Paper
13 September 2012 A test bench for ARGOS: integration of sub-systems and validation of the wavefront sensing
Author Affiliations +
Abstract
ARGOS, the wide eld Laser Guide Stars adaptive optics system for the Large Binocular Telescope, is now entering its installation phase. In the meanwhile, we have started a test bench in order to integrate various Argos sub-systems and demonstrate its wavefront measurements. To this objective, we rst validate three key components of the Argos wavefront sensor which we then integrate together. The test bench therefore comprises the Argos wavefront camera system - including a large frame, fast framerate, high quantum eciency and low readout noise pnCCD -, the slope computer, and a optical gating unit. While we present here the demonstration of those three key components, it is also a step to their system level integration that enables us to validate the wavefront measurements in term of noises, timing and computation. In the near future, those system will be integrated to the wavefront sensor system of ARGOS.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gilles Orban de Xivry and Sebastian Rabien "A test bench for ARGOS: integration of sub-systems and validation of the wavefront sensing", Proc. SPIE 8447, Adaptive Optics Systems III, 844751 (13 September 2012); https://doi.org/10.1117/12.926275
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Wavefront sensors

Cameras

Wavefronts

Adaptive optics

Sensors

Integrated optics

Imaging systems

RELATED CONTENT

A laser tomography test bed for extremely large telescopes
Proceedings of SPIE (August 04 2014)
HARMONI at ELT full scale prototype of the...
Proceedings of SPIE (August 29 2022)
The evolution of the ALIOLI instrument
Proceedings of SPIE (August 29 2022)
Near-infrared wavefront sensing
Proceedings of SPIE (July 26 2016)
Closed-loop wave-front correction using phase diversity
Proceedings of SPIE (August 28 1998)

Back to Top