Design of adaptive optics calibration source for the Giant Magellan Telescope

Ping Zhou, James H. Burge, Chunyu Zhao, Scott Benjamin, Brian Cuerden, Antonin Bouchez

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Scopus citations

Abstract

The Giant Magellan Telescope (GMT) is one of the extremely large telescopes of the next generation. The GMT adaptive optics (AO) system uses an adaptive secondary mirror and natural and laser guide stars to achieve diffraction-limited images. The AO calibration source provides sources at the telescope prime focus which replicate the properties of the natural and laser guide stars, to calibrate and verify the performance of the AO system. We present an optical design for this calibration source, and discuss the expected accuracy based on the tolerance analysis.

Original languageEnglish (US)
Title of host publicationAdaptive Optics Systems IV
EditorsJean-Pierre Veran, Enrico Marchetti, Laird M. Close
PublisherSPIE
ISBN (Electronic)9780819496164
DOIs
StatePublished - Jan 1 2014
EventAdaptive Optics Systems IV - Montreal, Canada
Duration: Jun 22 2014Jun 27 2014

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume9148
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Other

OtherAdaptive Optics Systems IV
CountryCanada
CityMontreal
Period6/22/146/27/14

Keywords

  • Adaptive optics
  • aberrations
  • calibration source
  • computer-generated hologram
  • laser guide star
  • natural guide star

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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  • Cite this

    Zhou, P., Burge, J. H., Zhao, C., Benjamin, S., Cuerden, B., & Bouchez, A. (2014). Design of adaptive optics calibration source for the Giant Magellan Telescope. In J-P. Veran, E. Marchetti, & L. M. Close (Eds.), Adaptive Optics Systems IV [91484Z] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9148). SPIE. https://doi.org/10.1117/12.2055204