Retinal adaptive optics imaging with a pyramid wavefront sensor

The pyramid wavefront sensor (P-WFS) has replaced the Shack-Hartmann (SH-) WFS as the sensor of choice for high-performance adaptive optics (AO) systems in astronomy. Many advantages of the P-WFS, such as its adjustable pupil sampling and superior sensitivity, are potentially of great benefit for AO...

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Detalles Bibliográficos
Autores principales: Brunner, Elisabeth, Shatokhina, Julia, Shirazi, Muhammad Faizan, Drexler, Wolfgang, Leitgeb, Rainer, Pollreisz, Andreas, Hitzenberger, Christoph K., Ramlau, Ronny, Pircher, Michael
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Optical Society of America 2021
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8548025/
https://www.ncbi.nlm.nih.gov/pubmed/34745716
http://dx.doi.org/10.1364/BOE.438915

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8548025/
https://www.ncbi.nlm.nih.gov/pubmed/34745716
http://dx.doi.org/10.1364/BOE.438915

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