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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. | |||||||
> > | SWIFT Project WebSWIFT 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. | |||||||
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