Experimental and on-sky demonstration of spectrally dispersed wavefront sensing using a photonic lantern

Adaptive optics (AO) systems are critical in any application where highly resolved imaging or beam control must be performed through a dynamic medium. Such applications include astronomy and free-space optical communications, where light propagates through the atmosphere, as well as medical microscopy and vision science, where light propagates through biological tissues. Recent works have demonstrated common-path wavefront sensors (WFSs) for adaptive optics using the photonic lantern (PL), a slowly varying waveguide that can efficiently couple multi-moded light into single-mode fibers (SMFs). We use the SCExAO astrophotonics platform at the 8 m Subaru Telescope to show that spectral dispersion of lantern outputs can improve correction fidelity, culminating with an on-sky demonstration of real-time wavefront control. This is the first, to the best of our knowledge, result for either a spectrally dispersed or a photonic lantern wavefront sensor. Combined with the benefits offered by lanterns in precision spectroscopy, our results suggest the future possibility of a unified wavefront sensing spectrograph using compact photonic devices.

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Publication Details

Journal
Optics Letters
Published
2025-03-24
DOI
https://doi.org/10.1364/ol.551624
Citations
4
Primary Topic
Adaptive optics and wavefront sensing
Type
article
Field-Weighted Citation Impact
4.99

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Experimental and on-sky demonstration of spectrally dispersed wavefront sensing using a photonic lantern

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Experimental and on-sky demonstration of spectrally dispersed wavefront sensing using a photonic lantern

Sergio G. Leon-Saval, Nemanja Jovanović, Yoo Jung Kim, Olivier Guyon, Julien Lozi, Kyohoon Ahn, Steph Sallum, Barnaby Norris, Yinzi Xin, Sébastien Vievard, Jonathan Lin, Daniel Levinstein, Christopher H. Betters, Vincent Déo, Michael P. Fitzgerald
article en
4 citations

Abstract

Adaptive optics (AO) systems are critical in any application where highly resolved imaging or beam control must be performed through a dynamic medium. Such applications include astronomy and free-space optical communications, where light propagates through the atmosphere, as well as medical microscopy and vision science, where light propagates through biological tissues. Recent works have demonstrated common-path wavefront sensors (WFSs) for adaptive optics using the photonic lantern (PL), a slowly varying waveguide that can efficiently couple multi-moded light into single-mode fibers (SMFs). We use the SCExAO astrophotonics platform at the 8 m Subaru Telescope to show that spectral dispersion of lantern outputs can improve correction fidelity, culminating with an on-sky demonstration of real-time wavefront control. This is the first, to the best of our knowledge, result for either a spectrally dispersed or a photonic lantern wavefront sensor. Combined with the benefits offered by lanterns in precision spectroscopy, our results suggest the future possibility of a unified wavefront sensing spectrograph using compact photonic devices.

Optics LettersVol. 50(8)
California Institute of Technology (US), The University of Sydney (AU), University of Arizona (US), Subaru (Japan) (JP), Korea Astronomy and Space Science Institute (KR), University of California System (US), Astrobiology Center (JP), National Astronomical Observatory of Japan (JP)
National Science Foundation, Japan Society for the Promotion of Science
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Openalex Percentile: Top 5%
Adaptive optics and wavefront sensing
4.99
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