The applications of deep neural networks to sdBV classification

With several new large-scale surveys on the horizon, including LSST, TESS, ZTF, and Evryscope, faster and more accurate analysis methods will be required to adequately process the enormous amount of data produced. Deep learning, used in industry for years now, allows for advanced feature detection i...

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Main Author: Boudreaux Thomas M.
Format: Article
Language:English
Published: De Gruyter 2017-12-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-D-17-0450
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author Boudreaux Thomas M.
author_facet Boudreaux Thomas M.
author_sort Boudreaux Thomas M.
collection DOAJ
description With several new large-scale surveys on the horizon, including LSST, TESS, ZTF, and Evryscope, faster and more accurate analysis methods will be required to adequately process the enormous amount of data produced. Deep learning, used in industry for years now, allows for advanced feature detection in minimally prepared datasets at very high speeds; however, despite the advantages of this method, its application to astrophysics has not yet been extensively explored. This dearth may be due to a lack of training data available to researchers. Here we generate synthetic data loosely mimicking the properties of acoustic mode pulsating stars and we show that two separate paradigms of deep learning - the Artificial Neural Network And the Convolutional Neural Network - can both be used to classify this synthetic data effectively. And that additionally this classification can be performed at relatively high levels of accuracy with minimal time spent adjusting network hyperparameters.
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spelling doaj.art-d52e126c1f1e4131a0adc7164c7a2e8d2022-12-21T22:08:02ZengDe GruyterOpen Astronomy2543-63762017-12-0126125826910.1515/astro-D-17-0450astro-D-17-0450The applications of deep neural networks to sdBV classificationBoudreaux Thomas M.0Department of Physics, High Point University, One University Parkway, High Point, NC 27268, USAWith several new large-scale surveys on the horizon, including LSST, TESS, ZTF, and Evryscope, faster and more accurate analysis methods will be required to adequately process the enormous amount of data produced. Deep learning, used in industry for years now, allows for advanced feature detection in minimally prepared datasets at very high speeds; however, despite the advantages of this method, its application to astrophysics has not yet been extensively explored. This dearth may be due to a lack of training data available to researchers. Here we generate synthetic data loosely mimicking the properties of acoustic mode pulsating stars and we show that two separate paradigms of deep learning - the Artificial Neural Network And the Convolutional Neural Network - can both be used to classify this synthetic data effectively. And that additionally this classification can be performed at relatively high levels of accuracy with minimal time spent adjusting network hyperparameters.https://doi.org/10.1515/astro-D-17-0450deep learningsdbv
spellingShingle Boudreaux Thomas M.
The applications of deep neural networks to sdBV classification
Open Astronomy
deep learning
sdbv
title The applications of deep neural networks to sdBV classification
title_full The applications of deep neural networks to sdBV classification
title_fullStr The applications of deep neural networks to sdBV classification
title_full_unstemmed The applications of deep neural networks to sdBV classification
title_short The applications of deep neural networks to sdBV classification
title_sort applications of deep neural networks to sdbv classification
topic deep learning
sdbv
url https://doi.org/10.1515/astro-D-17-0450
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