[1] Hege E K, Beckers J M, Strittmatter P A et al. Multiple mirror telescope as a phased array telescope[J]. Applied Optics, 24, 2565-2576(1985).

[2] Luo Q, Huang L H, Gu N T et al. Experimental study on phase diversity wavefront sensing technology in piston error detection[J]. Acta Physica Sinica, 61, 069501(2012).

[3] Yan Z J, Chen X Y, Zheng L X et al. Zero co-phasing reference calibration method based on dispersed interferogram for segmented mirror telescope[J]. Acta Physica Sinica, 65, 199501(2016).

[4] Chang J, Zhang Z H, Wang R R. A new sub-aperture stitching method of measuring special optical element[J]. Acta Physica Sinica, 60, 034218(2011).

[5] Chen B, Jie Z Y. Piston error correction method of optical multi-aperture based on image sharpness[J]. Laser & Optoelectronics Progress, 60, 2012001(2023).

[6] Ma H M, Tan L, Zhang J H et al. Review of co-phasing error detection for synthetic aperture imaging system based on deep learning[J]. Chinese Journal of Quantum Electronics, 39, 927-941(2022).

[7] Ma S F, Xian H, Wang S Q. Detection of piston error of synthetic aperture system using pyramid sensor[J]. Laser & Optoelectronics Progress, 60, 1528001(2023).

[8] Wizinowich P L, Chin J, Johansson E et al. Adaptive optics developments at Keck observatory[J]. Proceedings of SPIE, 6272, 627209(2006).

[9] McLean I S, Adkins S. Instrumentation at the Keck observatory[J]. Proceedings of SPIE, 5492, 1-12(2004).

[10] McLean I S, Adkins S M. Instrumentation at the Keck observatory[J]. Proceedings of SPIE, 7014, 701402(2008).

[11] Wizinowich P L, Le Mignant D, Bouchez A et al. Adaptive optics developments at Keck observatory[J]. Proceedings of SPIE, 5490, 1-11(2004).

[12] Adkins S M, Armandroff T E, Fitzgerald M P et al. New developments in instrumentation at the W. M. Keck Observatory[J]. Proceedings of SPIE, 9147, 914703(2014).

[13] Alvarez P, Espinosa J M R, Sánchez F. The Gran Telescopio Canarias (GTC) project[J]. New Astronomy Reviews, 42, 553-556(1998).

[14] Clampin M. Status of the James Webb space telescope (JWST)[J]. Proceedings of SPIE, 7010, 70100L(2008).

[15] Atkinson C, Texter S, Hellekson R et al. Status of the JWST optical telescope element[J]. Proceedings of SPIE, 6265, 62650T(2006).

[16] Acton D S, Towell T, Schwenker J et al. Demonstration of the James Webb Space Telescope commissioning on the JWST testbed telescope[J]. Proceedings of SPIE, 6265, 62650R(2006).

[17] Greenhouse M. The James Webb Space Telescope: mission overview and status[C](2016).

[18] Fu Y, Yuan S, Jin Z Y et al. Active alignment modeling and analysis of Chinese giant solar telescope[J]. Acta Optica Sinica, 42, 1211002(2022).

[19] Zhang W, Deng J, Long F N et al. Image quality evaluation for segmented mirror synthetic aperture optics[J]. Acta Optica Sinica, 28, 687-691(2008).

[20] Chen R L, Zhang T, Ma Z et al. Influences of the alignment errors on image quality of large segmented mirrors[J]. Acta Photonica Sinica, 38, 3240-3244(2009).

[21] Zhang L, Wang X K, Cheng Q et al. Optical co-phasing detection technology of segmented telescopes[J]. Laser & Optoelectronics Progress, 57, 230102(2020).

[22] Wang C C, Zou G Y, Pang Z H et al. Analysis on deployment error of segmented mirror optical system[J]. Acta Optica Sinica, 36, 1122005(2016).

[23] Huo Y L, Yang F, Wang F G. Overview of key technologies for segmented mirrors of large-aperture optical telescopes[J]. Chinese Optics, 15, 973-982(2022).

[24] Zhou R Z, Yan J X, Yu X et al[M]. Adaptive optics, 130-138(1996).

[25] Mazzoleni R, Gonté F, Surdej I et al. Design and performances of the Shack-Hartmann sensor within the Active Phasing Experiment[J]. Proceedings of SPIE, 7012, 70123A(2008).

[26] Mazzoleni R, Yaitskova N, Noethe L. Disentangling between low order telescope aberrations and segmentation errors using a Shack-Hartmann sensor[J]. Proceedings of SPIE, 7012, 701216(2008).

[27] Shen F, Jiang W H. The measurement error of wavefront phase with Shack-Hartmann wavefront sensor[J]. Acta Optica Sinica, 20, 666-671(2000).

[28] Dong R X, Li M, Jin K et al. Research on double star wavefront error detection with Shack-Hartmann wavefront sensor to calculate piston-removed anisoplanatic error[J]. Laser & Optoelectronics Progress, 59, 2101001(2022).

[29] Gonsalves R A. Phase retrieval and diversity in adaptive optics[J]. Optical Engineering, 21, 829-832(1982).

[30] Mugnier L M, Blanc A, Idier J. Phase diversity: a technique for wave-front sensing and for diffraction-limited imaging[J]. Advances in Imaging and Electron Physics, 141, 1-76(2006).

[31] Paxman R G, Fienup J R. Optical misalignment sensing and image reconstruction using phase diversity[J]. Journal of the Optical Society of America A, 5, 914-923(1988).

[32] Acton D S, Knight J S, Contos A et al. Wavefront sensing and controls for the James Webb Space Telescope[J]. Proceedings of SPIE, 8442, 84422H(2012).

[33] Cheetham A C, Tuthill P G, Sivaramakrishnan A et al. Fizeau interferometric cophasing of segmented mirrors[J]. Optics Express, 20, 29457-29471(2012).

[34] Cheetham A, Cvetojevic N, Norris B et al. Fizeau interferometric cophasing of segmented mirrors: experimental validation[J]. Optics Express, 22, 12924-12934(2014).

[35] Deprez M, Bellanger C, Lombard L et al. Piston and tilt interferometry for segmented wavefront sensing[J]. Optics Letters, 41, 1078-1081(2016).

[36] Deprez M, Wattellier B, Bellanger C et al. Phase measurement of a segmented wave front using PISton and TILt interferometry (PISTIL)[J]. Optics Express, 26, 5212-5224(2018).

[37] Rouze B, Primot J, Lanzoni P et al. High-dynamic range segmented mirror metrology by two-wavelength PISTIL interferometry: demonstration and performance[J]. Optics Express, 28, 32415-32425(2020).

[38] Song H L, Jiang W H, Xian H et al. Technology of co-phasing of the segmented mirrors based on a Michelson interferometric system[J]. Chinese Journal of Lasers, 35, 748-751(2008).

[39] Fan J L, Wang J, Wu Q Y et al. Tilt error of Golay3 telescope system[J]. Laser & Optoelectronics Progress, 49, 111102(2012).

[40] Zuo H, Zhang X, Zhang Y. Segmented mirror edge sensors based on equal thickness interference[J]. Acta Optica Sinica, 41, 1212002(2021).

[41] Qin S, Chan W K. A tip-tilt and piston detection approach for segmented telescopes[J]. Photonics, 8, 3(2020).

[42] Zhao W R, Cao G R. Active cophasing and aligning testbed with segmented mirrors[J]. Optics Express, 19, 8670-8683(2011).

[43] Wang S S, Zhu Q D, Cao G R. Cophasing methods of segmented space telescope[J]. Acta Optica Sinica, 29, 2435-2440(2009).

[44] Nella J, Atcheson P D, Atkinson C B et al. James Webb Space Telescope (JWST) observatory architecture and performance[J]. Proceedings of SPIE, 5487, 576-587(2004).