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Large Binocular Telescope Adaptive Optics System: New achievements and perspectives in adaptive optics

机译:大型双目望远镜自适应光学系统:新成果和新技术   自适应光学中的观点

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摘要

The Large Binocular Telescope (LBT) is a unique telescope featuring twoco-mounted optical trains with 8.4m primary mirrors. The telescope AdaptiveOptics (AO) system uses two innovative key components, namely an adaptivesecondary mirror with 672 actuators and a high-order pyramid wave-front sensor.During the on-sky commissioning such a system reached performances neverachieved before on large ground-based optical telescopes. Images with 40masresolution and Strehl Ratios higher than 80% have been acquired in H band (1.6micron). Such images showed a contrast as high as 10e-4. Based on theseresults, we compare the performances offered by a Natural Guide Star (NGS)system upgraded with the state-of-the-art technology and those delivered byexisting Laser Guide Star (LGS) systems. The comparison, in terms of skycoverage and performances, suggests rethinking the current role ascribed to NGSand LGS in the next generation of AO systems for the 8-10 meter classtelescopes and Extremely Large Telescopes (ELTs).
机译:大型双筒望远镜(LBT)是一款独特的望远镜,具有可同时安装8.4m主镜的双向安装光学火车。望远镜AdaptiveOptics(AO)系统使用两个创新的关键组件,即具有672个执行器的自适应辅助反射镜和一个高阶金字塔波阵面传感器,在空中调试期间,该系统在大型地面光学系统上达到了前所未有的性能望远镜。已在H波段(1.6微米)中获得了40像素分辨率和Strehl比率高于80%的图像。这样的图像显示出高达10e-4的对比度。基于这些结果,我们比较了使用最新技术升级的自然导星(NGS)系统提供的性能以及现有激光导星(LGS)系统提供的性能。从天空覆盖和性能方面的比较,建议重新考虑NGS和LGS在8-10米级望远镜和超大型望远镜(ELT)的下一代AO系统中的当前作用。

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