Open Access Paper
28 June 2006 Design of the KMOS multi-object integral-field spectrograph
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Abstract
KMOS is a near-infrared multi-object integral field spectrometer which has been selected as one of a suite of second-generation instruments to be constructed for the ESO VLT in Chile. The instrument will be built by a consortium of UK and German institutes working in partnership with ESO and is currently at the end of its preliminary design phase. We present the design status of KMOS and discuss the most novel technical aspects and the compliance with the technical specification.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Ray Sharples, Ralf Bender, Richard Bennett, Keith Burch, Paul Carter, Mark Casali, Paul Clark, Robert Content, Richard Davies, Roger Davies, Marc Dubbeldam, Gert Finger, Reinhard Genzel, Reinhold Haefner, Achim Hess, Markus Kissler-Patig, Ken Laidlaw, Matt Lehnert, Ian Lewis, Alan Moorwood, Bernard Muschielok, Natascha Förster-Schreiber, Jeff Pirard, Suzanne Ramsay Howat, Phil Rees, Josef Richter, David Robertson, Ian Robson, Roberto Saglia, Matthias Tecza, Naranjan Thatte, Stephen Todd, and Michael Wegner "Design of the KMOS multi-object integral-field spectrograph", Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 62691C (28 June 2006); https://doi.org/10.1117/12.669781
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Cited by 9 scholarly publications.
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KEYWORDS
Spectrographs

Mirrors

Astronomical imaging

Spectroscopy

Galactic astronomy

Calibration

Sensors

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