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Science / Physics / Adaptive optics / Shack–Hartmann wavefront sensor / Lenslet / Deformable mirror / Wavefront / Very Large Telescope / Ritchey–Chrétien telescope / Optics / Observational astronomy / Telescopes


Design of the Subaru laser guide star adaptive optics module
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Document Date: 2013-02-08 22:51:00


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City

Tokyo / Bellingham / Osaka / Hilo / /

Company

Telescope AG / Nalux Co. / Rockwell / /

Country

France / Japan / United States / /

Currency

USD / /

/

Facility

University of Tokyo / Institute of Astronomy / National Astronomical Observatory of Japan / /

IndustryTerm

monochromatic imaging performance / travel distance / electronics / diamond tool / re-imaging lenses / index-matching oil / /

OperatingSystem

L3 / /

Organization

Observatoire de Paris / Institute of Astronomy / University of Tokyo / Ministry of Education / Calibration Unit / /

Person

Yutaka Hayanoa / Yosuke Minowac / CAM BS / Naoto Kobayashic / Yukiko Kamatab / Stephen Colleya / Masayuki Hattoria / Masanori Iyeb / Thomas Kanea / Roberto Ragazzoni / Domenico Bonaccini Calia / Hideki Takamia / Makoto Watanabea / Brent L. Ellerbroek / CAM AQ CAM / Nobuo Arimotob / Olivier Guyona / Miwa Gotoa / Michael Eldreda / Path Spectral / /

Position

author / /

Product

Laser / Subaru laser / M-16 / M-9 / /

ProvinceOrState

Hawaii / Washington / /

Technology

laser / ADC / simulation / laser system / /

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