International audienceIn this paper, we describe Fourier-based Wave Front Sensors (WFS) as linear integral operators, characterized by their Kernel. In a first part, we derive the dependency of this quantity with respect to the WFS's optical parameters: pupil geometry, filtering mask, tip/tilt modulation. In a second part we focus the study on the special case of convolutional Kernels. The assumptions required to be in such a regime are described. We then show that these convolutional kernels allow to drastically simplify the WFS's model by summarizing its behavior in a concise and comprehensive quantity called the WFS's Impulse Response. We explain in particular how it allows to compute the sensor's sensitivity with respect to the spatial ...
International audienceTo reach the full potential of the new generation of ground based telescopes, ...
A novel wave-front sensor that estimates phase from Fourier intensity measurements is described, and...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
International audienceIn this paper, we describe Fourier-based Wave Front Sensors (WFS) as linear in...
International audienceIn this paper, we describe Fourier-based Wave Front Sensors (WFS) as linear in...
International audienceWe introduce in this paper a general formalism for Fourier-based wave front se...
In this article, we compare a set of Wave Front Sensors (WFS) based on Fourier filtering technique. ...
International audienceWe compare a set of wave front sensors (WFS) based on Fourier filtering techni...
Context. Adaptive optics (AO) is a technique allowing for ground-based telescopes’ angular resolutio...
International audienceContext. Adaptive optics (AO) is a technique allowing for ground-based telesco...
The Hartmann pattern lends itself naturally to Fourier analysis, providing directly mir-ror commands...
International audienceThe use of Fourier methods in wave-front reconstruction can significantly redu...
14 pages, 9 figures, submitted to JATISWavefront sensors encode phase information of an incoming wav...
International audienceTo reach the full potential of the new generation of ground based telescopes, ...
A novel wave-front sensor that estimates phase from Fourier intensity measurements is described, and...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
International audienceIn this paper, we describe Fourier-based Wave Front Sensors (WFS) as linear in...
International audienceIn this paper, we describe Fourier-based Wave Front Sensors (WFS) as linear in...
International audienceWe introduce in this paper a general formalism for Fourier-based wave front se...
In this article, we compare a set of Wave Front Sensors (WFS) based on Fourier filtering technique. ...
International audienceWe compare a set of wave front sensors (WFS) based on Fourier filtering techni...
Context. Adaptive optics (AO) is a technique allowing for ground-based telescopes’ angular resolutio...
International audienceContext. Adaptive optics (AO) is a technique allowing for ground-based telesco...
The Hartmann pattern lends itself naturally to Fourier analysis, providing directly mir-ror commands...
International audienceThe use of Fourier methods in wave-front reconstruction can significantly redu...
14 pages, 9 figures, submitted to JATISWavefront sensors encode phase information of an incoming wav...
International audienceTo reach the full potential of the new generation of ground based telescopes, ...
A novel wave-front sensor that estimates phase from Fourier intensity measurements is described, and...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...