Paper
22 July 2014 Baseline design of the LSST telescope mount assembly
Author Affiliations +
Abstract
The Large Synoptic Survey Telescope (LSST) is an 8.4 meter, 3.5 degree, wide-field survey telescope. The survey mission requires a short slew, settling time of 5 seconds for a 3.5 degree slew. Since it does not include a fast steering mirror, the telescope has stringent vibration limitations during observation. Meeting these requirements will be facilitated by a stiff compact Telescope Mount Assembly (TMA) riding on a robust pier and by added damping. The TMA must also be designed to facilitate maintenance. The design is an altitude over azimuth welded and bolted assembly fabricated from mild steel.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Douglas R. Neill, Ed Hileman, Jacques Sebag, William Gressler, Oliver Wiecha, Michael Warner, John Andrew, and Bill Schoening "Baseline design of the LSST telescope mount assembly", Proc. SPIE 9145, Ground-based and Airborne Telescopes V, 914518 (22 July 2014); https://doi.org/10.1117/12.2056432
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Cited by 1 scholarly publication.
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KEYWORDS
Telescopes

Mirrors

Large Synoptic Survey Telescope

Cameras

Optical instrument design

Domes

Capacitors

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