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A visible-light AO system for the 4.2 m SOAR telescope

机译:用于4.2 m SOAR望远镜的可见光AO系统

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Pushing the adaptive compensation of turbulence into the visible range remains a challenging task, despite the progress of AO technology. An AO system for SOAR, now under conceptual study, will be able to reach diffraction-limited resolution at 0.5-0.7 microns with natural guide stars as faint as magnitude 12, enabling studies of stellar vicinities for faint companions, nebulosity, etc. During the second stage of the project a Rayleigh laser guide star will be implemented. In this mode, only the lowest turbulent layers will be compensated. The angular resolution will be only two times better than natural seeing, but, in exchange, the uniformly compensated field will reach 2-3 arc-minutes, offering unique capabilities in crowded fields (clusters, nearby galaxies).
机译:尽管AO技术的进步,将湍流的自适应补偿推到可见范围仍然是一项艰巨的任务。目前正在概念研究中的用于SOAR的AO系统将能够在0.5-0.7微米处达到衍射极限分辨率,而自然导星的微弱程度为12级,从而能够研究微弱伴星的恒星​​附近,星云度等。该项目的第二阶段将实施瑞利激光制导星。在这种模式下,仅最低的湍流层将得到补偿。角分辨率将仅是自然观察的两倍,但是作为交换,均匀补偿的场将达到2-3弧分,在拥挤的场(团簇,附近的星系)中提供了独特的功能。

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