中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Non-parameter estimation algorithm to determine stellar effective temperature

文献类型:期刊论文

作者Zhang, JN; Wu, FC; Luo, AL; Zhao, YH
刊名SPECTROSCOPY AND SPECTRAL ANALYSIS
出版日期2005-12-01
卷号25期号:12页码:2088-2091
关键词stellar spectrum effective temperature of star non-parameter estimation PCA
英文摘要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.
WOS标题词Science & Technology ; Technology
类目[WOS]Spectroscopy
研究领域[WOS]Spectroscopy
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记录号WOS:000234388500047
公开日期2015-12-24
源URL[http://ir.ia.ac.cn/handle/173211/9189]  
专题自动化研究所_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.

入库方式: OAI收割

来源:自动化研究所

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