Paper
13 September 2012 Laboratory demonstration of real time frame selection with Magellan AO
Author Affiliations +
Abstract
The Magellan AO system combines a pyramid wavefront sensor and high-order adaptive secondary mirror, and will see first light on the Magellan Clay telescope in November 2012. With a 24 cm projected actuator pitch, this powerful system will enable good correction in the optical (0.5 to 1 μm). Realistic laboratory testing has produced Strehl ratios greater than 40% in i’ (0.765 μm) on bright simulated stars. On fainter stars our visible AO camera, VisAO, will work in the partially corrected regime with only short moments of good correction. We have developed a form of lucky imaging, called real time frame selection, which uses a fast shutter to block moments of bad correction, and quickly opens the shutter when the correction is good, enabling long integrations on a conventional CCD while maximizing Strehl ratio and resolution. The decision to open or shut is currently based on reconstructed WFS telemetry. Here we report on our implementation and testing of this technique in the Arcetri test tower in Florence, Italy, where we showed that long exposure i’ Strehl could be improved from 16% to 26% when the selection threshold was set to the best 10% of instantaneous Strehl.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jared R. Males, Laird M. Close, Derek Kopon, Fernando Quiros-Pacheco, Armando Riccardi, Marco Xompero, Alfio Puglisi, Victor Gasho, Katie M. Morzinski, and Katherine B. Follette "Laboratory demonstration of real time frame selection with Magellan AO", Proc. SPIE 8447, Adaptive Optics Systems III, 844742 (13 September 2012); https://doi.org/10.1117/12.926698
Lens.org Logo
CITATIONS
Cited by 7 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Adaptive optics

Camera shutters

Stars

Telescopes

Calibration

Charge-coupled devices

Turbulence

RELATED CONTENT


Back to Top