Wavefront Sensing in the VLT/ELT era VII

›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