The Keck Planet Imager and Characterizer: Phase I fiber injection unit early performance and commissioning

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

Abstract

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.
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
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。
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