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Proceedings Paper

On-sky AO test bench
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Paper Abstract

With the upcoming construction of ELTs, several existing technologies are being pushed beyond their performance limit and it became essential to develop and evaluate alternatives. We present a specifically designed focal plane box which will allow to evaluate, directly on-sky, the performance of a number of next generation adaptive optics related technologies The system will able us to compare the performance of several new wavefront sensors in contrast to a Shack-Hartman wavefront sensor. The system has been designed for the "Observatoire du Mont Mégantic" (OMM) which hosts a telescope having a 1.6-meter diameter primary. The OMM telescope, located halfway between Montreal and Quebec City, is known to be an excellent location to develop and test precursor instruments which can then be upscaled to larger telescopes (ex. SPIOMM which led to SITELLE at the CFHT). We present the results of the first run made at the telescope and also identify problems that were encountered. We also propose a series of modifications to the system that will help to solve these issues.

Paper Details

Date Published: 11 August 2016
PDF: 4 pages
Proc. SPIE 9909, Adaptive Optics Systems V, 99092V (11 August 2016); doi: 10.1117/12.2233029
Show Author Affiliations
Denis Brousseau, Univ. Laval (Canada)
Simon Thibault, Univ. Laval (Canada)
Jean-François Lavigne, ABB Measurement Systems (Canada)
Jean-Pierre Véran, NRC Herzberg (Canada)


Published in SPIE Proceedings Vol. 9909:
Adaptive Optics Systems V
Enrico Marchetti; Laird M. Close; Jean-Pierre Véran, Editor(s)

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