[1] Chi Dexia, Wang Yang, Ning Liqun, et al. Experimental research of camera calibration based on Zhang’s method [J]. Journal of Chinese Agricultural Mechanization, 2015, 36(2): 287-289, 337. (in Chinese)
[2] Smith K, Acton D S, Gallagher B, et al. Calibration results using highly aberrated images for aligning the JWST instruments to the telescope[C]//Proceedings of SPIE, 2016, 9904: 990442.
[3] N'Diaye M, Dohlen K, Caillat A, et al. Design optimization and lab demonstration of ZELDA: a Zernike sensor for near-coronagraph quasi-static measurements [C]//Proceedings of SPIE-The International Society for Optical Engineering, 2014, 9148: 91485H.
[4] Zhang Ning, Ye Lu, Song Ying. Design and detection for the photoelectric device usedin the point source transmission testing [J]. Chinese Journal of Scientific Instrument, 2018, 39(1): 92-99. (in Chinese)
[5] Codona J L. Differential optical transfer function wavefront sensing [J]. Optical Engineering, 2013, 52(9): 097105. doi:  10.1117/1.OE.52.9.097105
[6] Codona J L. Theory and application of differential OTF (dOTF) wavefront sensing[C]//Proceedings of SPIE-The International Society for Optical Engineering, 2012, 8447: 84476P.
[7] Codona J L, Doble N, Ellerbroek B L, et al. Experimental evaluation of differential OTF (dOTF) wavefront sensing[C]//Proceedings of SPIE-The International Society for Optical Engineering, 2012, 8447: 321-323.
[8] Jiang F Y, Ju G H, Qi X, et al. Cross-iteration deconvolution strategy for differential optical transfer function (dOTF) wavefront sensing [J]. Optics Letters, 2019, 44(17): 4283-4286. doi:  10.1364/OL.44.004283
[9] Knight J M, Rodack A T, Codona J L, et al. Deconvolution of differential OTF (dOTF) to measure high-resolution wavefront structure [C]//Techniques & Instrumentation for Detection of Exoplanets VII. International Society for Optics and Photonics, 2016, 9605: 960529.
[10] Korkiakoski V, Keller C U, Doelman N, et al. High-order wavefront correction with a spatial light modulator: Calibrations with dOTF method [C]//Adaptive Optics: Methods, Analysis and Applications, 2013: OM3A.4.
[11] Rodack A T, Knight J M, Codona J L, et al. Adaptive optics self-calibration using differential OTF (dOTF) [C]//Techniques & Instrumentation for Detection of Exoplanets VII. International Society for Optics and Photonics, 2015, 9605: 96052B.
[12] Hart M, Codona J L. Wavefront sensing with the differential optical transfer function[C]//Proceedings of SPIE-the Inter national Society for Optical Engineering, 2012, 8520: 85200I .
[13] Luo Yuzhuo, Ma Yu, Wang Wenna, et al. Application of environmental monitoring based on BP neural network optimized by FPSO [J]. Foreign Electronic Measurement Technology, 2018, 37(3): 136-142. (in Chinese)
[14] Zhang Dong, Gui Jie, Wang Xiaoling, et al. Phased array ultrasonic detection using equal height focusing algorithm [J]. Journal of Electronic Measurement and Instrumentation, 2018, 32(2): 42-47. (in Chinese)
[15] An Qichang, Zhang Jingxu, Yang Fei, et al. Evaluation of the performance of large telescope based on normalized point source sensitivity [J]. Infrared and Laser Engineering, 2016, 45(12): 1218001. (in Chinese) doi:  10.3788/IRLA201645.1218001
[16] Li Lixing, Huang Yongmei, Wang Qiang, et al. Noise adaptive Kalman filter for video point target tracking [J]. Electronic Measurement Technology, 2017(6): 170-174. (in Chinese) doi:  10.3969/j.issn.1002-7300.2017.06.038
[17] Tibor A, Abrams D C, Infantes D C, et al. Preliminary optical design for the WEAVE two-degree prime focus corrector [C]//Ground-based and Airborne Telescopes IV. International Society for Optics and Photonics, 2012, 8444: 84446J.
[18] Pazder J S, Vogiatzis K, Angeli G Z. Dome and mirror seeing estimates for the thirty meter telescope [C]//Proceedings of SPIE-The International Society for Optical Engineering, 2008, 7017: 70170R.
[19] Yang X F, Han C Y. Novel algorithm for computer-aided alignment of wide field of view complex optical system [J]. Key Engineering Materials, 2007, 364-366: 1066-1071.
[20] Kent S. Preliminary optical design for a 2.2 degree diameter prime focus corrector for the Blanco 4 meter telescope[C]//Proceedings of SPIE-The International Society for Optical Engineering, 2006, 6269: 626937.
[21] Blanco D, Pentland G, Smith C, et al. A prime focus corrector for the Lowell 4m telescope [C]//Conference on Specialized Optical Developments in Astronomy, 2003: 85-94.
[22] Tibor A, Abrams D C, Emilie L, et al. Final optical design for the WEAVE two-degree prime focus corrector [C]//Ground-based and Airborne Instrumentation for Astronomy V. International Society for Optics and Photonics, 2014, 9147: 914773.
[23] Doel P, Abbott T, Antonik M, et al. Design and status of the optical corrector for the DES survey instrument [C]//Ground-based and Airborne Instrumentation for Astronomy II. International Society for Optics and Photonics, 2008, 7014: 70141V.
[24] Poteet W M, Cauthen H K, Kappler N, et al. Design and fabrication of three 1.6-meter telescopes for the Korea Microlensing Telescope Network (KMTNet) [C]//Proceedings of SPIE-The International Society for Optical Engineering, 2012, 8444: 84445S.
[25] Liu Xiangyi, Wang Fuguo, Zhang Jingxu, et al. Study on moment correction method of primary mirror semi-active support [J]. Infrared and Laser Engineering, 2019, 48(5): 0518003. (in Chinese) doi:  10.3788/IRLA201948.0518003