Mr. Francisco Antonio Oyarzun Profile

Francisco Antonio Oyarzun

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Publications (3)

Proceedings Article | 28 August 2024 Presentation

Cassiopée: toward technological development for XAO on ELT

Benoît Neichel, Thierry Fusco, Jean-Luc Gach, Philippe Feautrier, Julien Charton, Piero Bruno, Francisco Oyarzun, Mathieu Motte, Jonathan Dray, Mahawa Cissé, Romain Fétick, Cédric Taïssir Heritier, Jean-Francois Sauvage

Proceedings Volume 13097, 130971G (2024) https://doi.org/10.1117/12.3019601

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Proceedings Article | 27 August 2024 Poster + Paper

Effects of the LGS geometry on the Shack-Hartmann wavefront sensor and the Pyramid wavefront sensor

F. Oyarzun, C. Heritier, V. Chambouleyron, T. Fusco, P. Rouquette, B. Neichel

Proceedings Volume 13097, 130974Q (2024) https://doi.org/10.1117/12.3018283

KEYWORDS: Telescopes, Wavefront sensors, Modulation, Spatial frequencies, Sodium, Image sensors, Covariance matrices, Simulations, Sensors, Wavefronts

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Proceedings Article | 30 August 2022 Poster + Paper

Fourier filter LGS wavefront sensing for ELT size telescopes

Francisco Oyarzún, Vincent Chambouleyron, Benoit Neichel, Thierry Fusco, Andrés Guesalaga

Proceedings Volume 12185, 121854W (2022) https://doi.org/10.1117/12.2629683

KEYWORDS: Wavefront sensors, Telescopes, Shearing interferometers, Sodium, Adaptive optics, Stars, Laser guide stars, Atmospheric propagation

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All the upcoming Extremely Large Telescopes (ELTs) include artificial Laser Guide Stars (LGS) to increase the sky coverage of their Adaptive Optics (AO) systems. Given the thickness of the sodium layer, where the LGS are created, these artificial stars end-up to be extended 3D objects. On a large pupil, like the ELTs, the sub-apertures of a Shack-Hartmann wavefront sensor see the LGS as an elongated object depending on their position with respect to the laser lunch telescope. As a result, a detector with a large number of pixels per sub-aperture is required to fully sample the elongated spots and minimize centroiding errors. As an alternative, we propose to explore the use of Fourier Filter Wavefront Sensors (FFWFS), such as the pyramid WFS but not only, as they could potentially offer an interesting alternative, significantly less pixel-intensive. As a first step, we developed a new method of simulating extended sources for FFWFS, which allows accelerating the simulation by a factor of over sixty times when compared to the traditional methods. Taking advantage of this, we then compare the performance of three sensors: the well-known Pyramid, the Ingot (as proposed by Ragazzoni) and a new promising candidate called the tilted Shearing interferometer. Sensitivity tests are performed for quantitative comparisons between these sensors. When comparing the sensitivity of a diffraction limited source with a 2D 1” source for a 3- and 4-sized Pyramid WFS, a 25 factor decrease was observed. This lost sensitivity is equivalent to a decrease in limiting magnitude of 6.7. Then, comparing the sensitivity of the Pyramid WFS and the Ingot WFS, the both had a similar behavior in the horizontal direction (across the elongation of the LGS), but the Pyramid had almost twice the sensitivity along the elongation, meaning that overall the Pyramid is more sensitive than the Ingot. The Tilted Shearing interferometer did not performed as expected, mainly because of diffraction and sampling effects that could be better understood in laboratory conditions.

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