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On-sky performances of an optical phasing sensor based on a cylindrical lenslet array for segmented telescopes

机译:基于圆柱形小透镜阵列的分段式光学相位传感器的空中性能

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New optical phasing sensor technologies have been studied with a test bench experiment, called Active Phasing Experiment, on-sky at the European Southern Observatory Very Large Telescope. One of the sensors was of the Shack-Hartmann type using cylindrical lenslets across the segment borders for the measurement of the phasing errors. With bright stars, the precision of the measurement of piston steps at a single border was better than 9 nm wavefront RMS, and the precision of the closed-loop correction of the piston errors of the segments across the whole mirror was better than 10 nm wavefront RMS. With dimmer stars of magnitude up to 14.5, precisions of the order of 22 nm wavefront RMS were obtained.
机译:欧洲南方天文台超大型望远镜正在测试一种名为“主动相位实验”的试验台实验,研究了新的光学相位传感器技术。其中一种传感器是Shack-Hartmann型传感器,使用跨过段边界的圆柱形小透镜来测量相位误差。对于明亮的星星,在单个边界处的活塞阶跃的测量精度优于9 nm波前RMS,并且对整个反射镜上的扇形段的活塞误差进行闭环校正的精度优于10 nm波前。均方根值使用数量级高达14.5的较暗恒星,可以获得22 nm波前RMS的精度。

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