Searching for RR Lyrae Stars by Imbalanced Learning
文献类型:期刊论文
作者 | Zhang,Jingyi1,2 |
刊名 | Publications of the Astronomical Society of the Pacific
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出版日期 | 2020-11-17 |
卷号 | 132期号:1018 |
关键词 | Astrostatistics Spectroscopy RR Lyrae variable stars Stellar photometry |
ISSN号 | 0004-6280 |
DOI | 10.1088/1538-3873/abc734 |
英文摘要 | Abstract As standard candles, RR Lyrae stars are taken as distance markers and age indicators, which is helpful to estimate the distance and age of globular clusters as well as galactic and extragalactic (Local Group) locations. At the same time, as tracers, they reveal the structure, chemical and dynamic evolution of the galaxy, as well as the substructure of the halo. However, the number of RR stars is very small compared with other types of stars in nature. With the development and operation of large-scale sky survey projects, they have made a qualitative leap in number. Compared with other types of stars, RR Lyrae stars are still not enough in number. Therefore, separating RR Lyrae stars from stars belongs to an imbalanced learning problem. It may be solved by popular imbalanced learning methods. |
语种 | 英语 |
WOS记录号 | IOP:0004-6280-132-1018-ABC734 |
出版者 | The Astronomical Society of the Pacific |
源URL | [http://ir.bao.ac.cn/handle/114a11/61657] ![]() |
专题 | 中国科学院国家天文台 |
通讯作者 | Zhang,Jingyi |
作者单位 | 1.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China; jyzhang@bao.ac.cn 2.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China |
推荐引用方式 GB/T 7714 | Zhang,Jingyi. Searching for RR Lyrae Stars by Imbalanced Learning[J]. Publications of the Astronomical Society of the Pacific,2020,132(1018). |
APA | Zhang,Jingyi.(2020).Searching for RR Lyrae Stars by Imbalanced Learning.Publications of the Astronomical Society of the Pacific,132(1018). |
MLA | Zhang,Jingyi."Searching for RR Lyrae Stars by Imbalanced Learning".Publications of the Astronomical Society of the Pacific 132.1018(2020). |
入库方式: OAI收割
来源:国家天文台
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