most citedExpected performance of the Pyramid wavefront sensor with a laser guide star for 40 m class telescopes

2 citations · 2 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2026

The infrared unmodulated pyramid wavefront sensor: simulations, lab and on sky

Muskan Shinde, Nicolas Blind, Isaac Dinis +13

Direct imaging of Earth-like exoplanets requires strong suppression of stellar light at small angular separations, achievable with extreme adaptive optics (XAO). The pyramid wavefr…

astro-ph.IM2026

RAMA: A new agile AO bench for the telescope FEELINGS

Matteo Pasinetti, Rodrigo Andres Munoz Gomez, Benjamin Andres Gonzalez Barraza +16

The ground-based observation of extended objects such as satellites suffer from severe atmospheric propagation constraints. Specifically, high tracking velocities and low-elevation…

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

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.IM2024

Performance comparison of the Shack-Hartmann and pyramid wavefront sensors with a laser guide star for 40 m telescopes

Francisco Oyarzun, Cedric-Taissir Heritier, Vincent Chambouleyron +3

Context. The new giant segmented mirror telescopes will use laser guide stars (LGS) for their adaptive optics (AO) systems. Two options to use as wavefront sensors (WFS) are the Sh…

astro-ph.IM2024★ 2 cited

Expected performance of the Pyramid wavefront sensor with a laser guide star for 40 m class telescopes

Francisco Oyarzún, Vincent Chambouleyron, Benoit Neichel +2

The use of artificial Laser Guide Stars (LGS) is planned for the new generation of giant segmented mirror telescopes, to extend the sky coverage of their adaptive optics systems. T…