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Ultraviolet astronomical spectrograph calibration with laser frequency combs from nanophotonic lithium niobate waveguides.

Markus LudwigFurkan AyhanTobias M SchmidtThibault WildiThibault VoumardRoman BlumZhichao YeFuchuan LeiFrançois WildiFrancesco PepeMahmoud A GaafarEwelina ObrzudDavide GrassaniOlivia HeftiSylvain KarlenSteve LecomteFrançois MoreauBruno ChazelasRico SottileVictor Torres-CompanyVictor BraschLuis Guillermo VillanuevaFrançois BouchyTobias Herr
Published in: Nature communications (2024)
Astronomical precision spectroscopy underpins searches for life beyond Earth, direct observation of the expanding Universe and constraining the potential variability of physical constants on cosmological scales. Laser frequency combs can provide the required accurate and precise calibration to the astronomical spectrographs. For cosmological studies, extending the calibration with such astrocombs to the ultraviolet spectral range is desirable, however, strong material dispersion and large spectral separation from the established infrared laser oscillators have made this challenging. Here, we demonstrate astronomical spectrograph calibration with an astrocomb in the ultraviolet spectral range below 400 nm. This is accomplished via chip-integrated highly nonlinear photonics in periodically-poled, nano-fabricated lithium niobate waveguides in conjunction with a robust infrared electro-optic comb generator, as well as a chip-integrated microresonator comb. These results demonstrate a viable route towards astronomical precision spectroscopy in the ultraviolet and could contribute to unlock the full potential of next-generation ground-based and future space-based instruments.
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