4.7 Article

Experience with wavefront sensor and deformable mirror interfaces for wide-field adaptive optics systems

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 459, Issue 2, Pages 1350-1359

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stw730

Keywords

instrumentation: adaptive optics; instrumentation: detectors

Funding

  1. UK Science and Technology Facilities Council [ST/K003569/1, ST/L00075X/1]
  2. FONDECYT [1150369]
  3. Agence Nationale de la Recherche (ANR) [06-BLAN-0191]
  4. CNRS/INSU, Obs. de Paris
  5. Univ. Paris Diderot
  6. European Commission [211257]
  7. OPTICON programme Infrastructures 2008-1 Grant [226604 (JRA1)]
  8. OPTICON programme Infrastructures 2012-1 Grant [312430 (WP1)]
  9. STFC [ST/N002660/1] Funding Source: UKRI
  10. Science and Technology Facilities Council [ST/N002660/1] Funding Source: researchfish

Ask authors/readers for more resources

Recent advances in adaptive optics (AO) have led to the implementation of wide field-of-view AO systems. A number of wide-field AO systems are also planned for the forthcoming Extremely Large Telescopes. Such systems have multiple wavefront sensors of different types, and usually multiple deformable mirrors (DMs). Here, we report on our experience integrating cameras and DMs with the real-time control systems of two wide-field AO systems. These are CANARY, which has been operating on-sky since 2010, and DRAGON, which is a laboratory AO real-time demonstrator instrument. We detail the issues and difficulties that arose, along with the solutions we developed. We also provide recommendations for consideration when developing future wide-field AO systems.

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