Feng Xue-qi , Tu Liang-ping , Zhong Zheng-di , Li Juan , Li Xin
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Firstly, five classical target detection algorithms are compared through experiments and the optimal YOLOX algorithm is selected as the basic algorithm. Then, the YOLOX-CS framework is constructed by combining different attention mechanisms and different optimizers. The data set uses images from the Sloan Digital Sky Survey (SDSS), labelled from LSBG in the <span><math><mrow><mi>α</mi><mo>.</mo><mn>40</mn></mrow></math></span>-SDSS DR7 (the cross coverage area of 40% HI Arecibo Legacy Fast ALFA Survey and SDSS Data Release7) survey. Due to the small number of samples in this data set, Deep Convolutional Generative Adversarial Networks (DCGAN) model is used to expand the experimental test data. After comparing with a series of target detection algorithms, YOLOX-CS has a good test result in searching LSBG recall rate and Average Precision (AP) value in two data sets before and after expansion. The recall rate and AP value in the test set without expansion data set reach 97.75% and 97.83%, respectively. In the expanded data set of DCGAN model, under the same test set, the recall rate reaches 99.10% and the AP value reaches 98.94%, which proves that the algorithm has excellent performance in LSBG search. Finally, the algorithm is applied to SDSS photometric data, and 765 LSBG candidates are obtained.</p></div>","PeriodicalId":35730,"journal":{"name":"Chinese Astronomy and Astrophysics","volume":"48 3","pages":"Pages 462-488"},"PeriodicalIF":0.0000,"publicationDate":"2024-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"YOLOX-CS: An Automatic Search Algorithm for Low Surface Brightness Galaxies\",\"authors\":\"Feng Xue-qi , Tu Liang-ping , Zhong Zheng-di , Li Juan , Li Xin\",\"doi\":\"10.1016/j.chinastron.2024.09.002\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>The characteristics of Low Surface Brightness Galaxies (LSBGs) are very important for understanding the overall characteristics of galaxies. It is of great significance to search and expand the samples of Low Surface Brightness Galaxies by modern machine learning, especially deep learning algorithm. LSBGs are difficult to discern automatically and accurately with traditional methods because of their obscure features. However, deep learning does have the advantage of automatically identifying complex and effective features. To solve this problem, an algorithm named You Only Look Once version X-CS (YOLOX-CS) is proposed to search LSBG in large sample sky survey. Firstly, five classical target detection algorithms are compared through experiments and the optimal YOLOX algorithm is selected as the basic algorithm. Then, the YOLOX-CS framework is constructed by combining different attention mechanisms and different optimizers. The data set uses images from the Sloan Digital Sky Survey (SDSS), labelled from LSBG in the <span><math><mrow><mi>α</mi><mo>.</mo><mn>40</mn></mrow></math></span>-SDSS DR7 (the cross coverage area of 40% HI Arecibo Legacy Fast ALFA Survey and SDSS Data Release7) survey. 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引用次数: 0
摘要
低表面亮度星系(LSBGs)的特征对于了解星系的整体特征非常重要。利用现代机器学习,特别是深度学习算法搜索和扩展低表面亮度星系样本具有重要意义。由于低表面亮度星系的特征不明显,传统方法很难自动准确地识别它们。然而,深度学习确实具有自动识别复杂而有效特征的优势。为了解决这个问题,我们提出了一种名为 "YOLOX-CS(You Only Look Once version X-CS)"的算法,用于在大样本巡天中搜索 LSBG。首先,通过实验比较了五种经典的目标检测算法,选出最优的 YOLOX 算法作为基本算法。然后,结合不同的注意机制和不同的优化器,构建了 YOLOX-CS 框架。数据集使用的是斯隆数字巡天(SDSS)的图像,由α.40-SDSS DR7(40% HI Arecibo Legacy Fast ALFA Survey 和 SDSS Data Release7 的交叉覆盖区)巡天中的 LSBG 标注。由于该数据集样本数量较少,因此使用深度卷积生成对抗网络(DCGAN)模型来扩展实验测试数据。经过与一系列目标检测算法的比较,YOLOX-CS 在扩展前后两个数据集的 LSBG 搜索召回率和平均精度(Average Precision,AP)值方面都取得了良好的测试结果。在未扩展数据集的测试集中,召回率和平均精度值分别达到了 97.75% 和 97.83%。在 DCGAN 模型的扩展数据集中,在相同的测试集下,召回率达到 99.10%,平均精确度(AP)达到 98.94%,这证明该算法在 LSBG 搜索中表现出色。最后,将该算法应用于 SDSS 测光数据,得到了 765 个 LSBG 候选者。
YOLOX-CS: An Automatic Search Algorithm for Low Surface Brightness Galaxies
The characteristics of Low Surface Brightness Galaxies (LSBGs) are very important for understanding the overall characteristics of galaxies. It is of great significance to search and expand the samples of Low Surface Brightness Galaxies by modern machine learning, especially deep learning algorithm. LSBGs are difficult to discern automatically and accurately with traditional methods because of their obscure features. However, deep learning does have the advantage of automatically identifying complex and effective features. To solve this problem, an algorithm named You Only Look Once version X-CS (YOLOX-CS) is proposed to search LSBG in large sample sky survey. Firstly, five classical target detection algorithms are compared through experiments and the optimal YOLOX algorithm is selected as the basic algorithm. Then, the YOLOX-CS framework is constructed by combining different attention mechanisms and different optimizers. The data set uses images from the Sloan Digital Sky Survey (SDSS), labelled from LSBG in the -SDSS DR7 (the cross coverage area of 40% HI Arecibo Legacy Fast ALFA Survey and SDSS Data Release7) survey. Due to the small number of samples in this data set, Deep Convolutional Generative Adversarial Networks (DCGAN) model is used to expand the experimental test data. After comparing with a series of target detection algorithms, YOLOX-CS has a good test result in searching LSBG recall rate and Average Precision (AP) value in two data sets before and after expansion. The recall rate and AP value in the test set without expansion data set reach 97.75% and 97.83%, respectively. In the expanded data set of DCGAN model, under the same test set, the recall rate reaches 99.10% and the AP value reaches 98.94%, which proves that the algorithm has excellent performance in LSBG search. Finally, the algorithm is applied to SDSS photometric data, and 765 LSBG candidates are obtained.
期刊介绍:
The vigorous growth of astronomical and astrophysical science in China led to an increase in papers on astrophysics which Acta Astronomica Sinica could no longer absorb. Translations of papers from two new journals the Chinese Journal of Space Science and Acta Astrophysica Sinica are added to the translation of Acta Astronomica Sinica to form the new journal Chinese Astronomy and Astrophysics. Chinese Astronomy and Astrophysics brings English translations of notable articles to astronomers and astrophysicists outside China.