activity
20152021
most citedPerformance of the VLT Planet Finder SPHERE II. Data analysis and Results for IFS in laboratory

156 citations · 186 across the 4 of their papers we have counts for

collaborators

13 papers

astro-ph.IM20213 cited

Current status of PAPYRUS : the pyramid based adaptive optics system at LAM/OHP

Muslimov E., Levraud N., Chambouleyron V. +23

The Provence Adaptive optics Pyramid Run System (PAPYRUS) is a pyramid-based Adaptive Optics (AO) system that will be installed at the Coude focus of the 1.52m telescope (T152) at…

astro-ph.IM20201 cited

Operational forecast of the PSF figures of merit

A. Turchi, G. Agapito, E. Masciadri +6

The optimization and scheduling of scientific observations done with instrumentation supported by adaptive optics could greatly benefit from the forecast of PSF figures of merit (F…

astro-ph.IM2020

Limitations imposed by optical turbulence profile structure and evolution on tomographic reconstruction for the ELT

O. J. D. Farley, J. Osborn, T. Morris +4

The performance of tomographic adaptive optics systems is intrinsically linked to the vertical profile of optical turbulence. Firstly, a sufficient number of discrete turbulent lay…

astro-ph.IM2020

Reconstruction of the ground-layer adaptive-optics point spread function for MUSE Wide Field Mode observations

Thierry Fusco, R. Bacon, S. Kamann +7

Here we describe a simple, efficient, and most importantly fully operational point-spread-function(PSF)-reconstruction approach for laser-assisted ground layer adaptive optics (GLA…

astro-ph.IM2020

Pushing Point spread function reconstruction to the next level. Application to SPHERE/ZIMPOL

Olivier Beltramo-Martin, Antonino Marasco, Thierry Fusco +4

Point spread function (PSF) reconstruction (PSF-R) is a well established technique to determine reliably and accurately the PSF from Adaptive Optics (AO) control loop data. We have…

astro-ph.SR2019

Dust production in the debris disk around HR 4796 A

J. Olofsson, J. Milli, P. Thébault +21

Debris disks are the natural by-products of the planet formation process. Scattered or polarized light observations are mostly sensitive to small dust grains that are released from…