Galaxy/Quasar Classification Based on Nearest Neighbor Method

LI Xiang-ru; LU Yu; ZHOU Jian-ming; WANG Yong-jun

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

Journals >Spectroscopy and Spectral Analysis >Volume 31 >Issue 9 >Page 2582 > Article

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

Galaxy/Quasar Classification Based on Nearest Neighbor Method

LI Xiang-ru^1、*, LU Yu¹, ZHOU Jian-ming², and WANG Yong-jun¹

Author Affiliations

¹[in Chinese]

²[in Chinese]

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

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 Copy Citation Text

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References

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

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

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

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

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

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

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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