[1] WANG Jian-li, CHEN Tao, ZHANG Jing-xu. General requirements and key technologies for the ground-based high resolution EO imaging telescope［J］. Optics and Precision Engineering, 2008, 16(Special): 1-16.

[2] ZHANG Wei, CAO Yi-ping. A wave-front measuring method for large scale telescope system［J］. High Power Laser and Particle Beams, 2006,18(2): 205-209.

[3] LIN Jing, LIU Zhong, JIN Zhen-yu. High-resolution image reconstruction technology applied to the optical testing of ground-based astronomical telescopes［J］. Astron, T&T-PNAOC, 2004,1(3): 188-195.

[4] WANG Yi-ming, QIN Song-nian. The test of light energy concentration for 1m reflector at Yunnan observation［J］. Acta Astronomica Sinica, 1981, 22(3): 310-314.

[5] ZHOU Wen-chao, PENG Yong, XU Hong-lai. Way to get integrative aberration of large aperture optical system in the outfield［J］. Infrared and Laser Engineering, 2008, 37(sup): 155-157.

[6] MA Pin-zhong. Shack-Hartmann wavefront sensor for 4.3m telescope［J］. Optical Technique, 1994, 20(3): 28-30.

[7] CURATU C, CURATU G, ROLLAND J. Fundamental and specific steps in Shack-Hartmann wavefront sensor design ［C］. SPIE, 2006, 6288: 1-8.

[8] NEAL D R, COPLAND J, NEAL D. Shack-Hartmann wavefront sensor precision and accuracy［C］. SPIE, 2002, 4779: 148-160.

[9] LI Hong-zhuang, LIU Xin-yue, WANG Zhi-chen, et al. Develop of multi-application and modular Hartmann wavefront sensor［J］. Optical Technique, 2011,37(3): 362-365.

[10] WU Jia-jie, CHEN Jia-bi, XU An-cheng, et al. Focal length measurement based on hartmann-shack principle［J］. Acta Photonica Sinica, 2011,40(6): 912-915.