Spectroscopy and Spectral Analysis, Volume. 32, Issue 10, 2858(2012)
A Novel Method to Determine the Redshifts of Active Galaxies Based on Wavelet Transform
[1] [1] Lewis I, Cannon R, Taylor K, et al. Monthly Notices of the Royal Astronomical Society, 2002, 333(2): 279.
[2] [2] York D G, Adelman J, Anderson J E, et al. The Astronomical Journal, 2000, 120(3): 1579.
[3] [3] Su Dingqiang, Cui Xiangqun, Wang Yanan, et al. Proc. SPIE, 1998, 3352: 76.
[4] [4] Tonry J, Davis M. The Astronomical Journal, 1979, 84: 1511.
[5] [5] Glazebrook K, Offer A R, Deeley K. The Astrophysical Journal, 1998, 492(1): 98.
[6] [6] Jolliffe I T. Principal Component Analysis, Series: Springer Series in Statistics, 2nd ed., Springer, NY, 2002. 63.
[9] [9] Donoho D L. Trans. Inform. Theory, 1995, 41(3): 613.
[10] [10] Abazajian K N, Adelman-McCarthy, Jennifer K, et al. The Astrophysical Journal Supplement, 2009, 182(2): 543.
[11] [11] Duan Fuqing, Liu Rong, Guo Ping, et al. Research in Astronomy and Astrophysics, 2009, 9(3): 341.
Get Citation
Copy Citation Text
TU Liang-ping, LUO A-li, JIANG Bin, WEI Peng, ZHAO Yong-heng, LIU Rong. A Novel Method to Determine the Redshifts of Active Galaxies Based on Wavelet Transform[J]. Spectroscopy and Spectral Analysis, 2012, 32(10): 2858
Received: Mar. 30, 2012
Accepted: --
Published Online: Nov. 22, 2012
The Author Email: Liang-ping TU (tlp_kd@163.com)