[1] D NEILL, G ANGELI, C CLAVER et al. Overview of the LSST Active Optics System, 9150(2014).

[2] [2] 2郭宁馨， 张景旭， 刘昌华， 等. 大口径大视场望远镜探测器平面度检测方法综述［J］. 激光与红外， 2020， 50（4）387-395. doi: 10.3969/j.issn.1001-5078.2020.04.001GUON X， ZHANGJ X， LIUC H， et al. Overview of CCDs flatness test method for large aperture and wide-field telescope［J］. Laser & Infrared， 2020， 50（4）387-395（in Chinese）. doi: 10.3969/j.issn.1001-5078.2020.04.001

[3] Q AN, X WU, X LIN et al. Large survey camera collimation and alignment at the observation site by curvature sensing. Optik, 242, 167273(2021).

[4] Q AN, X WU, X LIN et al. Alignment of DECam-like large survey telescope for real-time active optics and error analysis. Optics Communications, 484, 126685(2021).

[5] A ROODMAN, K REIL, C DAVIS. Wavefront Sensing and the Active Optics System of the Dark Energy Camera, 421-438(2014).

[6] [6] 6安其昌， 姜晰文， 李洪文， 等. 基于差分传递函数法的大口径平面镜检测［J］. 中国光学（中英文）， 2022（5）： 992-999. doi: 10.37188/co.2022-0122ANQ C， JIANGX W， LIH W， et al. Detection of large aperture flat mirror based on the differential optics transfer function method［J］. Chinese Optics， 2022（5）： 992-999.（in Chinese）. doi: 10.37188/co.2022-0122

[7] [7] 7姜晰文， 赵金宇， 吕天宇， 等. 大口径主焦点式光学系统的设计与装调［J］. 光学 精密工程， 2022， 30（23）： 2987-2994. doi: 10.37188/ope.20223023.2987JIANGX W， ZHAOJ Y， LÜT Y， et al. Design and alignment of large-aperture prime focus optical system［J］. Opt. Precision Eng.， 2022， 30（23）： 2987-2994.（in Chinese）. doi: 10.37188/ope.20223023.2987

[8] K K WESTORT. Design and Fabrication of High Performance Relay Lenses, 40-49(1985).

[9] P LANGEHANENBERG, E DUMITRESCU, J HEINISCH et al. Automated Measurement of Centering Errors and Relative Surface Distances for the Optimized Assembly of Micro-Optics, 91-98(2011).

[10] P LANGEHANENBERG, A RUPRECHT et al. Highly Accurate Measurement of Lens Surface Distances Within Optical Assemblies for Quality Testing, 116-123(2013).

[11] W RAINER, C ALAIN, G FABRICE. A novel low coherence fibre optic interferometer for position and thickness measurements with unattained accuracy. Optical Sensing II, 6189(2006).

[12] W Q ZHAO, R D SUN, L R QIU et al. Lenses axial space ray tracing measurement. Optics Express, 18, 3608(2010).

[13] [13] 13黄郑重， 曹良才. 面向高通量的多通道复用数字全息成像技术［J］. 中国光学（中英文）， 2022（6）： 1182-1193. doi: 10.37188/co.2022-0070HUANGZH ZH， CAOL C. Multi-channel multiplexing digital holographic imaging for high throughput［J］. Chinese Optics， 2022（6）： 1182-1193.（in Chinese）. doi: 10.37188/co.2022-0070

[14] C HILWEG, D SHADMANY et al. Limits and prospects for long-baseline optical fiber interferometry. Optica, 9, 1238(2022).

[15] M A MARTINOD, D MOURARD, P BÉRIO et al. Fibered visible interferometry and adaptive optics： friend at CHARA. Astronomy & Astrophysics, 618(2018).

[16] G PERRIN, J WOILLEZ, O LAI et al. Interferometric coupling of the keck telescopes with single-mode fibers. Science, 311, 194(2006).

[17] M M COLAVITA, P L WIZINOWICH, R L AKESON et al. The keck interferometer. Publications of the Astronomical Society of the Pacific, 125, 1226-1264(2013).

[18] F GONTÉ, J WOILLEZ, N SCHUHLER et al. VLT Interferometer Upgrade for the 2nd Generation of Interferometric Instruments, 9907, 528-538(2016).