Presentation + Paper
29 August 2022 20 GHz astronomical laser frequency comb with super-broadband spectral coverage
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Abstract
e report a latest generation of the laser frequency comb (LFC) for astronomy. The new features include all fiber coupled, alignment-free filter cavities; specially designed photonic crystal fiber for spectral broadening; reflective spectral flattening systems. All the features ensure the long-term stability of the whole LFC system. The LFC is designed to operate in two modes. The visible mode generates a supercontinuum from 445 nm to 870 nm, that covers 100 % spectral range of the Keck Planet Finder (KPF) spectrograph. The near-infrared mode offers a flat-top supercontinuum from 915 nm to 1450 nm, is prepared as a calibration source of the short-wavelength part of a near infrared (NIR) spectrograph
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yuanjie Wu, Zinan Huang, Tilo Steinmetz, Mark Yeo, Klaus Stockwald, and Ronald Holzwarth "20 GHz astronomical laser frequency comb with super-broadband spectral coverage", Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 121841J (29 August 2022); https://doi.org/10.1117/12.2624078
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KEYWORDS
Near infrared

Frequency combs

Astronomy

Calibration

Spectrographs

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