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Likelihood-vased method for detecting faint moving objects
https://kitami-it.repo.nii.ac.jp/records/8179
https://kitami-it.repo.nii.ac.jp/records/8179e7b4ec51-b8c4-4b29-85db-c79bc92f821d
| 名前 / ファイル | ライセンス | アクション |
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2005_Likelihood-vased method for detecting faint moving objects.pdf (399.4 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||||||||
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| 公開日 | 2016-06-17 | |||||||||||
| タイトル | ||||||||||||
| タイトル | Likelihood-vased method for detecting faint moving objects | |||||||||||
| 言語 | en | |||||||||||
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| 言語 | eng | |||||||||||
| キーワード | ||||||||||||
| 主題Scheme | Other | |||||||||||
| 主題 | data analysis | |||||||||||
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| 主題Scheme | Other | |||||||||||
| 主題 | minor planets | |||||||||||
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| 主題Scheme | Other | |||||||||||
| 主題 | asteroids | |||||||||||
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| 主題Scheme | Other | |||||||||||
| 主題 | image processing | |||||||||||
| 資源タイプ | ||||||||||||
| 資源 | http://purl.org/coar/resource_type/c_6501 | |||||||||||
| タイプ | journal article | |||||||||||
| アクセス権 | ||||||||||||
| アクセス権 | open access | |||||||||||
| アクセス権URI | http://purl.org/coar/access_right/c_abf2 | |||||||||||
| 著者 |
Miura, Noriaki
× Miura, Noriaki
× Itagaki, Kazuyuki
× Baba, Naoshi
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| 著者別名 | ||||||||||||
| 識別子Scheme | WEKO | |||||||||||
| 識別子 | 44861 | |||||||||||
| 識別子Scheme | KAKEN | |||||||||||
| 識別子URI | https://nrid.nii.ac.jp/ja/nrid/1000030209720 | |||||||||||
| 識別子 | 30209720 | |||||||||||
| 姓名 | 三浦, 則明 | |||||||||||
| 言語 | ja | |||||||||||
| 抄録 | ||||||||||||
| 内容記述タイプ | Abstract | |||||||||||
| 内容記述 | We present a novel method of detecting faint moving objects in the solar system. The method is based on the evaluation of relative likelihood, which is newly introduced in this paper. Features of this method are that no thresholding operation is required and that both spatial and temporal statistical processing is implemented. These features are advantageous for detecting faint objects. In addition, relative likelihood can be used to quantitatively assess the certainty of detected objects. We applied our method to data taken at two different observatories in Japan. Experimental results indicate that this method is capable of detecting faint moving objects with signals comparable to the noise level. |
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| 書誌情報 |
The Astronomical Journal 巻 130, p. 1278-1285, 発行日 2005-09 |
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| 権利 | ||||||||||||
| 権利情報 | c 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. | |||||||||||
| 出版者 | ||||||||||||
| 出版者 | The American Astronomical Society | |||||||||||
| 関連サイト | ||||||||||||
| URL | http://iopscience.iop.org/article/10.1086/431955 | |||||||||||
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| 言語 | en | |||||||||||
| 値 | publisher | |||||||||||
| 出版タイプ | ||||||||||||
| 出版タイプ | VoR | |||||||||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||||||||
