Starlight coupling through atmospheric turbulence into few-mode fibers and photonic lanterns in the presence of partial adaptive optics correction
Momen Diab, Aline N. Dinkelaker, John Davenport, Kalaga Madhav and, Martin M. Roth

TL;DR
This paper explores how combining low-order adaptive optics with photonic lanterns can improve starlight coupling efficiency into integrated astrophotonic devices despite atmospheric turbulence, through simulations and experimental validation.
Contribution
It demonstrates a practical hybrid approach that balances adaptive optics and waveguide degrees of freedom to enhance coupling efficiency and signal-to-noise ratio in astronomical instruments.
Findings
Hybrid system outperforms single-mode fiber coupling.
Trade-off analysis guides cost-effective system design.
Experimental results validate simulation predictions.
Abstract
Starlight corrupted by atmospheric turbulence cannot couple efficiently into astronomical instruments based on integrated optics as they require light of high spatial coherence to couple into their single-mode waveguides. Low-order adaptive optics in combination with photonic lanterns offer a practical approach to achieve efficient coupling into multiplexed astrophotonic devices. We investigate, aided by simulations and an experimental testbed, the trade-off between the degrees of freedom of the adaptive optics system and those of the input waveguide of an integrated optic component leading to a cost-effective hybrid system that achieves a signal-to-noise ratio higher than a standalone device fed by a single-mode fiber.
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