[1] YANG F, LIU G J, ZHAO H CH, et al.. Stiffness allocation and analysis of TMT M3S [J]. Opt. Precision Eng., 2016,24(1): 152-159.(in Chinese)

[2] WANG F G, AN Q CH. Evaluation of mirror surface figures for TMT based on Slope RMS [J].Opt. Precision Eng., 2014,22(5): 1171-1175.(in Chinese)

[3] WANG X K. Measurement of large off-axis convex asphere by systemic stitching testing method [J]. Opt. Precision Eng., 2016,9(1): 130-136.(IN Chinese)

[4] MACMARTIN, D G, THOMPSON P, COLAVITA M M, et al.. Dynamic analysis of the active-controlled segmented mirror of the Thirty Meter Telescope［J］. IEEE Trans. Control Sys. Tech., 2013,22:58-68.

[5] CHEN L S, HU ZH W. The research on the application of normalized point source sensitivity in wide field optical spectrometer of the thirty Meter Telescope [J]. ACTA ASTRONOMICA SINICA, 2016, 57(5):585-596.(in Chinese)

[6] PAZDER J S, VOGIATZIS K, ANGELI G Z. Dome and mirror seeing estimates for the Thirty Meter Telescope［J］. Proc. SPIE 7017, Modeling, Systems Engineering, and Project Management for Astronomy III, 70170R (July 09, 2008).

[7] RUDOLER S, HADAR O, FISHER M, et al.. Image resolution limits resulting from mechanical vibrations [J]. Opt. Eng., 1991, 30(5):577-589.

[8] HADAR O, DROR I, KOPEIKA N S. Image resolution limits resulting from mechanical vibrations. Part IV: real-time numerical calculation of optical transfer functions and experimental verification［J］. Opt. Eng. 1994,33(2): 566-578.

[9] DENG Y T, LI H W, WANG J L, et al.. Large telescope low speed control based on adaptive sliding mode control[J]. Chinese Optics, 2016,9(6): 713-720.(in Chinese)

[10] KOPEIKA N S, WULICH D. Image resolution limits resulting from mechanical vibrations［J］. Journal of Modern Optics, 2008, 55(3):401-407.

[11] YANG F, AN Q CH. Evaluation of mirror seeing based on PSSn [J]. Opt. Precision Eng., 2016, 24(5):979-985.(in Chinese)