论文标题
在大型双筒望远镜处的单模纤维耦合的表征
Characterization of Single-Mode Fiber Coupling at the Large Binocular Telescope
论文作者
论文摘要
优化天上的单模纤维(SMF)注入是开发精确的多普勒光谱仪和新的天体摄影技术的重要组成部分。我们于2016年4月在大型双目望远镜(LBT)上安装并测试了一个原型SMF注入系统。纤维注入单元是作为新仪器的脱发仪器的一部分而建立的,该工具是一种名为Ilocater的新仪器,该工具将使用自适应光学器件(AO)来喂养高分辨率的高分辨率,以供应高分辨率,近乎贴纸。在本文中,我们报告了明亮的M型星的Y波段SMF耦合测量值。我们将交付的strehl比和SMF耦合的理论期望与实验结果进行了比较,并评估了限制注入效率的基本效果。我们发现望远镜本身的瞳孔几何形状将纤维耦合限制为最大效率的rho_tel = 0.78。进一步的分析表明,AO校正,倾斜倾斜残差和静态(非共同路径)畸变的个体影响促成Rho_strehl = 0.33,Rho_tip/Tilt = 0.84和Rho_ncpa的耦合系数。这些效果结合起来导致所有观测值的平均y波段SMF效率为0.18。最后,我们研究了纤维耦合对径向速度(RV)精度的影响,这是恒星明显幅度的函数。
Optimizing on-sky single-mode fiber (SMF) injection is an essential part of developing precise Doppler spectrometers and new astrophotonics technologies. We installed and tested a prototype SMF injection system at the Large Binocular Telescope (LBT) in April 2016. The fiber injection unit was built as part of the de-risking process for a new instrument named iLocater that will use adaptive optics (AO) to feed a high resolution, near-infrared spectrograph. In this paper we report Y-band SMF coupling measurements for bright, M-type stars. We compare theoretical expectations for delivered Strehl ratio and SMF coupling to experimental results, and evaluate fundamental effects that limit injection efficiency. We find the pupil geometry of the telescope itself limits fiber coupling to a maximum efficiency of rho_tel=0.78. Further analysis shows the individual impact of AO correction, tip-tilt residuals, and static (non-common-path) aberrations contribute coupling coefficients of rho_Strehl=0.33, rho_tip/tilt=0.84, and rho_ncpa=0.8 respectively. Combined, these effects resulted in an average Y-band SMF efficiency of 0.18 for all observations. Finally, we investigate the impact of fiber coupling on radial velocity (RV) precision as a function of stellar apparent magnitude.