[1] Su D Q, Cui X Q, Wang Y N, et al. Large sky area multi-object fiber spectroscopic telescope (LAMOST) and its key technology [J]. Proc SPIE 1998, 76: 3352.
[2] Wang S G, Su D Q. Special configuration of a very large Schmidt telescope for extensive astronomical spectroscopic observation [J]. Appl Opt, 1996, 35: 5155.
[3] Su D Q , Cui X Q . Active optics in LAMOST [J]. Chinese Journal of Astronomy and Astrophysics, 2004, 4(1).
[4] Zhang Y. Research on LAMOST active optics technology . Nanjing: Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, 2005. 张勇. LAMOST主动光学技术研究 .南京:中国科学院南京天文光学技术研究所,2005.
[5] Zhang Y. Experimental research on the sampling point number of LAMOST active optics wavefront test [J]. Proc of SPIE, 2006, 6267:626735-1~12.
[6] Cui X Q, Su D Q, Li GP, et al. Experiment system of LAMOST active optics [J]. Proc of SPIE, 2004, 5489:974-985.
[7] Zhang Y. Progress of LAMOST wavefront sensing //Larry M Stepp, Roberto Gilmozzi, edited. Ground-based and Airborne Telescopes II, Proceedings of SPIE. 7012 (SPIE, Bellingham, WA 2008), 70123H.
[8] Du X X, Zhang Z C, Qi Y J, et al. Control system of position actuators for segmented mirror active optics in LAMOST [J]. Proc of SPIE, 2007, 6721:672106.
[9] 崔坤,张文明,王滨.基于Nios II的UART与PC间的数据通信 [J]. 电子技术, 2007(7/8):124-126.
|