We present a method to calibrate a high-resolution wavefront (WF)-correcting device with a single, static camera, located in the focal-plane; no moving of any component is needed. The method is based on a localized diversity and differential optical transfer functions to compute both the phase and amplitude in the pupil plane located upstream of the last imaging optics. An experiment with a spatial light modulator shows that the calibration is sufficient to robustly operate a focal-plane WF sensing algorithm controlling a WF corrector with 40,000 degrees of freedom. We estimate that the locations of identical WF corrector elements are determined with a spatial resolution of 0.3% compared to the pupil diameter. © 2013 Optical Society of Amer...
We present a promising approach to the extremely fast sensing and correction of small wavefront erro...
We present a liquid crystal method of correcting the phase of an aberrated wavefront using a spatial...
International audienceExoplanet direct imaging is a challenging goal of today's astronomical instrum...
We present a method to calibrate a high-resolution wavefront (WF)-correcting device with a single, s...
We present two complementary algorithms suitable for using focal-plane measurements to control a wav...
We present two complementary algorithms suitable for using focal-plane measurements to control a wav...
We present two complementary algorithms suitable for using focal-plane measurements to control a wav...
We investigate methods to calibrate the non-common path aberrations at an adaptive optics system hav...
We show how differential optical transfer function (dOTF) method is used to calibrate an adaptive op...
A key component of any adaptive optics system (AO) for the correction of wavefront aberrations, is t...
In astronomy and microscopy, distortions in the wavefront affect the dynamic range of a high contras...
Phase aberrations in optical systems,which occur in various applications such as astronomy, microsco...
International audienceWe describe new results obtained with the integrated Mach-Zehnder (iMZ) self r...
Point spread function (PSF) engineering is used in single emitter localization to measure the emitte...
We propose an efficient approximation to the nonlinear phase diversity (PD) method for wavefront rec...
We present a promising approach to the extremely fast sensing and correction of small wavefront erro...
We present a liquid crystal method of correcting the phase of an aberrated wavefront using a spatial...
International audienceExoplanet direct imaging is a challenging goal of today's astronomical instrum...
We present a method to calibrate a high-resolution wavefront (WF)-correcting device with a single, s...
We present two complementary algorithms suitable for using focal-plane measurements to control a wav...
We present two complementary algorithms suitable for using focal-plane measurements to control a wav...
We present two complementary algorithms suitable for using focal-plane measurements to control a wav...
We investigate methods to calibrate the non-common path aberrations at an adaptive optics system hav...
We show how differential optical transfer function (dOTF) method is used to calibrate an adaptive op...
A key component of any adaptive optics system (AO) for the correction of wavefront aberrations, is t...
In astronomy and microscopy, distortions in the wavefront affect the dynamic range of a high contras...
Phase aberrations in optical systems,which occur in various applications such as astronomy, microsco...
International audienceWe describe new results obtained with the integrated Mach-Zehnder (iMZ) self r...
Point spread function (PSF) engineering is used in single emitter localization to measure the emitte...
We propose an efficient approximation to the nonlinear phase diversity (PD) method for wavefront rec...
We present a promising approach to the extremely fast sensing and correction of small wavefront erro...
We present a liquid crystal method of correcting the phase of an aberrated wavefront using a spatial...
International audienceExoplanet direct imaging is a challenging goal of today's astronomical instrum...