巨型麦哲伦望远镜
參考資料

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1 2 3  Hutchins, Shana K. . Texas A&M Today. September 18, 2015  [2015-12-17]. （原始内容存档于2017-10-04）. There is special significance to the fourth mirror.  It will be the central unit. Without it, the other mirrors would be much more difficult to bring together to function as a single telescope. Also, our baseline plan starts the operations of the GMT with just these four mirrors, which will all have been cast once this one is complete.
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↑  Ketelsen, Dean, , 2012-01-15  [2012-04-08], （原始内容存档于2016-06-10）, While guests toured the facilities, the Lab staff ran both of our polishing machines on current projects, including this view of final polishing on the first GMT segment.
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 (PDF). . February 2006. p. 7-17 § 7.4.5  [2007-10-07]. （原始内容存档于2012-03-28）. The center segment and cell will not have a spare, thus observations will be interrupted every one or two years for the 1–2 week period required to recoat that mirror.
↑  
 (PDF), , p. 2-4 § 2.5.1, 2006  [2012-03-25], （原始内容存档于2012-03-28）, GMT is designed from the outset around adaptive optics (AO) with the goal of producing diffraction limited images at 1 μm and longer wavelengths.
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↑  . www.gmto.org. January 11, 2018  [2018-01-25]. （原始内容存档于2019-12-02） （美国英语）.
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↑  Martina, H. M.; Burgea, J. H.; Davisa, J. M.; Kimb, D. W.; Kingsleya, J. S.; Lawa, K.; Loeffa, A.; Lutza, R. D.; Merrilla, C.; Strittmattera, P. A.; Tuella, M. T.; Weinbergera, S. N.; Westa, S. C. Navarro, Ramón; Burge, James H. , 编. . SPIE Astronomical Telescopes + Instrumentation. Proc. SPIE 9912 (Edinburgh). 22 July 2016: 99120V. doi:10.1117/12.2234491. （原始内容存档 (PDF)于2016-12-20） 使用|archiveurl=需要含有|url= (帮助).  参数|journal=与模板{{cite conference}}不匹配（建议改用{{cite journal}}或|book-title=） (帮助); |contribution=被忽略 (帮助); 使用|accessdate=需要含有|url= (帮助)
↑  . GMT Newsletter, December 2017.   [2019-03-20]. （原始内容存档于2021-03-06）.