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Program

Week Mon. 23 Tue. 24 Wed. 25 List

Monday, September 23, 2024 ›

12:00

13:00

14:00

15:00

16:00

17:00

18:00

19:00

›12:00 (1h)

Arrival / Registration

12:00 - 13:00 (1h)

Arrival / Registration

Registration desk open for collection of badges, delegate packs, upload of presentation files.

›13:00 (10min)

Welcome
Tim Morris

› Scott Logic Lecture Theatre (MCS 0001)

13:00 - 13:10 (10min)

Welcome

Scott Logic Lecture Theatre (MCS 0001)

Tim Morris

›13:20 (1h20)

Laboratory and on sky demonstration of new designs and concepts

› Scott Logic Lecture Theatre (MCS 0001)

13:20 - 14:40 (1h20)

Laboratory and on sky demonstration of new designs and concepts

Scott Logic Lecture Theatre (MCS 0001)

› Spatiotemporal statistics of optical turbulence at the ground layer. - Dario Perez, Pontificia Universidad Católica de Valparaíso 13:20-13:40 (20min)

› MATTO - The Multi-Conjugate Adaptive Techniques Test Optics - Simone Di Filipo - INAF 13:40-14:00 (20min)

› The Asgard/BIFROST beam combination instrument for VLTI - Stefan Kraus, University of Exeter, Astrophysics Group 14:00-14:20 (20min)

› Using a pyramid wavefront sensor off-zero: from theory to practice - Arnaud STRIFFLING, DOTA, ONERA [Salon], Institut de Planétologie et d'Astrophysique de Grenoble, Laboratoire d'Astrophysique de Marseille 14:20-14:40 (20min)

›14:40 (40min)

Coffee break

› Scott Logic Lecture Theatre (MCS 0001)

14:40 - 15:20 (40min)

Coffee break

Scott Logic Lecture Theatre (MCS 0001)

›15:20 (1h40)

Hybrid and multi-stage WFSensing

› Scott Logic Lecture Theatre (MCS 0001)

15:20 - 17:00 (1h40)

Hybrid and multi-stage WFSensing

Scott Logic Lecture Theatre (MCS 0001)

› Co-phasing of Segmented Mirrors Using the Dispersed Fringe Sensor - Radhika Dharmadhikari, Indian Institute of Astrophysics, University of Calcutta 15:20-15:40 (20min)

› End-to-end numerical simulations of SAXO+, a two-stage AO system for high-contrast imaging - Charles Goulas, LESIA 15:40-16:00 (20min)

› The Phasing and Diagnostic Station of the ELT - Thomas Pfrommer, European Southern Observatory 16:00-16:20 (20min)

› Advances in SPAD array-based time-resolved wavefront sensing - Jean-Pierre Veran, NRC Herzberg Astronomy and Astrophysics 16:20-16:40 (20min)

› Phasing tests with the Natural Guide star Wavefront Sensor Prototype for the Giant Magellan Telescope - Cedric Plantet, INAF - Osservatorio Astrofisico di Arcetri 16:40-17:00 (20min)

›17:00 (20min)

Transfer to Ogden Centre West

17:00 - 17:20 (20min)

Transfer to Ogden Centre West

›17:20 (2h)

Poster Session

› Ogden Centre West

17:20 - 19:20 (2h)

Poster Session

Ogden Centre West

› Advances in real-time implementation for deep learning wavefront sensors - Benjamin Gonzalez, Pontificia Universidad Católica de Valparaíso 17:20-19:20 (2h)

› Diversification of Camera Technology in Support of Varied Wavefront Sensing Applications - Tom Seccull, Oxford Instruments Andor, 7 Millennium Way, Springvale Business Park, Belfast, BT12 7AL, UK 17:20-19:20 (2h)

› Durham Adaptive Optics (DAO) real-time controller - Barr David, Durham University 17:20-19:20 (2h)

› Emulating atmospheric surface layer conditions with a forced convector for optical turbulence studies - Pablo Garrido, Pontificia Universidad Católica de Valparaíso 17:20-19:20 (2h)

› Exploring the Axicon for modulation-free Wavefront Sensing using deep learning - Jorge Tapia, Pontificia Universidad Católica de Valparaíso 17:20-19:20 (2h)

› Holographic Modal Wavefront Sensing for Active and Adaptive Optics - Raveena Koliyatan Manamparambil, University of Galway 17:20-19:20 (2h)

› Joint deep learning optics and reconstruction for unmodulated pyramid wavefront sensing - Nicolas Hernandez, Pontificia Universidad Católica de Valparaíso 17:20-19:20 (2h)

› Neural Networks for Turbulence Prediction and Characterization in Adaptive Optics - Alejandro Buendía, Instituto Universitario de Ciencias y Tecnologías Espaciales de Asturias (ICTEA) 17:20-19:20 (2h)

› Piston sensing using multi-shot coded aperture complex wavefront sensing - Bastián Romero, Pontificia Universidad Católica de Valparaíso 17:20-19:20 (2h)

› Single Star SCIDAR: Atmospheric parameters profiling using the power spectrum of scintillation. - Youssef Errazzouki, Laboratoire de Physique des Hautes Energies et Astrophysique (LPHEA) FSSM, Cadi Ayyad University, Marrakech - Morocco 17:20-19:20 (2h)

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