[1] Jiang Wenhan. Adaptive optical technology[J]. Chinese Journal of Nature, 2006, 28(1): 7–13.
[2] Thompson L. Adaptive optics for astronomical telescopes, by John W. Hardy adaptive optics in astronomy, by Fran ois Roddier[J]. Physics Today, 2000, 53(4): 69.
[3] Schipani P, Noethe L, Magrin D, et al. Active optics system of the VLT survey telescope[J]. Applied Optics, 2016, 55(7): 1573–1583.
[4] Schipani P, D'Orsi S, Ferragina L, et al. Active optics primary mirror support system for the 2.6 m VST telescope[J]. Applied Optics, 2010, 49(8): 1234–1241.
[5] Wang Jin, Xian Hao, Wang Shengqian, et al. Effects of piston, tip-tilt and gap errors on image quality of the segmented tel-escope[J]. Opto-Electronic Engineering, 2014, 41(10): 55–62.
[6] Liao Zhou, Qiu Qi, Zhang Yudong. The far-field characteristics for large aperture segmented telescope system[J]. Opto-Electronic Engineering, 2015, 42(2): 1–8.
[7] Lu Changming, Rao Changhui, Huang Huiming, et al. Simu-lation of an astronomical adaptive optics imaging telescope[J]. Opto-Electronic Engineering, 2006, 33(1): 20–23.
[8] Baiocchi D. Design and control of lightweight, active space mirror[D]. Arizona: The University of Arizona, 2004: 22–32.
[9] Yellowhair J E. Advanced technologies for fabrication and testing of large flat mirrors[D]. Arizona: The University of Ari-zona, 2007: 27–34.
[10] Martin H M, Davison W B, DeRigne S T, et al. Active supports and force optimization for a 3.5 m honeycomb sandwich mir-ror[J]. Proceedings of SPIE, 1994, 2199: 251–262.
[11] Gray P M, Hill J M, Davison W B, et al. Support of large boro-silicate honeycomb mirrors[J]. Proceedings of SPIE, 1994, 2199: 691–702.