Automatic detection of cataclysmic variables from SDSS images

IF 4.5 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Publications of the Astronomical Society of Australia Pub Date : 2023-06-29 DOI:10.1017/pasa.2023.34
Junfeng Huang, Meixia Qu, Bin Jiang, Yanxia Zhang
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Abstract

Abstract Investigating rare and new objects have always been an important direction in astronomy. Cataclysmic variables (CVs) are ideal and natural celestial bodies for studying the accretion process of semi-detached binaries with accretion processes. However, the sample size of CVs must increase because a lager gap exists between the observational and the theoretical expanding CVs. Astronomy has entered the big data era and can provide massive images containing CV candidates. CVs as a type of faint celestial objects, are highly challenging to be identified directly from images using automatic manners. Deep learning has rapidly developed in intelligent image processing and has been widely applied in some astronomical fields with excellent detection results. YOLOX, as the latest YOLO framework, is advantageous in detecting small and dark targets. This work proposes an improved YOLOX-based framework according to the characteristics of CVs and Sloan Digital Sky Survey (SDSS) photometric images to train and verify the model to realise CV detection. We use the Convolutional Block Attention Module to increase the number of output features with the feature extraction network and adjust the feature fusion network to obtain fused features. Accordingly, the loss function is modified. Experimental results demonstrate that the improved model produces satisfactory results, with average accuracy (mean average Precision at 0.5) of 92.0%, Precision of 92.9%, Recall of 94.3%, and $F1-score$ of 93.6% on the test set. The proposed method can efficiently achieve the identification of CVs in test samples and search for CV candidates in unlabeled images. The image data vastly outnumber the spectra in the SDSS-released data. With supplementary follow-up observations or spectra, the proposed model can help astronomers in seeking and detecting CVs in a new manner to ensure that a more extensive CV catalog can be built. The proposed model may also be applied to the detection of other kinds of celestial objects.
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从SDSS图像中自动检测灾难性变量
研究罕见的新天体一直是天文学研究的重要方向。巨变星(cv)是研究具有吸积过程的半分离双星吸积过程的理想的自然天体。然而,cv的样本量必须增加,因为在观测值和理论扩展cv之间存在较大的差距。天文学已经进入了大数据时代,可以提供大量包含CV候选人的图像。cv作为一种微弱的天体,用自动方式从图像中直接识别是非常挑战。深度学习在智能图像处理方面发展迅速,在一些天文领域得到了广泛的应用,并取得了优异的检测效果。YOLOX作为最新的YOLO框架,在探测小目标和暗目标方面具有优势。本文根据CV和斯隆数字巡天(SDSS)光度图像的特点,提出了一种改进的基于yolox的框架,对模型进行训练和验证,实现CV检测。我们使用卷积块注意模块增加特征提取网络的输出特征数量,并调整特征融合网络以获得融合特征。因此,对损失函数进行了修正。实验结果表明,改进后的模型在测试集上的平均准确率为92.0%(平均精密度为0.5),精密度为92.9%,召回率为94.3%,$F1-score$为93.6%。该方法可以有效地实现对测试样本中的CV的识别和对未标记图像中的候选CV的搜索。图像数据远远超过sdss发布的光谱数据。通过补充后续观测或光谱,该模型可以帮助天文学家以新的方式寻找和探测CV,以确保建立更广泛的CV目录。所提出的模型也可应用于其他天体的探测。
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来源期刊
Publications of the Astronomical Society of Australia
Publications of the Astronomical Society of Australia 地学天文-天文与天体物理
CiteScore
5.90
自引率
9.50%
发文量
41
审稿时长
>12 weeks
期刊介绍: Publications of the Astronomical Society of Australia (PASA) publishes new and significant research in astronomy and astrophysics. PASA covers a wide range of topics within astronomy, including multi-wavelength observations, theoretical modelling, computational astronomy and visualisation. PASA also maintains its heritage of publishing results on southern hemisphere astronomy and on astronomy with Australian facilities. PASA publishes research papers, review papers and special series on topical issues, making use of expert international reviewers and an experienced Editorial Board. As an electronic-only journal, PASA publishes paper by paper, ensuring a rapid publication rate. There are no page charges. PASA''s Editorial Board approve a certain number of papers per year to be published Open Access without a publication fee.
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