On-sky wide-field adaptive optics correction using multiple laser guide stars at the MMT

Christoph Baranec, Michael Hart, N. Mark Milton, Thomas Stalcup, Keith Powell, Miguel Snyder, Vidhya Vaitheeswaran, Don McCarthy, Craig Kulesa

Research output: Contribution to journalArticle

20 Scopus citations

Abstract

We describe results from the first astronomical adaptive optics (AO) system to use multiple laser guide stars, located at the 6.5 m MMT telescope in Arizona. Its initial operational mode, ground-layer adaptive optics (GLAO), provides uniform stellar wave front correction within the 2′ diameter laser beacon constellation, reducing the stellar image widths by as much as 53%, from 070 to 033 at λ = 2.14 μm. GLAO is achieved by applying a correction to the telescope's adaptive secondary mirror that is an average of wave front measurements from five laser beacons supplemented with image motion from a faint stellar source. Optimization of the AO system in subsequent commissioning runs will further improve correction performance where it is predicted to deliver 01-02 resolution in the near-infrared during a majority of seeing conditions.

Original languageEnglish (US)
Pages (from-to)1814-1820
Number of pages7
JournalAstrophysical Journal
Volume693
Issue number2
DOIs
StatePublished - Mar 10 2009

Keywords

  • atmospheric effects
  • instrumentation: adaptive optics
  • instrumentation: high angular resolution
  • telescopes

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Baranec, C., Hart, M., Milton, N. M., Stalcup, T., Powell, K., Snyder, M., Vaitheeswaran, V., McCarthy, D., & Kulesa, C. (2009). On-sky wide-field adaptive optics correction using multiple laser guide stars at the MMT. Astrophysical Journal, 693(2), 1814-1820. https://doi.org/10.1088/0004-637X/693/2/1814