Data Mining for Gravitational Lenses and Interacting Galaxies
碩士 === 國立中央大學 === 天文研究所 === 92 === The scientific operations of space telescopes and ground-based facilities worldwide have produced a flood of astronomical data waiting to be analyzed. Thus the development of fast and efficient system is in urgent demand for the purpose of data mining. The discov...
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ndltd-TW-092NCU051990022016-06-08T04:13:37Z http://ndltd.ncl.edu.tw/handle/05382460875998395002 Data Mining for Gravitational Lenses and Interacting Galaxies 重力透鏡和交互作用星系的資料探勘 Sze-Yeong Tan 陳詩湧 碩士 國立中央大學 天文研究所 92 The scientific operations of space telescopes and ground-based facilities worldwide have produced a flood of astronomical data waiting to be analyzed. Thus the development of fast and efficient system is in urgent demand for the purpose of data mining. The discovery of gravitational lensing events and interacting galaxies are very important in the study of cosmology. However, both types of structures are relatively rare and often hidden in the mountain of images. For these reasons, we have developed an automatic system to identify these objects from image archives by shape analysis. First, candidates are selected with the shape parameter defined by our method and a line and an arc are then fitted to these potential candidates. From error analysis the best shape can be identified. The algorithm developed in this work has been tested on two of the gravitational lensing events found in the RCS and proved to be successful. Furthermore, it has also been applied to a portion of the RCS data set, which consists of 210 images and dozens of interacting galaxies have been found. Wing-Huen Ip 葉永烜 2004 學位論文 ; thesis 52 en_US |
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碩士 === 國立中央大學 === 天文研究所 === 92 === The scientific operations of space telescopes and ground-based facilities worldwide have produced a flood of astronomical data waiting to be analyzed. Thus the development of fast and efficient system is in urgent demand for the purpose of data mining.
The discovery of gravitational lensing events and interacting galaxies are very important in the study of cosmology. However, both types of structures are relatively rare and often hidden in the mountain of images. For these reasons, we have developed an automatic system to identify these objects from image archives by shape analysis.
First, candidates are selected with the shape parameter defined by our method and a line and an arc are then fitted to these potential candidates. From error analysis the best shape can be identified. The algorithm developed in this work has been tested on two of the gravitational lensing events found in the RCS and proved to be successful. Furthermore, it has also been applied to a portion of the RCS data set, which consists of 210 images and dozens of interacting galaxies have been found.
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Wing-Huen Ip |
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Wing-Huen Ip Sze-Yeong Tan 陳詩湧 |
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Sze-Yeong Tan 陳詩湧 |
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Sze-Yeong Tan 陳詩湧 Data Mining for Gravitational Lenses and Interacting Galaxies |
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Sze-Yeong Tan |
title |
Data Mining for Gravitational Lenses and Interacting Galaxies |
title_short |
Data Mining for Gravitational Lenses and Interacting Galaxies |
title_full |
Data Mining for Gravitational Lenses and Interacting Galaxies |
title_fullStr |
Data Mining for Gravitational Lenses and Interacting Galaxies |
title_full_unstemmed |
Data Mining for Gravitational Lenses and Interacting Galaxies |
title_sort |
data mining for gravitational lenses and interacting galaxies |
publishDate |
2004 |
url |
http://ndltd.ncl.edu.tw/handle/05382460875998395002 |
work_keys_str_mv |
AT szeyeongtan dataminingforgravitationallensesandinteractinggalaxies AT chénshīyǒng dataminingforgravitationallensesandinteractinggalaxies AT szeyeongtan zhònglìtòujìnghéjiāohùzuòyòngxīngxìdezīliàotànkān AT chénshīyǒng zhònglìtòujìnghéjiāohùzuòyòngxīngxìdezīliàotànkān |
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