A phase-shifting Zernike wavefront sensor has distinct advantages over other types of wavefront sensors. Chief among them are: 1) improved sensitivity to low-order aberrations and 2) efficient use of photons (hence reduced sensitivity to photon noise). We are in the process of deploying a phase-shifting Zernike wavefront sensor to be used with the real-time adaptive optics system for Palomar. Here we present the current state of the Zernike wavefront sensor to be integrated into the high-order adaptive optics system at Mount Palomar’s Hale Telescope
International audienceThe next generation of Giant Fragmented Telescopes will allow the study of fai...
Wavefront sensor is designed to measure both intensity distribution and phase distortion of optical ...
The National Solar Observatory at Sacramento Peak is developing adaptive optics (AO) for solar astro...
Aims. The Zernike wavefront sensor (ZWFS) is a concept belonging to the wide class of Fourier-filter...
International audienceThe Zernike wavefront sensor (ZWFS) is a concept belonging to the wide class F...
Because atmospheric turbulence causes distortions in stellar wavefronts, passive ground based telesc...
The PALM-3000 upgrade to the Palomar Adaptive Optics system on the 5.1 meter Hale telescope will del...
The canonical Zernike phase-contrast technique transforms a phase object in one plane into an intens...
For centuries telescopes have been used to achieve an understanding of the universe and our place am...
Phase Diversity (PD) is a wavefront-sensing technology that offers certain advantages in an Adaptive...
Static Zernike phase-contrast plates have been used extensively in microscopy for half a century and...
A conventional Zernike filter measures wavefront phase by superimposing the aberrated input beam wit...
To correct for the phase aberrations an adaptive optical system is usually used. The standard adapti...
We describe the practical implementation of a closed-loop adaptive-optics system incorporating a nov...
The wavefront sensor (WFS) is perhaps the most critical adaptive-optic subsystem, particularly for a...
International audienceThe next generation of Giant Fragmented Telescopes will allow the study of fai...
Wavefront sensor is designed to measure both intensity distribution and phase distortion of optical ...
The National Solar Observatory at Sacramento Peak is developing adaptive optics (AO) for solar astro...
Aims. The Zernike wavefront sensor (ZWFS) is a concept belonging to the wide class of Fourier-filter...
International audienceThe Zernike wavefront sensor (ZWFS) is a concept belonging to the wide class F...
Because atmospheric turbulence causes distortions in stellar wavefronts, passive ground based telesc...
The PALM-3000 upgrade to the Palomar Adaptive Optics system on the 5.1 meter Hale telescope will del...
The canonical Zernike phase-contrast technique transforms a phase object in one plane into an intens...
For centuries telescopes have been used to achieve an understanding of the universe and our place am...
Phase Diversity (PD) is a wavefront-sensing technology that offers certain advantages in an Adaptive...
Static Zernike phase-contrast plates have been used extensively in microscopy for half a century and...
A conventional Zernike filter measures wavefront phase by superimposing the aberrated input beam wit...
To correct for the phase aberrations an adaptive optical system is usually used. The standard adapti...
We describe the practical implementation of a closed-loop adaptive-optics system incorporating a nov...
The wavefront sensor (WFS) is perhaps the most critical adaptive-optic subsystem, particularly for a...
International audienceThe next generation of Giant Fragmented Telescopes will allow the study of fai...
Wavefront sensor is designed to measure both intensity distribution and phase distortion of optical ...
The National Solar Observatory at Sacramento Peak is developing adaptive optics (AO) for solar astro...