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| Indexado |
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| DOI | 10.1117/12.2629683 | ||||
| Año | 2022 | ||||
| Tipo | proceedings paper |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
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.
| Revista | ISSN |
|---|---|
| Proceedings Of Spie The International Society For Optical Engineering | 0277-786X |
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | LEMARIE-OYARZUN, FERNANDO RODOLFO | Hombre |
Pontificia Universidad Católica de Chile - Chile
|
| 2 | Chambouleyron, Vincent | Hombre |
Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia |
| 3 | Neichel, Benoit | Hombre |
Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia |
| 4 | Fusco, T. | Hombre |
Aix Marseille Univ - Francia
Laboratoire d'Astrophysique de Marseille - Francia |
| 5 | FERNANDEZ-GONZALEZ, FELIPE JOSE | Hombre |
Pontificia Universidad Católica de Chile - Chile
|
| 6 | Schreiber, L | - | |
| 7 | Schmidt, D | - | |
| 8 | Vernet, E | - |
| Fuente |
|---|
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| Agence Nationale de la Recherche |
| CNES |
| Centre National de la Recherche Scientifique |
| French National Research Agency (ANR) |
| Centre National d’Etudes Spatiales |
| INSU |
| LabEx FOCUS |
| ECOS-Conycit |
| Agencia Nacional de Investigación y Desarrollo |
| Chilean Agency for Research and Development |
| Action Spécifique Haute Résolution Angulaire |
| Chilean Agency for Research and Development (ANID) |
| Action Specifique Haute Resolution Angulaire (ASHRA) of CNRS/INSU |
| WOLF |
| ORP H2020 Framework Programme of the European Commission |
| DirecciOn de Postgrado de la Escuela de Ingenieria de la Pontificia Universidad CatMica de Chile |
| ECOS-CONYCIT France-Chile cooperation |
| STIC AmSud |
| SPIE |
| Programme In-vestissement Avenir F-CELT |
| ORP H2020 Framework Programme of the European Commission’s |
| APPLY |
| Dirección de Postgrado de la Escuela de Ingeniería de la Pontificia Universidad Católica de Chile |
| Programme Investissement Avenir F-CELT |
| ORP H2020 Framework Programme of the European Commission's |
| Agradecimiento |
|---|
| We would like to thank SPIE, the DirecciOn de Postgrado de la Escuela de Ingenieria de la Pontificia Universidad CatMica de Chile and the Chilean Agency for Research and Development (ANID) (grants Fondecyt 1190186 and Millennium Nucleus ACIP Science Initiative Program - NCN19_161) for their collaboration in the funding of this project. Special thanks to Jean-Francois Sauvage, Clementine Bechet, Felipe Pedreros, Camilo Weinberger, Jorge Tapia and Esther Soria for their guidance. This work benefited from the support of the the French National Research Agency (ANR) with WOLF (ANR18-CE31-0018), APPLY (ANR-19-CE31-0011) and LabEx FOCUS (ANR-11-LABX-0013); the Programme Investissement Avenir F-CELT (ANR-21-ESRE-0008), the Action Specifique Haute Resolution Angulaire (ASHRA) of CNRS/INSU co-funded by CNES, the ECOS-CONYCIT France-Chile cooperation (C20E02), the ORP H2020 Framework Programme of the European Commission's (Grant number 101004719) and STIC AmSud (21-STIC09). |
| We would like to thank SPIE, the Dirección de Postgrado de la Escuela de Ingeniería de la Pontificia Universidad Católica de Chile and the Chilean Agency for Research and Development (ANID) (grants Fondecyt 1190186 and Millennium Nucleus ACIP Science Initiative Program - NCN19 161) for their collaboration in the funding of this project. Special thanks to Jean-Francois Sauvage, Clementine Bechet, Felipe Pedreros, Camilo Weinberger, Jorge Tapia and Esther Soria for their guidance. |