Laboratory and telescope demonstration of the TP3-WFS for the adaptive optics segment of AOLI
| Autor: | C. Colodro-Conde, Craig D. Mackay, Roberto López, Rafael Toledo-Moreo, José Manuel Rodríguez-Ramos, A. Oscoz, L. F. Rodríguez-Ramos, M. Puga, Lucas Labadie, David L. King, B. Femenía, Balaji Muthusubramanian, A. Pérez Garrido, Rafael Rebolo, J. J. Fernandez-Valdivia, Isidro Villó-Pérez, Sergio Velasco, G. Rodriguez-Coira |
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| Přispěvatelé: | Ministerio de Economía, Industria y Competitividad, Ministerio de Educación, Cultura y Deporte, Fundación Seneca, Instituto de Astrofísica de Canarias |
| Rok vydání: | 2017 |
| Předmět: |
Physics
2203 Electrónica FOS: Physical sciences Library science Astronomy and Astrophysics 01 natural sciences adaptive optics [Instrumentation] law.invention 010309 optics Telescope Arquitectura y Tecnología de Computadoras high angular resolution [Instrumentation] Space and Planetary Science law 0103 physical sciences William Herschel Telescope Christian ministry European commission Astrophysics - Instrumentation and Methods for Astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) 010303 astronomy & astrophysics Remote sensing |
| Zdroj: | Repositorio Digital de la Universidad Politécnica de Cartagena instname |
| ISSN: | 1365-2966 0035-8711 |
| DOI: | 10.1093/mnras/stx262 |
| Popis: | AOLI (Adaptive Optics Lucky Imager) is a state-of-art instrument that combines adaptive optics (AO) and lucky imaging (LI) with the objective of obtaining diffraction limited images in visible wavelength at mid- and big-size ground-based telescopes. The key innovation of AOLI is the development and use of the new TP3-WFS (Two Pupil Plane Positions Wavefront Sensor). The TP3-WFS, working in visible band, represents an advance over classical wavefront sensors such as the Shack-Hartmann WFS (SH-WFS) because it can theoretically use fainter natural reference stars, which would ultimately provide better sky coverages to AO instruments using this newer sensor. This paper describes the software, algorithms and procedures that enabled AOLI to become the first astronomical instrument performing real-time adaptive optics corrections in a telescope with this new type of WFS, including the first control-related results at the William Herschel Telescope (WHT). Comment: 15 pages, 18 figures, Accepted 2017 January 27 |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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