In many scenarios, an Adaptive Optics (AO) control system operates in the presence of temporally non-white noise. We use a Kalman filter with a state space formulation that allows suppression of this colored noise, hence improving residual error over the case where the noise is assumed to be white. We demonstrate the effectiveness of this new filter in the case of the estimated Gemini Planet Imager tip-tilt environment, where there are both common-path and non-common path vibrations. We discuss how this same framework can also be used to suppress spatial aliasing during predictive wavefront control assuming frozen flow in a low-order AO system without a spatially filtered wavefront sensor, and present experimental measurements from Altair t...
Abstract. The wavefront aberrations induced by atmospheric turbulence can severely degrade the perfo...
International audienceWe present the results obtained with an end-to-end simulator of an Extreme Ada...
Quasi-static errors in the science leg and internal AO flexure will be corrected. Wavefront control ...
The visualization of objects within or beyond a turbulent medium is hampered by the aberrations the ...
Measurements of large ground telescopes are affected by the presence of the terrestrial atmospheric ...
International audienceWe build on a long-standing tradition in astronomical adaptive optics (AO) of ...
A new wavefront sensorless adaptive optics method is presented that can accurately correct for time-...
Telescope resolution is theoretically limited by the diffraction effect, and hence it is inversely p...
An Adaptive Optics (AO) system for astronomy is analysed from a control point of view. The focus is ...
We use telemetry data from the Gemini North ALTAIR adaptive optics system to investigate how well th...
This paper discusses various practical problems arising in the design and simulation of predictive c...
International audiencehe linear quadratic Gaussian regulator provides the minimum-variance control s...
We compare the performance of the Kalman filter (KF)-based and the minimum variance (MV) control alg...
International audienceThe fundamental issue of residual phase variance minimization in adaptive opti...
The Gemini Planet Imager instrument’s adaptive optics (AO) subsystem was designed specifically to fa...
Abstract. The wavefront aberrations induced by atmospheric turbulence can severely degrade the perfo...
International audienceWe present the results obtained with an end-to-end simulator of an Extreme Ada...
Quasi-static errors in the science leg and internal AO flexure will be corrected. Wavefront control ...
The visualization of objects within or beyond a turbulent medium is hampered by the aberrations the ...
Measurements of large ground telescopes are affected by the presence of the terrestrial atmospheric ...
International audienceWe build on a long-standing tradition in astronomical adaptive optics (AO) of ...
A new wavefront sensorless adaptive optics method is presented that can accurately correct for time-...
Telescope resolution is theoretically limited by the diffraction effect, and hence it is inversely p...
An Adaptive Optics (AO) system for astronomy is analysed from a control point of view. The focus is ...
We use telemetry data from the Gemini North ALTAIR adaptive optics system to investigate how well th...
This paper discusses various practical problems arising in the design and simulation of predictive c...
International audiencehe linear quadratic Gaussian regulator provides the minimum-variance control s...
We compare the performance of the Kalman filter (KF)-based and the minimum variance (MV) control alg...
International audienceThe fundamental issue of residual phase variance minimization in adaptive opti...
The Gemini Planet Imager instrument’s adaptive optics (AO) subsystem was designed specifically to fa...
Abstract. The wavefront aberrations induced by atmospheric turbulence can severely degrade the perfo...
International audienceWe present the results obtained with an end-to-end simulator of an Extreme Ada...
Quasi-static errors in the science leg and internal AO flexure will be corrected. Wavefront control ...