Spectral classification of stars based on LAMOST spectra | |
Liu, Chao1; Cui, Wen-Yuan2; Zhang, Bo1; Wan, Jun-Chen1; Deng, Li-Cai1; Hou, Yong-Hui3; Wang, Yue-Fei3; Yang, Ming1; Zhang, Yong3 | |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
2015-08-01 | |
卷号 | 15期号:8页码:1137-1153 |
关键词 | techniques: spectroscopic stars: general stars: fundamental parameters stars: statistics Galaxy: stellar contents |
英文摘要 | In this work, we select spectra of stars with high signal-to-noise ratio from LAMOST data and map their MK classes to the spectral features. The equivalent widths of prominent spectral lines, which play a similar role as multi-color photometry, form a clean stellar locus well ordered by MK classes. The advantage of the stellar locus in line indices is that it gives a natural and continuous classification of stars consistent with either broadly used MK classes or stellar astrophysical parameters. We also employ an SVM-based classification algorithm to assign MK classes to LAMOST stellar spectra. We find that the completenesses of the classifications are up to 90% for A and G type stars, but they are down to about 50% for OB and K type stars. About 40% of the OB and K type stars are mis-classified as A and G type stars, respectively. This is likely due to the difference in the spectral features between late B type and early A type stars or between late G and early K type stars being very weak. The relatively poor performance of the automatic MK classification with SVM suggests that the direct use of line indices to classify stars is likely a more preferable choice. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000360553400004 |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/5606] |
专题 | 国家天文台_光学天文研究部 |
作者单位 | 1.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China 2.Hebei Normal Univ, Dept Phys, Shijiazhuang 050024, Peoples R China 3.Chinese Acad Sci, Nanjing Inst Astron Opt & Technol, Natl Astron Observ, Nanjing 210042, Jiangsu, Peoples R China |
推荐引用方式 GB/T 7714 | Liu, Chao,Cui, Wen-Yuan,Zhang, Bo,et al. Spectral classification of stars based on LAMOST spectra[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2015,15(8):1137-1153. |
APA | Liu, Chao.,Cui, Wen-Yuan.,Zhang, Bo.,Wan, Jun-Chen.,Deng, Li-Cai.,...&Zhang, Yong.(2015).Spectral classification of stars based on LAMOST spectra.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,15(8),1137-1153. |
MLA | Liu, Chao,et al."Spectral classification of stars based on LAMOST spectra".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 15.8(2015):1137-1153. |
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