activity
20192026
most citedPyramid wavefront sensor optical gains compensation using a convolutional model

37 citations · 202 across the 41 of their papers we have counts for

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Showing 2026Show all

10 papers · 1 filter

astro-ph.IM2026

Modelling Fourier filtering wavefront sensors for PSD-based methods: the AOPERA tool

Romain Fétick, Vincent Chambouleyron, Lisa-Marie Mazzolo +6

Compensation of the atmospheric turbulence thanks to adaptive optics (AO) has now become commonly used for VLT or ELT class telescopes in order to retrieve a resolution close to th…

astro-ph.IM2026

On-sky demonstration of a vector Zernike wavefront sensor in a cascaded adaptive optics system

M. Motte, V. Chambouleyron, R. Fétick +13

To directly image and characterise Earth-like exoplanets, future high-contrast instruments will require adaptive-optics systems operating at increasingly high loop frequencies to r…

astro-ph.IM2026

RISTRETTO: Assembly and Testing of the Seven-spaxel, High-resolution, Diffraction-limited Spectrograph

Leonie Hoerner, Bruno Chazelas, Nathanaël Restori +24

The RISTRETTO project aims at the direct detection of the reflected light of extra-solar planets to measure albedos and detect possible biosignatures, using the high-contrast / hig…

astro-ph.IM2026

The Roman Coronagraph Community Participation Program: Using the Zernike wavefront sensor for a full characterisation of the Roman Space Telescope and the Coronagraph Instrument

Arthur Vigan, Alexis Bidot, Vincent Chambouleyron +4

The Roman Space Telescope Coronagraph Instrument (CGI) will demonstrate a series of technologies and techniques to enable the direct detection of reflected-light planets with space…

astro-ph.IM2026

Closing the loop on-sky with a vector-Zernike wavefront sensor using a convolutional neural network as phase reconstructor

Francisco Oyarzún, Mathieu Motte, Cedric-Taissir Heritier +11

Context: The new giant segmented mirror telescopes will use adaptive optics to reach the fundamental limits in resolving power. To accomplish this, new wavefront sensors (WFS) have…

astro-ph.IM2026

Cassiopee: Defining the next-generation deformable mirror and high-speed SWIR camera for adaptive optics applications

B. Neichel, T. Fusco, F. Oyarzun +14

Future adaptive optics (AO) systems for astronomy, optical communications, space situational awareness, and laser-based defense require a new generation of components operating at…

astro-ph.IM2026

Towards an Extended VLTI: Turbulence Characterization for Kilometer-Scale Optical Links at Paranal

B. Neichel, T. Pichon, G. Bourdarot +10

Future extensions of the VLTI aim to push infrared interferometry toward kilometer scale baselines, enabling angular resolutions of a few tens of micro-arcseconds. A first step wou…

astro-ph.IM2026

DD4AO control law for RISTRETTO: robustness, real-time performance, and on-sky validation with PAPYRUS

Isaac Dinis, Muskan Schinde, Nicolas Blind +11

This study presents DD4AO progress towards its implementation in the RISTRETTO instrument. DD4AO is a novel frequency-domain, data-driven controller for adaptive optics that levera…

astro-ph.IM2026

Experimentally-determined performance limits for joint imaging and wavefront sensing with a photonic lantern

Aditya R. Sengupta, Vincent Chambouleyron, Rebecca Jensen-Clem +16

The photonic lantern (PL) is a focal-plane wavefront sensor (WFS) that can be used for second-stage control of extreme adaptive optics (AO) systems. While the number of sensed mode…

astro-ph.IM2026

On-sky demonstration of reinforcement learning for adaptive optics control

Jalo Nousiainen, Vincent Chambouleyron, Benoit Neichel +7

Reinforcement learning (RL)-based algorithms have recently emerged as a promising approach for adaptive optics (AO) control. In simulations and laboratory experiments, they have de…