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Astronomy / Hubble Space Telescope / Telescopes / Observational astronomy / Spectrograph / W. M. Keck Observatory


A comparison of open versus closed loop flexure compensation systems for two Keck optical imaging spectrographs: ESI and DEIMOS Robert Kibrick, S. M. Faber, Andrew C. Phillips, Molly McVeigh, Dave Cowley, Matt Radovan,
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Document Date: 2002-07-30 17:09:09


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File Size: 347,09 KB

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Company

UCO/Lick Observatory Detector Laboratory / Orbit Semiconductor / MIT/Lincoln Laboratory / /

Currency

pence / /

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Event

Business Partnership / /

Facility

UCO/Lick Observatory Detector Laboratory / San Diego State University / Steve Allen UCO/Lick Observatory / University of California / /

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IndustryTerm

direct imaging slider / enclosed electronics ring / direct imaging / optical imaging spectrographs / exure compensation systems / software corrections / imaging / direct-imaging modes / control algorithm / systems / direct imaging mode / direct imaging mirror / electronics / /

NaturalFeature

Mauna Kea / /

Organization

MIT / San Diego State University / University of California / Santa Cruz / US Federal Reserve / /

Person

Kirk Gilmore / Chris Wright / Matt Radovan / However / Andrew C. Phillips / Robert Kibrick / Molly McVeigh / Dave Cowley / Dean Tucker / /

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Position

PI controller / Walker / FCS CCD controller / author / second generation controller / representative / controller / /

ProvinceOrState

California / /

Technology

S/N / control algorithm / spectroscopy / /

URL

http /

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