Wavefront Sensing in the VLT/ELT era V & AO workshop week II

›13:45 (15min)

Introduction
B. Neichel

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13:45 - 14:00 (15min)

Introduction

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B. Neichel

›14:00 (1h)

Post processing & pipelines
C. Kulcsar

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14:00 - 15:00 (1h)

Post processing & pipelines

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C. Kulcsar

› 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)

›15:00 (55min)

Wavefront sensing & calibration
C. Kulcsar

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15:00 - 15:55 (55min)

Wavefront sensing & calibration

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C. Kulcsar

› 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)

›15:55 (05min)

Animation

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15:55 - 16:00 (05min)

Animation

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›16:00 (1h)

Wavefront sensing & calibration
T. Fusco

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16:00 - 17:00 (1h)

Wavefront sensing & calibration

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T. Fusco

› 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)

› Visible pyramid wavefront sensor for MAPS - MMT Adaptive optics exoPlanet characterization System - Narsireddy Anugu, Steward Observatory 16:40-16:50 (10min)

›17:00 (1h)

Wavefront sensing & calibration
T. Fusco

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17:00 - 18:00 (1h)

Wavefront sensing & calibration

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T. Fusco

› 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)

›18:00 (15min)

Conclusion
B. Neichel

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18:00 - 18:15 (15min)

Conclusion

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B. Neichel