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Adaptive optics capabilities at the Large Binocular Telescope Observatory

We present an overview of the current and future adaptive optics systems at the LBTO along with the current and planned science instruments they feed. All the AO systems make use of the two 672 actuator adaptive secondary mirrors. They are (1) FLAO (NGS/SCAO) feeding the LUCI NIR imagers/spectrographs; (2) LBTI/AO (NGS/SCAO) feeding the NIR/MIR imagers and LBTI beam combiner; (3) the ARGOS LGS GLAO system feeding LUCIs; and (4) LINO-NIRVANA - an NGS/MCAO imager and interferometer system. AO performance of the current systems is presented along with proposed performances for the newer systems taking into account the future instrumentation.

Identiferoai:union.ndltd.org:arizona.edu/oai:arizona.openrepository.com:10150/622008
Date26 July 2016
CreatorsChristou, J. C., Brusa, G., Conrad, A., Esposito, S., Herbst, T., Hinz, P., Hill, J. M., Miller, D. L., Rabien, S., Rahmer, G., Taylor, G. E., Veillet, C., Zhang, X.
ContributorsUniv Arizona, Steward Observ, Large Binocular Telescope (United States), Large Binocular Telescope (United States), Large Binocular Telescope (United States), Arcetri Astrophysical Observatory (Italy), Max Planck Institute for Astronomy (Germany), Univ. of Arizona (United States), Large Binocular Telescope (United States), Large Binocular Telescope (United States), Max Planck Institut für Extraterrestrische Physik (Germany), Large Binocular Telescope (United States), Large Binocular Telescope (United States), Large Binocular Telescope (United States), Large Binocular Telescope (United States)
PublisherSPIE-INT SOC OPTICAL ENGINEERING
Source SetsUniversity of Arizona
LanguageEnglish
Detected LanguageEnglish
TypeArticle
Rights© 2016 SPIE
Relationhttp://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2231783

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