activity
20052026
most citedDisk and wind interaction in the young stellar object MWC 297 spatially resolved with VLTI/AMBER

96 citations · 626 across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.IM2026

Self-calibration of adaptive optics systems. Application to the THEMIS solar telescope

Clementine Bechet, Eric Thiebaut, Michel Tallon +3

The interaction matrix models the effects of deformable mirror (DM) commands as perceived by the wavefront sensor (WFS) and is the cornerstone of the Adaptive Optics (AO) control.…

astro-ph.IM2024★ 1 cited

Upgrading SPHERE with the second stage AO system SAXO+: non-common path aberrations estimation and correction

Johan Mazoyer, Charles Goulas, Fabrice Vidal +16

SAXO+ is a planned enhancement of the existing SAXO, the VLT/ SPHERE adaptive optics system, deployed on ESO's Very Large Telescope. This upgrade is designed to significantly enhan…

astro-ph.IM2023★ 1 cited

Closing the loop as an inverse problem: the real-time control of THEMIS adaptive optics

Éric Thiébaut, Michel Tallon, Isabelle Tallon-Bosc +4

We have taken advantage of the implementation of an adaptive optics system on the Themis solar telescope to implement innovative strategies based on an inverse problem formulation…

astro-ph.SR2020★ 22 cited

Optically thin circumstellar medium in Lyr A system

M. Brož, D. Mourard, J. Budaj +7

beta Lyr A is a complex binary system with an extensive observational dataset: light curves (from FUV to FIR), interferometric squared visibility, closure phase, triple product mea…

astro-ph.SR2020★ 19 cited

Precise calibration of the dependence of surface brightness-colour relations on colour and class for late-type stars

A. Salsi, N. Nardetto, D. Mourard +9

Surface brightness-colour relations (SBCRs) are used to derive the stellar angular diameters from photometric observations. They have various astrophysical applications, such as th…

astro-ph.SR2020★ 7 cited

Calibrating the surface brightness - color relation for late-type red giants stars in the visible domain using VEGA/CHARA interferometric observations

N. Nardetto, A. Salsi, D. Mourard +14

The surface brightness - color relationship (SBCR) is a poweful tool for determining the angular diameter of stars from photometry. It was for instance used to derive the distance…