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

Author:

Ludwig Markus,Ayhan FurkanORCID,Schmidt Tobias M.ORCID,Wildi ThibaultORCID,Voumard Thibault,Blum Roman,Ye ZhichaoORCID,Lei FuchuanORCID,Wildi François,Pepe Francesco,Gaafar Mahmoud A.ORCID,Obrzud Ewelina,Grassani Davide,Hefti Olivia,Karlen SylvainORCID,Lecomte Steve,Moreau François,Chazelas Bruno,Sottile Rico,Torres-Company VictorORCID,Brasch VictorORCID,Villanueva Luis G.ORCID,Bouchy François,Herr TobiasORCID

Abstract

AbstractAstronomical 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.

Funder

Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung

Publisher

Springer Science and Business Media LLC

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