• Spectroscopy and Spectral Analysis
  • Vol. 32, Issue 10, 2858 (2012)
TU Liang-ping1、2、*, LUO A-li2, JIANG Bin2、3, WEI Peng2, ZHAO Yong-heng2, and LIU Rong4
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
  • 3[in Chinese]
  • 4[in Chinese]
  • show less
    DOI: 10.3964/j.issn.1000-0593(2012)10-2858-05 Cite this Article
    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 Copy Citation Text show less
    References

    [1] Lewis I, Cannon R, Taylor K, et al. Monthly Notices of the Royal Astronomical Society, 2002, 333(2): 279.

    [2] York D G, Adelman J, Anderson J E, et al. The Astronomical Journal, 2000, 120(3): 1579.

    [3] Su Dingqiang, Cui Xiangqun, Wang Yanan, et al. Proc. SPIE, 1998, 3352: 76.

    [4] Tonry J, Davis M. The Astronomical Journal, 1979, 84: 1511.

    [5] Glazebrook K, Offer A R, Deeley K. The Astrophysical Journal, 1998, 492(1): 98.

    [6] Jolliffe I T. Principal Component Analysis, Series: Springer Series in Statistics, 2nd ed., Springer, NY, 2002. 63.

    [9] Donoho D L. Trans. Inform. Theory, 1995, 41(3): 613.

    [10] Abazajian K N, Adelman-McCarthy, Jennifer K, et al. The Astrophysical Journal Supplement, 2009, 182(2): 543.

    [11] Duan Fuqing, Liu Rong, Guo Ping, et al. Research in Astronomy and Astrophysics, 2009, 9(3): 341.

    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
    Download Citation