论文标题

SE-RESNET+SVM模型:从Lamost中搜索热门曲线的有效方法

Se-ResNet+SVM model: an effective method of searching for hot subdwarfs from LAMOST

论文作者

Zhongding, Cheng, xiaoming, Kong, Tianmin, Wu, Yude, Bu, Zhenxin, Lei, Yatao, Zhang, Zhenping, Yi, Meng, Liu

论文摘要

在本文中,我们将功能融合想法应用于SE-Resnet提取的抽象功能与经验特征融合到混合功能中,并将混合功能输入支持向量机(SVM),以对热subdwarfs进行分类。基于这个想法,我们构建了一个SE-Resnet+SVM模型,包括二进制分类模型和四级分类模型。四级分类模型可以进一步筛选通过二进制分类模型获得的热门候选者。由二进制组得出的F1值和测试集上的四类分类模型分别为96.17%和95.64%。然后,我们使用二进制分类模型在Lamost DR8的低分辨率光谱中对333,534个非FGK型光谱进行分类,并获得3,266个热分子subdwarf候选者的目录,其中1223个是新确定的。随后,当将阈值设置为0.5和0.9时,四级分类模型进一步过滤了3,266个候选者,409和296分别是新确定的。通过手动检查,在三个新确定的候选人中的真实数量是176、63和41,这三种情况的分类模型的相应精度分别为67.94%,84.88%和87.60%。最后,我们训练TEFF的MAE值为1212.65 k的SE-RESNET回归模型,对数G为0.32 DEX,[HE/H]训练0.32 DEX,并预测这176个热分颗粒恒星的大气参数。这提供了一定数量的样本,以帮助将来对热门群的研究。

In this paper, we apply the feature-integration idea to fuse the abstract features extracted by Se-ResNet with experience features into hybrid features and input the hybrid features to the Support Vector Machine (SVM) to classify Hot subdwarfs. Based on this idea, we construct a Se-ResNet+SVM model, including a binary classification model and a four-class classification model. The four-class classification model can further screen the hot subdwarf candidates obtained by the binary classification model. The F1 values derived by the binary and the four-class classification model on the test set are 96.17% and 95.64%, respectively. Then, we use the binary classification model to classify 333,534 nonFGK type spectra in the low-resolution spectra of LAMOST DR8 and obtain a catalog of 3,266 hot subdwarf candidates, of which 1223 are newly-determined. Subsequently, the four-class classification model further filtered the 3,266 candidates, 409 and 296 are newly-determined respectively when the thresholds were set at 0.5 and 0.9. Through manual inspection, The true number of hot subdwarfs in the three newly-determined canditates are 176, 63, and 41, the corresponding precision of the classification model in the three cases are 67.94%, 84.88%, and 87.60%, respectively. Finally, we train a Se-ResNet regression model with MAE values of 1212.65 K for Teff, 0.32 dex for log g and 0.24 for [He/H], and predict the atmospheric parameters of these 176 hot subdwarf stars. This provides a certain amount of samples to help for future studies of hot subdwarfs.

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