learning for supernovae detection
topic Applied Mathematics
Astronomy
url http://hdl.handle.net/11427/27090
work_keys_str_mv AT amargilad deeplearningforsupernovaedetection