Abstract
Laser frequency combs have properties that make them promising spectrograph calibration light sources. One drawback for this application is the high dynamic range in the supercontinuum spectra of some frequency combs. We aim to flatten the spectrum of a Ti:sapphire laser frequency comb to improve the calibration performance for a Fourier transform spectrograph. For this, we develop a compact Fourier transform optical pulse shaping setup, which enables control of the spectral envelope via dispersion of the light onto a spatial light modulator (SLM). We demonstrate that this setup allows us to flatten the comb spectrum in the wavelength range 780 to 980 nm. For 90% of the wavelength range, the dynamic range is below 3 dB. In the flattened spectra 3% more comb lines can be detected. The line center fit precision, however, is reduced due to noise caused by the SLM.
Cite
CITATION STYLE
Debus, M., Huke, P., Meyer, D., & Reiners, A. (2021). Spectral envelope control for a flat frequency comb spectrum. Journal of Astronomical Telescopes, Instruments, and Systems, 7(02). https://doi.org/10.1117/1.jatis.7.2.025005
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