Paper
29 October 1999 Postupgrade performance of the 3.8-m United Kingdom Infrared Telescope (UKIRT)
Author Affiliations +
Abstract
The upgraded 3.8 m UK Infrared Telescope is now provided with: (1) tip-tilt image stabilization by a light-weighted secondary mirror on piezo-electric actuators, controlled by a fast guider sampling at >= 40 Hz on guide stars V m6; (2) active primary mirror figure and secondary mirror alignment control, via a regularly-maintained look-up table; (3) active focus measurements and correction by the fast guider, supplementing a focus maintenance model which corrects for elastic and thermal changes; (4) ventilation of the 2600 m3 dome by 16 apertures totalling 50 m2; (5) insulation of the underside of the concrete dome floor; and (6) internal air circulation during the day, to reduce heating of the upper telescope steelwork.
© (1999) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Timothy G. Hawarden, Nicholas P. Rees, Timothy C. Chuter, Antonio C. Chrysostomou, Charles P. Cavedoni, Ralf-Rainer Rohloff, Eckhart Pitz, Donald G. Pettie, Richard J. Bennett, and Eli Ettedgui-Atad "Postupgrade performance of the 3.8-m United Kingdom Infrared Telescope (UKIRT)", Proc. SPIE 3785, Advanced Telescope Design, Fabrication, and Control, (29 October 1999); https://doi.org/10.1117/12.367622
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Cited by 3 scholarly publications.
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KEYWORDS
Telescopes

Mirrors

Image quality

Fluctuations and noise

Infrared telescopes

Manufacturing

Stars

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