Feature Extraction and Analysis of Double-Peaked Emission Line Spectra Based on Relevant Subspace

QU Cai-xia; YANG Hai-feng; CAI Jiang-hui; LUO A-li; ZHANG Ji-fu; NIE Yao-yao

doi:10.3964/j.issn.1000-0593(2019)06-1677-06

[1] Luo A L, Zhao Y H, Zhao G, et al. Research in Astronomy and Astrophysics, 2015, 15(8): 1095.

[2] Liu X W, Zhao G, Hou J L. Research in Astronomy and Astrophysics, 2015, 15(8): 1089.

[3] Wang M X, Luo A L, Song Y H, et al. Monthly Notices of the Royal Astronomical Society, 2018, 482(2): 1889.

[4] Liu J, Eracleous M, Halpern J P. The Astrophysical Journal, 2016, 817(1): 42.

[5] Kharb P, Das M, Subramanian S, et al. arXiv preprint arXiv, 2015, 1508: 07429.

[6] Das M, Kharb P, Honey M. Monthly Notices of the Royal Astronomical Society, 2017, 465(4): 4772.

[7] Yang H. A Study of Superimposed Components Recognition and Analysis on LAMOST Extragalactic Spectra, 2017.

[8] Eracleous M, Lewis K T, Halpern J P, et al. The Ultraviolet Spectra of Active Galaxies with Double-Peaked Balmer Emission Lines. American Astronomical Society Meeting Abstracts. 2015, 225.

[10] Comerford J M, Nevin R, Stemo A, et al. The Astrophysical Journal, 2018, 867(1): 66.

[11] Shi Z X, Luo A L, Comte G, et al. Research in Astronomy and Astrophysics, 2014, 14(10): 1234.

[12] Zhang L, Lin J, Karim R. Reliability Engineering & System Safety, 2015, 142: 482.

[13] Zhang J, Yu X, Li Y, et al. Knowledge-Based Systems, 2016, 99: 1.

[14] Piao M, Shon H S, Lee J Y, et al. IEEE Transactions on Power Systems, 2014, 29(6): 2628.