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SWIFT Project Web

 
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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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Latest News

 
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SWIFT with light baffles removed
 

Documentation

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Technical Reference

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Related Links

  • Palomar LGS
  • PALM-3000
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