Keck行星成像仪和表征仪:第一阶段光纤注入装置的早期性能和调试

Evan C. Morris, Jason J. Wang, J. Ruffio, J. Delorme, Jacklyn Pezzato, C. Bond, D. Mawet, A. Skemer
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引用次数: 4

摘要

Keck行星成像仪和表征器(KPIC)是Keck II自适应光学系统和仪器套件的升级版,旨在提高巨大系外行星的直接成像和高分辨率光谱表征能力。KPIC一期包括一个光纤注入单元(FIU),位于新型金字塔波前传感器的下游,将行星光耦合到单模光纤,并将其送入Keck的高分辨率红外光谱仪NIRSPEC。这使得高色散光谱(HDS)能够以更小的距离和更高的对比度直接成像系外行星,提高我们对这些物体的光谱表征能力。在这里,我们报告了KPIC第一阶段FIU调试的性能结果,包括对仪器的吞吐量、稳定性和灵敏度的分析。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Keck Planet Imager and Characterizer: Phase I fiber injection unit early performance and commissioning
The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system and instrument suite with the goal of improving direct imaging and high-resolution spectroscopic characterization capabilities for giant exoplanets. KPIC Phase I includes a fiber injection unit (FIU) downstream of a new pyramid wavefront sensor, coupling planet light to a single mode fiber fed into NIRSPEC, Keck’s high-resolution infrared spectrograph. This enables high-dispersion spectroscopy (HDS) of directly imaged exoplanets at smaller separation and higher contrast, improving our spectral characterization capabilities for these objects. Here, we report performance results from the KPIC Phase I FIU commissioning, including analysis of throughput, stability, and sensitivity of the instrument.
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