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    <    		SWIFT is an I-z band AO-assisted integral field spectrograph designed and built by the University of Oxford (PI: Niranjan Thatte). It combines high efficiency, low sky background, sensitive deep-depletion CCDs, and high order AO correction to complement near-infrared diffraction-limited IFS on 8-10m class telescopes. SWIFT is currently deployed behind the 241-actuator PALMAO system, at the Cassegrain focus of the Hale 5.1m telescope.
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    SWIFT Project Web

    SWIFT is an I-z band AO-assisted integral field spectrograph designed and built by the University of Oxford (PI: Niranjan Thatte). It combines high throughput, sensitive deep-depletion CCDs, high order adaptive optics correction, and low sky background to achieve exquisite sensitivity for extragalactic science. SWIFT saw first light on the 5.1 m Hale telescope in October 2008, and is currently fully available to the Palomar community.

     

    Partners: University of Oxford, Caltech

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    OIR Palomar/SWIFT Project web

    Project Scope: Design, build, and deploy an AO-fed integral field spectrograph

    Partners: Oxford University, Caltech

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    SWIFT is an I-z band AO-assisted integral field spectrograph designed and built by the University of Oxford (PI: Niranjan Thatte). It combines high efficiency, low sky background, sensitive deep-depletion CCDs, and high order AO correction to complement near-infrared diffraction-limited IFS on 8-10m class telescopes. SWIFT is currently deployed behind the 241-actuator PALMAO system, at the Cassegrain focus of the Hale 5.1m telescope.

    Partners: University of Oxford, Caltech

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    Revision 82009-04-25 - AntoninBouchez

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    Project Scope: Design, build, and deploy an AO-fed integral field spectrograph

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