• Spectroscopy and Spectral Analysis
  • Vol. 32, Issue 8, 2260 (2012)
PAN Jing-chang1、*, WANG Xing-xing1, WEI Peng2, JIANG Bin1、2, TU Liang-ping2、3, and LUO A-li1、2
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
  • 3[in Chinese]
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    DOI: 10.3964/j.issn.1000-0593(2012)08-2260-04 Cite this Article
    PAN Jing-chang, WANG Xing-xing, WEI Peng, JIANG Bin, TU Liang-ping, LUO A-li. An Automated Method to Fit Stellar Continuum Based on Statistic Windows[J]. Spectroscopy and Spectral Analysis, 2012, 32(8): 2260 Copy Citation Text show less
    References

    [1] Su D, Cui X, Wang Y, et al. SPIE, 1998, 3352: 76.

    [2] Newberg H J, Bai Z, Beers T, et al. AAS, 2012, 219.

    [3] Zhao G, Chen Y Q, Shi J R, et al. Chinese Journal of Astronomy and Astrophysics, 2006, 6: 265.

    [4] Gulati R K, Gupta R, Gothoskar P, et al. Bulletin of the Astronomical Society of India, 1996, 24: 21.

    [5] Soubiran C, Katz D, Cayrel R. Arxiv Preprint Astro-ph/9806234, 1998.

    [6] Luo A L, Yongheng Z. Chinese Journal of Astronomy and Astrophysics, 2000, 2(4): 427.

    [7] Lee Y S, Beers T C, Sivarani T, et al. The Astronomical Journal, 2008, 136: 2022.

    PAN Jing-chang, WANG Xing-xing, WEI Peng, JIANG Bin, TU Liang-ping, LUO A-li. An Automated Method to Fit Stellar Continuum Based on Statistic Windows[J]. Spectroscopy and Spectral Analysis, 2012, 32(8): 2260
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