GRAVITY+ 波前传感器:用于 VLTI 的高对比度、激光导星和自适应光学系统

G. Bourdarot, F. Eisenhauer, S. Yazıcı, H. Feuchtgruber, J-B Le Bouquin, M. Hartl, C. Rau, J. Graf, N. More, E. Wieprecht, F. Haussmann, F. Widmann, D. Lutz, R. Genzel, F. Gonte, S. Oberti, J. Kolb, J. Woillez, H. Bonnet, D. Schuppe, A. Brara, J. Hartwig, A. Goldbrunner, C. Furchtsam, F. Soller, S. Czempiel, J. Eibl, D. Huber, S. Uysal, I. Treffler, H. Ozdemir, V. Gopinatha, P. Bourget, A. Berdeu, S. Gillessen, T. Ott, P. Berio, O. Boebion, F. Millour, R. Dembet, C. Edouard, T. Gomes, T. Shimizu, A. Drescher, M. Fabricius, J. Shangguan, S. Lagarde, S. Robbe-Dubois, F. Allouche, H. Nowacki, D. Defrere, P. J. V. Garcia, S. Hoenig, L. Kreidbergg, T. Paumard, C. Straubmeier
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引用次数: 0

摘要

我们介绍了重力加自适应光学(GPAO)系统的波前传感器单元,该系统将装备 VLTI 的所有 8 米级望远镜,是 GRAVITY+ 项目的仪器部分。该系统包括每个波前传感器单元的两个模块:一个具有高阶 40x40Shack-Hartmann 的自然导星传感器和一个 30x30 激光导星传感器。最先进的自动光学校正将大大提高干涉测量的性能,特别是用于自然导星观测的高对比度观测和激光导星的全天空覆盖,这将是首次在 VLTI 仪器上实现。下面,我们将概述波前传感器单元系统在完成集成和鉴定之后的情况。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
GRAVITY+ Wavefront Sensors: High-Contrast, Laser Guide Star, Adaptive Optics systems for the VLTI
We present the Wavefront Sensor units of the Gravity Plus Adaptive Optics (GPAO) system, which will equip all 8m class telescopes of the VLTI and is an instrumental part of the GRAVITY+ project. It includes two modules for each Wavefront Sensor unit: a Natural Guide Star sensor with high-order 40x40 Shack-Hartmann and a Laser Guide Star 30x30 sensor. The state-of-the-art AO correction will considerably improve the performance for interferometry, in particular high-contrast observations for NGS observations and all-sky coverage with LGS, which will be implemented for the first time on VLTI instruments. In the following, we give an overview of the Wavefront Sensor units system after completion of their integration and characterization.
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