Spectroscopy and Spectral Analysis, Volume. 31, Issue 9, 2582(2011)

Galaxy/Quasar Classification Based on Nearest Neighbor Method

LI Xiang-ru1、*, LU Yu1, ZHOU Jian-ming2, and WANG Yong-jun1
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
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    References(7)

    [1] [1] Kent S M. Astrophysics and Space Science, 1994, 217(1-2): 27.

    [2] [2] Shanks T, Boyle B J, Croom S M, et al. ESO Astrophysics Symposia: Mining the Sky. Berlin: Springer, 2001. 143.

    [3] [3] Ramsey L W, Sebring T A, Sneden C A. Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. Hawaii: Society of Photo-Optical, 1994. 31.

    [6] [6] Li Xiangru, Hu Zhanyi, Zhao Yongheng, et al. Chinese Astronomy and Astrophysics, 2008, 32(1): 13.

    [8] [8] Li Xiangru, Hu Zhanyi. International Journal of Computer Vision, 2010, 89(1): 1.

    [9] [9] Boiman O, Shechtman E, Irani M. IEEE Conference on Computer Vision and Pattern Recognition, 2008. 1.

    [11] [11] Abazajian K N, Adelman-McCarthy J K, Agüeros M A, et al. The Astrophysical Journal Supplement, 2009, 182(2): 543.

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    LI Xiang-ru, LU Yu, ZHOU Jian-ming, WANG Yong-jun. Galaxy/Quasar Classification Based on Nearest Neighbor Method[J]. Spectroscopy and Spectral Analysis, 2011, 31(9): 2582

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    Paper Information

    Category: Research Articles

    Received: Nov. 19, 2010

    Accepted: --

    Published Online: Nov. 9, 2011

    The Author Email: LI Xiang-ru (xiangru.li@gmail.com)

    DOI:10.3964/j.issn.1000-0593(2011)09-2582-04

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