The IRIS2 infrared imager and spectrograph was built in-house by the AAO, and commissioned between October 2001 and July 2002. It provides the AAO with an infrared facility for
At its heart is a 1024x1024 Rockwell
HAWAII-1 HgCdTe infrared detector, illuminated by a f/8 to f/2.2 focal
reducer. Spectroscopy is achieved by the implementation of a slit wheel
allowing the insertion of a 1" wide slit (or multi-slit masks), and a wheel in
the collimated beam containing grisms. These grisms use ~50mm 45-degree prisms
of sapphire to deviate the beam and feed replica transmission gratings applied
to their surfaces.
The spatial scale of IRIS2 is 0.4486"/pixel, giving a field of view of 7.7' x 7.7. The 1" slit for spectroscopy corresponds to limiting spectroscopic resolution of 2.2 pixels on the detector. At this resolution the dispersion of the sapphire grisms provide R~2400.
If you have any queries about the status or use of IRIS2, please do not hesitate to contact either Chris Tinney, or Stuart Ryder.
These pages contain information on the functionality of the IRIS2 Infrared Imager and Spectrograph. Pages maintained by Chris Tinney mailto:cgt@aaoepp.aao.gov.au, Stuart Ryder (sdr@aaoepp.aao.gov.au) and Simon Ellis (sce@aaoepp.aao.gov.au).Page last modified on February 9, 2004 by Stuart Ryder