Paper
13 August 2014 Pre-shipment test of the ARGOS laser guide star wavefront sensor
Author Affiliations +
Abstract
We present the results of the laboratory characterization of the ARGOS LGS wavefront sensor (LGSW) and dichroic units. ARGOS is the laser guide star adaptive optics system of the Large Binocular Telescope (LBT). It implements a Ground Layer Adaptive Optics (GLAO) correction for LUCI, an infrared imager and multi-object spectrograph (MOS), using 3 pulsed Rayleigh beacons focused at 12km altitude. The LGSW is a Shack-Hartman sensor having 15 × 15 subaspertures over the telescope pupil. Each LGS is independently stabilized for on-sky jitter and gated to reduce spot elongation. The 3 LGS pupils are stabilized to compensate mechanical flexure and are arranged on a single detector. Two units of LGSW have been produced and tested at Arcetri Observatory. We report on the results obtained in the pre-shipment laboratory test: internal active flexure compensation loop performance, optomechanical stability under different gravity conditions, thermal cycling, Pockels cells performance. We also update on the upcoming installation and commissioning campaign at LBT.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Marco Bonaglia, Lorenzo Busoni, Tommaso Mazzoni, Alfio Puglisi, Jacopo Antichi, Simone Esposito, Gilles Orban de Xivry, and Sebastian Rabien "Pre-shipment test of the ARGOS laser guide star wavefront sensor", Proc. SPIE 9148, Adaptive Optics Systems IV, 91485G (13 August 2014); https://doi.org/10.1117/12.2056596
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Sensors

Telescopes

Calibration

Mirrors

Wavefront sensors

Adaptive optics

Cameras

RELATED CONTENT

ARGOS wavefront sensing: from detection to correction
Proceedings of SPIE (August 07 2014)
Experiences operating CFHT's adaptive optics system
Proceedings of SPIE (September 11 1998)
The Giant Magellan Telescope phasing system
Proceedings of SPIE (September 13 2012)
Astronomical imaging using ground-layer adaptive optics
Proceedings of SPIE (September 24 2007)
The Giant Magellan Telescope adaptive optics program
Proceedings of SPIE (September 13 2012)

Back to Top