中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A Machine Learning Based Morphological Classification of 14,245 Radio AGNs Selected from the Best–Heckman Sample

文献类型:期刊论文

作者Ma,Zhixian1; Xu,Haiguang2,3,7; Zhu,Jie1; Hu,Dan3; Li,Weitian3; Shan,Chenxi3; Zhu,Zhenghao3; Gu,Liyi4; Li,Jinjin5; Liu,Chengze3
刊名The Astrophysical Journal Supplement Series
出版日期2019-02-12
卷号240期号:2
关键词catalogs galaxies: statistics methods: data analysis radio continuum: galaxies techniques: miscellaneous
ISSN号0067-0049
DOI10.3847/1538-4365/aaf9a2
英文摘要Abstract We present a morphological classification of 14,245 radio active galactic nuclei (AGNs) into six types, i.e., typical Fanaroff–Riley Class I/II (FRI/II), FRI/II-like bent-tailed, X-shaped radio galaxy, and ringlike radio galaxy, by designing a convolutional neural network based autoencoder, namely MCRGNet, and applying it to a labeled radio galaxy (LRG) sample containing 1442 AGNs and an unlabeled radio galaxy (unLRG) sample containing 14,245 unlabeled AGNs selected from the Best–Heckman sample. We train MCRGNet and implement the classification task by a three-step strategy, i.e., pre-training, fine-tuning, and classification, which combines both unsupervised and supervised learnings. A four-layer dichotomous tree is designed to classify the radio AGNs, which leads to a significantly better performance than the direct six-type classification. On the LRG sample, our MCRGNet achieves a total precision of ~93% and an averaged sensitivity of ~87%, which are better than those obtained in previous works. On the unLRG sample, whose labels have been human-inspected, the neural network achieves a total precision of ~80%. Also, using Sloan Digital Sky Survey Data Release 7 to calculate the r-band absolute magnitude (Mopt) and using the flux densities to calculate the radio luminosity (Lradio), we find that the distributions of the unLRG sources on the Lradio–Mopt plane do not show an apparent redshift evolution and could confirm with a sufficiently large sample that there could not exist an abrupt separation between FRIs and FRIIs as reported in some previous works.
语种英语
WOS记录号IOP:0067-0049-240-2-AAF9A2
出版者The American Astronomical Society
源URL[http://ir.bao.ac.cn/handle/114a11/35481]  
专题中国科学院国家天文台
作者单位1.Department of Electronic Engineering, Shanghai Jiao Tong University, 800 Dongchuan Road, Minhang, Shanghai 200240, People’s Republic of China mazhixian@sjtu.edu.cn, zhujie@sjtu.edu.cn
2.IFSA Collaborative Innovation Center, Shanghai Jiao Tong University, Minhang, Shanghai 200240, People’s Republic of China
3.Department of Astronomy, Shanghai Jiao Tong University, 800 Dongchuan Road, Minhang, Shanghai 200240, People’s Republic of China
4.SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
5.Key Laboratory of Thin Film and Microfabrication Technology (Ministry of Education), Department of Micro/Nano Electronics, Shanghai Jiao Tong University, Shanghai 200240, People’s Republic of China
6.National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Beijing 100012, People’s Republic of China
7.School of Physics and Astronomy/Tsung-Dao Lee Institute, Shanghai Jiao Tong University, 800 Dongchuan Road, Minhang, Shanghai 200240, People’s Republic of China; hgxu@sjtu.edu.cn
推荐引用方式
GB/T 7714
Ma,Zhixian,Xu,Haiguang,Zhu,Jie,et al. A Machine Learning Based Morphological Classification of 14,245 Radio AGNs Selected from the Best–Heckman Sample[J]. The Astrophysical Journal Supplement Series,2019,240(2).
APA Ma,Zhixian.,Xu,Haiguang.,Zhu,Jie.,Hu,Dan.,Li,Weitian.,...&Wu,Xiangping.(2019).A Machine Learning Based Morphological Classification of 14,245 Radio AGNs Selected from the Best–Heckman Sample.The Astrophysical Journal Supplement Series,240(2).
MLA Ma,Zhixian,et al."A Machine Learning Based Morphological Classification of 14,245 Radio AGNs Selected from the Best–Heckman Sample".The Astrophysical Journal Supplement Series 240.2(2019).

入库方式: OAI收割

来源:国家天文台

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