Jean-Charles Cuillandre

Université Paris-Saclay
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Articles (11)

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 (∼0.2s) 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.

Year:

2024

Year:

2023

Year:

2023

Year:

2023

We present astrophot, a fast, powerful, and user-friendly python based astronomical image photometry solver. astrophot incorporates automatic differentiation and graphics processing unit (GPU), or parallel central processing unit (CPU), acceleration, powered by the machine learning library pytorch. Everything: astrophot can fit models for sky, stars, galaxies, point spread functions (PSFs), and more in a principled χ2 forward optimization, recovering Bayesian posterior information and covariance of all parameters. Everywhere: astrophot can optimize forward models on CPU or GPU; across images that are large, multiband, multi-epoch, rotated, dithered, and more. All at once: The models are optimized together, thus handling overlapping objects and including the covariance between parameters (including PSF and galaxy parameters). A number of optimization algorithms are available including Levenberg–Marquardt, Gradient descent, and No-U-Turn Markov chain Monte Carlo sampling. With an object-oriented user interface, astrophot makes it easy to quickly extract detailed information from complex astronomical data for individual images or large survey programs. This paper outlines novel features of the astrophot code and compares it to other popular astronomical image modelling software. astrophot is open-source, fully python based, and freely accessible at https://github.com/Autostronomy/AstroPhot .

Year:

2023

Year:

2023

Year:

2022

Year:

2022

Year:

2022

Year:

2021

Year:

2021

Collaborators (19)

Hervé Bouy

Professor of Astrophysics

University of Bordeaux

FRANCE
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William GILLARD

Associate professor

Aix-Marseille University

FRANCE
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C J A P Martins

-

PORTUGAL
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Vivienne Wild

University of St. Andrews

UNITED KINGDOM
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Connor Stone

Université de Montréal

CANADA
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Scott Wilkinson

University of Victoria

CANADA
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Seshadri Nadathur

University College London

UNITED KINGDOM
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Antonio da Silva

Prof. Auxiliar

Faculdade de Ciências da Universidade de Lisboa

PORTUGAL
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Stefano Camera

Associate Professor

Università degli Studi di Torino

ITALY
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Mike Hudson

Professor

University of Waterloo

CANADA
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Yannick Copin

Associate professor (with habilitation)

Institut de Physique des 2 Infinis de Lyon

FRANCE
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Sakurako Okamoto

助教/Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN
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Ludovic Van Waerbeke

Professor

The University of British Columbia

CANADA
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Henk Hoekstra

Full Professor

Leiden University

NETHERLANDS
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L Guzzo

Università degli Studi di Torino

ITALY
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Allan Hornstrup

Technical University of Denmark

DENMARK
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Nikhil Arora

-

UNITED ARAB EMIRATES
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Yashar Akrami

Adjunct Assistant Professor of Physics

Case Western Reserve University

UNITED STATES
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Chiara SIRIGNANO

Associate Professor

University of Padua

ITALY
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