Wide-field tracking with zenith-pointing telescopes

被引:9
作者
Hickson, P [1 ]
机构
[1] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
关键词
instrumentation : adaptive optics; instrumentation : interferometers; telescopes;
D O I
10.1046/j.1365-8711.2002.05098.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Equipped with a suitable optical relay system, telescopes employing low-cost fixed primary mirrors could point and track while delivering high-quality images to a fixed location. Such an optical tracking system would enable liquid-mirror telescopes to access a large area of sky and employ infrared detectors and adaptive optics. Such telescopes could also form the elements of an array in which light is combined either incoherently or interferometrically. Tracking of an extended field requires correction of all aberrations including distortion, field curvature and tilt. A specific design is developed that allows a 10-m liquid-mirror telescope to track objects for as long as 30 min and to point as far as 4degrees from the zenith, delivering a distortion-free diffraction-limited image to a stationary detector, spectrograph or interferometric beam combiner.
引用
收藏
页码:540 / 546
页数:7
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