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Optimization of the transmitted wavefront for the infrared adaptive optics system 被引量:4

Optimization of the transmitted wavefront for the infrared adaptive optics system
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摘要 The adaptive optics system for the second-generation Very Large Telescope-interferometer(VLTI)instrument GRAVITY consists of a novel cryogenic near-infrared wavefront sensor to be installed at each of the four unit telescopes of the Very Large Telescope(VLT).Feeding the GRAVITY wavefront sensor with light in the 1.4–2.4μm band,while suppressing laser light originating from the GRAVITY metrology system requires custom-built optical componets.In this paper,we present the development of a quantitative near-infraredpoint diffraction interferometric characterization technique,which allows measuring the transmitted wavefront error of the silicon entrance windows of the wavefront sensor cryostat.The technique can be readily applied to quantitative phase measurements in the near-infrared regime.Moreover,by employing a slightly off-axis optical setup,the proposed method can optimize the required spatial resolution and enable real time measurement capabilities.The feasibility of the proposed setup is demonstrated,followed by a theoretical analysis and experimental results.Our experimental results show that the phase error repeatability in the nanometer regime can be achieved. The adaptive optics system for the second-generation Very Large Telescope-interferometer(VLTI)instrument GRAVITY consists of a novel cryogenic near-infrared wavefront sensor to be installed at each of the four unit telescopes of the Very Large Telescope(VLT).Feeding the GRAVITY wavefront sensor with light in the 1.4–2.4μm band,while suppressing laser light originating from the GRAVITY metrology system requires custom-built optical componets.In this paper,we present the development of a quantitative near-infraredpoint diffraction interferometric characterization technique,which allows measuring the transmitted wavefront error of the silicon entrance windows of the wavefront sensor cryostat.The technique can be readily applied to quantitative phase measurements in the near-infrared regime.Moreover,by employing a slightly off-axis optical setup,the proposed method can optimize the required spatial resolution and enable real time measurement capabilities.The feasibility of the proposed setup is demonstrated,followed by a theoretical analysis and experimental results.Our experimental results show that the phase error repeatability in the nanometer regime can be achieved.
出处 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS 2014年第4期608-614,共7页 中国科学:物理学、力学、天文学(英文版)
关键词 自适应光学系统 近红外 优化 波阵面 甚大望远镜 波前传感器 低温恒温器 传送 adaptive optics non-common aberration point diffraction interferometry
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  • 1Gillessen S, Eisenhauer F, Perrin G, et al. GRAVITY: A four-telescope beam combiner instrument for the VLTI. SPIE, 2010, 7734: 77340-77350.
  • 2Kendrew S, Hippler S, Brandner W, et al. The GRAVITY Coudé Infrared Adaptive Optics (CIAO) system for the VLT interferometer. Proc SPIE, 2012, 8446: 88467.
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  • 6Bartko H, Gillessen S, Rabien S, et al. The fringe detection laser metrology for the GRAVITY interferometer at the VLTI. Proc SPIE, 2010, 7734: 773421.
  • 7Pengqian Y, Hippler S, Deen C, et al. Optimizing the transmission of the GRAVITY/VLTI near-infrared wavefront sensor. Proc SPIE, 2012, 8445: 844531.
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