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Wednesday, October 19, 2022
10:00
11:00
12:00
13:00
14:00
15:00
16:00
17:00
18:00
19:00
20:00
›10:50 (1h50)
WFS for HCI
Carlos Correia
› Main Room
10:50 - 12:40 (1h50)
WFS for HCI
Main Room
Carlos Correia
›
Adaptive Optics for High Contrast Imaging : from NACO to PCS
- Jean-Francois Sauvage, ONERA
11:10-11:40 (30min)
›
A Zernike wavefront sensor for the ELT-HARMONI high-contrast module - Results from a testbench under realistic observation conditions
- Adrien Hours, IPAG
11:40-12:00 (20min)
›
Calibration and performances of the integrated Mach-Zehnder (iMZ) wavefront sensor for extreme adaptive optics
- Camille Graf, Centre de Recherche Astrophysique de Lyon
12:00-12:20 (20min)
›
Towards On-Sky Focal Plane Wavefront Control of Residual Atmospheric Speckles
- Benjamin Gerard, Lawrence Livermore National Laboratory, University of California, Santa Cruz
12:20-12:40 (20min)
›14:20 (2h)
WFSensing for measuring phase-discontinuities
Enrico Pinna
› Main Room
14:20 - 16:20 (2h)
WFSensing for measuring phase-discontinuities
Main Room
Enrico Pinna
›
The baseline WFC strategy for the ESO ELT
- Henri Bonnet, European Southern Observatory
14:30-15:00 (30min)
›
A rotational shearing interferometer to sense across-the-spider phase discontinuity at ELT.
- Lorenzo Busoni, INAF - Osservatorio Astrofisico di Arcetri
15:00-15:20 (20min)
›
Petal mode measurement and reconstruction with pyramid assisted by spatial filtering
- Nicolas Levraud, Laboratoire d'Astrophysique de Marseille
15:20-15:40 (20min)
›
Pyramid Wavefront Sensors for the Detection of Small Phase discontinuities
- Deborah Malone, University of Galway, European Southern Observatory
15:40-16:00 (20min)
›
Two-wavelength focal-plane piston sensing: first experimental results with LIFT
- Cedric Plantet, INAF - Osservatorio Astrofisico di Arcetri
16:00-16:20 (20min)
›17:00 (1h10)
New WFS concepts
Lauren Schatz
› Main Room
17:00 - 18:10 (1h10)
New WFS concepts
Main Room
Lauren Schatz
›
N2ONCPA: a new low order Wavefront Sensor and its first experimental results.
- Alessandro Terreri, INAF - Osservatorio Astronomico di Roma, University of Rome "Tor Vergata" (UToV)
17:10-17:30 (20min)
›
Implementation of the crossed-sine wavefront sensor
- Yan FENG, Institut de Planétologie et d'Astrophysique de Grenoble
17:30-17:50 (20min)
›
Improved Pyramid Wavefront Sensor using a Diffractive Optical Layer
- Esteban Vera, Pontificia Universidad Católica de Valparaíso
17:50-18:10 (20min)
›18:30 (1h50)
Networking Dinner
18:30 - 20:20 (1h50)
Networking Dinner
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