› A single point spread function model for all adaptive-optics systems - Olivier Beltramo-Martin, Laboratoire dÁstrophysique de Marseille
14:00-14:20 (20min)
› Photometric and Astrometric Calibration in coronagraphic images using Alternating Satellite Speckles - Ananya Sahoo, SUBARU Telescope
14:20-14:30 (10min)
› Power Spectrum Extended, a new reconstruction method for post-OA short exposure imaging - Eric Cottalorda, Université Nice Sophia Antipolis, ArianeGroup
14:30-14:40 (10min)
› From symbolic functions to numerical code in the context of AO Simulations - Fabio Rossi, INAF - Osservatorio Astrofisico di Arcetri
14:40-14:50 (10min)
› Pyramid optical gain, how we manage it at LBT - Enrico Pinna, INAF - Osservatorio Astrofisico di Arcetri - Essna Ghose, INAF - Osservatorio Astrofisico di Arcetri
15:00-15:20 (20min)
› Practical implementation of PYROG method for the HSCAO Pyramid - charlotte bond, UK Astronomy Technology Centre - Jean-François Sauvage, DOTA, ONERA, Université Paris Saclay [Châtillon]
15:20-15:30 (10min)
› Self-optimizing adaptive optics control with Reinforcement Learning - Rico Landman, Leiden Observatory [Leiden]
15:30-15:40 (10min)
› Reduction of centroid anisoplanatism through machine learning - David Buscher, University of Cambridge
15:40-15:50 (10min)
› On-sky correction of static and quasi-static non-common path aberration with the pyramid wavefront sensor in Extreme Adaptive Optics. - Nour Skaf, Laboratoire d\'études spatiales et dínstrumentation en astrophysique
16:00-16:20 (20min)
› Dealing with Pyramid wavefront sensor non-linearities: a focal plane assisted method -
16:20-16:30 (10min)
› Prototype of an Adaptive Optics System for Intermediate Size Telescopes - Esther Soria Hernández, Instituto de Astrofisica de Canarias
16:30-16:40 (10min)
› Adaptive gain in closed-loop tilt control and adaptive optics -
17:10-17:20 (10min)
› The Ingot WFS on large telescopes: project and simulations - Elisa Portaluri, ADONI - Laboratorio Nazionale di Ottica Adattiva, INAF - Osservatorio Astronomico di Collurania
17:20-17:30 (10min)
› Prototype of a laser guide star wavefront sensor for the ELT - Zibo Ke, Laboratoire d'Astrophysique de Marseille
17:30-17:40 (10min)
› Faint IR Low Order Sensing: pushing the limiting magnitude of AOF's LTAO mode - Sylvain Oberti, European Southern Observatory
17:40-17:50 (10min)
Loading... 
zoom
