Title:
SWIFT: An AO-assisted I,z band integral field 
spectrograph
Authors:
M. Tecza, N. Thatte, F. Clarke, T. Goodsall, M. Symeonidis
Abstract:
SWIFT is an adaptive optics assisted integral 
field spectrograph covering the I and z astronomical bands (0.7µm-1.0µm). 
It builds on two recent developments (i) the improved ability of second 
generation adaptive optics systems to correct for atmospheric turbulence 
at wavelengths 1µm, and (ii) the availability of CCD array detectors with 
high quantum efficiency at very red wavelengths (close to the silicon band 
edge cut-off). Combining these with a state-of-the-art integral field unit 
design using an all-glass image slicer, SWIFT\'s design provides very high 
throughput and low scattered light. It is a dedicated integral field 
spectrograph, specifically built to address a range of interesting 
astrophysical questions.