Knowledge Commons of Institute of Automation,CAS
Non-parameter estimation algorithm to determine stellar effective temperature | |
Zhang, JN; Wu, FC; Luo, AL; Zhao, YH | |
发表期刊 | SPECTROSCOPY AND SPECTRAL ANALYSIS |
2005-12-01 | |
卷号 | 25期号:12页码:2088-2091 |
文章类型 | Article |
摘要 | The effective temperature of a star is one of the most important parameters, which determine the continuum and spectral lines in the stellar spectrum. A non-parameter estimation algorithm is proposed to estimate the stellar effective temperature in the present paper. Firstly, the spectrum data is processed by principal component analysis(PCA), then, an estimating model based on a Gaussian kernel function is set up using the PCA data and their temperatures. Experiments were carried out to verify the efficiency, and numerical robustness of the algorithm is also tested. |
关键词 | Stellar Spectrum Effective Temperature Of Star Non-parameter Estimation Pca |
WOS标题词 | Science & Technology ; Technology |
关键词[WOS] | ELODIE ECHELLE SPECTRA ; T-EFF ; LOG G ; ONLINE DETERMINATION ; LIBRARY ; FE/H |
收录类别 | SCI |
语种 | 英语 |
WOS研究方向 | Spectroscopy |
WOS类目 | Spectroscopy |
WOS记录号 | WOS:000234388500047 |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ia.ac.cn/handle/173211/9189 |
专题 | 09年以前成果 |
作者单位 | 1.Chinese Acad Sci, Inst Automat, Natl Lab Pattern Recognit, Beijing 100080, Peoples R China 2.Chinese Acad Sci, Natl Astron Obser, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Zhang, JN,Wu, FC,Luo, AL,et al. Non-parameter estimation algorithm to determine stellar effective temperature[J]. SPECTROSCOPY AND SPECTRAL ANALYSIS,2005,25(12):2088-2091. |
APA | Zhang, JN,Wu, FC,Luo, AL,&Zhao, YH.(2005).Non-parameter estimation algorithm to determine stellar effective temperature.SPECTROSCOPY AND SPECTRAL ANALYSIS,25(12),2088-2091. |
MLA | Zhang, JN,et al."Non-parameter estimation algorithm to determine stellar effective temperature".SPECTROSCOPY AND SPECTRAL ANALYSIS 25.12(2005):2088-2091. |
条目包含的文件 | 条目无相关文件。 |
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