Paper
30 September 2004 IRIS2: a working infrared multi-object spectrograph and camera
Chris G. Tinney, Stuart D. Ryder, Simon C. Ellis, Vladimir Churilov, John Dawson, Greg A. Smith, Lew Waller, John D. Whittard, Roger Haynes, Allan Lankshear, John R. Barton, C. J. Evans, Keith Shortridge, Tony Farrell, Jeremy Bailey
Author Affiliations +
Abstract
IRIS2 is a near-infrared imager and spectrograph based on a HAWAII1 HgCdTe detector. It provides wide-field (7.7’×7.7’) imaging capabilities at 0.4486”/pixel sampling, long-slit spectroscopy at λ/Δλ≈2400 in each of the J, H and K passbands, and the ability to do multi-object spectroscopy in up to three masks. These multi-slit masks are laser cut, and have been manufactured for both traditional multiple slit work (≈20-40 objects in a 3’×7.4’ field-of-view), multiple slit work in narrow-band filters (≈100 objects in a 5’×7.4’ field-of-view), and micro-hole spectroscopy in narrow-band filters allowing the observation of ≈200 objects in a 5’×7.4’ field.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Chris G. Tinney, Stuart D. Ryder, Simon C. Ellis, Vladimir Churilov, John Dawson, Greg A. Smith, Lew Waller, John D. Whittard, Roger Haynes, Allan Lankshear, John R. Barton, C. J. Evans, Keith Shortridge, Tony Farrell, and Jeremy Bailey "IRIS2: a working infrared multi-object spectrograph and camera", Proc. SPIE 5492, Ground-based Instrumentation for Astronomy, (30 September 2004); https://doi.org/10.1117/12.550980
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Cited by 46 scholarly publications.
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KEYWORDS
Telescopes

Sensors

Cameras

Optical filters

Spectroscopy

Molybdenum

Image quality

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