activity
20182024
most citedNon-modulated pyramid wavefront sensor: Use in sensing and correcting atmospheric turbulence

18 citations · 48 across the 15 of their papers we have counts for

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21 papers · 1 filter

astro-ph.IM20246 cited

Strategy for sensing petal mode in presence of AO residual turbulence with pyramid wavefront sensor

Nicolas Levraud, Vincent Chambouleyron, Jean François Sauvage +9

With the Extremely Large Telescope-generation telescopes come new challenges. The complexity of these telescopes' pupil creates new problems for Adaptive Optics. In particular, the…

astro-ph.IM2023

SOUL at LBT: commissioning results, science and future

Enrico Pinna, Fabio Rossi, Guido Agapito +27

The SOUL systems at the Large Bincoular Telescope can be seen such as precursor for the ELT SCAO systems, combining together key technologies such as EMCCD, Pyramid WFS and adaptiv…

astro-ph.IM202318 cited

Non-modulated pyramid wavefront sensor: Use in sensing and correcting atmospheric turbulence

Guido Agapito, Enrico Pinna, Simone Esposito +2

Context. The diffusion of adaptive optics systems in astronomical instrumentation for large ground-based telescopes is rapidly increasing and the pyramid wavefront sensor is replac…

astro-ph.IM2023

Contactless actuators and pyramid wavefront sensor, the SPLATT concept for space active optics: an overview of the project and the last laboratory results

Runa Briguglio, Marco Xompero, Marcello Scalera +13

In the last few years the concept of an active space telescope has been greatly developed, to meet demanding requirements with a substantial reduction of tolerances, risks and cost…

astro-ph.IM2022

PSF nowcast using PASSATA simulations -- Towards a PSF forecast

A. Turchi, G. Agapito, E. Masciadri +8

Characterizing the PSF of adaptive optics instruments is of paramount importance both for instrument design and observation planning/optimization. Simulation software, such as PASS…

astro-ph.IM20221 cited

Adapting the pyramid wavefront sensor for pupil fragmentation of the ELT class telescopes

Nicolas Levraud, Vincent Chambouleyron, Olivier Fauvarque +8

The next generation of Extremely Large Telescope (24 to 39m diameter) will suffer from the so-called "pupil fragmentation" problem. Due to their pupil shape complexity (segmentatio…