Classification for the Rotation Periods of Asteroids Using the Convolution Neural Network

碩士 === 國立中央大學 === 資訊工程學系 === 107 === In astronomical researches, the rotation periods of asteroids can be derived from their light curves which are the brightness as a function of time. Traditionally, a periodical analysis is performed on the light curve, and then astronomers determine the category...

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Main Authors: Tang-Cheng Lin, 林唐正
Other Authors: Meng-Feng Tsai
Format: Others
Language:zh-TW
Published: 2019
Online Access:http://ndltd.ncl.edu.tw/handle/qm34c4
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spelling ndltd-TW-107NCU053921172019-10-22T05:28:14Z http://ndltd.ncl.edu.tw/handle/qm34c4 Classification for the Rotation Periods of Asteroids Using the Convolution Neural Network 應用卷積類神經網路對小行星光變曲線圖之週期類別判別處理 Tang-Cheng Lin 林唐正 碩士 國立中央大學 資訊工程學系 107 In astronomical researches, the rotation periods of asteroids can be derived from their light curves which are the brightness as a function of time. Traditionally, a periodical analysis is performed on the light curve, and then astronomers determine the category of a possible period according to the folded light curve (i.e., a light curve folded to a particular period). This process was relied on human inspection, but it becomes very formidable due to the advancement in the technology of astronomical observation in the last decade that increases the volume of astronomical data set dramatically. Therefore, manual inspection is no longer feasible, and it is necessary to adopt an automatic method to replace the aforementioned time-consuming human review process. In this research, we use the asteroid light curves obtained from the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS). The light curves are fitted using the second-order Fourier series to find the possible rotation periods from the periodogram (i.e., the reduced 2 as a function of period). Then, a folded light curve of a certain period is generated. When a folded light curve shows a clear trend with a double-peak feature (i.e., similar to W), it is identified as a full rotation period. If a folded light curve only shows a single peak, a half rotation period is suggested (i.e., similar to V). The other cases are seen as no period found. Therefore, we deployed a deep learning technology, using convolutional neural network (CNN) as a network architecture, to construct a model to classify the folded light curves to W, V, and other shapes. From the study, we found that our model can precisely and yet much more effectively recognize a result consistent with that of human inspection. Meng-Feng Tsai 蔡孟峰 2019 學位論文 ; thesis 54 zh-TW
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description 碩士 === 國立中央大學 === 資訊工程學系 === 107 === In astronomical researches, the rotation periods of asteroids can be derived from their light curves which are the brightness as a function of time. Traditionally, a periodical analysis is performed on the light curve, and then astronomers determine the category of a possible period according to the folded light curve (i.e., a light curve folded to a particular period). This process was relied on human inspection, but it becomes very formidable due to the advancement in the technology of astronomical observation in the last decade that increases the volume of astronomical data set dramatically. Therefore, manual inspection is no longer feasible, and it is necessary to adopt an automatic method to replace the aforementioned time-consuming human review process. In this research, we use the asteroid light curves obtained from the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS). The light curves are fitted using the second-order Fourier series to find the possible rotation periods from the periodogram (i.e., the reduced 2 as a function of period). Then, a folded light curve of a certain period is generated. When a folded light curve shows a clear trend with a double-peak feature (i.e., similar to W), it is identified as a full rotation period. If a folded light curve only shows a single peak, a half rotation period is suggested (i.e., similar to V). The other cases are seen as no period found. Therefore, we deployed a deep learning technology, using convolutional neural network (CNN) as a network architecture, to construct a model to classify the folded light curves to W, V, and other shapes. From the study, we found that our model can precisely and yet much more effectively recognize a result consistent with that of human inspection.
author2 Meng-Feng Tsai
author_facet Meng-Feng Tsai
Tang-Cheng Lin
林唐正
author Tang-Cheng Lin
林唐正
spellingShingle Tang-Cheng Lin
林唐正
Classification for the Rotation Periods of Asteroids Using the Convolution Neural Network
author_sort Tang-Cheng Lin
title Classification for the Rotation Periods of Asteroids Using the Convolution Neural Network
title_short Classification for the Rotation Periods of Asteroids Using the Convolution Neural Network
title_full Classification for the Rotation Periods of Asteroids Using the Convolution Neural Network
title_fullStr Classification for the Rotation Periods of Asteroids Using the Convolution Neural Network
title_full_unstemmed Classification for the Rotation Periods of Asteroids Using the Convolution Neural Network
title_sort classification for the rotation periods of asteroids using the convolution neural network
publishDate 2019
url http://ndltd.ncl.edu.tw/handle/qm34c4
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