# Efficient injection from large telescopes into single-mode fibres: Enabling the era of ultra-precision astronomy

## TL;DR

This paper demonstrates high-efficiency coupling of large telescope light into single-mode fibres using adaptive optics, enabling advanced astronomical instruments with improved precision and new capabilities.

## Contribution

The study shows that with optimized pupil control and wavefront correction, efficient fibre coupling is achievable on large telescopes, advancing photonic instrument integration.

## Key findings

- Achieved 86% coupling efficiency in laboratory conditions at 1550 nm.
- On-sky coupling efficiency of ~50% with 60% Strehl ratio in H-band.
- Forecasted >67% coupling efficiency with >90% Strehl ratio.

## Abstract

Photonic technologies offer numerous advantages for astronomical instruments such as spectrographs and interferometers owing to their small footprints and diverse range of functionalities. Operating at the diffraction-limit, it is notoriously difficult to efficiently couple such devices directly with large telescopes. We demonstrate that with careful control of both the non-ideal pupil geometry of a telescope and residual wavefront errors, efficient coupling with single-mode devices can indeed be realised. A fibre injection was built within the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument. Light was coupled into a single-mode fibre operating in the near-IR (J-H bands) which was downstream of the extreme adaptive optics system and the pupil apodising optics. A coupling efficiency of 86% of the theoretical maximum limit was achieved at 1550 nm for a diffraction-limited beam in the laboratory, and was linearly correlated with Strehl ratio. The coupling efficiency was constant to within <30% in the range 1250-1600 nm. Preliminary on-sky data with a Strehl ratio of 60% in the H-band produced a coupling efficiency into a single-mode fibre of ~50%, consistent with expectations. The coupling was >40% for 84% of the time and >50% for 41% of the time. The laboratory results allow us to forecast that extreme adaptive optics levels of correction (Strehl ratio >90% in H-band) would allow coupling of >67% (of the order of coupling to multimode fibres currently). For Strehl ratios <20%, few-port photonic lanterns become a superior choice but the signal-to-noise must be considered. These results illustrate a clear path to efficient on-sky coupling into a single-mode fibre, which could be used to realise modal-noise-free radial velocity machines, very-long-baseline optical/near-IR interferometers and/or simply exploit photonic technologies in future instrument design.