Recently, deep neural network (DNN) based adaptive optics systems were proposed to address the issue of latency in existing wavefront sensorless (WFS-less) aberration correction techniques. Intensity images alone are sufficient for the DNN model to compute the necessary wavefront correction, removing the need for iterative processes and allowing practical real-time aberration correction to be implemented. Specifically, we generate the desired aberration correction phase profiles utilizing a DNN based system that outputs a set of coefficients for 27 terms of Zernike polynomials. We present an experimental realization of this technique using a spatial light modulator (SLM) on real physical turbulence-induced aberration. We report an aberratio...
peer reviewedFocal plane wavefront sensing (FPWFS) is appealing for several reasons. Notably, it off...
Light scattering and aberrations limit optical microscopy in biological tissue, which motivates the ...
Latency in the control loop of Adaptive Optics (AO) systems can severely limit its performance. Theo...
Traditional adaptive optics (AO) aberration correction algorithms require multiple iterations, so ar...
In this paper, research was conducted on Deep Learning Wavefront Sensing (DLWS) neural networks usin...
The Delft Center for Systems and Control (DCSC) 'Smart Optics' aim to achieve higher resolution imag...
High-contrast imaging systems in ground-based astronomy rely on a precise control of the wavefront....
Information on the correlations from solar Shack–Hartmann wavefront sensors is usually used for reco...
In high-contrast imaging applications, such as the direct imaging of exoplanets, a coronagraph is us...
We describe a new, simple wavefront sensing method that uses a single measurement of a defocused sta...
With the successful application of the Shack–Hartmann wavefront sensor in measuring aberrations of t...
editorial reviewedInstrumental aberrations strongly limit high-contrast imaging of exoplanets, espec...
Astronomical images, degraded by the effects of atmospheric turbulence, can be corrected in real-tim...
Static and quasi-static aberrations represent a great limit for high contrast imaging in large teles...
In visual experiments that require real-time partial correction of wavefront aberrations, small erro...
peer reviewedFocal plane wavefront sensing (FPWFS) is appealing for several reasons. Notably, it off...
Light scattering and aberrations limit optical microscopy in biological tissue, which motivates the ...
Latency in the control loop of Adaptive Optics (AO) systems can severely limit its performance. Theo...
Traditional adaptive optics (AO) aberration correction algorithms require multiple iterations, so ar...
In this paper, research was conducted on Deep Learning Wavefront Sensing (DLWS) neural networks usin...
The Delft Center for Systems and Control (DCSC) 'Smart Optics' aim to achieve higher resolution imag...
High-contrast imaging systems in ground-based astronomy rely on a precise control of the wavefront....
Information on the correlations from solar Shack–Hartmann wavefront sensors is usually used for reco...
In high-contrast imaging applications, such as the direct imaging of exoplanets, a coronagraph is us...
We describe a new, simple wavefront sensing method that uses a single measurement of a defocused sta...
With the successful application of the Shack–Hartmann wavefront sensor in measuring aberrations of t...
editorial reviewedInstrumental aberrations strongly limit high-contrast imaging of exoplanets, espec...
Astronomical images, degraded by the effects of atmospheric turbulence, can be corrected in real-tim...
Static and quasi-static aberrations represent a great limit for high contrast imaging in large teles...
In visual experiments that require real-time partial correction of wavefront aberrations, small erro...
peer reviewedFocal plane wavefront sensing (FPWFS) is appealing for several reasons. Notably, it off...
Light scattering and aberrations limit optical microscopy in biological tissue, which motivates the ...
Latency in the control loop of Adaptive Optics (AO) systems can severely limit its performance. Theo...