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Interferometry / Optical interferometry / Very Large Telescope / CHARA array / Closure phase / Radio telescope / W. M. Keck Observatory / Angular resolution / Adaptive optics / Observational astronomy / Astronomy / Telescopes


Document Date: 2009-04-07 14:10:35

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Company

Cepheid / Wilson / Naval Research Laboratory / baselines AB / MIRC / Bharmal N.A. / /

Country

United States / Ireland / /

Currency

USD / /

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Facility

Massachusetts Institute of Technology Colavita / University of Cambridge Buscher / /

IndustryTerm

technology areas / precise imaging / high-resolution imaging / natural technology / fringe detection systems / interferometry technology development / feed systems / detection software development / technology development / radio astronomical imaging / adaptive optics systems / interferometer technology / data post-processing / analysis software / technology support / interferometry technology / imaging / surface imaging / beam combination/fringe detection systems / software development / improved software / delay line control algorithm / /

MusicGroup

IR / Baselines / Wave / /

NaturalFeature

Mauna Kea / /

OperatingSystem

Cygnus / /

Organization

University of Cambridge Buscher / African Union / National Science Foundation / UC Berkeley / National Aeronautics and Space Administration / Astro2010 Review Committee / Massachusetts Institute of Technology / CHARA Array Georgia St. Univ. / Institute of Technology Colavita / /

Person

Mundy / /

/

ProvinceOrState

British Columbia / Massachusetts / /

Technology

delay line control algorithm / Optical interferometry technology / MIDI / natural technology / Existing interferometer technology / involve changing the delay line control algorithm / /

URL

http /

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