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    Journals >Spectroscopy and Spectral Analysis >Volume 32 >Issue 9 >Page 2583 > Article
    • Spectroscopy and Spectral Analysis
    • Vol. 32, Issue 9, 2583 (2012)
    Automatic Measurement of Physical Parameters of Stellar Spectra Based on the Haar Wavelet Features
    LU Yu1,*, LI Chen-lai2, and LI Xiang-ru1
    Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
    • show less
    DOI: 10.3964/j.issn.1000-0593(2012)09-2583-04 Cite this Article
    LU Yu, LI Chen-lai, LI Xiang-ru. Automatic Measurement of Physical Parameters of Stellar Spectra Based on the Haar Wavelet Features[J]. Spectroscopy and Spectral Analysis, 2012, 32(9): 2583 Copy Citation Text show less
    References

    [1] Cheng Li, et al. The Astronomical Journal, 2005, 129(2): 669.

    [2] Re Fiorentin P, et al. Astronomy & Astrophysics, 2007, 467(3): 1373.

    [3] Zhang Jifu, JIANG Yiyong, et al. Pattern Recognition Letters, 2009, 30(15): 1434.

    [4] Re Fiorentin, et al. Astrophysics, 2008, 254: 101.

    [5] Bailer-Jones C A L, Irwin Mike, von Hippel Ted. Monthly Notices of the Royal Astronomical Society, 1998, 298(2): 361.

    [6] Storrie-Lombardi M C, Irwin M J, von Hippel T, et al. Vistas in Astronomy, 1994, 38(3): 331.

    [7] Timothy C Beers, Silvia Rossi. The Astronomical Journal. 1999, 117(2): 4729.

    [8] Fuentes O, Gulati R K. Revista Mexicana de Astronomia Astrofisica (Serie de Conferencias). 2001, 209.

    [10] Zhang Jiannan, et al. Chinese Astronomy and Astrophysics, 2006, 30: 176.

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    LU Yu, LI Chen-lai, LI Xiang-ru. Automatic Measurement of Physical Parameters of Stellar Spectra Based on the Haar Wavelet Features[J]. Spectroscopy and Spectral Analysis, 2012, 32(9): 2583
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