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)
› 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)
› Advances in real-time implementation for deep learning wavefront sensors - Benjamin Gonzalez, Pontificia Universidad Católica de Valparaíso
17:20-19:20 (2h)
› Comparing the Shack-Harmann and Pyramid wavefront sensors with laser guide stars for 40 m telescopes - Francisco Oyarzun, Aix Marseille Université, CNRS, CNES, LAM
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)
› 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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Scott Logic Lecture Theatre (MCS 0001)
