TY - JOUR 
A1 - Colodro Conde, Carlos
AU - Toledo Moreo, Rafael
AU - Fernández Valdivia Juan José
AU - López López, Roberto
AU - Oscoz Abad, Alejandro
AU - Rebolo López, Rafael
AU - Femenia, Bruno
AU - Labadie, Lucas
AU - Mackay, Craig
AU - Pérez Garrido, Antonio
AU - Puga Antolín, Marta
AU - Rodríguez Coira, Gustavo
AU - Rodríguez Ramos, Luis Fernando
AU - Rodríguez Ramos, José Manuel
AU - Villo Pérez, Isidro
AU - King,  David L.
AU - Toledo Moreo, Rafael
T1 - Laboratory and telescope demonstration of the TP3-WFS for the adaptive optics segment of AOLI
Y1 - 2017
SN - 0035-8711
UR - http://hdl.handle.net/10317/6674
AB - 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 PositionsWavefront 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)
KW - Arquitectura y Tecnología de Computadoras
KW - Instrumentation: adaptive optics
KW - Instrumentation: high angular resolution
KW - 2203 Electrónica
LA - eng
PB - Blackwell
ER -