A Novel Method to Determine the Redshifts of Active Galaxies Based on Wavelet Transform
文献类型：期刊论文
| 作者 | Tu Liang-ping1,2; Luo A-li1 ; Jiang Bin1,3; We Peng1; Zhao Yong-heng1; Liu Rong4
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| 刊名 | SPECTROSCOPY AND SPECTRAL ANALYSIS
 |
| 出版日期 | 2012-10-01 |
| 卷号 | 32期号:10页码:2858-2862 |
| 关键词 | Active galaxy Redshift determination Wavelet transform Parzen window estimation |
| 英文摘要 | Automatically determining redshifts of galaxies is very important for astronomical research on large samples, such as large-scale structure of cosmological significance. Galaxies are generally divided into normal galaxies and active galaxies, and the spectra of active galaxies mostly have more obvious emission lines. In the present paper, the authors present a novel method to determine spectral redshifts of active galaxies rapidly based on wavelet transformation mainly, and it does not need to extract line information accurately. This method includes the following steps, Firstly, we denoised a spectrum to be processed; Secondly, the low-frequency spectrum was extracted based on wavelet transform, and then we could get the residual spectrum through the denoised spectrum subtracting the low-frequency spectrum; Thirdly, the authors calculated the standard deviation of the residual spectrum and determined a threshold value T, then retained the wavelength set whose corresponding flux was greater than T; Fourthly, according to the wavelength form of all the standard lines, we calculated all the candidate redshifts; Finally, utilizing the density estimation method based on Parzen window, we determined the redshift point with maximum density, and the average value of its neighborhood would be the final redshift of this spectrum. The experiments on simulated data and real data from SDSS-DR7 show that this method is robust and its correct rate is encouraging. And it can be expected to be applied in the project of LAMOST. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000309798600059 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6089]  |
| 专题 | 国家天文台_光学天文研究部 |
| 作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China 2.Univ Sci & Technol Liaoning, Sch Sci, Anshan 114051, Peoples R China 3.Shandong Univ Weihai, Sch Mech Elect & Informat Engn, Weihai 264209, Peoples R China 4.Beijing Inst Clothing Technol, Base Dept, Beijing 100029, Peoples R China |
| 推荐引用方式 GB/T 7714 | Tu Liang-ping,Luo A-li,Jiang Bin,et al. A Novel Method to Determine the Redshifts of Active Galaxies Based on Wavelet Transform[J]. SPECTROSCOPY AND SPECTRAL ANALYSIS,2012,32(10):2858-2862. |
| APA | Tu Liang-ping,Luo A-li,Jiang Bin,We Peng,Zhao Yong-heng,&Liu Rong.(2012).A Novel Method to Determine the Redshifts of Active Galaxies Based on Wavelet Transform.SPECTROSCOPY AND SPECTRAL ANALYSIS,32(10),2858-2862. |
| MLA | Tu Liang-ping,et al."A Novel Method to Determine the Redshifts of Active Galaxies Based on Wavelet Transform".SPECTROSCOPY AND SPECTRAL ANALYSIS 32.10(2012):2858-2862. |
入库方式： OAI收割
来源：国家天文台
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