GTCAO real time AO closed loop software implementation and initial computer performance analysis

Bibcode
2018SPIE10703E..76M
DOI
10.1117/12.2312437
Marco de la Rosa, J.; Núñez Cagigal, M.; Basden, A.; Tubío, O.; Rosich, J.; Rodríguez-Ramos, L. F.; Montilla, I.; Puga Antolín, M.; L. López, R.; Simoes, R.; Patrón, J.; Reyes, M.; Béjar, V. J. S.
Bibliographical reference

Proceedings of the SPIE, Volume 10703, id. 1070376 19 pp. (2018).

Advertised on:
7
2018
Number of authors
13
IAC number of authors
12
Citations
0
Refereed citations
0
Description
The Gran Telescopio Canarias Adaptive Optics (GTCAO) is a single-conjugated post-focal system with a Shack Hartmann wavefront sensor working at visible wavelength and one Deformable Mirror (DM) conjugated to the pupil. GTCAO does not include a fast tip-tilt mirror in its optical bench so it relies on the telescope secondary mirror (M2) to correct low frequency tip-tilt and offload the DM. This paper describes specific details of the software implementation of the mirror control for GTCAO, analyses its computational needs, presents the series of tests performed on the newly designed AO closed loop, and summarises software optimizations and operating system configurations set in order to optimise computer performance in the available hardware architecture
Related projects
Discovery of a system of super-Earths orbiting the star HD 176986 with about 5.7 and 9.2 Earth masses.
Very Low Mass Stars, Brown Dwarfs and Planets

Our goal is to study the processes that lead to the formation of low mass stars, brown dwarfs and planets and to characterize the physical properties of these objects in various evolutionary stages. Low mass stars and brown dwarfs are likely the most numerous type of objects in our Galaxy but due to their low intrinsic luminosity they are not so

Rafael
Rebolo López
In progress
Type
Non-refereed
Stellar & Interstellar Physics (FEEI)

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