96 kHz on-sky imaging on an adaptive optics system with a single-photon avalanche diode
Abstract
Astronomical observations requiring extremely high angular resolution necessitate advanced adaptive optics (AO) systems to overcome blurring caused by the atmosphere. In addition to obtaining much sharper point-spread functions (PSFs) with these systems, it is beneficial to be able to characterize the behaviour of the resulting PSF across time and wavelength. We have installed a commercially-available Single-photon avalanche diode (SPAD) array on the focal plane of the REVOLT AO testbench at the Dominion Astrophysical Observatory, allowing us to observe the visible PSF of the system at rates up to 96 kHz. This provides a time-resolved view of the PSF at ∼100 times the frequency of the AO system itself. We use this detector to analyze the high-frequency behaviour of the PSF of the AO system, including residual tip/tilt and deformable mirror response. We also explore the performance of AO-assisted lucky imaging, in which we average together only the frames which result in the best image quality. We find that high-framerate imaging can significantly improve the PSF beyond the native capabilities of the AO system.
Versions
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BibTeX
@misc{grosson2026onsky,
title = {{96 kHz on-sky imaging on an adaptive optics system with a single-photon avalanche diode}},
author = {Theodore A. Grosson and Maaike A. M. van Kooten and Kathryn Jackson and Jean-Pierre Veran and Simon Carrier},
howpublished = {arXiv},
year = {2026},
month = aug,
doi = {10.48550/arxiv.2608.28858},
eprint = {2608.28858},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2608.28858},
}
RIS
TY - UNPB
TI - 96 kHz on-sky imaging on an adaptive optics system with a single-photon avalanche diode
AU - Theodore A. Grosson
AU - Maaike A. M. van Kooten
AU - Kathryn Jackson
AU - Jean-Pierre Veran
AU - Simon Carrier
PY - 2026
DA - 2026/08/28
PB - arXiv
DO - 10.48550/arxiv.2608.28858
UR - https://arxiv.org/abs/2608.28858
AB - Astronomical observations requiring extremely high angular resolution necessitate advanced adaptive optics (AO) systems to overcome blurring caused by the atmosphere. In addition to obtaining much sharper point-spread functions (PSFs) with these systems, it is beneficial to be able to characterize the behaviour of the resulting PSF across time and wavelength. We have installed a commercially-available Single-photon avalanche diode (SPAD) array on the focal plane of the REVOLT AO testbench at the Dominion Astrophysical Observatory, allowing us to observe the visible PSF of the system at rates up to 96 kHz. This provides a time-resolved view of the PSF at ∼100 times the frequency of the AO system itself. We use this detector to analyze the high-frequency behaviour of the PSF of the AO system, including residual tip/tilt and deformable mirror response. We also explore the performance of AO-assisted lucky imaging, in which we average together only the frames which result in the best image quality. We find that high-framerate imaging can significantly improve the PSF beyond the native capabilities of the AO system.
ER -