• Spectroscopy and Spectral Analysis
  • Vol. 36, Issue 5, 1521 (2016)
PAN Jing-chang1、*, LUO A-li1、2, WEI Peng2, JIANG Bin1, LI Yin-bi2, and ZHENG Qiang3
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
  • 3[in Chinese]
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    DOI: 10.3964/j.issn.1000-0593(2016)05-1521-05 Cite this Article
    PAN Jing-chang, LUO A-li, WEI Peng, JIANG Bin, LI Yin-bi, ZHENG Qiang. A New Redshift Measuring Method for Low-Quality Galaxy Spectra Based on Multi Resolution Fusion Distance[J]. Spectroscopy and Spectral Analysis, 2016, 36(5): 1521 Copy Citation Text show less
    References

    [1] Cui X Q, Zhao Y H, Chu Y Q, et al. Research in Astronomy and Astrophysics, 2012, 12(9): 1197.

    [2] Zhao G, Zhao Y H, Chu Y Q, et al. Research in Astronomy and Astrophysics, 2012, 12(7): 723.

    [3] Luo A L, Zhang H T, Zhao Y H, et al. Research in Astronomy and Astrophysics, 2012, 12(9): 1243.

    [4] Han J S, Luo A L, Zhao Y H. Publications of the Astronomical Society of Japan, 2011, 63(6): 1313.

    [5] Wang F, Zhang H, Luo A, et al. Science China Physics, Mechanics and Astronomy, 2013, 56(10): 1833.

    [6] Sanchez Almeide J, Aguerri J Al, Munoz-Tunon C, et al. The Astrophysical Journal, 2010, 714(1): 487.

    PAN Jing-chang, LUO A-li, WEI Peng, JIANG Bin, LI Yin-bi, ZHENG Qiang. A New Redshift Measuring Method for Low-Quality Galaxy Spectra Based on Multi Resolution Fusion Distance[J]. Spectroscopy and Spectral Analysis, 2016, 36(5): 1521
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