[1] [1] NASA Webb Telescope Team. Aligning the Primary Mirr Segments of NASA’s James Webb Space Telescope with Light. [EBOL]. (20170920)[20240401]. https:www.nasa.govuniversealigningtheprimarymirrsegmentsofnasasjameswebbspacetelescopewithlight.

[3] [3] STROM S E, STEPP L M, GREGY B. Giant Segmented Mirr Telescope: A Point Design Based on Science Drivers[C]Future Giant Telescopes, August 2228, 2002, Hawaii, United States. SPIE, 2003: 116128.

[4] G ROUSSET, L M MUGNIER, F CASSAING et al. Imaging with Multi-aperture Optical Telescopes and an Application. Comptes Rendus de l’Académie des Sciences-Series IV-Physics, 2, 17-25(2001).

[6] [6] National Aeronautics Space Administration, Jet Propulsion Labaty. Keck Interferometer[EBOL]. (20030226)[20240401]. https:www.jpl.nasa.govimagespia04493keckinterferometer.

[7] [7] COLAVITA M M, WIZINOWICH P L, AKESON R L. Keck Interferometer Status Plans[C]New Frontiers in Stellar Interferometry pt.1, June 2125, 2004, Glasgow, United Kingdom. SPIE, 2004: 454463.

[8] P L WIZINOWICH, Mignant D LE, A H BOUCHEZ et al. The WM Keck Observatory Laser Guide Star Adaptive Optics System: Overview. Publications of the Astronomical Society of the Pacific, 118, 27-29(2006).

[9] [9] AVICOLA K, WATSON J A, BEEMAN B V, et al. Design Perfmance of the Tiptilt Subsystem f the Keck II Telescope Adaptive Optics System[J].Proceedings of SPIE The International Society f Optical Engineering, 1998,3353: 628637.

[10] J D DOWNIE, J W GOODMAN. Optimal Wavefront Control for Adaptive Segmented Mirrors. Applied Optics, 28, 5326-5332(1989).

[11] [11] TYSON R K, FRAZIER B W. Principles of Adaptive Optics[M]. Boca, Raton: CRC Press, 2022.

[12] S MARTIN, A BOOTH, K LIEWER et al. High Performance Testbed for Four-beam Infrared Interferometric Nulling and Exoplanet Detection. Applied Optics, 51, 3907-3921(2012).

[13] [13] National Aeronautics Space Administration. NASA’s Webb Reaches Alignment Milestone, Optics Wking Successfully [EBOL]. (20220316)[20240401]. https:www.nasa.govpressreleasenasaswebbreachesalignmentmilestoneopticswkingsuccessfully.

[14] [14] HIPPLER S. Adaptive Optics f Extremely Large Telescopes[J]. Journal of Astronomical Instrumentation, 2019, 8(2): 19500011195000121.

[15] [15] JOHNS M, MCCARTHY P, RAYBOULD K, et al. Giant Magellan Telescope: Overview[J]. Proceedings of SPIE The International Society f Optical Engineering, 2012, 8444: 526541.

[16] [16] RYAN K. Giant Magellan Telescope’s Final Mirr Fabrication Begins [EBOL]. (20230926)[20240401]. https:giantmagellan.g20230926thegiantmagellantelescopesfinalmirrfabricationbegins.

[17] [17] National Astronomical Observaty of Japan. The Segment Hling System (SHS) Its Precision Robotic H, Which Traverses under the Bridge[EBOL]. (20170206)[20240401]. https:www.tmt.gimage22.

[20] [20] CHUNG S J, MILLER D W, DE W O L. Design Implementation of Sparseaperture Imaging Systems[C]Highly Innovative Space Telescope Concepts, August 2228, 2002, Hawaii, United States. SPIE, 2002: 181192.

[21] R L KENDRICK, J N AUBRUN, R BELL et al. Wide-field Fizeau Imaging Telescope: Experimental Results. Applied Optics, 45, 4235-4240(2006).

[22] Zhaoyuan TONG, Meng LI, Chengbo CUI. et al. Design and Analysis of the Configuration of Deployable Membrane Sunshield. Chinese Space Science and Technology, 41, 82-88(2021).

[23] S P QUANZ, M OTTIGER, E FONTANET et al. Large Interferometer For Exoplanets (LIFE)-I Improved Exoplanet Detection Yield Estimates for a Large Mid-infrared Space-interferometer Mission. Astronomy & Astrophysics, 664, 1-22(2022).

[24] M SCHÖLLER. The Very Large Telescope Interferometer: Current Facility and Prospects. New Astronomy Reviews, 51, 628-638(2007).

[25] A GLINDEMANN, B BAUVIR, F DELPLANCKE et al. Light at the End of the Tunnel-first Fringes with the VLTI. The Messenger, 104, 2-5(2001).

[26] [26] GLINDEMANN A, ABUTER R, CARBOGNANI F, et al. The VLT Interferometer: A Unique Instrument f Highresolution Astronomy[C]Interferometry in Optical Astronomy, March 27April 1, 2000, Munich, Germany. SPIE, 2000: 212.

[27] [27] HAGUENAUER P, ALONSO J, BOURGET P, et al. The Very Large Telescope Interferometer: 2010 Edition[C]2010 Optical Infrared Interferometry II conference, June 27July 2, 2010, San Diego, Califnia, United States. SPIE, 2010: 5363.

[28] [28] MARTINOD M A,BERIO P, MOURARD D, et al. Long Baseline Interferometry in the Visible: The FRIEND Project[C]SPIE Conference on Optical Infrared Interferometry Imaging , June 2227, 2014, Quebec, Canada.SPIE, 2014: 347357.

[29] [29] LYNCH C N, PEREZ M R, KAMISATO P, et al. The Impact of the NASA – Keck Observaty Partnership[R]. Washington: National Aeronautics Space Administration, 2023: 138.

[30] L KALTENEGGER, M FRIDLUND. The Darwin Mission: Search for Extra-solar Planets. Advances in Space Research, 36, 1114-1122(2005).

[31] [31] LAWSON P R, LAY O P, JOHNSTON K J, et al. Terrestrial Pla Finder Interferometer Science Wking Group Rept[R]. Pasadena, CA: Jet Propulsion Labaty, 2007: 1217.

[32] [32] IREL M J. Longbaseline Space Interferometry f Astrophysics: A Fward Look at Scientific Potential Remaining Technical Challenges[C]SPIE Conference on Optical Infrared Interferometry Imaging VII, December 1418, 2020, Online Only. SPIE, 2020: 329337.

[33] T ITO. Formation-flying Interferometry in Geocentric Orbits. Astronomy & Astrophysics, 682, 1-18(2024).

[34] [34] LAWSON P R, LAY O P, JOHNSTON K J, et al. Terrestrial Pla Finder Interferometer (TPFI): Whitepaper f the AAAC Exopla Task Fce[R]. Pasadena, Califnia: Jet Propulsion Labaty, National Aeronautics Space Administration, 2007: 46.

[35] G LUND, H BONNET. DARWIN–The Infrared Space Interferometer. Comptes Rendus de l'Académie des Sciences-Series IV-Physics, 2, 137-148(2001).

[36] [36] UNWIN S C, BEICHMAN C A. Terrestrial Pla Finder: Science Overview[C]SPIE Astronomical Telescopes + Instrumentation, June 2125, 2004, Glasgow, United Kingdom. SPIE, 2004: 12161225.