Precise and accurate wavelength calibration of spectrographs is essential for key science cases, e.g. the search for extrasolar planets, a possible variation of fundamental constants and the direct observation of cosmic expansion.
A crucial tool for this are laser frequency combs (LFCs), directly linking the accuracy of atomic clocks to optical laser lines.
However, strong material dispersion and large spectral separation from the established infrared laser oscillators so far prevent the use of LFCs for spectrograph calibration in the blue and UV part of the spectrum. At OHP/SOPHIE, we demonstrated for the first time the calibration of an astronomical spectrograph using an astrocomb in the ultraviolet spectral range below 400nm. Key technology used were nano-fabricated, periodically-poled waveguides in lithium niobate photonic chips, fed by either a robust infrared electro-optic comb generator or a chip-integrated microresonator comb. In an end-to-end test, we could demonstrate stable and accurate LFC-based spectrograph calibration, showcasing a viable path towards precision wavelength calibration of spectrographs in the ultraviolet, crucial e.g. for the future ELT/ANDES.
Precision astronomical spectroscopy is vital for seeking life beyond Earth and often relies on detecting very small wavelength shifts over years. Precision of these instruments are ensured by regular wavelength calibration and laser frequency combs stabilized with frequency standards have recently emerged as suitable sources. In this work, we demonstrate wavelength calibration of an astronomical spectrograph in ultraviolet spectrum below 400 nm. This is achieved using second- and third- order nonlinear effects in thin-film, periodically poled lithium niobate waveguides with an infrared electro-optic comb generator at 18 GHz.
Continuous-wave (CW) laser-driven integrated Kerr microresonators enable broadband optical frequency combs with high repetition rates and low threshold power, in a compact footprint. A drawback of such microcombs is the low conversion efficiency from the pump laser to the comb lines, which is often in the few percent range or below. Here, complementing previously demonstrated approaches to increase conversion efficiency, we demonstrate a novel approach that leverages a chip-based rare-earth (Tm3+)-doped optical gain medium to boost the pump-to-comb conversion efficiency by more than one order of magnitude. Importantly, the gain medium does not require an additional pump laser, but recycles residual pump light from the Kerr-comb: the CW pump of the Kerr-comb (1610 nm) coincides with the pump wavelength of the on-chip gain medium, allowing unconverted pump power to be absorbed and transferred to the comb lines within gain window (1700 - 1900 nm). This enables a new class of highly efficient Kerr-combs for applications e.g. in data centers and optical computing.
Amplification of ultrafast optical pulses is key to a large number of applications in photonics. While ultrashort pulse amplification is well established in optical gain fibers, it is challenging to achieve in photonic-chip integrated waveguides, due to their inherent high-optical nonlinearity.
Here, we demonstrate for the first-time femtosecond pulse amplification on an integrated photonic chip. Our approach translates the concept of chirped pulse amplification to the chip level. Specifically, we leverage tailored all-normal dispersion, large mode-area gain waveguides to realize a low-nonlinearity, high-gain, short-length optical amplifier in which pulse propagation is dominated by dispersion. We show more than 17dB amplification of ultrashort pulses from a 1 GHz femtosecond source at center wavelength of 1815 nm. The amplified pulses have an on-chip output pulse peak power of 800 W with a pulse duration of 116 fs.
Dissipative Kerr solitons (DKS) in high-Q microresonators provide femtosecond pulses and frequency combs with high-repetition rate; they have seen applications from optical spectroscopy, data transfer and laser ranging to astronomical spectrograph calibration. Usually DKS are generated in ring-resonators, where only a limited set of design parameters are available. Here, we demonstrate DKS in an integrated high-Q Fabry-Perot microresonator formed by two photonic crystal reflectors in a waveguide. This platform opens a large design space with opportunities for extension of DKS into new wavelength ranges as well as generally phase-matching and spectral engineering for broadband frequency conversion in integrated nonlinear microresonators.
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