Spectroscopy and Spectral Analysis, Volume. 36, Issue 5, 1521(2016)
A New Redshift Measuring Method for Low-Quality Galaxy Spectra Based on Multi Resolution Fusion Distance
References(6)
[1] [1] Cui X Q, Zhao Y H, Chu Y Q, et al. Research in Astronomy and Astrophysics, 2012, 12(9): 1197.
[2] [2] Zhao G, Zhao Y H, Chu Y Q, et al. Research in Astronomy and Astrophysics, 2012, 12(7): 723.
[3] [3] Luo A L, Zhang H T, Zhao Y H, et al. Research in Astronomy and Astrophysics, 2012, 12(9): 1243.
[4] [4] Han J S, Luo A L, Zhao Y H. Publications of the Astronomical Society of Japan, 2011, 63(6): 1313.
[5] [5] Wang F, Zhang H, Luo A, et al. Science China Physics, Mechanics and Astronomy, 2013, 56(10): 1833.
[6] [6] Sanchez Almeide J, Aguerri J Al, Munoz-Tunon C, et al. The Astrophysical Journal, 2010, 714(1): 487.
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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
Paper Information
Received: Dec. 26, 2014
Accepted: --
Published Online: Dec. 20, 2016
The Author Email: Jing-chang PAN (pjc@sdu.edu.cn)
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