Ground-Based and Airborne Telescopes VIII 2020
DOI: 10.1117/12.2560614
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High precision machining in TMT (Thirty Meter Telescope) structure manufacturing

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Cited by 3 publications
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“…The Thirty Meter Telescope (TMT) is a typical Ritchey–Chrétien optical system, in which all active instruments work on Nasmyth platforms, and is designed to transmit light from 310 to 28,000 nm. However, to relay the optical beams from the secondary mirror to the active instruments of the TMT, the Giant Steerable Science Mirror (GSSM) has been proposed [ 1 , 2 , 3 ]. This is significantly different from other large telescopes, such as GMT, LAMOST [ 4 ], and E-ELT [ 5 ].…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…The Thirty Meter Telescope (TMT) is a typical Ritchey–Chrétien optical system, in which all active instruments work on Nasmyth platforms, and is designed to transmit light from 310 to 28,000 nm. However, to relay the optical beams from the secondary mirror to the active instruments of the TMT, the Giant Steerable Science Mirror (GSSM) has been proposed [ 1 , 2 , 3 ]. This is significantly different from other large telescopes, such as GMT, LAMOST [ 4 ], and E-ELT [ 5 ].…”
Section: Introductionmentioning
confidence: 99%
“…However, a kinematic coupling could effectively reduce the maintenance cycle of the M3CA. Due to the fact that the tertiary mirror is a flat oval mirror with a major diameter of 4 m, the out-of-plane error needs to be strictly controlled, as it has a significant influence on the telescope [ 3 ].…”
Section: Introductionmentioning
confidence: 99%