G. Lee, Yunjong Kim, Daewook Kim, Woowon Byun, Changsu Choi, Yongseok Lee, Dohoon Kim, Seunghyuk Chang, J. Ko
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引用次数: 0
摘要
我们开发了KASI-Deep Rolling Imaging Fast Telescope (K-DRIFT),采用300 mm口径离轴自由三镜设计,用于探测微弱和漫射低表面亮度结构。通过对K-DRIFT进行天空测试观测和一系列模拟来分析其性能,我们确定了导致光学性能下降的三个主要误差源。基于性能分析结果,K-DRIFT通过对中低频波前误差进行校正,成功地提高了成像性能。本文介绍了K-DRIFT的光学性能分析算法和光学性能改进。
Low-to-mid spatial frequency wavefront error control for off-axis freeform three-mirror KASI-deep rolling imaging fast telescope
We have developed the KASI-Deep Rolling Imaging Fast Telescope (K-DRIFT), adopting a 300 mm aperture off-axis freeform three-mirror design to detect faint and diffuse low-surface-brightness structures. By conducting the on-sky test observations and performing a series of simulations to analyze the performance of the K-DRIFT, we confirmed three main error sources causing optical performance degradation. The imaging performance of the K-DRIFT has successfully improved by correcting low-to-mid spatial frequency wavefront errors based on performance analysis results. This paper presents the K-DRIFT’s optical performance analysis algorithm and the optical performance improvement.