DanceCam: atmospheric turbulence mitigation in wide-field astronomical images with short-exposure video streams

Author:

Bialek Spencer12ORCID,Bertin Emmanuel23ORCID,Fabbro Sébastien14ORCID,Bouy Hervé56ORCID,Rivet Jean-Pierre7ORCID,Lai Olivier7ORCID,Cuillandre Jean-Charles3ORCID

Affiliation:

1. Department of Physics and Astronomy, University of Victoria , Victoria, BC V8W 3P2 , Canada

2. Canada–France–Hawaii Telescope , Kamuela, HI 96743 , USA

3. AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Cité , F-91191 Gif-sur-Yvette , France

4. National Research Council Herzberg Astronomy and Astrophysics , Victoria, BC V9E 2E7 , Canada

5. Laboratoire d’Astrophysique de Bordeaux, CNRS and Université de Bordeaux , Allée Geoffroy St. Hilaire, F-33165 Pessac , France

6. Institut Universitaire de France

7. Université Côte d’Azur, Observatoire de la Côte d’Azur , CNRS, Laboratoire J.–L. Lagrange, F-06304 Nice Cedex 4 , France

Abstract

ABSTRACT We introduce a novel technique to mitigate the adverse effects of atmospheric turbulence on astronomical imaging. Utilizing a video-to-image neural network trained on simulated data, our method processes a sliding sequence of short-exposure (∼0.2 s) stellar field images to reconstruct an image devoid of both turbulence and noise. We demonstrate the method with simulated and observed stellar fields, and show that the brief exposure sequence allows the network to accurately associate speckles to their originating stars and effectively disentangle light from adjacent sources across a range of seeing conditions, all while preserving flux to a lower signal-to-noise ratio than an average stack. This approach results in a marked improvement in angular resolution without compromising the astrometric stability of the final image.

Funder

European Research Council

Publisher

Oxford University Press (OUP)

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