Presentation + Paper
29 August 2022 The GMT telescope metrology system design
Breann N. Sitarski, Andrew Rakich, Hugo Chiquito, Wylie Rosenthal, Antonin H. Bouchez, William Schoenell, Bo Xin, Priscila Pires, Joel Nissen, P. Schurter, Richard T. Demers, Peter Thompson, Brian McLeod, Bijan Nemati, Glenn Brossus, Brian Walls, Heejoo Choi, Guillermo Gonzalez, David Nemati
Author Affiliations +
Abstract
The Giant Magellan Telescope will be a 25.4-m visible and infrared telescope at Las Campanas Observatory. The optical design consists of 7 8.4-m primary mirror segments that reflect light to 7 secondary mirror segments in a doubly segmented direct Gregorian configuration. GMT is developing a Telescope Metrology System (TMS) to decrease the complexity of alignment and increase observatory efficiency. The TMS has been developed to Preliminary Design Review level. A prototyping, modelling, and analysis effort has been completed. All components of the system were matured, and the edge-sensing strategy was significantly revised. This paper describes the current TMS design.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Breann N. Sitarski, Andrew Rakich, Hugo Chiquito, Wylie Rosenthal, Antonin H. Bouchez, William Schoenell, Bo Xin, Priscila Pires, Joel Nissen, P. Schurter, Richard T. Demers, Peter Thompson, Brian McLeod, Bijan Nemati, Glenn Brossus, Brian Walls, Heejoo Choi, Guillermo Gonzalez, and David Nemati "The GMT telescope metrology system design", Proc. SPIE 12182, Ground-based and Airborne Telescopes IX, 1218207 (29 August 2022); https://doi.org/10.1117/12.2630598
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KEYWORDS
Mirrors

Retroreflectors

Sensors

Telescopes

Error analysis

Collimators

Prototyping

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