The Richard F. Caris Mirror Lab at the University of Arizona is responsible for production of the eight 8.4 m segments for the primary mirror of the Giant Magellan Telescope, including one spare off-axis segment. We report on the successful casting of Segment 4, the center segment. Prior to generating the optical surface of Segment 2, we carried out a major upgrade of our 8.4 m Large Optical Generator. The upgrade includes new hardware and software to improve accuracy, safety, reliability and ease of use. We are currently carrying out an upgrade of our 8.4 m polishing machine that includes improved orbital polishing capabilities. We added and modified several components of the optical tests during the manufacture of Segment 1, and we have continued to improve the systems in preparation for Segments 2-8. We completed two projects that were prior commitments before GMT Segment 2: casting and polishing the combined primary and tertiary mirrors for the LSST, and casting and generating a 6.5 m mirror for the Tokyo Atacama Observatory.
No one sets out to be a mediocre leader. Some teams work well and deliver products that are on time and meet requirements. Through observation of successful and less than successful teams, lessons can be learned that will allow others to get the most out of each other. The lessons can be summed up in a series of sound bites including “One is not done until everyone is done”, BKSS (Because K Said So), and “Trust but Verify” that serve as a reminder of lessons that were hard earned.
Conference Committee Involvement (2)
Optical Modeling and System Alignment
12 August 2019 | San Diego, California, United States
Optical Modeling and Performance Predictions X
22 August 2018 | San Diego, California, United States