Colección SciELO Chile

Departamento Gestión de Conocimiento, Monitoreo y Prospección
Consultas o comentarios: productividad@anid.cl
Búsqueda Publicación
Búsqueda por Tema Título, Abstract y Keywords



Fourier filter LGS wavefront sensing for ELT size telescopes
Indexado
WoS WOS:000859295700133
Scopus SCOPUS_ID:85178514967
DOI 10.1117/12.2629683
Año 2022
Tipo proceedings paper

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



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.

Métricas Externas



PlumX Altmetric Dimensions

Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:

Disciplinas de Investigación



WOS
Sin Disciplinas
Scopus
Computer Science Applications
Electrical And Electronic Engineering
Electronic, Optical And Magnetic Materials
Applied Mathematics
Condensed Matter Physics
SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.


Autores - Afiliación



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 -

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento



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

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



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.

Muestra la fuente de financiamiento declarada en la publicación.