23 June 2006 Edge sensor design for the TMT
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The Thirty Meter Telescope project will design and build a thirty-meter diameter telescope for research in astronomy at optical and infrared wavelengths. The highly segmented primary mirror will use edge sensors to align and stabilize the relative piston, tip, and tilt degrees of freedom of the segments. We describe an edge sensor conceptual design and relate the sensor errors to the performance of the telescope as whole. We discuss the sensor calibration, installation, maintenance, and reliability.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Terry Mast, Terry Mast, Gary Chanan, Gary Chanan, Jerry Nelson, Jerry Nelson, Robert Minor, Robert Minor, Richard Jared, Richard Jared, } "Edge sensor design for the TMT", Proc. SPIE 6267, Ground-based and Airborne Telescopes, 62672S (23 June 2006); doi: 10.1117/12.672028; https://doi.org/10.1117/12.672028


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