activity
20192026
most citedPhysics-based model of the adaptive-optics corrected point-spread-function

64 citations · 83 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

High-contrast imaging of Galactic Cepheids with VLT/SPHERE

A. Gallenne, P. Kervella, N. R. Evans +10

Cepheids are key distance indicators and benchmarks for stellar evolution, yet most of them are members of binary or multiple systems. While spectroscopic surveys and Gaia proper-m…

astro-ph.IM2020★ 1 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★ 11 cited

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.IM2020★ 7 cited

Successful application of PSF-R techniques to the case of the globular cluster NGC6121 (M4)

D. Massari, A. Marasco, O. Beltramo-Martin +4

Precise photometric and astrometric measurements on astronomical images require an accurate knowledge of the Point Spread Function (PSF). When the PSF cannot be modelled directly f…

astro-ph.IM2019★ 64 cited

Physics-based model of the adaptive-optics corrected point-spread-function

Romain Fétick, Thierry Fusco, Benoit Neichel +8

Context. Adaptive optics (AO) systems greatly increase the resolution of large telescopes, but produce complex point spread function (PSF) shapes, varying in time and across the fi…