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A test bench for ARGOS: integration of sub-systems and validation of the wavefront sensing

机译:ARGOS的测试平台:子系统的集成和波前感测的验证

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ARGOS, the wide eld Laser Guide Stars adaptive optics system for the Large Binocular Telescope, is nowentering its installation phase. In the meanwhile, we have started a test bench in order to integrate variousArgos sub-systems and demonstrate its wavefront measurements. To this objective, we rst validate three keycomponents of the Argos wavefront sensor which we then integrate together. The test bench therefore comprisesthe Argos wavefront camera system - including a large frame, fast framerate, high quantum eciency and lowreadout noise pnCCD -, the slope computer, and a optical gating unit. While we present here the demonstrationof those three key components, it is also a step to their system level integration that enables us to validate thewavefront measurements in term of noises, timing and computation. In the near future, those system will beintegrated to the wavefront sensor system of ARGOS.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:ARGOS是用于大型双筒望远镜的宽视场激光导星自适应光学系统,目前正进入安装阶段。同时,我们已经开始建立一个测试台,以集成各种Argo子系统并演示其波前测量。为此,我们首先验证Argos波前传感器的三个关键组件,然后将它们集成在一起。因此,测试台包括Argos波前相机系统-包括大框架,快速帧频,高量子效率和低读出噪声pnCCD-,斜率计算机和光学选通单元。虽然我们在此演示这三个关键组件,但这也是对它们进行系统级集成的一步,这使我们能够从噪声,时序和计算方面验证波前测量。在不久的将来,这些系统将被集成到ARGOS的波前传感器系统中。©(2012)版权所有,光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

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