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

机译:大型双筒望远镜自适应光学系统:自适应光学的新成就和新观点

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摘要

The Large Binocular Telescope (LBT) is a unique telescope featuring two co-mounted optical trains with 8.4m primary mirrors. The telescope Adaptive Optics (AO) system uses two innovative key components, namely an adaptive secondary mirror with 672 actuators and a high-order pyramid wave-front sensor. During the on-sky commissioning such a system reached performances never achieved before on large ground-based optical telescopes. Images with 40mas resolution and Strehl Ratios higher than 80% have been acquired in H band (1.6 μm). Such images showed a contrast as high as 10~(-4). Based on these results, we compare the performances offered by a Natural Guide Star (NGS) system upgraded with the state-of-the-art technology and those delivered by existing Laser Guide Star (LGS) systems. The comparison, in terms of sky coverage and performances, suggests rethinking the current role ascribed to NGS and LGS in the next generation of AO systems for the 8-10 meter class telescopes and Extremely Large Telescopes (ELTs).
机译:大型双筒望远镜(LBT)是独特的望远镜,具有两个共同安装的光学火车和8.4m主镜。望远镜自适应光学(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前传感器。在空中调试期间,这种系统达到了大型地面光学望远镜从未有过的性能。已在H波段(1.6μm)中获得了分辨率为40mas和Strehl比高于80%的图像。这样的图像显示出高达10〜(-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的激光导星(LGS)系统提供的性能。从天空覆盖范围和性能方面进行的比较表明,对于在8至10米级望远镜和超大型望远镜(ELT)的下一代AO系统中归因于NGS和LGS的当前作用,我们需要重新考虑。

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  • 来源
  • 会议地点 San Diego CA(US)
  • 作者单位

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    LBT Observatory, Univ. of Arizona, 933 North Cherry Ave., Tucson AZ 85721, USA;

    LBT Observatory, Univ. of Arizona, 933 North Cherry Ave., Tucson AZ 85721, USA;

    LBT Observatory, Univ. of Arizona, 933 North Cherry Ave., Tucson AZ 85721, USA;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

    INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 航空仪表、航空设备、飞行控制与导航;
  • 关键词

    large binocular telescope; high-order adaptive optics; pyramid sensor; adaptive secondary mirror;

    机译:大型双筒望远镜;高阶自适应光学金字塔传感器自适应辅助镜;

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