Deep learning for supernovae detection
| dc.contributor.advisor | Bassett, Bruce | en_ZA |
| dc.contributor.author | Amar, Gilad | en_ZA |
| dc.date.accessioned | 2018-01-30T10:23:06Z | |
| dc.date.available | 2018-01-30T10:23:06Z | |
| dc.date.issued | 2017 | en_ZA |
| dc.description.abstract | 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. | en_ZA |
| dc.identifier.apacitation | Amar, G. (2017). <i>Deep learning for supernovae detection</i>. (Thesis). University of Cape Town ,Faculty of Science ,Cosmology and Gravity Group. Retrieved from http://hdl.handle.net/11427/27090 | en_ZA |
| dc.identifier.chicagocitation | Amar, Gilad. <i>"Deep learning for supernovae detection."</i> Thesis., University of Cape Town ,Faculty of Science ,Cosmology and Gravity Group, 2017. http://hdl.handle.net/11427/27090 | en_ZA |
| dc.identifier.citation | Amar, G. 2017. Deep learning for supernovae detection. University of Cape Town. | en_ZA |
| dc.identifier.ris | TY - Thesis / Dissertation AU - Amar, Gilad AB - 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. DA - 2017 DB - OpenUCT DP - University of Cape Town LK - https://open.uct.ac.za PB - University of Cape Town PY - 2017 T1 - Deep learning for supernovae detection TI - Deep learning for supernovae detection UR - http://hdl.handle.net/11427/27090 ER - | en_ZA |
| dc.identifier.uri | http://hdl.handle.net/11427/27090 | |
| dc.identifier.vancouvercitation | Amar G. Deep learning for supernovae detection. [Thesis]. University of Cape Town ,Faculty of Science ,Cosmology and Gravity Group, 2017 [cited yyyy month dd]. Available from: http://hdl.handle.net/11427/27090 | en_ZA |
| dc.language.iso | eng | en_ZA |
| dc.publisher.department | Cosmology and Gravity Group | en_ZA |
| dc.publisher.faculty | Faculty of Science | en_ZA |
| dc.publisher.institution | University of Cape Town | |
| dc.subject.other | Applied Mathematics | en_ZA |
| dc.subject.other | Astronomy | en_ZA |
| dc.title | Deep learning for supernovae detection | en_ZA |
| dc.type | Master Thesis | |
| dc.type.qualificationlevel | Masters | |
| dc.type.qualificationname | MSc | en_ZA |
| uct.type.filetype | Text | |
| uct.type.filetype | Image | |
| uct.type.publication | Research | en_ZA |
| uct.type.resource | Thesis | en_ZA |
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